pywcs-1.12/0000755001153600020070000000000012310355732014644 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/CHANGELOG0000644001153600020070000000561712310355627016072 0ustar cslocumSTSCI\science00000000000000Version 1.11 ============ NEW FEATURES: - Updated to wcslib version 4.8.2, which gives much more detailed error messages. Exceptions raised due to invalid WCS keywords should now be more informative. - Undefined values that are the result of p2s and s2p are now set to NaN. Previously, one had to examine the stat result vector to determine which results were invalid. - Added functions get_pc() and get_cdelt(). These provide a way to always get the canonical representation of the linear transformation matrix, whether the header specified it in PC, CD or CROTA form. BROADER COMPATIBILITY: - Supports Python 3.x - Long-running process will now release the Python GIL to better support Python multithreading. - Builds on Microsoft Windows using mingw32, mingw64 and Visual Studio 9.0 and 10.0 without severely patching wcslib. - pywcs will now run without pyfits, though the SIP and distortion lookup table functionality is unavailable. BUG FIXES: - The dimensions of the cd and pc matrices were formerly always returned as 2x2. They now are sized according to naxis. MISCELLANEOUS: - Lots of new unit tests - Setting wcs.wcs.cunit will now verify that the values are valid unit strings. Version 1.10 ============ - Adds a UnitConversion class, which gives access to wcslib's unit conversion functionality. Given two convertible unit strings, pywcs can convert arrays of values from one to the other. - Now uses wcslib 4.7 - Changes to some wcs values would not always calculate secondary values. Version 1.9 =========== - Support binary image arrays and pixel list format WCS by presenting a way to call wcslib's wcsbth() - Updated underlying wcslib to version 4.5, which fixes the following: - Fixed the interpretation of VELREF when translating AIPS-convention spectral types. Such translation is now handled by a new special- purpose function, spcaips(). The wcsprm struct has been augmented with an entry for velref which is filled by wcspih() and wcsbth(). Previously, selection by VELREF of the radio or optical velocity convention for type VELO was not properly handled. BUGS: - The "pc" member is now available with a default "raw" Wcsprm object. - Make properties that return arrays read-only, since modifying a (mutable) array could result in secondary values not being recomputed based on those changes. - float properties can now be set using int values Version 1.3a1 ============= Earlier versions of pywcs had two versions of every conversion method: X(...) -- treats the origin of pixel coordinates at (0, 0) X_fits(...) -- treats the origin of pixel coordinates at (1, 1) From version 1.3 onwards, there is only one method for each conversion, with an 'origin' argument: - 0: places the origin at (0, 0), which is the C/Numpy convention. - 1: places the origin at (1, 1), which is the Fortran/FITS convention. pywcs-1.12/defsetup.py0000644001153600020070000003073012310355627017043 0ustar cslocumSTSCI\science00000000000000#!/usr/bin/env python from __future__ import with_statement, division # confidence high CONTACT = "Michael Droettboom" EMAIL = "mdroe@stsci.edu" from distutils.core import setup, Extension from distutils.dist import Distribution from distutils.errors import DistutilsError import glob from os.path import join import os.path import shutil import sys if os.path.exists("pywcs"): srcroot = 'pywcs' else: srcroot = '.' sys.path.append(join('.', srcroot, "lib/pywcs")) sys.path.append('.') def b(s): return s.encode('ascii') if sys.version_info[0] >= 3: def string_escape(s): s = s.decode('ascii').encode('ascii', 'backslashreplace') s = s.replace(b('\n'), b('\\n')) return s.decode('ascii') from io import StringIO string_types = (str, bytes) else: def string_escape(s): return s.encode('string_escape') from cStringIO import StringIO string_types = (str, unicode) ###################################################################### # CONFIGURATION # BUILD may be 'debug', 'profile', or 'release' BUILD = 'release' OPENMP = False ###################################################################### # Helper class def write_if_different(filename, data): data = data.encode('ascii') if os.path.exists(filename): with open(filename, 'rb') as fd: original_data = fd.read() else: original_data = None if original_data != data: with open(filename, 'wb') as fd: fd.write(data) ###################################################################### # NUMPY try: import numpy except ImportError: print("numpy must be installed to build pywcs.") print("ABORTING.") raise major, minor, rest = numpy.__version__.split(".", 2) if (int(major), int(minor)) < (1, 3): print("numpy version 1.3 or later must be installed to build pywcs.") print("ABORTING.") raise ImportError try: numpy_include = numpy.get_include() except AttributeError: numpy_include = numpy.get_numpy_include() ###################################################################### # WCSLIB WCSVERSION = "4.10" WCSLIB = "wcslib" # Path to wcslib WCSLIB_PATCHED = "wcslib" WCSLIBC = join(WCSLIB_PATCHED, "C") # Path to wcslib source files WCSFILES = [ # List of wcslib files to compile 'flexed/wcsbth.c', 'flexed/wcspih.c', 'flexed/wcsulex.c', 'flexed/wcsutrn.c', 'cel.c', 'lin.c', 'log.c', 'prj.c', 'spc.c', 'sph.c', 'spx.c', 'tab.c', 'wcs.c', 'wcserr.c', 'wcsfix.c', 'wcshdr.c', 'wcsprintf.c', 'wcsunits.c', 'wcsutil.c'] WCSFILES = [join(WCSLIBC, x) for x in WCSFILES] ###################################################################### # WCSLIB CONFIGURATION # The only configuration parameter needed at compile-time is how to # specify a 64-bit signed integer. Python's ctypes module can get us # that information, but it is only available in Python 2.5 or later. # If we can't be absolutely certain, we default to "long long int", # which is correct on most platforms (x86, x86_64). If we find # platforms where this heuristic doesn't work, we may need to hardcode # for them. def determine_64_bit_int(): try: try: import ctypes except ImportError: raise ValueError() if ctypes.sizeof(ctypes.c_longlong) == 8: return "long long int" elif ctypes.sizeof(ctypes.c_long) == 8: return "long int" elif ctypes.sizeof(ctypes.c_int) == 8: return "int" else: raise ValueError() except ValueError: return "long long int" h_file = StringIO() h_file.write(""" /* WCSLIB library version number. */ #define WCSLIB_VERSION %s /* 64-bit integer data type. */ #define WCSLIB_INT64 %s /* Windows needs some other defines */ /* I think the only one we need is _WIN32, but the others don't hurt - Mark S. 2012-02-14 */ #if defined(_WIN32) || defined(_MSC_VER) || defined(__MINGW32__) || defined (__MINGW64__) /* */ #ifndef YY_NO_UNISTD_H #define YY_NO_UNISTD_H #endif #ifndef _CRT_SECURE_NO_WARNINGS #define _CRT_SECURE_NO_WARNINGS #endif #ifndef _NO_OLDNAMES /* for mingw32 */ #define _NO_OLDNAMES #endif #ifndef NO_OLDNAMES /* for mingw64 */ #define NO_OLDNAMES #endif #ifndef __STDC__ /* for MS Visual C */ #define __STDC__ 1 #endif #endif """ % (WCSVERSION, determine_64_bit_int())) write_if_different(join(srcroot, 'src', 'wcsconfig.h'), h_file.getvalue()) ###################################################################### # GENERATE DOCSTRINGS IN C docstrings = {} with open(join(srcroot, 'doc', 'docstrings.py'), 'rb') as fd: docstrings_content = fd.read() exec(docstrings_content, docstrings) keys = [key for key in docstrings.keys() if not key.startswith('__') and type(key) in string_types] keys.sort() for key in keys: docstrings[key] = docstrings[key].encode('utf8').lstrip() h_file = StringIO() h_file.write("""/* DO NOT EDIT! This file is autogenerated by setup.py. To edit its contents, edit doc/docstrings.py */ #ifndef __DOCSTRINGS_H__ #define __DOCSTRINGS_H__ void fill_docstrings(void); """) for key in keys: val = docstrings[key] h_file.write('extern char doc_%s[%d];\n' % (key, len(val))) h_file.write("\n#endif\n\n") write_if_different(join(srcroot, 'src', 'docstrings.h'), h_file.getvalue()) c_file = StringIO() c_file.write("""/* DO NOT EDIT! This file is autogenerated by setup.py. To edit its contents, edit doc/docstrings.py The weirdness here with strncpy is because some C compilers, notably MSVC, do not support string literals greater than 256 characters. */ #include #include "docstrings.h" """) for key in keys: val = docstrings[key] c_file.write('char doc_%s[%d];\n' % (key, len(val))) c_file.write("\nvoid fill_docstrings(void)\n{\n") for key in keys: val = docstrings[key] # For portability across various compilers, we need to fill the # docstrings in 256-character chunks for i in range(0, len(val), 256): chunk = string_escape(val[i:i+256]).replace('"', '\\"') c_file.write(' strncpy(doc_%s + %d, "%s", %d);\n' % ( key, i, chunk, min(len(val) - i, 256))) c_file.write("\n") c_file.write("\n}\n\n") write_if_different(join(srcroot, 'src', 'docstrings.c'), c_file.getvalue()) ###################################################################### # PYWCS-SPECIFIC AND WRAPPER SOURCE FILES PYWCS_VERSION = '1.11' VERSION = '%s-%s' % (PYWCS_VERSION, WCSVERSION) PYWCS_SOURCES = [ # List of pywcs files to compile 'distortion.c', 'distortion_wrap.c', 'docstrings.c', 'pipeline.c', 'pyutil.c', 'pywcs.c', 'pywcs_api.c', 'sip.c', 'sip_wrap.c', 'str_list_proxy.c', 'util.c', 'wcslib_wrap.c', 'wcslib_tabprm_wrap.c', 'wcslib_units_wrap.c', 'wcslib_wtbarr_wrap.c'] PYWCS_SOURCES = [join('src', x) for x in PYWCS_SOURCES] ###################################################################### # DISTUTILS SETUP def get_distutils_option(option, commands): """ Returns the value of the given distutils option. Parameters ---------- option : str The name of the option commands : list of str The list of commands on which this option is available Returns ------- val : str or None the value of the given distutils option. If the option is not set, returns None. """ # Pre-parse the Distutils command-line options and config files to # if the option is set. dist = Distribution() try: dist.parse_config_files() dist.parse_command_line() except DistutilsError: # Let distutils handle this itself return None except AttributeError: # This seems to get thrown for ./setup.py --help return None for cmd in commands: if cmd in dist.commands: break else: return None for cmd in commands: cmd_opts = dist.get_option_dict(cmd) if option in cmd_opts: return cmd_opts[option][1] else: return None def adjust_compiler(): """ This function detects broken compilers and switches to another. If the environment variable CC is explicitly set, or a compiler is specified on the commandline, no override is performed -- the purpose here is to only override a default compiler. The specific compilers with problems are: * The default compiler in XCode-4.2, llvm-gcc-4.2, segfaults when compiling wcslib. The set of broken compilers can be updated by changing the compiler_mapping variable. It is a list of 2-tuples where the first in the pair is a regular expression matching the version of the broken compiler, and the second is the compiler to change to. """ if 'CC' in os.environ: return if get_distutils_option( 'compiler', ['build', 'build_ext', 'build_clib']) is not None: return from distutils import ccompiler import subprocess import re compiler_mapping = [ ('i686-apple-darwin[0-9]*-llvm-gcc-4.2', 'clang') ] c = ccompiler.new_compiler() # The MSVC ccompiler class doesn't have a `compiler` member. if not hasattr(c, 'compiler'): return process = subprocess.Popen( c.compiler + ['--version'], stdout=subprocess.PIPE) output = process.communicate()[0].strip().decode('ascii') version = output.split()[0] for broken, fixed in compiler_mapping: if re.match(broken, version): os.environ['CC'] = fixed break adjust_compiler() libraries = [] define_macros = [('ECHO', None), ('WCSTRIG_MACRO', None), ('PYWCS_BUILD', None), ('_GNU_SOURCE', None)] undef_macros = [] extra_compile_args = [] extra_link_args = [] if BUILD.lower() == 'debug': define_macros.append(('DEBUG', None)) undef_macros.append('NDEBUG') if not sys.platform.startswith('sun') and \ not sys.platform == 'win32': extra_compile_args.extend(["-fno-inline", "-O0", "-g"]) elif BUILD.lower() == 'profile': define_macros.append(('NDEBUG', None)) undef_macros.append('DEBUG') if not sys.platform.startswith('sun'): extra_compile_args.extend(["-O3", "-g"]) elif BUILD.lower() == 'release': # Define ECHO as nothing to prevent spurious newlines from # printing within the libwcs parser define_macros.append(('NDEBUG', None)) undef_macros.append('DEBUG') else: raise ValueError("BUILD should be one of 'debug', 'profile', or 'release'") if sys.platform == 'win32': # we are also writing these into wcsconfig.h, but that include # file is not used by wcslib define_macros.extend([ ('YY_NO_UNISTD_H', None), ('_CRT_SECURE_NO_WARNINGS', None), ('_NO_OLDNAMES', None), # for mingw32 ('NO_OLDNAMES', None), # for mingw64 ('__STDC__', None) # for MSVC ]) if sys.platform.startswith('linux'): define_macros.append(('HAVE_SINCOS', None)) if not sys.platform.startswith('sun') and \ not sys.platform == 'win32': if OPENMP: extra_compile_args.append('-fopenmp') libraries.append('gomp') else: extra_compile_args.extend(['-Wno-unknown-pragmas']) PYWCS_EXTENSIONS = [ Extension('pywcs._pywcs', WCSFILES + PYWCS_SOURCES, include_dirs = [numpy_include, join(srcroot, WCSLIBC), WCSLIBC, join(srcroot, "src") ], define_macros=define_macros, undef_macros=undef_macros, extra_compile_args=extra_compile_args, extra_link_args=extra_link_args, libraries=libraries ) ] pkg = ["pywcs", "pywcs.tests"] setupargs = { 'version' : VERSION, 'description': "Python wrappers to WCSLIB", 'author' : CONTACT, 'author_email': EMAIL, 'url' : "http://projects.scipy.org/astropy/astrolib/wiki/WikiStart", 'platforms' : ["unix","windows"], 'ext_modules' : PYWCS_EXTENSIONS, 'data_files' : [ ( 'pywcs/include', ['src/*.h']), ( 'pywcs/include/wcslib', [ WCSLIBC + '/*.h'] ), ( 'pywcs/tests/maps', ['lib/pywcs/tests/maps/*.hdr']), ( 'pywcs/tests/nrao', ['lib/pywcs/tests/nrao/*.hdr']), ( 'pywcs/tests/spectra', ['lib/pywcs/tests/spectra/*.hdr']), ( 'pywcs/tests/data', ['lib/pywcs/tests/data/*.hdr', 'lib/pywcs/tests/data/*.fits']) ], 'package_dir' : { 'pywcs' : 'lib/pywcs', 'pywcs.tests' : 'lib/pywcs/tests'}, } pywcs-1.12/distribute_setup.py0000644001153600020070000003661512310355627020632 0ustar cslocumSTSCI\science00000000000000#!python """Bootstrap distribute installation If you want to use setuptools in your package's setup.py, just include this file in the same directory with it, and add this to the top of your setup.py:: from distribute_setup import use_setuptools use_setuptools() If you want to require a specific version of setuptools, set a download mirror, or use an alternate download directory, you can do so by supplying the appropriate options to ``use_setuptools()``. This file can also be run as a script to install or upgrade setuptools. """ import os import sys import time import fnmatch import tempfile import tarfile from distutils import log try: from site import USER_SITE except ImportError: USER_SITE = None try: import subprocess def _python_cmd(*args): args = (sys.executable,) + args return subprocess.call(args) == 0 except ImportError: # will be used for python 2.3 def _python_cmd(*args): args = (sys.executable,) + args # quoting arguments if windows if sys.platform == 'win32': def quote(arg): if ' ' in arg: return '"%s"' % arg return arg args = [quote(arg) for arg in args] return os.spawnl(os.P_WAIT, sys.executable, *args) == 0 DEFAULT_VERSION = "0.6.19" DEFAULT_URL = "http://pypi.python.org/packages/source/d/distribute/" SETUPTOOLS_FAKED_VERSION = "0.6c11" SETUPTOOLS_PKG_INFO = """\ Metadata-Version: 1.0 Name: setuptools Version: %s Summary: xxxx Home-page: xxx Author: xxx Author-email: xxx License: xxx Description: xxx """ % SETUPTOOLS_FAKED_VERSION def _install(tarball): # extracting the tarball tmpdir = tempfile.mkdtemp() log.warn('Extracting in %s', tmpdir) old_wd = os.getcwd() try: os.chdir(tmpdir) tar = tarfile.open(tarball) _extractall(tar) tar.close() # going in the directory subdir = os.path.join(tmpdir, os.listdir(tmpdir)[0]) os.chdir(subdir) log.warn('Now working in %s', subdir) # installing log.warn('Installing Distribute') if not _python_cmd('setup.py', 'install'): log.warn('Something went wrong during the installation.') log.warn('See the error message above.') finally: os.chdir(old_wd) def _build_egg(egg, tarball, to_dir): # extracting the tarball tmpdir = tempfile.mkdtemp() log.warn('Extracting in %s', tmpdir) old_wd = os.getcwd() try: os.chdir(tmpdir) tar = tarfile.open(tarball) _extractall(tar) tar.close() # going in the directory subdir = os.path.join(tmpdir, os.listdir(tmpdir)[0]) os.chdir(subdir) log.warn('Now working in %s', subdir) # building an egg log.warn('Building a Distribute egg in %s', to_dir) _python_cmd('setup.py', '-q', 'bdist_egg', '--dist-dir', to_dir) finally: os.chdir(old_wd) # returning the result log.warn(egg) if not os.path.exists(egg): raise IOError('Could not build the egg.') def _do_download(version, download_base, to_dir, download_delay): egg = os.path.join(to_dir, 'distribute-%s-py%d.%d.egg' % (version, sys.version_info[0], sys.version_info[1])) if not os.path.exists(egg): tarball = download_setuptools(version, download_base, to_dir, download_delay) _build_egg(egg, tarball, to_dir) sys.path.insert(0, egg) import setuptools setuptools.bootstrap_install_from = egg def use_setuptools(version=DEFAULT_VERSION, download_base=DEFAULT_URL, to_dir=os.curdir, download_delay=15, no_fake=True): # making sure we use the absolute path to_dir = os.path.abspath(to_dir) was_imported = 'pkg_resources' in sys.modules or \ 'setuptools' in sys.modules try: try: import pkg_resources if not hasattr(pkg_resources, '_distribute'): if not no_fake: _fake_setuptools() raise ImportError except ImportError: return _do_download(version, download_base, to_dir, download_delay) try: pkg_resources.require("distribute>="+version) return except pkg_resources.VersionConflict: e = sys.exc_info()[1] if was_imported: sys.stderr.write( "The required version of distribute (>=%s) is not available,\n" "and can't be installed while this script is running. Please\n" "install a more recent version first, using\n" "'easy_install -U distribute'." "\n\n(Currently using %r)\n" % (version, e.args[0])) sys.exit(2) else: del pkg_resources, sys.modules['pkg_resources'] # reload ok return _do_download(version, download_base, to_dir, download_delay) except pkg_resources.DistributionNotFound: return _do_download(version, download_base, to_dir, download_delay) finally: if not no_fake: _create_fake_setuptools_pkg_info(to_dir) def download_setuptools(version=DEFAULT_VERSION, download_base=DEFAULT_URL, to_dir=os.curdir, delay=15): """Download distribute from a specified location and return its filename `version` should be a valid distribute version number that is available as an egg for download under the `download_base` URL (which should end with a '/'). `to_dir` is the directory where the egg will be downloaded. `delay` is the number of seconds to pause before an actual download attempt. """ # making sure we use the absolute path to_dir = os.path.abspath(to_dir) try: from urllib.request import urlopen except ImportError: from urllib2 import urlopen tgz_name = "distribute-%s.tar.gz" % version url = download_base + tgz_name saveto = os.path.join(to_dir, tgz_name) src = dst = None if not os.path.exists(saveto): # Avoid repeated downloads try: log.warn("Downloading %s", url) src = urlopen(url) # Read/write all in one block, so we don't create a corrupt file # if the download is interrupted. data = src.read() dst = open(saveto, "wb") dst.write(data) finally: if src: src.close() if dst: dst.close() return os.path.realpath(saveto) def _no_sandbox(function): def __no_sandbox(*args, **kw): try: from setuptools.sandbox import DirectorySandbox if not hasattr(DirectorySandbox, '_old'): def violation(*args): pass DirectorySandbox._old = DirectorySandbox._violation DirectorySandbox._violation = violation patched = True else: patched = False except ImportError: patched = False try: return function(*args, **kw) finally: if patched: DirectorySandbox._violation = DirectorySandbox._old del DirectorySandbox._old return __no_sandbox def _patch_file(path, content): """Will backup the file then patch it""" existing_content = open(path).read() if existing_content == content: # already patched log.warn('Already patched.') return False log.warn('Patching...') _rename_path(path) f = open(path, 'w') try: f.write(content) finally: f.close() return True _patch_file = _no_sandbox(_patch_file) def _same_content(path, content): return open(path).read() == content def _rename_path(path): new_name = path + '.OLD.%s' % time.time() log.warn('Renaming %s into %s', path, new_name) os.rename(path, new_name) return new_name def _remove_flat_installation(placeholder): if not os.path.isdir(placeholder): log.warn('Unkown installation at %s', placeholder) return False found = False for file in os.listdir(placeholder): if fnmatch.fnmatch(file, 'setuptools*.egg-info'): found = True break if not found: log.warn('Could not locate setuptools*.egg-info') return log.warn('Removing elements out of the way...') pkg_info = os.path.join(placeholder, file) if os.path.isdir(pkg_info): patched = _patch_egg_dir(pkg_info) else: patched = _patch_file(pkg_info, SETUPTOOLS_PKG_INFO) if not patched: log.warn('%s already patched.', pkg_info) return False # now let's move the files out of the way for element in ('setuptools', 'pkg_resources.py', 'site.py'): element = os.path.join(placeholder, element) if os.path.exists(element): _rename_path(element) else: log.warn('Could not find the %s element of the ' 'Setuptools distribution', element) return True _remove_flat_installation = _no_sandbox(_remove_flat_installation) def _after_install(dist): log.warn('After install bootstrap.') placeholder = dist.get_command_obj('install').install_purelib _create_fake_setuptools_pkg_info(placeholder) def _create_fake_setuptools_pkg_info(placeholder): if not placeholder or not os.path.exists(placeholder): log.warn('Could not find the install location') return pyver = '%s.%s' % (sys.version_info[0], sys.version_info[1]) setuptools_file = 'setuptools-%s-py%s.egg-info' % \ (SETUPTOOLS_FAKED_VERSION, pyver) pkg_info = os.path.join(placeholder, setuptools_file) if os.path.exists(pkg_info): log.warn('%s already exists', pkg_info) return log.warn('Creating %s', pkg_info) f = open(pkg_info, 'w') try: f.write(SETUPTOOLS_PKG_INFO) finally: f.close() pth_file = os.path.join(placeholder, 'setuptools.pth') log.warn('Creating %s', pth_file) f = open(pth_file, 'w') try: f.write(os.path.join(os.curdir, setuptools_file)) finally: f.close() _create_fake_setuptools_pkg_info = _no_sandbox(_create_fake_setuptools_pkg_info) def _patch_egg_dir(path): # let's check if it's already patched pkg_info = os.path.join(path, 'EGG-INFO', 'PKG-INFO') if os.path.exists(pkg_info): if _same_content(pkg_info, SETUPTOOLS_PKG_INFO): log.warn('%s already patched.', pkg_info) return False _rename_path(path) os.mkdir(path) os.mkdir(os.path.join(path, 'EGG-INFO')) pkg_info = os.path.join(path, 'EGG-INFO', 'PKG-INFO') f = open(pkg_info, 'w') try: f.write(SETUPTOOLS_PKG_INFO) finally: f.close() return True _patch_egg_dir = _no_sandbox(_patch_egg_dir) def _before_install(): log.warn('Before install bootstrap.') _fake_setuptools() def _under_prefix(location): if 'install' not in sys.argv: return True args = sys.argv[sys.argv.index('install')+1:] for index, arg in enumerate(args): for option in ('--root', '--prefix'): if arg.startswith('%s=' % option): top_dir = arg.split('root=')[-1] return location.startswith(top_dir) elif arg == option: if len(args) > index: top_dir = args[index+1] return location.startswith(top_dir) if arg == '--user' and USER_SITE is not None: return location.startswith(USER_SITE) return True def _fake_setuptools(): log.warn('Scanning installed packages') try: import pkg_resources except ImportError: # we're cool log.warn('Setuptools or Distribute does not seem to be installed.') return ws = pkg_resources.working_set try: setuptools_dist = ws.find(pkg_resources.Requirement.parse('setuptools', replacement=False)) except TypeError: # old distribute API setuptools_dist = ws.find(pkg_resources.Requirement.parse('setuptools')) if setuptools_dist is None: log.warn('No setuptools distribution found') return # detecting if it was already faked setuptools_location = setuptools_dist.location log.warn('Setuptools installation detected at %s', setuptools_location) # if --root or --preix was provided, and if # setuptools is not located in them, we don't patch it if not _under_prefix(setuptools_location): log.warn('Not patching, --root or --prefix is installing Distribute' ' in another location') return # let's see if its an egg if not setuptools_location.endswith('.egg'): log.warn('Non-egg installation') res = _remove_flat_installation(setuptools_location) if not res: return else: log.warn('Egg installation') pkg_info = os.path.join(setuptools_location, 'EGG-INFO', 'PKG-INFO') if (os.path.exists(pkg_info) and _same_content(pkg_info, SETUPTOOLS_PKG_INFO)): log.warn('Already patched.') return log.warn('Patching...') # let's create a fake egg replacing setuptools one res = _patch_egg_dir(setuptools_location) if not res: return log.warn('Patched done.') _relaunch() def _relaunch(): log.warn('Relaunching...') # we have to relaunch the process # pip marker to avoid a relaunch bug if sys.argv[:3] == ['-c', 'install', '--single-version-externally-managed']: sys.argv[0] = 'setup.py' args = [sys.executable] + sys.argv sys.exit(subprocess.call(args)) def _extractall(self, path=".", members=None): """Extract all members from the archive to the current working directory and set owner, modification time and permissions on directories afterwards. `path' specifies a different directory to extract to. `members' is optional and must be a subset of the list returned by getmembers(). """ import copy import operator from tarfile import ExtractError directories = [] if members is None: members = self for tarinfo in members: if tarinfo.isdir(): # Extract directories with a safe mode. directories.append(tarinfo) tarinfo = copy.copy(tarinfo) tarinfo.mode = 448 # decimal for oct 0700 self.extract(tarinfo, path) # Reverse sort directories. if sys.version_info < (2, 4): def sorter(dir1, dir2): return cmp(dir1.name, dir2.name) directories.sort(sorter) directories.reverse() else: directories.sort(key=operator.attrgetter('name'), reverse=True) # Set correct owner, mtime and filemode on directories. for tarinfo in directories: dirpath = os.path.join(path, tarinfo.name) try: self.chown(tarinfo, dirpath) self.utime(tarinfo, dirpath) self.chmod(tarinfo, dirpath) except ExtractError: e = sys.exc_info()[1] if self.errorlevel > 1: raise else: self._dbg(1, "tarfile: %s" % e) def main(argv, version=DEFAULT_VERSION): """Install or upgrade setuptools and EasyInstall""" tarball = download_setuptools() _install(tarball) if __name__ == '__main__': main(sys.argv[1:]) pywcs-1.12/doc/0000755001153600020070000000000012310355732015411 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/doc/docstrings.py0000644001153600020070000016202512310355626020152 0ustar cslocumSTSCI\science00000000000000# Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) # Redistribution and use in source and binary forms, with or without # modification, are permitted provided that the following conditions are met: # 1. Redistributions of source code must retain the above copyright # notice, this list of conditions and the following disclaimer. # 2. Redistributions in binary form must reproduce the above # copyright notice, this list of conditions and the following # disclaimer in the documentation and/or other materials provided # with the distribution. # 3. The name of AURA and its representatives may not be used to # endorse or promote products derived from this software without # specific prior written permission. # THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED # WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF # MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE # DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, # INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, # BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS # OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND # ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR # TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE # USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH # DAMAGE. ########################################################################### from __future__ import division # confidence high del division # We don't want the "division" symbol in the namespace, since it # should have only docstrings # It gets to be really tedious to type long docstrings in ANSI C # syntax (since multi-line string literals are not valid). # Therefore, the docstrings are written here in doc/docstrings.py, # which are then converted by setup.py into docstrings.h, which is # included by pywcs.c import _docutil as __ a = """ ``double array[a_order+1][a_order+1]`` The `SIP`_ ``A_i_j`` matrix used for pixel to focal plane transformation. Its values may be changed in place, but it may not be resized, without creating a new `~pywcs.Sip` object. """ a_order = """ ``int`` (read-only) The order of the polynomial in the `SIP`_ ``A_i_j`` array (``A_ORDER``). """ all_pix2sky = """ all_pix2sky(pixcrd, origin) -> ``double array[ncoord][nelem]`` Transforms pixel coordinates to sky coordinates by doing all of the following: - Detector to image plane correction (optionally) - SIP distortion correction (optionally) - Paper IV distortion correction (optionally) - wcslib WCS transformation The first three (the distortion corrections) are done in parallel. - *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates. %s Returns an array of sky coordinates. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `ValueError`: Invalid coordinate transformation parameters. - `ValueError`: x- and y-coordinate arrays are not the same size. - `InvalidTransformError`: Invalid coordinate transformation. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. """ % __.ORIGIN() alt = """ ``str`` Character code for alternate coordinate descriptions. For example, the ``"a"`` in keyword names such as ``CTYPEia``. This is a space character for the primary coordinate description, or one of the 26 upper-case letters, A-Z. """ ap = """ ``double array[ap_order+1][ap_order+1]`` The `SIP`_ ``AP_i_j`` matrix used for focal plane to pixel transformation. Its values may be changed in place, but it may not be resized, without creating a new `~pywcs.Sip` object. """ ap_order = """ ``int`` (read-only) The order of the polynomial in the `SIP`_ ``AP_i_j`` array (``AP_ORDER``). """ axis_types = """ ``int array[naxis]`` An array of four-digit type codes for each axis. - First digit (i.e. 1000s): - 0: Non-specific coordinate type. - 1: Stokes coordinate. - 2: Celestial coordinate (including ``CUBEFACE``). - 3: Spectral coordinate. - Second digit (i.e. 100s): - 0: Linear axis. - 1: Quantized axis (``STOKES``, ``CUBEFACE``). - 2: Non-linear celestial axis. - 3: Non-linear spectral axis. - 4: Logarithmic axis. - 5: Tabular axis. - Third digit (i.e. 10s): - 0: Group number, e.g. lookup table number - The fourth digit is used as a qualifier depending on the axis type. - For celestial axes: - 0: Longitude coordinate. - 1: Latitude coordinate. - 2: ``CUBEFACE`` number. - For lookup tables: the axis number in a multidimensional table. ``CTYPEia`` in ``"4-3"`` form with unrecognized algorithm code will have its type set to -1 and generate an error. """ b = """ ``double array[b_order+1][b_order+1]`` The `SIP`_ ``B_i_j`` matrix used for pixel to focal plane transformation. Its values may be changed in place, but it may not be resized, without creating a new `~pywcs.Sip` object. """ b_order = """ ``int`` (read-only) The order of the polynomial in the `SIP`_ ``B_i_j`` array (``B_ORDER``). """ bp = """ ``double array[bp_order+1][bp_order+1]`` The `SIP`_ ``BP_i_j`` matrix used for focal plane to pixel transformation. Its values may be changed in place, but it may not be resized, without creating a new `~pywcs.Sip` object. """ bp_order = """ ``int`` (read-only) The order of the polynomial in the `SIP`_ ``BP_i_j`` array (``BP_ORDER``). """ cd = """ ``double array[naxis][naxis]`` The ``CDi_ja`` linear transformation matrix. For historical compatibility, three alternate specifications of the linear transforations are available in wcslib. The canonical ``PCi_ja`` with ``CDELTia``, ``CDi_ja``, and the deprecated ``CROTAia`` keywords. Although the latter may not formally co-exist with ``PCi_ja``, the approach here is simply to ignore them if given in conjunction with ``PCi_ja``. `~pywcs.Wcsprm.has_pc`, `~pywcs.Wcsprm.has_cd` and `~pywcs.Wcsprm.has_crota` can be used to determine which of these alternatives are present in the header. These alternate specifications of the linear transformation matrix are translated immediately to ``PCi_ja`` by `~pywcs.Wcsprm.set` and are nowhere visible to the lower-level routines. In particular, `~pywcs.Wcsprm.set` resets `~pywcs.Wcsprm.cdelt` to unity if ``CDi_ja`` is present (and no ``PCi_ja``). If no ``CROTAia`` is associated with the latitude axis, `set` reverts to a unity ``PCi_ja`` matrix. """ cdelt = """ ``double array[naxis]`` Coordinate increments (``CDELTia``) for each coord axis. If a ``CDi_ja`` linear transformation matrix is present, a warning is raised and `~pywcs.Wcsprm.cdelt` is ignored. The ``CDi_ja`` matrix may be deleted by:: del wcs.wcs.cd An undefined value is represented by NaN. """ cel_offset = """ ``boolean`` If `True`, an offset will be applied to ``(x, y)`` to force ``(x,y) = (0,0)`` at the fiducial point, (phi_0, theta_0). Default is `False`. """ celfix = """ Translates AIPS-convention celestial projection types, ``-NCP`` and ``-GLS``. Returns ``0`` for success; ``-1`` if no change required. """ cname = """ ``list of strings`` A list of the coordinate axis names, from ``CNAMEia``. """ colax = """ ``int array[naxis]`` An array recording the column numbers for each axis in a pixel list. """ colnum = """ ``int`` Where the coordinate representation is associated with an image-array column in a FITS binary table, this property may be used to record the relevant column number. It should be set to zero for an image header or pixel list. """ convert = """ convert(array) Perform the unit conversion on the elements of the given *array*, returning an array of the same shape. """ coord = """ ``double array[K_M]...[K_2][K_1][M]`` The tabular coordinate array, with the dimensions:: (K_M, ... K_2, K_1, M) (see `~pywcs._pywcs.Tabprm.K`) i.e. with the `M` dimension varying fastest so that the `M` elements of a coordinate vector are stored contiguously in memory. """ copy = """ Creates a deep copy of the WCS object. """ cpdis1 = """ `~pywcs.DistortionLookupTable` The pre-linear transformation distortion lookup table, ``CPDIS1``. """ cpdis2 = """ `~pywcs.DistortionLookupTable` The pre-linear transformation distortion lookup table, ``CPDIS2``. """ crder = """ ``double array[naxis]`` The random error in each coordinate axis, ``CRDERia``. An undefined value is represented by NaN. """ crota = """ ``double array[naxis]`` ``CROTAia`` keyvalues for each coordinate axis. For historical compatibility, three alternate specifications of the linear transforations are available in wcslib. The canonical ``PCi_ja`` with ``CDELTia``, ``CDi_ja``, and the deprecated ``CROTAia`` keywords. Although the latter may not formally co-exist with ``PCi_ja``, the approach here is simply to ignore them if given in conjunction with ``PCi_ja``. `~pywcs.Wcsprm.has_pc`, `~pywcs.Wcsprm.has_cd` and `~pywcs.Wcsprm.has_crota` can be used to determine which of these alternatives are present in the header. These alternate specifications of the linear transformation matrix are translated immediately to ``PCi_ja`` by `~pywcs.Wcsprm.set` and are nowhere visible to the lower-level routines. In particular, `~pywcs.Wcsprm.set` resets `~pywcs.Wcsprm.cdelt` to unity if ``CDi_ja`` is present (and no ``PCi_ja``). If no ``CROTAia`` is associated with the latitude axis, `set` reverts to a unity ``PCi_ja`` matrix. """ crpix = """ ``double array[naxis]`` Coordinate reference pixels (``CRPIXja``) for each pixel axis. """ crval = """ ``double array[naxis]`` Coordinate reference values (``CRVALia``) for each coordinate axis. """ crval_tabprm = """ ``double array[M]`` Array whose elements contain the index value for the reference pixel for each of the tabular coordinate axes. """ csyer = """ ``double array[naxis]`` The systematic error in the coordinate value axes, ``CSYERia``. An undefined value is represented by NaN. """ ctype = """ ``list of strings[naxis]`` List of ``CTYPEia`` keyvalues. The `~pywcs.Wcsprm.ctype` keyword values must be in upper case and there must be zero or one pair of matched celestial axis types, and zero or one spectral axis. """ cubeface = """ ``int`` Index into the ``pixcrd`` (pixel coordinate) array for the ``CUBEFACE`` axis. This is used for quadcube projections where the cube faces are stored on a separate axis. The quadcube projections (``TSC``, ``CSC``, ``QSC``) may be represented in FITS in either of two ways: - The six faces may be laid out in one plane and numbered as follows:: 0 4 3 2 1 4 3 2 5 Faces 2, 3 and 4 may appear on one side or the other (or both). The sky-to-pixel routines map faces 2, 3 and 4 to the left but the pixel-to-sky routines accept them on either side. - The ``COBE`` convention in which the six faces are stored in a three-dimensional structure using a ``CUBEFACE`` axis indexed from 0 to 5 as above. These routines support both methods; `~pywcs.Wcsprm.set` determines which is being used by the presence or absence of a ``CUBEFACE`` axis in `~pywcs.Wcsprm.ctype`. `~pywcs.Wcsprm.p2s` and `~pywcs.Wcsprm.s2p` translate the ``CUBEFACE`` axis representation to the single plane representation understood by the lower-level projection routines. """ cunit = """ ``list of strings[naxis]`` List of ``CUNITia`` keyvalues which define the units of measurement of the ``CRVALia``, ``CDELTia`` and ``CDi_ja`` keywords. As ``CUNITia`` is an optional header keyword, `~pywcs.Wcsprm.cunit` may be left blank but otherwise is expected to contain a standard units specification as defined by WCS Paper I. `~pywcs.Wcsprm.unitfix` is available to translate commonly used non-standard units specifications but this must be done as a separate step before invoking `~pywcs.Wcsprm.set`. For celestial axes, if `~pywcs.Wcsprm.cunit` is not blank, `~pywcs.Wcsprm.set` uses `wcsunits` to parse it and scale `~pywcs.Wcsprm.cdelt`, `~pywcs.Wcsprm.crval`, and `~pywcs.Wcsprm.cd` to decimal degrees. It then resets `~pywcs.Wcsprm.cunit` to ``"deg"``. For spectral axes, if `~pywcs.Wcsprm.cunit` is not blank, `~pywcs.Wcsprm.set` uses `wcsunits` to parse it and scale `~pywcs.Wcsprm.cdelt`, `~pywcs.Wcsprm.crval`, and `~pywcs.Wcsprm.cd` to SI units. It then resets `~pywcs.Wcsprm.cunit` accordingly. `~pywcs.Wcsprm.set` ignores `~pywcs.Wcsprm.cunit` for other coordinate types; `~pywcs.Wcsprm.cunit` may be used to label coordinate values. """ cylfix = """ cylfix() Fixes WCS keyvalues for malformed cylindrical projections. Returns ``0`` for success; ``-1`` if no change required. """ data = """ ``float array`` The array data for the `~pywcs.DistortionLookupTable`. """ data_wtbarr = """ ``double array`` The array data for the BINTABLE. """ dateavg = """ ``string`` Representative mid-point of the date of observation in ISO format, ``yyyy-mm-ddThh:mm:ss``. .. seealso:: `~pywcs.Wcsprm.dateobs` """ dateobs = """ ``string`` Start of the date of observation in ISO format, ``yyyy-mm-ddThh:mm:ss``. .. seealso:: `~pywcs.Wcsprm.dateavg` """ datfix = """ datfix() Translates the old ``DATE-OBS`` date format to year-2000 standard form ``(yyyy-mm-ddThh:mm:ss)`` and derives ``MJD-OBS`` from it if not already set. Alternatively, if `~pywcs.Wcsprm.mjdobs` is set and `~pywcs.Wcsprm.dateobs` isn't, then `~pywcs.Wcsprm.datfix` derives `~pywcs.Wcsprm.dateobs` from it. If both are set but disagree by more than half a day then `ValueError` is raised. Returns ``0`` for success; ``-1`` if no change required. """ delta = """ ``double array[M]`` (read-only) Array of interpolated indices into the coordinate array such that Upsilon_m, as defined in Paper III, is equal to (`~pywcs._pywcs.Tabprm.p0` [m] + 1) + delta[m]. """ det2im = """ Convert detector coordinates to image plane coordinates. """ det2im1 = """ A `~pywcs.DistortionLookupTable` object for detector to image plane correction in the *x*-axis. """ det2im2 = """ A `~pywcs.DistortionLookupTable` object for detector to image plane correction in the *y*-axis. """ dims = """ ``int array[ndim]`` (read-only) The dimensions of the tabular array `~pywcs._pywcs.Wtbarr.data`. """ DistortionLookupTable = """ DistortionLookupTable(*table*, *crpix*, *crval*, *cdelt*) - *table*: 2-dimensional array for the distortion lookup table. - *crpix*: the distortion array reference pixel (a 2-tuple) - *crval*: is the image array pixel coordinate (a 2-tuple) - *cdelt*: is the grid step size (a 2-tuple) Represents a single lookup table for a `Paper IV`_ distortion transformation. """ equinox = """ ``double`` The equinox associated with dynamical equatorial or ecliptic coordinate systems, ``EQUINOXa`` (or ``EPOCH`` in older headers). Not applicable to ICRS equatorial or ecliptic coordinates. An undefined value is represented by NaN. """ extlev = """ ``int`` (read-only) ``EXTLEV`` identifying the binary table extension. """ extnam = """ ``str`` (read-only) ``EXTNAME`` identifying the binary table extension. """ extrema = """ ``double array[K_M]...[K_2][2][M]`` (read-only) An array recording the minimum and maximum value of each element of the coordinate vector in each row of the coordinate array, with the dimensions:: (K_M, ... K_2, 2, M) (see `~pywcs._pywcs.Tabprm.K`). The minimum is recorded in the first element of the compressed K_1 dimension, then the maximum. This array is used by the inverse table lookup function to speed up table searches. """ extver = """ ``int`` (read-only) ``EXTVER`` identifying the binary table extension. """ find_all_wcs = """ find_all_wcs(relax=0, keysel=0) Find all WCS transformations in the header. - *header*: A string containing the raw FITS header data. - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to accept. See :ref:`relaxread` for details. - *keysel*: Vector of flag bits that may be used to restrict the keyword types considered: - ``WCSHDR_IMGHEAD``: Image header keywords. - ``WCSHDR_BIMGARR``: Binary table image array. - ``WCSHDR_PIXLIST``: Pixel list keywords. If zero, there is no restriction. If -1, wcspih() is called, rather than wcstbh(). Returns a list of `~pywcs._pywcs._Wcsprm` objects. """ fix = """ fix(translate_units='', naxis=0) Applies all of the corrections handled separately by `~pywcs.Wcsprm.datfix`, `~pywcs.Wcsprm.unitfix`, `~pywcs.Wcsprm.celfix`, `~pywcs.Wcsprm.spcfix` and `~pywcs.Wcsprm.cylfix`. - *translate_units*: string. Do potentially unsafe translations of non-standard unit strings. Although ``"S"`` is commonly used to represent seconds, its translation to ``"s"`` is potentially unsafe since the standard recognizes ``"S"`` formally as Siemens, however rarely that may be used. The same applies to ``"H"`` for hours (Henry), and ``"D"`` for days (Debye). This string controls what to do in such cases, and is case-insensitive. - If the string contains ``"s"``, translate ``"S"`` to ``"s"``. - If the string contains ``"h"``, translate ``"H"`` to ``"h"``. - If the string contains ``"d"``, translate ``"D"`` to ``"d"``. Thus ``''`` doesn't do any unsafe translations, whereas ``'shd'`` does all of them. - *naxis*: int array[naxis]. Image axis lengths. If this array is set to zero or ``None``, then `~pywcs.Wcsprm.cylfix` will not be invoked. Returns a dictionary containing the following keys, each referring to a status string for each of the sub-fix functions that were called: - `~pywcs.Wcsprm.datfix` - `~pywcs.Wcsprm.unitfix` - `~pywcs.Wcsprm.celfix` - `~pywcs.Wcsprm.spcfix` - `~pywcs.Wcsprm.cylfix` """ get_offset = """ get_offset(*x, y*) -> (*x, y*) Returns the offset from the distortion table for pixel point (*x, y*). """ get_cdelt = """ get_cdelt() -> double array[naxis] Coordinate increments (``CDELTia``) for each coord axis. Returns the ``CDELT`` offsets in read-only form. Unlike the `~pywcs.Wcsprm.cdelt` property, this works even when the header specifies the linear transformation matrix in one of the alternative ``CDi_ja`` or ``CROTAia`` forms. This is useful when you want access to the linear transformation matrix, but don't care how it was specified in the header. """ get_pc = """ get_pc() -> double array[naxis][naxis] Returns the ``PC`` matrix in read-only form. Unlike the `~pywcs.Wcsprm.pc` property, this works even when the header specifies the linear transformation matrix in one of the alternative ``CDi_ja`` or ``CROTAia`` forms. This is useful when you want access to the linear transformation matrix, but don't care how it was specified in the header. """ get_ps = """ get_ps() -> list of tuples Returns ``PSi_ma`` keywords for each *i* and *m*. Returned as a list of tuples of the form (*i*, *m*, *value*): - *i*: int. Axis number, as in ``PSi_ma``, (i.e. 1-relative) - *m*: int. Parameter number, as in ``PSi_ma``, (i.e. 0-relative) - *value*: string. Parameter value. .. seealso:: `~pywcs.Wcsprm.set_ps` """ get_pv = """ get_pv() -> list of tuples Returns ``PVi_ma`` keywords for each *i* and *m*. Returned as a list of tuples of the form (*i*, *m*, *value*): - *i*: int. Axis number, as in ``PVi_ma``, (i.e. 1-relative) - *m*: int. Parameter number, as in ``PVi_ma``, (i.e. 0-relative) - *value*: string. Parameter value. Note that, if they were not given, `~pywcs.Wcsprm.set` resets the entries for ``PVi_1a``, ``PVi_2a``, ``PVi_3a``, and ``PVi_4a`` for longitude axis *i* to match (``phi_0``, ``theta_0``), the native longitude and latitude of the reference point given by ``LONPOLEa`` and ``LATPOLEa``. .. seealso:: `~pywcs.Wcsprm.set_pv` """ has_cd = """ has_cd() -> bool Returns `True` if ``CDi_ja`` is present. ``CDi_ja`` is an alternate specification of the linear transformation matrix, maintained for historical compatibility. Matrix elements in the IRAF convention are equivalent to the product ``CDi_ja = CDELTia * PCi_ja``, but the defaults differ from that of the ``PCi_ja`` matrix. If one or more ``CDi_ja`` keywords are present then all unspecified ``CDi_ja`` default to zero. If no ``CDi_ja`` (or ``CROTAia``) keywords are present, then the header is assumed to be in ``PCi_ja`` form whether or not any ``PCi_ja`` keywords are present since this results in an interpretation of ``CDELTia`` consistent with the original FITS specification. While ``CDi_ja`` may not formally co-exist with ``PCi_ja``, it may co-exist with ``CDELTia`` and ``CROTAia`` which are to be ignored. .. seealso:: `cd` """ has_cdi_ja = """ has_cdi_ja() -> bool Alias for `~pywcs.Wcsprm.has_cd`. Maintained for backward compatibility. """ has_crota = """ has_crota() -> bool Returns `True` if ``CROTAia`` is present. ``CROTAia`` is an alternate specification of the linear transformation matrix, maintained for historical compatibility. In the AIPS convention, ``CROTAia`` may only be associated with the latitude axis of a celestial axis pair. It specifies a rotation in the image plane that is applied *after* the ``CDELTia``; any other ``CROTAia`` keywords are ignored. ``CROTAia`` may not formally co-exist with ``PCi_ja``. ``CROTAia`` and ``CDELTia`` may formally co-exist with ``CDi_ja`` but if so are to be ignored. .. seealso:: `~pywcs.Wcsprm.crota` """ has_crotaia = """ has_crota_ia() -> bool Alias for `~pywcs.Wcsprm.has_crota`. Maintained for backward compatibility. """ has_pc = """ has_pc() -> bool Returns `True` if ``PCi_ja`` is present. ``PCi_ja`` is the recommended way to specify the linear transformation matrix. .. seealso:: `~pywcs.Wcsprm.pc` """ has_pci_ja = """ has_pci_ja() -> bool Alias for `~pywcs.Wcsprm.has_pc`. Maintained for backward compatibility. """ have = """ The name of the unit being converted from. This value always uses standard unit names, even if the `UnitConverter` was initialized with a non-standard unit name. """ i = """ ``int`` (read-only) Image axis number. """ imgpix_matrix = """ ``double array[2][2]`` (read-only) Inverse of the matrix containing the product of the ``CDELTia`` diagonal matrix and the ``PCi_ja`` matrix. """ is_unity = """ is_unity() -> bool Returns `True` if the linear transformation matrix (`~pywcs.Wcsprm.cd`) is unity. """ K = """ ``int array[M]`` (read-only) An array of length `M` whose elements record the lengths of the axes of the coordinate array and of each indexing vector. """ kind = """ ``str`` (read-only) Character identifying the wcstab array type: - ``'c'``: coordinate array, - ``'i'``: index vector. """ lat = """ ``int`` (read-only) The index into the sky coordinate array containing latitude values. """ latpole = """ ``double`` The native latitude of the celestial pole, ``LATPOLEa`` (deg). """ lattyp = """ ``string`` (read-only) Celestial axis type for latitude, e.g. "RA", "DEC", "GLON", "GLAT", etc. extracted from 'RA--', 'DEC-', 'GLON', 'GLAT', etc. in the first four characters of ``CTYPEia`` but with trailing dashes removed. """ lng = """ ``int`` (read-only) The index into the sky coordinate array containing longitude values. """ lngtyp = """ ``string`` (read-only) Celestial axis type for longitude, e.g. "RA", "DEC", "GLON", "GLAT", etc. extracted from 'RA--', 'DEC-', 'GLON', 'GLAT', etc. in the first four characters of ``CTYPEia`` but with trailing dashes removed. """ lonpole = """ ``double`` The native longitude of the celestial pole, ``LONPOLEa`` (deg). """ M = """ ``int`` (read-only) Number of tabular coordinate axes. """ m = """ ``int`` (read-only) Array axis number for index vectors. """ map = """ ``int array[M]`` A vector of length `~pywcs._pywcs.Tabprm.M` that defines the association between axis *m* in the *M*-dimensional coordinate array (1 <= *m* <= *M*) and the indices of the intermediate world coordinate and world coordinate arrays. When the intermediate and world coordinate arrays contain the full complement of coordinate elements in image-order, as will usually be the case, then ``map[m-1] == i-1`` for axis *i* in the *N*-dimensional image (1 <= *i* <= *N*). In terms of the FITS keywords:: map[PVi_3a - 1] == i - 1. However, a different association may result if the intermediate coordinates, for example, only contains a (relevant) subset of intermediate world coordinate elements. For example, if *M* == 1 for an image with *N* > 1, it is possible to fill the intermediate coordinates with the relevant coordinate element with ``nelem`` set to 1. In this case ``map[0] = 0`` regardless of the value of *i*. """ mix = """ mix(mixpix, mixcel, vspan, vstep, viter, world, pixcrd, origin) Given either the celestial longitude or latitude plus an element of the pixel coordinate, solves for the remaining elements by iterating on the unknown celestial coordinate element using `~pywcs.Wcsprm.s2p`. - *mixpix*: int. Which element on the pixel coordinate is given. - *mixcel*: int. Which element of the celestial coordinate is given. If mixcel* = ``1``, celestial longitude is given in ``world[self.lng]``, latitude returned in ``world[self.lat]``. If *mixcel* = ``2``, celestial latitude is given in ``world[self.lat]``, longitude returned in ``world[self.lng]``. - *vspan*: pair of floats. Solution interval for the celestial coordinate, in degrees. The ordering of the two limits is irrelevant. Longitude ranges may be specified with any convenient normalization, for example ``(-120,+120)`` is the same as ``(240,480)``, except that the solution will be returned with the same normalization, i.e. lie within the interval specified. - *vstep*: float. Step size for solution search, in degrees. If ``0``, a sensible, although perhaps non-optimal default will be used. - *viter*: int. If a solution is not found then the step size will be halved and the search recommenced. *viter* controls how many times the step size is halved. The allowed range is 5 - 10. - *world*: double array[naxis]. World coordinate elements. ``world[self.lng]`` and ``world[self.lat]`` are the celestial longitude and latitude, in degrees. Which is given and which returned depends on the value of *mixcel*. All other elements are given. The results will be written to this array in-place. - *pixcrd*: double array[naxis]. Pixel coordinate. The element indicated by *mixpix* is given and the remaining elements will be written in-place. %s Returns dictionary with the following keys: - *phi* (double array[naxis]) - *theta* (double array[naxis]) - Longitude and latitude in the native coordinate system of the projection, in degrees. - *imgcrd* (double array[naxis]) - Image coordinate elements. ``imgcrd[self.lng]`` and ``imgcrd[self.lat]`` are the projected *x*- and *y*-coordinates, in decimal degrees. - *world* (double array[naxis]) - Another reference to the *world* argument passed in. **Exceptions:** - `MemoryError` Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError` Ill-conditioned coordinate transformation parameters. - `InvalidCoordinateError`: Invalid world coordinate. - `NoSolutionError`: No solution found in the specified interval. .. seealso:: `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng` .. note:: Initially, the specified solution interval is checked to see if it's a "crossing" interval. If it isn't, a search is made for a crossing solution by iterating on the unknown celestial coordinate starting at the upper limit of the solution interval and decrementing by the specified step size. A crossing is indicated if the trial value of the pixel coordinate steps through the value specified. If a crossing interval is found then the solution is determined by a modified form of "regula falsi" division of the crossing interval. If no crossing interval was found within the specified solution interval then a search is made for a "non-crossing" solution as may arise from a point of tangency. The process is complicated by having to make allowance for the discontinuities that occur in all map projections. Once one solution has been determined others may be found by subsequent invocations of `~pywcs.Wcsprm.mix` with suitably restricted solution intervals. Note the circumstance that arises when the solution point lies at a native pole of a projection in which the pole is represented as a finite curve, for example the zenithals and conics. In such cases two or more valid solutions may exist but `~pywcs.Wcsprm.mix` only ever returns one. Because of its generality, `~pywcs.Wcsprm.mix` is very compute-intensive. For compute-limited applications, more efficient special-case solvers could be written for simple projections, for example non-oblique cylindrical projections. """ % __.ORIGIN() mjdavg = """ ``double`` Modified Julian Date ``(MJD = JD - 2400000.5)``, ``MJD-AVG``, corresponding to ``DATE-AVG``. An undefined value is represented by NaN. .. seealso:: `~pywcs.Wcsprm.mjdobs` """ mjdobs = """ ``double`` Modified Julian Date ``(MJD = JD - 2400000.5)``, ``MJD-OBS``, corresponding to ``DATE-OBS``. An undefined value is represented by NaN. .. seealso:: `~pywcs.Wcsprm.mjdavg` """ name = """ ``string`` The name given to the coordinate representation ``WCSNAMEa``. """ naxis = """ ``int`` (read-only) The number of axes (pixel and coordinate), given by the ``NAXIS`` or ``WCSAXESa`` keyvalues. The number of coordinate axes is determined at parsing time, and can not be subsequently changed. It is determined from the highest of the following: 1. ``NAXIS`` 2. ``WCSAXESa`` 3. The highest axis number in any parameterized WCS keyword. The keyvalue, as well as the keyword, must be syntactically valid otherwise it will not be considered. If none of these keyword types is present, i.e. if the header only contains auxiliary WCS keywords for a particular coordinate representation, then no coordinate description is constructed for it. This value may differ for different coordinate representations of the same image. """ nc = """ ``int`` (read-only) Total number of coordinate vectors in the coordinate array being the product K_1 * K_2 * ... * K_M. """ ndim = """ ``int`` (read-only) Expected dimensionality of the wcstab array. """ obsgeo = """ ``double array[3]`` Location of the observer in a standard terrestrial reference frame, ``OBSGEO-X``, ``OBSGEO-Y``, ``OBSGEO-Z`` (in meters). An undefined value is represented by NaN. """ offset = """ ``double`` The offset of the unit conversion. """ p0 = """ ``int array[M]`` Vector of length `~pywcs._pywcs.Tabprm.M` of interpolated indices into the coordinate array such that Upsilon_m, as defined in Paper III, is equal to ``(p0[m] + 1) + delta[m]``. """ p2s = """ p2s(pixcrd, origin) Converts pixel to sky coordinates. - *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates. %s Returns a dictionary with the following keys: - *imgcrd*: double array[ncoord][nelem] - Array of intermediate sky coordinates. For celestial axes, ``imgcrd[][self.lng]`` and ``imgcrd[][self.lat]`` are the projected *x*-, and *y*-coordinates, in pseudo degrees. For spectral axes, ``imgcrd[][self.spec]`` is the intermediate spectral coordinate, in SI units. - *phi*: double array[ncoord] - *theta*: double array[ncoord] - Longitude and latitude in the native coordinate system of the projection, in degrees. - *world*: double array[ncoord][nelem] - Array of sky coordinates. For celestial axes, ``world[][self.lng]`` and ``world[][self.lat]`` are the celestial longitude and latitude, in degrees. For spectral axes, ``world[][self.spec]`` is the intermediate spectral coordinate, in SI units. - *stat*: int array[ncoord] - Status return value for each coordinate. ``0`` for success, ``1+`` for invalid pixel coordinate. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `ValueError`: *x*- and *y*-coordinate arrays are not the same size. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. .. seealso:: `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng` """ % __.ORIGIN() p4_pix2foc = """ p4_pix2foc(*pixcrd, origin*) -> double array[ncoord][nelem] Convert pixel coordinates to focal plane coordinates using `Paper IV`_ lookup-table distortion correction. - *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates. %s Returns an array of focal plane coordinates. - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % __.ORIGIN() pc = """ ``double array[naxis][naxis]`` The ``PCi_ja`` (pixel coordinate) transformation matrix. The order is:: [[PC1_1, PC1_2], [PC2_1, PC2_2]] For historical compatibility, three alternate specifications of the linear transforations are available in wcslib. The canonical ``PCi_ja`` with ``CDELTia``, ``CDi_ja``, and the deprecated ``CROTAia`` keywords. Although the latter may not formally co-exist with ``PCi_ja``, the approach here is simply to ignore them if given in conjunction with ``PCi_ja``. `~pywcs.Wcsprm.has_pc`, `~pywcs.Wcsprm.has_cd` and `~pywcs.Wcsprm.has_crota` can be used to determine which of these alternatives are present in the header. These alternate specifications of the linear transformation matrix are translated immediately to ``PCi_ja`` by `~pywcs.Wcsprm.set` and are nowhere visible to the lower-level routines. In particular, `~pywcs.Wcsprm.set` resets `~pywcs.Wcsprm.cdelt` to unity if ``CDi_ja`` is present (and no ``PCi_ja``). If no ``CROTAia`` is associated with the latitude axis, `set` reverts to a unity ``PCi_ja`` matrix. """ phi0 = """ ``double`` The native latitude of the fiducial point, i.e. the point whose celestial coordinates are given in ``ref[1:2]``. If undefined (NaN) the initialization routine, `~pywcs.Wcsprm.set`, will set this to a projection-specific default. .. seealso:: `~pywcs.Wcsprm.theta0` """ pix2foc = """ pix2foc(*pixcrd, origin*) -> double array[ncoord][nelem] Perform both `SIP`_ polynomial and `Paper IV`_ lookup-table distortion correction in parallel. - *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates. %s Returns an array of focal plane coordinates. **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % __.ORIGIN() piximg_matrix = """ ``double array[2][2]`` (read-only) Matrix containing the product of the ``CDELTia`` diagonal matrix and the ``PCi_ja`` matrix. """ power = """ ``double`` The exponent of the unit conversion. """ print_contents = """ print_contents() Print the contents of the `~pywcs.Wcsprm` object to stdout. Probably only useful for debugging purposes, and may be removed in the future. To get a string of the contents, use `repr`. """ print_contents_tabprm = """ print_contents() Print the contents of the `~pywcs._pywcs.Tabprm` object to stdout. Probably only useful for debugging purposes, and may be removed in the future. To get a string of the contents, use `repr`. """ radesys = """ ``string`` The equatorial or ecliptic coordinate system type, ``RADESYSa``. """ restfrq = """ ``double`` Rest frequency (Hz) from ``RESTFRQa``. An undefined value is represented by NaN. """ restwav = """ ``double`` Rest wavelength (m) from ``RESTWAVa``. An undefined value is represented by NaN. """ row = """ ``int`` (read-only) Table row number. """ s2p = """ s2p(sky, origin) Transforms sky coordinates to pixel coordinates. - *sky*: double array[ncoord][nelem]. Array of sky coordinates, in decimal degrees. %s Returns a dictionary with the following keys: - *phi*: double array[ncoord] - *theta*: double array[ncoord] - Longitude and latitude in the native coordinate system of the projection, in degrees. - *imgcrd*: double array[ncoord][nelem] - Array of intermediate sky coordinates. For celestial axes, ``imgcrd[][self.lng]`` and ``imgcrd[][self.lat]`` are the projected *x*-, and *y*-coordinates, in pseudo "degrees". For quadcube projections with a ``CUBEFACE`` axis, the face number is also returned in ``imgcrd[][self.cubeface]``. For spectral axes, ``imgcrd[][self.spec]`` is the intermediate spectral coordinate, in SI units. - *pixcrd*: double array[ncoord][nelem] - Array of pixel coordinates. Pixel coordinates are zero-based. - *stat*: int array[ncoord] - Status return value for each coordinate. ``0`` for success, ``1+`` for invalid pixel coordinate. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError` Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. .. seealso:: `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng` """ % (__.ORIGIN()) scale = """ ``double`` The scaling factor for the unit conversion. """ sense = """ ``int array[M]`` A vector of length `~pywcs._pywcs.Tabprm.M` whose elements indicate whether the corresponding indexing vector is monotonically increasing (+1), or decreasing (-1). """ set = """ set() Sets up a WCS object for use according to information supplied within it. Note that this routine need not be called directly; it will be invoked by `~pywcs.Wcsprm.p2s` and `~pywcs.Wcsprm.s2p` if necessary. Some attributes that are based on other attributes (such as `~pywcs.Wcsprm.lattyp` on `~pywcs.Wcsprm.ctype`) may not be correct until after `~pywcs.Wcsprm.set` is called. `~pywcs.Wcsprm.set` strips off trailing blanks in all string members. `~pywcs.Wcsprm.set` recognizes the ``NCP`` projection and converts it to the equivalent ``SIN`` projection and it also recognizes ``GLS`` as a synonym for ``SFL``. It does alias translation for the AIPS spectral types (``FREQ-LSR``, ``FELO-HEL``, etc.) but without changing the input header keywords. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. """ set_tabprm = """ set() Allocates memory for work arrays in the Tabprm class and sets up the class according to information supplied within it. Note that this routine need not be called directly; it will be invoked by functions that need it. **Exceptions:** - `MemoryError`: Memory allocation failed. - `InvalidTabularParameters`: Invalid tabular parameters. """ set_ps = """ set_ps(list) Sets `PSi_ma` keywords for each *i* and *m*. The input must be a sequence of tuples of the form (*i*, *m*, *value*): - *i*: int. Axis number, as in ``PSi_ma``, (i.e. 1-relative) - *m*: int. Parameter number, as in ``PSi_ma``, (i.e. 0-relative) - *value*: string. Parameter value. .. seealso:: `~pywcs.Wcsprm.get_ps` """ set_pv = """ set_pv(list) Sets `PVi_ma` keywords for each *i* and *m*. The input must be a sequence of tuples of the form (*i*, *m*, *value*): - *i*: int. Axis number, as in ``PVi_ma``, (i.e. 1-relative) - *m*: int. Parameter number, as in ``PVi_ma``, (i.e. 0-relative) - *value*: float. Parameter value. .. seealso:: `~pywcs.Wcsprm.get_pv` """ sip = """ Get/set the `~pywcs.Sip` object for performing `SIP`_ distortion correction. """ Sip = """ Sip(*a, b, ap, bp, crpix*) The `~pywcs.Sip` class performs polynomial distortion correction using the `SIP`_ convention in both directions. Shupe, D. L., M. Moshir, J. Li, D. Makovoz and R. Narron. 2005. "The SIP Convention for Representing Distortion in FITS Image Headers." ADASS XIV. - *a*: double array[m+1][m+1]. The ``A_i_j`` polynomial for pixel to focal plane transformation. Its size must be (*m* + 1, *m* + 1) where *m* = ``A_ORDER``. - *b*: double array[m+1][m+1]. The ``B_i_j`` polynomial for pixel to focal plane transformation. Its size must be (*m* + 1, *m* + 1) where *m* = ``B_ORDER``. - *ap*: double array[m+1][m+1]. The ``AP_i_j`` polynomial for pixel to focal plane transformation. Its size must be (*m* + 1, *m* + 1) where *m* = ``AP_ORDER``. - *bp*: double array[m+1][m+1]. The ``BP_i_j`` polynomial for pixel to focal plane transformation. Its size must be (*m* + 1, *m* + 1) where *m* = ``BP_ORDER``. - *crpix*: double array[2]. The reference pixel. """ sip_foc2pix = """ sip_foc2pix(*foccrd, origin*) -> double array[ncoord][nelem] Convert focal plane coordinates to pixel coordinates using the `SIP`_ polynomial distortion convention. - *foccrd*: double array[ncoord][nelem]. Array of focal plane coordinates. %s Returns an array of pixel coordinates. **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % __.ORIGIN() sip_pix2foc = """ sip_pix2foc(*pixcrd, origin*) -> double array[ncoord][nelem] Convert pixel coordinates to focal plane coordinates using the `SIP`_ polynomial distortion convention. - *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates. %s Returns an array of focal plane coordinates. **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % __.ORIGIN() spcfix = """ spcfix() -> int Translates AIPS-convention spectral coordinate types. {``FREQ``, ``VELO``, ``FELO``}-{``OBS``, ``HEL``, ``LSR``} (e.g. ``FREQ-LSR``, ``VELO-OBS``, ``FELO-HEL``) Returns ``0`` for success; ``-1`` if no change required. """ spec = """ ``int`` (read-only) The index containing the spectral axis values. """ specsys = """ ``string`` Spectral reference frame (standard of rest), ``SPECSYSa``. .. seealso:: `~pywcs.Wcsprm.ssysobs`, `~pywcs.Wcsprm.velosys`. """ sptr = """ sptr(ctype, i=-1) Translates the spectral axis in a WCS object. For example, a ``FREQ`` axis may be translated into ``ZOPT-F2W`` and vice versa. - *ctype*: string. Required spectral ``CTYPEia``, maximum of 8 characters. The first four characters are required to be given and are never modified. The remaining four, the algorithm code, are completely determined by, and must be consistent with, the first four characters. Wildcarding may be used, i.e. if the final three characters are specified as ``"???"``, or if just the eighth character is specified as ``"?"``, the correct algorithm code will be substituted and returned. - *i*: int. Index of the spectral axis (0-relative). If ``i < 0`` (or not provided), it will be set to the first spectral axis identified from the ``CTYPE`` keyvalues in the FITS header. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. - `InvalidSubimageSpecificationError`: Invalid subimage specification (no spectral axis). """ ssysobs = """ ``string`` The actual spectral reference frame in which there is no differential variation in the spectral coordinate across the field-of-view, ``SSYSOBSa``. .. seealso:: `~pywcs.Wcsprm.specsys`, `~pywcs.Wcsprm.velosys` """ ssyssrc = """ ``string`` The spectral reference frame (standard of rest) in which the redshift was measured, ``SSYSSRCa``. """ sub = """ sub(axes) Extracts the coordinate description for a subimage from a `~pywcs.WCS` object. The world coordinate system of the subimage must be separable in the sense that the world coordinates at any point in the subimage must depend only on the pixel coordinates of the axes extracted. In practice, this means that the ``PCi_ja`` matrix of the original image must not contain non-zero off-diagonal terms that associate any of the subimage axes with any of the non-subimage axes. `sub` can also add axes to a wcsprm struct. The new axes will be created using the defaults set by the Wcsprm constructor which produce a simple, unnamed, linear axis with world coordinates equal to the pixel coordinate. These default values can be changed before invoking `set`. No checks are performed to verify that the coordinate axes are consistent, that is done by `set`. - *axes*: int or a sequence. - If an int, include the first *N* axes in their original order. - If a sequence, may contain a combination of image axis numbers (1-relative) or special axis identifiers (see below). Order is significant; ``axes[0]`` is the axis number of the input image that corresponds to the first axis in the subimage, etc. Use an axis number of 0 to create a new axis using the defaults. - If ``0``, ``[]`` or ``None``, do a deep copy. Coordinate axes types may be specified using either strings or special integer constants. The available types are: - ``'longitude'`` / ``WCSSUB_LONGITUDE``: Celestial longitude - ``'latitude'`` / ``WCSSUB_LATITUDE``: Celestial latitude - ``'cubeface'`` / ``WCSSUB_CUBEFACE``: Quadcube ``CUBEFACE`` axis - ``'spectral'`` / ``WCSSUB_SPECTRAL``: Spectral axis - ``'stokes'`` / ``WCSSUB_STOKES``: Stokes axis - ``'celestial'`` / ``WCSSUB_CELESTIAL``: An alias for the combination of ``'longitude'``, ``'latitude'`` and ``'cubeface'``. Returns a `~pywcs.WCS` object, which is a deep copy of the original object. **Exceptions:** - `MemoryError`: Memory allocation failed. - `InvalidSubimageSpecificationError`: Invalid subimage specification (no spectral axis). - `NonseparableSubimageCoordinateSystem`: Non-separable subimage coordinate system. .. note:: Combinations of subimage axes of particular types may be extracted in the same order as they occur in the input image by combining the integer constants with the 'binary or' (``|``) operator. For example:: wcs.sub([WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_SPECTRAL]) would extract the longitude, latitude, and spectral axes in the same order as the input image. If one of each were present, the resulting object would have three dimensions. For convenience, ``WCSSUB_CELESTIAL`` is defined as the combination ``WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_CUBEFACE``. The codes may also be negated to extract all but the types specified, for example:: wcs.sub([ WCSSUB_LONGITUDE, WCSSUB_LATITUDE, WCSSUB_CUBEFACE, -(WCSSUB_SPECTRAL | WCSSUB_STOKES)]) The last of these specifies all axis types other than spectral or Stokes. Extraction is done in the order specified by `axes`, i.e. a longitude axis (if present) would be extracted first (via ``axes[0]``) and not subsequently (via ``axes[3]``). Likewise for the latitude and cubeface axes in this example. The number of dimensions in the returned object may be less than or greater than the length of `axes`. However, it will never exceed the number of axes in the input image. """ tab = """ ``list of Tabprm`` A list of tabular coordinate objects associated with this WCS. """ Tabprm = """ A class to store the information related to tabular coordinates, i.e. coordinates that are defined via a lookup table. This class can not be constructed directly from Python, but instead is returned from `~pywcs.Wcsprm.tab`. """ theta0 = """ ``double`` The native longitude of the fiducial point, i.e. the point whose celestial coordinates are given in ``ref[1:2]``. If undefined (NaN) the initialization routine, `~pywcs.Wcsprm.set`, will set this to a projection-specific default. .. seealso:: `~pywcs.Wcsprm.phi0` """ to_header = """ to_header(relax=False) `to_header` translates a WCS object into a FITS header. - If the `~pywcs.Wcsprm.colnum` member is non-zero then a binary table image array header will be produced. - Otherwise, if the `~pywcs.Wcsprm.colax` member is set non-zero then a pixel list header will be produced. - Otherwise, a primary image or image extension header will be produced. The output header will almost certainly differ from the input in a number of respects: 1. The output header only contains WCS-related keywords. In particular, it does not contain syntactically-required keywords such as ``SIMPLE``, ``NAXIS``, ``BITPIX``, or ``END``. 2. Deprecated (e.g. ``CROTAn``) or non-standard usage will be translated to standard (this is partially dependent on whether `fix` was applied). 3. Quantities will be converted to the units used internally, basically SI with the addition of degrees. 4. Floating-point quantities may be given to a different decimal precision. 5. Elements of the ``PCi_j`` matrix will be written if and only if they differ from the unit matrix. Thus, if the matrix is unity then no elements will be written. 6. Additional keywords such as ``WCSAXES``, ``CUNITia``, ``LONPOLEa`` and ``LATPOLEa`` may appear. 7. The original keycomments will be lost, although `~pywcs.Wcsprm.to_header` tries hard to write meaningful comments. 8. Keyword order may be changed. Keywords can be translated between the image array, binary table, and pixel lists forms by manipulating the `~pywcs.Wcsprm.colnum` or `~pywcs.Wcsprm.colax` members of the `~pywcs.Wcsprm.WCS` object. - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to write. See :ref:`relaxwrite` for details. Returns a raw FITS header as a string. """ ttype = """ ``str`` (read-only) ``TTYPEn`` identifying the column of the binary table that contains the wcstab array. """ UnitConverter = """ UnitConverter(have, want, translate_units='') Creates an object for performing conversion from one system of units to another. - *have* string: :ref:`fits-unit` to convert from, with or without surrounding square brackets (for inline specifications); text following the closing bracket is ignored. - *want* string: :ref:`fits-unit` to convert to, with or without surrounding square brackets (for inline specifications); text following the closing bracket is ignored. - *ctrl* string (optional): Do potentially unsafe translations of non-standard unit strings. Although ``"S"`` is commonly used to represent seconds, its recognizes ``"S"`` formally as Siemens, however rarely that may be translation to ``"s"`` is potentially unsafe since the standard used. The same applies to ``"H"`` for hours (Henry), and ``"D"`` for days (Debye). This string controls what to do in such cases, and is case-insensitive. - If the string contains ``"s"``, translate ``"S"`` to ``"s"``. - If the string contains ``"h"``, translate ``"H"`` to ``"h"``. - If the string contains ``"d"``, translate ``"D"`` to ``"d"``. Thus ``''`` doesn't do any unsafe translations, whereas ``'shd'`` does all of them. See :ref:`fits-unit` for more information. Use the returned object's `~pywcs.UnitConverter.convert` method to convert values from *have* to *want*. This function is permissive in accepting whitespace in all contexts in a units specification where it does not create ambiguity (e.g. not between a metric prefix and a basic unit string), including in strings like ``"log (m ** 2)"`` which is formally disallowed. **Exceptions:** - `ValueError`: Invalid numeric multiplier. - `SyntaxError`: Dangling binary operator. - `SyntaxError`: Invalid symbol in INITIAL context. - `SyntaxError`: Function in invalid context. - `SyntaxError`: Invalid symbol in EXPON context. - `SyntaxError`: Unbalanced bracket. - `SyntaxError`: Unbalanced parenthesis. - `SyntaxError`: Consecutive binary operators. - `SyntaxError`: Internal parser error. - `SyntaxError`: Non-conformant unit specifications. - `SyntaxError`: Non-conformant functions. - `ValueError`: Potentially unsafe translation. """ unitfix = """ unitfix(translate_units='') Translates non-standard ``CUNITia`` keyvalues. For example, ``DEG`` -> ``deg``, also stripping off unnecessary whitespace. - *translate_units*: string. Do potentially unsafe translations of non-standard unit strings. Although ``"S"`` is commonly used to represent seconds, its recognizes ``"S"`` formally as Siemens, however rarely that may be translation to ``"s"`` is potentially unsafe since the standard used. The same applies to ``"H"`` for hours (Henry), and ``"D"`` for days (Debye). This string controls what to do in such cases, and is case-insensitive. - If the string contains ``"s"``, translate ``"S"`` to ``"s"``. - If the string contains ``"h"``, translate ``"H"`` to ``"h"``. - If the string contains ``"d"``, translate ``"D"`` to ``"d"``. Thus ``''`` doesn't do any unsafe translations, whereas ``'shd'`` does all of them. See :ref:`fits-unit` for more information. Returns ``0`` for success; ``-1`` if no change required. """ velangl = """ ``double`` The angle in degrees that should be used to decompose an observed velocity into radial and transverse components. An undefined value is represented by NaN. """ velosys = """ ``double`` The relative radial velocity (m/s) between the observer and the selected standard of rest in the direction of the celestial reference coordinate, ``VELOSYSa``. An undefined value is represented by NaN. .. seealso:: `~pywcs.Wcsprm.specsys`, `~pywcs.Wcsprm.ssysobs` """ want = """ The name of the unit being converted to. This value always uses standard unit names, even if the `UnitConverter` was initialized with a non-standard unit name. """ wcs = """ A `~pywcs.Wcsprm` object to perform the basic `wcslib`_ WCS tranformation. """ Wcs = """ Wcs(*sip, cpdis, wcsprm, det2im*) Wcs objects amalgamate basic WCS (as provided by `wcslib`_), with `SIP`_ and `Paper IV`_ distortion operations. To perform all distortion corrections and WCS tranformation, use `all_pix2sky`. - *sip*: A `~pywcs.Sip` object or ``None`` - *cpdis*: A pair of `~pywcs.DistortionLookupTable` objects, or ``(None, None)``. - *wcsprm*: A `~pywcs.Wcsprm` object - *det2im*: A pair of `~pywcs.DistortionLookupTable` objects, or ``(None, None)``. """ Wcsprm = """ Wcsprm(header=None, key=' ', relax=False, naxis=2, keysel=0, colsel=None) `~pywcs.Wcsprm` is a direct wrapper around `wcslib`_, and provides access to the core WCS transformations that it supports. The FITS header parsing enforces correct FITS "keyword = value" syntax with regard to the equals sign occurring in columns 9 and 10. However, it does recognize free-format character (NOST 100-2.0, Sect. 5.2.1), integer (Sect. 5.2.3), and floating-point values (Sect. 5.2.4) for all keywords. - *header*: A PyFITS header object or a string containing the raw FITS header data or ``None``. If ``None``, the object will be initialized to default values. - *key*: The key referring to a particular WCS transform in the header. This may be either ``' '`` or ``'A'``-``'Z'`` and corresponds to the ``"a"`` part of ``"CTYPEia"``. (*key* may only be provided if *header* is also provided.) - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to accept. See :ref:`relaxread` for details. - *naxis*: The number of sky coordinates axes for the object. (*naxis* may only be provided if *header* is ``None``.) - *keysel*: Vector of flag bits that may be used to restrict the keyword types considered: - ``WCSHDR_IMGHEAD``: Image header keywords. - ``WCSHDR_BIMGARR``: Binary table image array. - ``WCSHDR_PIXLIST``: Pixel list keywords. If zero, there is no restriction. If -1, the underlying wcslib function ``wcspih()`` is called, rather than ``wcstbh()``. - *colsel*: A sequence of table column numbers used to restrict the keywords considered. ``None`` indicates no restriction. **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid key. - `KeyError`: Key not found in FITS header. """ Wtbarr = """ Classes to construct coordinate lookup tables from a binary table extension (BINTABLE). This class can not be constructed directly from Python, but instead is returned from `~pywcs.Wcsprm.wtb`. """ zsource = """ ``double`` The redshift, ``ZSOURCEa``, of the source. An undefined value is represented by NaN. """ pywcs-1.12/doc/make.bat0000644001153600020070000000557312310355626017032 0ustar cslocumSTSCI\science00000000000000@ECHO OFF REM Command file for Sphinx documentation set SPHINXBUILD=sphinx-build set ALLSPHINXOPTS=-d build/doctrees %SPHINXOPTS% source if NOT "%PAPER%" == "" ( set ALLSPHINXOPTS=-D latex_paper_size=%PAPER% %ALLSPHINXOPTS% ) if "%1" == "" goto help if "%1" == "help" ( :help echo.Please use `make ^` where ^ is one of echo. html to make standalone HTML files echo. dirhtml to make HTML files named index.html in directories echo. pickle to make pickle files echo. json to make JSON files echo. htmlhelp to make HTML files and a HTML help project echo. qthelp to make HTML files and a qthelp project echo. latex to make LaTeX files, you can set PAPER=a4 or PAPER=letter echo. changes to make an overview over all changed/added/deprecated items echo. linkcheck to check all external links for integrity echo. doctest to run all doctests embedded in the documentation if enabled goto end ) if "%1" == "clean" ( for /d %%i in (build\*) do rmdir /q /s %%i del /q /s build\* goto end ) if "%1" == "html" ( %SPHINXBUILD% -b html %ALLSPHINXOPTS% build/html echo. echo.Build finished. The HTML pages are in build/html. goto end ) if "%1" == "dirhtml" ( %SPHINXBUILD% -b dirhtml %ALLSPHINXOPTS% build/dirhtml echo. echo.Build finished. The HTML pages are in build/dirhtml. goto end ) if "%1" == "pickle" ( %SPHINXBUILD% -b pickle %ALLSPHINXOPTS% build/pickle echo. echo.Build finished; now you can process the pickle files. goto end ) if "%1" == "json" ( %SPHINXBUILD% -b json %ALLSPHINXOPTS% build/json echo. echo.Build finished; now you can process the JSON files. goto end ) if "%1" == "htmlhelp" ( %SPHINXBUILD% -b htmlhelp %ALLSPHINXOPTS% build/htmlhelp echo. echo.Build finished; now you can run HTML Help Workshop with the ^ .hhp project file in build/htmlhelp. goto end ) if "%1" == "qthelp" ( %SPHINXBUILD% -b qthelp %ALLSPHINXOPTS% build/qthelp echo. echo.Build finished; now you can run "qcollectiongenerator" with the ^ .qhcp project file in build/qthelp, like this: echo.^> qcollectiongenerator build\qthelp\pywcs.qhcp echo.To view the help file: echo.^> assistant -collectionFile build\qthelp\pywcs.ghc goto end ) if "%1" == "latex" ( %SPHINXBUILD% -b latex %ALLSPHINXOPTS% build/latex echo. echo.Build finished; the LaTeX files are in build/latex. goto end ) if "%1" == "changes" ( %SPHINXBUILD% -b changes %ALLSPHINXOPTS% build/changes echo. echo.The overview file is in build/changes. goto end ) if "%1" == "linkcheck" ( %SPHINXBUILD% -b linkcheck %ALLSPHINXOPTS% build/linkcheck echo. echo.Link check complete; look for any errors in the above output ^ or in build/linkcheck/output.txt. goto end ) if "%1" == "doctest" ( %SPHINXBUILD% -b doctest %ALLSPHINXOPTS% build/doctest echo. echo.Testing of doctests in the sources finished, look at the ^ results in build/doctest/output.txt. goto end ) :end pywcs-1.12/doc/Makefile0000644001153600020070000000563612310355626017065 0ustar cslocumSTSCI\science00000000000000# Makefile for Sphinx documentation # # You can set these variables from the command line. SPHINXOPTS = SPHINXBUILD = sphinx-build PAPER = # Internal variables. PAPEROPT_a4 = -D latex_paper_size=a4 PAPEROPT_letter = -D latex_paper_size=letter ALLSPHINXOPTS = -d build/doctrees $(PAPEROPT_$(PAPER)) $(SPHINXOPTS) source .PHONY: help clean html dirhtml pickle json htmlhelp qthelp latex changes linkcheck doctest help: @echo "Please use \`make ' where is one of" @echo " html to make standalone HTML files" @echo " dirhtml to make HTML files named index.html in directories" @echo " pickle to make pickle files" @echo " json to make JSON files" @echo " htmlhelp to make HTML files and a HTML help project" @echo " qthelp to make HTML files and a qthelp project" @echo " latex to make LaTeX files, you can set PAPER=a4 or PAPER=letter" @echo " changes to make an overview of all changed/added/deprecated items" @echo " linkcheck to check all external links for integrity" @echo " doctest to run all doctests embedded in the documentation (if enabled)" clean: -rm -rf build/* html: $(SPHINXBUILD) -b html $(ALLSPHINXOPTS) build/html @echo @echo "Build finished. The HTML pages are in build/html." dirhtml: $(SPHINXBUILD) -b dirhtml $(ALLSPHINXOPTS) build/dirhtml @echo @echo "Build finished. The HTML pages are in build/dirhtml." pickle: $(SPHINXBUILD) -b pickle $(ALLSPHINXOPTS) build/pickle @echo @echo "Build finished; now you can process the pickle files." json: $(SPHINXBUILD) -b json $(ALLSPHINXOPTS) build/json @echo @echo "Build finished; now you can process the JSON files." htmlhelp: $(SPHINXBUILD) -b htmlhelp $(ALLSPHINXOPTS) build/htmlhelp @echo @echo "Build finished; now you can run HTML Help Workshop with the" \ ".hhp project file in build/htmlhelp." qthelp: $(SPHINXBUILD) -b qthelp $(ALLSPHINXOPTS) build/qthelp @echo @echo "Build finished; now you can run "qcollectiongenerator" with the" \ ".qhcp project file in build/qthelp, like this:" @echo "# qcollectiongenerator build/qthelp/pywcs.qhcp" @echo "To view the help file:" @echo "# assistant -collectionFile build/qthelp/pywcs.qhc" latex: $(SPHINXBUILD) -b latex $(ALLSPHINXOPTS) build/latex @echo @echo "Build finished; the LaTeX files are in build/latex." @echo "Run \`make all-pdf' or \`make all-ps' in that directory to" \ "run these through (pdf)latex." changes: $(SPHINXBUILD) -b changes $(ALLSPHINXOPTS) build/changes @echo @echo "The overview file is in build/changes." linkcheck: $(SPHINXBUILD) -b linkcheck $(ALLSPHINXOPTS) build/linkcheck @echo @echo "Link check complete; look for any errors in the above output " \ "or in build/linkcheck/output.txt." doctest: $(SPHINXBUILD) -b doctest $(ALLSPHINXOPTS) build/doctest @echo "Testing of doctests in the sources finished, look at the " \ "results in build/doctest/output.txt." pywcs-1.12/doc/source/0000755001153600020070000000000012310355732016711 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/doc/source/api.rst0000644001153600020070000000072112310355626020216 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst API documentation ================= :mod:`pywcs` ------------ .. automodule:: pywcs Classes ------- .. toctree:: :maxdepth: 2 api_wcs.rst api_wcsprm.rst api_distortion.rst api_sip.rst api_units.rst relax.rst Testing pywcs ============= The unit tests are written for use with `nose `. To run them, install pywcs and then at the commandline:: nosetests pywcs.tests pywcs-1.12/doc/source/api_distortion.rst0000644001153600020070000000026112310355626022473 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst `DistortionLookupTable` ``````````````````````` .. autoclass:: pywcs.DistortionLookupTable :members: :inherited-members: :undoc-members: pywcs-1.12/doc/source/api_sip.rst0000644001153600020070000000017312310355626021072 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst `Sip` ````` .. autoclass:: pywcs.Sip :members: :inherited-members: :undoc-members: pywcs-1.12/doc/source/api_units.rst0000644001153600020070000002746112310355626021452 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst `UnitConverter` ``````````````` .. autoclass:: pywcs.UnitConverter :members: :inherited-members: :undoc-members: .. _fits-unit: FITS unit specification ``````````````````````` Supported units --------------- The following units are supported by the FITS standard: **SI base & supplementary units** ====================== ============ ================= Quantity Unit String Meaning ====================== ============ ================= length m metre mass kg kilogram time s second of time plane angle rad radian solid angle sr steradian temperature K kelvin electric current A ampere amount of substance mol mole luminous intensity cd candela ====================== ============ ================= **IAU-recognized derived units** ====================== ============ ================= ================== Quantity Unit String Meaning Equivalence ====================== ============ ================= ================== frequency Hz hertz s\ :sup:`-1` energy J joule N m power W watt J s\ :sup:`-1` electric potential V volts J C\ :sup:`-1` force N newton kg m s\ :sup:`-2` pressure, stress Pa pascal N m\ :sup:`-2` electric charge C coulomb A s electric resistance ohm ohm (Ω) V A\ :sup:`-1` electric conductance S siemens A V\ :sup:`-1` electric capacitance F farad C V\ :sup:`-1` magnetic flux Wb weber V s magnetic flux density T tesla Wb m\ :sup:`-2` inductance H henry Wb A\ :sup:`-1` luminous flux lm lumen cd sr illuminance lx lux lm m\ :sup:`-2` ====================== ============ ================= ================== **Additional units** ====================== ============ ======================== ============================================ Quantity Unit String Meaning Equivalence ====================== ============ ======================== ============================================ mass u unified atomic mass unit 1.6605387 x 10\ :sup:`-27` kg mass solMass solar mass 1.9891 x 10\ :sup:`30` kg plane angle deg degree of arc 1.745533 x 10\ :sup:`-2` rad plane angle arcsec second of arc 4.848137 x 10\ :sup:`-6` rad plane angle arcmin minute of arc 2.90888 x 10\ :sup:`-4` rad time min minute time h hour time d day 8.64 x 10\ :sup:`4` s time yr year (Julian) 3.15576 x10\ :sup:`-7` s (365.25 d) energy eV electron volt 1.602177 x 10\ :sup:`-19` J energy erg erg 10\ :sup:`-7` J energy Ry Rydberg 13.605692 eV length angstrom angstrom 10\ :sup:`-10` m length AU astronomical unit 1.49598 x 10\ :sup:`11` m length lyr light year 9.460530 x 10\ :sup:`-15` m length pc parsec 3.0857 x 10\ :sup:`-16` m length solRad solar radius 6.9599 x 10\ :sup:`8` m events count counts events photon photons flux density Jy jansky 10\ :sup:`-16` W m\ :sup:`-2` Hz\ :sup:`-1` flux density mag (stellar) magnitude flux density Crab 'crab' flux density beam beam Jy/beam flux density solLum solar luminosity magnetic field G gauss 10\ :sup:`-4` T area pixel (image/detector) pixel area voxel 3-d analog of pixel area barn barn 10\ :sup:`-28` m\ :sup:`2` device chan (detector) channel device byte (computer) byte device bit (computer) bits device adu A/D converter units misc bin numerous applications misc Sun wrt. sun ====================== ============ ======================== ============================================ Potentially unsafe translations of ``"D"``, ``"H"``, and ``"S"``, are optional, using the *translate_units* parameter. .. _unit-aliases: Unit aliases ------------ When converting non-standard units to standard ones, a case-sensitive match is required for the aliases listed below, in particular the only recognized aliases with metric prefixes are ``"KM"``, ``"KHZ"``, ``"MHZ"``, and ``"GHZ"``. ========== ============================================================= Unit Recognized aliases ========== ============================================================= Angstrom angstrom arcmin arcmins, ARCMIN, ARCMINS arcsec arcsecs, ARCSEC, ARCSECS beam BEAM byte Byte count ct d day, days, (D), DAY, DAYS deg degree, degrees, DEG, DEGREE, DEGREES GHz GHZ h hr, (H), HR Hz hz, HZ kHz KHZ Jy JY K kelvin, kelvins, Kelvin, Kelvins, KELVIN, KELVINS km KM m metre, meter, metres, meters, M, METRE, METER, METRES, METERS min MIN MHz MHZ Ohm ohm Pa pascal, pascals, Pascal, Pascals, PASCAL, PASCALS photon ph pixel pixels, PIXEL, PIXELS, pix rad radian, radians, RAD, RADIAN, RADIANS s sec, second, seconds, (S), SEC, SECOND, SECONDS V volt, volts, Volt, Volts, VOLT, VOLTS yr year, years, YR, YEAR, YEARS ========== ============================================================= The aliases ``"angstrom"``, ``"ohm"``, and ``"Byte"`` for (Angstrom, Ohm, and byte) are recognized by pywcs/wcslib itself as an unofficial extension of the standard, but they are converted to the standard form here. Prefixes -------- The following metric prefixes are supported: ======= ======= =================== Prefix String Magnitude ======= ======= =================== yocto y 10\ :sup:`-24` zepto z 10\ :sup:`-21` atto a 10\ :sup:`-18` femto f 10\ :sup:`-15` pico p 10\ :sup:`-12` nano n 10\ :sup:`-9` micro u 10\ :sup:`-6` milli m 10\ :sup:`-3` centi c 10\ :sup:`-2` deci d 10\ :sup:`-1` deka da 10\ :sup:`1` hecto h 10\ :sup:`2` kilo k 10\ :sup:`3` Mega M 10\ :sup:`6` Giga G 10\ :sup:`9` Tera T 10\ :sup:`12` Peta P 10\ :sup:`15` Exa E 10\ :sup:`18` Zetta Z 10\ :sup:`21` Yotta Y 10\ :sup:`24` ======= ======= =================== Table 6 of WCS Paper I lists eleven units for which metric prefixes are allowed. However, in this implementation only prefixes greater than unity are allowed for ``"a"`` (annum), ``"yr"`` (year), ``"pc"`` (parsec), ``"bit"``, and ``"byte"``, and only prefixes less than unity are allowed for ``"mag"`` (stellar magnitude). Metric prefix ``"P"`` (peta) is specifically forbidden for ``"a"`` (annum) to avoid confusion with ``"Pa"`` (Pascal, not peta-annum). Note that metric prefixes are specifically disallowed for ``"h"`` (hour) and ``"d"`` (day) so that ``"ph"`` (photons) cannot be interpreted as pico-hours, nor ``"cd"`` (candela) as centi-days. Operators --------- A compound unit is considered to be formed by a series of sub-strings of component units & mathematical operations. Each of these sub-strings must be separated by at least one space or a mathematical operator (``*`` or ``/``). Multiplication ============== Multiplicative units can be specified either: - by simply using one or more preceding spaces, e.g. ``str1 str2`` (The recommended method). - by the use of a single asterisk (``*``) with optional whitespace, e.g. ``str1 * str2``. Division ======== Units which form the denominator of a compound expression can be specified either: - by using a slash (``/``) with optional whitespace, e.g. ``str1 / str2``. If such a syntax is used, it is recommended that no space is included between the slash and the unit string. - by raising a multiplicative unit to a negative power (see below). It should be stressed that the slash character only effects the sub-string it immediately precedes. Thus, unless brackets are used, subsequent sub-strings which also form part of the denominator of the compound expression must also be preceded by a slash. For example, ``str1 /str2 str3`` is equivalent to ``str1 str3 /str2`` whilst ``str1 /str2 /str3`` is equivalent to ``str1 /(str2 * str3)``. Raising to Powers ================= A unit string raised to the power *y* is specified: - by using two asterisks (``**``) followed by the index enclosed within round brackets and with no preceding or intervening spaces, e.g. ``str1**(y)`` or ``str1**(-y)``. However, if *y* is positive, then the brackets need not be included, but a following space is recommended if additional sub-strings follow. Use of brackets =============== Any number of pairs of round brackets (``()``) may be used within the string for a compound unit in order to prevent ambiguities. As described within this section, a number of rules always/often require their use. However, it is suggested that conservative use is made of such pairs of brackets in order to minimize the total length of compound strings. (It should be remembered that a maximum of 68 characters are allowed in the card image of keywords.) Avoidance of underflows & overflows =================================== The inclusion of numerical factors within the unit string should generally be avoided (by the use of multiples and/or submultiples of component basic units). However, occasionally it may be preferable to include such factors on the grounds of user-friendliness and/or to minimize the risk of computer under- or overflows. In such cases, the numerical factor can simply be considered a basic unit string. The following additional guidelines are suggested: - the numerical factor should precede any unit strings - only powers of 10 are used as numerical factors Mathematical Operations & Functions =================================== A number of mathematical operations are supported. It should be noted that the (round) brackets are mandatory in all cases in which they are included in the table. =============== ================================================== String Meaning =============== ================================================== ``str1*str2`` Multiplication ``str1 /str2`` Division ``str1**(y)`` Raised to the power *y* ``log(str1)`` Common Logarithm (to base 10) ``ln(str1)`` Natural Logarithm ``exp(str1)`` Exponential (exp\ :sup:`str1`\ ) ``sqrt(str1)`` Square root ``sin(str1)`` Sine ``cos(str1)`` Cosine ``tan(str1)`` Tangent ``asin(str1)`` Arc Sine ``acos(str1)`` Arc Cosine ``atan(str1)`` Arc Tangent ``sinh(str1)`` Hyperbolic Sine ``cosh(str1)`` Hyperbolic Cosine ``tanh(str1)`` Hyperbolic Tangent =============== ================================================== Function types ``log()``, ``ln()`` and ``exp()`` may only occur at the start of the units specification. pywcs-1.12/doc/source/api_wcs.rst0000644001153600020070000000026512310355626021075 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst `WCS` ````` .. autoclass:: pywcs.WCS :members: :inherited-members: :undoc-members: functions ````````` .. autofunction:: pywcs.find_all_wcs pywcs-1.12/doc/source/api_wcsprm.rst0000644001153600020070000000056212310355626021614 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst `Wcsprm` ```````` .. autoclass:: pywcs.Wcsprm :members: :inherited-members: :undoc-members: `Tabprm` ```````` .. autoclass:: pywcs._pywcs.Tabprm :members: :inherited-members: :undoc-members: .. `Wtbarr` .. ```````` .. .. autoclass:: pywcs._pywcs.Wtbarr .. :members: .. :inherited-members: .. :undoc-members: pywcs-1.12/doc/source/conf.py0000644001153600020070000001506612310355626020222 0ustar cslocumSTSCI\science00000000000000# -*- coding: utf-8 -*- # # pywcs documentation build configuration file, created by # sphinx-quickstart on Thu Sep 17 12:58:53 2009. # # This file is execfile()d with the current directory set to its containing dir. # # Note that not all possible configuration values are present in this # autogenerated file. # # All configuration values have a default; values that are commented out # serve to show the default. from stsci.sphinxext.conf import * import sys, os import pywcs from pywcs.version import __version__ # If extensions (or modules to document with autodoc) are in another directory, # add these directories to sys.path here. If the directory is relative to the # documentation root, use os.path.abspath to make it absolute, like shown here. #sys.path.append(os.path.abspath('.')) # -- General configuration ----------------------------------------------------- # Add any Sphinx extension module names here, as strings. They can be extensions # coming with Sphinx (named 'sphinx.ext.*') or your custom ones. # extensions = ['sphinx.ext.autodoc', 'sphinx.ext.pngmath'] # Add any paths that contain templates here, relative to this directory. templates_path = ['_templates'] # The suffix of source filenames. source_suffix = '.rst' # The encoding of source files. #source_encoding = 'utf-8' # The master toctree document. master_doc = 'index' # General information about the project. project = u'pywcs' copyright = u'2009, Michael Droettboom (pywcs), 2009 Mark Calabretta (wcslib)' # The version info for the project you're documenting, acts as replacement for # |version| and |release|, also used in various other places throughout the # built documents. # # The short X.Y version. version = __version__ # The full version, including alpha/beta/rc tags. release = __version__ # The language for content autogenerated by Sphinx. Refer to documentation # for a list of supported languages. #language = None # There are two options for replacing |today|: either, you set today to some # non-false value, then it is used: #today = '' # Else, today_fmt is used as the format for a strftime call. #today_fmt = '%B %d, %Y' # List of documents that shouldn't be included in the build. #unused_docs = [] # List of directories, relative to source directory, that shouldn't be searched # for source files. exclude_trees = [] # The reST default role (used for this markup: `text`) to use for all documents. # default_role = 'obj' # If true, '()' will be appended to :func: etc. cross-reference text. #add_function_parentheses = True # If true, the current module name will be prepended to all description # unit titles (such as .. function::). #add_module_names = True # If true, sectionauthor and moduleauthor directives will be shown in the # output. They are ignored by default. #show_authors = False # The name of the Pygments (syntax highlighting) style to use. pygments_style = 'sphinx' # A list of ignored prefixes for module index sorting. #modindex_common_prefix = [] autoclass_content = 'both' # -- Options for HTML output --------------------------------------------------- # The theme to use for HTML and HTML Help pages. Major themes that come with # Sphinx are currently 'default' and 'sphinxdoc'. # html_theme = 'default' # Theme options are theme-specific and customize the look and feel of a theme # further. For a list of options available for each theme, see the # documentation. #html_theme_options = {} # Add any paths that contain custom themes here, relative to this directory. #html_theme_path = [] # The name for this set of Sphinx documents. If None, it defaults to # " v documentation". #html_title = None # A shorter title for the navigation bar. Default is the same as html_title. #html_short_title = None # The name of an image file (relative to this directory) to place at the top # of the sidebar. #html_logo = None # The name of an image file (within the static path) to use as favicon of the # docs. This file should be a Windows icon file (.ico) being 16x16 or 32x32 # pixels large. #html_favicon = None # Add any paths that contain custom static files (such as style sheets) here, # relative to this directory. They are copied after the builtin static files, # so a file named "default.css" will overwrite the builtin "default.css". html_static_path = ['_static'] # If not '', a 'Last updated on:' timestamp is inserted at every page bottom, # using the given strftime format. #html_last_updated_fmt = '%b %d, %Y' # If true, SmartyPants will be used to convert quotes and dashes to # typographically correct entities. #html_use_smartypants = True # Custom sidebar templates, maps document names to template names. #html_sidebars = {} # Additional templates that should be rendered to pages, maps page names to # template names. #html_additional_pages = {} # If false, no module index is generated. #html_use_modindex = True # If false, no index is generated. #html_use_index = True # If true, the index is split into individual pages for each letter. #html_split_index = False # If true, links to the reST sources are added to the pages. #html_show_sourcelink = True # If true, "Created using Sphinx" is shown in the HTML footer. Default is True. #html_show_sphinx = True # If true, "(C) Copyright ..." is shown in the HTML footer. Default is True. #html_show_copyright = True # If true, an OpenSearch description file will be output, and all pages will # contain a tag referring to it. The value of this option must be the # base URL from which the finished HTML is served. #html_use_opensearch = '' # If nonempty, this is the file name suffix for HTML files (e.g. ".xhtml"). #html_file_suffix = '' # Output file base name for HTML help builder. htmlhelp_basename = 'pywcsdoc' # -- Options for LaTeX output -------------------------------------------------- # The paper size ('letter' or 'a4'). #latex_paper_size = 'letter' # The font size ('10pt', '11pt' or '12pt'). #latex_font_size = '10pt' # Grouping the document tree into LaTeX files. List of tuples # (source start file, target name, title, author, documentclass [howto/manual]). latex_documents = [ ('index', 'pywcs.tex', u'pywcs Documentation', u'Michael Droettboom', 'manual'), ] # The name of an image file (relative to this directory) to place at the top of # the title page. #latex_logo = None # For "manual" documents, if this is true, then toplevel headings are parts, # not chapters. #latex_use_parts = False # Additional stuff for the LaTeX preamble. #latex_preamble = '' # Documents to append as an appendix to all manuals. #latex_appendices = [] # If false, no module index is generated. #latex_use_modindex = True pywcs-1.12/doc/source/examples.rst0000644001153600020070000000117512310355626021267 0ustar cslocumSTSCI\science00000000000000Example Usage ============= Loading WCS information from a FITS file ---------------------------------------- This example loads a FITS file (supplied on the commandline) and uses the WCS cards in its primary header to transform. .. literalinclude:: examples/from_file.py :language: python Building a WCS structure programmatically ----------------------------------------- This example, rather than starting from a FITS header, sets WCS values programmatically, uses those settings to transform some points, and then saves those settings to a new FITS header. .. literalinclude:: examples/programmatic.py :language: python pywcs-1.12/doc/source/index.rst0000644001153600020070000000115612310355626020557 0ustar cslocumSTSCI\science00000000000000.. pywcs documentation master file, created by sphinx-quickstart on Thu Sep 17 12:58:53 2009. You can adapt this file completely to your liking, but it should at least contain the root `toctree` directive. pywcs documentation =================== Python wrappers, SIP, Paper IV support (BSD License): `Michael Droettboom `_, Nadia Dencheva Space Telescope Science Institute wcslib (LGPL License): Mark Calabretta Australia Telescope National Facility, CSIRO (wcslib) .. automodule:: pywcs Contents: .. toctree:: :maxdepth: 2 examples.rst api.rst pywcs-1.12/doc/source/references.rst0000644001153600020070000000045612310355626021573 0ustar cslocumSTSCI\science00000000000000.. _wcslib: http://www.atnf.csiro.au/~mcalabre/WCS/ .. _pyfits: http://www.stsci.edu/resources/software_hardware/pyfits .. _Paper IV: http://www.atnf.csiro.au/people/mcalabre/WCS/index.html .. _SIP: http://ssc.spitzer.caltech.edu/postbcd/doc/shupeADASS.pdf .. _ds9: http://hea-www.harvard.edu/RD/ds9/ pywcs-1.12/doc/source/relax.rst0000644001153600020070000003434512310355626020571 0ustar cslocumSTSCI\science00000000000000.. include:: references.rst .. _relax: Relax constants ``````````````` .. _relaxread: Header-reading relaxation constants ----------------------------------- `~pywcs.WCS`, `~pywcs.Wcsprm` and `~pywcs.find_all_wcs` have a *relax* argument, which may be either `True`, `False` or an `int`. - If `True`, all non-standard WCS extensions recognized by the parser will be handled. - If `False` (default), none of the extensions (even those in the errata) will be handled. Non-conformant keywords will be handled in the same way as non-WCS keywords in the header, i.e. by simply ignoring them. - If an `int`, is is a bit field to provide fine-grained control over what non-standard WCS keywords to accept. The flag bits are subject to change in future and should be set by using the constants beginning with ``WCSHDR_`` in the `pywcs` module. For example, to accept ``CD00i00j`` and ``PC00i00j`` use:: relax = pywcs.WCSHDR_CD00i00j | pywcs.WCSHDR_PC00i00j The parser always treats ``EPOCH`` as subordinate to ``EQUINOXa`` if both are present, and ``VSOURCEa`` is always subordinate to ``ZSOURCEa``. Likewise, ``VELREF`` is subordinate to the formalism of WCS Paper III. The flag bits are: - `WCSHDR_none`: Don't accept any extensions (not even those in the errata). Treat non-conformant keywords in the same way as non-WCS keywords in the header, i.e. simply ignore them. (This is equivalent to the default behavior or passing `False`) - `WCSHDR_all`: Accept all extensions recognized by the parser. (This is equivalent to passing `True`). - `WCSHDR_CROTAia`: Accept ``CROTAia``, ``iCROTna``, ``TCROTna`` - `WCSHDR_EPOCHa`: Accept ``EPOCHa``. - `WCSHDR_VELREFa`: Accept ``VELREFa``. The constructor always recognizes the AIPS-convention keywords, ``CROTAn``, ``EPOCH``, and ``VELREF`` for the primary representation ``(a = ' ')`` but alternates are non-standard. The constructor accepts ``EPOCHa`` and ``VELREFa`` only if `WCSHDR_AUXIMG` is also enabled. - `WCSHDR_CD00i00j`: Accept ``CD00i00j``. - `WCSHDR_PC00i00j`: Accept ``PC00i00j``. - `WCSHDR_PROJPn`: Accept ``PROJPn`` These appeared in early drafts of WCS Paper I+II (before they were split) and are equivalent to ``CDi_ja``, ``PCi_ja``, and ``PVi_ma`` for the primary representation ``(a = ' ')``. ``PROJPn`` is equivalent to ``PVi_ma`` with ``m`` = ``n`` <= 9, and is associated exclusively with the latitude axis. - `WCSHDR_RADECSYS`: Accept ``RADECSYS``. This appeared in early drafts of WCS Paper I+II and was subsequently replaced by ``RADESYSa``. The construtor accepts ``RADECSYS`` only if `WCSHDR_AUXIMG` is also enabled. - `WCSHDR_VSOURCE`: Accept ``VSOURCEa`` or ``VSOUna``. This appeared in early drafts of WCS Paper III and was subsequently dropped in favour of ``ZSOURCEa`` and ``ZSOUna``. The constructor accepts ``VSOURCEa`` only if `WCSHDR_AUXIMG` is also enabled. - `WCSHDR_DOBSn`: Allow ``DOBSn``, the column-specific analogue of ``DATE-OBS``. By an oversight this was never formally defined in the standard. - `WCSHDR_LONGKEY`: Accept long forms of the alternate binary table and pixel list WCS keywords, i.e. with "a" non- blank. Specifically:: jCRPXna TCRPXna : jCRPXn jCRPna TCRPXn TCRPna CRPIXja - TPCn_ka : - ijPCna - TPn_ka PCi_ja - TCDn_ka : - ijCDna - TCn_ka CDi_ja iCDLTna TCDLTna : iCDLTn iCDEna TCDLTn TCDEna CDELTia iCUNIna TCUNIna : iCUNIn iCUNna TCUNIn TCUNna CUNITia iCTYPna TCTYPna : iCTYPn iCTYna TCTYPn TCTYna CTYPEia iCRVLna TCRVLna : iCRVLn iCRVna TCRVLn TCRVna CRVALia iPVn_ma TPVn_ma : - iVn_ma - TVn_ma PVi_ma iPSn_ma TPSn_ma : - iSn_ma - TSn_ma PSi_ma where the primary and standard alternate forms together with the image-header equivalent are shown rightwards of the colon. The long form of these keywords could be described as quasi- standard. ``TPCn_ka``, ``iPVn_ma``, and ``TPVn_ma`` appeared by mistake in the examples in WCS Paper II and subsequently these and also ``TCDn_ka``, ``iPSn_ma`` and ``TPSn_ma`` were legitimized by the errata to the WCS papers. Strictly speaking, the other long forms are non-standard and in fact have never appeared in any draft of the WCS papers nor in the errata. However, as natural extensions of the primary form they are unlikely to be written with any other intention. Thus it should be safe to accept them provided, of course, that the resulting keyword does not exceed the 8-character limit. If ``WCSHDR_CNAMn`` is enabled then also accept:: iCNAMna TCNAMna : --- iCNAna --- TCNAna CNAMEia iCRDEna TCRDEna : --- iCRDna --- TCRDna CRDERia iCSYEna TCSYEna : --- iCSYna --- TCSYna CSYERia Note that ``CNAMEia``, ``CRDERia``, ``CSYERia``, and their variants are not used by pywcs but are stored as auxiliary information. - `WCSHDR_CNAMn`: Accept ``iCNAMn``, ``iCRDEn``, ``iCSYEn``, ``TCNAMn``, ``TCRDEn``, and ``TCSYEn``, i.e. with ``a`` blank. While non-standard, these are the obvious analogues of ``iCTYPn``, ``TCTYPn``, etc. - `WCSHDR_AUXIMG`: Allow the image-header form of an auxiliary WCS keyword with representation-wide scope to provide a default value for all images. This default may be overridden by the column-specific form of the keyword. For example, a keyword like ``EQUINOXa`` would apply to all image arrays in a binary table, or all pixel list columns with alternate representation ``a`` unless overridden by ``EQUIna``. Specifically the keywords are:: LATPOLEa for LATPna LONPOLEa for LONPna RESTFREQ for RFRQna RESTFRQa for RFRQna RESTWAVa for RWAVna whose keyvalues are actually used by WCSLIB, and also keywords that provide auxiliary information that is simply stored in the wcsprm struct:: EPOCH - ... (No column-specific form.) EPOCHa - ... Only if WCSHDR_EPOCHa is set. EQUINOXa for EQUIna RADESYSa for RADEna RADECSYS for RADEna ... Only if WCSHDR_RADECSYS is set. SPECSYSa for SPECna SSYSOBSa for SOBSna SSYSSRCa for SSRCna VELOSYSa for VSYSna VELANGLa for VANGna VELREF - ... (No column-specific form.) VELREFa - ... Only if WCSHDR_VELREFa is set. VSOURCEa for VSOUna ... Only if WCSHDR_VSOURCE is set. WCSNAMEa for WCSNna ... Or TWCSna (see below). ZSOURCEa for ZSOUna DATE-AVG for DAVGn DATE-OBS for DOBSn MJD-AVG for MJDAn MJD-OBS for MJDOBn OBSGEO-X for OBSGXn OBSGEO-Y for OBSGYn OBSGEO-Z for OBSGZn where the image-header keywords on the left provide default values for the column specific keywords on the right. Keywords in the last group, such as ``MJD-OBS``, apply to all alternate representations, so ``MJD-OBS`` would provide a default value for all images in the header. This auxiliary inheritance mechanism applies to binary table image arrays and pixel lists alike. Most of these keywords have no default value, the exceptions being ``LONPOLEa`` and ``LATPOLEa``, and also ``RADESYSa`` and ``EQUINOXa`` which provide defaults for each other. Thus the only potential difficulty in using `WCSHDR_AUXIMG` is that of erroneously inheriting one of these four keywords. Unlike `WCSHDR_ALLIMG`, the existence of one (or all) of these auxiliary WCS image header keywords will not by itself cause a `~pywcs.Wcsprm` object to be created for alternate representation ``a``. This is because they do not provide sufficient information to create a non-trivial coordinate representation when used in conjunction with the default values of those keywords, such as ``CTYPEia``, that are parameterized by axis number. - `WCSHDR_ALLIMG`: Allow the image-header form of *all* image header WCS keywords to provide a default value for all image arrays in a binary table (n.b. not pixel list). This default may be overridden by the column-specific form of the keyword. For example, a keyword like ``CRPIXja`` would apply to all image arrays in a binary table with alternate representation ``a`` unless overridden by ``jCRPna``. Specifically the keywords are those listed above for `WCSHDR_AUXIMG` plus:: WCSAXESa for WCAXna which defines the coordinate dimensionality, and the following keywords which are parameterized by axis number:: CRPIXja for jCRPna PCi_ja for ijPCna CDi_ja for ijCDna CDELTia for iCDEna CROTAi for iCROTn CROTAia - ... Only if WCSHDR_CROTAia is set. CUNITia for iCUNna CTYPEia for iCTYna CRVALia for iCRVna PVi_ma for iVn_ma PSi_ma for iSn_ma CNAMEia for iCNAna CRDERia for iCRDna CSYERia for iCSYna where the image-header keywords on the left provide default values for the column specific keywords on the right. This full inheritance mechanism only applies to binary table image arrays, not pixel lists, because in the latter case there is no well-defined association between coordinate axis number and column number. Note that ``CNAMEia``, ``CRDERia``, ``CSYERia``, and their variants are not used by pywcs but are stored in the `~pywcs.Wcsprm` object as auxiliary information. Note especially that at least one `~pywcs.Wcsprm` object will be returned for each ``a`` found in one of the image header keywords listed above: - If the image header keywords for ``a`` **are not** inherited by a binary table, then the struct will not be associated with any particular table column number and it is up to the user to provide an association. - If the image header keywords for ``a`` **are** inherited by a binary table image array, then those keywords are considered to be "exhausted" and do not result in a separate `~pywcs.Wcsprm` object. .. _relaxwrite: Header-writing relaxation constants ----------------------------------- `~pywcs.WCS.to_header` and `~pywcs.WCS.to_header_string` has a *relax* argument which may be either `True`, `False` or an `int`. - If `True`, write all recognized extensions. - If `False` (default), none of the extensions (even those in the errata) will be written. - If an `int`, is is a bit field to provide fine-grained control over what non-standard WCS keywords to accept. The flag bits are subject to change in future and should be set by using the constants beginning with ``WCSHDO_`` in the `pywcs` module. The flag bits are: - `WCSHDO_none`: Don't use any extensions. - `WCSHDO_all`: Write all recognized extensions, equivalent to setting each flag bit. - `WCSHDO_safe`: Write all extensions that are considered to be safe and recommended. - `WCSHDO_DOBSn`: Write ``DOBSn``, the column-specific analogue of ``DATE-OBS`` for use in binary tables and pixel lists. WCS Paper III introduced ``DATE-AVG`` and ``DAVGn`` but by an oversight ``DOBSn`` (the obvious analogy) was never formally defined by the standard. The alternative to using ``DOBSn`` is to write ``DATE-OBS`` which applies to the whole table. This usage is considered to be safe and is recommended. - `WCSHDO_TPCn_ka`: WCS Paper I defined - ``TPn_ka`` and ``TCn_ka`` for pixel lists but WCS Paper II uses ``TPCn_ka`` in one example and subsequently the errata for the WCS papers legitimized the use of - ``TPCn_ka`` and ``TCDn_ka`` for pixel lists provided that the keyword does not exceed eight characters. This usage is considered to be safe and is recommended because of the non-mnemonic terseness of the shorter forms. - `WCSHDO_PVn_ma`: WCS Paper I defined - ``iVn_ma`` and ``iSn_ma`` for bintables and - ``TVn_ma`` and ``TSn_ma`` for pixel lists but WCS Paper II uses ``iPVn_ma`` and ``TPVn_ma`` in the examples and subsequently the errata for the WCS papers legitimized the use of - ``iPVn_ma`` and ``iPSn_ma`` for bintables and - ``TPVn_ma`` and ``TPSn_ma`` for pixel lists provided that the keyword does not exceed eight characters. This usage is considered to be safe and is recommended because of the non-mnemonic terseness of the shorter forms. - `WCSHDO_CRPXna`: For historical reasons WCS Paper I defined - ``jCRPXn``, ``iCDLTn``, ``iCUNIn``, ``iCTYPn``, and ``iCRVLn`` for bintables and - ``TCRPXn``, ``TCDLTn``, ``TCUNIn``, ``TCTYPn``, and ``TCRVLn`` for pixel lists for use without an alternate version specifier. However, because of the eight-character keyword constraint, in order to accommodate column numbers greater than 99 WCS Paper I also defined - ``jCRPna``, ``iCDEna``, ``iCUNna``, ``iCTYna`` and ``iCRVna`` for bintables and - ``TCRPna``, ``TCDEna``, ``TCUNna``, ``TCTYna`` and ``TCRVna`` for pixel lists for use with an alternate version specifier (the ``a``). Like the ``PC``, ``CD``, ``PV``, and ``PS`` keywords there is an obvious tendency to confuse these two forms for column numbers up to 99. It is very unlikely that any parser would reject keywords in the first set with a non-blank alternate version specifier so this usage is considered to be safe and is recommended. - `WCSHDO_CNAMna`: WCS Papers I and III defined - ``iCNAna``, ``iCRDna``, and ``iCSYna`` for bintables and - ``TCNAna``, ``TCRDna``, and ``TCSYna`` for pixel lists By analogy with the above, the long forms would be - ``iCNAMna``, ``iCRDEna``, and ``iCSYEna`` for bintables and - ``TCNAMna``, ``TCRDEna``, and ``TCSYEna`` for pixel lists Note that these keywords provide auxiliary information only, none of them are needed to compute world coordinates. This usage is potentially unsafe and is not recommended at this time. - `WCSHDO_WCSNna`: Write ``WCSNna`` instead of ``TWCSna`` for pixel lists. While the constructor treats ``WCSNna`` and ``TWCSna`` as equivalent, other parsers may not. Consequently, this usage is potentially unsafe and is not recommended at this time. - `WCSHDO_SIP`: Write out Simnple Imaging Polynomial (SIP) keywords pywcs-1.12/examples/0000755001153600020070000000000012310355732016462 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/examples/from_file.py0000644001153600020070000000212312310355627020777 0ustar cslocumSTSCI\science00000000000000# Load the WCS information from a fits header, and use it # to convert pixel coordinates to world coordinates. from __future__ import division # confidence high import numpy import pywcs import pyfits import sys # Load the FITS hdulist using pyfits hdulist = pyfits.open(sys.argv[-1]) # Parse the WCS keywords in the primary HDU wcs = pywcs.WCS(hdulist[0].header) # Print out the "name" of the WCS, as defined in the FITS header print wcs.wcs.name # Print out all of the settings that were parsed from the header wcs.wcs.print_contents() # Some pixel coordinates of interest. pixcrd = numpy.array([[0,0],[24,38],[45,98]], numpy.float_) # Convert pixel coordinates to world coordinates # The second argument is "origin" -- in this case we're declaring we # have 1-based (Fortran-like) coordinates. sky = wcs.wcs_pix2sky(pixcrd, 1) print sky # Convert the same coordinates back to pixel coordinates. pixcrd2 = wcs.wcs_sky2pix(sky, 1) print pixcrd2 # These should be the same as the original pixel coordinates, modulo # some floating-point error. assert numpy.max(numpy.abs(pixcrd - pixcrd2)) < 1e-6 pywcs-1.12/examples/programmatic.py0000644001153600020070000000255112310355627021527 0ustar cslocumSTSCI\science00000000000000# Set the WCS information manually by setting properties of the WCS # object. from __future__ import division # confidence high import numpy import pywcs import pyfits import sys # Create a new WCS object. The number of axes must be set # from the start wcs = pywcs.WCS(naxis=2) # Set up an "Airy's zenithal" projection # Vector properties may be set with Python lists, or Numpy arrays wcs.wcs.crpix = [-234.75, 8.3393] wcs.wcs.cdelt = numpy.array([-0.066667, 0.066667]) wcs.wcs.crval = [0, -90] wcs.wcs.ctype = ["RA---AIR", "DEC--AIR"] wcs.wcs.set_pv([(2, 1, 45.0)]) # Print out the "name" of the WCS, as defined in the FITS header print wcs.wcs.name wcs.wcs.print_contents() # Some pixel coordinates of interest. pixcrd = numpy.array([[0,0],[24,38],[45,98]], numpy.float_) # Convert pixel coordinates to world coordinates world = wcs.wcs_pix2sky(pixcrd, 1) print world # Convert the same coordinates back to pixel coordinates. pixcrd2 = wcs.wcs_sky2pix(world, 1) print pixcrd2 # These should be the same as the original pixel coordinates, modulo # some floating-point error. assert numpy.max(numpy.abs(pixcrd - pixcrd2)) < 1e-6 # Now, write out the WCS object as a FITS header header = wcs.to_header() # header is a PyFITS Header object. We can use it to create a new # PrimaryHDU and write it to a file. hdu = pyfits.PrimaryHDU(header=header) hdu.writeto('test.fits') pywcs-1.12/hooks.py0000644001153600020070000001201312310355627016341 0ustar cslocumSTSCI\science00000000000000import os from distutils.dist import Distribution def pywcs_hook(config) : WCSVERSION = config['metadata']['stsci_wcs_version'].strip() ## write wcsconfig.h write_if_different( 'src/wcsconfig.h', wcsconfig_h_proto % ( WCSVERSION, determine_64_bit_int()) ) ## circumvent buggy compilers adjust_compiler() return ###################################################################### def write_if_different(filename, data): data = data.encode('ascii') if os.path.exists(filename): with open(filename, 'rb') as fd: original_data = fd.read() else: original_data = None if original_data != data: with open(filename, 'wb') as fd: fd.write(data) ######################################################################u wcsconfig_h_proto = """ /* WCSLIB library version number. */ #define WCSLIB_VERSION %s /* 64-bit integer data type. */ #define WCSLIB_INT64 %s /* Windows needs some other defines */ /* I think the only one we need is _WIN32, but the others don't hurt - Mark S. 2012-02-14 */ #if defined(_WIN32) || defined(_MSC_VER) || defined(__MINGW32__) || defined (__MINGW64__) /* */ #ifndef YY_NO_UNISTD_H #define YY_NO_UNISTD_H #endif #ifndef _CRT_SECURE_NO_WARNINGS #define _CRT_SECURE_NO_WARNINGS #endif #ifndef _NO_OLDNAMES /* for mingw32 */ #define _NO_OLDNAMES #endif #ifndef NO_OLDNAMES /* for mingw64 */ #define NO_OLDNAMES #endif #ifndef __STDC__ /* for MS Visual C */ #define __STDC__ 1 #endif #endif """ # The only configuration parameter needed at compile-time is how to # specify a 64-bit signed integer. Python's ctypes module can get us # that information, but it is only available in Python 2.5 or later. # If we can't be absolutely certain, we default to "long long int", # which is correct on most platforms (x86, x86_64). If we find # platforms where this heuristic doesn't work, we may need to hardcode # for them. def determine_64_bit_int(): try: try: import ctypes except ImportError: raise ValueError() if ctypes.sizeof(ctypes.c_longlong) == 8: return "long long int" elif ctypes.sizeof(ctypes.c_long) == 8: return "long int" elif ctypes.sizeof(ctypes.c_int) == 8: return "int" else: raise ValueError() except ValueError: return "long long int" ###################################################################### def get_distutils_option(option, commands): """ Returns the value of the given distutils option. Parameters ---------- option : str The name of the option commands : list of str The list of commands on which this option is available Returns ------- val : str or None the value of the given distutils option. If the option is not set, returns None. """ # Pre-parse the Distutils command-line options and config files to # if the option is set. dist = Distribution() try: dist.parse_config_files() dist.parse_command_line() except DistutilsError: # Let distutils handle this itself return None except AttributeError: # This seems to get thrown for ./setup.py --help return None for cmd in commands: if cmd in dist.commands: break else: return None for cmd in commands: cmd_opts = dist.get_option_dict(cmd) if option in cmd_opts: return cmd_opts[option][1] else: return None def adjust_compiler(): """ This function detects broken compilers and switches to another. If the environment variable CC is explicitly set, or a compiler is specified on the commandline, no override is performed -- the purpose here is to only override a default compiler. The specific compilers with problems are: * The default compiler in XCode-4.2, llvm-gcc-4.2, segfaults when compiling wcslib. The set of broken compilers can be updated by changing the compiler_mapping variable. It is a list of 2-tuples where the first in the pair is a regular expression matching the version of the broken compiler, and the second is the compiler to change to. """ if 'CC' in os.environ: return if get_distutils_option( 'compiler', ['build', 'build_ext', 'build_clib']) is not None: return from distutils import ccompiler import subprocess import re compiler_mapping = [ ('i686-apple-darwin[0-9]*-llvm-gcc-4.2', 'clang') ] c = ccompiler.new_compiler() # The MSVC ccompiler class doesn't have a `compiler` member. if not hasattr(c, 'compiler'): return process = subprocess.Popen( c.compiler + ['--version'], stdout=subprocess.PIPE) output = process.communicate()[0].strip().decode('ascii') version = output.split()[0] for broken, fixed in compiler_mapping: if re.match(broken, version): os.environ['CC'] = fixed break pywcs-1.12/lib/0000755001153600020070000000000012310355732015412 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/0000755001153600020070000000000012310355732016557 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/__init__.py0000644001153600020070000000745412310355627020705 0ustar cslocumSTSCI\science00000000000000# Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) # Redistribution and use in source and binary forms, with or without # modification, are permitted provided that the following conditions are met: # 1. Redistributions of source code must retain the above copyright # notice, this list of conditions and the following disclaimer. # 2. Redistributions in binary form must reproduce the above # copyright notice, this list of conditions and the following # disclaimer in the documentation and/or other materials provided # with the distribution. # 3. The name of AURA and its representatives may not be used to # endorse or promote products derived from this software without # specific prior written permission. # THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED # WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF # MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE # DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, # INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, # BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS # OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND # ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR # TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE # USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH # DAMAGE. """ .. _wcslib: http://www.atnf.csiro.au/~mcalabre/WCS/ .. _pyfits: http://www.stsci.edu/resources/software_hardware/pyfits .. _Paper IV: http://www.atnf.csiro.au/people/mcalabre/WCS/index.html .. _SIP: http://ssc.spitzer.caltech.edu/postbcd/doc/shupeADASS.pdf .. _ds9: http://hea-www.harvard.edu/RD/ds9/ Pywcs provides transformations following the `SIP`_ conventions, `Paper IV`_ table lookup distortion, and the core WCS functionality provided by `wcslib`_. Each of these transformations can be used independently or together in a standard pipeline. The basic workflow is as follows: 1. ``import pywcs`` 2. Call the `pywcs.WCS` constructor with a `pyfits`_ header and/or hdulist object. 3. Optionally, if the FITS file uses any deprecated or non-standard features, you may need to call one of the `~pywcs.WCS.fix` methods on the object. 4. Use one of the following transformation methods: - `~WCS.all_pix2sky`: Perform all three transformations from pixel to sky coordinates. - `~WCS.wcs_pix2sky`: Perform just the core WCS transformation from pixel to sky coordinates. - `~WCS.wcs_sky2pix`: Perform just the core WCS transformation from sky to pixel coordinates. - `~WCS.sip_pix2foc`: Convert from pixel to focal plane coordinates using the `SIP`_ polynomial coefficients. - `~WCS.sip_foc2pix`: Convert from focal plane to pixel coordinates using the `SIP`_ polynomial coefficients. - `~WCS.p4_pix2foc`: Convert from pixel to focal plane coordinates using the table lookup distortion method described in `Paper IV`_. - `~WCS.det2im`: Convert from detector coordinates to image coordinates. Commonly used for narrow column correction. """ from __future__ import division # confidence high import sys if sys.version_info[0] >= 3: exec("from .pywcs import *") else: from .core import * def test( verbose=False ) : import os, sys, nose # find the directory where the test package lives from . import tests dir = os.path.dirname( tests.__file__ ) # get the name of the test package argv = [ 'nosetests', '--exe', dir ] # run nose try : return nose.main( argv = argv ) except SystemExit as e : return e.code from .version import * pywcs-1.12/lib/pywcs/_docutil.py0000644001153600020070000000557112310355627020746 0ustar cslocumSTSCI\science00000000000000# Copyright (C) 2008-2012 Association of Universities for Research in # Astronomy (AURA) # # Redistribution and use in source and binary forms, with or without # modification, are permitted provided that the following conditions # are met: # # 1. Redistributions of source code must retain the above # copyright notice, this list of conditions and the following # disclaimer. # # 2. Redistributions in binary form must reproduce the above # copyright notice, this list of conditions and the following # disclaimer in the documentation and/or other materials # provided with the distribution. # # 3. The name of AURA and its representatives may not be used to # endorse or promote products derived from this software without # specific prior written permission. # # THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR # IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED # WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE # ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, # INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES # (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR # SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) # HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, # STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) # ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED # OF THE POSSIBILITY OF SUCH DAMAGE. """ pywcs-specific utilities for generating boilerplate in docstrings. """ from __future__ import division # confidence high def _fix(content, indent=0): lines = content.split('\n') indent = '\n' + ' ' * indent return indent.join(lines) def TWO_OR_THREE_ARGS(out_type, naxis, indent=0): return _fix( """Either two or three arguments may be provided. - 2 arguments: An *N* x *%s* array of *x*- and *y*-coordinates, and an *origin*. - 3 arguments: 2 one-dimensional arrays of *x* and *y* coordinates, and an *origin*. Here, *origin* is the coordinate in the upper left corner of the image. In FITS and Fortran standards, this is 1. In Numpy and C standards this is 0. Returns the %s. If the input was a single array and origin, a single array is returned, otherwise a tuple of arrays is returned.""" % (naxis, out_type), indent) def ORIGIN(indent=0): return _fix( """ - *origin*: int. Specifies the origin of pixel values. The Fortran and FITS standards use an origin of 1. Numpy and C use array indexing with origin at 0. """, indent) def RA_DEC_ORDER(indent=0): return _fix( """ An optional keyword argument, *ra_dec_order*, may be provided, that when `True` will ensure that sky coordinates are always given and returned in as (*ra*, *dec*) pairs, regardless of the order of the axes specified by the in the ``CTYPE`` keywords. """, indent) pywcs-1.12/lib/pywcs/core.py0000644001153600020070000015155312310355627020076 0ustar cslocumSTSCI\science00000000000000# Copyright (C) 2008-2012 Association of Universities for Research in # Astronomy (AURA) # # Redistribution and use in source and binary forms, with or without # modification, are permitted provided that the following conditions # are met: # # 1. Redistributions of source code must retain the above # copyright notice, this list of conditions and the following # disclaimer. # # 2. Redistributions in binary form must reproduce the above # copyright notice, this list of conditions and the following # disclaimer in the documentation and/or other materials # provided with the distribution. # # 3. The name of AURA and its representatives may not be used to # endorse or promote products derived from this software without # specific prior written permission. # # THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR # IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED # WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE # ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, # INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES # (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR # SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) # HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, # STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) # ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED # OF THE POSSIBILITY OF SUCH DAMAGE. """ Under the hood, there are 3 separate classes that perform different parts of the transformation: - `~pywcs.Wcsprm`: Is a direct wrapper of the core WCS functionality in `wcslib`_. - `~pywcs.Sip`: Handles polynomial distortion as defined in the `SIP`_ convention. - `~pywcs.DistortionLookupTable`: Handles `Paper IV`_ distortion lookup tables. Additionally, the class `WCS` aggregates all of these transformations together in a pipeline: - Detector to image plane correction (by a pair of `~pywcs.DistortionLookupTable` objects). - `SIP`_ distortion correction (by an underlying `~pywcs.Sip` object) - `Paper IV`_ table-lookup distortion correction (by a pair of `~pywcs.DistortionLookupTable` objects). - `wcslib`_ WCS transformation (by a `~pywcs.Wcsprm` object) """ from __future__ import division # confidence high # stdlib import os import sys import copy import warnings if sys.version_info[0:2] >= (2, 6): from io import BytesIO else: from cStringIO import StringIO as BytesIO # third-party import numpy as np try: import pyfits HAS_PYFITS = True except ImportError: HAS_PYFITS = False # local if sys.version_info[0] >= 3: from . import _docutil as __ from . import _pywcs else: import _docutil as __ import _pywcs assert _pywcs._sanity_check(), \ """PyWcs did not pass its sanity check for your build on your platform. Please send details about your build and platform to mdroe@stsci.edu""" if sys.version_info[0] >= 3: string_types = (bytes,) else: string_types = (str, unicode) # bit flags for relax keyword WCSHDO_SIP = 0x40 # This is here for the sake of epydoc WCSBase = _pywcs._Wcs DistortionLookupTable = _pywcs.DistortionLookupTable Sip = _pywcs.Sip UnitConverter = _pywcs.UnitConverter class Wcsprm(_pywcs._Wcsprm): pass # Copy all the constants from the C extension into this module's namespace for key, val in _pywcs.__dict__.items(): if (key.startswith('WCSSUB') or key.startswith('WCSHDR') or key.startswith('WCSHDO')): locals()[key] = val # A wrapper around the C WCS type def _parse_keysel(keysel): keysel_flags = 0 if keysel is not None: for element in keysel: if element.lower() == 'image': keysel_flags |= _pywcs.WCSHDR_IMGHEAD elif element.lower() == 'binary': keysel_flags |= _pywcs.WCSHDR_BIMGARR elif element.lower() == 'pixel': keysel_flags |= _pywcs.WCSHDR_PIXLIST else: raise ValueError( "keysel must be a list of 'image', 'binary' and/or 'pixel'") else: keysel_flags = -1 return keysel_flags class WCS(WCSBase): """ WCS objects perform standard WCS transformations, and correct for `SIP`_ and `Paper IV`_ table-lookup distortions, based on the WCS keywords and supplementary data read from a FITS file. """ def __init__(self, header=None, fobj=None, key=' ', minerr=0.0, relax=False, naxis=None, keysel=None, colsel=None, fix=True): """ - *header*: A string containing the header content, or a PyFITS header object. If *header* is not provided or None, the object will be initialized to default values. - *fobj*: A PyFITS file (hdulist) object. It is needed when header keywords point to a `Paper IV`_ Lookup table distortion stored in a different extension. - *key*: A string. The name of a particular WCS transform to use. This may be either ``' '`` or ``'A'``-``'Z'`` and corresponds to the ``"a"`` part of the ``CTYPEia`` cards. *key* may only be provided if *header* is also provided. - *minerr*: A floating-point value. The minimum value a distortion correction must have in order to be applied. If the value of ``CQERRja`` is smaller than *minerr*, the corresponding distortion is not applied. - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to accept. See :ref:`relaxread` for details. - *naxis*: int or sequence. Extracts specific coordinate axes using :meth:`~pywcs.Wcsprm.sub`. If a header is provided, and *naxis* is not ``None``, *naxis* will be passed to :meth:`~pywcs.Wcsprm.sub` in order to select specific axes from the header. See :meth:`~pywcs.Wcsprm.sub` for more details about this parameter. - *keysel*: A list of flags used to select the keyword types considered by wcslib. When ``None``, only the standard image header keywords are considered (and the underlying wcspih() C function is called). To use binary table image array or pixel list keywords, *keysel* must be set. Each element in the list should be one of the following strings: - 'image': Image header keywords - 'binary': Binary table image array keywords - 'pixel': Pixel list keywords Keywords such as ``EQUIna`` or ``RFRQna`` that are common to binary table image arrays and pixel lists (including ``WCSNna`` and ``TWCSna``) are selected by both 'binary' and 'pixel'. - *colsel*: A sequence of table column numbers used to restrict the WCS transformations considered to only those pertaining to the specified columns. If `None`, there is no restriction. - *fix* : When `True` (default), call `fix` on the resulting object to fix any non-standard uses in the header. .. warning:: pywcs supports arbitrary *n* dimensions for the core WCS (the transformations handled by WCSLIB). However, the Paper IV lookup table and SIP distortions must be two dimensional. Therefore, if you try to create a WCS object where the core WCS has a different number of dimensions than 2 and that object also contains a Paper IV lookup table or SIP distortion, a `ValueError` exception will be raised. To avoid this, consider using the *naxis* kwarg to select two dimensions from the core WCS. **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid key. - `KeyError`: Key not found in FITS header. - `AssertionError`: Lookup table distortion present in the header but fobj not provided. """ if header is None: if naxis is None: naxis = 2 wcsprm = _pywcs._Wcsprm(header=None, key=key, relax=relax, naxis=naxis) self.naxis = wcsprm.naxis # Set some reasonable defaults. det2im = (None, None) cpdis = (None, None) sip = None else: keysel_flags = _parse_keysel(keysel) if isinstance(header, string_types): if HAS_PYFITS and os.path.exists(header): hdulist = pyfits.open(header) header = hdulist[0].header header_string = header.tostring() else: header_string = header elif HAS_PYFITS: assert isinstance(header, pyfits.Header) header_string = header.tostring() else: raise TypeError( "header must be a string or a pyfits.Header object") try: wcsprm = _pywcs._Wcsprm(header=header_string, key=key, relax=relax, keysel=keysel_flags, colsel=colsel) except _pywcs.NoWcsKeywordsFoundError: # The header may have SIP or distortions, but no core # WCS. That isn't an error -- we want a "default" # (identity) core Wcs transformation in that case. if colsel is None: wcsprm = _pywcs._Wcsprm(header=None, key=key, relax=relax, keysel=keysel_flags, colsel=colsel) else: raise if naxis is not None: wcsprm = wcsprm.sub(naxis) self.naxis = wcsprm.naxis det2im = self._read_det2im_kw(header, fobj, err=minerr) cpdis = self._read_distortion_kw( header, fobj, dist='CPDIS', err=minerr) sip = self._read_sip_kw(header) if (wcsprm.naxis != 2 and (det2im[0] or det2im[1] or cpdis[0] or cpdis[1] or sip)): raise ValueError( """ Paper IV lookup tables and SIP distortions only work in 2 dimensions. However, WCSLIB has detected %d dimensions in the core WCS keywords. To use core WCS in conjunction with Paper IV lookup tables or SIP distortion, you must select or reduce these to 2 dimensions using the naxis kwarg. """ % wcsprm.naxis) if fix: wcsprm.fix() self.get_naxis(header) WCSBase.__init__(self, sip, cpdis, wcsprm, det2im) def __copy__(self): new_copy = self.__class__() WCSBase.__init__(new_copy, self.sip, (self.cpdis1, self.cpdis2), self.wcs, (self.det2im1, self.det2im2)) new_copy.__dict__.update(self.__dict__) return new_copy def __deepcopy__(self, memo): new_copy = self.__class__() new_copy.naxis = copy.deepcopy(self.naxis, memo) WCSBase.__init__(new_copy, copy.deepcopy(self.sip, memo), (copy.deepcopy(self.cpdis1, memo), copy.deepcopy(self.cpdis2, memo)), copy.deepcopy(self.wcs, memo), (copy.deepcopy(self.det2im1, memo), copy.deepcopy(self.det2im2, memo))) for key in self.__dict__: val = self.__dict__[key] new_copy.__dict__[key] = copy.deepcopy(val, memo) return new_copy def copy(self): """ Return a shallow copy of the object. Convenience method so user doesn't have to import the :mod:`copy` stdlib module. """ return copy.copy(self) def deepcopy(self): """ Return a deep copy of the object. Convenience method so user doesn't have to import the :mod:`copy` stdlib module. """ return copy.deepcopy(self) def sub(self, axes=None): copy = self.deepcopy() copy.wcs = self.wcs.sub(axes) copy.naxis = copy.wcs.naxis return copy sub.__doc__ = _pywcs._Wcsprm.sub.__doc__ def calcFootprint(self, header=None, undistort=True): """ Calculates the footprint of the image on the sky. A footprint is defined as the positions of the corners of the image on the sky after all available distortions have been applied. Returns a (4, 2) array of (*x*, *y*) coordinates. """ if header is None: try: # classes that inherit from WCS and define naxis1/2 # do not require a header parameter naxis1 = self.naxis1 naxis2 = self.naxis2 except AttributeError : print("Need a valid header in order to calculate footprint\n") return None else: naxis1 = header.get('NAXIS1', None) naxis2 = header.get('NAXIS2', None) corners = np.zeros(shape=(4,2),dtype=np.float64) if naxis1 is None or naxis2 is None: return None corners[0,0] = 1. corners[0,1] = 1. corners[1,0] = 1. corners[1,1] = naxis2 corners[2,0] = naxis1 corners[2,1] = naxis2 corners[3,0] = naxis1 corners[3,1] = 1. if undistort: return self.all_pix2sky(corners, 1) else: return self.wcs_pix2sky(corners,1) def _read_det2im_kw(self, header, fobj, err=0.0): """ Create a `Paper IV`_ type lookup table for detector to image plane correction. """ if fobj is None: return (None, None) if not HAS_PYFITS: raise ImportError( "pyfits is required to use Paper IV lookup tables") if not isinstance(fobj, pyfits.HDUList): return (None, None) try: axiscorr = header['AXISCORR'] d2imdis = self._old_style_d2im(header, fobj, axiscorr) return d2imdis except KeyError: pass dist = 'D2IMDIS' d_kw = 'D2IM' err_kw = 'D2IMERR' tables = {} for i in range(1, self.naxis+1): d_error = header.get(err_kw+str(i), 0.0) if d_error < err: tables[i] = None continue distortion = dist+str(i) if distortion in header: dis = header[distortion].lower() if dis == 'lookup': if fobj is not None and not HAS_PYFITS: raise ImportError( "pyfits is required to use Paper IV lookup tables") assert isinstance(fobj, pyfits.HDUList), \ 'A pyfits HDUList is required for Lookup table distortion.' dp = (d_kw+str(i)).strip() d_extver = header.get(dp+'.EXTVER', 1) if i == header[dp+'.AXIS.%s'%i]: d_data = fobj['D2IMARR', d_extver].data else: d_data = (fobj['D2IMARR', d_extver].data).transpose() d_header = fobj['D2IMARR', d_extver].header d_crpix = (d_header.get('CRPIX1', 0.0), d_header.get('CRPIX2', 0.0)) d_crval = (d_header.get('CRVAL1', 0.0), d_header.get('CRVAL2', 0.0)) d_cdelt = (d_header.get('CDELT1', 1.0), d_header.get('CDELT2', 1.0)) d_lookup = DistortionLookupTable(d_data, d_crpix, d_crval, d_cdelt) tables[i] = d_lookup else: print('Polynomial distortion is not implemented.\n') else: tables[i] = None if not tables: return (None, None) else: return (tables.get(1), tables.get(2)) def _old_style_d2im(self, header, fobj, axiscorr): warnings.warn("The use of ``AXISCORR`` for D2IM correction has been deprecated." "The new style of this correction is described at" "" "PyWCS will read in files with ``AXISCORR`` but to_fits() will write" "out files in the new style", DeprecationWarning) cpdis = [None, None] crpix = [0.,0.] crval = [0.,0.] cdelt = [1.,1.] try: d2im_data = fobj[('D2IMARR', 1)].data except KeyError: return (None, None) except AttributeError: return (None, None) d2im_data = np.array([d2im_data]) d2im_hdr = fobj[('D2IMARR', 1)].header naxis = d2im_hdr['NAXIS'] for i in range(1,naxis+1): crpix[i-1] = d2im_hdr.get('CRPIX'+str(i), 0.0) crval[i-1] = d2im_hdr.get('CRVAL'+str(i), 0.0) cdelt[i-1] = d2im_hdr.get('CDELT'+str(i), 1.0) cpdis = DistortionLookupTable(d2im_data, crpix, crval, cdelt) if axiscorr == 1: return (cpdis, None) elif axiscorr == 2: return (None, cpdis) else: print "Expected AXISCORR to be 1 or 2" return (None, None) def _write_det2im(self, hdulist): """ Write out Detector to Image Correction to the given `pyfits.HDUList`. """ if self.det2im1 is None and self.det2im2 is None: return dist = 'D2IMDIS' d_kw = 'D2IM' err_kw = 'D2IMERR' def write_d2i(num, det2im): if det2im is None: return hdulist[0].header.update('%s%d' % (dist, num), value='LOOKUP', comment='Detector to image correction type') hdulist[0].header.update('%s%d.EXTVER' % (d_kw, num), value=num, comment='Version number of WCSDVARR extension') hdulist[0].header.update('%s%d.NAXES' % (d_kw, num), value=len(det2im.data.shape), comment='Number of independent variables in d2im function') for i in range(det2im.data.ndim): hdulist[0].header.update('%s%d.AXIS.%d' % (d_kw, num, i+1), value=i+1, comment='Axis number of the jth independent variable in a d2im function') image = pyfits.ImageHDU(det2im.data, name='D2IMARR') header = image.header header.update('CRPIX1', value=det2im.crpix[0], comment='Coordinate system reference pixel') header.update('CRPIX2', value=det2im.crpix[1], comment='Coordinate system reference pixel') header.update('CRVAL1', value=det2im.crval[0], comment='Coordinate system value at reference pixel') header.update('CRVAL2', value=det2im.crval[1], comment='Coordinate system value at reference pixel') header.update('CDELT1', value=det2im.cdelt[0], comment='Coordinate increment along axis') header.update('CDELT2', value=det2im.cdelt[1], comment='Coordinate increment along axis') image.update_ext_version(int(hdulist[0].header['%s%d.EXTVER' % (d_kw, num)])) hdulist.append(image) write_d2i(1, self.det2im1) write_d2i(2, self.det2im2) def _read_distortion_kw(self, header, fobj, dist='CPDIS', err=0.0): """ Reads `Paper IV`_ table-lookup distortion keywords and data, and returns a 2-tuple of `~pywcs.DistortionLookupTable` objects. If no `Paper IV`_ distortion keywords are found, ``(None, None)`` is returned. """ if isinstance(header, string_types): return (None, None) if dist == 'CPDIS': d_kw = 'DP' err_kw = 'CPERR' else: d_kw = 'DQ' err_kw = 'CQERR' tables = {} for i in range(1, self.naxis+1): d_error = header.get(err_kw+str(i), 0.0) if d_error < err: tables[i] = None continue distortion = dist+str(i) if distortion in header: dis = header[distortion].lower() if dis == 'lookup': if fobj is not None and not HAS_PYFITS: raise ImportError( "pyfits is required to use Paper IV lookup tables") assert isinstance(fobj, pyfits.HDUList), \ 'A pyfits HDUList is required for Lookup table distortion.' dp = (d_kw+str(i)).strip() d_extver = header.get(dp+'.EXTVER', 1) if i == header[dp+'.AXIS.%s'%i]: d_data = fobj['WCSDVARR', d_extver].data else: d_data = (fobj['WCSDVARR', d_extver].data).transpose() d_header = fobj['WCSDVARR', d_extver].header d_crpix = (d_header.get('CRPIX1', 0.0), d_header.get('CRPIX2', 0.0)) d_crval = (d_header.get('CRVAL1', 0.0), d_header.get('CRVAL2', 0.0)) d_cdelt = (d_header.get('CDELT1', 1.0), d_header.get('CDELT2', 1.0)) d_lookup = DistortionLookupTable(d_data, d_crpix, d_crval, d_cdelt) tables[i] = d_lookup else: print('Polynomial distortion is not implemented.\n') else: tables[i] = None if not tables: return (None, None) else: return (tables.get(1), tables.get(2)) def _write_distortion_kw(self, hdulist, dist='CPDIS'): """ Write out Paper IV distortion keywords to the given `pyfits.HDUList`. """ if self.cpdis1 is None and self.cpdis2 is None: return if dist == 'CPDIS': d_kw = 'DP' err_kw = 'CPERR' else: d_kw = 'DQ' err_kw = 'CQERR' def write_dist(num, cpdis): if cpdis is None: return hdulist[0].header.update('%s%d' % (dist, num), value='LOOKUP', comment='Prior distortion function type') hdulist[0].header.update('%s%d.EXTVER' % (d_kw, num), value=num, comment='Version number of WCSDVARR extension') hdulist[0].header.update('%s%d.NAXES' % (d_kw, num), value=len(cpdis.data.shape), comment='Number of independent variables in distortion function') for i in range(cpdis.data.ndim): hdulist[0].header.update('%s%d.AXIS.%d' % (d_kw, num, i+1), value=i+1, comment='Axis number of the jth independent variable in a distortion function') image = pyfits.ImageHDU(cpdis.data, name='WCSDVARR') header = image.header header.update('CRPIX1', value=cpdis.crpix[0], comment='Coordinate system reference pixel') header.update('CRPIX2', value=cpdis.crpix[1], comment='Coordinate system reference pixel') header.update('CRVAL1', value=cpdis.crval[0], comment='Coordinate system value at reference pixel') header.update('CRVAL2', value=cpdis.crval[1], comment='Coordinate system value at reference pixel') header.update('CDELT1', value=cpdis.cdelt[0], comment='Coordinate increment along axis') header.update('CDELT2', value=cpdis.cdelt[1], comment='Coordinate increment along axis') image.update_ext_version(int(hdulist[0].header['%s%d.EXTVER' % (d_kw, num)])) hdulist.append(image) write_dist(1, self.cpdis1) write_dist(2, self.cpdis2) def _read_sip_kw(self, header): """ Reads `SIP`_ header keywords and returns a `~pywcs.Sip` object. If no `SIP`_ header keywords are found, ``None`` is returned. """ if isinstance(header, string_types): # TODO: Parse SIP from a string without pyfits around return None if "A_ORDER" in header and header['A_ORDER'] > 1: if "B_ORDER" not in header: raise ValueError( "A_ORDER provided without corresponding B_ORDER " "keyword for SIP distortion") m = int(header["A_ORDER"]) a = np.zeros((m+1, m+1), np.double) for i in range(m+1): for j in range(m-i+1): a[i, j] = header.get(("A_%d_%d" % (i, j)), 0.0) m = int(header["B_ORDER"]) if m > 1: b = np.zeros((m+1, m+1), np.double) for i in range(m+1): for j in range(m-i+1): b[i, j] = header.get(("B_%d_%d" % (i, j)), 0.0) else: a = None b = None elif "B_ORDER" in header and header['B_ORDER'] > 1: raise ValueError( "B_ORDER provided without corresponding A_ORDER " "keyword for SIP distortion") else: a = None b = None if "AP_ORDER" in header and header['AP_ORDER'] > 1: if "BP_ORDER" not in header: raise ValueError( "AP_ORDER provided without corresponding BP_ORDER " "keyword for SIP distortion") m = int(header["AP_ORDER"]) ap = np.zeros((m+1, m+1), np.double) for i in range(m+1): for j in range(m-i+1): ap[i, j] = header.get("AP_%d_%d" % (i, j), 0.0) m = int(header["BP_ORDER"]) if m > 1: bp = np.zeros((m+1, m+1), np.double) for i in range(m+1): for j in range(m-i+1): bp[i, j] = header.get("BP_%d_%d" % (i, j), 0.0) else: ap = None bp = None elif "BP_ORDER" in header and header['BP_ORDER'] > 1: raise ValueError( "BP_ORDER provided without corresponding AP_ORDER " "keyword for SIP distortion") else: ap = None bp = None if a is None and b is None and ap is None and bp is None: return None if "CRPIX1" not in header or "CRPIX2" not in header: raise ValueError( "Header has SIP keywords without CRPIX keywords") crpix1 = header.get("CRPIX1") crpix2 = header.get("CRPIX2") return Sip(a, b, ap, bp, (crpix1, crpix2)) def _write_sip_kw(self): """ Write out SIP keywords. Returns a dictionary of key-value pairs. """ if self.sip is None: return {} keywords = {} def write_array(name, a): if a is None: return size = a.shape[0] keywords['%s_ORDER' % name] = size - 1 for i in range(size): for j in range(size - i): if a[i, j] != 0.0: keywords['%s_%d_%d' % (name, i, j)] = a[i, j] write_array('A', self.sip.a) write_array('B', self.sip.b) write_array('AP', self.sip.ap) write_array('BP', self.sip.bp) return keywords def _denormalize_sky(self, sky): if self.wcs.lngtyp != 'RA': raise ValueError( "WCS does not have longitude type of 'RA', therefore " + "(ra, dec) data can not be used as input") if self.wcs.lattype != 'DEC': raise ValueError( "WCS does not have longitude type of 'DEC', therefore " + "(ra, dec) data can not be used as input") if self.wcs.naxis == 2: if self.wcs.lng == 0 and self.wcs.lat == 1: return sky elif self.wcs.lng == 1 and self.wcs.lat == 0: # Reverse the order of the columns return sky[:,::-1] else: raise ValueError( "WCS does not have longitude and latitude celestial " + "axes, therefore (ra, dec) data can not be used as input") else: if self.wcs.lng < 0 or self.wcs.lat < 0: raise ValueError( "WCS does not have both longitude and latitude celestial " + "axes, therefore (ra, dec) data can not be used as input") out = np.zeros((sky.shape[0], self.wcs.naxis)) out[:,self.wcs.lng] = sky[:,0] out[:,self.wcs.lat] = sky[:,1] return out def _normalize_sky(self, sky): if self.wcs.lngtyp != 'RA': raise ValueError( "WCS does not have longitude type of 'RA', therefore " + "(ra, dec) data can not be returned") if self.wcs.lattype != 'DEC': raise ValueError( "WCS does not have longitude type of 'DEC', therefore " + "(ra, dec) data can not be returned") if self.wcs.naxis == 2: if self.wcs.lng == 0 and self.wcs.lat == 1: return sky elif self.wcs.lng == 1 and self.wcs.lat == 0: # Reverse the order of the columns return sky[:,::-1] else: raise ValueError( "WCS does not have longitude and latitude celestial " "axes, therefore (ra, dec) data can not be returned") else: if self.wcs.lng < 0 or self.wcs.lat < 0: raise ValueError( "WCS does not have both longitude and latitude celestial " "axes, therefore (ra, dec) data can not be returned") out = np.empty((sky.shape[0], 2)) out[:,0] = sky[:,self.wcs.lng] out[:,1] = sky[:,self.wcs.lat] return out def _array_converter(self, func, sky, *args, **kwargs): """ A helper function to support reading either a pair of arrays or a single Nx2 array. """ ra_dec_order = kwargs.get('ra_dec_order') if len(args) == 2: xy, origin = args try: xy = np.asarray(xy) origin = int(origin) except: raise TypeError( "When providing two arguments, they must be (xy, origin)") if ra_dec_order and sky == 'input': xy = self._denormalize_sky(xy) result = func(xy, origin) if ra_dec_order and sky == 'output': result = self._normalize_sky(result) return result elif len(args) == 3: x, y, origin = args try: x = np.asarray(x) y = np.asarray(y) origin = int(origin) except: raise TypeError( "When providing three arguments, they must be (x, y, origin)") if x.size != y.size: raise ValueError("x and y arrays are not the same size") length = x.size xy = np.hstack((x.reshape((length, 1)), y.reshape((length, 1)))) if ra_dec_order and sky == 'input': xy = self._denormalize_sky(xy) sky = func(xy, origin) if ra_dec_order and sky == 'output': sky = self._normalize_sky_output(sky) return sky[:, 0], sky[:, 1] return [sky[:, i] for i in range(sky.shape[1])] raise TypeError("Expected 2 or 3 arguments, %d given" % len(args)) def all_pix2sky(self, *args, **kwargs): return self._array_converter(self._all_pix2sky, 'output', *args, **kwargs) all_pix2sky.__doc__ = """ Transforms pixel coordinates to sky coordinates by doing all of the following in order: - Detector to image plane correction (optionally) - `SIP`_ distortion correction (optionally) - `Paper IV`_ table-lookup distortion correction (optionally) - `wcslib`_ WCS transformation %s %s For a transformation that is not two-dimensional, the two-argument form must be used. .. note:: The order of the axes for the result is determined by the `CTYPEia` keywords in the FITS header, therefore it may not always be of the form (*ra*, *dec*). The `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng`, `~pywcs.Wcsprm.lattyp` and `~pywcs.Wcsprm.lngtyp` members can be used to determine the order of the axes. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `ValueError`: Invalid coordinate transformation parameters. - `ValueError`: x- and y-coordinate arrays are not the same size. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS( 'sky coordinates, in degrees', 'naxis', 8), __.RA_DEC_ORDER(8)) def wcs_pix2sky(self, *args, **kwargs): if self.wcs is None: raise ValueError("No basic WCS settings were created.") return self._array_converter(lambda xy, o: self.wcs.p2s(xy, o)['world'], 'output', *args, **kwargs) wcs_pix2sky.__doc__ = """ Transforms pixel coordinates to sky coordinates by doing only the basic `wcslib`_ transformation. No `SIP`_ or `Paper IV`_ table lookup distortion correction is applied. To perform distortion correction, see `~pywcs.WCS.all_pix2sky`, `~pywcs.WCS.sip_pix2foc`, `~pywcs.WCS.p4_pix2foc`, or `~pywcs.WCS.pix2foc`. %s %s For a transformation that is not two-dimensional, the two-argument form must be used. .. note:: The order of the axes for the result is determined by the `CTYPEia` keywords in the FITS header, therefore it may not always be of the form (*ra*, *dec*). The `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng`, `~pywcs.Wcsprm.lattyp` and `~pywcs.Wcsprm.lngtyp` members can be used to determine the order of the axes. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `ValueError`: Invalid coordinate transformation parameters. - `ValueError`: x- and y-coordinate arrays are not the same size. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('sky coordinates, in degrees.', 'naxis', 8), __.RA_DEC_ORDER(8)) def wcs_sky2pix(self, *args, **kwargs): if self.wcs is None: raise ValueError("No basic WCS settings were created.") return self._array_converter(lambda xy, o: self.wcs.s2p(xy, o)['pixcrd'], 'input', *args, **kwargs) wcs_sky2pix.__doc__ = """ Transforms sky coordinates to pixel coordinates, using only the basic `wcslib`_ WCS transformation. No `SIP`_ or `Paper IV`_ table lookup distortion is applied. %s %s For a transformation that is not two-dimensional, the two-argument form must be used. .. note:: The order of the axes for the input sky array is determined by the `CTYPEia` keywords in the FITS header, therefore it may not always be of the form (*ra*, *dec*). The `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng`, `~pywcs.Wcsprm.lattyp` and `~pywcs.Wcsprm.lngtyp` members can be used to determine the order of the axes. **Exceptions:** - `MemoryError`: Memory allocation failed. - `SingularMatrixError`: Linear transformation matrix is singular. - `InconsistentAxisTypesError`: Inconsistent or unrecognized coordinate axis types. - `ValueError`: Invalid parameter value. - `InvalidTransformError`: Invalid coordinate transformation parameters. - `InvalidTransformError`: Ill-conditioned coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('pixel coordinates', 'naxis', 8), __.RA_DEC_ORDER(8)) def pix2foc(self, *args, **kwargs): return self._array_converter(self._pix2foc, None, *args, **kwargs) pix2foc.__doc__ = """ Convert pixel coordinates to focal plane coordinates using the `SIP`_ polynomial distortion convention and `Paper IV`_ table-lookup distortion correction. %s **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('focal coordinates', '2', 8)) def p4_pix2foc(self, *args, **kwargs): return self._array_converter(self._p4_pix2foc, None, *args, **kwargs) p4_pix2foc.__doc__ = """ Convert pixel coordinates to focal plane coordinates using `Paper IV`_ table-lookup distortion correction. %s **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('focal coordinates', '2', 8)) def det2im(self, *args, **kwargs): return self._array_converter(self._det2im, None, *args, **kwargs) det2im.__doc__ = """ Convert detector coordinates to image plane coordinates using `Paper IV`_ table-lookup distortion correction. %s **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('pixel coordinates', '2', 8)) def sip_pix2foc(self, *args, **kwargs): if self.sip is None: if len(args) == 2: return args[0] elif len(args) == 3: return args[:2] else: raise TypeError("Wrong number of arguments") return self._array_converter(self.sip.pix2foc, None, *args, **kwargs) sip_pix2foc.__doc__ = """ Convert pixel coordinates to focal plane coordinates using the `SIP`_ polynomial distortion convention. `Paper IV`_ table lookup distortion correction is not applied, even if that information existed in the FITS file that initialized this :class:`~pywcs.WCS` object. To correct for that, use `~pywcs.WCS.pix2foc` or `~pywcs.WCS.p4_pix2foc`. %s **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('focal coordinates', '2', 8)) def sip_foc2pix(self, *args, **kwargs): if self.sip is None: if len(args) == 2: return args[0] elif len(args) == 3: return args[:2] else: raise TypeError("Wrong number of arguments") return self._array_converter(self.sip.foc2pix, None, *args, **kwargs) sip_foc2pix.__doc__ = """ Convert focal plane coordinates to pixel coordinates using the `SIP`_ polynomial distortion convention. `Paper IV`_ table lookup distortion correction is not applied, even if that information existed in the FITS file that initialized this `~pywcs.WCS` object. %s **Exceptions:** - `MemoryError`: Memory allocation failed. - `ValueError`: Invalid coordinate transformation parameters. """ % (__.TWO_OR_THREE_ARGS('pixel coordinates', '2', 8)) def to_fits(self, relax=False, wkey=None): """ Generate a `pyfits.HDUList` object with all of the information stored in this object. This should be logically identical to the input FITS file, but it will be normalized in a number of ways. See `WCS.to_header` for some warnings about the output produced. - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to write. See :ref:`relaxwrite` for details. Returns a `pyfits.HDUList` object. """ if not HAS_PYFITS: raise ImportError( "pyfits is required to generate a FITS file") header = self.to_header(relax=relax, wkey=wkey) hdu = pyfits.PrimaryHDU(header=header) hdulist = pyfits.HDUList(hdu) self._write_det2im(hdulist) self._write_distortion_kw(hdulist) return hdulist def to_header(self, relax=False, wkey=None): """ Generate a `pyfits.Header` object with the basic WCS and SIP information stored in this object. This should be logically identical to the input FITS file, but it will be normalized in a number of ways. .. warning:: This function does not write out Paper IV distortion information, since that requires multiple FITS header data units. To get a full representation of everything in this object, use `to_fits`. The output header will almost certainly differ from the input in a number of respects: 1. The output header only contains WCS-related keywords. In particular, it does not contain syntactically-required keywords such as ``SIMPLE``, ``NAXIS``, ``BITPIX``, or ``END``. 2. Deprecated (e.g. ``CROTAn``) or non-standard usage will be translated to standard (this is partially dependent on whether `fix` was applied). 3. Quantities will be converted to the units used internally, basically SI with the addition of degrees. 4. Floating-point quantities may be given to a different decimal precision. 5. Elements of the ``PCi_j`` matrix will be written if and only if they differ from the unit matrix. Thus, if the matrix is unity then no elements will be written. 6. Additional keywords such as ``WCSAXES``, ``CUNITia``, ``LONPOLEa`` and ``LATPOLEa`` may appear. 7. The original keycomments will be lost, although `to_header` tries hard to write meaningful comments. 8. Keyword order may be changed. - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to write. See :ref:`relaxwrite` for details. - *wkey*: A string. The name of a particular WCS transform to use. This may be either ``' '`` or ``'A'``-``'Z'`` and corresponds to the ``"a"`` part of the ``CTYPEia`` cards. Returns a `pyfits.Header` object. """ if wkey: self.wcs.alt = wkey if not HAS_PYFITS: raise ImportError( "pyfits is required to generate a FITS header") dosip = False if (relax == True or relax == WCSHDO_all or (relax & WCSHDO_SIP)): dosip = True if relax not in (True, False): relax &= ~WCSHDO_SIP if self.wcs is not None: header_string = self.wcs.to_header(relax) cards = pyfits.CardList() for i in range(0, len(header_string), 80): card_string = header_string[i:i+80] if pyfits.__version__[0] >= '3': card = pyfits.Card.fromstring(card_string) else: card = pyfits.Card() card.fromstring(card_string) cards.append(card) header = pyfits.Header(cards) else: header = pyfits.Header() if dosip and self.sip is not None: for key, val in self._write_sip_kw().items(): header.update(key, val) return header def to_header_string(self, relax=False): """ Identical to `to_header`, but returns a string containing the header cards. """ return str(self.to_header(relax)) def __reduce__(self): """ Support pickling of WCS objects. This is done by serializing to an in-memory FITS file and dumping that as a string. """ if not HAS_PYFITS: raise ImportError( "pyfits is required for pickling support") hdulist = self.to_fits(relax=True) buffer = BytesIO() hdulist.writeto(buffer) return (_unpickle_wcs, (self.__class__, self.__dict__, buffer.getvalue(),)) def footprint_to_file(self, filename=None, color='green', width=2): """ Writes out a `ds9`_ style regions file. It can be loaded directly by `ds9`_. - *filename*: string. Output file name - default is ``'footprint.reg'`` - *color*: string. Color to use when plotting the line. - *width*: int. Width of the region line. """ if not filename: filename = 'footprint.reg' comments = '# Region file format: DS9 version 4.0 \n' comments += '# global color=green font="helvetica 12 bold select=1 highlite=1 edit=1 move=1 delete=1 include=1 fixed=0 source\n' f = open(filename, 'a') f.write(comments) f.write('linear\n') f.write('polygon(') self.footprint.tofile(f, sep=',') f.write(') # color=%s, width=%d \n' % (color, width)) f.close() def get_naxis(self, header=None): self.naxis1 = 0.0 self.naxis2 = 0.0 if header != None and not isinstance(header, string_types): self.naxis1 = header.get('NAXIS1', 0.0) self.naxis2 = header.get('NAXIS2', 0.0) def rotateCD(self, theta): _theta = DEGTORAD(theta) _mrot = np.zeros(shape=(2,2),dtype=np.double) _mrot[0] = (np.cos(_theta),np.sin(_theta)) _mrot[1] = (-np.sin(_theta),np.cos(_theta)) new_cd = np.dot(self.wcs.cd, _mrot) self.wcs.cd = new_cd def printwcs(self): """ Temporary function for internal use. """ print('WCS Keywords\n') if hasattr(self.wcs, 'cd'): print('CD_11 CD_12: %r %r' % (self.wcs.cd[0,0], self.wcs.cd[0,1])) print('CD_21 CD_22: %r %r' % (self.wcs.cd[1,0], self.wcs.cd[1,1])) print('CRVAL : %r %r' % (self.wcs.crval[0], self.wcs.crval[1])) print('CRPIX : %r %r' % (self.wcs.crpix[0], self.wcs.crpix[1])) print('NAXIS : %r %r' % (self.naxis1, self.naxis2)) def get_axis_types(self): """ ``list of dicts`` Similar to `self.wcsprm.axis_types <_pywcs._Wcsprm.axis_types>` but provides the information in a more Python-friendly format. Returns a list of dictionaries, one for each axis, each containing attributes about the type of that axis. Each dictionary has the following keys: - 'coordinate_type': - None: Non-specific coordinate type. - 'stokes': Stokes coordinate. - 'celestial': Celestial coordinate (including ``CUBEFACE``). - 'spectral': Spectral coordinate. - 'scale': - 'linear': Linear axis. - 'quantized': Quantized axis (``STOKES``, ``CUBEFACE``). - 'non-linear celestial': Non-linear celestial axis. - 'non-linear spectral': Non-linear spectral axis. - 'logarithmic': Logarithmic axis. - 'tabular': Tabular axis. - 'group' - Group number, e.g. lookup table number - 'number' - For celestial axes: - 0: Longitude coordinate. - 1: Latitude coordinate. - 2: ``CUBEFACE`` number. - For lookup tables: - the axis number in a multidimensional table. ``CTYPEia`` in ``"4-3"`` form with unrecognized algorithm code will generate an error. """ if self.wcs is None: raise AttributeError( "This WCS object does not have a wcsprm object.") coordinate_type_map = { 0: None, 1: 'stokes', 2: 'celestial', 3: 'spectral' } scale_map = { 0: 'linear', 1: 'quantized', 2: 'non-linear celestial', 3: 'non-linear spectral', 4: 'logarithmic', 5: 'tabular' } result = [] for axis_type in self.wcs.axis_types: subresult = {} coordinate_type = (axis_type // 1000) % 10 subresult['coordinate_type'] = coordinate_type_map[coordinate_type] scale = (axis_type // 100) % 10 subresult['scale'] = scale_map[scale] group = (axis_type // 10) % 10 subresult['group'] = group number = axis_type % 10 subresult['number'] = number result.append(subresult) return result def DEGTORAD(deg): return (deg * np.pi / 180.) def RADTODEG(rad): return (rad * 180. / np.pi) def find_all_wcs(header, relax=False, keysel=None): """ Find all the WCS transformations in the given header. - *header*: A string or PyFITS header object. - *relax*: Degree of permissiveness: - `False`: Recognize only FITS keywords defined by the published WCS standard. - `True`: Admit all recognized informal extensions of the WCS standard. - `int`: a bit field selecting specific extensions to accept. See :ref:`relaxread` for details. - *keysel*: A list of flags used to select the keyword types considered by wcslib. When ``None``, only the standard image header keywords are considered (and the underlying wcspih() C function is called). To use binary table image array or pixel list keywords, *keysel* must be set. Each element in the list should be one of the following strings: - 'image': Image header keywords - 'binary': Binary table image array keywords - 'pixel': Pixel list keywords Keywords such as ``EQUIna`` or ``RFRQna`` that are common to binary table image arrays and pixel lists (including ``WCSNna`` and ``TWCSna``) are selected by both 'binary' and 'pixel'. Returns a list of `WCS` objects. """ if isinstance(header, string_types): header_string = header elif HAS_PYFITS: assert isinstance(header, pyfits.Header) header_string = repr(header.ascard) else: raise TypeError( "header must be a string or pyfits.Header object") keysel_flags = _parse_keysel(keysel) wcsprms = _pywcs.find_all_wcs(header_string, relax, keysel_flags) result = [] for wcsprm in wcsprms: subresult = WCS() subresult.wcs = wcsprm result.append(subresult) return result def _unpickle_wcs(cls, dct, fits_data): """ Unpickles a WCS object from a serialized FITS string. """ if not HAS_PYFITS: raise ImportError( "pyfits is required for pickling support") self = cls.__new__(cls) self.__dict__.update(dct) buffer = BytesIO(fits_data) hdulist = pyfits.open(buffer) WCS.__init__(self, hdulist[0].header, hdulist) return self pywcs-1.12/lib/pywcs/hooks.py0000644001153600020070000000231212310355627020255 0ustar cslocumSTSCI\science00000000000000''' To compile another package that wants to link with the C code in pywcs: [build_ext] pre-hook.pywcs = pywcs.hooks.setup [extension=drizzlepac.cdriz] include_dirs = numpy pywcs libraries = pywcs m ''' import os def setup(command_obj) : # warning if we somehow get called when not building a c extension command_name = command_obj.get_command_name() if command_name != 'build_ext': log.warn('%s is meant to be used with the build_ext command only; ' 'it is not for use with the %s command.' % (__name__, command_name)) # get information from pywcs (ourselves) import pywcs pywcslib = pywcs.__path__[0] includes = [os.path.join(pywcslib, 'include'), os.path.join(pywcslib, 'include', 'wcslib')] # each place where the include directory is named exactly "pywcs", # replace it with the include directories computed above for extension in command_obj.extensions: if 'pywcs' not in extension.include_dirs: continue idx = extension.include_dirs.index('pywcs') for inc in includes: extension.include_dirs.insert(idx, inc) extension.include_dirs.remove('pywcs') pywcs-1.12/lib/pywcs/tests/0000755001153600020070000000000012310355732017721 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/tests/__init__.py0000644001153600020070000000000112310355627022024 0ustar cslocumSTSCI\science00000000000000 pywcs-1.12/lib/pywcs/tests/data/0000755001153600020070000000000012310355732020632 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/tests/data/3d_cd.hdr0000644001153600020070000000241712310355627022314 0ustar cslocumSTSCI\science00000000000000CD1_2 = -3.72E-05 CD1_3 = 0 CD1_1 = -4.12E-05 CUNIT3 = 'nm ' CUNIT2 = 'deg ' CTYPE1 = 'RA---TAN' NAXIS = 3 CTYPE3 = 'AWAV ' CD2_1 = -3.72E-05 CTYPE2 = 'DEC--TAN' CD2_3 = 0 CD2_2 = 4.12E-05 CUNIT1 = 'deg ' CD3_1 = 0 CD3_2 = 0 CD3_3 = 0.2 pywcs-1.12/lib/pywcs/tests/data/dist.fits0000644001153600020070000005500012310355627022467 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / conforms to FITS standard BITPIX = 8 / array data type NAXIS = 0 / number of array dimensions EXTEND = T WCSAXES = 2 / Number of coordinate axes CRPIX1 = 0 / Pixel coordinate of reference point CRPIX2 = 0 / Pixel coordinate of reference point CDELT1 = 1 / Coordinate increment at reference point CDELT2 = 1 / Coordinate increment at reference point CRVAL1 = 0 / Coordinate value at reference point CRVAL2 = 0 / Coordinate value at reference point LATPOLE = 90 / [deg] Native latitude of celestial pole RESTFRQ = 0 / [Hz] Line rest frequency RESTWAV = 0 / [Hz] Line rest wavelength AXISCORR= 2 D2IMEXT = 'test_d2i.fits' END XTENSION= 'IMAGE ' / Image extension BITPIX = -32 / array data type NAXIS = 1 / number of array dimensions NAXIS1 = 4096 PCOUNT = 0 / number of parameters GCOUNT = 1 / number of groups EXTNAME = 'D2IMARR ' / extension name CRPIX1 = 2048.0 CRPIX2 = 0.0 CRVAL1 = 2048.0 CRVAL2 = 0.0 CDELT1 = 1.0 CDELT2 = 1.0 END ¹}J¹Š!Žºì?º\A8º yݺÈ/jºðÕ¨» ¹b» 6 »ÃD»¾»T9» ¢ñ»‡;»*y^»E»]Bw»k»m C»b£»NØc»6»³}»»#:»?o»_ïn»xõ»ƒï»€Äq»[Gý»¿0ºµ½ºHº˜º(㲺±ý¸»#Ÿ:»E½»1*i»n5Àº©Q§;4Eï;-w¼;+Y;(A ;$úÅ;"˜û;R!;+Ã;(À; 8ž;(H:ú…õ:ñ½e:íÞà:è6<:åõ:ÛâZ:ÏD3:·TÄ:šnÂ:p˜¸:!¿9௴9’ =98 zd¸Óa¹e­²¹åi©ºCÉẓò#º¿p¸ºãw1» ,P» õk»Ô»¾»‡»Xl»X3»$ØY»=KS»X b»gü»n¬»fYM»Tö9»= œ»"ÕÉ»X+»þ°»7»WŽ>»sRÄ»‚·»ƒU»hnû»-Ö{ºÕ±ƒºgaøºÕܺ…ºÀ‚»Ϻ»E,»2í[»Y4±»33y;dÍ;.¦(;+Ì ;)%Ç;%gî;#x¬; 1Ò;O;uš;Zm;ç©:þéÈ:óa :ïžA:é:åõ:ßa:Ó*Ã:¿7[:¢/T:‚Ȧ:3X”9õ¨F9§Ð97ç48|RȸŒÑ.¹=”๾á˺+R‹º…÷º´ôoºØ²k»¦™»Cž»´»0Ÿ».×» “»f軟»5ࣻQÁ^»d}S»n¬»ieŠ»Z–\»C±»)`Ç»4+»ÀŒ»/±Ê»N‡»m4׶»„Q»s^»?…ýº÷ú:ºˆnwºæ#º*ÖºkºöA»>Jq»:O»D/»mlÛ:Áé;1jË;,>‘;*s‰;&GŸ;#åÔ;!‚;°; ~;Ï; ’;¦Î:ôh:ð±Ü:ëS|:åõ:áúÏ:Ö©‡:Æ`:©Nß:ŒÖæ:H˜±:Í9»üb9aØZ8¶–·û«Î¹vF¹¢®Éº¦üºoøº©¦ÊºÏ0ºûR&»°Ç» æz»IJ»¾»ˆ» è$»Ι»/Õ»Jœ 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Ó—»Ôƒ»ç‚»žÝ»ÊÈ»lû»":Z»9³%»Tþ·»f=o»n¬»gå'»Wö5»@‰ò»&,»7‚»`¯»3¢»RÕÚ»pE»ñv»ƒŸK»n1»6Ï*ºæyIºzsº%ªº ÿ̺‚·e»¼»B~g»6cƒ»NLú»U7ý;‡¯;/Ñ^;+òÆ;*„;%×™;#¾x; ¡};â¥;Tð;9Ä;C;„Z:ów :ð}•:êVh:åõ:àh¹:Ôél:´­:¥Î«:ˆ¢:=ÐŒ:9±{Ç9L×"8šø¸QÚž¹-õ¹°¯“º '’º}øݺ¯¸qºÔ†»)F»D÷»Ý»T¬»¿,»xŽ» ¨=»n¾»2C»ND »b¹~»m]„»jöÁ»], »Gð»,Þ»òÖ»Ô:»+ø»J‹z»iËK»HB»„mG»x\E»G•°»ËKº“Åκ(“äº eºT %ºá’Ë»7øá»>¤‘»;ç>»z˜:VÊ;3)w;,_î;*ã4;&·J;$U€;!-;¢;¡Ê;ù%; øé;°ç:ö&À:ñWè:ë¯D:æž:ã¹y:Øh0:ȵ]:­~Ã:Ë?:T“@: È39ÆtZ9u¥ß8Ò)·(X ¹ €õ¹‘¤º .ÿºbdmº£‹vºÊ`ŽºôW}»N» ÅÏ»S »¾»˜Ý» KI»ŸÎ»,,»FÓû»^[ »kž#»lÓ'»aŠ»MO˜»4N,»bÍ»nï»$úø»AÎ’»b¤»zEλ„'­»€M»WŽ »$˺®uºApº·«º01mººÂ6»(9•»Dïç»2e¡»s8ºbÓ;5!y;-?Ÿ;+P];'Û=;$©;"`Þ;îà;ƒm;¸‡; ¸J;¸:ù¥‚:ñ–í:ín¦:çÆ:屜:Ûã:Íóƒ:µ“Ø:˜­Õ:kUò:n9Ûlí9ŒÈw9 ™7à×(¸á¸¹p33¹î.@ºIíº—O̺Á£¦ºæˆÊ» _» …0»+º»¾»F¤»ȧ»AZ»&) »?D\»YŸ»hÜ»n¬»exØ»Sml»;K²»!à» `»O`»9ˆ»Y´ä»tÛ‘»ƒ =»‚ý»e%E»)t3ºÍ].º^iº 4}ºÆ.º˜¤»ÚN»EÓ »2 ç»^¯€»1 ;#Òo;.5ï;+½†;(é3;%/Ñ;#@;ùµ;“;  ; ê4;wo:ýÿ:ó Œ:ï.:è¤L:åõ:Þ€¦:ÒJM:½.s:Ÿþ,:€'B:.™=9ðe€9¡Á 9/=G8`C÷¸šØƒ¹FB ¹Ç¦aº1uÁº‰xíº·•ÐºÛSË»>Û» »DU»l»fô»{Í»Un» êä»7Ù©»SwY»e]Ë»n¬»hŒâ»YEª»B(»'¤Š»§S»;»1ªÐ»P¦Â»n½»»€ »ƒ×4»pÞ»;[Òºï5«º‚»€ºƒÛº `âºx5»Cè»@¿!»8V »I–»búJ:ãªe;0ŠY;,*®;*;m;&‚;#¾x; Ùf;Rv;ÄÁ;©•;©X;,:óæÞ:ð±Ü:ë6:åõ:á]:ÕÉ:Äsõ:§ñ:Š£Œ:C`:Kµ9¶¹›9WRË8¨-¸'ëë¹#yf¹©²tº齺vû¾º¬¸eºÑ¼‘ºþÓü»x©» v?»Œ•»¾»@¦» È™»H»0˜¡»L„À»a¡ð»lí²»kž}»^C–»H¹ ».d»Òy»Ï»*98»H\b»gê«»~0µ»„mG»zzN»K„» adºšêº-Û¥º-ºJҺ׆õ»4zR»@wè»8e?»{Œõ9Ý*Û;4 ;,—Ø;*æù;&ï3;$i;!¹;ÿµ;›;h÷; hº;X¡:÷b:ñ–í:ì:ævr:äb:ÙG×:ÊØ:¯­ä:’Š†:YÑ:FÁ9˲-9|¢ú8ßú_³Ipywcs-1.12/lib/pywcs/tests/data/outside_sky.hdr0000644001153600020070000000267712310355627023712 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / BITPIX = -32 / NAXIS = 2 / NAXIS1 = 2048 / NAXIS2 = 2048 / EXTEND = T / BSCALE = 1.00000000000E+00 / BZERO = 0.00000000000E+00 / CDELT1 = -8.19629704013E-02 / CRPIX1 = 1.02500000000E+03 / CRVAL1 = 79.95701 CTYPE1 = 'RA---SIN' / CDELT2 = 8.19629704013E-02 / CRPIX2 = 1.02500000000E+03 / CRVAL2 = -45.779 CTYPE2 = 'DEC--SIN' / EPOCH = 2.00000000000E+03 / PV2_1 = -0.755124458581295 PV2_2 = 0.209028857410973 pywcs-1.12/lib/pywcs/tests/data/sip.fits0000644001153600020070000001320012310355627022313 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / conforms to FITS standard BITPIX = 8 / array data type NAXIS = 0 / number of array dimensions WCSAXES = 2 / Number of coordinate axes CRPIX1 = 128.0 / Pixel coordinate of reference point CRPIX2 = 128.0 / Pixel coordinate of reference point PC1_1 = 0.000249756880272 / Coordinate transformation matrix element PC1_2 = 0.000230177809744 / Coordinate transformation matrix element PC2_1 = 0.000230428519265 / Coordinate transformation matrix element PC2_2 = -0.000249965770577 / Coordinate transformation matrix element CDELT1 = 1 / [deg] Coordinate increment at reference point CDELT2 = 1 / [deg] Coordinate increment at reference point CUNIT1 = 'deg' / Units of coordinate increment and value CUNIT2 = 'deg' / Units of coordinate increment and value CTYPE1 = 'RA---TAN-SIP' / Right ascension, gnomonic projection CTYPE2 = 'DEC--TAN-SIP' / Declination, gnomonic projection CRVAL1 = 202.482322805 / [deg] Coordinate value at reference point CRVAL2 = 47.17511893 / [deg] Coordinate value at reference point LONPOLE = 180 / [deg] Native longitude of celestial pole LATPOLE = 47.17511893 / [deg] Native latitude of celestial pole RESTFRQ = 0 / [Hz] Line rest frequency RESTWAV = 0 / [Hz] Line rest wavelength CRDER1 = 4.02509762361E-05 / [deg] Random error in coordinate CRDER2 = 3.42746131953E-05 / [deg] Random error in coordinate RADESYS = 'ICRS' / Equatorial coordinate system EQUINOX = 2000 / [yr] Equinox of equatorial coordinates BP_0_1 = -1.6588E-05 BP_0_2 = -2.3424E-05 A_3_0 = -1.4172E-07 B_3_0 = -2.0249E-08 BP_3_0 = 2.0482E-08 B_1_2 = -5.7813E-09 B_1_1 = -2.4386E-05 B_2_1 = -1.6583E-07 B_2_0 = 2.1197E-06 A_ORDER = 3 B_0_3 = -1.6168E-07 B_0_2 = 2.31E-05 BP_0_3 = 1.651E-07 B_ORDER = 3 BP_ORDER= 3 BP_1_2 = 3.8917E-09 AP_ORDER= 3 AP_3_0 = 1.4492E-07 A_1_1 = 2.1886E-05 BP_2_0 = -2.151E-06 A_1_2 = -1.6847E-07 AP_2_1 = 6.709E-09 AP_2_0 = 2.4146E-05 A_0_2 = 2.9656E-06 A_0_3 = 3.7746E-09 BP_1_1 = 2.4753E-05 BP_1_0 = -2.6783E-06 A_2_0 = -2.3863E-05 A_2_1 = -8.561E-09 AP_1_0 = -1.4897E-05 AP_1_1 = -2.225E-05 AP_1_2 = 1.7195E-07 BP_2_1 = 1.7E-07 AP_0_1 = -6.4275E-07 AP_0_3 = -3.582E-09 AP_0_2 = -2.9425E-06 END pywcs-1.12/lib/pywcs/tests/data/sip2.fits0000644001153600020070000001320012310355627022375 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / conforms to FITS standard BITPIX = 8 / array data type NAXIS = 0 / number of array dimensions WCSAXES = 2 / Number of coordinate axes CRPIX1 = 128.0 / Pixel coordinate of reference point CRPIX2 = 128.0 / Pixel coordinate of reference point PC1_1 = 0.000249756880272 / Coordinate transformation matrix element PC1_2 = 0.000230177809744 / Coordinate transformation matrix element PC2_1 = 0.000230428519265 / Coordinate transformation matrix element PC2_2 = -0.000249965770577 / Coordinate transformation matrix element CDELT1 = 1 / [deg] Coordinate increment at reference point CDELT2 = 1 / [deg] Coordinate increment at reference point CUNIT1 = 'deg' / Units of coordinate increment and value CUNIT2 = 'deg' / Units of coordinate increment and value CTYPE1 = 'RA---TAN-SIP' / Right ascension, gnomonic projection CTYPE2 = 'DEC--TAN-SIP' / Declination, gnomonic projection CRVAL1 = 202.482322805 / [deg] Coordinate value at reference point CRVAL2 = 47.17511893 / [deg] Coordinate value at reference point LONPOLE = 180 / [deg] Native longitude of celestial pole LATPOLE = 47.17511893 / [deg] Native latitude of celestial pole RESTFRQ = 0 / [Hz] Line rest frequency RESTWAV = 0 / [Hz] Line rest wavelength CRDER1 = 4.02509762361E-05 / [deg] Random error in coordinate CRDER2 = 3.42746131953E-05 / [deg] Random error in coordinate RADESYS = 'ICRS' / Equatorial coordinate system EQUINOX = 2000 / [yr] Equinox of equatorial coordinates A_3_0 = -1.4172E-07 B_3_0 = -2.0249E-08 B_1_2 = -5.7813E-09 B_1_1 = -2.4386E-05 B_2_1 = -1.6583E-07 B_2_0 = 2.1197E-06 A_ORDER = 3 B_0_3 = -1.6168E-07 B_0_2 = 2.31E-05 B_ORDER = 3 A_1_1 = 2.1886E-05 A_1_2 = -1.6847E-07 A_0_2 = 2.9656E-06 A_0_3 = 3.7746E-09 A_2_0 = -2.3863E-05 A_2_1 = -8.561E-09 END pywcs-1.12/lib/pywcs/tests/maps/0000755001153600020070000000000012310355732020661 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/tests/maps/1904-66_AIR.hdr0000644001153600020070000002210012310355626022676 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---AIR' CRPIX1 = -2.347545010835E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--AIR' CRPIX2 = 8.339330824422E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole PV2_1 = 4.500000000000E+01 / Projection parameter 1 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:43:31 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_AIR.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_AIT.hdr0000644001153600020070000002176012310355626022713 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---AIT' CRPIX1 = -2.462317116277E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--AIT' CRPIX2 = 7.115850027049E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:04:34 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_AIT.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_ARC.hdr0000644001153600020070000002176012310355626022703 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---ARC' CRPIX1 = -2.469419019050E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--ARC' CRPIX2 = 5.082274450444E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:35:43 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_ARC.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_AZP.hdr0000644001153600020070000002222012310355627022721 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---AZP' CRPIX1 = -2.541100848779E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--AZP' CRPIX2 = -1.134948542534E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole PV2_1 = 2.000000000000E+00 / Projection parameter 1 PV2_2 = 3.000000000000E+01 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:16:54 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_AZP.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_BON.hdr0000644001153600020070000002210012310355626022701 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---BON' CRPIX1 = -2.431263982441E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--BON' CRPIX2 = -3.307412668190E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole PV2_1 = 4.500000000000E+01 / Projection parameter 1 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:17:44 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_BON.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_CAR.hdr0000644001153600020070000002176012310355626022703 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---CAR' CRPIX1 = -2.482173814412E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--CAR' CRPIX2 = 7.527038199745E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:51:20 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_CAR.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_CEA.hdr0000644001153600020070000002210012310355627022654 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---CEA' CRPIX1 = -2.482173814412E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--CEA' CRPIX2 = 7.688571124876E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole PV2_1 = 1.000000000000E+00 / Projection parameter 1 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:48:41 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_CEA.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_COD.hdr0000644001153600020070000002222012310355626022673 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---COD' CRPIX1 = -2.153431714695E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--COD' CRPIX2 = 1.561302682707E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -4.500000000000E+01 / Native latitude of celestial pole PV2_1 = 4.500000000000E+01 / Projection parameter 1 PV2_2 = 2.500000000000E+01 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:12:30 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_COD.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_COE.hdr0000644001153600020070000002222012310355626022674 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---COE' CRPIX1 = -2.230375366798E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--COE' CRPIX2 = -1.435249668783E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 4.500000000000E+01 / Native latitude of celestial pole PV2_1 = -4.500000000000E+01 / Projection parameter 1 PV2_2 = 2.500000000000E+01 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:09:50 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_COE.continuum.fits". HISTORY Noise level of continuum map: 62 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_COO.hdr0000644001153600020070000002222012310355626022706 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---COO' CRPIX1 = -2.136486051767E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--COO' CRPIX2 = 1.292640949564E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -4.500000000000E+01 / Native latitude of celestial pole PV2_1 = 4.500000000000E+01 / Projection parameter 1 PV2_2 = 2.500000000000E+01 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:15:07 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_COO.continuum.fits". HISTORY Noise level of continuum map: 62 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_COP.hdr0000644001153600020070000002222012310355626022707 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---COP' CRPIX1 = -2.151923139086E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--COP' CRPIX2 = 1.505768272737E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -4.500000000000E+01 / Native latitude of celestial pole PV2_1 = 4.500000000000E+01 / Projection parameter 1 PV2_2 = 2.500000000000E+01 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:07:13 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_COP.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_CSC.hdr0000644001153600020070000002176012310355626022706 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---CSC' CRPIX1 = -2.686531829635E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--CSC' CRPIX2 = -7.043520126533E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:25:39 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_CSC.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_CYP.hdr0000644001153600020070000002222012310355627022722 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---CYP' CRPIX1 = -1.471055514007E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--CYP' CRPIX2 = 2.056099939277E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole PV2_1 = 1.000000000000E+00 / Projection parameter 1 PV2_2 = 7.071067811870E-01 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:46:07 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_CYP.continuum.fits". HISTORY Noise level of continuum map: 62 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_HPX.hdr0000644001153600020070000002234012310355626022730 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 / number of data axes NAXIS1 = 192 / length of data axis 1 NAXIS2 = 192 / length of data axis 2 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H BUNIT = 'Jy/beam ' / Pixel value is flux density CTYPE1 = 'RA---HPX' CRPIX1 = -248.217381441188 CDELT1 = -0.0666666666666667 CRVAL1 = 0. CTYPE2 = 'DEC--HPX' CRPIX2 = -8.21754831338666 CDELT2 = 0.0666666666666667 CRVAL2 = -90. LONPOLE = 180. / Native longitude of celestial pole LATPOLE = 0. / Native latitude of celestial pole RADESYS = 'FK5 ' / Equatorial coordinate system EQUINOX = 2000.0 / Equinox of equatorial coordinates BMAJ = 0.24000 / Beam major axis in degrees BMIN = 0.24000 / Beam minor axis in degrees BPA = 0.0 / Beam position angle in degrees HISTORY Single-dish continuum map HISTORY Formed on Mon 2005/03/07 04:03:52 GMT by "pksgridzilla" which was HISTORY compiled on Mar 6 2005 08:00:15 (local time) within HISTORY AIPS++ version 19.986.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_HPX.continuum.fits". HISTORY Noise level of continuum map: 57 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_MER.hdr0000644001153600020070000002176012310355627022722 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---MER' CRPIX1 = -2.482173814412E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--MER' CRPIX2 = 7.364978412864E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:53:59 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_MER.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_MOL.hdr0000644001153600020070000002176012310355627022726 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---MOL' CRPIX1 = -2.127655947497E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--MOL' CRPIX2 = -2.310670994515E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:01:55 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_MOL.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_NCP.hdr0000644001153600020070000002222012310355626022706 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---SIN' CRPIX1 = -2.371895431541E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--SIN' CRPIX2 = 7.688572009351E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole PV2_1 = 0.000000000000E+00 / Projection parameter 1 PV2_2 = -1.216796447506E-08 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:33:03 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_NCP.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_PAR.hdr0000644001153600020070000002176012310355626022720 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---PAR' CRPIX1 = -2.465551494284E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--PAR' CRPIX2 = 3.322937769653E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:59:17 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_PAR.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_PCO.hdr0000644001153600020070000002176012310355626022717 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---PCO' CRPIX1 = -2.462486098896E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--PCO' CRPIX2 = 3.620782775517E-01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:20:22 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_PCO.continuum.fits". HISTORY Noise level of continuum map: 62 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_QSC.hdr0000644001153600020070000002176012310355627022725 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---QSC' CRPIX1 = -2.583408175994E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--QSC' CRPIX2 = -8.258194421088E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:28:25 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_QSC.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_SFL.hdr0000644001153600020070000002176012310355627022723 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---SFL' CRPIX1 = -2.463483086237E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--SFL' CRPIX2 = 7.527038199745E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:56:37 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_SFL.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_SIN.hdr0000644001153600020070000002222012310355627022720 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---SIN' CRPIX1 = -2.371895431541E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--SIN' CRPIX2 = 7.688571124876E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole PV2_1 = 0.000000000000E+00 / Projection parameter 1 PV2_2 = 0.000000000000E+00 / Projection parameter 2 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:30:25 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_SIN.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_STG.hdr0000644001153600020070000002176012310355626022733 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---STG' CRPIX1 = -2.519459909290E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--STG' CRPIX2 = 3.744942537739E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:26:55 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_STG.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_SZP.hdr0000644001153600020070000002234012310355626022745 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---SZP' CRPIX1 = -2.478656972779E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--SZP' CRPIX2 = -2.262051956373E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole PV2_1 = 2.000000000000E+00 / Projection parameter 1 PV2_2 = 1.800000000000E+02 / Projection parameter 2 PV2_3 = 6.000000000000E+01 / Projection parameter 3 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:20:19 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_SZP.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_TAN.hdr0000644001153600020070000002176012310355626022720 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---TAN' CRPIX1 = -2.680658087122E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--TAN' CRPIX2 = -5.630437201085E-01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:23:37 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_TAN.continuum.fits". HISTORY Noise level of continuum map: 59 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_TSC.hdr0000644001153600020070000002176012310355627022730 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---TSC' CRPIX1 = -1.897220156818E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--TSC' CRPIX2 = 2.037416464676E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = 0.000000000000E+00 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 02:23:02 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_TSC.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_ZEA.hdr0000644001153600020070000002176012310355626022715 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---ZEA' CRPIX1 = -2.444880690361E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--ZEA' CRPIX2 = 5.738055949994E+00 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:40:52 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_ZEA.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/maps/1904-66_ZPN.hdr0000644001153600020070000002506012310355626022742 0ustar cslocumSTSCI\science00000000000000SIMPLE = T BITPIX = -32 / IEEE (big-endian) 32-bit floating point data NAXIS = 2 NAXIS1 = 192 NAXIS2 = 192 BUNIT = 'JY/BEAM ' CTYPE1 = 'RA---ZPN' CRPIX1 = -1.832937255632E+02 CDELT1 = -6.666666666667E-02 CRVAL1 = 0.000000000000E+00 CTYPE2 = 'DEC--ZPN' CRPIX2 = 2.209211120575E+01 CDELT2 = 6.666666666667E-02 CRVAL2 = -9.000000000000E+01 LONPOLE = 1.800000000000E+02 / Native longitude of celestial pole LATPOLE = -9.000000000000E+01 / Native latitude of celestial pole PV2_0 = 5.000000000000E-02 / Projection parameter 0 PV2_1 = 9.750000000000E-01 / Projection parameter 1 PV2_2 = -8.070000000000E-01 / Projection parameter 2 PV2_3 = 3.370000000000E-01 / Projection parameter 3 PV2_4 = -6.500000000000E-02 / Projection parameter 4 PV2_5 = 1.000000000000E-02 / Projection parameter 5 PV2_6 = 3.000000000000E-03 / Projection parameter 6 PV2_7 = -1.000000000000E-03 / Projection parameter 7 PV2_8 = 0.000000000000E+00 / Projection parameter 8 PV2_9 = 0.000000000000E+00 / Projection parameter 9 PV2_10 = 0.000000000000E+00 / Projection parameter 10 PV2_11 = 0.000000000000E+00 / Projection parameter 11 PV2_12 = 0.000000000000E+00 / Projection parameter 12 PV2_13 = 0.000000000000E+00 / Projection parameter 13 PV2_14 = 0.000000000000E+00 / Projection parameter 14 PV2_15 = 0.000000000000E+00 / Projection parameter 15 PV2_16 = 0.000000000000E+00 / Projection parameter 16 PV2_17 = 0.000000000000E+00 / Projection parameter 17 PV2_18 = 0.000000000000E+00 / Projection parameter 18 PV2_19 = 0.000000000000E+00 / Projection parameter 19 EQUINOX = 2.000000000000E+03 / Equinox of equatorial coordinates BMAJ = 2.399999936422E-01 / Beam major axis in degrees BMIN = 2.399999936422E-01 / Beam minor axis in degrees BPA = 0.000000000000E+00 / Beam position angle in degrees RESTFRQ = 1.420405750000E+09 / Line rest frequency, Hz HISTORY Parkes Multibeam continuum map HISTORY Formed on Mon 2004/02/09 01:38:20 GMT by "pksgridzilla" which was HISTORY compiled on Feb 9 2004 12:08:02 (local time) within HISTORY AIPS++ version 19.405.00 dated . HISTORY Polarization mode: A and B aggregated HISTORY Gridding parameters: HISTORY Method: WGTMED HISTORY Clip fraction: 0.000 HISTORY Tsys weighting: applied HISTORY Beam weight order: 1 HISTORY Beam FWHM: 14.4 arcmin HISTORY Beam normalization: applied HISTORY Smoothing kernel type: TOP-HAT HISTORY Kernel FWHM: 12.0 arcmin HISTORY Cutoff radius: 6.0 arcmin HISTORY Beam RSS cutoff: 0.0 HISTORY Input data sets: HISTORY 97-10-09_0356_193558-66_206a.sdfits HISTORY 97-10-12_0142_182123-66_193a.sdfits HISTORY 97-10-12_0151_182707-66_194a.sdfits HISTORY 97-10-12_0200_183252-66_195a.sdfits HISTORY 97-11-07_0510_183836-66_196a.sdfits HISTORY 97-11-07_0519_184420-66_197a.sdfits HISTORY 97-11-07_0528_185004-66_198a.sdfits HISTORY 97-11-07_0537_185548-66_199a.sdfits HISTORY 97-11-07_0546_190132-66_200a.sdfits HISTORY 97-11-07_0556_190717-66_201a.sdfits HISTORY 97-11-07_0645_191301-66_202a.sdfits HISTORY 97-11-07_0654_191845-66_203a.sdfits HISTORY 97-11-07_0703_192429-66_204a.sdfits HISTORY 97-11-07_0712_193013-66_205a.sdfits HISTORY 97-11-07_0724_194142-66_207a.sdfits HISTORY 97-11-18_0256_193815-66_206c.sdfits HISTORY 97-11-18_0306_194359-66_207c.sdfits HISTORY 97-11-19_0447_182341-66_193c.sdfits HISTORY 97-11-19_0456_182925-66_194c.sdfits HISTORY 97-11-19_0507_190350-66_200c.sdfits HISTORY 97-11-19_0516_190934-66_201c.sdfits HISTORY 97-11-19_0525_191519-66_202c.sdfits HISTORY 97-11-19_0534_192103-66_203c.sdfits HISTORY 97-11-19_0544_192647-66_204c.sdfits HISTORY 97-11-19_0553_193231-66_205c.sdfits HISTORY 97-11-19_0602_183509-66_195c.sdfits HISTORY 97-11-19_0612_184053-66_196c.sdfits HISTORY 97-11-19_0622_184638-66_197c.sdfits HISTORY 97-11-19_0631_185222-66_198c.sdfits HISTORY 97-11-19_0640_185806-66_199c.sdfits HISTORY 98-03-24_2107_193706-66_206b.sdfits HISTORY 98-03-24_2116_194251-66_207b.sdfits HISTORY 98-03-25_2020_190826-66_201b.sdfits HISTORY 98-03-25_2029_191410-66_202b.sdfits HISTORY 98-03-25_2038_191954-66_203b.sdfits HISTORY 98-03-25_2047_192538-66_204b.sdfits HISTORY 98-03-25_2056_193122-66_205b.sdfits HISTORY 98-03-26_2048_190459-66_200d.sdfits HISTORY 98-03-27_2034_191627-66_202d.sdfits HISTORY 98-03-27_2043_192212-66_203d.sdfits HISTORY 98-03-27_2052_192756-66_204d.sdfits HISTORY 98-03-27_2102_193340-66_205d.sdfits HISTORY 98-03-27_2111_193924-66_206d.sdfits HISTORY 98-03-27_2120_194508-66_207d.sdfits HISTORY 98-03-27_2130_191043-66_201d.sdfits HISTORY 98-05-10_2123_182232-66_193b.sdfits HISTORY 98-05-10_2133_182816-66_194b.sdfits HISTORY 98-05-10_2142_183400-66_195b.sdfits HISTORY 98-05-10_2151_183945-66_196b.sdfits HISTORY 98-05-10_2200_184529-66_197b.sdfits HISTORY 98-05-10_2209_185113-66_198b.sdfits HISTORY 98-05-10_2219_185657-66_199b.sdfits HISTORY 98-05-10_2228_190241-66_200b.sdfits HISTORY 98-05-13_2132_182450-66_193d.sdfits HISTORY 98-05-13_2151_183034-66_194d.sdfits HISTORY 98-05-13_2200_183618-66_195d.sdfits HISTORY 98-05-13_2210_184202-66_196d.sdfits HISTORY 98-05-13_2219_184746-66_197d.sdfits HISTORY 98-05-13_2228_185331-66_198d.sdfits HISTORY 98-05-13_2237_185915-66_199d.sdfits HISTORY 98-05-25_1711_182559-66_193e.sdfits HISTORY 98-05-25_1720_183143-66_194e.sdfits HISTORY 98-05-25_1729_183727-66_195e.sdfits HISTORY 98-05-25_1738_184311-66_196e.sdfits HISTORY 98-05-25_1747_184855-66_197e.sdfits HISTORY 98-05-25_1756_185439-66_198e.sdfits HISTORY 98-05-25_1806_190024-66_199e.sdfits HISTORY 98-05-25_1815_190608-66_200e.sdfits HISTORY 98-05-25_1824_191152-66_201e.sdfits HISTORY 98-05-25_1833_191736-66_202e.sdfits HISTORY 98-05-25_1842_192320-66_203e.sdfits HISTORY 98-05-25_1851_192905-66_204e.sdfits HISTORY 98-05-25_1901_193449-66_205e.sdfits HISTORY 98-05-25_1910_194033-66_206e.sdfits HISTORY 98-05-25_1919_194617-66_207e.sdfits HISTORY Original FITS filename "1904-66_ZPN.continuum.fits". HISTORY Noise level of continuum map: 61 mJy (RMS) pywcs-1.12/lib/pywcs/tests/nrao/0000755001153600020070000000000012310355732020660 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/tests/nrao/gls.hdr0000644001153600020070000000300212310355626022141 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / Written by GBES1: 8-Mar-1994 11:29:18.00 BITPIX = -32 / NAXIS = 2 / NAXIS1 = 640 / NAXIS2 = 512 / DATE = '08/03/94' / Creation date (DD/MM/YY) of FITS header CTYPE1 = 'RA---GLS' / Coordinate system and projection CRPIX1 = 352.000 / Reference pixel CRVAL1 = 0.00000 / value at reference CDELT1 = -1.40500 / increment at reference CD001001= 1.00000 / no rotation, skew CTYPE2 = 'DEC--GLS' / Coordinate system and projection CRPIX2 = 267.000 / Reference pixel CRVAL2 = 0.00000 / value at reference CDELT2 = 2.26000 / increment at reference CD002002= 1.00000 / no rotation, skew RADECSYS= 'FK5 ' / fundamental coordinate system EQUINOX = 2000.00 / equinox for coordinate system LONGPOLE= 180.000 / Projection system north pole pywcs-1.12/lib/pywcs/tests/nrao/m28opt.hdr0000644001153600020070000002643012310355626022517 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / BITPIX = 16 / NAXIS = 3 / NAXIS1 = 558 / NAXIS2 = 262 / NAXIS3 = 1 / EXTEND = T /Tables following main image BLOCKED = T /Tape may be blocked OBJECT = 'NONE ' TELESCOP= ' ' INSTRUME= ' ' OBSERVER= ' ' DATE-OBS= ' ' DATE-MAP= '13/09/94' BSCALE = 2.78159340659E-03 /REAL = TAPE * BSCALE + BZERO BZERO = 1.08125000000E+02 / BUNIT = ' ' EPOCH = 0.000000000E+00 /EPOCH OF RA DEC DATAMAX = 1.992500000E+02 /MAX PIXEL VALUE DATAMIN = 1.700000000E+01 /MIN PIXEL VALUE CTYPE1 = 'RA---ARC' CRVAL1 = 1.47927100003E+02 / CDELT1 = -2.247777738E-04 / CRPIX1 = 3.015000000E+02 / CROTA1 = 0.000000000E+00 / CTYPE2 = 'DEC--ARC' CRVAL2 = 6.99079999924E+01 / CDELT2 = 2.273333375E-04 / CRPIX2 = 9.550000000E+01 / CROTA2 = 2.426000023E+01 / CTYPE3 = 'FREQ ' CRVAL3 = 6.67000032461E+14 / CDELT3 = 1.000000000E+00 / CRPIX3 = 1.000000000E+00 / CROTA3 = 0.000000000E+00 / HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /Tape may be blocked HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY Created by fitstopgm. HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 2 HISTORY IMLOD INFILE = 'FITS2:M82BLUE.FITS ' HISTORY IMLOD RELEASE = '15JUL94' HISTORY TRANS RELEASE ='15JUL94 ' /********* Start 23-MAR-1994 09:33:39 HISTORY TRANS INNAME='M82 MW blue ' INCLASS='IMAP ' HISTORY TRANS INSEQ= 1 INDISK= 2 HISTORY TRANS OUTNAME='M82 in blue ' OUTCLASS='TRANS ' HISTORY TRANS OUTSEQ= 2 OUTDISK= 2 HISTORY TRANS BLC= 1., 1., 1., 1., 1., 1., 1. / Input image HISTORY TRANS TRC= 847.,1292., 1., 1., 1., 1., 1. / Input image HISTORY TRANS TRANCOD='-2-1 HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE3 = 'X ' / NEW Axis type HISTORY AXDEF CRVAL3 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT3 = -2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX3 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE1 = ' ' / OLD Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT1 = -1.00000E+00 / OLD Axis increment HISTORY AXDEF CRPIX1 = 647.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE1 = 'X ' / NEW Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT1 = -2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX1 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = ' ' / OLD Axis type HISTORY AXDEF CRVAL2 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT2 = -1.00000E+00 / OLD Axis increment HISTORY AXDEF CRPIX2 = 425.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'Y ' / NEW Axis type HISTORY AXDEF CRVAL2 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE3 = 'X ' / OLD Axis type HISTORY AXDEF CRVAL3 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT3 = -2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX3 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE3 = 'FREQ ' / NEW Axis type HISTORY AXDEF CRVAL3 = 9.999999870E+14 / NEW Reference pixel value HISTORY AXDEF CDELT3 = 2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX3 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE3 = 'FREQ ' / OLD Axis type HISTORY AXDEF CRVAL3 = 9.999999870E+14 / OLD Reference pixel value HISTORY AXDEF CDELT3 = 2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX3 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE3 = 'FREQ ' / NEW Axis type HISTORY AXDEF CRVAL3 = 9.999999870E+14 / NEW Reference pixel value HISTORY AXDEF CDELT3 = 1.00000E+00 / NEW Axis increment HISTORY AXDEF CRPIX3 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE1 = 'X ' / OLD Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT1 = -2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX1 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE1 = 'X ' / NEW Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT1 = 2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX1 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE1 = 'X ' / OLD Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT1 = 2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX1 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE1 = 'RA---ARC' / NEW Axis type HISTORY AXDEF CRVAL1 = 1.479284000E+02 / NEW Reference pixel value HISTORY AXDEF CDELT1 = -1.06583E-04 / NEW Axis increment HISTORY AXDEF CRPIX1 = 577.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = 'Y ' / OLD Axis type HISTORY AXDEF CRVAL2 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT2 = 2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX2 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'RA---ARC' / NEW Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 502.000 / NEW Reference pixel loc HISTORY PUTHEAD CROTA2 = 0.00000E+00 / old HISTORY PUTHEAD CROTA2 = 2.40000E+01 / new HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = 'RA---ARC' / OLD Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / OLD Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / OLD Axis increment HISTORY AXDEF CRPIX2 = 502.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'DEC--SIN' / NEW Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 502.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = 'DEC--SIN' / OLD Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / OLD Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / OLD Axis increment HISTORY AXDEF CRPIX2 = 502.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'DEC--ARC' / NEW Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 502.000 / NEW Reference pixel loc HISTORY PUTHEAD CROTA2 = 2.40000E+01 / old HISTORY PUTHEAD CROTA2 = -2.40000E+01 / new HISTORY PUTHEAD CROTA2 = -2.40000E+01 / old HISTORY PUTHEAD CROTA2 = 2.40000E+01 / new HISTORY PUTHEAD CROTA2 = 2.40000E+01 / old HISTORY PUTHEAD CROTA2 = 0.00000E+00 / new HISTORY PUTHEAD CROTA2 = 0.00000E+00 / old HISTORY PUTHEAD CROTA2 = 2.40000E+01 / new HISTORY PUTHEAD CRVAL3 = 9.999999870E+14 / old HISTORY PUTHEAD CRVAL3 = 6.670000325E+14 / new HISTORY PUTHEAD CROTA2 = 2.40000E+01 / old HISTORY PUTHEAD CROTA2 = 2.64000E+01 / new HISTORY PUTHEAD CDELT1 = -1.06583E-04 / old HISTORY PUTHEAD CDELT1 = -1.09861E-04 / new HISTORY PUTHEAD CDELT2 = 1.13917E-04 / old HISTORY PUTHEAD CDELT2 = 1.13667E-04 / new HISTORY PUTHEAD CDELT1 = -1.09861E-04 / old HISTORY PUTHEAD CDELT1 = -1.12389E-04 / new HISTORY PUTHEAD CROTA2 = 2.64000E+01 / old HISTORY PUTHEAD CROTA2 = 2.42600E+01 / new HISTORY PUTHEAD CRVAL1 = 1.479284000E+02 / old HISTORY PUTHEAD CRVAL1 = 1.479271000E+02 / new HISTORY PUTHEAD CRPIX1 = 5.77000E+02 / old HISTORY PUTHEAD CRPIX1 = 6.46000E+02 / new HISTORY PUTHEAD CRPIX2 = 5.02000E+02 / old HISTORY PUTHEAD CRPIX2 = 4.24000E+02 / new HISTORY PUTHEAD CRVAL2 = 6.992031002E+01 / old HISTORY PUTHEAD CRVAL2 = 6.990799999E+01 / new HISTORY SUBIM RELEASE ='15JUL94 ' /********* Start 25-MAR-1994 09:30:57 HISTORY SUBIM INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY SUBIM INSEQ= 2 INDISK= 2 HISTORY SUBIM INTYPE ='MA' USERID= 103 HISTORY SUBIM OUTNAME='M82 in blue ' OUTCLASS='SUBIM ' HISTORY SUBIM OUTSEQ= 1 OUTDISK= 2 HISTORY SUBIM BLC = 45, 235, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 1159, 759, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 2 YINC = 2 HISTORY SUBIM OPCODE = 'AVE ' HISTORY AIPS IMNAME='M82 in blue ' IMCLASS='SUBIM ' IMSEQ= 1 / HISTORY AIPS USERNO= 103 / HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 4 HISTORY IMLOD INFILE = 'FITS2:M82BLUE.FITS ' HISTORY IMLOD RELEASE = '15JAN95' HISTORY SUBIM RELEASE ='15JAN95 ' /********* Start 13-SEP-1994 12:59:44 HISTORY SUBIM INNAME='M82 in blue ' INCLASS='SUBIM ' HISTORY SUBIM INSEQ= 1 INDISK= 4 HISTORY SUBIM INTYPE ='MA' USERID= 103 HISTORY SUBIM OUTNAME='M82 ' OUTCLASS='Blue ' HISTORY SUBIM OUTSEQ= 3 OUTDISK= 4 HISTORY SUBIM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 558, 262, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 1 YINC = 1 HISTORY SUBIM OPCODE = ' ' ORIGIN = 'AIPSGorilla (NRAOCV IPX) 15JAN95' / DATE = '13/09/94' / File written on dd/mm/yy HISTORY AIPS IMNAME='M82 ' IMCLASS='Blue ' IMSEQ= 3 / HISTORY AIPS USERNO= 103 / ENDpywcs-1.12/lib/pywcs/tests/nrao/m82opt.hdr0000644001153600020070000004154412310355626022522 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / BITPIX = 16 / NAXIS = 3 / NAXIS1 = 558 / NAXIS2 = 262 / NAXIS3 = 1 / EXTEND = T /Tables following main image BLOCKED = T /Tape may be blocked OBJECT = 'NONE ' TELESCOP= ' ' INSTRUME= ' ' OBSERVER= ' ' DATE-OBS= ' ' DATE-MAP= '13/09/94' BSCALE = 2.78159340659E-03 /REAL = TAPE * BSCALE + BZERO BZERO = 1.08125000000E+02 / BUNIT = ' ' EPOCH = 0.000000000E+00 /EPOCH OF RA DEC DATAMAX = 1.992500000E+02 /MAX PIXEL VALUE DATAMIN = 1.700000000E+01 /MIN PIXEL VALUE CTYPE1 = 'RA---ARC' CRVAL1 = 1.47927100003E+02 / CDELT1 = -2.247777738E-04 / CRPIX1 = 3.015000000E+02 / CROTA1 = 0.000000000E+00 / CTYPE2 = 'DEC--ARC' CRVAL2 = 6.99079999924E+01 / CDELT2 = 2.273333375E-04 / CRPIX2 = 9.550000000E+01 / CROTA2 = 2.426000023E+01 / CTYPE3 = 'FREQ ' CRVAL3 = 6.67000032461E+14 / CDELT3 = 1.000000000E+00 / CRPIX3 = 1.000000000E+00 / CROTA3 = 0.000000000E+00 / HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /Tape may be blocked HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY Created by fitstopgm. HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 2 HISTORY IMLOD INFILE = 'FITS2:M82BLUE.FITS ' HISTORY IMLOD RELEASE = '15JUL94' HISTORY TRANS RELEASE ='15JUL94 ' /********* Start 23-MAR-1994 09:33:39 HISTORY TRANS INNAME='M82 MW blue ' INCLASS='IMAP ' HISTORY TRANS INSEQ= 1 INDISK= 2 HISTORY TRANS OUTNAME='M82 in blue ' OUTCLASS='TRANS ' HISTORY TRANS OUTSEQ= 2 OUTDISK= 2 HISTORY TRANS BLC= 1., 1., 1., 1., 1., 1., 1. / Input image HISTORY TRANS TRC= 847.,1292., 1., 1., 1., 1., 1. / Input image HISTORY TRANS TRANCOD='-2-1 HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE3 = 'X ' / NEW Axis type HISTORY AXDEF CRVAL3 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT3 = -2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX3 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE1 = ' ' / OLD Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT1 = -1.00000E+00 / OLD Axis increment HISTORY AXDEF CRPIX1 = 647.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE1 = 'X ' / NEW Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT1 = -2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX1 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = ' ' / OLD Axis type HISTORY AXDEF CRVAL2 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT2 = -1.00000E+00 / OLD Axis increment HISTORY AXDEF CRPIX2 = 425.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'Y ' / NEW Axis type HISTORY AXDEF CRVAL2 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE3 = 'X ' / OLD Axis type HISTORY AXDEF CRVAL3 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT3 = -2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX3 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE3 = 'FREQ ' / NEW Axis type HISTORY AXDEF CRVAL3 = 9.999999870E+14 / NEW Reference pixel value HISTORY AXDEF CDELT3 = 2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX3 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE3 = 'FREQ ' / OLD Axis type HISTORY AXDEF CRVAL3 = 9.999999870E+14 / OLD Reference pixel value HISTORY AXDEF CDELT3 = 2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX3 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE3 = 'FREQ ' / NEW Axis type HISTORY AXDEF CRVAL3 = 9.999999870E+14 / NEW Reference pixel value HISTORY AXDEF CDELT3 = 1.00000E+00 / NEW Axis increment HISTORY AXDEF CRPIX3 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE1 = 'X ' / OLD Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT1 = -2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX1 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE1 = 'X ' / NEW Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / NEW Reference pixel value HISTORY AXDEF CDELT1 = 2.77778E-04 / NEW Axis increment HISTORY AXDEF CRPIX1 = 1.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE1 = 'X ' / OLD Axis type HISTORY AXDEF CRVAL1 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT1 = 2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX1 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE1 = 'RA---ARC' / NEW Axis type HISTORY AXDEF CRVAL1 = 1.479284000E+02 / NEW Reference pixel value HISTORY AXDEF CDELT1 = -1.06583E-04 / NEW Axis increment HISTORY AXDEF CRPIX1 = 577.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = 'Y ' / OLD Axis type HISTORY AXDEF CRVAL2 = 0.000000000E+00 / OLD Reference pixel value HISTORY AXDEF CDELT2 = 2.77778E-04 / OLD Axis increment HISTORY AXDEF CRPIX2 = 1.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'RA---ARC' / NEW Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 502.000 / NEW Reference pixel loc HISTORY PUTHEAD CROTA2 = 0.00000E+00 / old HISTORY PUTHEAD CROTA2 = 2.40000E+01 / new HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = 'RA---ARC' / OLD Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / OLD Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / OLD Axis increment HISTORY AXDEF CRPIX2 = 502.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'DEC--SIN' / NEW Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 502.000 / NEW Reference pixel loc HISTORY AXDEF INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY AXDEF INSEQ= 2 INDISK= 2 HISTORY AXDEF CTYPE2 = 'DEC--SIN' / OLD Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / OLD Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / OLD Axis increment HISTORY AXDEF CRPIX2 = 502.000 / OLD Reference pixel loc HISTORY AXDEF CTYPE2 = 'DEC--ARC' / NEW Axis type HISTORY AXDEF CRVAL2 = 6.992031002E+01 / NEW Reference pixel value HISTORY AXDEF CDELT2 = 1.13917E-04 / NEW Axis increment HISTORY AXDEF CRPIX2 = 502.000 / NEW Reference pixel loc HISTORY PUTHEAD CROTA2 = 2.40000E+01 / old HISTORY PUTHEAD CROTA2 = -2.40000E+01 / new HISTORY PUTHEAD CROTA2 = -2.40000E+01 / old HISTORY PUTHEAD CROTA2 = 2.40000E+01 / new HISTORY PUTHEAD CROTA2 = 2.40000E+01 / old HISTORY PUTHEAD CROTA2 = 0.00000E+00 / new HISTORY PUTHEAD CROTA2 = 0.00000E+00 / old HISTORY PUTHEAD CROTA2 = 2.40000E+01 / new HISTORY PUTHEAD CRVAL3 = 9.999999870E+14 / old HISTORY PUTHEAD CRVAL3 = 6.670000325E+14 / new HISTORY PUTHEAD CROTA2 = 2.40000E+01 / old HISTORY PUTHEAD CROTA2 = 2.64000E+01 / new HISTORY PUTHEAD CDELT1 = -1.06583E-04 / old HISTORY PUTHEAD CDELT1 = -1.09861E-04 / new HISTORY PUTHEAD CDELT2 = 1.13917E-04 / old HISTORY PUTHEAD CDELT2 = 1.13667E-04 / new HISTORY PUTHEAD CDELT1 = -1.09861E-04 / old HISTORY PUTHEAD CDELT1 = -1.12389E-04 / new HISTORY PUTHEAD CROTA2 = 2.64000E+01 / old HISTORY PUTHEAD CROTA2 = 2.42600E+01 / new HISTORY PUTHEAD CRVAL1 = 1.479284000E+02 / old HISTORY PUTHEAD CRVAL1 = 1.479271000E+02 / new HISTORY PUTHEAD CRPIX1 = 5.77000E+02 / old HISTORY PUTHEAD CRPIX1 = 6.46000E+02 / new HISTORY PUTHEAD CRPIX2 = 5.02000E+02 / old HISTORY PUTHEAD CRPIX2 = 4.24000E+02 / new HISTORY PUTHEAD CRVAL2 = 6.992031002E+01 / old HISTORY PUTHEAD CRVAL2 = 6.990799999E+01 / new HISTORY SUBIM RELEASE ='15JUL94 ' /********* Start 25-MAR-1994 09:30:57 HISTORY SUBIM INNAME='M82 in blue ' INCLASS='TRANS ' HISTORY SUBIM INSEQ= 2 INDISK= 2 HISTORY SUBIM INTYPE ='MA' USERID= 103 HISTORY SUBIM OUTNAME='M82 in blue ' OUTCLASS='SUBIM ' HISTORY SUBIM OUTSEQ= 1 OUTDISK= 2 HISTORY SUBIM BLC = 45, 235, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 1159, 759, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 2 YINC = 2 HISTORY SUBIM OPCODE = 'AVE ' HISTORY AIPS IMNAME='M82 in blue ' IMCLASS='SUBIM ' IMSEQ= 1 / HISTORY AIPS USERNO= 103 / HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 4 HISTORY IMLOD INFILE = 'FITS2:M82BLUE.FITS ' HISTORY IMLOD RELEASE = '15JAN95' HISTORY SUBIM RELEASE ='15JAN95 ' /********* Start 13-SEP-1994 12:59:44 HISTORY SUBIM INNAME='M82 in blue ' INCLASS='SUBIM ' HISTORY SUBIM INSEQ= 1 INDISK= 4 HISTORY SUBIM INTYPE ='MA' USERID= 103 HISTORY SUBIM OUTNAME='M82 ' OUTCLASS='Blue ' HISTORY SUBIM OUTSEQ= 3 OUTDISK= 4 HISTORY SUBIM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 558, 262, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 1 YINC = 1 HISTORY SUBIM OPCODE = ' ' ORIGIN = 'AIPSGorilla (NRAOCV IPX) 15JAN95' / DATE = '13/09/94' / File written on dd/mm/yy HISTORY AIPS IMNAME='M82 ' IMCLASS='Blue ' IMSEQ= 3 / HISTORY AIPS USERNO= 103 / pywcs-1.12/lib/pywcs/tests/nrao/m82rad.hdr0000644001153600020070000002155712310355626022470 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / BITPIX = 16 / NAXIS = 4 / NAXIS1 = 558 / NAXIS2 = 262 / NAXIS3 = 1 / NAXIS4 = 1 / EXTEND = T /Tables following main image BLOCKED = T /Tape may be blocked OBJECT = 'U05322 ' TELESCOP= 'VLA ' INSTRUME= 'VLA ' OBSERVER= 'AC243 ' DATE-OBS= '06/02/89' DATE-MAP= '13/09/94' BSCALE = 1.95069823037E-06 /REAL = TAPE * BSCALE + BZERO BZERO = 5.48100471497E-02 / BUNIT = 'JY/BEAM ' EPOCH = 1.950000000E+03 /EPOCH OF RA DEC BLANK = -32768 / Blanked pixel tape value VELREF = 3 />256 RADIO, 1 LSR 2 HEL 3 OBS ALTRVAL = 1.00000000000E+05 /ALTENATE FREQ/VEL REF VALUE ALTRPIX = 1.000000000E+00 /ALTENATE FREQ/VEL REF PIXEL YSHIFT = 1.421085472E-14 /NET SHIFT OF PHASE CENTER INY DATAMAX = 1.187149212E-01 /MAX PIXEL VALUE DATAMIN = -9.094826877E-03 /MIN PIXEL VALUE CTYPE1 = 'RA---ARC' CRVAL1 = 1.47927100003E+02 / CDELT1 = -2.247777738E-04 / CRPIX1 = 3.015000000E+02 / CROTA1 = 0.000000000E+00 / CTYPE2 = 'DEC--ARC' CRVAL2 = 6.99079999924E+01 / CDELT2 = 2.273333375E-04 / CRPIX2 = 9.550000000E+01 / CROTA2 = 2.426000023E+01 / CTYPE3 = 'FREQ ' CRVAL3 = 1.49000000000E+09 / CDELT3 = 5.000000000E+07 / CRPIX3 = 1.000000000E+00 / CROTA3 = 0.000000000E+00 / CTYPE4 = 'STOKES ' CRVAL4 = 1.00000000000E+00 / CDELT4 = 1.000000000E+00 / CRPIX4 = 1.000000000E+00 / CROTA4 = 0.000000000E+00 / HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /Tape may be blocked HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /Tape may be blocked HISTORY AIPS IMNAME='NGC3034 ' IMCLASS='SUBIM ' IMSEQ= 1 / HISTORY AIPS USERNO= 135 / HISTORY AIPS CLEAN BMAJ= 5.0000E-04 BMIN= 5.0000E-04 BPA= 0.00 HISTORY AIPS CLEAN NITER= 2000 PRODUCT=1 / NORMAL HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 2 HISTORY IMLOD INFILE = 'FITS2:NGC3034.A ' HISTORY IMLOD RELEASE = '15JUL94' HISTORY SUBIM RELEASE ='15JUL94 ' /********* Start 25-MAR-1994 09:37:01 HISTORY SUBIM INNAME='M82 in radio' INCLASS='SUBIM ' HISTORY SUBIM INSEQ= 1 INDISK= 2 HISTORY SUBIM INTYPE ='MA' USERID= 103 HISTORY SUBIM OUTNAME='M82 in radio' OUTCLASS='SUBIM ' HISTORY SUBIM OUTSEQ= 2 OUTDISK= 2 HISTORY SUBIM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 256, 256, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 2 YINC = 2 HISTORY SUBIM OPCODE = 'AVE ' HISTORY HGEOM RELEASE ='15JUL94 ' /********* Start 25-MAR-1994 09:37:24 HISTORY HGEOM INNAME='M82 in radio' INCLASS='SUBIM ' HISTORY HGEOM INSEQ= 2 INDISK= 2 HISTORY HGEOM IN2NAME='M82 in blue ' IN2CLASS='SUBIM ' HISTORY HGEOM IN2SEQ= 1 IN2DISK= 2 HISTORY HGEOM OUTNAME='M82 in radio' OUTCLASS=' ' HISTORY HGEOM OUTSEQ= 1 OUTDISK= 2 HISTORY HGEOM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY HGEOM TRC = 128, 128, 1, 1, 1, 1, 1 HISTORY HGEOM IMSIZE = 558, 263 / Output image size HISTORY HGEOM / Interpolation order used was BiCubic HISTORY HGEOM / Indeterminate pixels filled with magic values HISTORY HGEOM / 131164 Pixels blanked due to memory limits or geometry HISTORY HGEOM / 0 Pixels blanked due to input blanked pixels HISTORY AIPS IMNAME='M82 in radio' IMCLASS='HGEOM ' IMSEQ= 1 / HISTORY AIPS USERNO= 103 / HISTORY AIPS CLEAN BMAJ= 5.0000E-04 BMIN= 5.0000E-04 BPA= 0.00 HISTORY AIPS CLEAN NITER= 2000 PRODUCT=1 / NORMAL HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 4 HISTORY IMLOD INFILE = 'FITS2:M82RADIO.FITS ' HISTORY IMLOD RELEASE = '15JAN95' HISTORY SUBIM RELEASE ='15JAN95 ' /********* Start 13-SEP-1994 13:00:09 HISTORY SUBIM INNAME='M82 in radio' INCLASS='HGEOM ' HISTORY SUBIM INSEQ= 1 INDISK= 4 HISTORY SUBIM INTYPE ='MA' USERID= 103 HISTORY SUBIM OUTNAME='M82 ' OUTCLASS='Radio ' HISTORY SUBIM OUTSEQ= 3 OUTDISK= 4 HISTORY SUBIM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 558, 262, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 1 YINC = 1 HISTORY SUBIM OPCODE = ' ' ORIGIN = 'AIPSGorilla (NRAOCV IPX) 15JAN95' / DATE = '13/09/94' / File written on dd/mm/yy HISTORY AIPS IMNAME='M82 ' IMCLASS='Radio ' IMSEQ= 3 / HISTORY AIPS USERNO= 103 / HISTORY AIPS CLEAN BMAJ= 5.0000E-04 BMIN= 5.0000E-04 BPA= 0.00 HISTORY AIPS CLEAN NITER= 2000 PRODUCT=1 / NORMAL pywcs-1.12/lib/pywcs/tests/nrao/ngc1316o.hdr0000644001153600020070000002514512310355626022631 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / BITPIX = 16 / NAXIS = 2 / NAXIS1 = 512 / NAXIS2 = 512 / EXTEND = T /Tables following main image BLOCKED = T /Tape may be blocked OBJECT = 'NONE ' TELESCOP= ' ' INSTRUME= ' ' OBSERVER= ' ' DATE-OBS= ' ' DATE-MAP= '24/03/94' BSCALE = 1.59240089202E-02 /REAL = TAPE * BSCALE + BZERO BZERO = 5.16219848633E+02 / BUNIT = ' ' EPOCH = 0.000000000E+00 /EPOCH OF RA DEC BLANK = -32768 / Blanked pixel tape value DATAMAX = 1.037890381E+03 /MAX PIXEL VALUE DATAMIN = -5.450668335E+00 /MIN PIXEL VALUE CTYPE1 = 'RA---SIN' CRVAL1 = 5.01966661513E+01 / CDELT1 = -1.944444492E-03 / CRPIX1 = 2.560000000E+02 / CROTA1 = 0.000000000E+00 / CTYPE2 = 'DEC--SIN' CRVAL2 = -3.73856168315E+01 / CDELT2 = 1.944444492E-03 / CRPIX2 = 2.570000000E+02 / CROTA2 = 0.000000000E+00 / HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /TAPE MAY BE BLOCKED HISTORY /-------------------------------------------------------------------- HISTORY /BEGIN "HISTORY" INFORMATION FOUND IN FITS TAPE HEADER BY IMLOD HISTORY /END FITS TAPE HEADER "HISTORY" INFORMATION HISTORY /-------------------------------------------------------------------- HISTORY IMLOD OUTNAME ='NGC1316 ' OUTCLASS ='OPT ' HISTORY IMLOD OUTSEQ = 1 INTAPE = 3 OUTDISK= 1 HISTORY IMLOD RELEASE = '15APR89' HISTORY TRANS RELEASE ='15APR89 ' /********* START 17-FEB-1989 08:47:28 HISTORY TRANS INNAME='NGC1316 ' INCLASS='OPT ' HISTORY TRANS INSEQ= 1 INDISK= 1 HISTORY TRANS OUTNAME='NGC1316/G ' OUTCLASS='OPT ' HISTORY TRANS OUTSEQ= 1 OUTDISK= 1 HISTORY TRANS BLC= 1., 1., 1., 1., 1., 1., 1. / INPUT IMAGE HISTORY TRANS TRC= 2001.,1401., 1., 1., 1., 1., 1. / INPUT IMAGE HISTORY TRANS TRANCOD='1-2 ' / OUTPUT AXIS ORDER HISTORY CNTR VERSION= 1 / PLOT FILE CREATED 17-FEB-1989 14:03:52 HISTORY CNTR VERSION= 2 / PLOT FILE CREATED 17-FEB-1989 14:07:08 HISTORY CNTR VERSION= 3 / PLOT FILE CREATED 17-FEB-1989 14:08:35 HISTORY PUTHEAD CTYPE1 =' ' / OLD HISTORY PUTHEAD CTYPE1 ='RA--TAN ' / NEW HISTORY PUTHEAD CTYPE1 ='RA--TAN ' / OLD HISTORY PUTHEAD CTYPE1 ='RA---TAN' / NEW HISTORY PUTHEAD CTYPE2 =' ' / OLD HISTORY PUTHEAD CTYPE2 ='DEC--TAN' / NEW HISTORY PUTHEAD CRVAL1 = 0.000000000E+00 / OLD HISTORY PUTHEAD CRVAL1 = 5.019667053E+01 / NEW HISTORY PUTHEAD CRVAL2 = 0.000000000E+00 / OLD HISTORY PUTHEAD CRVAL2 = -3.738555908E+01 / NEW HISTORY PUTHEAD CRPIX1 = 1.00000E+03 / OLD HISTORY PUTHEAD CRPIX1 = 7.02000E+02 / NEW HISTORY PUTHEAD CRPIX1 = 7.02000E+02 / OLD HISTORY PUTHEAD CRPIX1 = 9.97000E+02 / NEW HISTORY PUTHEAD CDELT1 = 1.00000E+00 / OLD HISTORY PUTHEAD CDELT1 = 3.05600E-02 / NEW HISTORY PUTHEAD CDELT2 = -1.00000E+00 / OLD HISTORY PUTHEAD CDELT2 = 3.05600E-02 / NEW HISTORY PUTHEAD CDELT2 = 3.05600E-02 / OLD HISTORY PUTHEAD CDELT2 = 5.09333E-04 / NEW HISTORY PUTHEAD CDELT2 = 5.09333E-04 / OLD HISTORY PUTHEAD CDELT2 = 5.09333E-04 / NEW HISTORY PUTHEAD CDELT1 = 3.05600E-02 / OLD HISTORY PUTHEAD CDELT1 = -5.09333E-04 / NEW HISTORY PUTHEAD CROTA1 = 0.00000E+00 / OLD HISTORY PUTHEAD CROTA1 = 3.00000E-01 / NEW HISTORY PUTHEAD CROTA1 = 3.00000E-01 / OLD HISTORY PUTHEAD CROTA1 = 0.00000E+00 / NEW HISTORY PUTHEAD CROTA1 = 0.00000E+00 / OLD HISTORY PUTHEAD CROTA1 = 3.00000E-01 / NEW HISTORY PUTHEAD CROTA1 = 3.00000E-01 / OLD HISTORY PUTHEAD CROTA1 = 5.00000E+00 / NEW HISTORY PUTHEAD CROTA2 = 0.00000E+00 / OLD HISTORY PUTHEAD CROTA2 = 5.00000E+00 / NEW HISTORY PUTHEAD CROTA1 = 5.00000E+00 / OLD HISTORY PUTHEAD CROTA1 = 0.00000E+00 / NEW HISTORY PUTHEAD CROTA1 = 0.00000E+00 / OLD HISTORY PUTHEAD CROTA1 = 0.00000E+00 / NEW HISTORY PUTHEAD CROTA2 = 5.00000E+00 / OLD HISTORY PUTHEAD CROTA2 = 0.00000E+00 / NEW HISTORY PUTHEAD CROTA1 = 0.00000E+00 / OLD HISTORY PUTHEAD CROTA1 = 1.00000E+00 / NEW HISTORY PUTHEAD CROTA1 = 1.00000E+00 / OLD HISTORY PUTHEAD CROTA1 = 0.00000E+00 / NEW HISTORY PUTHEAD CROTA2 = 0.00000E+00 / OLD HISTORY PUTHEAD CROTA2 = 1.00000E+00 / NEW HISTORY PUTHEAD CROTA2 = 1.00000E+00 / OLD HISTORY PUTHEAD CROTA2 = 3.00000E-01 / NEW HISTORY AIPS IMNAME='NGC1316/G ' IMCLASS='OPT ' IMSEQ= 1 / HISTORY AIPS USERNO= 51 / HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 3 HISTORY IMLOD RELEASE = '15JUL94' HISTORY SUBIM RELEASE ='15JUL94 ' /********* Start 24-MAR-1994 10:58:33 HISTORY SUBIM INNAME='NGC1316/G ' INCLASS='OPT ' HISTORY SUBIM INSEQ= 1 INDISK= 1 HISTORY SUBIM INTYPE ='MA' USERID= 100 HISTORY SUBIM OUTNAME='NGC1316/G ' OUTCLASS='SMOOTH' HISTORY SUBIM OUTSEQ= 1 OUTDISK= 1 HISTORY SUBIM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY SUBIM TRC = 2001, 1401, 1, 1, 1, 1, 1 HISTORY SUBIM XINC = 4 YINC = 4 HISTORY SUBIM OPCODE = 'AVE ' HISTORY HGEOM RELEASE ='15JUL94 ' /********* Start 24-MAR-1994 10:59:29 HISTORY HGEOM INNAME='NGC1316/G ' INCLASS='SMOOTH' HISTORY HGEOM INSEQ= 1 INDISK= 1 HISTORY HGEOM IN2NAME='FORNAX ' IN2CLASS='I ' HISTORY HGEOM IN2SEQ= 2 IN2DISK= 1 HISTORY HGEOM OUTNAME=' ' OUTCLASS='Optic ' HISTORY HGEOM OUTSEQ= 1 OUTDISK= 1 HISTORY HGEOM BLC = 1, 1, 1, 1, 1, 1, 1 HISTORY HGEOM TRC = 501, 351, 1, 1, 1, 1, 1 HISTORY HGEOM IMSIZE = 512, 512 / Output image size HISTORY HGEOM / Interpolation order used was BiCubic HISTORY HGEOM / Indeterminate pixels filled with magic values HISTORY HGEOM / 74383 Pixels blanked due to memory limits or geometry HISTORY HGEOM / 0 Pixels blanked due to input blanked pixels ORIGIN = 'AIPSGorilla (NRAOCV IPX) 15JUL94' / DATE = '24/03/94' / File written on dd/mm/yy HISTORY AIPS IMNAME='NGC1316/G ' IMCLASS='Optic ' IMSEQ= 1 / HISTORY AIPS USERNO= 100 / pywcs-1.12/lib/pywcs/tests/nrao/ngc1316r.hdr0000644001153600020070000002553012310355626022632 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / BITPIX = 16 / NAXIS = 4 / NAXIS1 = 512 / NAXIS2 = 512 / NAXIS3 = 1 / NAXIS4 = 1 / EXTEND = T /Tables following main image BLOCKED = T /Tape may be blocked OBJECT = 'F1 ' TELESCOP= ' ' INSTRUME= ' ' OBSERVER= 'INA ' DATE-OBS= '07/10/86' DATE-MAP= '06/09/88' BSCALE = 1.94159674120E-06 /REAL = TAPE * BSCALE + BZERO BZERO = 5.97180128098E-02 / BUNIT = 'JY/BEAM ' EPOCH = 1.950000000E+03 /EPOCH OF RA DEC OBSRA = 5.01966661513E+01 /ANTENNA POINTING RA OBSDEC = -3.73856168315E+01 /ANTENNA POINTING DEC YSHIFT = 7.105427358E-15 /NET SHIFT OF PHASE CENTER INY DATAMAX = 1.233247221E-01 /MAX PIXEL VALUE DATAMIN = -3.888696432E-03 /MIN PIXEL VALUE CTYPE1 = 'RA---SIN' CRVAL1 = 5.01966661513E+01 / CDELT1 = -1.944444492E-03 / CRPIX1 = 2.560000000E+02 / CROTA1 = 0.000000000E+00 / CTYPE2 = 'DEC--SIN' CRVAL2 = -3.73856168315E+01 / CDELT2 = 1.944444492E-03 / CRPIX2 = 2.570000000E+02 / CROTA2 = 0.000000000E+00 / CTYPE3 = 'FREQ ' CRVAL3 = 1.51000000000E+09 / CDELT3 = 1.690734863E+03 / CRPIX3 = 1.000000000E+00 / CROTA3 = 0.000000000E+00 / CTYPE4 = 'STOKES ' CRVAL4 = 1.00000000000E+00 / CDELT4 = 1.000000000E+00 / CRPIX4 = 1.000000000E+00 / CROTA4 = 0.000000000E+00 / HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /Tape may be blocked HISTORY -------------------------------------------------------------------- HISTORY /Begin "HISTORY" information found in fits tape header by IMLOD HISTORY BLOCKED = T /TAPE MAY BE BLOCKED HISTORY /-------------------------------------------------------------------- HISTORY /BEGIN "HISTORY" INFORMATION FOUND IN FITS TAPE HEADER BY IMLOD HISTORY BLOCKED = T /TAPE MAY BE BLOCKED HISTORY PUTHEAD OBSRA = 4.991666615E+01 / OLD HISTORY PUTHEAD OBSRA = 5.019666615E+01 / NEW HISTORY PUTHEAD OBSDEC = -3.736666683E+01 / OLD HISTORY PUTHEAD OBSDEC = -3.738561683E+01 / NEW HISTORY CNTR VERSION= 1 / PLOT FILE CREATED 08-SEP-1988 12:22:10 HISTORY GREYS VERSION= 2 / PLOT FILE CREATED 12-SEP-1988 19:08:19 HISTORY GREYS VERSION= 3 / PLOT FILE CREATED 13-SEP-1988 11:44:07 HISTORY GREYS VERSION= 4 / PLOT FILE CREATED 13-SEP-1988 12:40:37 HISTORY GREYS VERSION= 5 / PLOT FILE CREATED 13-SEP-1988 12:42:34 HISTORY GREYS VERSION= 6 / PLOT FILE CREATED 13-SEP-1988 12:44:28 HISTORY GREYS VERSION= 7 / PLOT FILE CREATED 13-SEP-1988 12:59:18 HISTORY GREYS VERSION= 8 / PLOT FILE CREATED 13-SEP-1988 13:03:15 HISTORY GREYS VERSION= 9 / PLOT FILE CREATED 13-SEP-1988 13:07:23 HISTORY GREYS VERSION= 10 / PLOT FILE CREATED 13-SEP-1988 13:25:50 HISTORY GREYS VERSION= 11 / PLOT FILE CREATED 13-SEP-1988 13:26:20 HISTORY GREYS VERSION= 12 / PLOT FILE CREATED 13-SEP-1988 13:32:00 HISTORY GREYS VERSION= 13 / PLOT FILE CREATED 13-SEP-1988 13:57:57 HISTORY GREYS VERSION= 14 / PLOT FILE CREATED 13-SEP-1988 14:00:53 HISTORY GREYS VERSION= 15 / PLOT FILE CREATED 13-SEP-1988 14:28:51 HISTORY GREYS VERSION= 16 / PLOT FILE CREATED 14-SEP-1988 12:00:40 HISTORY GREYS VERSION= 17 / PLOT FILE CREATED 14-SEP-1988 12:13:51 HISTORY GREYS VERSION= 18 / PLOT FILE CREATED 14-SEP-1988 12:15:36 HISTORY GREYS VERSION= 19 / PLOT FILE CREATED 15-SEP-1988 07:52:43 HISTORY GREYS VERSION= 20 / PLOT FILE CREATED 15-SEP-1988 08:11:42 HISTORY GREYS VERSION= 21 / PLOT FILE CREATED 15-SEP-1988 08:18:17 HISTORY GREYS VERSION= 22 / PLOT FILE CREATED 15-SEP-1988 08:44:40 HISTORY GREYS VERSION= 23 / PLOT FILE CREATED 15-SEP-1988 21:02:47 HISTORY GREYS VERSION= 24 / PLOT FILE CREATED 15-SEP-1988 21:09:45 HISTORY GREYS VERSION= 25 / PLOT FILE CREATED 15-SEP-1988 21:19:53 HISTORY GREYS VERSION= 26 / PLOT FILE CREATED 15-SEP-1988 21:28:01 HISTORY GREYS VERSION= 27 / PLOT FILE CREATED 15-SEP-1988 21:32:44 HISTORY GREYS VERSION= 28 / PLOT FILE CREATED 15-SEP-1988 21:38:55 HISTORY GREYS VERSION= 29 / PLOT FILE CREATED 15-SEP-1988 21:40:20 HISTORY GREYS VERSION= 30 / PLOT FILE CREATED 15-SEP-1988 21:42:44 HISTORY GREYS VERSION= 31 / PLOT FILE CREATED 15-SEP-1988 21:49:18 HISTORY GREYS VERSION= 32 / PLOT FILE CREATED 15-SEP-1988 21:53:40 HISTORY GREYS VERSION= 33 / PLOT FILE CREATED 15-SEP-1988 22:09:40 HISTORY GREYS VERSION= 1 / PLOT FILE CREATED 16-SEP-1988 14:54:15 HISTORY GREYS VERSION= 2 / PLOT FILE CREATED 16-SEP-1988 14:55:07 HISTORY GREYS VERSION= 3 / PLOT FILE CREATED 17-SEP-1988 17:17:18 HISTORY GREYS VERSION= 4 / PLOT FILE CREATED 17-SEP-1988 18:29:54 HISTORY GREYS VERSION= 5 / PLOT FILE CREATED 17-SEP-1988 18:30:43 HISTORY GREYS VERSION= 6 / PLOT FILE CREATED 17-SEP-1988 18:33:27 HISTORY GREYS VERSION= 7 / PLOT FILE CREATED 17-SEP-1988 18:35:44 HISTORY AIPS IMNAME='FORNAX/NOBL ' IMCLASS='I ' IMSEQ= 1 / HISTORY AIPS USERNO= 51 / HISTORY AIPS CLEAN BMAJ= 3.8889E-03 BMIN= 3.8889E-03 BPA= 0.00 HISTORY AIPS CLEAN NITER= 21 PRODUCT=4 / POINTS HISTORY /END FITS TAPE HEADER "HISTORY" INFORMATION HISTORY /-------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' ' OUTCLASS =' ' HISTORY IMLOD OUTSEQ = -1 INTAPE = 3 OUTDISK= 2 HISTORY IMLOD RELEASE = '15JAN89' HISTORY RENAM INNAME='FORNAX/NOBL ' INCLASS='I ' HISTORY RENAM INSEQ= 1 INDISK= 2 HISTORY RENAM OUTNAME='FORNAX ' OUTCLASS='I ' HISTORY RENAM OUTSEQ= 1 OUTDISK= 2 HISTORY PUTHEAD CRVAL3 = 1.384000000E+09 / OLD HISTORY PUTHEAD CRVAL3 = 1.510000000E+09 / NEW HISTORY AIPS IMNAME='FORNAX ' IMCLASS='I ' IMSEQ= 1 / HISTORY AIPS USERNO= 51 / HISTORY AIPS CLEAN BMAJ= 3.8889E-03 BMIN= 3.8889E-03 BPA= 0.00 HISTORY AIPS CLEAN NITER= 21 PRODUCT=4 / POINTS HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME ='FORNAX/NOBL ' OUTCLASS ='P ' HISTORY IMLOD OUTSEQ = 1 INTAPE = 1 OUTDISK= 2 HISTORY IMLOD RELEASE = '15OCT92' HISTORY AIPS IMNAME='FORNAX ' IMCLASS='I ' IMSEQ= 1 / HISTORY AIPS USERNO= 51 / HISTORY AIPS CLEAN BMAJ= 3.8889E-03 BMIN= 3.8889E-03 BPA= .00 HISTORY AIPS CLEAN NITER= 21 PRODUCT=4 / POINTS HISTORY /END FITS tape header "HISTORY" information HISTORY -------------------------------------------------------------------- HISTORY IMLOD OUTNAME =' HISTORY IMLOD OUTSEQ = 0 INTAPE = 1 OUTDISK= 1 HISTORY IMLOD INFILE = 'FITS2:FORNAXI ' HISTORY IMLOD RELEASE = '15JUL94' ORIGIN = 'AIPSGorilla (NRAOCV IPX) 15JUL94' / DATE = '24/03/94' / File written on dd/mm/yy HISTORY AIPS IMNAME='FORNAX ' IMCLASS='I ' IMSEQ= 1 / HISTORY AIPS USERNO= 100 / HISTORY AIPS CLEAN BMAJ= 3.8889E-03 BMIN= 3.8889E-03 BPA= 0.00 HISTORY AIPS CLEAN NITER= 21 PRODUCT=4 / POINTS pywcs-1.12/lib/pywcs/tests/spectra/0000755001153600020070000000000012310355732021362 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs/tests/spectra/orion-freq-1.hdr0000644001153600020070000007330012310355627024306 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 1 / number of data axes NAXIS1 = 4096 / length of data axis 1 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H COMMENT COMMENT This FITS file contains an example spectral WCS header constructed by COMMENT Mark Calabretta (ATNF) and Dirk Petry (ESO) based on an observation COMMENT of the Orion Kleinmann-Low nebula made by Andrew Walsh (JCU) and COMMENT Sven Thorwirth (MPIfR) using the Mopra radio telescope. COMMENT COMMENT The 110GHz 13CO 1-0 spectrum in this file is linear in frequency, as COMMENT observed, it being the Fourier transform of a lag spectrum produced COMMENT by a correlating spectrometer. COMMENT COMMENT The reference pixel has been placed deliberately well outside the COMMENT the spectrum in order to test spectral-WCS-interpreting software. COMMENT COMMENT Spectral representations are: COMMENT Frequency (default) ...frequency-like COMMENT E: Photon energy ...frequency-like COMMENT N: Wave number ...frequency-like COMMENT R: Radio velocity ...frequency-like COMMENT W: Wavelength ...wavelength-like COMMENT O: Optical velocity ...wavelength-like COMMENT Z: Redshift ...wavelength-like COMMENT V: Relativistic velocity ...velocity-like COMMENT B: Relativistic beta ...velocity-like COMMENT COMMENT The Mopra radio telescope is operated by the Australia Telescope COMMENT National Facility. COMMENT COMMENT Author: Mark Calabretta, Australia Telescope National Facility COMMENT http://www.atnf.csiro.au/~mcalabre/index.html COMMENT 2009-04-22 COMMENT ---------------------------------------------------------------------- COMMENT OBJECT = 'Orion-KL' / Orion Kleinmann-Low nebula MOLECULE= '13CO ' / Carbon(13) monoxide TRANSITI= '1-0 ' / 1-0 transition DATE-OBS= '2006-07-09T20:29:00' / Date of observation TELESCOP= 'ATNF Mopra' / 22m mm-wave telescope OBSERVER= 'Walsh/Thorwirth' / Observers BUNIT = 'K ' / Brightness units, Kelvin COMMENT COMMENT ------------------------------------------------------------ Frequency COMMENT CRPIX1 = 32768.0 / Pixel coordinate of reference point CTYPE1 = 'FREQ ' / Linear frequency axis (FFT of lag spectrum) CRVAL1 = 102.1189414E+9 / [Hz] Frequency of reference channel CDELT1 = -2.695372970E+5 / [Hz] Channel spacing (lower sideband) CUNIT1 = 'Hz ' / Units of coordinate increment and value COMMENT RESTFRQ = 110201353000.0 / [Hz] 13CO line rest frequency RESTWAV = 0.00272040633 / [m] 13CO line rest wavelength SPECSYS = 'LSRK ' / Reference frame of spectral coordinates SSYSOBS = 'TOPOCENT' / Reference frame of observation VELOSYS = 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRC = 'LSRK ' / Reference frame of source redshift ZSOURCE = 0.0000 / Redshift of the source COMMENT CRPIX2 = 1 CDELT2 = 1.0 CTYPE2 = 'RA ' CRVAL2 = 83.81042 / [deg] (05h35m14.5s) CUNIT2 = 'deg ' COMMENT CRPIX3 = 1 CDELT3 = 1.0 CTYPE3 = 'DEC ' CRVAL3 = -5.375222 / [deg] (-05:22:30.8) CUNIT3 = 'deg ' COMMENT RADESYS = 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOX = 2000.0 / Equinox J2000.0 COMMENT CRPIX4 = 1 CDELT4 = 1.0 CTYPE4 = 'STOKES ' CRVAL4 = 1 / Stokes I (total intensity) COMMENT COMMENT -------------------------------------------------------- Photon energy COMMENT CRPIX1E = 32768.0 / Pixel coordinate of reference point CTYPE1E = 'ENER ' / Photon energy, linear frequency axis CRVAL1E = 4.223303869E-4 / [eV] Photon energy of reference channel CDELT1E = -1.114717695E-9 / [eV] Channel spacing CUNIT1E = 'eV ' / Units of coordinate increment and value COMMENT RESTFRQE= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVE= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSE= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSE= 'TOPOCENT' / Reference frame of observation VELOSYSE= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCE= 'LSRK ' / Reference frame of source redshift ZSOURCEE= 0.0000 / Redshift of the source COMMENT CRPIX2E = 1 CDELT2E = 1.0 CTYPE2E = 'RA ' CRVAL2E = 83.81042 / [deg] (05h35m14.5s) CUNIT2E = 'deg ' COMMENT CRPIX3E = 1 CDELT3E = 1.0 CTYPE3E = 'DEC ' CRVAL3E = -5.375222 / [deg] (-05:22:30.8) CUNIT3E = 'deg ' COMMENT RADESYSE= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXE= 2000.0 / Equinox J2000.0 COMMENT CRPIX4E = 1 CDELT4E = 1.0 CTYPE4E = 'STOKES ' CRVAL4E = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------------------- Wave number COMMENT N: Wave number COMMENT CRPIX1N = 32768.0 / Pixel coordinate of reference point CTYPE1N = 'WAVN ' / Wave number, linear frequency axis CRVAL1N = 3.406321229E+2 / [/m] Wave number of reference channel CDELT1N = -8.990796460E-4 / [/m] Channel spacing CUNIT1N = '/m ' / Units of coordinate increment and value COMMENT RESTFRQN= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVN= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSN= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSN= 'TOPOCENT' / Reference frame of observation VELOSYSN= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCN= 'LSRK ' / Reference frame of source redshift ZSOURCEN= 0.0000 / Redshift of the source COMMENT CRPIX2N = 1 CDELT2N = 1.0 CTYPE2N = 'RA ' CRVAL2N = 83.81042 / [deg] (05h35m14.5s) CUNIT2N = 'deg ' COMMENT CRPIX3N = 1 CDELT3N = 1.0 CTYPE3N = 'DEC ' CRVAL3N = -5.375222 / [deg] (-05:22:30.8) CUNIT3N = 'deg ' COMMENT RADESYSN= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXN= 2000.0 / Equinox J2000.0 COMMENT CRPIX4N = 1 CDELT4N = 1.0 CTYPE4N = 'STOKES ' CRVAL4N = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------- Radio velocity COMMENT N: Wave number COMMENT R: Radio velocity COMMENT CRPIX1R = 32768.0 / Pixel coordinate of reference point CTYPE1R = 'VRAD ' / Radio velocity, linear frequency axis CRVAL1R = 2.198744369E+7 / [m/s] Radio velocity of reference channel CDELT1R = 7.332509683E+2 / [m/s] Channel spacing CUNIT1R = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQR= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVR= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSR= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSR= 'TOPOCENT' / Reference frame of observation VELOSYSR= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCR= 'LSRK ' / Reference frame of source redshift ZSOURCER= 0.0000 / Redshift of the source COMMENT CRPIX2R = 1 CDELT2R = 1.0 CTYPE2R = 'RA ' CRVAL2R = 83.81042 / [deg] (05h35m14.5s) CUNIT2R = 'deg ' COMMENT CRPIX3R = 1 CDELT3R = 1.0 CTYPE3R = 'DEC ' CRVAL3R = -5.375222 / [deg] (-05:22:30.8) CUNIT3R = 'deg ' COMMENT RADESYSR= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXR= 2000.0 / Equinox J2000.0 COMMENT CRPIX4R = 1 CDELT4R = 1.0 CTYPE4R = 'STOKES ' CRVAL4R = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------------- Wavelength COMMENT N: Wave number COMMENT R: Radio velocity COMMENT W: Wavelength COMMENT CRPIX1W = 32768.0 / Pixel coordinate of reference point CTYPE1W = 'WAVE-F2W' / Wavelength in vacuuo, non-linear axis CRVAL1W = 2.935718427E-3 / [m] Wavelength of reference channel CDELT1W = 7.748666397E-9 / [m] Channel spacing CUNIT1W = 'm ' / Units of coordinate increment and value COMMENT SPECSYSW= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSW= 'TOPOCENT' / Reference frame of observation VELOSYSW= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCW= 'LSRK ' / Reference frame of source redshift ZSOURCEW= 0.0000 / Redshift of the source COMMENT CRPIX2W = 1 CDELT2W = 1.0 CTYPE2W = 'RA ' CRVAL2W = 83.81042 / [deg] (05h35m14.5s) CUNIT2W = 'deg ' COMMENT CRPIX3W = 1 CDELT3W = 1.0 CTYPE3W = 'DEC ' CRVAL3W = -5.375222 / [deg] (-05:22:30.8) CUNIT3W = 'deg ' COMMENT RADESYSW= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXW= 2000.0 / Equinox J2000.0 COMMENT CRPIX4W = 1 CDELT4W = 1.0 CTYPE4W = 'STOKES ' CRVAL4W = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------- Optical velocity COMMENT CRPIX1O = 32768.0 / Pixel coordinate of reference point CTYPE1O = 'VOPT-F2W' / Optical velocity, non-linear axis CRVAL1O = 2.372768470E+7 / [m/s] Optical velocity of reference channel CDELT1O = 8.539135209E+2 / [m/s] Channel spacing CUNIT1O = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQO= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVO= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSO= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSO= 'TOPOCENT' / Reference frame of observation VELOSYSO= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCO= 'LSRK ' / Reference frame of source redshift ZSOURCEO= 0.0000 / Redshift of the source COMMENT CRPIX2O = 1 CDELT2O = 1.0 CTYPE2O = 'RA ' CRVAL2O = 83.81042 / [deg] (05h35m14.5s) CUNIT2O = 'deg ' COMMENT CRPIX3O = 1 CDELT3O = 1.0 CTYPE3O = 'DEC ' CRVAL3O = -5.375222 / [deg] (-05:22:30.8) CUNIT3O = 'deg ' COMMENT RADESYSO= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXO= 2000.0 / Equinox J2000.0 COMMENT CRPIX4O = 1 CDELT4O = 1.0 CTYPE4O = 'STOKES ' CRVAL4O = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------------- Redshift COMMENT N: Wave number COMMENT R: Radio velocity COMMENT W: Wavelength COMMENT O: Optical velocity COMMENT Z: Redshift COMMENT CRPIX1Z = 32768.0 / Pixel coordinate of reference point CTYPE1Z = 'ZOPT-F2W' / Redshift, non-linear axis CRVAL1Z = 7.914703679E-2 / [] Redshift of reference channel CDELT1Z = 2.848348910E-6 / [] Channel spacing COMMENT RESTFRQZ= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVZ= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSZ= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSZ= 'TOPOCENT' / Reference frame of observation VELOSYSZ= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCZ= 'LSRK ' / Reference frame of source redshift ZSOURCEZ= 0.0000 / Redshift of the source COMMENT CRPIX2Z = 1 CDELT2Z = 1.0 CTYPE2Z = 'RA ' CRVAL2Z = 83.81042 / [deg] (05h35m14.5s) CUNIT2Z = 'deg ' COMMENT CRPIX3Z = 1 CDELT3Z = 1.0 CTYPE3Z = 'DEC ' CRVAL3Z = -5.375222 / [deg] (-05:22:30.8) CUNIT3Z = 'deg ' COMMENT RADESYSZ= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXZ= 2000.0 / Equinox J2000.0 COMMENT CRPIX4Z = 1 CDELT4Z = 1.0 CTYPE4Z = 'STOKES ' CRVAL4Z = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------ Relativistic velocity COMMENT CRPIX1V = 32768.0 / Pixel coordinate of reference point CTYPE1V = 'VELO-F2V' / Relativistic velocity, non-linear axis CRVAL1V = 2.279141418E+7 / [m/s] Velocity of reference channel CDELT1V = 7.867122599E+2 / [m/s] Channel spacing CUNIT1V = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQV= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVV= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSV= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSV= 'TOPOCENT' / Reference frame of observation VELOSYSV= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCV= 'LSRK ' / Reference frame of source redshift ZSOURCEV= 0.0000 / Redshift of the source COMMENT CRPIX2V = 1 CDELT2V = 1.0 CTYPE2V = 'RA ' CRVAL2V = 83.81042 / [deg] (05h35m14.5s) CUNIT2V = 'deg ' COMMENT CRPIX3V = 1 CDELT3V = 1.0 CTYPE3V = 'DEC ' CRVAL3V = -5.375222 / [deg] (-05:22:30.8) CUNIT3V = 'deg ' COMMENT RADESYSV= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXV= 2000.0 / Equinox J2000.0 COMMENT CRPIX4V = 1 CDELT4V = 1.0 CTYPE4V = 'STOKES ' CRVAL4V = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------- Relativistic beta (v/c) COMMENT CRPIX1B = 32768.0 / Pixel coordinate of reference point CTYPE1B = 'BETA-F2V' / Relativistic beta (v/c), non-linear axis CRVAL1B = 7.602397448E-2 / [] Relativistic beta of reference channel CDELT1B = 2.624189632E-6 / [] Channel spacing COMMENT RESTFRQB= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVB= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSB= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSB= 'TOPOCENT' / Reference frame of observation VELOSYSB= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCB= 'LSRK ' / Reference frame of source redshift ZSOURCEB= 0.0000 / Redshift of the source COMMENT CRPIX2B = 1 CDELT2B = 1.0 CTYPE2B = 'RA ' CRVAL2B = 83.81042 / [deg] (05h35m14.5s) CUNIT2B = 'deg ' COMMENT CRPIX3B = 1 CDELT3B = 1.0 CTYPE3B = 'DEC ' CRVAL3B = -5.375222 / [deg] (-05:22:30.8) CUNIT3B = 'deg ' COMMENT RADESYSB= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXB= 2000.0 / Equinox J2000.0 COMMENT CRPIX4B = 1 CDELT4B = 1.0 CTYPE4B = 'STOKES ' CRVAL4B = 1 / Stokes I (total intensity) COMMENT HISTORY fimgcreate 1.0b at 2009-04-22T04:27:55 DATE = '2009-04-22T04:27:55' / file creation date (YYYY-MM-DDThh:mm:ss UT) pywcs-1.12/lib/pywcs/tests/spectra/orion-freq-4.hdr0000644001153600020070000007366012310355627024322 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 4 / number of data axes NAXIS1 = 4096 / length of data axis 1 NAXIS2 = 1 / length of data axis 2 NAXIS3 = 1 / length of data axis 3 NAXIS4 = 1 / length of data axis 4 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H COMMENT COMMENT This FITS file contains an example spectral WCS header constructed by COMMENT Mark Calabretta (ATNF) and Dirk Petry (ESO) based on an observation COMMENT of the Orion Kleinmann-Low nebula made by Andrew Walsh (JCU) and COMMENT Sven Thorwirth (MPIfR) using the Mopra radio telescope. COMMENT COMMENT The 110GHz 13CO 1-0 spectrum in this file is linear in frequency, as COMMENT observed, it being the Fourier transform of a lag spectrum produced COMMENT by a correlating spectrometer. COMMENT COMMENT The reference pixel has been placed deliberately well outside the COMMENT the spectrum in order to test spectral-WCS-interpreting software. COMMENT COMMENT Spectral representations are: COMMENT Frequency (default) ...frequency-like COMMENT E: Photon energy ...frequency-like COMMENT N: Wave number ...frequency-like COMMENT R: Radio velocity ...frequency-like COMMENT W: Wavelength ...wavelength-like COMMENT O: Optical velocity ...wavelength-like COMMENT Z: Redshift ...wavelength-like COMMENT V: Relativistic velocity ...velocity-like COMMENT B: Relativistic beta ...velocity-like COMMENT COMMENT The Mopra radio telescope is operated by the Australia Telescope COMMENT National Facility. COMMENT COMMENT Author: Mark Calabretta, Australia Telescope National Facility COMMENT http://www.atnf.csiro.au/~mcalabre/index.html COMMENT 2009-04-22 COMMENT ---------------------------------------------------------------------- COMMENT OBJECT = 'Orion-KL' / Orion Kleinmann-Low nebula MOLECULE= '13CO ' / Carbon(13) monoxide TRANSITI= '1-0 ' / 1-0 transition DATE-OBS= '2006-07-09T20:29:00' / Date of observation TELESCOP= 'ATNF Mopra' / 22m mm-wave telescope OBSERVER= 'Walsh/Thorwirth' / Observers BUNIT = 'K ' / Brightness units, Kelvin COMMENT COMMENT ------------------------------------------------------------ Frequency COMMENT CRPIX1 = 32768.0 / Pixel coordinate of reference point CTYPE1 = 'FREQ ' / Linear frequency axis (FFT of lag spectrum) CRVAL1 = 102.1189414E+9 / [Hz] Frequency of reference channel CDELT1 = -2.695372970E+5 / [Hz] Channel spacing (lower sideband) CUNIT1 = 'Hz ' / Units of coordinate increment and value COMMENT RESTFRQ = 110201353000.0 / [Hz] 13CO line rest frequency RESTWAV = 0.00272040633 / [m] 13CO line rest wavelength SPECSYS = 'LSRK ' / Reference frame of spectral coordinates SSYSOBS = 'TOPOCENT' / Reference frame of observation VELOSYS = 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRC = 'LSRK ' / Reference frame of source redshift ZSOURCE = 0.0000 / Redshift of the source COMMENT CRPIX2 = 1 CDELT2 = 1.0 CTYPE2 = 'RA ' CRVAL2 = 83.81042 / [deg] (05h35m14.5s) CUNIT2 = 'deg ' COMMENT CRPIX3 = 1 CDELT3 = 1.0 CTYPE3 = 'DEC ' CRVAL3 = -5.375222 / [deg] (-05:22:30.8) CUNIT3 = 'deg ' COMMENT RADESYS = 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOX = 2000.0 / Equinox J2000.0 COMMENT CRPIX4 = 1 CDELT4 = 1.0 CTYPE4 = 'STOKES ' CRVAL4 = 1 / Stokes I (total intensity) COMMENT COMMENT -------------------------------------------------------- Photon energy COMMENT CRPIX1E = 32768.0 / Pixel coordinate of reference point CTYPE1E = 'ENER ' / Photon energy, linear frequency axis CRVAL1E = 4.223303869E-4 / [eV] Photon energy of reference channel CDELT1E = -1.114717695E-9 / [eV] Channel spacing CUNIT1E = 'eV ' / Units of coordinate increment and value COMMENT RESTFRQE= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVE= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSE= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSE= 'TOPOCENT' / Reference frame of observation VELOSYSE= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCE= 'LSRK ' / Reference frame of source redshift ZSOURCEE= 0.0000 / Redshift of the source COMMENT CRPIX2E = 1 CDELT2E = 1.0 CTYPE2E = 'RA ' CRVAL2E = 83.81042 / [deg] (05h35m14.5s) CUNIT2E = 'deg ' COMMENT CRPIX3E = 1 CDELT3E = 1.0 CTYPE3E = 'DEC ' CRVAL3E = -5.375222 / [deg] (-05:22:30.8) CUNIT3E = 'deg ' COMMENT RADESYSE= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXE= 2000.0 / Equinox J2000.0 COMMENT CRPIX4E = 1 CDELT4E = 1.0 CTYPE4E = 'STOKES ' CRVAL4E = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------------------- Wave number COMMENT N: Wave number COMMENT CRPIX1N = 32768.0 / Pixel coordinate of reference point CTYPE1N = 'WAVN ' / Wave number, linear frequency axis CRVAL1N = 3.406321229E+2 / [/m] Wave number of reference channel CDELT1N = -8.990796460E-4 / [/m] Channel spacing CUNIT1N = '/m ' / Units of coordinate increment and value COMMENT RESTFRQN= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVN= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSN= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSN= 'TOPOCENT' / Reference frame of observation VELOSYSN= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCN= 'LSRK ' / Reference frame of source redshift ZSOURCEN= 0.0000 / Redshift of the source COMMENT CRPIX2N = 1 CDELT2N = 1.0 CTYPE2N = 'RA ' CRVAL2N = 83.81042 / [deg] (05h35m14.5s) CUNIT2N = 'deg ' COMMENT CRPIX3N = 1 CDELT3N = 1.0 CTYPE3N = 'DEC ' CRVAL3N = -5.375222 / [deg] (-05:22:30.8) CUNIT3N = 'deg ' COMMENT RADESYSN= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXN= 2000.0 / Equinox J2000.0 COMMENT CRPIX4N = 1 CDELT4N = 1.0 CTYPE4N = 'STOKES ' CRVAL4N = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------- Radio velocity COMMENT N: Wave number COMMENT R: Radio velocity COMMENT CRPIX1R = 32768.0 / Pixel coordinate of reference point CTYPE1R = 'VRAD ' / Radio velocity, linear frequency axis CRVAL1R = 2.198744369E+7 / [m/s] Radio velocity of reference channel CDELT1R = 7.332509683E+2 / [m/s] Channel spacing CUNIT1R = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQR= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVR= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSR= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSR= 'TOPOCENT' / Reference frame of observation VELOSYSR= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCR= 'LSRK ' / Reference frame of source redshift ZSOURCER= 0.0000 / Redshift of the source COMMENT CRPIX2R = 1 CDELT2R = 1.0 CTYPE2R = 'RA ' CRVAL2R = 83.81042 / [deg] (05h35m14.5s) CUNIT2R = 'deg ' COMMENT CRPIX3R = 1 CDELT3R = 1.0 CTYPE3R = 'DEC ' CRVAL3R = -5.375222 / [deg] (-05:22:30.8) CUNIT3R = 'deg ' COMMENT RADESYSR= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXR= 2000.0 / Equinox J2000.0 COMMENT CRPIX4R = 1 CDELT4R = 1.0 CTYPE4R = 'STOKES ' CRVAL4R = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------------- Wavelength COMMENT N: Wave number COMMENT R: Radio velocity COMMENT W: Wavelength COMMENT CRPIX1W = 32768.0 / Pixel coordinate of reference point CTYPE1W = 'WAVE-F2W' / Wavelength in vacuuo, non-linear axis CRVAL1W = 2.935718427E-3 / [m] Wavelength of reference channel CDELT1W = 7.748666397E-9 / [m] Channel spacing CUNIT1W = 'm ' / Units of coordinate increment and value COMMENT SPECSYSW= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSW= 'TOPOCENT' / Reference frame of observation VELOSYSW= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCW= 'LSRK ' / Reference frame of source redshift ZSOURCEW= 0.0000 / Redshift of the source COMMENT CRPIX2W = 1 CDELT2W = 1.0 CTYPE2W = 'RA ' CRVAL2W = 83.81042 / [deg] (05h35m14.5s) CUNIT2W = 'deg ' COMMENT CRPIX3W = 1 CDELT3W = 1.0 CTYPE3W = 'DEC ' CRVAL3W = -5.375222 / [deg] (-05:22:30.8) CUNIT3W = 'deg ' COMMENT RADESYSW= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXW= 2000.0 / Equinox J2000.0 COMMENT CRPIX4W = 1 CDELT4W = 1.0 CTYPE4W = 'STOKES ' CRVAL4W = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------- Optical velocity COMMENT CRPIX1O = 32768.0 / Pixel coordinate of reference point CTYPE1O = 'VOPT-F2W' / Optical velocity, non-linear axis CRVAL1O = 2.372768470E+7 / [m/s] Optical velocity of reference channel CDELT1O = 8.539135209E+2 / [m/s] Channel spacing CUNIT1O = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQO= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVO= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSO= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSO= 'TOPOCENT' / Reference frame of observation VELOSYSO= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCO= 'LSRK ' / Reference frame of source redshift ZSOURCEO= 0.0000 / Redshift of the source COMMENT CRPIX2O = 1 CDELT2O = 1.0 CTYPE2O = 'RA ' CRVAL2O = 83.81042 / [deg] (05h35m14.5s) CUNIT2O = 'deg ' COMMENT CRPIX3O = 1 CDELT3O = 1.0 CTYPE3O = 'DEC ' CRVAL3O = -5.375222 / [deg] (-05:22:30.8) CUNIT3O = 'deg ' COMMENT RADESYSO= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXO= 2000.0 / Equinox J2000.0 COMMENT CRPIX4O = 1 CDELT4O = 1.0 CTYPE4O = 'STOKES ' CRVAL4O = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------------- Redshift COMMENT N: Wave number COMMENT R: Radio velocity COMMENT W: Wavelength COMMENT O: Optical velocity COMMENT Z: Redshift COMMENT CRPIX1Z = 32768.0 / Pixel coordinate of reference point CTYPE1Z = 'ZOPT-F2W' / Redshift, non-linear axis CRVAL1Z = 7.914703679E-2 / [] Redshift of reference channel CDELT1Z = 2.848348910E-6 / [] Channel spacing COMMENT RESTFRQZ= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVZ= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSZ= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSZ= 'TOPOCENT' / Reference frame of observation VELOSYSZ= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCZ= 'LSRK ' / Reference frame of source redshift ZSOURCEZ= 0.0000 / Redshift of the source COMMENT CRPIX2Z = 1 CDELT2Z = 1.0 CTYPE2Z = 'RA ' CRVAL2Z = 83.81042 / [deg] (05h35m14.5s) CUNIT2Z = 'deg ' COMMENT CRPIX3Z = 1 CDELT3Z = 1.0 CTYPE3Z = 'DEC ' CRVAL3Z = -5.375222 / [deg] (-05:22:30.8) CUNIT3Z = 'deg ' COMMENT RADESYSZ= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXZ= 2000.0 / Equinox J2000.0 COMMENT CRPIX4Z = 1 CDELT4Z = 1.0 CTYPE4Z = 'STOKES ' CRVAL4Z = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------ Relativistic velocity COMMENT CRPIX1V = 32768.0 / Pixel coordinate of reference point CTYPE1V = 'VELO-F2V' / Relativistic velocity, non-linear axis CRVAL1V = 2.279141418E+7 / [m/s] Velocity of reference channel CDELT1V = 7.867122599E+2 / [m/s] Channel spacing CUNIT1V = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQV= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVV= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSV= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSV= 'TOPOCENT' / Reference frame of observation VELOSYSV= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCV= 'LSRK ' / Reference frame of source redshift ZSOURCEV= 0.0000 / Redshift of the source COMMENT CRPIX2V = 1 CDELT2V = 1.0 CTYPE2V = 'RA ' CRVAL2V = 83.81042 / [deg] (05h35m14.5s) CUNIT2V = 'deg ' COMMENT CRPIX3V = 1 CDELT3V = 1.0 CTYPE3V = 'DEC ' CRVAL3V = -5.375222 / [deg] (-05:22:30.8) CUNIT3V = 'deg ' COMMENT RADESYSV= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXV= 2000.0 / Equinox J2000.0 COMMENT CRPIX4V = 1 CDELT4V = 1.0 CTYPE4V = 'STOKES ' CRVAL4V = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------- Relativistic beta (v/c) COMMENT CRPIX1B = 32768.0 / Pixel coordinate of reference point CTYPE1B = 'BETA-F2V' / Relativistic beta (v/c), non-linear axis CRVAL1B = 7.602397448E-2 / [] Relativistic beta of reference channel CDELT1B = 2.624189632E-6 / [] Channel spacing COMMENT RESTFRQB= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVB= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSB= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSB= 'TOPOCENT' / Reference frame of observation VELOSYSB= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCB= 'LSRK ' / Reference frame of source redshift ZSOURCEB= 0.0000 / Redshift of the source COMMENT CRPIX2B = 1 CDELT2B = 1.0 CTYPE2B = 'RA ' CRVAL2B = 83.81042 / [deg] (05h35m14.5s) CUNIT2B = 'deg ' COMMENT CRPIX3B = 1 CDELT3B = 1.0 CTYPE3B = 'DEC ' CRVAL3B = -5.375222 / [deg] (-05:22:30.8) CUNIT3B = 'deg ' COMMENT RADESYSB= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXB= 2000.0 / Equinox J2000.0 COMMENT CRPIX4B = 1 CDELT4B = 1.0 CTYPE4B = 'STOKES ' CRVAL4B = 1 / Stokes I (total intensity) COMMENT HISTORY fimgcreate 1.0b at 2009-04-22T04:28:02 DATE = '2009-04-22T04:28:02' / file creation date (YYYY-MM-DDThh:mm:ss UT) pywcs-1.12/lib/pywcs/tests/spectra/orion-velo-1.hdr0000644001153600020070000007176012310355627024326 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 1 / number of data axes NAXIS1 = 4096 / length of data axis 1 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H COMMENT COMMENT This FITS file contains an example spectral WCS header constructed by COMMENT Mark Calabretta (ATNF) and Dirk Petry (ESO) based on an observation COMMENT of the Orion Kleinmann-Low nebula made by Andrew Walsh (JCU) and COMMENT Sven Thorwirth (MPIfR) using the Mopra radio telescope. COMMENT COMMENT The 110GHz 13CO 1-0 spectrum in this file is linear in relativistic COMMENT velocity having been regridded from a linear frequency axis, as COMMENT observed. COMMENT COMMENT The reference pixel has been placed deliberately well outside the COMMENT the spectrum in order to test spectral-WCS-interpreting software. COMMENT COMMENT Spectral representations are: COMMENT F: Frequency ...frequency-like COMMENT E: Photon energy ...frequency-like COMMENT N: Wave number ...frequency-like COMMENT R: Radio velocity ...frequency-like COMMENT W: Wavelength ...wavelength-like COMMENT O: Optical velocity ...wavelength-like COMMENT Z: Redshift ...wavelength-like COMMENT Relativistic velocity (default) ...velocity-like COMMENT B: Relativistic beta ...velocity-like COMMENT COMMENT The Mopra radio telescope is operated by the Australia Telescope COMMENT National Facility. COMMENT COMMENT Author: Mark Calabretta, Australia Telescope National Facility COMMENT http://www.atnf.csiro.au/~mcalabre/index.html COMMENT 2009-04-22 COMMENT ---------------------------------------------------------------------- COMMENT OBJECT = 'Orion-KL' / Orion Kleinmann-Low nebula MOLECULE= '13CO ' / Carbon(13) monoxide TRANSITI= '1-0 ' / 1-0 transition DATE-OBS= '2006-07-09T20:29:00' / Date of observation TELESCOP= 'ATNF Mopra' / 22m mm-wave telescope OBSERVER= 'Walsh/Thorwirth' / Observers BUNIT = 'K ' / Brightness units, Kelvin COMMENT COMMENT ------------------------------------------------------------ Frequency COMMENT CRPIX1F = 32768.0 / Pixel coordinate of reference point CTYPE1F = 'FREQ-V2F' / Frequency, non-linear axis CRVAL1F = 102.4071237E+9 / [Hz] Frequency of reference channel CDELT1F = -2.513721996E+5 / [Hz] Channel spacing CUNIT1F = 'Hz ' / Units of coordinate increment and value COMMENT RESTFRQF= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVF= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSF= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSF= 'TOPOCENT' / Reference frame of observation VELOSYSF= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCF= 'LSRK ' / Reference frame of source redshift ZSOURCEF= 0.0000 / Redshift of the source COMMENT CRPIX2F = 1 CDELT2F = 1.0 CTYPE2F = 'RA ' CRVAL2F = 83.81042 / [deg] (05h35m14.5s) CUNIT2F = 'deg ' COMMENT CRPIX3F = 1 CDELT3F = 1.0 CTYPE3F = 'DEC ' CRVAL3F = -5.375222 / [deg] (-05:22:30.8) CUNIT3F = 'deg ' COMMENT RADESYSF= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXF= 2000.0 / Equinox J2000.0 COMMENT CRPIX4F = 1 CDELT4F = 1.0 CTYPE4F = 'STOKES ' CRVAL4F = 1 / Stokes I (total intensity) COMMENT COMMENT -------------------------------------------------------- Photon energy COMMENT CRPIX1E = 32768.0 / Pixel coordinate of reference point CTYPE1E = 'ENER-V2F' / Photon energy, non-linear axis CRVAL1E = 4.235222141E-4 / [eV] Photon energy of reference channel CDELT1E = -1.039592821E-9 / [eV] Channel spacing CUNIT1E = 'eV ' / Units of coordinate increment and value COMMENT RESTFRQE= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVE= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSE= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSE= 'TOPOCENT' / Reference frame of observation VELOSYSE= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCE= 'LSRK ' / Reference frame of source redshift ZSOURCEE= 0.0000 / Redshift of the source COMMENT CRPIX2E = 1 CDELT2E = 1.0 CTYPE2E = 'RA ' CRVAL2E = 83.81042 / [deg] (05h35m14.5s) CUNIT2E = 'deg ' COMMENT CRPIX3E = 1 CDELT3E = 1.0 CTYPE3E = 'DEC ' CRVAL3E = -5.375222 / [deg] (-05:22:30.8) CUNIT3E = 'deg ' COMMENT RADESYSE= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXE= 2000.0 / Equinox J2000.0 COMMENT CRPIX4E = 1 CDELT4E = 1.0 CTYPE4E = 'STOKES ' CRVAL4E = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------------------- Wave number COMMENT CRPIX1N = 32768.0 / Pixel coordinate of reference point CTYPE1N = 'WAVN-V2F' / Wave number, non-linear axis CRVAL1N = 3.415933955E+2 / [/m] Wave number of reference channel CDELT1N = -8.384874032E-4 / [/m] Channel spacing CUNIT1N = '/m ' / Units of coordinate increment and value COMMENT RESTFRQN= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVN= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSN= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSN= 'TOPOCENT' / Reference frame of observation VELOSYSN= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCN= 'LSRK ' / Reference frame of source redshift ZSOURCEN= 0.0000 / Redshift of the source COMMENT CRPIX2N = 1 CDELT2N = 1.0 CTYPE2N = 'RA ' CRVAL2N = 83.81042 / [deg] (05h35m14.5s) CUNIT2N = 'deg ' COMMENT CRPIX3N = 1 CDELT3N = 1.0 CTYPE3N = 'DEC ' CRVAL3N = -5.375222 / [deg] (-05:22:30.8) CUNIT3N = 'deg ' COMMENT RADESYSN= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXN= 2000.0 / Equinox J2000.0 COMMENT CRPIX4N = 1 CDELT4N = 1.0 CTYPE4N = 'STOKES ' CRVAL4N = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------- Radio velocity COMMENT CRPIX1R = 32768.0 / Pixel coordinate of reference point CTYPE1R = 'VRAD-V2F' / Radio velocity, non-linear axis CRVAL1R = 2.120347082E+7 / [m/s] Radio velocity of reference channel CDELT1R = 6.838345224E+2 / [m/s] Channel spacing CUNIT1R = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQR= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVR= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSR= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSR= 'TOPOCENT' / Reference frame of observation VELOSYSR= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCR= 'LSRK ' / Reference frame of source redshift ZSOURCER= 0.0000 / Redshift of the source COMMENT CRPIX2R = 1 CDELT2R = 1.0 CTYPE2R = 'RA ' CRVAL2R = 83.81042 / [deg] (05h35m14.5s) CUNIT2R = 'deg ' COMMENT CRPIX3R = 1 CDELT3R = 1.0 CTYPE3R = 'DEC ' CRVAL3R = -5.375222 / [deg] (-05:22:30.8) CUNIT3R = 'deg ' COMMENT RADESYSR= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXR= 2000.0 / Equinox J2000.0 COMMENT CRPIX4R = 1 CDELT4R = 1.0 CTYPE4R = 'STOKES ' CRVAL4R = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------------- Wavelength COMMENT CRPIX1W = 32768.0 / Pixel coordinate of reference point CTYPE1W = 'WAVE-V2W' / Wavelength in vacuuo, linear axis CRVAL1W = 2.927457068E-3 / [m] Wavelength of reference channel CDELT1W = 7.185841143E-9 / [m] Channel spacing CUNIT1W = 'm ' / Units of coordinate increment and value COMMENT RESTFRQW= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVW= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSW= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSW= 'TOPOCENT' / Reference frame of observation VELOSYSW= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCW= 'LSRK ' / Reference frame of source redshift ZSOURCEW= 0.0000 / Redshift of the source COMMENT CRPIX2W = 1 CDELT2W = 1.0 CTYPE2W = 'RA ' CRVAL2W = 83.81042 / [deg] (05h35m14.5s) CUNIT2W = 'deg ' COMMENT CRPIX3W = 1 CDELT3W = 1.0 CTYPE3W = 'DEC ' CRVAL3W = -5.375222 / [deg] (-05:22:30.8) CUNIT3W = 'deg ' COMMENT RADESYSW= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXW= 2000.0 / Equinox J2000.0 COMMENT CRPIX4W = 1 CDELT4W = 1.0 CTYPE4W = 'STOKES ' CRVAL4W = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------- Optical velocity COMMENT CRPIX1O = 32768.0 / Pixel coordinate of reference point CTYPE1O = 'VOPT-V2W' / Optical velocity, linear axis CRVAL1O = 2.281727178E+7 / [m/s] Optical velocity of reference channel CDELT1O = 7.918894164E+2 / [m/s] Channel spacing CUNIT1O = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQO= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVO= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSO= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSO= 'TOPOCENT' / Reference frame of observation VELOSYSO= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCO= 'LSRK ' / Reference frame of source redshift ZSOURCEO= 0.0000 / Redshift of the source COMMENT CRPIX2O = 1 CDELT2O = 1.0 CTYPE2O = 'RA ' CRVAL2O = 83.81042 / [deg] (05h35m14.5s) CUNIT2O = 'deg ' COMMENT CRPIX3O = 1 CDELT3O = 1.0 CTYPE3O = 'DEC ' CRVAL3O = -5.375222 / [deg] (-05:22:30.8) CUNIT3O = 'deg ' COMMENT RADESYSO= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXO= 2000.0 / Equinox J2000.0 COMMENT CRPIX4O = 1 CDELT4O = 1.0 CTYPE4O = 'STOKES ' CRVAL4O = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------------- Redshift COMMENT CRPIX1Z = 32768.0 / Pixel coordinate of reference point CTYPE1Z = 'ZOPT-V2W' / Redshift, linear axis CRVAL1Z = 7.611022615E-2 / [] Redshift of reference channel CDELT1Z = 2.641458767E-6 / [] Channel spacing COMMENT RESTFRQZ= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVZ= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSZ= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSZ= 'TOPOCENT' / Reference frame of observation VELOSYSZ= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCZ= 'LSRK ' / Reference frame of source redshift ZSOURCEZ= 0.0000 / Redshift of the source COMMENT CRPIX2Z = 1 CDELT2Z = 1.0 CTYPE2Z = 'RA ' CRVAL2Z = 83.81042 / [deg] (05h35m14.5s) CUNIT2Z = 'deg ' COMMENT CRPIX3Z = 1 CDELT3Z = 1.0 CTYPE3Z = 'DEC ' CRVAL3Z = -5.375222 / [deg] (-05:22:30.8) CUNIT3Z = 'deg ' COMMENT RADESYSZ= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXZ= 2000.0 / Equinox J2000.0 COMMENT CRPIX4Z = 1 CDELT4Z = 1.0 CTYPE4Z = 'STOKES ' CRVAL4Z = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------ Relativistic velocity COMMENT CRPIX1 = 32768.0 / Pixel coordinate of reference point CTYPE1 = 'VELO ' / Relativistic velocity, non-linear axis CRVAL1 = 2.195128874E+7 / [m/s] Velocity of reference channel CDELT1 = 7.319359645E+2 / [m/s] Channel spacing CUNIT1 = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQ = 110201353000.0 / [Hz] 13CO line rest frequency RESTWAV = 0.00272040633 / [m] 13CO line rest wavelength SPECSYS = 'LSRK ' / Reference frame of spectral coordinates SSYSOBS = 'TOPOCENT' / Reference frame of observation VELOSYS = 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRC = 'LSRK ' / Reference frame of source redshift ZSOURCE = 0.0000 / Redshift of the source COMMENT CRPIX2 = 1 CDELT2 = 1.0 CTYPE2 = 'RA ' CRVAL2 = 83.81042 / [deg] (05h35m14.5s) CUNIT2 = 'deg ' COMMENT CRPIX3 = 1 CDELT3 = 1.0 CTYPE3 = 'DEC ' CRVAL3 = -5.375222 / [deg] (-05:22:30.8) CUNIT3 = 'deg ' COMMENT RADESYS = 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOX = 2000.0 / Equinox J2000.0 COMMENT CRPIX4 = 1 CDELT4 = 1.0 CTYPE4 = 'STOKES ' CRVAL4 = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------- Relativistic beta (v/c) COMMENT CRPIX1B = 32768.0 / Pixel coordinate of reference point CTYPE1B = 'BETA ' / Relativistic beta (v/c), non-linear axis CRVAL1B = 7.322161766E-2 / [] Relativistic beta of reference channel CDELT1B = 2.441475578E-6 / [] Channel spacing COMMENT RESTFRQB= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVB= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSB= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSB= 'TOPOCENT' / Reference frame of observation VELOSYSB= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCB= 'LSRK ' / Reference frame of source redshift ZSOURCEB= 0.0000 / Redshift of the source COMMENT CRPIX2B = 1 CDELT2B = 1.0 CTYPE2B = 'RA ' CRVAL2B = 83.81042 / [deg] (05h35m14.5s) CUNIT2B = 'deg ' COMMENT CRPIX3B = 1 CDELT3B = 1.0 CTYPE3B = 'DEC ' CRVAL3B = -5.375222 / [deg] (-05:22:30.8) CUNIT3B = 'deg ' COMMENT RADESYSB= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXB= 2000.0 / Equinox J2000.0 COMMENT CRPIX4B = 1 CDELT4B = 1.0 CTYPE4B = 'STOKES ' CRVAL4B = 1 / Stokes I (total intensity) COMMENT HISTORY fimgcreate 1.0b at 2009-04-22T04:28:25 DATE = '2009-04-22T04:28:25' / file creation date (YYYY-MM-DDThh:mm:ss UT) pywcs-1.12/lib/pywcs/tests/spectra/orion-velo-4.hdr0000644001153600020070000007234012310355627024324 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 4 / number of data axes NAXIS1 = 4096 / length of data axis 1 NAXIS2 = 1 / length of data axis 2 NAXIS3 = 1 / length of data axis 3 NAXIS4 = 1 / length of data axis 4 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H COMMENT COMMENT This FITS file contains an example spectral WCS header constructed by COMMENT Mark Calabretta (ATNF) and Dirk Petry (ESO) based on an observation COMMENT of the Orion Kleinmann-Low nebula made by Andrew Walsh (JCU) and COMMENT Sven Thorwirth (MPIfR) using the Mopra radio telescope. COMMENT COMMENT The 110GHz 13CO 1-0 spectrum in this file is linear in relativistic COMMENT velocity having been regridded from a linear frequency axis, as COMMENT observed. COMMENT COMMENT The reference pixel has been placed deliberately well outside the COMMENT the spectrum in order to test spectral-WCS-interpreting software. COMMENT COMMENT Spectral representations are: COMMENT F: Frequency ...frequency-like COMMENT E: Photon energy ...frequency-like COMMENT N: Wave number ...frequency-like COMMENT R: Radio velocity ...frequency-like COMMENT W: Wavelength ...wavelength-like COMMENT O: Optical velocity ...wavelength-like COMMENT Z: Redshift ...wavelength-like COMMENT Relativistic velocity (default) ...velocity-like COMMENT B: Relativistic beta ...velocity-like COMMENT COMMENT The Mopra radio telescope is operated by the Australia Telescope COMMENT National Facility. COMMENT COMMENT Author: Mark Calabretta, Australia Telescope National Facility COMMENT http://www.atnf.csiro.au/~mcalabre/index.html COMMENT 2009-04-22 COMMENT ---------------------------------------------------------------------- COMMENT OBJECT = 'Orion-KL' / Orion Kleinmann-Low nebula MOLECULE= '13CO ' / Carbon(13) monoxide TRANSITI= '1-0 ' / 1-0 transition DATE-OBS= '2006-07-09T20:29:00' / Date of observation TELESCOP= 'ATNF Mopra' / 22m mm-wave telescope OBSERVER= 'Walsh/Thorwirth' / Observers BUNIT = 'K ' / Brightness units, Kelvin COMMENT COMMENT ------------------------------------------------------------ Frequency COMMENT CRPIX1F = 32768.0 / Pixel coordinate of reference point CTYPE1F = 'FREQ-V2F' / Frequency, non-linear axis CRVAL1F = 102.4071237E+9 / [Hz] Frequency of reference channel CDELT1F = -2.513721996E+5 / [Hz] Channel spacing CUNIT1F = 'Hz ' / Units of coordinate increment and value COMMENT RESTFRQF= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVF= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSF= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSF= 'TOPOCENT' / Reference frame of observation VELOSYSF= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCF= 'LSRK ' / Reference frame of source redshift ZSOURCEF= 0.0000 / Redshift of the source COMMENT CRPIX2F = 1 CDELT2F = 1.0 CTYPE2F = 'RA ' CRVAL2F = 83.81042 / [deg] (05h35m14.5s) CUNIT2F = 'deg ' COMMENT CRPIX3F = 1 CDELT3F = 1.0 CTYPE3F = 'DEC ' CRVAL3F = -5.375222 / [deg] (-05:22:30.8) CUNIT3F = 'deg ' COMMENT RADESYSF= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXF= 2000.0 / Equinox J2000.0 COMMENT CRPIX4F = 1 CDELT4F = 1.0 CTYPE4F = 'STOKES ' CRVAL4F = 1 / Stokes I (total intensity) COMMENT COMMENT -------------------------------------------------------- Photon energy COMMENT CRPIX1E = 32768.0 / Pixel coordinate of reference point CTYPE1E = 'ENER-V2F' / Photon energy, non-linear axis CRVAL1E = 4.235222141E-4 / [eV] Photon energy of reference channel CDELT1E = -1.039592821E-9 / [eV] Channel spacing CUNIT1E = 'eV ' / Units of coordinate increment and value COMMENT RESTFRQE= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVE= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSE= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSE= 'TOPOCENT' / Reference frame of observation VELOSYSE= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCE= 'LSRK ' / Reference frame of source redshift ZSOURCEE= 0.0000 / Redshift of the source COMMENT CRPIX2E = 1 CDELT2E = 1.0 CTYPE2E = 'RA ' CRVAL2E = 83.81042 / [deg] (05h35m14.5s) CUNIT2E = 'deg ' COMMENT CRPIX3E = 1 CDELT3E = 1.0 CTYPE3E = 'DEC ' CRVAL3E = -5.375222 / [deg] (-05:22:30.8) CUNIT3E = 'deg ' COMMENT RADESYSE= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXE= 2000.0 / Equinox J2000.0 COMMENT CRPIX4E = 1 CDELT4E = 1.0 CTYPE4E = 'STOKES ' CRVAL4E = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------------------- Wave number COMMENT CRPIX1N = 32768.0 / Pixel coordinate of reference point CTYPE1N = 'WAVN-V2F' / Wave number, non-linear axis CRVAL1N = 3.415933955E+2 / [/m] Wave number of reference channel CDELT1N = -8.384874032E-4 / [/m] Channel spacing CUNIT1N = '/m ' / Units of coordinate increment and value COMMENT RESTFRQN= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVN= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSN= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSN= 'TOPOCENT' / Reference frame of observation VELOSYSN= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCN= 'LSRK ' / Reference frame of source redshift ZSOURCEN= 0.0000 / Redshift of the source COMMENT CRPIX2N = 1 CDELT2N = 1.0 CTYPE2N = 'RA ' CRVAL2N = 83.81042 / [deg] (05h35m14.5s) CUNIT2N = 'deg ' COMMENT CRPIX3N = 1 CDELT3N = 1.0 CTYPE3N = 'DEC ' CRVAL3N = -5.375222 / [deg] (-05:22:30.8) CUNIT3N = 'deg ' COMMENT RADESYSN= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXN= 2000.0 / Equinox J2000.0 COMMENT CRPIX4N = 1 CDELT4N = 1.0 CTYPE4N = 'STOKES ' CRVAL4N = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------- Radio velocity COMMENT CRPIX1R = 32768.0 / Pixel coordinate of reference point CTYPE1R = 'VRAD-V2F' / Radio velocity, non-linear axis CRVAL1R = 2.120347082E+7 / [m/s] Radio velocity of reference channel CDELT1R = 6.838345224E+2 / [m/s] Channel spacing CUNIT1R = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQR= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVR= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSR= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSR= 'TOPOCENT' / Reference frame of observation VELOSYSR= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCR= 'LSRK ' / Reference frame of source redshift ZSOURCER= 0.0000 / Redshift of the source COMMENT CRPIX2R = 1 CDELT2R = 1.0 CTYPE2R = 'RA ' CRVAL2R = 83.81042 / [deg] (05h35m14.5s) CUNIT2R = 'deg ' COMMENT CRPIX3R = 1 CDELT3R = 1.0 CTYPE3R = 'DEC ' CRVAL3R = -5.375222 / [deg] (-05:22:30.8) CUNIT3R = 'deg ' COMMENT RADESYSR= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXR= 2000.0 / Equinox J2000.0 COMMENT CRPIX4R = 1 CDELT4R = 1.0 CTYPE4R = 'STOKES ' CRVAL4R = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------------- Wavelength COMMENT CRPIX1W = 32768.0 / Pixel coordinate of reference point CTYPE1W = 'WAVE-V2W' / Wavelength in vacuuo, linear axis CRVAL1W = 2.927457068E-3 / [m] Wavelength of reference channel CDELT1W = 7.185841143E-9 / [m] Channel spacing CUNIT1W = 'm ' / Units of coordinate increment and value COMMENT RESTFRQW= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVW= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSW= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSW= 'TOPOCENT' / Reference frame of observation VELOSYSW= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCW= 'LSRK ' / Reference frame of source redshift ZSOURCEW= 0.0000 / Redshift of the source COMMENT CRPIX2W = 1 CDELT2W = 1.0 CTYPE2W = 'RA ' CRVAL2W = 83.81042 / [deg] (05h35m14.5s) CUNIT2W = 'deg ' COMMENT CRPIX3W = 1 CDELT3W = 1.0 CTYPE3W = 'DEC ' CRVAL3W = -5.375222 / [deg] (-05:22:30.8) CUNIT3W = 'deg ' COMMENT RADESYSW= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXW= 2000.0 / Equinox J2000.0 COMMENT CRPIX4W = 1 CDELT4W = 1.0 CTYPE4W = 'STOKES ' CRVAL4W = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------- Optical velocity COMMENT CRPIX1O = 32768.0 / Pixel coordinate of reference point CTYPE1O = 'VOPT-V2W' / Optical velocity, linear axis CRVAL1O = 2.281727178E+7 / [m/s] Optical velocity of reference channel CDELT1O = 7.918894164E+2 / [m/s] Channel spacing CUNIT1O = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQO= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVO= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSO= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSO= 'TOPOCENT' / Reference frame of observation VELOSYSO= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCO= 'LSRK ' / Reference frame of source redshift ZSOURCEO= 0.0000 / Redshift of the source COMMENT CRPIX2O = 1 CDELT2O = 1.0 CTYPE2O = 'RA ' CRVAL2O = 83.81042 / [deg] (05h35m14.5s) CUNIT2O = 'deg ' COMMENT CRPIX3O = 1 CDELT3O = 1.0 CTYPE3O = 'DEC ' CRVAL3O = -5.375222 / [deg] (-05:22:30.8) CUNIT3O = 'deg ' COMMENT RADESYSO= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXO= 2000.0 / Equinox J2000.0 COMMENT CRPIX4O = 1 CDELT4O = 1.0 CTYPE4O = 'STOKES ' CRVAL4O = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------------- Redshift COMMENT CRPIX1Z = 32768.0 / Pixel coordinate of reference point CTYPE1Z = 'ZOPT-V2W' / Redshift, linear axis CRVAL1Z = 7.611022615E-2 / [] Redshift of reference channel CDELT1Z = 2.641458767E-6 / [] Channel spacing COMMENT RESTFRQZ= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVZ= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSZ= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSZ= 'TOPOCENT' / Reference frame of observation VELOSYSZ= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCZ= 'LSRK ' / Reference frame of source redshift ZSOURCEZ= 0.0000 / Redshift of the source COMMENT CRPIX2Z = 1 CDELT2Z = 1.0 CTYPE2Z = 'RA ' CRVAL2Z = 83.81042 / [deg] (05h35m14.5s) CUNIT2Z = 'deg ' COMMENT CRPIX3Z = 1 CDELT3Z = 1.0 CTYPE3Z = 'DEC ' CRVAL3Z = -5.375222 / [deg] (-05:22:30.8) CUNIT3Z = 'deg ' COMMENT RADESYSZ= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXZ= 2000.0 / Equinox J2000.0 COMMENT CRPIX4Z = 1 CDELT4Z = 1.0 CTYPE4Z = 'STOKES ' CRVAL4Z = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------ Relativistic velocity COMMENT CRPIX1 = 32768.0 / Pixel coordinate of reference point CTYPE1 = 'VELO ' / Relativistic velocity, non-linear axis CRVAL1 = 2.195128874E+7 / [m/s] Velocity of reference channel CDELT1 = 7.319359645E+2 / [m/s] Channel spacing CUNIT1 = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQ = 110201353000.0 / [Hz] 13CO line rest frequency RESTWAV = 0.00272040633 / [m] 13CO line rest wavelength SPECSYS = 'LSRK ' / Reference frame of spectral coordinates SSYSOBS = 'TOPOCENT' / Reference frame of observation VELOSYS = 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRC = 'LSRK ' / Reference frame of source redshift ZSOURCE = 0.0000 / Redshift of the source COMMENT CRPIX2 = 1 CDELT2 = 1.0 CTYPE2 = 'RA ' CRVAL2 = 83.81042 / [deg] (05h35m14.5s) CUNIT2 = 'deg ' COMMENT CRPIX3 = 1 CDELT3 = 1.0 CTYPE3 = 'DEC ' CRVAL3 = -5.375222 / [deg] (-05:22:30.8) CUNIT3 = 'deg ' COMMENT RADESYS = 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOX = 2000.0 / Equinox J2000.0 COMMENT CRPIX4 = 1 CDELT4 = 1.0 CTYPE4 = 'STOKES ' CRVAL4 = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------- Relativistic beta (v/c) COMMENT CRPIX1B = 32768.0 / Pixel coordinate of reference point CTYPE1B = 'BETA ' / Relativistic beta (v/c), non-linear axis CRVAL1B = 7.322161766E-2 / [] Relativistic beta of reference channel CDELT1B = 2.441475578E-6 / [] Channel spacing COMMENT RESTFRQB= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVB= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSB= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSB= 'TOPOCENT' / Reference frame of observation VELOSYSB= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCB= 'LSRK ' / Reference frame of source redshift ZSOURCEB= 0.0000 / Redshift of the source COMMENT CRPIX2B = 1 CDELT2B = 1.0 CTYPE2B = 'RA ' CRVAL2B = 83.81042 / [deg] (05h35m14.5s) CUNIT2B = 'deg ' COMMENT CRPIX3B = 1 CDELT3B = 1.0 CTYPE3B = 'DEC ' CRVAL3B = -5.375222 / [deg] (-05:22:30.8) CUNIT3B = 'deg ' COMMENT RADESYSB= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXB= 2000.0 / Equinox J2000.0 COMMENT CRPIX4B = 1 CDELT4B = 1.0 CTYPE4B = 'STOKES ' CRVAL4B = 1 / Stokes I (total intensity) COMMENT HISTORY fimgcreate 1.0b at 2009-04-22T04:28:33 DATE = '2009-04-22T04:28:33' / file creation date (YYYY-MM-DDThh:mm:ss UT) pywcs-1.12/lib/pywcs/tests/spectra/orion-wave-1.hdr0000644001153600020070000007164012310355627024320 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 1 / number of data axes NAXIS1 = 4096 / length of data axis 1 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H COMMENT COMMENT This FITS file contains an example spectral WCS header constructed by COMMENT Mark Calabretta (ATNF) and Dirk Petry (ESO) based on an observation COMMENT of the Orion Kleinmann-Low nebula made by Andrew Walsh (JCU) and COMMENT Sven Thorwirth (MPIfR) using the Mopra radio telescope. COMMENT COMMENT The 110GHz 13CO 1-0 spectrum in this file is linear in wavelength, COMMENT having been regridded from a linear frequency axis, as observed. COMMENT COMMENT The reference pixel has been placed deliberately well outside the COMMENT the spectrum in order to test spectral-WCS-interpreting software. COMMENT COMMENT Spectral representations are: COMMENT F: Frequency ...frequency-like COMMENT E: Photon energy ...frequency-like COMMENT N: Wave number ...frequency-like COMMENT R: Radio velocity ...frequency-like COMMENT Wavelength (default) ...wavelength-like COMMENT O: Optical velocity ...wavelength-like COMMENT Z: Redshift ...wavelength-like COMMENT V: Relativistic velocity ...velocity-like COMMENT B: Relativistic beta ...velocity-like COMMENT COMMENT The Mopra radio telescope is operated by the Australia Telescope COMMENT National Facility. COMMENT COMMENT Author: Mark Calabretta, Australia Telescope National Facility COMMENT http://www.atnf.csiro.au/~mcalabre/index.html COMMENT 2009-04-22 COMMENT ---------------------------------------------------------------------- COMMENT OBJECT = 'Orion-KL' / Orion Kleinmann-Low nebula MOLECULE= '13CO ' / Carbon(13) monoxide TRANSITI= '1-0 ' / 1-0 transition DATE-OBS= '2006-07-09T20:29:00' / Date of observation TELESCOP= 'ATNF Mopra' / 22m mm-wave telescope OBSERVER= 'Walsh/Thorwirth' / Observers BUNIT = 'K ' / Brightness units, Kelvin COMMENT COMMENT ------------------------------------------------------------ Frequency COMMENT CRPIX1F = 32768.0 / Pixel coordinate of reference point CTYPE1F = 'FREQ-W2F' / Frequency, non-linear axis CRVAL1F = 102.6940613E+9 / [Hz] Frequency of reference channel CDELT1F = -2.332330873E+5 / [Hz] Channel spacing CUNIT1F = 'Hz ' / Units of coordinate increment and value COMMENT RESTFRQF= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVF= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSF= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSF= 'TOPOCENT' / Reference frame of observation VELOSYSF= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCF= 'LSRK ' / Reference frame of source redshift ZSOURCEF= 0.0000 / Redshift of the source COMMENT CRPIX2F = 1 CDELT2F = 1.0 CTYPE2F = 'RA ' CRVAL2F = 83.81042 / [deg] (05h35m14.5s) CUNIT2F = 'deg ' COMMENT CRPIX3F = 1 CDELT3F = 1.0 CTYPE3F = 'DEC ' CRVAL3F = -5.375222 / [deg] (-05:22:30.8) CUNIT3F = 'deg ' COMMENT RADESYSF= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXF= 2000.0 / Equinox J2000.0 COMMENT CRPIX4F = 1 CDELT4F = 1.0 CTYPE4F = 'STOKES ' CRVAL4F = 1 / Stokes I (total intensity) COMMENT COMMENT -------------------------------------------------------- Photon energy COMMENT CRPIX1E = 32768.0 / Pixel coordinate of reference point CTYPE1E = 'ENER-W2F' / Photon energy, non-linear axis CRVAL1E = 4.247088937E-4 / [eV] Photon energy of reference channel CDELT1E = -0.9645754124E-9 / [eV] Channel spacing CUNIT1E = 'eV ' / Units of coordinate increment and value COMMENT RESTFRQE= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVE= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSE= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSE= 'TOPOCENT' / Reference frame of observation VELOSYSE= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCE= 'LSRK ' / Reference frame of source redshift ZSOURCEE= 0.0000 / Redshift of the source COMMENT CRPIX2E = 1 CDELT2E = 1.0 CTYPE2E = 'RA ' CRVAL2E = 83.81042 / [deg] (05h35m14.5s) CUNIT2E = 'deg ' COMMENT CRPIX3E = 1 CDELT3E = 1.0 CTYPE3E = 'DEC ' CRVAL3E = -5.375222 / [deg] (-05:22:30.8) CUNIT3E = 'deg ' COMMENT RADESYSE= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXE= 2000.0 / Equinox J2000.0 COMMENT CRPIX4E = 1 CDELT4E = 1.0 CTYPE4E = 'STOKES ' CRVAL4E = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------------------- Wave number COMMENT CRPIX1N = 32768.0 / Pixel coordinate of reference point CTYPE1N = 'WAVN-W2F' / Wave number, non-linear axis CRVAL1N = 3.425505162E+2 / [/m] Wave number of reference channel CDELT1N = -7.779818375E-4 / [/m] Channel spacing CUNIT1N = '/m ' / Units of coordinate increment and value COMMENT RESTFRQN= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVN= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSN= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSN= 'TOPOCENT' / Reference frame of observation VELOSYSN= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCN= 'LSRK ' / Reference frame of source redshift ZSOURCEN= 0.0000 / Redshift of the source COMMENT CRPIX2N = 1 CDELT2N = 1.0 CTYPE2N = 'RA ' CRVAL2N = 83.81042 / [deg] (05h35m14.5s) CUNIT2N = 'deg ' COMMENT CRPIX3N = 1 CDELT3N = 1.0 CTYPE3N = 'DEC ' CRVAL3N = -5.375222 / [deg] (-05:22:30.8) CUNIT3N = 'deg ' COMMENT RADESYSN= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXN= 2000.0 / Equinox J2000.0 COMMENT CRPIX4N = 1 CDELT4N = 1.0 CTYPE4N = 'STOKES ' CRVAL4N = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------- Radio velocity COMMENT CRPIX1R = 32768.0 / Pixel coordinate of reference point CTYPE1R = 'VRAD-W2F' / Radio velocity, non-linear axis CRVAL1R = 2.042288396E+7 / [m/s] Radio velocity of reference channel CDELT1R = 6.344887666E+2 / [m/s] Channel spacing CUNIT1R = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQR= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVR= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSR= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSR= 'TOPOCENT' / Reference frame of observation VELOSYSR= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCR= 'LSRK ' / Reference frame of source redshift ZSOURCER= 0.0000 / Redshift of the source COMMENT CRPIX2R = 1 CDELT2R = 1.0 CTYPE2R = 'RA ' CRVAL2R = 83.81042 / [deg] (05h35m14.5s) CUNIT2R = 'deg ' COMMENT CRPIX3R = 1 CDELT3R = 1.0 CTYPE3R = 'DEC ' CRVAL3R = -5.375222 / [deg] (-05:22:30.8) CUNIT3R = 'deg ' COMMENT RADESYSR= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXR= 2000.0 / Equinox J2000.0 COMMENT CRPIX4R = 1 CDELT4R = 1.0 CTYPE4R = 'STOKES ' CRVAL4R = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------------- Wavelength COMMENT CRPIX1 = 32768.0 / Pixel coordinate of reference point CTYPE1 = 'WAVE ' / Wavelength in vacuuo, linear axis CRVAL1 = 2.919277457E-3 / [m] Wavelength of reference channel CDELT1 = 6.630101933E-9 / [m] Channel spacing CUNIT1 = 'm ' / Units of coordinate increment and value COMMENT RESTFRQ = 110201353000.0 / [Hz] 13CO line rest frequency RESTWAV = 0.00272040633 / [m] 13CO line rest wavelength SPECSYS = 'LSRK ' / Reference frame of spectral coordinates SSYSOBS = 'TOPOCENT' / Reference frame of observation VELOSYS = 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRC = 'LSRK ' / Reference frame of source redshift ZSOURCE = 0.0000 / Redshift of the source COMMENT CRPIX2 = 1 CDELT2 = 1.0 CTYPE2 = 'RA ' CRVAL2 = 83.81042 / [deg] (05h35m14.5s) CUNIT2 = 'deg ' COMMENT CRPIX3 = 1 CDELT3 = 1.0 CTYPE3 = 'DEC ' CRVAL3 = -5.375222 / [deg] (-05:22:30.8) CUNIT3 = 'deg ' COMMENT RADESYS = 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOX = 2000.0 / Equinox J2000.0 COMMENT CRPIX4 = 1 CDELT4 = 1.0 CTYPE4 = 'STOKES ' CRVAL4 = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------- Optical velocity COMMENT CRPIX1O = 32768.0 / Pixel coordinate of reference point CTYPE1O = 'VOPT ' / Optical velocity, linear axis CRVAL1O = 2.191586755E+7 / [m/s] Optical velocity of reference channel CDELT1O = 7.306462036E+2 / [m/s] Channel spacing CUNIT1O = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQO= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVO= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSO= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSO= 'TOPOCENT' / Reference frame of observation VELOSYSO= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCO= 'LSRK ' / Reference frame of source redshift ZSOURCEO= 0.0000 / Redshift of the source COMMENT CRPIX2O = 1 CDELT2O = 1.0 CTYPE2O = 'RA ' CRVAL2O = 83.81042 / [deg] (05h35m14.5s) CUNIT2O = 'deg ' COMMENT CRPIX3O = 1 CDELT3O = 1.0 CTYPE3O = 'DEC ' CRVAL3O = -5.375222 / [deg] (-05:22:30.8) CUNIT3O = 'deg ' COMMENT RADESYSO= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXO= 2000.0 / Equinox J2000.0 COMMENT CRPIX4O = 1 CDELT4O = 1.0 CTYPE4O = 'STOKES ' CRVAL4O = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------------- Redshift COMMENT CRPIX1Z = 32768.0 / Pixel coordinate of reference point CTYPE1Z = 'ZOPT ' / Redshift, linear axis CRVAL1Z = 7.310346531E-2 / [] Redshift of reference channel CDELT1Z = 2.437173398E-6 / [] Channel spacing COMMENT RESTFRQZ= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVZ= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSZ= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSZ= 'TOPOCENT' / Reference frame of observation VELOSYSZ= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCZ= 'LSRK ' / Reference frame of source redshift ZSOURCEZ= 0.0000 / Redshift of the source COMMENT CRPIX2Z = 1 CDELT2Z = 1.0 CTYPE2Z = 'RA ' CRVAL2Z = 83.81042 / [deg] (05h35m14.5s) CUNIT2Z = 'deg ' COMMENT CRPIX3Z = 1 CDELT3Z = 1.0 CTYPE3Z = 'DEC ' CRVAL3Z = -5.375222 / [deg] (-05:22:30.8) CUNIT3Z = 'deg ' COMMENT RADESYSZ= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXZ= 2000.0 / Equinox J2000.0 COMMENT CRPIX4Z = 1 CDELT4Z = 1.0 CTYPE4Z = 'STOKES ' CRVAL4Z = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------ Relativistic velocity COMMENT CRPIX1V = 32768.0 / Pixel coordinate of reference point CTYPE1V = 'VELO-W2V' / Relativistic velocity, non-linear axis CRVAL1V = 2.111679434E+7 / [m/s] Velocity of reference channel CDELT1V = 6.774939349E+2 / [m/s] Channel spacing CUNIT1V = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQV= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVV= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSV= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSV= 'TOPOCENT' / Reference frame of observation VELOSYSV= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCV= 'LSRK ' / Reference frame of source redshift ZSOURCEV= 0.0000 / Redshift of the source COMMENT CRPIX2V = 1 CDELT2V = 1.0 CTYPE2V = 'RA ' CRVAL2V = 83.81042 / [deg] (05h35m14.5s) CUNIT2V = 'deg ' COMMENT CRPIX3V = 1 CDELT3V = 1.0 CTYPE3V = 'DEC ' CRVAL3V = -5.375222 / [deg] (-05:22:30.8) CUNIT3V = 'deg ' COMMENT RADESYSV= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXV= 2000.0 / Equinox J2000.0 COMMENT CRPIX4V = 1 CDELT4V = 1.0 CTYPE4V = 'STOKES ' CRVAL4V = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------- Relativistic beta (v/c) COMMENT CRPIX1B = 32768.0 / Pixel coordinate of reference point CTYPE1B = 'BETA-W2V' / Relativistic beta (v/c), non-linear axis CRVAL1B = 7.043804396E-2 / [] Relativistic beta of reference channel CDELT1B = 2.259876514E-6 / [] Channel spacing COMMENT RESTFRQB= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVB= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSB= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSB= 'TOPOCENT' / Reference frame of observation VELOSYSB= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCB= 'LSRK ' / Reference frame of source redshift ZSOURCEB= 0.0000 / Redshift of the source COMMENT CRPIX2B = 1 CDELT2B = 1.0 CTYPE2B = 'RA ' CRVAL2B = 83.81042 / [deg] (05h35m14.5s) CUNIT2B = 'deg ' COMMENT CRPIX3B = 1 CDELT3B = 1.0 CTYPE3B = 'DEC ' CRVAL3B = -5.375222 / [deg] (-05:22:30.8) CUNIT3B = 'deg ' COMMENT RADESYSB= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXB= 2000.0 / Equinox J2000.0 COMMENT CRPIX4B = 1 CDELT4B = 1.0 CTYPE4B = 'STOKES ' CRVAL4B = 1 / Stokes I (total intensity) COMMENT HISTORY fimgcreate 1.0b at 2009-04-22T04:28:10 DATE = '2009-04-22T04:28:10' / file creation date (YYYY-MM-DDThh:mm:ss UT) pywcs-1.12/lib/pywcs/tests/spectra/orion-wave-4.hdr0000644001153600020070000007222012310355627024316 0ustar cslocumSTSCI\science00000000000000SIMPLE = T / file does conform to FITS standard BITPIX = -32 / number of bits per data pixel NAXIS = 4 / number of data axes NAXIS1 = 4096 / length of data axis 1 NAXIS2 = 1 / length of data axis 2 NAXIS3 = 1 / length of data axis 3 NAXIS4 = 1 / length of data axis 4 EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H COMMENT COMMENT This FITS file contains an example spectral WCS header constructed by COMMENT Mark Calabretta (ATNF) and Dirk Petry (ESO) based on an observation COMMENT of the Orion Kleinmann-Low nebula made by Andrew Walsh (JCU) and COMMENT Sven Thorwirth (MPIfR) using the Mopra radio telescope. COMMENT COMMENT The 110GHz 13CO 1-0 spectrum in this file is linear in wavelength, COMMENT having been regridded from a linear frequency axis, as observed. COMMENT COMMENT The reference pixel has been placed deliberately well outside the COMMENT the spectrum in order to test spectral-WCS-interpreting software. COMMENT COMMENT Spectral representations are: COMMENT F: Frequency ...frequency-like COMMENT E: Photon energy ...frequency-like COMMENT N: Wave number ...frequency-like COMMENT R: Radio velocity ...frequency-like COMMENT Wavelength (default) ...wavelength-like COMMENT O: Optical velocity ...wavelength-like COMMENT Z: Redshift ...wavelength-like COMMENT V: Relativistic velocity ...velocity-like COMMENT B: Relativistic beta ...velocity-like COMMENT COMMENT The Mopra radio telescope is operated by the Australia Telescope COMMENT National Facility. COMMENT COMMENT Author: Mark Calabretta, Australia Telescope National Facility COMMENT http://www.atnf.csiro.au/~mcalabre/index.html COMMENT 2009-04-22 COMMENT ---------------------------------------------------------------------- COMMENT OBJECT = 'Orion-KL' / Orion Kleinmann-Low nebula MOLECULE= '13CO ' / Carbon(13) monoxide TRANSITI= '1-0 ' / 1-0 transition DATE-OBS= '2006-07-09T20:29:00' / Date of observation TELESCOP= 'ATNF Mopra' / 22m mm-wave telescope OBSERVER= 'Walsh/Thorwirth' / Observers BUNIT = 'K ' / Brightness units, Kelvin COMMENT COMMENT ------------------------------------------------------------ Frequency COMMENT CRPIX1F = 32768.0 / Pixel coordinate of reference point CTYPE1F = 'FREQ-W2F' / Frequency, non-linear axis CRVAL1F = 102.6940613E+9 / [Hz] Frequency of reference channel CDELT1F = -2.332330873E+5 / [Hz] Channel spacing CUNIT1F = 'Hz ' / Units of coordinate increment and value COMMENT RESTFRQF= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVF= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSF= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSF= 'TOPOCENT' / Reference frame of observation VELOSYSF= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCF= 'LSRK ' / Reference frame of source redshift ZSOURCEF= 0.0000 / Redshift of the source COMMENT CRPIX2F = 1 CDELT2F = 1.0 CTYPE2F = 'RA ' CRVAL2F = 83.81042 / [deg] (05h35m14.5s) CUNIT2F = 'deg ' COMMENT CRPIX3F = 1 CDELT3F = 1.0 CTYPE3F = 'DEC ' CRVAL3F = -5.375222 / [deg] (-05:22:30.8) CUNIT3F = 'deg ' COMMENT RADESYSF= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXF= 2000.0 / Equinox J2000.0 COMMENT CRPIX4F = 1 CDELT4F = 1.0 CTYPE4F = 'STOKES ' CRVAL4F = 1 / Stokes I (total intensity) COMMENT COMMENT -------------------------------------------------------- Photon energy COMMENT CRPIX1E = 32768.0 / Pixel coordinate of reference point CTYPE1E = 'ENER-W2F' / Photon energy, non-linear axis CRVAL1E = 4.247088937E-4 / [eV] Photon energy of reference channel CDELT1E = -0.9645754124E-9 / [eV] Channel spacing CUNIT1E = 'eV ' / Units of coordinate increment and value COMMENT RESTFRQE= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVE= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSE= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSE= 'TOPOCENT' / Reference frame of observation VELOSYSE= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCE= 'LSRK ' / Reference frame of source redshift ZSOURCEE= 0.0000 / Redshift of the source COMMENT CRPIX2E = 1 CDELT2E = 1.0 CTYPE2E = 'RA ' CRVAL2E = 83.81042 / [deg] (05h35m14.5s) CUNIT2E = 'deg ' COMMENT CRPIX3E = 1 CDELT3E = 1.0 CTYPE3E = 'DEC ' CRVAL3E = -5.375222 / [deg] (-05:22:30.8) CUNIT3E = 'deg ' COMMENT RADESYSE= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXE= 2000.0 / Equinox J2000.0 COMMENT CRPIX4E = 1 CDELT4E = 1.0 CTYPE4E = 'STOKES ' CRVAL4E = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------------------- Wave number COMMENT CRPIX1N = 32768.0 / Pixel coordinate of reference point CTYPE1N = 'WAVN-W2F' / Wave number, non-linear axis CRVAL1N = 3.425505162E+2 / [/m] Wave number of reference channel CDELT1N = -7.779818375E-4 / [/m] Channel spacing CUNIT1N = '/m ' / Units of coordinate increment and value COMMENT RESTFRQN= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVN= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSN= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSN= 'TOPOCENT' / Reference frame of observation VELOSYSN= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCN= 'LSRK ' / Reference frame of source redshift ZSOURCEN= 0.0000 / Redshift of the source COMMENT CRPIX2N = 1 CDELT2N = 1.0 CTYPE2N = 'RA ' CRVAL2N = 83.81042 / [deg] (05h35m14.5s) CUNIT2N = 'deg ' COMMENT CRPIX3N = 1 CDELT3N = 1.0 CTYPE3N = 'DEC ' CRVAL3N = -5.375222 / [deg] (-05:22:30.8) CUNIT3N = 'deg ' COMMENT RADESYSN= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXN= 2000.0 / Equinox J2000.0 COMMENT CRPIX4N = 1 CDELT4N = 1.0 CTYPE4N = 'STOKES ' CRVAL4N = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------- Radio velocity COMMENT CRPIX1R = 32768.0 / Pixel coordinate of reference point CTYPE1R = 'VRAD-W2F' / Radio velocity, non-linear axis CRVAL1R = 2.042288396E+7 / [m/s] Radio velocity of reference channel CDELT1R = 6.344887666E+2 / [m/s] Channel spacing CUNIT1R = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQR= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVR= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSR= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSR= 'TOPOCENT' / Reference frame of observation VELOSYSR= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCR= 'LSRK ' / Reference frame of source redshift ZSOURCER= 0.0000 / Redshift of the source COMMENT CRPIX2R = 1 CDELT2R = 1.0 CTYPE2R = 'RA ' CRVAL2R = 83.81042 / [deg] (05h35m14.5s) CUNIT2R = 'deg ' COMMENT CRPIX3R = 1 CDELT3R = 1.0 CTYPE3R = 'DEC ' CRVAL3R = -5.375222 / [deg] (-05:22:30.8) CUNIT3R = 'deg ' COMMENT RADESYSR= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXR= 2000.0 / Equinox J2000.0 COMMENT CRPIX4R = 1 CDELT4R = 1.0 CTYPE4R = 'STOKES ' CRVAL4R = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------------- Wavelength COMMENT CRPIX1 = 32768.0 / Pixel coordinate of reference point CTYPE1 = 'WAVE ' / Wavelength in vacuuo, linear axis CRVAL1 = 2.919277457E-3 / [m] Wavelength of reference channel CDELT1 = 6.630101933E-9 / [m] Channel spacing CUNIT1 = 'm ' / Units of coordinate increment and value COMMENT RESTFRQ = 110201353000.0 / [Hz] 13CO line rest frequency RESTWAV = 0.00272040633 / [m] 13CO line rest wavelength SPECSYS = 'LSRK ' / Reference frame of spectral coordinates SSYSOBS = 'TOPOCENT' / Reference frame of observation VELOSYS = 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRC = 'LSRK ' / Reference frame of source redshift ZSOURCE = 0.0000 / Redshift of the source COMMENT CRPIX2 = 1 CDELT2 = 1.0 CTYPE2 = 'RA ' CRVAL2 = 83.81042 / [deg] (05h35m14.5s) CUNIT2 = 'deg ' COMMENT CRPIX3 = 1 CDELT3 = 1.0 CTYPE3 = 'DEC ' CRVAL3 = -5.375222 / [deg] (-05:22:30.8) CUNIT3 = 'deg ' COMMENT RADESYS = 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOX = 2000.0 / Equinox J2000.0 COMMENT CRPIX4 = 1 CDELT4 = 1.0 CTYPE4 = 'STOKES ' CRVAL4 = 1 / Stokes I (total intensity) COMMENT COMMENT ----------------------------------------------------- Optical velocity COMMENT CRPIX1O = 32768.0 / Pixel coordinate of reference point CTYPE1O = 'VOPT ' / Optical velocity, linear axis CRVAL1O = 2.191586755E+7 / [m/s] Optical velocity of reference channel CDELT1O = 7.306462036E+2 / [m/s] Channel spacing CUNIT1O = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQO= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVO= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSO= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSO= 'TOPOCENT' / Reference frame of observation VELOSYSO= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCO= 'LSRK ' / Reference frame of source redshift ZSOURCEO= 0.0000 / Redshift of the source COMMENT CRPIX2O = 1 CDELT2O = 1.0 CTYPE2O = 'RA ' CRVAL2O = 83.81042 / [deg] (05h35m14.5s) CUNIT2O = 'deg ' COMMENT CRPIX3O = 1 CDELT3O = 1.0 CTYPE3O = 'DEC ' CRVAL3O = -5.375222 / [deg] (-05:22:30.8) CUNIT3O = 'deg ' COMMENT RADESYSO= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXO= 2000.0 / Equinox J2000.0 COMMENT CRPIX4O = 1 CDELT4O = 1.0 CTYPE4O = 'STOKES ' CRVAL4O = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------------------- Redshift COMMENT CRPIX1Z = 32768.0 / Pixel coordinate of reference point CTYPE1Z = 'ZOPT ' / Redshift, linear axis CRVAL1Z = 7.310346531E-2 / [] Redshift of reference channel CDELT1Z = 2.437173398E-6 / [] Channel spacing COMMENT RESTFRQZ= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVZ= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSZ= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSZ= 'TOPOCENT' / Reference frame of observation VELOSYSZ= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCZ= 'LSRK ' / Reference frame of source redshift ZSOURCEZ= 0.0000 / Redshift of the source COMMENT CRPIX2Z = 1 CDELT2Z = 1.0 CTYPE2Z = 'RA ' CRVAL2Z = 83.81042 / [deg] (05h35m14.5s) CUNIT2Z = 'deg ' COMMENT CRPIX3Z = 1 CDELT3Z = 1.0 CTYPE3Z = 'DEC ' CRVAL3Z = -5.375222 / [deg] (-05:22:30.8) CUNIT3Z = 'deg ' COMMENT RADESYSZ= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXZ= 2000.0 / Equinox J2000.0 COMMENT CRPIX4Z = 1 CDELT4Z = 1.0 CTYPE4Z = 'STOKES ' CRVAL4Z = 1 / Stokes I (total intensity) COMMENT COMMENT ------------------------------------------------ Relativistic velocity COMMENT CRPIX1V = 32768.0 / Pixel coordinate of reference point CTYPE1V = 'VELO-W2V' / Relativistic velocity, non-linear axis CRVAL1V = 2.111679434E+7 / [m/s] Velocity of reference channel CDELT1V = 6.774939349E+2 / [m/s] Channel spacing CUNIT1V = 'm/s ' / Units of coordinate increment and value COMMENT RESTFRQV= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVV= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSV= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSV= 'TOPOCENT' / Reference frame of observation VELOSYSV= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCV= 'LSRK ' / Reference frame of source redshift ZSOURCEV= 0.0000 / Redshift of the source COMMENT CRPIX2V = 1 CDELT2V = 1.0 CTYPE2V = 'RA ' CRVAL2V = 83.81042 / [deg] (05h35m14.5s) CUNIT2V = 'deg ' COMMENT CRPIX3V = 1 CDELT3V = 1.0 CTYPE3V = 'DEC ' CRVAL3V = -5.375222 / [deg] (-05:22:30.8) CUNIT3V = 'deg ' COMMENT RADESYSV= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXV= 2000.0 / Equinox J2000.0 COMMENT CRPIX4V = 1 CDELT4V = 1.0 CTYPE4V = 'STOKES ' CRVAL4V = 1 / Stokes I (total intensity) COMMENT COMMENT ---------------------------------------------- Relativistic beta (v/c) COMMENT CRPIX1B = 32768.0 / Pixel coordinate of reference point CTYPE1B = 'BETA-W2V' / Relativistic beta (v/c), non-linear axis CRVAL1B = 7.043804396E-2 / [] Relativistic beta of reference channel CDELT1B = 2.259876514E-6 / [] Channel spacing COMMENT RESTFRQB= 110201353000.0 / [Hz] 13CO line rest frequency RESTWAVB= 0.00272040633 / [m] 13CO line rest wavelength SPECSYSB= 'LSRK ' / Reference frame of spectral coordinates SSYSOBSB= 'TOPOCENT' / Reference frame of observation VELOSYSB= 0.0 / [m/s] Bary-topo velocity towards the source SSYSSRCB= 'LSRK ' / Reference frame of source redshift ZSOURCEB= 0.0000 / Redshift of the source COMMENT CRPIX2B = 1 CDELT2B = 1.0 CTYPE2B = 'RA ' CRVAL2B = 83.81042 / [deg] (05h35m14.5s) CUNIT2B = 'deg ' COMMENT CRPIX3B = 1 CDELT3B = 1.0 CTYPE3B = 'DEC ' CRVAL3B = -5.375222 / [deg] (-05:22:30.8) CUNIT3B = 'deg ' COMMENT RADESYSB= 'FK5 ' / FK5 (IAU 1984) equatorial coordinates EQUINOXB= 2000.0 / Equinox J2000.0 COMMENT CRPIX4B = 1 CDELT4B = 1.0 CTYPE4B = 'STOKES ' CRVAL4B = 1 / Stokes I (total intensity) COMMENT HISTORY fimgcreate 1.0b at 2009-04-22T04:28:18 DATE = '2009-04-22T04:28:18' / file creation date (YYYY-MM-DDThh:mm:ss UT) pywcs-1.12/lib/pywcs/tests/test.py0000755001153600020070000002256512310355627021272 0ustar cslocumSTSCI\science00000000000000import glob import os import sys import numpy as np from numpy.testing import assert_array_almost_equal import pywcs ROOT_DIR = None def setup_module(): global ROOT_DIR # do not use __file__ here - we want to find the data files that # belong to the pywcs that we are testing, even if we are not running # this test from the installed copy of this file. Use pywcs.__file__ ROOT_DIR = os.path.join(os.path.dirname(pywcs.__file__), "tests") # test_maps() is a generator def test_maps(): # test_map() is the function that is called to perform the generated test def test_map(filename): # the test parameter is the base name of the file to use; find # the file in the installed pywcs test directory filename = os.path.join(ROOT_DIR, "maps", filename) fd = open(filename, 'rb') header = fd.read() fd.close() wcs = pywcs.WCS(header) world = wcs.wcs_pix2sky([[97, 97]], 1) assert_array_almost_equal(world, [[285.0, -66.25]], decimal=1) pix = wcs.wcs_sky2pix([[285.0, -66.25]], 1) assert_array_almost_equal(pix, [[97, 97]], decimal=0) # get the list of the hdr files that we want to test hdr_file_list = [ x for x in glob.glob(os.path.join(ROOT_DIR, "maps", "*.hdr")) ] # actually perform a test for each one for filename in hdr_file_list : # use the base name of the file, because everything we yield # will show up in the test name in the pandokia report filename = os.path.basename( filename ) # yield a function name and parameters to make a generated test yield test_map, filename # AFTER we tested with every file that we found, check to see that we # actually have the list we expect. If N=0, we will not have performed # any tests at all. If N < n_data_files, we are missing some files, # so we will have skipped some tests. Without this check, both cases # happen silently! # how many do we expect to see? n_data_files = 28 if len(hdr_file_list) != n_data_files : assert False, ( "test_maps has wrong number data files: found %d, expected " " %d, looking in %s" % ( len(hdr_file_list), n_data_files, ROOT_DIR ) ) # b.t.w. If this assert happens, nose reports one more test # than it would have otherwise. # test_spectra() is a generator def test_spectra(): # test_spectrum() is the function that is called to perform the generated test def test_spectrum(filename): # the test parameter is the base name of the file to use; find # the file in the installed pywcs test directory filename = os.path.join(ROOT_DIR, "spectra", filename) fd = open(filename, 'rb') header = fd.read() fd.close() wcs = pywcs.WCS(header) all = pywcs.find_all_wcs(header) assert len(all) == 9 # get the list of the hdr files that we want to test hdr_file_list = [ x for x in glob.glob(os.path.join(ROOT_DIR, "spectra", "*.hdr")) ] # actually perform a test for each one for filename in hdr_file_list : # use the base name of the file, because everything we yield # will show up in the test name in the pandokia report filename = os.path.basename( filename ) # yield a function name and parameters to make a generated test yield test_spectrum, filename # AFTER we tested with every file that we found, check to see that we # actually have the list we expect. If N=0, we will not have performed # any tests at all. If N < n_data_files, we are missing some files, # so we will have skipped some tests. Without this check, both cases # happen silently! # how many do we expect to see? n_data_files = 6 if len(hdr_file_list) != n_data_files : assert False, ( "test_spectra has wrong number data files: found %d, expected " " %d, looking in %s" % ( len(hdr_file_list), n_data_files, ROOT_DIR ) ) # b.t.w. If this assert happens, nose reports one more test # than it would have otherwise. # test_nraos() is a generator def test_nrao(): # test_nrao() is the function that is called to perform the generated test def test_nrao_file(filename): # the test parameter is the base name of the file to use; find # the file in the installed pywcs test directory filename = os.path.join(ROOT_DIR, "nrao", filename) fd = open(filename, 'rb') header = fd.read() fd.close() wcs = pywcs.WCS(header) wcs.wcs.set() # get the list of the hdr files that we want to test hdr_file_list = [ x for x in glob.glob(os.path.join(ROOT_DIR, "nrao", "*.hdr")) ] # actually perform a test for each one for filename in hdr_file_list : # use the base name of the file, because everything we yield # will show up in the test name in the pandokia report filename = os.path.basename( filename ) # yield a function name and parameters to make a generated test yield test_nrao_file, filename # AFTER we tested with every file that we found, check to see that we # actually have the list we expect. If N=0, we will not have performed # any tests at all. If N < n_data_files, we are missing some files, # so we will have skipped some tests. Without this check, both cases # happen silently! # how many do we expect to see? n_data_files = 6 if len(hdr_file_list) != n_data_files : assert False, ( "test_nraos has wrong number data files: found %d, expected " " %d, looking in %s" % ( len(hdr_file_list), n_data_files, ROOT_DIR ) ) # b.t.w. If this assert happens, nose reports one more test # than it would have otherwise. def test_units(): u = pywcs.UnitConverter("log(MHz)", "ln(Hz)") print(u.convert([1,2,3,4])) basic_units = "m s g rad sr K A mol cd".split() derived_units = "Hz J W V N Pa C Ohm ohm S F Wb T H lm lx".split() add_all_units = "eV Jy R G barn".split() add_sup_units = "a yr pc bit byte Byte".split() add_sub_units = "mag".split() general_units = "deg arcmin arcsec mas d h min erg Ry u D DEGREE DEGREES".split() astro_units = "Angstrom angstrom AU lyr beam solRad solMass solLum Sun".split() device_units = "adu bin chan count ct photon ph pixel pix voxel".split() sub_prefixes = "y z a f p n u m c d".split() sup_prefixes = "da h k M G T P E Z Y".split() def test_all_units(): def test_self(x): # x appears in the test name. If we would have had an ambiguous # test name, we had -xxx added to the unit name. Remove it if # necessary. if '-' in x : x = x.split('-')[0] # here is the test: try: u = pywcs.UnitConverter(x, x) except ValueError: e = sys.exc_info()[1] if str(e).startswith("ERROR 12 in wcsutrne") and \ x in ("S", "H", "D"): return else: raise assert u.scale == 1.0 assert u.offset == 0.0 assert u.power == 1.0 # list of all the units to test all = sorted(basic_units + derived_units + add_all_units + add_sup_units + add_sub_units + general_units + astro_units + device_units) # Pandokia has non-case-sensitve test names; since the unit name is # showing up in the test name, we want to disambiguate any name collisions. # Here is a list of all the lower-cased unit name names. all_lower = [ x.lower() for x in all ] # here are serial numbers to use to disambiguate unique_tags = { } for unit in all : # disambiguate the test name, if necessary l_unit = unit.lower() if unit != l_unit and l_unit in all_lower : n = unique_tags.get(l_unit, 1) unique_tags[n] = n + 1 # the test will tear off the part after the '-' unit = '%s-%d' % ( unit, n) # perform the test yield test_self, unit def test_unit_prefixes(): def test_self(x, p): unit = p + x try: u = pywcs.UnitConverter(unit, unit) except ValueError: e = sys.exc_info()[1] if str(e) == "Potentially unsafe translation" and \ x in ("S", "H", "D"): return else: raise assert u.scale == 1.0 assert u.offset == 0.0 assert u.power == 1.0 for unit in (basic_units + derived_units + add_all_units): for prefix in (sub_prefixes + sup_prefixes): yield test_self, unit, prefix for unit in add_sup_units: for prefix in sup_prefixes: yield test_self, unit, prefix for unit in add_sub_units: for prefix in sub_prefixes: yield test_self, unit, prefix def test_outside_sky(): """ From github issue #107 """ filename = os.path.join(ROOT_DIR, "data", "outside_sky.hdr") fd = open(filename, 'rb') header = fd.read() fd.close() w = pywcs.WCS(header) assert np.all(np.isnan(w.wcs_pix2sky([[100.,500.]], 0))) # outside sky assert np.all(np.isnan(w.wcs_pix2sky([[200.,200.]], 0))) # outside sky assert not np.any(np.isnan(w.wcs_pix2sky([[1000.,1000.]], 0))) pywcs-1.12/lib/pywcs/tests/test_pickle.py0000644001153600020070000000515512310355627022612 0ustar cslocumSTSCI\science00000000000000# TODO: Test that this works for subclasses import os try: import cPickle as pickle except ImportError: import pickle import numpy as np from numpy.testing import assert_array_almost_equal import pywcs ROOT_DIR = None def setup(): global ROOT_DIR ROOT_DIR = os.path.join(os.path.dirname(pywcs.__file__), "tests") def test_basic(): wcs = pywcs.WCS() s = pickle.dumps(wcs) wcs2 = pickle.loads(s) def test_dist(): try: import pyfits except ImportError: pass hdulist = pyfits.open(os.path.join(ROOT_DIR, "data", "dist.fits")) wcs1 = pywcs.WCS(hdulist[0].header, hdulist) assert wcs1.det2im2 is not None s = pickle.dumps(wcs1) wcs2 = pickle.loads(s) x = np.random.rand(2 ** 16, wcs1.wcs.naxis) world1 = wcs1.all_pix2sky(x, 1) world2 = wcs2.all_pix2sky(x, 1) assert_array_almost_equal(world1, world2) def test_sip(): try: import pyfits except ImportError: pass hdulist = pyfits.open(os.path.join(ROOT_DIR, "data", "sip.fits"), ignore_missing_end=True) wcs1 = pywcs.WCS(hdulist[0].header) assert wcs1.sip is not None s = pickle.dumps(wcs1) wcs2 = pickle.loads(s) x = np.random.rand(2 ** 16, wcs1.wcs.naxis) world1 = wcs1.all_pix2sky(x, 1) world2 = wcs2.all_pix2sky(x, 1) assert_array_almost_equal(world1, world2) def test_sip2(): try: import pyfits except ImportError: pass hdulist = pyfits.open(os.path.join(ROOT_DIR, "data", "sip2.fits"), ignore_missing_end=True) wcs1 = pywcs.WCS(hdulist[0].header) assert wcs1.sip is not None s = pickle.dumps(wcs1) wcs2 = pickle.loads(s) x = np.random.rand(2 ** 16, wcs1.wcs.naxis) world1 = wcs1.all_pix2sky(x, 1) world2 = wcs2.all_pix2sky(x, 1) assert_array_almost_equal(world1, world2) def test_wcs(): try: import pyfits except ImportError: pass filename = os.path.join(ROOT_DIR, "data", "outside_sky.hdr") fd = open(filename, 'rb') header = fd.read() fd.close() wcs1 = pywcs.WCS(header) s = pickle.dumps(wcs1) wcs2 = pickle.loads(s) x = np.random.rand(2 ** 16, wcs1.wcs.naxis) world1 = wcs1.all_pix2sky(x, 1) world2 = wcs2.all_pix2sky(x, 1) assert_array_almost_equal(world1, world2) class Sub(pywcs.WCS): def __init__(self, *args, **kwargs): self.foo = 42 def test_subclass(): wcs = Sub() s = pickle.dumps(wcs) wcs2 = pickle.loads(s) assert isinstance(wcs2, Sub) assert wcs.foo == 42 assert wcs2.foo == 42 assert wcs2.wcs is not None pywcs-1.12/lib/pywcs/tests/test_profiling.py0000644001153600020070000000723412310355627023334 0ustar cslocumSTSCI\science00000000000000import glob import os import sys import numpy as np from numpy.testing import assert_array_almost_equal import pywcs ROOT_DIR = None def setup(): global ROOT_DIR # do not use __file__ here - we want to find the data files that # belong to the pywcs that we are testing, even if we are not running # this test from the installed copy of this file. Use pywcs.__file__ ROOT_DIR = os.path.join(os.path.dirname(pywcs.__file__), 'tests') def test_maps(): def test_map(filename): filename = os.path.join(ROOT_DIR, "maps", filename) fd = open(filename, 'rb') header = fd.read() fd.close() wcs = pywcs.WCS(header) x = np.random.rand(2 ** 16, wcs.wcs.naxis) world = wcs.wcs_pix2sky(x, 1) pix = wcs.wcs_sky2pix(x, 1) # get the list of the hdr files that we want to test hdr_file_list = [ x for x in glob.glob(os.path.join(ROOT_DIR, "maps", "*.hdr")) ] # actually perform a test for each one for filename in hdr_file_list : # use the base name of the file, because everything we yield # will show up in the test name in the pandokia report filename = os.path.basename( filename ) # yield a function name and parameters to make a generated test yield test_map, filename # AFTER we tested with every file that we found, check to see that we # actually have the list we expect. If N=0, we will not have performed # any tests at all. If N < n_data_files, we are missing some files, # so we will have skipped some tests. Without this check, both cases # happen silently! # how many do we expect to see? n_data_files = 28 if len(hdr_file_list) != n_data_files : assert False, ( "test_maps has wrong number data files: found %d, expected " " %d, looking in %s" % ( len(hdr_file_list), n_data_files, ROOT_DIR ) ) # b.t.w. If this assert happens, nose reports one more test # than it would have otherwise. def test_spectra(): def test_spectrum(filename): filename = os.path.join(ROOT_DIR, "spectra", filename) fd = open(filename, 'rb') header = fd.read() fd.close() wcs = pywcs.WCS(header) x = np.random.rand(2 ** 16, wcs.wcs.naxis) world = wcs.wcs_pix2sky(x, 1) pix = wcs.wcs_sky2pix(x, 1) # get the list of the hdr files that we want to test hdr_file_list = [ x for x in glob.glob(os.path.join(ROOT_DIR, "spectra", "*.hdr")) ] # actually perform a test for each one for filename in hdr_file_list : # use the base name of the file, because everything we yield # will show up in the test name in the pandokia report filename = os.path.basename( filename ) # yield a function name and parameters to make a generated test yield test_spectrum, filename # AFTER we tested with every file that we found, check to see that we # actually have the list we expect. If N=0, we will not have performed # any tests at all. If N < n_data_files, we are missing some files, # so we will have skipped some tests. Without this check, both cases # happen silently! # how many do we expect to see? n_data_files = 6 if len(hdr_file_list) != n_data_files : assert False, ( "test_spectra has wrong number data files: found %d, expected " " %d, looking in %s" % ( len(hdr_file_list), n_data_files, ROOT_DIR ) ) # b.t.w. If this assert happens, nose reports one more test # than it would have otherwise. pywcs-1.12/lib/pywcs/tests/test_wcsprm.py0000644001153600020070000003240212310355627022651 0ustar cslocumSTSCI\science00000000000000import os import sys from nose.tools import raises from numpy.testing import assert_array_equal import numpy as np import pywcs from pywcs import _pywcs def b(s): return s.encode('ascii') ###################################################################### ROOT_DIR = None def setup(): global ROOT_DIR ROOT_DIR = os.path.join(os.path.dirname(pywcs.__file__), "tests") def test_alt(): w = _pywcs._Wcsprm() assert w.alt == b(" ") w.alt = b("X") assert w.alt == b("X") del w.alt assert w.alt == b(" ") @raises(ValueError) def test_alt_invalid1(): w = _pywcs._Wcsprm() w.alt = b("$") @raises(ValueError) def test_alt_invalid2(): w = _pywcs._Wcsprm() w.alt = b(" ") def test_axis_types(): w = _pywcs._Wcsprm() assert_array_equal(w.axis_types, [0, 0]) def test_cd(): w = _pywcs._Wcsprm() w.cd = [[1, 0], [0, 1]] assert w.cd.dtype == np.float assert w.has_cd() == True assert_array_equal(w.cd, [[1, 0], [0, 1]]) del w.cd assert w.has_cd() == False @raises(AttributeError) def test_cd_missing(): w = _pywcs._Wcsprm() assert w.has_cd() == False w.cd @raises(AttributeError) def test_cd_missing2(): w = _pywcs._Wcsprm() w.cd = [[1, 0], [0, 1]] assert w.has_cd() == True del w.cd assert w.has_cd() == False w.cd @raises(ValueError) def test_cd_invalid(): w = _pywcs._Wcsprm() w.cd = [1, 0, 0, 1] def test_cdelt(): w = _pywcs._Wcsprm() assert_array_equal(w.cdelt, [1, 1]) w.cdelt = [42, 54] assert_array_equal(w.cdelt, [42, 54]) @raises(TypeError) def test_cdelt_delete(): w = _pywcs._Wcsprm() del w.cdelt def test_cel_offset(): w = _pywcs._Wcsprm() assert w.cel_offset is False w.cel_offset = 'foo' assert w.cel_offset is True w.cel_offset = 0 assert w.cel_offset is False def test_celfix(): # TODO: We need some data with -NCP or -GLS projections to test # with. For now, this is just a smoke test w = _pywcs._Wcsprm() assert w.celfix() == -1 def test_cname(): w = _pywcs._Wcsprm() # Test that this works as an iterator for x in w.cname: assert x == b('') assert list(w.cname) == [b(''), b('')] w.cname = [b('foo'), b('bar')] assert list(w.cname) == [b('foo'), b('bar')] @raises(TypeError) def test_cname_invalid(): w = _pywcs._Wcsprm() w.cname = [42, 54] def test_colax(): w = _pywcs._Wcsprm() assert w.colax.dtype == np.intc assert_array_equal(w.colax, [0, 0]) w.colax = [42, 54] assert_array_equal(w.colax, [42, 54]) w.colax[0] = 0 assert_array_equal(w.colax, [0, 54]) def test_colnum(): w = _pywcs._Wcsprm() assert w.colnum == 0 w.colnum = 42 assert w.colnum == 42 @raises(TypeError) def test_colnum_invalid(): w = _pywcs._Wcsprm() w.colnum = 'foo' def test_crder(): w = _pywcs._Wcsprm() assert w.crder.dtype == np.float assert np.all(np.isnan(w.crder)) w.crder[0] = 0 assert np.isnan(w.crder[1]) assert w.crder[0] == 0 def test_crota(): w = _pywcs._Wcsprm() w.crota = [1, 0] assert w.crota.dtype == np.float assert w.has_crota() == True assert_array_equal(w.crota, [1, 0]) del w.crota assert w.has_crota() == False @raises(AttributeError) def test_crota_missing(): w = _pywcs._Wcsprm() assert w.has_crota() == False w.crota @raises(AttributeError) def test_crota_missing2(): w = _pywcs._Wcsprm() w.crota = [1, 0] assert w.has_crota() == True del w.crota assert w.has_crota() == False w.crota def test_crpix(): w = _pywcs._Wcsprm() assert w.crpix.dtype == np.float assert_array_equal(w.crpix, [0, 0]) w.crpix = [42, 54] assert_array_equal(w.crpix, [42, 54]) w.crpix[0] = 0 assert_array_equal(w.crpix, [0, 54]) def test_crval(): w = _pywcs._Wcsprm() assert w.crval.dtype == np.float assert_array_equal(w.crval, [0, 0]) w.crval = [42, 54] assert_array_equal(w.crval, [42, 54]) w.crval[0] = 0 assert_array_equal(w.crval, [0, 54]) def test_csyer(): w = _pywcs._Wcsprm() assert w.crder.dtype == np.float assert np.all(np.isnan(w.crder)) w.crder[0] = 0 assert np.isnan(w.crder[1]) assert w.crder[0] == 0 def test_ctype(): w = _pywcs._Wcsprm() assert list(w.ctype) == [b(''), b('')] w.ctype = [b('RA---TAN'), b('DEC--TAN')] assert_array_equal(w.axis_types, [2200, 2201]) assert w.lat == 1 assert w.lng == 0 assert w.lattyp == b('DEC') assert w.lngtyp == b('RA') assert list(w.ctype) == [b('RA---TAN'), b('DEC--TAN')] w.ctype = [b('foo'), b('bar')] assert_array_equal(w.axis_types, [0, 0]) assert list(w.ctype) == [b('foo'), b('bar')] assert w.lat == -1 assert w.lng == -1 assert w.lattyp == b('DEC') assert w.lngtyp == b('RA') def test_cubeface(): w = _pywcs._Wcsprm() assert w.cubeface == -1 def test_cunit(): w = _pywcs._Wcsprm() assert list(w.cunit) == [b(''), b('')] w.cunit = [b('m'), b('km')] @raises(ValueError) def test_cunit_invalid(): w = _pywcs._Wcsprm() w.cunit[0] = b('foo') @raises(ValueError) def test_cunit_invalid2(): w = _pywcs._Wcsprm() w.cunit = [b('foo'), b('bar')] def test_cylfix(): # TODO: We need some data with broken cylindrical projections to # test with. For now, this is just a smoke test. w = _pywcs._Wcsprm() assert w.cylfix() == -1 def test_dateavg(): w = _pywcs._Wcsprm() assert w.dateavg == b('') # TODO: When dateavg is verified, check that it works def test_dateobs(): w = _pywcs._Wcsprm() assert w.dateobs == b('') # TODO: When dateavg is verified, check that it works def test_datfix(): w = _pywcs._Wcsprm() w.dateobs = b('31/12/99') status = w.datfix() assert status == 0 assert w.dateobs == b('1999-12-31') assert w.mjdobs == 51543.0 def test_equinox(): w = _pywcs._Wcsprm() assert np.isnan(w.equinox) w.equinox = 0 assert w.equinox == 0 del w.equinox assert np.isnan(w.equinox) def test_fix(): w = _pywcs._Wcsprm() assert w.fix() == { 'cylfix': 'No change', 'datfix': 'No change', 'spcfix': 'No change', 'unitfix':'No change', 'celfix': 'No change'} def test_fix2(): w = _pywcs._Wcsprm() w.dateobs = b('31/12/99') status = w.fix() assert status == { 'cylfix': 'No change', 'datfix': "Changed '31/12/99' to '1999-12-31'", 'spcfix': 'No change', 'unitfix': 'No change', 'celfix': 'No change'} assert w.dateobs == b('1999-12-31') assert w.mjdobs == 51543.0 def test_fix3(): w = _pywcs._Wcsprm() w.dateobs = b('31/12/F9') assert w.fix() == { 'cylfix': 'No change', 'datfix': "Invalid parameter value: invalid date '31/12/F9'", 'spcfix': 'No change', 'unitfix':'No change', 'celfix': 'No change'} assert w.dateobs == b('31/12/F9') assert np.isnan(w.mjdobs) def test_get_ps(): # TODO: We need some data with PSi_ma keywords w = _pywcs._Wcsprm() assert len(w.get_ps()) == 0 def test_get_pv(): # TODO: We need some data with PVi_ma keywords w = _pywcs._Wcsprm() assert len(w.get_pv()) == 0 @raises(AssertionError) def test_imgpix_matrix(): w = _pywcs._Wcsprm() w.imgpix_matrix @raises(AttributeError) def test_imgpix_matrix(): w = _pywcs._Wcsprm() w.imgpix_matrix = None def test_isunity(): w = _pywcs._Wcsprm() assert(w.is_unity()) def test_lat(): w = _pywcs._Wcsprm() assert w.lat == -1 @raises(AttributeError) def test_lat_set(): w = _pywcs._Wcsprm() w.lat = 0 def test_latpole(): w = _pywcs._Wcsprm() assert w.latpole == 90.0 w.latpole = 45.0 assert w.latpole == 45.0 del w.latpole assert w.latpole == 90.0 def test_lattyp(): w = _pywcs._Wcsprm() print(repr(w.lattyp)) assert w.lattyp == b(" ") @raises(AttributeError) def test_lattyp_set(): w = _pywcs._Wcsprm() w.lattyp = 0 def test_lng(): w = _pywcs._Wcsprm() assert w.lng == -1 @raises(AttributeError) def test_lng_set(): w = _pywcs._Wcsprm() w.lng = 0 def test_lngtyp(): w = _pywcs._Wcsprm() assert w.lngtyp == b(" ") @raises(AttributeError) def test_lngtyp_set(): w = _pywcs._Wcsprm() w.lngtyp = 0 def test_lonpole(): w = _pywcs._Wcsprm() assert np.isnan(w.lonpole) w.lonpole = 45.0 assert w.lonpole == 45.0 del w.lonpole assert np.isnan(w.lonpole) def test_mjdavg(): w = _pywcs._Wcsprm() assert np.isnan(w.mjdavg) w.mjdavg = 45.0 assert w.mjdavg == 45.0 del w.mjdavg assert np.isnan(w.mjdavg) def test_mjdobs(): w = _pywcs._Wcsprm() assert np.isnan(w.mjdobs) w.mjdobs = 45.0 assert w.mjdobs == 45.0 del w.mjdobs assert np.isnan(w.mjdobs) def test_name(): w = _pywcs._Wcsprm() assert w.name == b('') w.name = b('foo') assert w.name == b('foo') def test_naxis(): w = _pywcs._Wcsprm() assert w.naxis == 2 @raises(AttributeError) def test_naxis_set(): w = _pywcs._Wcsprm() w.naxis = 4 def test_obsgeo(): w = _pywcs._Wcsprm() assert np.all(np.isnan(w.obsgeo)) w.obsgeo = [1,2,3] assert_array_equal(w.obsgeo, [1,2,3]) del w.obsgeo assert np.all(np.isnan(w.obsgeo)) def test_pc(): w = _pywcs._Wcsprm() assert w.has_pc() assert_array_equal(w.pc, [[1, 0], [0, 1]]) w.cd = [[1, 0], [0, 1]] assert not w.has_pc() del w.cd assert w.has_pc() assert_array_equal(w.pc, [[1, 0], [0, 1]]) @raises(AttributeError) def test_pc_missing(): w = _pywcs._Wcsprm() w.cd = [[1, 0], [0, 1]] assert not w.has_pc() w.pc def test_phi0(): w = _pywcs._Wcsprm() assert np.isnan(w.phi0) w.phi0 = 42.0 assert w.phi0 == 42.0 del w.phi0 assert np.isnan(w.phi0) @raises(AssertionError) def test_piximg_matrix(): w = _pywcs._Wcsprm() w.piximg_matrix @raises(AttributeError) def test_piximg_matrix(): w = _pywcs._Wcsprm() w.piximg_matrix = None def test_print_contents(): # In general, this is human-consumable, so we don't care if the # content changes, just check the type w = _pywcs._Wcsprm() assert isinstance(str(w), str) def test_radesys(): w = _pywcs._Wcsprm() assert w.radesys == b('') w.radesys = b('foo') assert w.radesys == b('foo') def test_restfrq(): w = _pywcs._Wcsprm() assert w.restfrq == 0.0 w.restfrq = np.nan assert np.isnan(w.restfrq) def test_restwav(): w = _pywcs._Wcsprm() assert w.restwav == 0.0 w.restwav = np.nan assert np.isnan(w.restwav) def test_set_ps(): w = _pywcs._Wcsprm() data = [(0, 0, "param1"), (1, 1, "param2")] w.set_ps(data) assert w.get_ps() == data def test_set_ps_realloc(): w = _pywcs._Wcsprm() w.set_ps([(0, 0, "param1")] * 16) def test_set_pv(): w = _pywcs._Wcsprm() data = [(0, 0, 42.), (1, 1, 54.)] w.set_pv(data) assert w.get_pv() == data def test_set_pv_realloc(): w = _pywcs._Wcsprm() w.set_pv([(0, 0, 42.)] * 16) def test_spcfix(): # TODO: We need some data with broken spectral headers here to # really test header = open(os.path.join(ROOT_DIR, 'spectra', 'orion-velo-1.hdr'), 'rb').read() w = _pywcs._Wcsprm(header) assert w.spcfix() == -1 def test_spec(): w = _pywcs._Wcsprm() assert w.spec == -1 @raises(AttributeError) def test_spec_set(): w = _pywcs._Wcsprm() w.spec = 0 def test_specsys(): w = _pywcs._Wcsprm() assert w.specsys == b('') w.specsys = b('foo') assert w.specsys == b('foo') def test_sptr(): #TODO: Write me pass def test_ssysobs(): w = _pywcs._Wcsprm() assert w.ssysobs == b('') w.ssysobs = b('foo') assert w.ssysobs == b('foo') def test_ssyssrc(): w = _pywcs._Wcsprm() assert w.ssyssrc == b('') w.ssyssrc = b('foo') assert w.ssyssrc == b('foo') def test_tab(): w = _pywcs._Wcsprm() assert len(w.tab) == 0 # TODO: Inject some headers that have tables and test def test_theta0(): w = _pywcs._Wcsprm() assert np.isnan(w.theta0) w.theta0 = 42.0 assert w.theta0 == 42.0 del w.theta0 assert np.isnan(w.theta0) def test_toheader(): w = _pywcs._Wcsprm() if sys.version_info[0] >= 3: assert isinstance(w.to_header(), bytes) else: assert isinstance(w.to_header(), str) def test_velangl(): w = _pywcs._Wcsprm() assert w.velangl == 0.0 w.velangl = 42.0 assert w.velangl == 42.0 del w.velangl assert np.isnan(w.velangl) def test_velosys(): w = _pywcs._Wcsprm() assert np.isnan(w.velosys) w.velosys = 42.0 assert w.velosys == 42.0 del w.velosys assert np.isnan(w.velosys) def test_zsource(): w = _pywcs._Wcsprm() assert np.isnan(w.zsource) w.zsource = 42.0 assert w.zsource == 42.0 del w.zsource assert np.isnan(w.zsource) def test_cd_3d(): header = open(os.path.join(ROOT_DIR, 'data', '3d_cd.hdr'), 'rb').read() w = _pywcs._Wcsprm(header) assert w.cd.shape == (3, 3) assert w.get_pc().shape == (3, 3) assert w.get_cdelt().shape == (3,) @raises(RuntimeError) def test_get_pc(): header = open(os.path.join(ROOT_DIR, 'data', '3d_cd.hdr'), 'rb').read() w = _pywcs._Wcsprm(header) w.get_pc()[0,0] = 42 @raises(_pywcs.SingularMatrixError) def test_detailed_err(): w = _pywcs._Wcsprm() w.pc = [[0,0],[0,0]] w.set() pywcs-1.12/lib/pywcs/version.py0000644001153600020070000000613012310355730020614 0ustar cslocumSTSCI\science00000000000000"""This is an automatically generated file created by stsci.distutils.hooks.version_setup_hook. Do not modify this file by hand. """ __all__ = ['__version__', '__vdate__', '__svn_revision__', '__svn_full_info__', '__setup_datetime__'] import datetime __version__ = '1.12' __vdate__ = 'unspecified' __svn_revision__ = '3949:3950' __svn_full_info__ = 'Path: pywcs\nURL: https://aeon.stsci.edu/ssb/svn/astrolib/tags/release_1.12/pywcs\nRepository Root: https://aeon.stsci.edu/ssb/svn/astrolib\nRepository UUID: 90a0a646-be8a-0410-bb88-9290da87bc01\nRevision: 3949\nNode Kind: directory\nSchedule: normal\nLast Changed Author: cslocum\nLast Changed Rev: 3945\nLast Changed Date: 2014-03-13 12:16:54 -0400 (Thu, 13 Mar 2014)' __setup_datetime__ = datetime.datetime(2014, 3, 13, 12, 24, 56, 925642) # what version of stsci.distutils created this version.py stsci_distutils_version = '0.3.7' if '.dev' in __version__: def update_svn_info(): """Update the SVN info if running out of an SVN working copy.""" import os import string import subprocess global __svn_revision__ global __svn_full_info__ path = os.path.abspath(os.path.dirname(__file__)) run_svnversion = True try: pipe = subprocess.Popen(['svn', 'info', path], stdout=subprocess.PIPE, stderr=subprocess.PIPE) stdout, _ = pipe.communicate() if pipe.returncode == 0: lines = [] for line in stdout.splitlines(): line = line.decode('latin1').strip() if not line: continue lines.append(line) if not lines: __svn_full_info__ = ['unknown'] else: __svn_full_info__ = lines else: run_svnversion = False except OSError: run_svnversion = False if run_svnversion: # If updating the __svn_full_info__ succeeded then use its output # to find the base of the working copy and use svnversion to get # the svn revision. for line in __svn_full_info__: if line.startswith('Working Copy Root Path'): path = line.split(':', 1)[1].strip() break try: pipe = subprocess.Popen(['svnversion', path], stdout=subprocess.PIPE, stderr=subprocess.PIPE) stdout, _ = pipe.communicate() if pipe.returncode == 0: stdout = stdout.decode('latin1').strip() if stdout and stdout[0] in string.digits: __svn_revision__ = stdout except OSError: pass # Convert __svn_full_info__ back to a string if isinstance(__svn_full_info__, list): __svn_full_info__ = '\n'.join(__svn_full_info__) update_svn_info() del update_svn_info pywcs-1.12/lib/pywcs.egg-info/0000755001153600020070000000000012310355732020251 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/lib/pywcs.egg-info/dependency_links.txt0000644001153600020070000000000112310355731024316 0ustar cslocumSTSCI\science00000000000000 pywcs-1.12/lib/pywcs.egg-info/not-zip-safe0000644001153600020070000000000112310355701022473 0ustar cslocumSTSCI\science00000000000000 pywcs-1.12/lib/pywcs.egg-info/PKG-INFO0000644001153600020070000001316712310355731021355 0ustar cslocumSTSCI\science00000000000000Metadata-Version: 1.1 Name: pywcs Version: 1.12 Summary: Python wrappers to WCSLIB Home-page: http://www.scipy.org/AstroLib Author: Michael Droettboom Author-email: mdroe@stsci.edu License: UNKNOWN Description: Introduction ------------ pywcs is a set of routines for handling the FITS World Coordinate System (WCS) standard. It is a thin wrapper around the high- and mid-level interfaces of Dr. Mark Calabretta's WCSLIB available here: http://www.atnf.csiro.au/people/mcalabre/WCS/ In addition, there are extensions (written in C) to support Spitzer Simple Imaging Polynomial (SIP) convention keywords and Paper IV table lookup distortion. Please direct any questions to: help@stsci.edu Build instructions ------------------ pywcs includes its own copy of WCSLIB. pywcs requires: - Numpy 1.3 or later - pyfits 1.4 or later pywcs uses the standard Python distutils system to build and install itself. From the command line run:: python setup.py install to install pywcs. Building documentation ---------------------- Optionally, the documentation can be built using Sphinx (http://sphinx.pocoo.org). After installing pywcs, 'cd' into the 'doc' directory and:: make html The documentation is also available online at: http://stsdas.stsci.edu/astrolib/pywcs/index.html Version 1.11 ============ NEW FEATURES: - Updated to wcslib version 4.8.2, which gives much more detailed error messages. Exceptions raised due to invalid WCS keywords should now be more informative. - Undefined values that are the result of p2s and s2p are now set to NaN. Previously, one had to examine the stat result vector to determine which results were invalid. - Added functions get_pc() and get_cdelt(). These provide a way to always get the canonical representation of the linear transformation matrix, whether the header specified it in PC, CD or CROTA form. BROADER COMPATIBILITY: - Supports Python 3.x - Long-running process will now release the Python GIL to better support Python multithreading. - Builds on Microsoft Windows using mingw32, mingw64 and Visual Studio 9.0 and 10.0 without severely patching wcslib. - pywcs will now run without pyfits, though the SIP and distortion lookup table functionality is unavailable. BUG FIXES: - The dimensions of the cd and pc matrices were formerly always returned as 2x2. They now are sized according to naxis. MISCELLANEOUS: - Lots of new unit tests - Setting wcs.wcs.cunit will now verify that the values are valid unit strings. Version 1.10 ============ - Adds a UnitConversion class, which gives access to wcslib's unit conversion functionality. Given two convertible unit strings, pywcs can convert arrays of values from one to the other. - Now uses wcslib 4.7 - Changes to some wcs values would not always calculate secondary values. Version 1.9 =========== - Support binary image arrays and pixel list format WCS by presenting a way to call wcslib's wcsbth() - Updated underlying wcslib to version 4.5, which fixes the following: - Fixed the interpretation of VELREF when translating AIPS-convention spectral types. Such translation is now handled by a new special- purpose function, spcaips(). The wcsprm struct has been augmented with an entry for velref which is filled by wcspih() and wcsbth(). Previously, selection by VELREF of the radio or optical velocity convention for type VELO was not properly handled. BUGS: - The "pc" member is now available with a default "raw" Wcsprm object. - Make properties that return arrays read-only, since modifying a (mutable) array could result in secondary values not being recomputed based on those changes. - float properties can now be set using int values Version 1.3a1 ============= Earlier versions of pywcs had two versions of every conversion method: X(...) -- treats the origin of pixel coordinates at (0, 0) X_fits(...) -- treats the origin of pixel coordinates at (1, 1) From version 1.3 onwards, there is only one method for each conversion, with an 'origin' argument: - 0: places the origin at (0, 0), which is the C/Numpy convention. - 1: places the origin at (1, 1), which is the Fortran/FITS convention. Platform: UNKNOWN Classifier: Intended Audience :: Science/Research Classifier: License :: OSI Approved :: BSD License Classifier: Operating System :: OS Independent Classifier: Programming Language :: Python Classifier: Topic :: Scientific/Engineering :: Astronomy Classifier: Topic :: Software Development :: Libraries :: Python Modules pywcs-1.12/lib/pywcs.egg-info/requires.txt0000644001153600020070000000003212310355731022643 0ustar cslocumSTSCI\science00000000000000pyfits>=2.4.0 numpy>=1.5.1pywcs-1.12/lib/pywcs.egg-info/SOURCES.txt0000644001153600020070000003323712310355732022145 0ustar cslocumSTSCI\science00000000000000CHANGELOG LICENSE MANIFEST.in README defsetup.py distribute_setup.py hooks.py patch_wcslib.sh setup.cfg setup.py stsci_distutils_hack.py doc/Makefile doc/docstrings.py doc/make.bat doc/source/api.rst doc/source/api_distortion.rst doc/source/api_sip.rst doc/source/api_units.rst doc/source/api_wcs.rst doc/source/api_wcsprm.rst doc/source/conf.py doc/source/examples doc/source/examples.rst doc/source/index.rst doc/source/references.rst doc/source/relax.rst examples/from_file.py examples/programmatic.py lib/pywcs_setup.py lib/pywcs/__init__.py lib/pywcs/_docutil.py lib/pywcs/core.py lib/pywcs/hooks.py lib/pywcs/version.py lib/pywcs.egg-info/PKG-INFO lib/pywcs.egg-info/SOURCES.txt lib/pywcs.egg-info/dependency_links.txt lib/pywcs.egg-info/not-zip-safe lib/pywcs.egg-info/requires.txt lib/pywcs.egg-info/top_level.txt lib/pywcs/tests/__init__.py lib/pywcs/tests/test.py lib/pywcs/tests/test_pickle.py lib/pywcs/tests/test_profiling.py lib/pywcs/tests/test_wcsprm.py lib/pywcs/tests/data/3d_cd.hdr lib/pywcs/tests/data/dist.fits lib/pywcs/tests/data/outside_sky.hdr lib/pywcs/tests/data/sip.fits lib/pywcs/tests/data/sip2.fits lib/pywcs/tests/maps/1904-66_AIR.hdr lib/pywcs/tests/maps/1904-66_AIT.hdr lib/pywcs/tests/maps/1904-66_ARC.hdr lib/pywcs/tests/maps/1904-66_AZP.hdr lib/pywcs/tests/maps/1904-66_BON.hdr lib/pywcs/tests/maps/1904-66_CAR.hdr 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pywcs-1.12/lib/pywcs_setup.py0000644001153600020070000003001112310355627020347 0ustar cslocumSTSCI\science00000000000000from __future__ import with_statement, division import glob import os import shutil import sys import textwrap from distutils.dist import Distribution from stsci.distutils.hooks import is_display_option if sys.version_info[0] >= 3: def b(s): return s.encode('ascii') def string_escape(s): s = s.decode('ascii').encode('ascii', 'backslashreplace') s = s.replace(b('\n'), b('\\n')) return s.decode('ascii') from io import StringIO else: def string_escape(s): return s.encode('string_escape') from cStringIO import StringIO # BUILD should be 'debug', 'profile' or 'release' # TODO: How often is this actually mucked with? Would it be worth adding a # custom command that adds a command-line option for this? BUILD = 'release' OPENMP = False def setup_hook(config): if is_display_option(): return WCSLIB_VERSION = config['metadata']['stsci_wcs_version'].strip() # Ensure that headers are copied to the correct location for installation # purposes if 'packages_root' in config['files']: root = config['files']['packages_root'] else: root = '' include_dir = os.path.join(root, 'pywcs', 'include') wcslib_include_dir = os.path.join(include_dir, 'wcslib') for d in [include_dir, wcslib_include_dir]: if not os.path.exists(d): os.mkdir(d) for header in glob.glob(os.path.join('src', '*.h')): shutil.copy2(header, include_dir) for header in glob.glob(os.path.join('wcslib', 'C', '*.h')): shutil.copy2(header, wcslib_include_dir) # WCSLIB CONFIGURATION wcsconfig_h = StringIO() wcsconfig_h.write( wcsconfig_h_proto % ( WCSLIB_VERSION, _determine_64_bit_int() )) _write_if_different(os.path.join('src', 'wcsconfig.h'), wcsconfig_h.getvalue()) _generate_c_docstrings(config) # Some compilers don't work - work around that. _adjust_compiler() # Add/remove macros and compile args based on the build type libraries = [] define_macros = [] undef_macros = [] extra_compile_args = [] if BUILD.lower() == 'debug': define_macros.append(('DEBUG', None)) undef_macros.append('NDEBUG') if not sys.platform.startswith('sun') and not sys.platform == 'win32': extra_compile_args.extend(["-fno-inline", "-O0", "-g"]) elif BUILD.lower() == 'profile': define_macros.append(('NDEBUG', None)) undef_macros.append('DEBUG') if not sys.platform.startswith('sun'): extra_compile_args.extend(["-O3", "-g"]) elif BUILD.lower() == 'release': # Define ECHO as nothing to prevent spurious newlines from # printing within the libwcs parser define_macros.append(('NDEBUG', None)) undef_macros.append('DEBUG') else: raise ValueError("BUILD should be one of 'debug', 'profile', or " "'release'; got %s" % BUILD) if sys.platform == 'win32': # This duplicates a bunch of macros defined in wcsconfig_h_proto # (below). When compiling wcslib, not everything includes that # include file, so we also define these macros on the command line. define_macros.append(('YY_NO_UNISTD_H', None)) define_macros.append(('_CRT_SECURE_NO_WARNINGS', None)) define_macros.append(('_NO_OLDNAMES', None)) define_macros.append(('NO_OLDNAMES', None)) define_macros.append(('__STDC__', None)) if sys.platform.startswith('linux'): define_macros.append(('HAVE_SINCOS', None)) if not sys.platform.startswith('sun') and not sys.platform == 'win32': if OPENMP: extra_compile_args.append('-fopenmp') libraries.append('gomp') else: extra_compile_args.extend(['-Wno-unknown-pragmas']) for idx, m in enumerate(define_macros): if m[1] is not None: define_macros[idx] = '%s = %s' % m else: define_macros[idx] = m[0] ext_opts = [('libraries', libraries), ('define_macros', define_macros), ('undef_macros', undef_macros), ('extra_compile_args', extra_compile_args)] ext = config['extension=pywcs._pywcs'] for opt, value in ext_opts: if opt in ext: ext[opt] += '\n' + '\n'.join(value) else: ext[opt] = '\n'.join(value) def _generate_c_docstrings(config): # GENERATE DOCSTRINGS IN C docstrings = {} # We need to temporarily add lib/pywcs to the path for this to work if 'packages_root' in config['files']: root = config['files']['packages_root'] else: root = '' pywcs_path = os.path.join(root, 'pywcs') if not pywcs_path in sys.path: clean_path = True sys.path.insert(0, pywcs_path) else: clean_path = False try: with open(os.path.join('doc', 'docstrings.py')) as f: exec(f.read(), docstrings) finally: if clean_path: sys.path.remove(pywcs_path) for key, val in list(docstrings.items()): if not (isinstance(key, str) and not key.startswith('__')): del docstrings[key] for key, val in docstrings.items(): docstrings[key] = val.encode('utf8').lstrip() docstrings = sorted(docstrings.items()) docstrings_h = StringIO() docstrings_h.write(textwrap.dedent(""" /* DO NOT EDIT! This file is autogenerated by setup.p. To edit its contents, edit doc/docstrings.py */ #ifndef __DOCSTRINGS_H__ #define __DOCSTRINGS_H__ void fill_docstrings(void); """)) for key, val in docstrings: docstrings_h.write('extern char doc_%s[%d];\n' % (key, len(val))) docstrings_h.write('\n#endif\n\n') _write_if_different(os.path.join('src', 'docstrings.h'), docstrings_h.getvalue()) docstrings_c = StringIO() docstrings_c.write(textwrap.dedent(""" /* DO NOT EDIT! This file is autogenerated by setup.py. To edit its contents, edit doc/docstrings.py The weirdness here with strncpy is because some C compilers, notably MSVC, do not support string literals greater than 256 characters. */ #include #include "docstrings.h" """)) for key, val in docstrings: docstrings_c.write('char doc_%s[%d];\n' % (key, len(val))) docstrings_c.write('\nvoid fill_docstrings(void)\n{\n') for key, val in docstrings: # For portability across various compilers, we need to fill the # docstrings in 256-character chunks for idx in range(0, len(val), 256): chunk = string_escape(val[idx:idx + 256]).replace('"', '\\"') docstrings_c.write(' strncpy(doc_%s + %d, "%s", %d);\n' % (key, idx, chunk, min(len(val) - idx, 256))) docstrings_c.write('\n') docstrings_c.write('\n}\n\n') _write_if_different(os.path.join('src', 'docstrings.c'), docstrings_c.getvalue()) # The only configuration parameter needed at compile-time is how to # specify a 64-bit signed integer. Python's ctypes module can get us # that information, but it is only available in Python 2.5 or later. # If we can't be absolutely certain, we default to "long long int", # which is correct on most platforms (x86, x86_64). If we find # platforms where this heuristic doesn't work, we may need to hardcode # for them. def _determine_64_bit_int(): try: try: import ctypes except ImportError: raise ValueError if ctypes.sizeof(ctypes.c_longlong) == 8: return 'long long int' elif ctypes.sizeof(ctypes.c_long) == 8: return 'long int' elif ctypes.sizeof(ctypes.c_int) == 8: return 'int' else: raise ValueError except ValueError: return 'long long int' def _write_if_different(filename, data): data = data.encode('ascii') if os.path.exists(filename): fd = open(filename, 'rb') original_data = fd.read() fd.close() else: original_data = None if original_data != data: fd = open(filename, 'wb') fd.write(data) fd.close() # def _adjust_compiler(): """ This function detects broken compilers and switches to another. If the environment variable CC is explicitly set, or a compiler is specified on the commandline, no override is performed -- the purpose here is to only override a default compiler. The specific compilers with problems are: * The default compiler in XCode-4.2, llvm-gcc-4.2, segfaults when compiling wcslib. The set of broken compilers can be updated by changing the compiler_mapping variable. It is a list of 2-tuples where the first in the pair is a regular expression matching the version of the broken compiler, and the second is the compiler to change to. """ if 'CC' in os.environ: return if get_distutils_option( 'compiler', ['build', 'build_ext', 'build_clib']) is not None: return from distutils import ccompiler import subprocess import re compiler_mapping = [ ('i686-apple-darwin[0-9]*-llvm-gcc-4.2', 'clang') ] c = ccompiler.new_compiler() # The MSVC ccompiler class doesn't have a `compiler` member. if not hasattr(c, 'compiler'): return process = subprocess.Popen( c.compiler + ['--version'], stdout=subprocess.PIPE) output = process.communicate()[0].strip().decode('ascii') version = output.split()[0] for broken, fixed in compiler_mapping: if re.match(broken, version): os.environ['CC'] = fixed break def get_distutils_option(option, commands): """ Returns the value of the given distutils option. Parameters ---------- option : str The name of the option commands : list of str The list of commands on which this option is available Returns ------- val : str or None the value of the given distutils option. If the option is not set, returns None. """ # Pre-parse the Distutils command-line options and config files to # if the option is set. dist = Distribution() try: dist.parse_config_files() dist.parse_command_line() except DistutilsError: # Let distutils handle this itself return None except AttributeError: # This seems to get thrown for ./setup.py --help return None for cmd in commands: if cmd in dist.commands: break else: return None for cmd in commands: cmd_opts = dist.get_option_dict(cmd) if option in cmd_opts: return cmd_opts[option][1] else: return None # The prototype for the standard header file wcsconfig_h_proto = """ /* WCSLIB library version number. */ #define WCSLIB_VERSION %s /* 64-bit integer data type. */ #define WCSLIB_INT64 %s /* Windows needs some other defines */ /* I think the only one we need is _WIN32, but the others don't hurt - Mark S. 2012-02-14 */ #if defined(_WIN32) || defined(_MSC_VER) || defined(__MINGW32__) || defined (__MINGW64__) /* * There is a lexical analyzer that was generated by flex. Tell it * that we don't have unistd.h */ #ifndef YY_NO_UNISTD_H #define YY_NO_UNISTD_H #endif /* * Visual C++ will warn you about certain functions that have a * high risk of buffer overflows, such as strcpy(). This * tells the compiler to shut up about it. */ #ifndef _CRT_SECURE_NO_WARNINGS #define _CRT_SECURE_NO_WARNINGS #endif /* * Suppress definition of wcsset() by system include files. * I don't know what's up with mingw. * In Visual C, the __STDC__ excludes non-standard things that * would otherwise be defined in the header files. */ #ifndef _NO_OLDNAMES /* for mingw32 */ #define _NO_OLDNAMES #endif #ifndef NO_OLDNAMES /* for mingw64 */ #define NO_OLDNAMES #endif #ifndef __STDC__ /* for MS Visual C */ #define __STDC__ 1 #endif #endif """ pywcs-1.12/LICENSE0000644001153600020070000000267512310355627015666 0ustar cslocumSTSCI\science00000000000000Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. pywcs-1.12/MANIFEST.in0000644001153600020070000000041612310355627016406 0ustar cslocumSTSCI\science00000000000000include CHANGELOG defsetup.py LICENSE MANIFEST.in README stsci_distutils_hack.py recursive-include wcslib * recursive-include src *.c *.h include doc/docstrings.py doc/make.bat doc/Makefile recursive-include doc/source *.rst *.py recursive-include lib/pywcs/tests *.hdr pywcs-1.12/patch_wcslib.sh0000755001153600020070000000006612310355627017652 0ustar cslocumSTSCI\science00000000000000#!/bin/sh cat patches/*.patch | patch -p0 -b -d wcslibpywcs-1.12/patches/0000755001153600020070000000000012310355732016273 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/patches/extended_ctype.patch0000644001153600020070000000072012310355626022321 0ustar cslocumSTSCI\science00000000000000Index: C/wcs.c =================================================================== --- C/wcs.c +++ C/wcs.c @@ -1688,7 +1688,8 @@ } /* Process linear axes. */ - if (!(strlen(ctypei) == 8 && ctypei[4] == '-')) { + if (!(strlen(ctypei) == 8 && ctypei[4] == '-') || + (strlen(ctypei) > 8 && ctypei[8] == '-')) { /* Identify Stokes, celestial and spectral types. */ if (strcmp(ctypei, "STOKES") == 0) { /* STOKES axis. */ pywcs-1.12/PKG-INFO0000644001153600020070000001316712310355732015751 0ustar cslocumSTSCI\science00000000000000Metadata-Version: 1.1 Name: pywcs Version: 1.12 Summary: Python wrappers to WCSLIB Home-page: http://www.scipy.org/AstroLib Author: Michael Droettboom Author-email: mdroe@stsci.edu License: UNKNOWN Description: Introduction ------------ pywcs is a set of routines for handling the FITS World Coordinate System (WCS) standard. It is a thin wrapper around the high- and mid-level interfaces of Dr. Mark Calabretta's WCSLIB available here: http://www.atnf.csiro.au/people/mcalabre/WCS/ In addition, there are extensions (written in C) to support Spitzer Simple Imaging Polynomial (SIP) convention keywords and Paper IV table lookup distortion. Please direct any questions to: help@stsci.edu Build instructions ------------------ pywcs includes its own copy of WCSLIB. pywcs requires: - Numpy 1.3 or later - pyfits 1.4 or later pywcs uses the standard Python distutils system to build and install itself. From the command line run:: python setup.py install to install pywcs. Building documentation ---------------------- Optionally, the documentation can be built using Sphinx (http://sphinx.pocoo.org). After installing pywcs, 'cd' into the 'doc' directory and:: make html The documentation is also available online at: http://stsdas.stsci.edu/astrolib/pywcs/index.html Version 1.11 ============ NEW FEATURES: - Updated to wcslib version 4.8.2, which gives much more detailed error messages. Exceptions raised due to invalid WCS keywords should now be more informative. - Undefined values that are the result of p2s and s2p are now set to NaN. Previously, one had to examine the stat result vector to determine which results were invalid. - Added functions get_pc() and get_cdelt(). These provide a way to always get the canonical representation of the linear transformation matrix, whether the header specified it in PC, CD or CROTA form. BROADER COMPATIBILITY: - Supports Python 3.x - Long-running process will now release the Python GIL to better support Python multithreading. - Builds on Microsoft Windows using mingw32, mingw64 and Visual Studio 9.0 and 10.0 without severely patching wcslib. - pywcs will now run without pyfits, though the SIP and distortion lookup table functionality is unavailable. BUG FIXES: - The dimensions of the cd and pc matrices were formerly always returned as 2x2. They now are sized according to naxis. MISCELLANEOUS: - Lots of new unit tests - Setting wcs.wcs.cunit will now verify that the values are valid unit strings. Version 1.10 ============ - Adds a UnitConversion class, which gives access to wcslib's unit conversion functionality. Given two convertible unit strings, pywcs can convert arrays of values from one to the other. - Now uses wcslib 4.7 - Changes to some wcs values would not always calculate secondary values. Version 1.9 =========== - Support binary image arrays and pixel list format WCS by presenting a way to call wcslib's wcsbth() - Updated underlying wcslib to version 4.5, which fixes the following: - Fixed the interpretation of VELREF when translating AIPS-convention spectral types. Such translation is now handled by a new special- purpose function, spcaips(). The wcsprm struct has been augmented with an entry for velref which is filled by wcspih() and wcsbth(). Previously, selection by VELREF of the radio or optical velocity convention for type VELO was not properly handled. BUGS: - The "pc" member is now available with a default "raw" Wcsprm object. - Make properties that return arrays read-only, since modifying a (mutable) array could result in secondary values not being recomputed based on those changes. - float properties can now be set using int values Version 1.3a1 ============= Earlier versions of pywcs had two versions of every conversion method: X(...) -- treats the origin of pixel coordinates at (0, 0) X_fits(...) -- treats the origin of pixel coordinates at (1, 1) From version 1.3 onwards, there is only one method for each conversion, with an 'origin' argument: - 0: places the origin at (0, 0), which is the C/Numpy convention. - 1: places the origin at (1, 1), which is the Fortran/FITS convention. Platform: UNKNOWN Classifier: Intended Audience :: Science/Research Classifier: License :: OSI Approved :: BSD License Classifier: Operating System :: OS Independent Classifier: Programming Language :: Python Classifier: Topic :: Scientific/Engineering :: Astronomy Classifier: Topic :: Software Development :: Libraries :: Python Modules pywcs-1.12/README0000644001153600020070000000211012310355627015521 0ustar cslocumSTSCI\science00000000000000Introduction ------------ pywcs is a set of routines for handling the FITS World Coordinate System (WCS) standard. It is a thin wrapper around the high- and mid-level interfaces of Dr. Mark Calabretta's WCSLIB available here: http://www.atnf.csiro.au/people/mcalabre/WCS/ In addition, there are extensions (written in C) to support Spitzer Simple Imaging Polynomial (SIP) convention keywords and Paper IV table lookup distortion. Please direct any questions to: help@stsci.edu Build instructions ------------------ pywcs includes its own copy of WCSLIB. pywcs requires: - Numpy 1.3 or later - pyfits 1.4 or later pywcs uses the standard Python distutils system to build and install itself. From the command line run:: python setup.py install to install pywcs. Building documentation ---------------------- Optionally, the documentation can be built using Sphinx (http://sphinx.pocoo.org). After installing pywcs, 'cd' into the 'doc' directory and:: make html The documentation is also available online at: http://stsdas.stsci.edu/astrolib/pywcs/index.html pywcs-1.12/setup.cfg0000644001153600020070000000417012310355732016467 0ustar cslocumSTSCI\science00000000000000[metadata] name = pywcs version = 1.12 stsci_wcs_version = 4.10 author = Michael Droettboom author-email = mdroe@stsci.edu home-page = http://www.scipy.org/AstroLib summary = Python wrappers to WCSLIB description-file = README CHANGELOG classifier = Intended Audience :: Science/Research License :: OSI Approved :: BSD License Operating System :: OS Independent Programming Language :: Python Topic :: Scientific/Engineering :: Astronomy Topic :: Software Development :: Libraries :: Python Modules requires-python = >=2.6 requires-dist = pyfits (>=2.4.0) numpy (>=1.5.1) [files] packages_root = lib packages = pywcs pywcs.tests data_files = pywcs/include = src/*.h pywcs/include/wcslib = wcslib/C/*.h pywcs/tests/maps = lib/pywcs/tests/maps/*.hdr pywcs/tests/nrao = lib/pywcs/tests/nrao/*.hdr pywcs/tests/spectra = lib/pywcs/tests/spectra/*.hdr pywcs/tests/data = lib/pywcs/tests/data/*.hdr pywcs/tests/data = lib/pywcs/tests/data/*.fits [install_data] pre-hook.glob-data-files = stsci.distutils.hooks.glob_data_files [global] setup_hooks = stsci.distutils.hooks.tag_svn_revision stsci.distutils.hooks.version_setup_hook hooks.pywcs_hook stsci.distutils.hooks.use_packages_root pywcs_setup.setup_hook [extension=pywcs._pywcs] sources = src/distortion.c src/distortion_wrap.c src/docstrings.c src/pipeline.c src/pyutil.c src/pywcs.c src/pywcs_api.c src/sip.c src/sip_wrap.c src/str_list_proxy.c src/util.c src/wcslib_tabprm_wrap.c src/wcslib_units_wrap.c src/wcslib_wrap.c src/wcslib_wtbarr_wrap.c wcslib/C/flexed/wcsbth.c wcslib/C/flexed/wcspih.c wcslib/C/flexed/wcsulex.c wcslib/C/flexed/wcsutrn.c wcslib/C/cel.c wcslib/C/lin.c wcslib/C/log.c wcslib/C/prj.c wcslib/C/spc.c wcslib/C/sph.c wcslib/C/spx.c wcslib/C/tab.c wcslib/C/wcs.c wcslib/C/wcserr.c wcslib/C/wcsfix.c wcslib/C/wcshdr.c wcslib/C/wcsprintf.c wcslib/C/wcsunits.c wcslib/C/wcsutil.c include_dirs = src wcslib/C numpy define_macros = ECHO WCSTRIG_MACRO PYWCS_BUILD _GNU_SOURCE [build_ext] pre-hook.numpy-extension-hook = stsci.distutils.hooks.numpy_extension_hook [egg_info] tag_build = tag_date = 0 tag_svn_revision = 0 pywcs-1.12/setup.py0000644001153600020070000000046612310355627016367 0ustar cslocumSTSCI\science00000000000000#!/usr/bin/env python try: from setuptools import setup except ImportError: from distribute_setup import use_setuptools use_setuptools() from setuptools import setup setup( setup_requires=['d2to1>=0.2.3', 'stsci.distutils>=0.3.2'], d2to1=True, use_2to3=True, zip_safe=False ) pywcs-1.12/src/0000755001153600020070000000000012310355732015433 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/src/distortion.c0000644001153600020070000001605112310355626020002 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #include "distortion.h" #include #include #include #include /* TODO: n-dimensional support */ int distortion_lookup_t_init( distortion_lookup_t* lookup) { unsigned int i; for (i = 0; i < NAXES; ++i) { lookup->naxis[i] = 0; lookup->crpix[i] = 0.0; lookup->crval[i] = 0.0; lookup->cdelt[i] = 1.0; } lookup->data = NULL; return 0; } void distortion_lookup_t_free( /*@unused@*/ distortion_lookup_t* lookup) { /*@empty@*/ } /** * Get a value at a specific integral location in the lookup table. * (This is nothing more special than an array lookup with range * checking.) */ static pywcs_inline float get_dist_clamp( const float* const data, const unsigned int* const naxis, const int x, const int y) { return data[ ((naxis[0] * CLAMP(y, 0, naxis[1] - 1)) + CLAMP(x, 0, naxis[0] - 1))]; } static pywcs_inline float get_dist( const float* const data, const unsigned int* const naxis, const int x, const int y) { return data[(naxis[0] * y) + x]; } /** * Converts a pixel coordinate to a fractional coordinate in the * lookup table on a single axis */ static pywcs_inline double image_coord_to_distortion_coord( const distortion_lookup_t * const lookup, const unsigned int axis, const double img) { double result; assert(lookup != NULL); assert(axis < NAXES); /* The "- 1./stepsize" is here because the input coordinates are 1-based, but this is a C-array underneath */ result = ( ((img - lookup->crval[axis]) / lookup->cdelt[axis]) + lookup->crpix[axis]) - 1.0/lookup->cdelt[axis]; return CLAMP(result, 0.0, (double)(lookup->naxis[axis] - 1)); } /** * Converts a pixel coordinate to a fractional coordinate in the * lookup table. */ static pywcs_inline void image_coords_to_distortion_coords( const distortion_lookup_t * const lookup, const double * const img /* [NAXES] */, /* Output parameters */ /*@out@*/ double *dist /* [NAXES] */) { unsigned int i; assert(lookup != NULL); assert(img != NULL); assert(dist != NULL); for (i = 0; i < NAXES; ++i) { dist[i] = image_coord_to_distortion_coord(lookup, i, img[i]); } } pywcs_inline double get_distortion_offset( const distortion_lookup_t * const lookup, const double * const img /*[NAXES]*/) { double dist[NAXES]; double dist_floor[NAXES]; int dist_ifloor[NAXES]; double dist_weight[NAXES]; double dist_iweight[NAXES]; double result; const unsigned int* naxis = lookup->naxis; const float* data = lookup->data; unsigned int i; assert(lookup != NULL); assert(img != NULL); image_coords_to_distortion_coords(lookup, img, dist); for (i = 0; i < NAXES; ++i) { dist_floor[i] = floor(dist[i]); dist_ifloor[i] = (int)dist_floor[i]; dist_weight[i] = dist[i] - dist_floor[i]; dist_iweight[i] = 1.0 - dist_weight[i]; } /* If we may need to clamp the lookups, use this slower approach */ if (dist_ifloor[0] < 0 || dist_ifloor[1] < 0 || dist_ifloor[0] >= lookup->naxis[0] - 1 || dist_ifloor[1] >= lookup->naxis[1] - 1) { result = (double)get_dist_clamp(data, naxis, dist_ifloor[0], dist_ifloor[1]) * dist_iweight[0] * dist_iweight[1] + (double)get_dist_clamp(data, naxis, dist_ifloor[0], dist_ifloor[1] + 1) * dist_iweight[0] * dist_weight[1] + (double)get_dist_clamp(data, naxis, dist_ifloor[0] + 1, dist_ifloor[1]) * dist_weight[0] * dist_iweight[1] + (double)get_dist_clamp(data, naxis, dist_ifloor[0] + 1, dist_ifloor[1] + 1) * dist_weight[0] * dist_weight[1]; /* Else, we don't need to clamp 4 times for each pixel */ } else { result = (double)get_dist(data, naxis, dist_ifloor[0], dist_ifloor[1]) * dist_iweight[0] * dist_iweight[1] + (double)get_dist(data, naxis, dist_ifloor[0], dist_ifloor[1] + 1) * dist_iweight[0] * dist_weight[1] + (double)get_dist(data, naxis, dist_ifloor[0] + 1, dist_ifloor[1]) * dist_weight[0] * dist_iweight[1] + (double)get_dist(data, naxis, dist_ifloor[0] + 1, dist_ifloor[1] + 1) * dist_weight[0] * dist_weight[1]; } return result; } int p4_pix2deltas( const unsigned int naxes, const distortion_lookup_t **lookup, /* [NAXES] */ const unsigned int nelem, const double* pix, /* [NAXES][nelem] */ double *foc /* [NAXES][nelem] */) { int i; double* foc0; const double* pix0; const double* pixend; assert(naxes == NAXES); assert(lookup != NULL); assert(pix != NULL); assert(foc != NULL); #ifndef NDEBUG unsigned int k; for (k = 0; k < naxes; ++k) { if (lookup[k] != NULL) { assert(lookup[k]->data != NULL); } } #endif if (pix == NULL || foc == NULL) { return 1; } pixend = pix + nelem * NAXES; /* This can't be parallelized, because pix may be equal to foc */ /* For the same reason, i needs to be in the inner loop */ for (pix0 = pix, foc0 = foc; pix0 < pixend; pix0 += NAXES, foc0 += NAXES) { for (i = 0; i < NAXES; ++i) { if (lookup[i]) { foc0[i] += get_distortion_offset(lookup[i], pix0); } } } return 0; } int p4_pix2foc( const unsigned int naxes, const distortion_lookup_t **lookup, /* [NAXES] */ const unsigned int nelem, const double* pix, /* [NAXES][nelem] */ double *foc /* [NAXES][nelem] */) { assert(pix); assert(foc); if (pix != foc) { memcpy(foc, pix, sizeof(double) * naxes * nelem); } return p4_pix2deltas(naxes, lookup, nelem, pix, foc); } pywcs-1.12/src/distortion.h0000644001153600020070000000777112310355626020020 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __DISTORTION_H__ #define __DISTORTION_H__ #include "util.h" /* TODO: This is all two-dimensional. Should be made multi-dimensional in the future. */ #define NAXES 2 #define MAXAXES 6 /** A structure to contain the information for a single distortion lookup table */ typedef struct { unsigned int naxis[NAXES]; /* size of distortion image */ double crpix[NAXES]; double crval[NAXES]; double cdelt[NAXES]; /* The data is not "owned" by this structure. It is the user's responsibility to free it. */ /*@shared@*/ /*@null@*/ float *data; } distortion_lookup_t; /** Initialize a lookup table to reasonable default values. */ int distortion_lookup_t_init(distortion_lookup_t* lookup); /** Cleanup after a lookup table. Currently does nothing, but may do something in the future, so please call it when you are done with the lookup table. It does not free the data pointed to be the lookup table -- it is the user's responsibility to free that array. */ void distortion_lookup_t_free(distortion_lookup_t* lookup); /** Lookup the distortion offset for a particular pixel coordinate in the lookup table. @param lookup A lookup table object @param A coordinate pair @return The offset as determined by binlinear interpolation in the lookup table */ double get_distortion_offset( const distortion_lookup_t * const lookup, const double * const img /* [NAXES] */); /** Perform just the distortion table part of Paper IV. @param naxes @param lookups A pair of lookup table objects @param nelem @param pix [in]: An array of pixel coordinates @param foc [out]: An array of focal plane coordinates @return A wcslib error code */ int p4_pix2foc( const unsigned int naxes, const distortion_lookup_t** lookups, /* [NAXES] */ const unsigned int nelem, const double* pix, /* [NAXES][nelem] */ double *foc /* [NAXES][nelem] */); /** Perform just the distortion table part of Paper IV, by adding distortion to the values already in place in foc. @param naxes @param lookups A pair of lookup table objects @param nelem @param pix [in]: An array of pixel coordinates @param foc [in/out]: An array of focal plane coordinates @return A wcslib error code */ int p4_pix2deltas( const unsigned int naxes, const distortion_lookup_t** lookups, /* [NAXES] */ const unsigned int nelem, const double* pix, /* [NAXES][nelem] */ double *foc /* [NAXES][nelem] */); #endif /* __DISTORTION_H__ */ pywcs-1.12/src/distortion_wrap.c0000644001153600020070000002432612310355626021037 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "distortion_wrap.h" #include "docstrings.h" #include /* From Python */ static int PyDistLookup_traverse( PyDistLookup* self, visitproc visit, void* arg) { Py_VISIT(self->py_data); return 0; } static int PyDistLookup_clear( PyDistLookup* self) { PyObject* tmp; tmp = (PyObject*)self->py_data; self->py_data = NULL; Py_XDECREF(tmp); return 0; } static void PyDistLookup_dealloc( PyDistLookup* self) { distortion_lookup_t_free(&self->x); Py_XDECREF(self->py_data); Py_TYPE(self)->tp_free((PyObject*)self); } /*@null@*/ static PyObject * PyDistLookup_new( PyTypeObject* type, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyDistLookup* self; self = (PyDistLookup*)type->tp_alloc(type, 0); if (self != NULL) { if (distortion_lookup_t_init(&self->x)) { return NULL; } self->py_data = NULL; } return (PyObject*)self; } static int PyDistLookup_init( PyDistLookup* self, PyObject* args, /*@unused@*/ PyObject* kwds) { PyObject* py_array_obj = NULL; PyArrayObject* array_obj = NULL; if (!PyArg_ParseTuple(args, "O(dd)(dd)(dd):DistortionLookupTable.__init__", &py_array_obj, &(self->x.crpix[0]), &(self->x.crpix[1]), &(self->x.crval[0]), &(self->x.crval[1]), &(self->x.cdelt[0]), &(self->x.cdelt[1]))) { return -1; } array_obj = (PyArrayObject*)PyArray_ContiguousFromAny(py_array_obj, PyArray_FLOAT32, 2, 2); if (array_obj == NULL) { return -1; } self->py_data = array_obj; self->x.naxis[0] = (unsigned int)PyArray_DIM(array_obj, 1); self->x.naxis[1] = (unsigned int)PyArray_DIM(array_obj, 0); self->x.data = (float *)PyArray_DATA(array_obj); return 0; } static PyObject* PyDistLookup_get_cdelt( PyDistLookup* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 2; return get_double_array("cdelt", self->x.cdelt, 1, &naxis, (PyObject*)self); } static int PyDistLookup_set_cdelt( PyDistLookup* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 2; return set_double_array("cdelt", value, 1, &naxis, self->x.cdelt); } static PyObject* PyDistLookup_get_crpix( PyDistLookup* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 2; return get_double_array("crpix", self->x.crpix, 1, &naxis, (PyObject*)self); } static int PyDistLookup_set_crpix( PyDistLookup* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 2; return set_double_array("crpix", value, 1, &naxis, self->x.crpix); } static PyObject* PyDistLookup_get_crval( PyDistLookup* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 2; return get_double_array("crval", self->x.crval, 1, &naxis, (PyObject*)self); } static int PyDistLookup_set_crval( PyDistLookup* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 2; return set_double_array("crval", value, 1, &naxis, self->x.crval); } /*@shared@*/ static PyObject* PyDistLookup_get_data( PyDistLookup* self, /*@unused@*/ void* closure) { if (self->py_data == NULL) { Py_INCREF(Py_None); return Py_None; } else { Py_INCREF(self->py_data); return (PyObject*)self->py_data; } } static int PyDistLookup_set_data( PyDistLookup* self, PyObject* value, /*@unused@*/ void* closure) { PyArrayObject* value_array = NULL; if (value == NULL) { Py_XDECREF(self->py_data); self->py_data = NULL; self->x.data = NULL; return 0; } value_array = (PyArrayObject*)PyArray_ContiguousFromAny(value, PyArray_FLOAT32, 2, 2); if (value_array == NULL) { return -1; } Py_XDECREF(self->py_data); self->py_data = value_array; self->x.naxis[0] = (unsigned int)PyArray_DIM(value_array, 1); self->x.naxis[1] = (unsigned int)PyArray_DIM(value_array, 0); self->x.data = (float *)PyArray_DATA(value_array); return 0; } /*@null@*/ static PyObject* PyDistLookup_get_offset( PyDistLookup* self, PyObject* args, /*@unused@*/ PyObject* kwds) { double coord[NAXES]; double result; if (self->x.data == NULL) { PyErr_SetString(PyExc_RuntimeError, "No data has been set for the lookup table"); return NULL; } if (!PyArg_ParseTuple(args, "dd:get_offset", &coord[0], &coord[1])) { return NULL; } result = get_distortion_offset(&self->x, coord); return PyFloat_FromDouble(result); } static PyObject* PyDistLookup___copy__( PyDistLookup* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyDistLookup* copy = NULL; int i = 0; copy = (PyDistLookup*)PyDistLookup_new(&PyDistLookupType, NULL, NULL); if (copy == NULL) { return NULL; } for (i = 0; i < 2; ++i) { copy->x.naxis[i] = self->x.naxis[i]; copy->x.crpix[i] = self->x.crpix[i]; copy->x.crval[i] = self->x.crval[i]; copy->x.cdelt[i] = self->x.cdelt[i]; } if (self->py_data) { PyDistLookup_set_data(copy, (PyObject*)self->py_data, NULL); } return (PyObject*)copy; } static PyObject* PyDistLookup___deepcopy__( PyDistLookup* self, PyObject* memo, /*@unused@*/ PyObject* kwds) { PyDistLookup* copy; PyObject* obj_copy; int i = 0; copy = (PyDistLookup*)PyDistLookup_new(&PyDistLookupType, NULL, NULL); if (copy == NULL) { return NULL; } for (i = 0; i < 2; ++i) { copy->x.naxis[i] = self->x.naxis[i]; copy->x.crpix[i] = self->x.crpix[i]; copy->x.crval[i] = self->x.crval[i]; copy->x.cdelt[i] = self->x.cdelt[i]; } if (self->py_data) { obj_copy = get_deepcopy((PyObject*)self->py_data, memo); if (obj_copy == NULL) { Py_DECREF(copy); return NULL; } PyDistLookup_set_data(copy, (PyObject*)obj_copy, NULL); Py_DECREF(obj_copy); } return (PyObject*)copy; } static PyGetSetDef PyDistLookup_getset[] = { {"cdelt", (getter)PyDistLookup_get_cdelt, (setter)PyDistLookup_set_cdelt, (char *)doc_cdelt}, {"crpix", (getter)PyDistLookup_get_crpix, (setter)PyDistLookup_set_crpix, (char *)doc_crpix}, {"crval", (getter)PyDistLookup_get_crval, (setter)PyDistLookup_set_crval, (char *)doc_crval}, {"data", (getter)PyDistLookup_get_data, (setter)PyDistLookup_set_data, (char *)doc_data}, {NULL} }; static PyMethodDef PyDistLookup_methods[] = { {"__copy__", (PyCFunction)PyDistLookup___copy__, METH_NOARGS, NULL}, {"__deepcopy__", (PyCFunction)PyDistLookup___deepcopy__, METH_O, NULL}, {"get_offset", (PyCFunction)PyDistLookup_get_offset, METH_VARARGS, doc_get_offset}, {NULL} }; PyTypeObject PyDistLookupType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs.DistortionLookupTable", /*tp_name*/ sizeof(PyDistLookup), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyDistLookup_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ 0, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ 0, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE | Py_TPFLAGS_HAVE_GC, /*tp_flags*/ doc_DistortionLookupTable, /* tp_doc */ (traverseproc)PyDistLookup_traverse, /* tp_traverse */ (inquiry)PyDistLookup_clear, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PyDistLookup_methods, /* tp_methods */ 0, /* tp_members */ PyDistLookup_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ (initproc)PyDistLookup_init, /* tp_init */ 0, /* tp_alloc */ PyDistLookup_new, /* tp_new */ }; int _setup_distortion_type( PyObject* m) { if (PyType_Ready(&PyDistLookupType) < 0) { return -1; } Py_INCREF(&PyDistLookupType); return PyModule_AddObject(m, "DistortionLookupTable", (PyObject *)&PyDistLookupType); } pywcs-1.12/src/distortion_wrap.h0000644001153600020070000000352612310355626021043 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __DISTORTION_WRAP_H__ #define __DISTORTION_WRAP_H__ #include "pyutil.h" #include "distortion.h" extern PyTypeObject PyDistLookupType; typedef struct { PyObject_HEAD distortion_lookup_t x; /*@null@*/ /*@shared@*/ PyArrayObject* py_data; } PyDistLookup; int _setup_distortion_type( PyObject* m); #endif pywcs-1.12/src/docstrings.c0000644001153600020070000021271012310355701017755 0ustar cslocumSTSCI\science00000000000000 /* DO NOT EDIT! This file is autogenerated by setup.py. To edit its contents, edit doc/docstrings.py The weirdness here with strncpy is because some C compilers, notably MSVC, do not support string literals greater than 256 characters. */ #include #include "docstrings.h" char doc_DistortionLookupTable[369]; char doc_K[152]; char doc_M[56]; char doc_Sip[1017]; char doc_Tabprm[226]; char doc_UnitConverter[2216]; char doc_Wcs[482]; char doc_Wcsprm[1979]; char doc_Wtbarr[195]; char doc_a[222]; char doc_a_order[94]; char doc_all_pix2sky[1204]; char doc_alt[236]; char doc_ap[225]; char doc_ap_order[96]; char doc_axis_types[916]; char doc_b[222]; char doc_b_order[94]; char doc_bp[225]; char doc_bp_order[96]; char doc_cd[1002]; char doc_cdelt[302]; char doc_cel_offset[153]; char doc_celfix[136]; char doc_cname[76]; char doc_colax[91]; char doc_colnum[235]; char doc_convert[120]; char doc_coord[278]; char doc_copy[39]; char doc_cpdis1[99]; char doc_cpdis2[99]; char doc_crder[123]; char doc_crota[998]; char doc_crpix[88]; char doc_crval[93]; char doc_crval_tabprm[131]; char doc_csyer[132]; char doc_ctype[222]; char doc_cubeface[1209]; char doc_cunit[1161]; char doc_cylfix[127]; char doc_data[72]; char doc_data_wtbarr[51]; char doc_dateavg[146]; char doc_dateobs[127]; char doc_datfix[453]; char doc_delta[195]; char doc_det2im[57]; char doc_det2im1[96]; char doc_det2im2[96]; char doc_dims[98]; char doc_equinox[242]; char doc_extlev[72]; char doc_extnam[73]; char doc_extrema[439]; char doc_extver[72]; char doc_find_all_wcs[846]; char doc_fix[1382]; char doc_get_cdelt[446]; char doc_get_offset[103]; char doc_get_pc[385]; char doc_get_ps[363]; char doc_get_pv[647]; char doc_has_cd[859]; char doc_has_cdi_ja[96]; char doc_has_crota[614]; char doc_has_crotaia[101]; char doc_has_pc[176]; char doc_has_pci_ja[96]; char doc_have[163]; char doc_i[40]; char doc_imgpix_matrix[143]; char doc_is_unity[102]; char doc_kind[129]; char doc_lat[89]; char doc_latpole[75]; char doc_lattyp[227]; char doc_lng[90]; char doc_lngtyp[228]; char doc_lonpole[76]; char doc_m[58]; char doc_map[941]; char doc_mix[4642]; char doc_mjdavg[189]; char doc_mjdobs[189]; char doc_name[74]; char doc_naxis[760]; char doc_nc[121]; char doc_ndim[66]; char doc_obsgeo[186]; char doc_offset[47]; char doc_p0[196]; char doc_p2s[1821]; char doc_p4_pix2foc[556]; char doc_pc[1069]; char doc_phi0[283]; char doc_pix2foc[558]; char doc_piximg_matrix[128]; char doc_power[49]; char doc_print_contents[204]; char doc_print_contents_tabprm[210]; char doc_radesys[77]; char doc_restfrq[94]; char doc_restwav[94]; char doc_row[39]; char doc_s2p[1710]; char doc_scale[56]; char doc_sense[182]; char doc_set[1178]; char doc_set_ps[354]; char doc_set_pv[353]; char doc_set_tabprm[346]; char doc_sip[77]; char doc_sip_foc2pix[573]; char doc_sip_pix2foc[571]; char doc_spcfix[237]; char doc_spec[68]; char doc_specsys[139]; char doc_sptr[1354]; char doc_ssysobs[226]; char doc_ssyssrc[110]; char doc_sub[3548]; char doc_tab[83]; char doc_theta0[282]; char doc_to_header[2086]; char doc_ttype[107]; char doc_unitfix[1008]; char doc_velangl[169]; char doc_velosys[282]; char doc_want[161]; char doc_wcs[75]; char doc_zsource[98]; void fill_docstrings(void) { strncpy(doc_DistortionLookupTable + 0, "DistortionLookupTable(*table*, *crpix*, *crval*, *cdelt*)\n\n- *table*: 2-dimensional array for the distortion lookup table.\n\n- *crpix*: the distortion array reference pixel (a 2-tuple)\n\n- *crval*: is the image array pixel coordinate (a 2-tuple)\n\n- *cdelt*: ", 256); strncpy(doc_DistortionLookupTable + 256, "is the grid step size (a 2-tuple)\n\nRepresents a single lookup table for a `Paper IV`_ distortion\ntransformation.\n", 113); strncpy(doc_K + 0, "``int array[M]`` (read-only)\n\nAn array of length `M` whose elements record the lengths of the axes of\nthe coordinate array and of each indexing vector.\n", 152); strncpy(doc_M + 0, "``int`` (read-only)\n\nNumber of tabular coordinate axes.\n", 56); strncpy(doc_Sip + 0, "Sip(*a, b, ap, bp, crpix*)\n\nThe `~pywcs.Sip` class performs polynomial distortion correction using\nthe `SIP`_ convention in both directions.\n\n Shupe, D. L., M. Moshir, J. Li, D. Makovoz and R. Narron. 2005.\n \"The SIP Convention for Representing Distor", 256); strncpy(doc_Sip + 256, "tion in FITS Image\n Headers.\" ADASS XIV.\n\n- *a*: double array[m+1][m+1]. The ``A_i_j`` polynomial for pixel to\n focal plane transformation. Its size must be (*m* + 1, *m* + 1)\n where *m* = ``A_ORDER``.\n\n- *b*: double array[m+1][m+1]. The ``B_i_j`` ", 256); strncpy(doc_Sip + 512, "polynomial for pixel to\n focal plane transformation. Its size must be (*m* + 1, *m* + 1)\n where *m* = ``B_ORDER``.\n\n- *ap*: double array[m+1][m+1]. The ``AP_i_j`` polynomial for pixel\n to focal plane transformation. Its size must be (*m* + 1, *m* + 1", 256); strncpy(doc_Sip + 768, ")\n where *m* = ``AP_ORDER``.\n\n- *bp*: double array[m+1][m+1]. The ``BP_i_j`` polynomial for pixel to\n focal plane transformation. Its size must be (*m* + 1, *m* + 1) where\n *m* = ``BP_ORDER``.\n\n- *crpix*: double array[2]. The reference pixel.\n", 249); strncpy(doc_Tabprm + 0, "A class to store the information related to tabular coordinates,\ni.e. coordinates that are defined via a lookup table.\n\nThis class can not be constructed directly from Python, but instead is\nreturned from `~pywcs.Wcsprm.tab`.\n", 226); strncpy(doc_UnitConverter + 0, "UnitConverter(have, want, translate_units=\'\')\n\nCreates an object for performing conversion from one system of units\nto another.\n\n- *have* string: :ref:`fits-unit` to convert from, with or without\n surrounding square brackets (for inline specifications); t", 256); strncpy(doc_UnitConverter + 256, "ext\n following the closing bracket is ignored.\n\n- *want* string: :ref:`fits-unit` to convert to, with or without\n surrounding square brackets (for inline specifications); text\n following the closing bracket is ignored.\n\n- *ctrl* string (optional): Do po", 256); strncpy(doc_UnitConverter + 512, "tentially unsafe translations of\n non-standard unit strings.\n\n Although ``\"S\"`` is commonly used to represent seconds, its\n recognizes ``\"S\"`` formally as Siemens, however rarely that may be\n translation to ``\"s\"`` is potentially unsafe since the stand", 256); strncpy(doc_UnitConverter + 768, "ard\n used. The same applies to ``\"H\"`` for hours (Henry), and ``\"D\"``\n for days (Debye).\n\n This string controls what to do in such cases, and is\n case-insensitive.\n\n - If the string contains ``\"s\"``, translate ``\"S\"`` to ``\"s\"``.\n\n - If the string c", 256); strncpy(doc_UnitConverter + 1024, "ontains ``\"h\"``, translate ``\"H\"`` to ``\"h\"``.\n\n - If the string contains ``\"d\"``, translate ``\"D\"`` to ``\"d\"``.\n\n Thus ``\'\'`` doesn\'t do any unsafe translations, whereas ``\'shd\'``\n does all of them.\n\n See :ref:`fits-unit` for more information.\n\nUse th", 256); strncpy(doc_UnitConverter + 1280, "e returned object\'s `~pywcs.UnitConverter.convert` method to\nconvert values from *have* to *want*.\n\nThis function is permissive in accepting whitespace in all contexts in\na units specification where it does not create ambiguity (e.g. not\nbetween a metric p", 256); strncpy(doc_UnitConverter + 1536, "refix and a basic unit string), including in strings\nlike ``\"log (m ** 2)\"`` which is formally disallowed.\n\n**Exceptions:**\n\n- `ValueError`: Invalid numeric multiplier.\n\n- `SyntaxError`: Dangling binary operator.\n\n- `SyntaxError`: Invalid symbol in INITIAL", 256); strncpy(doc_UnitConverter + 1792, " context.\n\n- `SyntaxError`: Function in invalid context.\n\n- `SyntaxError`: Invalid symbol in EXPON context.\n\n- `SyntaxError`: Unbalanced bracket.\n\n- `SyntaxError`: Unbalanced parenthesis.\n\n- `SyntaxError`: Consecutive binary operators.\n\n- `SyntaxError`: In", 256); strncpy(doc_UnitConverter + 2048, "ternal parser error.\n\n- `SyntaxError`: Non-conformant unit specifications.\n\n- `SyntaxError`: Non-conformant functions.\n\n- `ValueError`: Potentially unsafe translation.\n", 168); strncpy(doc_Wcs + 0, "Wcs(*sip, cpdis, wcsprm, det2im*)\n\nWcs objects amalgamate basic WCS (as provided by `wcslib`_), with\n`SIP`_ and `Paper IV`_ distortion operations.\n\nTo perform all distortion corrections and WCS tranformation, use\n`all_pix2sky`.\n\n- *sip*: A `~pywcs.Sip` obj", 256); strncpy(doc_Wcs + 256, "ect or ``None``\n\n- *cpdis*: A pair of `~pywcs.DistortionLookupTable` objects, or\n ``(None, None)``.\n\n- *wcsprm*: A `~pywcs.Wcsprm` object\n\n- *det2im*: A pair of `~pywcs.DistortionLookupTable` objects, or\n ``(None, None)``.\n", 226); strncpy(doc_Wcsprm + 0, "Wcsprm(header=None, key=\' \', relax=False, naxis=2, keysel=0, colsel=None)\n\n`~pywcs.Wcsprm` is a direct wrapper around `wcslib`_, and provides\naccess to the core WCS transformations that it supports.\n\nThe FITS header parsing enforces correct FITS \"keyword =", 256); strncpy(doc_Wcsprm + 256, " value\" syntax\nwith regard to the equals sign occurring in columns 9 and 10.\nHowever, it does recognize free-format character (NOST 100-2.0,\nSect. 5.2.1), integer (Sect. 5.2.3), and floating-point values\n(Sect. 5.2.4) for all keywords.\n\n- *header*: A PyFIT", 256); strncpy(doc_Wcsprm + 512, "S header object or a string containing the raw FITS\n header data or ``None``. If ``None``, the object will be\n initialized to default values.\n\n- *key*: The key referring to a particular WCS transform in the\n header. This may be either ``\' \'`` or ``\'A\'", 256); strncpy(doc_Wcsprm + 768, "``-``\'Z\'`` and\n corresponds to the ``\"a\"`` part of ``\"CTYPEia\"``. (*key*\n may only be provided if *header* is also provided.)\n\n- *relax*: Degree of permissiveness:\n\n - `False`: Recognize only FITS keywords defined by the published\n WCS standard.", 256); strncpy(doc_Wcsprm + 1024, "\n\n - `True`: Admit all recognized informal extensions of the WCS\n standard.\n\n - `int`: a bit field selecting specific extensions to accept. See\n :ref:`relaxread` for details.\n\n- *naxis*: The number of sky coordinates axes for the object.\n ", 256); strncpy(doc_Wcsprm + 1280, " (*naxis* may only be provided if *header* is ``None``.)\n\n- *keysel*: Vector of flag bits that may be used to restrict the\n keyword types considered:\n\n - ``WCSHDR_IMGHEAD``: Image header keywords.\n\n - ``WCSHDR_BIMGARR``: Binary table image array.\n", 256); strncpy(doc_Wcsprm + 1536, "\n - ``WCSHDR_PIXLIST``: Pixel list keywords.\n\n If zero, there is no restriction. If -1, the underlying wcslib\n function ``wcspih()`` is called, rather than ``wcstbh()``.\n\n- *colsel*: A sequence of table column numbers used to restrict the\n keywor", 256); strncpy(doc_Wcsprm + 1792, "ds considered. ``None`` indicates no restriction.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `ValueError`: Invalid key.\n\n- `KeyError`: Key not found in FITS header.\n", 187); strncpy(doc_Wtbarr + 0, "Classes to construct coordinate lookup tables from a binary table\nextension (BINTABLE).\n\nThis class can not be constructed directly from Python, but instead is\nreturned from `~pywcs.Wcsprm.wtb`.\n", 195); strncpy(doc_a + 0, "``double array[a_order+1][a_order+1]``\n\nThe `SIP`_ ``A_i_j`` matrix used for pixel to focal plane\ntransformation.\n\nIts values may be changed in place, but it may not be resized, without\ncreating a new `~pywcs.Sip` object.\n", 222); strncpy(doc_a_order + 0, "``int`` (read-only)\n\nThe order of the polynomial in the `SIP`_ ``A_i_j`` array (``A_ORDER``).\n", 94); strncpy(doc_all_pix2sky + 0, "all_pix2sky(pixcrd, origin) -> ``double array[ncoord][nelem]``\n\nTransforms pixel coordinates to sky coordinates by doing all of the\nfollowing:\n\n - Detector to image plane correction (optionally)\n\n - SIP distortion correction (optionally)\n\n - Paper", 256); strncpy(doc_all_pix2sky + 256, " IV distortion correction (optionally)\n\n - wcslib WCS transformation\n\nThe first three (the distortion corrections) are done in parallel.\n\n- *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates.\n\n\n- *origin*: int. Specifies the origin of pi", 256); strncpy(doc_all_pix2sky + 512, "xel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns an array of sky coordinates.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `SingularMatrixError`: Linear trans", 256); strncpy(doc_all_pix2sky + 768, "formation matrix is singular.\n\n- `InconsistentAxisTypesError`: Inconsistent or unrecognized\n coordinate axis types.\n\n- `ValueError`: Invalid parameter value.\n\n- `ValueError`: Invalid coordinate transformation parameters.\n\n- `ValueError`: x- and y-coordina", 256); strncpy(doc_all_pix2sky + 1024, "te arrays are not the same size.\n\n- `InvalidTransformError`: Invalid coordinate transformation.\n\n- `InvalidTransformError`: Ill-conditioned coordinate transformation\n parameters.\n", 180); strncpy(doc_alt + 0, "``str``\n\nCharacter code for alternate coordinate descriptions. For example,\nthe ``\"a\"`` in keyword names such as ``CTYPEia``. This is a space\ncharacter for the primary coordinate description, or one of the 26\nupper-case letters, A-Z.\n", 236); strncpy(doc_ap + 0, "``double array[ap_order+1][ap_order+1]``\n\nThe `SIP`_ ``AP_i_j`` matrix used for focal plane to pixel\ntransformation. Its values may be changed in place, but it may not be\nresized, without creating a new `~pywcs.Sip` object.\n", 225); strncpy(doc_ap_order + 0, "``int`` (read-only)\n\nThe order of the polynomial in the `SIP`_ ``AP_i_j`` array\n(``AP_ORDER``).\n", 96); strncpy(doc_axis_types + 0, "``int array[naxis]``\n\nAn array of four-digit type codes for each axis.\n\n- First digit (i.e. 1000s):\n\n - 0: Non-specific coordinate type.\n\n - 1: Stokes coordinate.\n\n - 2: Celestial coordinate (including ``CUBEFACE``).\n\n - 3: Spectral coordinate.\n\n- Seco", 256); strncpy(doc_axis_types + 256, "nd digit (i.e. 100s):\n\n - 0: Linear axis.\n\n - 1: Quantized axis (``STOKES``, ``CUBEFACE``).\n\n - 2: Non-linear celestial axis.\n\n - 3: Non-linear spectral axis.\n\n - 4: Logarithmic axis.\n\n - 5: Tabular axis.\n\n- Third digit (i.e. 10s):\n\n - 0: Group numb", 256); strncpy(doc_axis_types + 512, "er, e.g. lookup table number\n\n- The fourth digit is used as a qualifier depending on the axis type.\n\n - For celestial axes:\n\n - 0: Longitude coordinate.\n\n - 1: Latitude coordinate.\n\n - 2: ``CUBEFACE`` number.\n\n - For lookup tables: the axis numb", 256); strncpy(doc_axis_types + 768, "er in a multidimensional table.\n\n``CTYPEia`` in ``\"4-3\"`` form with unrecognized algorithm code will\nhave its type set to -1 and generate an error.\n", 148); strncpy(doc_b + 0, "``double array[b_order+1][b_order+1]``\n\nThe `SIP`_ ``B_i_j`` matrix used for pixel to focal plane\ntransformation. Its values may be changed in place, but it may not be\nresized, without creating a new `~pywcs.Sip` object.\n", 222); strncpy(doc_b_order + 0, "``int`` (read-only)\n\nThe order of the polynomial in the `SIP`_ ``B_i_j`` array\n(``B_ORDER``).\n", 94); strncpy(doc_bp + 0, "``double array[bp_order+1][bp_order+1]``\n\nThe `SIP`_ ``BP_i_j`` matrix used for focal plane to pixel\ntransformation. Its values may be changed in place, but it may not be\nresized, without creating a new `~pywcs.Sip` object.\n", 225); strncpy(doc_bp_order + 0, "``int`` (read-only)\n\nThe order of the polynomial in the `SIP`_ ``BP_i_j`` array\n(``BP_ORDER``).\n", 96); strncpy(doc_cd + 0, "``double array[naxis][naxis]``\n\nThe ``CDi_ja`` linear transformation matrix.\n\nFor historical compatibility, three alternate specifications of the\nlinear transforations are available in wcslib. The canonical\n``PCi_ja`` with ``CDELTia``, ``CDi_ja``, and the", 256); strncpy(doc_cd + 256, " deprecated\n``CROTAia`` keywords. Although the latter may not formally co-exist\nwith ``PCi_ja``, the approach here is simply to ignore them if given\nin conjunction with ``PCi_ja``.\n\n`~pywcs.Wcsprm.has_pc`, `~pywcs.Wcsprm.has_cd` and\n`~pywcs.Wcsprm.has_cro", 256); strncpy(doc_cd + 512, "ta` can be used to determine which of these\nalternatives are present in the header.\n\nThese alternate specifications of the linear transformation matrix are\ntranslated immediately to ``PCi_ja`` by `~pywcs.Wcsprm.set` and are\nnowhere visible to the lower-lev", 256); strncpy(doc_cd + 768, "el routines. In particular,\n`~pywcs.Wcsprm.set` resets `~pywcs.Wcsprm.cdelt` to unity if\n``CDi_ja`` is present (and no ``PCi_ja``). If no ``CROTAia`` is\nassociated with the latitude axis, `set` reverts to a unity ``PCi_ja``\nmatrix.\n", 234); strncpy(doc_cdelt + 0, "``double array[naxis]``\n\nCoordinate increments (``CDELTia``) for each coord axis.\n\nIf a ``CDi_ja`` linear transformation matrix is present, a warning is\nraised and `~pywcs.Wcsprm.cdelt` is ignored. The ``CDi_ja`` matrix\nmay be deleted by::\n\n del wcs.wcs.", 256); strncpy(doc_cdelt + 256, "cd\n\nAn undefined value is represented by NaN.\n", 46); strncpy(doc_cel_offset + 0, "``boolean``\n\nIf `True`, an offset will be applied to ``(x, y)`` to force ``(x,y) =\n(0,0)`` at the fiducial point, (phi_0, theta_0). Default is\n`False`.\n", 153); strncpy(doc_celfix + 0, "Translates AIPS-convention celestial projection types, ``-NCP`` and\n``-GLS``.\n\nReturns ``0`` for success; ``-1`` if no change required.\n", 136); strncpy(doc_cname + 0, "``list of strings``\n\nA list of the coordinate axis names, from ``CNAMEia``.\n", 76); strncpy(doc_colax + 0, "``int array[naxis]``\n\nAn array recording the column numbers for each axis in a pixel list.\n", 91); strncpy(doc_colnum + 0, "``int``\n\nWhere the coordinate representation is associated with an image-array\ncolumn in a FITS binary table, this property may be used to record the\nrelevant column number.\n\nIt should be set to zero for an image header or pixel list.\n", 235); strncpy(doc_convert + 0, "convert(array)\n\nPerform the unit conversion on the elements of the given *array*,\nreturning an array of the same shape.\n", 120); strncpy(doc_coord + 0, "``double array[K_M]...[K_2][K_1][M]``\n\nThe tabular coordinate array, with the dimensions::\n\n (K_M, ... K_2, K_1, M)\n\n(see `~pywcs._pywcs.Tabprm.K`) i.e. with the `M` dimension varying\nfastest so that the `M` elements of a coordinate vector are stored\nco", 256); strncpy(doc_coord + 256, "ntiguously in memory.\n", 22); strncpy(doc_copy + 0, "Creates a deep copy of the WCS object.\n", 39); strncpy(doc_cpdis1 + 0, "`~pywcs.DistortionLookupTable`\n\nThe pre-linear transformation distortion lookup table, ``CPDIS1``.\n", 99); strncpy(doc_cpdis2 + 0, "`~pywcs.DistortionLookupTable`\n\nThe pre-linear transformation distortion lookup table, ``CPDIS2``.\n", 99); strncpy(doc_crder + 0, "``double array[naxis]``\n\nThe random error in each coordinate axis, ``CRDERia``.\n\nAn undefined value is represented by NaN.\n", 123); strncpy(doc_crota + 0, "``double array[naxis]``\n\n``CROTAia`` keyvalues for each coordinate axis.\n\nFor historical compatibility, three alternate specifications of the\nlinear transforations are available in wcslib. The canonical\n``PCi_ja`` with ``CDELTia``, ``CDi_ja``, and the dep", 256); strncpy(doc_crota + 256, "recated\n``CROTAia`` keywords. Although the latter may not formally co-exist\nwith ``PCi_ja``, the approach here is simply to ignore them if given\nin conjunction with ``PCi_ja``.\n\n`~pywcs.Wcsprm.has_pc`, `~pywcs.Wcsprm.has_cd` and\n`~pywcs.Wcsprm.has_crota` ", 256); strncpy(doc_crota + 512, "can be used to determine which of these\nalternatives are present in the header.\n\nThese alternate specifications of the linear transformation matrix are\ntranslated immediately to ``PCi_ja`` by `~pywcs.Wcsprm.set` and are\nnowhere visible to the lower-level r", 256); strncpy(doc_crota + 768, "outines. In particular,\n`~pywcs.Wcsprm.set` resets `~pywcs.Wcsprm.cdelt` to unity if\n``CDi_ja`` is present (and no ``PCi_ja``). If no ``CROTAia`` is\nassociated with the latitude axis, `set` reverts to a unity ``PCi_ja``\nmatrix.\n", 230); strncpy(doc_crpix + 0, "``double array[naxis]``\n\nCoordinate reference pixels (``CRPIXja``) for each pixel axis.\n", 88); strncpy(doc_crval + 0, "``double array[naxis]``\n\nCoordinate reference values (``CRVALia``) for each coordinate axis.\n", 93); strncpy(doc_crval_tabprm + 0, "``double array[M]``\n\nArray whose elements contain the index value for the reference pixel\nfor each of the tabular coordinate axes.\n", 131); strncpy(doc_csyer + 0, "``double array[naxis]``\n\nThe systematic error in the coordinate value axes, ``CSYERia``.\n\nAn undefined value is represented by NaN.\n", 132); strncpy(doc_ctype + 0, "``list of strings[naxis]``\n\nList of ``CTYPEia`` keyvalues.\n\nThe `~pywcs.Wcsprm.ctype` keyword values must be in upper case and\nthere must be zero or one pair of matched celestial axis types, and\nzero or one spectral axis.\n", 222); strncpy(doc_cubeface + 0, "``int``\n\nIndex into the ``pixcrd`` (pixel coordinate) array for the\n``CUBEFACE`` axis. This is used for quadcube projections where the\ncube faces are stored on a separate axis.\n\nThe quadcube projections (``TSC``, ``CSC``, ``QSC``) may be\nrepresented in FI", 256); strncpy(doc_cubeface + 256, "TS in either of two ways:\n\n - The six faces may be laid out in one plane and numbered as\n follows::\n\n\n 0\n\n 4 3 2 1 4 3 2\n\n 5\n\n Faces", 256); strncpy(doc_cubeface + 512, " 2, 3 and 4 may appear on one side or the other (or both).\n The sky-to-pixel routines map faces 2, 3 and 4 to the left but\n the pixel-to-sky routines accept them on either side.\n\n - The ``COBE`` convention in which the six faces are stored in ", 256); strncpy(doc_cubeface + 768, "a\n three-dimensional structure using a ``CUBEFACE`` axis indexed\n from 0 to 5 as above.\n\nThese routines support both methods; `~pywcs.Wcsprm.set` determines\nwhich is being used by the presence or absence of a ``CUBEFACE`` axis\nin `~pywcs.Wcsprm.c", 256); strncpy(doc_cubeface + 1024, "type`. `~pywcs.Wcsprm.p2s` and `~pywcs.Wcsprm.s2p`\ntranslate the ``CUBEFACE`` axis representation to the single plane\nrepresentation understood by the lower-level projection routines.\n", 185); strncpy(doc_cunit + 0, "``list of strings[naxis]``\n\nList of ``CUNITia`` keyvalues which define the units of measurement of\nthe ``CRVALia``, ``CDELTia`` and ``CDi_ja`` keywords.\n\nAs ``CUNITia`` is an optional header keyword, `~pywcs.Wcsprm.cunit`\nmay be left blank but otherwise is", 256); strncpy(doc_cunit + 256, " expected to contain a standard\nunits specification as defined by WCS Paper I.\n`~pywcs.Wcsprm.unitfix` is available to translate commonly used\nnon-standard units specifications but this must be done as a separate\nstep before invoking `~pywcs.Wcsprm.set`.\n\n", 256); strncpy(doc_cunit + 512, "For celestial axes, if `~pywcs.Wcsprm.cunit` is not blank,\n`~pywcs.Wcsprm.set` uses `wcsunits` to parse it and scale\n`~pywcs.Wcsprm.cdelt`, `~pywcs.Wcsprm.crval`, and `~pywcs.Wcsprm.cd`\nto decimal degrees. It then resets `~pywcs.Wcsprm.cunit` to\n``\"deg\"``", 256); strncpy(doc_cunit + 768, ".\n\nFor spectral axes, if `~pywcs.Wcsprm.cunit` is not blank,\n`~pywcs.Wcsprm.set` uses `wcsunits` to parse it and scale\n`~pywcs.Wcsprm.cdelt`, `~pywcs.Wcsprm.crval`, and `~pywcs.Wcsprm.cd`\nto SI units. It then resets `~pywcs.Wcsprm.cunit` accordingly.\n\n`~p", 256); strncpy(doc_cunit + 1024, "ywcs.Wcsprm.set` ignores `~pywcs.Wcsprm.cunit` for other coordinate\ntypes; `~pywcs.Wcsprm.cunit` may be used to label coordinate values.\n", 137); strncpy(doc_cylfix + 0, "cylfix()\n\nFixes WCS keyvalues for malformed cylindrical projections.\n\nReturns ``0`` for success; ``-1`` if no change required.\n", 127); strncpy(doc_data + 0, "``float array``\n\nThe array data for the `~pywcs.DistortionLookupTable`.\n", 72); strncpy(doc_data_wtbarr + 0, "``double array``\n\nThe array data for the BINTABLE.\n", 51); strncpy(doc_dateavg + 0, "``string``\n\nRepresentative mid-point of the date of observation in ISO format,\n``yyyy-mm-ddThh:mm:ss``.\n\n.. seealso::\n\n `~pywcs.Wcsprm.dateobs`\n", 146); strncpy(doc_dateobs + 0, "``string``\n\nStart of the date of observation in ISO format,\n``yyyy-mm-ddThh:mm:ss``.\n\n.. seealso::\n\n `~pywcs.Wcsprm.dateavg`\n", 127); strncpy(doc_datfix + 0, "datfix()\n\nTranslates the old ``DATE-OBS`` date format to year-2000 standard form\n``(yyyy-mm-ddThh:mm:ss)`` and derives ``MJD-OBS`` from it if not\nalready set. Alternatively, if `~pywcs.Wcsprm.mjdobs` is set and\n`~pywcs.Wcsprm.dateobs` isn\'t, then `~pywcs.", 256); strncpy(doc_datfix + 256, "Wcsprm.datfix` derives\n`~pywcs.Wcsprm.dateobs` from it. If both are set but disagree by more\nthan half a day then `ValueError` is raised.\n\nReturns ``0`` for success; ``-1`` if no change required.\n", 197); strncpy(doc_delta + 0, "``double array[M]`` (read-only)\n\nArray of interpolated indices into the coordinate array such that\nUpsilon_m, as defined in Paper III, is equal to\n(`~pywcs._pywcs.Tabprm.p0` [m] + 1) + delta[m].\n", 195); strncpy(doc_det2im + 0, "Convert detector coordinates to image plane coordinates.\n", 57); strncpy(doc_det2im1 + 0, "A `~pywcs.DistortionLookupTable` object for detector to image plane\ncorrection in the *x*-axis.\n", 96); strncpy(doc_det2im2 + 0, "A `~pywcs.DistortionLookupTable` object for detector to image plane\ncorrection in the *y*-axis.\n", 96); strncpy(doc_dims + 0, "``int array[ndim]`` (read-only)\n\nThe dimensions of the tabular array `~pywcs._pywcs.Wtbarr.data`.\n", 98); strncpy(doc_equinox + 0, "``double``\n\nThe equinox associated with dynamical equatorial or ecliptic\ncoordinate systems, ``EQUINOXa`` (or ``EPOCH`` in older headers). Not\napplicable to ICRS equatorial or ecliptic coordinates.\n\nAn undefined value is represented by NaN.\n", 242); strncpy(doc_extlev + 0, "``int`` (read-only)\n\n``EXTLEV`` identifying the binary table extension.\n", 72); strncpy(doc_extnam + 0, "``str`` (read-only)\n\n``EXTNAME`` identifying the binary table extension.\n", 73); strncpy(doc_extrema + 0, "``double array[K_M]...[K_2][2][M]`` (read-only)\n\nAn array recording the minimum and maximum value of each element of\nthe coordinate vector in each row of the coordinate array, with the\ndimensions::\n\n (K_M, ... K_2, 2, M)\n\n(see `~pywcs._pywcs.Tabprm.K`).", 256); strncpy(doc_extrema + 256, " The minimum is recorded in the first\nelement of the compressed K_1 dimension, then the maximum. This array\nis used by the inverse table lookup function to speed up table\nsearches.\n", 183); strncpy(doc_extver + 0, "``int`` (read-only)\n\n``EXTVER`` identifying the binary table extension.\n", 72); strncpy(doc_find_all_wcs + 0, "find_all_wcs(relax=0, keysel=0)\n\nFind all WCS transformations in the header.\n\n- *header*: A string containing the raw FITS header data.\n\n- *relax*: Degree of permissiveness:\n\n - `False`: Recognize only FITS keywords defined by the published\n WCS st", 256); strncpy(doc_find_all_wcs + 256, "andard.\n\n - `True`: Admit all recognized informal extensions of the WCS\n standard.\n\n - `int`: a bit field selecting specific extensions to accept. See\n :ref:`relaxread` for details.\n\n- *keysel*: Vector of flag bits that may be used to rest", 256); strncpy(doc_find_all_wcs + 512, "rict the\n keyword types considered:\n\n - ``WCSHDR_IMGHEAD``: Image header keywords.\n\n - ``WCSHDR_BIMGARR``: Binary table image array.\n\n - ``WCSHDR_PIXLIST``: Pixel list keywords.\n\n If zero, there is no restriction. If -1, wcspih() is called,", 256); strncpy(doc_find_all_wcs + 768, "\n rather than wcstbh().\n\nReturns a list of `~pywcs._pywcs._Wcsprm` objects.\n", 78); strncpy(doc_fix + 0, "fix(translate_units=\'\', naxis=0)\n\nApplies all of the corrections handled separately by\n`~pywcs.Wcsprm.datfix`, `~pywcs.Wcsprm.unitfix`,\n`~pywcs.Wcsprm.celfix`, `~pywcs.Wcsprm.spcfix` and\n`~pywcs.Wcsprm.cylfix`.\n\n- *translate_units*: string. Do potentially ", 256); strncpy(doc_fix + 256, "unsafe translations of\n non-standard unit strings.\n\n Although ``\"S\"`` is commonly used to represent seconds, its\n translation to ``\"s\"`` is potentially unsafe since the standard\n recognizes ``\"S\"`` formally as Siemens, however rarely that may be\n used", 256); strncpy(doc_fix + 512, ". The same applies to ``\"H\"`` for hours (Henry), and ``\"D\"``\n for days (Debye).\n\n This string controls what to do in such cases, and is\n case-insensitive.\n\n - If the string contains ``\"s\"``, translate ``\"S\"`` to ``\"s\"``.\n\n - If the string contains ``", 256); strncpy(doc_fix + 768, "\"h\"``, translate ``\"H\"`` to ``\"h\"``.\n\n - If the string contains ``\"d\"``, translate ``\"D\"`` to ``\"d\"``.\n\n Thus ``\'\'`` doesn\'t do any unsafe translations, whereas ``\'shd\'``\n does all of them.\n\n- *naxis*: int array[naxis]. Image axis lengths. If this", 256); strncpy(doc_fix + 1024, " array is\n set to zero or ``None``, then `~pywcs.Wcsprm.cylfix` will not be\n invoked.\n\nReturns a dictionary containing the following keys, each referring to\na status string for each of the sub-fix functions that were\ncalled:\n\n- `~pywcs.Wcsprm.datfix`\n\n- ", 256); strncpy(doc_fix + 1280, "`~pywcs.Wcsprm.unitfix`\n\n- `~pywcs.Wcsprm.celfix`\n\n- `~pywcs.Wcsprm.spcfix`\n\n- `~pywcs.Wcsprm.cylfix`\n", 102); strncpy(doc_get_cdelt + 0, "get_cdelt() -> double array[naxis]\n\nCoordinate increments (``CDELTia``) for each coord axis.\n\nReturns the ``CDELT`` offsets in read-only form. Unlike the\n`~pywcs.Wcsprm.cdelt` property, this works even when the header\nspecifies the linear transformation m", 256); strncpy(doc_get_cdelt + 256, "atrix in one of the alternative\n``CDi_ja`` or ``CROTAia`` forms. This is useful when you want access\nto the linear transformation matrix, but don\'t care how it was\nspecified in the header.\n", 190); strncpy(doc_get_offset + 0, "get_offset(*x, y*) -> (*x, y*)\n\nReturns the offset from the distortion table for pixel point (*x, y*).\n", 103); strncpy(doc_get_pc + 0, "get_pc() -> double array[naxis][naxis]\n\nReturns the ``PC`` matrix in read-only form. Unlike the\n`~pywcs.Wcsprm.pc` property, this works even when the header specifies\nthe linear transformation matrix in one of the alternative ``CDi_ja``\nor ``CROTAia`` for", 256); strncpy(doc_get_pc + 256, "ms. This is useful when you want access to the\nlinear transformation matrix, but don\'t care how it was specified in\nthe header.\n", 129); strncpy(doc_get_ps + 0, "get_ps() -> list of tuples\n\nReturns ``PSi_ma`` keywords for each *i* and *m*. Returned as a list\nof tuples of the form (*i*, *m*, *value*):\n\n - *i*: int. Axis number, as in ``PSi_ma``, (i.e. 1-relative)\n\n - *m*: int. Parameter number, as in ``PSi_", 256); strncpy(doc_get_ps + 256, "ma``, (i.e. 0-relative)\n\n - *value*: string. Parameter value.\n\n.. seealso::\n\n `~pywcs.Wcsprm.set_ps`\n", 107); strncpy(doc_get_pv + 0, "get_pv() -> list of tuples\n\nReturns ``PVi_ma`` keywords for each *i* and *m*. Returned as a list\nof tuples of the form (*i*, *m*, *value*):\n\n - *i*: int. Axis number, as in ``PVi_ma``, (i.e. 1-relative)\n\n - *m*: int. Parameter number, as in ``PVi_", 256); strncpy(doc_get_pv + 256, "ma``, (i.e. 0-relative)\n\n - *value*: string. Parameter value.\n\nNote that, if they were not given, `~pywcs.Wcsprm.set` resets the\nentries for ``PVi_1a``, ``PVi_2a``, ``PVi_3a``, and ``PVi_4a`` for\nlongitude axis *i* to match (``phi_0``, ``theta_0``), the", 256); strncpy(doc_get_pv + 512, " native\nlongitude and latitude of the reference point given by ``LONPOLEa``\nand ``LATPOLEa``.\n\n.. seealso::\n\n `~pywcs.Wcsprm.set_pv`\n", 135); strncpy(doc_has_cd + 0, "has_cd() -> bool\n\nReturns `True` if ``CDi_ja`` is present. ``CDi_ja`` is an alternate\nspecification of the linear transformation matrix, maintained for\nhistorical compatibility.\n\nMatrix elements in the IRAF convention are equivalent to the product\n``CDi_j", 256); strncpy(doc_has_cd + 256, "a = CDELTia * PCi_ja``, but the defaults differ from that of\nthe ``PCi_ja`` matrix. If one or more ``CDi_ja`` keywords are present\nthen all unspecified ``CDi_ja`` default to zero. If no ``CDi_ja`` (or\n``CROTAia``) keywords are present, then the header is", 256); strncpy(doc_has_cd + 512, " assumed to be in\n``PCi_ja`` form whether or not any ``PCi_ja`` keywords are present\nsince this results in an interpretation of ``CDELTia`` consistent with\nthe original FITS specification.\n\nWhile ``CDi_ja`` may not formally co-exist with ``PCi_ja``, it may", 256); strncpy(doc_has_cd + 768, "\nco-exist with ``CDELTia`` and ``CROTAia`` which are to be ignored.\n\n.. seealso::\n\n `cd`\n", 91); strncpy(doc_has_cdi_ja + 0, "has_cdi_ja() -> bool\n\nAlias for `~pywcs.Wcsprm.has_cd`. Maintained for backward\ncompatibility.\n", 96); strncpy(doc_has_crota + 0, "has_crota() -> bool\n\nReturns `True` if ``CROTAia`` is present. ``CROTAia`` is an\nalternate specification of the linear transformation matrix,\nmaintained for historical compatibility.\n\nIn the AIPS convention, ``CROTAia`` may only be associated with the\nlat", 256); strncpy(doc_has_crota + 256, "itude axis of a celestial axis pair. It specifies a rotation in\nthe image plane that is applied *after* the ``CDELTia``; any other\n``CROTAia`` keywords are ignored.\n\n``CROTAia`` may not formally co-exist with ``PCi_ja``. ``CROTAia`` and\n``CDELTia`` may f", 256); strncpy(doc_has_crota + 512, "ormally co-exist with ``CDi_ja`` but if so are to be\nignored.\n\n.. seealso::\n\n `~pywcs.Wcsprm.crota`\n", 102); strncpy(doc_has_crotaia + 0, "has_crota_ia() -> bool\n\nAlias for `~pywcs.Wcsprm.has_crota`. Maintained for backward\ncompatibility.\n", 101); strncpy(doc_has_pc + 0, "has_pc() -> bool\n\nReturns `True` if ``PCi_ja`` is present. ``PCi_ja`` is the\nrecommended way to specify the linear transformation matrix.\n\n.. seealso::\n\n `~pywcs.Wcsprm.pc`\n", 176); strncpy(doc_has_pci_ja + 0, "has_pci_ja() -> bool\n\nAlias for `~pywcs.Wcsprm.has_pc`. Maintained for backward\ncompatibility.\n", 96); strncpy(doc_have + 0, "The name of the unit being converted from.\n\nThis value always uses standard unit names, even if the\n`UnitConverter` was initialized with a non-standard unit name.\n", 163); strncpy(doc_i + 0, "``int`` (read-only)\n\nImage axis number.\n", 40); strncpy(doc_imgpix_matrix + 0, "``double array[2][2]`` (read-only)\n\nInverse of the matrix containing the product of the ``CDELTia``\ndiagonal matrix and the ``PCi_ja`` matrix.\n", 143); strncpy(doc_is_unity + 0, "is_unity() -> bool\n\nReturns `True` if the linear transformation matrix\n(`~pywcs.Wcsprm.cd`) is unity.\n", 102); strncpy(doc_kind + 0, "``str`` (read-only)\n\nCharacter identifying the wcstab array type:\n\n - ``\'c\'``: coordinate array,\n - ``\'i\'``: index vector.\n", 129); strncpy(doc_lat + 0, "``int`` (read-only)\n\nThe index into the sky coordinate array containing latitude values.\n", 89); strncpy(doc_latpole + 0, "``double``\n\nThe native latitude of the celestial pole, ``LATPOLEa`` (deg).\n", 75); strncpy(doc_lattyp + 0, "``string`` (read-only)\n\nCelestial axis type for latitude, e.g. \"RA\", \"DEC\", \"GLON\", \"GLAT\",\netc. extracted from \'RA--\', \'DEC-\', \'GLON\', \'GLAT\', etc. in the first\nfour characters of ``CTYPEia`` but with trailing dashes removed.\n", 227); strncpy(doc_lng + 0, "``int`` (read-only)\n\nThe index into the sky coordinate array containing longitude values.\n", 90); strncpy(doc_lngtyp + 0, "``string`` (read-only)\n\nCelestial axis type for longitude, e.g. \"RA\", \"DEC\", \"GLON\", \"GLAT\",\netc. extracted from \'RA--\', \'DEC-\', \'GLON\', \'GLAT\', etc. in the first\nfour characters of ``CTYPEia`` but with trailing dashes removed.\n", 228); strncpy(doc_lonpole + 0, "``double``\n\nThe native longitude of the celestial pole, ``LONPOLEa`` (deg).\n", 76); strncpy(doc_m + 0, "``int`` (read-only)\n\nArray axis number for index vectors.\n", 58); strncpy(doc_map + 0, "``int array[M]``\n\nA vector of length `~pywcs._pywcs.Tabprm.M`\nthat defines the association between axis *m* in the *M*-dimensional\ncoordinate array (1 <= *m* <= *M*) and the indices of the intermediate world\ncoordinate and world coordinate arrays.\n\nWhen th", 256); strncpy(doc_map + 256, "e intermediate and world coordinate arrays contain the full\ncomplement of coordinate elements in image-order, as will usually be\nthe case, then ``map[m-1] == i-1`` for axis *i* in the *N*-dimensional\nimage (1 <= *i* <= *N*). In terms of the FITS keywords:", 256); strncpy(doc_map + 512, ":\n\n map[PVi_3a - 1] == i - 1.\n\nHowever, a different association may result if the intermediate\ncoordinates, for example, only contains a (relevant) subset of\nintermediate world coordinate elements. For example, if *M* == 1 for\nan image with *N* > 1, it", 256); strncpy(doc_map + 768, " is possible to fill the intermediate\ncoordinates with the relevant coordinate element with ``nelem`` set to\n1. In this case ``map[0] = 0`` regardless of the value of *i*.\n", 173); strncpy(doc_mix + 0, "mix(mixpix, mixcel, vspan, vstep, viter, world, pixcrd, origin)\n\nGiven either the celestial longitude or latitude plus an element of\nthe pixel coordinate, solves for the remaining elements by iterating\non the unknown celestial coordinate element using `~py", 256); strncpy(doc_mix + 256, "wcs.Wcsprm.s2p`.\n\n- *mixpix*: int. Which element on the pixel coordinate is given.\n\n- *mixcel*: int. Which element of the celestial coordinate is\n given. If mixcel* = ``1``, celestial longitude is given in\n ``world[self.lng]``, latitude returned in ``w", 256); strncpy(doc_mix + 512, "orld[self.lat]``. If\n *mixcel* = ``2``, celestial latitude is given in\n ``world[self.lat]``, longitude returned in ``world[self.lng]``.\n\n- *vspan*: pair of floats. Solution interval for the celestial\n coordinate, in degrees. The ordering of the two l", 256); strncpy(doc_mix + 768, "imits is\n irrelevant. Longitude ranges may be specified with any convenient\n normalization, for example ``(-120,+120)`` is the same as\n ``(240,480)``, except that the solution will be returned with the\n same normalization, i.e. lie within the interval", 256); strncpy(doc_mix + 1024, " specified.\n\n- *vstep*: float. Step size for solution search, in degrees. If\n ``0``, a sensible, although perhaps non-optimal default will be\n used.\n\n- *viter*: int. If a solution is not found then the step size will be\n halved and the search recomme", 256); strncpy(doc_mix + 1280, "nced. *viter* controls how many times\n the step size is halved. The allowed range is 5 - 10.\n\n- *world*: double array[naxis]. World coordinate elements.\n ``world[self.lng]`` and ``world[self.lat]`` are the celestial\n longitude and latitude, in degree", 256); strncpy(doc_mix + 1536, "s. Which is given and which\n returned depends on the value of *mixcel*. All other elements are\n given. The results will be written to this array in-place.\n\n- *pixcrd*: double array[naxis]. Pixel coordinate. The element\n indicated by *mixpix* is giv", 256); strncpy(doc_mix + 1792, "en and the remaining elements will be\n written in-place.\n\n\n- *origin*: int. Specifies the origin of pixel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns dictionary with the follo", 256); strncpy(doc_mix + 2048, "wing keys:\n\n- *phi* (double array[naxis])\n\n- *theta* (double array[naxis])\n\n - Longitude and latitude in the native coordinate system of the\n projection, in degrees.\n\n- *imgcrd* (double array[naxis])\n\n - Image coordinate elements. ``imgcrd[self.lng]`", 256); strncpy(doc_mix + 2304, "` and\n ``imgcrd[self.lat]`` are the projected *x*- and *y*-coordinates,\n in decimal degrees.\n\n- *world* (double array[naxis])\n\n - Another reference to the *world* argument passed in.\n\n**Exceptions:**\n\n- `MemoryError` Memory allocation failed.\n\n- `Si", 256); strncpy(doc_mix + 2560, "ngularMatrixError`: Linear transformation matrix is singular.\n\n- `InconsistentAxisTypesError`: Inconsistent or unrecognized\n coordinate axis types.\n\n- `ValueError`: Invalid parameter value.\n\n- `InvalidTransformError`: Invalid coordinate transformation\n p", 256); strncpy(doc_mix + 2816, "arameters.\n\n- `InvalidTransformError` Ill-conditioned coordinate transformation\n parameters.\n\n- `InvalidCoordinateError`: Invalid world coordinate.\n\n- `NoSolutionError`: No solution found in the specified interval.\n\n.. seealso::\n\n `~pywcs.Wcsprm.lat`, `", 256); strncpy(doc_mix + 3072, "~pywcs.Wcsprm.lng`\n\n.. note::\n\n Initially, the specified solution interval is checked to see if it\'s\n a \"crossing\" interval. If it isn\'t, a search is made for a crossing\n solution by iterating on the unknown celestial coordinate starting\n at the upper", 256); strncpy(doc_mix + 3328, " limit of the solution interval and decrementing by the\n specified step size. A crossing is indicated if the trial value of\n the pixel coordinate steps through the value specified. If a\n crossing interval is found then the solution is determined by a\n", 256); strncpy(doc_mix + 3584, " modified form of \"regula falsi\" division of the crossing interval.\n If no crossing interval was found within the specified solution\n interval then a search is made for a \"non-crossing\" solution as may\n arise from a point of tangency. The process is c", 256); strncpy(doc_mix + 3840, "omplicated by\n having to make allowance for the discontinuities that occur in all\n map projections.\n\n Once one solution has been determined others may be found by\n subsequent invocations of `~pywcs.Wcsprm.mix` with suitably\n restricted solution interv", 256); strncpy(doc_mix + 4096, "als.\n\n Note the circumstance that arises when the solution point lies at a\n native pole of a projection in which the pole is represented as a\n finite curve, for example the zenithals and conics. In such cases\n two or more valid solutions may exist but", 256); strncpy(doc_mix + 4352, " `~pywcs.Wcsprm.mix` only\n ever returns one.\n\n Because of its generality, `~pywcs.Wcsprm.mix` is very\n compute-intensive. For compute-limited applications, more efficient\n special-case solvers could be written for simple projections, for\n example non", 256); strncpy(doc_mix + 4608, "-oblique cylindrical projections.\n", 34); strncpy(doc_mjdavg + 0, "``double``\n\nModified Julian Date ``(MJD = JD - 2400000.5)``, ``MJD-AVG``,\ncorresponding to ``DATE-AVG``.\n\nAn undefined value is represented by NaN.\n\n.. seealso::\n\n `~pywcs.Wcsprm.mjdobs`\n", 189); strncpy(doc_mjdobs + 0, "``double``\n\nModified Julian Date ``(MJD = JD - 2400000.5)``, ``MJD-OBS``,\ncorresponding to ``DATE-OBS``.\n\nAn undefined value is represented by NaN.\n\n.. seealso::\n\n `~pywcs.Wcsprm.mjdavg`\n", 189); strncpy(doc_name + 0, "``string``\n\nThe name given to the coordinate representation ``WCSNAMEa``.\n", 74); strncpy(doc_naxis + 0, "``int`` (read-only)\n\nThe number of axes (pixel and coordinate), given by the ``NAXIS`` or\n``WCSAXESa`` keyvalues.\n\nThe number of coordinate axes is determined at parsing time, and can\nnot be subsequently changed.\n\nIt is determined from the highest of the f", 256); strncpy(doc_naxis + 256, "ollowing:\n\n 1. ``NAXIS``\n\n 2. ``WCSAXESa``\n\n 3. The highest axis number in any parameterized WCS keyword. The\n keyvalue, as well as the keyword, must be syntactically valid\n otherwise it will not be considered.\n\nIf none of these keyword types i", 256); strncpy(doc_naxis + 512, "s present, i.e. if the header only\ncontains auxiliary WCS keywords for a particular coordinate\nrepresentation, then no coordinate description is constructed for it.\n\nThis value may differ for different coordinate representations of the\nsame image.\n", 248); strncpy(doc_nc + 0, "``int`` (read-only)\n\nTotal number of coordinate vectors in the coordinate array being the\nproduct K_1 * K_2 * ... * K_M.\n", 121); strncpy(doc_ndim + 0, "``int`` (read-only)\n\nExpected dimensionality of the wcstab array.\n", 66); strncpy(doc_obsgeo + 0, "``double array[3]``\n\nLocation of the observer in a standard terrestrial reference frame,\n``OBSGEO-X``, ``OBSGEO-Y``, ``OBSGEO-Z`` (in meters).\n\nAn undefined value is represented by NaN.\n", 186); strncpy(doc_offset + 0, "``double``\n\nThe offset of the unit conversion.\n", 47); strncpy(doc_p0 + 0, "``int array[M]``\n\nVector of length `~pywcs._pywcs.Tabprm.M` of interpolated indices into\nthe coordinate array such that Upsilon_m, as defined in Paper III, is\nequal to ``(p0[m] + 1) + delta[m]``.\n", 196); strncpy(doc_p2s + 0, "p2s(pixcrd, origin)\n\nConverts pixel to sky coordinates.\n\n- *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates.\n\n\n- *origin*: int. Specifies the origin of pixel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use a", 256); strncpy(doc_p2s + 256, "rray indexing\n with origin at 0.\n\n\nReturns a dictionary with the following keys:\n\n- *imgcrd*: double array[ncoord][nelem]\n\n - Array of intermediate sky coordinates. For celestial axes,\n ``imgcrd[][self.lng]`` and ``imgcrd[][self.lat]`` are the\n pr", 256); strncpy(doc_p2s + 512, "ojected *x*-, and *y*-coordinates, in pseudo degrees. For\n spectral axes, ``imgcrd[][self.spec]`` is the intermediate\n spectral coordinate, in SI units.\n\n- *phi*: double array[ncoord]\n\n- *theta*: double array[ncoord]\n\n - Longitude and latitude in t", 256); strncpy(doc_p2s + 768, "he native coordinate system of the\n projection, in degrees.\n\n- *world*: double array[ncoord][nelem]\n\n - Array of sky coordinates. For celestial axes,\n ``world[][self.lng]`` and ``world[][self.lat]`` are the celestial\n longitude and latitude, in ", 256); strncpy(doc_p2s + 1024, "degrees. For spectral axes,\n ``world[][self.spec]`` is the intermediate spectral coordinate, in\n SI units.\n\n- *stat*: int array[ncoord]\n\n - Status return value for each coordinate. ``0`` for success,\n ``1+`` for invalid pixel coordinate.\n\n**Exce", 256); strncpy(doc_p2s + 1280, "ptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `SingularMatrixError`: Linear transformation matrix is singular.\n\n- `InconsistentAxisTypesError`: Inconsistent or unrecognized\n coordinate axis types.\n\n- `ValueError`: Invalid parameter value.\n\n- `V", 256); strncpy(doc_p2s + 1536, "alueError`: *x*- and *y*-coordinate arrays are not the same size.\n\n- `InvalidTransformError`: Invalid coordinate transformation\n parameters.\n\n- `InvalidTransformError`: Ill-conditioned coordinate transformation\n parameters.\n\n.. seealso::\n\n `~pywcs.Wcsp", 256); strncpy(doc_p2s + 1792, "rm.lat`, `~pywcs.Wcsprm.lng`\n", 29); strncpy(doc_p4_pix2foc + 0, "p4_pix2foc(*pixcrd, origin*) -> double array[ncoord][nelem]\n\nConvert pixel coordinates to focal plane coordinates using `Paper IV`_\nlookup-table distortion correction.\n\n- *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates.\n\n\n- *origin*: int", 256); strncpy(doc_p4_pix2foc + 256, ". Specifies the origin of pixel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns an array of focal plane coordinates.\n\n- `MemoryError`: Memory allocation failed.\n\n- `ValueError`: In", 256); strncpy(doc_p4_pix2foc + 512, "valid coordinate transformation parameters.\n", 44); strncpy(doc_pc + 0, "``double array[naxis][naxis]``\n\nThe ``PCi_ja`` (pixel coordinate) transformation matrix. The order is::\n\n [[PC1_1, PC1_2],\n [PC2_1, PC2_2]]\n\nFor historical compatibility, three alternate specifications of the\nlinear transforations are available in wcsl", 256); strncpy(doc_pc + 256, "ib. The canonical\n``PCi_ja`` with ``CDELTia``, ``CDi_ja``, and the deprecated\n``CROTAia`` keywords. Although the latter may not formally co-exist\nwith ``PCi_ja``, the approach here is simply to ignore them if given\nin conjunction with ``PCi_ja``.\n\n`~pywc", 256); strncpy(doc_pc + 512, "s.Wcsprm.has_pc`, `~pywcs.Wcsprm.has_cd` and\n`~pywcs.Wcsprm.has_crota` can be used to determine which of these\nalternatives are present in the header.\n\nThese alternate specifications of the linear transformation matrix are\ntranslated immediately to ``PCi_j", 256); strncpy(doc_pc + 768, "a`` by `~pywcs.Wcsprm.set` and are\nnowhere visible to the lower-level routines. In particular,\n`~pywcs.Wcsprm.set` resets `~pywcs.Wcsprm.cdelt` to unity if\n``CDi_ja`` is present (and no ``PCi_ja``). If no ``CROTAia`` is\nassociated with the latitude axis,", 256); strncpy(doc_pc + 1024, " `set` reverts to a unity ``PCi_ja``\nmatrix.\n", 45); strncpy(doc_phi0 + 0, "``double``\n\nThe native latitude of the fiducial point, i.e. the point whose\ncelestial coordinates are given in ``ref[1:2]``. If undefined (NaN)\nthe initialization routine, `~pywcs.Wcsprm.set`, will set this to a\nprojection-specific default.\n\n.. seealso::\n", 256); strncpy(doc_phi0 + 256, "\n `~pywcs.Wcsprm.theta0`\n", 27); strncpy(doc_pix2foc + 0, "pix2foc(*pixcrd, origin*) -> double array[ncoord][nelem]\n\nPerform both `SIP`_ polynomial and `Paper IV`_ lookup-table distortion\ncorrection in parallel.\n\n- *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates.\n\n\n- *origin*: int. Specifies the", 256); strncpy(doc_pix2foc + 256, " origin of pixel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns an array of focal plane coordinates.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `ValueError`: ", 256); strncpy(doc_pix2foc + 512, "Invalid coordinate transformation parameters.\n", 46); strncpy(doc_piximg_matrix + 0, "``double array[2][2]`` (read-only)\n\nMatrix containing the product of the ``CDELTia`` diagonal matrix and\nthe ``PCi_ja`` matrix.\n", 128); strncpy(doc_power + 0, "``double``\n\nThe exponent of the unit conversion.\n", 49); strncpy(doc_print_contents + 0, "print_contents()\n\nPrint the contents of the `~pywcs.Wcsprm` object to stdout. Probably\nonly useful for debugging purposes, and may be removed in the future.\n\nTo get a string of the contents, use `repr`.\n", 204); strncpy(doc_print_contents_tabprm + 0, "print_contents()\n\nPrint the contents of the `~pywcs._pywcs.Tabprm` object to stdout.\nProbably only useful for debugging purposes, and may be removed in the\nfuture.\n\nTo get a string of the contents, use `repr`.\n", 210); strncpy(doc_radesys + 0, "``string``\n\nThe equatorial or ecliptic coordinate system type, ``RADESYSa``.\n", 77); strncpy(doc_restfrq + 0, "``double``\n\nRest frequency (Hz) from ``RESTFRQa``.\n\nAn undefined value is represented by NaN.\n", 94); strncpy(doc_restwav + 0, "``double``\n\nRest wavelength (m) from ``RESTWAVa``.\n\nAn undefined value is represented by NaN.\n", 94); strncpy(doc_row + 0, "``int`` (read-only)\n\nTable row number.\n", 39); strncpy(doc_s2p + 0, "s2p(sky, origin)\n\nTransforms sky coordinates to pixel coordinates.\n\n- *sky*: double array[ncoord][nelem]. Array of sky coordinates, in\n decimal degrees.\n\n\n- *origin*: int. Specifies the origin of pixel values. The Fortran and\n FITS standards use an ori", 256); strncpy(doc_s2p + 256, "gin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns a dictionary with the following keys:\n\n- *phi*: double array[ncoord]\n\n- *theta*: double array[ncoord]\n\n - Longitude and latitude in the native coordinate system of the\n projection,", 256); strncpy(doc_s2p + 512, " in degrees.\n\n- *imgcrd*: double array[ncoord][nelem]\n\n - Array of intermediate sky coordinates. For celestial axes,\n ``imgcrd[][self.lng]`` and ``imgcrd[][self.lat]`` are the\n projected *x*-, and *y*-coordinates, in pseudo \"degrees\". For\n quad", 256); strncpy(doc_s2p + 768, "cube projections with a ``CUBEFACE`` axis, the face number is\n also returned in ``imgcrd[][self.cubeface]``. For spectral axes,\n ``imgcrd[][self.spec]`` is the intermediate spectral coordinate,\n in SI units.\n\n- *pixcrd*: double array[ncoord][nele", 256); strncpy(doc_s2p + 1024, "m]\n\n - Array of pixel coordinates. Pixel coordinates are\n zero-based.\n\n- *stat*: int array[ncoord]\n\n - Status return value for each coordinate. ``0`` for\n success, ``1+`` for invalid pixel coordinate.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allo", 256); strncpy(doc_s2p + 1280, "cation failed.\n\n- `SingularMatrixError`: Linear transformation matrix is singular.\n\n- `InconsistentAxisTypesError` Inconsistent or unrecognized coordinate\n axis types.\n\n- `ValueError`: Invalid parameter value.\n\n- `InvalidTransformError`: Invalid coordinat", 256); strncpy(doc_s2p + 1536, "e transformation\n parameters.\n\n- `InvalidTransformError`: Ill-conditioned coordinate transformation\n parameters.\n\n.. seealso::\n\n `~pywcs.Wcsprm.lat`, `~pywcs.Wcsprm.lng`\n", 174); strncpy(doc_scale + 0, "``double``\n\nThe scaling factor for the unit conversion.\n", 56); strncpy(doc_sense + 0, "``int array[M]``\n\nA vector of length `~pywcs._pywcs.Tabprm.M` whose elements indicate\nwhether the corresponding indexing vector is monotonically increasing\n(+1), or decreasing (-1).\n", 182); strncpy(doc_set + 0, "set()\n\nSets up a WCS object for use according to information supplied within\nit.\n\nNote that this routine need not be called directly; it will be invoked\nby `~pywcs.Wcsprm.p2s` and `~pywcs.Wcsprm.s2p` if necessary.\n\nSome attributes that are based on other a", 256); strncpy(doc_set + 256, "ttributes (such as\n`~pywcs.Wcsprm.lattyp` on `~pywcs.Wcsprm.ctype`) may not be correct\nuntil after `~pywcs.Wcsprm.set` is called.\n\n`~pywcs.Wcsprm.set` strips off trailing blanks in all string members.\n\n`~pywcs.Wcsprm.set` recognizes the ``NCP`` projection ", 256); strncpy(doc_set + 512, "and converts it\nto the equivalent ``SIN`` projection and it also recognizes ``GLS`` as\na synonym for ``SFL``. It does alias translation for the AIPS\nspectral types (``FREQ-LSR``, ``FELO-HEL``, etc.) but without changing\nthe input header keywords.\n\n**Excep", 256); strncpy(doc_set + 768, "tions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `SingularMatrixError`: Linear transformation matrix is singular.\n\n- `InconsistentAxisTypesError`: Inconsistent or unrecognized\n coordinate axis types.\n\n- `ValueError`: Invalid parameter value.\n\n- `In", 256); strncpy(doc_set + 1024, "validTransformError`: Invalid coordinate transformation\n parameters.\n\n- `InvalidTransformError`: Ill-conditioned coordinate transformation\n parameters.\n", 154); strncpy(doc_set_ps + 0, "set_ps(list)\n\nSets `PSi_ma` keywords for each *i* and *m*. The input must be a\nsequence of tuples of the form (*i*, *m*, *value*):\n\n - *i*: int. Axis number, as in ``PSi_ma``, (i.e. 1-relative)\n\n - *m*: int. Parameter number, as in ``PSi_ma``, (i.", 256); strncpy(doc_set_ps + 256, "e. 0-relative)\n\n - *value*: string. Parameter value.\n\n.. seealso::\n\n `~pywcs.Wcsprm.get_ps`\n", 98); strncpy(doc_set_pv + 0, "set_pv(list)\n\nSets `PVi_ma` keywords for each *i* and *m*. The input must be a\nsequence of tuples of the form (*i*, *m*, *value*):\n\n - *i*: int. Axis number, as in ``PVi_ma``, (i.e. 1-relative)\n\n - *m*: int. Parameter number, as in ``PVi_ma``, (i.", 256); strncpy(doc_set_pv + 256, "e. 0-relative)\n\n - *value*: float. Parameter value.\n\n.. seealso::\n\n `~pywcs.Wcsprm.get_pv`\n", 97); strncpy(doc_set_tabprm + 0, "set()\n\nAllocates memory for work arrays in the Tabprm class and sets up\nthe class according to information supplied within it.\n\nNote that this routine need not be called directly; it will be invoked by\nfunctions that need it.\n\n**Exceptions:**\n\n- `MemoryErr", 256); strncpy(doc_set_tabprm + 256, "or`: Memory allocation failed.\n\n- `InvalidTabularParameters`: Invalid tabular parameters.\n", 90); strncpy(doc_sip + 0, "Get/set the `~pywcs.Sip` object for performing `SIP`_ distortion\ncorrection.\n", 77); strncpy(doc_sip_foc2pix + 0, "sip_foc2pix(*foccrd, origin*) -> double array[ncoord][nelem]\n\nConvert focal plane coordinates to pixel coordinates using the `SIP`_\npolynomial distortion convention.\n\n- *foccrd*: double array[ncoord][nelem]. Array of focal plane\n coordinates.\n\n\n- *origin", 256); strncpy(doc_sip_foc2pix + 256, "*: int. Specifies the origin of pixel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns an array of pixel coordinates.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n-", 256); strncpy(doc_sip_foc2pix + 512, " `ValueError`: Invalid coordinate transformation parameters.\n", 61); strncpy(doc_sip_pix2foc + 0, "sip_pix2foc(*pixcrd, origin*) -> double array[ncoord][nelem]\n\nConvert pixel coordinates to focal plane coordinates using the `SIP`_\npolynomial distortion convention.\n\n- *pixcrd*: double array[ncoord][nelem]. Array of pixel coordinates.\n\n\n- *origin*: int. ", 256); strncpy(doc_sip_pix2foc + 256, "Specifies the origin of pixel values. The Fortran and\n FITS standards use an origin of 1. Numpy and C use array indexing\n with origin at 0.\n\n\nReturns an array of focal plane coordinates.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `", 256); strncpy(doc_sip_pix2foc + 512, "ValueError`: Invalid coordinate transformation parameters.\n", 59); strncpy(doc_spcfix + 0, "spcfix() -> int\n\nTranslates AIPS-convention spectral coordinate types. {``FREQ``,\n``VELO``, ``FELO``}-{``OBS``, ``HEL``, ``LSR``} (e.g. ``FREQ-LSR``,\n``VELO-OBS``, ``FELO-HEL``)\n\nReturns ``0`` for success; ``-1`` if no change required.\n", 237); strncpy(doc_spec + 0, "``int`` (read-only)\n\nThe index containing the spectral axis values.\n", 68); strncpy(doc_specsys + 0, "``string``\n\nSpectral reference frame (standard of rest), ``SPECSYSa``.\n\n.. seealso::\n\n `~pywcs.Wcsprm.ssysobs`, `~pywcs.Wcsprm.velosys`.\n", 139); strncpy(doc_sptr + 0, "sptr(ctype, i=-1)\n\nTranslates the spectral axis in a WCS object. For example, a ``FREQ``\naxis may be translated into ``ZOPT-F2W`` and vice versa.\n\n- *ctype*: string. Required spectral ``CTYPEia``, maximum of 8\n characters. The first four characters are", 256); strncpy(doc_sptr + 256, " required to be given and\n are never modified. The remaining four, the algorithm code, are\n completely determined by, and must be consistent with, the first\n four characters. Wildcarding may be used, i.e. if the final three\n characters are specified", 256); strncpy(doc_sptr + 512, " as ``\"???\"``, or if just the eighth\n character is specified as ``\"?\"``, the correct algorithm code will\n be substituted and returned.\n\n- *i*: int. Index of the spectral axis (0-relative). If ``i < 0`` (or not\n provided), it will be set to the first s", 256); strncpy(doc_sptr + 768, "pectral axis identified\n from the ``CTYPE`` keyvalues in the FITS header.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `SingularMatrixError`: Linear transformation matrix is singular.\n\n- `InconsistentAxisTypesError`: Inconsistent or unr", 256); strncpy(doc_sptr + 1024, "ecognized\n coordinate axis types.\n\n- `ValueError`: Invalid parameter value.\n\n- `InvalidTransformError`: Invalid coordinate transformation\n parameters.\n\n- `InvalidTransformError`: Ill-conditioned coordinate transformation\n parameters.\n\n- `InvalidSubimage", 256); strncpy(doc_sptr + 1280, "SpecificationError`: Invalid subimage specification\n (no spectral axis).\n", 74); strncpy(doc_ssysobs + 0, "``string``\n\nThe actual spectral reference frame in which there is no differential\nvariation in the spectral coordinate across the field-of-view,\n``SSYSOBSa``.\n\n.. seealso::\n\n `~pywcs.Wcsprm.specsys`, `~pywcs.Wcsprm.velosys`\n", 226); strncpy(doc_ssyssrc + 0, "``string``\n\nThe spectral reference frame (standard of rest) in which the redshift\nwas measured, ``SSYSSRCa``.\n", 110); strncpy(doc_sub + 0, "sub(axes)\n\nExtracts the coordinate description for a subimage from a `~pywcs.WCS`\nobject.\n\nThe world coordinate system of the subimage must be separable in the\nsense that the world coordinates at any point in the subimage must\ndepend only on the pixel coor", 256); strncpy(doc_sub + 256, "dinates of the axes extracted. In\npractice, this means that the ``PCi_ja`` matrix of the original image\nmust not contain non-zero off-diagonal terms that associate any of the\nsubimage axes with any of the non-subimage axes.\n\n`sub` can also add axes to a w", 256); strncpy(doc_sub + 512, "csprm struct. The new axes will be\ncreated using the defaults set by the Wcsprm constructor which produce\na simple, unnamed, linear axis with world coordinates equal to the\npixel coordinate. These default values can be changed before\ninvoking `set`.\n\nNo ", 256); strncpy(doc_sub + 768, "checks are performed to verify that the coordinate axes are\nconsistent, that is done by `set`.\n\n- *axes*: int or a sequence.\n\n - If an int, include the first *N* axes in their original\n order.\n\n - If a sequence, may contain a combination of image axis", 256); strncpy(doc_sub + 1024, " numbers\n (1-relative) or special axis identifiers (see below). Order is\n significant; ``axes[0]`` is the axis number of the input image\n that corresponds to the first axis in the subimage, etc. Use an\n axis number of 0 to create a new axis u", 256); strncpy(doc_sub + 1280, "sing the defaults.\n\n - If ``0``, ``[]`` or ``None``, do a deep copy.\n\nCoordinate axes types may be specified using either strings or\nspecial integer constants. The available types are:\n\n - ``\'longitude\'`` / ``WCSSUB_LONGITUDE``: Celestial longitude\n\n -", 256); strncpy(doc_sub + 1536, " ``\'latitude\'`` / ``WCSSUB_LATITUDE``: Celestial latitude\n\n - ``\'cubeface\'`` / ``WCSSUB_CUBEFACE``: Quadcube ``CUBEFACE`` axis\n\n - ``\'spectral\'`` / ``WCSSUB_SPECTRAL``: Spectral axis\n\n - ``\'stokes\'`` / ``WCSSUB_STOKES``: Stokes axis\n\n - ``\'celestial\'``", 256); strncpy(doc_sub + 1792, " / ``WCSSUB_CELESTIAL``: An alias for the\n combination of ``\'longitude\'``, ``\'latitude\'`` and ``\'cubeface\'``.\n\nReturns a `~pywcs.WCS` object, which is a deep copy of the original\nobject.\n\n**Exceptions:**\n\n- `MemoryError`: Memory allocation failed.\n\n- `I", 256); strncpy(doc_sub + 2048, "nvalidSubimageSpecificationError`: Invalid subimage specification\n (no spectral axis).\n\n- `NonseparableSubimageCoordinateSystem`: Non-separable subimage\n coordinate system.\n\n.. note::\n\n Combinations of subimage axes of particular types may be extracted\n", 256); strncpy(doc_sub + 2304, " in the same order as they occur in the input image by combining the\n integer constants with the \'binary or\' (``|``) operator. For\n example::\n\n wcs.sub([WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_SPECTRAL])\n\n would extract the longitude, latitude,", 256); strncpy(doc_sub + 2560, " and spectral axes in the same\n order as the input image. If one of each were present, the\n resulting object would have three dimensions.\n\n For convenience, ``WCSSUB_CELESTIAL`` is defined as the combination\n ``WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCS", 256); strncpy(doc_sub + 2816, "SUB_CUBEFACE``.\n\n The codes may also be negated to extract all but the types\n specified, for example::\n\n wcs.sub([\n WCSSUB_LONGITUDE,\n WCSSUB_LATITUDE,\n WCSSUB_CUBEFACE,\n -(WCSSUB_SPECTRAL | WCSSUB_STOKES)])\n\n The last of these sp", 256); strncpy(doc_sub + 3072, "ecifies all axis types other than spectral or\n Stokes. Extraction is done in the order specified by `axes`, i.e. a\n longitude axis (if present) would be extracted first (via\n ``axes[0]``) and not subsequently (via ``axes[3]``). Likewise for\n the lati", 256); strncpy(doc_sub + 3328, "tude and cubeface axes in this example.\n\n The number of dimensions in the returned object may be less than or\n greater than the length of `axes`. However, it will never exceed\n the number of axes in the input image.\n", 220); strncpy(doc_tab + 0, "``list of Tabprm``\n\nA list of tabular coordinate objects associated with this WCS.\n", 83); strncpy(doc_theta0 + 0, "``double``\n\nThe native longitude of the fiducial point, i.e. the point whose\ncelestial coordinates are given in ``ref[1:2]``. If undefined (NaN)\nthe initialization routine, `~pywcs.Wcsprm.set`, will set this to a\nprojection-specific default.\n\n.. seealso::", 256); strncpy(doc_theta0 + 256, "\n\n `~pywcs.Wcsprm.phi0`\n", 26); strncpy(doc_to_header + 0, "to_header(relax=False)\n\n`to_header` translates a WCS object into a FITS header.\n\n - If the `~pywcs.Wcsprm.colnum` member is non-zero then a binary\n table image array header will be produced.\n\n - Otherwise, if the `~pywcs.Wcsprm.colax` member is ", 256); strncpy(doc_to_header + 256, "set non-zero\n then a pixel list header will be produced.\n\n - Otherwise, a primary image or image extension header will be\n produced.\n\nThe output header will almost certainly differ from the input in a\nnumber of respects:\n\n 1. The output hea", 256); strncpy(doc_to_header + 512, "der only contains WCS-related keywords. In\n particular, it does not contain syntactically-required keywords\n such as ``SIMPLE``, ``NAXIS``, ``BITPIX``, or ``END``.\n\n 2. Deprecated (e.g. ``CROTAn``) or non-standard usage will be\n trans", 256); strncpy(doc_to_header + 768, "lated to standard (this is partially dependent on whether\n `fix` was applied).\n\n 3. Quantities will be converted to the units used internally,\n basically SI with the addition of degrees.\n\n 4. Floating-point quantities may be given to a di", 256); strncpy(doc_to_header + 1024, "fferent decimal\n precision.\n\n 5. Elements of the ``PCi_j`` matrix will be written if and only if\n they differ from the unit matrix. Thus, if the matrix is unity\n then no elements will be written.\n\n 6. Additional keywords such as ``", 256); strncpy(doc_to_header + 1280, "WCSAXES``, ``CUNITia``,\n ``LONPOLEa`` and ``LATPOLEa`` may appear.\n\n 7. The original keycomments will be lost, although\n `~pywcs.Wcsprm.to_header` tries hard to write meaningful\n comments.\n\n 8. Keyword order may be changed.\n\nKeyword", 256); strncpy(doc_to_header + 1536, "s can be translated between the image array, binary table, and\npixel lists forms by manipulating the `~pywcs.Wcsprm.colnum` or\n`~pywcs.Wcsprm.colax` members of the `~pywcs.Wcsprm.WCS` object.\n\n- *relax*: Degree of permissiveness:\n\n - `False`: Recognize ", 256); strncpy(doc_to_header + 1792, "only FITS keywords defined by the published\n WCS standard.\n\n - `True`: Admit all recognized informal extensions of the WCS\n standard.\n\n - `int`: a bit field selecting specific extensions to write.\n See :ref:`relaxwrite` for details.\n\nR", 256); strncpy(doc_to_header + 2048, "eturns a raw FITS header as a string.\n", 38); strncpy(doc_ttype + 0, "``str`` (read-only)\n\n``TTYPEn`` identifying the column of the binary table that contains\nthe wcstab array.\n", 107); strncpy(doc_unitfix + 0, "unitfix(translate_units=\'\')\n\nTranslates non-standard ``CUNITia`` keyvalues. For example, ``DEG`` ->\n``deg``, also stripping off unnecessary whitespace.\n\n- *translate_units*: string. Do potentially unsafe translations of\n non-standard unit strings.\n\n Al", 256); strncpy(doc_unitfix + 256, "though ``\"S\"`` is commonly used to represent seconds, its\n recognizes ``\"S\"`` formally as Siemens, however rarely that may be\n translation to ``\"s\"`` is potentially unsafe since the standard\n used. The same applies to ``\"H\"`` for hours (Henry), and ``\"", 256); strncpy(doc_unitfix + 512, "D\"``\n for days (Debye).\n\n This string controls what to do in such cases, and is\n case-insensitive.\n\n - If the string contains ``\"s\"``, translate ``\"S\"`` to ``\"s\"``.\n\n - If the string contains ``\"h\"``, translate ``\"H\"`` to ``\"h\"``.\n\n - If the string c", 256); strncpy(doc_unitfix + 768, "ontains ``\"d\"``, translate ``\"D\"`` to ``\"d\"``.\n\n Thus ``\'\'`` doesn\'t do any unsafe translations, whereas ``\'shd\'``\n does all of them.\n\n See :ref:`fits-unit` for more information.\n\nReturns ``0`` for success; ``-1`` if no change required.\n", 240); strncpy(doc_velangl + 0, "``double``\n\nThe angle in degrees that should be used to decompose an observed\nvelocity into radial and transverse components.\n\nAn undefined value is represented by NaN.\n", 169); strncpy(doc_velosys + 0, "``double``\n\nThe relative radial velocity (m/s) between the observer and the\nselected standard of rest in the direction of the celestial reference\ncoordinate, ``VELOSYSa``.\n\nAn undefined value is represented by NaN.\n\n.. seealso::\n\n `~pywcs.Wcsprm.specsys`", 256); strncpy(doc_velosys + 256, ", `~pywcs.Wcsprm.ssysobs`\n", 26); strncpy(doc_want + 0, "The name of the unit being converted to.\n\nThis value always uses standard unit names, even if the\n`UnitConverter` was initialized with a non-standard unit name.\n", 161); strncpy(doc_wcs + 0, "A `~pywcs.Wcsprm` object to perform the basic `wcslib`_ WCS\ntranformation.\n", 75); strncpy(doc_zsource + 0, "``double``\n\nThe redshift, ``ZSOURCEa``, of the source.\n\nAn undefined value is represented by NaN.\n", 98); } pywcs-1.12/src/docstrings.h0000644001153600020070000000772112310355701017766 0ustar cslocumSTSCI\science00000000000000 /* DO NOT EDIT! This file is autogenerated by setup.p. To edit its contents, edit doc/docstrings.py */ #ifndef __DOCSTRINGS_H__ #define __DOCSTRINGS_H__ void fill_docstrings(void); extern char doc_DistortionLookupTable[369]; extern char doc_K[152]; extern char doc_M[56]; extern char doc_Sip[1017]; extern char doc_Tabprm[226]; extern char doc_UnitConverter[2216]; extern char doc_Wcs[482]; extern char doc_Wcsprm[1979]; extern char doc_Wtbarr[195]; extern char doc_a[222]; extern char doc_a_order[94]; extern char doc_all_pix2sky[1204]; extern char doc_alt[236]; extern char doc_ap[225]; extern char doc_ap_order[96]; extern char doc_axis_types[916]; extern char doc_b[222]; extern char doc_b_order[94]; extern char doc_bp[225]; extern char doc_bp_order[96]; extern char doc_cd[1002]; extern char doc_cdelt[302]; extern char doc_cel_offset[153]; extern char doc_celfix[136]; extern char doc_cname[76]; extern char doc_colax[91]; extern char doc_colnum[235]; extern char doc_convert[120]; extern char doc_coord[278]; extern char doc_copy[39]; extern char doc_cpdis1[99]; extern char doc_cpdis2[99]; extern char doc_crder[123]; extern char doc_crota[998]; extern char doc_crpix[88]; extern char doc_crval[93]; extern char doc_crval_tabprm[131]; extern char doc_csyer[132]; extern char doc_ctype[222]; extern char doc_cubeface[1209]; extern char doc_cunit[1161]; extern char doc_cylfix[127]; extern char doc_data[72]; extern char doc_data_wtbarr[51]; extern char doc_dateavg[146]; extern char doc_dateobs[127]; extern char doc_datfix[453]; extern char doc_delta[195]; extern char doc_det2im[57]; extern char doc_det2im1[96]; extern char doc_det2im2[96]; extern char doc_dims[98]; extern char doc_equinox[242]; extern char doc_extlev[72]; extern char doc_extnam[73]; extern char doc_extrema[439]; extern char doc_extver[72]; extern char doc_find_all_wcs[846]; extern char doc_fix[1382]; extern char doc_get_cdelt[446]; extern char doc_get_offset[103]; extern char doc_get_pc[385]; extern char doc_get_ps[363]; extern char doc_get_pv[647]; extern char doc_has_cd[859]; extern char doc_has_cdi_ja[96]; extern char doc_has_crota[614]; extern char doc_has_crotaia[101]; extern char doc_has_pc[176]; extern char doc_has_pci_ja[96]; extern char doc_have[163]; extern char doc_i[40]; extern char doc_imgpix_matrix[143]; extern char doc_is_unity[102]; extern char doc_kind[129]; extern char doc_lat[89]; extern char doc_latpole[75]; extern char doc_lattyp[227]; extern char doc_lng[90]; extern char doc_lngtyp[228]; extern char doc_lonpole[76]; extern char doc_m[58]; extern char doc_map[941]; extern char doc_mix[4642]; extern char doc_mjdavg[189]; extern char doc_mjdobs[189]; extern char doc_name[74]; extern char doc_naxis[760]; extern char doc_nc[121]; extern char doc_ndim[66]; extern char doc_obsgeo[186]; extern char doc_offset[47]; extern char doc_p0[196]; extern char doc_p2s[1821]; extern char doc_p4_pix2foc[556]; extern char doc_pc[1069]; extern char doc_phi0[283]; extern char doc_pix2foc[558]; extern char doc_piximg_matrix[128]; extern char doc_power[49]; extern char doc_print_contents[204]; extern char doc_print_contents_tabprm[210]; extern char doc_radesys[77]; extern char doc_restfrq[94]; extern char doc_restwav[94]; extern char doc_row[39]; extern char doc_s2p[1710]; extern char doc_scale[56]; extern char doc_sense[182]; extern char doc_set[1178]; extern char doc_set_ps[354]; extern char doc_set_pv[353]; extern char doc_set_tabprm[346]; extern char doc_sip[77]; extern char doc_sip_foc2pix[573]; extern char doc_sip_pix2foc[571]; extern char doc_spcfix[237]; extern char doc_spec[68]; extern char doc_specsys[139]; extern char doc_sptr[1354]; extern char doc_ssysobs[226]; extern char doc_ssyssrc[110]; extern char doc_sub[3548]; extern char doc_tab[83]; extern char doc_theta0[282]; extern char doc_to_header[2086]; extern char doc_ttype[107]; extern char doc_unitfix[1008]; extern char doc_velangl[169]; extern char doc_velosys[282]; extern char doc_want[161]; extern char doc_wcs[75]; extern char doc_zsource[98]; #endif pywcs-1.12/src/isnan.h0000644001153600020070000000223612310355626016721 0ustar cslocumSTSCI\science00000000000000#ifndef __ISNAN_H__ #define __ISNAN_H__ #include "wcsconfig.h" typedef unsigned WCSLIB_INT64 Int64; #if !defined(U64) #define U64(u) (* (Int64 *) &(u) ) #endif /* U64 */ #if !defined(isnan64) #if !defined(_MSC_VER) #define isnan64(u) \ ( (( U64(u) & 0x7ff0000000000000LL) == 0x7ff0000000000000LL) && ((U64(u) & 0x000fffffffffffffLL) != 0)) ? 1:0 #else #define isnan64(u) \ ( (( U64(u) & 0x7ff0000000000000i64) == 0x7ff0000000000000i64) && ((U64(u) & 0x000fffffffffffffi64) != 0)) ? 1:0 #endif #endif /* isnan64 */ #if !defined(isinf64) #if !defined(_MSC_VER) #define isinf64(u) \ ( (( U64(u) & 0x7ff0000000000000LL) == 0x7ff0000000000000LL) && ((U64(u) & 0x000fffffffffffffLL) == 0)) ? 1:0 #else #define isinf64(u) \ ( (( U64(u) & 0x7ff0000000000000i64) == 0x7ff0000000000000i64) && ((U64(u) & 0x000fffffffffffffi64) == 0)) ? 1:0 #endif #endif /* isinf64 */ #if !defined(isfinite64) #if !defined(_MSC_VER) #define isfinite64(u) \ ( (( U64(u) & 0x7ff0000000000000LL) != 0x7ff0000000000000LL)) ? 1:0 #else #define isfinite64(u) \ ( (( U64(u) & 0x7ff0000000000000i64) != 0x7ff0000000000000i64)) ? 1:0 #endif #endif /* isfinite64 */ #endif /* __ISNAN_H__ */ pywcs-1.12/src/pipeline.c0000644001153600020070000001714712310355626017420 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #include "pipeline.h" #include "util.h" #include #include #include #define PIP_ERRMSG(status) WCSERR_SET(status) void pipeline_clear( pipeline_t* pipeline) { pipeline->det2im[0] = NULL; pipeline->det2im[1] = NULL; pipeline->sip = NULL; pipeline->cpdis[0] = NULL; pipeline->cpdis[1] = NULL; pipeline->wcs = NULL; pipeline->err = NULL; } void pipeline_init( pipeline_t* pipeline, /*@shared@*/ distortion_lookup_t** det2im /* [2] */, /*@shared@*/ sip_t* sip, /*@shared@*/ distortion_lookup_t** cpdis /* [2] */, /*@shared@*/ struct wcsprm* wcs) { pipeline->det2im[0] = det2im[0]; pipeline->det2im[1] = det2im[1]; pipeline->sip = sip; pipeline->cpdis[0] = cpdis[0]; pipeline->cpdis[1] = cpdis[1]; pipeline->wcs = wcs; pipeline->err = NULL; } void pipeline_free( pipeline_t* pipeline) { free(pipeline->err); pipeline->err = NULL; } int pipeline_all_pixel2world( pipeline_t* pipeline, const unsigned int ncoord, const unsigned int nelem, const double* const pixcrd /* [ncoord][nelem] */, double* world /* [ncoord][nelem] */) { static const char* function = "pipeline_all_pixel2world"; const double* wcs_input = NULL; double* wcs_output = NULL; int has_det2im; int has_sip; int has_p4; int has_wcs; int status = 1; struct wcserr **err; /* Temporary buffer for performing WCS calculations */ unsigned char* buffer = NULL; unsigned char* mem = NULL; /*@null@*/ double* tmp; /*@null@*/ double* imgcrd; /*@null@*/ double* phi; /*@null@*/ double* theta; /*@null@*/ int* stat; if (pipeline == NULL || pixcrd == NULL || world == NULL) { return WCSERR_NULL_POINTER; } err = &(pipeline->err); has_det2im = pipeline->det2im[0] != NULL || pipeline->det2im[1] != NULL; has_sip = pipeline->sip != NULL; has_p4 = pipeline->cpdis[0] != NULL || pipeline->cpdis[1] != NULL; has_wcs = pipeline->wcs != NULL; if (has_det2im || has_sip || has_p4) { if (nelem != 2) { status = wcserr_set( PIP_ERRMSG(WCSERR_BAD_COORD_TRANS), "Data must be 2-dimensional when Paper IV lookup table or SIP transform is present."); goto exit; } } if (has_wcs) { buffer = mem = malloc( ncoord * nelem * sizeof(double) + /* imgcrd */ ncoord * sizeof(double) + /* phi */ ncoord * sizeof(double) + /* theta */ ncoord * nelem * sizeof(double) + /* tmp */ ncoord * nelem * sizeof(int) /* stat */ ); if (buffer == NULL) { status = wcserr_set( PIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } imgcrd = (double *)mem; mem += ncoord * nelem * sizeof(double); phi = (double *)mem; mem += ncoord * sizeof(double); theta = (double *)mem; mem += ncoord * sizeof(double); tmp = (double *)mem; mem += ncoord * nelem * sizeof(double); stat = (int *)mem; /* mem += ncoord * nelem * sizeof(int); */ if (has_det2im || has_sip || has_p4) { status = pipeline_pix2foc(pipeline, ncoord, nelem, pixcrd, tmp); if (status != 0) { goto exit; } wcs_input = tmp; wcs_output = world; } else { wcs_input = pixcrd; wcs_output = world; } if ((status = wcsp2s(pipeline->wcs, (int)ncoord, (int)nelem, wcs_input, imgcrd, phi, theta, wcs_output, stat))) { wcserr_copy(pipeline->wcs->err, pipeline->err); } if (status == 8) { set_invalid_to_nan((int)ncoord, (int)nelem, wcs_output, stat); } } else { if (has_det2im || has_sip || has_p4) { status = pipeline_pix2foc(pipeline, ncoord, nelem, pixcrd, world); } } exit: free(buffer); return status; } int pipeline_pix2foc( pipeline_t* pipeline, const unsigned int ncoord, const unsigned int nelem, const double* const pixcrd /* [ncoord][nelem] */, double* foc /* [ncoord][nelem] */) { static const char* function = "pipeline_pix2foc"; int has_det2im; int has_sip; int has_p4; const double * input = NULL; double * tmp = NULL; int status = 1; struct wcserr **err; assert(nelem == 2); assert(pixcrd != foc); if (pipeline == NULL || pixcrd == NULL || foc == NULL) { return WCSERR_NULL_POINTER; } err = &(pipeline->err); has_det2im = pipeline->det2im[0] != NULL || pipeline->det2im[1] != NULL; has_sip = pipeline->sip != NULL; has_p4 = pipeline->cpdis[0] != NULL || pipeline->cpdis[1] != NULL; if (has_det2im) { if (has_sip || has_p4) { tmp = malloc(ncoord * nelem * sizeof(double)); if (tmp == NULL) { status = wcserr_set( PIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } memcpy(tmp, pixcrd, sizeof(double) * ncoord * nelem); status = p4_pix2deltas(2, (void*)pipeline->det2im, ncoord, pixcrd, tmp); if (status) { wcserr_set(PIP_ERRMSG(WCSERR_NULL_POINTER), "NULL pointer passed"); goto exit; } input = tmp; memcpy(foc, input, sizeof(double) * ncoord * nelem); } else { memcpy(foc, pixcrd, sizeof(double) * ncoord * nelem); status = p4_pix2deltas(2, (void*)pipeline->det2im, ncoord, pixcrd, foc); if (status) { wcserr_set(PIP_ERRMSG(WCSERR_NULL_POINTER), "NULL pointer passed"); goto exit; } } } else { /* Copy pixcrd to foc as a starting point. The "deltas" functions below will undistort from there */ memcpy(foc, pixcrd, sizeof(double) * ncoord * nelem); input = pixcrd; } if (has_sip) { status = sip_pix2deltas(pipeline->sip, 2, ncoord, input, foc); if (status) { wcserr_copy(pipeline->sip->err, pipeline->err); goto exit; } } if (has_p4) { status = p4_pix2deltas(2, (void*)pipeline->cpdis, ncoord, input, foc); if (status) { wcserr_set(PIP_ERRMSG(WCSERR_NULL_POINTER), "NULL pointer passed"); goto exit; } } status = 0; exit: free(tmp); return status; } pywcs-1.12/src/pipeline.h0000644001153600020070000000731412310355626017420 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __PIPELINE_H__ #define __PIPELINE_H__ #include "sip.h" #include "distortion.h" #include "wcs.h" typedef struct { distortion_lookup_t* det2im[2]; /*@shared@*/ /*@null@*/ sip_t* sip; distortion_lookup_t* cpdis[2]; /*@shared@*/ /*@null@*/ struct wcsprm* wcs; struct wcserr* err; } pipeline_t; /** Initialize all the values in a pipeline_t to NULL. */ void pipeline_clear( pipeline_t* pipeline); /** Set all the values of a pipeline_t. */ void pipeline_init( pipeline_t* pipeline, /*@shared@*/ distortion_lookup_t** det2im /* [2] */, /*@shared@*/ sip_t* sip, /*@shared@*/ distortion_lookup_t** cpdis /* [2] */, /*@shared@*/ struct wcsprm* wcs); /** Free all the temporary buffers of a pipeline_t. It does not free the underlying sip_t, distortion_lookup_t or wcsprm objects. */ void pipeline_free( pipeline_t* pipeline); /** Perform the entire pipeline from pixel coordinates to world coordinates, in the following order: - Detector to image plane correction (optionally) - SIP distortion correction (optionally) - Paper IV distortion correction (optionally) - wcslib WCS transformation @param ncoord: @param nelem: @param pixcrd [in]: Array of pixel coordinates. @param world [out]: Array of sky coordinates (output). @return: A wcslib error code. */ int pipeline_all_pixel2world( pipeline_t* pipeline, const unsigned int ncoord, const unsigned int nelem, const double* const pixcrd /* [ncoord][nelem] */, double* world /* [ncoord][nelem] */); /** Perform just the distortion correction part of the pipeline from pixel coordinates to focal plane coordinates. - Detector to image plane correction (optionally) - SIP distortion correction (optionally) - Paper IV distortion correction (optionally) @param ncoord: @param nelem: @param pixcrd [in]: Array of pixel coordinates. @param foc [out]: Array of focal plane coordinates. @return: A wcslib error code. */ int pipeline_pix2foc( pipeline_t* pipeline, const unsigned int ncoord, const unsigned int nelem, const double* const pixcrd /* [ncoord][nelem] */, double* foc /* [ncoord][nelem] */); #endif pywcs-1.12/src/pyutil.c0000644001153600020070000005345712310355626017145 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY /* util.h must be imported first */ #include "pyutil.h" #include "wcsfix.h" #include "wcsprintf.h" #include "wcsunits.h" /*@null@*/ static pywcs_inline PyObject* _PyArrayProxy_New( /*@shared@*/ PyObject* self, int nd, const npy_intp* dims, int typenum, const void* data, const int flags) { PyArray_Descr* type_descr = NULL; PyObject* result = NULL; type_descr = (PyArray_Descr*)PyArray_DescrFromType(typenum); if (type_descr == NULL) { return NULL; } result = (PyObject*)PyArray_NewFromDescr( &PyArray_Type, type_descr, nd, (npy_intp*)dims, NULL, (void*)data, NPY_C_CONTIGUOUS | flags, NULL); if (result == NULL) { return NULL; } Py_INCREF(self); PyArray_BASE(result) = (PyObject*)self; return result; } /*@null@*/ PyObject* PyArrayProxy_New( /*@shared@*/ PyObject* self, int nd, const npy_intp* dims, int typenum, const void* data) { return _PyArrayProxy_New(self, nd, dims, typenum, data, NPY_WRITEABLE); } /*@null@*/ PyObject* PyArrayReadOnlyProxy_New( /*@shared@*/ PyObject* self, int nd, const npy_intp* dims, int typenum, const void* data) { return _PyArrayProxy_New(self, nd, dims, typenum, data, 0); } void preoffset_array( PyArrayObject* array, int value) { npy_intp size; double *data; if (value == 1) { return; } size = PyArray_Size((PyObject*)array); data = (double*)PyArray_DATA(array); offset_c_array(data, size, (double)(1 - value)); } void unoffset_array( PyArrayObject* array, int value) { npy_intp size; double *data; if (value == 1) { return; } size = PyArray_Size((PyObject*)array); data = (double*)PyArray_DATA(array); offset_c_array(data, size, (double)-(1 - value)); } void copy_array_to_c_double( PyArrayObject* array, double* dest) { npy_intp size = 1; double* data = NULL; size = PyArray_Size((PyObject*)array); data = (double*)PyArray_DATA(array); memcpy(dest, data, size * sizeof(double)); } void copy_array_to_c_int( PyArrayObject* array, int* dest) { npy_intp size = 1; int* data = NULL; size = PyArray_Size((PyObject*)array); data = (int*)PyArray_DATA(array); memcpy(dest, data, size * sizeof(int)); } int is_null( /*@null@*/ void *p) { if (p == NULL) { PyErr_SetString(PyExc_AssertionError, "Underlying object is NULL."); return 1; } return 0; } /* wcslib represents undefined values using its own special constant, UNDEFINED. To be consistent with the Pythonic way of doing things, it's nicer to represent undefined values using NaN. Unfortunately, in order to get nice mutable arrays in Python, Python must be able to edit the wcsprm values directly. The solution is to store NaNs in the struct "canonically", but convert those NaNs to/from UNDEFINED around every call into a wcslib function. It's not as computationally expensive as it sounds, as all these arrays are quite small. */ static pywcs_inline void wcsprm_fix_values( struct wcsprm* x, value_fixer_t value_fixer) { unsigned int naxis = (unsigned int)x->naxis; value_fixer(x->cd, 4); value_fixer(x->cdelt, naxis); value_fixer(x->crder, naxis); value_fixer(x->crota, naxis); value_fixer(x->crpix, naxis); value_fixer(x->crval, naxis); value_fixer(x->csyer, naxis); value_fixer(&x->equinox, 1); value_fixer(&x->latpole, 1); value_fixer(&x->lonpole, 1); value_fixer(&x->mjdavg, 1); value_fixer(&x->mjdobs, 1); value_fixer(x->obsgeo, 3); value_fixer(&x->cel.phi0, 1); value_fixer(&x->restfrq, 1); value_fixer(&x->restwav, 1); value_fixer(&x->cel.theta0, 1); value_fixer(&x->velangl, 1); value_fixer(&x->velosys, 1); value_fixer(&x->zsource, 1); } void wcsprm_c2python( /*@null@*/ struct wcsprm* x) { if (x != NULL) { wcsprm_fix_values(x, &undefined2nan); } } void wcsprm_python2c( /*@null@*/ struct wcsprm* x) { if (x != NULL) { wcsprm_fix_values(x, &nan2undefined); } } /*************************************************************************** * Exceptions * ***************************************************************************/ PyObject* WcsExc_SingularMatrix; PyObject* WcsExc_InconsistentAxisTypes; PyObject* WcsExc_InvalidTransform; PyObject* WcsExc_InvalidCoordinate; PyObject* WcsExc_NoSolution; PyObject* WcsExc_InvalidSubimageSpecification; PyObject* WcsExc_NonseparableSubimageCoordinateSystem; PyObject* WcsExc_NoWcsKeywordsFound; PyObject* WcsExc_InvalidTabularParameters; /* This is an array mapping the wcs status codes to Python exception * types. The exception string is stored as part of wcslib itself in * wcs_errmsg. */ PyObject** wcs_errexc[14]; #define DEFINE_EXCEPTION(exc) \ WcsExc_##exc = PyErr_NewException("_pywcs." #exc "Error", PyExc_ValueError, NULL); \ if (WcsExc_##exc == NULL) \ return 1; \ PyModule_AddObject(m, #exc "Error", WcsExc_##exc); \ int _define_exceptions( PyObject* m) { DEFINE_EXCEPTION(SingularMatrix); DEFINE_EXCEPTION(InconsistentAxisTypes); DEFINE_EXCEPTION(InvalidTransform); DEFINE_EXCEPTION(InvalidCoordinate); DEFINE_EXCEPTION(NoSolution); DEFINE_EXCEPTION(InvalidSubimageSpecification); DEFINE_EXCEPTION(NonseparableSubimageCoordinateSystem); DEFINE_EXCEPTION(NoWcsKeywordsFound); DEFINE_EXCEPTION(InvalidTabularParameters); return 0; } const char* wcslib_get_error_message(int status) { return wcs_errmsg[status]; } void wcserr_to_python_exc(const struct wcserr *err) { PyObject *exc; if (err == NULL) { PyErr_SetString(PyExc_RuntimeError, "NULL error object in wcslib"); } else { if (err->status > 0 && err->status <= WCS_ERRMSG_MAX) { exc = *wcs_errexc[err->status]; } else { exc = PyExc_RuntimeError; } /* This is technically not thread-safe -- make sure we have the GIL */ wcsprintf_set(NULL); wcserr_prt(err, ""); PyErr_SetString(exc, wcsprintf_buf()); } } void wcs_to_python_exc(const struct wcsprm *wcs) { PyObject* exc; const struct wcserr *err = wcs->err; if (err == NULL) { PyErr_SetString(PyExc_RuntimeError, "NULL error object in wcslib"); } else { if (err->status > 0 && err->status < WCS_ERRMSG_MAX) { exc = *wcs_errexc[err->status]; } else { exc = PyExc_RuntimeError; } /* This is technically not thread-safe -- make sure we have the GIL */ wcsprintf_set(NULL); wcsperr(wcs, ""); PyErr_SetString(exc, wcsprintf_buf()); } } void wcserr_fix_to_python_exc(const struct wcserr *err) { PyObject *exc; if (err == NULL) { PyErr_SetString(PyExc_RuntimeError, "NULL error object in wcslib"); } else { if (err->status > 0 && err->status <= FIXERR_NO_REF_PIX_VAL) { exc = PyExc_ValueError; } else { exc = PyExc_RuntimeError; } /* This is technically not thread-safe -- make sure we have the GIL */ wcsprintf_set(NULL); wcserr_prt(err, ""); PyErr_SetString(exc, wcsprintf_buf()); } } void wcserr_units_to_python_exc(const struct wcserr *err) { PyObject *exc; if (err == NULL) { PyErr_SetString(PyExc_RuntimeError, "NULL error object in wcslib"); } else { if (err->status > 0 && err->status <= UNITSERR_UNSAFE_TRANS) { exc = PyExc_ValueError; } else { exc = PyExc_RuntimeError; } /* This is technically not thread-safe -- make sure we have the GIL */ wcsprintf_set(NULL); wcserr_prt(err, ""); PyErr_SetString(exc, wcsprintf_buf()); } } /*************************************************************************** Property helpers ***************************************************************************/ #define SHAPE_STR_LEN 128 /* Helper function to display the desired shape of an array as a string, eg. 2x2 */ static void shape_to_string( npy_int ndims, const npy_intp* dims, char* str /* [SHAPE_STR_LEN] */) { int i; char value[32]; /* More than large enough to hold string rep of a 64-bit integer (way overkill) */ if (ndims > 3) { strncpy(str, "ERROR", 6); return; } str[0] = 0; for (i = 0; i < ndims; ++i) { snprintf(value, 32, "%d", (int)dims[i]); strncat(str, value, 32); if (i != ndims - 1) { strncat(str, "x", 2); } } } /* get_string is inlined */ int set_string( const char* propname, PyObject* value, char* dest, Py_ssize_t maxlen) { char* buffer; Py_ssize_t len; if (check_delete(propname, value)) { return -1; } #if PY3K if (PyBytes_AsStringAndSize(value, &buffer, &len) == -1) { return -1; } #else if (PyString_AsStringAndSize(value, &buffer, &len) == -1) { return -1; } #endif if (len > maxlen) { PyErr_Format( PyExc_ValueError, "'%s' must be less than %u characters", propname, (unsigned int)maxlen); return -1; } strncpy(dest, buffer, (size_t)maxlen); return 0; } /* get_bool is inlined */ int set_bool( const char* propname, PyObject* value, int* dest) { if (check_delete(propname, value)) { return -1; } *dest = PyObject_IsTrue(value); return 0; } /* get_int is inlined */ int set_int( const char* propname, PyObject* value, int* dest) { long value_int; if (check_delete(propname, value)) { return -1; } #if PY3K value_int = PyLong_AsLong(value); #else value_int = PyInt_AsLong(value); #endif if (value_int == -1 && PyErr_Occurred()) { return -1; } if ((unsigned long)value_int > 0x7fffffff) { return -1; } *dest = (int)value_int; return 0; } /* get_double is inlined */ int set_double( const char* propname, PyObject* value, double* dest) { if (check_delete(propname, value)) { return -1; } *dest = PyFloat_AsDouble(value); if (PyErr_Occurred()) { return -1; } else { return 0; } } /* get_double_array is inlined */ int set_double_array( const char* propname, PyObject* value, npy_int ndims, const npy_intp* dims, double* dest) { PyArrayObject* value_array = NULL; npy_int i = 0; PyObject* ignored = NULL; char shape_str[SHAPE_STR_LEN]; if (check_delete(propname, value)) { return -1; } value_array = (PyArrayObject*)PyArray_ContiguousFromAny(value, PyArray_DOUBLE, ndims, ndims); if (value_array == NULL) { return -1; } if (dims != NULL) { for (i = 0; i < ndims; ++i) { if (PyArray_DIM(value_array, i) != dims[i]) { shape_to_string(ndims, dims, shape_str); ignored = PyErr_Format( PyExc_ValueError, "'%s' array is the wrong shape, must be %s", propname, shape_str); Py_DECREF(value_array); return -1; } } } copy_array_to_c_double(value_array, dest); Py_DECREF(value_array); return 0; } int set_int_array( const char* propname, PyObject* value, npy_int ndims, const npy_intp* dims, int* dest) { PyArrayObject* value_array = NULL; npy_int i = 0; PyObject* ignored = NULL; char shape_str[SHAPE_STR_LEN]; if (check_delete(propname, value)) { return -1; } value_array = (PyArrayObject*)PyArray_ContiguousFromAny(value, PyArray_INT, ndims, ndims); if (value_array == NULL) { return -1; } if (dims != NULL) { for (i = 0; i < ndims; ++i) { if (PyArray_DIM(value_array, i) != dims[i]) { shape_to_string(ndims, dims, shape_str); ignored = PyErr_Format( PyExc_ValueError, "'%s' array is the wrong shape, must be %s", propname, shape_str); Py_DECREF(value_array); return -1; } } } copy_array_to_c_int(value_array, dest); Py_DECREF(value_array); return 0; } /* get_str_list is inlined */ /* set_str_list is inlined */ int set_str_list_verified( const char* propname, PyObject* value, Py_ssize_t len, Py_ssize_t maxlen, char (*dest)[72], str_verify_fn verify) { PyObject* str = NULL; char* str_char = NULL; Py_ssize_t str_len = 0; Py_ssize_t i = 0; PyObject* ignored = NULL; if (check_delete(propname, value)) { return -1; } if (maxlen == 0) { maxlen = 68; } if (!PySequence_Check(value)) { ignored = PyErr_Format( PyExc_TypeError, "'%s' must be a sequence of strings", propname); return -1; } if (PySequence_Size(value) != len) { ignored = PyErr_Format( PyExc_ValueError, "len(%s) must be %u", propname, (unsigned int)len); return -1; } /* We go through the list twice, once to verify that the list is in the correct format, and then again to do the data copy. This way, we won't partially copy the contents and then throw an exception. */ for (i = 0; i < len; ++i) { str = PySequence_GetItem(value, i); if (str == NULL) { return -1; } #if PY3K if (!PyBytes_CheckExact(str)) { #else if (!PyString_CheckExact(str)) { #endif ignored = PyErr_Format( PyExc_TypeError, #if PY3K "'%s' must be a sequence of bytes", #else "'%s' must be a sequence of strings", #endif propname); Py_DECREF(str); return -1; } #if PY3K if (PyBytes_Size(str) > maxlen) { #else if (PyString_Size(str) > maxlen) { #endif ignored = PyErr_Format( PyExc_TypeError, #if PY3K "Each bytes in '%s' must be less than %u characters", #else "Each string in '%s' must be less than %u characters", #endif propname, (unsigned int)maxlen); Py_DECREF(str); return -1; } if (verify) { #if PY3K str_char = PyBytes_AsString(str); #else str_char = PyString_AsString(str); #endif if (!verify(str_char)) { Py_DECREF(str); return -1; } } Py_DECREF(str); } for (i = 0; i < len; ++i) { str = PySequence_GetItem(value, i); if (str == NULL) { /* Theoretically, something has gone really wrong here, since we've already verified the list. */ ignored = PyErr_Format( PyExc_RuntimeError, "Input values have changed underneath us. Something is seriously wrong."); return -1; } /* We already know its a string of the correct length */ #if PY3K if (PyBytes_AsStringAndSize(str, &str_char, &str_len)) { #else if (PyString_AsStringAndSize(str, &str_char, &str_len)) { #endif /* Theoretically, something has gone really wrong here, since we've already verified the list. */ ignored = PyErr_Format( PyExc_RuntimeError, "Input values have changed underneath us. Something is seriously wrong."); Py_DECREF(str); return -1; } strncpy(dest[i], str_char, (size_t)maxlen); Py_DECREF(str); } return 0; } /*@null@*/ PyObject* get_pscards( /*@unused@*/ const char* propname, struct pscard* ps, int nps) { PyObject* result = NULL; PyObject* subresult = NULL; Py_ssize_t i = 0; if (nps < 0) { return NULL; } result = PyList_New((Py_ssize_t)nps); if (result == NULL) { return NULL; } for (i = 0; i < (Py_ssize_t)nps; ++i) { subresult = Py_BuildValue("iis", ps[i].i, ps[i].m, ps[i].value); if (subresult == NULL) { Py_DECREF(result); return NULL; } if (PyList_SetItem(result, i, subresult)) { Py_DECREF(subresult); Py_DECREF(result); return NULL; } } return result; } int set_pscards( /*@unused@*/ const char* propname, PyObject* value, struct pscard** ps, int *nps, int *npsmax) { PyObject* subvalue = NULL; Py_ssize_t i = 0; Py_ssize_t size = 0; int ival = 0; int mval = 0; char* strvalue = 0; void* newmem = NULL; if (!PySequence_Check(value)) return -1; size = PySequence_Size(value); if (size > 0x7fffffff) { return -1; } if (size > (Py_ssize_t)*npsmax) { newmem = malloc(sizeof(struct pscard) * size); if (newmem == NULL) { PyErr_SetString(PyExc_MemoryError, "Could not allocate memory."); return -1; } free(*ps); *ps = newmem; *npsmax = (int)size; } /* Verify the entire list for correct types first, so we don't have to undo anything copied into the canonical array. */ for (i = 0; i < size; ++i) { subvalue = PySequence_GetItem(value, i); if (subvalue == NULL) { return -1; } if (!PyArg_ParseTuple(subvalue, "iis", &ival, &mval, &strvalue)) { Py_DECREF(subvalue); return -1; } Py_DECREF(subvalue); } for (i = 0; i < size; ++i) { subvalue = PySequence_GetItem(value, i); if (subvalue == NULL) { return -1; } if (!PyArg_ParseTuple(subvalue, "iis", &ival, &mval, &strvalue)) { Py_DECREF(subvalue); return -1; } Py_DECREF(subvalue); (*ps)[i].i = ival; (*ps)[i].m = mval; strncpy((*ps)[i].value, strvalue, 72); (*ps)[i].value[71] = '\0'; (*nps) = i + 1; } return 0; } /*@null@*/ PyObject* get_pvcards( /*@unused@*/ const char* propname, struct pvcard* pv, int npv) { PyObject* result = NULL; PyObject* subresult = NULL; Py_ssize_t i = 0; result = PyList_New((Py_ssize_t)npv); if (result == NULL) { return NULL; } for (i = 0; i < (Py_ssize_t)npv; ++i) { subresult = Py_BuildValue("iid", pv[i].i, pv[i].m, pv[i].value); if (subresult == NULL) { Py_DECREF(result); return NULL; } if (PyList_SetItem(result, i, subresult)) { Py_DECREF(subresult); Py_DECREF(result); return NULL; } } return result; } int set_pvcards( /*@propname@*/ const char* propname, PyObject* value, struct pvcard** pv, int *npv, int *npvmax) { PyObject* subvalue = NULL; int i = 0; Py_ssize_t size = 0; int ival = 0; int mval = 0; double dblvalue = 0.0; void* newmem = NULL; if (!PySequence_Check(value)) { return -1; } size = PySequence_Size(value); if (size > 0x7fffffff) { return -1; } if (size > (Py_ssize_t)*npvmax) { newmem = malloc(sizeof(struct pvcard) * size); if (newmem == NULL) { PyErr_SetString(PyExc_MemoryError, "Could not allocate memory."); return -1; } free(*pv); *pv = newmem; *npvmax = (int)size; } /* Verify the entire list for correct types first, so we don't have to undo anything copied into the canonical array. */ for (i = 0; i < size; ++i) { subvalue = PySequence_GetItem(value, i); if (subvalue == NULL) { return -1; } if (!PyArg_ParseTuple(subvalue, "iid", &ival, &mval, &dblvalue)) { Py_DECREF(subvalue); return -1; } Py_DECREF(subvalue); } for (i = 0; i < size; ++i) { subvalue = PySequence_GetItem(value, i); if (subvalue == NULL) { return -1; } if (!PyArg_ParseTuple(subvalue, "iid", &ival, &mval, &dblvalue)) { Py_DECREF(subvalue); return -1; } Py_DECREF(subvalue); (*pv)[i].i = ival; (*pv)[i].m = mval; (*pv)[i].value = dblvalue; (*npv) = i + 1; } return 0; } PyObject* get_deepcopy( PyObject* obj, PyObject* memo) { if (PyObject_HasAttrString(obj, "__deepcopy__")) { return PyObject_CallMethod(obj, "__deepcopy__", "O", memo); } else { return PyObject_CallMethod(obj, "__copy__", ""); } } /*************************************************************************** * Miscellaneous helper functions * ***************************************************************************/ int parse_unsafe_unit_conversion_spec( const char* arg, int* ctrl) { const char* p = NULL; *ctrl = 0; p = arg; for (p = arg; *p != '\0'; ++p) { switch (*p) { case 's': case 'S': *ctrl |= 1; break; case 'h': case 'H': *ctrl |= 2; break; case 'd': case 'D': *ctrl |= 4; break; default: PyErr_SetString( PyExc_ValueError, "translate_units may only contain the characters 's', 'h' or 'd'"); return 1; } } return 0; } pywcs-1.12/src/pyutil.h0000644001153600020070000002231712310355626017141 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __PYUTIL_H__ #define __PYUTIL_H__ #include "util.h" #define PY_ARRAY_UNIQUE_SYMBOL pywcs_numpy_api #include #include #include #if PY_MAJOR_VERSION >= 3 #define PY3K 1 #else #define PY3K 0 #ifndef Py_TYPE #define Py_TYPE(ob) (((PyObject*)(ob))->ob_type) #endif #endif /* Py_ssize_t for old Pythons */ /* This code is as recommended by: */ /* http://www.python.org/dev/peps/pep-0353/#conversion-guidelines */ #if PY_VERSION_HEX < 0x02050000 #if !defined(PY_SSIZE_T_MIN) typedef int Py_ssize_t; # define PY_SSIZE_T_MAX INT_MAX # define PY_SSIZE_T_MIN INT_MIN #endif #define lenfunc inquiry #define ssizeargfunc intargfunc #define ssizeobjargproc intobjargproc #endif PyObject* PyArrayProxy_New( PyObject* self, int nd, const npy_intp* dims, int typenum, const void* data); PyObject* PyArrayReadOnlyProxy_New( PyObject* self, int nd, const npy_intp* dims, int typenum, const void* data); typedef int (*str_verify_fn)(char *); /*@null@*/ PyObject * PyStrListProxy_New( PyObject* owner, Py_ssize_t size, Py_ssize_t maxsize, char (*array)[72], str_verify_fn verify ); int _setup_str_list_proxy_type( PyObject* m); static pywcs_inline void offset_c_array( double* value, npy_intp size, double offset) { double* end = value + size; for ( ; value != end; ++value) { *value += offset; } } static pywcs_inline void nan2undefined( double* value, unsigned int nvalues) { double* end = value + nvalues; for ( ; value != end; ++value) { if (isnan64(*value)) { *value = UNDEFINED; } } } static pywcs_inline void undefined2nan( double* value, unsigned int nvalues) { double* end = value + nvalues; for ( ; value != end; ++value) { if (*value == UNDEFINED) { *value = (double)NPY_NAN; } } } void preoffset_array( PyArrayObject* array, int value); void unoffset_array( PyArrayObject* array, int value); void copy_array_to_c_double( PyArrayObject* array, double* dest); void copy_array_to_c_int( PyArrayObject* array, int* dest); /** Returns TRUE if pointer is NULL, and sets Python exception */ int is_null(/*@null@*/ void *); typedef void (*value_fixer_t)(double*, unsigned int); void wcsprm_c2python( /*@null@*/ struct wcsprm* x); void wcsprm_python2c( /*@null@*/ struct wcsprm* x); /*************************************************************************** * Exceptions * ***************************************************************************/ extern PyObject* WcsExc_SingularMatrix; extern PyObject* WcsExc_InconsistentAxisTypes; extern PyObject* WcsExc_InvalidTransform; extern PyObject* WcsExc_InvalidCoordinate; extern PyObject* WcsExc_NoSolution; extern PyObject* WcsExc_InvalidSubimageSpecification; extern PyObject* WcsExc_NonseparableSubimageCoordinateSystem; extern PyObject* WcsExc_NoWcsKeywordsFound; extern PyObject* WcsExc_InvalidTabularParameters; /* This is an array mapping the wcs status codes to Python exception * types. The exception string is stored as part of wcslib itself in * wcs_errmsg. */ extern PyObject** wcs_errexc[14]; #define WCS_ERRMSG_MAX 14 #define WCSFIX_ERRMSG_MAX 11 int _define_exceptions(PyObject* m); const char* wcslib_get_error_message(int stat); void wcserr_to_python_exc(const struct wcserr *err); void wcs_to_python_exc(const struct wcsprm *wcs); void wcserr_fix_to_python_exc(const struct wcserr *err); void wcserr_units_to_python_exc(const struct wcserr *err); /*************************************************************************** Property helpers ***************************************************************************/ static pywcs_inline int check_delete( const char* propname, PyObject* value) { PyObject* ignored; if (value == NULL) { ignored = PyErr_Format(PyExc_TypeError, "'%s' can not be deleted", propname); return -1; } return 0; } static pywcs_inline PyObject* get_string( /*@unused@*/ const char* propname, const char* value) { #if PY3K return PyBytes_FromString(value); #else return PyString_FromString(value); #endif } int set_string( const char* propname, PyObject* value, char* dest, Py_ssize_t maxlen); static pywcs_inline PyObject* get_bool( /*@unused@*/ const char* propname, long value) { return PyBool_FromLong(value); } int set_bool( const char* propname, PyObject* value, int* dest); static pywcs_inline PyObject* get_int( /*@unused@*/ const char* propname, long value) { #if PY3K return PyLong_FromLong(value); #else return PyInt_FromLong(value); #endif } int set_int( const char* propname, PyObject* value, int* dest); static pywcs_inline PyObject* get_double( const char* propname, double value) { return PyFloat_FromDouble(value); } int set_double( const char* propname, PyObject* value, double* dest); /*@null@*/ static pywcs_inline PyObject* get_double_array( /*@unused@*/ const char* propname, double* value, npy_intp ndims, const npy_intp* dims, /*@shared@*/ PyObject* owner) { return PyArrayProxy_New(owner, ndims, dims, PyArray_DOUBLE, value); } /*@null@*/ static pywcs_inline PyObject* get_double_array_readonly( /*@unused@*/ const char* propname, double* value, npy_intp ndims, const npy_intp* dims, /*@shared@*/ PyObject* owner) { return PyArrayReadOnlyProxy_New(owner, ndims, dims, PyArray_DOUBLE, value); } int set_double_array( const char* propname, PyObject* value, npy_int ndims, const npy_intp* dims, double* dest); /*@null@*/ static pywcs_inline PyObject* get_int_array( /*@unused@*/ const char* propname, int* value, npy_int ndims, const npy_intp* dims, /*@shared@*/ PyObject* owner) { return PyArrayProxy_New(owner, ndims, dims, PyArray_INT, value); } int set_int_array( const char* propname, PyObject* value, npy_int ndims, const npy_intp* dims, int* dest); static pywcs_inline PyObject* get_str_list_verified( /*@unused@*/ const char* propname, char (*array)[72], Py_ssize_t len, Py_ssize_t maxlen, PyObject* owner, str_verify_fn verify) { return PyStrListProxy_New(owner, len, maxlen, array, verify); } static pywcs_inline PyObject* get_str_list( /*@unused@*/ const char* propname, char (*array)[72], Py_ssize_t len, Py_ssize_t maxlen, PyObject* owner) { return get_str_list_verified(propname, array, len, maxlen, owner, NULL); } int set_str_list_verified( const char* propname, PyObject* value, Py_ssize_t len, Py_ssize_t maxlen, char (*dest)[72], str_verify_fn verify); static pywcs_inline int set_str_list( const char* propname, PyObject* value, Py_ssize_t len, Py_ssize_t maxlen, char (*dest)[72]) { return set_str_list_verified(propname, value, len, maxlen, dest, NULL); } PyObject* get_pscards( const char* propname, struct pscard* ps, int nps); int set_pscards( const char* propname, PyObject* value, struct pscard** ps, int *nps, int *npsmax); PyObject* get_pvcards( const char* propname, struct pvcard* pv, int npv); int set_pvcards( const char* propname, PyObject* value, struct pvcard** pv, int *npv, int *npvmax); PyObject* get_deepcopy( PyObject* obj, PyObject* memo); /*************************************************************************** Miscellaneous helper functions ***************************************************************************/ int parse_unsafe_unit_conversion_spec( const char* arg, int* ctrl); #endif /* __PYUTIL_H__ */ pywcs-1.12/src/pywcs.c0000644001153600020070000006403212310355626016753 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #include "pywcs.h" #include "wcslib_wrap.h" #include "wcslib_tabprm_wrap.h" #include "wcslib_units_wrap.h" #include "wcslib_wtbarr_wrap.h" #include "distortion_wrap.h" #include "sip_wrap.h" #include "docstrings.h" #include "pywcs_api.h" #include /* from Python */ #include #include /*************************************************************************** * Pywcs type ***************************************************************************/ static PyTypeObject PyWcsType; static int _setup_pywcs_type(PyObject* m); /*************************************************************************** * PyWcs methods */ static int PyWcs_traverse( PyWcs* self, visitproc visit, void* arg) { Py_VISIT(self->py_det2im[0]); Py_VISIT(self->py_det2im[1]); Py_VISIT(self->py_sip); Py_VISIT(self->py_distortion_lookup[0]); Py_VISIT(self->py_distortion_lookup[1]); Py_VISIT(self->py_wcsprm); return 0; } static int PyWcs_clear( PyWcs* self) { PyObject* tmp; tmp = self->py_det2im[0]; self->py_det2im[0] = NULL; Py_XDECREF(tmp); tmp = self->py_det2im[1]; self->py_det2im[1] = NULL; Py_XDECREF(tmp); tmp = self->py_sip; self->py_sip = NULL; Py_XDECREF(tmp); tmp = self->py_distortion_lookup[0]; self->py_distortion_lookup[0] = NULL; Py_XDECREF(tmp); tmp = self->py_distortion_lookup[1]; self->py_distortion_lookup[1] = NULL; Py_XDECREF(tmp); tmp = self->py_wcsprm; self->py_wcsprm = NULL; Py_XDECREF(tmp); return 0; } static void PyWcs_dealloc( PyWcs* self) { int ignored; ignored = PyWcs_clear(self); pipeline_free(&self->x); Py_TYPE(self)->tp_free((PyObject*)self); } /*@null@*/ static PyObject * PyWcs_new( PyTypeObject* type, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyWcs* self; self = (PyWcs*)type->tp_alloc(type, 0); if (self != NULL) { pipeline_clear(&self->x); self->py_det2im[0] = NULL; self->py_det2im[1] = NULL; self->py_sip = NULL; self->py_distortion_lookup[0] = NULL; self->py_distortion_lookup[1] = NULL; self->py_wcsprm = NULL; } return (PyObject*)self; } static int PyWcs_init( PyWcs* self, PyObject* args, /*@unused@*/ PyObject* kwds) { size_t i; PyObject* py_sip; PyObject* py_wcsprm; PyObject* py_distortion_lookup[2]; PyObject* py_det2im[2]; if (!PyArg_ParseTuple (args, "O(OO)O(OO):Wcs.__init__", &py_sip, &py_distortion_lookup[0], &py_distortion_lookup[1], &py_wcsprm, &py_det2im[0], &py_det2im[1])) { return -1; } /* Check and set Distortion lookup tables */ for (i = 0; i < 2; ++i) { if (py_det2im[i] != NULL && py_det2im[i] != Py_None) { if (!PyObject_TypeCheck(py_det2im[i], &PyDistLookupType)) { PyErr_SetString(PyExc_TypeError, "Arg 4 must be a pair of DistortionLookupTable or None objects"); return -1; } self->py_det2im[i] = py_det2im[i]; self->x.det2im[i] = &(((PyDistLookup*)py_det2im[i])->x); } } /* Check and set SIP */ if (py_sip != NULL && py_sip != Py_None) { if (!PyObject_TypeCheck(py_sip, &PySipType)) { PyErr_SetString(PyExc_TypeError, "Arg 1 must be Sip object"); return -1; } self->py_sip = py_sip; self->x.sip = &(((PySip*)py_sip)->x); } /* Check and set Distortion lookup tables */ for (i = 0; i < 2; ++i) { if (py_distortion_lookup[i] != NULL && py_distortion_lookup[i] != Py_None) { if (!PyObject_TypeCheck(py_distortion_lookup[i], &PyDistLookupType)) { PyErr_SetString(PyExc_TypeError, "Arg 2 must be a pair of DistortionLookupTable or None objects"); return -1; } self->py_distortion_lookup[i] = py_distortion_lookup[i]; self->x.cpdis[i] = &(((PyDistLookup*)py_distortion_lookup[i])->x); } } /* Set and lookup Wcsprm object */ if (py_wcsprm != NULL && py_wcsprm != Py_None) { if (!PyObject_TypeCheck(py_wcsprm, &PyWcsprmType)) { PyErr_SetString(PyExc_TypeError, "Arg 3 must be Wcsprm object"); return -1; } self->py_wcsprm = py_wcsprm; self->x.wcs = &(((PyWcsprm*)py_wcsprm)->x); } Py_XINCREF(self->py_sip); Py_XINCREF(self->py_distortion_lookup[0]); Py_XINCREF(self->py_distortion_lookup[1]); Py_XINCREF(self->py_wcsprm); Py_XINCREF(self->py_det2im[0]); Py_XINCREF(self->py_det2im[1]); return 0; } /*@null@*/ static PyObject* PyWcs_all_pix2sky( PyWcs* self, PyObject* args, PyObject* kwds) { int naxis = 2; PyObject* pixcrd_obj = NULL; int origin = 1; PyArrayObject* pixcrd = NULL; PyArrayObject* world = NULL; int status = -1; const char* keywords[] = { "pixcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords( args, kwds, "Oi:all_pix2sky", (char **)keywords, &pixcrd_obj, &origin)) { return NULL; } naxis = self->x.wcs->naxis; pixcrd = (PyArrayObject*)PyArray_ContiguousFromAny(pixcrd_obj, PyArray_DOUBLE, 2, 2); if (pixcrd == NULL) { return NULL; } if (PyArray_DIM(pixcrd, 1) < naxis) { PyErr_Format( PyExc_RuntimeError, "Input array must be 2-dimensional, where the second dimension >= %d", naxis); goto exit; } world = (PyArrayObject*)PyArray_SimpleNew(2, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (world == NULL) { goto exit; } /* Make the call */ Py_BEGIN_ALLOW_THREADS preoffset_array(pixcrd, origin); wcsprm_python2c(self->x.wcs); status = pipeline_all_pixel2world(&self->x, (unsigned int)PyArray_DIM(pixcrd, 0), (unsigned int)PyArray_DIM(pixcrd, 1), (double*)PyArray_DATA(pixcrd), (double*)PyArray_DATA(world)); wcsprm_c2python(self->x.wcs); unoffset_array(pixcrd, origin); Py_END_ALLOW_THREADS /* unoffset_array(world, origin); */ exit: Py_XDECREF(pixcrd); if (status == 0 || status == 8) { return (PyObject*)world; } else if (status == -1) { PyErr_SetString( PyExc_ValueError, "Wrong number of dimensions in input array. Expected 2."); return NULL; } else { Py_DECREF(world); if (status == -1) { /* exception already set */ return NULL; } else { wcserr_to_python_exc(self->x.err); return NULL; } } } /*@null@*/ static PyObject* PyWcs_p4_pix2foc( PyWcs* self, PyObject* args, PyObject* kwds) { PyObject* pixcrd_obj = NULL; int origin = 1; PyArrayObject* pixcrd = NULL; PyArrayObject* foccrd = NULL; int status = -1; const char* keywords[] = { "pixcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords(args, kwds, "Oi:p4_pix2foc", (char **)keywords, &pixcrd_obj, &origin)) { return NULL; } if (self->x.cpdis[0] == NULL && self->x.cpdis[1] == NULL) { Py_INCREF(pixcrd_obj); return pixcrd_obj; } pixcrd = (PyArrayObject*)PyArray_ContiguousFromAny(pixcrd_obj, PyArray_DOUBLE, 2, 2); if (pixcrd == NULL) { return NULL; } if (PyArray_DIM(pixcrd, 1) != NAXES) { PyErr_SetString(PyExc_ValueError, "Pixel array must be an Nx2 array"); goto exit; } foccrd = (PyArrayObject*)PyArray_SimpleNew(2, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (foccrd == NULL) { status = 2; goto exit; } Py_BEGIN_ALLOW_THREADS preoffset_array(pixcrd, origin); status = p4_pix2foc(2, (void *)self->x.cpdis, (unsigned int)PyArray_DIM(pixcrd, 0), (double*)PyArray_DATA(pixcrd), (double*)PyArray_DATA(foccrd)); unoffset_array(pixcrd, origin); unoffset_array(foccrd, origin); Py_END_ALLOW_THREADS exit: Py_XDECREF(pixcrd); if (status == 0) { return (PyObject*)foccrd; } else { Py_XDECREF(foccrd); if (status == -1) { /* Exception already set */ return NULL; } else { PyErr_SetString(PyExc_MemoryError, "NULL pointer passed"); return NULL; } } } /*@null@*/ static PyObject* PyWcs_det2im( PyWcs* self, PyObject* args, PyObject* kwds) { PyObject* detcrd_obj = NULL; int origin = 1; PyArrayObject* detcrd = NULL; PyArrayObject* imcrd = NULL; int status = -1; const char* keywords[] = { "detcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords(args, kwds, "Oi:det2im", (char **)keywords, &detcrd_obj, &origin)) { return NULL; } if (self->x.det2im[0] == NULL && self->x.det2im[1] == NULL) { Py_INCREF(detcrd_obj); return detcrd_obj; } detcrd = (PyArrayObject*)PyArray_ContiguousFromAny(detcrd_obj, PyArray_DOUBLE, 2, 2); if (detcrd == NULL) { return NULL; } if (PyArray_DIM(detcrd, 1) != NAXES) { PyErr_SetString(PyExc_ValueError, "Pixel array must be an Nx2 array"); goto exit; } imcrd = (PyArrayObject*)PyArray_SimpleNew(2, PyArray_DIMS(detcrd), PyArray_DOUBLE); if (imcrd == NULL) { status = 2; goto exit; } Py_BEGIN_ALLOW_THREADS preoffset_array(detcrd, origin); status = p4_pix2foc(2, (void *)self->x.det2im, (unsigned int)PyArray_DIM(detcrd, 0), (double*)PyArray_DATA(detcrd), (double*)PyArray_DATA(imcrd)); unoffset_array(detcrd, origin); unoffset_array(imcrd, origin); Py_END_ALLOW_THREADS exit: Py_XDECREF(detcrd); if (status == 0) { return (PyObject*)imcrd; } else { Py_XDECREF(imcrd); if (status == -1) { /* Exception already set */ return NULL; } else { PyErr_SetString(PyExc_MemoryError, "NULL pointer passed"); return NULL; } } } /*@null@*/ static PyObject* PyWcs_pix2foc( PyWcs* self, PyObject* args, PyObject* kwds) { PyObject* pixcrd_obj = NULL; int origin = 1; PyArrayObject* pixcrd = NULL; PyArrayObject* foccrd = NULL; int status = -1; const char* keywords[] = { "pixcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords(args, kwds, "Oi:pix2foc", (char **)keywords, &pixcrd_obj, &origin)) { return NULL; } pixcrd = (PyArrayObject*)PyArray_ContiguousFromAny(pixcrd_obj, PyArray_DOUBLE, 2, 2); if (pixcrd == NULL) { return NULL; } if (PyArray_DIM(pixcrd, 1) != NAXES) { PyErr_SetString(PyExc_ValueError, "Pixel array must be an Nx2 array"); goto _exit; } foccrd = (PyArrayObject*)PyArray_SimpleNew(2, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (foccrd == NULL) { goto _exit; } Py_BEGIN_ALLOW_THREADS preoffset_array(pixcrd, origin); status = pipeline_pix2foc(&self->x, (unsigned int)PyArray_DIM(pixcrd, 0), (unsigned int)PyArray_DIM(pixcrd, 1), (double*)PyArray_DATA(pixcrd), (double*)PyArray_DATA(foccrd)); unoffset_array(pixcrd, origin); unoffset_array(foccrd, origin); Py_END_ALLOW_THREADS _exit: Py_XDECREF(pixcrd); if (status == 0) { return (PyObject*)foccrd; } else { Py_XDECREF(foccrd); if (status == -1) { /* Exception already set */ return NULL; } else { wcserr_to_python_exc(self->x.err); return NULL; } } } /*@null@*/ static PyObject* PyWcs_get_wcs( PyWcs* self, /*@unused@*/ void* closure) { if (self->py_wcsprm) { Py_INCREF(self->py_wcsprm); return self->py_wcsprm; } Py_INCREF(Py_None); return Py_None; } static int PyWcs_set_wcs( PyWcs* self, /*@shared@*/ PyObject* value, /*@unused@*/ void* closure) { Py_XDECREF(self->py_wcsprm); self->py_wcsprm = NULL; self->x.wcs = NULL; if (value != NULL && value != Py_None) { if (!PyObject_TypeCheck(value, &PyWcsprmType)) { PyErr_SetString(PyExc_TypeError, "wcs must be Wcsprm object"); return -1; } Py_INCREF(value); self->py_wcsprm = value; self->x.wcs = &(((PyWcsprm*)value)->x); } return 0; } static PyObject* PyWcs_get_cpdis1( PyWcs* self, /*@unused@*/ void* closure) { if (self->py_distortion_lookup[0]) { Py_INCREF(self->py_distortion_lookup[0]); return self->py_distortion_lookup[0]; } Py_INCREF(Py_None); return Py_None; } static int PyWcs_set_cpdis1( PyWcs* self, /*@shared@*/ PyObject* value, /*@unused@*/ void* closure) { Py_XDECREF(self->py_distortion_lookup[0]); self->py_distortion_lookup[0] = NULL; self->x.cpdis[0] = NULL; if (value != NULL && value != Py_None) { if (!PyObject_TypeCheck(value, &PyDistLookupType)) { PyErr_SetString(PyExc_TypeError, "cpdis1 must be DistortionLookupTable object"); return -1; } Py_INCREF(value); self->py_distortion_lookup[0] = value; self->x.cpdis[0] = &(((PyDistLookup*)value)->x); } return 0; } /*@shared@*/ static PyObject* PyWcs_get_cpdis2( PyWcs* self, /*@unused@*/ void* closure) { if (self->py_distortion_lookup[1]) { Py_INCREF(self->py_distortion_lookup[1]); return self->py_distortion_lookup[1]; } Py_INCREF(Py_None); return Py_None; } static int PyWcs_set_cpdis2( PyWcs* self, /*@shared@*/ PyObject* value, /*@unused@*/ void* closure) { Py_XDECREF(self->py_distortion_lookup[1]); self->py_distortion_lookup[1] = NULL; self->x.cpdis[1] = NULL; if (value != NULL && value != Py_None) { if (!PyObject_TypeCheck(value, &PyDistLookupType)) { PyErr_SetString(PyExc_TypeError, "cpdis2 must be DistortionLookupTable object"); return -1; } Py_INCREF(value); self->py_distortion_lookup[1] = value; self->x.cpdis[1] = &(((PyDistLookup*)value)->x); } return 0; } static PyObject* PyWcs_get_det2im1( PyWcs* self, /*@unused@*/ void* closure) { if (self->py_det2im[0]) { Py_INCREF(self->py_det2im[0]); return self->py_det2im[0]; } Py_INCREF(Py_None); return Py_None; } static int PyWcs_set_det2im1( PyWcs* self, /*@shared@*/ PyObject* value, /*@unused@*/ void* closure) { Py_XDECREF(self->py_det2im[0]); self->py_det2im[0] = NULL; self->x.det2im[0] = NULL; if (value != NULL && value != Py_None) { if (!PyObject_TypeCheck(value, &PyDistLookupType)) { PyErr_SetString(PyExc_TypeError, "det2im1 must be DistortionLookupTable object"); return -1; } Py_INCREF(value); self->py_det2im[0] = value; self->x.det2im[0] = &(((PyDistLookup*)value)->x); } return 0; } /*@shared@*/ static PyObject* PyWcs_get_det2im2( PyWcs* self, /*@unused@*/ void* closure) { if (self->py_det2im[1]) { Py_INCREF(self->py_det2im[1]); return self->py_det2im[1]; } Py_INCREF(Py_None); return Py_None; } static int PyWcs_set_det2im2( PyWcs* self, /*@shared@*/ PyObject* value, /*@unused@*/ void* closure) { Py_XDECREF(self->py_det2im[1]); self->py_det2im[1] = NULL; self->x.det2im[1] = NULL; if (value != NULL && value != Py_None) { if (!PyObject_TypeCheck(value, &PyDistLookupType)) { PyErr_SetString(PyExc_TypeError, "det2im2 must be DistortionLookupTable object"); return -1; } Py_INCREF(value); self->py_det2im[1] = value; self->x.det2im[1] = &(((PyDistLookup*)value)->x); } return 0; } /*@shared@*/ static PyObject* PyWcs_get_sip( PyWcs* self, /*@unused@*/ void* closure) { if (self->py_sip) { Py_INCREF(self->py_sip); return self->py_sip; } Py_INCREF(Py_None); return Py_None; } static int PyWcs_set_sip( PyWcs* self, /*@shared@*/ PyObject* value, /*@unused@*/ void* closure) { Py_XDECREF(self->py_sip); self->py_sip = NULL; self->x.sip = NULL; if (value != NULL && value != Py_None) { if (!PyObject_TypeCheck(value, &PySipType)) { PyErr_SetString(PyExc_TypeError, "sip must be Sip object"); return -1; } Py_INCREF(value); self->py_sip = value; self->x.sip = &(((PySip*)value)->x); } return 0; } static PyObject* PyWcs___copy__( PyWcs* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyObject* copy = NULL; copy = PyWcs_new(&PyWcsType, NULL, NULL); if (copy == NULL) { return NULL; } if (self->py_det2im[0]) { PyWcs_set_det2im1((PyWcs*)copy, self->py_det2im[0], NULL); } if (self->py_det2im[1]) { PyWcs_set_det2im2((PyWcs*)copy, self->py_det2im[1], NULL); } if (self->py_sip) { PyWcs_set_sip((PyWcs*)copy, self->py_sip, NULL); } if (self->py_distortion_lookup[0]) { PyWcs_set_cpdis1((PyWcs*)copy, self->py_distortion_lookup[0], NULL); } if (self->py_distortion_lookup[1]) { PyWcs_set_cpdis2((PyWcs*)copy, self->py_distortion_lookup[1], NULL); } if (self->py_wcsprm) { PyWcs_set_wcs((PyWcs*)copy, self->py_wcsprm, NULL); } return copy; } static int _deepcopy_helper( PyWcs* copy, PyObject* item, int (*function)(PyWcs*, PyObject*, void*), PyObject* memo) { PyObject* obj_copy; if (item) { obj_copy = get_deepcopy(item, memo); if (obj_copy == NULL) { return 1; } if (function(copy, obj_copy, NULL)) { Py_DECREF(obj_copy); return 1; } Py_DECREF(obj_copy); } return 0; } static PyObject* PyWcs___deepcopy__( PyWcs* self, PyObject* memo, /*@unused@*/ PyObject* kwds) { PyWcs* copy; copy = (PyWcs*)PyWcs_new(&PyWcsType, NULL, NULL); if (copy == NULL) { return NULL; } if (_deepcopy_helper(copy, self->py_det2im[0], PyWcs_set_det2im1, memo) || _deepcopy_helper(copy, self->py_det2im[1], PyWcs_set_det2im2, memo) || _deepcopy_helper(copy, self->py_sip, PyWcs_set_sip, memo) || _deepcopy_helper(copy, self->py_distortion_lookup[0], PyWcs_set_cpdis1, memo) || _deepcopy_helper(copy, self->py_distortion_lookup[1], PyWcs_set_det2im1, memo) || _deepcopy_helper(copy, self->py_wcsprm, PyWcs_set_wcs, memo)) { Py_DECREF(copy); return NULL; } return (PyObject*)copy; } static PyObject* _sanity_check( PyObject* self, PyObject* args, PyObject* kwds) { if (sizeof(WCSLIB_INT64) != 8) { Py_INCREF(Py_False); return Py_False; } Py_INCREF(Py_True); return Py_True; } /*************************************************************************** * PyWcs definition structures */ static PyGetSetDef PyWcs_getset[] = { {"det2im1", (getter)PyWcs_get_det2im1, (setter)PyWcs_set_det2im1, (char *)doc_det2im1}, {"det2im2", (getter)PyWcs_get_det2im2, (setter)PyWcs_set_det2im2, (char *)doc_det2im2}, {"cpdis1", (getter)PyWcs_get_cpdis1, (setter)PyWcs_set_cpdis1, (char *)doc_cpdis1}, {"cpdis2", (getter)PyWcs_get_cpdis2, (setter)PyWcs_set_cpdis2, (char *)doc_cpdis2}, {"sip", (getter)PyWcs_get_sip, (setter)PyWcs_set_sip, (char *)doc_sip}, {"wcs", (getter)PyWcs_get_wcs, (setter)PyWcs_set_wcs, (char *)doc_wcs}, {NULL} }; static PyMethodDef PyWcs_methods[] = { {"_all_pix2sky", (PyCFunction)PyWcs_all_pix2sky, METH_VARARGS|METH_KEYWORDS, doc_all_pix2sky}, {"__copy__", (PyCFunction)PyWcs___copy__, METH_NOARGS, NULL}, {"__deepcopy__", (PyCFunction)PyWcs___deepcopy__, METH_O, NULL}, {"_det2im", (PyCFunction)PyWcs_det2im, METH_VARARGS|METH_KEYWORDS, doc_det2im}, {"_p4_pix2foc", (PyCFunction)PyWcs_p4_pix2foc, METH_VARARGS|METH_KEYWORDS, doc_p4_pix2foc}, {"_pix2foc", (PyCFunction)PyWcs_pix2foc, METH_VARARGS|METH_KEYWORDS, doc_pix2foc}, {NULL} }; static PyMethodDef module_methods[] = { {"_sanity_check", (PyCFunction)_sanity_check, METH_NOARGS, ""}, {"find_all_wcs", (PyCFunction)PyWcsprm_find_all_wcs, METH_VARARGS|METH_KEYWORDS, doc_find_all_wcs}, {NULL} /* Sentinel */ }; static PyTypeObject PyWcsType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs._Wcs", /*tp_name*/ sizeof(PyWcs), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyWcs_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ 0, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ 0, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE | Py_TPFLAGS_HAVE_GC, /*tp_flags*/ doc_Wcs, /* tp_doc */ (traverseproc)PyWcs_traverse, /* tp_traverse */ (inquiry)PyWcs_clear, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PyWcs_methods, /* tp_methods */ 0, /* tp_members */ PyWcs_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ (initproc)PyWcs_init, /* tp_init */ 0, /* tp_alloc */ PyWcs_new, /* tp_new */ }; /*************************************************************************** * Module-level ***************************************************************************/ int _setup_pywcs_type( PyObject* m) { if (PyType_Ready(&PyWcsType) < 0) return -1; Py_INCREF(&PyWcsType); return PyModule_AddObject(m, "_Wcs", (PyObject *)&PyWcsType); } struct module_state { /* The Sun compiler can't handle empty structs */ #if defined(__SUNPRO_C) || defined(_MSC_VER) int _dummy; #endif }; #if PY3K static struct PyModuleDef moduledef = { PyModuleDef_HEAD_INIT, "_pywcs", NULL, sizeof(struct module_state), module_methods, NULL, NULL, NULL, NULL }; #define INITERROR return NULL PyMODINIT_FUNC PyInit__pywcs(void) #else #define INITERROR return PyMODINIT_FUNC init_pywcs(void) #endif { PyObject* m; wcs_errexc[0] = NULL; /* Success */ wcs_errexc[1] = &PyExc_MemoryError; /* Null wcsprm pointer passed */ wcs_errexc[2] = &PyExc_MemoryError; /* Memory allocation failed */ wcs_errexc[3] = &WcsExc_SingularMatrix; /* Linear transformation matrix is singular */ wcs_errexc[4] = &WcsExc_InconsistentAxisTypes; /* Inconsistent or unrecognized coordinate axis types */ wcs_errexc[5] = &PyExc_ValueError; /* Invalid parameter value */ wcs_errexc[6] = &WcsExc_InvalidTransform; /* Invalid coordinate transformation parameters */ wcs_errexc[7] = &WcsExc_InvalidTransform; /* Ill-conditioned coordinate transformation parameters */ wcs_errexc[8] = &WcsExc_InvalidCoordinate; /* One or more of the pixel coordinates were invalid, */ /* as indicated by the stat vector */ wcs_errexc[9] = &WcsExc_InvalidCoordinate; /* One or more of the world coordinates were invalid, */ /* as indicated by the stat vector */ wcs_errexc[10] = &WcsExc_InvalidCoordinate; /* Invalid world coordinate */ wcs_errexc[11] = &WcsExc_NoSolution; /* no solution found in the specified interval */ wcs_errexc[12] = &WcsExc_InvalidSubimageSpecification; /* Invalid subimage specification (no spectral axis) */ wcs_errexc[13] = &WcsExc_NonseparableSubimageCoordinateSystem; /* Non-separable subimage coordinate system */ #if PY3K m = PyModule_Create(&moduledef); #else m = Py_InitModule3("_pywcs", module_methods, NULL); #endif if (m == NULL) INITERROR; import_array(); fill_docstrings(); if (_setup_api(m) || _setup_str_list_proxy_type(m) || _setup_wcsprm_type(m) || _setup_tabprm_type(m) || _setup_units_type(m) || /* _setup_wtbarr_type(m) || */ _setup_distortion_type(m) || _setup_sip_type(m) || _setup_pywcs_type(m) || _define_exceptions(m)) { Py_DECREF(m); INITERROR; } #if PY3K return m; #endif } pywcs-1.12/src/pywcs.h0000644001153600020070000000421712310355626016757 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __PYWCS_H__ #define __PYWCS_H__ /* * This is necessary to avoid the wcsset() function that is in the * Windows libraries. We define it here so that any other module that * also uses pywcs C code can also get the right behavior. */ #ifdef _WIN32 #define __STDC__ 1 #endif /* util.h must be imported first */ #include "pyutil.h" #include "pipeline.h" typedef struct { PyObject_HEAD pipeline_t x; /*@shared@*/ PyObject* py_det2im[2]; /*@null@*/ /*@shared@*/ PyObject* py_sip; /*@shared@*/ PyObject* py_distortion_lookup[2]; /*@null@*/ /*@shared@*/ PyObject* py_wcsprm; } PyWcs; #endif /* __PYWCS_H__ */ pywcs-1.12/src/pywcs_api.c0000644001153600020070000000554412310355626017607 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ #define NO_IMPORT_ARRAY #include "pywcs_api.h" int PyWcs_GetCVersion(void) { return REVISION; } void* PyWcs_API[] = { /* 0 */ (void *)PyWcs_GetCVersion, /* pyutil.h */ /* 1 */ (void *)wcsprm_python2c, /* 2 */ (void *)wcsprm_c2python, /* distortion.h */ /* 3 */ (void *)distortion_lookup_t_init, /* 4 */ (void *)distortion_lookup_t_free, /* 5 */ (void *)get_distortion_offset, /* 6 */ (void *)p4_pix2foc, /* 7 */ (void *)p4_pix2deltas, /* sip.h */ /* 8 */ (void *)sip_clear, /* 9 */ (void *)sip_init, /* 10 */ (void *)sip_free, /* 11 */ (void *)sip_pix2foc, /* 12 */ (void *)sip_pix2deltas, /* 13 */ (void *)sip_foc2pix, /* 14 */ (void *)sip_foc2deltas, /* pipeline.h */ /* 15 */ (void *)pipeline_clear, /* 16 */ (void *)pipeline_init, /* 17 */ (void *)pipeline_free, /* 18 */ (void *)pipeline_all_pixel2world, /* 19 */ (void *)pipeline_pix2foc, /* wcs.h */ /* 20 */ (void *)wcsp2s, /* 21 */ (void *)wcss2p, /* 22 */ (void *)wcsprt, /* new for api version 2 */ /* 23 */ (void *)wcslib_get_error_message, /* new for api version 3 */ /* 24 */ (void *)wcsprintf_buf }; int _setup_api(PyObject *m) { PyObject* c_api; #if PY_VERSION_HEX >= 0x03020000 c_api = PyCapsule_New((void *)PyWcs_API, "_pywcs._PYWCS_API", NULL); #else c_api = PyCObject_FromVoidPtr((void *)PyWcs_API, NULL); #endif PyModule_AddObject(m, "_PYWCS_API", c_api); return 0; } pywcs-1.12/src/pywcs_api.h0000644001153600020070000001404012310355626017603 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ #ifndef PYWCS_API_H #define PYWCS_API_H #include "wcsconfig.h" #include "pyutil.h" #include "distortion.h" #include "pipeline.h" #include "sip.h" #include "wcs.h" #include "wcsprintf.h" /* HOW TO UPDATE THE PUBLIC API This code uses a table of function pointers to dynamically expose the public API to other code that wants to use pywcs from C. Each function should be: 1) Declared, as usual for C, in a .h file 2) Defined in a .c file that is compiled as part of the _pywcs.so file 3) Have a macro that maps the function name to a position in the function table. That macro should go in this file (pywcs_api.h) 4) An entry in the function table, which lives in pywcs_api.c Every time the function signatures change, or functions are added or removed from the table, the value of REVISION should be incremented. This allows for a rudimentary version check upon dynamic linking to the pywcs module. */ #define REVISION 3 #ifdef PYWCS_BUILD int _setup_api(PyObject* m); #else #if defined(NO_IMPORT_PYWCS_API) extern void** PyWcs_API; #else void** PyWcs_API; #endif /* defined(NO_IMPORT_PYWCS_API) */ /* Function macros that delegate to a function pointer in the PyWCS_API table */ #define PyWcs_GetCVersion (*(int (*)(void)) PyWcs_API[0]) #define wcsprm_python2c (*(void (*)(struct wcsprm*)) PyWcs_API[1]) #define wcsprm_c2python (*(void (*)(struct wcsprm*)) PyWcs_API[2]) #define distortion_lookup_t_init (*(int (*)(distortion_lookup_t* lookup)) PyWcs_API[3]) #define distortion_lookup_t_free (*(void (*)(distortion_lookup_t* lookup)) PyWcs_API[4]) #define get_distortion_offset (*(double (*)(const distortion_lookup_t*, const double* const)) PyWcs_API[5]) #define p4_pix2foc (*(int (*)(const unsigned int, const distortion_lookup_t**, const unsigned int, const double *, double *)) PyWcs_API[6]) #define p4_pix2deltas (*(int (*)(const unsigned int, const distortion_lookup_t**, const unsigned int, const double *, double *)) PyWcs_API[7]) #define sip_clear (*(void (*)(sip_t*) PyWcs_API[8])) #define sip_init (*(int (*)(sip_t*, unsigned int, double*, unsigned int, double*, unsigned int, double*, unsigned int, double*, double*)) PyWcs_API[9]) #define sip_free (*(void (*)(sip_t*) PyWcs_API[10])) #define sip_pix2foc (*(int (*)(sip_t*, unsigned int, unsigned int, double*, double*)) PyWcs_API[11]) #define sip_pix2deltas (*(int (*)(sip_t*, unsigned int, unsigned int, double*, double*)) PyWcs_API[12]) #define sip_foc2pix (*(int (*)(sip_t*, unsigned int, unsigned int, double*, double*)) PyWcs_API[13]) #define sip_foc2deltas (*(int (*)(sip_t*, unsigned int, unsigned int, double*, double*)) PyWcs_API[14]) #define pipeline_clear (*(void (*)(pipeline_t*)) PyWcs_API[15]) #define pipeline_init (*(void (*)(pipeline_t*, sip_t*, distortion_lookup_t**, struct wcsprm*)) PyWcs_API[16]) #define pipeline_free (*(void (*)(pipeline_t*)) PyWcs_API[17]) #define pipeline_all_pixel2world (*(int (*)(pipeline_t*, unsigned int, unsigned int, double*, double*)) PyWcs_API[18]) #define pipeline_pix2foc (*(int (*)(pipeline_t*, unsigned int, unsigned int, double*, double*)) PyWcs_API[19]) #define wcsp2s (*(int (*)(struct wcsprm *, int, int, const double[], double[], double[], double[], double[], int[])) PyWcs_API[20]) #define wcss2p (*(int (*)(struct wcsprm *, int, int, const double[], double[], double[], double[], double[], int[])) PyWcs_API[21]) #define wcsprt (*(int (*)(struct wcsprm *)) PyWcs_API[22]) #define wcslib_get_error_message (*(const char* (*)(int)) PyWcs_API[23]) #define wcsprintf_buf (*(const char * (*)()) PyWCS_API[24]) #ifndef NO_IMPORT_PYWCS_API int import_pywcs(void) { PyObject *pywcs_module = NULL; PyObject *c_api = NULL; int status = -1; #if PY_VERSION_HEX >= 0x03020000 PyWcs_API = (void **)PyCapsule_Import("pywcs._pywcs._WCS_API", 0); if (PyWcs_API == NULL) goto exit; #else pywcs_module = PyImport_ImportModule("pywcs._pywcs"); if (pywcs_module == NULL) goto exit; c_api = PyObject_GetAttrString(pywcs_module, "_PYWCS_API"); if (c_api == NULL) goto exit; if (PyCObject_Check(c_api)) { PyWcs_API = (void **)PyCObject_AsVoidPtr(c_api); } else { goto exit; } #endif /* Perform runtime check of C API version */ if (REVISION != PyWcs_GetCVersion()) { PyErr_Format( PyExc_ImportError, "module compiled against " \ "ABI version '%x' but this version of pywcs is '%x'", \ (int)REVISION, (int)PyWcs_GetCVersion()); return -1; } exit: Py_XDECREF(pywcs_module); Py_XDECREF(c_api); return status; } #endif /* !defined(NO_IMPORT_PYWCS_API) */ #endif /* PYWCS_BUILD */ #endif /* PYWCS_API_H */ pywcs-1.12/src/sip.c0000644001153600020070000002140312310355626016374 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #include "sip.h" #include #include #include #define SIP_ERRMSG(status) WCSERR_SET(status) void sip_clear( sip_t* sip) { assert(sip != NULL); sip->a_order = 0; sip->a = NULL; sip->b_order = 0; sip->b = NULL; sip->ap_order = 0; sip->ap = NULL; sip->bp_order = 0; sip->bp = NULL; sip->crpix[0] = 0.0; sip->crpix[1] = 0.0; sip->scratch = NULL; sip->err = NULL; } int sip_init( sip_t* sip, const unsigned int a_order, const double* a, const unsigned int b_order, const double* b, const unsigned int ap_order, const double* ap, const unsigned int bp_order, const double* bp, const double* crpix /* [2] */) { unsigned int a_size = 0; unsigned int b_size = 0; unsigned int ap_size = 0; unsigned int bp_size = 0; unsigned int scratch_size = 0; int status = 0; struct wcserr** err = NULL; static const char *function = "sip_init"; assert(sip != NULL); sip_clear(sip); err = &(sip->err); /* We we have one of A/B or AP/BP, we must have both. */ if ((a == NULL) ^ (b == NULL)) { return wcserr_set( SIP_ERRMSG(WCSERR_BAD_COORD_TRANS), "Both A and B SIP transform must be defined"); } if ((ap == NULL) ^ (bp == NULL)) { return wcserr_set( SIP_ERRMSG(WCSERR_BAD_COORD_TRANS), "Both AP and BP SIP transform must be defined"); } if (a != NULL) { sip->a_order = a_order; a_size = (a_order + 1) * (a_order + 1) * sizeof(double); sip->a = malloc(a_size); if (sip->a == NULL) { sip_free(sip); status = wcserr_set( SIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } memcpy(sip->a, a, a_size); if (a_order > scratch_size) { scratch_size = a_order; } sip->b_order = b_order; b_size = (b_order + 1) * (b_order + 1) * sizeof(double); sip->b = malloc(b_size); if (sip->b == NULL) { sip_free(sip); status = wcserr_set( SIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } memcpy(sip->b, b, b_size); if (b_order > scratch_size) { scratch_size = b_order; } } if (ap != NULL) { sip->ap_order = ap_order; ap_size = (ap_order + 1) * (ap_order + 1) * sizeof(double); sip->ap = malloc(ap_size); if (sip->ap == NULL) { sip_free(sip); status = wcserr_set( SIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } memcpy(sip->ap, ap, ap_size); if (ap_order > scratch_size) { scratch_size = ap_order; } sip->bp_order = bp_order; bp_size = (bp_order + 1) * (bp_order + 1) * sizeof(double); sip->bp = malloc(bp_size); if (sip->bp == NULL) { sip_free(sip); status = wcserr_set( SIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } memcpy(sip->bp, bp, bp_size); if (bp_order > scratch_size) { scratch_size = bp_order; } } scratch_size = (scratch_size + 1) * sizeof(double); sip->scratch = malloc(scratch_size); if (sip->scratch == NULL) { sip_free(sip); status = wcserr_set( SIP_ERRMSG(WCSERR_MEMORY), "Memory allocation failed"); goto exit; } sip->crpix[0] = crpix[0]; sip->crpix[1] = crpix[1]; exit: return status; } void sip_free(sip_t* sip) { free(sip->a); sip->a = NULL; free(sip->b); sip->b = NULL; free(sip->ap); sip->ap = NULL; free(sip->bp); sip->bp = NULL; free(sip->scratch); sip->scratch = NULL; free(sip->err); sip->err = NULL; } static pywcs_inline double lu( const unsigned int order, const double* const matrix, const int x, const int y) { int index; assert(x >= 0 && x <= (int)order); assert(y >= 0 && y <= (int)order); index = x * ((int)order + 1) + y; assert(index >= 0 && index < ((int)order + 1) * ((int)order + 1)); return matrix[index]; } static int sip_compute( /*@unused@*/ const unsigned int naxes, const unsigned int nelem, const unsigned int m, /*@null@*/ const double* a, const unsigned int n, /*@null@*/ const double* b, const double* crpix /* [2] */, /*@null@*/ double* tmp, /*@null@*/ const double* input /* [NAXES][nelem] */, /*@null@*/ double* output /* [NAXES][nelem] */) { unsigned int i; int j, k; double x, y; double sum; const double* input_ptr; double* output_ptr; assert(a != NULL); assert(b != NULL); assert(crpix != NULL); assert(tmp != NULL); assert(input != NULL); assert(output != NULL); /* Avoid segfaults */ if (input == NULL || output == NULL || tmp == NULL || crpix == NULL) { return 1; } /* If we have one, we must have both... */ if ((a == NULL) ^ (b == NULL)) { return 6; } /* If no distortion, just return values */ if (a == NULL /* && b == NULL ... implied */) { return 0; } input_ptr = input; output_ptr = output; for (i = 0; i < nelem; ++i) { x = *input_ptr++ - crpix[0]; y = *input_ptr++ - crpix[1]; for (j = 0; j <= (int)m; ++j) { tmp[j] = lu(m, a, (int)m-j, j); for (k = j-1; k >= 0; --k) { tmp[j] = (y * tmp[j]) + lu(m, a, (int)m-j, k); } } sum = tmp[0]; for (j = (int)m; j > 0; --j) { sum = x * sum + tmp[(int)m - j + 1]; } *output_ptr++ += sum; for (j = 0; j <= (int)n; ++j) { tmp[j] = lu(n, b, (int)n-j, j); for (k = j-1; k >= 0; --k) { tmp[j] = (y * tmp[j]) + lu(n, b, (int)n-j, k); } } sum = tmp[0]; for (j = (int)n; j > 0; --j) { sum = x * sum + tmp[n - j + 1]; } *output_ptr++ += sum; } return 0; } int sip_pix2deltas( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* pix /* [NAXES][nelem] */, double* deltas /* [NAXES][nelem] */) { if (sip == NULL) { return 1; } return sip_compute(naxes, nelem, sip->a_order, sip->a, sip->b_order, sip->b, sip->crpix, (double *)sip->scratch, pix, deltas); } int sip_foc2deltas( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* foc /* [NAXES][nelem] */, double* deltas /* [NAXES][nelem] */) { if (sip == NULL) { return 1; } return sip_compute(naxes, nelem, sip->ap_order, sip->ap, sip->bp_order, sip->bp, sip->crpix, (double *)sip->scratch, foc, deltas); } int sip_pix2foc( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* pix /* [NAXES][nelem] */, double* foc /* [NAXES][nelem] */) { assert(pix); assert(foc); if (pix != foc) { memcpy(foc, pix, sizeof(double) * naxes * nelem); } return sip_pix2deltas(sip, naxes, nelem, pix, foc); } int sip_foc2pix( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* foc /* [NAXES][nelem] */, double* pix /* [NAXES][nelem] */) { assert(pix); assert(foc); if (pix != foc) { memcpy(pix, foc, sizeof(double) * naxes * nelem); } return sip_foc2deltas(sip, naxes, nelem, foc, pix); } pywcs-1.12/src/sip.h0000644001153600020070000001306312310355626016404 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __SIP_H__ #define __SIP_H__ #include "util.h" typedef struct { unsigned int a_order; /*@null@*/ /*@shared@*/ double* a; unsigned int b_order; /*@null@*/ /*@shared@*/ double* b; unsigned int ap_order; /*@null@*/ /*@shared@*/ double* ap; unsigned int bp_order; /*@null@*/ /*@shared@*/ double* bp; double crpix[2]; /*@null@*/ double* scratch; struct wcserr* err; } sip_t; /** Sets all the values of the sip_t structure to NULLs or zeros. */ void sip_clear(sip_t* sip); /** Set the values of the sip_t structure. The values expected are all exactly as defined in the FITS SIP header keywords. The arrays/matrices are all *copied* into the SIP struct. To free the memory that sip_t allocates for itself, call sip_free. @param a_order: The order of the A_i_j matrix @param a: The A_i_j array, which must be of size [a_order+1][a_order+1] @param b_order: The order of the B_i_j matrix @param b: The B_i_j array, which must be of size [b_order+1][b_order+1] @param ap_order: The order of the AP_i_j matrix @param ap: The AP_i_j array, which must be of size [ap_order+1][ap_order+1] @param bp_order: The order of the BP_i_j matrix @param bp: The BP_i_j array, which must be of size [bp_order+1][bp_order+1] @param crpix: The position of the reference pixel */ int sip_init( sip_t* sip, const unsigned int a_order, const double* a, const unsigned int b_order, const double* b, const unsigned int ap_order, const double* ap, const unsigned int bp_order, const double* bp, const double* crpix /* [2] */); /** Frees the memory allocated for the sip_t struct. */ void sip_free(sip_t* sip); /** Converts pixel coordinates to focal plane coordinates using the SIP polynomial distortion convention, and the values stored in the sip_t struct. @param naxes @param nelem @param pix [in]: An array of pixel coordinates @param foc [out]: An array of focal plane coordinates @return A wcslib error code */ int sip_pix2foc( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* pix /* [NAXES][nelem] */, double* foc /* [NAXES][nelem] */); /** Computes the offset deltas necessary to convert pixel coordinates to focal plane coordinates using the SIP polynomial distortion convention, and the values stored in the sip_t struct. The deltas are added to the existing values in pix. @param naxes @param nelem @param pix [in]: An array of pixel coordinates @param foc [in/out]: An array of deltas, that when added to pix results in focal plane coordinates. @return A wcslib error code */ int sip_pix2deltas( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* pix /* [NAXES][nelem] */, double* foc /* [NAXES][nelem] */); /** Adds the offset deltas necessary to convert focal plane coordinates to pixel coordinates using the SIP polynomial distortion convention, and the values stored in the sip_t struct. The deltas are added to the existing values in pix. @param naxes @param nelem @param foc [in]: An array of focal plane coordinates @param pix [in/out]: An array of pixel coordinates @return A wcslib error code */ int sip_foc2pix( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* foc /* [NAXES][nelem] */, double* pix /* [NAXES][nelem] */); /** Computes the offset deltas necessary to convert focal plane coordinates to pixel coordinates using the SIP polynomial distortion convention, and the values stored in the sip_t struct. The deltas are added to the existing values in foc. @param naxes @param nelem @param foc [in]: An array of focal plane coordinates @param foc [in/out]: An array of deltas, that when added to pix results in focal plane coordinates. @return A wcslib error code */ int sip_foc2deltas( const sip_t* sip, const unsigned int naxes, const unsigned int nelem, const double* foc /* [NAXES][nelem] */, double* deltas /* [NAXES][nelem] */); #endif pywcs-1.12/src/sip_wrap.c0000644001153600020070000003343612310355626017436 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "sip_wrap.h" #include "docstrings.h" #include "wcs.h" static void PySip_dealloc( PySip* self) { sip_free(&self->x); Py_TYPE(self)->tp_free((PyObject*)self); } /*@null@*/ static PyObject * PySip_new( PyTypeObject* type, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PySip* self; self = (PySip*)type->tp_alloc(type, 0); if (self != NULL) { sip_clear(&self->x); } return (PyObject*)self; } static int convert_matrix( /*@null@*/ PyObject* pyobj, PyArrayObject** array, double** data, unsigned int* order) { if (pyobj == Py_None) { *array = NULL; *data = NULL; *order = 0; return 0; } *array = (PyArrayObject*)PyArray_ContiguousFromAny( pyobj, PyArray_DOUBLE, 2, 2); if (*array == NULL) { return -1; } if (PyArray_DIM(*array, 0) != PyArray_DIM(*array, 1)) { PyErr_SetString(PyExc_ValueError, "Matrix must be square."); return -1; } *data = (double*)PyArray_DATA(*array); *order = (unsigned int)PyArray_DIM(*array, 0) - 1; return 0; } static int PySip_init( PySip* self, PyObject* args, /*@unused@*/ PyObject* kwds) { PyObject* py_a = NULL; PyObject* py_b = NULL; PyObject* py_ap = NULL; PyObject* py_bp = NULL; PyObject* py_crpix = NULL; PyArrayObject* a = NULL; PyArrayObject* b = NULL; PyArrayObject* ap = NULL; PyArrayObject* bp = NULL; PyArrayObject* crpix = NULL; double* a_data = NULL; double* b_data = NULL; double* ap_data = NULL; double* bp_data = NULL; unsigned int a_order = 0; unsigned int b_order = 0; unsigned int ap_order = 0; unsigned int bp_order = 0; int status = -1; if (!PyArg_ParseTuple(args, "OOOOO:Sip.__init__", &py_a, &py_b, &py_ap, &py_bp, &py_crpix)) { return -1; } if (convert_matrix(py_a, &a, &a_data, &a_order) || convert_matrix(py_b, &b, &b_data, &b_order) || convert_matrix(py_ap, &ap, &ap_data, &ap_order) || convert_matrix(py_bp, &bp, &bp_data, &bp_order)) { goto exit; } crpix = (PyArrayObject*)PyArray_ContiguousFromAny(py_crpix, PyArray_DOUBLE, 1, 1); if (crpix == NULL) { goto exit; } if (PyArray_DIM(crpix, 0) != 2) { PyErr_SetString(PyExc_ValueError, "CRPIX wrong length"); goto exit; } status = sip_init(&self->x, a_order, a_data, b_order, b_data, ap_order, ap_data, bp_order, bp_data, PyArray_DATA(crpix)); exit: Py_XDECREF(a); Py_XDECREF(b); Py_XDECREF(ap); Py_XDECREF(bp); Py_XDECREF(crpix); if (status == 0) { return 0; } else if (status == -1) { /* Exception already set */ return -1; } else { wcserr_to_python_exc(self->x.err); return -1; } } /*@null@*/ static PyObject* PySip_pix2foc( PySip* self, PyObject* args, PyObject* kwds) { PyObject* pixcrd_obj = NULL; int origin = 1; PyArrayObject* pixcrd = NULL; PyArrayObject* foccrd = NULL; int status = -1; const char* keywords[] = { "pixcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords(args, kwds, "Oi:pix2foc", (char **)keywords, &pixcrd_obj, &origin)) { return NULL; } if (self->x.a == NULL || self->x.b == NULL) { PyErr_SetString( PyExc_ValueError, "SIP object does not have coefficients for pix2foc transformation (A and B)"); return NULL; } pixcrd = (PyArrayObject*)PyArray_ContiguousFromAny(pixcrd_obj, PyArray_DOUBLE, 2, 2); if (pixcrd == NULL) { goto exit; } if (PyArray_DIM(pixcrd, 1) != 2) { PyErr_SetString(PyExc_ValueError, "Pixel array must be an Nx2 array"); goto exit; } foccrd = (PyArrayObject*)PyArray_SimpleNew(2, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (foccrd == NULL) { goto exit; } Py_BEGIN_ALLOW_THREADS preoffset_array(pixcrd, origin); status = sip_pix2foc(&self->x, (unsigned int)PyArray_DIM(pixcrd, 1), (unsigned int)PyArray_DIM(pixcrd, 0), (const double*)PyArray_DATA(pixcrd), (double*)PyArray_DATA(foccrd)); unoffset_array(pixcrd, origin); unoffset_array(foccrd, origin); Py_END_ALLOW_THREADS exit: Py_XDECREF(pixcrd); if (status == 0) { return (PyObject*)foccrd; } else { Py_XDECREF(foccrd); if (status == -1) { /* Exception already set */ return NULL; } else { wcserr_to_python_exc(self->x.err); return NULL; } } } /*@null@*/ static PyObject* PySip_foc2pix( PySip* self, PyObject* args, PyObject* kwds) { PyObject* foccrd_obj = NULL; int origin = 1; PyArrayObject* foccrd = NULL; PyArrayObject* pixcrd = NULL; int status = -1; const char* keywords[] = { "foccrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords(args, kwds, "Oi:foc2pix", (char **)keywords, &foccrd_obj, &origin)) { return NULL; } if (self->x.ap == NULL || self->x.bp == NULL) { PyErr_SetString( PyExc_ValueError, "SIP object does not have coefficients for foc2pix transformation (AP and BP)"); return NULL; } foccrd = (PyArrayObject*)PyArray_ContiguousFromAny(foccrd_obj, PyArray_DOUBLE, 2, 2); if (foccrd == NULL) { goto exit; } if (PyArray_DIM(foccrd, 1) != 2) { PyErr_SetString(PyExc_ValueError, "Pixel array must be an Nx2 array"); goto exit; } pixcrd = (PyArrayObject*)PyArray_SimpleNew(2, PyArray_DIMS(foccrd), PyArray_DOUBLE); if (pixcrd == NULL) { status = 2; goto exit; } Py_BEGIN_ALLOW_THREADS preoffset_array(foccrd, origin); status = sip_foc2pix(&self->x, (unsigned int)PyArray_DIM(pixcrd, 1), (unsigned int)PyArray_DIM(pixcrd, 0), (double*)PyArray_DATA(foccrd), (double*)PyArray_DATA(pixcrd)); unoffset_array(foccrd, origin); unoffset_array(pixcrd, origin); Py_END_ALLOW_THREADS exit: Py_XDECREF(foccrd); if (status == 0) { return (PyObject*)pixcrd; } else { Py_XDECREF(pixcrd); if (status == -1) { /* Exception already set */ return NULL; } else { wcserr_to_python_exc(self->x.err); return NULL; } } } /*@null@*/ static PyObject* PySip_get_a( PySip* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (self->x.a == NULL) { Py_INCREF(Py_None); return Py_None; } dims[0] = (npy_intp)self->x.a_order + 1; dims[1] = (npy_intp)self->x.a_order + 1; return get_double_array("a", self->x.a, 2, dims, (PyObject*)self); } /*@null@*/ static PyObject* PySip_get_b( PySip* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (self->x.b == NULL) { Py_INCREF(Py_None); return Py_None; } dims[0] = (npy_intp)self->x.b_order + 1; dims[1] = (npy_intp)self->x.b_order + 1; return get_double_array("b", self->x.b, 2, dims, (PyObject*)self); } /*@null@*/ static PyObject* PySip_get_ap( PySip* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (self->x.ap == NULL) { Py_INCREF(Py_None); return Py_None; } dims[0] = (npy_intp)self->x.ap_order + 1; dims[1] = (npy_intp)self->x.ap_order + 1; return get_double_array("ap", self->x.ap, 2, dims, (PyObject*)self); } /*@null@*/ static PyObject* PySip_get_bp( PySip* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (self->x.bp == NULL) { Py_INCREF(Py_None); return Py_None; } dims[0] = (npy_intp)self->x.bp_order + 1; dims[1] = (npy_intp)self->x.bp_order + 1; return get_double_array("bp", self->x.bp, 2, dims, (PyObject*)self); } static PyObject* PySip_get_a_order( PySip* self, /*@unused@*/ void* closure) { return get_int("a_order", (long int)self->x.a_order); } static PyObject* PySip_get_b_order( PySip* self, /*@unused@*/ void* closure) { return get_int("b_order", (long int)self->x.b_order); } static PyObject* PySip_get_ap_order( PySip* self, /*@unused@*/ void* closure) { return get_int("ap_order", (long int)self->x.ap_order); } static PyObject* PySip_get_bp_order( PySip* self, /*@unused@*/ void* closure) { return get_int("bp_order", (long int)self->x.bp_order); } static PyObject* PySip_get_crpix( PySip* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 2; return get_double_array("crpix", self->x.crpix, 1, &naxis, (PyObject*)self); } static PyObject* PySip___copy__( PySip* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PySip* copy = NULL; copy = (PySip*)PySip_new(&PySipType, NULL, NULL); if (copy == NULL) { return NULL; } if (sip_init(©->x, self->x.a_order, self->x.a, self->x.b_order, self->x.b, self->x.ap_order, self->x.ap, self->x.bp_order, self->x.bp, self->x.crpix)) { Py_DECREF(copy); return NULL; } return (PyObject*)copy; } static PyGetSetDef PySip_getset[] = { {"a", (getter)PySip_get_a, NULL, (char *)doc_a}, {"a_order", (getter)PySip_get_a_order, NULL, (char *)doc_a_order}, {"b", (getter)PySip_get_b, NULL, (char *)doc_b}, {"b_order", (getter)PySip_get_b_order, NULL, (char *)doc_b_order}, {"ap", (getter)PySip_get_ap, NULL, (char *)doc_ap}, {"ap_order", (getter)PySip_get_ap_order, NULL, (char *)doc_ap_order}, {"bp", (getter)PySip_get_bp, NULL, (char *)doc_bp}, {"bp_order", (getter)PySip_get_bp_order, NULL, (char *)doc_bp_order}, {"crpix", (getter)PySip_get_crpix, NULL, (char *)doc_crpix}, {NULL} }; static PyMethodDef PySip_methods[] = { {"__copy__", (PyCFunction)PySip___copy__, METH_NOARGS, NULL}, {"__deepcopy__", (PyCFunction)PySip___copy__, METH_O, NULL}, {"pix2foc", (PyCFunction)PySip_pix2foc, METH_VARARGS|METH_KEYWORDS, doc_sip_pix2foc}, {"foc2pix", (PyCFunction)PySip_foc2pix, METH_VARARGS|METH_KEYWORDS, doc_sip_foc2pix}, {NULL} }; PyTypeObject PySipType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs.Sip", /*tp_name*/ sizeof(PySip), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PySip_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ 0, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ 0, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE, /*tp_flags*/ doc_Sip, /* tp_doc */ 0, /* tp_traverse */ 0, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PySip_methods, /* tp_methods */ 0, /* tp_members */ PySip_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ (initproc)PySip_init, /* tp_init */ 0, /* tp_alloc */ PySip_new, /* tp_new */ }; int _setup_sip_type( PyObject* m) { if (PyType_Ready(&PySipType) < 0) return -1; Py_INCREF(&PySipType); return PyModule_AddObject(m, "Sip", (PyObject *)&PySipType); } pywcs-1.12/src/sip_wrap.h0000644001153600020070000000333112310355626017432 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __SIP_WRAP_H__ #define __SIP_WRAP_H__ #include "pyutil.h" #include "sip.h" extern PyTypeObject PySipType; typedef struct { PyObject_HEAD sip_t x; } PySip; int _setup_sip_type( PyObject* m); #endif pywcs-1.12/src/str_list_proxy.c0000644001153600020070000002040012310355626020701 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "pyutil.h" /*************************************************************************** * List-of-strings proxy object ***************************************************************************/ static PyTypeObject PyStrListProxyType; typedef struct { PyObject_HEAD /*@null@*/ /*@shared@*/ PyObject* pyobject; Py_ssize_t size; Py_ssize_t maxsize; char (*array)[72]; str_verify_fn verify; } PyStrListProxy; static void PyStrListProxy_dealloc( PyStrListProxy* self) { Py_XDECREF(self->pyobject); Py_TYPE(self)->tp_free((PyObject*)self); } /*@null@*/ static PyObject * PyStrListProxy_new( PyTypeObject* type, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyStrListProxy* self = NULL; self = (PyStrListProxy*)type->tp_alloc(type, 0); if (self != NULL) { self->pyobject = NULL; } return (PyObject*)self; } static int PyStrListProxy_traverse( PyStrListProxy* self, visitproc visit, void *arg) { int vret; if (self->pyobject) { vret = visit(self->pyobject, arg); if (vret != 0) { return vret; } } return 0; } static int PyStrListProxy_clear( PyStrListProxy *self) { PyObject *tmp; tmp = self->pyobject; self->pyobject = NULL; Py_XDECREF(tmp); return 0; } /*@null@*/ PyObject * PyStrListProxy_New( /*@shared@*/ PyObject* owner, Py_ssize_t size, Py_ssize_t maxsize, char (*array)[72], str_verify_fn verify) { PyStrListProxy* self = NULL; if (maxsize == 0) { maxsize = 68; } self = (PyStrListProxy*)PyStrListProxyType.tp_alloc(&PyStrListProxyType, 0); if (self == NULL) { return NULL; } Py_XINCREF(owner); self->pyobject = owner; self->size = size; self->maxsize = maxsize; self->array = array; self->verify = verify; return (PyObject*)self; } static Py_ssize_t PyStrListProxy_len( PyStrListProxy* self) { return self->size; } /*@null@*/ static PyObject* PyStrListProxy_getitem( PyStrListProxy* self, Py_ssize_t index) { if (index >= self->size) { PyErr_SetString(PyExc_IndexError, "index out of range"); return NULL; } #if PY3K return PyBytes_FromString(self->array[index]); #else return PyString_FromString(self->array[index]); #endif } static int PyStrListProxy_setitem( PyStrListProxy* self, Py_ssize_t index, PyObject* arg) { char* value; Py_ssize_t value_length; if (index > self->size) { PyErr_SetString(PyExc_IndexError, "index out of range"); return -1; } #if PY3K if (PyBytes_AsStringAndSize(arg, &value, &value_length)) { #else if (PyString_AsStringAndSize(arg, &value, &value_length)) { #endif return -1; } if (value_length >= self->maxsize) { PyErr_Format(PyExc_ValueError, "string must be less than %zd characters", self->maxsize); return -1; } if (self->verify && !self->verify(value)) { return -1; } strncpy(self->array[index], value, self->maxsize); return 0; } /*@null@*/ static PyObject* PyStrListProxy_repr( PyStrListProxy* self) { char* buffer = NULL; char* wp = NULL; char* rp = NULL; Py_ssize_t i = 0; Py_ssize_t j = 0; PyObject* result = NULL; /* These are in descending order, so we can exit the loop quickly. They are in pairs: (char_to_escape, char_escaped) */ const char* escapes = "\\\\''\rr\ff\vv\nn\tt\bb\aa"; const char* e = NULL; char next_char = '\0'; /* Overallocating to allow for escaped characters */ buffer = malloc((size_t)self->size*self->maxsize*2 + 2); if (buffer == NULL) { PyErr_SetString(PyExc_MemoryError, "Could not allocate memory."); return NULL; } wp = buffer; *wp++ = '['; for (i = 0; i < self->size; ++i) { *wp++ = '\''; rp = self->array[i]; for (j = 0; j < self->maxsize && *rp != '\0'; ++j) { /* Check if this character should be escaped */ e = escapes; next_char = *rp++; do { if (next_char > *e) { break; } else if (next_char == *e) { *wp++ = '\\'; next_char = *(++e); break; } else { e += 2; } } while (*e != '\0'); *wp++ = next_char; } *wp++ = '\''; /* Add a comma for all but the last one */ if (i != self->size - 1) { *wp++ = ','; *wp++ = ' '; } } *wp++ = ']'; *wp++ = '\0'; #if PY3K result = PyUnicode_FromString(buffer); #else result = PyString_FromString(buffer); #endif free(buffer); return result; } static PySequenceMethods PyStrListProxy_sequence_methods = { (lenfunc)PyStrListProxy_len, NULL, NULL, (ssizeargfunc)PyStrListProxy_getitem, NULL, (ssizeobjargproc)PyStrListProxy_setitem, NULL, NULL, NULL, NULL }; static PyTypeObject PyStrListProxyType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs.StrListProxy", /*tp_name*/ sizeof(PyStrListProxy), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyStrListProxy_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ (reprfunc)PyStrListProxy_repr, /*tp_repr*/ 0, /*tp_as_number*/ &PyStrListProxy_sequence_methods, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ (reprfunc)PyStrListProxy_repr, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_HAVE_GC, /*tp_flags*/ 0, /* tp_doc */ (traverseproc)PyStrListProxy_traverse, /* tp_traverse */ (inquiry)PyStrListProxy_clear, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ 0, /* tp_methods */ 0, /* tp_members */ 0, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ 0, /* tp_init */ 0, /* tp_alloc */ PyStrListProxy_new, /* tp_new */ }; int _setup_str_list_proxy_type( /*@unused@*/ PyObject* m) { if (PyType_Ready(&PyStrListProxyType) < 0) { return 1; } return 0; } pywcs-1.12/src/str_list_proxy.h0000644001153600020070000000422112310355626020711 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __STR_LIST_PROXY_H__ #define __STR_LIST_PROXY_H__ #include "pyutil.h" /*************************************************************************** * List-of-strings proxy object * * A Python object that looks like a list of strings, but is back by a C * char * list[]; ***************************************************************************/ typedef int (*str_verify_fn)(const char *); /*@null@*/ PyObject * PyStrListProxy_New( PyObject* owner, Py_ssize_t size, Py_ssize_t maxsize, char (*array)[72], str_verify_fn verify ); int _setup_str_list_proxy_type( PyObject* m); #endif /* __STR_LIST_PROXY_H__ */ pywcs-1.12/src/util.c0000644001153600020070000000404212310355626016556 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "util.h" #include #include void set_invalid_to_nan( const int ncoord, const int nelem, double* const data, const int* const stat) { int i = 0; double* d = data; const int* s = stat; const int* s_end = stat + ncoord; double n; #ifndef NAN #define INF (DBL_MAX+DBL_MAX) #define NAN (INF-INF) #endif n = NAN; for ( ; s != s_end; ++s) { if (*s) { for (i = 0; i < nelem; ++i) { *d++ = n; } } else { d += nelem; } } } pywcs-1.12/src/util.h0000644001153600020070000000376512310355626016576 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __UTIL_H__ #define __UTIL_H__ #ifdef __SUNPRO_C #define pywcs_inline #endif #ifdef _MSC_VER #define pywcs_inline __inline #endif #ifndef pywcs_inline #define pywcs_inline inline #endif #include #include #include "isnan.h" #undef CLAMP #define CLAMP(x, low, high) (((x) > (high)) ? (high) : (((x) < (low)) ? (low) : (x))) void set_invalid_to_nan( const int ncoord, const int nelem, double* const data, const int* const stat); #endif /* __UTIL_H__ */ pywcs-1.12/src/wcsconfig.h0000644001153600020070000000225012310355731017564 0ustar cslocumSTSCI\science00000000000000 /* WCSLIB library version number. */ #define WCSLIB_VERSION 4.10 /* 64-bit integer data type. */ #define WCSLIB_INT64 long long int /* Windows needs some other defines */ /* I think the only one we need is _WIN32, but the others don't hurt - Mark S. 2012-02-14 */ #if defined(_WIN32) || defined(_MSC_VER) || defined(__MINGW32__) || defined (__MINGW64__) /* * There is a lexical analyzer that was generated by flex. Tell it * that we don't have unistd.h */ #ifndef YY_NO_UNISTD_H #define YY_NO_UNISTD_H #endif /* * Visual C++ will warn you about certain functions that have a * high risk of buffer overflows, such as strcpy(). This * tells the compiler to shut up about it. */ #ifndef _CRT_SECURE_NO_WARNINGS #define _CRT_SECURE_NO_WARNINGS #endif /* * Suppress definition of wcsset() by system include files. * I don't know what's up with mingw. * In Visual C, the __STDC__ excludes non-standard things that * would otherwise be defined in the header files. */ #ifndef _NO_OLDNAMES /* for mingw32 */ #define _NO_OLDNAMES #endif #ifndef NO_OLDNAMES /* for mingw64 */ #define NO_OLDNAMES #endif #ifndef __STDC__ /* for MS Visual C */ #define __STDC__ 1 #endif #endif pywcs-1.12/src/wcslib_tabprm_wrap.c0000644001153600020070000003020312310355626021460 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "wcslib_tabprm_wrap.h" #include #include #include /* It gets to be really tedious to type long docstrings in ANSI C syntax (since multi-line strings literals are not valid). Therefore, the docstrings are written in doc/docstrings.py, which are then converted by setup.py into docstrings.h, which we include here. */ #include "docstrings.h" /*************************************************************************** * Helper functions * ***************************************************************************/ static pywcs_inline void note_change(PyTabprm* self) { self->x->flag = 0; } static int make_fancy_dims(PyTabprm* self, npy_intp* ndims, npy_intp* dims) { npy_intp i, M; M = (npy_intp)self->x->M; if (M + 1 > NPY_MAXDIMS) { PyErr_SetString(PyExc_ValueError, "Too many dimensions"); return -1; } *ndims = M + 1; for (i = 0; i < M; ++i) { dims[i] = self->x->K[M-1-i]; } dims[M] = M; return 0; } PyObject** tab_errexc[6]; static void wcslib_tab_to_python_exc(int status) { if (status > 0 && status < 6) { PyErr_SetString(*tab_errexc[status], tab_errmsg[status]); } else { PyErr_SetString( PyExc_RuntimeError, "Unknown error occurred. Something is seriously wrong."); } } /*************************************************************************** * PyTabprm methods */ static int PyTabprm_traverse( PyTabprm* self, visitproc visit, void *arg) { int vret; vret = visit(self->owner, arg); if (vret != 0) { return vret; } return 0; } static int PyTabprm_clear( PyTabprm* self) { PyObject* tmp; tmp = self->owner; self->owner = NULL; Py_XDECREF(tmp); return 0; } static void PyTabprm_dealloc( PyTabprm* self) { PyTabprm_clear(self); Py_TYPE(self)->tp_free((PyObject*)self); } PyTabprm* PyTabprm_cnew(PyObject* wcsprm, struct tabprm* x) { PyTabprm* self; self = (PyTabprm*)(&PyTabprmType)->tp_alloc(&PyTabprmType, 0); self->x = x; Py_INCREF(wcsprm); self->owner = wcsprm; return self; } static int PyTabprm_cset( PyTabprm* self) { int status = 0; status = tabset(self->x); if (status == 0) { return 0; } else { wcslib_tab_to_python_exc(status); return -1; } } /*@null@*/ static PyObject* PyTabprm_set( PyTabprm* self) { if (PyTabprm_cset(self)) { return NULL; } Py_INCREF(Py_None); return Py_None; } /*@null@*/ static PyObject* PyTabprm_print_contents( PyTabprm* self) { int ignored; if (PyTabprm_cset(self)) { return NULL; } /* This is not thread-safe, but since we're holding onto the GIL, we can assume we won't have thread conflicts */ wcsprintf_set(NULL); ignored = tabprt(self->x); printf("%s", wcsprintf_buf()); Py_INCREF(Py_None); return Py_None; } /*@null@*/ static PyObject* PyTabprm___str__( PyTabprm* self) { int ignored; if (PyTabprm_cset(self)) { return NULL; } /* This is not thread-safe, but since we're holding onto the GIL, we can assume we won't have thread conflicts */ wcsprintf_set(NULL); ignored = tabprt(self->x); #if PY3K return PyUnicode_FromString(wcsprintf_buf()); #else return PyString_FromString(wcsprintf_buf()); #endif } /*************************************************************************** * Member getters/setters (properties) */ /*@null@*/ static PyObject* PyTabprm_get_coord( PyTabprm* self, /*@unused@*/ void* closure) { npy_intp ndims; npy_intp dims[NPY_MAXDIMS]; if (is_null(self->x->coord)) { return NULL; } if (make_fancy_dims(self, &ndims, dims)) { return NULL; } return get_double_array("coord", self->x->coord, ndims, dims, (PyObject*)self); } /*@null@*/ static int PyTabprm_set_coord( PyTabprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp ndims; npy_intp dims[NPY_MAXDIMS]; if (is_null(self->x->coord)) { return -1; } if (make_fancy_dims(self, &ndims, dims)) { return -1; } return set_double_array("coord", value, ndims, dims, self->x->coord); } /*@null@*/ static PyObject* PyTabprm_get_crval( PyTabprm* self, /*@unused@*/ void* closure) { Py_ssize_t M = 0; if (is_null(self->x->crval)) { return NULL; } M = (Py_ssize_t)self->x->M; return get_double_array("crval", self->x->crval, 1, &M, (PyObject*)self); } static int PyTabprm_set_crval( PyTabprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp M = 0; if (is_null(self->x->crval)) { return -1; } M = (Py_ssize_t)self->x->M; note_change(self); return set_double_array("crval", value, 1, &M, self->x->crval); } /*@null@*/ static PyObject* PyTabprm_get_delta( PyTabprm* self, /*@unused@*/ void* closure) { Py_ssize_t M = 0; if (is_null(self->x->delta)) { return NULL; } M = (Py_ssize_t)self->x->M; return get_double_array("delta", self->x->delta, 1, &M, (PyObject*)self); } /*@null@*/ static PyObject* PyTabprm_get_extrema( PyTabprm* self, /*@unused@*/ void* closure) { npy_intp ndims; npy_intp dims[NPY_MAXDIMS]; if (is_null(self->x->coord)) { return NULL; } if (make_fancy_dims(self, &ndims, dims)) { return NULL; } dims[ndims-2] = 2; return get_double_array("extrema", self->x->extrema, ndims, dims, (PyObject*)self); } /*@null@*/ static PyObject* PyTabprm_get_K( PyTabprm* self, /*@unused@*/ void* closure) { Py_ssize_t M = 0; if (is_null(self->x->K)) { return NULL; } M = (Py_ssize_t)self->x->M; return get_int_array("K", self->x->K, 1, &M, (PyObject*)self); } /*@null@*/ static PyObject* PyTabprm_get_M( PyTabprm* self, /*@unused@*/ void* closure) { return get_int("M", self->x->M); } /*@null@*/ static PyObject* PyTabprm_get_map( PyTabprm* self, /*@unused@*/ void* closure) { Py_ssize_t M = 0; if (is_null(self->x->map)) { return NULL; } M = (Py_ssize_t)self->x->M; return get_int_array("map", self->x->map, 1, &M, (PyObject*)self); } static int PyTabprm_set_map( PyTabprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp M = 0; if (is_null(self->x->map)) { return -1; } M = (Py_ssize_t)self->x->M; note_change(self); return set_int_array("map", value, 1, &M, self->x->map); } /*@null@*/ static PyObject* PyTabprm_get_nc( PyTabprm* self, /*@unused@*/ void* closure) { return get_int("nc", self->x->nc); } /*@null@*/ static PyObject* PyTabprm_get_p0( PyTabprm* self, /*@unused@*/ void* closure) { Py_ssize_t M = 0; if (is_null(self->x->p0)) { return NULL; } M = (Py_ssize_t)self->x->M; return get_int_array("p0", self->x->p0, 1, &M, (PyObject*)self); } /*@null@*/ static PyObject* PyTabprm_get_sense( PyTabprm* self, /*@unused@*/ void* closure) { Py_ssize_t M = 0; if (is_null(self->x->sense)) { return NULL; } M = (Py_ssize_t)self->x->M; return get_int_array("sense", self->x->sense, 1, &M, (PyObject*)self); } /*************************************************************************** * PyTabprm definition structures */ static PyGetSetDef PyTabprm_getset[] = { {"coord", (getter)PyTabprm_get_coord, (setter)PyTabprm_set_coord, (char *)doc_coord}, {"crval", (getter)PyTabprm_get_crval, (setter)PyTabprm_set_crval, (char *)doc_crval_tabprm}, {"delta", (getter)PyTabprm_get_delta, NULL, (char *)doc_delta}, {"extrema", (getter)PyTabprm_get_extrema, NULL, (char *)doc_extrema}, {"K", (getter)PyTabprm_get_K, NULL, (char *)doc_K}, {"M", (getter)PyTabprm_get_M, NULL, (char *)doc_M}, {"map", (getter)PyTabprm_get_map, (setter)PyTabprm_set_map, (char *)doc_map}, {"nc", (getter)PyTabprm_get_nc, NULL, (char *)doc_nc}, {"p0", (getter)PyTabprm_get_p0, NULL, (char *)doc_p0}, {"sense", (getter)PyTabprm_get_sense, NULL, (char *)doc_sense}, {NULL} }; static PyMethodDef PyTabprm_methods[] = { {"print_contents", (PyCFunction)PyTabprm_print_contents, METH_NOARGS, doc_print_contents_tabprm}, {"set", (PyCFunction)PyTabprm_set, METH_NOARGS, doc_set_tabprm}, {NULL} }; PyTypeObject PyTabprmType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs.Tabprm", /*tp_name*/ sizeof(PyTabprm), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyTabprm_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ (reprfunc)PyTabprm___str__, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ (reprfunc)PyTabprm___str__, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE, /*tp_flags*/ doc_Tabprm, /* tp_doc */ (traverseproc)PyTabprm_traverse, /* tp_traverse */ (inquiry)PyTabprm_clear, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PyTabprm_methods, /* tp_methods */ 0, /* tp_members */ PyTabprm_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ 0, /* tp_init */ 0, /* tp_alloc */ 0, /* tp_new */ }; int _setup_tabprm_type( PyObject* m) { if (PyType_Ready(&PyTabprmType) < 0) { return -1; } Py_INCREF(&PyTabprmType); PyModule_AddObject(m, "Tabprm", (PyObject *)&PyTabprmType); tab_errexc[0] = NULL; /* Success */ tab_errexc[1] = &PyExc_MemoryError; /* Null wcsprm pointer passed */ tab_errexc[2] = &PyExc_MemoryError; /* Memory allocation failed */ tab_errexc[3] = &WcsExc_InvalidTabularParameters; /* Invalid tabular parameters */ tab_errexc[4] = &WcsExc_InvalidCoordinate; /* One or more of the x coordinates were invalid */ tab_errexc[5] = &WcsExc_InvalidCoordinate; /* One or more of the world coordinates were invalid */ return 0; } pywcs-1.12/src/wcslib_tabprm_wrap.h0000644001153600020070000000351312310355626021471 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __WCSLIB_TABPRM_WRAP_H__ #define __WCSLIB_TABPRM_WRAP_H__ #include "pyutil.h" #include "wcs.h" extern PyTypeObject PyTabprmType; typedef struct { PyObject_HEAD struct tabprm* x; PyObject* owner; } PyTabprm; PyTabprm* PyTabprm_cnew(PyObject* wcsprm, struct tabprm* x); int _setup_tabprm_type(PyObject* m); #endif pywcs-1.12/src/wcslib_units_wrap.c0000644001153600020070000002537312310355626021351 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "wcslib_units_wrap.h" #include /* It gets to be really tedious to type long docstrings in ANSI C syntax (since multi-line strings literals are not valid). Therefore, the docstrings are written in doc/docstrings.py, which are then converted by setup.py into docstrings.h, which we include here. */ #include "docstrings.h" /*************************************************************************** * PyTabprm methods */ static int PyUnits_traverse( PyUnits* self, visitproc visit, void *arg) { return 0; } static int PyUnits_clear( PyUnits* self) { return 0; } static void PyUnits_dealloc( PyUnits* self) { PyUnits_clear(self); Py_TYPE(self)->tp_free((PyObject*)self); } PyUnits* PyUnits_cnew( const char* const have, const char* const want, const double scale, const double offset, const double power) { PyUnits* self; self = (PyUnits*)(&PyUnitsType)->tp_alloc(&PyUnitsType, 0); if (have == NULL) { self->have[0] = 0; } else { strncpy(self->have, have, 80); } if (want == NULL) { self->want[0] = 0; } else { strncpy(self->want, want, 80); } self->scale = scale; self->offset = offset; self->power = power; return self; } static PyObject * PyUnits_new( PyTypeObject* type, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyUnits* self; self = (PyUnits*)type->tp_alloc(type, 0); self->have[0] = 0; self->want[0] = 0; self->scale = 1.0; self->offset = 0.0; self->power = 1.0; return (PyObject*)self; } static int PyUnits_init( PyUnits* self, PyObject* args, PyObject* kwds) { int status = -1; char* have; char* want; char* ctrl_str = NULL; int ctrl = 0; const char* keywords[] = {"have", "want", "translate_units", NULL}; struct wcserr* err = NULL; if (!PyArg_ParseTupleAndKeywords(args, kwds, "ss|s:UnitConverter.__init__", (char **)keywords, &have, &want, &ctrl_str)) { goto exit; } if (ctrl_str != NULL) { if (parse_unsafe_unit_conversion_spec(ctrl_str, &ctrl)) { goto exit; } } /* Copy the strings since we can't have wcslib monkeying with the data in a Python string */ strncpy(self->have, have, 80); strncpy(self->want, want, 80); status = wcsutrne(ctrl, self->have, &err); if (status != -1 && status != 0) { goto exit; } status = wcsutrne(ctrl, self->want, &err); if (status != -1 && status != 0) { goto exit; } status = wcsunitse(self->have, self->want, &self->scale, &self->offset, &self->power, &err); exit: if (PyErr_Occurred()) { return -1; } else if (status == 0) { return 0; } else { wcserr_units_to_python_exc(err); free(err); return -1; } } /*@null@*/ static PyObject* PyUnits___str__( PyUnits* self) { #define BUF_SIZE 1 << 8 char buffer[BUF_SIZE]; char scale[BUF_SIZE]; char offset[BUF_SIZE]; char power[BUF_SIZE]; if (self->scale != 1.0) { snprintf(scale, BUF_SIZE, "*%.12g", self->scale); } else { scale[0] = 0; } if (self->offset != 0.0) { snprintf(offset, BUF_SIZE, " + %.12g", self->offset); } else { offset[0] = 0; } if (self->power != 1.0) { snprintf(power, BUF_SIZE, " ** %.12g", self->power); } else { power[0] = 0; } snprintf(buffer, 1 << 8, "", self->have, self->want, scale, offset, power); #if PY3K return PyUnicode_FromString(buffer); #else return PyString_FromString(buffer); #endif } static PyObject* PyUnits_convert( PyUnits* self, PyObject* args, PyObject* kwds) { int status = 1; PyObject* input = NULL; PyArrayObject* input_arr = NULL; PyArrayObject* output_arr = NULL; PyObject* input_iter = NULL; PyObject* output_iter = NULL; double input_val; double output_val; if (!PyArg_ParseTuple(args, "O:UnitConverter.convert", &input)) { goto exit; } input_arr = (PyArrayObject*)PyArray_FromObject( input, NPY_DOUBLE, 0, NPY_MAXDIMS); if (input_arr == NULL) { goto exit; } output_arr = (PyArrayObject*)PyArray_SimpleNew( PyArray_NDIM(input_arr), PyArray_DIMS(input_arr), PyArray_DOUBLE); if (output_arr == NULL) { goto exit; } input_iter = PyArray_IterNew((PyObject*)input_arr); if (input_iter == NULL) { goto exit; } output_iter = PyArray_IterNew((PyObject*)output_arr); if (output_iter == NULL) { goto exit; } if (self->power != 1.0) { while (PyArray_ITER_NOTDONE(input_iter)) { input_val = *(double *)PyArray_ITER_DATA(input_iter); output_val = pow(self->scale*input_val + self->offset, self->power); if (errno) { PyErr_SetFromErrno(PyExc_ValueError); goto exit; } *(double *)PyArray_ITER_DATA(output_iter) = output_val; PyArray_ITER_NEXT(input_iter); PyArray_ITER_NEXT(output_iter); } } else { while (PyArray_ITER_NOTDONE(input_iter)) { input_val = *(double *)PyArray_ITER_DATA(input_iter); output_val = self->scale*input_val + self->offset; *(double *)PyArray_ITER_DATA(output_iter) = output_val; PyArray_ITER_NEXT(input_iter); PyArray_ITER_NEXT(output_iter); } } status = 0; exit: Py_XDECREF((PyObject*)input_arr); Py_XDECREF(input_iter); Py_XDECREF(output_iter); if (status) { Py_XDECREF((PyObject*)output_arr); return NULL; } return (PyObject*)output_arr; } /*************************************************************************** * Member getters/setters (properties) */ /*@null@*/ static PyObject* PyUnits_get_have( PyUnits* self, /*@unused@*/ void* closure) { #if PY3K return PyUnicode_FromString(self->have); #else return PyString_FromString(self->have); #endif } /*@null@*/ static PyObject* PyUnits_get_want( PyUnits* self, /*@unused@*/ void* closure) { #if PY3K return PyUnicode_FromString(self->want); #else return PyString_FromString(self->want); #endif } /*@null@*/ static PyObject* PyUnits_get_scale( PyUnits* self, /*@unused@*/ void* closure) { return get_double("scale", self->scale); } /*@null@*/ static PyObject* PyUnits_get_offset( PyUnits* self, /*@unused@*/ void* closure) { return get_double("offset", self->offset); } /*@null@*/ static PyObject* PyUnits_get_power( PyUnits* self, /*@unused@*/ void* closure) { return get_double("power", self->power); } /*************************************************************************** * PyUnits definition structures */ static PyGetSetDef PyUnits_getset[] = { {"have", (getter)PyUnits_get_have, NULL, (char *)doc_have}, {"want", (getter)PyUnits_get_want, NULL, (char *)doc_want}, {"scale", (getter)PyUnits_get_scale, NULL, (char *)doc_scale}, {"offset", (getter)PyUnits_get_offset, NULL, (char *)doc_offset}, {"power", (getter)PyUnits_get_power, NULL, (char *)doc_power}, {NULL} }; static PyMethodDef PyUnits_methods[] = { {"convert", (PyCFunction)PyUnits_convert, METH_VARARGS, doc_convert}, {NULL} }; PyTypeObject PyUnitsType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs.UnitConverter", /*tp_name*/ sizeof(PyUnits), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyUnits_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ (reprfunc)PyUnits___str__, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ (reprfunc)PyUnits___str__, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE, /*tp_flags*/ doc_UnitConverter, /* tp_doc */ (traverseproc)PyUnits_traverse, /* tp_traverse */ (inquiry)PyUnits_clear, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PyUnits_methods, /* tp_methods */ 0, /* tp_members */ PyUnits_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ (initproc)PyUnits_init, /* tp_init */ 0, /* tp_alloc */ PyUnits_new, /* tp_new */ }; int _setup_units_type( PyObject* m) { if (PyType_Ready(&PyUnitsType) < 0) { return -1; } Py_INCREF(&PyUnitsType); PyModule_AddObject(m, "UnitConverter", (PyObject *)&PyUnitsType); return 0; } pywcs-1.12/src/wcslib_units_wrap.h0000644001153600020070000000372312310355626021351 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __WCSLIB_UNITS_WRAP_H__ #define __WCSLIB_UNITS_WRAP_H__ #include "pyutil.h" #include "wcsunits.h" extern PyTypeObject PyUnitsType; typedef struct { PyObject_HEAD char have[80]; char want[80]; double scale; double offset; double power; } PyUnits; PyUnits* PyUnits_cnew( const char* const have, const char* const want, const double scale, const double offset, const double power); int _setup_units_type(PyObject* m); #endif pywcs-1.12/src/wcslib_wrap.c0000644001153600020070000022352012310355626020121 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "wcslib_wrap.h" #include "wcslib_tabprm_wrap.h" #include "wcslib_wtbarr_wrap.h" #include "wcslib_units_wrap.h" #include /* from Python */ #include #include #include #include #include #include #include "isnan.h" #include "distortion.h" /* It gets to be really tedious to type long docstrings in ANSI C syntax (since multi-line strings literals are not valid). Therefore, the docstrings are written in doc/docstrings.py, which are then converted by setup.py into docstrings.h, which we include here. */ #include "docstrings.h" /*************************************************************************** * Helper functions * ***************************************************************************/ enum e_altlin { has_pc = 1, has_cd = 2, has_crota = 4 }; static int is_valid_alt_key( const char* key) { if (key[1] != '\0' || !(key[0] == ' ' || (key[0] >= 'A' && key[0] <= 'Z'))) { PyErr_SetString(PyExc_ValueError, "key must be ' ' or 'A'-'Z'"); return 0; } return 1; } /*************************************************************************** * PyWcsprm methods */ static int PyWcsprm_cset(PyWcsprm* self, const int convert); static pywcs_inline void note_change(PyWcsprm* self) { self->x.flag = 0; } static void PyWcsprm_dealloc( PyWcsprm* self) { int ignored; ignored = wcsfree(&self->x); Py_TYPE(self)->tp_free((PyObject*)self); } static PyWcsprm* PyWcsprm_cnew(void) { PyWcsprm* self; self = (PyWcsprm*)(&PyWcsprmType)->tp_alloc(&PyWcsprmType, 0); return self; } static PyObject * PyWcsprm_new( PyTypeObject* type, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { PyWcsprm* self; self = (PyWcsprm*)type->tp_alloc(type, 0); return (PyObject*)self; } static int PyWcsprm_init( PyWcsprm* self, PyObject* args, PyObject* kwds) { int status; PyObject* header_obj = NULL; char * header = NULL; Py_ssize_t header_length = 0; Py_ssize_t nkeyrec = 0; char * key = " "; PyObject* relax_obj = NULL; int relax = 0; int naxis = -1; int keysel = -1; PyObject* colsel = Py_None; PyArrayObject* colsel_array = NULL; int* colsel_ints = NULL; int ctrl = 0; int nreject = 0; int nwcs = 0; struct wcsprm* wcs = NULL; int i = 0; const char* keywords[] = {"header", "key", "relax", "naxis", "keysel", "colsel", NULL}; PyObject* ignored = NULL; int ignored_int; if (!PyArg_ParseTupleAndKeywords( args, kwds, "|OsOiiO:WCSBase.__init__", (char **)keywords, &header_obj, &key, &relax_obj, &naxis, &keysel, &colsel)) { return -1; } if (header_obj == NULL || header_obj == Py_None) { if (relax_obj != NULL && relax_obj != Py_False) { PyErr_SetString( PyExc_ValueError, "If no header is provided, relax may not be provided either."); return -1; } if (keysel > 0) { PyErr_SetString( PyExc_ValueError, "If no header is provided, keysel may not be provided either."); return -1; } if (colsel != Py_None) { PyErr_SetString( PyExc_ValueError, "If no header is provided, colsel may not be provided either."); return -1; } /* Default number of axes is 2 */ if (naxis < 0) { naxis = 2; } if (naxis < 1 || naxis > 15) { PyErr_SetString( PyExc_ValueError, "naxis must be in range 1-15"); return -1; } note_change(self); self->x.flag = -1; status = wcsini(1, naxis, &self->x); if (status != 0) { PyErr_SetString( PyExc_MemoryError, self->x.err->msg); return -1; } self->x.alt[0] = key[0]; if (PyWcsprm_cset(self, 0)) { return -1; } wcsprm_c2python(&self->x); return 0; } else { /* header != NULL */ #if PY3K if (PyBytes_AsStringAndSize(header_obj, &header, &header_length)) { #else if (PyString_AsStringAndSize(header_obj, &header, &header_length)) { #endif return -1; } if (relax_obj == Py_True) { relax = WCSHDR_all; } else if (relax_obj == NULL || relax_obj == Py_False) { relax = WCSHDR_none; } else { #if PY3K relax = PyLong_AsLong(relax_obj); #else relax = PyInt_AsLong(relax_obj); #endif if (relax == -1) { PyErr_SetString( PyExc_ValueError, "relax must be True, False or an integer."); return -1; } } if (!is_valid_alt_key(key)) { return -1; } if (naxis >= 0) { PyErr_SetString( PyExc_ValueError, "naxis may not be provided if a header is provided."); return -1; } nkeyrec = header_length / 80; if (nkeyrec > 0x7fffffff) { PyErr_SetString( PyExc_MemoryError, "header is too long"); return -1; } if (colsel != Py_None) { colsel_array = (PyArrayObject*) PyArray_ContiguousFromAny( colsel, 1, 1, PyArray_INT); if (colsel_array == NULL) { return -1; } colsel_ints = malloc(sizeof(int) * (PyArray_DIM(colsel_array, 0) + 1)); if (colsel_ints == NULL) { Py_DECREF(colsel_array); PyErr_SetString( PyExc_MemoryError, "Memory allocation error."); return -1; } colsel_ints[0] = PyArray_DIM(colsel_array, 0); for (i = 0; i < colsel_ints[0]; ++i) { colsel_ints[i+1] = colsel_array->data[i]; } Py_DECREF(colsel_array); } if (keysel < 0) { status = wcspih( header, (int)nkeyrec, relax, ctrl, &nreject, &nwcs, &wcs); } else { status = wcsbth( header, (int)nkeyrec, relax, ctrl, keysel, colsel_ints, &nreject, &nwcs, &wcs); } free(colsel_ints); if (status != 0) { PyErr_SetString( PyExc_MemoryError, "Memory allocation error."); return -1; } if (nwcs == 0) { PyErr_SetString( WcsExc_NoWcsKeywordsFound, "No WCS keywords found in the given header"); return -1; } /* Find the desired WCS */ for (i = 0; i < nwcs; ++i) { if (wcs[i].alt[0] == key[0]) { break; } } if (i >= nwcs) { ignored_int = wcsvfree(&nwcs, &wcs); ignored = PyErr_Format( PyExc_KeyError, "No WCS with key '%s' was found in the given header", key); return -1; } if (wcscopy(1, wcs + i, &self->x) != 0) { ignored_int = wcsvfree(&nwcs, &wcs); PyErr_SetString( PyExc_MemoryError, self->x.err->msg); return -1; } note_change(self); wcsprm_c2python(&self->x); ignored_int = wcsvfree(&nwcs, &wcs); return 0; } } /*@null@*/ static PyObject* PyWcsprm_copy( PyWcsprm* self) { PyWcsprm* copy = NULL; int status; copy = PyWcsprm_cnew(); if (copy == NULL) { return NULL; } wcsprm_python2c(&self->x); status = wcscopy(1, &self->x, ©->x); wcsprm_c2python(&self->x); if (status == 0) { if (PyWcsprm_cset(copy, 0)) { Py_XDECREF(copy); return NULL; } wcsprm_c2python(©->x); return (PyObject*)copy; } else { Py_XDECREF(copy); wcs_to_python_exc(&(self->x)); return NULL; } } PyObject* PyWcsprm_find_all_wcs( PyObject* __, PyObject* args, PyObject* kwds) { PyObject* header_obj = NULL; char * header = NULL; Py_ssize_t header_length = 0; Py_ssize_t nkeyrec = 0; PyObject* relax_obj = NULL; int relax = 0; int keysel = 0; int ctrl = 0; int nreject = 0; int nwcs = 0; struct wcsprm* wcs = NULL; PyObject* result = NULL; PyWcsprm* subresult = NULL; int i = 0; int ignored = 0; const char* keywords[] = {"header", "relax", "keysel", NULL}; int status = -1; if (!PyArg_ParseTupleAndKeywords( args, kwds, "O|Oi:find_all_wcs", (char **)keywords, &header_obj, &relax_obj, &keysel)) { return NULL; } #if PY3K if (PyBytes_AsStringAndSize(header_obj, &header, &header_length)) { #else if (PyString_AsStringAndSize(header_obj, &header, &header_length)) { #endif return NULL; } nkeyrec = header_length / 80; if (nkeyrec > 0x7fffffff) { PyErr_SetString( PyExc_MemoryError, "header is too long"); return NULL; } if (relax_obj == Py_True) { relax = WCSHDR_all; } else if (relax_obj == NULL || relax_obj == Py_False) { relax = WCSHDR_none; } else { #if PY3K relax = PyLong_AsLong(relax_obj); #else relax = PyInt_AsLong(relax_obj); #endif if (relax == -1) { PyErr_SetString( PyExc_ValueError, "relax must be True, False or an integer."); return NULL; } } Py_BEGIN_ALLOW_THREADS if (keysel < 0) { status = wcspih( header, (int)nkeyrec, relax, ctrl, &nreject, &nwcs, &wcs); } else { status = wcsbth( header, (int)nkeyrec, relax, ctrl, keysel, NULL, &nreject, &nwcs, &wcs); } Py_END_ALLOW_THREADS if (status != 0) { PyErr_SetString( PyExc_MemoryError, "Memory allocation error."); return NULL; } result = PyList_New(nwcs); if (result == NULL) { ignored = wcsvfree(&nwcs, &wcs); return NULL; } for (i = 0; i < nwcs; ++i) { subresult = PyWcsprm_cnew(); if (wcscopy(1, wcs + i, &subresult->x) != 0) { Py_DECREF(result); ignored = wcsvfree(&nwcs, &wcs); PyErr_SetString( PyExc_MemoryError, "Could not initialize wcsprm object"); return NULL; } if (PyList_SetItem(result, i, (PyObject *)subresult) == -1) { Py_DECREF(subresult); Py_DECREF(result); ignored = wcsvfree(&nwcs, &wcs); return NULL; } subresult->x.flag = 0; if (PyWcsprm_cset(subresult, 0)) { Py_DECREF(subresult); Py_DECREF(result); ignored = wcsvfree(&nwcs, &wcs); return NULL; } wcsprm_c2python(&subresult->x); } ignored = wcsvfree(&nwcs, &wcs); return result; } static PyObject* PyWcsprm_celfix( PyWcsprm* self) { int status = 0; wcsprm_python2c(&self->x); status = celfix(&self->x); wcsprm_c2python(&self->x); if (status <= 0) { #if PY3K return PyLong_FromLong((long)status); #else return PyInt_FromLong((long)status); #endif } else { wcserr_fix_to_python_exc(self->x.err); return NULL; } } /*@null@*/ static PyObject* PyWcsprm_cylfix( PyWcsprm* self, PyObject* args, PyObject* kwds) { PyObject* naxis_obj = NULL; PyArrayObject* naxis_array = NULL; int* naxis = NULL; int status = 0; const char* keywords[] = {"naxis", NULL}; PyObject* ignored = NULL; if (!PyArg_ParseTupleAndKeywords( args, kwds, "|O:cylfix", (char **)keywords, &naxis_obj)) { return NULL; } if (naxis_obj != NULL) { naxis_array = (PyArrayObject*)PyArray_ContiguousFromAny( naxis_obj, 1, 1, PyArray_INT); if (naxis_array == NULL) { return NULL; } if (PyArray_DIM(naxis_array, 0) != self->x.naxis) { ignored = PyErr_Format( PyExc_ValueError, "naxis must be same length as the number of axes of " "the Wcsprm object (%d).", self->x.naxis); Py_DECREF(naxis_array); return NULL; } naxis = (int*)PyArray_DATA(naxis_array); } wcsprm_python2c(&self->x); status = cylfix(naxis, &self->x); wcsprm_c2python(&self->x); Py_XDECREF(naxis_array); if (status <= 0) { #if PY3K return PyLong_FromLong((long)status); #else return PyInt_FromLong((long)status); #endif } else { wcserr_fix_to_python_exc(self->x.err); return NULL; } } static PyObject* PyWcsprm_datfix( PyWcsprm* self) { int status = 0; wcsprm_python2c(&self->x); status = datfix(&self->x); wcsprm_c2python(&self->x); if (status <= 0) { #if PY3K return PyLong_FromLong((long)status); #else return PyInt_FromLong((long)status); #endif } else { wcserr_fix_to_python_exc(self->x.err); return NULL; } } /*@null@*/ static PyObject* PyWcsprm_fix( PyWcsprm* self, PyObject* args, PyObject* kwds) { char* translate_units = NULL; int ctrl = 0; PyObject* naxis_obj = NULL; PyArrayObject* naxis_array = NULL; int* naxis = NULL; int stat[NWCSFIX]; struct wcserr err[NWCSFIX]; int status = 0; PyObject* subresult; PyObject* result; int i = 0; int msg_index = 0; const char* message; PyObject* ignored = NULL; struct message_map_entry { const char* name; const int index; }; const struct message_map_entry message_map[5] = { {"datfix", DATFIX}, {"unitfix", UNITFIX}, {"celfix", CELFIX}, {"spcfix", SPCFIX}, {"cylfix", CYLFIX}, }; const char* keywords[] = {"translate_units", "naxis", NULL}; if (!PyArg_ParseTupleAndKeywords( args, kwds, "|sO:fix", (char **)keywords, &translate_units, &naxis_obj)) { return NULL; } if (translate_units != NULL) { if (parse_unsafe_unit_conversion_spec(translate_units, &ctrl)) { return NULL; } } if (naxis_obj != NULL) { naxis_array = (PyArrayObject*)PyArray_ContiguousFromAny( naxis_obj, 1, 1, PyArray_INT); if (naxis_array == NULL) { return NULL; } if (PyArray_DIM(naxis_array, 0) != self->x.naxis) { ignored = PyErr_Format( PyExc_ValueError, "naxis must be same length as the number of axes of " "the Wcprm object (%d).", self->x.naxis); Py_DECREF(naxis_array); return NULL; } naxis = (int*)PyArray_DATA(naxis_array); } memset(err, 0, sizeof(struct wcserr) * NWCSFIX); wcsprm_python2c(&self->x); status = wcsfixi(ctrl, naxis, &self->x, stat, err); wcsprm_c2python(&self->x); /* We're done with this already, so deref now so we don't have to remember later */ Py_XDECREF(naxis_array); result = PyDict_New(); if (result == NULL) { return NULL; } for (i = 0; i < 5; ++i) { msg_index = stat[message_map[i].index]; message = err[message_map[i].index].msg; if (message == NULL || message[0] == 0) { if (msg_index == FIXERR_SUCCESS) { message = "Success"; } else if (msg_index == FIXERR_NO_CHANGE) { message = "No change"; } else if (msg_index == FIXERR_UNITS_ALIAS && message_map[i].index == CYLFIX){ message = "No change"; } } #if PY3K subresult = PyUnicode_FromString(message); #else subresult = PyString_FromString(message); #endif if (subresult == NULL || PyDict_SetItemString(result, message_map[i].name, subresult)) { Py_XDECREF(subresult); Py_XDECREF(result); return NULL; } Py_XDECREF(subresult); } return result; } /*@null@*/ static PyObject* PyWcsprm_get_cdelt_func( PyWcsprm* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { Py_ssize_t naxis = 0; if (is_null(self->x.cdelt)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } naxis = self->x.naxis; return get_double_array_readonly("cdelt", self->x.cdelt, 1, &naxis, (PyObject*)self); } /*@null@*/ static PyObject* PyWcsprm_get_pc_func( PyWcsprm* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { npy_intp dims[2]; if (is_null(self->x.pc)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; return get_double_array_readonly("pc", self->x.pc, 2, dims, (PyObject*)self); } /*@null@*/ static PyObject* PyWcsprm_get_ps( PyWcsprm* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { if (self->x.ps == NULL) { PyErr_SetString( PyExc_AssertionError, "No PSi_ma records present."); return NULL; } return get_pscards("ps", self->x.ps, self->x.nps); } /*@null@*/ static PyObject* PyWcsprm_get_pv( PyWcsprm* self, /*@unused@*/ PyObject* args, /*@unused@*/ PyObject* kwds) { if (self->x.pv == NULL) { PyErr_SetString( PyExc_AssertionError, "No PVi_ma records present."); return NULL; } return get_pvcards("pv", self->x.pv, self->x.npv); } static PyObject* PyWcsprm_has_cdi_ja( PyWcsprm* self) { int result = 0; result = self->x.altlin & has_cd; return PyBool_FromLong(result); } static PyObject* PyWcsprm_has_crotaia( PyWcsprm* self) { int result = 0; result = self->x.altlin & has_crota; return PyBool_FromLong(result); } static PyObject* PyWcsprm_has_pci_ja( PyWcsprm* self) { int result = 0; result = (self->x.altlin == 0 || self->x.altlin & has_pc); return PyBool_FromLong(result); } static PyObject* PyWcsprm_is_unity( PyWcsprm* self) { if (PyWcsprm_cset(self, 1)) { return NULL; } return PyBool_FromLong(self->x.lin.unity); } /*@null@*/ static PyObject* PyWcsprm_mix( PyWcsprm* self, PyObject* args, PyObject* kwds) { int mixpix = 0; int mixcel = 0; double vspan[2] = {0, 0}; double vstep = 0; int viter = 0; Py_ssize_t naxis = 0; PyObject* world_obj = NULL; PyObject* pixcrd_obj = NULL; int origin = 1; PyArrayObject* world = NULL; PyArrayObject* phi = NULL; PyArrayObject* theta = NULL; PyArrayObject* imgcrd = NULL; PyArrayObject* pixcrd = NULL; int status = -1; PyObject* result = NULL; PyObject* ignored = NULL; const char* keywords[] = { "mixpix", "mixcel", "vspan", "vstep", "viter", "world", "pixcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords( args, kwds, "ii(dd)diOOi:mix", (char **)keywords, &mixpix, &mixcel, &vspan[0], &vspan[1], &vstep, &viter, &world_obj, &pixcrd_obj, &origin)) { return NULL; } if (viter < 5 || viter > 10) { PyErr_SetString( PyExc_ValueError, "viter must be in the range 5 - 10"); goto exit; } world = (PyArrayObject*)PyArray_ContiguousFromAny (world_obj, PyArray_DOUBLE, 1, 1); if (world == NULL) { PyErr_SetString( PyExc_TypeError, "Argument 6 (world) must be a 1-dimensional numpy array"); goto exit; } if ((int)PyArray_DIM(world, 0) != self->x.naxis) { ignored = PyErr_Format( PyExc_TypeError, "Argument 6 (world) must be the same length as the number " "of axes (%d)", self->x.naxis); goto exit; } pixcrd = (PyArrayObject*)PyArray_ContiguousFromAny (pixcrd_obj, PyArray_DOUBLE, 1, 1); if (pixcrd == NULL) { PyErr_SetString( PyExc_TypeError, "Argument 7 (pixcrd) must be a 1-dimensional numpy array"); goto exit; } if ((int)PyArray_DIM(pixcrd, 0) != self->x.naxis) { ignored = PyErr_Format( PyExc_TypeError, "Argument 7 (pixcrd) must be the same length as the " "number of axes (%d)", self->x.naxis); goto exit; } if (mixpix < 1 || mixpix > self->x.naxis) { PyErr_SetString( PyExc_ValueError, "Argument 1 (mixpix) must specify a pixel coordinate " "axis number"); goto exit; } if (mixcel < 1 || mixcel > 2) { PyErr_SetString( PyExc_ValueError, "Argument 2 (mixcel) must specify a celestial coordinate " "axis number (1 for latitude, 2 for longitude)"); goto exit; } /* Now we allocate a bunch of numpy arrays to store the * results in. */ naxis = (Py_ssize_t)self->x.naxis; phi = (PyArrayObject*)PyArray_SimpleNew (1, &naxis, PyArray_DOUBLE); if (phi == NULL) { goto exit; } theta = (PyArrayObject*)PyArray_SimpleNew (1, &naxis, PyArray_DOUBLE); if (theta == NULL) { goto exit; } imgcrd = (PyArrayObject*)PyArray_SimpleNew (1, &naxis, PyArray_DOUBLE); if (imgcrd == NULL) { goto exit; } /* Convert pixel coordinates to 1-based */ Py_BEGIN_ALLOW_THREADS preoffset_array(pixcrd, origin); wcsprm_python2c(&self->x); status = wcsmix( &self->x, mixpix, mixcel, vspan, vstep, viter, (double*)PyArray_DATA(world), (double*)PyArray_DATA(phi), (double*)PyArray_DATA(theta), (double*)PyArray_DATA(imgcrd), (double*)PyArray_DATA(pixcrd)); wcsprm_c2python(&self->x); unoffset_array(pixcrd, origin); unoffset_array(imgcrd, origin); Py_END_ALLOW_THREADS if (status == 0) { result = PyDict_New(); if (result == NULL || PyDict_SetItemString(result, "imgcrd", (PyObject*)imgcrd) || PyDict_SetItemString(result, "phi", (PyObject*)phi) || PyDict_SetItemString(result, "theta", (PyObject*)theta) || PyDict_SetItemString(result, "world", (PyObject*)world)) { goto exit; } } exit: Py_XDECREF(world); Py_XDECREF(phi); Py_XDECREF(theta); Py_XDECREF(imgcrd); Py_XDECREF(pixcrd); if (status == 0) { return result; } else { Py_XDECREF(result); if (status == -1) { /* The error message has already been set */ return NULL; } else { wcs_to_python_exc(&(self->x)); return NULL; } } } /*@null@*/ static PyObject* PyWcsprm_p2s( PyWcsprm* self, PyObject* args, PyObject* kwds) { int naxis = 2; int ncoord = 0; int nelem = 0; PyObject* pixcrd_obj = NULL; int origin = 1; PyArrayObject* pixcrd = NULL; PyArrayObject* imgcrd = NULL; PyArrayObject* phi = NULL; PyArrayObject* theta = NULL; PyArrayObject* world = NULL; PyArrayObject* stat = NULL; PyObject* result = NULL; int status = 0; const char* keywords[] = { "pixcrd", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords( args, kwds, "Oi:p2s", (char **)keywords, &pixcrd_obj, &origin)) { return NULL; } naxis = self->x.naxis; pixcrd = (PyArrayObject*)PyArray_ContiguousFromAny (pixcrd_obj, PyArray_DOUBLE, 2, 2); if (pixcrd == NULL) { return NULL; } if (PyArray_DIM(pixcrd, 1) < naxis) { PyErr_Format( PyExc_RuntimeError, "Input array must be 2-dimensional, where the second dimension >= %d", naxis); goto exit; } /* Now we allocate a bunch of numpy arrays to store the results in. */ imgcrd = (PyArrayObject*)PyArray_SimpleNew( 2, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (imgcrd == NULL) { goto exit; } phi = (PyArrayObject*)PyArray_SimpleNew( 1, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (phi == NULL) { goto exit; } theta = (PyArrayObject*)PyArray_SimpleNew( 1, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (theta == NULL) { goto exit; } world = (PyArrayObject*)PyArray_SimpleNew( 2, PyArray_DIMS(pixcrd), PyArray_DOUBLE); if (world == NULL) { goto exit; } stat = (PyArrayObject*)PyArray_SimpleNew( 1, PyArray_DIMS(pixcrd), PyArray_INT); if (stat == NULL) { goto exit; } /* Make the call */ Py_BEGIN_ALLOW_THREADS ncoord = PyArray_DIM(pixcrd, 0); nelem = PyArray_DIM(pixcrd, 1); preoffset_array(pixcrd, origin); wcsprm_python2c(&self->x); status = wcsp2s( &self->x, ncoord, nelem, (double*)PyArray_DATA(pixcrd), (double*)PyArray_DATA(imgcrd), (double*)PyArray_DATA(phi), (double*)PyArray_DATA(theta), (double*)PyArray_DATA(world), (int*)PyArray_DATA(stat)); wcsprm_c2python(&self->x); unoffset_array(pixcrd, origin); /* unoffset_array(world, origin); */ unoffset_array(imgcrd, origin); if (status == 8) { set_invalid_to_nan( ncoord, nelem, (double*)PyArray_DATA(imgcrd), (int*)PyArray_DATA(stat)); set_invalid_to_nan( ncoord, 1, (double*)PyArray_DATA(phi), (int*)PyArray_DATA(stat)); set_invalid_to_nan( ncoord, 1, (double*)PyArray_DATA(theta), (int*)PyArray_DATA(stat)); set_invalid_to_nan( ncoord, nelem, (double*)PyArray_DATA(world), (int*)PyArray_DATA(stat)); } Py_END_ALLOW_THREADS if (status == 0 || status == 8) { result = PyDict_New(); if (result == NULL || PyDict_SetItemString(result, "imgcrd", (PyObject*)imgcrd) || PyDict_SetItemString(result, "phi", (PyObject*)phi) || PyDict_SetItemString(result, "theta", (PyObject*)theta) || PyDict_SetItemString(result, "world", (PyObject*)world) || PyDict_SetItemString(result, "stat", (PyObject*)stat)) { goto exit; } } exit: Py_XDECREF(pixcrd); Py_XDECREF(imgcrd); Py_XDECREF(phi); Py_XDECREF(theta); Py_XDECREF(world); Py_XDECREF(stat); if (status == 0 || status == 8) { return result; } else { Py_XDECREF(result); if (status == -1) { /* Exception already set */ return NULL; } else { wcs_to_python_exc(&(self->x)); return NULL; } } } /*@null@*/ static PyObject* PyWcsprm_s2p( PyWcsprm* self, PyObject* args, PyObject* kwds) { int naxis = 2; int ncoord = 0; int nelem = 0; PyObject* world_obj = NULL; int origin = 1; PyArrayObject* world = NULL; PyArrayObject* phi = NULL; PyArrayObject* theta = NULL; PyArrayObject* imgcrd = NULL; PyArrayObject* pixcrd = NULL; PyArrayObject* stat = NULL; PyObject* result = NULL; int status = -1; const char* keywords[] = { "world", "origin", NULL }; if (!PyArg_ParseTupleAndKeywords( args, kwds, "Oi:s2p", (char **)keywords, &world_obj, &origin)) { return NULL; } naxis = self->x.naxis; world = (PyArrayObject*)PyArray_ContiguousFromAny( world_obj, PyArray_DOUBLE, 2, 2); if (world == NULL) { return NULL; } if (PyArray_DIM(world, 1) < naxis) { PyErr_Format( PyExc_RuntimeError, "Input array must be 2-dimensional, where the second dimension >= %d", naxis); goto exit; } /* Now we allocate a bunch of numpy arrays to store the * results in. */ phi = (PyArrayObject*)PyArray_SimpleNew( 1, PyArray_DIMS(world), PyArray_DOUBLE); if (phi == NULL) { goto exit; } theta = (PyArrayObject*)PyArray_SimpleNew( 1, PyArray_DIMS(world), PyArray_DOUBLE); if (phi == NULL) { goto exit; } imgcrd = (PyArrayObject*)PyArray_SimpleNew( 2, PyArray_DIMS(world), PyArray_DOUBLE); if (theta == NULL) { goto exit; } pixcrd = (PyArrayObject*)PyArray_SimpleNew( 2, PyArray_DIMS(world), PyArray_DOUBLE); if (pixcrd == NULL) { goto exit; } stat = (PyArrayObject*)PyArray_SimpleNew( 1, PyArray_DIMS(world), PyArray_INT); if (stat == NULL) { goto exit; } /* Make the call */ Py_BEGIN_ALLOW_THREADS ncoord = PyArray_DIM(world, 0); nelem = PyArray_DIM(world, 1); /* preoffset_array(world, origin); */ wcsprm_python2c(&self->x); status = wcss2p( &self->x, ncoord, nelem, (double*)PyArray_DATA(world), (double*)PyArray_DATA(phi), (double*)PyArray_DATA(theta), (double*)PyArray_DATA(imgcrd), (double*)PyArray_DATA(pixcrd), (int*)PyArray_DATA(stat)); wcsprm_c2python(&self->x); /* unoffset_array(world, origin); */ unoffset_array(pixcrd, origin); unoffset_array(imgcrd, origin); if (status == 8) { set_invalid_to_nan( ncoord, 1, (double*)PyArray_DATA(phi), (int*)PyArray_DATA(stat)); set_invalid_to_nan( ncoord, 1, (double*)PyArray_DATA(theta), (int*)PyArray_DATA(stat)); set_invalid_to_nan( ncoord, nelem, (double*)PyArray_DATA(imgcrd), (int*)PyArray_DATA(stat)); set_invalid_to_nan( ncoord, nelem, (double*)PyArray_DATA(pixcrd), (int*)PyArray_DATA(stat)); } Py_END_ALLOW_THREADS if (status == 0 || status == 9) { result = PyDict_New(); if (result == NULL || PyDict_SetItemString(result, "phi", (PyObject*)phi) || PyDict_SetItemString(result, "theta", (PyObject*)theta) || PyDict_SetItemString(result, "imgcrd", (PyObject*)imgcrd) || PyDict_SetItemString(result, "pixcrd", (PyObject*)pixcrd) || PyDict_SetItemString(result, "stat", (PyObject*)stat)) { goto exit; } } exit: Py_XDECREF(pixcrd); Py_XDECREF(imgcrd); Py_XDECREF(phi); Py_XDECREF(theta); Py_XDECREF(world); Py_XDECREF(stat); if (status == 0 || status == 9) { return result; } else { Py_XDECREF(result); if (status == -1) { /* Exception already set */ return NULL; } else { wcs_to_python_exc(&(self->x)); return NULL; } } } static int PyWcsprm_cset( PyWcsprm* self, const int convert) { int status = 0; if (convert) wcsprm_python2c(&self->x); status = wcsset(&self->x); if (convert) wcsprm_c2python(&self->x); if (status == 0) { return 0; } else { wcs_to_python_exc(&(self->x)); return 1; } } /*@null@*/ static PyObject* PyWcsprm_set( PyWcsprm* self) { if (PyWcsprm_cset(self, 1)) { return NULL; } Py_INCREF(Py_None); return Py_None; } /*@null@*/ static PyObject* PyWcsprm_set_ps( PyWcsprm* self, PyObject* arg, /*@unused@*/ PyObject* kwds) { if (is_null(self->x.ps)) { return NULL; } if (set_pscards("ps", arg, &self->x.ps, &self->x.nps, &self->x.npsmax)) { self->x.m_ps = self->x.ps; return NULL; } self->x.m_ps = self->x.ps; note_change(self); Py_INCREF(Py_None); return Py_None; } /*@null@*/ static PyObject* PyWcsprm_set_pv( PyWcsprm* self, PyObject* arg, /*@unused@*/ PyObject* kwds) { if (is_null(self->x.pv)) { return NULL; } if (set_pvcards("pv", arg, &self->x.pv, &self->x.npv, &self->x.npvmax)) { self->x.m_pv = self->x.pv; return NULL; } self->x.m_pv = self->x.pv; note_change(self); Py_INCREF(Py_None); return Py_None; } /* TODO: This is convenient for debugging for now -- but it's not very * Pythonic. It should probably be hooked into __str__ or something. */ /*@null@*/ static PyObject* PyWcsprm_print_contents( PyWcsprm* self) { int ignored; /* This is not thread-safe, but since we're holding onto the GIL, we can assume we won't have thread conflicts */ wcsprintf_set(NULL); wcsprm_python2c(&self->x); if (PyWcsprm_cset(self, 0)) { wcsprm_c2python(&self->x); return NULL; } ignored = wcsprt(&self->x); wcsprm_c2python(&self->x); printf("%s", wcsprintf_buf()); Py_INCREF(Py_None); return Py_None; } /*@null@*/ static PyObject* PyWcsprm_spcfix( PyWcsprm* self) { int status = 0; wcsprm_python2c(&self->x); status = spcfix(&self->x); wcsprm_c2python(&self->x); if (status <= 0) { #if PY3K return PyLong_FromLong((long)status); #else return PyInt_FromLong((long)status); #endif } else { wcserr_fix_to_python_exc(self->x.err); return NULL; } } /*@null@*/ static PyObject* PyWcsprm_sptr( PyWcsprm* self, PyObject* args, PyObject* kwds) { int i = -1; char* py_ctype = NULL; char ctype[9]; int status = 0; const char* keywords[] = {"ctype", "i", NULL}; if (!PyArg_ParseTupleAndKeywords( args, kwds, "s|i:sptr", (char **)keywords, &py_ctype, &i)) { return NULL; } if (strlen(py_ctype) > 8) { PyErr_SetString( PyExc_ValueError, "ctype string has more than 8 characters."); } strncpy(ctype, py_ctype, 9); wcsprm_python2c(&self->x); status = wcssptr(&self->x, &i, ctype); wcsprm_c2python(&self->x); if (status == 0) { Py_INCREF(Py_None); return Py_None; } else { wcs_to_python_exc(&(self->x)); return NULL; } } /*@null@*/ static PyObject* PyWcsprm___str__( PyWcsprm* self) { /* This is not thread-safe, but since we're holding onto the GIL, we can assume we won't have thread conflicts */ wcsprintf_set(NULL); wcsprm_python2c(&self->x); if (PyWcsprm_cset(self, 0)) { wcsprm_c2python(&self->x); return NULL; } wcsprt(&self->x); wcsprm_c2python(&self->x); #if PY3K return PyUnicode_FromString(wcsprintf_buf()); #else return PyString_FromString(wcsprintf_buf()); #endif } /*@null@*/ static PyObject* PyWcsprm_sub( PyWcsprm* self, PyObject* args, PyObject* kwds) { int i = -1; Py_ssize_t tmp = 0; PyObject* py_axes = NULL; PyWcsprm* py_dest_wcs = NULL; PyObject* element = NULL; #if PY3K PyObject* element_utf8 = NULL; #endif char* element_str = NULL; int element_val = 0; int nsub = 0; int alloc_size = 0; int* axes = NULL; int status = -1; const char* keywords[] = {"axes", NULL}; if (!PyArg_ParseTupleAndKeywords( args, kwds, "|O:sub", (char **)keywords, &py_axes)) { goto exit; } if (py_axes == NULL || py_axes == Py_None) { /* leave all variables as is */ } else if (PySequence_Check(py_axes)) { tmp = PySequence_Size(py_axes); if (tmp == -1) { goto exit; } nsub = (int)tmp; axes = malloc(nsub * sizeof(int)); if (axes == NULL) { PyErr_SetString(PyExc_MemoryError, "Out of memory"); goto exit; } for (i = 0; i < nsub; ++i) { element = PySequence_GetItem(py_axes, i); if (element == NULL) { goto exit; } #if PY3K if (PyUnicode_Check(element)) { element_utf8 = PyUnicode_AsUTF8String(element); if (element_utf8 == NULL) { goto exit; } element_str = PyBytes_AsString(element_utf8); Py_DECREF(element_utf8); element_utf8 = NULL; #else if (PyString_Check(element)) { /* Doesn't return NULL, because we already known it's a string */ element_str = PyString_AsString(element); #endif if (strncmp(element_str, "longitude", 10) == 0) { element_val = WCSSUB_LONGITUDE; } else if (strncmp(element_str, "latitude", 9) == 0) { element_val = WCSSUB_LATITUDE; } else if (strncmp(element_str, "cubeface", 9) == 0) { element_val = WCSSUB_CUBEFACE; } else if (strncmp(element_str, "spectral", 9) == 0) { element_val = WCSSUB_SPECTRAL; } else if (strncmp(element_str, "stokes", 7) == 0) { element_val = WCSSUB_STOKES; } else if (strncmp(element_str, "celestial", 10) == 0) { element_val = WCSSUB_CELESTIAL; } else { PyErr_SetString( PyExc_ValueError, "string values for axis sequence must be one of 'latitude', 'longitude', 'cubeface', 'spectral', 'stokes', or 'celestial'"); goto exit; } #if PY3K } else if (PyLong_Check(element)) { tmp = (Py_ssize_t)PyLong_AsSsize_t(element); #else } else if (PyInt_Check(element)) { tmp = (Py_ssize_t)PyInt_AsLong(element); #endif if (tmp == -1 && PyErr_Occurred()) { goto exit; } element_val = (int)tmp; } else { PyErr_SetString( PyExc_TypeError, "axes sequence must contain either strings or ints"); goto exit; } axes[i] = element_val; Py_DECREF(element); element = NULL; } #if PY3K } else if (PyLong_Check(py_axes)) { tmp = (Py_ssize_t)PyLong_AsSsize_t(py_axes); #else } else if (PyInt_Check(py_axes)) { tmp = (Py_ssize_t)PyInt_AsLong(py_axes); #endif if (tmp == -1 && PyErr_Occurred()) { goto exit; } nsub = (int)tmp; if (nsub < 0 || nsub > self->x.naxis) { PyErr_Format( PyExc_ValueError, "If axes is an int, it must be in the range 0-self.naxis (%d)", self->x.naxis); goto exit; } } else { PyErr_SetString( PyExc_TypeError, "axes must None, a sequence or an integer"); goto exit; } if (nsub == 0) { alloc_size = self->x.naxis; } else { alloc_size = nsub; } py_dest_wcs = (PyWcsprm*)PyWcsprm_cnew(); py_dest_wcs->x.flag = -1; status = wcsini(1, alloc_size, &py_dest_wcs->x); if (status != 0) { goto exit; } wcsprm_python2c(&self->x); status = wcssub(0, &self->x, &nsub, axes, &py_dest_wcs->x); wcsprm_c2python(&self->x); if (PyWcsprm_cset(py_dest_wcs, 0)) { goto exit; } wcsprm_c2python(&py_dest_wcs->x); if (status != 0) { goto exit; } exit: free(axes); Py_XDECREF(element); #if PY3K Py_XDECREF(element_utf8); #endif if (status == 0) { return (PyObject*)py_dest_wcs; } else if (status == -1) { Py_XDECREF(py_dest_wcs); /* Exception already set */ return NULL; } else { wcs_to_python_exc(&(py_dest_wcs->x)); Py_XDECREF(py_dest_wcs); return NULL; } } /*@null@*/ static PyObject* PyWcsprm_to_header( PyWcsprm* self, PyObject* args, PyObject* kwds) { PyObject* relax_obj = NULL; int relax = 0; int nkeyrec = 0; char* header = NULL; int status = -1; PyObject* result = NULL; const char* keywords[] = {"relax", NULL}; if (!PyArg_ParseTupleAndKeywords( args, kwds, "|O:to_header", (char **)keywords, &relax_obj)) { goto exit; } if (relax_obj == Py_True) { relax = WCSHDO_all; } else if (relax_obj == NULL || relax_obj == Py_False) { relax = WCSHDO_none; } else { #if PY3K relax = PyLong_AsLong(relax_obj); #else relax = PyInt_AsLong(relax_obj); #endif if (relax == -1) { PyErr_SetString( PyExc_ValueError, "relax must be True, False or an integer."); return NULL; } } wcsprm_python2c(&self->x); status = wcshdo(relax, &self->x, &nkeyrec, &header); wcsprm_c2python(&self->x); if (status != 0) { PyErr_SetString( PyExc_RuntimeError, "Unknown error occurred. Something is seriously wrong."); goto exit; } /* Just return the raw header string. PyFITS on the Python side will help to parse and use this information. */ #if PY3K result = PyBytes_FromStringAndSize(header, (Py_ssize_t)nkeyrec * 80); #else result = PyString_FromStringAndSize(header, (Py_ssize_t)nkeyrec * 80); #endif exit: free(header); return result; } /*@null@*/ static PyObject* PyWcsprm_unitfix( PyWcsprm* self, PyObject* args, PyObject* kwds) { char* translate_units = NULL; int ctrl = 0; int status = 0; const char* keywords[] = {"translate_units", NULL}; if (!PyArg_ParseTupleAndKeywords( args, kwds, "|s:unitfix", (char **)keywords, &translate_units)) { return NULL; } if (translate_units != NULL) { if (parse_unsafe_unit_conversion_spec(translate_units, &ctrl)) { return NULL; } } status = unitfix(ctrl, &self->x); if (status <= 0) { #if PY3K return PyLong_FromLong((long)status); #else return PyInt_FromLong((long)status); #endif } else { wcserr_fix_to_python_exc(self->x.err); return NULL; } } /*************************************************************************** * Member getters/setters (properties) */ /*@null@*/ static PyObject* PyWcsprm_get_alt( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.alt)) { return NULL; } /* Force a null-termination of this single-character string */ self->x.alt[1] = '\0'; return get_string("alt", self->x.alt); } static int PyWcsprm_set_alt( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { char value_string[2]; if (is_null(self->x.alt)) { return -1; } if (value == NULL) { /* deletion */ self->x.alt[0] = ' '; self->x.alt[1] = '\0'; note_change(self); return 0; } if (set_string("alt", value, value_string, 2)) { return -1; } if (!is_valid_alt_key(value_string)) { return -1; } strncpy(self->x.alt, value_string, 2); note_change(self); return 0; } /*@null@*/ static PyObject* PyWcsprm_get_axis_types( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.types)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_int_array("axis_types", self->x.types, 1, &naxis, (PyObject*)self); } /*@null@*/ static PyObject* PyWcsprm_get_cd( PyWcsprm* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (is_null(self->x.cd)) { return NULL; } if ((self->x.altlin & has_cd) == 0) { PyErr_SetString(PyExc_AttributeError, "No cd is present."); return NULL; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; return get_double_array("cd", self->x.cd, 2, dims, (PyObject*)self); } static int PyWcsprm_set_cd( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp dims[2]; if (is_null(self->x.cd)) { return -1; } if (value == NULL) { self->x.altlin &= ~has_cd; note_change(self); return 0; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; if (set_double_array("cd", value, 2, dims, self->x.cd)) { return -1; } self->x.altlin |= has_cd; note_change(self); return 0; } /*@null@*/ static PyObject* PyWcsprm_get_cdelt( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.cdelt)) { return NULL; } naxis = self->x.naxis; if (self->x.altlin & has_cd) { PyErr_WarnEx(NULL, "cdelt will be ignored since cd is present", 1); } return get_double_array("cdelt", self->x.cdelt, 1, &naxis, (PyObject*)self); } /*@null@*/ static int PyWcsprm_set_cdelt( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp dims; if (is_null(self->x.cdelt)) { return -1; } dims = (npy_int)self->x.naxis; if (self->x.altlin & has_cd) { PyErr_WarnEx(NULL, "cdelt will be ignored since cd is present", 1); } note_change(self); return set_double_array("cdelt", value, 1, &dims, self->x.cdelt); } static PyObject* PyWcsprm_get_cel_offset( PyWcsprm* self, /*@unused@*/ void* closure) { return get_bool("cel_offset", self->x.cel.offset); } static int PyWcsprm_set_cel_offset( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); return set_bool("cel_offset", value, &self->x.cel.offset); } /*@null@*/ static PyObject* PyWcsprm_get_cname( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.cname)) { return NULL; } return get_str_list("cname", self->x.cname, (Py_ssize_t)self->x.naxis, 68, (PyObject*)self); } /*@null@*/ static int PyWcsprm_set_cname( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.cname)) { return -1; } note_change(self); return set_str_list("cname", value, (Py_ssize_t)self->x.naxis, 0, self->x.cname); } /*@null@*/ static PyObject* PyWcsprm_get_colax( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.colax)) { return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_int_array("colax", self->x.colax, 1, &naxis, (PyObject*)self); } static int PyWcsprm_set_colax( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 0; if (is_null(self->x.colax)) { return -1; } naxis = (Py_ssize_t)self->x.naxis; note_change(self); return set_int_array("colax", value, 1, &naxis, self->x.colax); } static PyObject* PyWcsprm_get_colnum( PyWcsprm* self, /*@unused@*/ void* closure) { return get_int("colnum", self->x.colnum); } static int PyWcsprm_set_colnum( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); return set_int("colnum", value, &self->x.colnum); } /*@null@*/ static PyObject* PyWcsprm_get_crder( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.crder)) { return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_double_array("crder", self->x.crder, 1, &naxis, (PyObject*)self); } static int PyWcsprm_set_crder( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 0; if (is_null(self->x.crder)) { return -1; } naxis = (Py_ssize_t)self->x.naxis; note_change(self); return set_double_array("crder", value, 1, &naxis, self->x.crder); } /*@null@*/ static PyObject* PyWcsprm_get_crota( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.crota)) { return NULL; } if ((self->x.altlin & has_crota) == 0) { PyErr_SetString(PyExc_AttributeError, "No crota is present."); return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_double_array("crota", self->x.crota, 1, &naxis, (PyObject*)self); } static int PyWcsprm_set_crota( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 0; if (is_null(self->x.crota)) { return -1; } if (value == NULL) { /* Deletion */ self->x.altlin &= ~has_crota; note_change(self); return 0; } naxis = (Py_ssize_t)self->x.naxis; if (set_double_array("crota", value, 1, &naxis, self->x.crota)) { return -1; } self->x.altlin |= has_crota; note_change(self); return 0; } /*@null@*/ static PyObject* PyWcsprm_get_crpix( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.crpix)) { return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_double_array("crpix", self->x.crpix, 1, &naxis, (PyObject*)self); } static int PyWcsprm_set_crpix( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis = 0; if (is_null(self->x.crpix)) { return -1; } naxis = (Py_ssize_t)self->x.naxis; note_change(self); return set_double_array("crpix", value, 1, &naxis, self->x.crpix); } /*@null@*/ static PyObject* PyWcsprm_get_crval( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis = 0; if (is_null(self->x.crval)) { return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_double_array("crval", self->x.crval, 1, &naxis, (PyObject*)self); } static int PyWcsprm_set_crval( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis; if (is_null(self->x.crval)) { return -1; } naxis = (Py_ssize_t)self->x.naxis; note_change(self); return set_double_array("crval", value, 1, &naxis, self->x.crval); } /*@null@*/ static PyObject* PyWcsprm_get_csyer( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t naxis; if (is_null(self->x.csyer)) { return NULL; } naxis = (Py_ssize_t)self->x.naxis; return get_double_array("csyer", self->x.csyer, 1, &naxis, (PyObject*)self); } static int PyWcsprm_set_csyer( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp naxis; if (is_null(self->x.csyer)) { return -1; } naxis = (Py_ssize_t)self->x.naxis; note_change(self); return set_double_array("csyer", value, 1, &naxis, self->x.csyer); } /*@null@*/ static PyObject* PyWcsprm_get_ctype( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.ctype)) { return NULL; } return get_str_list("ctype", self->x.ctype, self->x.naxis, 68, (PyObject*)self); } static int PyWcsprm_set_ctype( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.ctype)) { return -1; } note_change(self); return set_str_list("ctype", value, (Py_ssize_t)self->x.naxis, 0, self->x.ctype); } static PyObject* PyWcsprm_get_cubeface( PyWcsprm* self, /*@unused@*/ void* closure) { return get_int("cubeface", self->x.cubeface); } static int PyWcsprm_set_cubeface( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); return set_int("cubeface", value, &self->x.cubeface); } static int unit_verify(char* val) { int status, func; double scale, units[WCSUNITS_NTYPE]; struct wcserr *err = NULL; status = wcsulexe(val, &func, &scale, units, &err); if (status == 0) { return 1; } else { wcserr_units_to_python_exc(err); free(err); return 0; } } /*@null@*/ static PyObject* PyWcsprm_get_cunit( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.cunit)) { return NULL; } return get_str_list_verified( "cunit", self->x.cunit, (Py_ssize_t)self->x.naxis, 68, (PyObject*)self, unit_verify); } static int PyWcsprm_set_cunit( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.cunit)) { return -1; } note_change(self); return set_str_list_verified( "cunit", value, (Py_ssize_t)self->x.naxis, 0, self->x.cunit, unit_verify); } /*@null@*/ static PyObject* PyWcsprm_get_dateavg( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.dateavg)) { return NULL; } return get_string("dateavg", self->x.dateavg); } static int PyWcsprm_set_dateavg( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.dateavg)) { return -1; } note_change(self); /* TODO: Verify that this looks like a date string */ return set_string("dateavg", value, self->x.dateavg, 72); } /*@null@*/ static PyObject* PyWcsprm_get_dateobs( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.dateobs)) { return NULL; } return get_string("dateobs", self->x.dateobs); } static int PyWcsprm_set_dateobs( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.dateobs)) { return -1; } note_change(self); return set_string("dateobs", value, self->x.dateobs, 72); } static PyObject* PyWcsprm_get_equinox( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("equinox", self->x.equinox); } static int PyWcsprm_set_equinox( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (value == NULL) { /* deletion */ self->x.equinox = (double)NPY_NAN; return 0; } note_change(self); return set_double("equinox", value, &self->x.equinox); } /*@null@*/ static PyObject* PyWcsprm_get_imgpix_matrix( PyWcsprm* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (is_null(self->x.lin.imgpix)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; return get_double_array("imgpix_matrix", self->x.lin.imgpix, 2, dims, (PyObject*)self); } static PyObject* PyWcsprm_get_lat( PyWcsprm* self, /*@unused@*/ void* closure) { if (PyWcsprm_cset(self, 1)) { return NULL; } return get_int("lat", self->x.lat); } static PyObject* PyWcsprm_get_latpole( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("latpole", self->x.latpole); } static int PyWcsprm_set_latpole( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); if (value == NULL) { self->x.latpole = 90.0; return 0; } return set_double("latpole", value, &self->x.latpole); } /*@null@*/ static PyObject* PyWcsprm_get_lattyp( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.lattyp)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } return get_string("lattyp", self->x.lattyp); } static PyObject* PyWcsprm_get_lng( PyWcsprm* self, /*@unused@*/ void* closure) { if (PyWcsprm_cset(self, 1)) { return NULL; } return get_int("lng", self->x.lng); } /*@null@*/ static PyObject* PyWcsprm_get_lngtyp( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.lngtyp)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } return get_string("lngtyp", self->x.lngtyp); } static PyObject* PyWcsprm_get_lonpole( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("lonpole", self->x.lonpole); } static int PyWcsprm_set_lonpole( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); if (value == NULL) { self->x.lonpole = (double)NPY_NAN; return 0; } return set_double("lonpole", value, &self->x.lonpole); } static PyObject* PyWcsprm_get_mjdavg( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("mjdavg", self->x.mjdavg); } static int PyWcsprm_set_mjdavg( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); if (value == NULL) { self->x.mjdavg = (double)NPY_NAN; return 0; } return set_double("mjdavg", value, &self->x.mjdavg); } static PyObject* PyWcsprm_get_mjdobs( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("mjdobs", self->x.mjdobs); } static int PyWcsprm_set_mjdobs( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); if (value == NULL) { self->x.mjdobs = (double)NPY_NAN; return 0; } return set_double("mjdobs", value, &self->x.mjdobs); } /*@null@*/ static PyObject* PyWcsprm_get_name( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.wcsname)) { return NULL; } return get_string("name", self->x.wcsname); } static int PyWcsprm_set_name( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.wcsname)) { return -1; } note_change(self); return set_string("name", value, self->x.wcsname, 72); } static PyObject* PyWcsprm_get_naxis( PyWcsprm* self, /*@unused@*/ void* closure) { return get_int("naxis", self->x.naxis); } /*@null@*/ static PyObject* PyWcsprm_get_obsgeo( PyWcsprm* self, /*@unused@*/ void* closure) { Py_ssize_t size = 3; if (is_null(self->x.obsgeo)) { return NULL; } return get_double_array("obsgeo", self->x.obsgeo, 1, &size, (PyObject*)self); } static int PyWcsprm_set_obsgeo( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp size = 3; if (is_null(self->x.obsgeo)) { return -1; } note_change(self); if (value == NULL) { self->x.obsgeo[0] = NPY_NAN; self->x.obsgeo[1] = NPY_NAN; self->x.obsgeo[2] = NPY_NAN; return 0; } return set_double_array("obsgeo", value, 1, &size, self->x.obsgeo); } /*@null@*/ static PyObject* PyWcsprm_get_pc( PyWcsprm* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (is_null(self->x.pc)) { return NULL; } if (self->x.altlin != 0 && (self->x.altlin & has_pc) == 0) { PyErr_SetString(PyExc_AttributeError, "No pc is present."); return NULL; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; return get_double_array("pc", self->x.pc, 2, dims, (PyObject*)self); } static int PyWcsprm_set_pc( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp dims[2]; int i, j, naxis; double* pc; if (is_null(self->x.pc)) { return -1; } note_change(self); if (value == NULL) { /* deletion */ self->x.altlin &= ~has_pc; /* If this results in deleting all flags, pc is still the default, so we should set the pc matrix itself to default values. */ naxis = self->x.naxis; pc = self->x.pc; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++) { if (j == i) { *pc = 1.0; } else { *pc = 0.0; } pc++; } } note_change(self); return 0; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; if (set_double_array("pc", value, 2, dims, self->x.pc)) { return -1; } self->x.altlin |= has_pc; note_change(self); return 0; } static PyObject* PyWcsprm_get_phi0( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("phi0", self->x.cel.phi0); } static int PyWcsprm_set_phi0( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); if (value == NULL) { self->x.cel.phi0 = (double)NPY_NAN; return 0; } return set_double("phi0", value, &(self->x.cel.phi0)); } static PyObject* PyWcsprm_get_piximg_matrix( PyWcsprm* self, /*@unused@*/ void* closure) { npy_intp dims[2]; if (is_null(self->x.lin.piximg)) { return NULL; } if (PyWcsprm_cset(self, 1)) { return NULL; } dims[0] = self->x.naxis; dims[1] = self->x.naxis; return get_double_array("piximg_matrix", self->x.lin.piximg, 2, dims, (PyObject*)self); } static PyObject* PyWcsprm_get_radesys( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.radesys)) { return NULL; } return get_string("radesys", self->x.radesys); } static int PyWcsprm_set_radesys( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.radesys)) { return -1; } note_change(self); return set_string("radesys", value, self->x.radesys, 72); } static PyObject* PyWcsprm_get_restfrq( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("restfrq", self->x.restfrq); } static int PyWcsprm_set_restfrq( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (value == NULL) { /* deletion */ self->x.restfrq = (double)NPY_NAN; return 0; } note_change(self); return set_double("restfrq", value, &self->x.restfrq); } static PyObject* PyWcsprm_get_restwav( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("restwav", self->x.restwav); } static int PyWcsprm_set_restwav( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (value == NULL) { /* deletion */ self->x.restwav = (double)NPY_NAN; return 0; } note_change(self); return set_double("restwav", value, &self->x.restwav); } static PyObject* PyWcsprm_get_spec( PyWcsprm* self, /*@unused@*/ void* closure) { return get_int("spec", self->x.spec); } /*@null@*/ static PyObject* PyWcsprm_get_specsys( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.specsys)) { return NULL; } return get_string("specsys", self->x.specsys); } static int PyWcsprm_set_specsys( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.specsys)) { return -1; } note_change(self); return set_string("specsys", value, self->x.specsys, 72); } /*@null@*/ static PyObject* PyWcsprm_get_ssysobs( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.ssysobs)) { return NULL; } return get_string("ssysobs", self->x.ssysobs); } static int PyWcsprm_set_ssysobs( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.ssysobs)) { return -1; } note_change(self); return set_string("ssysobs", value, self->x.ssysobs, 72); } /*@null@*/ static PyObject* PyWcsprm_get_ssyssrc( PyWcsprm* self, /*@unused@*/ void* closure) { if (is_null(self->x.ssyssrc)) { return NULL; } return get_string("ssyssrc", self->x.ssyssrc); } static int PyWcsprm_set_ssyssrc( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (is_null(self->x.ssyssrc)) { return -1; } note_change(self); return set_string("ssyssrc", value, self->x.ssyssrc, 72); } static PyObject* PyWcsprm_get_tab( PyWcsprm* self, /*@unused@*/ void* closure) { PyObject* result; PyObject* subresult; int i, ntab; ntab = self->x.ntab; result = PyList_New(ntab); if (result == NULL) { return NULL; } for (i = 0; i < ntab; ++i) { subresult = (PyObject *)PyTabprm_cnew((PyObject *)self, &(self->x.tab[i])); if (subresult == NULL) { Py_DECREF(result); return NULL; } if (PyList_SetItem(result, i, subresult) == -1) { Py_DECREF(subresult); Py_DECREF(result); return NULL; } } return result; } static PyObject* PyWcsprm_get_theta0( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("theta0", self->x.cel.theta0); } static int PyWcsprm_set_theta0( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { note_change(self); if (value == NULL) { self->x.cel.theta0 = (double)NPY_NAN; return 0; } return set_double("theta0", value, &self->x.cel.theta0); } static PyObject* PyWcsprm_get_velangl( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("velangl", self->x.velangl); } static int PyWcsprm_set_velangl( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (value == NULL) { /* deletion */ self->x.velangl = (double)NPY_NAN; return 0; } note_change(self); return set_double("velangl", value, &self->x.velangl); } static PyObject* PyWcsprm_get_velosys( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("velosys", self->x.velosys); } static int PyWcsprm_set_velosys( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (value == NULL) { /* deletion */ self->x.velosys = (double)NPY_NAN; return 0; } note_change(self); return set_double("velosys", value, &self->x.velosys); } /* static PyObject* */ /* PyWcsprm_get_wtb( */ /* PyWcsprm* self, */ /* /\*@unused@*\/ void* closure) { */ /* PyObject* result; */ /* PyObject* subresult; */ /* int i, nwtb; */ /* nwtb = self->x.nwtb; */ /* result = PyList_New(nwtb); */ /* if (result == NULL) { */ /* return NULL; */ /* } */ /* for (i = 0; i < nwtb; ++i) { */ /* subresult = (PyObject *)PyWtbarr_cnew((PyObject *)self, &(self->x.wtb[i])); */ /* if (subresult == NULL) { */ /* Py_DECREF(result); */ /* return NULL; */ /* } */ /* if (PyList_SetItem(result, i, subresult) == -1) { */ /* Py_DECREF(subresult); */ /* Py_DECREF(result); */ /* return NULL; */ /* } */ /* } */ /* return result; */ /* } */ static PyObject* PyWcsprm_get_zsource( PyWcsprm* self, /*@unused@*/ void* closure) { return get_double("zsource", self->x.zsource); } static int PyWcsprm_set_zsource( PyWcsprm* self, PyObject* value, /*@unused@*/ void* closure) { if (value == NULL) { /* deletion */ self->x.zsource = (double)NPY_NAN; return 0; } note_change(self); return set_double("zsource", value, &self->x.zsource); } /*************************************************************************** * PyWcsprm definition structures */ static PyGetSetDef PyWcsprm_getset[] = { {"alt", (getter)PyWcsprm_get_alt, (setter)PyWcsprm_set_alt, (char *)doc_alt}, {"axis_types", (getter)PyWcsprm_get_axis_types, NULL, (char *)doc_axis_types}, {"cd", (getter)PyWcsprm_get_cd, (setter)PyWcsprm_set_cd, (char *)doc_cd}, {"cdelt", (getter)PyWcsprm_get_cdelt, (setter)PyWcsprm_set_cdelt, (char *)doc_cdelt}, {"cel_offset", (getter)PyWcsprm_get_cel_offset, (setter)PyWcsprm_set_cel_offset, (char *)doc_cel_offset}, {"cname", (getter)PyWcsprm_get_cname, (setter)PyWcsprm_set_cname, (char *)doc_cname}, {"colax", (getter)PyWcsprm_get_colax, (setter)PyWcsprm_set_colax, (char *)doc_colax}, {"colnum", (getter)PyWcsprm_get_colnum, (setter)PyWcsprm_set_colnum, (char *)doc_colnum}, {"crder", (getter)PyWcsprm_get_crder, (setter)PyWcsprm_set_crder, (char *)doc_crder}, {"crota", (getter)PyWcsprm_get_crota, (setter)PyWcsprm_set_crota, (char *)doc_crota}, {"crpix", (getter)PyWcsprm_get_crpix, (setter)PyWcsprm_set_crpix, (char *)doc_crpix}, {"crval", (getter)PyWcsprm_get_crval, (setter)PyWcsprm_set_crval, (char *)doc_crval}, {"csyer", (getter)PyWcsprm_get_csyer, (setter)PyWcsprm_set_csyer, (char *)doc_csyer}, {"ctype", (getter)PyWcsprm_get_ctype, (setter)PyWcsprm_set_ctype, (char *)doc_ctype}, {"cubeface", (getter)PyWcsprm_get_cubeface, (setter)PyWcsprm_set_cubeface, (char *)doc_cubeface}, {"cunit", (getter)PyWcsprm_get_cunit, (setter)PyWcsprm_set_cunit, (char *)doc_cunit}, {"dateavg", (getter)PyWcsprm_get_dateavg, (setter)PyWcsprm_set_dateavg, (char *)doc_dateavg}, {"dateobs", (getter)PyWcsprm_get_dateobs, (setter)PyWcsprm_set_dateobs, (char *)doc_dateobs}, {"equinox", (getter)PyWcsprm_get_equinox, (setter)PyWcsprm_set_equinox, (char *)doc_equinox}, {"imgpix_matrix", (getter)PyWcsprm_get_imgpix_matrix, NULL, (char *)doc_imgpix_matrix}, {"lat", (getter)PyWcsprm_get_lat, NULL, (char *)doc_lat}, {"latpole", (getter)PyWcsprm_get_latpole, (setter)PyWcsprm_set_latpole, (char *)doc_latpole}, {"lattyp", (getter)PyWcsprm_get_lattyp, NULL, (char *)doc_lattyp}, {"lng", (getter)PyWcsprm_get_lng, NULL, (char *)doc_lng}, {"lngtyp", (getter)PyWcsprm_get_lngtyp, NULL, (char *)doc_lngtyp}, {"lonpole", (getter)PyWcsprm_get_lonpole, (setter)PyWcsprm_set_lonpole, (char *)doc_lonpole}, {"mjdavg", (getter)PyWcsprm_get_mjdavg, (setter)PyWcsprm_set_mjdavg, (char *)doc_mjdavg}, {"mjdobs", (getter)PyWcsprm_get_mjdobs, (setter)PyWcsprm_set_mjdobs, (char *)doc_mjdobs}, {"name", (getter)PyWcsprm_get_name, (setter)PyWcsprm_set_name, (char *)doc_name}, {"naxis", (getter)PyWcsprm_get_naxis, NULL, (char *)doc_naxis}, {"obsgeo", (getter)PyWcsprm_get_obsgeo, (setter)PyWcsprm_set_obsgeo, (char *)doc_obsgeo}, {"pc", (getter)PyWcsprm_get_pc, (setter)PyWcsprm_set_pc, (char *)doc_pc}, {"phi0", (getter)PyWcsprm_get_phi0, (setter)PyWcsprm_set_phi0, (char *)doc_phi0}, {"piximg_matrix", (getter)PyWcsprm_get_piximg_matrix, NULL, (char *)doc_piximg_matrix}, {"radesys", (getter)PyWcsprm_get_radesys, (setter)PyWcsprm_set_radesys, (char *)doc_radesys}, {"restfrq", (getter)PyWcsprm_get_restfrq, (setter)PyWcsprm_set_restfrq, (char *)doc_restfrq}, {"restwav", (getter)PyWcsprm_get_restwav, (setter)PyWcsprm_set_restwav, (char *)doc_restwav}, {"spec", (getter)PyWcsprm_get_spec, NULL, (char *)doc_spec}, {"specsys", (getter)PyWcsprm_get_specsys, (setter)PyWcsprm_set_specsys, (char *)doc_specsys}, {"ssysobs", (getter)PyWcsprm_get_ssysobs, (setter)PyWcsprm_set_ssysobs, (char *)doc_ssysobs}, {"ssyssrc", (getter)PyWcsprm_get_ssyssrc, (setter)PyWcsprm_set_ssyssrc, (char *)doc_ssyssrc}, {"tab", (getter)PyWcsprm_get_tab, NULL, (char *)doc_tab}, {"theta0", (getter)PyWcsprm_get_theta0, (setter)PyWcsprm_set_theta0, (char *)doc_theta0}, {"velangl", (getter)PyWcsprm_get_velangl, (setter)PyWcsprm_set_velangl, (char *)doc_velangl}, {"velosys", (getter)PyWcsprm_get_velosys, (setter)PyWcsprm_set_velosys, (char *)doc_velosys}, /* {"wtb", (getter)PyWcsprm_get_wtb, NULL, (char *)doc_tab}, */ {"zsource", (getter)PyWcsprm_get_zsource, (setter)PyWcsprm_set_zsource, (char *)doc_zsource}, {NULL} }; static PyMethodDef PyWcsprm_methods[] = { {"celfix", (PyCFunction)PyWcsprm_celfix, METH_NOARGS, doc_celfix}, {"__copy__", (PyCFunction)PyWcsprm_copy, METH_NOARGS, doc_copy}, {"cylfix", (PyCFunction)PyWcsprm_cylfix, METH_VARARGS|METH_KEYWORDS, doc_cylfix}, {"datfix", (PyCFunction)PyWcsprm_datfix, METH_NOARGS, doc_datfix}, {"__deepcopy__", (PyCFunction)PyWcsprm_copy, METH_O, doc_copy}, {"fix", (PyCFunction)PyWcsprm_fix, METH_VARARGS|METH_KEYWORDS, doc_fix}, {"get_cdelt", (PyCFunction)PyWcsprm_get_cdelt_func, METH_NOARGS, doc_get_cdelt}, {"get_pc", (PyCFunction)PyWcsprm_get_pc_func, METH_NOARGS, doc_get_pc}, {"get_ps", (PyCFunction)PyWcsprm_get_ps, METH_NOARGS, doc_get_ps}, {"get_pv", (PyCFunction)PyWcsprm_get_pv, METH_NOARGS, doc_get_pv}, {"has_cd", (PyCFunction)PyWcsprm_has_cdi_ja, METH_NOARGS, doc_has_cd}, {"has_cdi_ja", (PyCFunction)PyWcsprm_has_cdi_ja, METH_NOARGS, doc_has_cdi_ja}, {"has_crota", (PyCFunction)PyWcsprm_has_crotaia, METH_NOARGS, doc_has_crota}, {"has_crotaia", (PyCFunction)PyWcsprm_has_crotaia, METH_NOARGS, doc_has_crotaia}, {"has_pc", (PyCFunction)PyWcsprm_has_pci_ja, METH_NOARGS, doc_has_pc}, {"has_pci_ja", (PyCFunction)PyWcsprm_has_pci_ja, METH_NOARGS, doc_has_pci_ja}, {"is_unity", (PyCFunction)PyWcsprm_is_unity, METH_NOARGS, doc_is_unity}, {"mix", (PyCFunction)PyWcsprm_mix, METH_VARARGS|METH_KEYWORDS, doc_mix}, {"p2s", (PyCFunction)PyWcsprm_p2s, METH_VARARGS|METH_KEYWORDS, doc_p2s}, {"print_contents", (PyCFunction)PyWcsprm_print_contents, METH_NOARGS, doc_print_contents}, {"s2p", (PyCFunction)PyWcsprm_s2p, METH_VARARGS|METH_KEYWORDS, doc_s2p}, {"set", (PyCFunction)PyWcsprm_set, METH_NOARGS, doc_set}, {"set_ps", (PyCFunction)PyWcsprm_set_ps, METH_O, doc_set_ps}, {"set_pv", (PyCFunction)PyWcsprm_set_pv, METH_O, doc_set_pv}, {"spcfix", (PyCFunction)PyWcsprm_spcfix, METH_NOARGS, doc_spcfix}, {"sptr", (PyCFunction)PyWcsprm_sptr, METH_VARARGS|METH_KEYWORDS, doc_sptr}, {"sub", (PyCFunction)PyWcsprm_sub, METH_VARARGS|METH_KEYWORDS, doc_sub}, {"to_header", (PyCFunction)PyWcsprm_to_header, METH_VARARGS|METH_KEYWORDS, doc_to_header}, {"unitfix", (PyCFunction)PyWcsprm_unitfix, METH_VARARGS|METH_KEYWORDS, doc_unitfix}, {NULL} }; PyTypeObject PyWcsprmType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs._Wcsprm", /*tp_name*/ sizeof(PyWcsprm), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyWcsprm_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ (reprfunc)PyWcsprm___str__, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ (reprfunc)PyWcsprm___str__, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE, /*tp_flags*/ doc_Wcsprm, /* tp_doc */ 0, /* tp_traverse */ 0, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PyWcsprm_methods, /* tp_methods */ 0, /* tp_members */ PyWcsprm_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ (initproc)PyWcsprm_init, /* tp_init */ 0, /* tp_alloc */ PyWcsprm_new, /* tp_new */ }; #define CONSTANT(a) PyModule_AddIntConstant(m, #a, a) int _setup_wcsprm_type( PyObject* m) { if (PyType_Ready(&PyWcsprmType) < 0) { return -1; } Py_INCREF(&PyWcsprmType); wcsprintf_set(NULL); wcserr_enable(1); return ( PyModule_AddObject(m, "_Wcsprm", (PyObject *)&PyWcsprmType) || CONSTANT(WCSSUB_LONGITUDE) || CONSTANT(WCSSUB_LATITUDE) || CONSTANT(WCSSUB_CUBEFACE) || CONSTANT(WCSSUB_SPECTRAL) || CONSTANT(WCSSUB_STOKES) || CONSTANT(WCSSUB_CELESTIAL) || CONSTANT(WCSHDR_IMGHEAD) || CONSTANT(WCSHDR_BIMGARR) || CONSTANT(WCSHDR_PIXLIST) || CONSTANT(WCSHDR_none) || CONSTANT(WCSHDR_all) || CONSTANT(WCSHDR_CROTAia) || CONSTANT(WCSHDR_EPOCHa) || CONSTANT(WCSHDR_VELREFa) || CONSTANT(WCSHDR_CD00i00j) || CONSTANT(WCSHDR_PC00i00j) || CONSTANT(WCSHDR_PROJPn) || CONSTANT(WCSHDR_RADECSYS) || CONSTANT(WCSHDR_VSOURCE) || CONSTANT(WCSHDR_DOBSn) || CONSTANT(WCSHDR_LONGKEY) || CONSTANT(WCSHDR_CNAMn) || CONSTANT(WCSHDR_AUXIMG) || CONSTANT(WCSHDR_ALLIMG) || CONSTANT(WCSHDO_none) || CONSTANT(WCSHDO_all) || CONSTANT(WCSHDO_safe) || CONSTANT(WCSHDO_DOBSn) || CONSTANT(WCSHDO_TPCn_ka) || CONSTANT(WCSHDO_PVn_ma) || CONSTANT(WCSHDO_CRPXna) || CONSTANT(WCSHDO_CNAMna) || CONSTANT(WCSHDO_WCSNna)); } pywcs-1.12/src/wcslib_wrap.h0000644001153600020070000000347112310355626020127 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __WCSLIB_WRAP_H__ #define __WCSLIB_WRAP_H__ #include "pyutil.h" extern PyTypeObject PyWcsprmType; typedef struct { PyObject_HEAD struct wcsprm x; } PyWcsprm; int _setup_wcsprm_type(PyObject* m); PyObject* PyWcsprm_find_all_wcs( PyObject* self, PyObject* args, PyObject* kwds); #endif pywcs-1.12/src/wcslib_wtbarr_wrap.c0000644001153600020070000002100612310355626021475 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #define NO_IMPORT_ARRAY #include "wcslib_wtbarr_wrap.h" #include /* It gets to be really tedious to type long docstrings in ANSI C syntax (since multi-line strings literals are not valid). Therefore, the docstrings are written in doc/docstrings.py, which are then converted by setup.py into docstrings.h, which we include here. */ #include "docstrings.h" /*************************************************************************** * Helper functions * ***************************************************************************/ /*************************************************************************** * PyWtbarr methods */ static int PyWtbarr_traverse( PyWtbarr* self, visitproc visit, void *arg) { int vret; vret = visit(self->owner, arg); if (vret != 0) { return vret; } return 0; } static int PyWtbarr_clear( PyWtbarr* self) { PyObject* tmp; tmp = self->owner; self->owner = NULL; Py_XDECREF(tmp); return 0; } static void PyWtbarr_dealloc( PyWtbarr* self) { PyWtbarr_clear(self); Py_TYPE(self)->tp_free((PyObject*)self); } PyWtbarr* PyWtbarr_cnew(PyObject* wcsprm, struct wtbarr* x) { PyWtbarr* self; self = (PyWtbarr*)(&PyWtbarrType)->tp_alloc(&PyWtbarrType, 0); self->x = x; Py_INCREF(wcsprm); self->owner = wcsprm; return self; } /*************************************************************************** * Member getters/setters (properties) */ /*@null@*/ static PyObject* PyWtbarr_get_data( PyWtbarr* self, /*@unused@*/ void* closure) { npy_intp ndims; npy_intp dims[NPY_MAXDIMS]; npy_intp i; if (is_null(self->x->arrayp)) { return NULL; } ndims = (Py_ssize_t)self->x->ndim; for (i = 0; i < ndims; ++i) { dims[i] = self->x->dimlen[i]; } return get_double_array("data", *self->x->arrayp, ndims, dims, (PyObject*)self); } /*@null@*/ static int PyWtbarr_set_data( PyWtbarr* self, PyObject* value, /*@unused@*/ void* closure) { npy_intp ndims; npy_intp dims[NPY_MAXDIMS]; npy_intp i; if (is_null(self->x->arrayp)) { return -1; } ndims = (Py_ssize_t)self->x->ndim; for (i = 0; i < ndims; ++i) { dims[i] = self->x->dimlen[i]; } return set_double_array("data", value, ndims, dims, *self->x->arrayp); } /*@null@*/ static PyObject* PyWtbarr_get_dims( PyWtbarr* self, /*@unused@*/ void* closure) { Py_ssize_t ndims = 0; if (is_null(self->x->dimlen)) { return NULL; } ndims = (Py_ssize_t)self->x->ndim; return get_int_array("dims", self->x->dimlen, 1, &ndims, (PyObject*)self); } /*@null@*/ static PyObject* PyWtbarr_get_extlev( PyWtbarr* self, /*@unused@*/ void* closure) { return get_int("extlev", self->x->extlev); } /*@null@*/ static PyObject* PyWtbarr_get_extnam( PyWtbarr* self, /*@unused@*/ void* closure) { return get_string("extnam", self->x->extnam); } /*@null@*/ static PyObject* PyWtbarr_get_extver( PyWtbarr* self, /*@unused@*/ void* closure) { return get_int("extver", self->x->extver); } /*@null@*/ static PyObject* PyWtbarr_get_i( PyWtbarr* self, /*@unused@*/ void* closure) { return get_int("i", self->x->i); } /*@null@*/ static PyObject* PyWtbarr_get_kind( PyWtbarr* self, /*@unused@*/ void* closure) { char kind = (char)self->x->kind; #if PY3K return PyUnicode_FromStringAndSize(&kind, 1); #else return PyString_FromStringAndSize(&kind, 1); #endif } /*@null@*/ static PyObject* PyWtbarr_get_m( PyWtbarr* self, /*@unused@*/ void* closure) { return get_int("m", self->x->m); } /*@null@*/ static PyObject* PyWtbarr_get_ndim( PyWtbarr* self, /*@unused@*/ void* closure) { return get_int("ndim", self->x->ndim); } /*@null@*/ static PyObject* PyWtbarr_get_row( PyWtbarr* self, /*@unused@*/ void* closure) { return get_int("row", self->x->row); } /*@null@*/ static PyObject* PyWtbarr_get_ttype( PyWtbarr* self, /*@unused@*/ void* closure) { return get_string("ttype", self->x->ttype); } /*************************************************************************** * PyWtbarr definition structures */ static PyGetSetDef PyWtbarr_getset[] = { {"data", (getter)PyWtbarr_get_data, (setter)PyWtbarr_set_data, (char *)doc_data}, {"dims", (getter)PyWtbarr_get_dims, NULL, (char *)doc_dims}, {"extlev", (getter)PyWtbarr_get_extlev, NULL, (char *)doc_extlev}, {"extnam", (getter)PyWtbarr_get_extnam, NULL, (char *)doc_extnam}, {"extver", (getter)PyWtbarr_get_extver, NULL, (char *)doc_extver}, {"i", (getter)PyWtbarr_get_i, NULL, (char *)doc_i}, {"kind", (getter)PyWtbarr_get_kind, NULL, (char *)doc_kind}, {"m", (getter)PyWtbarr_get_m, NULL, (char *)doc_m}, {"ndim", (getter)PyWtbarr_get_ndim, NULL, (char *)doc_ndim}, {"row", (getter)PyWtbarr_get_row, NULL, (char *)doc_row}, {"ttype", (getter)PyWtbarr_get_ttype, NULL, (char *)doc_ttype}, {NULL} }; static PyMethodDef PyWtbarr_methods[] = { {NULL} }; PyTypeObject PyWtbarrType = { #if PY3K PyVarObject_HEAD_INIT(NULL, 0) #else PyObject_HEAD_INIT(NULL) 0, /*ob_size*/ #endif "pywcs.Wtbarr", /*tp_name*/ sizeof(PyWtbarr), /*tp_basicsize*/ 0, /*tp_itemsize*/ (destructor)PyWtbarr_dealloc, /*tp_dealloc*/ 0, /*tp_print*/ 0, /*tp_getattr*/ 0, /*tp_setattr*/ 0, /*tp_compare*/ 0, /*tp_repr*/ 0, /*tp_as_number*/ 0, /*tp_as_sequence*/ 0, /*tp_as_mapping*/ 0, /*tp_hash */ 0, /*tp_call*/ 0, /*tp_str*/ 0, /*tp_getattro*/ 0, /*tp_setattro*/ 0, /*tp_as_buffer*/ Py_TPFLAGS_DEFAULT | Py_TPFLAGS_BASETYPE, /*tp_flags*/ doc_Wtbarr, /* tp_doc */ (traverseproc)PyWtbarr_traverse, /* tp_traverse */ (inquiry)PyWtbarr_clear, /* tp_clear */ 0, /* tp_richcompare */ 0, /* tp_weaklistoffset */ 0, /* tp_iter */ 0, /* tp_iternext */ PyWtbarr_methods, /* tp_methods */ 0, /* tp_members */ PyWtbarr_getset, /* tp_getset */ 0, /* tp_base */ 0, /* tp_dict */ 0, /* tp_descr_get */ 0, /* tp_descr_set */ 0, /* tp_dictoffset */ 0, /* tp_init */ 0, /* tp_alloc */ 0, /* tp_new */ }; int _setup_wtbarr_type( PyObject* m) { if (PyType_Ready(&PyWtbarrType) < 0) { return -1; } Py_INCREF(&PyWtbarrType); PyModule_AddObject(m, "Wtbarr", (PyObject *)&PyWtbarrType); return 0; } pywcs-1.12/src/wcslib_wtbarr_wrap.h0000644001153600020070000000351312310355626021505 0ustar cslocumSTSCI\science00000000000000/* Copyright (C) 2008-2012 Association of Universities for Research in Astronomy (AURA) Redistribution and use in source and binary forms, with or without modification, are permitted provided that the following conditions are met: 1. Redistributions of source code must retain the above copyright notice, this list of conditions and the following disclaimer. 2. Redistributions in binary form must reproduce the above copyright notice, this list of conditions and the following disclaimer in the documentation and/or other materials provided with the distribution. 3. The name of AURA and its representatives may not be used to endorse or promote products derived from this software without specific prior written permission. THIS SOFTWARE IS PROVIDED BY AURA ``AS IS'' AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR A PARTICULAR PURPOSE ARE DISCLAIMED. IN NO EVENT SHALL AURA BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL, SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE. */ /* Author: Michael Droettboom mdroe@stsci.edu */ #ifndef __WCSLIB_WTBARR_WRAP_H__ #define __WCSLIB_WTBARR_WRAP_H__ #include "pyutil.h" #include "wcs.h" extern PyTypeObject PyWtbarrType; typedef struct { PyObject_HEAD struct wtbarr* x; PyObject* owner; } PyWtbarr; PyWtbarr* PyWtbarr_cnew(PyObject* wcsprm, struct wtbarr* x); int _setup_wtbarr_type(PyObject* m); #endif pywcs-1.12/stsci_distutils_hack.py0000644001153600020070000002152112310355627021441 0ustar cslocumSTSCI\science00000000000000# # $HeadURL: https://www.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/pytools/lib/stsci_distutils_hack.py $ # $Rev: 7917 $ # # Implements setup.py code common to many of our packages. # # The new standard stsci module setup.py is just # # import pytools.stsci_distutils_hack # pytools.stsci_distutils_hack.run( pytools_version = "XX" ) # # where XX is the version of pytools you expect for the install to work # from __future__ import division # confidence high """ Special handling for stsci_python package installation. stsci_python is distributed as a single package, but it contains packages that are also distributed separately. When we use this module to install our package, we can use the exact same definition file to control the setup.py of the individual package _and_ the setup.py of stsci_python. This module also preserves revision control data in the installed or distributed files. If you are not a developer at STScI, this module is probably not of much interest to you. """ __docformat__ = 'restructuredtext' ######## ######## ######## ######## ######## ######## ######## ######## # # actually perform the install # # NOTE: This is not used to install pytools itself! import sys def run( pytools_version = None ) : """ Perform a stsci_python install based on the information in defsetup.py * gather our subversion revision number and the install time * perform the install usage: import pytools.stsci_distutils_hack pytools.stsci_distutils_hack.run(pytools_version = "3.0") """ if not hasattr(sys, 'version_info') or sys.version_info < (2,3,0,'alpha',0): raise SystemExit("Python 2.3 or later required.") if pytools_version : # Only try to import pytools if we are asked to check for a version. # # ( We may have been extracted from pytools and bundled with a package. # In that case, we do not want to risk finding some _other_ pytools # and comparing that version. ) import pytools # bug: should use distutils version comparator to perform ">" comparisons if ( pytools.__version__ != pytools_version ) : print("wrong version of pytools!") print("have %s" % pytools.__version__) print("want %s" % pytools_version) sys.exit(1) from distutils.core import setup from defsetup import setupargs, pkg # collect our subversion information __set_svn_version__() # save the date when we last ran setup.py __set_setup_date__() if "version" in sys.argv : sys.exit(0) # If they have multiple packages, we have to allow them to give a list. # That is the unusual case, so we let them give a string if they have a single # package. if isinstance(pkg,str) : pkg = [ pkg ] # If they have multiple packages, they have to specify package_dir. Otherwise, # we can create one for them. setup( name = pkg[0], packages = pkg, **setupargs ) ######## ######## ######## ######## ######## ######## ######## ######## # # This part fixes install_data to put data files in the same directory # with the python library files, which is where our packages want # them. # # This is essentially "smart_install_data" as used in the old # setup.py files, except that it also understands wildcards # and os-specific paths. This means the module author can # ask for data files with # "data/generic/*" # instead of # glob.glob(os.path.join('data', 'generic', '*')) import os import glob import distutils.util import distutils.command.install_data o = distutils.command.install_data.install_data # same trick as smart_install_data used: save the old run() method and # insert our own run method ahead of it o.old_run = o.run def new_run ( self ) : """ Hack for distutils to cause install_data to be in the same directory as the python library files. Our packages expect this. """ # We want our data files in the directory with the library files install_cmd = self.get_finalized_command('install') self.install_dir = getattr(install_cmd, 'install_lib') # self.data_files is a list of # ( destination_directory, [ source_file, source_file, source_file ] ) # # We want to do wildcard expansion on all the file names. # l = [ ] for f in self.data_files : ( dest_dir, files ) = f fl = [ ] for ff in files : ff = distutils.util.convert_path(ff) ff = glob.glob(ff) fl.extend(ff) dest_dir = distutils.util.convert_path(dest_dir) l.append( ( dest_dir, fl ) ) self.data_files = l # now use the original run() function to finish return distutils.command.install_data.install_data.old_run(self) o.run = new_run ######## ######## ######## ######## ######## ######## ######## ######## # # Function to collect svn version information - used to be stsci_python/version.py # with multiple copies in the system. # import os.path import re # # This is the entry point. All you need to do is call this function from your # setup.py according to the example above. It will create a file called # lib/svn_version.py ; After that, you can # # # find out what subversion information applies to yourpackage # import yourpackage.svn_version # print yourpackage.svn_version.__svn_version__ # print yourpackage.svn_version.__full_svn_info__ # def __set_svn_version__(path="./", fname='svn_version.py' ) : # # path is the package where the version information will be stored. Default # is "this package", but from a higher level package, you can specify a directory # of a package to process # # fname is the name of the file to store the version information in. Never change # this. # info = None rev = __get_svn_rev__(path) version_file = os.path.join(path,'lib',fname) # if we are unable to determine the revision, we default to leaving the # revision file unchanged. Otherwise, we fill it in with whatever # we have if rev is None: if os.path.exists(version_file) : return revision = 'Unable to determine SVN revision' else: if ( rev == 'exported' or rev == 'unknown' ) and os.path.exists(version_file) : return revision = str(rev) info = __get_full_info__(path) # now we can write the version information f = open(version_file,'w') f.write("__svn_version__ = %s\n" % repr(revision)) # info will be a multi-line string. We are not using repr(info) # for readability; the output of "svn info" can not contain ''' # unless you are doing something bad. f.write("\n__full_svn_info__ = '''\n%s'''\n\n" % info) f.close() def __get_svn_rev__(path): m = None try: # with popen3, stderr goes into a pipe where we ignore it, # This means the user does not see errors. cmd = 'svnversion '+path (sin, sout, serr) = os.popen3(cmd) # pick up the first line of output m=sout.read().strip() # if it looks like valid svnversion output, return it if m == 'exported' : return m if re.match('^[0-9][0-9:]*[A-Z]*$',m) : return m # if we get here, it was not valid - that probably means # an error of some kind. except: pass return None def __get_full_info__(path): info = None try: # with popen3, stderr goes into a pipe where we ignore it, # This means the user does not see errors. (sin, sout, serr) = os.popen3('svn info %s' % path) # pick up all the lines of output info = [l.strip() for l in sout.readlines()] # if no output, there was an error and we don't know anything if len(info) == 0 : return "unknown" # there was output, so join it all together return '\n'.join(info) except: pass return "unknown" ######## ######## ######## ######## ######## ######## ######## ######## # # note when we last ran setup.py -- what we really want is when the # software was installed, but we can use the time we ran setup.py as # a proxy for that. # def __set_setup_date__( path="./", fname='svn_version.py') : import datetime file = os.path.join(path,'lib',fname) d = datetime.datetime.now() l = [ ] try : # we don't expect this to fail ever, but it might f = open(file,"r") for line in f : if line.find("# setupdate") < 0 : l.append(line) f.close() except IOError : pass f=open(file,"w") for line in l : f.write(line) f.write("%s # setupdate\n" % "import datetime") f.write("%s # setupdate\n" % ("setupdate = "+repr(d))) f.close() pywcs-1.12/wcslib/0000755001153600020070000000000012310355732016127 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/C/0000755001153600020070000000000012310355732016311 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/C/cel.c0000644001153600020070000003032112310355626017221 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: cel.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsprintf.h" #include "wcstrig.h" #include "sph.h" #include "cel.h" const int CELSET = 137; /* Map status return value to message. */ const char *cel_errmsg[] = { "Success", "Null celprm pointer passed", "Invalid projection parameters", "Invalid coordinate transformation parameters", "Ill-conditioned coordinate transformation parameters", "One or more of the (x,y) coordinates were invalid", "One or more of the (lng,lat) coordinates were invalid"}; /* Convenience macro for invoking wcserr_set(). */ #define CEL_ERRMSG(status) WCSERR_SET(status), cel_errmsg[status] /*--------------------------------------------------------------------------*/ int celini(cel) struct celprm *cel; { register int k; if (cel == 0x0) return CELERR_NULL_POINTER; cel->flag = 0; cel->offset = 0; cel->phi0 = UNDEFINED; cel->theta0 = UNDEFINED; cel->ref[0] = 0.0; cel->ref[1] = 0.0; cel->ref[2] = UNDEFINED; cel->ref[3] = +90.0; for (k = 0; k < 5; cel->euler[k++] = 0.0); cel->latpreq = -1; cel->err = 0x0; return prjini(&(cel->prj)); } /*--------------------------------------------------------------------------*/ int celfree(cel) struct celprm *cel; { if (cel == 0x0) return CELERR_NULL_POINTER; if (cel->err) free(cel->err); cel->err = 0x0; prjfree(&(cel->prj)); return 0; } /*--------------------------------------------------------------------------*/ int celprt(cel) const struct celprm *cel; { int i; if (cel == 0x0) return CELERR_NULL_POINTER; wcsprintf(" flag: %d\n", cel->flag); wcsprintf(" offset: %d\n", cel->offset); if (undefined(cel->phi0)) { wcsprintf(" phi0: UNDEFINED\n"); } else { wcsprintf(" phi0: %9f\n", cel->phi0); } if (undefined(cel->theta0)) { wcsprintf(" theta0: UNDEFINED\n"); } else { wcsprintf(" theta0: %9f\n", cel->theta0); } wcsprintf(" ref:"); for (i = 0; i < 4; i++) { wcsprintf(" %- 11.5g", cel->ref[i]); } wcsprintf("\n"); wcsprintf(" prj: (see below)\n"); wcsprintf(" euler:"); for (i = 0; i < 5; i++) { wcsprintf(" %- 11.5g", cel->euler[i]); } wcsprintf("\n"); wcsprintf(" latpreq: %d", cel->latpreq); if (cel->latpreq == 0) { wcsprintf(" (not required)\n"); } else if (cel->latpreq == 1) { wcsprintf(" (disambiguation)\n"); } else if (cel->latpreq == 2) { wcsprintf(" (specification)\n"); } else { wcsprintf(" (UNDEFINED)\n"); } wcsprintf(" isolat: %d\n", cel->isolat); WCSPRINTF_PTR(" err: ", cel->err, "\n"); if (cel->err) { wcserr_prt(cel->err, " "); } wcsprintf("\n"); wcsprintf(" prj.*\n"); prjprt(&(cel->prj)); return 0; } /*--------------------------------------------------------------------------*/ int celset(cel) struct celprm *cel; { static const char *function = "celset"; const double tol = 1.0e-10; double clat0, cphip, cthe0, lat0, lng0, phip, slat0, slz, sphip, sthe0; double latp, latp1, latp2, lngp; double u, v, x, y, z; struct prjprm *celprj; struct wcserr **err; if (cel == 0x0) return CELERR_NULL_POINTER; err = &(cel->err); /* Initialize the projection driver routines. */ celprj = &(cel->prj); if (cel->offset) { celprj->phi0 = cel->phi0; celprj->theta0 = cel->theta0; } else { /* Ensure that these are undefined - no fiducial offset. */ celprj->phi0 = UNDEFINED; celprj->theta0 = UNDEFINED; } if (prjset(celprj)) { return wcserr_set(CEL_ERRMSG(CELERR_BAD_PARAM)); } /* Defaults set by the projection routines. */ if (undefined(cel->phi0)) { cel->phi0 = celprj->phi0; } if (undefined(cel->theta0)) { cel->theta0 = celprj->theta0; } else if (fabs(cel->theta0) > 90.0) { if (fabs(cel->theta0) > 90.0 + tol) { return wcserr_set(WCSERR_SET(CELERR_BAD_COORD_TRANS), "Invalid coordinate transformation parameters: theta0 > 90"); } if (cel->theta0 > 90.0) { cel->theta0 = 90.0; } else { cel->theta0 = -90.0; } } lng0 = cel->ref[0]; lat0 = cel->ref[1]; phip = cel->ref[2]; latp = cel->ref[3]; /* Set default for native longitude of the celestial pole? */ if (undefined(phip) || phip == 999.0) { phip = (lat0 < cel->theta0) ? 180.0 : 0.0; phip += cel->phi0; if (phip < -180.0) { phip += 360.0; } else if (phip > 180.0) { phip -= 360.0; } cel->ref[2] = phip; } /* Compute celestial coordinates of the native pole. */ cel->latpreq = 0; if (cel->theta0 == 90.0) { /* Fiducial point at the native pole. */ lngp = lng0; latp = lat0; } else { /* Fiducial point away from the native pole. */ sincosd(lat0, &slat0, &clat0); sincosd(cel->theta0, &sthe0, &cthe0); if (phip == cel->phi0) { sphip = 0.0; cphip = 1.0; u = cel->theta0; v = 90.0 - lat0; } else { sincosd(phip - cel->phi0, &sphip, &cphip); x = cthe0*cphip; y = sthe0; z = sqrt(x*x + y*y); if (z == 0.0) { if (slat0 != 0.0) { return wcserr_set(WCSERR_SET(CELERR_BAD_COORD_TRANS), "Invalid coordinate description:\n" "lat0 == 0 is required for |phip - phi0| = 90 and theta0 == 0"); } /* latp determined solely by LATPOLEa in this case. */ cel->latpreq = 2; if (latp > 90.0) { latp = 90.0; } else if (latp < -90.0) { latp = -90.0; } } else { slz = slat0/z; if (fabs(slz) > 1.0) { if ((fabs(slz) - 1.0) < tol) { if (slz > 0.0) { slz = 1.0; } else { slz = -1.0; } } else { return wcserr_set(WCSERR_SET(CELERR_BAD_COORD_TRANS), "Invalid coordinate description:\n|lat0| <= %.3f is required " "for these values of phip, phi0, and theta0", asind(z)); } } u = atan2d(y,x); v = acosd(slz); } } if (cel->latpreq == 0) { latp1 = u + v; if (latp1 > 180.0) { latp1 -= 360.0; } else if (latp1 < -180.0) { latp1 += 360.0; } latp2 = u - v; if (latp2 > 180.0) { latp2 -= 360.0; } else if (latp2 < -180.0) { latp2 += 360.0; } if (fabs(latp1) < 90.0+tol && fabs(latp2) < 90.0+tol) { /* There are two valid solutions for latp. */ cel->latpreq = 1; } if (fabs(latp-latp1) < fabs(latp-latp2)) { if (fabs(latp1) < 90.0+tol) { latp = latp1; } else { latp = latp2; } } else { if (fabs(latp2) < 90.0+tol) { latp = latp2; } else { latp = latp1; } } /* Account for rounding error. */ if (fabs(latp) < 90.0+tol) { if (latp > 90.0) { latp = 90.0; } else if (latp < -90.0) { latp = -90.0; } } } z = cosd(latp)*clat0; if (fabs(z) < tol) { if (fabs(clat0) < tol) { /* Celestial pole at the fiducial point. */ lngp = lng0; } else if (latp > 0.0) { /* Celestial north pole at the native pole.*/ lngp = lng0 + phip - cel->phi0 - 180.0; } else { /* Celestial south pole at the native pole. */ lngp = lng0 - phip + cel->phi0; } } else { x = (sthe0 - sind(latp)*slat0)/z; y = sphip*cthe0/clat0; if (x == 0.0 && y == 0.0) { /* Sanity check (shouldn't be possible). */ return wcserr_set(WCSERR_SET(CELERR_BAD_COORD_TRANS), "Invalid coordinate transformation parameters, internal error"); } lngp = lng0 - atan2d(y,x); } /* Make celestial longitude of the native pole the same sign as at the fiducial point. */ if (lng0 >= 0.0) { if (lngp < 0.0) { lngp += 360.0; } else if (lngp > 360.0) { lngp -= 360.0; } } else { if (lngp > 0.0) { lngp -= 360.0; } else if (lngp < -360.0) { lngp += 360.0; } } } /* Reset LATPOLEa. */ cel->ref[3] = latp; /* Set the Euler angles. */ cel->euler[0] = lngp; cel->euler[1] = 90.0 - latp; cel->euler[2] = phip; sincosd(cel->euler[1], &cel->euler[4], &cel->euler[3]); cel->isolat = (cel->euler[4] == 0.0); cel->flag = CELSET; /* Check for ill-conditioned parameters. */ if (fabs(latp) > 90.0+tol) { return wcserr_set(WCSERR_SET(CELERR_ILL_COORD_TRANS), "Ill-conditioned coordinate transformation parameters\nNo valid " "solution for latp for these values of phip, phi0, and theta0"); } return 0; } /*--------------------------------------------------------------------------*/ int celx2s(cel, nx, ny, sxy, sll, x, y, phi, theta, lng, lat, stat) struct celprm *cel; int nx, ny, sxy, sll; const double x[], y[]; double phi[], theta[]; double lng[], lat[]; int stat[]; { static const char *function = "celx2s"; int nphi, status; struct prjprm *celprj; struct wcserr **err; /* Initialize. */ if (cel == 0x0) return CELERR_NULL_POINTER; err = &(cel->err); if (cel->flag != CELSET) { if ((status = celset(cel))) return status; } /* Apply spherical deprojection. */ celprj = &(cel->prj); if ((status = celprj->prjx2s(celprj, nx, ny, sxy, 1, x, y, phi, theta, stat))) { if (status == PRJERR_BAD_PIX) { status = CELERR_BAD_PIX; } wcserr_set(CEL_ERRMSG(status)); if (status != CELERR_BAD_PIX) return status; } nphi = (ny > 0) ? (nx*ny) : nx; /* Compute celestial coordinates. */ sphx2s(cel->euler, nphi, 0, 1, sll, phi, theta, lng, lat); return status; } /*--------------------------------------------------------------------------*/ int cels2x(cel, nlng, nlat, sll, sxy, lng, lat, phi, theta, x, y, stat) struct celprm *cel; int nlng, nlat, sll, sxy; const double lng[], lat[]; double phi[], theta[]; double x[], y[]; int stat[]; { static const char *function = "cels2x"; int nphi, ntheta, status; struct prjprm *celprj; struct wcserr **err; /* Initialize. */ if (cel == 0x0) return CELERR_NULL_POINTER; err = &(cel->err); if (cel->flag != CELSET) { if ((status = celset(cel))) return status; } /* Compute native coordinates. */ sphs2x(cel->euler, nlng, nlat, sll, 1, lng, lat, phi, theta); if (cel->isolat) { /* Constant celestial latitude -> constant native latitude. */ nphi = nlng; ntheta = nlat; } else { nphi = (nlat > 0) ? (nlng*nlat) : nlng; ntheta = 0; } /* Apply the spherical projection. */ celprj = &(cel->prj); if ((status = celprj->prjs2x(celprj, nphi, ntheta, 1, sxy, phi, theta, x, y, stat))) { if (status != PRJERR_BAD_PARAM) { status = CELERR_BAD_WORLD; } return wcserr_set(CEL_ERRMSG(status)); } return 0; } pywcs-1.12/wcslib/C/cel.h0000644001153600020070000004261212310355626017234 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: cel.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of celestial coordinates in FITS", * Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077 (Paper II) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the cel routines * --------------------------- * These routines implement the part of the FITS World Coordinate System (WCS) * standard that deals with celestial coordinates. They define methods to be * used for computing celestial world coordinates from intermediate world * coordinates (a linear transformation of image pixel coordinates), and vice * versa. They are based on the celprm struct which contains all information * needed for the computations. This struct contains some elements that must * be set by the user, and others that are maintained by these routines, * somewhat like a C++ class but with no encapsulation. * * Routine celini() is provided to initialize the celprm struct with default * values, celfree() reclaims any memory that may have been allocated to store * an error message, and celprt() prints its contents. * * A setup routine, celset(), computes intermediate values in the celprm struct * from parameters in it that were supplied by the user. The struct always * needs to be set up by celset() but it need not be called explicitly - refer * to the explanation of celprm::flag. * * celx2s() and cels2x() implement the WCS celestial coordinate * transformations. In fact, they are high level driver routines for the lower * level spherical coordinate rotation and projection routines described in * sph.h and prj.h. * * * celini() - Default constructor for the celprm struct * ---------------------------------------------------- * celini() sets all members of a celprm struct to default values. It should * be used to initialize every celprm struct. * * Returned: * cel struct celprm* * Celestial transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null celprm pointer passed. * * * celfree() - Destructor for the celprm struct * -------------------------------------------- * celfree() frees any memory that may have been allocated to store an error * message in the celprm struct. * * Given: * cel struct celprm* * Celestial transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null celprm pointer passed. * * * celprt() - Print routine for the celprm struct * ---------------------------------------------- * celprt() prints the contents of a celprm struct using wcsprintf(). Mainly * intended for diagnostic purposes. * * Given: * cel const struct celprm* * Celestial transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null celprm pointer passed. * * * celset() - Setup routine for the celprm struct * ---------------------------------------------- * celset() sets up a celprm struct according to information supplied within * it. * * Note that this routine need not be called directly; it will be invoked by * celx2s() and cels2x() if celprm::flag is anything other than a predefined * magic value. * * Given and returned: * cel struct celprm* * Celestial transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null celprm pointer passed. * 2: Invalid projection parameters. * 3: Invalid coordinate transformation parameters. * 4: Ill-conditioned coordinate transformation * parameters. * * For returns > 1, a detailed error message is set in * celprm::err if enabled, see wcserr_enable(). * * * celx2s() - Pixel-to-world celestial transformation * -------------------------------------------------- * celx2s() transforms (x,y) coordinates in the plane of projection to * celestial coordinates (lng,lat). * * Given and returned: * cel struct celprm* * Celestial transformation parameters. * * Given: * nx,ny int Vector lengths. * * sxy,sll int Vector strides. * * x,y const double[] * Projected coordinates in pseudo "degrees". * * Returned: * phi,theta double[] Longitude and latitude (phi,theta) in the native * coordinate system of the projection [deg]. * * lng,lat double[] Celestial longitude and latitude (lng,lat) of the * projected point [deg]. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of (x,y). * * Function return value: * int Status return value: * 0: Success. * 1: Null celprm pointer passed. * 2: Invalid projection parameters. * 3: Invalid coordinate transformation parameters. * 4: Ill-conditioned coordinate transformation * parameters. * 5: One or more of the (x,y) coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * celprm::err if enabled, see wcserr_enable(). * * * cels2x() - World-to-pixel celestial transformation * -------------------------------------------------- * cels2x() transforms celestial coordinates (lng,lat) to (x,y) coordinates in * the plane of projection. * * Given and returned: * cel struct celprm* * Celestial transformation parameters. * * Given: * nlng,nlat int Vector lengths. * * sll,sxy int Vector strides. * * lng,lat const double[] * Celestial longitude and latitude (lng,lat) of the * projected point [deg]. * * Returned: * phi,theta double[] Longitude and latitude (phi,theta) in the native * coordinate system of the projection [deg]. * * x,y double[] Projected coordinates in pseudo "degrees". * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of (lng,lat). * * Function return value: * int Status return value: * 0: Success. * 1: Null celprm pointer passed. * 2: Invalid projection parameters. * 3: Invalid coordinate transformation parameters. * 4: Ill-conditioned coordinate transformation * parameters. * 6: One or more of the (lng,lat) coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * celprm::err if enabled, see wcserr_enable(). * * * celprm struct - Celestial transformation parameters * --------------------------------------------------- * The celprm struct contains information required to transform celestial * coordinates. It consists of certain members that must be set by the user * ("given") and others that are set by the WCSLIB routines ("returned"). Some * of the latter are supplied for informational purposes and others are for * internal use only. * * Returned celprm struct members must not be modified by the user. * * int flag * (Given and returned) This flag must be set to zero whenever any of the * following celprm struct members are set or changed: * * - celprm::offset, * - celprm::phi0, * - celprm::theta0, * - celprm::ref[4], * - celprm::prj: * - prjprm::code, * - prjprm::r0, * - prjprm::pv[], * - prjprm::phi0, * - prjprm::theta0. * * This signals the initialization routine, celset(), to recompute the * returned members of the celprm struct. celset() will reset flag to * indicate that this has been done. * * int offset * (Given) If true (non-zero), an offset will be applied to (x,y) to * force (x,y) = (0,0) at the fiducial point, (phi_0,theta_0). * Default is 0 (false). * * double phi0 * (Given) The native longitude, phi_0 [deg], and ... * * double theta0 * (Given) ... the native latitude, theta_0 [deg], of the fiducial point, * i.e. the point whose celestial coordinates are given in * celprm::ref[1:2]. If undefined (set to a magic value by prjini()) the * initialization routine, celset(), will set this to a projection-specific * default. * * double ref[4] * (Given) The first pair of values should be set to the celestial * longitude and latitude of the fiducial point [deg] - typically right * ascension and declination. These are given by the CRVALia keywords in * FITS. * * (Given and returned) The second pair of values are the native longitude, * phi_p [deg], and latitude, theta_p [deg], of the celestial pole (the * latter is the same as the celestial latitude of the native pole, * delta_p) and these are given by the FITS keywords LONPOLEa and LATPOLEa * (or by PVi_2a and PVi_3a attached to the longitude axis which take * precedence if defined). * * LONPOLEa defaults to phi_0 (see above) if the celestial latitude of the * fiducial point of the projection is greater than or equal to the native * latitude, otherwise phi_0 + 180 [deg]. (This is the condition for the * celestial latitude to increase in the same direction as the native * latitude at the fiducial point.) ref[2] may be set to UNDEFINED (from * wcsmath.h) or 999.0 to indicate that the correct default should be * substituted. * * theta_p, the native latitude of the celestial pole (or equally the * celestial latitude of the native pole, delta_p) is often determined * uniquely by CRVALia and LONPOLEa in which case LATPOLEa is ignored. * However, in some circumstances there are two valid solutions for theta_p * and LATPOLEa is used to choose between them. LATPOLEa is set in ref[3] * and the solution closest to this value is used to reset ref[3]. It is * therefore legitimate, for example, to set ref[3] to +90.0 to choose the * more northerly solution - the default if the LATPOLEa keyword is omitted * from the FITS header. For the special case where the fiducial point of * the projection is at native latitude zero, its celestial latitude is * zero, and LONPOLEa = +/- 90.0 then the celestial latitude of the native * pole is not determined by the first three reference values and LATPOLEa * specifies it completely. * * The returned value, celprm::latpreq, specifies how LATPOLEa was actually * used. * * struct prjprm prj * (Given and returned) Projection parameters described in the prologue to * prj.h. * * double euler[5] * (Returned) Euler angles and associated intermediaries derived from the * coordinate reference values. The first three values are the Z-, X-, and * Z'-Euler angles [deg], and the remaining two are the cosine and sine of * the X-Euler angle. * * int latpreq * (Returned) For informational purposes, this indicates how the LATPOLEa * keyword was used * - 0: Not required, theta_p (== delta_p) was determined uniquely by the * CRVALia and LONPOLEa keywords. * - 1: Required to select between two valid solutions of theta_p. * - 2: theta_p was specified solely by LATPOLEa. * * int isolat * (Returned) True if the spherical rotation preserves the magnitude of the * latitude, which occurs iff the axes of the native and celestial * coordinates are coincident. It signals an opportunity to cache * intermediate calculations common to all elements in a vector * computation. * * struct wcserr *err * (Returned) If enabled, when an error status is returned this struct * contains detailed information about the error, see wcserr_enable(). * * void *padding * (An unused variable inserted for alignment purposes only.) * * Global variable: const char *cel_errmsg[] - Status return messages * ------------------------------------------------------------------ * Status messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_CEL #define WCSLIB_CEL #include "prj.h" #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif extern const char *cel_errmsg[]; enum cel_errmsg_enum { CELERR_SUCCESS = 0, /* Success. */ CELERR_NULL_POINTER = 1, /* Null celprm pointer passed. */ CELERR_BAD_PARAM = 2, /* Invalid projection parameters. */ CELERR_BAD_COORD_TRANS = 3, /* Invalid coordinate transformation parameters. */ CELERR_ILL_COORD_TRANS = 4, /* Ill-conditioned coordinated transformation parameters. */ CELERR_BAD_PIX = 5, /* One or more of the (x,y) coordinates were invalid. */ CELERR_BAD_WORLD = 6 /* One or more of the (lng,lat) coordinates were invalid. */ }; struct celprm { /* Initialization flag (see the prologue above). */ /*------------------------------------------------------------------------*/ int flag; /* Set to zero to force initialization. */ /* Parameters to be provided (see the prologue above). */ /*------------------------------------------------------------------------*/ int offset; /* Force (x,y) = (0,0) at (phi_0,theta_0). */ double phi0, theta0; /* Native coordinates of fiducial point. */ double ref[4]; /* Celestial coordinates of fiducial */ /* point and native coordinates of */ /* celestial pole. */ struct prjprm prj; /* Projection parameters (see prj.h). */ /* Information derived from the parameters supplied. */ /*------------------------------------------------------------------------*/ double euler[5]; /* Euler angles and functions thereof. */ int latpreq; /* LATPOLEa requirement. */ int isolat; /* True if |latitude| is preserved. */ /* Error handling */ /*------------------------------------------------------------------------*/ struct wcserr *err; /* Private */ /*------------------------------------------------------------------------*/ void *padding; /* (Dummy inserted for alignment purposes.) */ }; /* Size of the celprm struct in int units, used by the Fortran wrappers. */ #define CELLEN (sizeof(struct celprm)/sizeof(int)) int celini(struct celprm *cel); int celfree(struct celprm *cel); int celprt(const struct celprm *cel); int celset(struct celprm *cel); int celx2s(struct celprm *cel, int nx, int ny, int sxy, int sll, const double x[], const double y[], double phi[], double theta[], double lng[], double lat[], int stat[]); int cels2x(struct celprm *cel, int nlng, int nlat, int sll, int sxy, const double lng[], const double lat[], double phi[], double theta[], double x[], double y[], int stat[]); /* Deprecated. */ #define celini_errmsg cel_errmsg #define celprt_errmsg cel_errmsg #define celset_errmsg cel_errmsg #define celx2s_errmsg cel_errmsg #define cels2x_errmsg cel_errmsg #ifdef __cplusplus } #endif #endif /* WCSLIB_CEL */ pywcs-1.12/wcslib/C/fitshdr.h0000644001153600020070000004323212310355626020133 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: fitshdr.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * The Flexible Image Transport System (FITS), a data format widely used in * astronomy for data interchange and archive, is described in * * "Definition of The Flexible Image Transport System (FITS)", * Hanisch, R.J., Farris, A., Greisen, E.W., et al. 2001, A&A, 376, 359 * * which formalizes NOST 100-2.0, a document produced by the NASA/Science * Office of Standards and Technology, see http://fits.gsfc.nasa.gov. * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the fitshdr routines * ------------------------------- * fitshdr() is a generic FITS header parser provided to handle keyrecords that * are ignored by the WCS header parsers, wcspih() and wcsbth(). Typically the * latter may be set to remove WCS keyrecords from a header leaving fitshdr() * to handle the remainder. * * * fitshdr() - FITS header parser routine * -------------------------------------- * fitshdr() parses a character array containing a FITS header, extracting * all keywords and their values into an array of fitskey structs. * * Given: * header const char [] * Character array containing the (entire) FITS header, * for example, as might be obtained conveniently via the * CFITSIO routine fits_hdr2str(). * * Each header "keyrecord" (formerly "card image") * consists of exactly 80 7-bit ASCII printing characters * in the range 0x20 to 0x7e (which excludes NUL, BS, * TAB, LF, FF and CR) especially noting that the * keyrecords are NOT null-terminated. * * nkeyrec int Number of keyrecords in header[]. * * nkeyids int Number of entries in keyids[]. * * Given and returned: * keyids struct fitskeyid [] * While all keywords are extracted from the header, * keyids[] provides a convienient way of indexing them. * The fitskeyid struct contains three members; * fitskeyid::name must be set by the user while * fitskeyid::count and fitskeyid::name are returned by * fitshdr(). All matched keywords will have their * fitskey::keyno member negated. * * Returned: * nreject int* Number of header keyrecords rejected for syntax * errors. * * keys struct fitskey** * Pointer to an array of nkeyrec fitskey structs * containing all keywords and keyvalues extracted from * the header. * * Memory for the array is allocated by fitshdr() and * this must be freed by the user by invoking free() on * the array. * * Function return value: * int Status return value: * 0: Success. * 1: Null fitskey pointer passed. * 2: Memory allocation failed. * 3: Fatal error returned by Flex parser. * * Notes: * 1: Keyword parsing is done in accordance with the syntax defined by * NOST 100-2.0, noting the following points in particular: * * a: Sect. 5.1.2.1 specifies that keywords be left-justified in columns * 1-8, blank-filled with no embedded spaces, composed only of the * ASCII characters ABCDEFGHJKLMNOPQRSTUVWXYZ0123456789-_ * * fitshdr() accepts any characters in columns 1-8 but flags keywords * that do not conform to standard syntax. * * b: Sect. 5.1.2.2 defines the "value indicator" as the characters "= " * occurring in columns 9 and 10. If these are absent then the * keyword has no value and columns 9-80 may contain any ASCII text * (but see note 2 for CONTINUE keyrecords). This is copied to the * comment member of the fitskey struct. * * c: Sect. 5.1.2.3 states that a keyword may have a null (undefined) * value if the value/comment field, columns 11-80, consists entirely * of spaces, possibly followed by a comment. * * d: Sect. 5.1.1 states that trailing blanks in a string keyvalue are * not significant and the parser always removes them. A string * containing nothing but blanks will be replaced with a single * blank. * * Sect. 5.2.1 also states that a quote character (') in a string * value is to be represented by two successive quote characters and * the parser removes the repeated quote. * * e: The parser recognizes free-format character (NOST 100-2.0, * Sect. 5.2.1), integer (Sect. 5.2.3), and floating-point values * (Sect. 5.2.4) for all keywords. * * f: Sect. 5.2.3 offers no comment on the size of an integer keyvalue * except indirectly in limiting it to 70 digits. The parser will * translates an integer keyvalue to a 32-bit signed integer if it * lies in the range -2147483648 to +2147483647, otherwise it * interprets it as a 64-bit signed integer if possible, or else a * "very long" integer (see fitskey::type). * * g: END not followed by 77 blanks is not considered to be a legitimate * end keyrecord. * * 2: The parser supports a generalization of the OGIP Long String Keyvalue * Convention (v1.0) whereby strings may be continued onto successive * header keyrecords. A keyrecord contains a segment of a continued * string if and only if * * a: it contains the pseudo-keyword CONTINUE, * * b: columns 9 and 10 are both blank, * * c: columns 11 to 80 contain what would be considered a valid string * keyvalue, including optional keycomment, if column 9 had contained * '=', * * d: the previous keyrecord contained either a valid string keyvalue or * a valid CONTINUE keyrecord. * * If any of these conditions is violated, the keyrecord is considered in * isolation. * * Syntax errors in keycomments in a continued string are treated more * permissively than usual; the '/' delimiter may be omitted provided that * parsing of the string keyvalue is not compromised. However, the * FITSHDR_COMMENT status bit will be set for the keyrecord (see * fitskey::status). * * As for normal strings, trailing blanks in a continued string are not * significant. * * In the OGIP convention "the '&' character is used as the last non-blank * character of the string to indicate that the string is (probably) * continued on the following keyword". This additional syntax is not * required by fitshdr(), but if '&' does occur as the last non-blank * character of a continued string keyvalue then it will be removed, along * with any trailing blanks. However, blanks that occur before the '&' * will be preserved. * * * fitskeyid struct - Keyword indexing * ----------------------------------- * fitshdr() uses the fitskeyid struct to return indexing information for * specified keywords. The struct contains three members, the first of which, * fitskeyid::name, must be set by the user with the remainder returned by * fitshdr(). * * char name[12]: * (Given) Name of the required keyword. This is to be set by the user; * the '.' character may be used for wildcarding. Trailing blanks will be * replaced with nulls. * * int count: * (Returned) The number of matches found for the keyword. * * int idx[2]: * (Returned) Indices into keys[], the array of fitskey structs returned by * fitshdr(). Note that these are 0-relative array indices, not keyrecord * numbers. * * If the keyword is found in the header the first index will be set to the * array index of its first occurrence, otherwise it will be set to -1. * * If multiples of the keyword are found, the second index will be set to * the array index of its last occurrence, otherwise it will be set to -1. * * * fitskey struct - Keyword/value information * ------------------------------------------ * fitshdr() returns an array of fitskey structs, each of which contains the * result of parsing one FITS header keyrecord. All members of the fitskey * struct are returned by fitshdr(), none are given by the user. * * int keyno * (Returned) Keyrecord number (1-relative) in the array passed as input to * fitshdr(). This will be negated if the keyword matched any specified in * the keyids[] index. * * int keyid * (Returned) Index into the first entry in keyids[] with which the * keyrecord matches, else -1. * * int status * (Returned) Status flag bit-vector for the header keyrecord employing the * following bit masks defined as preprocessor macros: * * - FITSHDR_KEYWORD: Illegal keyword syntax. * - FITSHDR_KEYVALUE: Illegal keyvalue syntax. * - FITSHDR_COMMENT: Illegal keycomment syntax. * - FITSHDR_KEYREC: Illegal keyrecord, e.g. an END keyrecord with * trailing text. * - FITSHDR_TRAILER: Keyrecord following a valid END keyrecord. * * The header keyrecord is syntactically correct if no bits are set. * * char keyword[12] * (Returned) Keyword name, null-filled for keywords of less than eight * characters (trailing blanks replaced by nulls). * * Use * = sprintf(dst, "%.8s", keyword) * * to copy it to a character array with null-termination, or * = sprintf(dst, "%8.8s", keyword) * * to blank-fill to eight characters followed by null-termination. * * int type * (Returned) Keyvalue data type: * - 0: No keyvalue. * - 1: Logical, represented as int. * - 2: 32-bit signed integer. * - 3: 64-bit signed integer (see below). * - 4: Very long integer (see below). * - 5: Floating point (stored as double). * - 6: Integer complex (stored as double[2]). * - 7: Floating point complex (stored as double[2]). * - 8: String. * - 8+10*n: Continued string (described below and in fitshdr() note 2). * * A negative type indicates that a syntax error was encountered when * attempting to parse a keyvalue of the particular type. * * Comments on particular data types: * - 64-bit signed integers lie in the range * = (-9223372036854775808 <= int64 < -2147483648) || = (+2147483647 < int64 <= +9223372036854775807) * * A native 64-bit data type may be defined via preprocessor macro * WCSLIB_INT64 defined in wcsconfig.h, e.g. as 'long long int'; this * will be typedef'd to 'int64' here. If WCSLIB_INT64 is not set, then * int64 is typedef'd to int[3] instead and fitskey::keyvalue is to be * computed as * = ((keyvalue.k[2]) * 1000000000 + = keyvalue.k[1]) * 1000000000 + = keyvalue.k[0] * * and may reported via * = if (keyvalue.k[2]) { = printf("%d%09d%09d", keyvalue.k[2], abs(keyvalue.k[1]), = abs(keyvalue.k[0])); = } else { = printf("%d%09d", keyvalue.k[1], abs(keyvalue.k[0])); = } * * where keyvalue.k[0] and keyvalue.k[1] range from -999999999 to * +999999999. * * - Very long integers, up to 70 decimal digits in length, are encoded * in keyvalue.l as an array of int[8], each of which stores 9 decimal * digits. fitskey::keyvalue is to be computed as * = (((((((keyvalue.l[7]) * 1000000000 + = keyvalue.l[6]) * 1000000000 + = keyvalue.l[5]) * 1000000000 + = keyvalue.l[4]) * 1000000000 + = keyvalue.l[3]) * 1000000000 + = keyvalue.l[2]) * 1000000000 + = keyvalue.l[1]) * 1000000000 + = keyvalue.l[0] * * - Continued strings are not reconstructed, they remain split over * successive fitskey structs in the keys[] array returned by * fitshdr(). fitskey::keyvalue data type, 8 + 10n, indicates the * segment number, n, in the continuation. * * int padding * (An unused variable inserted for alignment purposes only.) * * union keyvalue * (Returned) A union comprised of * * - fitskey::i, * - fitskey::k, * - fitskey::l, * - fitskey::f, * - fitskey::c, * - fitskey::s, * * used by the fitskey struct to contain the value associated with a * keyword. * * int i * (Returned) Logical (fitskey::type == 1) and 32-bit signed integer * (fitskey::type == 2) data types in the fitskey::keyvalue union. * * int64 k * (Returned) 64-bit signed integer (fitskey::type == 3) data type in the * fitskey::keyvalue union. * * int l[8] * (Returned) Very long integer (fitskey::type == 4) data type in the * fitskey::keyvalue union. * * double f * (Returned) Floating point (fitskey::type == 5) data type in the * fitskey::keyvalue union. * * double c[2] * (Returned) Integer and floating point complex (fitskey::type == 6 || 7) * data types in the fitskey::keyvalue union. * * char s[72] * (Returned) Null-terminated string (fitskey::type == 8) data type in the * fitskey::keyvalue union. * * int ulen * (Returned) Where a keycomment contains a units string in the standard * form, e.g. [m/s], the ulen member indicates its length, inclusive of * square brackets. Otherwise ulen is zero. * * char comment[84] * (Returned) Keycomment, i.e. comment associated with the keyword or, for * keyrecords rejected because of syntax errors, the compete keyrecord * itself with null-termination. * * Comments are null-terminated with trailing spaces removed. Leading * spaces are also removed from keycomments (i.e. those immediately * following the '/' character), but not from COMMENT or HISTORY keyrecords * or keyrecords without a value indicator ("= " in columns 9-80). * * * Global variable: const char *fitshdr_errmsg[] - Status return messages * ---------------------------------------------------------------------- * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_FITSHDR #define WCSLIB_FITSHDR #include "wcsconfig.h" #ifdef __cplusplus extern "C" { #endif #define FITSHDR_KEYWORD 0x01 #define FITSHDR_KEYVALUE 0x02 #define FITSHDR_COMMENT 0x04 #define FITSHDR_KEYREC 0x08 #define FITSHDR_CARD 0x08 /* Alias for backwards compatibility. */ #define FITSHDR_TRAILER 0x10 extern const char *fitshdr_errmsg[]; #ifdef WCSLIB_INT64 typedef WCSLIB_INT64 int64; #else typedef int int64[3]; #endif /* Struct used for indexing the keywords. */ struct fitskeyid { char name[12]; /* Keyword name, null-terminated. */ int count; /* Number of occurrences of keyword. */ int idx[2]; /* Indices into fitskey array. */ }; /* Size of the fitskeyid struct in int units, used by the Fortran wrappers. */ #define KEYIDLEN (sizeof(struct fitskeyid)/sizeof(int)) /* Struct used for storing FITS keywords. */ struct fitskey { int keyno; /* Header keyrecord sequence number (1-rel).*/ int keyid; /* Index into fitskeyid[]. */ int status; /* Header keyrecord status bit flags. */ char keyword[12]; /* Keyword name, null-filled. */ int type; /* Keyvalue type (see above). */ int padding; /* (Dummy inserted for alignment purposes.) */ union { int i; /* 32-bit integer and logical values. */ int64 k; /* 64-bit integer values. */ int l[8]; /* Very long signed integer values. */ double f; /* Floating point values. */ double c[2]; /* Complex values. */ char s[72]; /* String values, null-terminated. */ } keyvalue; /* Keyvalue. */ int ulen; /* Length of units string. */ char comment[84]; /* Comment (or keyrecord), null-terminated. */ }; /* Size of the fitskey struct in int units, used by the Fortran wrappers. */ #define KEYLEN (sizeof(struct fitskey)/sizeof(int)) int fitshdr(const char header[], int nkeyrec, int nkeyids, struct fitskeyid keyids[], int *nreject, struct fitskey **keys); #ifdef __cplusplus } #endif #endif /* WCSLIB_FITSHDR */ pywcs-1.12/wcslib/C/fitshdr.l0000644001153600020070000003052212310355626020135 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: fitshdr.l,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * fitshdr.l is a Flex description file containing a lexical scanner * definition for extracting keywords and keyvalues from a FITS header. * * It requires Flex v2.5.4 or later. * * Refer to fitshdr.h for a description of the user interface and operating * notes. * *===========================================================================*/ /* Options. */ %option full %option never-interactive %option nounput %option noyywrap %option outfile="fitshdr.c" %option prefix="fitshdr" /* Keywords. */ KEYCHR [-_A-Z0-9] KW1 {KEYCHR}{1}" "{7} KW2 {KEYCHR}{2}" "{6} KW3 {KEYCHR}{3}" "{5} KW4 {KEYCHR}{4}" "{4} KW5 {KEYCHR}{5}" "{3} KW6 {KEYCHR}{6}" "{2} KW7 {KEYCHR}{7}" "{1} KW8 {KEYCHR}{8} KEYWORD ({KW1}|{KW2}|{KW3}|{KW4}|{KW5}|{KW6}|{KW7}|{KW8}) /* Keyvalue data types. */ LOGICAL [TF] INT32 [+-]?0*[0-9]{1,9} INT64 [+-]?0*[0-9]{10,18} INTVL [+-]?0*[0-9]{19,} INTEGER [+-]?[0-9]+ FLOAT [+-]?([0-9]+\.?[0-9]*|\.[0-9]+)([eE][+-]?[0-9]+)? ICOMPLX \(" "*{INTEGER}" "*," "*{INTEGER}" "*\) FCOMPLX \(" "*{FLOAT}" "*," "*{FLOAT}" "*\) STRING '([^']|'')*' /* Characters forming standard unit strings (jwBIQX are not used). */ UNITSTR \[[-+*/^(). 0-9a-zA-Z]+\] /* Exclusive start states. */ %x VALUE INLINE UNITS COMMENT ERROR FLUSH %{ #include #include #include #include #include #include "fitshdr.h" #define YY_DECL int fitshdr(const char header[], int nkeyrec, int nkeyids, \ struct fitskeyid keyids[], int *nreject, \ struct fitskey **keys) #define YY_INPUT(inbuff, count, bufsize) \ { \ if (fitshdr_nkeyrec) { \ strncpy(inbuff, fitshdr_hdr, 80); \ inbuff[80] = '\n'; \ fitshdr_hdr += 80; \ fitshdr_nkeyrec--; \ count = 81; \ } else { \ count = YY_NULL; \ } \ } /* These global variables are required by YY_INPUT. */ const char *fitshdr_hdr; int fitshdr_nkeyrec; /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf fitshdr_abort_jmp_env; #define exit(status) longjmp(fitshdr_abort_jmp_env, status) /* Map status return value to message. */ const char *fitshdr_errmsg[] = { "Success", "Null fitskey pointer-pointer passed", "Memory allocation failed", "Fatal error returned by Flex parser"}; %} %% char *cptr, ctmp[72]; int blank, continuation, end, j, k, keyno; double dtmp; struct fitskey *kptr; struct fitskeyid *iptr; void nullfill(char cptr[], int len); int yylex_destroy(void); fitshdr_hdr = header; fitshdr_nkeyrec = nkeyrec; *nreject = 0; keyno = 0; if (keys == 0x0) { return 1; } /* Allocate memory for the required number of fitskey structs. */ /* Recall that calloc() initializes allocated memory to zero. */ if (!(kptr = *keys = calloc(nkeyrec, sizeof(struct fitskey)))) { return 2; } /* Initialize keyids[]. */ iptr = keyids; for (j = 0; j < nkeyids; j++, iptr++) { iptr->count = 0; iptr->idx[0] = -1; iptr->idx[1] = -1; } blank = 0; continuation = 0; end = 0; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(fitshdr_abort_jmp_env)) { return 3; } BEGIN(INITIAL); ^" "{80} { /* A completely blank keyrecord. */ strncpy(kptr->keyword, yytext, 8); yyless(0); blank = 1; BEGIN(COMMENT); } ^(COMMENT|HISTORY|" "{8}) { strncpy(kptr->keyword, yytext, 8); BEGIN(COMMENT); } ^END" "{77} { strncpy(kptr->keyword, yytext, 8); end = 1; BEGIN(FLUSH); } ^END" "{5}=" "+ { /* Illegal END keyrecord. */ strncpy(kptr->keyword, yytext, 8); kptr->status |= FITSHDR_KEYREC; BEGIN(VALUE); } ^END" "{5} { /* Illegal END keyrecord. */ strncpy(kptr->keyword, yytext, 8); kptr->status |= FITSHDR_KEYREC; BEGIN(COMMENT); } ^{KEYWORD}=" "+ { strncpy(kptr->keyword, yytext, 8); BEGIN(VALUE); } ^CONTINUE" "+{STRING} { /* Continued string keyvalue. */ strncpy(kptr->keyword, yytext, 8); if (keyno > 0 && (kptr-1)->type%10 == 8) { /* Put back the string keyvalue. */ for (k = 10; yytext[k] != '\''; k++); yyless(k); continuation = 1; BEGIN(VALUE); } else { /* Not a valid continuation. */ yyless(8); BEGIN(COMMENT); } } ^{KEYWORD} { /* Keyword without value. */ strncpy(kptr->keyword, yytext, 8); BEGIN(COMMENT); } ^.{8}=" "+ { /* Illegal keyword, carry on regardless. */ strncpy(kptr->keyword, yytext, 8); kptr->status |= FITSHDR_KEYWORD; BEGIN(VALUE); } ^.{8} { /* Illegal keyword, carry on regardless. */ strncpy(kptr->keyword, yytext, 8); kptr->status |= FITSHDR_KEYWORD; BEGIN(COMMENT); } " "*/\/ { /* Null keyvalue. */ BEGIN(INLINE); } {LOGICAL} { /* Logical keyvalue. */ kptr->type = 1; kptr->keyvalue.i = (*yytext == 'T'); BEGIN(INLINE); } {INT32} { /* 32-bit signed integer keyvalue. */ kptr->type = 2; if (sscanf(yytext, "%d", &(kptr->keyvalue.i)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } {INT64} { /* 64-bit signed integer keyvalue (up to 18 digits). */ if (sscanf(yytext, "%lf", &dtmp) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } else if (INT_MIN <= dtmp && dtmp <= INT_MAX) { /* Can be accomodated as a 32-bit signed integer. */ kptr->type = 2; if (sscanf(yytext, "%d", &(kptr->keyvalue.i)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } } else { /* 64-bit signed integer. */ kptr->type = 3; #ifdef WCSLIB_INT64 /* Native 64-bit integer is available. */ if (sscanf(yytext, "%lld", &(kptr->keyvalue.k)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } #else /* 64-bit integer (up to 18 digits) implemented as int[3]. */ kptr->keyvalue.k[2] = 0; sprintf(ctmp, "%%%dd%%9d", yyleng-9); if (sscanf(yytext, ctmp, kptr->keyvalue.k+1, kptr->keyvalue.k) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } else if (*yytext == '-') { kptr->keyvalue.k[0] *= -1; } #endif } BEGIN(INLINE); } {INTVL} { /* Very long integer keyvalue (and 19-digit int64). */ kptr->type = 4; strcpy(ctmp, yytext); k = yyleng; for (j = 0; j < 8; j++) { /* Read it backwards. */ k -= 9; if (k < 0) k = 0; if (sscanf(ctmp+k, "%d", kptr->keyvalue.l+j) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } if (*yytext == '-') { kptr->keyvalue.l[j] = -abs(kptr->keyvalue.l[j]); } if (k == 0) break; ctmp[k] = '\0'; } /* Can it be accomodated as a 64-bit signed integer? */ if (j == 2 && abs(kptr->keyvalue.l[2]) <= 9 && abs(kptr->keyvalue.l[1]) <= 223372036 && kptr->keyvalue.l[0] <= 854775807 && kptr->keyvalue.l[0] >= -854775808) { kptr->type = 3; #ifdef WCSLIB_INT64 /* Native 64-bit integer is available. */ kptr->keyvalue.l[2] = 0; if (sscanf(yytext, "%lld", &(kptr->keyvalue.k)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } #endif } BEGIN(INLINE); } {FLOAT} { /* Float keyvalue. */ kptr->type = 5; if (sscanf(yytext, "%lf", &(kptr->keyvalue.f)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } {ICOMPLX} { /* Integer complex keyvalue. */ kptr->type = 6; if (sscanf(yytext, "(%lf,%lf)", kptr->keyvalue.c, kptr->keyvalue.c+1) < 2) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } {FCOMPLX} { /* Floating point complex keyvalue. */ kptr->type = 7; if (sscanf(yytext, "(%lf,%lf)", kptr->keyvalue.c, kptr->keyvalue.c+1) < 2) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } {STRING} { /* String keyvalue. */ kptr->type = 8; cptr = kptr->keyvalue.s; strcpy(cptr, yytext+1); /* Squeeze out repeated quotes. */ k = 0; for (j = 0; j < 72; j++) { if (k < j) { cptr[k] = cptr[j]; } if (cptr[j] == '\0') { if (k) cptr[k-1] = '\0'; break; } else if (cptr[j] == '\'' && cptr[j+1] == '\'') { j++; } k++; } if (*cptr) { /* Retain the initial blank in all-blank strings. */ nullfill(cptr+1, 71); } else { nullfill(cptr, 72); } BEGIN(INLINE); } . { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } " "*$ { BEGIN(FLUSH); } " "*\/" "*$ { BEGIN(FLUSH); } " "*\/" "* { BEGIN(UNITS); } " " { kptr->status |= FITSHDR_COMMENT; BEGIN(ERROR); } . { /* Keyvalue parsing must now also be suspect. */ kptr->status |= FITSHDR_COMMENT; kptr->type = 0; BEGIN(ERROR); } {UNITSTR} { kptr->ulen = yyleng; yymore(); BEGIN(COMMENT); } . { yymore(); BEGIN(COMMENT); } .* { strcpy(kptr->comment, yytext); nullfill(kptr->comment, 84); BEGIN(FLUSH); } .* { if (!continuation) kptr->type = -abs(kptr->type); sprintf(kptr->comment, "%.80s", fitshdr_hdr-80); kptr->comment[80] = '\0'; nullfill(kptr->comment+80, 4); BEGIN(FLUSH); } .*\n { /* Discard the rest of the input line. */ kptr->keyno = ++keyno; /* Null-fill the keyword. */ kptr->keyword[8] = '\0'; nullfill(kptr->keyword, 12); /* Do indexing. */ iptr = keyids; kptr->keyid = -1; for (j = 0; j < nkeyids; j++, iptr++) { cptr = iptr->name; cptr[8] = '\0'; nullfill(cptr, 12); for (k = 0; k < 8; k++, cptr++) { if (*cptr != '.' && *cptr != kptr->keyword[k]) break; } if (k == 8) { /* Found a match. */ iptr->count++; if (iptr->idx[0] == -1) { iptr->idx[0] = keyno-1; } else { iptr->idx[1] = keyno-1; } kptr->keyno = -abs(kptr->keyno); if (kptr->keyid < 0) kptr->keyid = j; } } /* Deal with continued strings. */ if (continuation) { /* Tidy up the previous string keyvalue. */ if ((kptr-1)->type == 8) (kptr-1)->type += 10; cptr = (kptr-1)->keyvalue.s; if (cptr[strlen(cptr)-1] == '&') cptr[strlen(cptr)-1] = '\0'; kptr->type = (kptr-1)->type + 10; } /* Check for keyrecords following the END keyrecord. */ if (end && (end++ > 1) && !blank) { kptr->status |= FITSHDR_TRAILER; } if (kptr->status) (*nreject)++; kptr++; blank = 0; continuation = 0; BEGIN(INITIAL); } <> { /* End-of-input. */ yylex_destroy(); return 0; } %% /*--------------------------------------------------------------------------*/ void nullfill(char cptr[], int len) { int j, k; /* Null-fill the string. */ for (j = 0; j < len; j++) { if (cptr[j] == '\0') { for (k = j+1; k < len; k++) { cptr[k] = '\0'; } break; } } for (k = j-1; k >= 0; k--) { if (cptr[k] != ' ') break; cptr[k] = '\0'; } return; } pywcs-1.12/wcslib/C/flexed/0000755001153600020070000000000012310355732017560 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/C/flexed/fitshdr.c0000644001153600020070000201213512310355626021375 0ustar cslocumSTSCI\science00000000000000#line 2 "fitshdr.c" #line 4 "fitshdr.c" #define YY_INT_ALIGNED short int /* A lexical scanner generated by flex */ #define yy_create_buffer fitshdr_create_buffer #define yy_delete_buffer fitshdr_delete_buffer #define yy_flex_debug fitshdr_flex_debug #define yy_init_buffer fitshdr_init_buffer #define yy_flush_buffer fitshdr_flush_buffer #define yy_load_buffer_state fitshdr_load_buffer_state #define yy_switch_to_buffer fitshdr_switch_to_buffer #define yyin fitshdrin #define yyleng fitshdrleng #define yylex fitshdrlex #define yylineno fitshdrlineno #define yyout fitshdrout #define yyrestart fitshdrrestart #define yytext fitshdrtext #define yywrap fitshdrwrap #define yyalloc fitshdralloc #define yyrealloc fitshdrrealloc #define yyfree fitshdrfree #define FLEX_SCANNER #define YY_FLEX_MAJOR_VERSION 2 #define YY_FLEX_MINOR_VERSION 5 #define YY_FLEX_SUBMINOR_VERSION 35 #if YY_FLEX_SUBMINOR_VERSION > 0 #define FLEX_BETA #endif /* First, we deal with platform-specific or compiler-specific issues. */ /* begin standard C headers. */ #include #include #include #include /* end standard C headers. */ /* flex integer type definitions */ #ifndef FLEXINT_H #define FLEXINT_H /* C99 systems have . Non-C99 systems may or may not. */ #if defined (__STDC_VERSION__) && __STDC_VERSION__ >= 199901L /* C99 says to define __STDC_LIMIT_MACROS before including stdint.h, * if you want the limit (max/min) macros for int types. */ #ifndef __STDC_LIMIT_MACROS #define __STDC_LIMIT_MACROS 1 #endif #include typedef int8_t flex_int8_t; typedef uint8_t flex_uint8_t; typedef int16_t flex_int16_t; typedef uint16_t flex_uint16_t; typedef int32_t flex_int32_t; typedef uint32_t flex_uint32_t; #else typedef signed char flex_int8_t; typedef short int flex_int16_t; typedef int flex_int32_t; typedef unsigned char flex_uint8_t; typedef unsigned short int flex_uint16_t; typedef unsigned int flex_uint32_t; /* Limits of integral types. */ #ifndef INT8_MIN #define INT8_MIN (-128) #endif #ifndef INT16_MIN #define INT16_MIN (-32767-1) #endif #ifndef INT32_MIN #define INT32_MIN (-2147483647-1) #endif #ifndef INT8_MAX #define INT8_MAX (127) #endif #ifndef INT16_MAX #define INT16_MAX (32767) #endif #ifndef INT32_MAX #define INT32_MAX (2147483647) #endif #ifndef UINT8_MAX #define UINT8_MAX (255U) #endif #ifndef UINT16_MAX #define UINT16_MAX (65535U) #endif #ifndef UINT32_MAX #define UINT32_MAX (4294967295U) #endif #endif /* ! C99 */ #endif /* ! FLEXINT_H */ #ifdef __cplusplus /* The "const" storage-class-modifier is valid. */ #define YY_USE_CONST #else /* ! __cplusplus */ /* C99 requires __STDC__ to be defined as 1. */ #if defined (__STDC__) #define YY_USE_CONST #endif /* defined (__STDC__) */ #endif /* ! __cplusplus */ #ifdef YY_USE_CONST #define yyconst const #else #define yyconst #endif /* Returned upon end-of-file. */ #define YY_NULL 0 /* Promotes a possibly negative, possibly signed char to an unsigned * integer for use as an array index. If the signed char is negative, * we want to instead treat it as an 8-bit unsigned char, hence the * double cast. */ #define YY_SC_TO_UI(c) ((unsigned int) (unsigned char) c) /* Enter a start condition. This macro really ought to take a parameter, * but we do it the disgusting crufty way forced on us by the ()-less * definition of BEGIN. */ #define BEGIN (yy_start) = 1 + 2 * /* Translate the current start state into a value that can be later handed * to BEGIN to return to the state. The YYSTATE alias is for lex * compatibility. */ #define YY_START (((yy_start) - 1) / 2) #define YYSTATE YY_START /* Action number for EOF rule of a given start state. */ #define YY_STATE_EOF(state) (YY_END_OF_BUFFER + state + 1) /* Special action meaning "start processing a new file". */ #define YY_NEW_FILE fitshdrrestart(fitshdrin ) #define YY_END_OF_BUFFER_CHAR 0 /* Size of default input buffer. */ #ifndef YY_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k. * Moreover, YY_BUF_SIZE is 2*YY_READ_BUF_SIZE in the general case. * Ditto for the __ia64__ case accordingly. */ #define YY_BUF_SIZE 32768 #else #define YY_BUF_SIZE 16384 #endif /* __ia64__ */ #endif /* The state buf must be large enough to hold one state per character in the main buffer. */ #define YY_STATE_BUF_SIZE ((YY_BUF_SIZE + 2) * sizeof(yy_state_type)) #ifndef YY_TYPEDEF_YY_BUFFER_STATE #define YY_TYPEDEF_YY_BUFFER_STATE typedef struct yy_buffer_state *YY_BUFFER_STATE; #endif extern int fitshdrleng; extern FILE *fitshdrin, *fitshdrout; #define EOB_ACT_CONTINUE_SCAN 0 #define EOB_ACT_END_OF_FILE 1 #define EOB_ACT_LAST_MATCH 2 #define YY_LESS_LINENO(n) /* Return all but the first "n" matched characters back to the input stream. */ #define yyless(n) \ do \ { \ /* Undo effects of setting up fitshdrtext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ *yy_cp = (yy_hold_char); \ YY_RESTORE_YY_MORE_OFFSET \ (yy_c_buf_p) = yy_cp = yy_bp + yyless_macro_arg - YY_MORE_ADJ; \ YY_DO_BEFORE_ACTION; /* set up fitshdrtext again */ \ } \ while ( 0 ) #define unput(c) yyunput( c, (yytext_ptr) ) #ifndef YY_TYPEDEF_YY_SIZE_T #define YY_TYPEDEF_YY_SIZE_T typedef size_t yy_size_t; #endif #ifndef YY_STRUCT_YY_BUFFER_STATE #define YY_STRUCT_YY_BUFFER_STATE struct yy_buffer_state { FILE *yy_input_file; char *yy_ch_buf; /* input buffer */ char *yy_buf_pos; /* current position in input buffer */ /* Size of input buffer in bytes, not including room for EOB * characters. */ yy_size_t yy_buf_size; /* Number of characters read into yy_ch_buf, not including EOB * characters. */ int yy_n_chars; /* Whether we "own" the buffer - i.e., we know we created it, * and can realloc() it to grow it, and should free() it to * delete it. */ int yy_is_our_buffer; /* Whether this is an "interactive" input source; if so, and * if we're using stdio for input, then we want to use getc() * instead of fread(), to make sure we stop fetching input after * each newline. */ int yy_is_interactive; /* Whether we're considered to be at the beginning of a line. * If so, '^' rules will be active on the next match, otherwise * not. */ int yy_at_bol; int yy_bs_lineno; /**< The line count. */ int yy_bs_column; /**< The column count. */ /* Whether to try to fill the input buffer when we reach the * end of it. */ int yy_fill_buffer; int yy_buffer_status; #define YY_BUFFER_NEW 0 #define YY_BUFFER_NORMAL 1 /* When an EOF's been seen but there's still some text to process * then we mark the buffer as YY_EOF_PENDING, to indicate that we * shouldn't try reading from the input source any more. We might * still have a bunch of tokens to match, though, because of * possible backing-up. * * When we actually see the EOF, we change the status to "new" * (via fitshdrrestart()), so that the user can continue scanning by * just pointing fitshdrin at a new input file. */ #define YY_BUFFER_EOF_PENDING 2 }; #endif /* !YY_STRUCT_YY_BUFFER_STATE */ /* Stack of input buffers. */ static size_t yy_buffer_stack_top = 0; /**< index of top of stack. */ static size_t yy_buffer_stack_max = 0; /**< capacity of stack. */ static YY_BUFFER_STATE * yy_buffer_stack = 0; /**< Stack as an array. */ /* We provide macros for accessing buffer states in case in the * future we want to put the buffer states in a more general * "scanner state". * * Returns the top of the stack, or NULL. */ #define YY_CURRENT_BUFFER ( (yy_buffer_stack) \ ? (yy_buffer_stack)[(yy_buffer_stack_top)] \ : NULL) /* Same as previous macro, but useful when we know that the buffer stack is not * NULL or when we need an lvalue. For internal use only. */ #define YY_CURRENT_BUFFER_LVALUE (yy_buffer_stack)[(yy_buffer_stack_top)] /* yy_hold_char holds the character lost when fitshdrtext is formed. */ static char yy_hold_char; static int yy_n_chars; /* number of characters read into yy_ch_buf */ int fitshdrleng; /* Points to current character in buffer. */ static char *yy_c_buf_p = (char *) 0; static int yy_init = 0; /* whether we need to initialize */ static int yy_start = 0; /* start state number */ /* Flag which is used to allow fitshdrwrap()'s to do buffer switches * instead of setting up a fresh fitshdrin. A bit of a hack ... */ static int yy_did_buffer_switch_on_eof; void fitshdrrestart (FILE *input_file ); void fitshdr_switch_to_buffer (YY_BUFFER_STATE new_buffer ); YY_BUFFER_STATE fitshdr_create_buffer (FILE *file,int size ); void fitshdr_delete_buffer (YY_BUFFER_STATE b ); void fitshdr_flush_buffer (YY_BUFFER_STATE b ); void fitshdrpush_buffer_state (YY_BUFFER_STATE new_buffer ); void fitshdrpop_buffer_state (void ); static void fitshdrensure_buffer_stack (void ); static void fitshdr_load_buffer_state (void ); static void fitshdr_init_buffer (YY_BUFFER_STATE b,FILE *file ); #define YY_FLUSH_BUFFER fitshdr_flush_buffer(YY_CURRENT_BUFFER ) YY_BUFFER_STATE fitshdr_scan_buffer (char *base,yy_size_t size ); YY_BUFFER_STATE fitshdr_scan_string (yyconst char *yy_str ); YY_BUFFER_STATE fitshdr_scan_bytes (yyconst char *bytes,int len ); void *fitshdralloc (yy_size_t ); void *fitshdrrealloc (void *,yy_size_t ); void fitshdrfree (void * ); #define yy_new_buffer fitshdr_create_buffer #define yy_set_interactive(is_interactive) \ { \ if ( ! YY_CURRENT_BUFFER ){ \ fitshdrensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ fitshdr_create_buffer(fitshdrin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_is_interactive = is_interactive; \ } #define yy_set_bol(at_bol) \ { \ if ( ! YY_CURRENT_BUFFER ){\ fitshdrensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ fitshdr_create_buffer(fitshdrin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = at_bol; \ } #define YY_AT_BOL() (YY_CURRENT_BUFFER_LVALUE->yy_at_bol) /* Begin user sect3 */ #define fitshdrwrap(n) 1 #define YY_SKIP_YYWRAP typedef char YY_CHAR; FILE *fitshdrin = (FILE *) 0, *fitshdrout = (FILE *) 0; typedef int yy_state_type; extern int fitshdrlineno; int fitshdrlineno = 1; extern char *fitshdrtext; #define yytext_ptr fitshdrtext static yyconst flex_int16_t yy_nxt[][128] = { { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 }, { 15, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16, 16 }, { 15, 17, 17, 17, 17, 17, 17, 17, 17, 17, 16, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 18, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 19, 17, 17, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 17, 17, 17, 17, 17, 17, 17, 19, 19, 20, 19, 21, 19, 19, 22, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 19, 17, 17, 17, 17, 19, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17, 17 }, { 15, 23, 23, 23, 23, 23, 23, 23, 23, 23, 16, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 24, 23, 23, 23, 23, 23, 23, 25, 26, 23, 23, 27, 23, 27, 28, 29, 30, 31, 31, 31, 31, 31, 31, 31, 31, 31, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 32, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 32, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23 }, { 15, 23, 23, 23, 23, 23, 23, 23, 23, 23, 16, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 24, 23, 23, 23, 23, 23, 23, 25, 26, 23, 23, 27, 23, 27, 28, 29, 30, 31, 31, 31, 31, 31, 31, 31, 31, 31, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 32, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 32, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23, 23 }, { 15, 33, 33, 33, 33, 33, 33, 33, 33, 33, 34, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 35, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 36, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33 }, { 15, 33, 33, 33, 33, 33, 33, 33, 33, 33, 34, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 35, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 36, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33, 33 }, { 15, 37, 37, 37, 37, 37, 37, 37, 37, 37, 16, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 38, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37 }, { 15, 37, 37, 37, 37, 37, 37, 37, 37, 37, 16, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 38, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37, 37 }, { 15, 39, 39, 39, 39, 39, 39, 39, 39, 39, 16, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39 }, { 15, 39, 39, 39, 39, 39, 39, 39, 39, 39, 16, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39, 39 }, { 15, 40, 40, 40, 40, 40, 40, 40, 40, 40, 16, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40 }, { 15, 40, 40, 40, 40, 40, 40, 40, 40, 40, 16, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40, 40 }, { 15, 41, 41, 41, 41, 41, 41, 41, 41, 41, 42, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41 }, { 15, 41, 41, 41, 41, 41, 41, 41, 41, 41, 42, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41, 41 }, { -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15, -15 }, { 15, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, -16, 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-548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548, -548 }, { 15, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549, -549 }, { 15, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550, -550 }, } ; static yy_state_type yy_get_previous_state (void ); static yy_state_type yy_try_NUL_trans (yy_state_type current_state ); static int yy_get_next_buffer (void ); static void yy_fatal_error (yyconst char msg[] ); /* Done after the current pattern has been matched and before the * corresponding action - sets up fitshdrtext. */ #define YY_DO_BEFORE_ACTION \ (yytext_ptr) = yy_bp; \ (yytext_ptr) -= (yy_more_len); \ fitshdrleng = (size_t) (yy_cp - (yytext_ptr)); \ (yy_hold_char) = *yy_cp; \ *yy_cp = '\0'; \ (yy_c_buf_p) = yy_cp; #define YY_NUM_RULES 31 #define YY_END_OF_BUFFER 32 /* This struct is not used in this scanner, but its presence is necessary. */ struct yy_trans_info { flex_int32_t yy_verify; flex_int32_t yy_nxt; }; static yyconst flex_int16_t yy_accept[551] = { 0, 0, 0, 0, 0, 0, 0, 0, 0, 28, 28, 29, 29, 0, 0, 32, 31, 31, 31, 31, 31, 31, 31, 20, 20, 20, 20, 20, 20, 11, 13, 13, 12, 25, 21, 24, 23, 27, 27, 28, 29, 31, 30, 0, 0, 0, 0, 0, 0, 0, 0, 11, 0, 19, 0, 0, 0, 0, 0, 13, 13, 16, 16, 13, 13, 0, 13, 21, 0, 23, 22, 23, 0, 28, 29, 0, 30, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 16, 13, 13, 13, 0, 16, 13, 26, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 13, 13, 13, 13, 13, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 17, 0, 0, 0, 13, 13, 13, 13, 13, 13, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 18, 0, 0, 0, 0, 13, 13, 13, 13, 13, 13, 13, 0, 0, 0, 0, 0, 0, 0, 0, 0, 2, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 10, 2, 8, 8, 8, 5, 13, 13, 13, 13, 13, 13, 13, 13, 13, 0, 0, 0, 0, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 9, 0, 6, 0, 0, 4, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 0, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 0, 0, 7, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 14, 14, 14, 14, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 14, 14, 14, 14, 15, 0, 0, 13, 13, 13, 13, 13, 13, 13, 13, 13, 13, 14, 14, 14, 14, 14, 14, 14, 14, 14, 15, 15, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 3 } ; static yy_state_type yy_last_accepting_state; static char *yy_last_accepting_cpos; static yyconst yy_state_type yy_NUL_trans[551] = { 0, 16, 17, 23, 23, 33, 33, 37, 37, 39, 39, 40, 40, 41, 41, 0, 0, 43, 43, 43, 43, 43, 43, 0, 0, 52, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 73, 74, 75, 0, 77, 77, 77, 77, 77, 77, 77, 0, 0, 52, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 73, 74, 75, 0, 100, 100, 100, 100, 100, 100, 100, 100, 100, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 124, 124, 124, 124, 124, 124, 124, 124, 124, 124, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 150, 150, 150, 150, 150, 150, 150, 150, 150, 150, 150, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 175, 175, 175, 175, 175, 175, 175, 175, 175, 175, 175, 175, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 195, 195, 195, 195, 195, 195, 195, 195, 195, 195, 195, 195, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 259, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 259, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 } ; extern int fitshdr_flex_debug; int fitshdr_flex_debug = 0; /* The intent behind this definition is that it'll catch * any uses of REJECT which flex missed. */ #define REJECT reject_used_but_not_detected static int yy_more_flag = 0; static int yy_more_len = 0; #define yymore() ((yy_more_flag) = 1) #define YY_MORE_ADJ (yy_more_len) #define YY_RESTORE_YY_MORE_OFFSET char *fitshdrtext; #line 1 "fitshdr.l" /*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: fitshdr.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * fitshdr.l is a Flex description file containing a lexical scanner * definition for extracting keywords and keyvalues from a FITS header. * * It requires Flex v2.5.4 or later. * * Refer to fitshdr.h for a description of the user interface and operating * notes. * *===========================================================================*/ /* Options. */ /* Keywords. */ /* Keyvalue data types. */ /* Characters forming standard unit strings (jwBIQX are not used). */ /* Exclusive start states. */ #line 82 "fitshdr.l" #include #include #include #include #include #include "fitshdr.h" #define YY_DECL int fitshdr(const char header[], int nkeyrec, int nkeyids, \ struct fitskeyid keyids[], int *nreject, \ struct fitskey **keys) #define YY_INPUT(inbuff, count, bufsize) \ { \ if (fitshdr_nkeyrec) { \ strncpy(inbuff, fitshdr_hdr, 80); \ inbuff[80] = '\n'; \ fitshdr_hdr += 80; \ fitshdr_nkeyrec--; \ count = 81; \ } else { \ count = YY_NULL; \ } \ } /* These global variables are required by YY_INPUT. */ const char *fitshdr_hdr; int fitshdr_nkeyrec; /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf fitshdr_abort_jmp_env; #define exit(status) longjmp(fitshdr_abort_jmp_env, status) /* Map status return value to message. */ const char *fitshdr_errmsg[] = { "Success", "Null fitskey pointer-pointer passed", "Memory allocation failed", "Fatal error returned by Flex parser"}; #line 10174 "fitshdr.c" #define INITIAL 0 #define VALUE 1 #define INLINE 2 #define UNITS 3 #define COMMENT 4 #define ERROR 5 #define FLUSH 6 #ifndef YY_NO_UNISTD_H /* Special case for "unistd.h", since it is non-ANSI. We include it way * down here because we want the user's section 1 to have been scanned first. * The user has a chance to override it with an option. */ #include #endif #ifndef YY_EXTRA_TYPE #define YY_EXTRA_TYPE void * #endif static int yy_init_globals (void ); /* Accessor methods to globals. These are made visible to non-reentrant scanners for convenience. */ int fitshdrlex_destroy (void ); int fitshdrget_debug (void ); void fitshdrset_debug (int debug_flag ); YY_EXTRA_TYPE fitshdrget_extra (void ); void fitshdrset_extra (YY_EXTRA_TYPE user_defined ); FILE *fitshdrget_in (void ); void fitshdrset_in (FILE * in_str ); FILE *fitshdrget_out (void ); void fitshdrset_out (FILE * out_str ); int fitshdrget_leng (void ); char *fitshdrget_text (void ); int fitshdrget_lineno (void ); void fitshdrset_lineno (int line_number ); /* Macros after this point can all be overridden by user definitions in * section 1. */ #ifndef YY_SKIP_YYWRAP #ifdef __cplusplus extern "C" int fitshdrwrap (void ); #else extern int fitshdrwrap (void ); #endif #endif #ifndef yytext_ptr static void yy_flex_strncpy (char *,yyconst char *,int ); #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * ); #endif #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void ); #else static int input (void ); #endif #endif /* Amount of stuff to slurp up with each read. */ #ifndef YY_READ_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k */ #define YY_READ_BUF_SIZE 16384 #else #define YY_READ_BUF_SIZE 8192 #endif /* __ia64__ */ #endif /* Copy whatever the last rule matched to the standard output. */ #ifndef ECHO /* This used to be an fputs(), but since the string might contain NUL's, * we now use fwrite(). */ #define ECHO do { if (fwrite( fitshdrtext, fitshdrleng, 1, fitshdrout )) {} } while (0) #endif /* Gets input and stuffs it into "buf". number of characters read, or YY_NULL, * is returned in "result". */ #ifndef YY_INPUT #define YY_INPUT(buf,result,max_size) \ errno=0; \ while ( (result = read( fileno(fitshdrin), (char *) buf, max_size )) < 0 ) \ { \ if( errno != EINTR) \ { \ YY_FATAL_ERROR( "input in flex scanner failed" ); \ break; \ } \ errno=0; \ clearerr(fitshdrin); \ }\ \ #endif /* No semi-colon after return; correct usage is to write "yyterminate();" - * we don't want an extra ';' after the "return" because that will cause * some compilers to complain about unreachable statements. */ #ifndef yyterminate #define yyterminate() return YY_NULL #endif /* Number of entries by which start-condition stack grows. */ #ifndef YY_START_STACK_INCR #define YY_START_STACK_INCR 25 #endif /* Report a fatal error. */ #ifndef YY_FATAL_ERROR #define YY_FATAL_ERROR(msg) yy_fatal_error( msg ) #endif /* end tables serialization structures and prototypes */ /* Default declaration of generated scanner - a define so the user can * easily add parameters. */ #ifndef YY_DECL #define YY_DECL_IS_OURS 1 extern int fitshdrlex (void); #define YY_DECL int fitshdrlex (void) #endif /* !YY_DECL */ /* Code executed at the beginning of each rule, after fitshdrtext and fitshdrleng * have been set up. */ #ifndef YY_USER_ACTION #define YY_USER_ACTION #endif /* Code executed at the end of each rule. */ #ifndef YY_BREAK #define YY_BREAK break; #endif #define YY_RULE_SETUP \ if ( fitshdrleng > 0 ) \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = \ (fitshdrtext[fitshdrleng - 1] == '\n'); \ YY_USER_ACTION /** The main scanner function which does all the work. */ YY_DECL { register yy_state_type yy_current_state; register char *yy_cp, *yy_bp; register int yy_act; #line 124 "fitshdr.l" char *cptr, ctmp[72]; int blank, continuation, end, j, k, keyno; double dtmp; struct fitskey *kptr; struct fitskeyid *iptr; void nullfill(char cptr[], int len); int fitshdrlex_destroy(void); fitshdr_hdr = header; fitshdr_nkeyrec = nkeyrec; *nreject = 0; keyno = 0; if (keys == 0x0) { return 1; } /* Allocate memory for the required number of fitskey structs. */ /* Recall that calloc() initializes allocated memory to zero. */ if (!(kptr = *keys = calloc(nkeyrec, sizeof(struct fitskey)))) { return 2; } /* Initialize keyids[]. */ iptr = keyids; for (j = 0; j < nkeyids; j++, iptr++) { iptr->count = 0; iptr->idx[0] = -1; iptr->idx[1] = -1; } blank = 0; continuation = 0; end = 0; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(fitshdr_abort_jmp_env)) { return 3; } BEGIN(INITIAL); #line 10397 "fitshdr.c" if ( !(yy_init) ) { (yy_init) = 1; #ifdef YY_USER_INIT YY_USER_INIT; #endif if ( ! (yy_start) ) (yy_start) = 1; /* first start state */ if ( ! fitshdrin ) fitshdrin = stdin; if ( ! fitshdrout ) fitshdrout = stdout; if ( ! YY_CURRENT_BUFFER ) { fitshdrensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = fitshdr_create_buffer(fitshdrin,YY_BUF_SIZE ); } fitshdr_load_buffer_state( ); } while ( 1 ) /* loops until end-of-file is reached */ { (yy_more_len) = 0; if ( (yy_more_flag) ) { (yy_more_len) = (yy_c_buf_p) - (yytext_ptr); (yy_more_flag) = 0; } yy_cp = (yy_c_buf_p); /* Support of fitshdrtext. */ *yy_cp = (yy_hold_char); /* yy_bp points to the position in yy_ch_buf of the start of * the current run. */ yy_bp = yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); yy_match: while ( (yy_current_state = yy_nxt[yy_current_state][ YY_SC_TO_UI(*yy_cp) ]) > 0 ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } ++yy_cp; } yy_current_state = -yy_current_state; yy_find_action: yy_act = yy_accept[yy_current_state]; YY_DO_BEFORE_ACTION; do_action: /* This label is used only to access EOF actions. */ switch ( yy_act ) { /* beginning of action switch */ case 0: /* must back up */ /* undo the effects of YY_DO_BEFORE_ACTION */ *yy_cp = (yy_hold_char); yy_cp = (yy_last_accepting_cpos) + 1; yy_current_state = (yy_last_accepting_state); goto yy_find_action; case 1: YY_RULE_SETUP #line 168 "fitshdr.l" { /* A completely blank keyrecord. */ strncpy(kptr->keyword, fitshdrtext, 8); yyless(0); blank = 1; BEGIN(COMMENT); } YY_BREAK case 2: YY_RULE_SETUP #line 176 "fitshdr.l" { strncpy(kptr->keyword, fitshdrtext, 8); BEGIN(COMMENT); } YY_BREAK case 3: YY_RULE_SETUP #line 181 "fitshdr.l" { strncpy(kptr->keyword, fitshdrtext, 8); end = 1; BEGIN(FLUSH); } YY_BREAK case 4: YY_RULE_SETUP #line 187 "fitshdr.l" { /* Illegal END keyrecord. */ strncpy(kptr->keyword, fitshdrtext, 8); kptr->status |= FITSHDR_KEYREC; BEGIN(VALUE); } YY_BREAK case 5: YY_RULE_SETUP #line 194 "fitshdr.l" { /* Illegal END keyrecord. */ strncpy(kptr->keyword, fitshdrtext, 8); kptr->status |= FITSHDR_KEYREC; BEGIN(COMMENT); } YY_BREAK case 6: YY_RULE_SETUP #line 201 "fitshdr.l" { strncpy(kptr->keyword, fitshdrtext, 8); BEGIN(VALUE); } YY_BREAK case 7: /* rule 7 can match eol */ YY_RULE_SETUP #line 206 "fitshdr.l" { /* Continued string keyvalue. */ strncpy(kptr->keyword, fitshdrtext, 8); if (keyno > 0 && (kptr-1)->type%10 == 8) { /* Put back the string keyvalue. */ for (k = 10; fitshdrtext[k] != '\''; k++); yyless(k); continuation = 1; BEGIN(VALUE); } else { /* Not a valid continuation. */ yyless(8); BEGIN(COMMENT); } } YY_BREAK case 8: YY_RULE_SETUP #line 224 "fitshdr.l" { /* Keyword without value. */ strncpy(kptr->keyword, fitshdrtext, 8); BEGIN(COMMENT); } YY_BREAK case 9: YY_RULE_SETUP #line 230 "fitshdr.l" { /* Illegal keyword, carry on regardless. */ strncpy(kptr->keyword, fitshdrtext, 8); kptr->status |= FITSHDR_KEYWORD; BEGIN(VALUE); } YY_BREAK case 10: YY_RULE_SETUP #line 237 "fitshdr.l" { /* Illegal keyword, carry on regardless. */ strncpy(kptr->keyword, fitshdrtext, 8); kptr->status |= FITSHDR_KEYWORD; BEGIN(COMMENT); } YY_BREAK case 11: *yy_cp = (yy_hold_char); /* undo effects of setting up fitshdrtext */ (yy_c_buf_p) = yy_cp -= 1; YY_DO_BEFORE_ACTION; /* set up fitshdrtext again */ YY_RULE_SETUP #line 244 "fitshdr.l" { /* Null keyvalue. */ BEGIN(INLINE); } YY_BREAK case 12: YY_RULE_SETUP #line 249 "fitshdr.l" { /* Logical keyvalue. */ kptr->type = 1; kptr->keyvalue.i = (*fitshdrtext == 'T'); BEGIN(INLINE); } YY_BREAK case 13: YY_RULE_SETUP #line 256 "fitshdr.l" { /* 32-bit signed integer keyvalue. */ kptr->type = 2; if (sscanf(fitshdrtext, "%d", &(kptr->keyvalue.i)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } YY_BREAK case 14: YY_RULE_SETUP #line 267 "fitshdr.l" { /* 64-bit signed integer keyvalue (up to 18 digits). */ if (sscanf(fitshdrtext, "%lf", &dtmp) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } else if (INT_MIN <= dtmp && dtmp <= INT_MAX) { /* Can be accomodated as a 32-bit signed integer. */ kptr->type = 2; if (sscanf(fitshdrtext, "%d", &(kptr->keyvalue.i)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } } else { /* 64-bit signed integer. */ kptr->type = 3; #ifdef WCSLIB_INT64 /* Native 64-bit integer is available. */ if (sscanf(fitshdrtext, "%lld", &(kptr->keyvalue.k)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } #else /* 64-bit integer (up to 18 digits) implemented as int[3]. */ kptr->keyvalue.k[2] = 0; sprintf(ctmp, "%%%dd%%9d", fitshdrleng-9); if (sscanf(fitshdrtext, ctmp, kptr->keyvalue.k+1, kptr->keyvalue.k) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } else if (*fitshdrtext == '-') { kptr->keyvalue.k[0] *= -1; } #endif } BEGIN(INLINE); } YY_BREAK case 15: YY_RULE_SETUP #line 308 "fitshdr.l" { /* Very long integer keyvalue (and 19-digit int64). */ kptr->type = 4; strcpy(ctmp, fitshdrtext); k = fitshdrleng; for (j = 0; j < 8; j++) { /* Read it backwards. */ k -= 9; if (k < 0) k = 0; if (sscanf(ctmp+k, "%d", kptr->keyvalue.l+j) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } if (*fitshdrtext == '-') { kptr->keyvalue.l[j] = -abs(kptr->keyvalue.l[j]); } if (k == 0) break; ctmp[k] = '\0'; } /* Can it be accomodated as a 64-bit signed integer? */ if (j == 2 && abs(kptr->keyvalue.l[2]) <= 9 && abs(kptr->keyvalue.l[1]) <= 223372036 && kptr->keyvalue.l[0] <= 854775807 && kptr->keyvalue.l[0] >= -854775808) { kptr->type = 3; #ifdef WCSLIB_INT64 /* Native 64-bit integer is available. */ kptr->keyvalue.l[2] = 0; if (sscanf(fitshdrtext, "%lld", &(kptr->keyvalue.k)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } #endif } BEGIN(INLINE); } YY_BREAK case 16: YY_RULE_SETUP #line 349 "fitshdr.l" { /* Float keyvalue. */ kptr->type = 5; if (sscanf(fitshdrtext, "%lf", &(kptr->keyvalue.f)) < 1) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } YY_BREAK case 17: YY_RULE_SETUP #line 360 "fitshdr.l" { /* Integer complex keyvalue. */ kptr->type = 6; if (sscanf(fitshdrtext, "(%lf,%lf)", kptr->keyvalue.c, kptr->keyvalue.c+1) < 2) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } YY_BREAK case 18: YY_RULE_SETUP #line 372 "fitshdr.l" { /* Floating point complex keyvalue. */ kptr->type = 7; if (sscanf(fitshdrtext, "(%lf,%lf)", kptr->keyvalue.c, kptr->keyvalue.c+1) < 2) { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } BEGIN(INLINE); } YY_BREAK case 19: /* rule 19 can match eol */ YY_RULE_SETUP #line 384 "fitshdr.l" { /* String keyvalue. */ kptr->type = 8; cptr = kptr->keyvalue.s; strcpy(cptr, fitshdrtext+1); /* Squeeze out repeated quotes. */ k = 0; for (j = 0; j < 72; j++) { if (k < j) { cptr[k] = cptr[j]; } if (cptr[j] == '\0') { if (k) cptr[k-1] = '\0'; break; } else if (cptr[j] == '\'' && cptr[j+1] == '\'') { j++; } k++; } if (*cptr) { /* Retain the initial blank in all-blank strings. */ nullfill(cptr+1, 71); } else { nullfill(cptr, 72); } BEGIN(INLINE); } YY_BREAK case 20: YY_RULE_SETUP #line 417 "fitshdr.l" { kptr->status |= FITSHDR_KEYVALUE; BEGIN(ERROR); } YY_BREAK case 21: *yy_cp = (yy_hold_char); /* undo effects of setting up fitshdrtext */ (yy_c_buf_p) = yy_cp -= 1; YY_DO_BEFORE_ACTION; /* set up fitshdrtext again */ YY_RULE_SETUP #line 422 "fitshdr.l" { BEGIN(FLUSH); } YY_BREAK case 22: *yy_cp = (yy_hold_char); /* undo effects of setting up fitshdrtext */ (yy_c_buf_p) = yy_cp -= 1; YY_DO_BEFORE_ACTION; /* set up fitshdrtext again */ YY_RULE_SETUP #line 426 "fitshdr.l" { BEGIN(FLUSH); } YY_BREAK case 23: YY_RULE_SETUP #line 430 "fitshdr.l" { BEGIN(UNITS); } YY_BREAK case 24: YY_RULE_SETUP #line 434 "fitshdr.l" { kptr->status |= FITSHDR_COMMENT; BEGIN(ERROR); } YY_BREAK case 25: YY_RULE_SETUP #line 439 "fitshdr.l" { /* Keyvalue parsing must now also be suspect. */ kptr->status |= FITSHDR_COMMENT; kptr->type = 0; BEGIN(ERROR); } YY_BREAK case 26: YY_RULE_SETUP #line 446 "fitshdr.l" { kptr->ulen = fitshdrleng; yymore(); BEGIN(COMMENT); } YY_BREAK case 27: YY_RULE_SETUP #line 452 "fitshdr.l" { yymore(); BEGIN(COMMENT); } YY_BREAK case 28: YY_RULE_SETUP #line 457 "fitshdr.l" { strcpy(kptr->comment, fitshdrtext); nullfill(kptr->comment, 84); BEGIN(FLUSH); } YY_BREAK case 29: YY_RULE_SETUP #line 463 "fitshdr.l" { if (!continuation) kptr->type = -abs(kptr->type); sprintf(kptr->comment, "%.80s", fitshdr_hdr-80); kptr->comment[80] = '\0'; nullfill(kptr->comment+80, 4); BEGIN(FLUSH); } YY_BREAK case 30: /* rule 30 can match eol */ YY_RULE_SETUP #line 473 "fitshdr.l" { /* Discard the rest of the input line. */ kptr->keyno = ++keyno; /* Null-fill the keyword. */ kptr->keyword[8] = '\0'; nullfill(kptr->keyword, 12); /* Do indexing. */ iptr = keyids; kptr->keyid = -1; for (j = 0; j < nkeyids; j++, iptr++) { cptr = iptr->name; cptr[8] = '\0'; nullfill(cptr, 12); for (k = 0; k < 8; k++, cptr++) { if (*cptr != '.' && *cptr != kptr->keyword[k]) break; } if (k == 8) { /* Found a match. */ iptr->count++; if (iptr->idx[0] == -1) { iptr->idx[0] = keyno-1; } else { iptr->idx[1] = keyno-1; } kptr->keyno = -abs(kptr->keyno); if (kptr->keyid < 0) kptr->keyid = j; } } /* Deal with continued strings. */ if (continuation) { /* Tidy up the previous string keyvalue. */ if ((kptr-1)->type == 8) (kptr-1)->type += 10; cptr = (kptr-1)->keyvalue.s; if (cptr[strlen(cptr)-1] == '&') cptr[strlen(cptr)-1] = '\0'; kptr->type = (kptr-1)->type + 10; } /* Check for keyrecords following the END keyrecord. */ if (end && (end++ > 1) && !blank) { kptr->status |= FITSHDR_TRAILER; } if (kptr->status) (*nreject)++; kptr++; blank = 0; continuation = 0; BEGIN(INITIAL); } YY_BREAK case YY_STATE_EOF(INITIAL): case YY_STATE_EOF(VALUE): case YY_STATE_EOF(INLINE): case YY_STATE_EOF(UNITS): case YY_STATE_EOF(COMMENT): case YY_STATE_EOF(ERROR): case YY_STATE_EOF(FLUSH): #line 529 "fitshdr.l" { /* End-of-input. */ fitshdrlex_destroy(); return 0; } YY_BREAK case 31: YY_RULE_SETUP #line 535 "fitshdr.l" ECHO; YY_BREAK #line 10957 "fitshdr.c" case YY_END_OF_BUFFER: { /* Amount of text matched not including the EOB char. */ int yy_amount_of_matched_text = (int) (yy_cp - (yytext_ptr)) - 1; /* Undo the effects of YY_DO_BEFORE_ACTION. */ *yy_cp = (yy_hold_char); YY_RESTORE_YY_MORE_OFFSET if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_NEW ) { /* We're scanning a new file or input source. It's * possible that this happened because the user * just pointed fitshdrin at a new source and called * fitshdrlex(). If so, then we have to assure * consistency between YY_CURRENT_BUFFER and our * globals. Here is the right place to do so, because * this is the first action (other than possibly a * back-up) that will match for the new input source. */ (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; YY_CURRENT_BUFFER_LVALUE->yy_input_file = fitshdrin; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_NORMAL; } /* Note that here we test for yy_c_buf_p "<=" to the position * of the first EOB in the buffer, since yy_c_buf_p will * already have been incremented past the NUL character * (since all states make transitions on EOB to the * end-of-buffer state). Contrast this with the test * in input(). */ if ( (yy_c_buf_p) <= &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) { /* This was really a NUL. */ yy_state_type yy_next_state; (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); /* Okay, we're now positioned to make the NUL * transition. We couldn't have * yy_get_previous_state() go ahead and do it * for us because it doesn't know how to deal * with the possibility of jamming (and we don't * want to build jamming into it because then it * will run more slowly). */ yy_next_state = yy_try_NUL_trans( yy_current_state ); yy_bp = (yytext_ptr) + YY_MORE_ADJ; if ( yy_next_state ) { /* Consume the NUL. */ yy_cp = ++(yy_c_buf_p); yy_current_state = yy_next_state; goto yy_match; } else { yy_cp = (yy_c_buf_p); goto yy_find_action; } } else switch ( yy_get_next_buffer( ) ) { case EOB_ACT_END_OF_FILE: { (yy_did_buffer_switch_on_eof) = 0; if ( fitshdrwrap( ) ) { /* Note: because we've taken care in * yy_get_next_buffer() to have set up * fitshdrtext, we can now set up * yy_c_buf_p so that if some total * hoser (like flex itself) wants to * call the scanner after we return the * YY_NULL, it'll still work - another * YY_NULL will get returned. */ (yy_c_buf_p) = (yytext_ptr) + YY_MORE_ADJ; yy_act = YY_STATE_EOF(YY_START); goto do_action; } else { if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; } break; } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_match; case EOB_ACT_LAST_MATCH: (yy_c_buf_p) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)]; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_find_action; } break; } default: YY_FATAL_ERROR( "fatal flex scanner internal error--no action found" ); } /* end of action switch */ } /* end of scanning one token */ } /* end of fitshdrlex */ /* yy_get_next_buffer - try to read in a new buffer * * Returns a code representing an action: * EOB_ACT_LAST_MATCH - * EOB_ACT_CONTINUE_SCAN - continue scanning from current position * EOB_ACT_END_OF_FILE - end of file */ static int yy_get_next_buffer (void) { register char *dest = YY_CURRENT_BUFFER_LVALUE->yy_ch_buf; register char *source = (yytext_ptr); register int number_to_move, i; int ret_val; if ( (yy_c_buf_p) > &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] ) YY_FATAL_ERROR( "fatal flex scanner internal error--end of buffer missed" ); if ( YY_CURRENT_BUFFER_LVALUE->yy_fill_buffer == 0 ) { /* Don't try to fill the buffer, so this is an EOF. */ if ( (yy_c_buf_p) - (yytext_ptr) - YY_MORE_ADJ == 1 ) { /* We matched a single character, the EOB, so * treat this as a final EOF. */ return EOB_ACT_END_OF_FILE; } else { /* We matched some text prior to the EOB, first * process it. */ return EOB_ACT_LAST_MATCH; } } /* Try to read more data. */ /* First move last chars to start of buffer. */ number_to_move = (int) ((yy_c_buf_p) - (yytext_ptr)) - 1; for ( i = 0; i < number_to_move; ++i ) *(dest++) = *(source++); if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_EOF_PENDING ) /* don't do the read, it's not guaranteed to return an EOF, * just force an EOF */ YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = 0; else { int num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; while ( num_to_read <= 0 ) { /* Not enough room in the buffer - grow it. */ /* just a shorter name for the current buffer */ YY_BUFFER_STATE b = YY_CURRENT_BUFFER; int yy_c_buf_p_offset = (int) ((yy_c_buf_p) - b->yy_ch_buf); if ( b->yy_is_our_buffer ) { int new_size = b->yy_buf_size * 2; if ( new_size <= 0 ) b->yy_buf_size += b->yy_buf_size / 8; else b->yy_buf_size *= 2; b->yy_ch_buf = (char *) /* Include room in for 2 EOB chars. */ fitshdrrealloc((void *) b->yy_ch_buf,b->yy_buf_size + 2 ); } else /* Can't grow it, we don't own it. */ b->yy_ch_buf = 0; if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "fatal error - scanner input buffer overflow" ); (yy_c_buf_p) = &b->yy_ch_buf[yy_c_buf_p_offset]; num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; } if ( num_to_read > YY_READ_BUF_SIZE ) num_to_read = YY_READ_BUF_SIZE; /* Read in more data. */ YY_INPUT( (&YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]), (yy_n_chars), (size_t) num_to_read ); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } if ( (yy_n_chars) == 0 ) { if ( number_to_move == YY_MORE_ADJ ) { ret_val = EOB_ACT_END_OF_FILE; fitshdrrestart(fitshdrin ); } else { ret_val = EOB_ACT_LAST_MATCH; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_EOF_PENDING; } } else ret_val = EOB_ACT_CONTINUE_SCAN; if ((yy_size_t) ((yy_n_chars) + number_to_move) > YY_CURRENT_BUFFER_LVALUE->yy_buf_size) { /* Extend the array by 50%, plus the number we really need. */ yy_size_t new_size = (yy_n_chars) + number_to_move + ((yy_n_chars) >> 1); YY_CURRENT_BUFFER_LVALUE->yy_ch_buf = (char *) fitshdrrealloc((void *) YY_CURRENT_BUFFER_LVALUE->yy_ch_buf,new_size ); if ( ! YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in yy_get_next_buffer()" ); } (yy_n_chars) += number_to_move; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] = YY_END_OF_BUFFER_CHAR; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] = YY_END_OF_BUFFER_CHAR; (yytext_ptr) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[0]; return ret_val; } /* yy_get_previous_state - get the state just before the EOB char was reached */ static yy_state_type yy_get_previous_state (void) { register yy_state_type yy_current_state; register char *yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); for ( yy_cp = (yytext_ptr) + YY_MORE_ADJ; yy_cp < (yy_c_buf_p); ++yy_cp ) { if ( *yy_cp ) { yy_current_state = yy_nxt[yy_current_state][YY_SC_TO_UI(*yy_cp)]; } else yy_current_state = yy_NUL_trans[yy_current_state]; if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_current_state; } /* yy_try_NUL_trans - try to make a transition on the NUL character * * synopsis * next_state = yy_try_NUL_trans( current_state ); */ static yy_state_type yy_try_NUL_trans (yy_state_type yy_current_state ) { register int yy_is_jam; register char *yy_cp = (yy_c_buf_p); yy_current_state = yy_NUL_trans[yy_current_state]; yy_is_jam = (yy_current_state == 0); if ( ! yy_is_jam ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_is_jam ? 0 : yy_current_state; } #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void) #else static int input (void) #endif { int c; *(yy_c_buf_p) = (yy_hold_char); if ( *(yy_c_buf_p) == YY_END_OF_BUFFER_CHAR ) { /* yy_c_buf_p now points to the character we want to return. * If this occurs *before* the EOB characters, then it's a * valid NUL; if not, then we've hit the end of the buffer. */ if ( (yy_c_buf_p) < &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) /* This was really a NUL. */ *(yy_c_buf_p) = '\0'; else { /* need more input */ int offset = (yy_c_buf_p) - (yytext_ptr); ++(yy_c_buf_p); switch ( yy_get_next_buffer( ) ) { case EOB_ACT_LAST_MATCH: /* This happens because yy_g_n_b() * sees that we've accumulated a * token and flags that we need to * try matching the token before * proceeding. But for input(), * there's no matching to consider. * So convert the EOB_ACT_LAST_MATCH * to EOB_ACT_END_OF_FILE. */ /* Reset buffer status. */ fitshdrrestart(fitshdrin ); /*FALLTHROUGH*/ case EOB_ACT_END_OF_FILE: { if ( fitshdrwrap( ) ) return EOF; if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; #ifdef __cplusplus return yyinput(); #else return input(); #endif } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + offset; break; } } } c = *(unsigned char *) (yy_c_buf_p); /* cast for 8-bit char's */ *(yy_c_buf_p) = '\0'; /* preserve fitshdrtext */ (yy_hold_char) = *++(yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_at_bol = (c == '\n'); return c; } #endif /* ifndef YY_NO_INPUT */ /** Immediately switch to a different input stream. * @param input_file A readable stream. * * @note This function does not reset the start condition to @c INITIAL . */ void fitshdrrestart (FILE * input_file ) { if ( ! YY_CURRENT_BUFFER ){ fitshdrensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = fitshdr_create_buffer(fitshdrin,YY_BUF_SIZE ); } fitshdr_init_buffer(YY_CURRENT_BUFFER,input_file ); fitshdr_load_buffer_state( ); } /** Switch to a different input buffer. * @param new_buffer The new input buffer. * */ void fitshdr_switch_to_buffer (YY_BUFFER_STATE new_buffer ) { /* TODO. We should be able to replace this entire function body * with * fitshdrpop_buffer_state(); * fitshdrpush_buffer_state(new_buffer); */ fitshdrensure_buffer_stack (); if ( YY_CURRENT_BUFFER == new_buffer ) return; if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } YY_CURRENT_BUFFER_LVALUE = new_buffer; fitshdr_load_buffer_state( ); /* We don't actually know whether we did this switch during * EOF (fitshdrwrap()) processing, but the only time this flag * is looked at is after fitshdrwrap() is called, so it's safe * to go ahead and always set it. */ (yy_did_buffer_switch_on_eof) = 1; } static void fitshdr_load_buffer_state (void) { (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; (yytext_ptr) = (yy_c_buf_p) = YY_CURRENT_BUFFER_LVALUE->yy_buf_pos; fitshdrin = YY_CURRENT_BUFFER_LVALUE->yy_input_file; (yy_hold_char) = *(yy_c_buf_p); } /** Allocate and initialize an input buffer state. * @param file A readable stream. * @param size The character buffer size in bytes. When in doubt, use @c YY_BUF_SIZE. * * @return the allocated buffer state. */ YY_BUFFER_STATE fitshdr_create_buffer (FILE * file, int size ) { YY_BUFFER_STATE b; b = (YY_BUFFER_STATE) fitshdralloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in fitshdr_create_buffer()" ); b->yy_buf_size = size; /* yy_ch_buf has to be 2 characters longer than the size given because * we need to put in 2 end-of-buffer characters. */ b->yy_ch_buf = (char *) fitshdralloc(b->yy_buf_size + 2 ); if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in fitshdr_create_buffer()" ); b->yy_is_our_buffer = 1; fitshdr_init_buffer(b,file ); return b; } /** Destroy the buffer. * @param b a buffer created with fitshdr_create_buffer() * */ void fitshdr_delete_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; if ( b == YY_CURRENT_BUFFER ) /* Not sure if we should pop here. */ YY_CURRENT_BUFFER_LVALUE = (YY_BUFFER_STATE) 0; if ( b->yy_is_our_buffer ) fitshdrfree((void *) b->yy_ch_buf ); fitshdrfree((void *) b ); } /* Initializes or reinitializes a buffer. * This function is sometimes called more than once on the same buffer, * such as during a fitshdrrestart() or at EOF. */ static void fitshdr_init_buffer (YY_BUFFER_STATE b, FILE * file ) { int oerrno = errno; fitshdr_flush_buffer(b ); b->yy_input_file = file; b->yy_fill_buffer = 1; /* If b is the current buffer, then fitshdr_init_buffer was _probably_ * called from fitshdrrestart() or through yy_get_next_buffer. * In that case, we don't want to reset the lineno or column. */ if (b != YY_CURRENT_BUFFER){ b->yy_bs_lineno = 1; b->yy_bs_column = 0; } b->yy_is_interactive = 0; errno = oerrno; } /** Discard all buffered characters. On the next scan, YY_INPUT will be called. * @param b the buffer state to be flushed, usually @c YY_CURRENT_BUFFER. * */ void fitshdr_flush_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; b->yy_n_chars = 0; /* We always need two end-of-buffer characters. The first causes * a transition to the end-of-buffer state. The second causes * a jam in that state. */ b->yy_ch_buf[0] = YY_END_OF_BUFFER_CHAR; b->yy_ch_buf[1] = YY_END_OF_BUFFER_CHAR; b->yy_buf_pos = &b->yy_ch_buf[0]; b->yy_at_bol = 1; b->yy_buffer_status = YY_BUFFER_NEW; if ( b == YY_CURRENT_BUFFER ) fitshdr_load_buffer_state( ); } /** Pushes the new state onto the stack. The new state becomes * the current state. This function will allocate the stack * if necessary. * @param new_buffer The new state. * */ void fitshdrpush_buffer_state (YY_BUFFER_STATE new_buffer ) { if (new_buffer == NULL) return; fitshdrensure_buffer_stack(); /* This block is copied from fitshdr_switch_to_buffer. */ if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } /* Only push if top exists. Otherwise, replace top. */ if (YY_CURRENT_BUFFER) (yy_buffer_stack_top)++; YY_CURRENT_BUFFER_LVALUE = new_buffer; /* copied from fitshdr_switch_to_buffer. */ fitshdr_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } /** Removes and deletes the top of the stack, if present. * The next element becomes the new top. * */ void fitshdrpop_buffer_state (void) { if (!YY_CURRENT_BUFFER) return; fitshdr_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; if ((yy_buffer_stack_top) > 0) --(yy_buffer_stack_top); if (YY_CURRENT_BUFFER) { fitshdr_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } } /* Allocates the stack if it does not exist. * Guarantees space for at least one push. */ static void fitshdrensure_buffer_stack (void) { int num_to_alloc; if (!(yy_buffer_stack)) { /* First allocation is just for 2 elements, since we don't know if this * scanner will even need a stack. We use 2 instead of 1 to avoid an * immediate realloc on the next call. */ num_to_alloc = 1; (yy_buffer_stack) = (struct yy_buffer_state**)fitshdralloc (num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in fitshdrensure_buffer_stack()" ); memset((yy_buffer_stack), 0, num_to_alloc * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; (yy_buffer_stack_top) = 0; return; } if ((yy_buffer_stack_top) >= ((yy_buffer_stack_max)) - 1){ /* Increase the buffer to prepare for a possible push. */ int grow_size = 8 /* arbitrary grow size */; num_to_alloc = (yy_buffer_stack_max) + grow_size; (yy_buffer_stack) = (struct yy_buffer_state**)fitshdrrealloc ((yy_buffer_stack), num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in fitshdrensure_buffer_stack()" ); /* zero only the new slots.*/ memset((yy_buffer_stack) + (yy_buffer_stack_max), 0, grow_size * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; } } /** Setup the input buffer state to scan directly from a user-specified character buffer. * @param base the character buffer * @param size the size in bytes of the character buffer * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE fitshdr_scan_buffer (char * base, yy_size_t size ) { YY_BUFFER_STATE b; if ( size < 2 || base[size-2] != YY_END_OF_BUFFER_CHAR || base[size-1] != YY_END_OF_BUFFER_CHAR ) /* They forgot to leave room for the EOB's. */ return 0; b = (YY_BUFFER_STATE) fitshdralloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in fitshdr_scan_buffer()" ); b->yy_buf_size = size - 2; /* "- 2" to take care of EOB's */ b->yy_buf_pos = b->yy_ch_buf = base; b->yy_is_our_buffer = 0; b->yy_input_file = 0; b->yy_n_chars = b->yy_buf_size; b->yy_is_interactive = 0; b->yy_at_bol = 1; b->yy_fill_buffer = 0; b->yy_buffer_status = YY_BUFFER_NEW; fitshdr_switch_to_buffer(b ); return b; } /** Setup the input buffer state to scan a string. The next call to fitshdrlex() will * scan from a @e copy of @a str. * @param yystr a NUL-terminated string to scan * * @return the newly allocated buffer state object. * @note If you want to scan bytes that may contain NUL values, then use * fitshdr_scan_bytes() instead. */ YY_BUFFER_STATE fitshdr_scan_string (yyconst char * yystr ) { return fitshdr_scan_bytes(yystr,strlen(yystr) ); } /** Setup the input buffer state to scan the given bytes. The next call to fitshdrlex() will * scan from a @e copy of @a bytes. * @param yybytes the byte buffer to scan * @param _yybytes_len the number of bytes in the buffer pointed to by @a bytes. * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE fitshdr_scan_bytes (yyconst char * yybytes, int _yybytes_len ) { YY_BUFFER_STATE b; char *buf; yy_size_t n; int i; /* Get memory for full buffer, including space for trailing EOB's. */ n = _yybytes_len + 2; buf = (char *) fitshdralloc(n ); if ( ! buf ) YY_FATAL_ERROR( "out of dynamic memory in fitshdr_scan_bytes()" ); for ( i = 0; i < _yybytes_len; ++i ) buf[i] = yybytes[i]; buf[_yybytes_len] = buf[_yybytes_len+1] = YY_END_OF_BUFFER_CHAR; b = fitshdr_scan_buffer(buf,n ); if ( ! b ) YY_FATAL_ERROR( "bad buffer in fitshdr_scan_bytes()" ); /* It's okay to grow etc. this buffer, and we should throw it * away when we're done. */ b->yy_is_our_buffer = 1; return b; } #ifndef YY_EXIT_FAILURE #define YY_EXIT_FAILURE 2 #endif static void yy_fatal_error (yyconst char* msg ) { (void) fprintf( stderr, "%s\n", msg ); exit( YY_EXIT_FAILURE ); } /* Redefine yyless() so it works in section 3 code. */ #undef yyless #define yyless(n) \ do \ { \ /* Undo effects of setting up fitshdrtext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ fitshdrtext[fitshdrleng] = (yy_hold_char); \ (yy_c_buf_p) = fitshdrtext + yyless_macro_arg; \ (yy_hold_char) = *(yy_c_buf_p); \ *(yy_c_buf_p) = '\0'; \ fitshdrleng = yyless_macro_arg; \ } \ while ( 0 ) /* Accessor methods (get/set functions) to struct members. */ /** Get the current line number. * */ int fitshdrget_lineno (void) { return fitshdrlineno; } /** Get the input stream. * */ FILE *fitshdrget_in (void) { return fitshdrin; } /** Get the output stream. * */ FILE *fitshdrget_out (void) { return fitshdrout; } /** Get the length of the current token. * */ int fitshdrget_leng (void) { return fitshdrleng; } /** Get the current token. * */ char *fitshdrget_text (void) { return fitshdrtext; } /** Set the current line number. * @param line_number * */ void fitshdrset_lineno (int line_number ) { fitshdrlineno = line_number; } /** Set the input stream. This does not discard the current * input buffer. * @param in_str A readable stream. * * @see fitshdr_switch_to_buffer */ void fitshdrset_in (FILE * in_str ) { fitshdrin = in_str ; } void fitshdrset_out (FILE * out_str ) { fitshdrout = out_str ; } int fitshdrget_debug (void) { return fitshdr_flex_debug; } void fitshdrset_debug (int bdebug ) { fitshdr_flex_debug = bdebug ; } static int yy_init_globals (void) { /* Initialization is the same as for the non-reentrant scanner. * This function is called from fitshdrlex_destroy(), so don't allocate here. */ (yy_buffer_stack) = 0; (yy_buffer_stack_top) = 0; (yy_buffer_stack_max) = 0; (yy_c_buf_p) = (char *) 0; (yy_init) = 0; (yy_start) = 0; /* Defined in main.c */ #ifdef YY_STDINIT fitshdrin = stdin; fitshdrout = stdout; #else fitshdrin = (FILE *) 0; fitshdrout = (FILE *) 0; #endif /* For future reference: Set errno on error, since we are called by * fitshdrlex_init() */ return 0; } /* fitshdrlex_destroy is for both reentrant and non-reentrant scanners. */ int fitshdrlex_destroy (void) { /* Pop the buffer stack, destroying each element. */ while(YY_CURRENT_BUFFER){ fitshdr_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; fitshdrpop_buffer_state(); } /* Destroy the stack itself. */ fitshdrfree((yy_buffer_stack) ); (yy_buffer_stack) = NULL; /* Reset the globals. This is important in a non-reentrant scanner so the next time * fitshdrlex() is called, initialization will occur. */ yy_init_globals( ); return 0; } /* * Internal utility routines. */ #ifndef yytext_ptr static void yy_flex_strncpy (char* s1, yyconst char * s2, int n ) { register int i; for ( i = 0; i < n; ++i ) s1[i] = s2[i]; } #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * s ) { register int n; for ( n = 0; s[n]; ++n ) ; return n; } #endif void *fitshdralloc (yy_size_t size ) { return (void *) malloc( size ); } void *fitshdrrealloc (void * ptr, yy_size_t size ) { /* The cast to (char *) in the following accommodates both * implementations that use char* generic pointers, and those * that use void* generic pointers. It works with the latter * because both ANSI C and C++ allow castless assignment from * any pointer type to void*, and deal with argument conversions * as though doing an assignment. */ return (void *) realloc( (char *) ptr, size ); } void fitshdrfree (void * ptr ) { free( (char *) ptr ); /* see fitshdrrealloc() for (char *) cast */ } #define YYTABLES_NAME "yytables" #line 535 "fitshdr.l" /*--------------------------------------------------------------------------*/ void nullfill(char cptr[], int len) { int j, k; /* Null-fill the string. */ for (j = 0; j < len; j++) { if (cptr[j] == '\0') { for (k = j+1; k < len; k++) { cptr[k] = '\0'; } break; } } for (k = j-1; k >= 0; k--) { if (cptr[k] != ' ') break; cptr[k] = '\0'; } return; } pywcs-1.12/wcslib/C/flexed/README0000644001153600020070000000040612310355626020442 0ustar cslocumSTSCI\science00000000000000This directory contains C code generated by flex 2.5.35 under Debian lenny from the Flex description files (*.l) in the parent directory. These pre-generated source files may be used during installation if Flex 2.5.9 or later is not available on the build host. pywcs-1.12/wcslib/C/flexed/wcsbth.c0000644001153600020070000334422412310355626021234 0ustar cslocumSTSCI\science00000000000000#line 2 "wcsbth.c" #line 4 "wcsbth.c" #define YY_INT_ALIGNED short int /* A lexical scanner generated by flex */ #define yy_create_buffer wcsbth_create_buffer #define yy_delete_buffer wcsbth_delete_buffer #define yy_flex_debug wcsbth_flex_debug #define yy_init_buffer wcsbth_init_buffer #define yy_flush_buffer wcsbth_flush_buffer #define yy_load_buffer_state wcsbth_load_buffer_state #define yy_switch_to_buffer wcsbth_switch_to_buffer #define yyin wcsbthin #define yyleng wcsbthleng #define yylex wcsbthlex #define yylineno wcsbthlineno #define yyout wcsbthout #define yyrestart wcsbthrestart #define yytext wcsbthtext #define yywrap wcsbthwrap #define yyalloc wcsbthalloc #define yyrealloc wcsbthrealloc #define yyfree wcsbthfree #define FLEX_SCANNER #define YY_FLEX_MAJOR_VERSION 2 #define YY_FLEX_MINOR_VERSION 5 #define YY_FLEX_SUBMINOR_VERSION 35 #if YY_FLEX_SUBMINOR_VERSION > 0 #define FLEX_BETA #endif /* First, we deal with platform-specific or compiler-specific issues. */ /* begin standard C headers. */ #include #include #include #include /* end standard C headers. */ /* flex integer type definitions */ #ifndef FLEXINT_H #define FLEXINT_H /* C99 systems have . Non-C99 systems may or may not. */ #if defined (__STDC_VERSION__) && __STDC_VERSION__ >= 199901L /* C99 says to define __STDC_LIMIT_MACROS before including stdint.h, * if you want the limit (max/min) macros for int types. */ #ifndef __STDC_LIMIT_MACROS #define __STDC_LIMIT_MACROS 1 #endif #include typedef int8_t flex_int8_t; typedef uint8_t flex_uint8_t; typedef int16_t flex_int16_t; typedef uint16_t flex_uint16_t; typedef int32_t flex_int32_t; typedef uint32_t flex_uint32_t; #else typedef signed char flex_int8_t; typedef short int flex_int16_t; typedef int flex_int32_t; typedef unsigned char flex_uint8_t; typedef unsigned short int flex_uint16_t; typedef unsigned int flex_uint32_t; /* Limits of integral types. */ #ifndef INT8_MIN #define INT8_MIN (-128) #endif #ifndef INT16_MIN #define INT16_MIN (-32767-1) #endif #ifndef INT32_MIN #define INT32_MIN (-2147483647-1) #endif #ifndef INT8_MAX #define INT8_MAX (127) #endif #ifndef INT16_MAX #define INT16_MAX (32767) #endif #ifndef INT32_MAX #define INT32_MAX (2147483647) #endif #ifndef UINT8_MAX #define UINT8_MAX (255U) #endif #ifndef UINT16_MAX #define UINT16_MAX (65535U) #endif #ifndef UINT32_MAX #define UINT32_MAX (4294967295U) #endif #endif /* ! C99 */ #endif /* ! FLEXINT_H */ #ifdef __cplusplus /* The "const" storage-class-modifier is valid. */ #define YY_USE_CONST #else /* ! __cplusplus */ /* C99 requires __STDC__ to be defined as 1. */ #if defined (__STDC__) #define YY_USE_CONST #endif /* defined (__STDC__) */ #endif /* ! __cplusplus */ #ifdef YY_USE_CONST #define yyconst const #else #define yyconst #endif /* Returned upon end-of-file. */ #define YY_NULL 0 /* Promotes a possibly negative, possibly signed char to an unsigned * integer for use as an array index. If the signed char is negative, * we want to instead treat it as an 8-bit unsigned char, hence the * double cast. */ #define YY_SC_TO_UI(c) ((unsigned int) (unsigned char) c) /* Enter a start condition. This macro really ought to take a parameter, * but we do it the disgusting crufty way forced on us by the ()-less * definition of BEGIN. */ #define BEGIN (yy_start) = 1 + 2 * /* Translate the current start state into a value that can be later handed * to BEGIN to return to the state. The YYSTATE alias is for lex * compatibility. */ #define YY_START (((yy_start) - 1) / 2) #define YYSTATE YY_START /* Action number for EOF rule of a given start state. */ #define YY_STATE_EOF(state) (YY_END_OF_BUFFER + state + 1) /* Special action meaning "start processing a new file". */ #define YY_NEW_FILE wcsbthrestart(wcsbthin ) #define YY_END_OF_BUFFER_CHAR 0 /* Size of default input buffer. */ #ifndef YY_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k. * Moreover, YY_BUF_SIZE is 2*YY_READ_BUF_SIZE in the general case. * Ditto for the __ia64__ case accordingly. */ #define YY_BUF_SIZE 32768 #else #define YY_BUF_SIZE 16384 #endif /* __ia64__ */ #endif /* The state buf must be large enough to hold one state per character in the main buffer. */ #define YY_STATE_BUF_SIZE ((YY_BUF_SIZE + 2) * sizeof(yy_state_type)) #ifndef YY_TYPEDEF_YY_BUFFER_STATE #define YY_TYPEDEF_YY_BUFFER_STATE typedef struct yy_buffer_state *YY_BUFFER_STATE; #endif extern int wcsbthleng; extern FILE *wcsbthin, *wcsbthout; #define EOB_ACT_CONTINUE_SCAN 0 #define EOB_ACT_END_OF_FILE 1 #define EOB_ACT_LAST_MATCH 2 #define YY_LESS_LINENO(n) /* Return all but the first "n" matched characters back to the input stream. */ #define yyless(n) \ do \ { \ /* Undo effects of setting up wcsbthtext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ *yy_cp = (yy_hold_char); \ YY_RESTORE_YY_MORE_OFFSET \ (yy_c_buf_p) = yy_cp = yy_bp + yyless_macro_arg - YY_MORE_ADJ; \ YY_DO_BEFORE_ACTION; /* set up wcsbthtext again */ \ } \ while ( 0 ) #define unput(c) yyunput( c, (yytext_ptr) ) #ifndef YY_TYPEDEF_YY_SIZE_T #define YY_TYPEDEF_YY_SIZE_T typedef size_t yy_size_t; #endif #ifndef YY_STRUCT_YY_BUFFER_STATE #define YY_STRUCT_YY_BUFFER_STATE struct yy_buffer_state { FILE *yy_input_file; char *yy_ch_buf; /* input buffer */ char *yy_buf_pos; /* current position in input buffer */ /* Size of input buffer in bytes, not including room for EOB * characters. */ yy_size_t yy_buf_size; /* Number of characters read into yy_ch_buf, not including EOB * characters. */ int yy_n_chars; /* Whether we "own" the buffer - i.e., we know we created it, * and can realloc() it to grow it, and should free() it to * delete it. */ int yy_is_our_buffer; /* Whether this is an "interactive" input source; if so, and * if we're using stdio for input, then we want to use getc() * instead of fread(), to make sure we stop fetching input after * each newline. */ int yy_is_interactive; /* Whether we're considered to be at the beginning of a line. * If so, '^' rules will be active on the next match, otherwise * not. */ int yy_at_bol; int yy_bs_lineno; /**< The line count. */ int yy_bs_column; /**< The column count. */ /* Whether to try to fill the input buffer when we reach the * end of it. */ int yy_fill_buffer; int yy_buffer_status; #define YY_BUFFER_NEW 0 #define YY_BUFFER_NORMAL 1 /* When an EOF's been seen but there's still some text to process * then we mark the buffer as YY_EOF_PENDING, to indicate that we * shouldn't try reading from the input source any more. We might * still have a bunch of tokens to match, though, because of * possible backing-up. * * When we actually see the EOF, we change the status to "new" * (via wcsbthrestart()), so that the user can continue scanning by * just pointing wcsbthin at a new input file. */ #define YY_BUFFER_EOF_PENDING 2 }; #endif /* !YY_STRUCT_YY_BUFFER_STATE */ /* Stack of input buffers. */ static size_t yy_buffer_stack_top = 0; /**< index of top of stack. */ static size_t yy_buffer_stack_max = 0; /**< capacity of stack. */ static YY_BUFFER_STATE * yy_buffer_stack = 0; /**< Stack as an array. */ /* We provide macros for accessing buffer states in case in the * future we want to put the buffer states in a more general * "scanner state". * * Returns the top of the stack, or NULL. */ #define YY_CURRENT_BUFFER ( (yy_buffer_stack) \ ? (yy_buffer_stack)[(yy_buffer_stack_top)] \ : NULL) /* Same as previous macro, but useful when we know that the buffer stack is not * NULL or when we need an lvalue. For internal use only. */ #define YY_CURRENT_BUFFER_LVALUE (yy_buffer_stack)[(yy_buffer_stack_top)] /* yy_hold_char holds the character lost when wcsbthtext is formed. */ static char yy_hold_char; static int yy_n_chars; /* number of characters read into yy_ch_buf */ int wcsbthleng; /* Points to current character in buffer. */ static char *yy_c_buf_p = (char *) 0; static int yy_init = 0; /* whether we need to initialize */ static int yy_start = 0; /* start state number */ /* Flag which is used to allow wcsbthwrap()'s to do buffer switches * instead of setting up a fresh wcsbthin. A bit of a hack ... */ static int yy_did_buffer_switch_on_eof; void wcsbthrestart (FILE *input_file ); void wcsbth_switch_to_buffer (YY_BUFFER_STATE new_buffer ); YY_BUFFER_STATE wcsbth_create_buffer (FILE *file,int size ); void wcsbth_delete_buffer (YY_BUFFER_STATE b ); void wcsbth_flush_buffer (YY_BUFFER_STATE b ); void wcsbthpush_buffer_state (YY_BUFFER_STATE new_buffer ); void wcsbthpop_buffer_state (void ); static void wcsbthensure_buffer_stack (void ); static void wcsbth_load_buffer_state (void ); static void wcsbth_init_buffer (YY_BUFFER_STATE b,FILE *file ); #define YY_FLUSH_BUFFER wcsbth_flush_buffer(YY_CURRENT_BUFFER ) YY_BUFFER_STATE wcsbth_scan_buffer (char *base,yy_size_t size ); YY_BUFFER_STATE wcsbth_scan_string (yyconst char *yy_str ); YY_BUFFER_STATE wcsbth_scan_bytes (yyconst char *bytes,int len ); void *wcsbthalloc (yy_size_t ); void *wcsbthrealloc (void *,yy_size_t ); void wcsbthfree (void * ); #define yy_new_buffer wcsbth_create_buffer #define yy_set_interactive(is_interactive) \ { \ if ( ! YY_CURRENT_BUFFER ){ \ wcsbthensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcsbth_create_buffer(wcsbthin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_is_interactive = is_interactive; \ } #define yy_set_bol(at_bol) \ { \ if ( ! YY_CURRENT_BUFFER ){\ wcsbthensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcsbth_create_buffer(wcsbthin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = at_bol; \ } #define YY_AT_BOL() (YY_CURRENT_BUFFER_LVALUE->yy_at_bol) /* Begin user sect3 */ #define wcsbthwrap(n) 1 #define YY_SKIP_YYWRAP typedef char YY_CHAR; FILE *wcsbthin = (FILE *) 0, *wcsbthout = (FILE *) 0; typedef int yy_state_type; extern int wcsbthlineno; int wcsbthlineno = 1; extern char *wcsbthtext; #define yytext_ptr wcsbthtext static yyconst flex_int16_t yy_nxt[][128] = { { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 }, { 67, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68 }, { 67, 69, 69, 69, 69, 69, 69, 69, 69, 69, 68, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 70, 70, 70, 70, 70, 70, 70, 70, 70, 69, 69, 69, 69, 69, 69, 69, 69, 69, 71, 72, 73, 69, 69, 69, 69, 69, 69, 74, 75, 69, 76, 77, 69, 78, 79, 80, 69, 81, 82, 69, 69, 83, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69, 69 }, { 67, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 84, 84, 84, 84, 84, 84, 84, 84, 84, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68 }, { 67, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 84, 84, 84, 84, 84, 84, 84, 84, 84, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68, 68 }, { 67, 85, 85, 85, 85, 85, 85, 85, 85, 85, 68, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 86, 86, 86, 86, 86, 86, 86, 86, 86, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85 }, { 67, 85, 85, 85, 85, 85, 85, 85, 85, 85, 68, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 86, 86, 86, 86, 86, 86, 86, 86, 86, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85, 85 }, { 67, 87, 87, 87, 87, 87, 87, 87, 87, 87, 68, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 88, 88, 88, 88, 88, 88, 88, 88, 88, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87 }, { 67, 87, 87, 87, 87, 87, 87, 87, 87, 87, 68, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 88, 88, 88, 88, 88, 88, 88, 88, 88, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87, 87 }, { 67, 89, 89, 89, 89, 89, 89, 89, 89, 89, 68, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 90, 90, 90, 90, 90, 90, 90, 90, 90, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89 }, { 67, 89, 89, 89, 89, 89, 89, 89, 89, 89, 68, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 90, 90, 90, 90, 90, 90, 90, 90, 90, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89, 89 }, { 67, 91, 91, 91, 91, 91, 91, 91, 91, 91, 68, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 92, 92, 92, 92, 92, 92, 92, 92, 92, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91 }, { 67, 91, 91, 91, 91, 91, 91, 91, 91, 91, 68, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 92, 92, 92, 92, 92, 92, 92, 92, 92, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 91, 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sets up wcsbthtext. */ #define YY_DO_BEFORE_ACTION \ (yytext_ptr) = yy_bp; \ wcsbthleng = (size_t) (yy_cp - yy_bp); \ (yy_hold_char) = *yy_cp; \ *yy_cp = '\0'; \ (yy_c_buf_p) = yy_cp; #define YY_NUM_RULES 283 #define YY_END_OF_BUFFER 284 /* This struct is not used in this scanner, but its presence is necessary. */ struct yy_trans_info { flex_int32_t yy_verify; flex_int32_t yy_nxt; }; static yyconst flex_int16_t yy_accept[927] = { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 278, 278, 280, 280, 281, 281, 0, 0, 284, 283, 126, 126, 126, 126, 126, 126, 126, 126, 126, 126, 126, 126, 126, 126, 126, 283, 148, 148, 140, 140, 149, 149, 141, 141, 161, 161, 161, 283, 182, 182, 171, 171, 187, 187, 198, 198, 199, 199, 230, 230, 265, 265, 243, 243, 266, 266, 244, 244, 268, 268, 201, 202, 200, 209, 209, 210, 210, 218, 218, 219, 219, 270, 270, 272, 272, 271, 274, 274, 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51, 49, 0, 93, 0, 0, 0, 103, 0, 54, 56, 108, 106, 110, 0, 28, 0, 71, 76, 0, 15, 46, 81, 41, 36, 0, 122, 114, 0, 0, 0, 0, 112, 0, 0, 121, 0, 0, 124, 142, 143, 144, 145, 146, 147, 0, 0, 0, 0, 0, 0, 162, 163, 164, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 203, 204, 205, 211, 212, 213, 214, 27, 70, 75, 31, 14, 45, 80, 40, 35, 25, 68, 73, 30, 12, 43, 78, 38, 33, 0, 0, 0, 0, 0, 0, 0, 0, 0, 95, 0, 97, 99, 101, 62, 0, 0, 0, 0, 0, 0, 0, 29, 72, 77, 32, 16, 47, 82, 42, 37, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 170, 167, 169, 165, 166, 168, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 236, 234, 235, 231, 232, 233, 0, 0, 0, 0, 0, 0, 0, 0, 242, 240, 241, 237, 238, 239, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 160, 159, 155, 158, 152, 153, 157, 150, 151, 154, 156, 181, 177, 180, 174, 176, 179, 172, 173, 175, 178, 229, 225, 228, 222, 223, 227, 220, 221, 224, 226, 260, 250, 259, 248, 249, 258, 245, 246, 247, 257, 264, 256, 263, 254, 255, 262, 251, 252, 253, 261, 0, 0, 0, 0, 0, 0, 0, 90, 50, 48, 0, 0, 0, 0, 102, 0, 52, 55, 105, 107, 109, 0, 113, 111, 0, 0, 0, 0, 0, 0, 0, 0, 0, 120, 0, 0, 0, 0, 0, 0, 123, 83, 85, 86, 87, 88, 0, 89, 92, 94, 96, 98, 100, 104, 53, 0, 115, 117, 118, 119, 116, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 3, 0, 0, 4, 0, 0, 5, 0, 0, 2, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 6, 0, 7, 0, 8, 0, 9, 0, 10, 0, 11, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 125 } ; static yy_state_type yy_last_accepting_state; static char *yy_last_accepting_cpos; static yyconst yy_state_type yy_NUL_trans[927] = { 0, 68, 69, 68, 68, 85, 85, 87, 87, 89, 89, 91, 91, 93, 93, 68, 68, 97, 97, 99, 99, 101, 101, 103, 103, 105, 105, 107, 107, 109, 109, 111, 111, 113, 113, 115, 115, 117, 117, 119, 119, 120, 120, 122, 122, 124, 124, 126, 126, 128, 128, 130, 130, 132, 132, 135, 135, 139, 139, 141, 141, 144, 144, 145, 145, 146, 146, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 247, 0, 0, 251, 252, 253, 254, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 247, 0, 0, 251, 251, 252, 253, 254, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 847, 0, 849, 0, 851, 0, 853, 0, 855, 0, 857, 0, 847, 0, 849, 0, 851, 0, 853, 0, 855, 0, 857, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 } ; extern int wcsbth_flex_debug; int wcsbth_flex_debug = 0; /* The intent behind this definition is that it'll catch * any uses of REJECT which flex missed. */ #define REJECT reject_used_but_not_detected #define yymore() yymore_used_but_not_detected #define YY_MORE_ADJ 0 #define YY_RESTORE_YY_MORE_OFFSET char *wcsbthtext; #line 1 "wcsbth.l" /*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsbth.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcsbth.l is a Flex description file containing the definition of a lexical * scanner for parsing the WCS keyrecords for one or more image arrays and/or * pixel lists in a FITS binary table header. It can also handle primary image * and image extension headers. * * wcsbth.l requires Flex v2.5.4 or later. Refer to wcshdr.h for a description * of the user interface and operating notes. * * Implementation notes * -------------------- * wcsbth() may be invoked with an option that causes it to recognise the * image-header form of WCS keywords as defaults for each alternate coordinate * representation (up to 27). By design, with this option enabled wcsbth() can * also handle primary image and image extension headers, effectively treating * them as a single-column binary table though with WCS keywords of a different * form. * * NAXIS is always 2 for binary tables, it refers to the two-dimensional nature * of the table. Thus NAXIS does not count the number of image axes in either * image arrays or pixels lists and for the latter there is not even a formal * equivalent of WCSAXESa. Hence NAXIS is always ignored and a first pass * through the header is required to determine the number of images, the number * of alternate coordinate representations for each image (up to 27), and the * number of coordinate axes in each representation; this pass also counts the * number of iPVn_ma and iPSn_ma or TVk_ma and TSk_ma keywords in each * representation. * * On completion of the first pass, the association between column number and * axis number is defined for each representation of a pixel list. Memory is * allocated for an array of the required number of wcsprm structs and each of * these is initialized appropriately. These structs are filled in the second * pass. * * It is permissible for a scalar table column to contain degenerate (single- * point) image arrays and simultaneously form one axis of a pixel list. * * The parser does not check for duplicated keywords, for most keywords it * accepts the last encountered. * * wcsbth() does not currently handle the Green Bank convention. * *===========================================================================*/ /* Options. */ /* Indices for parameterized keywords. */ /* Alternate coordinate system identifier. */ /* Keyvalue data types. */ /* Exclusive start states. */ #line 112 "wcsbth.l" #include #include #include #include #include #include "wcs.h" #include "wcshdr.h" #include "wcsmath.h" /* Codes used for keyvalue data types. */ #define INTEGER 0 #define FLOAT 1 #define STRING 2 /* Bit masks used for keyword types: */ #define IMGAUX 0x1 /* Auxiliary image header, e.g. LONPOLEa or */ /* DATE-OBS. */ #define IMGAXIS 0x2 /* Image header with axis number, e.g. */ /* CTYPEia. */ #define IMGHEAD 0x3 /* Image header of either type. */ #define BIMGARR 0x4 /* Binary table image array with axis */ /* number, e.g. iCTYna. */ #define PIXLIST 0x8 /* Pixel list, e.g. TCTYna. */ #define BINTAB 0xC /* Shared binary table image array (without */ /* axis number) or pixel list, e.g. LONPna */ /* or OBSGXn. */ #define YY_DECL int wcsbth(char *header, int nkeyrec, int relax, int ctrl, \ int keysel, int *colsel, int *nreject, int *nwcs, \ struct wcsprm **wcs) #define YY_INPUT(inbuff, count, bufsize) \ { \ if (wcsbth_nkeyrec) { \ strncpy(inbuff, wcsbth_hdr, 80); \ inbuff[80] = '\n'; \ wcsbth_hdr += 80; \ wcsbth_nkeyrec--; \ count = 81; \ } else { \ count = YY_NULL; \ } \ } /* A convenience macro to get around incompatibilities between unput() and yyless(): put wcsbthtext followed by a blank back onto the input stream. */ #define WCSBTH_PUTBACK \ sprintf(stmp, "%s ", wcsbthtext); \ itmp = strlen(stmp); \ while (itmp) unput(stmp[--itmp]); /* These global variables are required by YY_INPUT. */ char *wcsbth_hdr; int wcsbth_nkeyrec; /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcsbth_abort_jmp_env; #define exit(status) longjmp(wcsbth_abort_jmp_env, status) /* Struct used internally for header bookkeeping. */ struct wcsbth_alts { int ncol, ialt, icol, imgherit; short int (*arridx)[27]; short int pixidx[27]; short int pad1; unsigned int *pixlist; unsigned char (*npv)[27]; unsigned char (*nps)[27]; unsigned char pixnpv[27]; unsigned char pixnps[27]; unsigned char pad2[2]; }; int wcsbth_pass1(int keytype, int i, int j, int n, int k, char a, char ptype, struct wcsbth_alts *alts); int wcsbth_init1(struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs); struct wcsprm *wcsbth_idx(struct wcsprm *wcs, struct wcsbth_alts *alts, int keytype, int n, char a); int wcsbth_colax(struct wcsprm *wcs, struct wcsbth_alts *alts, int k, char a); int wcsbth_epoch(void *wptr); int wcsbth_vsource(void *wptr); int wcsbth_final(struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs); #line 16850 "wcsbth.c" #define INITIAL 0 #define CCCCCia 1 #define iCCCna 2 #define iCCCCn 3 #define TCCCna 4 #define TCCCCn 5 #define CCi_ja 6 #define ijCCna 7 #define TCn_ka 8 #define TCCn_ka 9 #define CROTAi 10 #define iCROTn 11 #define TCROTn 12 #define CCi_ma 13 #define iCn_ma 14 #define iCCn_ma 15 #define TCn_ma 16 #define TCCn_ma 17 #define PROJPm 18 #define CCCCCCCC 19 #define CCCCCCCa 20 #define CCCCna 21 #define CCCCCna 22 #define CCCCn 23 #define CCCCCn 24 #define VALUE 25 #define INTEGER_VAL 26 #define FLOAT_VAL 27 #define STRING_VAL 28 #define COMMENT 29 #define DISCARD 30 #define ERROR 31 #define FLUSH 32 #ifndef YY_NO_UNISTD_H /* Special case for "unistd.h", since it is non-ANSI. We include it way * down here because we want the user's section 1 to have been scanned first. * The user has a chance to override it with an option. */ #include #endif #ifndef YY_EXTRA_TYPE #define YY_EXTRA_TYPE void * #endif static int yy_init_globals (void ); /* Accessor methods to globals. These are made visible to non-reentrant scanners for convenience. */ int wcsbthlex_destroy (void ); int wcsbthget_debug (void ); void wcsbthset_debug (int debug_flag ); YY_EXTRA_TYPE wcsbthget_extra (void ); void wcsbthset_extra (YY_EXTRA_TYPE user_defined ); FILE *wcsbthget_in (void ); void wcsbthset_in (FILE * in_str ); FILE *wcsbthget_out (void ); void wcsbthset_out (FILE * out_str ); int wcsbthget_leng (void ); char *wcsbthget_text (void ); int wcsbthget_lineno (void ); void wcsbthset_lineno (int line_number ); /* Macros after this point can all be overridden by user definitions in * section 1. */ #ifndef YY_SKIP_YYWRAP #ifdef __cplusplus extern "C" int wcsbthwrap (void ); #else extern int wcsbthwrap (void ); #endif #endif static void yyunput (int c,char *buf_ptr ); #ifndef yytext_ptr static void yy_flex_strncpy (char *,yyconst char *,int ); #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * ); #endif #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void ); #else static int input (void ); #endif #endif /* Amount of stuff to slurp up with each read. */ #ifndef YY_READ_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k */ #define YY_READ_BUF_SIZE 16384 #else #define YY_READ_BUF_SIZE 8192 #endif /* __ia64__ */ #endif /* Copy whatever the last rule matched to the standard output. */ #ifndef ECHO /* This used to be an fputs(), but since the string might contain NUL's, * we now use fwrite(). */ #define ECHO do { if (fwrite( wcsbthtext, wcsbthleng, 1, wcsbthout )) {} } while (0) #endif /* Gets input and stuffs it into "buf". number of characters read, or YY_NULL, * is returned in "result". */ #ifndef YY_INPUT #define YY_INPUT(buf,result,max_size) \ errno=0; \ while ( (result = read( fileno(wcsbthin), (char *) buf, max_size )) < 0 ) \ { \ if( errno != EINTR) \ { \ YY_FATAL_ERROR( "input in flex scanner failed" ); \ break; \ } \ errno=0; \ clearerr(wcsbthin); \ }\ \ #endif /* No semi-colon after return; correct usage is to write "yyterminate();" - * we don't want an extra ';' after the "return" because that will cause * some compilers to complain about unreachable statements. */ #ifndef yyterminate #define yyterminate() return YY_NULL #endif /* Number of entries by which start-condition stack grows. */ #ifndef YY_START_STACK_INCR #define YY_START_STACK_INCR 25 #endif /* Report a fatal error. */ #ifndef YY_FATAL_ERROR #define YY_FATAL_ERROR(msg) yy_fatal_error( msg ) #endif /* end tables serialization structures and prototypes */ /* Default declaration of generated scanner - a define so the user can * easily add parameters. */ #ifndef YY_DECL #define YY_DECL_IS_OURS 1 extern int wcsbthlex (void); #define YY_DECL int wcsbthlex (void) #endif /* !YY_DECL */ /* Code executed at the beginning of each rule, after wcsbthtext and wcsbthleng * have been set up. */ #ifndef YY_USER_ACTION #define YY_USER_ACTION #endif /* Code executed at the end of each rule. */ #ifndef YY_BREAK #define YY_BREAK break; #endif #define YY_RULE_SETUP \ if ( wcsbthleng > 0 ) \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = \ (wcsbthtext[wcsbthleng - 1] == '\n'); \ YY_USER_ACTION /** The main scanner function which does all the work. */ YY_DECL { register yy_state_type yy_current_state; register char *yy_cp, *yy_bp; register int yy_act; #line 202 "wcsbth.l" /* Keyword indices, as used in the WCS papers, e.g. iVn_ma, TPn_ka. */ char a; int i, j, k, m, n; char *cptr, *errmsg, errtxt[80], exclude[1000], *extkey, *hptr, ptype, stmp[16]; int altlin, ialt, icol, incl, ipass, ipx, itmp, ix, jx, keytype, nsel, npass, status, valtype, voff; void *vptr, *wptr; struct wcsbth_alts alts; struct wcsprm *wcsp, wcstem; int (*special)(void *); int wcsbthlex_destroy(void); /* The data structures produced. */ *nwcs = 0; *wcs = 0x0; /* Parameters used to implement YY_INPUT. */ wcsbth_hdr = header; wcsbth_nkeyrec = nkeyrec; /* Our handle on the input stream. */ hptr = header; *nreject = 0; /* Keyword parameters. */ i = j = 0; n = k = 0; m = 0; a = ' '; /* Header bookkeeping. */ alts.ncol = 0; alts.arridx = 0x0; alts.pixlist = 0x0; alts.npv = 0x0; alts.nps = 0x0; for (ialt = 0; ialt < 27; ialt++) { alts.pixidx[ialt] = 0; alts.pixnpv[ialt] = 0; alts.pixnps[ialt] = 0; } /* For decoding the keyvalue. */ keytype = 0; valtype = -1; vptr = 0x0; /* For keywords that require special handling. */ altlin = 0; ptype = ' '; special = 0x0; /* Selection by column number. */ nsel = colsel ? colsel[0] : 0; incl = (nsel > 0); for (icol = 0; icol < 1000; icol++) { exclude[icol] = incl; } for (icol = 1; icol <= abs(nsel); icol++) { itmp = colsel[icol]; if (0 < itmp && itmp < 1000) { exclude[itmp] = !incl; } } exclude[0] = 0; /* Selection by keyword type. */ itmp = keysel; keysel = 0; if (itmp) { if (itmp & WCSHDR_IMGHEAD) keysel |= IMGHEAD; if (itmp & WCSHDR_BIMGARR) keysel |= BIMGARR; if (itmp & WCSHDR_PIXLIST) keysel |= PIXLIST; } if (keysel == 0) { keysel = IMGHEAD | BINTAB; } /* Control variables. */ ipass = 1; npass = 2; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcsbth_abort_jmp_env)) { return 4; } BEGIN(INITIAL); #line 17151 "wcsbth.c" if ( !(yy_init) ) { (yy_init) = 1; #ifdef YY_USER_INIT YY_USER_INIT; #endif if ( ! (yy_start) ) (yy_start) = 1; /* first start state */ if ( ! wcsbthin ) wcsbthin = stdin; if ( ! wcsbthout ) wcsbthout = stdout; if ( ! YY_CURRENT_BUFFER ) { wcsbthensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcsbth_create_buffer(wcsbthin,YY_BUF_SIZE ); } wcsbth_load_buffer_state( ); } while ( 1 ) /* loops until end-of-file is reached */ { yy_cp = (yy_c_buf_p); /* Support of wcsbthtext. */ *yy_cp = (yy_hold_char); /* yy_bp points to the position in yy_ch_buf of the start of * the current run. */ yy_bp = yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); yy_match: while ( (yy_current_state = yy_nxt[yy_current_state][ YY_SC_TO_UI(*yy_cp) ]) > 0 ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } ++yy_cp; } yy_current_state = -yy_current_state; yy_find_action: yy_act = yy_accept[yy_current_state]; YY_DO_BEFORE_ACTION; do_action: /* This label is used only to access EOF actions. */ switch ( yy_act ) { /* beginning of action switch */ case 0: /* must back up */ /* undo the effects of YY_DO_BEFORE_ACTION */ *yy_cp = (yy_hold_char); yy_cp = (yy_last_accepting_cpos) + 1; yy_current_state = (yy_last_accepting_state); goto yy_find_action; case 1: YY_RULE_SETUP #line 296 "wcsbth.l" { if (ipass == 1) { if (alts.ncol == 0) { sscanf(wcsbthtext, "TFIELDS = %d", &(alts.ncol)); BEGIN(FLUSH); } else { errmsg = "Duplicate or out-of-sequence TFIELDS keyword"; BEGIN(ERROR); } } else { BEGIN(FLUSH); } } YY_BREAK case 2: YY_RULE_SETUP #line 311 "wcsbth.l" { keytype = IMGAXIS; if (!(keytype & keysel)) { /* Ignore this key type. */ BEGIN(DISCARD); } else { if (relax & WCSHDR_ALLIMG) { if (ipass == 1) { sscanf(wcsbthtext, "WCSAXES%c= %d", &a, &i); wcsbth_pass1(IMGAXIS, i, 0, 0, 0, a, ' ', &alts); } BEGIN(FLUSH); } else if (relax & WCSHDR_reject) { errmsg = "Image-header keyword WCSAXESa in binary table"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } } YY_BREAK case 3: #line 339 "wcsbth.l" case 4: #line 340 "wcsbth.l" case 5: YY_RULE_SETUP #line 340 "wcsbth.l" { keytype = BIMGARR; /* Note that a blank in the sscanf() format string matches zero or more of them in the input. */ sscanf(wcsbthtext, "WCAX%d%c = %d", &n, &a, &i); if (!(keytype & keysel) || exclude[n]) { /* Ignore this key type or column. */ BEGIN(DISCARD); } else { if (ipass == 1) { wcsbth_pass1(BIMGARR, i, 0, n, 0, a, ' ', &alts); } BEGIN(FLUSH); } } YY_BREAK case 6: /* rule 6 can match eol */ #line 359 "wcsbth.l" case 7: /* rule 7 can match eol */ #line 360 "wcsbth.l" case 8: /* rule 8 can match eol */ YY_RULE_SETUP #line 360 "wcsbth.l" { /* Cross-reference supplier. */ keytype = BIMGARR; errmsg = "Cross-references are not currently implemented"; BEGIN(ERROR); } YY_BREAK case 9: /* rule 9 can match eol */ #line 368 "wcsbth.l" case 10: /* rule 10 can match eol */ #line 369 "wcsbth.l" case 11: /* rule 11 can match eol */ YY_RULE_SETUP #line 369 "wcsbth.l" { /* Cross-reference consumer. */ keytype = BIMGARR; errmsg = "Cross-references are not currently implemented"; BEGIN(ERROR); } YY_BREAK case 12: YY_RULE_SETUP #line 376 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crpix); extkey = "CRPIXja"; BEGIN(CCCCCia); } YY_BREAK case 13: #line 385 "wcsbth.l" case 14: YY_RULE_SETUP #line 385 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crpix); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { extkey = "jCRPXn"; BEGIN(iCCCCn); } } YY_BREAK case 15: #line 400 "wcsbth.l" case 16: YY_RULE_SETUP #line 400 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crpix); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { extkey = "TCRPXn"; BEGIN(TCCCCn); } } YY_BREAK case 17: YY_RULE_SETUP #line 412 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pc); altlin = 1; extkey = "PCi_ja"; BEGIN(CCi_ja); } YY_BREAK case 18: YY_RULE_SETUP #line 421 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pc); altlin = 1; sscanf(wcsbthtext, "%1d%1d", &i, &j); BEGIN(ijCCna); } YY_BREAK case 19: #line 432 "wcsbth.l" case 20: YY_RULE_SETUP #line 432 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pc); altlin = 1; if (wcsbthleng == 2) { BEGIN(TCn_ka); } else { extkey = "TPCn_ka"; BEGIN(TCCn_ka); } } YY_BREAK case 21: YY_RULE_SETUP #line 445 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.cd); altlin = 2; extkey = "CDi_ja"; BEGIN(CCi_ja); } YY_BREAK case 22: YY_RULE_SETUP #line 454 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.cd); altlin = 2; sscanf(wcsbthtext, "%1d%1d", &i, &j); BEGIN(ijCCna); } YY_BREAK case 23: #line 465 "wcsbth.l" case 24: YY_RULE_SETUP #line 465 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.cd); altlin = 2; if (wcsbthleng == 2) { BEGIN(TCn_ka); } else { extkey = "TCDn_ka"; BEGIN(TCCn_ka); } } YY_BREAK case 25: YY_RULE_SETUP #line 478 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.cdelt); extkey = "CDELTia"; BEGIN(CCCCCia); } YY_BREAK case 26: #line 487 "wcsbth.l" case 27: YY_RULE_SETUP #line 487 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.cdelt); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { extkey = "iCDLTn"; BEGIN(iCCCCn); } } YY_BREAK case 28: #line 502 "wcsbth.l" case 29: YY_RULE_SETUP #line 502 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.cdelt); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { extkey = "TCDLTn"; BEGIN(TCCCCn); } } YY_BREAK case 30: YY_RULE_SETUP #line 514 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crota); altlin = 4; extkey = "CROTAi"; BEGIN(CROTAi); } YY_BREAK case 31: YY_RULE_SETUP #line 523 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crota); altlin = 4; sscanf(wcsbthtext, "%d", &i); extkey = "iCROTn"; BEGIN(iCROTn); } YY_BREAK case 32: YY_RULE_SETUP #line 534 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crota); altlin = 4; extkey = "TCROTn"; BEGIN(TCROTn); } YY_BREAK case 33: YY_RULE_SETUP #line 543 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.cunit); extkey = "CUNITia"; BEGIN(CCCCCia); } YY_BREAK case 34: #line 552 "wcsbth.l" case 35: YY_RULE_SETUP #line 552 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.cunit); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { extkey = "iCUNIn"; BEGIN(iCCCCn); } } YY_BREAK case 36: #line 567 "wcsbth.l" case 37: YY_RULE_SETUP #line 567 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.cunit); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { extkey = "TCUNIn"; BEGIN(TCCCCn); } } YY_BREAK case 38: YY_RULE_SETUP #line 579 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.ctype); extkey = "CTYPEia"; BEGIN(CCCCCia); } YY_BREAK case 39: #line 588 "wcsbth.l" case 40: YY_RULE_SETUP #line 588 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.ctype); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { extkey = "iCTYPn"; BEGIN(iCCCCn); } } YY_BREAK case 41: #line 603 "wcsbth.l" case 42: YY_RULE_SETUP #line 603 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.ctype); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { extkey = "TCTYPn"; BEGIN(TCCCCn); } } YY_BREAK case 43: YY_RULE_SETUP #line 615 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crval); extkey = "CRVALia"; BEGIN(CCCCCia); } YY_BREAK case 44: #line 624 "wcsbth.l" case 45: YY_RULE_SETUP #line 624 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crval); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { extkey = "iCRVLn"; BEGIN(iCCCCn); } } YY_BREAK case 46: #line 639 "wcsbth.l" case 47: YY_RULE_SETUP #line 639 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crval); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { extkey = "TCRVLn"; BEGIN(TCCCCn); } } YY_BREAK case 48: #line 652 "wcsbth.l" case 49: YY_RULE_SETUP #line 652 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.lonpole); if (wcsbthleng == 7) { extkey = "LONPOLEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 50: #line 665 "wcsbth.l" case 51: YY_RULE_SETUP #line 665 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.latpole); if (wcsbthleng == 7) { extkey = "LATPOLEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 52: #line 678 "wcsbth.l" case 53: #line 679 "wcsbth.l" case 54: YY_RULE_SETUP #line 679 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.restfrq); if (wcsbthleng == 8) { unput(' '); extkey = "RESTFREQ"; BEGIN(CCCCCCCa); } else if (wcsbthleng == 7) { extkey = "RESTFRQa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 55: #line 696 "wcsbth.l" case 56: YY_RULE_SETUP #line 696 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.restwav); if (wcsbthleng == 7) { extkey = "RESTWAVa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 57: YY_RULE_SETUP #line 708 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; extkey = "PVi_ma"; BEGIN(CCi_ma); } YY_BREAK case 58: #line 718 "wcsbth.l" case 59: YY_RULE_SETUP #line 718 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 2) { BEGIN(iCn_ma); } else { extkey = "iPVn_ma"; BEGIN(iCCn_ma); } } YY_BREAK case 60: #line 734 "wcsbth.l" case 61: YY_RULE_SETUP #line 734 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; if (wcsbthleng == 2) { BEGIN(TCn_ma); } else { extkey = "TPVn_ma"; BEGIN(TCCn_ma); } } YY_BREAK case 62: YY_RULE_SETUP #line 747 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; BEGIN(PROJPm); } YY_BREAK case 63: YY_RULE_SETUP #line 755 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.ps); ptype = 's'; extkey = "PSi_ma"; BEGIN(CCi_ma); } YY_BREAK case 64: #line 765 "wcsbth.l" case 65: YY_RULE_SETUP #line 765 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.ps); ptype = 's'; sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 2) { BEGIN(iCn_ma); } else { extkey = "iPSn_ma"; BEGIN(iCCn_ma); } } YY_BREAK case 66: #line 781 "wcsbth.l" case 67: YY_RULE_SETUP #line 781 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.ps); ptype = 's'; if (wcsbthleng == 2) { BEGIN(TCn_ma); } else { extkey = "TPSn_ma"; BEGIN(TCCn_ma); } } YY_BREAK case 68: YY_RULE_SETUP #line 794 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.cname); extkey = "CNAMEia"; BEGIN(CCCCCia); } YY_BREAK case 69: #line 803 "wcsbth.l" case 70: YY_RULE_SETUP #line 803 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.cname); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "iCNAMn"; BEGIN(iCCCCn); } } YY_BREAK case 71: #line 819 "wcsbth.l" case 72: YY_RULE_SETUP #line 819 "wcsbth.l" { valtype = STRING; vptr = &(wcstem.cname); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "TCNAMn"; BEGIN(TCCCCn); } } YY_BREAK case 73: YY_RULE_SETUP #line 832 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crder); extkey = "CRDERia"; BEGIN(CCCCCia); } YY_BREAK case 74: #line 841 "wcsbth.l" case 75: YY_RULE_SETUP #line 841 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crder); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "iCRDEn"; BEGIN(iCCCCn); } } YY_BREAK case 76: #line 857 "wcsbth.l" case 77: YY_RULE_SETUP #line 857 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.crder); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "TCRDEn"; BEGIN(TCCCCn); } } YY_BREAK case 78: YY_RULE_SETUP #line 870 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.csyer); extkey = "CSYERia"; BEGIN(CCCCCia); } YY_BREAK case 79: #line 879 "wcsbth.l" case 80: YY_RULE_SETUP #line 879 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.csyer); sscanf(wcsbthtext, "%d", &i); if (wcsbthleng == 4) { BEGIN(iCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "iCSYEn"; BEGIN(iCCCCn); } } YY_BREAK case 81: #line 895 "wcsbth.l" case 82: YY_RULE_SETUP #line 895 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.csyer); if (wcsbthleng == 4) { BEGIN(TCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "TCSYEn"; BEGIN(TCCCCn); } } YY_BREAK case 83: #line 909 "wcsbth.l" case 84: YY_RULE_SETUP #line 909 "wcsbth.l" { valtype = STRING; vptr = wcstem.dateavg; if (wcsbthleng == 8) { extkey = "DATE-AVG"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCn); } } YY_BREAK case 85: YY_RULE_SETUP #line 921 "wcsbth.l" { valtype = STRING; vptr = wcstem.dateobs; extkey = "DATE-OBS"; BEGIN(CCCCCCCC); } YY_BREAK case 86: #line 930 "wcsbth.l" case 87: #line 931 "wcsbth.l" case 88: YY_RULE_SETUP #line 931 "wcsbth.l" { if (relax & WCSHDR_DOBSn) { valtype = STRING; vptr = wcstem.dateobs; yyless(4); BEGIN(CCCCn); } else { keytype = BINTAB; if (relax & WCSHDR_reject) { errmsg = "DOBSna keyword is non-standard"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } YY_BREAK case 89: YY_RULE_SETUP #line 950 "wcsbth.l" { sscanf(wcsbthtext, "EPOCH%c", &a); if (a == ' ' || (relax & WCSHDR_EPOCHa)) { valtype = FLOAT; vptr = &(wcstem.equinox); special = wcsbth_epoch; unput(a); extkey = "EPOCH"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "EPOCH keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } YY_BREAK case 90: #line 974 "wcsbth.l" case 91: YY_RULE_SETUP #line 974 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.equinox); if (wcsbthleng == 7) { extkey = "EQUINOXa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 92: #line 987 "wcsbth.l" case 93: YY_RULE_SETUP #line 987 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.mjdavg); if (wcsbthleng == 8) { extkey = "MJD-AVG"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCn); } } YY_BREAK case 94: #line 1000 "wcsbth.l" case 95: YY_RULE_SETUP #line 1000 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.mjdobs); if (wcsbthleng == 8) { extkey = "MJD-OBS"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } YY_BREAK case 96: #line 1013 "wcsbth.l" case 97: YY_RULE_SETUP #line 1013 "wcsbth.l" { valtype = FLOAT; vptr = wcstem.obsgeo; if (wcsbthleng == 8) { extkey = "OBSGEO-X"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } YY_BREAK case 98: #line 1026 "wcsbth.l" case 99: YY_RULE_SETUP #line 1026 "wcsbth.l" { valtype = FLOAT; vptr = wcstem.obsgeo + 1; if (wcsbthleng == 8) { extkey = "OBSGEO-Y"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } YY_BREAK case 100: #line 1039 "wcsbth.l" case 101: YY_RULE_SETUP #line 1039 "wcsbth.l" { valtype = FLOAT; vptr = wcstem.obsgeo + 2; if (wcsbthleng == 8) { extkey = "OBSGEO-Z"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } YY_BREAK case 102: #line 1052 "wcsbth.l" case 103: YY_RULE_SETUP #line 1052 "wcsbth.l" { valtype = STRING; vptr = wcstem.radesys; if (wcsbthleng == 7) { extkey = "RADESYSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 104: YY_RULE_SETUP #line 1064 "wcsbth.l" { if (relax & WCSHDR_RADECSYS) { valtype = STRING; vptr = wcstem.radesys; unput(' '); extkey = "RADECSYS"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "RADECSYS keyword is non-standard"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } YY_BREAK case 105: #line 1085 "wcsbth.l" case 106: YY_RULE_SETUP #line 1085 "wcsbth.l" { valtype = STRING; vptr = wcstem.specsys; if (wcsbthleng == 7) { extkey = "SPECSYSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 107: #line 1098 "wcsbth.l" case 108: YY_RULE_SETUP #line 1098 "wcsbth.l" { valtype = STRING; vptr = wcstem.ssysobs; if (wcsbthleng == 7) { extkey = "SSYSOBSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 109: #line 1111 "wcsbth.l" case 110: YY_RULE_SETUP #line 1111 "wcsbth.l" { valtype = STRING; vptr = wcstem.ssyssrc; if (wcsbthleng == 7) { extkey = "SSYSSRCa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 111: #line 1124 "wcsbth.l" case 112: YY_RULE_SETUP #line 1124 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.velosys); if (wcsbthleng == 7) { extkey = "VELOSYSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 113: #line 1137 "wcsbth.l" case 114: YY_RULE_SETUP #line 1137 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.velangl); if (wcsbthleng == 7) { extkey = "VELANGLa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 115: YY_RULE_SETUP #line 1149 "wcsbth.l" { sscanf(wcsbthtext, "VELREF%c", &a); if (a == ' ' || (relax & WCSHDR_VELREFa)) { valtype = INTEGER; vptr = &(wcstem.velref); unput(a); extkey = "VELREF"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "VELREF keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } YY_BREAK case 116: YY_RULE_SETUP #line 1171 "wcsbth.l" { if (relax & WCSHDR_VSOURCE) { valtype = FLOAT; vptr = &(wcstem.zsource); special = wcsbth_vsource; yyless(7); extkey = "VSOURCEa"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "VSOURCEa keyword is deprecated"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } YY_BREAK case 117: #line 1193 "wcsbth.l" case 118: #line 1194 "wcsbth.l" case 119: YY_RULE_SETUP #line 1194 "wcsbth.l" { if (relax & WCSHDR_VSOURCE) { valtype = FLOAT; vptr = &(wcstem.zsource); special = wcsbth_vsource; yyless(4); BEGIN(CCCCna); } else { keytype = BINTAB; if (relax & WCSHDR_reject) { errmsg = "VSOUna keyword is deprecated"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } } YY_BREAK case 120: #line 1216 "wcsbth.l" case 121: #line 1217 "wcsbth.l" case 122: YY_RULE_SETUP #line 1217 "wcsbth.l" { valtype = STRING; vptr = wcstem.wcsname; if (wcsbthleng == 7) { extkey = "WCSNAMEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 123: #line 1230 "wcsbth.l" case 124: YY_RULE_SETUP #line 1230 "wcsbth.l" { valtype = FLOAT; vptr = &(wcstem.zsource); if (wcsbthleng == 7) { extkey = "ZSOURCEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } YY_BREAK case 125: YY_RULE_SETUP #line 1242 "wcsbth.l" { yyless(0); if (wcsbth_nkeyrec) { wcsbth_nkeyrec = 0; errmsg = "Keyrecords following the END keyrecord were ignored"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 126: YY_RULE_SETUP #line 1253 "wcsbth.l" { yyless(0); BEGIN(DISCARD); } YY_BREAK case 127: #line 1259 "wcsbth.l" case 128: YY_RULE_SETUP #line 1259 "wcsbth.l" { /* Image-header keyword. */ keytype = IMGAXIS; if (relax & WCSHDR_ALLIMG) { sscanf(wcsbthtext, "%d%c", &i, &a); BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 129: YY_RULE_SETUP #line 1278 "wcsbth.l" { /* Invalid axis number in image-header keyword. */ keytype = IMGAXIS; if (relax & WCSHDR_ALLIMG) { /* Will also be flagged by as invalid. */ sscanf(wcsbthtext, "%3d", &i); BEGIN(VALUE); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 130: #line 1293 "wcsbth.l" case 131: #line 1294 "wcsbth.l" case 132: #line 1295 "wcsbth.l" case 133: #line 1296 "wcsbth.l" case 134: #line 1297 "wcsbth.l" case 135: YY_RULE_SETUP #line 1297 "wcsbth.l" { if (vptr) { WCSBTH_PUTBACK; BEGIN((YY_START == iCCCCn) ? iCCCna : TCCCna); } else { keytype = (YY_START == iCCCCn) ? BIMGARR : PIXLIST; if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword is non-standard", extkey); BEGIN(ERROR); } else { BEGIN(DISCARD); } } } YY_BREAK case 136: #line 1314 "wcsbth.l" case 137: #line 1315 "wcsbth.l" case 138: #line 1316 "wcsbth.l" case 139: YY_RULE_SETUP #line 1316 "wcsbth.l" { if (vptr && (relax & WCSHDR_LONGKEY)) { WCSBTH_PUTBACK; BEGIN((YY_START == iCCCCn) ? iCCCna : TCCCna); } else { keytype = (YY_START == iCCCna) ? BIMGARR : PIXLIST; if (relax & WCSHDR_reject) { errmsg = errtxt; if (!vptr) { sprintf(errmsg, "%s keyword is non-standard", extkey); } else { sprintf(errmsg, "%s keyword may not have an alternate version code", extkey); } BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } } YY_BREAK case 140: #line 1341 "wcsbth.l" case 141: YY_RULE_SETUP #line 1341 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 142: #line 1346 "wcsbth.l" case 143: #line 1347 "wcsbth.l" case 144: #line 1348 "wcsbth.l" case 145: #line 1349 "wcsbth.l" case 146: #line 1350 "wcsbth.l" case 147: YY_RULE_SETUP #line 1350 "wcsbth.l" { sscanf(wcsbthtext, "%d%c", &n, &a); if (YY_START == TCCCna) i = wcsbth_colax(*wcs, &alts, n, a); keytype = (YY_START == iCCCna) ? BIMGARR : PIXLIST; BEGIN(VALUE); } YY_BREAK case 148: #line 1358 "wcsbth.l" case 149: YY_RULE_SETUP #line 1358 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 150: #line 1363 "wcsbth.l" case 151: #line 1364 "wcsbth.l" case 152: #line 1365 "wcsbth.l" case 153: YY_RULE_SETUP #line 1365 "wcsbth.l" { /* Image-header keyword. */ if (relax & WCSHDR_ALLIMG) { sscanf(wcsbthtext, "%d_%d%c", &i, &j, &a); keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 154: #line 1385 "wcsbth.l" case 155: #line 1386 "wcsbth.l" case 156: #line 1387 "wcsbth.l" case 157: #line 1388 "wcsbth.l" case 158: #line 1389 "wcsbth.l" case 159: YY_RULE_SETUP #line 1389 "wcsbth.l" { /* Invalid axis number in image-header keyword. */ if (relax & WCSHDR_ALLIMG) { /* Will be flagged by as invalid. */ sscanf(wcsbthtext, "%d_%d", &i, &j); keytype = IMGAXIS; BEGIN(VALUE); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 160: YY_RULE_SETUP #line 1403 "wcsbth.l" { /* This covers the defunct forms CD00i00j and PC00i00j. */ if (((relax & WCSHDR_PC00i00j) && (altlin == 1)) || ((relax & WCSHDR_CD00i00j) && (altlin == 2))) { sscanf(wcsbthtext, "%3d%3d", &i, &j); a = ' '; keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Defunct form of %si_ja keyword", (altlin==1) ? "PC" : "CD"); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 161: YY_RULE_SETUP #line 1424 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 162: #line 1429 "wcsbth.l" case 163: #line 1430 "wcsbth.l" case 164: YY_RULE_SETUP #line 1430 "wcsbth.l" { sscanf(wcsbthtext, "%d%c", &n, &a); keytype = BIMGARR; BEGIN(VALUE); } YY_BREAK case 165: #line 1437 "wcsbth.l" case 166: #line 1438 "wcsbth.l" case 167: #line 1439 "wcsbth.l" case 168: #line 1440 "wcsbth.l" case 169: #line 1441 "wcsbth.l" case 170: YY_RULE_SETUP #line 1441 "wcsbth.l" { if (relax & WCSHDR_LONGKEY) { WCSBTH_PUTBACK; BEGIN(TCn_ka); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword is non-standard", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 171: YY_RULE_SETUP #line 1457 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 172: #line 1462 "wcsbth.l" case 173: #line 1463 "wcsbth.l" case 174: #line 1464 "wcsbth.l" case 175: #line 1465 "wcsbth.l" case 176: #line 1466 "wcsbth.l" case 177: YY_RULE_SETUP #line 1466 "wcsbth.l" { sscanf(wcsbthtext, "%d_%d%c", &n, &k, &a); i = wcsbth_colax(*wcs, &alts, n, a); j = wcsbth_colax(*wcs, &alts, k, a); keytype = PIXLIST; BEGIN(VALUE); } YY_BREAK case 178: #line 1475 "wcsbth.l" case 179: #line 1476 "wcsbth.l" case 180: #line 1477 "wcsbth.l" case 181: YY_RULE_SETUP #line 1477 "wcsbth.l" { sscanf(wcsbthtext, "%d_%d", &n, &k); a = ' '; i = wcsbth_colax(*wcs, &alts, n, a); j = wcsbth_colax(*wcs, &alts, k, a); keytype = PIXLIST; BEGIN(VALUE); } YY_BREAK case 182: YY_RULE_SETUP #line 1486 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 183: #line 1491 "wcsbth.l" case 184: YY_RULE_SETUP #line 1491 "wcsbth.l" { yyless(0); BEGIN(CCCCCia); } YY_BREAK case 185: #line 1497 "wcsbth.l" case 186: YY_RULE_SETUP #line 1497 "wcsbth.l" { if (relax & WCSHDR_CROTAia) { yyless(0); BEGIN(CCCCCia); } else if (relax & WCSHDR_reject) { errmsg = "CROTAn keyword may not have an alternate version code"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 187: YY_RULE_SETUP #line 1512 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 188: #line 1517 "wcsbth.l" case 189: #line 1518 "wcsbth.l" case 190: #line 1519 "wcsbth.l" case 191: #line 1520 "wcsbth.l" case 192: #line 1521 "wcsbth.l" case 193: YY_RULE_SETUP #line 1521 "wcsbth.l" { WCSBTH_PUTBACK; BEGIN((YY_START == iCROTn) ? iCCCna : TCCCna); } YY_BREAK case 194: #line 1527 "wcsbth.l" case 195: #line 1528 "wcsbth.l" case 196: #line 1529 "wcsbth.l" case 197: YY_RULE_SETUP #line 1529 "wcsbth.l" { if (relax & WCSHDR_CROTAia) { WCSBTH_PUTBACK; BEGIN((YY_START == iCROTn) ? iCCCna : TCCCna); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword may not have an alternate version code", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 198: #line 1547 "wcsbth.l" case 199: YY_RULE_SETUP #line 1547 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 200: #line 1552 "wcsbth.l" case 201: YY_RULE_SETUP #line 1552 "wcsbth.l" { /* Image-header keyword. */ if (relax & (WCSHDR_AUXIMG | WCSHDR_ALLIMG)) { if (YY_START == CCCCCCCa) { sscanf(wcsbthtext, "%c", &a); } else { a = 0; unput(wcsbthtext[0]); } keytype = IMGAUX; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 202: YY_RULE_SETUP #line 1576 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 203: #line 1581 "wcsbth.l" case 204: #line 1582 "wcsbth.l" case 205: #line 1583 "wcsbth.l" case 206: #line 1584 "wcsbth.l" case 207: YY_RULE_SETUP #line 1584 "wcsbth.l" { sscanf(wcsbthtext, "%d%c", &n, &a); keytype = BINTAB; BEGIN(VALUE); } YY_BREAK case 208: YY_RULE_SETUP #line 1590 "wcsbth.l" { sscanf(wcsbthtext, "%d", &n); a = ' '; keytype = BINTAB; BEGIN(VALUE); } YY_BREAK case 209: #line 1598 "wcsbth.l" case 210: YY_RULE_SETUP #line 1598 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 211: #line 1603 "wcsbth.l" case 212: #line 1604 "wcsbth.l" case 213: #line 1605 "wcsbth.l" case 214: #line 1606 "wcsbth.l" case 215: #line 1607 "wcsbth.l" case 216: #line 1608 "wcsbth.l" case 217: YY_RULE_SETUP #line 1608 "wcsbth.l" { sscanf(wcsbthtext, "%d", &n); a = 0; keytype = BINTAB; BEGIN(VALUE); } YY_BREAK case 218: #line 1616 "wcsbth.l" case 219: YY_RULE_SETUP #line 1616 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 220: #line 1621 "wcsbth.l" case 221: #line 1622 "wcsbth.l" case 222: #line 1623 "wcsbth.l" case 223: YY_RULE_SETUP #line 1623 "wcsbth.l" { /* Image-header keyword. */ if (relax & WCSHDR_ALLIMG) { sscanf(wcsbthtext, "%d_%d%c", &i, &m, &a); keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 224: #line 1643 "wcsbth.l" case 225: #line 1644 "wcsbth.l" case 226: #line 1645 "wcsbth.l" case 227: #line 1646 "wcsbth.l" case 228: #line 1647 "wcsbth.l" case 229: YY_RULE_SETUP #line 1647 "wcsbth.l" { /* Invalid parameter in image-header keyword. */ if (relax & WCSHDR_ALLIMG) { /* Will be flagged by as invalid. */ sscanf(wcsbthtext, "%d_%d", &i, &m); keytype = IMGAXIS; BEGIN(VALUE); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 230: YY_RULE_SETUP #line 1661 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 231: #line 1666 "wcsbth.l" case 232: #line 1667 "wcsbth.l" case 233: #line 1668 "wcsbth.l" case 234: #line 1669 "wcsbth.l" case 235: #line 1670 "wcsbth.l" case 236: #line 1671 "wcsbth.l" case 237: #line 1672 "wcsbth.l" case 238: #line 1673 "wcsbth.l" case 239: #line 1674 "wcsbth.l" case 240: #line 1675 "wcsbth.l" case 241: #line 1676 "wcsbth.l" case 242: YY_RULE_SETUP #line 1676 "wcsbth.l" { if (relax & WCSHDR_LONGKEY) { WCSBTH_PUTBACK; BEGIN((YY_START == iCCn_ma) ? iCn_ma : TCn_ma); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword is non-standard", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 243: #line 1693 "wcsbth.l" case 244: YY_RULE_SETUP #line 1693 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 245: #line 1698 "wcsbth.l" case 246: #line 1699 "wcsbth.l" case 247: #line 1700 "wcsbth.l" case 248: #line 1701 "wcsbth.l" case 249: #line 1702 "wcsbth.l" case 250: #line 1703 "wcsbth.l" case 251: #line 1704 "wcsbth.l" case 252: #line 1705 "wcsbth.l" case 253: #line 1706 "wcsbth.l" case 254: #line 1707 "wcsbth.l" case 255: #line 1708 "wcsbth.l" case 256: YY_RULE_SETUP #line 1708 "wcsbth.l" { sscanf(wcsbthtext, "%d_%d%c", &n, &m, &a); if (YY_START == TCn_ma) i = wcsbth_colax(*wcs, &alts, n, a); keytype = (YY_START == iCn_ma) ? BIMGARR : PIXLIST; BEGIN(VALUE); } YY_BREAK case 257: #line 1716 "wcsbth.l" case 258: #line 1717 "wcsbth.l" case 259: #line 1718 "wcsbth.l" case 260: #line 1719 "wcsbth.l" case 261: #line 1720 "wcsbth.l" case 262: #line 1721 "wcsbth.l" case 263: #line 1722 "wcsbth.l" case 264: YY_RULE_SETUP #line 1722 "wcsbth.l" { /* Invalid combinations will be flagged by . */ sscanf(wcsbthtext, "%d_%d", &n, &m); a = ' '; if (YY_START == TCn_ma) i = wcsbth_colax(*wcs, &alts, n, a); keytype = (YY_START == iCn_ma) ? BIMGARR : PIXLIST; BEGIN(VALUE); } YY_BREAK case 265: #line 1732 "wcsbth.l" case 266: YY_RULE_SETUP #line 1732 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 267: YY_RULE_SETUP #line 1736 "wcsbth.l" { if (relax & WCSHDR_PROJPn) { sscanf(wcsbthtext, "%d", &m); i = 0; a = ' '; keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = "PROJPn keyword is defunct"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } YY_BREAK case 268: YY_RULE_SETUP #line 1754 "wcsbth.l" { BEGIN(DISCARD); } YY_BREAK case 269: YY_RULE_SETUP #line 1758 "wcsbth.l" { /* Do checks on i, j, m, n, k. */ if (!(keytype & keysel)) { /* Selection by keyword type. */ BEGIN(DISCARD); } else if (exclude[n] || exclude[k]) { /* One or other column is not selected. */ if (k && (exclude[n] != exclude[k])) { /* For keywords such as TCn_ka, both columns must be excluded. User error, so return immediately. */ wcsbthlex_destroy(); return 3; } else { BEGIN(DISCARD); } } else if (i > 99 || j > 99 || m > 99 || n > 999 || k > 999) { if (relax & WCSHDR_reject) { errmsg = errtxt; if (i > 99 || j > 99) { sprintf(errmsg, "Axis number exceeds 99"); } else if (m > 99) { sprintf(errmsg, "Parameter number exceeds 99"); } else if (n > 999 || k > 999) { sprintf(errmsg, "Column number exceeds 999"); } BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } else if (ipass == 2 && npass == 3 && (keytype & BINTAB)) { /* Skip keyvalues that won't be inherited. */ BEGIN(FLUSH); } else if (ipass == 3 && (keytype & IMGHEAD)) { /* IMGHEAD keytypes are always dealt with on the second pass. */ BEGIN(FLUSH); } else if (vptr) { alts.icol = 0; alts.ialt = 0; voff = (char *)vptr - (char *)(&wcstem); if (valtype == INTEGER) { BEGIN(INTEGER_VAL); } else if (valtype == FLOAT) { BEGIN(FLOAT_VAL); } else if (valtype == STRING) { BEGIN(STRING_VAL); } else { errmsg = errtxt; sprintf(errmsg, "Internal parser ERROR, bad data type: %d", valtype); BEGIN(ERROR); } } else { errmsg = "Internal parser ERROR, null pointer"; BEGIN(ERROR); } } YY_BREAK case 270: YY_RULE_SETUP #line 1825 "wcsbth.l" { errmsg = "Invalid KEYWORD = VALUE syntax"; BEGIN(ERROR); } YY_BREAK case 271: YY_RULE_SETUP #line 1830 "wcsbth.l" { if (ipass == 1) { /* Do first-pass bookkeeping. */ wcsbth_pass1(keytype, i, j, n, k, a, ptype, &alts); BEGIN(FLUSH); } else { /* Update each coordinate representation. */ while ((wcsp = wcsbth_idx(*wcs, &alts, keytype, n, a))) { wptr = (void *)((char *)wcsp + voff); /* Read the keyvalue. */ if (special) { special(wptr); } else { sscanf(wcsbthtext, "%d", (int *)wptr); } } BEGIN(COMMENT); } } YY_BREAK case 272: YY_RULE_SETUP #line 1853 "wcsbth.l" { errmsg = "An integer value was expected"; BEGIN(ERROR); } YY_BREAK case 273: YY_RULE_SETUP #line 1858 "wcsbth.l" { if (ipass == 1) { /* Do first-pass bookkeeping. */ wcsbth_pass1(keytype, i, j, n, k, a, ptype, &alts); BEGIN(FLUSH); } else { /* Update each coordinate representation. */ while ((wcsp = wcsbth_idx(*wcs, &alts, keytype, n, a))) { wptr = (void *)((char *)wcsp + voff); /* Apply keyword parameterization. */ if (ptype == 'v') { ipx = wcsp->npv++; wcsp->pv[ipx].i = i; wcsp->pv[ipx].m = m; wptr = &(wcsp->pv[ipx].value); } else if (j) { /* Is the de-reference necessary? */ wptr = *((double **)wptr) + (i - 1)*(wcsp->naxis) + (j - 1); } else if (i) { wptr = *((double **)wptr) + (i - 1); } /* Read the keyvalue. */ if (special) { special(wptr); } else { sscanf(wcsbthtext, "%lf", (double *)wptr); } /* Flag the presence of PC, or CD and/or CROTA. */ if (altlin) { wcsp->altlin |= altlin; altlin = 0; } } BEGIN(COMMENT); } } YY_BREAK case 274: YY_RULE_SETUP #line 1902 "wcsbth.l" { errmsg = "A floating-point value was expected"; BEGIN(ERROR); } YY_BREAK case 275: /* rule 275 can match eol */ YY_RULE_SETUP #line 1907 "wcsbth.l" { if (ipass == 1) { /* Do first-pass bookkeeping. */ wcsbth_pass1(keytype, i, j, n, k, a, ptype, &alts); BEGIN(FLUSH); } else { /* Update each coordinate representation. */ while ((wcsp = wcsbth_idx(*wcs, &alts, keytype, n, a))) { wptr = (void *)((char *)wcsp + voff); /* Apply keyword parameterization. */ if (ptype == 's') { ipx = wcsp->nps++; wcsp->ps[ipx].i = i; wcsp->ps[ipx].m = m; wptr = wcsp->ps[ipx].value; } else if (j) { wptr = *((char (**)[72])wptr) + (i - 1)*(wcsp->naxis) + (j - 1); } else if (i) { wptr = *((char (**)[72])wptr) + (i - 1); } /* Read the keyvalue. */ cptr = (char *)wptr; strcpy(cptr, wcsbthtext+1); /* Squeeze out repeated quotes. */ ix = 0; for (jx = 0; jx < 72; jx++) { if (ix < jx) { cptr[ix] = cptr[jx]; } if (cptr[jx] == '\0') { if (ix) cptr[ix-1] = '\0'; break; } else if (cptr[jx] == '\'' && cptr[jx+1] == '\'') { jx++; } ix++; } } BEGIN(COMMENT); } } YY_BREAK case 276: YY_RULE_SETUP #line 1959 "wcsbth.l" { errmsg = "A string value was expected"; BEGIN(ERROR); } YY_BREAK case 277: #line 1965 "wcsbth.l" case 278: YY_RULE_SETUP #line 1965 "wcsbth.l" { BEGIN(FLUSH); } YY_BREAK case 279: YY_RULE_SETUP #line 1969 "wcsbth.l" { errmsg = "Malformed keycomment"; BEGIN(ERROR); } YY_BREAK case 280: YY_RULE_SETUP #line 1974 "wcsbth.l" { if (ipass == npass) { if (ctrl < 0) { /* Preserve discards. */ if (hptr < wcsbth_hdr-80) { strncpy(hptr, wcsbth_hdr-80, 80); } hptr += 80; } else if (ctrl > 2) { fprintf(stderr, "%.80s\n Discarded.\n", wcsbth_hdr-80); } } BEGIN(FLUSH); } YY_BREAK case 281: YY_RULE_SETUP #line 1991 "wcsbth.l" { (*nreject)++; if (ipass == npass) { if (ctrl == -1) { if (hptr < wcsbth_hdr-80) { /* Preserve rejects. */ strncpy(hptr, wcsbth_hdr-80, 80); } hptr += 80; } if (abs(ctrl) > 1) { fprintf(stderr, "%.80s\n%4d: %s.\n", wcsbth_hdr-80, *nreject, errmsg); } } BEGIN(FLUSH); } YY_BREAK case 282: /* rule 282 can match eol */ YY_RULE_SETUP #line 2011 "wcsbth.l" { /* Throw away the rest of the line and reset for the next one. */ i = j = 0; n = k = 0; m = 0; a = ' '; keytype = 0; valtype = -1; vptr = 0x0; altlin = 0; ptype = ' '; special = 0x0; BEGIN(INITIAL); } YY_BREAK case YY_STATE_EOF(INITIAL): case YY_STATE_EOF(CCCCCia): case YY_STATE_EOF(iCCCna): case YY_STATE_EOF(iCCCCn): case YY_STATE_EOF(TCCCna): case YY_STATE_EOF(TCCCCn): case YY_STATE_EOF(CCi_ja): case YY_STATE_EOF(ijCCna): case YY_STATE_EOF(TCn_ka): case YY_STATE_EOF(TCCn_ka): case YY_STATE_EOF(CROTAi): case YY_STATE_EOF(iCROTn): case YY_STATE_EOF(TCROTn): case YY_STATE_EOF(CCi_ma): case YY_STATE_EOF(iCn_ma): case YY_STATE_EOF(iCCn_ma): case YY_STATE_EOF(TCn_ma): case YY_STATE_EOF(TCCn_ma): case YY_STATE_EOF(PROJPm): case YY_STATE_EOF(CCCCCCCC): case YY_STATE_EOF(CCCCCCCa): case YY_STATE_EOF(CCCCna): case YY_STATE_EOF(CCCCCna): case YY_STATE_EOF(CCCCn): case YY_STATE_EOF(CCCCCn): case YY_STATE_EOF(VALUE): case YY_STATE_EOF(INTEGER_VAL): case YY_STATE_EOF(FLOAT_VAL): case YY_STATE_EOF(STRING_VAL): case YY_STATE_EOF(COMMENT): case YY_STATE_EOF(DISCARD): case YY_STATE_EOF(ERROR): case YY_STATE_EOF(FLUSH): #line 2028 "wcsbth.l" { /* End-of-input. */ if (ipass == 1) { if ((status = wcsbth_init1(&alts, nwcs, wcs)) || *nwcs == 0) { wcsbthlex_destroy(); return status; } if (alts.imgherit) npass = 3; if (abs(ctrl) > 2) { if (*nwcs == 1) { fprintf(stderr, "Found one coordinate representation.\n"); } else { fprintf(stderr, "Found %d coordinate representations.\n", *nwcs); } } } if (ipass++ < npass) { wcsbth_hdr = header; wcsbth_nkeyrec = nkeyrec; *nreject = 0; i = j = 0; k = n = 0; m = 0; a = ' '; keytype = 0; valtype = -1; vptr = 0x0; altlin = 0; ptype = ' '; special = 0x0; wcsbthrestart(wcsbthin); } else { wcsbthlex_destroy(); if (ctrl < 0) { *hptr = '\0'; } else if (ctrl == 1) { fprintf(stderr, "%d WCS keyrecords were rejected.\n", *nreject); } return wcsbth_final(&alts, nwcs, wcs); } } YY_BREAK case 283: YY_RULE_SETUP #line 2081 "wcsbth.l" ECHO; YY_BREAK #line 19589 "wcsbth.c" case YY_END_OF_BUFFER: { /* Amount of text matched not including the EOB char. */ int yy_amount_of_matched_text = (int) (yy_cp - (yytext_ptr)) - 1; /* Undo the effects of YY_DO_BEFORE_ACTION. */ *yy_cp = (yy_hold_char); YY_RESTORE_YY_MORE_OFFSET if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_NEW ) { /* We're scanning a new file or input source. It's * possible that this happened because the user * just pointed wcsbthin at a new source and called * wcsbthlex(). If so, then we have to assure * consistency between YY_CURRENT_BUFFER and our * globals. Here is the right place to do so, because * this is the first action (other than possibly a * back-up) that will match for the new input source. */ (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; YY_CURRENT_BUFFER_LVALUE->yy_input_file = wcsbthin; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_NORMAL; } /* Note that here we test for yy_c_buf_p "<=" to the position * of the first EOB in the buffer, since yy_c_buf_p will * already have been incremented past the NUL character * (since all states make transitions on EOB to the * end-of-buffer state). Contrast this with the test * in input(). */ if ( (yy_c_buf_p) <= &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) { /* This was really a NUL. */ yy_state_type yy_next_state; (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); /* Okay, we're now positioned to make the NUL * transition. We couldn't have * yy_get_previous_state() go ahead and do it * for us because it doesn't know how to deal * with the possibility of jamming (and we don't * want to build jamming into it because then it * will run more slowly). */ yy_next_state = yy_try_NUL_trans( yy_current_state ); yy_bp = (yytext_ptr) + YY_MORE_ADJ; if ( yy_next_state ) { /* Consume the NUL. */ yy_cp = ++(yy_c_buf_p); yy_current_state = yy_next_state; goto yy_match; } else { yy_cp = (yy_c_buf_p); goto yy_find_action; } } else switch ( yy_get_next_buffer( ) ) { case EOB_ACT_END_OF_FILE: { (yy_did_buffer_switch_on_eof) = 0; if ( wcsbthwrap( ) ) { /* Note: because we've taken care in * yy_get_next_buffer() to have set up * wcsbthtext, we can now set up * yy_c_buf_p so that if some total * hoser (like flex itself) wants to * call the scanner after we return the * YY_NULL, it'll still work - another * YY_NULL will get returned. */ (yy_c_buf_p) = (yytext_ptr) + YY_MORE_ADJ; yy_act = YY_STATE_EOF(YY_START); goto do_action; } else { if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; } break; } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_match; case EOB_ACT_LAST_MATCH: (yy_c_buf_p) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)]; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_find_action; } break; } default: YY_FATAL_ERROR( "fatal flex scanner internal error--no action found" ); } /* end of action switch */ } /* end of scanning one token */ } /* end of wcsbthlex */ /* yy_get_next_buffer - try to read in a new buffer * * Returns a code representing an action: * EOB_ACT_LAST_MATCH - * EOB_ACT_CONTINUE_SCAN - continue scanning from current position * EOB_ACT_END_OF_FILE - end of file */ static int yy_get_next_buffer (void) { register char *dest = YY_CURRENT_BUFFER_LVALUE->yy_ch_buf; register char *source = (yytext_ptr); register int number_to_move, i; int ret_val; if ( (yy_c_buf_p) > &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] ) YY_FATAL_ERROR( "fatal flex scanner internal error--end of buffer missed" ); if ( YY_CURRENT_BUFFER_LVALUE->yy_fill_buffer == 0 ) { /* Don't try to fill the buffer, so this is an EOF. */ if ( (yy_c_buf_p) - (yytext_ptr) - YY_MORE_ADJ == 1 ) { /* We matched a single character, the EOB, so * treat this as a final EOF. */ return EOB_ACT_END_OF_FILE; } else { /* We matched some text prior to the EOB, first * process it. */ return EOB_ACT_LAST_MATCH; } } /* Try to read more data. */ /* First move last chars to start of buffer. */ number_to_move = (int) ((yy_c_buf_p) - (yytext_ptr)) - 1; for ( i = 0; i < number_to_move; ++i ) *(dest++) = *(source++); if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_EOF_PENDING ) /* don't do the read, it's not guaranteed to return an EOF, * just force an EOF */ YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = 0; else { int num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; while ( num_to_read <= 0 ) { /* Not enough room in the buffer - grow it. */ /* just a shorter name for the current buffer */ YY_BUFFER_STATE b = YY_CURRENT_BUFFER; int yy_c_buf_p_offset = (int) ((yy_c_buf_p) - b->yy_ch_buf); if ( b->yy_is_our_buffer ) { int new_size = b->yy_buf_size * 2; if ( new_size <= 0 ) b->yy_buf_size += b->yy_buf_size / 8; else b->yy_buf_size *= 2; b->yy_ch_buf = (char *) /* Include room in for 2 EOB chars. */ wcsbthrealloc((void *) b->yy_ch_buf,b->yy_buf_size + 2 ); } else /* Can't grow it, we don't own it. */ b->yy_ch_buf = 0; if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "fatal error - scanner input buffer overflow" ); (yy_c_buf_p) = &b->yy_ch_buf[yy_c_buf_p_offset]; num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; } if ( num_to_read > YY_READ_BUF_SIZE ) num_to_read = YY_READ_BUF_SIZE; /* Read in more data. */ YY_INPUT( (&YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]), (yy_n_chars), (size_t) num_to_read ); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } if ( (yy_n_chars) == 0 ) { if ( number_to_move == YY_MORE_ADJ ) { ret_val = EOB_ACT_END_OF_FILE; wcsbthrestart(wcsbthin ); } else { ret_val = EOB_ACT_LAST_MATCH; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_EOF_PENDING; } } else ret_val = EOB_ACT_CONTINUE_SCAN; if ((yy_size_t) ((yy_n_chars) + number_to_move) > YY_CURRENT_BUFFER_LVALUE->yy_buf_size) { /* Extend the array by 50%, plus the number we really need. */ yy_size_t new_size = (yy_n_chars) + number_to_move + ((yy_n_chars) >> 1); YY_CURRENT_BUFFER_LVALUE->yy_ch_buf = (char *) wcsbthrealloc((void *) YY_CURRENT_BUFFER_LVALUE->yy_ch_buf,new_size ); if ( ! YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in yy_get_next_buffer()" ); } (yy_n_chars) += number_to_move; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] = YY_END_OF_BUFFER_CHAR; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] = YY_END_OF_BUFFER_CHAR; (yytext_ptr) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[0]; return ret_val; } /* yy_get_previous_state - get the state just before the EOB char was reached */ static yy_state_type yy_get_previous_state (void) { register yy_state_type yy_current_state; register char *yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); for ( yy_cp = (yytext_ptr) + YY_MORE_ADJ; yy_cp < (yy_c_buf_p); ++yy_cp ) { if ( *yy_cp ) { yy_current_state = yy_nxt[yy_current_state][YY_SC_TO_UI(*yy_cp)]; } else yy_current_state = yy_NUL_trans[yy_current_state]; if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_current_state; } /* yy_try_NUL_trans - try to make a transition on the NUL character * * synopsis * next_state = yy_try_NUL_trans( current_state ); */ static yy_state_type yy_try_NUL_trans (yy_state_type yy_current_state ) { register int yy_is_jam; register char *yy_cp = (yy_c_buf_p); yy_current_state = yy_NUL_trans[yy_current_state]; yy_is_jam = (yy_current_state == 0); if ( ! yy_is_jam ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_is_jam ? 0 : yy_current_state; } static void yyunput (int c, register char * yy_bp ) { register char *yy_cp; yy_cp = (yy_c_buf_p); /* undo effects of setting up wcsbthtext */ *yy_cp = (yy_hold_char); if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) { /* need to shift things up to make room */ /* +2 for EOB chars. */ register int number_to_move = (yy_n_chars) + 2; register char *dest = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[ YY_CURRENT_BUFFER_LVALUE->yy_buf_size + 2]; register char *source = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]; while ( source > YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) *--dest = *--source; yy_cp += (int) (dest - source); yy_bp += (int) (dest - source); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_buf_size; if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) YY_FATAL_ERROR( "flex scanner push-back overflow" ); } *--yy_cp = (char) c; (yytext_ptr) = yy_bp; (yy_hold_char) = *yy_cp; (yy_c_buf_p) = yy_cp; } #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void) #else static int input (void) #endif { int c; *(yy_c_buf_p) = (yy_hold_char); if ( *(yy_c_buf_p) == YY_END_OF_BUFFER_CHAR ) { /* yy_c_buf_p now points to the character we want to return. * If this occurs *before* the EOB characters, then it's a * valid NUL; if not, then we've hit the end of the buffer. */ if ( (yy_c_buf_p) < &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) /* This was really a NUL. */ *(yy_c_buf_p) = '\0'; else { /* need more input */ int offset = (yy_c_buf_p) - (yytext_ptr); ++(yy_c_buf_p); switch ( yy_get_next_buffer( ) ) { case EOB_ACT_LAST_MATCH: /* This happens because yy_g_n_b() * sees that we've accumulated a * token and flags that we need to * try matching the token before * proceeding. But for input(), * there's no matching to consider. * So convert the EOB_ACT_LAST_MATCH * to EOB_ACT_END_OF_FILE. */ /* Reset buffer status. */ wcsbthrestart(wcsbthin ); /*FALLTHROUGH*/ case EOB_ACT_END_OF_FILE: { if ( wcsbthwrap( ) ) return EOF; if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; #ifdef __cplusplus return yyinput(); #else return input(); #endif } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + offset; break; } } } c = *(unsigned char *) (yy_c_buf_p); /* cast for 8-bit char's */ *(yy_c_buf_p) = '\0'; /* preserve wcsbthtext */ (yy_hold_char) = *++(yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_at_bol = (c == '\n'); return c; } #endif /* ifndef YY_NO_INPUT */ /** Immediately switch to a different input stream. * @param input_file A readable stream. * * @note This function does not reset the start condition to @c INITIAL . */ void wcsbthrestart (FILE * input_file ) { if ( ! YY_CURRENT_BUFFER ){ wcsbthensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcsbth_create_buffer(wcsbthin,YY_BUF_SIZE ); } wcsbth_init_buffer(YY_CURRENT_BUFFER,input_file ); wcsbth_load_buffer_state( ); } /** Switch to a different input buffer. * @param new_buffer The new input buffer. * */ void wcsbth_switch_to_buffer (YY_BUFFER_STATE new_buffer ) { /* TODO. We should be able to replace this entire function body * with * wcsbthpop_buffer_state(); * wcsbthpush_buffer_state(new_buffer); */ wcsbthensure_buffer_stack (); if ( YY_CURRENT_BUFFER == new_buffer ) return; if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } YY_CURRENT_BUFFER_LVALUE = new_buffer; wcsbth_load_buffer_state( ); /* We don't actually know whether we did this switch during * EOF (wcsbthwrap()) processing, but the only time this flag * is looked at is after wcsbthwrap() is called, so it's safe * to go ahead and always set it. */ (yy_did_buffer_switch_on_eof) = 1; } static void wcsbth_load_buffer_state (void) { (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; (yytext_ptr) = (yy_c_buf_p) = YY_CURRENT_BUFFER_LVALUE->yy_buf_pos; wcsbthin = YY_CURRENT_BUFFER_LVALUE->yy_input_file; (yy_hold_char) = *(yy_c_buf_p); } /** Allocate and initialize an input buffer state. * @param file A readable stream. * @param size The character buffer size in bytes. When in doubt, use @c YY_BUF_SIZE. * * @return the allocated buffer state. */ YY_BUFFER_STATE wcsbth_create_buffer (FILE * file, int size ) { YY_BUFFER_STATE b; b = (YY_BUFFER_STATE) wcsbthalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcsbth_create_buffer()" ); b->yy_buf_size = size; /* yy_ch_buf has to be 2 characters longer than the size given because * we need to put in 2 end-of-buffer characters. */ b->yy_ch_buf = (char *) wcsbthalloc(b->yy_buf_size + 2 ); if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in wcsbth_create_buffer()" ); b->yy_is_our_buffer = 1; wcsbth_init_buffer(b,file ); return b; } /** Destroy the buffer. * @param b a buffer created with wcsbth_create_buffer() * */ void wcsbth_delete_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; if ( b == YY_CURRENT_BUFFER ) /* Not sure if we should pop here. */ YY_CURRENT_BUFFER_LVALUE = (YY_BUFFER_STATE) 0; if ( b->yy_is_our_buffer ) wcsbthfree((void *) b->yy_ch_buf ); wcsbthfree((void *) b ); } /* Initializes or reinitializes a buffer. * This function is sometimes called more than once on the same buffer, * such as during a wcsbthrestart() or at EOF. */ static void wcsbth_init_buffer (YY_BUFFER_STATE b, FILE * file ) { int oerrno = errno; wcsbth_flush_buffer(b ); b->yy_input_file = file; b->yy_fill_buffer = 1; /* If b is the current buffer, then wcsbth_init_buffer was _probably_ * called from wcsbthrestart() or through yy_get_next_buffer. * In that case, we don't want to reset the lineno or column. */ if (b != YY_CURRENT_BUFFER){ b->yy_bs_lineno = 1; b->yy_bs_column = 0; } b->yy_is_interactive = 0; errno = oerrno; } /** Discard all buffered characters. On the next scan, YY_INPUT will be called. * @param b the buffer state to be flushed, usually @c YY_CURRENT_BUFFER. * */ void wcsbth_flush_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; b->yy_n_chars = 0; /* We always need two end-of-buffer characters. The first causes * a transition to the end-of-buffer state. The second causes * a jam in that state. */ b->yy_ch_buf[0] = YY_END_OF_BUFFER_CHAR; b->yy_ch_buf[1] = YY_END_OF_BUFFER_CHAR; b->yy_buf_pos = &b->yy_ch_buf[0]; b->yy_at_bol = 1; b->yy_buffer_status = YY_BUFFER_NEW; if ( b == YY_CURRENT_BUFFER ) wcsbth_load_buffer_state( ); } /** Pushes the new state onto the stack. The new state becomes * the current state. This function will allocate the stack * if necessary. * @param new_buffer The new state. * */ void wcsbthpush_buffer_state (YY_BUFFER_STATE new_buffer ) { if (new_buffer == NULL) return; wcsbthensure_buffer_stack(); /* This block is copied from wcsbth_switch_to_buffer. */ if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } /* Only push if top exists. Otherwise, replace top. */ if (YY_CURRENT_BUFFER) (yy_buffer_stack_top)++; YY_CURRENT_BUFFER_LVALUE = new_buffer; /* copied from wcsbth_switch_to_buffer. */ wcsbth_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } /** Removes and deletes the top of the stack, if present. * The next element becomes the new top. * */ void wcsbthpop_buffer_state (void) { if (!YY_CURRENT_BUFFER) return; wcsbth_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; if ((yy_buffer_stack_top) > 0) --(yy_buffer_stack_top); if (YY_CURRENT_BUFFER) { wcsbth_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } } /* Allocates the stack if it does not exist. * Guarantees space for at least one push. */ static void wcsbthensure_buffer_stack (void) { int num_to_alloc; if (!(yy_buffer_stack)) { /* First allocation is just for 2 elements, since we don't know if this * scanner will even need a stack. We use 2 instead of 1 to avoid an * immediate realloc on the next call. */ num_to_alloc = 1; (yy_buffer_stack) = (struct yy_buffer_state**)wcsbthalloc (num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcsbthensure_buffer_stack()" ); memset((yy_buffer_stack), 0, num_to_alloc * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; (yy_buffer_stack_top) = 0; return; } if ((yy_buffer_stack_top) >= ((yy_buffer_stack_max)) - 1){ /* Increase the buffer to prepare for a possible push. */ int grow_size = 8 /* arbitrary grow size */; num_to_alloc = (yy_buffer_stack_max) + grow_size; (yy_buffer_stack) = (struct yy_buffer_state**)wcsbthrealloc ((yy_buffer_stack), num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcsbthensure_buffer_stack()" ); /* zero only the new slots.*/ memset((yy_buffer_stack) + (yy_buffer_stack_max), 0, grow_size * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; } } /** Setup the input buffer state to scan directly from a user-specified character buffer. * @param base the character buffer * @param size the size in bytes of the character buffer * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcsbth_scan_buffer (char * base, yy_size_t size ) { YY_BUFFER_STATE b; if ( size < 2 || base[size-2] != YY_END_OF_BUFFER_CHAR || base[size-1] != YY_END_OF_BUFFER_CHAR ) /* They forgot to leave room for the EOB's. */ return 0; b = (YY_BUFFER_STATE) wcsbthalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcsbth_scan_buffer()" ); b->yy_buf_size = size - 2; /* "- 2" to take care of EOB's */ b->yy_buf_pos = b->yy_ch_buf = base; b->yy_is_our_buffer = 0; b->yy_input_file = 0; b->yy_n_chars = b->yy_buf_size; b->yy_is_interactive = 0; b->yy_at_bol = 1; b->yy_fill_buffer = 0; b->yy_buffer_status = YY_BUFFER_NEW; wcsbth_switch_to_buffer(b ); return b; } /** Setup the input buffer state to scan a string. The next call to wcsbthlex() will * scan from a @e copy of @a str. * @param yystr a NUL-terminated string to scan * * @return the newly allocated buffer state object. * @note If you want to scan bytes that may contain NUL values, then use * wcsbth_scan_bytes() instead. */ YY_BUFFER_STATE wcsbth_scan_string (yyconst char * yystr ) { return wcsbth_scan_bytes(yystr,strlen(yystr) ); } /** Setup the input buffer state to scan the given bytes. The next call to wcsbthlex() will * scan from a @e copy of @a bytes. * @param yybytes the byte buffer to scan * @param _yybytes_len the number of bytes in the buffer pointed to by @a bytes. * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcsbth_scan_bytes (yyconst char * yybytes, int _yybytes_len ) { YY_BUFFER_STATE b; char *buf; yy_size_t n; int i; /* Get memory for full buffer, including space for trailing EOB's. */ n = _yybytes_len + 2; buf = (char *) wcsbthalloc(n ); if ( ! buf ) YY_FATAL_ERROR( "out of dynamic memory in wcsbth_scan_bytes()" ); for ( i = 0; i < _yybytes_len; ++i ) buf[i] = yybytes[i]; buf[_yybytes_len] = buf[_yybytes_len+1] = YY_END_OF_BUFFER_CHAR; b = wcsbth_scan_buffer(buf,n ); if ( ! b ) YY_FATAL_ERROR( "bad buffer in wcsbth_scan_bytes()" ); /* It's okay to grow etc. this buffer, and we should throw it * away when we're done. */ b->yy_is_our_buffer = 1; return b; } #ifndef YY_EXIT_FAILURE #define YY_EXIT_FAILURE 2 #endif static void yy_fatal_error (yyconst char* msg ) { (void) fprintf( stderr, "%s\n", msg ); exit( YY_EXIT_FAILURE ); } /* Redefine yyless() so it works in section 3 code. */ #undef yyless #define yyless(n) \ do \ { \ /* Undo effects of setting up wcsbthtext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ wcsbthtext[wcsbthleng] = (yy_hold_char); \ (yy_c_buf_p) = wcsbthtext + yyless_macro_arg; \ (yy_hold_char) = *(yy_c_buf_p); \ *(yy_c_buf_p) = '\0'; \ wcsbthleng = yyless_macro_arg; \ } \ while ( 0 ) /* Accessor methods (get/set functions) to struct members. */ /** Get the current line number. * */ int wcsbthget_lineno (void) { return wcsbthlineno; } /** Get the input stream. * */ FILE *wcsbthget_in (void) { return wcsbthin; } /** Get the output stream. * */ FILE *wcsbthget_out (void) { return wcsbthout; } /** Get the length of the current token. * */ int wcsbthget_leng (void) { return wcsbthleng; } /** Get the current token. * */ char *wcsbthget_text (void) { return wcsbthtext; } /** Set the current line number. * @param line_number * */ void wcsbthset_lineno (int line_number ) { wcsbthlineno = line_number; } /** Set the input stream. This does not discard the current * input buffer. * @param in_str A readable stream. * * @see wcsbth_switch_to_buffer */ void wcsbthset_in (FILE * in_str ) { wcsbthin = in_str ; } void wcsbthset_out (FILE * out_str ) { wcsbthout = out_str ; } int wcsbthget_debug (void) { return wcsbth_flex_debug; } void wcsbthset_debug (int bdebug ) { wcsbth_flex_debug = bdebug ; } static int yy_init_globals (void) { /* Initialization is the same as for the non-reentrant scanner. * This function is called from wcsbthlex_destroy(), so don't allocate here. */ (yy_buffer_stack) = 0; (yy_buffer_stack_top) = 0; (yy_buffer_stack_max) = 0; (yy_c_buf_p) = (char *) 0; (yy_init) = 0; (yy_start) = 0; /* Defined in main.c */ #ifdef YY_STDINIT wcsbthin = stdin; wcsbthout = stdout; #else wcsbthin = (FILE *) 0; wcsbthout = (FILE *) 0; #endif /* For future reference: Set errno on error, since we are called by * wcsbthlex_init() */ return 0; } /* wcsbthlex_destroy is for both reentrant and non-reentrant scanners. */ int wcsbthlex_destroy (void) { /* Pop the buffer stack, destroying each element. */ while(YY_CURRENT_BUFFER){ wcsbth_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; wcsbthpop_buffer_state(); } /* Destroy the stack itself. */ wcsbthfree((yy_buffer_stack) ); (yy_buffer_stack) = NULL; /* Reset the globals. This is important in a non-reentrant scanner so the next time * wcsbthlex() is called, initialization will occur. */ yy_init_globals( ); return 0; } /* * Internal utility routines. */ #ifndef yytext_ptr static void yy_flex_strncpy (char* s1, yyconst char * s2, int n ) { register int i; for ( i = 0; i < n; ++i ) s1[i] = s2[i]; } #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * s ) { register int n; for ( n = 0; s[n]; ++n ) ; return n; } #endif void *wcsbthalloc (yy_size_t size ) { return (void *) malloc( size ); } void *wcsbthrealloc (void * ptr, yy_size_t size ) { /* The cast to (char *) in the following accommodates both * implementations that use char* generic pointers, and those * that use void* generic pointers. It works with the latter * because both ANSI C and C++ allow castless assignment from * any pointer type to void*, and deal with argument conversions * as though doing an assignment. */ return (void *) realloc( (char *) ptr, size ); } void wcsbthfree (void * ptr ) { free( (char *) ptr ); /* see wcsbthrealloc() for (char *) cast */ } #define YYTABLES_NAME "yytables" #line 2081 "wcsbth.l" /*---------------------------------------------------------------------------- * Perform first-pass tasks: * * 1) Count the number of coordinate axes in each of the 27 possible alternate * image-header coordinate representations. Also count the number of PVi_ma * and PSi_ma keywords in each representation. * * 2) Determine the number of binary table columns that have an image array * with a coordinate representation (up to 999), and count the number of * coordinate axes in each of the 27 possible alternates. Also count the * number of iVn_ma and iSn_ma keywords in each representation. * * 3) Determine the number of alternate pixel list coordinate representations * (up to 27) and the table columns associated with each. Also count the * number of TVn_ma and TSn_ma keywords in each representation. * * In the first pass alts->arridx[icol][27] is used to determine the number of * axes in each of 27 possible image-header coordinate descriptions (icol == 0) * and each of the 27 possible coordinate representations for an image array in * each column. * * The elements of alts->pixlist[icol] are used as bit arrays to flag which of * the 27 possible pixel list coordinate representations are associated with * each table column. *---------------------------------------------------------------------------*/ int wcsbth_pass1( int keytype, int i, int j, int n, int k, char a, char ptype, struct wcsbth_alts *alts) { int ialt, icol, mask, ncol; if (a == 0) { /* Keywords such as DATE-OBS go along for the ride. */ return 0; } ncol = alts->ncol; /* Do we need to allocate memory for alts? */ if (alts->arridx == 0x0) { if (ncol == 0) { /* Can only happen if TFIELDS is missing or out-of-sequence. If n and k are both zero then we may be processing an image header so leave ncol alone - the array will be realloc'd later if required. */ if (n || k) { /* The header is mangled, assume the worst. */ ncol = 999; } } if (!(alts->arridx = calloc((1 + ncol)*27, sizeof(short int))) || !(alts->npv = calloc((1 + ncol)*27, sizeof(unsigned char))) || !(alts->nps = calloc((1 + ncol)*27, sizeof(unsigned char))) || !(alts->pixlist = calloc((1 + ncol), sizeof(unsigned int)))) { if (alts->arridx) free(alts->arridx); if (alts->npv) free(alts->npv); if (alts->nps) free(alts->nps); if (alts->pixlist) free(alts->pixlist); return 2; } alts->ncol = ncol; } else if (n > ncol || k > ncol) { /* Can only happen if TFIELDS or the WCS keyword is wrong; carry on. */ ncol = 999; if (!(alts->arridx = realloc(alts->arridx, 27*(1 + ncol)*sizeof(short int))) || !(alts->npv = realloc(alts->npv, 27*(1 + ncol)*sizeof(unsigned char))) || !(alts->nps = realloc(alts->nps, 27*(1 + ncol)*sizeof(unsigned char))) || !(alts->pixlist = realloc(alts->pixlist, (1 + ncol)*sizeof(unsigned int)))) { if (alts->arridx) free(alts->arridx); if (alts->npv) free(alts->npv); if (alts->nps) free(alts->nps); if (alts->pixlist) free(alts->pixlist); return 2; } /* Since realloc() doesn't initialize the extra memory. */ for (icol = (1 + alts->ncol); icol < (1 + ncol); icol++) { for (ialt = 0; ialt < 27; ialt++) { alts->arridx[icol][ialt] = 0; alts->npv[icol][ialt] = 0; alts->nps[icol][ialt] = 0; alts->pixlist[icol] = 0; } } alts->ncol = ncol; } ialt = 0; if (a != ' ') { ialt = a - 'A' + 1; } /* A BINTAB keytype such as LONPna, in conjunction with an IMGAXIS keytype causes a table column to be recognized as an image array. */ if (keytype & IMGHEAD || keytype & BIMGARR) { /* n == 0 is expected for IMGHEAD keywords. */ if (i == 0 && j == 0) { if (alts->arridx[n][ialt] == 0) { /* Flag that an auxiliary keyword was seen. */ alts->arridx[n][ialt] = -1; } } else { /* Record the maximum axis number found. */ if (alts->arridx[n][ialt] < i) { alts->arridx[n][ialt] = i; } if (alts->arridx[n][ialt] < j) { alts->arridx[n][ialt] = j; } } if (ptype == 'v') { alts->npv[n][ialt]++; } else if (ptype == 's') { alts->nps[n][ialt]++; } } /* BINTAB keytypes, which apply both to pixel lists as well as binary table image arrays, never contribute to recognizing a table column as a pixel list axis. A PIXLIST keytype is required for that. */ if (keytype == PIXLIST) { mask = 1 << ialt; /* n > 0 for PIXLIST keytypes. */ alts->pixlist[n] |= mask; if (k) alts->pixlist[k] |= mask; /* Used as a flag over all columns. */ alts->pixlist[0] |= mask; if (ptype == 'v') { alts->pixnpv[ialt]++; } else if (ptype == 's') { alts->pixnps[ialt]++; } } return 0; } /*---------------------------------------------------------------------------- * Perform initializations at the end of the first pass: * * 1) Determine the required number of wcsprm structs, allocate memory for * an array of them and initialize each one. *---------------------------------------------------------------------------*/ int wcsbth_init1( struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs) { int ialt, icol, inherit[27], ix, mask, ncol, npsmax, npvmax, status = 0; struct wcsprm *wcsp; if (alts->arridx == 0x0) { *nwcs = 0; return 0; } /* Determine the number of axes in each pixel list representation. */ ncol = alts->ncol; for (ialt = 0, mask = 1; ialt < 27; ialt++, mask <<= 1) { alts->pixidx[ialt] = 0; if (alts->pixlist[0] | mask) { for (icol = 1; icol <= ncol; icol++) { if (alts->pixlist[icol] & mask) { alts->pixidx[ialt]++; } } } } /* Find the total number of coordinate representations. */ *nwcs = 0; alts->imgherit = 0; for (ialt = 0; ialt < 27; ialt++) { inherit[ialt] = 0; for (icol = 1; icol <= ncol; icol++) { if (alts->arridx[icol][ialt] < 0) { /* No BIMGARR keytype but there's at least one BINTAB. */ if (alts->arridx[0][ialt] > 0) { /* There is an IMGAXIS keytype that we will inherit, so count this representation. */ alts->arridx[icol][ialt] = alts->arridx[0][ialt]; } else { alts->arridx[icol][ialt] = 0; } } if (alts->arridx[icol][ialt]) { if (alts->arridx[0][ialt]) { /* All IMGHEAD keywords are inherited for this ialt. */ inherit[ialt] = 1; if (alts->arridx[icol][ialt] < alts->arridx[0][ialt]) { /* The extra axes are also inherited. */ alts->arridx[icol][ialt] = alts->arridx[0][ialt]; } } (*nwcs)++; } } /* Count every "a" found in any IMGHEAD keyword... */ if (alts->arridx[0][ialt]) { if (inherit[ialt]) { /* ...but not if the IMGHEAD keywords will be inherited. */ alts->arridx[0][ialt] = 0; alts->imgherit = 1; } else { (*nwcs)++; } } /* We need a struct for every "a" found in a PIXLIST keyword. */ if (alts->pixidx[ialt]) { (*nwcs)++; } } if (*nwcs) { /* Allocate memory for the required number of wcsprm structs. */ if (!(*wcs = calloc(*nwcs, sizeof(struct wcsprm)))) { return 2; } /* Record the current values of NPVMAX and NPSMAX. */ npvmax = wcsnpv(-1); npsmax = wcsnps(-1); /* Initialize each wcsprm struct. */ wcsp = *wcs; *nwcs = 0; for (icol = 0; icol <= ncol; icol++) { for (ialt = 0; ialt < 27; ialt++) { if (alts->arridx[icol][ialt]) { /* Image-header representations that are not for inheritance (icol == 0) or binary table image array representations. */ wcsp->flag = -1; wcsnpv(alts->npv[icol][ialt]); wcsnps(alts->nps[icol][ialt]); if ((status = wcsini(1, (int)(alts->arridx[icol][ialt]), wcsp))) { wcsvfree(nwcs, wcs); break; } /* Record the alternate version code. */ if (ialt) { wcsp->alt[0] = 'A' + ialt - 1; } /* Record the table column number. */ wcsp->colnum = icol; /* On the second pass alts->arridx[icol][27] indexes the array of wcsprm structs. */ alts->arridx[icol][ialt] = (*nwcs)++; wcsp++; } else { /* Signal that this column has no WCS for this "a". */ alts->arridx[icol][ialt] = -1; } } } for (ialt = 0; ialt < 27; ialt++) { if (alts->pixidx[ialt]) { /* Pixel lists representations. */ wcsp->flag = -1; wcsnpv(alts->pixnpv[ialt]); wcsnps(alts->pixnps[ialt]); if ((status = wcsini(1, (int)(alts->pixidx[ialt]), wcsp))) { wcsvfree(nwcs, wcs); break; } /* Record the alternate version code. */ if (ialt) { wcsp->alt[0] = 'A' + ialt - 1; } /* Record the pixel list column numbers. */ mask = (1 << ialt); for (icol = 1, ix = 0; icol <= ncol; icol++) { if (alts->pixlist[icol] & mask) { wcsp->colax[ix++] = icol; } } /* alts->pixidx[] indexes the array of wcsprm structs. */ alts->pixidx[ialt] = (*nwcs)++; wcsp++; } else { /* Signal that this column is not a pixel list axis for this "a". */ alts->pixidx[ialt] = -1; } } /* Restore the original values of NPVMAX and NPSMAX. */ wcsnpv(npvmax); wcsnps(npsmax); } return status; } /*---------------------------------------------------------------------------- * Return a pointer to the next wcsprm struct for a particular column number * and alternate. *---------------------------------------------------------------------------*/ struct wcsprm *wcsbth_idx( struct wcsprm *wcs, struct wcsbth_alts *alts, int keytype, int n, char a) { const char as[] = " ABCDEFGHIJKLMNOPQRSTUVWXYZ"; int iwcs; if (!wcs) return 0x0; iwcs = -1; for (; iwcs < 0 && alts->ialt < 27; alts->ialt++) { /* Note that a == 0 applies to every alternate, otherwise this loop simply determines the appropriate value of alts->ialt. */ if (a && a != as[alts->ialt]) continue; if (keytype & (IMGHEAD | BIMGARR)) { for (; iwcs < 0 && alts->icol <= alts->ncol; alts->icol++) { /* Image header keywords, n == 0, apply to all columns, otherwise this loop simply determines the appropriate value of alts->icol. */ if (n && n != alts->icol) continue; iwcs = alts->arridx[alts->icol][alts->ialt]; } /* Break out of the loop to stop alts->ialt from being incremented. */ if (iwcs >= 0) break; /* Start from scratch for the next alts->ialt. */ alts->icol = 0; } if (keytype & (IMGAUX | PIXLIST)) { iwcs = alts->pixidx[alts->ialt]; } } return (iwcs >= 0) ? (wcs + iwcs) : 0x0; } /*---------------------------------------------------------------------------- * Return the axis number associated with the specified column number in a * particular pixel list coordinate representation. *---------------------------------------------------------------------------*/ int wcsbth_colax( struct wcsprm *wcs, struct wcsbth_alts *alts, int n, char a) { int ix; struct wcsprm *wcsp; if (!wcs) return 0; wcsp = wcs; if (a != ' ') { wcsp += alts->pixidx[a-'A'+1]; } for (ix = 0; ix < wcsp->naxis; ix++) { if (wcsp->colax[ix] == n) { return ++ix; } } return 0; } /*---------------------------------------------------------------------------- * Interpret EPOCH keywords. *---------------------------------------------------------------------------*/ int wcsbth_epoch(void *wptr) { double *equinox; /* If EQUINOXa is currently undefined then set it from EPOCHa. */ equinox = (double *)wptr; if (undefined(*equinox)) { sscanf(wcsbthtext, "%lf", equinox); } return 0; } /*---------------------------------------------------------------------------- * Interpret VSOURCE keywords. *---------------------------------------------------------------------------*/ int wcsbth_vsource(void *wptr) { double beta, c = 299792458.0, vsource, *zsource; /* If ZSOURCEa is currently undefined then set it from VSOURCEa. */ zsource = (double *)wptr; if (undefined(*zsource)) { sscanf(wcsbthtext, "%lf", &vsource); /* Convert relativistic Doppler velocity to redshift. */ beta = vsource/c; *zsource = (1.0 + beta)/sqrt(1.0 - beta*beta) - 1.0; } return 0; } /*---------------------------------------------------------------------------- * Tie up loose ends. *---------------------------------------------------------------------------*/ int wcsbth_final( struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs) { int ialt, status; if (alts->arridx) free(alts->arridx); if (alts->npv) free(alts->npv); if (alts->nps) free(alts->nps); if (alts->pixlist) free(alts->pixlist); for (ialt = 0; ialt < *nwcs; ialt++) { /* Interpret -TAB header keywords. */ if ((status = wcstab(*wcs+ialt))) { wcsvfree(nwcs, wcs); return status; } } return 0; } pywcs-1.12/wcslib/C/flexed/wcspih.c0000644001153600020070000156073712310355626021246 0ustar cslocumSTSCI\science00000000000000#line 2 "wcspih.c" #line 4 "wcspih.c" #define YY_INT_ALIGNED short int /* A lexical scanner generated by flex */ #define yy_create_buffer wcspih_create_buffer #define yy_delete_buffer wcspih_delete_buffer #define yy_flex_debug wcspih_flex_debug #define yy_init_buffer wcspih_init_buffer #define yy_flush_buffer wcspih_flush_buffer #define yy_load_buffer_state wcspih_load_buffer_state #define yy_switch_to_buffer wcspih_switch_to_buffer #define yyin wcspihin #define yyleng wcspihleng #define yylex wcspihlex #define yylineno wcspihlineno #define yyout wcspihout #define yyrestart wcspihrestart #define yytext wcspihtext #define yywrap wcspihwrap #define yyalloc wcspihalloc #define yyrealloc wcspihrealloc #define yyfree wcspihfree #define FLEX_SCANNER #define YY_FLEX_MAJOR_VERSION 2 #define YY_FLEX_MINOR_VERSION 5 #define YY_FLEX_SUBMINOR_VERSION 35 #if YY_FLEX_SUBMINOR_VERSION > 0 #define FLEX_BETA #endif /* First, we deal with platform-specific or compiler-specific issues. */ /* begin standard C headers. */ #include #include #include #include /* end standard C headers. */ /* flex integer type definitions */ #ifndef FLEXINT_H #define FLEXINT_H /* C99 systems have . Non-C99 systems may or may not. */ #if defined (__STDC_VERSION__) && __STDC_VERSION__ >= 199901L /* C99 says to define __STDC_LIMIT_MACROS before including stdint.h, * if you want the limit (max/min) macros for int types. */ #ifndef __STDC_LIMIT_MACROS #define __STDC_LIMIT_MACROS 1 #endif #include typedef int8_t flex_int8_t; typedef uint8_t flex_uint8_t; typedef int16_t flex_int16_t; typedef uint16_t flex_uint16_t; typedef int32_t flex_int32_t; typedef uint32_t flex_uint32_t; #else typedef signed char flex_int8_t; typedef short int flex_int16_t; typedef int flex_int32_t; typedef unsigned char flex_uint8_t; typedef unsigned short int flex_uint16_t; typedef unsigned int flex_uint32_t; /* Limits of integral types. */ #ifndef INT8_MIN #define INT8_MIN (-128) #endif #ifndef INT16_MIN #define INT16_MIN (-32767-1) #endif #ifndef INT32_MIN #define INT32_MIN (-2147483647-1) #endif #ifndef INT8_MAX #define INT8_MAX (127) #endif #ifndef INT16_MAX #define INT16_MAX (32767) #endif #ifndef INT32_MAX #define INT32_MAX (2147483647) #endif #ifndef UINT8_MAX #define UINT8_MAX (255U) #endif #ifndef UINT16_MAX #define UINT16_MAX (65535U) #endif #ifndef UINT32_MAX #define UINT32_MAX (4294967295U) #endif #endif /* ! C99 */ #endif /* ! FLEXINT_H */ #ifdef __cplusplus /* The "const" storage-class-modifier is valid. */ #define YY_USE_CONST #else /* ! __cplusplus */ /* C99 requires __STDC__ to be defined as 1. */ #if defined (__STDC__) #define YY_USE_CONST #endif /* defined (__STDC__) */ #endif /* ! __cplusplus */ #ifdef YY_USE_CONST #define yyconst const #else #define yyconst #endif /* Returned upon end-of-file. */ #define YY_NULL 0 /* Promotes a possibly negative, possibly signed char to an unsigned * integer for use as an array index. If the signed char is negative, * we want to instead treat it as an 8-bit unsigned char, hence the * double cast. */ #define YY_SC_TO_UI(c) ((unsigned int) (unsigned char) c) /* Enter a start condition. This macro really ought to take a parameter, * but we do it the disgusting crufty way forced on us by the ()-less * definition of BEGIN. */ #define BEGIN (yy_start) = 1 + 2 * /* Translate the current start state into a value that can be later handed * to BEGIN to return to the state. The YYSTATE alias is for lex * compatibility. */ #define YY_START (((yy_start) - 1) / 2) #define YYSTATE YY_START /* Action number for EOF rule of a given start state. */ #define YY_STATE_EOF(state) (YY_END_OF_BUFFER + state + 1) /* Special action meaning "start processing a new file". */ #define YY_NEW_FILE wcspihrestart(wcspihin ) #define YY_END_OF_BUFFER_CHAR 0 /* Size of default input buffer. */ #ifndef YY_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k. * Moreover, YY_BUF_SIZE is 2*YY_READ_BUF_SIZE in the general case. * Ditto for the __ia64__ case accordingly. */ #define YY_BUF_SIZE 32768 #else #define YY_BUF_SIZE 16384 #endif /* __ia64__ */ #endif /* The state buf must be large enough to hold one state per character in the main buffer. */ #define YY_STATE_BUF_SIZE ((YY_BUF_SIZE + 2) * sizeof(yy_state_type)) #ifndef YY_TYPEDEF_YY_BUFFER_STATE #define YY_TYPEDEF_YY_BUFFER_STATE typedef struct yy_buffer_state *YY_BUFFER_STATE; #endif extern int wcspihleng; extern FILE *wcspihin, *wcspihout; #define EOB_ACT_CONTINUE_SCAN 0 #define EOB_ACT_END_OF_FILE 1 #define EOB_ACT_LAST_MATCH 2 #define YY_LESS_LINENO(n) /* Return all but the first "n" matched characters back to the input stream. */ #define yyless(n) \ do \ { \ /* Undo effects of setting up wcspihtext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ *yy_cp = (yy_hold_char); \ YY_RESTORE_YY_MORE_OFFSET \ (yy_c_buf_p) = yy_cp = yy_bp + yyless_macro_arg - YY_MORE_ADJ; \ YY_DO_BEFORE_ACTION; /* set up wcspihtext again */ \ } \ while ( 0 ) #define unput(c) yyunput( c, (yytext_ptr) ) #ifndef YY_TYPEDEF_YY_SIZE_T #define YY_TYPEDEF_YY_SIZE_T typedef size_t yy_size_t; #endif #ifndef YY_STRUCT_YY_BUFFER_STATE #define YY_STRUCT_YY_BUFFER_STATE struct yy_buffer_state { FILE *yy_input_file; char *yy_ch_buf; /* input buffer */ char *yy_buf_pos; /* current position in input buffer */ /* Size of input buffer in bytes, not including room for EOB * characters. */ yy_size_t yy_buf_size; /* Number of characters read into yy_ch_buf, not including EOB * characters. */ int yy_n_chars; /* Whether we "own" the buffer - i.e., we know we created it, * and can realloc() it to grow it, and should free() it to * delete it. */ int yy_is_our_buffer; /* Whether this is an "interactive" input source; if so, and * if we're using stdio for input, then we want to use getc() * instead of fread(), to make sure we stop fetching input after * each newline. */ int yy_is_interactive; /* Whether we're considered to be at the beginning of a line. * If so, '^' rules will be active on the next match, otherwise * not. */ int yy_at_bol; int yy_bs_lineno; /**< The line count. */ int yy_bs_column; /**< The column count. */ /* Whether to try to fill the input buffer when we reach the * end of it. */ int yy_fill_buffer; int yy_buffer_status; #define YY_BUFFER_NEW 0 #define YY_BUFFER_NORMAL 1 /* When an EOF's been seen but there's still some text to process * then we mark the buffer as YY_EOF_PENDING, to indicate that we * shouldn't try reading from the input source any more. We might * still have a bunch of tokens to match, though, because of * possible backing-up. * * When we actually see the EOF, we change the status to "new" * (via wcspihrestart()), so that the user can continue scanning by * just pointing wcspihin at a new input file. */ #define YY_BUFFER_EOF_PENDING 2 }; #endif /* !YY_STRUCT_YY_BUFFER_STATE */ /* Stack of input buffers. */ static size_t yy_buffer_stack_top = 0; /**< index of top of stack. */ static size_t yy_buffer_stack_max = 0; /**< capacity of stack. */ static YY_BUFFER_STATE * yy_buffer_stack = 0; /**< Stack as an array. */ /* We provide macros for accessing buffer states in case in the * future we want to put the buffer states in a more general * "scanner state". * * Returns the top of the stack, or NULL. */ #define YY_CURRENT_BUFFER ( (yy_buffer_stack) \ ? (yy_buffer_stack)[(yy_buffer_stack_top)] \ : NULL) /* Same as previous macro, but useful when we know that the buffer stack is not * NULL or when we need an lvalue. For internal use only. */ #define YY_CURRENT_BUFFER_LVALUE (yy_buffer_stack)[(yy_buffer_stack_top)] /* yy_hold_char holds the character lost when wcspihtext is formed. */ static char yy_hold_char; static int yy_n_chars; /* number of characters read into yy_ch_buf */ int wcspihleng; /* Points to current character in buffer. */ static char *yy_c_buf_p = (char *) 0; static int yy_init = 0; /* whether we need to initialize */ static int yy_start = 0; /* start state number */ /* Flag which is used to allow wcspihwrap()'s to do buffer switches * instead of setting up a fresh wcspihin. A bit of a hack ... */ static int yy_did_buffer_switch_on_eof; void wcspihrestart (FILE *input_file ); void wcspih_switch_to_buffer (YY_BUFFER_STATE new_buffer ); YY_BUFFER_STATE wcspih_create_buffer (FILE *file,int size ); void wcspih_delete_buffer (YY_BUFFER_STATE b ); void wcspih_flush_buffer (YY_BUFFER_STATE b ); void wcspihpush_buffer_state (YY_BUFFER_STATE new_buffer ); void wcspihpop_buffer_state (void ); static void wcspihensure_buffer_stack (void ); static void wcspih_load_buffer_state (void ); static void wcspih_init_buffer (YY_BUFFER_STATE b,FILE *file ); #define YY_FLUSH_BUFFER wcspih_flush_buffer(YY_CURRENT_BUFFER ) YY_BUFFER_STATE wcspih_scan_buffer (char *base,yy_size_t size ); YY_BUFFER_STATE wcspih_scan_string (yyconst char *yy_str ); YY_BUFFER_STATE wcspih_scan_bytes (yyconst char *bytes,int len ); void *wcspihalloc (yy_size_t ); void *wcspihrealloc (void *,yy_size_t ); void wcspihfree (void * ); #define yy_new_buffer wcspih_create_buffer #define yy_set_interactive(is_interactive) \ { \ if ( ! YY_CURRENT_BUFFER ){ \ wcspihensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcspih_create_buffer(wcspihin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_is_interactive = is_interactive; \ } #define yy_set_bol(at_bol) \ { \ if ( ! YY_CURRENT_BUFFER ){\ wcspihensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcspih_create_buffer(wcspihin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = at_bol; \ } #define YY_AT_BOL() (YY_CURRENT_BUFFER_LVALUE->yy_at_bol) /* Begin user sect3 */ #define wcspihwrap(n) 1 #define YY_SKIP_YYWRAP typedef char YY_CHAR; FILE *wcspihin = (FILE *) 0, *wcspihout = (FILE *) 0; typedef int yy_state_type; extern int wcspihlineno; int wcspihlineno = 1; extern char *wcspihtext; #define yytext_ptr wcspihtext static yyconst flex_int16_t yy_nxt[][128] = { { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 }, { 33, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34, 34 }, { 33, 35, 35, 35, 35, 35, 35, 35, 35, 35, 34, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 36, 37, 38, 35, 35, 35, 35, 35, 35, 39, 40, 41, 42, 43, 35, 44, 45, 35, 35, 46, 47, 35, 35, 48, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35, 35 }, { 33, 49, 49, 49, 49, 49, 49, 49, 49, 49, 34, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 50, 50, 50, 50, 50, 50, 50, 50, 50, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49 }, { 33, 49, 49, 49, 49, 49, 49, 49, 49, 49, 34, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 50, 50, 50, 50, 50, 50, 50, 50, 50, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49, 49 }, { 33, 51, 51, 51, 51, 51, 51, 51, 51, 51, 34, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 52, 52, 52, 52, 52, 52, 52, 52, 52, 52, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51 }, { 33, 51, 51, 51, 51, 51, 51, 51, 51, 51, 34, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 52, 52, 52, 52, 52, 52, 52, 52, 52, 52, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51, 51 }, { 33, 53, 53, 53, 53, 53, 53, 53, 53, 53, 34, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 54, 54, 54, 54, 54, 54, 54, 54, 54, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53 }, { 33, 53, 53, 53, 53, 53, 53, 53, 53, 53, 34, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 54, 54, 54, 54, 54, 54, 54, 54, 54, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53, 53 }, { 33, 55, 55, 55, 55, 55, 55, 55, 55, 55, 34, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 56, 57, 57, 57, 57, 57, 57, 57, 57, 57, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55 }, { 33, 55, 55, 55, 55, 55, 55, 55, 55, 55, 34, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 56, 57, 57, 57, 57, 57, 57, 57, 57, 57, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 55, 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-440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440, -440 }, } ; static yy_state_type yy_get_previous_state (void ); static yy_state_type yy_try_NUL_trans (yy_state_type current_state ); static int yy_get_next_buffer (void ); static void yy_fatal_error (yyconst char msg[] ); /* Done after the current pattern has been matched and before the * corresponding action - sets up wcspihtext. */ #define YY_DO_BEFORE_ACTION \ (yytext_ptr) = yy_bp; \ wcspihleng = (size_t) (yy_cp - yy_bp); \ (yy_hold_char) = *yy_cp; \ *yy_cp = '\0'; \ (yy_c_buf_p) = yy_cp; #define YY_NUM_RULES 94 #define YY_END_OF_BUFFER 95 /* This struct is not used in this scanner, but its presence is necessary. */ struct yy_trans_info { flex_int32_t yy_verify; flex_int32_t yy_nxt; }; static yyconst flex_int16_t yy_accept[441] = { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 89, 89, 91, 91, 92, 92, 0, 0, 95, 94, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 63, 63, 79, 79, 47, 47, 59, 59, 59, 77, 77, 66, 64, 65, 81, 81, 83, 83, 82, 85, 85, 85, 84, 87, 87, 90, 89, 88, 91, 92, 94, 93, 5, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 4, 0, 18, 16, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 80, 82, 0, 84, 84, 84, 84, 0, 0, 86, 89, 88, 88, 91, 92, 0, 93, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 60, 61, 62, 78, 44, 45, 46, 0, 0, 0, 0, 0, 0, 0, 0, 84, 0, 84, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 6, 19, 20, 7, 3, 10, 21, 9, 8, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 17, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 58, 57, 53, 56, 50, 51, 55, 48, 49, 52, 54, 76, 72, 75, 69, 70, 74, 67, 68, 71, 73, 0, 0, 0, 0, 25, 12, 11, 0, 0, 0, 0, 0, 31, 0, 13, 15, 33, 34, 35, 36, 37, 0, 0, 0, 40, 41, 22, 23, 0, 24, 26, 27, 0, 28, 29, 30, 32, 14, 38, 39, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 1, 0, 0, 2, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 42 } ; static yy_state_type yy_last_accepting_state; static char *yy_last_accepting_cpos; static yyconst yy_state_type yy_NUL_trans[441] = { 0, 34, 35, 49, 49, 51, 51, 53, 53, 55, 55, 58, 58, 60, 60, 62, 62, 63, 63, 65, 65, 68, 68, 72, 72, 74, 74, 77, 77, 78, 78, 79, 79, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 126, 0, 0, 130, 131, 132, 133, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 126, 0, 0, 130, 130, 131, 132, 133, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 } ; extern int wcspih_flex_debug; int wcspih_flex_debug = 0; /* The intent behind this definition is that it'll catch * any uses of REJECT which flex missed. */ #define REJECT reject_used_but_not_detected #define yymore() yymore_used_but_not_detected #define YY_MORE_ADJ 0 #define YY_RESTORE_YY_MORE_OFFSET char *wcspihtext; #line 1 "wcspih.l" /*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcspih.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcspih.l is a Flex description file containing the definition of a lexical * scanner for parsing the WCS keyrecords from a FITS primary image or image * extension header. * * wcspih.l requires Flex v2.5.4 or later. Refer to wcshdr.h for a description * of the user interface and operating notes. * * Implementation notes * -------------------- * Use of the WCSAXESa keyword is not mandatory. Its default value is "the * larger of NAXIS and the largest index of these keywords [i.e. CRPIXj, PCi_j * or CDi_j, CDELTi, CTYPEi, CRVALi, and CUNITi] found in the FITS header". * Consequently the definition of WCSAXESa effectively invalidates the use of * NAXIS for determining the number of coordinate axes and forces a preliminary * pass through the header to determine the "largest index" in headers where * WCSAXESa was omitted. * * Furthermore, since the use of WCSAXESa is optional, there is no way to * determine the number of coordinate representations (the "a" value) other * than by parsing all of the WCS keywords in the header; even if WCSAXESa was * specified for some representations it cannot be known in advance whether it * was specified for all of those present in the header. * * Hence the definition of WCSAXESa forces the scanner to be implemented in two * passes. The first pass is used to determine the number of coordinate * representations (up to 27) and the number of coordinate axes in each. * Effectively WCSAXESa is ignored unless it exceeds the "largest index" in * which case the keywords for the extra axes assume their default values. The * number of PVi_ma and PSi_ma keywords in each representation is also counted * in the first pass. * * On completion of the first pass, memory is allocated for an array of the * required number of wcsprm structs and each of these is initialized * appropriately. These structs are filled in the second pass. * * The parser does not check for duplicated keywords, it accepts the last * encountered. * *===========================================================================*/ /* Options. */ /* Indices for parameterized keywords. */ /* Alternate coordinate system identifier. */ /* Keyvalue data types. */ /* Exclusive start states. */ #line 105 "wcspih.l" #include #include #include #include #include #include "wcs.h" #include "wcshdr.h" #include "wcsmath.h" #define INTEGER 0 #define FLOAT 1 #define STRING 2 #define YY_DECL int wcspih(char *header, int nkeyrec, int relax, int ctrl, \ int *nreject, int *nwcs, struct wcsprm **wcs) #define YY_INPUT(inbuff, count, bufsize) \ { \ if (wcspih_nkeyrec) { \ strncpy(inbuff, wcspih_hdr, 80); \ inbuff[80] = '\n'; \ wcspih_hdr += 80; \ wcspih_nkeyrec--; \ count = 81; \ } else { \ count = YY_NULL; \ } \ } /* These global variables are required by YY_INPUT. */ char *wcspih_hdr; int wcspih_nkeyrec; int wcspih_final(int alts[], double epoch[], double vsource[], int *nwcs, struct wcsprm **wcs); int wcspih_inits(int naxis, int alts[], int npv[], int nps[], int *nwcs, struct wcsprm **wcs); void wcspih_naxes(int naxis, int i, int j, char a, int alts[], int *npptr); /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcspih_abort_jmp_env; #define exit(status) longjmp(wcspih_abort_jmp_env, status) #line 8283 "wcspih.c" #define INITIAL 0 #define CROTAi 1 #define PROJPn 2 #define CCCCCia 3 #define CCi_ja 4 #define CCi_ma 5 #define CCCCCCCa 6 #define CCCCCCCC 7 #define VALUE 8 #define INTEGER_VAL 9 #define FLOAT_VAL 10 #define STRING_VAL 11 #define COMMENT 12 #define DISCARD 13 #define ERROR 14 #define FLUSH 15 #ifndef YY_NO_UNISTD_H /* Special case for "unistd.h", since it is non-ANSI. We include it way * down here because we want the user's section 1 to have been scanned first. * The user has a chance to override it with an option. */ #include #endif #ifndef YY_EXTRA_TYPE #define YY_EXTRA_TYPE void * #endif static int yy_init_globals (void ); /* Accessor methods to globals. These are made visible to non-reentrant scanners for convenience. */ int wcspihlex_destroy (void ); int wcspihget_debug (void ); void wcspihset_debug (int debug_flag ); YY_EXTRA_TYPE wcspihget_extra (void ); void wcspihset_extra (YY_EXTRA_TYPE user_defined ); FILE *wcspihget_in (void ); void wcspihset_in (FILE * in_str ); FILE *wcspihget_out (void ); void wcspihset_out (FILE * out_str ); int wcspihget_leng (void ); char *wcspihget_text (void ); int wcspihget_lineno (void ); void wcspihset_lineno (int line_number ); /* Macros after this point can all be overridden by user definitions in * section 1. */ #ifndef YY_SKIP_YYWRAP #ifdef __cplusplus extern "C" int wcspihwrap (void ); #else extern int wcspihwrap (void ); #endif #endif static void yyunput (int c,char *buf_ptr ); #ifndef yytext_ptr static void yy_flex_strncpy (char *,yyconst char *,int ); #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * ); #endif #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void ); #else static int input (void ); #endif #endif /* Amount of stuff to slurp up with each read. */ #ifndef YY_READ_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k */ #define YY_READ_BUF_SIZE 16384 #else #define YY_READ_BUF_SIZE 8192 #endif /* __ia64__ */ #endif /* Copy whatever the last rule matched to the standard output. */ #ifndef ECHO /* This used to be an fputs(), but since the string might contain NUL's, * we now use fwrite(). */ #define ECHO do { if (fwrite( wcspihtext, wcspihleng, 1, wcspihout )) {} } while (0) #endif /* Gets input and stuffs it into "buf". number of characters read, or YY_NULL, * is returned in "result". */ #ifndef YY_INPUT #define YY_INPUT(buf,result,max_size) \ errno=0; \ while ( (result = read( fileno(wcspihin), (char *) buf, max_size )) < 0 ) \ { \ if( errno != EINTR) \ { \ YY_FATAL_ERROR( "input in flex scanner failed" ); \ break; \ } \ errno=0; \ clearerr(wcspihin); \ }\ \ #endif /* No semi-colon after return; correct usage is to write "yyterminate();" - * we don't want an extra ';' after the "return" because that will cause * some compilers to complain about unreachable statements. */ #ifndef yyterminate #define yyterminate() return YY_NULL #endif /* Number of entries by which start-condition stack grows. */ #ifndef YY_START_STACK_INCR #define YY_START_STACK_INCR 25 #endif /* Report a fatal error. */ #ifndef YY_FATAL_ERROR #define YY_FATAL_ERROR(msg) yy_fatal_error( msg ) #endif /* end tables serialization structures and prototypes */ /* Default declaration of generated scanner - a define so the user can * easily add parameters. */ #ifndef YY_DECL #define YY_DECL_IS_OURS 1 extern int wcspihlex (void); #define YY_DECL int wcspihlex (void) #endif /* !YY_DECL */ /* Code executed at the beginning of each rule, after wcspihtext and wcspihleng * have been set up. */ #ifndef YY_USER_ACTION #define YY_USER_ACTION #endif /* Code executed at the end of each rule. */ #ifndef YY_BREAK #define YY_BREAK break; #endif #define YY_RULE_SETUP \ if ( wcspihleng > 0 ) \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = \ (wcspihtext[wcspihleng - 1] == '\n'); \ YY_USER_ACTION /** The main scanner function which does all the work. */ YY_DECL { register yy_state_type yy_current_state; register char *yy_cp, *yy_bp; register int yy_act; #line 151 "wcspih.l" /* Keyword indices, as used in the WCS papers, e.g. PCi_ja, PVi_ma. */ char a; int i, j, m; char *cptr, *errmsg, errtxt[80], *hptr, *keep; int altlin, alts[27], ialt, idx, ipx, ix, jx, naxis, *npptr, nps[27], npv[27], pass, status, valtype, voff; double epoch[27], vsource[27]; void *vptr, *wptr; struct wcsprm *wcsp; int wcspihlex_destroy(void); naxis = 0; for (ialt = 0; ialt < 27; ialt++) { alts[ialt] = 0; npv[ialt] = 0; nps[ialt] = 0; epoch[ialt] = UNDEFINED; vsource[ialt] = UNDEFINED; } /* Parameters used to implement YY_INPUT. */ wcspih_hdr = header; wcspih_nkeyrec = nkeyrec; /* Our handle on the input stream. */ hptr = header; keep = 0x0; *nreject = 0; /* Keyword parameters. */ i = j = m = 0; a = ' '; /* For decoding the keyvalue. */ valtype = -1; idx = -1; vptr = 0x0; /* For keywords that require special handling. */ altlin = 0; npptr = 0x0; /* The data structures produced. */ *nwcs = 0; *wcs = 0x0; pass = 1; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcspih_abort_jmp_env)) { return 3; } BEGIN(INITIAL); #line 8531 "wcspih.c" if ( !(yy_init) ) { (yy_init) = 1; #ifdef YY_USER_INIT YY_USER_INIT; #endif if ( ! (yy_start) ) (yy_start) = 1; /* first start state */ if ( ! wcspihin ) wcspihin = stdin; if ( ! wcspihout ) wcspihout = stdout; if ( ! YY_CURRENT_BUFFER ) { wcspihensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcspih_create_buffer(wcspihin,YY_BUF_SIZE ); } wcspih_load_buffer_state( ); } while ( 1 ) /* loops until end-of-file is reached */ { yy_cp = (yy_c_buf_p); /* Support of wcspihtext. */ *yy_cp = (yy_hold_char); /* yy_bp points to the position in yy_ch_buf of the start of * the current run. */ yy_bp = yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); yy_match: while ( (yy_current_state = yy_nxt[yy_current_state][ YY_SC_TO_UI(*yy_cp) ]) > 0 ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } ++yy_cp; } yy_current_state = -yy_current_state; yy_find_action: yy_act = yy_accept[yy_current_state]; YY_DO_BEFORE_ACTION; do_action: /* This label is used only to access EOF actions. */ switch ( yy_act ) { /* beginning of action switch */ case 0: /* must back up */ /* undo the effects of YY_DO_BEFORE_ACTION */ *yy_cp = (yy_hold_char); yy_cp = (yy_last_accepting_cpos) + 1; yy_current_state = (yy_last_accepting_state); goto yy_find_action; case 1: YY_RULE_SETUP #line 209 "wcspih.l" { if (pass == 1) { sscanf(wcspihtext, "NAXIS = %d", &naxis); } if (naxis < 0) { errmsg = errtxt; sprintf(errmsg, "Negative value of NAXIS ignored: %d", naxis); naxis = 0; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 2: YY_RULE_SETUP #line 224 "wcspih.l" { if (pass == 1) { sscanf(wcspihtext, "WCSAXES%c= %d", &a, &i); wcspih_naxes(naxis, i, 0, a, alts, 0); } BEGIN(FLUSH); } YY_BREAK case 3: YY_RULE_SETUP #line 232 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crpix); BEGIN(CCCCCia); } YY_BREAK case 4: YY_RULE_SETUP #line 238 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->pc); altlin = 1; BEGIN(CCi_ja); } YY_BREAK case 5: YY_RULE_SETUP #line 245 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->cd); altlin = 2; BEGIN(CCi_ja); } YY_BREAK case 6: YY_RULE_SETUP #line 252 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->cdelt); BEGIN(CCCCCia); } YY_BREAK case 7: YY_RULE_SETUP #line 258 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crota); altlin = 4; BEGIN(CROTAi); } YY_BREAK case 8: YY_RULE_SETUP #line 265 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = &((*wcs)->cunit); BEGIN(CCCCCia); } YY_BREAK case 9: YY_RULE_SETUP #line 271 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = &((*wcs)->ctype); BEGIN(CCCCCia); } YY_BREAK case 10: YY_RULE_SETUP #line 277 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crval); BEGIN(CCCCCia); } YY_BREAK case 11: YY_RULE_SETUP #line 283 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->lonpole); BEGIN(CCCCCCCa); } YY_BREAK case 12: YY_RULE_SETUP #line 289 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->latpole); BEGIN(CCCCCCCa); } YY_BREAK case 13: YY_RULE_SETUP #line 295 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->restfrq); BEGIN(CCCCCCCa); } YY_BREAK case 14: YY_RULE_SETUP #line 301 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->restfrq); unput(' '); BEGIN(CCCCCCCa); } YY_BREAK case 15: YY_RULE_SETUP #line 308 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->restwav); BEGIN(CCCCCCCa); } YY_BREAK case 16: YY_RULE_SETUP #line 314 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->pv); npptr = npv; BEGIN(CCi_ma); } YY_BREAK case 17: YY_RULE_SETUP #line 321 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->pv); npptr = npv; BEGIN(PROJPn); } YY_BREAK case 18: YY_RULE_SETUP #line 328 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = &((*wcs)->ps); npptr = nps; BEGIN(CCi_ma); } YY_BREAK case 19: YY_RULE_SETUP #line 335 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = &((*wcs)->cname); BEGIN(CCCCCia); } YY_BREAK case 20: YY_RULE_SETUP #line 341 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crder); BEGIN(CCCCCia); } YY_BREAK case 21: YY_RULE_SETUP #line 347 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->csyer); BEGIN(CCCCCia); } YY_BREAK case 22: YY_RULE_SETUP #line 353 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->dateavg; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 23: YY_RULE_SETUP #line 360 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->dateobs; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 24: YY_RULE_SETUP #line 367 "wcspih.l" { sscanf(wcspihtext, "EPOCH%c", &a); if (a == ' ' || relax & WCSHDR_EPOCHa) { valtype = FLOAT; if (pass == 2) { vptr = epoch; if (a >= 'A') { vptr = (void *)((double *)vptr + alts[a-'A'+1]); } } unput(' '); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "EPOCH keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 25: YY_RULE_SETUP #line 391 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->equinox); BEGIN(CCCCCCCa); } YY_BREAK case 26: YY_RULE_SETUP #line 397 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->mjdavg); if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 27: YY_RULE_SETUP #line 404 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->mjdobs); if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 28: YY_RULE_SETUP #line 411 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = (*wcs)->obsgeo; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 29: YY_RULE_SETUP #line 418 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = (*wcs)->obsgeo + 1; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 30: YY_RULE_SETUP #line 425 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = (*wcs)->obsgeo + 2; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } YY_BREAK case 31: YY_RULE_SETUP #line 432 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->radesys; BEGIN(CCCCCCCa); } YY_BREAK case 32: YY_RULE_SETUP #line 438 "wcspih.l" { if (relax & WCSHDR_RADECSYS) { valtype = STRING; if (pass == 2) vptr = (*wcs)->radesys; unput(' '); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "RADECSYS is non-standard, use RADESYSa"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 33: YY_RULE_SETUP #line 454 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->specsys; BEGIN(CCCCCCCa); } YY_BREAK case 34: YY_RULE_SETUP #line 460 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->ssysobs; BEGIN(CCCCCCCa); } YY_BREAK case 35: YY_RULE_SETUP #line 466 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->ssyssrc; BEGIN(CCCCCCCa); } YY_BREAK case 36: YY_RULE_SETUP #line 472 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->velangl); BEGIN(CCCCCCCa); } YY_BREAK case 37: YY_RULE_SETUP #line 478 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->velosys); BEGIN(CCCCCCCa); } YY_BREAK case 38: YY_RULE_SETUP #line 484 "wcspih.l" { sscanf(wcspihtext, "VELREF%c", &a); if (a == ' ' || relax & WCSHDR_VELREFa) { valtype = INTEGER; if (pass == 2) vptr = &((*wcs)->velref); unput(a); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "VELREF keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 39: YY_RULE_SETUP #line 503 "wcspih.l" { sscanf(wcspihtext, "VSOURCE%c", &a); if (relax & WCSHDR_VSOURCE) { valtype = FLOAT; if (pass == 2) { vptr = vsource; if (a >= 'A') { vptr = (void *)((double *)vptr + alts[a-'A'+1]); } } unput(' '); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "Deprecated VSOURCEa keyword rejected"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 40: YY_RULE_SETUP #line 527 "wcspih.l" { valtype = STRING; if (pass == 2) vptr = (*wcs)->wcsname; BEGIN(CCCCCCCa); } YY_BREAK case 41: YY_RULE_SETUP #line 533 "wcspih.l" { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->zsource); BEGIN(CCCCCCCa); } YY_BREAK case 42: YY_RULE_SETUP #line 539 "wcspih.l" { yyless(0); if (wcspih_nkeyrec) { wcspih_nkeyrec = 0; errmsg = "Keyrecords following the END keyrecord were ignored"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 43: YY_RULE_SETUP #line 550 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 44: #line 555 "wcspih.l" case 45: YY_RULE_SETUP #line 555 "wcspih.l" { sscanf(wcspihtext, "%d%c", &i, &a); idx = i - 1; BEGIN(VALUE); } YY_BREAK case 46: YY_RULE_SETUP #line 561 "wcspih.l" { /* Invalid axis number will be caught by . */ sscanf(wcspihtext, "%3d", &i); BEGIN(VALUE); } YY_BREAK case 47: YY_RULE_SETUP #line 567 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 48: #line 572 "wcspih.l" case 49: #line 573 "wcspih.l" case 50: #line 574 "wcspih.l" case 51: YY_RULE_SETUP #line 574 "wcspih.l" { sscanf(wcspihtext, "%d_%d%c", &i, &j, &a); if (pass == 2) { wcsp = *wcs; if (a != ' ') { wcsp += alts[a-'A'+1]; } idx = (i-1)*(wcsp->naxis) + j - 1; } BEGIN(VALUE); } YY_BREAK case 52: #line 588 "wcspih.l" case 53: #line 589 "wcspih.l" case 54: #line 590 "wcspih.l" case 55: #line 591 "wcspih.l" case 56: #line 592 "wcspih.l" case 57: YY_RULE_SETUP #line 592 "wcspih.l" { /* Invalid axis numbers will be caught by . */ sscanf(wcspihtext, "%d_%d", &i, &j); BEGIN(VALUE); } YY_BREAK case 58: YY_RULE_SETUP #line 598 "wcspih.l" { /* This covers the defunct forms CD00i00j and PC00i00j. */ if (((relax & WCSHDR_PC00i00j) && (altlin == 1)) || ((relax & WCSHDR_CD00i00j) && (altlin == 2))) { sscanf(wcspihtext, "%3d%3d", &i, &j); a = ' '; if (pass == 2) { idx = (i-1)*((*wcs)->naxis) + j - 1; } BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Defunct form of %si_ja keyword", (altlin==1) ? "PC" : "CD"); BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 59: YY_RULE_SETUP #line 620 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 60: #line 625 "wcspih.l" case 61: YY_RULE_SETUP #line 625 "wcspih.l" { sscanf(wcspihtext, "%d%c", &i, &a); if (a == ' ' || relax & WCSHDR_CROTAia) { idx = i - 1; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = "CROTAn keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 62: YY_RULE_SETUP #line 640 "wcspih.l" { sscanf(wcspihtext, "%d", &i); a = ' '; idx = i - 1; BEGIN(VALUE); } YY_BREAK case 63: YY_RULE_SETUP #line 647 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 64: #line 652 "wcspih.l" case 65: YY_RULE_SETUP #line 652 "wcspih.l" { idx = -1; if (YY_START == CCCCCCCa) { sscanf(wcspihtext, "%c", &a); } else { unput(wcspihtext[0]); a = 0; } BEGIN(VALUE); } YY_BREAK case 66: YY_RULE_SETUP #line 664 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 67: #line 669 "wcspih.l" case 68: #line 670 "wcspih.l" case 69: #line 671 "wcspih.l" case 70: YY_RULE_SETUP #line 671 "wcspih.l" { sscanf(wcspihtext, "%d_%d%c", &i, &m, &a); idx = -1; BEGIN(VALUE); } YY_BREAK case 71: #line 678 "wcspih.l" case 72: #line 679 "wcspih.l" case 73: #line 680 "wcspih.l" case 74: #line 681 "wcspih.l" case 75: #line 682 "wcspih.l" case 76: YY_RULE_SETUP #line 682 "wcspih.l" { /* Invalid parameters will be caught by . */ sscanf(wcspihtext, "%d_%d", &i, &m); BEGIN(VALUE); } YY_BREAK case 77: YY_RULE_SETUP #line 688 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 78: YY_RULE_SETUP #line 692 "wcspih.l" { if (relax & WCSHDR_PROJPn) { sscanf(wcspihtext, "%d", &m); i = 0; a = ' '; idx = -1; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = "Defunct PROJPn keyword rejected"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } YY_BREAK case 79: YY_RULE_SETUP #line 709 "wcspih.l" { BEGIN(DISCARD); } YY_BREAK case 80: YY_RULE_SETUP #line 713 "wcspih.l" { /* Do checks on i, j & m. */ if (i > 99 || j > 99 || m > 99) { if (relax & WCSHDR_reject) { errmsg = errtxt; if (i > 99 || j > 99) { sprintf(errmsg, "Axis number exceeds 99"); } else if (m > 99) { sprintf(errmsg, "Parameter number exceeds 99"); } BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } else { if (valtype == INTEGER) { BEGIN(INTEGER_VAL); } else if (valtype == FLOAT) { BEGIN(FLOAT_VAL); } else if (valtype == STRING) { BEGIN(STRING_VAL); } else { errmsg = errtxt; sprintf(errmsg, "Internal parser ERROR, bad data type: %d", valtype); BEGIN(ERROR); } } } YY_BREAK case 81: YY_RULE_SETUP #line 746 "wcspih.l" { errmsg = "Invalid KEYWORD = VALUE syntax"; BEGIN(ERROR); } YY_BREAK case 82: YY_RULE_SETUP #line 751 "wcspih.l" { if (pass == 1) { wcspih_naxes(naxis, i, j, a, alts, npptr); BEGIN(FLUSH); } else { if (vptr) { /* Determine the coordinate representation. */ for (ialt = 0; ialt < *nwcs; ialt++) { /* The loop here is for keywords that apply */ /* to every alternate; these have a == 0. */ if (a >= 'A') { ialt = alts[a-'A'+1]; } wptr = vptr; if (ialt) { voff = (char *)(*wcs+ialt) - (char *)(*wcs); wptr = (void *)((char *)vptr + voff); } /* Apply keyword parameterization. */ if (idx >= 0) { wptr = *((int **)wptr) + idx; } /* Read the keyvalue. */ sscanf(wcspihtext, "%d", (int *)wptr); if (a) break; } BEGIN(COMMENT); } else { errmsg = "Internal parser ERROR, null int pointer"; BEGIN(ERROR); } } } YY_BREAK case 83: YY_RULE_SETUP #line 792 "wcspih.l" { errmsg = "An integer value was expected"; BEGIN(ERROR); } YY_BREAK case 84: YY_RULE_SETUP #line 797 "wcspih.l" { if (pass == 1) { wcspih_naxes(naxis, i, j, a, alts, npptr); BEGIN(FLUSH); } else { if (vptr) { /* Determine the coordinate representation. */ for (ialt = 0; ialt < *nwcs; ialt++) { /* The loop here is for keywords like MJD-OBS that */ /* apply to every alternate; these have a == 0. */ if (a >= 'A') { ialt = alts[a-'A'+1]; } wptr = vptr; if (ialt) { voff = (char *)(*wcs+ialt) - (char *)(*wcs); wptr = (void *)((char *)vptr + voff); } /* Apply keyword parameterization. */ if (idx >= 0) { wptr = *((double **)wptr) + idx; } else if (npptr == npv) { ipx = (*wcs+ialt)->npv++; (*wcs+ialt)->pv[ipx].i = i; (*wcs+ialt)->pv[ipx].m = m; wptr = &((*wcs+ialt)->pv[ipx].value); } /* Read the keyvalue. */ sscanf(wcspihtext, "%lf", (double *)wptr); /* Flag the presence of PCi_ja, or CDi_ja and/or CROTAia. */ if (altlin) { (*wcs+ialt)->altlin |= altlin; altlin = 0; } if (a) break; } BEGIN(COMMENT); } else { errmsg = "Internal parser ERROR, null float pointer"; BEGIN(ERROR); } } } YY_BREAK case 85: YY_RULE_SETUP #line 850 "wcspih.l" { errmsg = "A floating-point value was expected"; BEGIN(ERROR); } YY_BREAK case 86: /* rule 86 can match eol */ YY_RULE_SETUP #line 855 "wcspih.l" { if (pass == 1) { wcspih_naxes(naxis, i, j, a, alts, npptr); BEGIN(FLUSH); } else { if (vptr) { /* Determine the coordinate representation. */ for (ialt = 0; ialt < *nwcs; ialt++) { /* The loop here is for keywords like DATE-OBS that */ /* apply to every alternate; these have a == 0. */ if (a >= 'A') { ialt = alts[a-'A'+1]; } wptr = vptr; if (ialt) { voff = (char *)(*wcs+ialt) - (char *)(*wcs); wptr = (void *)((char *)vptr + voff); } /* Apply keyword parameterization. */ if (idx >= 0) { wptr = *((char (**)[72])wptr) + idx; } else if (npptr == nps) { ipx = (*wcs+ialt)->nps++; (*wcs+ialt)->ps[ipx].i = i; (*wcs+ialt)->ps[ipx].m = m; wptr = (*wcs+ialt)->ps[ipx].value; } /* Read the keyvalue. */ cptr = (char *)wptr; strcpy(cptr, wcspihtext+1); /* Squeeze out repeated quotes. */ ix = 0; for (jx = 0; jx < 72; jx++) { if (ix < jx) { cptr[ix] = cptr[jx]; } if (cptr[jx] == '\0') { if (ix) cptr[ix-1] = '\0'; break; } else if (cptr[jx] == '\'' && cptr[jx+1] == '\'') { jx++; } ix++; } if (a) break; } BEGIN(COMMENT); } else { errmsg = "Internal parser ERROR, null string pointer"; BEGIN(ERROR); } } } YY_BREAK case 87: YY_RULE_SETUP #line 920 "wcspih.l" { errmsg = "A string value was expected"; BEGIN(ERROR); } YY_BREAK case 88: #line 926 "wcspih.l" case 89: YY_RULE_SETUP #line 926 "wcspih.l" { BEGIN(FLUSH); } YY_BREAK case 90: YY_RULE_SETUP #line 930 "wcspih.l" { errmsg = "Malformed keycomment"; BEGIN(ERROR); } YY_BREAK case 91: YY_RULE_SETUP #line 935 "wcspih.l" { if (pass == 2) { if (ctrl < 0) { /* Preserve discards. */ keep = wcspih_hdr - 80; } else if (ctrl > 2) { fprintf(stderr, "%.80s\n Discarded.\n", wcspih_hdr-80); } } BEGIN(FLUSH); } YY_BREAK case 92: YY_RULE_SETUP #line 948 "wcspih.l" { (*nreject)++; if (pass == 2) { if (ctrl%10 == -1) { /* Preserve rejects. */ keep = wcspih_hdr - 80; } if (abs(ctrl%10) > 1) { fprintf(stderr, "%.80s\n%4d: %s.\n", wcspih_hdr-80, *nreject, errmsg); } } BEGIN(FLUSH); } YY_BREAK case 93: /* rule 93 can match eol */ YY_RULE_SETUP #line 964 "wcspih.l" { if (pass == 2 && keep) { if (hptr < keep) { strncpy(hptr, keep, 80); } hptr += 80; } i = j = m = 0; a = ' '; valtype = -1; keep = 0x0; altlin = 0; npptr = 0x0; BEGIN(INITIAL); } YY_BREAK case YY_STATE_EOF(INITIAL): case YY_STATE_EOF(CROTAi): case YY_STATE_EOF(PROJPn): case YY_STATE_EOF(CCCCCia): case YY_STATE_EOF(CCi_ja): case YY_STATE_EOF(CCi_ma): case YY_STATE_EOF(CCCCCCCa): case YY_STATE_EOF(CCCCCCCC): case YY_STATE_EOF(VALUE): case YY_STATE_EOF(INTEGER_VAL): case YY_STATE_EOF(FLOAT_VAL): case YY_STATE_EOF(STRING_VAL): case YY_STATE_EOF(COMMENT): case YY_STATE_EOF(DISCARD): case YY_STATE_EOF(ERROR): case YY_STATE_EOF(FLUSH): #line 981 "wcspih.l" { /* End-of-input. */ if (pass == 1) { if ((status = wcspih_inits(naxis, alts, npv, nps, nwcs, wcs)) || *nwcs == 0) { wcspihlex_destroy(); return status; } if (abs(ctrl%10) > 2) { if (*nwcs == 1) { fprintf(stderr, "Found one coordinate representation.\n"); } else { fprintf(stderr, "Found %d coordinate representations.\n", *nwcs); } } wcspih_hdr = header; wcspih_nkeyrec = nkeyrec; *nreject = 0; pass = 2; i = j = m = 0; a = ' '; valtype = -1; wcspihrestart(wcspihin); } else { wcspihlex_destroy(); if (ctrl < 0) { *hptr = '\0'; } else if (ctrl == 1) { fprintf(stderr, "%d WCS keyrecords were rejected.\n", *nreject); } return wcspih_final(alts, epoch, vsource, nwcs, wcs); } } YY_BREAK case 94: YY_RULE_SETUP #line 1024 "wcspih.l" ECHO; YY_BREAK #line 9681 "wcspih.c" case YY_END_OF_BUFFER: { /* Amount of text matched not including the EOB char. */ int yy_amount_of_matched_text = (int) (yy_cp - (yytext_ptr)) - 1; /* Undo the effects of YY_DO_BEFORE_ACTION. */ *yy_cp = (yy_hold_char); YY_RESTORE_YY_MORE_OFFSET if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_NEW ) { /* We're scanning a new file or input source. It's * possible that this happened because the user * just pointed wcspihin at a new source and called * wcspihlex(). If so, then we have to assure * consistency between YY_CURRENT_BUFFER and our * globals. Here is the right place to do so, because * this is the first action (other than possibly a * back-up) that will match for the new input source. */ (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; YY_CURRENT_BUFFER_LVALUE->yy_input_file = wcspihin; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_NORMAL; } /* Note that here we test for yy_c_buf_p "<=" to the position * of the first EOB in the buffer, since yy_c_buf_p will * already have been incremented past the NUL character * (since all states make transitions on EOB to the * end-of-buffer state). Contrast this with the test * in input(). */ if ( (yy_c_buf_p) <= &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) { /* This was really a NUL. */ yy_state_type yy_next_state; (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); /* Okay, we're now positioned to make the NUL * transition. We couldn't have * yy_get_previous_state() go ahead and do it * for us because it doesn't know how to deal * with the possibility of jamming (and we don't * want to build jamming into it because then it * will run more slowly). */ yy_next_state = yy_try_NUL_trans( yy_current_state ); yy_bp = (yytext_ptr) + YY_MORE_ADJ; if ( yy_next_state ) { /* Consume the NUL. */ yy_cp = ++(yy_c_buf_p); yy_current_state = yy_next_state; goto yy_match; } else { yy_cp = (yy_c_buf_p); goto yy_find_action; } } else switch ( yy_get_next_buffer( ) ) { case EOB_ACT_END_OF_FILE: { (yy_did_buffer_switch_on_eof) = 0; if ( wcspihwrap( ) ) { /* Note: because we've taken care in * yy_get_next_buffer() to have set up * wcspihtext, we can now set up * yy_c_buf_p so that if some total * hoser (like flex itself) wants to * call the scanner after we return the * YY_NULL, it'll still work - another * YY_NULL will get returned. */ (yy_c_buf_p) = (yytext_ptr) + YY_MORE_ADJ; yy_act = YY_STATE_EOF(YY_START); goto do_action; } else { if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; } break; } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_match; case EOB_ACT_LAST_MATCH: (yy_c_buf_p) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)]; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_find_action; } break; } default: YY_FATAL_ERROR( "fatal flex scanner internal error--no action found" ); } /* end of action switch */ } /* end of scanning one token */ } /* end of wcspihlex */ /* yy_get_next_buffer - try to read in a new buffer * * Returns a code representing an action: * EOB_ACT_LAST_MATCH - * EOB_ACT_CONTINUE_SCAN - continue scanning from current position * EOB_ACT_END_OF_FILE - end of file */ static int yy_get_next_buffer (void) { register char *dest = YY_CURRENT_BUFFER_LVALUE->yy_ch_buf; register char *source = (yytext_ptr); register int number_to_move, i; int ret_val; if ( (yy_c_buf_p) > &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] ) YY_FATAL_ERROR( "fatal flex scanner internal error--end of buffer missed" ); if ( YY_CURRENT_BUFFER_LVALUE->yy_fill_buffer == 0 ) { /* Don't try to fill the buffer, so this is an EOF. */ if ( (yy_c_buf_p) - (yytext_ptr) - YY_MORE_ADJ == 1 ) { /* We matched a single character, the EOB, so * treat this as a final EOF. */ return EOB_ACT_END_OF_FILE; } else { /* We matched some text prior to the EOB, first * process it. */ return EOB_ACT_LAST_MATCH; } } /* Try to read more data. */ /* First move last chars to start of buffer. */ number_to_move = (int) ((yy_c_buf_p) - (yytext_ptr)) - 1; for ( i = 0; i < number_to_move; ++i ) *(dest++) = *(source++); if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_EOF_PENDING ) /* don't do the read, it's not guaranteed to return an EOF, * just force an EOF */ YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = 0; else { int num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; while ( num_to_read <= 0 ) { /* Not enough room in the buffer - grow it. */ /* just a shorter name for the current buffer */ YY_BUFFER_STATE b = YY_CURRENT_BUFFER; int yy_c_buf_p_offset = (int) ((yy_c_buf_p) - b->yy_ch_buf); if ( b->yy_is_our_buffer ) { int new_size = b->yy_buf_size * 2; if ( new_size <= 0 ) b->yy_buf_size += b->yy_buf_size / 8; else b->yy_buf_size *= 2; b->yy_ch_buf = (char *) /* Include room in for 2 EOB chars. */ wcspihrealloc((void *) b->yy_ch_buf,b->yy_buf_size + 2 ); } else /* Can't grow it, we don't own it. */ b->yy_ch_buf = 0; if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "fatal error - scanner input buffer overflow" ); (yy_c_buf_p) = &b->yy_ch_buf[yy_c_buf_p_offset]; num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; } if ( num_to_read > YY_READ_BUF_SIZE ) num_to_read = YY_READ_BUF_SIZE; /* Read in more data. */ YY_INPUT( (&YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]), (yy_n_chars), (size_t) num_to_read ); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } if ( (yy_n_chars) == 0 ) { if ( number_to_move == YY_MORE_ADJ ) { ret_val = EOB_ACT_END_OF_FILE; wcspihrestart(wcspihin ); } else { ret_val = EOB_ACT_LAST_MATCH; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_EOF_PENDING; } } else ret_val = EOB_ACT_CONTINUE_SCAN; if ((yy_size_t) ((yy_n_chars) + number_to_move) > YY_CURRENT_BUFFER_LVALUE->yy_buf_size) { /* Extend the array by 50%, plus the number we really need. */ yy_size_t new_size = (yy_n_chars) + number_to_move + ((yy_n_chars) >> 1); YY_CURRENT_BUFFER_LVALUE->yy_ch_buf = (char *) wcspihrealloc((void *) YY_CURRENT_BUFFER_LVALUE->yy_ch_buf,new_size ); if ( ! YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in yy_get_next_buffer()" ); } (yy_n_chars) += number_to_move; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] = YY_END_OF_BUFFER_CHAR; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] = YY_END_OF_BUFFER_CHAR; (yytext_ptr) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[0]; return ret_val; } /* yy_get_previous_state - get the state just before the EOB char was reached */ static yy_state_type yy_get_previous_state (void) { register yy_state_type yy_current_state; register char *yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); for ( yy_cp = (yytext_ptr) + YY_MORE_ADJ; yy_cp < (yy_c_buf_p); ++yy_cp ) { if ( *yy_cp ) { yy_current_state = yy_nxt[yy_current_state][YY_SC_TO_UI(*yy_cp)]; } else yy_current_state = yy_NUL_trans[yy_current_state]; if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_current_state; } /* yy_try_NUL_trans - try to make a transition on the NUL character * * synopsis * next_state = yy_try_NUL_trans( current_state ); */ static yy_state_type yy_try_NUL_trans (yy_state_type yy_current_state ) { register int yy_is_jam; register char *yy_cp = (yy_c_buf_p); yy_current_state = yy_NUL_trans[yy_current_state]; yy_is_jam = (yy_current_state == 0); if ( ! yy_is_jam ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_is_jam ? 0 : yy_current_state; } static void yyunput (int c, register char * yy_bp ) { register char *yy_cp; yy_cp = (yy_c_buf_p); /* undo effects of setting up wcspihtext */ *yy_cp = (yy_hold_char); if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) { /* need to shift things up to make room */ /* +2 for EOB chars. */ register int number_to_move = (yy_n_chars) + 2; register char *dest = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[ YY_CURRENT_BUFFER_LVALUE->yy_buf_size + 2]; register char *source = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]; while ( source > YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) *--dest = *--source; yy_cp += (int) (dest - source); yy_bp += (int) (dest - source); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_buf_size; if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) YY_FATAL_ERROR( "flex scanner push-back overflow" ); } *--yy_cp = (char) c; (yytext_ptr) = yy_bp; (yy_hold_char) = *yy_cp; (yy_c_buf_p) = yy_cp; } #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void) #else static int input (void) #endif { int c; *(yy_c_buf_p) = (yy_hold_char); if ( *(yy_c_buf_p) == YY_END_OF_BUFFER_CHAR ) { /* yy_c_buf_p now points to the character we want to return. * If this occurs *before* the EOB characters, then it's a * valid NUL; if not, then we've hit the end of the buffer. */ if ( (yy_c_buf_p) < &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) /* This was really a NUL. */ *(yy_c_buf_p) = '\0'; else { /* need more input */ int offset = (yy_c_buf_p) - (yytext_ptr); ++(yy_c_buf_p); switch ( yy_get_next_buffer( ) ) { case EOB_ACT_LAST_MATCH: /* This happens because yy_g_n_b() * sees that we've accumulated a * token and flags that we need to * try matching the token before * proceeding. But for input(), * there's no matching to consider. * So convert the EOB_ACT_LAST_MATCH * to EOB_ACT_END_OF_FILE. */ /* Reset buffer status. */ wcspihrestart(wcspihin ); /*FALLTHROUGH*/ case EOB_ACT_END_OF_FILE: { if ( wcspihwrap( ) ) return EOF; if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; #ifdef __cplusplus return yyinput(); #else return input(); #endif } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + offset; break; } } } c = *(unsigned char *) (yy_c_buf_p); /* cast for 8-bit char's */ *(yy_c_buf_p) = '\0'; /* preserve wcspihtext */ (yy_hold_char) = *++(yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_at_bol = (c == '\n'); return c; } #endif /* ifndef YY_NO_INPUT */ /** Immediately switch to a different input stream. * @param input_file A readable stream. * * @note This function does not reset the start condition to @c INITIAL . */ void wcspihrestart (FILE * input_file ) { if ( ! YY_CURRENT_BUFFER ){ wcspihensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcspih_create_buffer(wcspihin,YY_BUF_SIZE ); } wcspih_init_buffer(YY_CURRENT_BUFFER,input_file ); wcspih_load_buffer_state( ); } /** Switch to a different input buffer. * @param new_buffer The new input buffer. * */ void wcspih_switch_to_buffer (YY_BUFFER_STATE new_buffer ) { /* TODO. We should be able to replace this entire function body * with * wcspihpop_buffer_state(); * wcspihpush_buffer_state(new_buffer); */ wcspihensure_buffer_stack (); if ( YY_CURRENT_BUFFER == new_buffer ) return; if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } YY_CURRENT_BUFFER_LVALUE = new_buffer; wcspih_load_buffer_state( ); /* We don't actually know whether we did this switch during * EOF (wcspihwrap()) processing, but the only time this flag * is looked at is after wcspihwrap() is called, so it's safe * to go ahead and always set it. */ (yy_did_buffer_switch_on_eof) = 1; } static void wcspih_load_buffer_state (void) { (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; (yytext_ptr) = (yy_c_buf_p) = YY_CURRENT_BUFFER_LVALUE->yy_buf_pos; wcspihin = YY_CURRENT_BUFFER_LVALUE->yy_input_file; (yy_hold_char) = *(yy_c_buf_p); } /** Allocate and initialize an input buffer state. * @param file A readable stream. * @param size The character buffer size in bytes. When in doubt, use @c YY_BUF_SIZE. * * @return the allocated buffer state. */ YY_BUFFER_STATE wcspih_create_buffer (FILE * file, int size ) { YY_BUFFER_STATE b; b = (YY_BUFFER_STATE) wcspihalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcspih_create_buffer()" ); b->yy_buf_size = size; /* yy_ch_buf has to be 2 characters longer than the size given because * we need to put in 2 end-of-buffer characters. */ b->yy_ch_buf = (char *) wcspihalloc(b->yy_buf_size + 2 ); if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in wcspih_create_buffer()" ); b->yy_is_our_buffer = 1; wcspih_init_buffer(b,file ); return b; } /** Destroy the buffer. * @param b a buffer created with wcspih_create_buffer() * */ void wcspih_delete_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; if ( b == YY_CURRENT_BUFFER ) /* Not sure if we should pop here. */ YY_CURRENT_BUFFER_LVALUE = (YY_BUFFER_STATE) 0; if ( b->yy_is_our_buffer ) wcspihfree((void *) b->yy_ch_buf ); wcspihfree((void *) b ); } /* Initializes or reinitializes a buffer. * This function is sometimes called more than once on the same buffer, * such as during a wcspihrestart() or at EOF. */ static void wcspih_init_buffer (YY_BUFFER_STATE b, FILE * file ) { int oerrno = errno; wcspih_flush_buffer(b ); b->yy_input_file = file; b->yy_fill_buffer = 1; /* If b is the current buffer, then wcspih_init_buffer was _probably_ * called from wcspihrestart() or through yy_get_next_buffer. * In that case, we don't want to reset the lineno or column. */ if (b != YY_CURRENT_BUFFER){ b->yy_bs_lineno = 1; b->yy_bs_column = 0; } b->yy_is_interactive = 0; errno = oerrno; } /** Discard all buffered characters. On the next scan, YY_INPUT will be called. * @param b the buffer state to be flushed, usually @c YY_CURRENT_BUFFER. * */ void wcspih_flush_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; b->yy_n_chars = 0; /* We always need two end-of-buffer characters. The first causes * a transition to the end-of-buffer state. The second causes * a jam in that state. */ b->yy_ch_buf[0] = YY_END_OF_BUFFER_CHAR; b->yy_ch_buf[1] = YY_END_OF_BUFFER_CHAR; b->yy_buf_pos = &b->yy_ch_buf[0]; b->yy_at_bol = 1; b->yy_buffer_status = YY_BUFFER_NEW; if ( b == YY_CURRENT_BUFFER ) wcspih_load_buffer_state( ); } /** Pushes the new state onto the stack. The new state becomes * the current state. This function will allocate the stack * if necessary. * @param new_buffer The new state. * */ void wcspihpush_buffer_state (YY_BUFFER_STATE new_buffer ) { if (new_buffer == NULL) return; wcspihensure_buffer_stack(); /* This block is copied from wcspih_switch_to_buffer. */ if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } /* Only push if top exists. Otherwise, replace top. */ if (YY_CURRENT_BUFFER) (yy_buffer_stack_top)++; YY_CURRENT_BUFFER_LVALUE = new_buffer; /* copied from wcspih_switch_to_buffer. */ wcspih_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } /** Removes and deletes the top of the stack, if present. * The next element becomes the new top. * */ void wcspihpop_buffer_state (void) { if (!YY_CURRENT_BUFFER) return; wcspih_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; if ((yy_buffer_stack_top) > 0) --(yy_buffer_stack_top); if (YY_CURRENT_BUFFER) { wcspih_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } } /* Allocates the stack if it does not exist. * Guarantees space for at least one push. */ static void wcspihensure_buffer_stack (void) { int num_to_alloc; if (!(yy_buffer_stack)) { /* First allocation is just for 2 elements, since we don't know if this * scanner will even need a stack. We use 2 instead of 1 to avoid an * immediate realloc on the next call. */ num_to_alloc = 1; (yy_buffer_stack) = (struct yy_buffer_state**)wcspihalloc (num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcspihensure_buffer_stack()" ); memset((yy_buffer_stack), 0, num_to_alloc * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; (yy_buffer_stack_top) = 0; return; } if ((yy_buffer_stack_top) >= ((yy_buffer_stack_max)) - 1){ /* Increase the buffer to prepare for a possible push. */ int grow_size = 8 /* arbitrary grow size */; num_to_alloc = (yy_buffer_stack_max) + grow_size; (yy_buffer_stack) = (struct yy_buffer_state**)wcspihrealloc ((yy_buffer_stack), num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcspihensure_buffer_stack()" ); /* zero only the new slots.*/ memset((yy_buffer_stack) + (yy_buffer_stack_max), 0, grow_size * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; } } /** Setup the input buffer state to scan directly from a user-specified character buffer. * @param base the character buffer * @param size the size in bytes of the character buffer * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcspih_scan_buffer (char * base, yy_size_t size ) { YY_BUFFER_STATE b; if ( size < 2 || base[size-2] != YY_END_OF_BUFFER_CHAR || base[size-1] != YY_END_OF_BUFFER_CHAR ) /* They forgot to leave room for the EOB's. */ return 0; b = (YY_BUFFER_STATE) wcspihalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcspih_scan_buffer()" ); b->yy_buf_size = size - 2; /* "- 2" to take care of EOB's */ b->yy_buf_pos = b->yy_ch_buf = base; b->yy_is_our_buffer = 0; b->yy_input_file = 0; b->yy_n_chars = b->yy_buf_size; b->yy_is_interactive = 0; b->yy_at_bol = 1; b->yy_fill_buffer = 0; b->yy_buffer_status = YY_BUFFER_NEW; wcspih_switch_to_buffer(b ); return b; } /** Setup the input buffer state to scan a string. The next call to wcspihlex() will * scan from a @e copy of @a str. * @param yystr a NUL-terminated string to scan * * @return the newly allocated buffer state object. * @note If you want to scan bytes that may contain NUL values, then use * wcspih_scan_bytes() instead. */ YY_BUFFER_STATE wcspih_scan_string (yyconst char * yystr ) { return wcspih_scan_bytes(yystr,strlen(yystr) ); } /** Setup the input buffer state to scan the given bytes. The next call to wcspihlex() will * scan from a @e copy of @a bytes. * @param yybytes the byte buffer to scan * @param _yybytes_len the number of bytes in the buffer pointed to by @a bytes. * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcspih_scan_bytes (yyconst char * yybytes, int _yybytes_len ) { YY_BUFFER_STATE b; char *buf; yy_size_t n; int i; /* Get memory for full buffer, including space for trailing EOB's. */ n = _yybytes_len + 2; buf = (char *) wcspihalloc(n ); if ( ! buf ) YY_FATAL_ERROR( "out of dynamic memory in wcspih_scan_bytes()" ); for ( i = 0; i < _yybytes_len; ++i ) buf[i] = yybytes[i]; buf[_yybytes_len] = buf[_yybytes_len+1] = YY_END_OF_BUFFER_CHAR; b = wcspih_scan_buffer(buf,n ); if ( ! b ) YY_FATAL_ERROR( "bad buffer in wcspih_scan_bytes()" ); /* It's okay to grow etc. this buffer, and we should throw it * away when we're done. */ b->yy_is_our_buffer = 1; return b; } #ifndef YY_EXIT_FAILURE #define YY_EXIT_FAILURE 2 #endif static void yy_fatal_error (yyconst char* msg ) { (void) fprintf( stderr, "%s\n", msg ); exit( YY_EXIT_FAILURE ); } /* Redefine yyless() so it works in section 3 code. */ #undef yyless #define yyless(n) \ do \ { \ /* Undo effects of setting up wcspihtext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ wcspihtext[wcspihleng] = (yy_hold_char); \ (yy_c_buf_p) = wcspihtext + yyless_macro_arg; \ (yy_hold_char) = *(yy_c_buf_p); \ *(yy_c_buf_p) = '\0'; \ wcspihleng = yyless_macro_arg; \ } \ while ( 0 ) /* Accessor methods (get/set functions) to struct members. */ /** Get the current line number. * */ int wcspihget_lineno (void) { return wcspihlineno; } /** Get the input stream. * */ FILE *wcspihget_in (void) { return wcspihin; } /** Get the output stream. * */ FILE *wcspihget_out (void) { return wcspihout; } /** Get the length of the current token. * */ int wcspihget_leng (void) { return wcspihleng; } /** Get the current token. * */ char *wcspihget_text (void) { return wcspihtext; } /** Set the current line number. * @param line_number * */ void wcspihset_lineno (int line_number ) { wcspihlineno = line_number; } /** Set the input stream. This does not discard the current * input buffer. * @param in_str A readable stream. * * @see wcspih_switch_to_buffer */ void wcspihset_in (FILE * in_str ) { wcspihin = in_str ; } void wcspihset_out (FILE * out_str ) { wcspihout = out_str ; } int wcspihget_debug (void) { return wcspih_flex_debug; } void wcspihset_debug (int bdebug ) { wcspih_flex_debug = bdebug ; } static int yy_init_globals (void) { /* Initialization is the same as for the non-reentrant scanner. * This function is called from wcspihlex_destroy(), so don't allocate here. */ (yy_buffer_stack) = 0; (yy_buffer_stack_top) = 0; (yy_buffer_stack_max) = 0; (yy_c_buf_p) = (char *) 0; (yy_init) = 0; (yy_start) = 0; /* Defined in main.c */ #ifdef YY_STDINIT wcspihin = stdin; wcspihout = stdout; #else wcspihin = (FILE *) 0; wcspihout = (FILE *) 0; #endif /* For future reference: Set errno on error, since we are called by * wcspihlex_init() */ return 0; } /* wcspihlex_destroy is for both reentrant and non-reentrant scanners. */ int wcspihlex_destroy (void) { /* Pop the buffer stack, destroying each element. */ while(YY_CURRENT_BUFFER){ wcspih_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; wcspihpop_buffer_state(); } /* Destroy the stack itself. */ wcspihfree((yy_buffer_stack) ); (yy_buffer_stack) = NULL; /* Reset the globals. This is important in a non-reentrant scanner so the next time * wcspihlex() is called, initialization will occur. */ yy_init_globals( ); return 0; } /* * Internal utility routines. */ #ifndef yytext_ptr static void yy_flex_strncpy (char* s1, yyconst char * s2, int n ) { register int i; for ( i = 0; i < n; ++i ) s1[i] = s2[i]; } #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * s ) { register int n; for ( n = 0; s[n]; ++n ) ; return n; } #endif void *wcspihalloc (yy_size_t size ) { return (void *) malloc( size ); } void *wcspihrealloc (void * ptr, yy_size_t size ) { /* The cast to (char *) in the following accommodates both * implementations that use char* generic pointers, and those * that use void* generic pointers. It works with the latter * because both ANSI C and C++ allow castless assignment from * any pointer type to void*, and deal with argument conversions * as though doing an assignment. */ return (void *) realloc( (char *) ptr, size ); } void wcspihfree (void * ptr ) { free( (char *) ptr ); /* see wcspihrealloc() for (char *) cast */ } #define YYTABLES_NAME "yytables" #line 1024 "wcspih.l" /*---------------------------------------------------------------------------- * Determine the number of coordinate representations (up to 27) and the * number of coordinate axes in each, and count the number of PVi_ma and * PSi_ma keywords in each representation. *---------------------------------------------------------------------------*/ void wcspih_naxes(int naxis, int i, int j, char a, int alts[], int *npptr) { /* On the first pass alts[] is used to determine the number of axes */ /* for each of the 27 possible alternate coordinate descriptions. */ int ialt, *ip; if (a == 0) { return; } ialt = 0; if (a != ' ') { ialt = a - 'A' + 1; } ip = alts + ialt; if (*ip < naxis) { *ip = naxis; } /* i or j can be greater than naxis. */ if (*ip < i) { *ip = i; } if (*ip < j) { *ip = j; } if (npptr) { npptr[ialt]++; } } /*---------------------------------------------------------------------------- * Allocate memory for an array of the required number of wcsprm structs and * initialize each of them. *---------------------------------------------------------------------------*/ int wcspih_inits( int naxis, int alts[], int npv[], int nps[], int *nwcs, struct wcsprm **wcs) { int ialt, npsmax, npvmax, status = 0; struct wcsprm *wcsp; /* Find the number of coordinate descriptions. */ *nwcs = 0; for (ialt = 0; ialt < 27; ialt++) { if (alts[ialt]) (*nwcs)++; } if (!(*nwcs) && naxis) { /* NAXIS is non-zero but there were no WCS keywords with an alternate version code; create a default WCS with blank alternate version. */ wcspih_naxes(naxis, 0, 0, ' ', alts, 0x0); *nwcs = 1; } if (*nwcs) { /* Allocate memory for the required number of wcsprm structs. */ if (!(*wcs = calloc(*nwcs, sizeof(struct wcsprm)))) { return 2; } /* Record the current values of NPVMAX and NPSMAX. */ npvmax = wcsnpv(-1); npsmax = wcsnps(-1); /* Initialize each wcsprm struct. */ wcsp = *wcs; *nwcs = 0; for (ialt = 0; ialt < 27; ialt++) { if (alts[ialt]) { wcsp->flag = -1; wcsnpv(npv[ialt]); wcsnps(nps[ialt]); if ((status = wcsini(1, alts[ialt], wcsp))) { wcsvfree(nwcs, wcs); break; } /* Record the alternate version code. */ if (ialt) { wcsp->alt[0] = 'A' + ialt - 1; } /* On the second pass alts[] indexes the array of wcsprm structs. */ alts[ialt] = (*nwcs)++; wcsp++; } } /* Restore the original values of NPVMAX and NPSMAX. */ wcsnpv(npvmax); wcsnps(npsmax); } return status; } /*---------------------------------------------------------------------------- * Interpret special keywords encountered for each coordinate representation. *---------------------------------------------------------------------------*/ int wcspih_final( int alts[], double epoch[], double vsource[], int *nwcs, struct wcsprm **wcs) { int ialt, status; double beta, c = 299792458.0; for (ialt = 0; ialt < *nwcs; ialt++) { /* Check for EPOCH overriding EQUINOXa. */ if (undefined((*wcs+ialt)->equinox) && !undefined(epoch[ialt])) { /* Set EQUINOXa. */ (*wcs+ialt)->equinox = epoch[ialt]; } /* Check for VSOURCEa overriding ZSOURCEa. */ if (undefined((*wcs+ialt)->zsource) && !undefined(vsource[ialt])) { /* Convert relativistic Doppler velocity to redshift. */ beta = vsource[ialt]/c; (*wcs+ialt)->zsource = (1.0+beta)/sqrt(1.0 - beta*beta) - 1.0; } /* Interpret -TAB header keywords. */ if ((status = wcstab(*wcs+ialt))) { wcsvfree(nwcs, wcs); return status; } } return 0; } pywcs-1.12/wcslib/C/flexed/wcsulex.c0000644001153600020070000135070712310355626021435 0ustar cslocumSTSCI\science00000000000000#line 2 "wcsulex.c" #line 4 "wcsulex.c" #define YY_INT_ALIGNED short int /* A lexical scanner generated by flex */ #define yy_create_buffer wcsulex_create_buffer #define yy_delete_buffer wcsulex_delete_buffer #define yy_flex_debug wcsulex_flex_debug #define yy_init_buffer wcsulex_init_buffer #define yy_flush_buffer wcsulex_flush_buffer #define yy_load_buffer_state wcsulex_load_buffer_state #define yy_switch_to_buffer wcsulex_switch_to_buffer #define yyin wcsulexin #define yyleng wcsulexleng #define yylex wcsulexlex #define yylineno wcsulexlineno #define yyout wcsulexout #define yyrestart wcsulexrestart #define yytext wcsulextext #define yywrap wcsulexwrap #define yyalloc wcsulexalloc #define yyrealloc wcsulexrealloc #define yyfree wcsulexfree #define FLEX_SCANNER #define YY_FLEX_MAJOR_VERSION 2 #define YY_FLEX_MINOR_VERSION 5 #define YY_FLEX_SUBMINOR_VERSION 35 #if YY_FLEX_SUBMINOR_VERSION > 0 #define FLEX_BETA #endif /* First, we deal with platform-specific or compiler-specific issues. */ /* begin standard C headers. */ #include #include #include #include /* end standard C headers. */ /* flex integer type definitions */ #ifndef FLEXINT_H #define FLEXINT_H /* C99 systems have . Non-C99 systems may or may not. */ #if defined (__STDC_VERSION__) && __STDC_VERSION__ >= 199901L /* C99 says to define __STDC_LIMIT_MACROS before including stdint.h, * if you want the limit (max/min) macros for int types. */ #ifndef __STDC_LIMIT_MACROS #define __STDC_LIMIT_MACROS 1 #endif #include typedef int8_t flex_int8_t; typedef uint8_t flex_uint8_t; typedef int16_t flex_int16_t; typedef uint16_t flex_uint16_t; typedef int32_t flex_int32_t; typedef uint32_t flex_uint32_t; #else typedef signed char flex_int8_t; typedef short int flex_int16_t; typedef int flex_int32_t; typedef unsigned char flex_uint8_t; typedef unsigned short int flex_uint16_t; typedef unsigned int flex_uint32_t; /* Limits of integral types. */ #ifndef INT8_MIN #define INT8_MIN (-128) #endif #ifndef INT16_MIN #define INT16_MIN (-32767-1) #endif #ifndef INT32_MIN #define INT32_MIN (-2147483647-1) #endif #ifndef INT8_MAX #define INT8_MAX (127) #endif #ifndef INT16_MAX #define INT16_MAX (32767) #endif #ifndef INT32_MAX #define INT32_MAX (2147483647) #endif #ifndef UINT8_MAX #define UINT8_MAX (255U) #endif #ifndef UINT16_MAX #define UINT16_MAX (65535U) #endif #ifndef UINT32_MAX #define UINT32_MAX (4294967295U) #endif #endif /* ! C99 */ #endif /* ! FLEXINT_H */ #ifdef __cplusplus /* The "const" storage-class-modifier is valid. */ #define YY_USE_CONST #else /* ! __cplusplus */ /* C99 requires __STDC__ to be defined as 1. */ #if defined (__STDC__) #define YY_USE_CONST #endif /* defined (__STDC__) */ #endif /* ! __cplusplus */ #ifdef YY_USE_CONST #define yyconst const #else #define yyconst #endif /* Returned upon end-of-file. */ #define YY_NULL 0 /* Promotes a possibly negative, possibly signed char to an unsigned * integer for use as an array index. If the signed char is negative, * we want to instead treat it as an 8-bit unsigned char, hence the * double cast. */ #define YY_SC_TO_UI(c) ((unsigned int) (unsigned char) c) /* Enter a start condition. This macro really ought to take a parameter, * but we do it the disgusting crufty way forced on us by the ()-less * definition of BEGIN. */ #define BEGIN (yy_start) = 1 + 2 * /* Translate the current start state into a value that can be later handed * to BEGIN to return to the state. The YYSTATE alias is for lex * compatibility. */ #define YY_START (((yy_start) - 1) / 2) #define YYSTATE YY_START /* Action number for EOF rule of a given start state. */ #define YY_STATE_EOF(state) (YY_END_OF_BUFFER + state + 1) /* Special action meaning "start processing a new file". */ #define YY_NEW_FILE wcsulexrestart(wcsulexin ) #define YY_END_OF_BUFFER_CHAR 0 /* Size of default input buffer. */ #ifndef YY_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k. * Moreover, YY_BUF_SIZE is 2*YY_READ_BUF_SIZE in the general case. * Ditto for the __ia64__ case accordingly. */ #define YY_BUF_SIZE 32768 #else #define YY_BUF_SIZE 16384 #endif /* __ia64__ */ #endif /* The state buf must be large enough to hold one state per character in the main buffer. */ #define YY_STATE_BUF_SIZE ((YY_BUF_SIZE + 2) * sizeof(yy_state_type)) #ifndef YY_TYPEDEF_YY_BUFFER_STATE #define YY_TYPEDEF_YY_BUFFER_STATE typedef struct yy_buffer_state *YY_BUFFER_STATE; #endif extern int wcsulexleng; extern FILE *wcsulexin, *wcsulexout; #define EOB_ACT_CONTINUE_SCAN 0 #define EOB_ACT_END_OF_FILE 1 #define EOB_ACT_LAST_MATCH 2 #define YY_LESS_LINENO(n) /* Return all but the first "n" matched characters back to the input stream. */ #define yyless(n) \ do \ { \ /* Undo effects of setting up wcsulextext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ *yy_cp = (yy_hold_char); \ YY_RESTORE_YY_MORE_OFFSET \ (yy_c_buf_p) = yy_cp = yy_bp + yyless_macro_arg - YY_MORE_ADJ; \ YY_DO_BEFORE_ACTION; /* set up wcsulextext again */ \ } \ while ( 0 ) #define unput(c) yyunput( c, (yytext_ptr) ) #ifndef YY_TYPEDEF_YY_SIZE_T #define YY_TYPEDEF_YY_SIZE_T typedef size_t yy_size_t; #endif #ifndef YY_STRUCT_YY_BUFFER_STATE #define YY_STRUCT_YY_BUFFER_STATE struct yy_buffer_state { FILE *yy_input_file; char *yy_ch_buf; /* input buffer */ char *yy_buf_pos; /* current position in input buffer */ /* Size of input buffer in bytes, not including room for EOB * characters. */ yy_size_t yy_buf_size; /* Number of characters read into yy_ch_buf, not including EOB * characters. */ int yy_n_chars; /* Whether we "own" the buffer - i.e., we know we created it, * and can realloc() it to grow it, and should free() it to * delete it. */ int yy_is_our_buffer; /* Whether this is an "interactive" input source; if so, and * if we're using stdio for input, then we want to use getc() * instead of fread(), to make sure we stop fetching input after * each newline. */ int yy_is_interactive; /* Whether we're considered to be at the beginning of a line. * If so, '^' rules will be active on the next match, otherwise * not. */ int yy_at_bol; int yy_bs_lineno; /**< The line count. */ int yy_bs_column; /**< The column count. */ /* Whether to try to fill the input buffer when we reach the * end of it. */ int yy_fill_buffer; int yy_buffer_status; #define YY_BUFFER_NEW 0 #define YY_BUFFER_NORMAL 1 /* When an EOF's been seen but there's still some text to process * then we mark the buffer as YY_EOF_PENDING, to indicate that we * shouldn't try reading from the input source any more. We might * still have a bunch of tokens to match, though, because of * possible backing-up. * * When we actually see the EOF, we change the status to "new" * (via wcsulexrestart()), so that the user can continue scanning by * just pointing wcsulexin at a new input file. */ #define YY_BUFFER_EOF_PENDING 2 }; #endif /* !YY_STRUCT_YY_BUFFER_STATE */ /* Stack of input buffers. */ static size_t yy_buffer_stack_top = 0; /**< index of top of stack. */ static size_t yy_buffer_stack_max = 0; /**< capacity of stack. */ static YY_BUFFER_STATE * yy_buffer_stack = 0; /**< Stack as an array. */ /* We provide macros for accessing buffer states in case in the * future we want to put the buffer states in a more general * "scanner state". * * Returns the top of the stack, or NULL. */ #define YY_CURRENT_BUFFER ( (yy_buffer_stack) \ ? (yy_buffer_stack)[(yy_buffer_stack_top)] \ : NULL) /* Same as previous macro, but useful when we know that the buffer stack is not * NULL or when we need an lvalue. For internal use only. */ #define YY_CURRENT_BUFFER_LVALUE (yy_buffer_stack)[(yy_buffer_stack_top)] /* yy_hold_char holds the character lost when wcsulextext is formed. */ static char yy_hold_char; static int yy_n_chars; /* number of characters read into yy_ch_buf */ int wcsulexleng; /* Points to current character in buffer. */ static char *yy_c_buf_p = (char *) 0; static int yy_init = 0; /* whether we need to initialize */ static int yy_start = 0; /* start state number */ /* Flag which is used to allow wcsulexwrap()'s to do buffer switches * instead of setting up a fresh wcsulexin. A bit of a hack ... */ static int yy_did_buffer_switch_on_eof; void wcsulexrestart (FILE *input_file ); void wcsulex_switch_to_buffer (YY_BUFFER_STATE new_buffer ); YY_BUFFER_STATE wcsulex_create_buffer (FILE *file,int size ); void wcsulex_delete_buffer (YY_BUFFER_STATE b ); void wcsulex_flush_buffer (YY_BUFFER_STATE b ); void wcsulexpush_buffer_state (YY_BUFFER_STATE new_buffer ); void wcsulexpop_buffer_state (void ); static void wcsulexensure_buffer_stack (void ); static void wcsulex_load_buffer_state (void ); static void wcsulex_init_buffer (YY_BUFFER_STATE b,FILE *file ); #define YY_FLUSH_BUFFER wcsulex_flush_buffer(YY_CURRENT_BUFFER ) YY_BUFFER_STATE wcsulex_scan_buffer (char *base,yy_size_t size ); YY_BUFFER_STATE wcsulex_scan_string (yyconst char *yy_str ); YY_BUFFER_STATE wcsulex_scan_bytes (yyconst char *bytes,int len ); void *wcsulexalloc (yy_size_t ); void *wcsulexrealloc (void *,yy_size_t ); void wcsulexfree (void * ); #define yy_new_buffer wcsulex_create_buffer #define yy_set_interactive(is_interactive) \ { \ if ( ! YY_CURRENT_BUFFER ){ \ wcsulexensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcsulex_create_buffer(wcsulexin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_is_interactive = is_interactive; \ } #define yy_set_bol(at_bol) \ { \ if ( ! YY_CURRENT_BUFFER ){\ wcsulexensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcsulex_create_buffer(wcsulexin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = at_bol; \ } #define YY_AT_BOL() (YY_CURRENT_BUFFER_LVALUE->yy_at_bol) /* Begin user sect3 */ #define wcsulexwrap(n) 1 #define YY_SKIP_YYWRAP typedef char YY_CHAR; FILE *wcsulexin = (FILE *) 0, *wcsulexout = (FILE *) 0; typedef int yy_state_type; extern int wcsulexlineno; int wcsulexlineno = 1; extern char *wcsulextext; #define yytext_ptr wcsulextext static yyconst flex_int16_t yy_nxt[][128] = { { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 }, { 13, 14, 14, 14, 14, 14, 14, 14, 14, 14, 15, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 16, 14, 14, 14, 14, 14, 14, 14, 17, 14, 18, 14, 14, 14, 18, 19, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 20, 21, 22, 23, 24, 22, 25, 26, 14, 27, 28, 14, 24, 22, 29, 30, 14, 31, 32, 33, 14, 22, 34, 14, 24, 24, 14, 14, 35, 14, 14, 14, 36, 37, 38, 39, 40, 41, 28, 42, 14, 14, 24, 43, 44, 41, 29, 45, 14, 46, 47, 14, 48, 49, 14, 14, 50, 41, 14, 14, 14, 14, 14 }, { 13, 14, 14, 14, 14, 14, 14, 14, 14, 14, 15, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 51, 14, 14, 14, 14, 14, 14, 14, 17, 14, 52, 14, 14, 14, 52, 19, 14, 53, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 14, 20, 21, 22, 23, 24, 22, 25, 26, 14, 27, 28, 14, 24, 22, 29, 30, 14, 31, 32, 33, 14, 22, 34, 14, 24, 24, 54, 14, 35, 14, 14, 14, 36, 37, 38, 39, 55, 41, 28, 42, 14, 14, 24, 56, 44, 41, 29, 45, 14, 46, 47, 14, 48, 49, 14, 14, 50, 41, 14, 14, 14, 14, 14 }, { 13, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 58, 59, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57 }, { 13, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 58, 59, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57, 57 }, { 13, 60, 60, 60, 60, 60, 60, 60, 60, 60, 15, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 61, 60, 62, 60, 60, 60, 60, 60, 63, 60, 60, 64, 60, 60, 60, 65, 60, 60, 60, 60, 66, 67, 60, 60, 60, 60, 60, 60, 68, 60, 69, 70, 60, 71, 60, 72, 60, 60, 73, 60, 74, 75, 60, 76, 60, 60, 60, 60, 77, 60, 60, 60, 78, 79, 60, 60, 60, 60, 60 }, { 13, 60, 60, 60, 60, 60, 60, 60, 60, 60, 15, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 60, 61, 60, 62, 60, 60, 60, 60, 60, 63, 60, 60, 64, 60, 60, 60, 65, 60, 60, 60, 60, 66, 67, 60, 60, 60, 60, 60, 60, 68, 60, 69, 70, 60, 71, 60, 72, 60, 60, 73, 60, 74, 75, 60, 76, 60, 60, 60, 60, 77, 60, 60, 60, 78, 79, 60, 60, 60, 60, 60 }, { 13, 80, 80, 80, 80, 80, 80, 80, 80, 80, 15, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 81, 82, 83, 84, 80, 85, 86, 87, 80, 88, 89, 80, 80, 90, 91, 92, 80, 93, 94, 95, 80, 96, 97, 80, 80, 80, 80, 80, 80, 80, 80, 80, 98, 99, 100, 101, 102, 80, 103, 104, 80, 80, 80, 105, 106, 80, 91, 107, 80, 108, 109, 80, 110, 111, 80, 80, 112, 80, 80, 80, 80, 80, 80 }, { 13, 80, 80, 80, 80, 80, 80, 80, 80, 80, 15, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 80, 81, 82, 83, 84, 80, 85, 86, 87, 80, 88, 89, 80, 80, 90, 91, 92, 80, 93, 94, 95, 80, 96, 97, 80, 80, 80, 80, 80, 80, 80, 80, 80, 98, 99, 100, 101, 102, 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-364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, 366, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364, -364 }, { 13, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365, -365 }, { 13, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366, -366 }, } ; static yy_state_type yy_get_previous_state (void ); static yy_state_type yy_try_NUL_trans (yy_state_type current_state ); static int yy_get_next_buffer (void ); static void yy_fatal_error (yyconst char msg[] ); /* Done after the current pattern has been matched and before the * corresponding action - sets up wcsulextext. */ #define YY_DO_BEFORE_ACTION \ (yytext_ptr) = yy_bp; \ (yytext_ptr) -= (yy_more_len); \ wcsulexleng = (size_t) (yy_cp - (yytext_ptr)); \ (yy_hold_char) = *yy_cp; \ *yy_cp = '\0'; \ (yy_c_buf_p) = yy_cp; #define YY_NUM_RULES 118 #define YY_END_OF_BUFFER 119 /* This struct is not used in this scanner, but its presence is necessary. */ struct yy_trans_info { flex_int32_t yy_verify; flex_int32_t yy_nxt; }; static yyconst flex_int16_t yy_accept[367] = { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 117, 117, 119, 20, 118, 9, 11, 12, 14, 15, 20, 15, 15, 20, 15, 15, 15, 15, 20, 20, 15, 15, 15, 15, 19, 15, 20, 20, 15, 20, 20, 15, 20, 15, 20, 20, 15, 15, 20, 20, 1, 8, 20, 2, 20, 20, 23, 21, 22, 44, 41, 38, 37, 40, 39, 43, 42, 31, 25, 24, 30, 35, 36, 26, 28, 29, 27, 33, 32, 105, 45, 105, 57, 61, 66, 67, 69, 72, 74, 83, 105, 105, 89, 92, 99, 101, 103, 46, 105, 105, 62, 105, 68, 70, 105, 78, 105, 105, 93, 100, 105, 105, 116, 113, 112, 111, 116, 111, 114, 107, 115, 106, 117, 9, 15, 0, 0, 16, 0, 16, 16, 16, 16, 0, 0, 16, 17, 0, 0, 0, 0, 16, 0, 0, 16, 0, 15, 15, 0, 15, 15, 0, 0, 0, 16, 0, 0, 0, 0, 15, 0, 0, 15, 0, 0, 0, 0, 0, 0, 0, 15, 15, 0, 0, 0, 0, 0, 15, 1, 13, 4, 0, 0, 0, 23, 34, 51, 0, 0, 71, 73, 0, 85, 91, 0, 104, 0, 0, 0, 0, 0, 58, 0, 0, 60, 0, 65, 0, 75, 76, 0, 0, 0, 0, 86, 87, 0, 0, 0, 97, 0, 46, 113, 112, 111, 0, 111, 114, 107, 115, 106, 0, 0, 0, 0, 0, 111, 114, 107, 117, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 15, 0, 0, 0, 15, 0, 0, 0, 3, 0, 0, 6, 0, 0, 0, 84, 98, 47, 0, 0, 0, 54, 55, 0, 0, 63, 64, 77, 79, 80, 81, 82, 0, 88, 90, 0, 0, 0, 0, 110, 0, 0, 0, 108, 0, 0, 0, 0, 0, 18, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 7, 0, 5, 0, 56, 0, 0, 52, 53, 59, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 10, 0, 0, 0, 0, 88, 0, 0, 0, 102, 0, 109, 0, 0, 0, 0, 49, 50, 87, 94, 0, 96, 0, 0, 95, 48 } ; static yy_state_type yy_last_accepting_state; static char *yy_last_accepting_cpos; static yyconst yy_state_type yy_NUL_trans[367] = { 0, 14, 14, 57, 57, 60, 60, 80, 80, 113, 113, 123, 123, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 185, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 240, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 185, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 240, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 } ; extern int wcsulex_flex_debug; int wcsulex_flex_debug = 0; /* The intent behind this definition is that it'll catch * any uses of REJECT which flex missed. */ #define REJECT reject_used_but_not_detected static int yy_more_flag = 0; static int yy_more_len = 0; #define yymore() ((yy_more_flag) = 1) #define YY_MORE_ADJ (yy_more_len) #define YY_RESTORE_YY_MORE_OFFSET char *wcsulextext; #line 1 "wcsulex.l" /*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsulex.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcsulex.l is a Flex description file containing the definition of a * recursive, multi-buffered lexical scanner that parses FITS units * specifications. * * It requires Flex v2.5.4 or later. * * Refer to wcsunits.h for a description of the user interface and operating * notes. * *===========================================================================*/ /* Options. */ /* Exponents. */ /* Metric prefixes. */ /* Basic and derived SI units. */ /* Additional recognized units: all metric prefixes allowed. */ /* Additional recognized units: only super-metric prefixes allowed. */ /* Additional recognized units: only sub-metric prefixes allowed. */ /* Additional recognized units for which NO metric prefixes are allowed. */ /* All additional recognized units. */ /* Exclusive start states. */ #line 91 "wcsulex.l" /* To get the prototype for fileno() from stdio.h when gcc is invoked with * -std=c89 (same as -ansi) or -std=c99 since we do not define YY_INPUT. */ #define _POSIX_SOURCE 1 #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsunits.h" #define YY_DECL int wcsulexe(const char unitstr[], int *func, double *scale, \ double units[], struct wcserr **err) /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcsulex_abort_jmp_env; #define exit(status) longjmp(wcsulex_abort_jmp_env, status) #line 6937 "wcsulex.c" #define INITIAL 0 #define PAREN 1 #define PREFIX 2 #define UNITS 3 #define EXPON 4 #define FLUSH 5 #ifndef YY_NO_UNISTD_H /* Special case for "unistd.h", since it is non-ANSI. We include it way * down here because we want the user's section 1 to have been scanned first. * The user has a chance to override it with an option. */ #include #endif #ifndef YY_EXTRA_TYPE #define YY_EXTRA_TYPE void * #endif static int yy_init_globals (void ); /* Accessor methods to globals. These are made visible to non-reentrant scanners for convenience. */ int wcsulexlex_destroy (void ); int wcsulexget_debug (void ); void wcsulexset_debug (int debug_flag ); YY_EXTRA_TYPE wcsulexget_extra (void ); void wcsulexset_extra (YY_EXTRA_TYPE user_defined ); FILE *wcsulexget_in (void ); void wcsulexset_in (FILE * in_str ); FILE *wcsulexget_out (void ); void wcsulexset_out (FILE * out_str ); int wcsulexget_leng (void ); char *wcsulexget_text (void ); int wcsulexget_lineno (void ); void wcsulexset_lineno (int line_number ); /* Macros after this point can all be overridden by user definitions in * section 1. */ #ifndef YY_SKIP_YYWRAP #ifdef __cplusplus extern "C" int wcsulexwrap (void ); #else extern int wcsulexwrap (void ); #endif #endif static void yyunput (int c,char *buf_ptr ); #ifndef yytext_ptr static void yy_flex_strncpy (char *,yyconst char *,int ); #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * ); #endif #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void ); #else static int input (void ); #endif #endif /* Amount of stuff to slurp up with each read. */ #ifndef YY_READ_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k */ #define YY_READ_BUF_SIZE 16384 #else #define YY_READ_BUF_SIZE 8192 #endif /* __ia64__ */ #endif /* Copy whatever the last rule matched to the standard output. */ #ifndef ECHO /* This used to be an fputs(), but since the string might contain NUL's, * we now use fwrite(). */ #define ECHO do { if (fwrite( wcsulextext, wcsulexleng, 1, wcsulexout )) {} } while (0) #endif /* Gets input and stuffs it into "buf". number of characters read, or YY_NULL, * is returned in "result". */ #ifndef YY_INPUT #define YY_INPUT(buf,result,max_size) \ errno=0; \ while ( (result = read( fileno(wcsulexin), (char *) buf, max_size )) < 0 ) \ { \ if( errno != EINTR) \ { \ YY_FATAL_ERROR( "input in flex scanner failed" ); \ break; \ } \ errno=0; \ clearerr(wcsulexin); \ }\ \ #endif /* No semi-colon after return; correct usage is to write "yyterminate();" - * we don't want an extra ';' after the "return" because that will cause * some compilers to complain about unreachable statements. */ #ifndef yyterminate #define yyterminate() return YY_NULL #endif /* Number of entries by which start-condition stack grows. */ #ifndef YY_START_STACK_INCR #define YY_START_STACK_INCR 25 #endif /* Report a fatal error. */ #ifndef YY_FATAL_ERROR #define YY_FATAL_ERROR(msg) yy_fatal_error( msg ) #endif /* end tables serialization structures and prototypes */ /* Default declaration of generated scanner - a define so the user can * easily add parameters. */ #ifndef YY_DECL #define YY_DECL_IS_OURS 1 extern int wcsulexlex (void); #define YY_DECL int wcsulexlex (void) #endif /* !YY_DECL */ /* Code executed at the beginning of each rule, after wcsulextext and wcsulexleng * have been set up. */ #ifndef YY_USER_ACTION #define YY_USER_ACTION #endif /* Code executed at the end of each rule. */ #ifndef YY_BREAK #define YY_BREAK break; #endif #define YY_RULE_SETUP \ if ( wcsulexleng > 0 ) \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = \ (wcsulextext[wcsulexleng - 1] == '\n'); \ YY_USER_ACTION /** The main scanner function which does all the work. */ YY_DECL { register yy_state_type yy_current_state; register char *yy_cp, *yy_bp; register int yy_act; #line 113 "wcsulex.l" static const char *function = "wcsulexe"; int bracket = 0; int operator = 0; int paren = 0; int status = 0; int func_r, i, j; double dexp, expon, factor, factor_r, types[WCSUNITS_NTYPE]; YY_BUFFER_STATE buf; void add(double *factor, double types[], double *expon, double *scale, double units[]); int wcsulexlex_destroy(void); *func = 0; for (i = 0; i < WCSUNITS_NTYPE; i++) { units[i] = 0.0; types[i] = 0.0; } expon = 1.0; factor = 1.0; *scale = 1.0; wcsulex_scan_string(unitstr); /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcsulex_abort_jmp_env)) { return wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error parsing '%s'", unitstr); } BEGIN(INITIAL); #ifdef DEBUG fprintf(stderr, "\n%s ->\n", unitstr); #endif #line 7154 "wcsulex.c" if ( !(yy_init) ) { (yy_init) = 1; #ifdef YY_USER_INIT YY_USER_INIT; #endif if ( ! (yy_start) ) (yy_start) = 1; /* first start state */ if ( ! wcsulexin ) wcsulexin = stdin; if ( ! wcsulexout ) wcsulexout = stdout; if ( ! YY_CURRENT_BUFFER ) { wcsulexensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcsulex_create_buffer(wcsulexin,YY_BUF_SIZE ); } wcsulex_load_buffer_state( ); } while ( 1 ) /* loops until end-of-file is reached */ { (yy_more_len) = 0; if ( (yy_more_flag) ) { (yy_more_len) = (yy_c_buf_p) - (yytext_ptr); (yy_more_flag) = 0; } yy_cp = (yy_c_buf_p); /* Support of wcsulextext. */ *yy_cp = (yy_hold_char); /* yy_bp points to the position in yy_ch_buf of the start of * the current run. */ yy_bp = yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); yy_match: while ( (yy_current_state = yy_nxt[yy_current_state][ YY_SC_TO_UI(*yy_cp) ]) > 0 ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } ++yy_cp; } yy_current_state = -yy_current_state; yy_find_action: yy_act = yy_accept[yy_current_state]; YY_DO_BEFORE_ACTION; do_action: /* This label is used only to access EOF actions. */ switch ( yy_act ) { /* beginning of action switch */ case 0: /* must back up */ /* undo the effects of YY_DO_BEFORE_ACTION */ *yy_cp = (yy_hold_char); yy_cp = (yy_last_accepting_cpos) + 1; yy_current_state = (yy_last_accepting_state); goto yy_find_action; case 1: YY_RULE_SETUP #line 150 "wcsulex.l" { /* Pretend initial whitespace doesn't exist. */ yy_set_bol(1); } YY_BREAK case 2: YY_RULE_SETUP #line 155 "wcsulex.l" { if (bracket++) { BEGIN(FLUSH); } else { yy_set_bol(1); } } YY_BREAK case 3: YY_RULE_SETUP #line 163 "wcsulex.l" { status = wcserr_set(WCSERR_SET(UNITSERR_BAD_NUM_MULTIPLIER), "Invalid exponent in '%s'", unitstr); BEGIN(FLUSH); } YY_BREAK case 4: YY_RULE_SETUP #line 169 "wcsulex.l" { factor = 10.0; BEGIN(EXPON); } YY_BREAK case 5: YY_RULE_SETUP #line 174 "wcsulex.l" { *func = 1; unput('('); BEGIN(PAREN); } YY_BREAK case 6: YY_RULE_SETUP #line 180 "wcsulex.l" { *func = 2; unput('('); BEGIN(PAREN); } YY_BREAK case 7: YY_RULE_SETUP #line 186 "wcsulex.l" { *func = 3; unput('('); BEGIN(PAREN); } YY_BREAK case 8: YY_RULE_SETUP #line 192 "wcsulex.l" { /* Leading binary multiply. */ status = wcserr_set(WCSERR_SET(UNITSERR_DANGLING_BINOP), "Dangling binary operator in '%s'", unitstr); BEGIN(FLUSH); } YY_BREAK case 9: YY_RULE_SETUP #line 199 "wcsulex.l" /* Discard whitespace in INITIAL context. */ YY_BREAK case 10: YY_RULE_SETUP #line 201 "wcsulex.l" { expon /= 2.0; unput('('); BEGIN(PAREN); } YY_BREAK case 11: YY_RULE_SETUP #line 207 "wcsulex.l" { /* Gather terms in parentheses. */ yyless(0); BEGIN(PAREN); } YY_BREAK case 12: YY_RULE_SETUP #line 213 "wcsulex.l" { if (operator++) { BEGIN(FLUSH); } } YY_BREAK case 13: #line 220 "wcsulex.l" case 14: YY_RULE_SETUP #line 220 "wcsulex.l" { if (operator++) { BEGIN(FLUSH); } else { expon *= -1.0; } } YY_BREAK case 15: YY_RULE_SETUP #line 228 "wcsulex.l" { operator = 0; yyless(0); BEGIN(UNITS); } YY_BREAK case 16: #line 235 "wcsulex.l" case 17: #line 236 "wcsulex.l" case 18: YY_RULE_SETUP #line 236 "wcsulex.l" { operator = 0; yyless(0); BEGIN(PREFIX); } YY_BREAK case 19: YY_RULE_SETUP #line 242 "wcsulex.l" { bracket = !bracket; BEGIN(FLUSH); } YY_BREAK case 20: YY_RULE_SETUP #line 247 "wcsulex.l" { status = wcserr_set(WCSERR_SET(UNITSERR_BAD_INITIAL_SYMBOL), "Invalid symbol in INITIAL context in '%s'", unitstr); BEGIN(FLUSH); } YY_BREAK case 21: YY_RULE_SETUP #line 253 "wcsulex.l" { paren++; operator = 0; yymore(); } YY_BREAK case 22: YY_RULE_SETUP #line 259 "wcsulex.l" { paren--; if (paren) { /* Not balanced yet. */ yymore(); } else { /* Balanced; strip off the outer parentheses and recurse. */ wcsulextext[wcsulexleng-1] = '\0'; buf = YY_CURRENT_BUFFER; status = wcsulexe(wcsulextext+1, &func_r, &factor_r, types, err); wcsulex_switch_to_buffer(buf); if (func_r) { status = wcserr_set(WCSERR_SET(UNITSERR_FUNCTION_CONTEXT), "Function in invalid context in '%s'", unitstr); } if (status) { BEGIN(FLUSH); } else { factor *= factor_r; BEGIN(EXPON); } } } YY_BREAK case 23: /* rule 23 can match eol */ YY_RULE_SETUP #line 287 "wcsulex.l" { yymore(); } YY_BREAK case 24: YY_RULE_SETUP #line 291 "wcsulex.l" { factor = 1e-1; BEGIN(UNITS); } YY_BREAK case 25: YY_RULE_SETUP #line 296 "wcsulex.l" { factor = 1e-2; BEGIN(UNITS); } YY_BREAK case 26: YY_RULE_SETUP #line 301 "wcsulex.l" { factor = 1e-3; BEGIN(UNITS); } YY_BREAK case 27: YY_RULE_SETUP #line 306 "wcsulex.l" { factor = 1e-6; BEGIN(UNITS); } YY_BREAK case 28: YY_RULE_SETUP #line 311 "wcsulex.l" { factor = 1e-9; BEGIN(UNITS); } YY_BREAK case 29: YY_RULE_SETUP #line 316 "wcsulex.l" { factor = 1e-12; BEGIN(UNITS); } YY_BREAK case 30: YY_RULE_SETUP #line 321 "wcsulex.l" { factor = 1e-15; BEGIN(UNITS); } YY_BREAK case 31: YY_RULE_SETUP #line 326 "wcsulex.l" { factor = 1e-18; BEGIN(UNITS); } YY_BREAK case 32: YY_RULE_SETUP #line 331 "wcsulex.l" { factor = 1e-21; BEGIN(UNITS); } YY_BREAK case 33: YY_RULE_SETUP #line 336 "wcsulex.l" { factor = 1e-24; BEGIN(UNITS); } YY_BREAK case 34: YY_RULE_SETUP #line 341 "wcsulex.l" { factor = 1e+1; BEGIN(UNITS); } YY_BREAK case 35: YY_RULE_SETUP #line 346 "wcsulex.l" { factor = 1e+2; BEGIN(UNITS); } YY_BREAK case 36: YY_RULE_SETUP #line 351 "wcsulex.l" { factor = 1e+3; BEGIN(UNITS); } YY_BREAK case 37: YY_RULE_SETUP #line 356 "wcsulex.l" { factor = 1e+6; BEGIN(UNITS); } YY_BREAK case 38: YY_RULE_SETUP #line 361 "wcsulex.l" { factor = 1e+9; BEGIN(UNITS); } YY_BREAK case 39: YY_RULE_SETUP #line 366 "wcsulex.l" { factor = 1e+12; BEGIN(UNITS); } YY_BREAK case 40: YY_RULE_SETUP #line 371 "wcsulex.l" { factor = 1e+15; BEGIN(UNITS); } YY_BREAK case 41: YY_RULE_SETUP #line 376 "wcsulex.l" { factor = 1e+18; BEGIN(UNITS); } YY_BREAK case 42: YY_RULE_SETUP #line 381 "wcsulex.l" { factor = 1e+21; BEGIN(UNITS); } YY_BREAK case 43: YY_RULE_SETUP #line 386 "wcsulex.l" { factor = 1e+24; BEGIN(UNITS); } YY_BREAK case 44: YY_RULE_SETUP #line 391 "wcsulex.l" { /* Internal parser error. */ status = wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error parsing '%s'", unitstr); BEGIN(FLUSH); } YY_BREAK case 45: YY_RULE_SETUP #line 398 "wcsulex.l" { /* Ampere. */ types[WCSUNITS_CHARGE] += 1.0; types[WCSUNITS_TIME] -= 1.0; BEGIN(EXPON); } YY_BREAK case 46: YY_RULE_SETUP #line 405 "wcsulex.l" { /* Year (annum). */ factor *= 31557600.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } YY_BREAK case 47: YY_RULE_SETUP #line 412 "wcsulex.l" { /* Analogue-to-digital converter units. */ types[WCSUNITS_COUNT] += 1.0; BEGIN(EXPON); } YY_BREAK case 48: YY_RULE_SETUP #line 418 "wcsulex.l" { /* Angstrom. */ factor *= 1e-10; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 49: YY_RULE_SETUP #line 425 "wcsulex.l" { /* Minute of arc. */ factor /= 60.0; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 50: YY_RULE_SETUP #line 432 "wcsulex.l" { /* Second of arc. */ factor /= 3600.0; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 51: YY_RULE_SETUP #line 439 "wcsulex.l" { /* Astronomical unit. */ factor *= 1.49598e+11; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 52: YY_RULE_SETUP #line 446 "wcsulex.l" { /* Barn. */ factor *= 1e-28; types[WCSUNITS_LENGTH] += 2.0; BEGIN(EXPON); } YY_BREAK case 53: YY_RULE_SETUP #line 453 "wcsulex.l" { /* Beam, as in Jy/beam. */ types[WCSUNITS_BEAM] += 1.0; BEGIN(EXPON); } YY_BREAK case 54: YY_RULE_SETUP #line 459 "wcsulex.l" { /* Bin (e.g. histogram). */ types[WCSUNITS_BIN] += 1.0; BEGIN(EXPON); } YY_BREAK case 55: YY_RULE_SETUP #line 465 "wcsulex.l" { /* Bit. */ types[WCSUNITS_BIT] += 1.0; BEGIN(EXPON); } YY_BREAK case 56: YY_RULE_SETUP #line 471 "wcsulex.l" { /* Byte. */ factor *= 8.0; types[WCSUNITS_BIT] += 1.0; BEGIN(EXPON); } YY_BREAK case 57: YY_RULE_SETUP #line 478 "wcsulex.l" { /* Coulomb. */ types[WCSUNITS_CHARGE] += 1.0; BEGIN(EXPON); } YY_BREAK case 58: YY_RULE_SETUP #line 484 "wcsulex.l" { /* Candela. */ types[WCSUNITS_LUMINTEN] += 1.0; BEGIN(EXPON); } YY_BREAK case 59: YY_RULE_SETUP #line 490 "wcsulex.l" { /* Channel. */ types[WCSUNITS_BIN] += 1.0; BEGIN(EXPON); } YY_BREAK case 60: YY_RULE_SETUP #line 496 "wcsulex.l" { /* Count. */ types[WCSUNITS_COUNT] += 1.0; BEGIN(EXPON); } YY_BREAK case 61: YY_RULE_SETUP #line 502 "wcsulex.l" { /* Debye. */ factor *= 1e-29 / 3.0; types[WCSUNITS_CHARGE] += 1.0; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 62: YY_RULE_SETUP #line 510 "wcsulex.l" { /* Day. */ factor *= 86400.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } YY_BREAK case 63: YY_RULE_SETUP #line 517 "wcsulex.l" { /* Degree. */ types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 64: YY_RULE_SETUP #line 523 "wcsulex.l" { /* Erg. */ factor *= 1e-7; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 65: YY_RULE_SETUP #line 532 "wcsulex.l" { /* Electron volt. */ factor *= 1.6021765e-19; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 66: YY_RULE_SETUP #line 541 "wcsulex.l" { /* Farad. */ types[WCSUNITS_MASS] -= 1.0; types[WCSUNITS_LENGTH] -= 2.0; types[WCSUNITS_TIME] += 3.0; types[WCSUNITS_CHARGE] += 2.0; BEGIN(EXPON); } YY_BREAK case 67: YY_RULE_SETUP #line 550 "wcsulex.l" { /* Gauss. */ factor *= 1e-4; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } YY_BREAK case 68: YY_RULE_SETUP #line 559 "wcsulex.l" { /* Gram. */ factor *= 1e-3; types[WCSUNITS_MASS] += 1.0; BEGIN(EXPON); } YY_BREAK case 69: YY_RULE_SETUP #line 566 "wcsulex.l" { /* Henry. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] += 2.0; types[WCSUNITS_CHARGE] -= 2.0; BEGIN(EXPON); } YY_BREAK case 70: YY_RULE_SETUP #line 575 "wcsulex.l" { /* Hour. */ factor *= 3600.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } YY_BREAK case 71: YY_RULE_SETUP #line 582 "wcsulex.l" { /* Hertz. */ types[WCSUNITS_TIME] -= 1.0; BEGIN(EXPON); } YY_BREAK case 72: YY_RULE_SETUP #line 588 "wcsulex.l" { /* Joule. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 73: YY_RULE_SETUP #line 596 "wcsulex.l" { /* Jansky. */ factor *= 1e-26; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 74: YY_RULE_SETUP #line 604 "wcsulex.l" { /* Kelvin. */ types[WCSUNITS_TEMPERATURE] += 1.0; BEGIN(EXPON); } YY_BREAK case 75: YY_RULE_SETUP #line 610 "wcsulex.l" { /* Lumen. */ types[WCSUNITS_LUMINTEN] += 1.0; types[WCSUNITS_SOLID_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 76: YY_RULE_SETUP #line 617 "wcsulex.l" { /* Lux. */ types[WCSUNITS_LUMINTEN] += 1.0; types[WCSUNITS_SOLID_ANGLE] += 1.0; types[WCSUNITS_LENGTH] -= 2.0; BEGIN(EXPON); } YY_BREAK case 77: YY_RULE_SETUP #line 625 "wcsulex.l" { /* Light year. */ factor *= 2.99792458e8 * 31557600.0; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 78: YY_RULE_SETUP #line 632 "wcsulex.l" { /* Metre. */ types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 79: YY_RULE_SETUP #line 638 "wcsulex.l" { /* Stellar magnitude. */ types[WCSUNITS_MAGNITUDE] += 1.0; BEGIN(EXPON); } YY_BREAK case 80: YY_RULE_SETUP #line 644 "wcsulex.l" { /* Milli-arcsec. */ factor /= 3600e+3; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 81: YY_RULE_SETUP #line 651 "wcsulex.l" { /* Minute. */ factor *= 60.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } YY_BREAK case 82: YY_RULE_SETUP #line 658 "wcsulex.l" { /* Mole. */ types[WCSUNITS_MOLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 83: YY_RULE_SETUP #line 664 "wcsulex.l" { /* Newton. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 1.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 84: YY_RULE_SETUP #line 672 "wcsulex.l" { /* Ohm. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 1.0; types[WCSUNITS_CHARGE] -= 2.0; BEGIN(EXPON); } YY_BREAK case 85: YY_RULE_SETUP #line 681 "wcsulex.l" { /* Pascal. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] -= 1.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 86: YY_RULE_SETUP #line 689 "wcsulex.l" { /* Parsec. */ factor *= 3.0857e16; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 87: YY_RULE_SETUP #line 696 "wcsulex.l" { /* Photon. */ types[WCSUNITS_COUNT] += 1.0; BEGIN(EXPON); } YY_BREAK case 88: YY_RULE_SETUP #line 702 "wcsulex.l" { /* Pixel. */ types[WCSUNITS_PIXEL] += 1.0; BEGIN(EXPON); } YY_BREAK case 89: YY_RULE_SETUP #line 708 "wcsulex.l" { /* Rayleigh. */ factor *= 1e10 / (4.0 * PI); types[WCSUNITS_LENGTH] -= 2.0; types[WCSUNITS_TIME] -= 1.0; types[WCSUNITS_SOLID_ANGLE] -= 1.0; BEGIN(EXPON); } YY_BREAK case 90: YY_RULE_SETUP #line 717 "wcsulex.l" { /* Radian. */ factor *= 180.0 / PI; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 91: YY_RULE_SETUP #line 724 "wcsulex.l" { /* Rydberg. */ factor *= 13.605692 * 1.6021765e-19; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } YY_BREAK case 92: YY_RULE_SETUP #line 733 "wcsulex.l" { /* Siemen. */ types[WCSUNITS_MASS] -= 1.0; types[WCSUNITS_LENGTH] -= 2.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] += 2.0; BEGIN(EXPON); } YY_BREAK case 93: YY_RULE_SETUP #line 742 "wcsulex.l" { /* Second. */ types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } YY_BREAK case 94: YY_RULE_SETUP #line 748 "wcsulex.l" { /* Solar luminosity. */ factor *= 3.8268e26; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 3.0; BEGIN(EXPON); } YY_BREAK case 95: YY_RULE_SETUP #line 757 "wcsulex.l" { /* Solar mass. */ factor *= 1.9891e30; types[WCSUNITS_MASS] += 1.0; BEGIN(EXPON); } YY_BREAK case 96: YY_RULE_SETUP #line 764 "wcsulex.l" { /* Solar radius. */ factor *= 6.9599e8; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } YY_BREAK case 97: YY_RULE_SETUP #line 771 "wcsulex.l" { /* Steradian. */ types[WCSUNITS_SOLID_ANGLE] += 1.0; BEGIN(EXPON); } YY_BREAK case 98: YY_RULE_SETUP #line 777 "wcsulex.l" { /* Sun (with respect to). */ types[WCSUNITS_SOLRATIO] += 1.0; BEGIN(EXPON); } YY_BREAK case 99: YY_RULE_SETUP #line 783 "wcsulex.l" { /* Tesla. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } YY_BREAK case 100: YY_RULE_SETUP #line 791 "wcsulex.l" { /* Unified atomic mass unit. */ factor *= 1.6605387e-27; types[WCSUNITS_MASS] += 1.0; BEGIN(EXPON); } YY_BREAK case 101: YY_RULE_SETUP #line 798 "wcsulex.l" { /* Volt. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 1.0; types[WCSUNITS_TIME] -= 2.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } YY_BREAK case 102: YY_RULE_SETUP #line 807 "wcsulex.l" { /* Voxel. */ types[WCSUNITS_VOXEL] += 1.0; BEGIN(EXPON); } YY_BREAK case 103: YY_RULE_SETUP #line 813 "wcsulex.l" { /* Watt. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 3.0; BEGIN(EXPON); } YY_BREAK case 104: YY_RULE_SETUP #line 821 "wcsulex.l" { /* Weber. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } YY_BREAK case 105: YY_RULE_SETUP #line 830 "wcsulex.l" { /* Internal parser error. */ status = wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error parsing '%s'", unitstr); BEGIN(FLUSH); } YY_BREAK case 106: YY_RULE_SETUP #line 837 "wcsulex.l" { /* Exponentiation. */ if (operator++) { BEGIN(FLUSH); } } YY_BREAK case 107: YY_RULE_SETUP #line 844 "wcsulex.l" { sscanf(wcsulextext, " %d", &i); expon *= (double)i; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } YY_BREAK case 108: YY_RULE_SETUP #line 852 "wcsulex.l" { sscanf(wcsulextext, " (%d)", &i); expon *= (double)i; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } YY_BREAK case 109: YY_RULE_SETUP #line 860 "wcsulex.l" { sscanf(wcsulextext, " (%d/%d)", &i, &j); expon *= (double)i / (double)j; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } YY_BREAK case 110: YY_RULE_SETUP #line 868 "wcsulex.l" { sscanf(wcsulextext, " (%lf)", &dexp); expon *= dexp; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } YY_BREAK case 111: YY_RULE_SETUP #line 876 "wcsulex.l" { /* Multiply. */ if (operator++) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); BEGIN(INITIAL); } } YY_BREAK case 112: YY_RULE_SETUP #line 886 "wcsulex.l" { /* Multiply. */ if (operator) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); unput('('); BEGIN(INITIAL); } } YY_BREAK case 113: YY_RULE_SETUP #line 897 "wcsulex.l" { /* Multiply. */ if (operator) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); BEGIN(INITIAL); } } YY_BREAK case 114: YY_RULE_SETUP #line 907 "wcsulex.l" { /* Divide. */ if (operator++) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); expon = -1.0; BEGIN(INITIAL); } } YY_BREAK case 115: YY_RULE_SETUP #line 918 "wcsulex.l" { add(&factor, types, &expon, scale, units); bracket = !bracket; BEGIN(FLUSH); } YY_BREAK case 116: YY_RULE_SETUP #line 924 "wcsulex.l" { status = wcserr_set(WCSERR_SET(UNITSERR_BAD_EXPON_SYMBOL), "Invalid symbol in EXPON context in '%s'", unitstr); BEGIN(FLUSH); } YY_BREAK case 117: YY_RULE_SETUP #line 930 "wcsulex.l" { /* Discard any remaining input. */ } YY_BREAK case YY_STATE_EOF(INITIAL): case YY_STATE_EOF(PAREN): case YY_STATE_EOF(PREFIX): case YY_STATE_EOF(UNITS): case YY_STATE_EOF(EXPON): case YY_STATE_EOF(FLUSH): #line 934 "wcsulex.l" { /* End-of-string. */ if (YY_START == EXPON) { add(&factor, types, &expon, scale, units); } wcsulexlex_destroy(); if (bracket) { status = wcserr_set(WCSERR_SET(UNITSERR_UNBAL_BRACKET), "Unbalanced bracket in '%s'", unitstr); } else if (paren) { status = wcserr_set(WCSERR_SET(UNITSERR_UNBAL_PAREN), "Unbalanced parenthesis in '%s'", unitstr); } else if (operator == 1) { status = wcserr_set(WCSERR_SET(UNITSERR_DANGLING_BINOP), "Dangling binary operator in '%s'", unitstr); } else if (operator) { status = wcserr_set(WCSERR_SET(UNITSERR_CONSEC_BINOPS), "Consecutive binary operators in '%s'", unitstr); #ifdef DEBUG } else { fprintf(stderr, "EOS\n"); #endif } if (status) { for (i = 0; i < WCSUNITS_NTYPE; i++) { units[i] = 0.0; *scale = 0.0; } } return status; } YY_BREAK case 118: YY_RULE_SETUP #line 970 "wcsulex.l" ECHO; YY_BREAK #line 8410 "wcsulex.c" case YY_END_OF_BUFFER: { /* Amount of text matched not including the EOB char. */ int yy_amount_of_matched_text = (int) (yy_cp - (yytext_ptr)) - 1; /* Undo the effects of YY_DO_BEFORE_ACTION. */ *yy_cp = (yy_hold_char); YY_RESTORE_YY_MORE_OFFSET if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_NEW ) { /* We're scanning a new file or input source. It's * possible that this happened because the user * just pointed wcsulexin at a new source and called * wcsulexlex(). If so, then we have to assure * consistency between YY_CURRENT_BUFFER and our * globals. Here is the right place to do so, because * this is the first action (other than possibly a * back-up) that will match for the new input source. */ (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; YY_CURRENT_BUFFER_LVALUE->yy_input_file = wcsulexin; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_NORMAL; } /* Note that here we test for yy_c_buf_p "<=" to the position * of the first EOB in the buffer, since yy_c_buf_p will * already have been incremented past the NUL character * (since all states make transitions on EOB to the * end-of-buffer state). Contrast this with the test * in input(). */ if ( (yy_c_buf_p) <= &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) { /* This was really a NUL. */ yy_state_type yy_next_state; (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); /* Okay, we're now positioned to make the NUL * transition. We couldn't have * yy_get_previous_state() go ahead and do it * for us because it doesn't know how to deal * with the possibility of jamming (and we don't * want to build jamming into it because then it * will run more slowly). */ yy_next_state = yy_try_NUL_trans( yy_current_state ); yy_bp = (yytext_ptr) + YY_MORE_ADJ; if ( yy_next_state ) { /* Consume the NUL. */ yy_cp = ++(yy_c_buf_p); yy_current_state = yy_next_state; goto yy_match; } else { yy_cp = (yy_c_buf_p); goto yy_find_action; } } else switch ( yy_get_next_buffer( ) ) { case EOB_ACT_END_OF_FILE: { (yy_did_buffer_switch_on_eof) = 0; if ( wcsulexwrap( ) ) { /* Note: because we've taken care in * yy_get_next_buffer() to have set up * wcsulextext, we can now set up * yy_c_buf_p so that if some total * hoser (like flex itself) wants to * call the scanner after we return the * YY_NULL, it'll still work - another * YY_NULL will get returned. */ (yy_c_buf_p) = (yytext_ptr) + YY_MORE_ADJ; yy_act = YY_STATE_EOF(YY_START); goto do_action; } else { if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; } break; } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_match; case EOB_ACT_LAST_MATCH: (yy_c_buf_p) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)]; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_find_action; } break; } default: YY_FATAL_ERROR( "fatal flex scanner internal error--no action found" ); } /* end of action switch */ } /* end of scanning one token */ } /* end of wcsulexlex */ /* yy_get_next_buffer - try to read in a new buffer * * Returns a code representing an action: * EOB_ACT_LAST_MATCH - * EOB_ACT_CONTINUE_SCAN - continue scanning from current position * EOB_ACT_END_OF_FILE - end of file */ static int yy_get_next_buffer (void) { register char *dest = YY_CURRENT_BUFFER_LVALUE->yy_ch_buf; register char *source = (yytext_ptr); register int number_to_move, i; int ret_val; if ( (yy_c_buf_p) > &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] ) YY_FATAL_ERROR( "fatal flex scanner internal error--end of buffer missed" ); if ( YY_CURRENT_BUFFER_LVALUE->yy_fill_buffer == 0 ) { /* Don't try to fill the buffer, so this is an EOF. */ if ( (yy_c_buf_p) - (yytext_ptr) - YY_MORE_ADJ == 1 ) { /* We matched a single character, the EOB, so * treat this as a final EOF. */ return EOB_ACT_END_OF_FILE; } else { /* We matched some text prior to the EOB, first * process it. */ return EOB_ACT_LAST_MATCH; } } /* Try to read more data. */ /* First move last chars to start of buffer. */ number_to_move = (int) ((yy_c_buf_p) - (yytext_ptr)) - 1; for ( i = 0; i < number_to_move; ++i ) *(dest++) = *(source++); if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_EOF_PENDING ) /* don't do the read, it's not guaranteed to return an EOF, * just force an EOF */ YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = 0; else { int num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; while ( num_to_read <= 0 ) { /* Not enough room in the buffer - grow it. */ /* just a shorter name for the current buffer */ YY_BUFFER_STATE b = YY_CURRENT_BUFFER; int yy_c_buf_p_offset = (int) ((yy_c_buf_p) - b->yy_ch_buf); if ( b->yy_is_our_buffer ) { int new_size = b->yy_buf_size * 2; if ( new_size <= 0 ) b->yy_buf_size += b->yy_buf_size / 8; else b->yy_buf_size *= 2; b->yy_ch_buf = (char *) /* Include room in for 2 EOB chars. */ wcsulexrealloc((void *) b->yy_ch_buf,b->yy_buf_size + 2 ); } else /* Can't grow it, we don't own it. */ b->yy_ch_buf = 0; if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "fatal error - scanner input buffer overflow" ); (yy_c_buf_p) = &b->yy_ch_buf[yy_c_buf_p_offset]; num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; } if ( num_to_read > YY_READ_BUF_SIZE ) num_to_read = YY_READ_BUF_SIZE; /* Read in more data. */ YY_INPUT( (&YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]), (yy_n_chars), (size_t) num_to_read ); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } if ( (yy_n_chars) == 0 ) { if ( number_to_move == YY_MORE_ADJ ) { ret_val = EOB_ACT_END_OF_FILE; wcsulexrestart(wcsulexin ); } else { ret_val = EOB_ACT_LAST_MATCH; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_EOF_PENDING; } } else ret_val = EOB_ACT_CONTINUE_SCAN; if ((yy_size_t) ((yy_n_chars) + number_to_move) > YY_CURRENT_BUFFER_LVALUE->yy_buf_size) { /* Extend the array by 50%, plus the number we really need. */ yy_size_t new_size = (yy_n_chars) + number_to_move + ((yy_n_chars) >> 1); YY_CURRENT_BUFFER_LVALUE->yy_ch_buf = (char *) wcsulexrealloc((void *) YY_CURRENT_BUFFER_LVALUE->yy_ch_buf,new_size ); if ( ! YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in yy_get_next_buffer()" ); } (yy_n_chars) += number_to_move; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] = YY_END_OF_BUFFER_CHAR; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] = YY_END_OF_BUFFER_CHAR; (yytext_ptr) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[0]; return ret_val; } /* yy_get_previous_state - get the state just before the EOB char was reached */ static yy_state_type yy_get_previous_state (void) { register yy_state_type yy_current_state; register char *yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); for ( yy_cp = (yytext_ptr) + YY_MORE_ADJ; yy_cp < (yy_c_buf_p); ++yy_cp ) { if ( *yy_cp ) { yy_current_state = yy_nxt[yy_current_state][YY_SC_TO_UI(*yy_cp)]; } else yy_current_state = yy_NUL_trans[yy_current_state]; if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_current_state; } /* yy_try_NUL_trans - try to make a transition on the NUL character * * synopsis * next_state = yy_try_NUL_trans( current_state ); */ static yy_state_type yy_try_NUL_trans (yy_state_type yy_current_state ) { register int yy_is_jam; register char *yy_cp = (yy_c_buf_p); yy_current_state = yy_NUL_trans[yy_current_state]; yy_is_jam = (yy_current_state == 0); if ( ! yy_is_jam ) { if ( yy_accept[yy_current_state] ) { (yy_last_accepting_state) = yy_current_state; (yy_last_accepting_cpos) = yy_cp; } } return yy_is_jam ? 0 : yy_current_state; } static void yyunput (int c, register char * yy_bp ) { register char *yy_cp; yy_cp = (yy_c_buf_p); /* undo effects of setting up wcsulextext */ *yy_cp = (yy_hold_char); if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) { /* need to shift things up to make room */ /* +2 for EOB chars. */ register int number_to_move = (yy_n_chars) + 2; register char *dest = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[ YY_CURRENT_BUFFER_LVALUE->yy_buf_size + 2]; register char *source = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]; while ( source > YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) *--dest = *--source; yy_cp += (int) (dest - source); yy_bp += (int) (dest - source); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_buf_size; if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) YY_FATAL_ERROR( "flex scanner push-back overflow" ); } *--yy_cp = (char) c; (yytext_ptr) = yy_bp; (yy_hold_char) = *yy_cp; (yy_c_buf_p) = yy_cp; } #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void) #else static int input (void) #endif { int c; *(yy_c_buf_p) = (yy_hold_char); if ( *(yy_c_buf_p) == YY_END_OF_BUFFER_CHAR ) { /* yy_c_buf_p now points to the character we want to return. * If this occurs *before* the EOB characters, then it's a * valid NUL; if not, then we've hit the end of the buffer. */ if ( (yy_c_buf_p) < &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) /* This was really a NUL. */ *(yy_c_buf_p) = '\0'; else { /* need more input */ int offset = (yy_c_buf_p) - (yytext_ptr); ++(yy_c_buf_p); switch ( yy_get_next_buffer( ) ) { case EOB_ACT_LAST_MATCH: /* This happens because yy_g_n_b() * sees that we've accumulated a * token and flags that we need to * try matching the token before * proceeding. But for input(), * there's no matching to consider. * So convert the EOB_ACT_LAST_MATCH * to EOB_ACT_END_OF_FILE. */ /* Reset buffer status. */ wcsulexrestart(wcsulexin ); /*FALLTHROUGH*/ case EOB_ACT_END_OF_FILE: { if ( wcsulexwrap( ) ) return EOF; if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; #ifdef __cplusplus return yyinput(); #else return input(); #endif } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + offset; break; } } } c = *(unsigned char *) (yy_c_buf_p); /* cast for 8-bit char's */ *(yy_c_buf_p) = '\0'; /* preserve wcsulextext */ (yy_hold_char) = *++(yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_at_bol = (c == '\n'); return c; } #endif /* ifndef YY_NO_INPUT */ /** Immediately switch to a different input stream. * @param input_file A readable stream. * * @note This function does not reset the start condition to @c INITIAL . */ void wcsulexrestart (FILE * input_file ) { if ( ! YY_CURRENT_BUFFER ){ wcsulexensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcsulex_create_buffer(wcsulexin,YY_BUF_SIZE ); } wcsulex_init_buffer(YY_CURRENT_BUFFER,input_file ); wcsulex_load_buffer_state( ); } /** Switch to a different input buffer. * @param new_buffer The new input buffer. * */ void wcsulex_switch_to_buffer (YY_BUFFER_STATE new_buffer ) { /* TODO. We should be able to replace this entire function body * with * wcsulexpop_buffer_state(); * wcsulexpush_buffer_state(new_buffer); */ wcsulexensure_buffer_stack (); if ( YY_CURRENT_BUFFER == new_buffer ) return; if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } YY_CURRENT_BUFFER_LVALUE = new_buffer; wcsulex_load_buffer_state( ); /* We don't actually know whether we did this switch during * EOF (wcsulexwrap()) processing, but the only time this flag * is looked at is after wcsulexwrap() is called, so it's safe * to go ahead and always set it. */ (yy_did_buffer_switch_on_eof) = 1; } static void wcsulex_load_buffer_state (void) { (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; (yytext_ptr) = (yy_c_buf_p) = YY_CURRENT_BUFFER_LVALUE->yy_buf_pos; wcsulexin = YY_CURRENT_BUFFER_LVALUE->yy_input_file; (yy_hold_char) = *(yy_c_buf_p); } /** Allocate and initialize an input buffer state. * @param file A readable stream. * @param size The character buffer size in bytes. When in doubt, use @c YY_BUF_SIZE. * * @return the allocated buffer state. */ YY_BUFFER_STATE wcsulex_create_buffer (FILE * file, int size ) { YY_BUFFER_STATE b; b = (YY_BUFFER_STATE) wcsulexalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcsulex_create_buffer()" ); b->yy_buf_size = size; /* yy_ch_buf has to be 2 characters longer than the size given because * we need to put in 2 end-of-buffer characters. */ b->yy_ch_buf = (char *) wcsulexalloc(b->yy_buf_size + 2 ); if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in wcsulex_create_buffer()" ); b->yy_is_our_buffer = 1; wcsulex_init_buffer(b,file ); return b; } /** Destroy the buffer. * @param b a buffer created with wcsulex_create_buffer() * */ void wcsulex_delete_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; if ( b == YY_CURRENT_BUFFER ) /* Not sure if we should pop here. */ YY_CURRENT_BUFFER_LVALUE = (YY_BUFFER_STATE) 0; if ( b->yy_is_our_buffer ) wcsulexfree((void *) b->yy_ch_buf ); wcsulexfree((void *) b ); } /* Initializes or reinitializes a buffer. * This function is sometimes called more than once on the same buffer, * such as during a wcsulexrestart() or at EOF. */ static void wcsulex_init_buffer (YY_BUFFER_STATE b, FILE * file ) { int oerrno = errno; wcsulex_flush_buffer(b ); b->yy_input_file = file; b->yy_fill_buffer = 1; /* If b is the current buffer, then wcsulex_init_buffer was _probably_ * called from wcsulexrestart() or through yy_get_next_buffer. * In that case, we don't want to reset the lineno or column. */ if (b != YY_CURRENT_BUFFER){ b->yy_bs_lineno = 1; b->yy_bs_column = 0; } b->yy_is_interactive = 0; errno = oerrno; } /** Discard all buffered characters. On the next scan, YY_INPUT will be called. * @param b the buffer state to be flushed, usually @c YY_CURRENT_BUFFER. * */ void wcsulex_flush_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; b->yy_n_chars = 0; /* We always need two end-of-buffer characters. The first causes * a transition to the end-of-buffer state. The second causes * a jam in that state. */ b->yy_ch_buf[0] = YY_END_OF_BUFFER_CHAR; b->yy_ch_buf[1] = YY_END_OF_BUFFER_CHAR; b->yy_buf_pos = &b->yy_ch_buf[0]; b->yy_at_bol = 1; b->yy_buffer_status = YY_BUFFER_NEW; if ( b == YY_CURRENT_BUFFER ) wcsulex_load_buffer_state( ); } /** Pushes the new state onto the stack. The new state becomes * the current state. This function will allocate the stack * if necessary. * @param new_buffer The new state. * */ void wcsulexpush_buffer_state (YY_BUFFER_STATE new_buffer ) { if (new_buffer == NULL) return; wcsulexensure_buffer_stack(); /* This block is copied from wcsulex_switch_to_buffer. */ if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } /* Only push if top exists. Otherwise, replace top. */ if (YY_CURRENT_BUFFER) (yy_buffer_stack_top)++; YY_CURRENT_BUFFER_LVALUE = new_buffer; /* copied from wcsulex_switch_to_buffer. */ wcsulex_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } /** Removes and deletes the top of the stack, if present. * The next element becomes the new top. * */ void wcsulexpop_buffer_state (void) { if (!YY_CURRENT_BUFFER) return; wcsulex_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; if ((yy_buffer_stack_top) > 0) --(yy_buffer_stack_top); if (YY_CURRENT_BUFFER) { wcsulex_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } } /* Allocates the stack if it does not exist. * Guarantees space for at least one push. */ static void wcsulexensure_buffer_stack (void) { int num_to_alloc; if (!(yy_buffer_stack)) { /* First allocation is just for 2 elements, since we don't know if this * scanner will even need a stack. We use 2 instead of 1 to avoid an * immediate realloc on the next call. */ num_to_alloc = 1; (yy_buffer_stack) = (struct yy_buffer_state**)wcsulexalloc (num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcsulexensure_buffer_stack()" ); memset((yy_buffer_stack), 0, num_to_alloc * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; (yy_buffer_stack_top) = 0; return; } if ((yy_buffer_stack_top) >= ((yy_buffer_stack_max)) - 1){ /* Increase the buffer to prepare for a possible push. */ int grow_size = 8 /* arbitrary grow size */; num_to_alloc = (yy_buffer_stack_max) + grow_size; (yy_buffer_stack) = (struct yy_buffer_state**)wcsulexrealloc ((yy_buffer_stack), num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcsulexensure_buffer_stack()" ); /* zero only the new slots.*/ memset((yy_buffer_stack) + (yy_buffer_stack_max), 0, grow_size * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; } } /** Setup the input buffer state to scan directly from a user-specified character buffer. * @param base the character buffer * @param size the size in bytes of the character buffer * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcsulex_scan_buffer (char * base, yy_size_t size ) { YY_BUFFER_STATE b; if ( size < 2 || base[size-2] != YY_END_OF_BUFFER_CHAR || base[size-1] != YY_END_OF_BUFFER_CHAR ) /* They forgot to leave room for the EOB's. */ return 0; b = (YY_BUFFER_STATE) wcsulexalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcsulex_scan_buffer()" ); b->yy_buf_size = size - 2; /* "- 2" to take care of EOB's */ b->yy_buf_pos = b->yy_ch_buf = base; b->yy_is_our_buffer = 0; b->yy_input_file = 0; b->yy_n_chars = b->yy_buf_size; b->yy_is_interactive = 0; b->yy_at_bol = 1; b->yy_fill_buffer = 0; b->yy_buffer_status = YY_BUFFER_NEW; wcsulex_switch_to_buffer(b ); return b; } /** Setup the input buffer state to scan a string. The next call to wcsulexlex() will * scan from a @e copy of @a str. * @param yystr a NUL-terminated string to scan * * @return the newly allocated buffer state object. * @note If you want to scan bytes that may contain NUL values, then use * wcsulex_scan_bytes() instead. */ YY_BUFFER_STATE wcsulex_scan_string (yyconst char * yystr ) { return wcsulex_scan_bytes(yystr,strlen(yystr) ); } /** Setup the input buffer state to scan the given bytes. The next call to wcsulexlex() will * scan from a @e copy of @a bytes. * @param yybytes the byte buffer to scan * @param _yybytes_len the number of bytes in the buffer pointed to by @a bytes. * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcsulex_scan_bytes (yyconst char * yybytes, int _yybytes_len ) { YY_BUFFER_STATE b; char *buf; yy_size_t n; int i; /* Get memory for full buffer, including space for trailing EOB's. */ n = _yybytes_len + 2; buf = (char *) wcsulexalloc(n ); if ( ! buf ) YY_FATAL_ERROR( "out of dynamic memory in wcsulex_scan_bytes()" ); for ( i = 0; i < _yybytes_len; ++i ) buf[i] = yybytes[i]; buf[_yybytes_len] = buf[_yybytes_len+1] = YY_END_OF_BUFFER_CHAR; b = wcsulex_scan_buffer(buf,n ); if ( ! b ) YY_FATAL_ERROR( "bad buffer in wcsulex_scan_bytes()" ); /* It's okay to grow etc. this buffer, and we should throw it * away when we're done. */ b->yy_is_our_buffer = 1; return b; } #ifndef YY_EXIT_FAILURE #define YY_EXIT_FAILURE 2 #endif static void yy_fatal_error (yyconst char* msg ) { (void) fprintf( stderr, "%s\n", msg ); exit( YY_EXIT_FAILURE ); } /* Redefine yyless() so it works in section 3 code. */ #undef yyless #define yyless(n) \ do \ { \ /* Undo effects of setting up wcsulextext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ wcsulextext[wcsulexleng] = (yy_hold_char); \ (yy_c_buf_p) = wcsulextext + yyless_macro_arg; \ (yy_hold_char) = *(yy_c_buf_p); \ *(yy_c_buf_p) = '\0'; \ wcsulexleng = yyless_macro_arg; \ } \ while ( 0 ) /* Accessor methods (get/set functions) to struct members. */ /** Get the current line number. * */ int wcsulexget_lineno (void) { return wcsulexlineno; } /** Get the input stream. * */ FILE *wcsulexget_in (void) { return wcsulexin; } /** Get the output stream. * */ FILE *wcsulexget_out (void) { return wcsulexout; } /** Get the length of the current token. * */ int wcsulexget_leng (void) { return wcsulexleng; } /** Get the current token. * */ char *wcsulexget_text (void) { return wcsulextext; } /** Set the current line number. * @param line_number * */ void wcsulexset_lineno (int line_number ) { wcsulexlineno = line_number; } /** Set the input stream. This does not discard the current * input buffer. * @param in_str A readable stream. * * @see wcsulex_switch_to_buffer */ void wcsulexset_in (FILE * in_str ) { wcsulexin = in_str ; } void wcsulexset_out (FILE * out_str ) { wcsulexout = out_str ; } int wcsulexget_debug (void) { return wcsulex_flex_debug; } void wcsulexset_debug (int bdebug ) { wcsulex_flex_debug = bdebug ; } static int yy_init_globals (void) { /* Initialization is the same as for the non-reentrant scanner. * This function is called from wcsulexlex_destroy(), so don't allocate here. */ (yy_buffer_stack) = 0; (yy_buffer_stack_top) = 0; (yy_buffer_stack_max) = 0; (yy_c_buf_p) = (char *) 0; (yy_init) = 0; (yy_start) = 0; /* Defined in main.c */ #ifdef YY_STDINIT wcsulexin = stdin; wcsulexout = stdout; #else wcsulexin = (FILE *) 0; wcsulexout = (FILE *) 0; #endif /* For future reference: Set errno on error, since we are called by * wcsulexlex_init() */ return 0; } /* wcsulexlex_destroy is for both reentrant and non-reentrant scanners. */ int wcsulexlex_destroy (void) { /* Pop the buffer stack, destroying each element. */ while(YY_CURRENT_BUFFER){ wcsulex_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; wcsulexpop_buffer_state(); } /* Destroy the stack itself. */ wcsulexfree((yy_buffer_stack) ); (yy_buffer_stack) = NULL; /* Reset the globals. This is important in a non-reentrant scanner so the next time * wcsulexlex() is called, initialization will occur. */ yy_init_globals( ); return 0; } /* * Internal utility routines. */ #ifndef yytext_ptr static void yy_flex_strncpy (char* s1, yyconst char * s2, int n ) { register int i; for ( i = 0; i < n; ++i ) s1[i] = s2[i]; } #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * s ) { register int n; for ( n = 0; s[n]; ++n ) ; return n; } #endif void *wcsulexalloc (yy_size_t size ) { return (void *) malloc( size ); } void *wcsulexrealloc (void * ptr, yy_size_t size ) { /* The cast to (char *) in the following accommodates both * implementations that use char* generic pointers, and those * that use void* generic pointers. It works with the latter * because both ANSI C and C++ allow castless assignment from * any pointer type to void*, and deal with argument conversions * as though doing an assignment. */ return (void *) realloc( (char *) ptr, size ); } void wcsulexfree (void * ptr ) { free( (char *) ptr ); /* see wcsulexrealloc() for (char *) cast */ } #define YYTABLES_NAME "yytables" #line 970 "wcsulex.l" /*---------------------------------------------------------------------------- * Accumulate a term in a units specification and reset work variables. *---------------------------------------------------------------------------*/ void add( double *factor, double types[], double *expon, double *scale, double units[]) { int i; *scale *= pow(*factor, *expon); for (i = 0; i < WCSUNITS_NTYPE; i++) { units[i] += *expon * types[i]; types[i] = 0.0; } *expon = 1.0; *factor = 1.0; return; } pywcs-1.12/wcslib/C/flexed/wcsutrn.c0000644001153600020070000066655212310355626021457 0ustar cslocumSTSCI\science00000000000000#line 2 "wcsutrn.c" #line 4 "wcsutrn.c" #define YY_INT_ALIGNED short int /* A lexical scanner generated by flex */ #define yy_create_buffer wcsutrn_create_buffer #define yy_delete_buffer wcsutrn_delete_buffer #define yy_flex_debug wcsutrn_flex_debug #define yy_init_buffer wcsutrn_init_buffer #define yy_flush_buffer wcsutrn_flush_buffer #define yy_load_buffer_state wcsutrn_load_buffer_state #define yy_switch_to_buffer wcsutrn_switch_to_buffer #define yyin wcsutrnin #define yyleng wcsutrnleng #define yylex wcsutrnlex #define yylineno wcsutrnlineno #define yyout wcsutrnout #define yyrestart wcsutrnrestart #define yytext wcsutrntext #define yywrap wcsutrnwrap #define yyalloc wcsutrnalloc #define yyrealloc wcsutrnrealloc #define yyfree wcsutrnfree #define FLEX_SCANNER #define YY_FLEX_MAJOR_VERSION 2 #define YY_FLEX_MINOR_VERSION 5 #define YY_FLEX_SUBMINOR_VERSION 35 #if YY_FLEX_SUBMINOR_VERSION > 0 #define FLEX_BETA #endif /* First, we deal with platform-specific or compiler-specific issues. */ /* begin standard C headers. */ #include #include #include #include /* end standard C headers. */ /* flex integer type definitions */ #ifndef FLEXINT_H #define FLEXINT_H /* C99 systems have . Non-C99 systems may or may not. */ #if defined (__STDC_VERSION__) && __STDC_VERSION__ >= 199901L /* C99 says to define __STDC_LIMIT_MACROS before including stdint.h, * if you want the limit (max/min) macros for int types. */ #ifndef __STDC_LIMIT_MACROS #define __STDC_LIMIT_MACROS 1 #endif #include typedef int8_t flex_int8_t; typedef uint8_t flex_uint8_t; typedef int16_t flex_int16_t; typedef uint16_t flex_uint16_t; typedef int32_t flex_int32_t; typedef uint32_t flex_uint32_t; #else typedef signed char flex_int8_t; typedef short int flex_int16_t; typedef int flex_int32_t; typedef unsigned char flex_uint8_t; typedef unsigned short int flex_uint16_t; typedef unsigned int flex_uint32_t; /* Limits of integral types. */ #ifndef INT8_MIN #define INT8_MIN (-128) #endif #ifndef INT16_MIN #define INT16_MIN (-32767-1) #endif #ifndef INT32_MIN #define INT32_MIN (-2147483647-1) #endif #ifndef INT8_MAX #define INT8_MAX (127) #endif #ifndef INT16_MAX #define INT16_MAX (32767) #endif #ifndef INT32_MAX #define INT32_MAX (2147483647) #endif #ifndef UINT8_MAX #define UINT8_MAX (255U) #endif #ifndef UINT16_MAX #define UINT16_MAX (65535U) #endif #ifndef UINT32_MAX #define UINT32_MAX (4294967295U) #endif #endif /* ! C99 */ #endif /* ! FLEXINT_H */ #ifdef __cplusplus /* The "const" storage-class-modifier is valid. */ #define YY_USE_CONST #else /* ! __cplusplus */ /* C99 requires __STDC__ to be defined as 1. */ #if defined (__STDC__) #define YY_USE_CONST #endif /* defined (__STDC__) */ #endif /* ! __cplusplus */ #ifdef YY_USE_CONST #define yyconst const #else #define yyconst #endif /* Returned upon end-of-file. */ #define YY_NULL 0 /* Promotes a possibly negative, possibly signed char to an unsigned * integer for use as an array index. If the signed char is negative, * we want to instead treat it as an 8-bit unsigned char, hence the * double cast. */ #define YY_SC_TO_UI(c) ((unsigned int) (unsigned char) c) /* Enter a start condition. This macro really ought to take a parameter, * but we do it the disgusting crufty way forced on us by the ()-less * definition of BEGIN. */ #define BEGIN (yy_start) = 1 + 2 * /* Translate the current start state into a value that can be later handed * to BEGIN to return to the state. The YYSTATE alias is for lex * compatibility. */ #define YY_START (((yy_start) - 1) / 2) #define YYSTATE YY_START /* Action number for EOF rule of a given start state. */ #define YY_STATE_EOF(state) (YY_END_OF_BUFFER + state + 1) /* Special action meaning "start processing a new file". */ #define YY_NEW_FILE wcsutrnrestart(wcsutrnin ) #define YY_END_OF_BUFFER_CHAR 0 /* Size of default input buffer. */ #ifndef YY_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k. * Moreover, YY_BUF_SIZE is 2*YY_READ_BUF_SIZE in the general case. * Ditto for the __ia64__ case accordingly. */ #define YY_BUF_SIZE 32768 #else #define YY_BUF_SIZE 16384 #endif /* __ia64__ */ #endif /* The state buf must be large enough to hold one state per character in the main buffer. */ #define YY_STATE_BUF_SIZE ((YY_BUF_SIZE + 2) * sizeof(yy_state_type)) #ifndef YY_TYPEDEF_YY_BUFFER_STATE #define YY_TYPEDEF_YY_BUFFER_STATE typedef struct yy_buffer_state *YY_BUFFER_STATE; #endif extern int wcsutrnleng; extern FILE *wcsutrnin, *wcsutrnout; #define EOB_ACT_CONTINUE_SCAN 0 #define EOB_ACT_END_OF_FILE 1 #define EOB_ACT_LAST_MATCH 2 #define YY_LESS_LINENO(n) /* Return all but the first "n" matched characters back to the input stream. */ #define yyless(n) \ do \ { \ /* Undo effects of setting up wcsutrntext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ *yy_cp = (yy_hold_char); \ YY_RESTORE_YY_MORE_OFFSET \ (yy_c_buf_p) = yy_cp = yy_bp + yyless_macro_arg - YY_MORE_ADJ; \ YY_DO_BEFORE_ACTION; /* set up wcsutrntext again */ \ } \ while ( 0 ) #define unput(c) yyunput( c, (yytext_ptr) ) #ifndef YY_TYPEDEF_YY_SIZE_T #define YY_TYPEDEF_YY_SIZE_T typedef size_t yy_size_t; #endif #ifndef YY_STRUCT_YY_BUFFER_STATE #define YY_STRUCT_YY_BUFFER_STATE struct yy_buffer_state { FILE *yy_input_file; char *yy_ch_buf; /* input buffer */ char *yy_buf_pos; /* current position in input buffer */ /* Size of input buffer in bytes, not including room for EOB * characters. */ yy_size_t yy_buf_size; /* Number of characters read into yy_ch_buf, not including EOB * characters. */ int yy_n_chars; /* Whether we "own" the buffer - i.e., we know we created it, * and can realloc() it to grow it, and should free() it to * delete it. */ int yy_is_our_buffer; /* Whether this is an "interactive" input source; if so, and * if we're using stdio for input, then we want to use getc() * instead of fread(), to make sure we stop fetching input after * each newline. */ int yy_is_interactive; /* Whether we're considered to be at the beginning of a line. * If so, '^' rules will be active on the next match, otherwise * not. */ int yy_at_bol; int yy_bs_lineno; /**< The line count. */ int yy_bs_column; /**< The column count. */ /* Whether to try to fill the input buffer when we reach the * end of it. */ int yy_fill_buffer; int yy_buffer_status; #define YY_BUFFER_NEW 0 #define YY_BUFFER_NORMAL 1 /* When an EOF's been seen but there's still some text to process * then we mark the buffer as YY_EOF_PENDING, to indicate that we * shouldn't try reading from the input source any more. We might * still have a bunch of tokens to match, though, because of * possible backing-up. * * When we actually see the EOF, we change the status to "new" * (via wcsutrnrestart()), so that the user can continue scanning by * just pointing wcsutrnin at a new input file. */ #define YY_BUFFER_EOF_PENDING 2 }; #endif /* !YY_STRUCT_YY_BUFFER_STATE */ /* Stack of input buffers. */ static size_t yy_buffer_stack_top = 0; /**< index of top of stack. */ static size_t yy_buffer_stack_max = 0; /**< capacity of stack. */ static YY_BUFFER_STATE * yy_buffer_stack = 0; /**< Stack as an array. */ /* We provide macros for accessing buffer states in case in the * future we want to put the buffer states in a more general * "scanner state". * * Returns the top of the stack, or NULL. */ #define YY_CURRENT_BUFFER ( (yy_buffer_stack) \ ? (yy_buffer_stack)[(yy_buffer_stack_top)] \ : NULL) /* Same as previous macro, but useful when we know that the buffer stack is not * NULL or when we need an lvalue. For internal use only. */ #define YY_CURRENT_BUFFER_LVALUE (yy_buffer_stack)[(yy_buffer_stack_top)] /* yy_hold_char holds the character lost when wcsutrntext is formed. */ static char yy_hold_char; static int yy_n_chars; /* number of characters read into yy_ch_buf */ int wcsutrnleng; /* Points to current character in buffer. */ static char *yy_c_buf_p = (char *) 0; static int yy_init = 0; /* whether we need to initialize */ static int yy_start = 0; /* start state number */ /* Flag which is used to allow wcsutrnwrap()'s to do buffer switches * instead of setting up a fresh wcsutrnin. A bit of a hack ... */ static int yy_did_buffer_switch_on_eof; void wcsutrnrestart (FILE *input_file ); void wcsutrn_switch_to_buffer (YY_BUFFER_STATE new_buffer ); YY_BUFFER_STATE wcsutrn_create_buffer (FILE *file,int size ); void wcsutrn_delete_buffer (YY_BUFFER_STATE b ); void wcsutrn_flush_buffer (YY_BUFFER_STATE b ); void wcsutrnpush_buffer_state (YY_BUFFER_STATE new_buffer ); void wcsutrnpop_buffer_state (void ); static void wcsutrnensure_buffer_stack (void ); static void wcsutrn_load_buffer_state (void ); static void wcsutrn_init_buffer (YY_BUFFER_STATE b,FILE *file ); #define YY_FLUSH_BUFFER wcsutrn_flush_buffer(YY_CURRENT_BUFFER ) YY_BUFFER_STATE wcsutrn_scan_buffer (char *base,yy_size_t size ); YY_BUFFER_STATE wcsutrn_scan_string (yyconst char *yy_str ); YY_BUFFER_STATE wcsutrn_scan_bytes (yyconst char *bytes,int len ); void *wcsutrnalloc (yy_size_t ); void *wcsutrnrealloc (void *,yy_size_t ); void wcsutrnfree (void * ); #define yy_new_buffer wcsutrn_create_buffer #define yy_set_interactive(is_interactive) \ { \ if ( ! YY_CURRENT_BUFFER ){ \ wcsutrnensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcsutrn_create_buffer(wcsutrnin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_is_interactive = is_interactive; \ } #define yy_set_bol(at_bol) \ { \ if ( ! YY_CURRENT_BUFFER ){\ wcsutrnensure_buffer_stack (); \ YY_CURRENT_BUFFER_LVALUE = \ wcsutrn_create_buffer(wcsutrnin,YY_BUF_SIZE ); \ } \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = at_bol; \ } #define YY_AT_BOL() (YY_CURRENT_BUFFER_LVALUE->yy_at_bol) /* Begin user sect3 */ #define wcsutrnwrap(n) 1 #define YY_SKIP_YYWRAP typedef char YY_CHAR; FILE *wcsutrnin = (FILE *) 0, *wcsutrnout = (FILE *) 0; typedef int yy_state_type; extern int wcsutrnlineno; int wcsutrnlineno = 1; extern char *wcsutrntext; #define yytext_ptr wcsutrntext static yyconst flex_int16_t yy_nxt[][128] = { { 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 }, { 7, 8, 8, 8, 8, 8, 8, 8, 8, 8, 8, 8, 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-190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, -190, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -190, -190, -190, -190, -190, -190, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -190, -190, -190, -190, -190 }, { 7, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, -191, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -191, -191, -191, -191, -191, -191, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -191, -191, -191, -191, -191 }, { 7, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, -192, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -192, -192, -192, -192, -192, -192, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -192, -192, -192, -192, -192 }, { 7, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, -193, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -193, -193, -193, -193, -193, -193, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -193, -193, -193, -193, -193 }, { 7, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, -194, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -194, -194, -194, -194, -194, -194, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -194, -194, -194, -194, -194 }, { 7, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, -195, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -195, -195, -195, -195, -195, -195, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -195, -195, -195, -195, -195 }, { 7, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, -196, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -196, -196, -196, -196, -196, -196, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -196, -196, -196, -196, -196 }, { 7, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, -197, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -197, -197, -197, -197, -197, -197, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -197, -197, -197, -197, -197 }, { 7, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, -198, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -198, -198, -198, -198, -198, -198, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 202, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -198, -198, -198, -198, -198 }, { 7, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, -199, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -199, -199, -199, -199, -199, -199, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -199, -199, -199, -199, -199 }, { 7, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, -200, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -200, -200, -200, -200, -200, -200, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -200, -200, -200, -200, -200 }, { 7, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, -201, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -201, -201, -201, -201, -201, -201, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -201, -201, -201, -201, -201 }, { 7, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, -202, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -202, -202, -202, -202, -202, -202, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, 43, -202, -202, -202, -202, -202 }, } ; static yy_state_type yy_get_previous_state (void ); static yy_state_type yy_try_NUL_trans (yy_state_type current_state ); static int yy_get_next_buffer (void ); static void yy_fatal_error (yyconst char msg[] ); /* Done after the current pattern has been matched and before the * corresponding action - sets up wcsutrntext. */ #define YY_DO_BEFORE_ACTION \ (yytext_ptr) = yy_bp; \ wcsutrnleng = (size_t) (yy_cp - yy_bp); \ (yy_hold_char) = *yy_cp; \ *yy_cp = '\0'; \ (yy_c_buf_p) = yy_cp; #define YY_NUM_RULES 37 #define YY_END_OF_BUFFER 38 /* This struct is not used in this scanner, but its presence is necessary. */ struct yy_trans_info { flex_int32_t yy_verify; flex_int32_t yy_nxt; }; static yyconst flex_int16_t yy_accept[203] = { 0, 0, 0, 0, 0, 36, 36, 38, 3, 2, 31, 31, 31, 10, 31, 14, 31, 31, 20, 31, 31, 31, 28, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 2, 1, 35, 37, 35, 32, 36, 2, 31, 31, 31, 31, 31, 31, 31, 13, 15, 17, 31, 31, 19, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 30, 31, 31, 31, 31, 31, 31, 31, 31, 31, 2, 1, 33, 33, 34, 32, 36, 31, 31, 31, 9, 11, 12, 31, 16, 31, 31, 22, 21, 23, 31, 31, 31, 26, 27, 31, 31, 31, 31, 31, 9, 31, 31, 31, 31, 27, 31, 31, 31, 7, 8, 9, 31, 31, 31, 31, 31, 31, 31, 31, 31, 31, 29, 29, 30, 31, 31, 31, 9, 31, 31, 31, 31, 31, 31, 30, 31, 31, 31, 31, 31, 20, 20, 31, 25, 31, 31, 31, 29, 29, 30, 31, 31, 31, 31, 20, 20, 31, 31, 31, 5, 6, 11, 18, 18, 20, 20, 24, 25, 24, 26, 27, 31, 31, 31, 11, 20, 20, 26, 27, 5, 6, 11, 18, 18, 24, 24, 26, 27, 31, 11, 26, 27, 4 } ; static yyconst yy_state_type yy_NUL_trans[203] = { 0, 8, 8, 37, 37, 41, 41, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 81, 0, 85, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 81, 0, 0, 85, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0, 0 } ; extern int wcsutrn_flex_debug; int wcsutrn_flex_debug = 0; /* The intent behind this definition is that it'll catch * any uses of REJECT which flex missed. */ #define REJECT reject_used_but_not_detected #define yymore() yymore_used_but_not_detected #define YY_MORE_ADJ 0 #define YY_RESTORE_YY_MORE_OFFSET char *wcsutrntext; #line 1 "wcsutrn.l" /*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsutrn.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcsutrn.l is a Flex description file containing the definition of a lexical * scanner that translates non-standard FITS units specifications. * * It requires Flex v2.5.4 or later. * * Refer to wcsunits.h for a description of the user interface and operating * notes. * *===========================================================================*/ /* Options. */ /* Exclusive start states. */ #line 55 "wcsutrn.l" /* To get the prototype for fileno() from stdio.h when gcc is invoked with * -std=c89 (same as -ansi) or -std=c99 since we do not define YY_INPUT. */ #define _POSIX_SOURCE 1 #include #include #include #include #include "wcserr.h" #include "wcsunits.h" #define YY_DECL int wcsutrne(int ctrl, char unitstr[], struct wcserr **err) /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcsutrn_abort_jmp_env; #define exit(status) longjmp(wcsutrn_abort_jmp_env, status) #line 4048 "wcsutrn.c" #define INITIAL 0 #define NEXT 1 #define FLUSH 2 #ifndef YY_NO_UNISTD_H /* Special case for "unistd.h", since it is non-ANSI. We include it way * down here because we want the user's section 1 to have been scanned first. * The user has a chance to override it with an option. */ #include #endif #ifndef YY_EXTRA_TYPE #define YY_EXTRA_TYPE void * #endif static int yy_init_globals (void ); /* Accessor methods to globals. These are made visible to non-reentrant scanners for convenience. */ int wcsutrnlex_destroy (void ); int wcsutrnget_debug (void ); void wcsutrnset_debug (int debug_flag ); YY_EXTRA_TYPE wcsutrnget_extra (void ); void wcsutrnset_extra (YY_EXTRA_TYPE user_defined ); FILE *wcsutrnget_in (void ); void wcsutrnset_in (FILE * in_str ); FILE *wcsutrnget_out (void ); void wcsutrnset_out (FILE * out_str ); int wcsutrnget_leng (void ); char *wcsutrnget_text (void ); int wcsutrnget_lineno (void ); void wcsutrnset_lineno (int line_number ); /* Macros after this point can all be overridden by user definitions in * section 1. */ #ifndef YY_SKIP_YYWRAP #ifdef __cplusplus extern "C" int wcsutrnwrap (void ); #else extern int wcsutrnwrap (void ); #endif #endif static void yyunput (int c,char *buf_ptr ); #ifndef yytext_ptr static void yy_flex_strncpy (char *,yyconst char *,int ); #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * ); #endif #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void ); #else static int input (void ); #endif #endif /* Amount of stuff to slurp up with each read. */ #ifndef YY_READ_BUF_SIZE #ifdef __ia64__ /* On IA-64, the buffer size is 16k, not 8k */ #define YY_READ_BUF_SIZE 16384 #else #define YY_READ_BUF_SIZE 8192 #endif /* __ia64__ */ #endif /* Copy whatever the last rule matched to the standard output. */ #ifndef ECHO /* This used to be an fputs(), but since the string might contain NUL's, * we now use fwrite(). */ #define ECHO do { if (fwrite( wcsutrntext, wcsutrnleng, 1, wcsutrnout )) {} } while (0) #endif /* Gets input and stuffs it into "buf". number of characters read, or YY_NULL, * is returned in "result". */ #ifndef YY_INPUT #define YY_INPUT(buf,result,max_size) \ errno=0; \ while ( (result = read( fileno(wcsutrnin), (char *) buf, max_size )) < 0 ) \ { \ if( errno != EINTR) \ { \ YY_FATAL_ERROR( "input in flex scanner failed" ); \ break; \ } \ errno=0; \ clearerr(wcsutrnin); \ }\ \ #endif /* No semi-colon after return; correct usage is to write "yyterminate();" - * we don't want an extra ';' after the "return" because that will cause * some compilers to complain about unreachable statements. */ #ifndef yyterminate #define yyterminate() return YY_NULL #endif /* Number of entries by which start-condition stack grows. */ #ifndef YY_START_STACK_INCR #define YY_START_STACK_INCR 25 #endif /* Report a fatal error. */ #ifndef YY_FATAL_ERROR #define YY_FATAL_ERROR(msg) yy_fatal_error( msg ) #endif /* end tables serialization structures and prototypes */ /* Default declaration of generated scanner - a define so the user can * easily add parameters. */ #ifndef YY_DECL #define YY_DECL_IS_OURS 1 extern int wcsutrnlex (void); #define YY_DECL int wcsutrnlex (void) #endif /* !YY_DECL */ /* Code executed at the beginning of each rule, after wcsutrntext and wcsutrnleng * have been set up. */ #ifndef YY_USER_ACTION #define YY_USER_ACTION #endif /* Code executed at the end of each rule. */ #ifndef YY_BREAK #define YY_BREAK break; #endif #define YY_RULE_SETUP \ if ( wcsutrnleng > 0 ) \ YY_CURRENT_BUFFER_LVALUE->yy_at_bol = \ (wcsutrntext[wcsutrnleng - 1] == '\n'); \ YY_USER_ACTION /** The main scanner function which does all the work. */ YY_DECL { register yy_state_type yy_current_state; register char *yy_cp, *yy_bp; register int yy_act; #line 75 "wcsutrn.l" static const char *function = "wcsutrne"; char orig[80], subs[80]; int bracket = 0; int unsafe = 0; int status = -1; YY_BUFFER_STATE inbuff; int wcsutrnlex_destroy(void); *orig = '\0'; *subs = '\0'; inbuff = wcsutrn_scan_string(unitstr); *unitstr = '\0'; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcsutrn_abort_jmp_env)) { return wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units translator error parsing '%s'", unitstr); } BEGIN(INITIAL); #ifdef DEBUG fprintf(stderr, "\n%s ->\n", unitstr); #endif #line 4253 "wcsutrn.c" if ( !(yy_init) ) { (yy_init) = 1; #ifdef YY_USER_INIT YY_USER_INIT; #endif if ( ! (yy_start) ) (yy_start) = 1; /* first start state */ if ( ! wcsutrnin ) wcsutrnin = stdin; if ( ! wcsutrnout ) wcsutrnout = stdout; if ( ! YY_CURRENT_BUFFER ) { wcsutrnensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcsutrn_create_buffer(wcsutrnin,YY_BUF_SIZE ); } wcsutrn_load_buffer_state( ); } while ( 1 ) /* loops until end-of-file is reached */ { yy_cp = (yy_c_buf_p); /* Support of wcsutrntext. */ *yy_cp = (yy_hold_char); /* yy_bp points to the position in yy_ch_buf of the start of * the current run. */ yy_bp = yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); yy_match: while ( (yy_current_state = yy_nxt[yy_current_state][ YY_SC_TO_UI(*yy_cp) ]) > 0 ) ++yy_cp; yy_current_state = -yy_current_state; yy_find_action: yy_act = yy_accept[yy_current_state]; YY_DO_BEFORE_ACTION; do_action: /* This label is used only to access EOF actions. */ switch ( yy_act ) { /* beginning of action switch */ case 1: YY_RULE_SETUP #line 103 "wcsutrn.l" { /* Looks like a keycomment. */ strcat(unitstr, "["); bracket = 1; } YY_BREAK case 2: YY_RULE_SETUP #line 109 "wcsutrn.l" /* Discard leading whitespace. */ YY_BREAK case 3: /* rule 3 can match eol */ YY_RULE_SETUP #line 111 "wcsutrn.l" { /* Non-alphabetic character. */ strcat(unitstr, wcsutrntext); if (bracket && *wcsutrntext == ']') { BEGIN(FLUSH); } } YY_BREAK case 4: YY_RULE_SETUP #line 119 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "Angstrom"); BEGIN(NEXT); } YY_BREAK case 5: YY_RULE_SETUP #line 125 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "arcmin"); BEGIN(NEXT); } YY_BREAK case 6: YY_RULE_SETUP #line 131 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "arcsec"); BEGIN(NEXT); } YY_BREAK case 7: YY_RULE_SETUP #line 137 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "beam"); BEGIN(NEXT); } YY_BREAK case 8: YY_RULE_SETUP #line 143 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "byte"); BEGIN(NEXT); } YY_BREAK case 9: YY_RULE_SETUP #line 149 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "d"); BEGIN(NEXT); } YY_BREAK case 10: YY_RULE_SETUP #line 155 "wcsutrn.l" { unsafe = 1; strcpy(orig, wcsutrntext); strcpy(subs, (ctrl & 4) ? "d" : "D"); BEGIN(NEXT); } YY_BREAK case 11: YY_RULE_SETUP #line 162 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "deg"); BEGIN(NEXT); } YY_BREAK case 12: YY_RULE_SETUP #line 168 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "GHz"); BEGIN(NEXT); } YY_BREAK case 13: YY_RULE_SETUP #line 174 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "h"); BEGIN(NEXT); } YY_BREAK case 14: YY_RULE_SETUP #line 180 "wcsutrn.l" { unsafe = 1; strcpy(orig, wcsutrntext); strcpy(subs, (ctrl & 2) ? "h" : "H"); BEGIN(NEXT); } YY_BREAK case 15: YY_RULE_SETUP #line 187 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "Hz"); BEGIN(NEXT); } YY_BREAK case 16: YY_RULE_SETUP #line 193 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "kHz"); BEGIN(NEXT); } YY_BREAK case 17: YY_RULE_SETUP #line 199 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "Jy"); BEGIN(NEXT); } YY_BREAK case 18: YY_RULE_SETUP #line 205 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "K"); BEGIN(NEXT); } YY_BREAK case 19: YY_RULE_SETUP #line 211 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "km"); BEGIN(NEXT); } YY_BREAK case 20: YY_RULE_SETUP #line 217 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "m"); BEGIN(NEXT); } YY_BREAK case 21: YY_RULE_SETUP #line 223 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "min"); BEGIN(NEXT); } YY_BREAK case 22: YY_RULE_SETUP #line 229 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "MHz"); BEGIN(NEXT); } YY_BREAK case 23: YY_RULE_SETUP #line 235 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "ohm"); BEGIN(NEXT); } YY_BREAK case 24: YY_RULE_SETUP #line 241 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "Pa"); BEGIN(NEXT); } YY_BREAK case 25: YY_RULE_SETUP #line 247 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "pixel"); BEGIN(NEXT); } YY_BREAK case 26: YY_RULE_SETUP #line 253 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "rad"); BEGIN(NEXT); } YY_BREAK case 27: YY_RULE_SETUP #line 259 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "s"); BEGIN(NEXT); } YY_BREAK case 28: YY_RULE_SETUP #line 265 "wcsutrn.l" { unsafe = 1; strcpy(orig, wcsutrntext); strcpy(subs, (ctrl & 1) ? "s" : "S"); BEGIN(NEXT); } YY_BREAK case 29: YY_RULE_SETUP #line 272 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "V"); BEGIN(NEXT); } YY_BREAK case 30: YY_RULE_SETUP #line 278 "wcsutrn.l" { strcpy(orig, wcsutrntext); strcpy(subs, "yr"); BEGIN(NEXT); } YY_BREAK case 31: YY_RULE_SETUP #line 284 "wcsutrn.l" { /* Not a recognized alias. */ strcpy(orig, wcsutrntext); strcpy(subs, orig); BEGIN(NEXT); } YY_BREAK case 32: YY_RULE_SETUP #line 291 "wcsutrn.l" { /* Reject the alias match. */ strcat(orig, wcsutrntext); strcpy(subs, orig); } YY_BREAK case 33: /* rule 33 can match eol */ YY_RULE_SETUP #line 297 "wcsutrn.l" { /* Discard separating whitespace. */ unput(wcsutrntext[wcsutrnleng-1]); } YY_BREAK case 34: YY_RULE_SETUP #line 302 "wcsutrn.l" { /* Compress separating whitespace. */ strcat(unitstr, subs); strcat(unitstr, " "); if (strcmp(orig, subs)) status = 0; unput(wcsutrntext[wcsutrnleng-1]); *subs = '\0'; BEGIN(INITIAL); } YY_BREAK case 35: YY_RULE_SETUP #line 312 "wcsutrn.l" { /* Copy anything else unchanged. */ strcat(unitstr, subs); if (strcmp(orig, subs)) status = 0; unput(*wcsutrntext); *subs = '\0'; BEGIN(INITIAL); } YY_BREAK case 36: YY_RULE_SETUP #line 321 "wcsutrn.l" { /* Copy out remaining input. */ strcat(unitstr, wcsutrntext); } YY_BREAK case YY_STATE_EOF(INITIAL): case YY_STATE_EOF(NEXT): case YY_STATE_EOF(FLUSH): #line 326 "wcsutrn.l" { /* End-of-string. */ if (*subs) { strcat(unitstr, subs); if (strcmp(orig, subs)) status = 0; } wcsutrnlex_destroy(); if (unsafe) { return wcserr_set(WCSERR_SET(UNITSERR_UNSAFE_TRANS), "Unsafe unit translation in '%s'", unitstr); } return status; } YY_BREAK case 37: YY_RULE_SETUP #line 341 "wcsutrn.l" ECHO; YY_BREAK #line 4667 "wcsutrn.c" case YY_END_OF_BUFFER: { /* Amount of text matched not including the EOB char. */ int yy_amount_of_matched_text = (int) (yy_cp - (yytext_ptr)) - 1; /* Undo the effects of YY_DO_BEFORE_ACTION. */ *yy_cp = (yy_hold_char); YY_RESTORE_YY_MORE_OFFSET if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_NEW ) { /* We're scanning a new file or input source. It's * possible that this happened because the user * just pointed wcsutrnin at a new source and called * wcsutrnlex(). If so, then we have to assure * consistency between YY_CURRENT_BUFFER and our * globals. Here is the right place to do so, because * this is the first action (other than possibly a * back-up) that will match for the new input source. */ (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; YY_CURRENT_BUFFER_LVALUE->yy_input_file = wcsutrnin; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_NORMAL; } /* Note that here we test for yy_c_buf_p "<=" to the position * of the first EOB in the buffer, since yy_c_buf_p will * already have been incremented past the NUL character * (since all states make transitions on EOB to the * end-of-buffer state). Contrast this with the test * in input(). */ if ( (yy_c_buf_p) <= &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) { /* This was really a NUL. */ yy_state_type yy_next_state; (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); /* Okay, we're now positioned to make the NUL * transition. We couldn't have * yy_get_previous_state() go ahead and do it * for us because it doesn't know how to deal * with the possibility of jamming (and we don't * want to build jamming into it because then it * will run more slowly). */ yy_next_state = yy_try_NUL_trans( yy_current_state ); yy_bp = (yytext_ptr) + YY_MORE_ADJ; if ( yy_next_state ) { /* Consume the NUL. */ yy_cp = ++(yy_c_buf_p); yy_current_state = yy_next_state; goto yy_match; } else { yy_cp = (yy_c_buf_p); goto yy_find_action; } } else switch ( yy_get_next_buffer( ) ) { case EOB_ACT_END_OF_FILE: { (yy_did_buffer_switch_on_eof) = 0; if ( wcsutrnwrap( ) ) { /* Note: because we've taken care in * yy_get_next_buffer() to have set up * wcsutrntext, we can now set up * yy_c_buf_p so that if some total * hoser (like flex itself) wants to * call the scanner after we return the * YY_NULL, it'll still work - another * YY_NULL will get returned. */ (yy_c_buf_p) = (yytext_ptr) + YY_MORE_ADJ; yy_act = YY_STATE_EOF(YY_START); goto do_action; } else { if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; } break; } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + yy_amount_of_matched_text; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_match; case EOB_ACT_LAST_MATCH: (yy_c_buf_p) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)]; yy_current_state = yy_get_previous_state( ); yy_cp = (yy_c_buf_p); yy_bp = (yytext_ptr) + YY_MORE_ADJ; goto yy_find_action; } break; } default: YY_FATAL_ERROR( "fatal flex scanner internal error--no action found" ); } /* end of action switch */ } /* end of scanning one token */ } /* end of wcsutrnlex */ /* yy_get_next_buffer - try to read in a new buffer * * Returns a code representing an action: * EOB_ACT_LAST_MATCH - * EOB_ACT_CONTINUE_SCAN - continue scanning from current position * EOB_ACT_END_OF_FILE - end of file */ static int yy_get_next_buffer (void) { register char *dest = YY_CURRENT_BUFFER_LVALUE->yy_ch_buf; register char *source = (yytext_ptr); register int number_to_move, i; int ret_val; if ( (yy_c_buf_p) > &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] ) YY_FATAL_ERROR( "fatal flex scanner internal error--end of buffer missed" ); if ( YY_CURRENT_BUFFER_LVALUE->yy_fill_buffer == 0 ) { /* Don't try to fill the buffer, so this is an EOF. */ if ( (yy_c_buf_p) - (yytext_ptr) - YY_MORE_ADJ == 1 ) { /* We matched a single character, the EOB, so * treat this as a final EOF. */ return EOB_ACT_END_OF_FILE; } else { /* We matched some text prior to the EOB, first * process it. */ return EOB_ACT_LAST_MATCH; } } /* Try to read more data. */ /* First move last chars to start of buffer. */ number_to_move = (int) ((yy_c_buf_p) - (yytext_ptr)) - 1; for ( i = 0; i < number_to_move; ++i ) *(dest++) = *(source++); if ( YY_CURRENT_BUFFER_LVALUE->yy_buffer_status == YY_BUFFER_EOF_PENDING ) /* don't do the read, it's not guaranteed to return an EOF, * just force an EOF */ YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = 0; else { int num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; while ( num_to_read <= 0 ) { /* Not enough room in the buffer - grow it. */ /* just a shorter name for the current buffer */ YY_BUFFER_STATE b = YY_CURRENT_BUFFER; int yy_c_buf_p_offset = (int) ((yy_c_buf_p) - b->yy_ch_buf); if ( b->yy_is_our_buffer ) { int new_size = b->yy_buf_size * 2; if ( new_size <= 0 ) b->yy_buf_size += b->yy_buf_size / 8; else b->yy_buf_size *= 2; b->yy_ch_buf = (char *) /* Include room in for 2 EOB chars. */ wcsutrnrealloc((void *) b->yy_ch_buf,b->yy_buf_size + 2 ); } else /* Can't grow it, we don't own it. */ b->yy_ch_buf = 0; if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "fatal error - scanner input buffer overflow" ); (yy_c_buf_p) = &b->yy_ch_buf[yy_c_buf_p_offset]; num_to_read = YY_CURRENT_BUFFER_LVALUE->yy_buf_size - number_to_move - 1; } if ( num_to_read > YY_READ_BUF_SIZE ) num_to_read = YY_READ_BUF_SIZE; /* Read in more data. */ YY_INPUT( (&YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]), (yy_n_chars), (size_t) num_to_read ); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } if ( (yy_n_chars) == 0 ) { if ( number_to_move == YY_MORE_ADJ ) { ret_val = EOB_ACT_END_OF_FILE; wcsutrnrestart(wcsutrnin ); } else { ret_val = EOB_ACT_LAST_MATCH; YY_CURRENT_BUFFER_LVALUE->yy_buffer_status = YY_BUFFER_EOF_PENDING; } } else ret_val = EOB_ACT_CONTINUE_SCAN; if ((yy_size_t) ((yy_n_chars) + number_to_move) > YY_CURRENT_BUFFER_LVALUE->yy_buf_size) { /* Extend the array by 50%, plus the number we really need. */ yy_size_t new_size = (yy_n_chars) + number_to_move + ((yy_n_chars) >> 1); YY_CURRENT_BUFFER_LVALUE->yy_ch_buf = (char *) wcsutrnrealloc((void *) YY_CURRENT_BUFFER_LVALUE->yy_ch_buf,new_size ); if ( ! YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in yy_get_next_buffer()" ); } (yy_n_chars) += number_to_move; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] = YY_END_OF_BUFFER_CHAR; YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars) + 1] = YY_END_OF_BUFFER_CHAR; (yytext_ptr) = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[0]; return ret_val; } /* yy_get_previous_state - get the state just before the EOB char was reached */ static yy_state_type yy_get_previous_state (void) { register yy_state_type yy_current_state; register char *yy_cp; yy_current_state = (yy_start); yy_current_state += YY_AT_BOL(); for ( yy_cp = (yytext_ptr) + YY_MORE_ADJ; yy_cp < (yy_c_buf_p); ++yy_cp ) { if ( *yy_cp ) { yy_current_state = yy_nxt[yy_current_state][YY_SC_TO_UI(*yy_cp)]; } else yy_current_state = yy_NUL_trans[yy_current_state]; } return yy_current_state; } /* yy_try_NUL_trans - try to make a transition on the NUL character * * synopsis * next_state = yy_try_NUL_trans( current_state ); */ static yy_state_type yy_try_NUL_trans (yy_state_type yy_current_state ) { register int yy_is_jam; yy_current_state = yy_NUL_trans[yy_current_state]; yy_is_jam = (yy_current_state == 0); return yy_is_jam ? 0 : yy_current_state; } static void yyunput (int c, register char * yy_bp ) { register char *yy_cp; yy_cp = (yy_c_buf_p); /* undo effects of setting up wcsutrntext */ *yy_cp = (yy_hold_char); if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) { /* need to shift things up to make room */ /* +2 for EOB chars. */ register int number_to_move = (yy_n_chars) + 2; register char *dest = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[ YY_CURRENT_BUFFER_LVALUE->yy_buf_size + 2]; register char *source = &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[number_to_move]; while ( source > YY_CURRENT_BUFFER_LVALUE->yy_ch_buf ) *--dest = *--source; yy_cp += (int) (dest - source); yy_bp += (int) (dest - source); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_buf_size; if ( yy_cp < YY_CURRENT_BUFFER_LVALUE->yy_ch_buf + 2 ) YY_FATAL_ERROR( "flex scanner push-back overflow" ); } *--yy_cp = (char) c; (yytext_ptr) = yy_bp; (yy_hold_char) = *yy_cp; (yy_c_buf_p) = yy_cp; } #ifndef YY_NO_INPUT #ifdef __cplusplus static int yyinput (void) #else static int input (void) #endif { int c; *(yy_c_buf_p) = (yy_hold_char); if ( *(yy_c_buf_p) == YY_END_OF_BUFFER_CHAR ) { /* yy_c_buf_p now points to the character we want to return. * If this occurs *before* the EOB characters, then it's a * valid NUL; if not, then we've hit the end of the buffer. */ if ( (yy_c_buf_p) < &YY_CURRENT_BUFFER_LVALUE->yy_ch_buf[(yy_n_chars)] ) /* This was really a NUL. */ *(yy_c_buf_p) = '\0'; else { /* need more input */ int offset = (yy_c_buf_p) - (yytext_ptr); ++(yy_c_buf_p); switch ( yy_get_next_buffer( ) ) { case EOB_ACT_LAST_MATCH: /* This happens because yy_g_n_b() * sees that we've accumulated a * token and flags that we need to * try matching the token before * proceeding. But for input(), * there's no matching to consider. * So convert the EOB_ACT_LAST_MATCH * to EOB_ACT_END_OF_FILE. */ /* Reset buffer status. */ wcsutrnrestart(wcsutrnin ); /*FALLTHROUGH*/ case EOB_ACT_END_OF_FILE: { if ( wcsutrnwrap( ) ) return EOF; if ( ! (yy_did_buffer_switch_on_eof) ) YY_NEW_FILE; #ifdef __cplusplus return yyinput(); #else return input(); #endif } case EOB_ACT_CONTINUE_SCAN: (yy_c_buf_p) = (yytext_ptr) + offset; break; } } } c = *(unsigned char *) (yy_c_buf_p); /* cast for 8-bit char's */ *(yy_c_buf_p) = '\0'; /* preserve wcsutrntext */ (yy_hold_char) = *++(yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_at_bol = (c == '\n'); return c; } #endif /* ifndef YY_NO_INPUT */ /** Immediately switch to a different input stream. * @param input_file A readable stream. * * @note This function does not reset the start condition to @c INITIAL . */ void wcsutrnrestart (FILE * input_file ) { if ( ! YY_CURRENT_BUFFER ){ wcsutrnensure_buffer_stack (); YY_CURRENT_BUFFER_LVALUE = wcsutrn_create_buffer(wcsutrnin,YY_BUF_SIZE ); } wcsutrn_init_buffer(YY_CURRENT_BUFFER,input_file ); wcsutrn_load_buffer_state( ); } /** Switch to a different input buffer. * @param new_buffer The new input buffer. * */ void wcsutrn_switch_to_buffer (YY_BUFFER_STATE new_buffer ) { /* TODO. We should be able to replace this entire function body * with * wcsutrnpop_buffer_state(); * wcsutrnpush_buffer_state(new_buffer); */ wcsutrnensure_buffer_stack (); if ( YY_CURRENT_BUFFER == new_buffer ) return; if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } YY_CURRENT_BUFFER_LVALUE = new_buffer; wcsutrn_load_buffer_state( ); /* We don't actually know whether we did this switch during * EOF (wcsutrnwrap()) processing, but the only time this flag * is looked at is after wcsutrnwrap() is called, so it's safe * to go ahead and always set it. */ (yy_did_buffer_switch_on_eof) = 1; } static void wcsutrn_load_buffer_state (void) { (yy_n_chars) = YY_CURRENT_BUFFER_LVALUE->yy_n_chars; (yytext_ptr) = (yy_c_buf_p) = YY_CURRENT_BUFFER_LVALUE->yy_buf_pos; wcsutrnin = YY_CURRENT_BUFFER_LVALUE->yy_input_file; (yy_hold_char) = *(yy_c_buf_p); } /** Allocate and initialize an input buffer state. * @param file A readable stream. * @param size The character buffer size in bytes. When in doubt, use @c YY_BUF_SIZE. * * @return the allocated buffer state. */ YY_BUFFER_STATE wcsutrn_create_buffer (FILE * file, int size ) { YY_BUFFER_STATE b; b = (YY_BUFFER_STATE) wcsutrnalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcsutrn_create_buffer()" ); b->yy_buf_size = size; /* yy_ch_buf has to be 2 characters longer than the size given because * we need to put in 2 end-of-buffer characters. */ b->yy_ch_buf = (char *) wcsutrnalloc(b->yy_buf_size + 2 ); if ( ! b->yy_ch_buf ) YY_FATAL_ERROR( "out of dynamic memory in wcsutrn_create_buffer()" ); b->yy_is_our_buffer = 1; wcsutrn_init_buffer(b,file ); return b; } /** Destroy the buffer. * @param b a buffer created with wcsutrn_create_buffer() * */ void wcsutrn_delete_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; if ( b == YY_CURRENT_BUFFER ) /* Not sure if we should pop here. */ YY_CURRENT_BUFFER_LVALUE = (YY_BUFFER_STATE) 0; if ( b->yy_is_our_buffer ) wcsutrnfree((void *) b->yy_ch_buf ); wcsutrnfree((void *) b ); } /* Initializes or reinitializes a buffer. * This function is sometimes called more than once on the same buffer, * such as during a wcsutrnrestart() or at EOF. */ static void wcsutrn_init_buffer (YY_BUFFER_STATE b, FILE * file ) { int oerrno = errno; wcsutrn_flush_buffer(b ); b->yy_input_file = file; b->yy_fill_buffer = 1; /* If b is the current buffer, then wcsutrn_init_buffer was _probably_ * called from wcsutrnrestart() or through yy_get_next_buffer. * In that case, we don't want to reset the lineno or column. */ if (b != YY_CURRENT_BUFFER){ b->yy_bs_lineno = 1; b->yy_bs_column = 0; } b->yy_is_interactive = 0; errno = oerrno; } /** Discard all buffered characters. On the next scan, YY_INPUT will be called. * @param b the buffer state to be flushed, usually @c YY_CURRENT_BUFFER. * */ void wcsutrn_flush_buffer (YY_BUFFER_STATE b ) { if ( ! b ) return; b->yy_n_chars = 0; /* We always need two end-of-buffer characters. The first causes * a transition to the end-of-buffer state. The second causes * a jam in that state. */ b->yy_ch_buf[0] = YY_END_OF_BUFFER_CHAR; b->yy_ch_buf[1] = YY_END_OF_BUFFER_CHAR; b->yy_buf_pos = &b->yy_ch_buf[0]; b->yy_at_bol = 1; b->yy_buffer_status = YY_BUFFER_NEW; if ( b == YY_CURRENT_BUFFER ) wcsutrn_load_buffer_state( ); } /** Pushes the new state onto the stack. The new state becomes * the current state. This function will allocate the stack * if necessary. * @param new_buffer The new state. * */ void wcsutrnpush_buffer_state (YY_BUFFER_STATE new_buffer ) { if (new_buffer == NULL) return; wcsutrnensure_buffer_stack(); /* This block is copied from wcsutrn_switch_to_buffer. */ if ( YY_CURRENT_BUFFER ) { /* Flush out information for old buffer. */ *(yy_c_buf_p) = (yy_hold_char); YY_CURRENT_BUFFER_LVALUE->yy_buf_pos = (yy_c_buf_p); YY_CURRENT_BUFFER_LVALUE->yy_n_chars = (yy_n_chars); } /* Only push if top exists. Otherwise, replace top. */ if (YY_CURRENT_BUFFER) (yy_buffer_stack_top)++; YY_CURRENT_BUFFER_LVALUE = new_buffer; /* copied from wcsutrn_switch_to_buffer. */ wcsutrn_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } /** Removes and deletes the top of the stack, if present. * The next element becomes the new top. * */ void wcsutrnpop_buffer_state (void) { if (!YY_CURRENT_BUFFER) return; wcsutrn_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; if ((yy_buffer_stack_top) > 0) --(yy_buffer_stack_top); if (YY_CURRENT_BUFFER) { wcsutrn_load_buffer_state( ); (yy_did_buffer_switch_on_eof) = 1; } } /* Allocates the stack if it does not exist. * Guarantees space for at least one push. */ static void wcsutrnensure_buffer_stack (void) { int num_to_alloc; if (!(yy_buffer_stack)) { /* First allocation is just for 2 elements, since we don't know if this * scanner will even need a stack. We use 2 instead of 1 to avoid an * immediate realloc on the next call. */ num_to_alloc = 1; (yy_buffer_stack) = (struct yy_buffer_state**)wcsutrnalloc (num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcsutrnensure_buffer_stack()" ); memset((yy_buffer_stack), 0, num_to_alloc * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; (yy_buffer_stack_top) = 0; return; } if ((yy_buffer_stack_top) >= ((yy_buffer_stack_max)) - 1){ /* Increase the buffer to prepare for a possible push. */ int grow_size = 8 /* arbitrary grow size */; num_to_alloc = (yy_buffer_stack_max) + grow_size; (yy_buffer_stack) = (struct yy_buffer_state**)wcsutrnrealloc ((yy_buffer_stack), num_to_alloc * sizeof(struct yy_buffer_state*) ); if ( ! (yy_buffer_stack) ) YY_FATAL_ERROR( "out of dynamic memory in wcsutrnensure_buffer_stack()" ); /* zero only the new slots.*/ memset((yy_buffer_stack) + (yy_buffer_stack_max), 0, grow_size * sizeof(struct yy_buffer_state*)); (yy_buffer_stack_max) = num_to_alloc; } } /** Setup the input buffer state to scan directly from a user-specified character buffer. * @param base the character buffer * @param size the size in bytes of the character buffer * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcsutrn_scan_buffer (char * base, yy_size_t size ) { YY_BUFFER_STATE b; if ( size < 2 || base[size-2] != YY_END_OF_BUFFER_CHAR || base[size-1] != YY_END_OF_BUFFER_CHAR ) /* They forgot to leave room for the EOB's. */ return 0; b = (YY_BUFFER_STATE) wcsutrnalloc(sizeof( struct yy_buffer_state ) ); if ( ! b ) YY_FATAL_ERROR( "out of dynamic memory in wcsutrn_scan_buffer()" ); b->yy_buf_size = size - 2; /* "- 2" to take care of EOB's */ b->yy_buf_pos = b->yy_ch_buf = base; b->yy_is_our_buffer = 0; b->yy_input_file = 0; b->yy_n_chars = b->yy_buf_size; b->yy_is_interactive = 0; b->yy_at_bol = 1; b->yy_fill_buffer = 0; b->yy_buffer_status = YY_BUFFER_NEW; wcsutrn_switch_to_buffer(b ); return b; } /** Setup the input buffer state to scan a string. The next call to wcsutrnlex() will * scan from a @e copy of @a str. * @param yystr a NUL-terminated string to scan * * @return the newly allocated buffer state object. * @note If you want to scan bytes that may contain NUL values, then use * wcsutrn_scan_bytes() instead. */ YY_BUFFER_STATE wcsutrn_scan_string (yyconst char * yystr ) { return wcsutrn_scan_bytes(yystr,strlen(yystr) ); } /** Setup the input buffer state to scan the given bytes. The next call to wcsutrnlex() will * scan from a @e copy of @a bytes. * @param yybytes the byte buffer to scan * @param _yybytes_len the number of bytes in the buffer pointed to by @a bytes. * * @return the newly allocated buffer state object. */ YY_BUFFER_STATE wcsutrn_scan_bytes (yyconst char * yybytes, int _yybytes_len ) { YY_BUFFER_STATE b; char *buf; yy_size_t n; int i; /* Get memory for full buffer, including space for trailing EOB's. */ n = _yybytes_len + 2; buf = (char *) wcsutrnalloc(n ); if ( ! buf ) YY_FATAL_ERROR( "out of dynamic memory in wcsutrn_scan_bytes()" ); for ( i = 0; i < _yybytes_len; ++i ) buf[i] = yybytes[i]; buf[_yybytes_len] = buf[_yybytes_len+1] = YY_END_OF_BUFFER_CHAR; b = wcsutrn_scan_buffer(buf,n ); if ( ! b ) YY_FATAL_ERROR( "bad buffer in wcsutrn_scan_bytes()" ); /* It's okay to grow etc. this buffer, and we should throw it * away when we're done. */ b->yy_is_our_buffer = 1; return b; } #ifndef YY_EXIT_FAILURE #define YY_EXIT_FAILURE 2 #endif static void yy_fatal_error (yyconst char* msg ) { (void) fprintf( stderr, "%s\n", msg ); exit( YY_EXIT_FAILURE ); } /* Redefine yyless() so it works in section 3 code. */ #undef yyless #define yyless(n) \ do \ { \ /* Undo effects of setting up wcsutrntext. */ \ int yyless_macro_arg = (n); \ YY_LESS_LINENO(yyless_macro_arg);\ wcsutrntext[wcsutrnleng] = (yy_hold_char); \ (yy_c_buf_p) = wcsutrntext + yyless_macro_arg; \ (yy_hold_char) = *(yy_c_buf_p); \ *(yy_c_buf_p) = '\0'; \ wcsutrnleng = yyless_macro_arg; \ } \ while ( 0 ) /* Accessor methods (get/set functions) to struct members. */ /** Get the current line number. * */ int wcsutrnget_lineno (void) { return wcsutrnlineno; } /** Get the input stream. * */ FILE *wcsutrnget_in (void) { return wcsutrnin; } /** Get the output stream. * */ FILE *wcsutrnget_out (void) { return wcsutrnout; } /** Get the length of the current token. * */ int wcsutrnget_leng (void) { return wcsutrnleng; } /** Get the current token. * */ char *wcsutrnget_text (void) { return wcsutrntext; } /** Set the current line number. * @param line_number * */ void wcsutrnset_lineno (int line_number ) { wcsutrnlineno = line_number; } /** Set the input stream. This does not discard the current * input buffer. * @param in_str A readable stream. * * @see wcsutrn_switch_to_buffer */ void wcsutrnset_in (FILE * in_str ) { wcsutrnin = in_str ; } void wcsutrnset_out (FILE * out_str ) { wcsutrnout = out_str ; } int wcsutrnget_debug (void) { return wcsutrn_flex_debug; } void wcsutrnset_debug (int bdebug ) { wcsutrn_flex_debug = bdebug ; } static int yy_init_globals (void) { /* Initialization is the same as for the non-reentrant scanner. * This function is called from wcsutrnlex_destroy(), so don't allocate here. */ (yy_buffer_stack) = 0; (yy_buffer_stack_top) = 0; (yy_buffer_stack_max) = 0; (yy_c_buf_p) = (char *) 0; (yy_init) = 0; (yy_start) = 0; /* Defined in main.c */ #ifdef YY_STDINIT wcsutrnin = stdin; wcsutrnout = stdout; #else wcsutrnin = (FILE *) 0; wcsutrnout = (FILE *) 0; #endif /* For future reference: Set errno on error, since we are called by * wcsutrnlex_init() */ return 0; } /* wcsutrnlex_destroy is for both reentrant and non-reentrant scanners. */ int wcsutrnlex_destroy (void) { /* Pop the buffer stack, destroying each element. */ while(YY_CURRENT_BUFFER){ wcsutrn_delete_buffer(YY_CURRENT_BUFFER ); YY_CURRENT_BUFFER_LVALUE = NULL; wcsutrnpop_buffer_state(); } /* Destroy the stack itself. */ wcsutrnfree((yy_buffer_stack) ); (yy_buffer_stack) = NULL; /* Reset the globals. This is important in a non-reentrant scanner so the next time * wcsutrnlex() is called, initialization will occur. */ yy_init_globals( ); return 0; } /* * Internal utility routines. */ #ifndef yytext_ptr static void yy_flex_strncpy (char* s1, yyconst char * s2, int n ) { register int i; for ( i = 0; i < n; ++i ) s1[i] = s2[i]; } #endif #ifdef YY_NEED_STRLEN static int yy_flex_strlen (yyconst char * s ) { register int n; for ( n = 0; s[n]; ++n ) ; return n; } #endif void *wcsutrnalloc (yy_size_t size ) { return (void *) malloc( size ); } void *wcsutrnrealloc (void * ptr, yy_size_t size ) { /* The cast to (char *) in the following accommodates both * implementations that use char* generic pointers, and those * that use void* generic pointers. It works with the latter * because both ANSI C and C++ allow castless assignment from * any pointer type to void*, and deal with argument conversions * as though doing an assignment. */ return (void *) realloc( (char *) ptr, size ); } void wcsutrnfree (void * ptr ) { free( (char *) ptr ); /* see wcsutrnrealloc() for (char *) cast */ } #define YYTABLES_NAME "yytables" #line 341 "wcsutrn.l" pywcs-1.12/wcslib/C/getwcstab.c0000644001153600020070000001036312310355626020445 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: getwcstab.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include "getwcstab.h" /*--------------------------------------------------------------------------*/ int fits_read_wcstab( fitsfile *fptr, int nwtb, wtbarr *wtb, int *status) { int anynul, colnum, hdunum, iwtb, m, naxis, nostat; long *naxes = 0, nelem; wtbarr *wtbp; if (*status) return *status; if (fptr == 0) { return (*status = NULL_INPUT_PTR); } if (nwtb == 0) return 0; /* Zero the array pointers. */ wtbp = wtb; for (iwtb = 0; iwtb < nwtb; iwtb++, wtbp++) { *wtbp->arrayp = 0x0; } /* Save HDU number so that we can move back to it later. */ fits_get_hdu_num(fptr, &hdunum); wtbp = wtb; for (iwtb = 0; iwtb < nwtb; iwtb++, wtbp++) { /* Move to the required binary table extension. */ if (fits_movnam_hdu(fptr, BINARY_TBL, (char *)(wtbp->extnam), wtbp->extver, status)) { goto cleanup; } /* Locate the table column. */ if (fits_get_colnum(fptr, CASEINSEN, (char *)(wtbp->ttype), &colnum, status)) { goto cleanup; } /* Get the array dimensions and check for consistency. */ if (wtbp->ndim < 1) { *status = NEG_AXIS; goto cleanup; } if (!(naxes = calloc(wtbp->ndim, sizeof(long)))) { *status = MEMORY_ALLOCATION; goto cleanup; } if (fits_read_tdim(fptr, colnum, wtbp->ndim, &naxis, naxes, status)) { goto cleanup; } if (naxis != wtbp->ndim) { if (wtbp->kind == 'c' && wtbp->ndim == 2) { /* Allow TDIMn to be omitted for degenerate coordinate arrays. */ naxis = 2; naxes[1] = naxes[0]; naxes[0] = 1; } else { *status = BAD_TDIM; goto cleanup; } } if (wtbp->kind == 'c') { /* Coordinate array; calculate the array size. */ nelem = naxes[0]; for (m = 0; m < naxis-1; m++) { *(wtbp->dimlen + m) = naxes[m+1]; nelem *= naxes[m+1]; } } else { /* Index vector; check length. */ if ((nelem = naxes[0]) != *(wtbp->dimlen)) { /* N.B. coordinate array precedes the index vectors. */ *status = BAD_TDIM; goto cleanup; } } free(naxes); naxes = 0; /* Allocate memory for the array. */ if (!(*wtbp->arrayp = calloc((size_t)nelem, sizeof(double)))) { *status = MEMORY_ALLOCATION; goto cleanup; } /* Read the array from the table. */ if (fits_read_col_dbl(fptr, colnum, wtbp->row, 1L, nelem, 0.0, *wtbp->arrayp, &anynul, status)) { goto cleanup; } } cleanup: /* Move back to the starting HDU. */ nostat = 0; fits_movabs_hdu(fptr, hdunum, 0, &nostat); /* Release allocated memory. */ if (naxes) free(naxes); if (*status) { wtbp = wtb; for (iwtb = 0; iwtb < nwtb; iwtb++, wtbp++) { if (*wtbp->arrayp) free(*wtbp->arrayp); } } return *status; } pywcs-1.12/wcslib/C/getwcstab.h0000644001153600020070000001640512310355626020455 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: getwcstab.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * Summary of the getwcstab routines * --------------------------------- * fits_read_wcstab(), an implementation of a FITS table reading routine for * 'TAB' coordinates, is provided for CFITSIO programmers. It has been * incorporated into CFITSIO as of v3.006 with the definitions in this file, * getwcstab.h, moved into fitsio.h. * * fits_read_wcstab() is not included in the WCSLIB object library but the * source code is presented here as it may be useful for programmers using an * older version of CFITSIO than 3.006, or as a programming template for * non-CFITSIO programmers. * * * fits_read_wcstab() - FITS 'TAB' table reading routine * ---------------------------------------------------- * fits_read_wcstab() extracts arrays from a binary table required in * constructing 'TAB' coordinates. * * Given: * fptr fitsfile * * Pointer to the file handle returned, for example, by * the fits_open_file() routine in CFITSIO. * * nwtb int Number of arrays to be read from the binary table(s). * * Given and returned: * wtb wtbarr * Address of the first element of an array of wtbarr * typedefs. This wtbarr typedef is defined to match the * wtbarr struct defined in WCSLIB. An array of such * structs returned by the WCSLIB function wcstab() as * discussed in the notes below. * * Returned: * status int * CFITSIO status value. * * Function return value: * int CFITSIO status value. * * Notes: * In order to maintain WCSLIB and CFITSIO as independent libraries it is not * permissible for any CFITSIO library code to include WCSLIB header files, * or vice versa. However, the CFITSIO function fits_read_wcstab() accepts * an array of wtbarr structs defined in wcs.h within WCSLIB. * * The problem therefore is to define the wtbarr struct within fitsio.h * without including wcs.h, especially noting that wcs.h will often (but not * always) be included together with fitsio.h in an applications program that * uses fits_read_wcstab(). * * The solution adopted is for WCSLIB to define "struct wtbarr" while * fitsio.h defines "typedef wtbarr" as an untagged struct with identical * members. This allows both wcs.h and fitsio.h to define a wtbarr data type * without conflict by virtue of the fact that structure tags and typedef * names share different name spaces in C; Appendix A, Sect. A11.1 (p227) of * the K&R ANSI edition states that: * * Identifiers fall into several name spaces that do not interfere with one * another; the same identifier may be used for different purposes, even in * the same scope, if the uses are in different name spaces. These classes * are: objects, functions, typedef names, and enum constants; labels; tags * of structures, unions, and enumerations; and members of each structure * or union individually. * * Therefore, declarations within WCSLIB look like * = struct wtbarr *w; * * while within CFITSIO they are simply * = wtbarr *w; * * As suggested by the commonality of the names, these are really the same * aggregate data type. However, in passing a (struct wtbarr *) to * fits_read_wcstab() a cast to (wtbarr *) is formally required. * * When using WCSLIB and CFITSIO together in C++ the situation is complicated * by the fact that typedefs and structs share the same namespace; C++ * Annotated Reference Manual, Sect. 7.1.3 (p105). In that case the wtbarr * struct in wcs.h is renamed by preprocessor macro substitution to wtbarr_s * to distinguish it from the typedef defined in fitsio.h. However, the * scope of this macro substitution is limited to wcs.h itself and CFITSIO * programmer code, whether in C++ or C, should always use the wtbarr * typedef. * * * wtbarr typedef * -------------- * The wtbarr typedef is defined as a struct containing the following members: * * int i * Image axis number. * * int m * Array axis number for index vectors. * * int kind * Character identifying the array type: * - c: coordinate array, * - i: index vector. * * char extnam[72] * EXTNAME identifying the binary table extension. * * int extver * EXTVER identifying the binary table extension. * * int extlev * EXTLEV identifying the binary table extension. * * char ttype[72] * TTYPEn identifying the column of the binary table that contains the * array. * * long row * Table row number. * * int ndim * Expected dimensionality of the array. * * int *dimlen * Address of the first element of an array of int of length ndim into * which the array axis lengths are to be written. * * double **arrayp * Pointer to an array of double which is to be allocated by the user * and into which the array is to be written. * *===========================================================================*/ #ifndef WCSLIB_GETWCSTAB #define WCSLIB_GETWCSTAB #ifdef __cplusplus extern "C" { #endif #include typedef struct { int i; /* Image axis number. */ int m; /* Array axis number for index vectors. */ int kind; /* Array type, 'c' (coord) or 'i' (index). */ char extnam[72]; /* EXTNAME of binary table extension. */ int extver; /* EXTVER of binary table extension. */ int extlev; /* EXTLEV of binary table extension. */ char ttype[72]; /* TTYPEn of column containing the array. */ long row; /* Table row number. */ int ndim; /* Expected array dimensionality. */ int *dimlen; /* Where to write the array axis lengths. */ double **arrayp; /* Where to write the address of the array */ /* allocated to store the array. */ } wtbarr; int fits_read_wcstab(fitsfile *fptr, int nwtb, wtbarr *wtb, int *status); #ifdef __cplusplus } #endif #endif /* WCSLIB_GETWCSTAB */ pywcs-1.12/wcslib/C/GNUmakefile0000644001153600020070000003327512310355626020377 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile for building WCSLIB 4.10 and its test suite. # # Summary of the main targets # --------------------------- # build: Build the library. # # clean: Delete intermediate object files. # # cleaner: clean, and also delete the test executables. # # cleanest (distclean or realclean): cleaner, and also delete the object # library the C source files generated by 'flex'. # # check (or test): Compile and run the test programs. By default they are # executed in batch mode, and non-graphical tests only report # "PASS" on success. Use # # make MODE=interactive check # # to run them interactively with full diagnostic output. To skip # graphical tests even if PGPLOT is available, use # # make CHECK=nopgplot check # # tests: Compile the test programs (but don't run them). # # Notes: # 1) If you need to make changes then preferably modify ../makedefs.in # instead and re-run configure. # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: GNUmakefile,v 4.10 2012/02/05 23:41:44 cal103 Exp $ #----------------------------------------------------------------------------- # Get configure settings. include ../makedefs FLEXMODS := $(patsubst %.l,%.c,$(wildcard *.l)) MODULES := $(sort \ $(patsubst %.c,%.o, \ $(filter-out getwcstab.c,$(wildcard *.c)) $(FLEXMODS))) ifeq "$(WCSTRIG)" "MACRO" CPPFLAGS += -DWCSTRIG_MACRO MODULES := $(filter-out wcstrig.o, $(MODULES)) else ifeq "$(WCSTRIG)" "NATIVE" MODULES := $(filter-out wcstrig.o, $(MODULES)) endif endif # For building the sharable library. PICLIB := libwcs-PIC.a CPPFLAGS += -I. -I.. vpath %.c test vpath %.h .. vpath %.in .. # For building and exercising the test suite # ------------------------------------------ # Signals tfitshdr to use wcshdr(). ifneq "$(DO_WCSHDR)" "" CPPFLAGS += -DDO_WCSHDR endif # Test programs that don't require CFITSIO or PGPLOT. TEST_N := tlin tlog tprj1 tsph tsphdpa tspx ttab1 twcs twcssub tpih1 tbth1 \ tfitshdr tunits twcsfix # Test programs that require CFITSIO (they don't need PGPLOT). TEST_C := twcstab twcshdr # Test programs that require PGPLOT but not PGSBOX. TEST_P := tspc tprj2 tcel1 tcel2 ttab2 ttab3 twcsmix # Test programs that require PGPLOT and PGSBOX. TEST_B := tpih2 # Test programs that aren't automatically exercised. TEST_X := tsphdpa twcshdr TESTS := $(TEST_N) # Add test programs that require CFITSIO if we have it. ifneq "$(CFITSIOINC)" "" ifneq "$(CFITSIOLIB)" "" TESTS += $(TEST_C) endif endif # Add test programs that require PGPLOT if we have it. ifneq "$(CHECK)" "nopgplot" ifneq "$(PGPLOTINC)" "" ifneq "$(PGPLOTLIB)" "" TESTS += $(TEST_P) $(TEST_B) endif endif endif # Remove tests that aren't automatically exercised. TESTS := $(filter-out $(TEST_X), $(TESTS)) PGSBOXLIB := ../pgsbox/libpgsbox-$(LIBVER).a # Pattern rules #-------------- ifeq "$(FLEX)" "flex" %.c : %.l -@ echo '' -@ $(RM) $@ $(FLEX) $(FLFLAGS) -t $< | sed -e 's/^[ ]*#/#/' > $@ else %.c : %.l -@ echo '' -@ $(RM) $@ cp flexed/$@ . endif $(WCSLIB)(%.o) : %.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) -c $< $(AR) r $(WCSLIB) $% -@ $(RM) $% $(PICLIB)(%.o) : %.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) $(SHRFLAGS) -c $< $(AR) r $(PICLIB) $% -@ $(RM) $% %.i : %.c -@ echo '' -@ $(RM) $@ $(CPP) $(CPPFLAGS) $(CFLAGS) $< > $@ # Print out include file dependencies. %.d : %.c -@ echo '' -@ $(CPP) $(CPPFLAGS) $(CFLAGS) $< | \ sed -n -e 's|^# 1 "\([^/].*\.h\)".*|\1|p' | \ sort -u # Use 'make FLAVOUR=Linux run_%' to have VALGRIND defined (from flavours). run_% : % -@ echo '' -@ $(TIMER) @ if [ '$(MODE)' = interactive -o '$(VALGRIND)' ] ; then \ printf 'Press to run $<: ' ; \ read DUMMY ; \ fi ; \ if [ '$(VALGRIND)' ] ; then \ if [ '$<' = tunits ] ; then \ $(VALGRIND) ./$< < test/units_test ; \ else \ $(VALGRIND) ./$< ; \ fi ; \ else \ if [ '$(filter $<, $(TEST_N) $(TEST_C))' ] ; then \ if [ '$<' = tunits ] ; then \ if [ '$(MODE)' = interactive ] ; then \ ./$< < test/units_test 2>&1 | tee $<.out ; \ else \ ./$< < test/units_test > $<.out 2>&1 ; \ fi ; \ else \ if [ '$(MODE)' = interactive ] ; then \ ./$< < /dev/null 2>&1 | tee $<.out ; \ else \ ./$< < /dev/null > $<.out 2>&1 ; \ fi ; \ fi ; \ if grep 'PASS:' $<.out > /dev/null ; then \ if [ '$(MODE)' != interactive ] ; then \ head -2 $<.out ; \ grep 'PASS:' $<.out ; \ fi ; \ echo 'PASS: C/$<' >> test_results ; \ elif [ -f 'test/$<.out' ] ; then \ trap 'rm -f run_test.tmp' 0 1 2 3 15 ; \ sed -e 's/0x[0-9a-f][0-9a-f][0-9a-f]*/0x
/g' $<.out > \ run_test.tmp ; \ mv -f run_test.tmp $<.out ; \ if cmp -s $<.out test/$<.out ; then \ if [ '$(MODE)' != interactive ] ; then \ head -1 $<.out ; \ fi ; \ echo '' ; \ echo 'PASS: Output agrees with C/test/$<.out' ; \ echo 'PASS: C/$<' >> test_results ; \ else \ if [ '$(MODE)' != interactive ] ; then \ cat $<.out ; \ fi ; \ echo '' ; \ echo 'FAIL: Output disagrees with C/test/$<.out' ; \ echo 'FAIL: C/$<' >> test_results ; \ fi ; \ elif [ '$(MODE)' != interactive ] ; then \ cat $<.out ; \ echo 'FAIL: C/$<' >> test_results ; \ fi ; \ elif [ '$(MODE)' = interactive ] ; then \ ./$< ; \ else \ if [ '$<' = tcel2 ] ; then \ echo N | ./$< ; \ else \ ./$< < /dev/null 2>&1 ; \ fi ; \ fi ; \ fi -@ echo '' # Static and static pattern rules #-------------------------------- .PHONY : build check clean cleaner cleanest distclean install lib realclean \ run_% test tests build : lib lib : $(FLEXMODS) $(WCSLIB) $(SHRLIB) $(WCSLIB) : $(MODULES:%=$(WCSLIB)(%)) -@ echo '' $(RANLIB) $@ $(SHRLIB) : $(PICLIB) -@ echo '' -@ $(RM) -r tmp mkdir tmp && \ cd tmp && \ trap 'cd .. ; $(RM) -r tmp' 0 1 2 3 15 ; \ $(AR) x ../$(PICLIB) && \ $(SHRLD) $(LDFLAGS) -o $@ *.o && \ mv $@ .. $(PICLIB) : $(MODULES:%.o=$(PICLIB)(%.o)) ; install : build - if [ ! -d "$(LIBDIR)" ] ; then \ $(INSTALL) -d -m 2775 $(LIBDIR) ; \ fi $(INSTALL) -m 644 $(WCSLIB) $(LIBDIR) $(RANLIB) $(LIBDIR)/$(WCSLIB) - if [ -h "$(LIBDIR)/libwcs.a" ] ; then \ $(RM) $(LIBDIR)/libwcs.a ; \ fi - $(LN_S) $(WCSLIB) $(LIBDIR)/libwcs.a - if [ "$(SHRLIB)" != "" ] ; then \ $(INSTALL) -m 644 $(SHRLIB) $(LIBDIR) ; \ if [ -h "$(LIBDIR)/$(SONAME)" ] ; then \ $(RM) $(LIBDIR)/$(SONAME) ; \ fi ; \ $(LN_S) $(SHRLIB) $(LIBDIR)/$(SONAME) ; \ if [ "$(SHRLN)" != "" ] ; then \ if [ -h "$(LIBDIR)/$(SHRLN)" ] ; then \ $(RM) $(LIBDIR)/$(SHRLN) ; \ fi ; \ $(LN_S) $(SONAME) $(LIBDIR)/$(SHRLN) ; \ fi ; \ fi - if [ ! -d "$(INCDIR)" ] ; then \ $(INSTALL) -d -m 2775 $(INCDIR) ; \ fi $(INSTALL) -m 444 *.h $(INCDIR) $(RM) $(INCLINK) $(LN_S) $(notdir $(INCDIR)) $(INCLINK) clean : - $(RM) -r *.o *.i a.out t*.out core *.dSYM $(EXTRA_CLEAN) cleaner : clean - $(RM) .gdb_history - $(RM) $(TEST_N) $(TEST_X) - $(RM) $(TEST_P) tpih2 twcstab twcshdr - $(RM) tofits bth.fits pih.fits wcstab.fits - $(RM) t*_cfitsio test_results cleanest distclean realclean : cleaner - $(RM) ../wcsconfig.h ../wcsconfig_tests.h - $(RM) fitshdr.c wcsbth.c wcspih.c wcsulex.c wcsutrn.c - $(RM) $(PICLIB) libwcs-*.a libwcs.so.* libwcs.*.dylib check test : tests $(TESTS:%=run_%) tests : $(TESTS) $(TEST_X) $(TEST_N) : % : test/%.c $(WCSLIB) -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) $(LDFLAGS) -o $@ $< $(WCSLIB) $(LIBS) -@ $(RM) $@.o $(TEST_P) : % : test/%.c $(WCSLIB) -@ echo '' $(CC) $(CPPFLAGS) $(PGPLOTINC) $(CFLAGS) -c -o $@.o $< $(LD) $(LDFLAGS) -o $@ $@.o $(PGPLOTLIB) $(WCSLIB) $(FLIBS) $(LIBS) -@ $(RM) $@.o tpih2 : test/tpih2.c $(PGSBOXLIB) $(WCSLIB) -@ echo '' $(CC) $(CPPFLAGS) -I../pgsbox $(PGPLOTINC) $(CFLAGS) -c -o $@.o $< $(LD) $(LDFLAGS) -o $@ $@.o $(PGSBOXLIB) $(PGPLOTLIB) $(WCSLIB) \ $(FLIBS) $(LIBS) -@ $(RM) $@.o tfitshdr_cfitsio tpih1_cfitsio tbth1_cfitsio : %_cfitsio : test/%.c $(WCSLIB) -@ echo '' $(CC) -DDO_CFITSIO $(CPPFLAGS) $(CFITSIOINC) $(CFLAGS) \ $(LDFLAGS) -o $@ $< $(CFITSIOLIB) $(WCSLIB) $(LIBS) -@ $(RM) $@.o tpih2_cfitsio : test/tpih2.c $(PGSBOXLIB) $(WCSLIB) -@ echo '' $(CC) -DDO_CFITSIO $(CPPFLAGS) -I../pgsbox $(PGPLOTINC) \ $(CFITSIOINC) $(CFLAGS) -c -o $@.o $< $(LD) $(LDFLAGS) -o $@ $@.o $(PGSBOXLIB) $(PGPLOTLIB) \ $(CFITSIOLIB) $(WCSLIB) $(FLIBS) $(LIBS) -@ $(RM) $@.o twcstab : test/twcstab.c $(GETWCSTAB) $(WCSLIB) -@ echo '' $(CC) $(CPPFLAGS) $(CFITSIOINC) $(CFLAGS) $(LDFLAGS) -o $@ $< \ $(GETWCSTAB) $(CFITSIOLIB) $(WCSLIB) $(LIBS) -@ $(RM) $@.o twcshdr : test/twcshdr.c $(GETWCSTAB) $(WCSLIB) -@ echo '' $(CC) $(CPPFLAGS) $(CFITSIOINC) $(CFLAGS) $(LDFLAGS) -o $@ $< \ $(GETWCSTAB) $(CFITSIOLIB) $(WCSLIB) $(LIBS) -@ $(RM) $@.o getwcstab.o : getwcstab.c getwcstab.h -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) $(CFITSIOINC) -c $< $(PGSBOXLIB) : -@ echo '' $(MAKE) -C ../pgsbox lib tofits : test/tofits.c $(CC) $(CPPFLAGS) $(CFLAGS) -o $@ $< pih.fits : test/pih.keyrec tofits ./tofits < $< > $@ bth.fits : test/bth.keyrec tofits ./tofits < $< > $@ GNUmakefile : ../makedefs ; ../makedefs ../wcsconfig.h ../wcsconfig_tests.h : makedefs.in wcsconfig.h.in \ wcsconfig_tests.h.in ../config.status -@ $(RM) ../wcsconfig.h ../wcsconfig_tests.h cd .. && ./config.status show :: -@ -@ echo ' FLEXMODS := $(FLEXMODS)' -@ -@ echo ' MODULES := $(MODULES)' # Dependencies (use the %.d pattern rule to list them) #----------------------------------------------------- $(WCSLIB)(cel.o) : cel.h prj.h sph.h wcsconfig.h wcserr.h wcsmath.h \ wcsprintf.h wcstrig.h $(WCSLIB)(fitshdr.o) : wcsconfig.h fitshdr.h $(WCSLIB)(lin.o) : lin.h wcserr.h wcsprintf.h $(WCSLIB)(log.o) : log.h $(WCSLIB)(prj.o) : prj.h wcsconfig.h wcserr.h wcsmath.h wcsprintf.h \ wcstrig.h wcsutil.h $(WCSLIB)(spc.o) : spc.h spx.h wcserr.h wcsmath.h wcsprintf.h wcstrig.h \ wcsutil.h $(WCSLIB)(sph.o) : sph.h wcsconfig.h wcstrig.h $(WCSLIB)(spx.o) : spx.h wcserr.h wcsmath.h $(WCSLIB)(tab.o) : tab.h wcserr.h wcsmath.h wcsprintf.h $(WCSLIB)(wcs.o) : cel.h lin.h log.h prj.h spc.h sph.h spx.h tab.h \ wcs.h wcsconfig.h wcserr.h wcsmath.h wcsprintf.h \ wcstrig.h wcsunits.h wcsutil.h $(WCSLIB)(wcsbth.o) : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcserr.h \ wcshdr.h wcsmath.h $(WCSLIB)(wcserr.o) : wcserr.h wcsprintf.h $(WCSLIB)(wcsfix.o) : cel.h lin.h prj.h spc.h sph.h spx.h tab.h wcs.h \ wcserr.h wcsfix.h wcsmath.h wcsunits.h wcsutil.h $(WCSLIB)(wcshdr.o) : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcserr.h \ wcshdr.h wcsmath.h wcsutil.h $(WCSLIB)(wcspih.o) : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcserr.h \ wcshdr.h wcsmath.h $(WCSLIB)(wcsprintf.o): wcsprintf.h $(WCSLIB)(wcstrig.o) : wcsconfig.h wcsmath.h wcstrig.h $(WCSLIB)(wcsulex.o) : wcserr.h wcsmath.h wcsunits.h $(WCSLIB)(wcsunits.o) : wcserr.h wcsunits.h $(WCSLIB)(wcsutil.o) : wcsutil.h $(WCSLIB)(wcsutrn.o) : wcserr.h wcsunits.h tbth1 tbth1_cfitsio : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcsconfig.h \ wcsconfig_tests.h wcserr.h wcsfix.h wcshdr.h tcel1 : cel.h prj.h wcserr.h tcel2 : cel.h prj.h wcserr.h tfitshdr tfitshdr_cfitsio : fitshdr.h wcsconfig.h wcsconfig_tests.h tlin : lin.h wcserr.h tlog : log.h tpih1 tpih1_cfitsio : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcsconfig.h \ wcsconfig_tests.h wcserr.h wcsfix.h wcshdr.h wcsprintf.h tpih2 tpih2_cfitsio : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcsconfig.h \ wcsconfig_tests.h wcserr.h wcshdr.h tprj1 : prj.h wcsconfig.h wcserr.h wcstrig.h tprj2 : prj.h wcserr.h tspc : spc.h spx.h wcsconfig.h wcserr.h wcstrig.h tsph : sph.h wcsconfig.h wcstrig.h tsphdpa : sph.h tspx : spx.h wcserr.h ttab1 : tab.h wcserr.h ttab2 : tab.h wcserr.h ttab3 : prj.h tab.h wcserr.h tunits : wcserr.h wcsunits.h twcs : cel.h lin.h log.h prj.h spc.h sph.h spx.h tab.h wcs.h wcsconfig.h \ wcsconfig_tests.h wcserr.h wcsfix.h wcshdr.h wcslib.h wcsmath.h \ wcsprintf.h wcstrig.h wcsunits.h wcsutil.h twcsfix : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcserr.h wcsfix.h \ wcsunits.h twcshdr : cel.h fitshdr.h getwcstab.h lin.h log.h prj.h spc.h sph.h spx.h \ tab.h wcs.h wcsconfig.h wcserr.h wcsfix.h wcshdr.h wcslib.h \ wcsmath.h wcsprintf.h wcstrig.h wcsunits.h wcsutil.h twcsmix : cel.h lin.h prj.h spc.h sph.h spx.h tab.h wcs.h wcserr.h twcssub : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h wcserr.h twcstab : cel.h fitshdr.h getwcstab.h lin.h log.h prj.h spc.h sph.h spx.h \ tab.h wcs.h wcsconfig.h wcserr.h wcsfix.h wcshdr.h wcslib.h \ wcsmath.h wcsprintf.h wcstrig.h wcsunits.h wcsutil.h run_tbth1 run_tbth1_cfitsio : bth.fits run_tfitshdr run_tfitshdr_cfitsio : pih.fits run_tpih1 run_tpih1_cfitsio : pih.fits run_tpih2 run_tpih2_cfitsio : pih.fits pywcs-1.12/wcslib/C/lin.c0000644001153600020070000004063012310355626017244 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: lin.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include "wcserr.h" #include "wcsprintf.h" #include "lin.h" const int LINSET = 137; /* Map status return value to message. */ const char *lin_errmsg[] = { "Success", "Null linprm pointer passed", "Memory allocation failed", "PCi_ja matrix is singular"}; /* Convenience macro for invoking wcserr_set(). */ #define LIN_ERRMSG(status) WCSERR_SET(status), lin_errmsg[status] /*--------------------------------------------------------------------------*/ int linini(alloc, naxis, lin) int alloc, naxis; struct linprm *lin; { static const char *function = "linini"; int i, j; double *pc; struct wcserr **err; if (lin == 0x0) return LINERR_NULL_POINTER; /* Initialize error message handling. */ err = &(lin->err); if (lin->flag != -1) { if (lin->err) free(lin->err); } lin->err = 0x0; /* Initialize memory management. */ if (lin->flag == -1 || lin->m_flag != LINSET) { lin->m_flag = 0; lin->m_naxis = 0x0; lin->m_crpix = 0x0; lin->m_pc = 0x0; lin->m_cdelt = 0x0; } if (naxis < 1) { return wcserr_set(WCSERR_SET(LINERR_MEMORY), "naxis must be positive (got %d)", naxis); } /* Allocate memory for arrays if required. */ if (alloc || lin->crpix == 0x0 || lin->pc == 0x0 || lin->cdelt == 0x0) { /* Was sufficient allocated previously? */ if (lin->m_flag == LINSET && lin->m_naxis < naxis) { /* No, free it. */ linfree(lin); } if (alloc || lin->crpix == 0x0) { if (lin->m_crpix) { /* In case the caller fiddled with it. */ lin->crpix = lin->m_crpix; } else { if (!(lin->crpix = calloc(naxis, sizeof(double)))) { return wcserr_set(LIN_ERRMSG(LINERR_MEMORY)); } lin->m_flag = LINSET; lin->m_naxis = naxis; lin->m_crpix = lin->crpix; } } if (alloc || lin->pc == 0x0) { if (lin->m_pc) { /* In case the caller fiddled with it. */ lin->pc = lin->m_pc; } else { if (!(lin->pc = calloc(naxis*naxis, sizeof(double)))) { linfree(lin); return wcserr_set(LIN_ERRMSG(LINERR_MEMORY)); } lin->m_flag = LINSET; lin->m_naxis = naxis; lin->m_pc = lin->pc; } } if (alloc || lin->cdelt == 0x0) { if (lin->m_cdelt) { /* In case the caller fiddled with it. */ lin->cdelt = lin->m_cdelt; } else { if (!(lin->cdelt = calloc(naxis, sizeof(double)))) { linfree(lin); return wcserr_set(LIN_ERRMSG(LINERR_MEMORY)); } lin->m_flag = LINSET; lin->m_naxis = naxis; lin->m_cdelt = lin->cdelt; } } } /* Free memory allocated by linset(). */ if (lin->flag == LINSET) { if (lin->piximg) free(lin->piximg); if (lin->imgpix) free(lin->imgpix); } lin->piximg = 0x0; lin->imgpix = 0x0; lin->i_naxis = 0x0; lin->flag = 0; lin->naxis = naxis; /* CRPIXja defaults to 0.0. */ for (j = 0; j < naxis; j++) { lin->crpix[j] = 0.0; } /* PCi_ja defaults to the unit matrix. */ pc = lin->pc; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++) { if (j == i) { *pc = 1.0; } else { *pc = 0.0; } pc++; } } /* CDELTia defaults to 1.0. */ for (i = 0; i < naxis; i++) { lin->cdelt[i] = 1.0; } return 0; } /*--------------------------------------------------------------------------*/ int lincpy(alloc, linsrc, lindst) int alloc; const struct linprm *linsrc; struct linprm *lindst; { static const char *function = "lincpy"; int i, j, naxis, status; const double *srcp; double *dstp; struct wcserr **err; if (linsrc == 0x0) return LINERR_NULL_POINTER; if (lindst == 0x0) return LINERR_NULL_POINTER; err = &(lindst->err); naxis = linsrc->naxis; if (naxis < 1) { return wcserr_set(WCSERR_SET(LINERR_MEMORY), "naxis must be positive (got %d)", naxis); } if ((status = linini(alloc, naxis, lindst))) { return status; } srcp = linsrc->crpix; dstp = lindst->crpix; for (j = 0; j < naxis; j++) { *(dstp++) = *(srcp++); } srcp = linsrc->pc; dstp = lindst->pc; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++) { *(dstp++) = *(srcp++); } } srcp = linsrc->cdelt; dstp = lindst->cdelt; for (i = 0; i < naxis; i++) { *(dstp++) = *(srcp++); } return 0; } /*--------------------------------------------------------------------------*/ int linfree(lin) struct linprm *lin; { if (lin == 0x0) return LINERR_NULL_POINTER; if (lin->flag != -1) { /* Free memory allocated by linini(). */ if (lin->m_flag == LINSET) { if (lin->crpix == lin->m_crpix) lin->crpix = 0x0; if (lin->pc == lin->m_pc) lin->pc = 0x0; if (lin->cdelt == lin->m_cdelt) lin->cdelt = 0x0; if (lin->m_crpix) free(lin->m_crpix); if (lin->m_pc) free(lin->m_pc); if (lin->m_cdelt) free(lin->m_cdelt); } } lin->m_flag = 0; lin->m_naxis = 0; lin->m_crpix = 0x0; lin->m_pc = 0x0; lin->m_cdelt = 0x0; /* Free memory allocated by linset(). */ if (lin->flag == LINSET) { if (lin->piximg) free(lin->piximg); if (lin->imgpix) free(lin->imgpix); } lin->piximg = 0x0; lin->imgpix = 0x0; lin->i_naxis = 0; if (lin->err) free(lin->err); lin->err = 0x0; lin->flag = 0; return 0; } /*--------------------------------------------------------------------------*/ int linprt(lin) const struct linprm *lin; { int i, j, k; if (lin == 0x0) return LINERR_NULL_POINTER; if (lin->flag != LINSET) { wcsprintf("The linprm struct is UNINITIALIZED.\n"); return 0; } wcsprintf(" flag: %d\n", lin->flag); wcsprintf(" naxis: %d\n", lin->naxis); WCSPRINTF_PTR(" crpix: ", lin->crpix, "\n"); wcsprintf(" "); for (i = 0; i < lin->naxis; i++) { wcsprintf(" %- 11.5g", lin->crpix[i]); } wcsprintf("\n"); k = 0; WCSPRINTF_PTR(" pc: ", lin->pc, "\n"); for (i = 0; i < lin->naxis; i++) { wcsprintf(" pc[%d][]:", i); for (j = 0; j < lin->naxis; j++) { wcsprintf(" %- 11.5g", lin->pc[k++]); } wcsprintf("\n"); } WCSPRINTF_PTR(" cdelt: ", lin->cdelt, "\n"); wcsprintf(" "); for (i = 0; i < lin->naxis; i++) { wcsprintf(" %- 11.5g", lin->cdelt[i]); } wcsprintf("\n"); wcsprintf(" unity: %d\n", lin->unity); WCSPRINTF_PTR(" err: ", lin->err, "\n"); if (lin->err) { wcserr_prt(lin->err, " "); } if (lin->piximg == 0x0) { wcsprintf(" piximg: (nil)\n"); } else { k = 0; for (i = 0; i < lin->naxis; i++) { wcsprintf("piximg[%d][]:", i); for (j = 0; j < lin->naxis; j++) { wcsprintf(" %- 11.5g", lin->piximg[k++]); } wcsprintf("\n"); } } if (lin->imgpix == 0x0) { wcsprintf(" imgpix: (nil)\n"); } else { k = 0; for (i = 0; i < lin->naxis; i++) { wcsprintf("imgpix[%d][]:", i); for (j = 0; j < lin->naxis; j++) { wcsprintf(" %- 11.5g", lin->imgpix[k++]); } wcsprintf("\n"); } } wcsprintf(" m_flag: %d\n", lin->m_flag); wcsprintf(" m_naxis: %d\n", lin->m_naxis); WCSPRINTF_PTR(" m_crpix: ", lin->m_crpix, ""); if (lin->m_crpix == lin->crpix) wcsprintf(" (= crpix)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_pc: ", lin->m_pc, ""); if (lin->m_pc == lin->pc) wcsprintf(" (= pc)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_cdelt: ", lin->m_cdelt, ""); if (lin->m_cdelt == lin->cdelt) wcsprintf(" (= cdelt)"); wcsprintf("\n"); return 0; } /*--------------------------------------------------------------------------*/ int linset(lin) struct linprm *lin; { static const char *function = "linset"; int i, j, n, status; double *pc, *piximg; struct wcserr **err; if (lin == 0x0) return LINERR_NULL_POINTER; err = &(lin->err); n = lin->naxis; /* Check for a unit matrix. */ lin->unity = 1; pc = lin->pc; for (i = 0; i < n; i++) { for (j = 0; j < n; j++) { if (j == i) { if (*(pc++) != 1.0) { lin->unity = 0; break; } } else { if (*(pc++) != 0.0) { lin->unity = 0; break; } } } } if (lin->unity) { if (lin->flag == LINSET) { /* Free memory that may have been allocated previously. */ if (lin->piximg) free(lin->piximg); if (lin->imgpix) free(lin->imgpix); } lin->piximg = 0x0; lin->imgpix = 0x0; lin->i_naxis = 0; } else { if (lin->flag != LINSET || lin->i_naxis < n) { if (lin->flag == LINSET) { /* Free memory that may have been allocated previously. */ if (lin->piximg) free(lin->piximg); if (lin->imgpix) free(lin->imgpix); } /* Allocate memory for internal arrays. */ if (!(lin->piximg = calloc(n*n, sizeof(double)))) { return wcserr_set(LIN_ERRMSG(LINERR_MEMORY)); } if (!(lin->imgpix = calloc(n*n, sizeof(double)))) { free(lin->piximg); return wcserr_set(LIN_ERRMSG(LINERR_MEMORY)); } lin->i_naxis = n; } /* Compute the pixel-to-image transformation matrix. */ pc = lin->pc; piximg = lin->piximg; for (i = 0; i < n; i++) { for (j = 0; j < n; j++) { *(piximg++) = lin->cdelt[i] * (*(pc++)); } } /* Compute the image-to-pixel transformation matrix. */ if ((status = matinv(n, lin->piximg, lin->imgpix))) { return wcserr_set(LIN_ERRMSG(status)); } } lin->flag = LINSET; return 0; } /*--------------------------------------------------------------------------*/ int linp2x(lin, ncoord, nelem, pixcrd, imgcrd) struct linprm *lin; int ncoord, nelem; const double pixcrd[]; double imgcrd[]; { int i, j, k, n, status; double temp; register const double *pix; register double *img, *piximg; /* Initialize. */ if (lin == 0x0) return LINERR_NULL_POINTER; if (lin->flag != LINSET) { if ((status = linset(lin))) return status; } n = lin->naxis; /* Convert pixel coordinates to intermediate world coordinates. */ pix = pixcrd; img = imgcrd; if (lin->unity) { for (k = 0; k < ncoord; k++) { for (i = 0; i < n; i++) { *(img++) = lin->cdelt[i] * (*(pix++) - lin->crpix[i]); } pix += (nelem - n); img += (nelem - n); } } else { for (k = 0; k < ncoord; k++) { for (i = 0; i < n; i++) { img[i] = 0.0; } for (j = 0; j < n; j++) { /* Column-wise multiplication allows this to be cached. */ temp = *(pix++) - lin->crpix[j]; piximg = lin->piximg + j; for (i = 0; i < n; i++, piximg += n) { img[i] += *piximg * temp; } } pix += (nelem - n); img += nelem; } } return 0; } /*--------------------------------------------------------------------------*/ int linx2p(lin, ncoord, nelem, imgcrd, pixcrd) struct linprm *lin; int ncoord, nelem; const double imgcrd[]; double pixcrd[]; { int i, j, k, n, status; register const double *img; register double *imgpix, *pix; /* Initialize. */ if (lin == 0x0) return LINERR_NULL_POINTER; if (lin->flag != LINSET) { if ((status = linset(lin))) return status; } n = lin->naxis; /* Convert intermediate world coordinates to pixel coordinates. */ img = imgcrd; pix = pixcrd; if (lin->unity) { for (k = 0; k < ncoord; k++) { for (j = 0; j < n; j++) { *(pix++) = (*(img++) / lin->cdelt[j]) + lin->crpix[j]; } pix += (nelem - n); img += (nelem - n); } } else { for (k = 0; k < ncoord; k++) { imgpix = lin->imgpix; for (j = 0; j < n; j++) { *pix = 0.0; for (i = 0; i < n; i++) { *pix += *imgpix * img[i]; imgpix++; } *(pix++) += lin->crpix[j]; } pix += (nelem - n); img += nelem; } } return 0; } /*--------------------------------------------------------------------------*/ int matinv(int n, const double mat[], double inv[]) { register int i, ij, ik, j, k, kj, pj; int itemp, *mxl, *lxm, pivot; double colmax, *lu, *rowmax, dtemp; /* Allocate memory for internal arrays. */ if (!(mxl = calloc(n, sizeof(int)))) { return LINERR_MEMORY; } if (!(lxm = calloc(n, sizeof(int)))) { free(mxl); return LINERR_MEMORY; } if (!(rowmax = calloc(n, sizeof(double)))) { free(mxl); free(lxm); return LINERR_MEMORY; } if (!(lu = calloc(n*n, sizeof(double)))) { free(mxl); free(lxm); free(rowmax); return LINERR_MEMORY; } /* Initialize arrays. */ for (i = 0, ij = 0; i < n; i++) { /* Vector that records row interchanges. */ mxl[i] = i; rowmax[i] = 0.0; for (j = 0; j < n; j++, ij++) { dtemp = fabs(mat[ij]); if (dtemp > rowmax[i]) rowmax[i] = dtemp; lu[ij] = mat[ij]; } /* A row of zeroes indicates a singular matrix. */ if (rowmax[i] == 0.0) { free(mxl); free(lxm); free(rowmax); free(lu); return LINERR_SINGULAR_MTX; } } /* Form the LU triangular factorization using scaled partial pivoting. */ for (k = 0; k < n; k++) { /* Decide whether to pivot. */ colmax = fabs(lu[k*n+k]) / rowmax[k]; pivot = k; for (i = k+1; i < n; i++) { ik = i*n + k; dtemp = fabs(lu[ik]) / rowmax[i]; if (dtemp > colmax) { colmax = dtemp; pivot = i; } } if (pivot > k) { /* We must pivot, interchange the rows of the design matrix. */ for (j = 0, pj = pivot*n, kj = k*n; j < n; j++, pj++, kj++) { dtemp = lu[pj]; lu[pj] = lu[kj]; lu[kj] = dtemp; } /* Amend the vector of row maxima. */ dtemp = rowmax[pivot]; rowmax[pivot] = rowmax[k]; rowmax[k] = dtemp; /* Record the interchange for later use. */ itemp = mxl[pivot]; mxl[pivot] = mxl[k]; mxl[k] = itemp; } /* Gaussian elimination. */ for (i = k+1; i < n; i++) { ik = i*n + k; /* Nothing to do if lu[ik] is zero. */ if (lu[ik] != 0.0) { /* Save the scaling factor. */ lu[ik] /= lu[k*n+k]; /* Subtract rows. */ for (j = k+1; j < n; j++) { lu[i*n+j] -= lu[ik]*lu[k*n+j]; } } } } /* mxl[i] records which row of mat corresponds to row i of lu. */ /* lxm[i] records which row of lu corresponds to row i of mat. */ for (i = 0; i < n; i++) { lxm[mxl[i]] = i; } /* Determine the inverse matrix. */ for (i = 0, ij = 0; i < n; i++) { for (j = 0; j < n; j++, ij++) { inv[ij] = 0.0; } } for (k = 0; k < n; k++) { inv[lxm[k]*n+k] = 1.0; /* Forward substitution. */ for (i = lxm[k]+1; i < n; i++) { for (j = lxm[k]; j < i; j++) { inv[i*n+k] -= lu[i*n+j]*inv[j*n+k]; } } /* Backward substitution. */ for (i = n-1; i >= 0; i--) { for (j = i+1; j < n; j++) { inv[i*n+k] -= lu[i*n+j]*inv[j*n+k]; } inv[i*n+k] /= lu[i*n+i]; } } free(mxl); free(lxm); free(rowmax); free(lu); return 0; } pywcs-1.12/wcslib/C/lin.h0000644001153600020070000004111112310355626017244 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: lin.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the lin routines * --------------------------- * These routines apply the linear transformation defined by the FITS WCS * standard. They are based on the linprm struct which contains all * information needed for the computations. The struct contains some members * that must be set by the user, and others that are maintained by these * routines, somewhat like a C++ class but with no encapsulation. * * Three routines, linini(), lincpy(), and linfree() are provided to manage the * linprm struct, and another, linprt(), prints its contents. * * A setup routine, linset(), computes intermediate values in the linprm struct * from parameters in it that were supplied by the user. The struct always * needs to be set up by linset() but need not be called explicitly - refer to * the explanation of linprm::flag. * * linp2x() and linx2p() implement the WCS linear transformations. * * An auxiliary matrix inversion routine, matinv(), is included. It uses * LU-triangular factorization with scaled partial pivoting. * * * linini() - Default constructor for the linprm struct * ---------------------------------------------------- * linini() allocates memory for arrays in a linprm struct and sets all members * of the struct to default values. * * PLEASE NOTE: every linprm struct should be initialized by linini(), possibly * repeatedly. On the first invokation, and only the first invokation, * linprm::flag must be set to -1 to initialize memory management, regardless * of whether linini() will actually be used to allocate memory. * * Given: * alloc int If true, allocate memory unconditionally for arrays in * the linprm struct. * * If false, it is assumed that pointers to these arrays * have been set by the user except if they are null * pointers in which case memory will be allocated for * them regardless. (In other words, setting alloc true * saves having to initalize these pointers to zero.) * * naxis int The number of world coordinate axes, used to determine * array sizes. * * Given and returned: * lin struct linprm* * Linear transformation parameters. Note that, in order * to initialize memory management linprm::flag should be * set to -1 when lin is initialized for the first time * (memory leaks may result if it had already been * initialized). * * Function return value: * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * 2: Memory allocation failed. * * For returns > 1, a detailed error message is set in * linprm::err if enabled, see wcserr_enable(). * * * lincpy() - Copy routine for the linprm struct * --------------------------------------------- * lincpy() does a deep copy of one linprm struct to another, using linini() to * allocate memory for its arrays if required. Only the "information to be * provided" part of the struct is copied; a call to linset() is required to * initialize the remainder. * * Given: * alloc int If true, allocate memory for the crpix, pc, and cdelt * arrays in the destination. Otherwise, it is assumed * that pointers to these arrays have been set by the * user except if they are null pointers in which case * memory will be allocated for them regardless. * * linsrc const struct linprm* * Struct to copy from. * * Given and returned: * lindst struct linprm* * Struct to copy to. linprm::flag should be set to -1 * if lindst was not previously initialized (memory leaks * may result if it was previously initialized). * * Function return value: * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * 2: Memory allocation failed. * * For returns > 1, a detailed error message is set in * linprm::err if enabled, see wcserr_enable(). * * * linfree() - Destructor for the linprm struct * -------------------------------------------- * linfree() frees memory allocated for the linprm arrays by linini() and/or * linset(). linini() keeps a record of the memory it allocates and linfree() * will only attempt to free this. * * PLEASE NOTE: linfree() must not be invoked on a linprm struct that was not * initialized by linini(). * * Given: * lin struct linprm* * Linear transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * * * linprt() - Print routine for the linprm struct * ---------------------------------------------- * linprt() prints the contents of a linprm struct using wcsprintf(). Mainly * intended for diagnostic purposes. * * Given: * lin const struct linprm* * Linear transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * * * linset() - Setup routine for the linprm struct * ---------------------------------------------- * linset(), if necessary, allocates memory for the linprm::piximg and * linprm::imgpix arrays and sets up the linprm struct according to information * supplied within it - refer to the explanation of linprm::flag. * * Note that this routine need not be called directly; it will be invoked by * linp2x() and linx2p() if the linprm::flag is anything other than a * predefined magic value. * * Given and returned: * lin struct linprm* * Linear transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * 2: Memory allocation failed. * 3: PCi_ja matrix is singular. * * For returns > 1, a detailed error message is set in * linprm::err if enabled, see wcserr_enable(). * * * linp2x() - Pixel-to-world linear transformation * ----------------------------------------------- * linp2x() transforms pixel coordinates to intermediate world coordinates. * * Given and returned: * lin struct linprm* * Linear transformation parameters. * * Given: * ncoord, * nelem int The number of coordinates, each of vector length nelem * but containing lin.naxis coordinate elements. * * pixcrd const double[ncoord][nelem] * Array of pixel coordinates. * * Returned: * imgcrd double[ncoord][nelem] * Array of intermediate world coordinates. * * Function return value: * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * 2: Memory allocation failed. * 3: PCi_ja matrix is singular. * * For returns > 1, a detailed error message is set in * linprm::err if enabled, see wcserr_enable(). * * * linx2p() - World-to-pixel linear transformation * ----------------------------------------------- * linx2p() transforms intermediate world coordinates to pixel coordinates. * * Given and returned: * lin struct linprm* * Linear transformation parameters. * * Given: * ncoord, * nelem int The number of coordinates, each of vector length nelem * but containing lin.naxis coordinate elements. * * imgcrd const double[ncoord][nelem] * Array of intermediate world coordinates. * * Returned: * pixcrd double[ncoord][nelem] * Array of pixel coordinates. * * int Status return value: * 0: Success. * 1: Null linprm pointer passed. * 2: Memory allocation failed. * 3: PCi_ja matrix is singular. * * For returns > 1, a detailed error message is set in * linprm::err if enabled, see wcserr_enable(). * * * linprm struct - Linear transformation parameters * ------------------------------------------------ * The linprm struct contains all of the information required to perform a * linear transformation. It consists of certain members that must be set by * the user ("given") and others that are set by the WCSLIB routines * ("returned"). * * int flag * (Given and returned) This flag must be set to zero whenever any of the * following members of the linprm struct are set or modified: * * - linprm::naxis (q.v., not normally set by the user), * - linprm::pc, * - linprm::cdelt. * * This signals the initialization routine, linset(), to recompute the * returned members of the linprm struct. linset() will reset flag to * indicate that this has been done. * * PLEASE NOTE: flag should be set to -1 when linini() is called for the * first time for a particular linprm struct in order to initialize memory * management. It must ONLY be used on the first initialization otherwise * memory leaks may result. * * int naxis * (Given or returned) Number of pixel and world coordinate elements. * * If linini() is used to initialize the linprm struct (as would normally * be the case) then it will set naxis from the value passed to it as a * function argument. The user should not subsequently modify it. * * double *crpix * (Given) Pointer to the first element of an array of double containing * the coordinate reference pixel, CRPIXja. * * double *pc * (Given) Pointer to the first element of the PCi_ja (pixel coordinate) * transformation matrix. The expected order is * = struct linprm lin; = lin.pc = {PC1_1, PC1_2, PC2_1, PC2_2}; * * This may be constructed conveniently from a 2-D array via * = double m[2][2] = {{PC1_1, PC1_2}, = {PC2_1, PC2_2}}; * * which is equivalent to * = double m[2][2]; = m[0][0] = PC1_1; = m[0][1] = PC1_2; = m[1][0] = PC2_1; = m[1][1] = PC2_2; * * The storage order for this 2-D array is the same as for the 1-D array, * whence * = lin.pc = *m; * * would be legitimate. * * double *cdelt * (Given) Pointer to the first element of an array of double containing * the coordinate increments, CDELTia. * * int unity * (Returned) True if the linear transformation matrix is unity. * * int padding * (An unused variable inserted for alignment purposes only.) * * double *piximg * (Returned) Pointer to the first element of the matrix containing the * product of the CDELTia diagonal matrix and the PCi_ja matrix. * * double *imgpix * (Returned) Pointer to the first element of the inverse of the * linprm::piximg matrix. * * struct wcserr *err * (Returned) If enabled, when an error status is returned this struct * contains detailed information about the error, see wcserr_enable(). * * int i_naxis * (For internal use only.) * int m_flag * (For internal use only.) * int m_naxis * (For internal use only.) * int m_padding * (For internal use only.) * double *m_crpix * (For internal use only.) * double *m_pc * (For internal use only.) * double *m_cdelt * (For internal use only.) * void *padding2 * (For internal use only.) * * * Global variable: const char *lin_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_LIN #define WCSLIB_LIN #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif extern const char *lin_errmsg[]; enum lin_errmsg_enum { LINERR_SUCCESS = 0, /* Success. */ LINERR_NULL_POINTER = 1, /* Null linprm pointer passed. */ LINERR_MEMORY = 2, /* Memory allocation failed. */ LINERR_SINGULAR_MTX = 3 /* PCi_ja matrix is singular. */ }; struct linprm { /* Initialization flag (see the prologue above). */ /*------------------------------------------------------------------------*/ int flag; /* Set to zero to force initialization. */ /* Parameters to be provided (see the prologue above). */ /*------------------------------------------------------------------------*/ int naxis; /* The number of axes, given by NAXIS. */ double *crpix; /* CRPIXja keywords for each pixel axis. */ double *pc; /* PCi_ja linear transformation matrix. */ double *cdelt; /* CDELTia keywords for each coord axis. */ /* Information derived from the parameters supplied. */ /*------------------------------------------------------------------------*/ double *piximg; /* Product of CDELTia and PCi_ja matrices. */ double *imgpix; /* Inverse of the piximg matrix. */ int unity; /* True if the PCi_ja matrix is unity. */ /* Error handling */ /*------------------------------------------------------------------------*/ int padding; /* (Dummy inserted for alignment purposes.) */ struct wcserr *err; /* Private - the remainder are for memory management. */ /*------------------------------------------------------------------------*/ int i_naxis; int m_flag, m_naxis, m_padding; double *m_crpix, *m_pc, *m_cdelt; void *padding2; }; /* Size of the linprm struct in int units, used by the Fortran wrappers. */ #define LINLEN (sizeof(struct linprm)/sizeof(int)) int linini(int alloc, int naxis, struct linprm *lin); int lincpy(int alloc, const struct linprm *linsrc, struct linprm *lindst); int linfree(struct linprm *lin); int linprt(const struct linprm *lin); int linset(struct linprm *lin); int linp2x(struct linprm *lin, int ncoord, int nelem, const double pixcrd[], double imgcrd[]); int linx2p(struct linprm *lin, int ncoord, int nelem, const double imgcrd[], double pixcrd[]); int matinv(int n, const double mat[], double inv[]); /* Deprecated. */ #define linini_errmsg lin_errmsg #define lincpy_errmsg lin_errmsg #define linfree_errmsg lin_errmsg #define linprt_errmsg lin_errmsg #define linset_errmsg lin_errmsg #define linp2x_errmsg lin_errmsg #define linx2p_errmsg lin_errmsg #ifdef __cplusplus } #endif #endif /* WCSLIB_LIN */ pywcs-1.12/wcslib/C/log.c0000644001153600020070000000552612310355626017250 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: log.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include "log.h" /* Map status return value to message. */ const char *log_errmsg[] = { "Success", "", "Invalid log-coordinate reference value", "One or more of the x coordinates were invalid", "One or more of the world coordinates were invalid"}; /*--------------------------------------------------------------------------*/ int logx2s( double crval, int nx, int sx, int slogc, const double x[], double logc[], int stat[]) { register int ix; register int *statp; register const double *xp; register double *logcp; if (crval <= 0.0) { return LOGERR_BAD_LOG_REF_VAL; } xp = x; logcp = logc; statp = stat; for (ix = 0; ix < nx; ix++, xp += sx, logcp += slogc) { *logcp = crval * exp((*xp) / crval); *(statp++) = 0; } return 0; } /*--------------------------------------------------------------------------*/ int logs2x( double crval, int nlogc, int slogc, int sx, const double logc[], double x[], int stat[]) { int status; register int ilogc; register int *statp; register const double *logcp; register double *xp; if (crval <= 0.0) { return LOGERR_BAD_LOG_REF_VAL; } xp = x; logcp = logc; statp = stat; status = 0; for (ilogc = 0; ilogc < nlogc; ilogc++, logcp += slogc, xp += sx) { if (*logcp > 0.0) { *xp = crval * log(*logcp / crval); *(statp++) = 0; } else { *(statp++) = 1; status = LOGERR_BAD_WORLD; } } return status; } pywcs-1.12/wcslib/C/log.h0000644001153600020070000001351112310355626017246 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: log.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement logarithmic coordinate systems as * defined by the FITS World Coordinate System (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the log routines * --------------------------- * These routines implement the part of the FITS WCS standard that deals with * logarithmic coordinates. They define methods to be used for computing * logarithmic world coordinates from intermediate world coordinates (a linear * transformation of image pixel coordinates), and vice versa. * * logx2s() and logs2x() implement the WCS logarithmic coordinate * transformations. * * Argument checking: * ------------------ * The input log-coordinate values are only checked for values that would * result in floating point exceptions and the same is true for the * log-coordinate reference value. * * Accuracy: * --------- * No warranty is given for the accuracy of these routines (refer to the * copyright notice); intending users must satisfy for themselves their * adequacy for the intended purpose. However, closure effectively to within * double precision rounding error was demonstrated by test routine tlog.c * which accompanies this software. * * * logx2s() - Transform to logarithmic coordinates * ----------------------------------------------- * logx2s() transforms intermediate world coordinates to logarithmic * coordinates. * * Given and returned: * crval double Log-coordinate reference value (CRVALia). * * Given: * nx int Vector length. * * sx int Vector stride. * * slogc int Vector stride. * * x const double[] * Intermediate world coordinates, in SI units. * * Returned: * logc double[] Logarithmic coordinates, in SI units. * * stat int[] Status return value status for each vector element: * 0: Success. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid log-coordinate reference value. * * * logs2x() - Transform logarithmic coordinates * -------------------------------------------- * logs2x() transforms logarithmic world coordinates to intermediate world * coordinates. * * Given and returned: * crval double Log-coordinate reference value (CRVALia). * * Given: * nlogc int Vector length. * * slogc int Vector stride. * * sx int Vector stride. * * logc const double[] * Logarithmic coordinates, in SI units. * * Returned: * x double[] Intermediate world coordinates, in SI units. * * stat int[] Status return value status for each vector element: * 0: Success. * 1: Invalid value of logc. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid log-coordinate reference value. * 4: One or more of the world-coordinate values * are incorrect, as indicated by the stat vector. * * * Global variable: const char *log_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_LOG #define WCSLIB_LOG #ifdef __cplusplus extern "C" { #endif extern const char *log_errmsg[]; enum log_errmsg_enum { LOGERR_SUCCESS = 0, /* Success. */ LOGERR_NULL_POINTER = 1, /* Null pointer passed. */ LOGERR_BAD_LOG_REF_VAL = 2, /* Invalid log-coordinate reference value. */ LOGERR_BAD_X = 3, /* One or more of the x coordinates were invalid. */ LOGERR_BAD_WORLD = 4 /* One or more of the world coordinates were invalid. */ }; int logx2s(double crval, int nx, int sx, int slogc, const double x[], double logc[], int stat[]); int logs2x(double crval, int nlogc, int slogc, int sx, const double logc[], double x[], int stat[]); #ifdef __cplusplus } #endif #endif /* WCSLIB_LOG */ pywcs-1.12/wcslib/C/prj.c0000644001153600020070000052601612310355626017264 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: prj.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsprintf.h" #include "wcstrig.h" #include "wcsutil.h" #include "prj.h" /* Projection categories. */ const int ZENITHAL = 1; const int CYLINDRICAL = 2; const int PSEUDOCYLINDRICAL = 3; const int CONVENTIONAL = 4; const int CONIC = 5; const int POLYCONIC = 6; const int QUADCUBE = 7; const int HEALPIX = 8; const char prj_categories[9][32] = {"undefined", "zenithal", "cylindrical", "pseudocylindrical", "conventional", "conic", "polyconic", "quadcube", "HEALPix"}; /* Projection codes. */ const int prj_ncode = 27; const char prj_codes[27][4] = {"AZP", "SZP", "TAN", "STG", "SIN", "ARC", "ZPN", "ZEA", "AIR", "CYP", "CEA", "CAR", "MER", "COP", "COE", "COD", "COO", "SFL", "PAR", "MOL", "AIT", "BON", "PCO", "TSC", "CSC", "QSC", "HPX"}; const int AZP = 101; const int SZP = 102; const int TAN = 103; const int STG = 104; const int SIN = 105; const int ARC = 106; const int ZPN = 107; const int ZEA = 108; const int AIR = 109; const int CYP = 201; const int CEA = 202; const int CAR = 203; const int MER = 204; const int SFL = 301; const int PAR = 302; const int MOL = 303; const int AIT = 401; const int COP = 501; const int COE = 502; const int COD = 503; const int COO = 504; const int BON = 601; const int PCO = 602; const int TSC = 701; const int CSC = 702; const int QSC = 703; const int HPX = 801; /* Map status return value to message. */ const char *prj_errmsg[] = { "Success", "Null prjprm pointer passed", "Invalid projection parameters", "One or more of the (x,y) coordinates were invalid", "One or more of the (phi,theta) coordinates were invalid"}; /* Convenience macros for generating common error messages. */ #define PRJERR_BAD_PARAM_SET(function) \ wcserr_set(&(prj->err), PRJERR_BAD_PARAM, function, __FILE__, __LINE__, \ "Invalid parameters for %s projection", prj->name); #define PRJERR_BAD_PIX_SET(function) \ wcserr_set(&(prj->err), PRJERR_BAD_PIX, function, __FILE__, __LINE__, \ "One or more of the (x, y) coordinates were invalid for %s projection", \ prj->name); #define PRJERR_BAD_WORLD_SET(function) \ wcserr_set(&(prj->err), PRJERR_BAD_WORLD, function, __FILE__, __LINE__, \ "One or more of the (lat, lng) coordinates were invalid for " \ "%s projection", prj->name); #define copysign(X, Y) ((Y) < 0.0 ? -fabs(X) : fabs(X)) /*============================================================================ * Generic routines. * * prjini initializes a prjprm struct to default values. * * prjprt prints the contents of a prjprm struct. * * prjset invokes the specific initialization routine based on the projection * code in the prjprm struct. * * prjx2s invokes the specific deprojection routine based on the pointer-to- * function stored in the prjprm struct. * * prjs2x invokes the specific projection routine based on the pointer-to- * function stored in the prjprm struct. * *---------------------------------------------------------------------------*/ int prjini(prj) struct prjprm *prj; { register int k; if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = 0; strcpy(prj->code, " "); prj->pv[0] = 0.0; prj->pv[1] = UNDEFINED; prj->pv[2] = UNDEFINED; prj->pv[3] = UNDEFINED; for (k = 4; k < PVN; prj->pv[k++] = 0.0); prj->r0 = 0.0; prj->phi0 = UNDEFINED; prj->theta0 = UNDEFINED; prj->bounds = 1; strcpy(prj->name, "undefined"); for (k = 9; k < 40; prj->name[k++] = '\0'); prj->category = 0; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = 0; prj->x0 = 0.0; prj->y0 = 0.0; for (k = 0; k < 10; prj->w[k++] = 0.0); prj->m = 0; prj->n = 0; prj->err = 0x0; return 0; } /*--------------------------------------------------------------------------*/ int prjfree(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->err) free(prj->err); prj->err = 0x0; return 0; } /*--------------------------------------------------------------------------*/ int prjprt(prj) const struct prjprm *prj; { char hext[32]; int i, n; if (prj == 0x0) return PRJERR_NULL_POINTER; wcsprintf(" flag: %d\n", prj->flag); wcsprintf(" code: \"%s\"\n", prj->code); wcsprintf(" r0: %9f\n", prj->r0); wcsprintf(" pv:"); if (prj->pvrange) { n = (prj->pvrange)%100; if (prj->pvrange/100) { wcsprintf(" (0)"); } else { wcsprintf(" %- 11.5g", prj->pv[0]); n--; } for (i = 1; i <= n; i++) { if (i%5 == 1) { wcsprintf("\n "); } if (undefined(prj->pv[i])) { wcsprintf(" UNDEFINED "); } else { wcsprintf(" %- 11.5g", prj->pv[i]); } } wcsprintf("\n"); } else { wcsprintf(" (not used)\n"); } if (undefined(prj->phi0)) { wcsprintf(" phi0: UNDEFINED\n"); } else { wcsprintf(" phi0: %9f\n", prj->phi0); } if (undefined(prj->theta0)) { wcsprintf(" theta0: UNDEFINED\n"); } else { wcsprintf(" theta0: %9f\n", prj->theta0); } wcsprintf(" bounds: %d\n", prj->bounds); wcsprintf("\n"); wcsprintf(" name: \"%s\"\n", prj->name); wcsprintf(" category: %d (%s)\n", prj->category, prj_categories[prj->category]); wcsprintf(" pvrange: %d\n", prj->pvrange); wcsprintf(" simplezen: %d\n", prj->simplezen); wcsprintf(" equiareal: %d\n", prj->equiareal); wcsprintf(" conformal: %d\n", prj->conformal); wcsprintf(" global: %d\n", prj->global); wcsprintf(" divergent: %d\n", prj->divergent); wcsprintf(" x0: %f\n", prj->x0); wcsprintf(" y0: %f\n", prj->y0); WCSPRINTF_PTR(" err: ", prj->err, "\n"); if (prj->err) { wcserr_prt(prj->err, " "); } wcsprintf(" w[]:"); for (i = 0; i < 5; i++) { wcsprintf(" %- 11.5g", prj->w[i]); } wcsprintf("\n "); for (i = 5; i < 10; i++) { wcsprintf(" %- 11.5g", prj->w[i]); } wcsprintf("\n"); wcsprintf(" m: %d\n", prj->m); wcsprintf(" n: %d\n", prj->n); wcsprintf(" prjx2s: %s\n", wcsutil_fptr2str((int (*)())prj->prjx2s, hext)); wcsprintf(" prjs2x: %s\n", wcsutil_fptr2str((int (*)())prj->prjs2x, hext)); return 0; } /*--------------------------------------------------------------------------*/ int prjset(prj) struct prjprm *prj; { static const char *function = "prjset"; int status; struct wcserr **err; if (prj == 0x0) return PRJERR_NULL_POINTER; err = &(prj->err); /* Invoke the relevant initialization routine. */ prj->code[3] = '\0'; if (strcmp(prj->code, "AZP") == 0) { status = azpset(prj); } else if (strcmp(prj->code, "SZP") == 0) { status = szpset(prj); } else if (strcmp(prj->code, "TAN") == 0) { status = tanset(prj); } else if (strcmp(prj->code, "STG") == 0) { status = stgset(prj); } else if (strcmp(prj->code, "SIN") == 0) { status = sinset(prj); } else if (strcmp(prj->code, "ARC") == 0) { status = arcset(prj); } else if (strcmp(prj->code, "ZPN") == 0) { status = zpnset(prj); } else if (strcmp(prj->code, "ZEA") == 0) { status = zeaset(prj); } else if (strcmp(prj->code, "AIR") == 0) { status = airset(prj); } else if (strcmp(prj->code, "CYP") == 0) { status = cypset(prj); } else if (strcmp(prj->code, "CEA") == 0) { status = ceaset(prj); } else if (strcmp(prj->code, "CAR") == 0) { status = carset(prj); } else if (strcmp(prj->code, "MER") == 0) { status = merset(prj); } else if (strcmp(prj->code, "SFL") == 0) { status = sflset(prj); } else if (strcmp(prj->code, "PAR") == 0) { status = parset(prj); } else if (strcmp(prj->code, "MOL") == 0) { status = molset(prj); } else if (strcmp(prj->code, "AIT") == 0) { status = aitset(prj); } else if (strcmp(prj->code, "COP") == 0) { status = copset(prj); } else if (strcmp(prj->code, "COE") == 0) { status = coeset(prj); } else if (strcmp(prj->code, "COD") == 0) { status = codset(prj); } else if (strcmp(prj->code, "COO") == 0) { status = cooset(prj); } else if (strcmp(prj->code, "BON") == 0) { status = bonset(prj); } else if (strcmp(prj->code, "PCO") == 0) { status = pcoset(prj); } else if (strcmp(prj->code, "TSC") == 0) { status = tscset(prj); } else if (strcmp(prj->code, "CSC") == 0) { status = cscset(prj); } else if (strcmp(prj->code, "QSC") == 0) { status = qscset(prj); } else if (strcmp(prj->code, "HPX") == 0) { status = hpxset(prj); } else { /* Unrecognized projection code. */ status = wcserr_set(WCSERR_SET(PRJERR_BAD_PARAM), "Unrecognized projection code '%s'", prj->code); } return status; } /*--------------------------------------------------------------------------*/ int prjx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int status; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag == 0) { if ((status = prjset(prj))) return status; } return prj->prjx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat); } /*--------------------------------------------------------------------------*/ int prjs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int status; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag == 0) { if ((status = prjset(prj))) return status; } return prj->prjs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat); } /*============================================================================ * Internal helper routine used by the *set() routines that forces * (x,y) = (0,0) at (phi0,theta0). *---------------------------------------------------------------------------*/ int prjoff(prj, phi0, theta0) struct prjprm *prj; const double phi0, theta0; { int stat; double x0, y0; if (prj == 0x0) return PRJERR_NULL_POINTER; prj->x0 = 0.0; prj->y0 = 0.0; if (undefined(prj->phi0) || undefined(prj->theta0)) { /* Set both to the projection-specific default if either undefined. */ prj->phi0 = phi0; prj->theta0 = theta0; } else { if (prj->prjs2x(prj, 1, 1, 1, 1, &(prj->phi0), &(prj->theta0), &x0, &y0, &stat)) { return PRJERR_BAD_PARAM_SET("prjoff"); } prj->x0 = x0; prj->y0 = y0; } return 0; } /*============================================================================ * AZP: zenithal/azimuthal perspective projection. * * Given: * prj->pv[1] Distance parameter, mu in units of r0. * prj->pv[2] Tilt angle, gamma in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag AZP * prj->code "AZP" * prj->x0 Offset in x. * prj->y0 Offset in y. * prj->w[0] r0*(mu+1) * prj->w[1] tan(gamma) * prj->w[2] sec(gamma) * prj->w[3] cos(gamma) * prj->w[4] sin(gamma) * prj->w[5] asin(-1/mu) for |mu| >= 1, -90 otherwise * prj->w[6] mu*cos(gamma) * prj->w[7] 1 if |mu*cos(gamma)| < 1, 0 otherwise * prj->prjx2s Pointer to azpx2s(). * prj->prjs2x Pointer to azps2x(). *===========================================================================*/ int azpset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = AZP; strcpy(prj->code, "AZP"); if (undefined(prj->pv[1])) prj->pv[1] = 0.0; if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "zenithal/azimuthal perspective"); prj->category = ZENITHAL; prj->pvrange = 102; prj->simplezen = prj->pv[2] == 0.0; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = prj->pv[1] <= 1.0; prj->w[0] = prj->r0*(prj->pv[1] + 1.0); if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("azpset"); } prj->w[3] = cosd(prj->pv[2]); if (prj->w[3] == 0.0) { return PRJERR_BAD_PARAM_SET("azpset"); } prj->w[2] = 1.0/prj->w[3]; prj->w[4] = sind(prj->pv[2]); prj->w[1] = prj->w[4] / prj->w[3]; if (fabs(prj->pv[1]) > 1.0) { prj->w[5] = asind(-1.0/prj->pv[1]); } else { prj->w[5] = -90.0; } prj->w[6] = prj->pv[1] * prj->w[3]; prj->w[7] = (fabs(prj->w[6]) < 1.0) ? 1.0 : 0.0; prj->prjx2s = azpx2s; prj->prjs2x = azps2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int azpx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double a, b, q, r, s, t, xj, yj, yc, yc2; const double tol = 1.0e-13; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != AZP) { if ((status = azpset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yc = yj*prj->w[3]; yc2 = yc*yc; q = prj->w[0] + yj*prj->w[4]; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yc2); if (r == 0.0) { *phip = 0.0; *thetap = 90.0; *(statp++) = 0; } else { *phip = atan2d(xj, -yc); s = r / q; t = s*prj->pv[1]/sqrt(s*s + 1.0); s = atan2d(1.0, s); if (fabs(t) > 1.0) { if (fabs(t) > 1.0+tol) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("azpx2s"); continue; } t = copysign(90.0, t); } else { t = asind(t); } a = s - t; b = s + t + 180.0; if (a > 90.0) a -= 360.0; if (b > 90.0) b -= 360.0; *thetap = (a > b) ? a : b; *(statp++) = 0; } } } return status; } /*--------------------------------------------------------------------------*/ int azps2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double a, b, cosphi, costhe, r, s, sinphi, sinthe, t; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != AZP) { if ((status = azpset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sincosd(*thetap, &sinthe, &costhe); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { s = prj->w[1]*(*yp); t = (prj->pv[1] + sinthe) + costhe*s; if (t == 0.0) { *xp = 0.0; *yp = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_WORLD_SET("azps2x"); } else { r = prj->w[0]*costhe/t; /* Bounds checking. */ istat = 0; if (prj->bounds) { if (*thetap < prj->w[5]) { /* Overlap. */ istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("azps2x"); } else if (prj->w[7] > 0.0) { /* Divergence. */ t = prj->pv[1] / sqrt(1.0 + s*s); if (fabs(t) <= 1.0) { s = atand(-s); t = asind(t); a = s - t; b = s + t + 180.0; if (a > 90.0) a -= 360.0; if (b > 90.0) b -= 360.0; if (*thetap < ((a > b) ? a : b)) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("azps2x"); } } } } *xp = r*(*xp) - prj->x0; *yp = -r*(*yp)*prj->w[2] - prj->y0; *(statp++) = istat; } } } return status; } /*============================================================================ * SZP: slant zenithal perspective projection. * * Given: * prj->pv[1] Distance of the point of projection from the centre of the * generating sphere, mu in units of r0. * prj->pv[2] Native longitude, phi_c, and ... * prj->pv[3] Native latitude, theta_c, on the planewards side of the * intersection of the line through the point of projection * and the centre of the generating sphere, phi_c in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag SZP * prj->code "SZP" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] 1/r0 * prj->w[1] xp = -mu*cos(theta_c)*sin(phi_c) * prj->w[2] yp = mu*cos(theta_c)*cos(phi_c) * prj->w[3] zp = mu*sin(theta_c) + 1 * prj->w[4] r0*xp * prj->w[5] r0*yp * prj->w[6] r0*zp * prj->w[7] (zp - 1)^2 * prj->w[8] asin(1-zp) if |1 - zp| < 1, -90 otherwise * prj->prjx2s Pointer to szpx2s(). * prj->prjs2x Pointer to szps2x(). *===========================================================================*/ int szpset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = SZP; strcpy(prj->code, "SZP"); if (undefined(prj->pv[1])) prj->pv[1] = 0.0; if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (undefined(prj->pv[3])) prj->pv[3] = 90.0; if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "slant zenithal perspective"); prj->category = ZENITHAL; prj->pvrange = 103; prj->simplezen = prj->pv[3] == 90.0; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = prj->pv[1] <= 1.0; prj->w[0] = 1.0/prj->r0; prj->w[3] = prj->pv[1] * sind(prj->pv[3]) + 1.0; if (prj->w[3] == 0.0) { return PRJERR_BAD_PARAM_SET("szpset"); } prj->w[1] = -prj->pv[1] * cosd(prj->pv[3]) * sind(prj->pv[2]); prj->w[2] = prj->pv[1] * cosd(prj->pv[3]) * cosd(prj->pv[2]); prj->w[4] = prj->r0 * prj->w[1]; prj->w[5] = prj->r0 * prj->w[2]; prj->w[6] = prj->r0 * prj->w[3]; prj->w[7] = (prj->w[3] - 1.0) * prj->w[3] - 1.0; if (fabs(prj->w[3] - 1.0) < 1.0) { prj->w[8] = asind(1.0 - prj->w[3]); } else { prj->w[8] = -90.0; } prj->prjx2s = szpx2s; prj->prjs2x = szps2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int szpx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double a, b, c, d, r2, sinth1, sinth2, sinthe, t, x1, xr, xy, y1, yr, z; const double tol = 1.0e-13; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != SZP) { if ((status = szpset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xr = (*xp + prj->x0)*prj->w[0]; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xr; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yr = (*yp + prj->y0)*prj->w[0]; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xr = *phip; r2 = xr*xr + yr*yr; x1 = (xr - prj->w[1])/prj->w[3]; y1 = (yr - prj->w[2])/prj->w[3]; xy = xr*x1 + yr*y1; if (r2 < 1.0e-10) { /* Use small angle formula. */ z = r2/2.0; *thetap = 90.0 - R2D*sqrt(r2/(1.0 + xy)); } else { t = x1*x1 + y1*y1; a = t + 1.0; b = xy - t; c = r2 - xy - xy + t - 1.0; d = b*b - a*c; /* Check for a solution. */ if (d < 0.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("szpx2s"); continue; } d = sqrt(d); /* Choose solution closest to pole. */ sinth1 = (-b + d)/a; sinth2 = (-b - d)/a; sinthe = (sinth1 > sinth2) ? sinth1 : sinth2; if (sinthe > 1.0) { if (sinthe-1.0 < tol) { sinthe = 1.0; } else { sinthe = (sinth1 < sinth2) ? sinth1 : sinth2; } } if (sinthe < -1.0) { if (sinthe+1.0 > -tol) { sinthe = -1.0; } } if (sinthe > 1.0 || sinthe < -1.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("szpx2s"); continue; } *thetap = asind(sinthe); z = 1.0 - sinthe; } *phip = atan2d(xr - x1*z, -(yr - y1*z)); *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int szps2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double a, b, cosphi, r, s, sinphi, t, u, v; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != SZP) { if ((status = szpset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { s = 1.0 - sind(*thetap); t = prj->w[3] - s; if (t == 0.0) { for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = 0.0; *yp = 0.0; *(statp++) = 1; } if (!status) status = PRJERR_BAD_WORLD_SET("szps2x"); } else { r = prj->w[6]*cosd(*thetap)/t; u = prj->w[4]*s/t + prj->x0; v = prj->w[5]*s/t + prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { /* Bounds checking. */ istat = 0; if (prj->bounds) { if (*thetap < prj->w[8]) { /* Divergence. */ istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("szps2x"); } else if (fabs(prj->pv[1]) > 1.0) { /* Overlap. */ s = prj->w[1]*(*xp) - prj->w[2]*(*yp); t = 1.0/sqrt(prj->w[7] + s*s); if (fabs(t) <= 1.0) { s = atan2d(s, prj->w[3] - 1.0); t = asind(t); a = s - t; b = s + t + 180.0; if (a > 90.0) a -= 360.0; if (b > 90.0) b -= 360.0; if (*thetap < ((a > b) ? a : b)) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("szps2x"); } } } } *xp = r*(*xp) - u; *yp = -r*(*yp) - v; *(statp++) = istat; } } } return status; } /*============================================================================ * TAN: gnomonic projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag TAN * prj->code "TAN" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->prjx2s Pointer to tanx2s(). * prj->prjs2x Pointer to tans2x(). *===========================================================================*/ int tanset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = TAN; strcpy(prj->code, "TAN"); if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "gnomonic"); prj->category = ZENITHAL; prj->pvrange = 0; prj->simplezen = 1; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = 1; prj->prjx2s = tanx2s; prj->prjs2x = tans2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int tanx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double r, xj, yj, yj2; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != TAN) { if ((status = tanset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yj2); if (r == 0.0) { *phip = 0.0; } else { *phip = atan2d(xj, -yj); } *thetap = atan2d(prj->r0, r); *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int tans2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, r, s, sinphi; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != TAN) { if ((status = tanset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { s = sind(*thetap); if (s == 0.0) { for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = 0.0; *yp = 0.0; *(statp++) = 1; } if (!status) status = PRJERR_BAD_WORLD_SET("tans2x"); } else { r = prj->r0*cosd(*thetap)/s; istat = 0; if (prj->bounds && s < 0.0) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("tans2x"); } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = istat; } } } return status; } /*============================================================================ * STG: stereographic projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag STG * prj->code "STG" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] 2*r0 * prj->w[1] 1/(2*r0) * prj->prjx2s Pointer to stgx2s(). * prj->prjs2x Pointer to stgs2x(). *===========================================================================*/ int stgset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = STG; strcpy(prj->code, "STG"); strcpy(prj->name, "stereographic"); prj->category = ZENITHAL; prj->pvrange = 0; prj->simplezen = 1; prj->equiareal = 0; prj->conformal = 1; prj->global = 0; prj->divergent = 1; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 360.0/PI; prj->w[1] = PI/360.0; } else { prj->w[0] = 2.0*prj->r0; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = stgx2s; prj->prjs2x = stgs2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int stgx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double r, xj, yj, yj2; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != STG) { if ((status = stgset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yj2); if (r == 0.0) { *phip = 0.0; } else { *phip = atan2d(xj, -yj); } *thetap = 90.0 - 2.0*atand(r*prj->w[1]); *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int stgs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, r, s, sinphi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != STG) { if ((status = stgset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { s = 1.0 + sind(*thetap); if (s == 0.0) { for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = 0.0; *yp = 0.0; *(statp++) = 1; } if (!status) status = PRJERR_BAD_WORLD_SET("stgs2x"); } else { r = prj->w[0]*cosd(*thetap)/s; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = 0; } } } return status; } /*============================================================================ * SIN: orthographic/synthesis projection. * * Given: * prj->pv[1:2] Obliqueness parameters, xi and eta. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag SIN * prj->code "SIN" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] 1/r0 * prj->w[1] xi**2 + eta**2 * prj->w[2] xi**2 + eta**2 + 1 * prj->w[3] xi**2 + eta**2 - 1 * prj->prjx2s Pointer to sinx2s(). * prj->prjs2x Pointer to sins2x(). *===========================================================================*/ int sinset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = SIN; strcpy(prj->code, "SIN"); if (undefined(prj->pv[1])) prj->pv[1] = 0.0; if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "orthographic/synthesis"); prj->category = ZENITHAL; prj->pvrange = 102; prj->simplezen = (prj->pv[1] == 0.0 && prj->pv[2] == 0.0); prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = 0; prj->w[0] = 1.0/prj->r0; prj->w[1] = prj->pv[1]*prj->pv[1] + prj->pv[2]*prj->pv[2]; prj->w[2] = prj->w[1] + 1.0; prj->w[3] = prj->w[1] - 1.0; prj->prjx2s = sinx2s; prj->prjs2x = sins2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int sinx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; const double tol = 1.0e-13; double a, b, c, d, eta, r2, sinth1, sinth2, sinthe, x0, xi, x1, xy, y0, y02, y1, z; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != SIN) { if ((status = sinset(prj))) return status; } xi = prj->pv[1]; eta = prj->pv[2]; if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { x0 = (*xp + prj->x0)*prj->w[0]; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = x0; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { y0 = (*yp + prj->y0)*prj->w[0]; y02 = y0*y0; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { /* Compute intermediaries. */ x0 = *phip; r2 = x0*x0 + y02; if (prj->w[1] == 0.0) { /* Orthographic projection. */ if (r2 != 0.0) { *phip = atan2d(x0, -y0); } else { *phip = 0.0; } if (r2 < 0.5) { *thetap = acosd(sqrt(r2)); } else if (r2 <= 1.0) { *thetap = asind(sqrt(1.0 - r2)); } else { *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("sinx2s") continue; } } else { /* "Synthesis" projection. */ xy = x0*xi + y0*eta; if (r2 < 1.0e-10) { /* Use small angle formula. */ z = r2/2.0; *thetap = 90.0 - R2D*sqrt(r2/(1.0 + xy)); } else { a = prj->w[2]; b = xy - prj->w[1]; c = r2 - xy - xy + prj->w[3]; d = b*b - a*c; /* Check for a solution. */ if (d < 0.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("sinx2s") continue; } d = sqrt(d); /* Choose solution closest to pole. */ sinth1 = (-b + d)/a; sinth2 = (-b - d)/a; sinthe = (sinth1 > sinth2) ? sinth1 : sinth2; if (sinthe > 1.0) { if (sinthe-1.0 < tol) { sinthe = 1.0; } else { sinthe = (sinth1 < sinth2) ? sinth1 : sinth2; } } if (sinthe < -1.0) { if (sinthe+1.0 > -tol) { sinthe = -1.0; } } if (sinthe > 1.0 || sinthe < -1.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("sinx2s") continue; } *thetap = asind(sinthe); z = 1.0 - sinthe; } x1 = -y0 + eta*z; y1 = x0 - xi*z; if (x1 == 0.0 && y1 == 0.0) { *phip = 0.0; } else { *phip = atan2d(y1,x1); } } *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int sins2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, costhe, sinphi, r, t, z, z1, z2; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != SIN) { if ((status = sinset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { t = (90.0 - fabs(*thetap))*D2R; if (t < 1.0e-5) { if (*thetap > 0.0) { z = t*t/2.0; } else { z = 2.0 - t*t/2.0; } costhe = t; } else { z = 1.0 - sind(*thetap); costhe = cosd(*thetap); } r = prj->r0*costhe; if (prj->w[1] == 0.0) { /* Orthographic projection. */ istat = 0; if (prj->bounds && *thetap < 0.0) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("sins2x"); } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = istat; } } else { /* "Synthesis" projection. */ z *= prj->r0; z1 = prj->pv[1]*z - prj->x0; z2 = prj->pv[2]*z - prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { istat = 0; if (prj->bounds) { t = -atand(prj->pv[1]*(*xp) - prj->pv[2]*(*yp)); if (*thetap < t) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("sins2x"); } } *xp = r*(*xp) + z1; *yp = -r*(*yp) + z2; *(statp++) = istat; } } } return status; } /*============================================================================ * ARC: zenithal/azimuthal equidistant projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag ARC * prj->code "ARC" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->prjx2s Pointer to arcx2s(). * prj->prjs2x Pointer to arcs2x(). *===========================================================================*/ int arcset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = ARC; strcpy(prj->code, "ARC"); strcpy(prj->name, "zenithal/azimuthal equidistant"); prj->category = ZENITHAL; prj->pvrange = 0; prj->simplezen = 1; prj->equiareal = 0; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = arcx2s; prj->prjs2x = arcs2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int arcx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double r, xj, yj, yj2; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != ARC) { if ((status = arcset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yj2); if (r == 0.0) { *phip = 0.0; *thetap = 90.0; } else { *phip = atan2d(xj, -yj); *thetap = 90.0 - r*prj->w[1]; } *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int arcs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, r, sinphi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != ARC) { if ((status = arcset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { r = prj->w[0]*(90.0 - *thetap); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = 0; } } return 0; } /*============================================================================ * ZPN: zenithal/azimuthal polynomial projection. * * Given: * prj->pv[] Polynomial coefficients. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag ZPN * prj->code "ZPN" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->n Degree of the polynomial, N. * prj->w[0] Co-latitude of the first point of inflection, radian. * prj->w[1] Radius of the first point of inflection (N > 1), radian. * prj->prjx2s Pointer to zpnx2s(). * prj->prjs2x Pointer to zpns2x(). *===========================================================================*/ int zpnset(prj) struct prjprm *prj; { int j, k, m; double d, d1, d2, r, zd, zd1, zd2; const double tol = 1.0e-13; if (prj == 0x0) return PRJERR_NULL_POINTER; strcpy(prj->code, "ZPN"); prj->flag = ZPN; if (undefined(prj->pv[1])) prj->pv[1] = 0.0; if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (undefined(prj->pv[3])) prj->pv[3] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "zenithal/azimuthal polynomial"); prj->category = ZENITHAL; prj->pvrange = 30; prj->simplezen = 1; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = 0; /* Find the highest non-zero coefficient. */ for (k = PVN-1; k >= 0 && prj->pv[k] == 0.0; k--); if (k < 0) { return PRJERR_BAD_PARAM_SET("zpnset"); } prj->n = k; if (k < 2) { /* No point of inflection. */ prj->w[0] = PI; } else { /* Find the point of inflection closest to the pole. */ zd1 = 0.0; d1 = prj->pv[1]; if (d1 <= 0.0) { return PRJERR_BAD_PARAM_SET("zpnset"); } /* Find the point where the derivative first goes negative. */ for (j = 0; j < 180; j++) { zd2 = j*D2R; d2 = 0.0; for (m = k; m > 0; m--) { d2 = d2*zd2 + m*prj->pv[m]; } if (d2 <= 0.0) break; zd1 = zd2; d1 = d2; } if (j == 180) { /* No negative derivative -> no point of inflection. */ zd = PI; prj->global = 1; } else { /* Find where the derivative is zero. */ for (j = 1; j <= 10; j++) { zd = zd1 - d1*(zd2-zd1)/(d2-d1); d = 0.0; for (m = k; m > 0; m--) { d = d*zd + m*prj->pv[m]; } if (fabs(d) < tol) break; if (d < 0.0) { zd2 = zd; d2 = d; } else { zd1 = zd; d1 = d; } } } r = 0.0; for (m = k; m >= 0; m--) { r = r*zd + prj->pv[m]; } prj->w[0] = zd; prj->w[1] = r; } prj->prjx2s = zpnx2s; prj->prjs2x = zpns2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int zpnx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int j, k, m, mx, my, rowlen, rowoff, status; double a, b, c, d, lambda, r, r1, r2, rt, xj, yj, yj2, zd, zd1, zd2; const double tol = 1.0e-13; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != ZPN) { if ((status = zpnset(prj))) return status; } k = prj->n; if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yj2)/prj->r0; if (r == 0.0) { *phip = 0.0; } else { *phip = atan2d(xj, -yj); } if (k < 1) { /* Constant - no solution. */ return PRJERR_BAD_PARAM_SET("zpnx2s"); } else if (k == 1) { /* Linear. */ zd = (r - prj->pv[0])/prj->pv[1]; } else if (k == 2) { /* Quadratic. */ a = prj->pv[2]; b = prj->pv[1]; c = prj->pv[0] - r; d = b*b - 4.0*a*c; if (d < 0.0) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("zpnx2s"); continue; } d = sqrt(d); /* Choose solution closest to pole. */ zd1 = (-b + d)/(2.0*a); zd2 = (-b - d)/(2.0*a); zd = (zd1zd2) ? zd1 : zd2; if (zd < 0.0) { if (zd < -tol) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("zpnx2s"); continue; } zd = 0.0; } else if (zd > PI) { if (zd > PI+tol) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("zpnx2s"); continue; } zd = PI; } } else { /* Higher order - solve iteratively. */ zd1 = 0.0; r1 = prj->pv[0]; zd2 = prj->w[0]; r2 = prj->w[1]; if (r < r1) { if (r < r1-tol) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("zpnx2s"); continue; } zd = zd1; } else if (r > r2) { if (r > r2+tol) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("zpnx2s"); continue; } zd = zd2; } else { /* Disect the interval. */ for (j = 0; j < 100; j++) { lambda = (r2 - r)/(r2 - r1); if (lambda < 0.1) { lambda = 0.1; } else if (lambda > 0.9) { lambda = 0.9; } zd = zd2 - lambda*(zd2 - zd1); rt = 0.0; for (m = k; m >= 0; m--) { rt = (rt * zd) + prj->pv[m]; } if (rt < r) { if (r-rt < tol) break; r1 = rt; zd1 = zd; } else { if (rt-r < tol) break; r2 = rt; zd2 = zd; } if (fabs(zd2-zd1) < tol) break; } } } *thetap = 90.0 - zd*R2D; *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int zpns2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int m, mphi, mtheta, rowlen, rowoff, status; double cosphi, r, s, sinphi; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != ZPN) { if ((status = zpnset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { s = (90.0 - *thetap)*D2R; r = 0.0; for (m = prj->n; m >= 0; m--) { r = r*s + prj->pv[m]; } r *= prj->r0; istat = 0; if (prj->bounds && s > prj->w[0]) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("zpns2x"); } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = istat; } } return status; } /*============================================================================ * ZEA: zenithal/azimuthal equal area projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag ZEA * prj->code "ZEA" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] 2*r0 * prj->w[1] 1/(2*r0) * prj->prjx2s Pointer to zeax2s(). * prj->prjs2x Pointer to zeas2x(). *===========================================================================*/ int zeaset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = ZEA; strcpy(prj->code, "ZEA"); strcpy(prj->name, "zenithal/azimuthal equal area"); prj->category = ZENITHAL; prj->pvrange = 0; prj->simplezen = 1; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 360.0/PI; prj->w[1] = PI/360.0; } else { prj->w[0] = 2.0*prj->r0; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = zeax2s; prj->prjs2x = zeas2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int zeax2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double r, s, xj, yj, yj2; const double tol = 1.0e-12; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != ZEA) { if ((status = zeaset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yj2); if (r == 0.0) { *phip = 0.0; } else { *phip = atan2d(xj, -yj); } s = r*prj->w[1]; if (fabs(s) > 1.0) { if (fabs(r - prj->w[0]) < tol) { *thetap = -90.0; } else { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("zeax2s"); continue; } } else { *thetap = 90.0 - 2.0*asind(s); } *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int zeas2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, r, sinphi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != ZEA) { if ((status = zeaset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { r = prj->w[0]*sind((90.0 - *thetap)/2.0); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = 0; } } return 0; } /*============================================================================ * AIR: Airy's projection. * * Given: * prj->pv[1] Latitude theta_b within which the error is minimized, in * degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 90.0 if undefined. * * Returned: * prj->flag AIR * prj->code "AIR" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] 2*r0 * prj->w[1] ln(cos(xi_b))/tan(xi_b)**2, where xi_b = (90-theta_b)/2 * prj->w[2] 1/2 - prj->w[1] * prj->w[3] 2*r0*prj->w[2] * prj->w[4] tol, cutoff for using small angle approximation, in * radians. * prj->w[5] prj->w[2]*tol * prj->w[6] (180/pi)/prj->w[2] * prj->prjx2s Pointer to airx2s(). * prj->prjs2x Pointer to airs2x(). *===========================================================================*/ int airset(prj) struct prjprm *prj; { const double tol = 1.0e-4; double cosxi; if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = AIR; strcpy(prj->code, "AIR"); if (undefined(prj->pv[1])) prj->pv[1] = 90.0; if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "Airy's zenithal"); prj->category = ZENITHAL; prj->pvrange = 101; prj->simplezen = 1; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = 1; prj->w[0] = 2.0*prj->r0; if (prj->pv[1] == 90.0) { prj->w[1] = -0.5; prj->w[2] = 1.0; } else if (prj->pv[1] > -90.0) { cosxi = cosd((90.0 - prj->pv[1])/2.0); prj->w[1] = log(cosxi)*(cosxi*cosxi)/(1.0-cosxi*cosxi); prj->w[2] = 0.5 - prj->w[1]; } else { return PRJERR_BAD_PARAM_SET("airset"); } prj->w[3] = prj->w[0] * prj->w[2]; prj->w[4] = tol; prj->w[5] = prj->w[2]*tol; prj->w[6] = R2D/prj->w[2]; prj->prjx2s = airx2s; prj->prjs2x = airs2x; return prjoff(prj, 0.0, 90.0); } /*--------------------------------------------------------------------------*/ int airx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int k, mx, my, rowlen, rowoff, status; double cosxi, lambda, r, r1, r2, rt, tanxi, x1, x2, xi, xj, yj, yj2; const double tol = 1.0e-12; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != AIR) { if ((status = airset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + yj2)/prj->w[0]; if (r == 0.0) { *phip = 0.0; } else { *phip = atan2d(xj, -yj); } if (r == 0.0) { xi = 0.0; } else if (r < prj->w[5]) { xi = r*prj->w[6]; } else { /* Find a solution interval. */ x1 = x2 = 1.0; r1 = r2 = 0.0; for (k = 0; k < 30; k++) { x2 = x1/2.0; tanxi = sqrt(1.0-x2*x2)/x2; r2 = -(log(x2)/tanxi + prj->w[1]*tanxi); if (r2 >= r) break; x1 = x2; r1 = r2; } if (k == 30) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("airx2s"); continue; } for (k = 0; k < 100; k++) { /* Weighted division of the interval. */ lambda = (r2-r)/(r2-r1); if (lambda < 0.1) { lambda = 0.1; } else if (lambda > 0.9) { lambda = 0.9; } cosxi = x2 - lambda*(x2-x1); tanxi = sqrt(1.0-cosxi*cosxi)/cosxi; rt = -(log(cosxi)/tanxi + prj->w[1]*tanxi); if (rt < r) { if (r-rt < tol) break; r1 = rt; x1 = cosxi; } else { if (rt-r < tol) break; r2 = rt; x2 = cosxi; } } if (k == 100) { *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("airx2s"); continue; } xi = acosd(cosxi); } *thetap = 90.0 - 2.0*xi; *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int airs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, cosxi, r, tanxi, xi, sinphi; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != AIR) { if ((status = airset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { istat = 0; if (*thetap == 90.0) { r = 0.0; } else if (*thetap > -90.0) { xi = D2R*(90.0 - *thetap)/2.0; if (xi < prj->w[4]) { r = xi*prj->w[3]; } else { cosxi = cosd((90.0 - *thetap)/2.0); tanxi = sqrt(1.0-cosxi*cosxi)/cosxi; r = -prj->w[0]*(log(cosxi)/tanxi + prj->w[1]*tanxi); } } else { r = 0.0; istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("airs2x"); } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - prj->y0; *(statp++) = istat; } } return status; } /*============================================================================ * CYP: cylindrical perspective projection. * * Given: * prj->pv[1] Distance of point of projection from the centre of the * generating sphere, mu, in units of r0. * prj->pv[2] Radius of the cylinder of projection, lambda, in units of * r0. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag CYP * prj->code "CYP" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*lambda*(pi/180) * prj->w[1] (180/pi)/(r0*lambda) * prj->w[2] r0*(mu + lambda) * prj->w[3] 1/(r0*(mu + lambda)) * prj->prjx2s Pointer to cypx2s(). * prj->prjs2x Pointer to cyps2x(). *===========================================================================*/ int cypset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = CYP; strcpy(prj->code, "CYP"); if (undefined(prj->pv[1])) prj->pv[1] = 1.0; if (undefined(prj->pv[2])) prj->pv[2] = 1.0; strcpy(prj->name, "cylindrical perspective"); prj->category = CYLINDRICAL; prj->pvrange = 102; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = prj->pv[1] < -1.0 || 0.0 < prj->pv[1]; prj->divergent = !prj->global; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = prj->pv[2]; if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("cypset"); } prj->w[1] = 1.0/prj->w[0]; prj->w[2] = R2D*(prj->pv[1] + prj->pv[2]); if (prj->w[2] == 0.0) { return PRJERR_BAD_PARAM_SET("cypset"); } prj->w[3] = 1.0/prj->w[2]; } else { prj->w[0] = prj->r0*prj->pv[2]*D2R; if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("cypset"); } prj->w[1] = 1.0/prj->w[0]; prj->w[2] = prj->r0*(prj->pv[1] + prj->pv[2]); if (prj->w[2] == 0.0) { return PRJERR_BAD_PARAM_SET("cypset"); } prj->w[3] = 1.0/prj->w[2]; } prj->prjx2s = cypx2s; prj->prjs2x = cyps2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int cypx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double eta, s, t; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CYP) { if ((status = cypset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { s = prj->w[1]*(*xp + prj->x0); phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; phip += rowlen; } } /* Do y dependence. */ yp = y; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { eta = prj->w[3]*(*yp + prj->y0); t = atan2d(eta,1.0) + asind(eta*prj->pv[1]/sqrt(eta*eta+1.0)); for (ix = 0; ix < mx; ix++, thetap += spt) { *thetap = t; *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int cyps2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double eta, xi; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CYP) { if ((status = cypset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0]*(*phip) - prj->x0; xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { eta = prj->pv[1] + cosd(*thetap); istat = 0; if (eta == 0.0) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("cyps2x"); } else { eta = prj->w[2]*sind(*thetap)/eta; } eta -= prj->y0; for (iphi = 0; iphi < mphi; iphi++, yp += sxy) { *yp = eta; *(statp++) = istat; } } return status; } /*============================================================================ * CEA: cylindrical equal area projection. * * Given: * prj->pv[1] Square of the cosine of the latitude at which the * projection is conformal, lambda. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag CEA * prj->code "CEA" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->w[2] r0/lambda * prj->w[3] lambda/r0 * prj->prjx2s Pointer to ceax2s(). * prj->prjs2x Pointer to ceas2x(). *===========================================================================*/ int ceaset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = CEA; strcpy(prj->code, "CEA"); if (undefined(prj->pv[1])) prj->pv[1] = 1.0; strcpy(prj->name, "cylindrical equal area"); prj->category = CYLINDRICAL; prj->pvrange = 101; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; if (prj->pv[1] <= 0.0 || prj->pv[1] > 1.0) { return PRJERR_BAD_PARAM_SET("ceaset"); } prj->w[2] = prj->r0/prj->pv[1]; prj->w[3] = prj->pv[1]/prj->r0; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = R2D/prj->r0; if (prj->pv[1] <= 0.0 || prj->pv[1] > 1.0) { return PRJERR_BAD_PARAM_SET("ceaset"); } prj->w[2] = prj->r0/prj->pv[1]; prj->w[3] = prj->pv[1]/prj->r0; } prj->prjx2s = ceax2s; prj->prjs2x = ceas2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int ceax2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double s; const double tol = 1.0e-13; register int istat, ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CEA) { if ((status = ceaset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { s = prj->w[1]*(*xp + prj->x0); phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; phip += rowlen; } } /* Do y dependence. */ yp = y; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { s = prj->w[3]*(*yp + prj->y0); istat = 0; if (fabs(s) > 1.0) { if (fabs(s) > 1.0+tol) { s = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("ceax2s"); } else { s = copysign(90.0, s); } } else { s = asind(s); } for (ix = 0; ix < mx; ix++, thetap += spt) { *thetap = s; *(statp++) = istat; } } return status; } /*--------------------------------------------------------------------------*/ int ceas2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double eta, xi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CEA) { if ((status = ceaset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0]*(*phip) - prj->x0; xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { eta = prj->w[2]*sind(*thetap) - prj->y0; for (iphi = 0; iphi < mphi; iphi++, yp += sxy) { *yp = eta; *(statp++) = 0; } } return 0; } /*============================================================================ * CAR: Plate carree projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag CAR * prj->code "CAR" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->prjx2s Pointer to carx2s(). * prj->prjs2x Pointer to cars2x(). *===========================================================================*/ int carset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = CAR; strcpy(prj->code, "CAR"); strcpy(prj->name, "plate caree"); prj->category = CYLINDRICAL; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = carx2s; prj->prjs2x = cars2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int carx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double s, t; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CAR) { if ((status = carset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { s = prj->w[1]*(*xp + prj->x0); phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; phip += rowlen; } } /* Do y dependence. */ yp = y; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { t = prj->w[1]*(*yp + prj->y0); for (ix = 0; ix < mx; ix++, thetap += spt) { *thetap = t; *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int cars2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double eta, xi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CAR) { if ((status = carset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0]*(*phip) - prj->x0; xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { eta = prj->w[0]*(*thetap) - prj->y0; for (iphi = 0; iphi < mphi; iphi++, yp += sxy) { *yp = eta; *(statp++) = 0; } } return 0; } /*============================================================================ * MER: Mercator's projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag MER * prj->code "MER" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->prjx2s Pointer to merx2s(). * prj->prjs2x Pointer to mers2x(). *===========================================================================*/ int merset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = MER; strcpy(prj->code, "MER"); strcpy(prj->name, "Mercator's"); prj->category = CYLINDRICAL; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 1; prj->global = 0; prj->divergent = 1; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = merx2s; prj->prjs2x = mers2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int merx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double s, t; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != MER) { if ((status = merset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { s = prj->w[1]*(*xp + prj->x0); phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; phip += rowlen; } } /* Do y dependence. */ yp = y; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { t = 2.0*atand(exp((*yp + prj->y0)/prj->r0)) - 90.0; for (ix = 0; ix < mx; ix++, thetap += spt) { *thetap = t; *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int mers2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double eta, xi; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != MER) { if ((status = merset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0]*(*phip) - prj->x0; xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { istat = 0; if (*thetap <= -90.0 || *thetap >= 90.0) { eta = 0.0; istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("mers2x"); } else { eta = prj->r0*log(tand((*thetap+90.0)/2.0)) - prj->y0; } for (iphi = 0; iphi < mphi; iphi++, yp += sxy) { *yp = eta; *(statp++) = istat; } } return status; } /*============================================================================ * SFL: Sanson-Flamsteed ("global sinusoid") projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag SFL * prj->code "SFL" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->prjx2s Pointer to sflx2s(). * prj->prjs2x Pointer to sfls2x(). *===========================================================================*/ int sflset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = SFL; strcpy(prj->code, "SFL"); strcpy(prj->name, "Sanson-Flamsteed"); prj->category = PSEUDOCYLINDRICAL; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = sflx2s; prj->prjs2x = sfls2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int sflx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double s, t, yj; register int istat, ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != SFL) { if ((status = sflset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { s = prj->w[1]*(*xp + prj->x0); phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; s = cos(yj/prj->r0); istat = 0; if (s == 0.0) { istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("sflx2s"); } else { s = 1.0/s; } t = prj->w[1]*yj; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { *phip *= s; *thetap = t; *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int sfls2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double eta, xi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != SFL) { if ((status = sflset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0]*(*phip); xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { xi = cosd(*thetap); eta = prj->w[0]*(*thetap) - prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = xi*(*xp) - prj->x0; *yp = eta; *(statp++) = 0; } } return 0; } /*============================================================================ * PAR: parabolic projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag PAR * prj->code "PAR" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->w[2] pi*r0 * prj->w[3] 1/(pi*r0) * prj->prjx2s Pointer to parx2s(). * prj->prjs2x Pointer to pars2x(). *===========================================================================*/ int parset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = PAR; strcpy(prj->code, "PAR"); strcpy(prj->name, "parabolic"); prj->category = PSEUDOCYLINDRICAL; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; prj->w[2] = 180.0; prj->w[3] = 1.0/prj->w[2]; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = 1.0/prj->w[0]; prj->w[2] = PI*prj->r0; prj->w[3] = 1.0/prj->w[2]; } prj->prjx2s = parx2s; prj->prjs2x = pars2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int parx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double r, s, t, xj; const double tol = 1.0e-13; register int istat, ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != PAR) { if ((status = parset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; s = prj->w[1]*xj; t = fabs(xj) - tol; phip = phi + rowoff; thetap = theta + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; *thetap = t; phip += rowlen; thetap += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { r = prj->w[3]*(*yp + prj->y0); istat = 0; if (r > 1.0 || r < -1.0) { s = 0.0; t = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("parx2s"); } else { s = 1.0 - 4.0*r*r; if (s == 0.0) { /* Deferred test. */ istat = -1; } else { s = 1.0/s; } t = 3.0*asind(r); } for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { if (istat < 0) { if (*thetap < 0.0) { *(statp++) = 0; } else { *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("parx2s"); } } *phip *= s; *thetap = t; } } return status; } /*--------------------------------------------------------------------------*/ int pars2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double eta, s, xi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != PAR) { if ((status = parset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0]*(*phip); xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { s = sind((*thetap)/3.0); xi = (1.0 - 4.0*s*s); eta = prj->w[2]*s - prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = xi*(*xp) - prj->x0; *yp = eta; *(statp++) = 0; } } return 0; } /*============================================================================ * MOL: Mollweide's projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag MOL * prj->code "MOL" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] sqrt(2)*r0 * prj->w[1] sqrt(2)*r0/90 * prj->w[2] 1/(sqrt(2)*r0) * prj->w[3] 90/r0 * prj->prjx2s Pointer to molx2s(). * prj->prjs2x Pointer to mols2x(). *===========================================================================*/ int molset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = MOL; strcpy(prj->code, "MOL"); if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "Mollweide's"); prj->category = PSEUDOCYLINDRICAL; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; prj->w[0] = SQRT2*prj->r0; prj->w[1] = prj->w[0]/90.0; prj->w[2] = 1.0/prj->w[0]; prj->w[3] = 90.0/prj->r0; prj->w[4] = 2.0/PI; prj->prjx2s = molx2s; prj->prjs2x = mols2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int molx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double r, s, t, xj, y0, yj, z; const double tol = 1.0e-12; register int istat, ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != MOL) { if ((status = molset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; s = prj->w[3]*xj; t = fabs(xj) - tol; phip = phi + rowoff; thetap = theta + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; *thetap = t; phip += rowlen; thetap += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; y0 = yj/prj->r0; r = 2.0 - y0*y0; istat = 0; if (r <= tol) { if (r < -tol) { istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("molx2s"); } else { /* OK if fabs(x) < tol whence phi = 0.0. */ istat = -1; } r = 0.0; s = 0.0; } else { r = sqrt(r); s = 1.0/r; } z = yj*prj->w[2]; if (fabs(z) > 1.0) { if (fabs(z) > 1.0+tol) { z = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("molx2s"); } else { z = copysign(1.0, z) + y0*r/PI; } } else { z = asin(z)*prj->w[4] + y0*r/PI; } if (fabs(z) > 1.0) { if (fabs(z) > 1.0+tol) { z = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("molx2s"); } else { z = copysign(1.0, z); } } t = asind(z); for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { if (istat < 0) { if (*thetap < 0.0) { *(statp++) = 0; } else { *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("molx2s"); } } *phip *= s; *thetap = t; } } return status; } /*--------------------------------------------------------------------------*/ int mols2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int k, mphi, mtheta, rowlen, rowoff, status; double eta, gamma, resid, u, v, v0, v1, xi; const double tol = 1.0e-13; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != MOL) { if ((status = molset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[1]*(*phip); xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = xi; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { if (fabs(*thetap) == 90.0) { xi = 0.0; eta = copysign(prj->w[0], *thetap); } else if (*thetap == 0.0) { xi = 1.0; eta = 0.0; } else { u = PI*sind(*thetap); v0 = -PI; v1 = PI; v = u; for (k = 0; k < 100; k++) { resid = (v - u) + sin(v); if (resid < 0.0) { if (resid > -tol) break; v0 = v; } else { if (resid < tol) break; v1 = v; } v = (v0 + v1)/2.0; } gamma = v/2.0; xi = cos(gamma); eta = prj->w[0]*sin(gamma); } eta -= prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = xi*(*xp) - prj->x0; *yp = eta; *(statp++) = 0; } } return 0; } /*============================================================================ * AIT: Hammer-Aitoff projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag AIT * prj->code "AIT" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] 2*r0**2 * prj->w[1] 1/(2*r0)**2 * prj->w[2] 1/(4*r0)**2 * prj->w[3] 1/(2*r0) * prj->prjx2s Pointer to aitx2s(). * prj->prjs2x Pointer to aits2x(). *===========================================================================*/ int aitset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = AIT; strcpy(prj->code, "AIT"); if (prj->r0 == 0.0) prj->r0 = R2D; strcpy(prj->name, "Hammer-Aitoff"); prj->category = CONVENTIONAL; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; prj->w[0] = 2.0*prj->r0*prj->r0; prj->w[1] = 1.0/(2.0*prj->w[0]); prj->w[2] = prj->w[1]/4.0; prj->w[3] = 1.0/(2.0*prj->r0); prj->prjx2s = aitx2s; prj->prjs2x = aits2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int aitx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double s, t, x0, xj, y0, yj, yj2, z; const double tol = 1.0e-13; register int ix, iy, istat, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != AIT) { if ((status = aitset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; s = 1.0 - xj*xj*prj->w[2]; t = xj*prj->w[3]; phip = phi + rowoff; thetap = theta + rowoff; for (iy = 0; iy < my; iy++) { *phip = s; *thetap = t; phip += rowlen; thetap += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; yj2 = yj*yj*prj->w[1]; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { s = *phip - yj2; istat = 0; if (s < 0.5) { if (s < 0.5-tol) { istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("aitx2s"); } s = 0.5; } z = sqrt(s); x0 = 2.0*z*z - 1.0; y0 = z*(*thetap); if (x0 == 0.0 && y0 == 0.0) { *phip = 0.0; } else { *phip = 2.0*atan2d(y0, x0); } t = z*yj/prj->r0; if (fabs(t) > 1.0) { if (fabs(t) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("aitx2s"); } t = copysign(90.0, t); } else { t = asind(t); } *thetap = t; *(statp++) = istat; } } return status; } /*--------------------------------------------------------------------------*/ int aits2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double cosphi, costhe, sinphi, sinthe, w; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != AIT) { if ((status = aitset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { w = (*phip)/2.0; sincosd(w, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinphi; *yp = cosphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sincosd(*thetap, &sinthe, &costhe); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { w = sqrt(prj->w[0]/(1.0 + costhe*(*yp))); *xp = 2.0*w*costhe*(*xp) - prj->x0; *yp = w*sinthe - prj->y0; *(statp++) = 0; } } return 0; } /*============================================================================ * COP: conic perspective projection. * * Given: * prj->pv[1] sigma = (theta2+theta1)/2 * prj->pv[2] delta = (theta2-theta1)/2, where theta1 and theta2 are the * latitudes of the standard parallels, in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to sigma if undefined. * prj->theta0 Reset to sigma if undefined. * * Returned: * prj->flag COP * prj->code "COP" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] C = sin(sigma) * prj->w[1] 1/C * prj->w[2] Y0 = r0*cos(delta)*cot(sigma) * prj->w[3] r0*cos(delta) * prj->w[4] 1/(r0*cos(delta) * prj->w[5] cot(sigma) * prj->prjx2s Pointer to copx2s(). * prj->prjs2x Pointer to cops2x(). *===========================================================================*/ int copset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = COP; strcpy(prj->code, "COP"); strcpy(prj->name, "conic perspective"); if (undefined(prj->pv[1])) { return PRJERR_BAD_PARAM_SET("copset"); } if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; prj->category = CONIC; prj->pvrange = 102; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 0; prj->divergent = 1; prj->w[0] = sind(prj->pv[1]); if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("copset"); } prj->w[1] = 1.0/prj->w[0]; prj->w[3] = prj->r0*cosd(prj->pv[2]); if (prj->w[3] == 0.0) { return PRJERR_BAD_PARAM_SET("copset"); } prj->w[4] = 1.0/prj->w[3]; prj->w[5] = 1.0/tand(prj->pv[1]); prj->w[2] = prj->w[3]*prj->w[5]; prj->prjx2s = copx2s; prj->prjs2x = cops2x; return prjoff(prj, 0.0, prj->pv[1]); } /*--------------------------------------------------------------------------*/ int copx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double alpha, dy, dy2, r, xj; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COP) { if ((status = copset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { dy = prj->w[2] - (*yp + prj->y0); dy2 = dy*dy; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + dy2); if (prj->pv[1] < 0.0) r = -r; if (r == 0.0) { alpha = 0.0; } else { alpha = atan2d(xj/r, dy/r); } *phip = alpha*prj->w[1]; *thetap = prj->pv[1] + atand(prj->w[5] - r*prj->w[4]); *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int cops2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double alpha, cosalpha, r, s, t, sinalpha, y0; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COP) { if ((status = copset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { alpha = prj->w[0]*(*phip); sincosd(alpha, &sinalpha, &cosalpha); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinalpha; *yp = cosalpha; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; y0 = prj->y0 - prj->w[2]; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { t = *thetap - prj->pv[1]; s = cosd(t); istat = 0; if (s == 0.0) { r = 0.0; istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("cops2x"); } else { r = prj->w[2] - prj->w[3]*sind(t)/s; if (prj->bounds && r*prj->w[0] < 0.0) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("cops2x"); } } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - y0; *(statp++) = istat; } } return status; } /*============================================================================ * COE: conic equal area projection. * * Given: * prj->pv[1] sigma = (theta2+theta1)/2 * prj->pv[2] delta = (theta2-theta1)/2, where theta1 and theta2 are the * latitudes of the standard parallels, in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to sigma if undefined. * prj->theta0 Reset to sigma if undefined. * * Returned: * prj->flag COE * prj->code "COE" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] C = (sin(theta1) + sin(theta2))/2 * prj->w[1] 1/C * prj->w[2] Y0 = chi*sqrt(psi - 2C*sind(sigma)) * prj->w[3] chi = r0/C * prj->w[4] psi = 1 + sin(theta1)*sin(theta2) * prj->w[5] 2C * prj->w[6] (1 + sin(theta1)*sin(theta2))*(r0/C)**2 * prj->w[7] C/(2*r0**2) * prj->w[8] chi*sqrt(psi + 2C) * prj->prjx2s Pointer to coex2s(). * prj->prjs2x Pointer to coes2x(). *===========================================================================*/ int coeset(prj) struct prjprm *prj; { double theta1, theta2; if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = COE; strcpy(prj->code, "COE"); strcpy(prj->name, "conic equal area"); if (undefined(prj->pv[1])) { return PRJERR_BAD_PARAM_SET("coeset"); } if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; prj->category = CONIC; prj->pvrange = 102; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; theta1 = prj->pv[1] - prj->pv[2]; theta2 = prj->pv[1] + prj->pv[2]; prj->w[0] = (sind(theta1) + sind(theta2))/2.0; if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("coeset"); } prj->w[1] = 1.0/prj->w[0]; prj->w[3] = prj->r0/prj->w[0]; prj->w[4] = 1.0 + sind(theta1)*sind(theta2); prj->w[5] = 2.0*prj->w[0]; prj->w[6] = prj->w[3]*prj->w[3]*prj->w[4]; prj->w[7] = 1.0/(2.0*prj->r0*prj->w[3]); prj->w[8] = prj->w[3]*sqrt(prj->w[4] + prj->w[5]); prj->w[2] = prj->w[3]*sqrt(prj->w[4] - prj->w[5]*sind(prj->pv[1])); prj->prjx2s = coex2s; prj->prjs2x = coes2x; return prjoff(prj, 0.0, prj->pv[1]); } /*--------------------------------------------------------------------------*/ int coex2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double alpha, dy, dy2, r, t, w, xj; const double tol = 1.0e-12; register int ix, iy, istat, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COE) { if ((status = coeset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { dy = prj->w[2] - (*yp + prj->y0); dy2 = dy*dy; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + dy2); if (prj->pv[1] < 0.0) r = -r; if (r == 0.0) { alpha = 0.0; } else { alpha = atan2d(xj/r, dy/r); } istat = 0; if (fabs(r - prj->w[8]) < tol) { t = -90.0; } else { w = (prj->w[6] - r*r)*prj->w[7]; if (fabs(w) > 1.0) { if (fabs(w-1.0) < tol) { t = 90.0; } else if (fabs(w+1.0) < tol) { t = -90.0; } else { t = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("coex2s"); } } else { t = asind(w); } } *phip = alpha*prj->w[1]; *thetap = t; *(statp++) = istat; } } return status; } /*--------------------------------------------------------------------------*/ int coes2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double alpha, cosalpha, r, sinalpha, y0; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COE) { if ((status = coeset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { alpha = prj->w[0]*(*phip); sincosd(alpha, &sinalpha, &cosalpha); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinalpha; *yp = cosalpha; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; y0 = prj->y0 - prj->w[2]; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { if (*thetap == -90.0) { r = prj->w[8]; } else { r = prj->w[3]*sqrt(prj->w[4] - prj->w[5]*sind(*thetap)); } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - y0; *(statp++) = 0; } } return 0; } /*============================================================================ * COD: conic equidistant projection. * * Given: * prj->pv[1] sigma = (theta2+theta1)/2 * prj->pv[2] delta = (theta2-theta1)/2, where theta1 and theta2 are the * latitudes of the standard parallels, in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to sigma if undefined. * prj->theta0 Reset to sigma if undefined. * * Returned: * prj->flag COD * prj->code "COD" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] C = r0*sin(sigma)*sin(delta)/delta * prj->w[1] 1/C * prj->w[2] Y0 = delta*cot(delta)*cot(sigma) * prj->w[3] Y0 + sigma * prj->prjx2s Pointer to codx2s(). * prj->prjs2x Pointer to cods2x(). *===========================================================================*/ int codset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = COD; strcpy(prj->code, "COD"); strcpy(prj->name, "conic equidistant"); if (undefined(prj->pv[1])) { return PRJERR_BAD_PARAM_SET("codset"); } if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; prj->category = CONIC; prj->pvrange = 102; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->pv[2] == 0.0) { prj->w[0] = prj->r0*sind(prj->pv[1])*D2R; } else { prj->w[0] = prj->r0*sind(prj->pv[1])*sind(prj->pv[2])/prj->pv[2]; } if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("codset"); } prj->w[1] = 1.0/prj->w[0]; prj->w[2] = prj->r0*cosd(prj->pv[2])*cosd(prj->pv[1])/prj->w[0]; prj->w[3] = prj->w[2] + prj->pv[1]; prj->prjx2s = codx2s; prj->prjs2x = cods2x; return prjoff(prj, 0.0, prj->pv[1]); } /*--------------------------------------------------------------------------*/ int codx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double alpha, dy, dy2, r, xj; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COD) { if ((status = codset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { dy = prj->w[2] - (*yp + prj->y0); dy2 = dy*dy; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + dy2); if (prj->pv[1] < 0.0) r = -r; if (r == 0.0) { alpha = 0.0; } else { alpha = atan2d(xj/r, dy/r); } *phip = alpha*prj->w[1]; *thetap = prj->w[3] - r; *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int cods2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double alpha, cosalpha, r, sinalpha, y0; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COD) { if ((status = codset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { alpha = prj->w[0]*(*phip); sincosd(alpha, &sinalpha, &cosalpha); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinalpha; *yp = cosalpha; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; y0 = prj->y0 - prj->w[2]; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { r = prj->w[3] - *thetap; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - y0; *(statp++) = 0; } } return 0; } /*============================================================================ * COO: conic orthomorphic projection. * * Given: * prj->pv[1] sigma = (theta2+theta1)/2 * prj->pv[2] delta = (theta2-theta1)/2, where theta1 and theta2 are the * latitudes of the standard parallels, in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to sigma if undefined. * prj->theta0 Reset to sigma if undefined. * * Returned: * prj->flag COO * prj->code "COO" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] C = ln(cos(theta2)/cos(theta1))/ln(tan(tau2)/tan(tau1)) * where tau1 = (90 - theta1)/2 * tau2 = (90 - theta2)/2 * prj->w[1] 1/C * prj->w[2] Y0 = psi*tan((90-sigma)/2)**C * prj->w[3] psi = (r0*cos(theta1)/C)/tan(tau1)**C * prj->w[4] 1/psi * prj->prjx2s Pointer to coox2s(). * prj->prjs2x Pointer to coos2x(). *===========================================================================*/ int cooset(prj) struct prjprm *prj; { double cos1, cos2, tan1, tan2, theta1, theta2; if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = COO; strcpy(prj->code, "COO"); strcpy(prj->name, "conic orthomorphic"); if (undefined(prj->pv[1])) { return PRJERR_BAD_PARAM_SET("cooset"); } if (undefined(prj->pv[2])) prj->pv[2] = 0.0; if (prj->r0 == 0.0) prj->r0 = R2D; prj->category = CONIC; prj->pvrange = 102; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 1; prj->global = 0; prj->divergent = 1; theta1 = prj->pv[1] - prj->pv[2]; theta2 = prj->pv[1] + prj->pv[2]; tan1 = tand((90.0 - theta1)/2.0); cos1 = cosd(theta1); if (theta1 == theta2) { prj->w[0] = sind(theta1); } else { tan2 = tand((90.0 - theta2)/2.0); cos2 = cosd(theta2); prj->w[0] = log(cos2/cos1)/log(tan2/tan1); } if (prj->w[0] == 0.0) { return PRJERR_BAD_PARAM_SET("cooset"); } prj->w[1] = 1.0/prj->w[0]; prj->w[3] = prj->r0*(cos1/prj->w[0])/pow(tan1,prj->w[0]); if (prj->w[3] == 0.0) { return PRJERR_BAD_PARAM_SET("cooset"); } prj->w[2] = prj->w[3]*pow(tand((90.0 - prj->pv[1])/2.0),prj->w[0]); prj->w[4] = 1.0/prj->w[3]; prj->prjx2s = coox2s; prj->prjs2x = coos2x; return prjoff(prj, 0.0, prj->pv[1]); } /*--------------------------------------------------------------------------*/ int coox2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double alpha, dy, dy2, r, t, xj; register int ix, iy, istat, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COO) { if ((status = cooset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { dy = prj->w[2] - (*yp + prj->y0); dy2 = dy*dy; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + dy2); if (prj->pv[1] < 0.0) r = -r; if (r == 0.0) { alpha = 0.0; } else { alpha = atan2d(xj/r, dy/r); } istat = 0; if (r == 0.0) { if (prj->w[0] < 0.0) { t = -90.0; } else { t = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("coox2s"); } } else { t = 90.0 - 2.0*atand(pow(r*prj->w[4],prj->w[1])); } *phip = alpha*prj->w[1]; *thetap = t; *(statp++) = istat; } } return status; } /*--------------------------------------------------------------------------*/ int coos2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double alpha, cosalpha, r, sinalpha, y0; register int iphi, itheta, istat, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != COO) { if ((status = cooset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { alpha = prj->w[0]*(*phip); sincosd(alpha, &sinalpha, &cosalpha); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = sinalpha; *yp = cosalpha; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; y0 = prj->y0 - prj->w[2]; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { istat = 0; if (*thetap == -90.0) { r = 0.0; if (prj->w[0] >= 0.0) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("coos2x"); } } else { r = prj->w[3]*pow(tand((90.0 - *thetap)/2.0),prj->w[0]); } for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *xp = r*(*xp) - prj->x0; *yp = -r*(*yp) - y0; *(statp++) = istat; } } return status; } /*============================================================================ * BON: Bonne's projection. * * Given: * prj->pv[1] Bonne conformal latitude, theta1, in degrees. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag BON * prj->code "BON" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[1] r0*pi/180 * prj->w[2] Y0 = r0*(cot(theta1) + theta1*pi/180) * prj->prjx2s Pointer to bonx2s(). * prj->prjs2x Pointer to bons2x(). *===========================================================================*/ int bonset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = BON; strcpy(prj->code, "BON"); strcpy(prj->name, "Bonne's"); if (undefined(prj->pv[1])) { return PRJERR_BAD_PARAM_SET("bonset"); } if (prj->pv[1] == 0.0) { /* Sanson-Flamsteed. */ return sflset(prj); } prj->category = POLYCONIC; prj->pvrange = 101; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[1] = 1.0; prj->w[2] = prj->r0*cosd(prj->pv[1])/sind(prj->pv[1]) + prj->pv[1]; } else { prj->w[1] = prj->r0*D2R; prj->w[2] = prj->r0*(cosd(prj->pv[1])/sind(prj->pv[1]) + prj->pv[1]*D2R); } prj->prjx2s = bonx2s; prj->prjs2x = bons2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int bonx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double alpha, dy, dy2, costhe, r, s, t, xj; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->pv[1] == 0.0) { /* Sanson-Flamsteed. */ return sflx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat); } if (prj->flag != BON) { if ((status = bonset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { dy = prj->w[2] - (*yp + prj->y0); dy2 = dy*dy; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; r = sqrt(xj*xj + dy2); if (prj->pv[1] < 0.0) r = -r; if (r == 0.0) { alpha = 0.0; } else { alpha = atan2d(xj/r, dy/r); } t = (prj->w[2] - r)/prj->w[1]; costhe = cosd(t); if (costhe == 0.0) { s = 0.0; } else { s = alpha*(r/prj->r0)/costhe; } *phip = s; *thetap = t; *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int bons2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double alpha, cosalpha, r, s, sinalpha, y0; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->pv[1] == 0.0) { /* Sanson-Flamsteed. */ return sfls2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat); } if (prj->flag != BON) { if ((status = bonset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } y0 = prj->y0 - prj->w[2]; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { s = prj->r0*(*phip); xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = s; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { r = prj->w[2] - prj->w[1]*(*thetap); s = cosd(*thetap)/r; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { alpha = s*(*xp); sincosd(alpha, &sinalpha, &cosalpha); *xp = r*sinalpha - prj->x0; *yp = -r*cosalpha - y0; *(statp++) = 0; } } return 0; } /*============================================================================ * PCO: polyconic projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag PCO * prj->code "PCO" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/180) * prj->w[1] 1/r0 * prj->w[2] 2*r0 * prj->prjx2s Pointer to pcox2s(). * prj->prjs2x Pointer to pcos2x(). *===========================================================================*/ int pcoset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = PCO; strcpy(prj->code, "PCO"); strcpy(prj->name, "polyconic"); prj->category = POLYCONIC; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; prj->w[2] = 360.0/PI; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = 1.0/prj->w[0]; prj->w[2] = 2.0*prj->r0; } prj->prjx2s = pcox2s; prj->prjs2x = pcos2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int pcox2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double f, fneg, fpos, lambda, tanthe, the, theneg, thepos, w, x1, xj, xx, yj, ymthe, y1; const double tol = 1.0e-12; register int ix, iy, k, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != PCO) { if ((status = pcoset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xj = *xp + prj->x0; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xj; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yj = *yp + prj->y0; w = fabs(yj*prj->w[1]); for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xj = *phip; if (w < tol) { *phip = xj*prj->w[1]; *thetap = 0.0; } else if (fabs(w-90.0) < tol) { *phip = 0.0; *thetap = copysign(90.0, yj); } else { /* Iterative solution using weighted division of the interval. */ if (yj > 0.0) { thepos = 90.0; } else { thepos = -90.0; } theneg = 0.0; xx = xj*xj; ymthe = yj - prj->w[0]*thepos; fpos = xx + ymthe*ymthe; fneg = -999.0; for (k = 0; k < 64; k++) { if (fneg < -100.0) { /* Equal division of the interval. */ the = (thepos+theneg)/2.0; } else { /* Weighted division of the interval. */ lambda = fpos/(fpos-fneg); if (lambda < 0.1) { lambda = 0.1; } else if (lambda > 0.9) { lambda = 0.9; } the = thepos - lambda*(thepos-theneg); } /* Compute the residue. */ ymthe = yj - prj->w[0]*(the); tanthe = tand(the); f = xx + ymthe*(ymthe - prj->w[2]/tanthe); /* Check for convergence. */ if (fabs(f) < tol) break; if (fabs(thepos-theneg) < tol) break; /* Redefine the interval. */ if (f > 0.0) { thepos = the; fpos = f; } else { theneg = the; fneg = f; } } x1 = prj->r0 - ymthe*tanthe; y1 = xj*tanthe; if (x1 == 0.0 && y1 == 0.0) { *phip = 0.0; } else { *phip = atan2d(y1, x1)/sind(the); } *thetap = the; } *(statp++) = 0; } } return 0; } /*--------------------------------------------------------------------------*/ int pcos2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int mphi, mtheta, rowlen, rowoff, status; double alpha, costhe, cotthe, sinthe, therad; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != PCO) { if ((status = pcoset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xp = x + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = *phip; xp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { therad = (*thetap)*D2R; sincosd(*thetap, &sinthe, &costhe); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { if (sinthe == 0.0) { *xp = prj->w[0]*(*xp) - prj->x0; *yp = -prj->y0; } else { alpha = (*xp)*sinthe; cotthe = costhe/sinthe; *xp = prj->r0*cotthe*sind(alpha) - prj->x0; *yp = prj->r0*(cotthe*(1.0 - cosd(alpha)) + therad) - prj->y0; } *(statp++) = 0; } } return 0; } /*============================================================================ * TSC: tangential spherical cube projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag TSC * prj->code "TSC" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/4) * prj->w[1] (4/pi)/r0 * prj->prjx2s Pointer to tscx2s(). * prj->prjs2x Pointer to tscs2x(). *===========================================================================*/ int tscset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = TSC; strcpy(prj->code, "TSC"); strcpy(prj->name, "tangential spherical cube"); prj->category = QUADCUBE; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 45.0; prj->w[1] = 1.0/45.0; } else { prj->w[0] = prj->r0*PI/4.0; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = tscx2s; prj->prjs2x = tscs2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int tscx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int mx, my, rowlen, rowoff, status; double l, m, n, xf, yf; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != TSC) { if ((status = tscset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xf = (*xp + prj->x0)*prj->w[1]; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xf; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yf = (*yp + prj->y0)*prj->w[1]; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xf = *phip; /* Check bounds. */ if (fabs(xf) <= 1.0) { if (fabs(yf) > 3.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("tscx2s"); continue; } } else { if (fabs(xf) > 7.0 || fabs(yf) > 1.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("tscx2s"); continue; } } /* Map negative faces to the other side. */ if (xf < -1.0) xf += 8.0; /* Determine the face. */ if (xf > 5.0) { /* face = 4 */ xf = xf - 6.0; m = -1.0/sqrt(1.0 + xf*xf + yf*yf); l = -m*xf; n = -m*yf; } else if (xf > 3.0) { /* face = 3 */ xf = xf - 4.0; l = -1.0/sqrt(1.0 + xf*xf + yf*yf); m = l*xf; n = -l*yf; } else if (xf > 1.0) { /* face = 2 */ xf = xf - 2.0; m = 1.0/sqrt(1.0 + xf*xf + yf*yf); l = -m*xf; n = m*yf; } else if (yf > 1.0) { /* face = 0 */ yf = yf - 2.0; n = 1.0/sqrt(1.0 + xf*xf + yf*yf); l = -n*yf; m = n*xf; } else if (yf < -1.0) { /* face = 5 */ yf = yf + 2.0; n = -1.0/sqrt(1.0 + xf*xf + yf*yf); l = -n*yf; m = -n*xf; } else { /* face = 1 */ l = 1.0/sqrt(1.0 + xf*xf + yf*yf); m = l*xf; n = l*yf; } if (l == 0.0 && m == 0.0) { *phip = 0.0; } else { *phip = atan2d(m, l); } *thetap = asind(n); *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int tscs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int face, mphi, mtheta, rowlen, rowoff, status; double cosphi, costhe, l, m, n, sinphi, sinthe, x0, xf, y0, yf, zeta; const double tol = 1.0e-12; register int iphi, istat, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != TSC) { if ((status = tscset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = cosphi; *yp = sinphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sincosd(*thetap, &sinthe, &costhe); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { l = costhe*(*xp); m = costhe*(*yp); n = sinthe; face = 0; zeta = n; if (l > zeta) { face = 1; zeta = l; } if (m > zeta) { face = 2; zeta = m; } if (-l > zeta) { face = 3; zeta = -l; } if (-m > zeta) { face = 4; zeta = -m; } if (-n > zeta) { face = 5; zeta = -n; } switch (face) { case 1: xf = m/zeta; yf = n/zeta; x0 = 0.0; y0 = 0.0; break; case 2: xf = -l/zeta; yf = n/zeta; x0 = 2.0; y0 = 0.0; break; case 3: xf = -m/zeta; yf = n/zeta; x0 = 4.0; y0 = 0.0; break; case 4: xf = l/zeta; yf = n/zeta; x0 = 6.0; y0 = 0.0; break; case 5: xf = m/zeta; yf = l/zeta; x0 = 0.0; y0 = -2.0; break; default: /* face == 0 */ xf = m/zeta; yf = -l/zeta; x0 = 0.0; y0 = 2.0; break; } istat = 0; if (fabs(xf) > 1.0) { if (fabs(xf) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("tscs2x"); } xf = copysign(1.0, xf); } if (fabs(yf) > 1.0) { if (fabs(yf) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("tscs2x"); } yf = copysign(1.0, yf); } *xp = prj->w[0]*(xf + x0) - prj->x0; *yp = prj->w[0]*(yf + y0) - prj->y0; *(statp++) = istat; } } return status; } /*============================================================================ * CSC: COBE quadrilateralized spherical cube projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag CSC * prj->code "CSC" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/4) * prj->w[1] (4/pi)/r0 * prj->prjx2s Pointer to cscx2s(). * prj->prjs2x Pointer to cscs2x(). *===========================================================================*/ int cscset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = CSC; strcpy(prj->code, "CSC"); strcpy(prj->name, "COBE quadrilateralized spherical cube"); prj->category = QUADCUBE; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 0; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 45.0; prj->w[1] = 1.0/45.0; } else { prj->w[0] = prj->r0*PI/4.0; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = cscx2s; prj->prjs2x = cscs2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int cscx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int face, mx, my, rowlen, rowoff, status; double l, m, n; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; float chi, psi, xf, xx, yf, yy, z0, z1, z2, z3, z4, z5, z6; const float p00 = -0.27292696; const float p10 = -0.07629969; const float p20 = -0.22797056; const float p30 = 0.54852384; const float p40 = -0.62930065; const float p50 = 0.25795794; const float p60 = 0.02584375; const float p01 = -0.02819452; const float p11 = -0.01471565; const float p21 = 0.48051509; const float p31 = -1.74114454; const float p41 = 1.71547508; const float p51 = -0.53022337; const float p02 = 0.27058160; const float p12 = -0.56800938; const float p22 = 0.30803317; const float p32 = 0.98938102; const float p42 = -0.83180469; const float p03 = -0.60441560; const float p13 = 1.50880086; const float p23 = -0.93678576; const float p33 = 0.08693841; const float p04 = 0.93412077; const float p14 = -1.41601920; const float p24 = 0.33887446; const float p05 = -0.63915306; const float p15 = 0.52032238; const float p06 = 0.14381585; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CSC) { if ((status = cscset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xf = (*xp + prj->x0)*prj->w[1]; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xf; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yf = (*yp + prj->y0)*prj->w[1]; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xf = *phip; /* Check bounds. */ if (fabs(xf) <= 1.0) { if (fabs(yf) > 3.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("cscx2s"); continue; } } else { if (fabs(xf) > 7.0 || fabs(yf) > 1.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("cscx2s"); continue; } } /* Map negative faces to the other side. */ if (xf < -1.0) xf += 8.0; /* Determine the face. */ if (xf > 5.0) { face = 4; xf = xf - 6.0; } else if (xf > 3.0) { face = 3; xf = xf - 4.0; } else if (xf > 1.0) { face = 2; xf = xf - 2.0; } else if (yf > 1.0) { face = 0; yf = yf - 2.0; } else if (yf < -1.0) { face = 5; yf = yf + 2.0; } else { face = 1; } xx = xf*xf; yy = yf*yf; z0 = p00 + xx*(p10 + xx*(p20 + xx*(p30 + xx*(p40 + xx*(p50 + xx*(p60)))))); z1 = p01 + xx*(p11 + xx*(p21 + xx*(p31 + xx*(p41 + xx*(p51))))); z2 = p02 + xx*(p12 + xx*(p22 + xx*(p32 + xx*(p42)))); z3 = p03 + xx*(p13 + xx*(p23 + xx*(p33))); z4 = p04 + xx*(p14 + xx*(p24)); z5 = p05 + xx*(p15); z6 = p06; chi = z0 + yy*(z1 + yy*(z2 + yy*(z3 + yy*(z4 + yy*(z5 + yy*z6))))); chi = xf + xf*(1.0 - xx)*chi; z0 = p00 + yy*(p10 + yy*(p20 + yy*(p30 + yy*(p40 + yy*(p50 + yy*(p60)))))); z1 = p01 + yy*(p11 + yy*(p21 + yy*(p31 + yy*(p41 + yy*(p51))))); z2 = p02 + yy*(p12 + yy*(p22 + yy*(p32 + yy*(p42)))); z3 = p03 + yy*(p13 + yy*(p23 + yy*(p33))); z4 = p04 + yy*(p14 + yy*(p24)); z5 = p05 + yy*(p15); z6 = p06; psi = z0 + xx*(z1 + xx*(z2 + xx*(z3 + xx*(z4 + xx*(z5 + xx*z6))))); psi = yf + yf*(1.0 - yy)*psi; switch (face) { case 1: l = 1.0/sqrt(chi*chi + psi*psi + 1.0); m = chi*l; n = psi*l; break; case 2: m = 1.0/sqrt(chi*chi + psi*psi + 1.0); l = -chi*m; n = psi*m; break; case 3: l = -1.0/sqrt(chi*chi + psi*psi + 1.0); m = chi*l; n = -psi*l; break; case 4: m = -1.0/sqrt(chi*chi + psi*psi + 1.0); l = -chi*m; n = -psi*m; break; case 5: n = -1.0/sqrt(chi*chi + psi*psi + 1.0); l = -psi*n; m = -chi*n; break; default: /* face == 0 */ n = 1.0/sqrt(chi*chi + psi*psi + 1.0); l = -psi*n; m = chi*n; break; } if (l == 0.0 && m == 0.0) { *phip = 0.0; } else { *phip = atan2d(m, l); } *thetap = asind(n); *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int cscs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int face, mphi, mtheta, rowlen, rowoff, status; double cosphi, costhe, eta, l, m, n, sinphi, sinthe, xi, zeta; const float tol = 1.0e-7; register int iphi, istat, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; float chi, chi2, chi2psi2, chi4, chipsi, psi, psi2, psi4, chi2co, psi2co, x0, xf, y0, yf; const float gstar = 1.37484847732; const float mm = 0.004869491981; const float gamma = -0.13161671474; const float omega1 = -0.159596235474; const float d0 = 0.0759196200467; const float d1 = -0.0217762490699; const float c00 = 0.141189631152; const float c10 = 0.0809701286525; const float c01 = -0.281528535557; const float c11 = 0.15384112876; const float c20 = -0.178251207466; const float c02 = 0.106959469314; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != CSC) { if ((status = cscset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = cosphi; *yp = sinphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sincosd(*thetap, &sinthe, &costhe); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { l = costhe*(*xp); m = costhe*(*yp); n = sinthe; face = 0; zeta = n; if (l > zeta) { face = 1; zeta = l; } if (m > zeta) { face = 2; zeta = m; } if (-l > zeta) { face = 3; zeta = -l; } if (-m > zeta) { face = 4; zeta = -m; } if (-n > zeta) { face = 5; zeta = -n; } switch (face) { case 1: xi = m; eta = n; x0 = 0.0; y0 = 0.0; break; case 2: xi = -l; eta = n; x0 = 2.0; y0 = 0.0; break; case 3: xi = -m; eta = n; x0 = 4.0; y0 = 0.0; break; case 4: xi = l; eta = n; x0 = 6.0; y0 = 0.0; break; case 5: xi = m; eta = l; x0 = 0.0; y0 = -2.0; break; default: /* face == 0 */ xi = m; eta = -l; x0 = 0.0; y0 = 2.0; break; } chi = xi/zeta; psi = eta/zeta; chi2 = chi*chi; psi2 = psi*psi; chi2co = 1.0 - chi2; psi2co = 1.0 - psi2; /* Avoid floating underflows. */ chipsi = fabs(chi*psi); chi4 = (chi2 > 1.0e-16) ? chi2*chi2 : 0.0; psi4 = (psi2 > 1.0e-16) ? psi2*psi2 : 0.0; chi2psi2 = (chipsi > 1.0e-16) ? chi2*psi2 : 0.0; xf = chi*(chi2 + chi2co*(gstar + psi2*(gamma*chi2co + mm*chi2 + psi2co*(c00 + c10*chi2 + c01*psi2 + c11*chi2psi2 + c20*chi4 + c02*psi4)) + chi2*(omega1 - chi2co*(d0 + d1*chi2)))); yf = psi*(psi2 + psi2co*(gstar + chi2*(gamma*psi2co + mm*psi2 + chi2co*(c00 + c10*psi2 + c01*chi2 + c11*chi2psi2 + c20*psi4 + c02*chi4)) + psi2*(omega1 - psi2co*(d0 + d1*psi2)))); istat = 0; if (fabs(xf) > 1.0) { if (fabs(xf) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("cscs2x"); } xf = copysign(1.0, xf); } if (fabs(yf) > 1.0) { if (fabs(yf) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("cscs2x"); } yf = copysign(1.0, yf); } *xp = prj->w[0]*(xf + x0) - prj->x0; *yp = prj->w[0]*(yf + y0) - prj->y0; *(statp++) = istat; } } return status; } /*============================================================================ * QSC: quadrilaterilized spherical cube projection. * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag QSC * prj->code "QSC" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->w[0] r0*(pi/4) * prj->w[1] (4/pi)/r0 * prj->prjx2s Pointer to qscx2s(). * prj->prjs2x Pointer to qscs2x(). *===========================================================================*/ int qscset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = QSC; strcpy(prj->code, "QSC"); strcpy(prj->name, "quadrilateralized spherical cube"); prj->category = QUADCUBE; prj->pvrange = 0; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 45.0; prj->w[1] = 1.0/45.0; } else { prj->w[0] = prj->r0*PI/4.0; prj->w[1] = 1.0/prj->w[0]; } prj->prjx2s = qscx2s; prj->prjs2x = qscs2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int qscx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int direct, face, mx, my, rowlen, rowoff, status; double cosw, l, m, n, omega, sinw, tau, xf, yf, w, zeco, zeta; const double tol = 1.0e-12; register int ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != QSC) { if ((status = qscset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { xf = (*xp + prj->x0)*prj->w[1]; phip = phi + rowoff; for (iy = 0; iy < my; iy++) { *phip = xf; phip += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yf = (*yp + prj->y0)*prj->w[1]; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { xf = *phip; /* Check bounds. */ if (fabs(xf) <= 1.0) { if (fabs(yf) > 3.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("qscx2s"); continue; } } else { if (fabs(xf) > 7.0 || fabs(yf) > 1.0) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("qscx2s"); continue; } } /* Map negative faces to the other side. */ if (xf < -1.0) xf += 8.0; /* Determine the face. */ if (xf > 5.0) { face = 4; xf -= 6.0; } else if (xf > 3.0) { face = 3; xf -= 4.0; } else if (xf > 1.0) { face = 2; xf -= 2.0; } else if (yf > 1.0) { face = 0; yf -= 2.0; } else if (yf < -1.0) { face = 5; yf += 2.0; } else { face = 1; } direct = (fabs(xf) > fabs(yf)); if (direct) { if (xf == 0.0) { omega = 0.0; tau = 1.0; zeta = 1.0; zeco = 0.0; } else { w = 15.0*yf/xf; omega = sind(w)/(cosd(w) - SQRT2INV); tau = 1.0 + omega*omega; zeco = xf*xf*(1.0 - 1.0/sqrt(1.0 + tau)); zeta = 1.0 - zeco; } } else { if (yf == 0.0) { omega = 0.0; tau = 1.0; zeta = 1.0; zeco = 0.0; } else { w = 15.0*xf/yf; sincosd(w, &sinw, &cosw); omega = sinw/(cosw - SQRT2INV); tau = 1.0 + omega*omega; zeco = yf*yf*(1.0 - 1.0/sqrt(1.0 + tau)); zeta = 1.0 - zeco; } } if (zeta < -1.0) { if (zeta < -1.0-tol) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("qscx2s"); continue; } zeta = -1.0; zeco = 2.0; w = 0.0; } else { w = sqrt(zeco*(2.0-zeco)/tau); } switch (face) { case 1: l = zeta; if (direct) { m = w; if (xf < 0.0) m = -m; n = m*omega; } else { n = w; if (yf < 0.0) n = -n; m = n*omega; } break; case 2: m = zeta; if (direct) { l = w; if (xf > 0.0) l = -l; n = -l*omega; } else { n = w; if (yf < 0.0) n = -n; l = -n*omega; } break; case 3: l = -zeta; if (direct) { m = w; if (xf > 0.0) m = -m; n = -m*omega; } else { n = w; if (yf < 0.0) n = -n; m = -n*omega; } break; case 4: m = -zeta; if (direct) { l = w; if (xf < 0.0) l = -l; n = l*omega; } else { n = w; if (yf < 0.0) n = -n; l = n*omega; } break; case 5: n = -zeta; if (direct) { m = w; if (xf < 0.0) m = -m; l = m*omega; } else { l = w; if (yf < 0.0) l = -l; m = l*omega; } break; default: /* face == 0 */ n = zeta; if (direct) { m = w; if (xf < 0.0) m = -m; l = -m*omega; } else { l = w; if (yf > 0.0) l = -l; m = -l*omega; } break; } if (l == 0.0 && m == 0.0) { *phip = 0.0; } else { *phip = atan2d(m, l); } *thetap = asind(n); *(statp++) = 0; } } return status; } /*--------------------------------------------------------------------------*/ int qscs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int face, mphi, mtheta, rowlen, rowoff, status; double cosphi, costhe, eta, l, m, n, omega, p, sinphi, sinthe, t, tau, x0, xf, xi, y0, yf, zeco, zeta; const double tol = 1.0e-12; register int iphi, istat, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != QSC) { if ((status = qscset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } status = 0; /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { sincosd(*phip, &sinphi, &cosphi); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *xp = cosphi; *yp = sinphi; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sincosd(*thetap, &sinthe, &costhe); for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { if (fabs(*thetap) == 90.0) { *xp = -prj->x0; *yp = copysign(2.0*prj->w[0], *thetap) - prj->y0; *(statp++) = 0; continue; } l = costhe*(*xp); m = costhe*(*yp); n = sinthe; face = 0; zeta = n; if (l > zeta) { face = 1; zeta = l; } if (m > zeta) { face = 2; zeta = m; } if (-l > zeta) { face = 3; zeta = -l; } if (-m > zeta) { face = 4; zeta = -m; } if (-n > zeta) { face = 5; zeta = -n; } zeco = 1.0 - zeta; switch (face) { case 1: xi = m; eta = n; if (zeco < 1.0e-8) { /* Small angle formula. */ t = (*thetap)*D2R; p = atan2(*yp, *xp); zeco = (p*p + t*t)/2.0; } x0 = 0.0; y0 = 0.0; break; case 2: xi = -l; eta = n; if (zeco < 1.0e-8) { /* Small angle formula. */ t = (*thetap)*D2R; p = atan2(*yp, *xp) - PI/2.0; zeco = (p*p + t*t)/2.0; } x0 = 2.0; y0 = 0.0; break; case 3: xi = -m; eta = n; if (zeco < 1.0e-8) { /* Small angle formula. */ t = (*thetap)*D2R; p = atan2(*yp, *xp); p -= copysign(PI, p); zeco = (p*p + t*t)/2.0; } x0 = 4.0; y0 = 0.0; break; case 4: xi = l; eta = n; if (zeco < 1.0e-8) { /* Small angle formula. */ t = (*thetap)*D2R; p = atan2(*yp, *xp) + PI/2.0; zeco = (p*p + t*t)/2.0; } x0 = 6; y0 = 0.0; break; case 5: xi = m; eta = l; if (zeco < 1.0e-8) { /* Small angle formula. */ t = (*thetap + 90.0)*D2R; zeco = t*t/2.0; } x0 = 0.0; y0 = -2; break; default: /* face == 0 */ xi = m; eta = -l; if (zeco < 1.0e-8) { /* Small angle formula. */ t = (90.0 - *thetap)*D2R; zeco = t*t/2.0; } x0 = 0.0; y0 = 2.0; break; } xf = 0.0; yf = 0.0; if (xi != 0.0 || eta != 0.0) { if (-xi > fabs(eta)) { omega = eta/xi; tau = 1.0 + omega*omega; xf = -sqrt(zeco/(1.0 - 1.0/sqrt(1.0+tau))); yf = (xf/15.0)*(atand(omega) - asind(omega/sqrt(tau+tau))); } else if (xi > fabs(eta)) { omega = eta/xi; tau = 1.0 + omega*omega; xf = sqrt(zeco/(1.0 - 1.0/sqrt(1.0+tau))); yf = (xf/15.0)*(atand(omega) - asind(omega/sqrt(tau+tau))); } else if (-eta >= fabs(xi)) { omega = xi/eta; tau = 1.0 + omega*omega; yf = -sqrt(zeco/(1.0 - 1.0/sqrt(1.0+tau))); xf = (yf/15.0)*(atand(omega) - asind(omega/sqrt(tau+tau))); } else if (eta >= fabs(xi)) { omega = xi/eta; tau = 1.0 + omega*omega; yf = sqrt(zeco/(1.0 - 1.0/sqrt(1.0+tau))); xf = (yf/15.0)*(atand(omega) - asind(omega/sqrt(tau+tau))); } } istat = 0; if (fabs(xf) > 1.0) { if (fabs(xf) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("qscs2x"); } xf = copysign(1.0, xf); } if (fabs(yf) > 1.0) { if (fabs(yf) > 1.0+tol) { istat = 1; if (!status) status = PRJERR_BAD_WORLD_SET("qscs2x"); } yf = copysign(1.0, yf); } *xp = prj->w[0]*(xf + x0) - prj->x0; *yp = prj->w[0]*(yf + y0) - prj->y0; *(statp++) = istat; } } return status; } /*============================================================================ * HPX: HEALPix projection. * * Given: * prj->pv[1] H - the number of facets in longitude. * prj->pv[2] K - the number of facets in latitude * * Given and/or returned: * prj->r0 Reset to 180/pi if 0. * prj->phi0 Reset to 0.0 if undefined. * prj->theta0 Reset to 0.0 if undefined. * * Returned: * prj->flag HPX * prj->code "HPX" * prj->x0 Fiducial offset in x. * prj->y0 Fiducial offset in y. * prj->m True if H is odd. * prj->n True if K is odd. * prj->w[0] r0*(pi/180) * prj->w[1] (180/pi)/r0 * prj->w[2] (K-1)/K * prj->w[3] 90*K/H * prj->w[4] (K+1)/2 * prj->w[5] 90*(K-1)/H * prj->w[6] 180/H * prj->w[7] H/360 * prj->w[8] r0*(pi/180)*(90*K/H) * prj->w[9] r0*(pi/180)*(180/H) * prj->prjx2s Pointer to hpxx2s(). * prj->prjs2x Pointer to hpxs2x(). *===========================================================================*/ int hpxset(prj) struct prjprm *prj; { if (prj == 0x0) return PRJERR_NULL_POINTER; prj->flag = HPX; strcpy(prj->code, "HPX"); if (undefined(prj->pv[1])) prj->pv[1] = 4.0; if (undefined(prj->pv[2])) prj->pv[2] = 3.0; strcpy(prj->name, "HEALPix"); prj->category = HEALPIX; prj->pvrange = 102; prj->simplezen = 0; prj->equiareal = 1; prj->conformal = 0; prj->global = 1; prj->divergent = 0; if (prj->pv[1] <= 0.0 || prj->pv[2] <= 0.0) { return PRJERR_BAD_PARAM_SET("hpxset"); } prj->m = ((int)(prj->pv[1]+0.5))%2; prj->n = ((int)(prj->pv[2]+0.5))%2; if (prj->r0 == 0.0) { prj->r0 = R2D; prj->w[0] = 1.0; prj->w[1] = 1.0; } else { prj->w[0] = prj->r0*D2R; prj->w[1] = R2D/prj->r0; } prj->w[2] = (prj->pv[2] - 1.0) / prj->pv[2]; prj->w[3] = 90.0 * prj->pv[2] / prj->pv[1]; prj->w[4] = (prj->pv[2] + 1.0) / 2.0; prj->w[5] = 90.0 * (prj->pv[2] - 1.0) / prj->pv[1]; prj->w[6] = 180.0 / prj->pv[1]; prj->w[7] = prj->pv[1] / 360.0; prj->w[8] = prj->w[3] * prj->w[0]; prj->w[9] = prj->w[6] * prj->w[0]; prj->prjx2s = hpxx2s; prj->prjs2x = hpxs2x; return prjoff(prj, 0.0, 0.0); } /*--------------------------------------------------------------------------*/ int hpxx2s(prj, nx, ny, sxy, spt, x, y, phi, theta, stat) struct prjprm *prj; int nx, ny, sxy, spt; const double x[], y[]; double phi[], theta[]; int stat[]; { int h, mx, my, offset, rowlen, rowoff, status; double absy, s, sigma, t, yr; const double slim = prj->w[6] + 1e-12; const double ylim = prj->w[9] * prj->w[4]; register int istat, ix, iy, *statp; register const double *xp, *yp; register double *phip, *thetap; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != HPX) { if ((status = hpxset(prj))) return status; } if (ny > 0) { mx = nx; my = ny; } else { mx = 1; my = 1; ny = nx; } status = 0; /* Do x dependence. */ xp = x; rowoff = 0; rowlen = nx*spt; for (ix = 0; ix < nx; ix++, rowoff += spt, xp += sxy) { s = prj->w[1] * (*xp + prj->x0); /* x_c for K odd or theta > 0. */ t = -180.0 + (2.0 * floor((*xp + 180.0) * prj->w[7]) + 1.0) * prj->w[6]; t = prj->w[1] * (*xp - t); phip = phi + rowoff; thetap = theta + rowoff; for (iy = 0; iy < my; iy++) { /* theta[] is used to hold (x - x_c). */ *phip = s; *thetap = t; phip += rowlen; thetap += rowlen; } } /* Do y dependence. */ yp = y; phip = phi; thetap = theta; statp = stat; for (iy = 0; iy < ny; iy++, yp += sxy) { yr = prj->w[1]*(*yp + prj->y0); absy = fabs(yr); istat = 0; if (absy <= prj->w[5]) { /* Equatorial regime. */ t = asind(yr/prj->w[3]); for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { *thetap = t; *(statp++) = 0; } } else if (absy <= ylim) { /* Polar regime. */ offset = (prj->n || *yp > 0.0) ? 0 : 1; sigma = prj->w[4] - absy / prj->w[6]; if (sigma == 0.0) { s = 1e9; t = 90.0; } else { t = 1.0 - sigma*sigma/prj->pv[2]; if (t < -1.0) { s = 0.0; t = 0.0; istat = 1; if (!status) status = PRJERR_BAD_PIX_SET("hpxx2s"); } else { s = 1.0/sigma; t = asind(t); } } if (*yp < 0.0) t = -t; for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { if (offset) { /* Offset the southern polar half-facets for even K. */ h = (int)floor(*phip / prj->w[6]) + prj->m; if (h%2) { *thetap -= prj->w[6]; } else { *thetap += prj->w[6]; } } /* Recall that theta[] holds (x - x_c). */ s *= *thetap; if (fabs(s) < slim) { if (s != 0.0) s -= *thetap; *phip += s; *thetap = t; *(statp++) = istat; } else { /* Out-of-bounds. */ *phip = 0.0; *thetap = 0.0; *(statp++) = 1; if (!status) status = PRJERR_BAD_PIX_SET("hpxx2s"); } } } else { /* Beyond latitude range. */ for (ix = 0; ix < mx; ix++, phip += spt, thetap += spt) { *phip = 0.0; *thetap = 0.0; *(statp++) = 1; } if (!status) status = PRJERR_BAD_PIX_SET("hpxx2s"); } } return status; } /*--------------------------------------------------------------------------*/ int hpxs2x(prj, nphi, ntheta, spt, sxy, phi, theta, x, y, stat) struct prjprm *prj; int nphi, ntheta, spt, sxy; const double phi[], theta[]; double x[], y[]; int stat[]; { int h, mphi, mtheta, offset, rowlen, rowoff, status; double abssin, eta, sigma, sinthe, t, xi; register int iphi, itheta, *statp; register const double *phip, *thetap; register double *xp, *yp; /* Initialize. */ if (prj == 0x0) return PRJERR_NULL_POINTER; if (prj->flag != HPX) { if ((status = hpxset(prj))) return status; } if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Do phi dependence. */ phip = phi; rowoff = 0; rowlen = nphi*sxy; for (iphi = 0; iphi < nphi; iphi++, rowoff += sxy, phip += spt) { xi = prj->w[0] * (*phip) - prj->x0; /* phi_c for K odd or theta > 0. */ t = -180.0 + (2.0*floor((*phip+180.0) * prj->w[7]) + 1.0) * prj->w[6]; t = prj->w[0] * (*phip - t); xp = x + rowoff; yp = y + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { /* y[] is used to hold (phi - phi_c). */ *xp = xi; *yp = t; xp += rowlen; yp += rowlen; } } /* Do theta dependence. */ thetap = theta; xp = x; yp = y; statp = stat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sinthe = sind(*thetap); abssin = fabs(sinthe); if (abssin <= prj->w[2]) { /* Equatorial regime. */ eta = prj->w[8] * sinthe - prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { *yp = eta; *(statp++) = 0; } } else { /* Polar regime. */ offset = (prj->n || *thetap > 0.0) ? 0 : 1; sigma = sqrt(prj->pv[2]*(1.0 - abssin)); xi = sigma - 1.0; eta = prj->w[9] * (prj->w[4] - sigma); if (*thetap < 0) eta = -eta; eta -= prj->y0; for (iphi = 0; iphi < mphi; iphi++, xp += sxy, yp += sxy) { if (offset) { /* Offset the southern polar half-facets for even K. */ h = (int)floor((*xp + prj->x0) / prj->w[9]) + prj->m; if (h%2) { *yp -= prj->w[9]; } else { *yp += prj->w[9]; } } /* Recall that y[] holds (phi - phi_c). */ *xp += *yp * xi; *yp = eta; *(statp++) = 0; /* Put the phi = 180 meridian in the expected place. */ if (180.0 < *xp) *xp = 360.0 - *xp; } } } return 0; } pywcs-1.12/wcslib/C/prj.h0000644001153600020070000006631012310355626017265 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: prj.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the spherical map projections * recognized by the FITS World Coordinate System (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of celestial coordinates in FITS", * Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077 (Paper II) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the prj routines * --------------------------- * These routines implement the spherical map projections defined by the FITS * WCS standard. They are based on the prjprm struct which contains all * information needed for the computations. The struct contains some members * that must be set by the user, and others that are maintained by these * routines, somewhat like a C++ class but with no encapsulation. * * Routine prjini() is provided to initialize the prjprm struct with default * values, prjfree() reclaims any memory that may have been allocated to store * an error message, and prjprt() prints its contents. * * Setup routines for each projection with names of the form ???set(), where * "???" is the down-cased three-letter projection code, compute intermediate * values in the prjprm struct from parameters in it that were supplied by the * user. The struct always needs to be set by the projection's setup routine * but that need not be called explicitly - refer to the explanation of * prjprm::flag. * * Each map projection is implemented via separate functions for the spherical * projection, ???s2x(), and deprojection, ???x2s(). * * A set of driver routines, prjset(), prjx2s(), and prjs2x(), provides a * generic interface to the specific projection routines which they invoke * via pointers-to-functions stored in the prjprm struct. * * In summary, the routines are: * - prjini() Initialization routine for the prjprm struct. * - prjprt() Routine to print the prjprm struct. * * - prjset(), prjx2s(), prjs2x(): Generic driver routines * * - azpset(), azpx2s(), azps2x(): AZP (zenithal/azimuthal perspective) * - szpset(), szpx2s(), szps2x(): SZP (slant zenithal perspective) * - tanset(), tanx2s(), tans2x(): TAN (gnomonic) * - stgset(), stgx2s(), stgs2x(): STG (stereographic) * - sinset(), sinx2s(), sins2x(): SIN (orthographic/synthesis) * - arcset(), arcx2s(), arcs2x(): ARC (zenithal/azimuthal equidistant) * - zpnset(), zpnx2s(), zpns2x(): ZPN (zenithal/azimuthal polynomial) * - zeaset(), zeax2s(), zeas2x(): ZEA (zenithal/azimuthal equal area) * - airset(), airx2s(), airs2x(): AIR (Airy) * - cypset(), cypx2s(), cyps2x(): CYP (cylindrical perspective) * - ceaset(), ceax2s(), ceas2x(): CEA (cylindrical equal area) * - carset(), carx2s(), cars2x(): CAR (Plate carree) * - merset(), merx2s(), mers2x(): MER (Mercator) * - sflset(), sflx2s(), sfls2x(): SFL (Sanson-Flamsteed) * - parset(), parx2s(), pars2x(): PAR (parabolic) * - molset(), molx2s(), mols2x(): MOL (Mollweide) * - aitset(), aitx2s(), aits2x(): AIT (Hammer-Aitoff) * - copset(), copx2s(), cops2x(): COP (conic perspective) * - coeset(), coex2s(), coes2x(): COE (conic equal area) * - codset(), codx2s(), cods2x(): COD (conic equidistant) * - cooset(), coox2s(), coos2x(): COO (conic orthomorphic) * - bonset(), bonx2s(), bons2x(): BON (Bonne) * - pcoset(), pcox2s(), pcos2x(): PCO (polyconic) * - tscset(), tscx2s(), tscs2x(): TSC (tangential spherical cube) * - cscset(), cscx2s(), cscs2x(): CSC (COBE spherical cube) * - qscset(), qscx2s(), qscs2x(): QSC (quadrilateralized spherical cube) * - hpxset(), hpxx2s(), hpxs2x(): HPX (HEALPix) * * Argument checking (projection routines): * ---------------------------------------- * The values of phi and theta (the native longitude and latitude) normally lie * in the range [-180,180] for phi, and [-90,90] for theta. However, all * projection routines will accept any value of phi and will not normalize it. * * The projection routines do not explicitly check that theta lies within the * range [-90,90]. They do check for any value of theta that produces an * invalid argument to the projection equations (e.g. leading to division by * zero). The projection routines for AZP, SZP, TAN, SIN, ZPN, and COP also * return error 2 if (phi,theta) corresponds to the overlapped (far) side of * the projection but also return the corresponding value of (x,y). This * strict bounds checking may be relaxed at any time by setting prjprm::bounds * to 0 (rather than 1); the projections need not be reinitialized. * * Argument checking (deprojection routines): * ------------------------------------------ * Error checking on the projected coordinates (x,y) is limited to that * required to ascertain whether a solution exists. Where a solution does * exist no check is made that the value of phi and theta obtained lie within * the ranges [-180,180] for phi, and [-90,90] for theta. * * Accuracy: * --------- * No warranty is given for the accuracy of these routines (refer to the * copyright notice); intending users must satisfy for themselves their * adequacy for the intended purpose. However, closure to a precision of at * least 1E-10 degree of longitude and latitude has been verified for typical * projection parameters on the 1 degree graticule of native longitude and * latitude (to within 5 degrees of any latitude where the projection may * diverge). Refer to the tprj1.c and tprj2.c test routines that accompany * this software. * * * prjini() - Default constructor for the prjprm struct * ---------------------------------------------------- * prjini() sets all members of a prjprm struct to default values. It should * be used to initialize every prjprm struct. * * Returned: * prj struct prjprm* * Projection parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * * * prjfree() - Destructor for the prjprm struct * -------------------------------------------- * prjfree() frees any memory that may have been allocated to store an error * message in the prjprm struct. * * Given: * prj struct prjprm* * Projection parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * * * prjprt() - Print routine for the prjprm struct * ---------------------------------------------- * prjprt() prints the contents of a prjprm struct using wcsprintf(). Mainly * intended for diagnostic purposes. * * Given: * prj const struct prjprm* * Projection parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * * * prjset() - Generic setup routine for the prjprm struct * ------------------------------------------------------ * prjset() sets up a prjprm struct according to information supplied within * it. * * Note that this routine need not be called directly; it will be invoked by * prjx2s() and prjs2x() if prj.flag is anything other than a predefined magic * value. * * The one important distinction between prjset() and the setup routines for * the specific projections is that the projection code must be defined in the * prjprm struct in order for prjset() to identify the required projection. * Once prjset() has initialized the prjprm struct, prjx2s() and prjs2x() use * the pointers to the specific projection and deprojection routines contained * therein. * * Given and returned: * prj struct prjprm* * Projection parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * 2: Invalid projection parameters. * * For returns > 1, a detailed error message is set in * prjprm::err if enabled, see wcserr_enable(). * * * prjx2s() - Generic Cartesian-to-spherical deprojection * ------------------------------------------------------ * Deproject Cartesian (x,y) coordinates in the plane of projection to native * spherical coordinates (phi,theta). * * The projection is that specified by prjprm::code. * * Given and returned: * prj struct prjprm* * Projection parameters. * * Given: * nx,ny int Vector lengths. * * sxy,spt int Vector strides. * * x,y const double[] * Projected coordinates. * * Returned: * phi,theta double[] Longitude and latitude (phi,theta) of the projected * point in native spherical coordinates [deg]. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of (x,y). * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * 2: Invalid projection parameters. * 3: One or more of the (x,y) coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * prjprm::err if enabled, see wcserr_enable(). * * * prjs2x() - Generic spherical-to-Cartesian projection * ---------------------------------------------------- * Project native spherical coordinates (phi,theta) to Cartesian (x,y) * coordinates in the plane of projection. * * The projection is that specified by prjprm::code. * * Given and returned: * prj struct prjprm* * Projection parameters. * * Given: * nphi, * ntheta int Vector lengths. * * spt,sxy int Vector strides. * * phi,theta const double[] * Longitude and latitude (phi,theta) of the projected * point in native spherical coordinates [deg]. * * Returned: * x,y double[] Projected coordinates. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of (phi,theta). * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * 2: Invalid projection parameters. * 4: One or more of the (phi,theta) coordinates * were, invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * prjprm::err if enabled, see wcserr_enable(). * * * ???set() - Specific setup routines for the prjprm struct * -------------------------------------------------------- * Set up a prjprm struct for a particular projection according to information * supplied within it. * * Given and returned: * prj struct prjprm* * Projection parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * 2: Invalid projection parameters. * * For returns > 1, a detailed error message is set in * prjprm::err if enabled, see wcserr_enable(). * * * ???x2s() - Specific Cartesian-to-spherical deprojection routines * ---------------------------------------------------------------- * Transform (x,y) coordinates in the plane of projection to native spherical * coordinates (phi,theta). * * Given and returned: * prj struct prjprm* * Projection parameters. * * Given: * nx,ny int Vector lengths. * * sxy,spt int Vector strides. * * x,y const double[] * Projected coordinates. * * Returned: * phi,theta double[] Longitude and latitude of the projected point in * native spherical coordinates [deg]. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of (x,y). * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * 2: Invalid projection parameters. * 3: One or more of the (x,y) coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * prjprm::err if enabled, see wcserr_enable(). * * * ???s2x() - Specific spherical-to-Cartesian projection routines *--------------------------------------------------------------- * Transform native spherical coordinates (phi,theta) to (x,y) coordinates in * the plane of projection. * * Given and returned: * prj struct prjprm* * Projection parameters. * * Given: * nphi, * ntheta int Vector lengths. * * spt,sxy int Vector strides. * * phi,theta const double[] * Longitude and latitude of the projected point in * native spherical coordinates [deg]. * * Returned: * x,y double[] Projected coordinates. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of (phi,theta). * * Function return value: * int Status return value: * 0: Success. * 1: Null prjprm pointer passed. * 2: Invalid projection parameters. * 4: One or more of the (phi,theta) coordinates * were, invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * prjprm::err if enabled, see wcserr_enable(). * * * prjprm struct - Projection parameters * ------------------------------------- * The prjprm struct contains all information needed to project or deproject * native spherical coordinates. It consists of certain members that must be * set by the user ("given") and others that are set by the WCSLIB routines * ("returned"). Some of the latter are supplied for informational purposes * while others are for internal use only. * * int flag * (Given and returned) This flag must be set to zero whenever any of the * following prjprm struct members are set or changed: * * - prjprm::code, * - prjprm::r0, * - prjprm::pv[], * - prjprm::phi0, * - prjprm::theta0. * * This signals the initialization routine (prjset() or ???set()) to * recompute the returned members of the prjprm struct. flag will then be * reset to indicate that this has been done. * * Note that flag need not be reset when prjprm::bounds is changed. * * char code[4] * (Given) Three-letter projection code defined by the FITS standard. * * double r0 * (Given) The radius of the generating sphere for the projection, a linear * scaling parameter. If this is zero, it will be reset to its default * value of 180/pi (the value for FITS WCS). * * double pv[30] * (Given) Projection parameters. These correspond to the PVi_ma keywords * in FITS, so pv[0] is PVi_0a, pv[1] is PVi_1a, etc., where i denotes the * latitude-like axis. Many projections use pv[1] (PVi_1a), some also use * pv[2] (PVi_2a) and SZP uses pv[3] (PVi_3a). ZPN is currently the only * projection that uses any of the others. * * Usage of the pv[] array as it applies to each projection is described in * the prologue to each trio of projection routines in prj.c. * * double phi0 * (Given) The native longitude, phi_0 [deg], and ... * double theta0 * (Given) ... the native latitude, theta_0 [deg], of the reference point, * i.e. the point (x,y) = (0,0). If undefined (set to a magic value by * prjini()) the initialization routine will set this to a * projection-specific default. * * int bounds * (Given) Controls strict bounds checking for the AZP, SZP, TAN, SIN, ZPN, * and COP projections; set to zero to disable checking. * * The remaining members of the prjprm struct are maintained by the setup * routines and must not be modified elsewhere: * * char name[40] * (Returned) Long name of the projection. * * Provided for information only, not used by the projection routines. * * int category * (Returned) Projection category matching the value of the relevant global * variable: * * - ZENITHAL, * - CYLINDRICAL, * - PSEUDOCYLINDRICAL, * - CONVENTIONAL, * - CONIC, * - POLYCONIC, * - QUADCUBE, and * - HEALPIX. * * The category name may be identified via the prj_categories character * array, e.g. * = struct prjprm prj; = ... = printf("%s\n", prj_categories[prj.category]); * * Provided for information only, not used by the projection routines. * * int pvrange * (Returned) Range of projection parameter indices: 100 times the first * allowed index plus the number of parameters, e.g. TAN is 0 (no * parameters), SZP is 103 (1 to 3), and ZPN is 30 (0 to 29). * * Provided for information only, not used by the projection routines. * * int simplezen * (Returned) True if the projection is a radially-symmetric zenithal * projection. * * Provided for information only, not used by the projection routines. * * int equiareal * (Returned) True if the projection is equal area. * * Provided for information only, not used by the projection routines. * * int conformal * (Returned) True if the projection is conformal. * * Provided for information only, not used by the projection routines. * * int global * (Returned) True if the projection can represent the whole sphere in a * finite, non-overlapped mapping. * * Provided for information only, not used by the projection routines. * * int divergent * (Returned) True if the projection diverges in latitude. * * Provided for information only, not used by the projection routines. * * double x0 * (Returned) The offset in x, and ... * double y0 * (Returned) ... the offset in y used to force (x,y) = (0,0) at * (phi_0,theta_0). * * struct wcserr *err * (Returned) If enabled, when an error status is returned this struct * contains detailed information about the error, see wcserr_enable(). * * void *padding * (An unused variable inserted for alignment purposes only.) * * double w[10] * (Returned) Intermediate floating-point values derived from the * projection parameters, cached here to save recomputation. * * Usage of the w[] array as it applies to each projection is described in * the prologue to each trio of projection routines in prj.c. * * int n * (Returned) Intermediate integer value (used only for the ZPN and HPX * projections). * * int (*prjx2s)(PRJX2S_ARGS) * (Returned) Pointer to the projection ... * int (*prjs2x)(PRJ_ARGS) * (Returned) ... and deprojection routines. * * * Global variable: const char *prj_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_PROJ #define WCSLIB_PROJ #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif /* Total number of projection parameters; 0 to PVN-1. */ #define PVN 30 extern const char *prj_errmsg[]; enum prj_errmsg_enum { PRJERR_SUCCESS = 0, /* Success. */ PRJERR_NULL_POINTER = 1, /* Null prjprm pointer passed. */ PRJERR_BAD_PARAM = 2, /* Invalid projection parameters. */ PRJERR_BAD_PIX = 3, /* One or more of the (x, y) coordinates were invalid. */ PRJERR_BAD_WORLD = 4 /* One or more of the (phi, theta) coordinates were invalid. */ }; extern const int CONIC, CONVENTIONAL, CYLINDRICAL, POLYCONIC, PSEUDOCYLINDRICAL, QUADCUBE, ZENITHAL, HEALPIX; extern const char prj_categories[9][32]; extern const int prj_ncode; extern const char prj_codes[27][4]; #ifdef PRJX2S_ARGS #undef PRJX2S_ARGS #endif #ifdef PRJS2X_ARGS #undef PRJS2X_ARGS #endif /* For use in declaring deprojection function prototypes. */ #define PRJX2S_ARGS struct prjprm *prj, int nx, int ny, int sxy, int spt, \ const double x[], const double y[], double phi[], double theta[], int stat[] /* For use in declaring projection function prototypes. */ #define PRJS2X_ARGS struct prjprm *prj, int nx, int ny, int sxy, int spt, \ const double phi[], const double theta[], double x[], double y[], int stat[] struct prjprm { /* Initialization flag (see the prologue above). */ /*------------------------------------------------------------------------*/ int flag; /* Set to zero to force initialization. */ /* Parameters to be provided (see the prologue above). */ /*------------------------------------------------------------------------*/ char code[4]; /* Three-letter projection code. */ double r0; /* Radius of the generating sphere. */ double pv[PVN]; /* Projection parameters. */ double phi0, theta0; /* Fiducial native coordinates. */ int bounds; /* Enable strict bounds checking. */ /* Information derived from the parameters supplied. */ /*------------------------------------------------------------------------*/ char name[40]; /* Projection name. */ int category; /* Projection category. */ int pvrange; /* Range of projection parameter indices. */ int simplezen; /* Is it a simple zenithal projection? */ int equiareal; /* Is it an equal area projection? */ int conformal; /* Is it a conformal projection? */ int global; /* Can it map the whole sphere? */ int divergent; /* Does the projection diverge in latitude? */ double x0, y0; /* Fiducial offsets. */ /* Error handling */ /*------------------------------------------------------------------------*/ struct wcserr *err; /* Private */ /*------------------------------------------------------------------------*/ void *padding; /* (Dummy inserted for alignment purposes.) */ double w[10]; /* Intermediate values. */ int m, n; /* Intermediate values. */ int (*prjx2s)(PRJX2S_ARGS); /* Pointers to the spherical projection and */ int (*prjs2x)(PRJS2X_ARGS); /* deprojection functions. */ }; /* Size of the prjprm struct in int units, used by the Fortran wrappers. */ #define PRJLEN (sizeof(struct prjprm)/sizeof(int)) /* Use the preprocessor to help declare function prototypes (see above). */ int prjini(struct prjprm *prj); int prjfree(struct prjprm *prj); int prjprt(const struct prjprm *prj); int prjset(struct prjprm *prj); int prjx2s(PRJX2S_ARGS); int prjs2x(PRJS2X_ARGS); int azpset(struct prjprm *prj); int azpx2s(PRJX2S_ARGS); int azps2x(PRJS2X_ARGS); int szpset(struct prjprm *prj); int szpx2s(PRJX2S_ARGS); int szps2x(PRJS2X_ARGS); int tanset(struct prjprm *prj); int tanx2s(PRJX2S_ARGS); int tans2x(PRJS2X_ARGS); int stgset(struct prjprm *prj); int stgx2s(PRJX2S_ARGS); int stgs2x(PRJS2X_ARGS); int sinset(struct prjprm *prj); int sinx2s(PRJX2S_ARGS); int sins2x(PRJS2X_ARGS); int arcset(struct prjprm *prj); int arcx2s(PRJX2S_ARGS); int arcs2x(PRJS2X_ARGS); int zpnset(struct prjprm *prj); int zpnx2s(PRJX2S_ARGS); int zpns2x(PRJS2X_ARGS); int zeaset(struct prjprm *prj); int zeax2s(PRJX2S_ARGS); int zeas2x(PRJS2X_ARGS); int airset(struct prjprm *prj); int airx2s(PRJX2S_ARGS); int airs2x(PRJS2X_ARGS); int cypset(struct prjprm *prj); int cypx2s(PRJX2S_ARGS); int cyps2x(PRJS2X_ARGS); int ceaset(struct prjprm *prj); int ceax2s(PRJX2S_ARGS); int ceas2x(PRJS2X_ARGS); int carset(struct prjprm *prj); int carx2s(PRJX2S_ARGS); int cars2x(PRJS2X_ARGS); int merset(struct prjprm *prj); int merx2s(PRJX2S_ARGS); int mers2x(PRJS2X_ARGS); int sflset(struct prjprm *prj); int sflx2s(PRJX2S_ARGS); int sfls2x(PRJS2X_ARGS); int parset(struct prjprm *prj); int parx2s(PRJX2S_ARGS); int pars2x(PRJS2X_ARGS); int molset(struct prjprm *prj); int molx2s(PRJX2S_ARGS); int mols2x(PRJS2X_ARGS); int aitset(struct prjprm *prj); int aitx2s(PRJX2S_ARGS); int aits2x(PRJS2X_ARGS); int copset(struct prjprm *prj); int copx2s(PRJX2S_ARGS); int cops2x(PRJS2X_ARGS); int coeset(struct prjprm *prj); int coex2s(PRJX2S_ARGS); int coes2x(PRJS2X_ARGS); int codset(struct prjprm *prj); int codx2s(PRJX2S_ARGS); int cods2x(PRJS2X_ARGS); int cooset(struct prjprm *prj); int coox2s(PRJX2S_ARGS); int coos2x(PRJS2X_ARGS); int bonset(struct prjprm *prj); int bonx2s(PRJX2S_ARGS); int bons2x(PRJS2X_ARGS); int pcoset(struct prjprm *prj); int pcox2s(PRJX2S_ARGS); int pcos2x(PRJS2X_ARGS); int tscset(struct prjprm *prj); int tscx2s(PRJX2S_ARGS); int tscs2x(PRJS2X_ARGS); int cscset(struct prjprm *prj); int cscx2s(PRJX2S_ARGS); int cscs2x(PRJS2X_ARGS); int qscset(struct prjprm *prj); int qscx2s(PRJX2S_ARGS); int qscs2x(PRJS2X_ARGS); int hpxset(struct prjprm *prj); int hpxx2s(PRJX2S_ARGS); int hpxs2x(PRJS2X_ARGS); /* Deprecated. */ #define prjini_errmsg prj_errmsg #define prjprt_errmsg prj_errmsg #define prjset_errmsg prj_errmsg #define prjx2s_errmsg prj_errmsg #define prjs2x_errmsg prj_errmsg #ifdef __cplusplus } #endif #endif /* WCSLIB_PROJ */ pywcs-1.12/wcslib/C/spc.c0000644001153600020070000010527112310355626017252 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: spc.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsprintf.h" #include "wcstrig.h" #include "wcsutil.h" #include "spc.h" #include "spx.h" /* Spectral algorithm codes. */ #define F2S 100; /* Axis linear in frequency. */ #define W2S 200; /* Axis linear in vacuum wavelengths. */ #define A2S 300; /* Axis linear in air wavelengths. */ #define V2S 400; /* Axis linear in velocity. */ #define GRI 500; /* Grism in vacuum. */ #define GRA 600; /* Grism in air. */ /* S-type spectral variables. */ #define FREQ 0; /* Frequency-like. */ #define AFRQ 1; /* Frequency-like. */ #define ENER 2; /* Frequency-like. */ #define WAVN 3; /* Frequency-like. */ #define VRAD 4; /* Frequency-like. */ #define WAVE 10; /* Vacuum wavelength-like. */ #define VOPT 11; /* Vacuum wavelength-like. */ #define ZOPT 12; /* Vacuum wavelength-like. */ #define AWAV 20; /* Air wavelength-like. */ #define VELO 30; /* Velocity-like. */ #define BETA 31; /* Velocity-like. */ /* Map status return value to message. */ const char *spc_errmsg[] = { "Success", "Null spcprm pointer passed", "Invalid spectral parameters", "One or more of x coordinates were invalid", "One or more of the spec coordinates were invalid"}; /* Convenience macro for invoking wcserr_set(). */ #define SPC_ERRMSG(status) WCSERR_SET(status), spc_errmsg[status] #define C 2.99792458e8 /*--------------------------------------------------------------------------*/ int spcini(struct spcprm *spc) { register int k; if (spc == 0x0) return SPCERR_NULL_POINTER; spc->flag = 0; strcpy(spc->type, " "); strcpy(spc->code, " "); spc->crval = UNDEFINED; spc->restfrq = 0.0; spc->restwav = 0.0; for (k = 0; k < 7; k++) { spc->pv[k] = UNDEFINED; } for (k = 0; k < 6; k++) { spc->w[k] = 0.0; } spc->isGrism = 0; spc->err = 0x0; spc->spxX2P = 0x0; spc->spxP2S = 0x0; spc->spxS2P = 0x0; spc->spxP2X = 0x0; return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcfree(spc) struct spcprm *spc; { if (spc == 0x0) return SPCERR_NULL_POINTER; if (spc->err) free(spc->err); spc->err = 0x0; return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcprt(const struct spcprm *spc) { char hext[32]; int i; if (spc == 0x0) return SPCERR_NULL_POINTER; wcsprintf(" flag: %d\n", spc->flag); wcsprintf(" type: \"%s\"\n", spc->type); wcsprintf(" code: \"%s\"\n", spc->code); if (undefined(spc->crval)) { wcsprintf(" crval: UNDEFINED\n"); } else { wcsprintf(" crval: %- 11.4g\n", spc->crval); } wcsprintf(" restfrq: %f\n", spc->restfrq); wcsprintf(" restwav: %f\n", spc->restwav); wcsprintf(" pv:"); if (spc->isGrism) { for (i = 0; i < 5; i++) { if (undefined(spc->pv[i])) { wcsprintf(" UNDEFINED "); } else { wcsprintf(" %- 11.4g", spc->pv[i]); } } wcsprintf("\n "); for (i = 5; i < 7; i++) { if (undefined(spc->pv[i])) { wcsprintf(" UNDEFINED "); } else { wcsprintf(" %- 11.4g", spc->pv[i]); } } wcsprintf("\n"); } else { wcsprintf(" (not used)\n"); } wcsprintf(" w:"); for (i = 0; i < 3; i++) { wcsprintf(" %- 11.4g", spc->w[i]); } if (spc->isGrism) { wcsprintf("\n "); for (i = 3; i < 6; i++) { wcsprintf(" %- 11.4g", spc->w[i]); } wcsprintf("\n"); } else { wcsprintf(" (remainder unused)\n"); } wcsprintf(" isGrism: %d\n", spc->isGrism); WCSPRINTF_PTR(" err: ", spc->err, "\n"); if (spc->err) { wcserr_prt(spc->err, " "); } wcsprintf(" spxX2P: %s\n", wcsutil_fptr2str((int (*)())spc->spxX2P, hext)); wcsprintf(" spxP2S: %s\n", wcsutil_fptr2str((int (*)())spc->spxP2S, hext)); wcsprintf(" spxS2P: %s\n", wcsutil_fptr2str((int (*)())spc->spxS2P, hext)); wcsprintf(" spxP2X: %s\n", wcsutil_fptr2str((int (*)())spc->spxP2X, hext)); return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcset(struct spcprm *spc) { static const char *function = "spcset"; char ctype[9], ptype, xtype; int restreq, status; double alpha, beta_r, crvalX, dn_r, dXdS, epsilon, G, m, lambda_r, n_r, t, restfrq, restwav, theta; struct wcserr **err; if (spc == 0x0) return SPCERR_NULL_POINTER; err = &(spc->err); if (undefined(spc->crval)) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Spectral crval is undefined"); } spc->type[4] = '\0'; spc->code[3] = '\0'; spc->w[0] = 0.0; /* Analyse the spectral axis type. */ sprintf(ctype, "%s-%s", spc->type, spc->code); restfrq = spc->restfrq; restwav = spc->restwav; if ((status = spcspxe(ctype, spc->crval, restfrq, restwav, &ptype, &xtype, &restreq, &crvalX, &dXdS, &(spc->err)))) { return status; } /* Satisfy rest frequency/wavelength requirements. */ if (restreq) { if (restreq == 3 && restfrq == 0.0 && restwav == 0.0) { /* VRAD-V2F, VOPT-V2W, and ZOPT-V2W require the rest frequency or */ /* wavelength for the S-P and P-X transformations but not for S-X */ /* so supply a phoney value. */ restwav = 1.0; } if (restfrq == 0.0) { restfrq = C/restwav; } else { restwav = C/restfrq; } if (ptype == 'F') { spc->w[0] = restfrq; } else if (ptype != 'V') { spc->w[0] = restwav; } else { if (xtype == 'F') { spc->w[0] = restfrq; } else { spc->w[0] = restwav; } } } spc->w[1] = crvalX; spc->w[2] = dXdS; /* Set pointers-to-functions for the linear part of the transformation. */ if (ptype == 'F') { if (strcmp(spc->type, "FREQ") == 0) { /* Frequency. */ spc->flag = FREQ; spc->spxP2S = 0x0; spc->spxS2P = 0x0; } else if (strcmp(spc->type, "AFRQ") == 0) { /* Angular frequency. */ spc->flag = AFRQ; spc->spxP2S = freqafrq; spc->spxS2P = afrqfreq; } else if (strcmp(spc->type, "ENER") == 0) { /* Photon energy. */ spc->flag = ENER; spc->spxP2S = freqener; spc->spxS2P = enerfreq; } else if (strcmp(spc->type, "WAVN") == 0) { /* Wave number. */ spc->flag = WAVN; spc->spxP2S = freqwavn; spc->spxS2P = wavnfreq; } else if (strcmp(spc->type, "VRAD") == 0) { /* Radio velocity. */ spc->flag = VRAD; spc->spxP2S = freqvrad; spc->spxS2P = vradfreq; } } else if (ptype == 'W') { if (strcmp(spc->type, "WAVE") == 0) { /* Vacuum wavelengths. */ spc->flag = WAVE; spc->spxP2S = 0x0; spc->spxS2P = 0x0; } else if (strcmp(spc->type, "VOPT") == 0) { /* Optical velocity. */ spc->flag = VOPT; spc->spxP2S = wavevopt; spc->spxS2P = voptwave; } else if (strcmp(spc->type, "ZOPT") == 0) { /* Redshift. */ spc->flag = ZOPT; spc->spxP2S = wavezopt; spc->spxS2P = zoptwave; } } else if (ptype == 'A') { if (strcmp(spc->type, "AWAV") == 0) { /* Air wavelengths. */ spc->flag = AWAV; spc->spxP2S = 0x0; spc->spxS2P = 0x0; } } else if (ptype == 'V') { if (strcmp(spc->type, "VELO") == 0) { /* Relativistic velocity. */ spc->flag = VELO; spc->spxP2S = 0x0; spc->spxS2P = 0x0; } else if (strcmp(spc->type, "BETA") == 0) { /* Velocity ratio (v/c). */ spc->flag = BETA; spc->spxP2S = velobeta; spc->spxS2P = betavelo; } } /* Set pointers-to-functions for the non-linear part of the spectral */ /* transformation. */ spc->isGrism = 0; if (xtype == 'F') { /* Axis is linear in frequency. */ if (ptype == 'F') { spc->spxX2P = 0x0; spc->spxP2X = 0x0; } else if (ptype == 'W') { spc->spxX2P = freqwave; spc->spxP2X = wavefreq; } else if (ptype == 'A') { spc->spxX2P = freqawav; spc->spxP2X = awavfreq; } else if (ptype == 'V') { spc->spxX2P = freqvelo; spc->spxP2X = velofreq; } spc->flag += F2S; } else if (xtype == 'W' || xtype == 'w') { /* Axis is linear in vacuum wavelengths. */ if (ptype == 'F') { spc->spxX2P = wavefreq; spc->spxP2X = freqwave; } else if (ptype == 'W') { spc->spxX2P = 0x0; spc->spxP2X = 0x0; } else if (ptype == 'A') { spc->spxX2P = waveawav; spc->spxP2X = awavwave; } else if (ptype == 'V') { spc->spxX2P = wavevelo; spc->spxP2X = velowave; } if (xtype == 'W') { spc->flag += W2S; } else { /* Grism in vacuum. */ spc->isGrism = 1; spc->flag += GRI; } } else if (xtype == 'A' || xtype == 'a') { /* Axis is linear in air wavelengths. */ if (ptype == 'F') { spc->spxX2P = awavfreq; spc->spxP2X = freqawav; } else if (ptype == 'W') { spc->spxX2P = awavwave; spc->spxP2X = waveawav; } else if (ptype == 'A') { spc->spxX2P = 0x0; spc->spxP2X = 0x0; } else if (ptype == 'V') { spc->spxX2P = awavvelo; spc->spxP2X = veloawav; } if (xtype == 'A') { spc->flag += A2S; } else { /* Grism in air. */ spc->isGrism = 2; spc->flag += GRA; } } else if (xtype == 'V') { /* Axis is linear in relativistic velocity. */ if (ptype == 'F') { spc->spxX2P = velofreq; spc->spxP2X = freqvelo; } else if (ptype == 'W') { spc->spxX2P = velowave; spc->spxP2X = wavevelo; } else if (ptype == 'A') { spc->spxX2P = veloawav; spc->spxP2X = awavvelo; } else if (ptype == 'V') { spc->spxX2P = 0x0; spc->spxP2X = 0x0; } spc->flag += V2S; } /* Check for grism axes. */ if (spc->isGrism) { /* Axis is linear in "grism parameter"; work in wavelength. */ lambda_r = crvalX; /* Set defaults. */ if (undefined(spc->pv[0])) spc->pv[0] = 0.0; if (undefined(spc->pv[1])) spc->pv[1] = 0.0; if (undefined(spc->pv[2])) spc->pv[2] = 0.0; if (undefined(spc->pv[3])) spc->pv[3] = 1.0; if (undefined(spc->pv[4])) spc->pv[4] = 0.0; if (undefined(spc->pv[5])) spc->pv[5] = 0.0; if (undefined(spc->pv[6])) spc->pv[6] = 0.0; /* Compute intermediaries. */ G = spc->pv[0]; m = spc->pv[1]; alpha = spc->pv[2]; n_r = spc->pv[3]; dn_r = spc->pv[4]; epsilon = spc->pv[5]; theta = spc->pv[6]; t = G*m/cosd(epsilon); beta_r = asind(t*lambda_r - n_r*sind(alpha)); t -= dn_r*sind(alpha); spc->w[1] = -tand(theta); spc->w[2] *= t / (cosd(beta_r)*cosd(theta)*cosd(theta)); spc->w[3] = beta_r + theta; spc->w[4] = (n_r - dn_r*lambda_r)*sind(alpha); spc->w[5] = 1.0 / t; } return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcx2s( struct spcprm *spc, int nx, int sx, int sspec, const double x[], double spec[], int stat[]) { static const char *function = "spcx2s"; int statP2S, status = SPCERR_SUCCESS, statX2P; double beta; register int ix; register int *statp; register const double *xp; register double *specp; struct wcserr **err; /* Initialize. */ if (spc == 0x0) return SPCERR_NULL_POINTER; err = &(spc->err); if (spc->flag == 0) { if ((status = spcset(spc))) return status; } /* Convert intermediate world coordinate x to X. */ xp = x; specp = spec; statp = stat; for (ix = 0; ix < nx; ix++, xp += sx, specp += sspec) { *specp = spc->w[1] + (*xp)*spc->w[2]; *(statp++) = 0; } /* If X is the grism parameter then convert it to wavelength. */ if (spc->isGrism) { specp = spec; for (ix = 0; ix < nx; ix++, specp += sspec) { beta = atand(*specp) + spc->w[3]; *specp = (sind(beta) + spc->w[4]) * spc->w[5]; } } /* Apply the non-linear step of the algorithm chain to convert the */ /* X-type spectral variable to P-type intermediate spectral variable. */ if (spc->spxX2P) { if ((statX2P = spc->spxX2P(spc->w[0], nx, sspec, sspec, spec, spec, stat))) { if (statX2P == SPXERR_BAD_INSPEC_COORD) { status = SPCERR_BAD_X; } else if (statX2P == SPXERR_BAD_SPEC_PARAMS) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral parameters: Frequency or wavelength is 0"); } else { return wcserr_set(SPC_ERRMSG(statX2P)); } } } /* Apply the linear step of the algorithm chain to convert P-type */ /* intermediate spectral variable to the required S-type variable. */ if (spc->spxP2S) { if ((statP2S = spc->spxP2S(spc->w[0], nx, sspec, sspec, spec, spec, stat))) { if (statP2S == SPXERR_BAD_INSPEC_COORD) { status = SPCERR_BAD_X; } else if (statP2S == SPXERR_BAD_SPEC_PARAMS) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral parameters: Frequency or wavelength is 0"); } else { return wcserr_set(SPC_ERRMSG(statP2S)); } } } if (status) { wcserr_set(SPC_ERRMSG(status)); } return status; } /*--------------------------------------------------------------------------*/ int spcs2x( struct spcprm *spc, int nspec, int sspec, int sx, const double spec[], double x[], int stat[]) { static const char *function = "spcs2x"; int statP2X, status = SPCERR_SUCCESS, statS2P; double beta, s; register int ispec; register int *statp; register const double *specp; register double *xp; struct wcserr **err; /* Initialize. */ if (spc == 0x0) return SPCERR_NULL_POINTER; err = &(spc->err); if (spc->flag == 0) { if ((status = spcset(spc))) return status; } /* Apply the linear step of the algorithm chain to convert the S-type */ /* spectral variable to P-type intermediate spectral variable. */ if (spc->spxS2P) { if ((statS2P = spc->spxS2P(spc->w[0], nspec, sspec, sx, spec, x, stat))) { if (statS2P == SPXERR_BAD_INSPEC_COORD) { status = SPCERR_BAD_SPEC; } else if (statS2P == SPXERR_BAD_SPEC_PARAMS) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral parameters: Frequency or wavelength is 0"); } else { return wcserr_set(SPC_ERRMSG(statS2P)); } } } else { /* Just a copy. */ xp = x; specp = spec; statp = stat; for (ispec = 0; ispec < nspec; ispec++, specp += sspec, xp += sx) { *xp = *specp; *(statp++) = 0; } } /* Apply the non-linear step of the algorithm chain to convert P-type */ /* intermediate spectral variable to X-type spectral variable. */ if (spc->spxP2X) { if ((statP2X = spc->spxP2X(spc->w[0], nspec, sx, sx, x, x, stat))) { if (statP2X == SPCERR_BAD_SPEC) { status = SPCERR_BAD_SPEC; } else if (statP2X == SPXERR_BAD_SPEC_PARAMS) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral parameters: Frequency or wavelength is 0"); } else { return wcserr_set(SPC_ERRMSG(statP2X)); } } } if (spc->isGrism) { /* Convert X-type spectral variable (wavelength) to grism parameter. */ xp = x; statp = stat; for (ispec = 0; ispec < nspec; ispec++, xp += sx, statp++) { if (*statp) continue; s = *xp/spc->w[5] - spc->w[4]; if (fabs(s) <= 1.0) { beta = asind(s); *xp = tand(beta - spc->w[3]); } else { *statp = 1; } } } /* Convert X-type spectral variable to intermediate world coordinate x. */ xp = x; statp = stat; for (ispec = 0; ispec < nspec; ispec++, xp += sx) { if (*(statp++)) continue; *xp -= spc->w[1]; *xp /= spc->w[2]; } if (status) { wcserr_set(SPC_ERRMSG(status)); } return status; } /*--------------------------------------------------------------------------*/ int spctyp( const char ctypei[9], char stype[], char scode[], char sname[], char units[], char *ptype, char *xtype, int *restreq) { return spctype( ctypei, stype, scode, sname, units, ptype, xtype, restreq, NULL); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spctype( const char ctypei[9], char stype[], char scode[], char sname[], char units[], char *ptype, char *xtype, int *restreq, struct wcserr **err) { static const char *function = "spctype"; char ctype[9], ptype_t, sname_t[32], units_t[8], xtype_t; int restreq_t = 0; /* Copy with blank padding. */ sprintf(ctype, "%-8.8s", ctypei); ctype[8] = '\0'; /* Validate the S-type spectral variable. */ if (strncmp(ctype, "FREQ", 4) == 0) { strcpy(sname_t, "Frequency"); strcpy(units_t, "Hz"); ptype_t = 'F'; } else if (strncmp(ctype, "AFRQ", 4) == 0) { strcpy(sname_t, "Angular frequency"); strcpy(units_t, "rad/s"); ptype_t = 'F'; } else if (strncmp(ctype, "ENER", 4) == 0) { strcpy(sname_t, "Photon energy"); strcpy(units_t, "J"); ptype_t = 'F'; } else if (strncmp(ctype, "WAVN", 4) == 0) { strcpy(sname_t, "Wavenumber"); strcpy(units_t, "/m"); ptype_t = 'F'; } else if (strncmp(ctype, "VRAD", 4) == 0) { strcpy(sname_t, "Radio velocity"); strcpy(units_t, "m/s"); ptype_t = 'F'; restreq_t = 1; } else if (strncmp(ctype, "WAVE", 4) == 0) { strcpy(sname_t, "Vacuum wavelength"); strcpy(units_t, "m"); ptype_t = 'W'; } else if (strncmp(ctype, "VOPT", 4) == 0) { strcpy(sname_t, "Optical velocity"); strcpy(units_t, "m/s"); ptype_t = 'W'; restreq_t = 1; } else if (strncmp(ctype, "ZOPT", 4) == 0) { strcpy(sname_t, "Redshift"); strcpy(units_t, ""); ptype_t = 'W'; restreq_t = 1; } else if (strncmp(ctype, "AWAV", 4) == 0) { strcpy(sname_t, "Air wavelength"); strcpy(units_t, "m"); ptype_t = 'A'; } else if (strncmp(ctype, "VELO", 4) == 0) { strcpy(sname_t, "Relativistic velocity"); strcpy(units_t, "m/s"); ptype_t = 'V'; } else if (strncmp(ctype, "BETA", 4) == 0) { strcpy(sname_t, "Velocity ratio (v/c)"); strcpy(units_t, ""); ptype_t = 'V'; } else { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Unknown spectral type '%s'", ctype); } /* Determine X-type and validate the spectral algorithm code. */ if ((xtype_t = ctype[5]) == ' ') { /* The algorithm code must be completely blank. */ if (strcmp(ctype+4, " ") != 0) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral algorithm '%s'", ctype+4); } xtype_t = ptype_t; } else if (ctype[4] != '-') { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral type '%s'", ctype); } else if (strcmp(ctype+5, "LOG") == 0 || strcmp(ctype+5, "TAB") == 0) { /* Logarithmic or tabular axis, not linear in any spectral type. */ } else if (xtype_t == 'G') { /* Validate the algorithm code. */ if (ctype[6] != 'R') { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral algorithm '%s'", xtype_t); } /* Grism coordinates... */ if (ctype[7] == 'I') { /* ...in vacuum. */ xtype_t = 'w'; } else if (ctype[7] == 'A') { /* ...in air. */ xtype_t = 'a'; } else { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral algorithm '%s'", xtype_t); } } else if (ctype[6] != '2') { /* Algorithm code has invalid syntax. */ return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Invalid spectral algorithm syntax '%s'", xtype_t); } else if (ctype[7] != ptype_t && ctype[7] != '?') { /* The P-, and S-type variables are inconsistent. */ return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "In spectral type '%s', P- and S-type variables are inconsistent", ctype); } else if (ctype[7] == ctype[5]) { /* Degenerate algorithm code. */ sprintf(ctype+4, " "); } /* Rest freq/wavelength required for transformation between P and X? */ if (strchr("FWAwa", (int)xtype_t)) { if (ptype_t == 'V') { restreq_t += 2; } } else if (xtype_t == 'V') { if (strchr("FWAwa", (int)ptype_t)) { restreq_t += 2; } } else if (strchr("LT", (int)xtype_t) == 0) { /* Invalid X-type variable code. */ return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "In spectral type '%s', invalid X-type variable code", ctype); } /* Copy results. */ if (stype) { strncpy(stype, ctype, 4); stype[4] = '\0'; } if (scode) strcpy(scode, ctype+5); if (sname) strcpy(sname, sname_t); if (units) strcpy(units, units_t); if (ptype) *ptype = ptype_t; if (xtype) *xtype = xtype_t; if (restreq) *restreq = restreq_t; return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcspx( const char ctypeS[9], double crvalS, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalX, double *dXdS) { return spcspxe(ctypeS, crvalS, restfrq, restwav, ptype, xtype, restreq, crvalX, dXdS, 0x0); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spcspxe( const char ctypeS[9], double crvalS, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalX, double *dXdS, struct wcserr **err) { static const char *function = "spcspxe"; char scode[4], stype[5], type[8]; int status; double dPdS, dXdP; struct spxprm spx; /* Analyse the spectral axis code. */ if ((status = spctype(ctypeS, stype, scode, 0x0, 0x0, ptype, xtype, restreq, err))) { return status; } if (strstr("LT", xtype)) { /* Can't handle logarithmic or tabular coordinates. */ return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Can't handle logarithmic or tabular coordinates"); } /* Do we have rest frequency and/or wavelength as required? */ if ((*restreq)%3 && restfrq == 0.0 && restwav == 0.0) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Missing required rest frequency or wavelength"); } /* Compute all spectral parameters and their derivatives. */ strcpy(type, stype); spx.err = (err ? *err : 0x0); if ((status = specx(type, crvalS, restfrq, restwav, &spx))) { status = SPCERR_BAD_SPEC_PARAMS; if (err) { (*err)->status = status; } else { free(spx.err); } return status; } /* Transform S-P (linear) and P-X (non-linear). */ dPdS = 0.0; dXdP = 0.0; if (*ptype == 'F') { if (strcmp(stype, "FREQ") == 0) { dPdS = 1.0; } else if (strcmp(stype, "AFRQ") == 0) { dPdS = spx.dfreqafrq; } else if (strcmp(stype, "ENER") == 0) { dPdS = spx.dfreqener; } else if (strcmp(stype, "WAVN") == 0) { dPdS = spx.dfreqwavn; } else if (strcmp(stype, "VRAD") == 0) { dPdS = spx.dfreqvrad; } if (*xtype == 'F') { *crvalX = spx.freq; dXdP = 1.0; } else if (*xtype == 'W' || *xtype == 'w') { *crvalX = spx.wave; dXdP = spx.dwavefreq; } else if (*xtype == 'A' || *xtype == 'a') { *crvalX = spx.awav; dXdP = spx.dawavfreq; } else if (*xtype == 'V') { *crvalX = spx.velo; dXdP = spx.dvelofreq; } } else if (*ptype == 'W' || *ptype == 'w') { if (strcmp(stype, "WAVE") == 0) { dPdS = 1.0; } else if (strcmp(stype, "VOPT") == 0) { dPdS = spx.dwavevopt; } else if (strcmp(stype, "ZOPT") == 0) { dPdS = spx.dwavezopt; } if (*xtype == 'F') { *crvalX = spx.freq; dXdP = spx.dfreqwave; } else if (*xtype == 'W' || *xtype == 'w') { *crvalX = spx.wave; dXdP = 1.0; } else if (*xtype == 'A' || *xtype == 'a') { *crvalX = spx.awav; dXdP = spx.dawavwave; } else if (*xtype == 'V') { *crvalX = spx.velo; dXdP = spx.dvelowave; } } else if (*ptype == 'A' || *ptype == 'a') { if (strcmp(stype, "AWAV") == 0) { dPdS = 1.0; } if (*xtype == 'F') { *crvalX = spx.freq; dXdP = spx.dfreqawav; } else if (*xtype == 'W' || *xtype == 'w') { *crvalX = spx.wave; dXdP = spx.dwaveawav; } else if (*xtype == 'A' || *xtype == 'a') { *crvalX = spx.awav; dXdP = 1.0; } else if (*xtype == 'V') { *crvalX = spx.velo; dXdP = spx.dveloawav; } } else if (*ptype == 'V') { if (strcmp(stype, "VELO") == 0) { dPdS = 1.0; } else if (strcmp(stype, "BETA") == 0) { dPdS = spx.dvelobeta; } if (*xtype == 'F') { *crvalX = spx.freq; dXdP = spx.dfreqvelo; } else if (*xtype == 'W' || *xtype == 'w') { *crvalX = spx.wave; dXdP = spx.dwavevelo; } else if (*xtype == 'A' || *xtype == 'a') { *crvalX = spx.awav; dXdP = spx.dawavvelo; } else if (*xtype == 'V') { *crvalX = spx.velo; dXdP = 1.0; } } *dXdS = dXdP * dPdS; return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcxps( const char ctypeS[9], double crvalX, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalS, double *dSdX) { return spcxpse(ctypeS, crvalX, restfrq, restwav, ptype, xtype, restreq, crvalS, dSdX, NULL); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spcxpse( const char ctypeS[9], double crvalX, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalS, double *dSdX, struct wcserr **err) { static const char *function = "spcxpse"; char scode[4], stype[5], type[8]; int status; double dPdX, dSdP; struct spxprm spx; /* Analyse the spectral axis type. */ if ((status = spctype(ctypeS, stype, scode, 0x0, 0x0, ptype, xtype, restreq, err))) { return status; } if (strstr("LT", xtype)) { /* Can't handle logarithmic or tabular coordinates. */ return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Can't handle logarithmic or tabular coordinates"); } /* Do we have rest frequency and/or wavelength as required? */ if ((*restreq)%3 && restfrq == 0.0 && restwav == 0.0) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Missing required rest frequency or wavelength"); } /* Compute all spectral parameters and their derivatives. */ if (*xtype == 'F') { strcpy(type, "FREQ"); } else if (*xtype == 'W' || *xtype == 'w') { strcpy(type, "WAVE"); } else if (*xtype == 'A' || *xtype == 'a') { strcpy(type, "AWAV"); } else if (*xtype == 'V') { strcpy(type, "VELO"); } spx.err = (err ? *err : 0x0); if (specx(type, crvalX, restfrq, restwav, &spx)) { status = SPCERR_BAD_SPEC_PARAMS; if (err) { (*err)->status = status; } else { free(spx.err); } return status; } /* Transform X-P (non-linear) and P-S (linear). */ dPdX = 0.0; dSdP = 0.0; if (*ptype == 'F') { if (*xtype == 'F') { dPdX = 1.0; } else if (*xtype == 'W' || *xtype == 'w') { dPdX = spx.dfreqwave; } else if (*xtype == 'A' || *xtype == 'a') { dPdX = spx.dfreqawav; } else if (*xtype == 'V') { dPdX = spx.dfreqvelo; } if (strcmp(stype, "FREQ") == 0) { *crvalS = spx.freq; dSdP = 1.0; } else if (strcmp(stype, "AFRQ") == 0) { *crvalS = spx.afrq; dSdP = spx.dafrqfreq; } else if (strcmp(stype, "ENER") == 0) { *crvalS = spx.ener; dSdP = spx.denerfreq; } else if (strcmp(stype, "WAVN") == 0) { *crvalS = spx.wavn; dSdP = spx.dwavnfreq; } else if (strcmp(stype, "VRAD") == 0) { *crvalS = spx.vrad; dSdP = spx.dvradfreq; } } else if (*ptype == 'W') { if (*xtype == 'F') { dPdX = spx.dwavefreq; } else if (*xtype == 'W' || *xtype == 'w') { dPdX = 1.0; } else if (*xtype == 'A' || *xtype == 'a') { dPdX = spx.dwaveawav; } else if (*xtype == 'V') { dPdX = spx.dwavevelo; } if (strcmp(stype, "WAVE") == 0) { *crvalS = spx.wave; dSdP = 1.0; } else if (strcmp(stype, "VOPT") == 0) { *crvalS = spx.vopt; dSdP = spx.dvoptwave; } else if (strcmp(stype, "ZOPT") == 0) { *crvalS = spx.zopt; dSdP = spx.dzoptwave; } } else if (*ptype == 'A') { if (*xtype == 'F') { dPdX = spx.dawavfreq; } else if (*xtype == 'W' || *xtype == 'w') { dPdX = spx.dawavwave; } else if (*xtype == 'A' || *xtype == 'a') { dPdX = 1.0; } else if (*xtype == 'V') { dPdX = spx.dawavvelo; } if (strcmp(stype, "AWAV") == 0) { *crvalS = spx.awav; dSdP = 1.0; } } else if (*ptype == 'V') { if (*xtype == 'F') { dPdX = spx.dvelofreq; } else if (*xtype == 'W' || *xtype == 'w') { dPdX = spx.dvelowave; } else if (*xtype == 'A' || *xtype == 'a') { dPdX = spx.dveloawav; } else if (*xtype == 'V') { dPdX = 1.0; } if (strcmp(stype, "VELO") == 0) { *crvalS = spx.velo; dSdP = 1.0; } else if (strcmp(stype, "BETA") == 0) { *crvalS = spx.beta; dSdP = spx.dbetavelo; } } *dSdX = dSdP * dPdX; return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spctrn( const char ctypeS1[9], double crvalS1, double cdeltS1, double restfrq, double restwav, char ctypeS2[9], double *crvalS2, double *cdeltS2) { return spctrne(ctypeS1, crvalS1, cdeltS1, restfrq, restwav, ctypeS2, crvalS2, cdeltS2, NULL); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spctrne( const char ctypeS1[9], double crvalS1, double cdeltS1, double restfrq, double restwav, char ctypeS2[9], double *crvalS2, double *cdeltS2, struct wcserr **err) { static const char *function = "spctrne"; char *cp, ptype1, ptype2, xtype1, xtype2; int restreq, status; double crvalX, dS2dX, dXdS1; if ((status = spcspxe(ctypeS1, crvalS1, restfrq, restwav, &ptype1, &xtype1, &restreq, &crvalX, &dXdS1, err))) { return status; } /* Blank fill. */ ctypeS2[8] = '\0'; for (cp = ctypeS2; *cp; cp++); while (cp < ctypeS2+8) *(cp++) = ' '; if (strncmp(ctypeS2+5, "???", 3) == 0) { /* Set the algorithm code if required. */ if (xtype1 == 'w') { strcpy(ctypeS2+5, "GRI"); } else if (xtype1 == 'a') { strcpy(ctypeS2+5, "GRA"); } else { ctypeS2[5] = xtype1; ctypeS2[6] = '2'; } } if ((status = spcxpse(ctypeS2, crvalX, restfrq, restwav, &ptype2, &xtype2, &restreq, crvalS2, &dS2dX, err))) { return status; } /* Are the X-types compatible? */ if (xtype2 != xtype1) { return wcserr_set(WCSERR_SET(SPCERR_BAD_SPEC_PARAMS), "Incompatible X-types '%c' and '%c'", xtype1, xtype2); } if (ctypeS2[7] == '?') { if (ptype2 == xtype2) { strcpy(ctypeS2+4, " "); } else { ctypeS2[7] = ptype2; } } *cdeltS2 = dS2dX * dXdS1 * cdeltS1; return SPCERR_SUCCESS; } /*--------------------------------------------------------------------------*/ int spcaips( const char ctypeA[9], int velref, char ctype[9], char specsys[9]) { const char *frames[] = {"LSRK", "BARYCENT", "TOPOCENT", "LSRD", "GEOCENTR", "SOURCE", "GALACTOC"}; char *fcode; int ivf, status; /* Make a null-filled copy of ctypeA. */ if (ctype != ctypeA) strncpy(ctype, ctypeA, 8); ctype[8] = '\0'; wcsutil_null_fill(9, ctype); *specsys = '\0'; /* Is it a recognized AIPS-convention type? */ status = SPCERR_NO_CHANGE; if (strncmp(ctype, "FREQ", 4) == 0 || strncmp(ctype, "VELO", 4) == 0 || strncmp(ctype, "FELO", 4) == 0) { /* Look for the Doppler frame. */ if (*(fcode = ctype+4)) { if (strcmp(fcode, "-LSR") == 0) { strcpy(specsys, "LSRK"); } else if (strcmp(fcode, "-HEL") == 0) { strcpy(specsys, "BARYCENT"); } else if (strcmp(fcode, "-OBS") == 0) { strcpy(specsys, "TOPOCENT"); } else { /* Not a recognized AIPS spectral type. */ return SPCERR_NO_CHANGE; } *fcode = '\0'; status = SPCERR_SUCCESS; } /* VELREF takes precedence if present. */ ivf = velref%256; if (0 < ivf && ivf <= 7) { strcpy(specsys, frames[ivf-1]); status = SPCERR_SUCCESS; } else if (ivf) { status = SPCERR_BAD_SPEC_PARAMS; } if (strcmp(ctype, "VELO") == 0) { /* Check that we found an AIPS-convention Doppler frame. */ if (*specsys) { /* 'VELO' in AIPS means radio or optical depending on VELREF. */ ivf = velref/256; if (ivf == 0) { strcpy(ctype, "VOPT"); } else if (ivf == 1) { strcpy(ctype, "VRAD"); } else { status = SPCERR_BAD_SPEC_PARAMS; } } } else if (strcmp(ctype, "FELO") == 0) { /* Uniform in frequency but expressed as an optical velocity (strictly we should also have found an AIPS-convention Doppler frame). */ strcpy(ctype, "VOPT-F2W"); if (status < 0) status = SPCERR_SUCCESS; } } return status; } pywcs-1.12/wcslib/C/spc.h0000644001153600020070000011301412310355626017251 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: spc.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the spectral coordinate systems * recognized by the FITS World Coordinate System (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the spc routines * --------------------------- * These routines implement the part of the FITS WCS standard that deals with * spectral coordinates. They define methods to be used for computing spectral * world coordinates from intermediate world coordinates (a linear * transformation of image pixel coordinates), and vice versa. They are based * on the spcprm struct which contains all information needed for the * computations. The struct contains some members that must be set by the * user, and others that are maintained by these routines, somewhat like a * C++ class but with no encapsulation. * * Routine spcini() is provided to initialize the spcprm struct with default * values, spcfree() reclaims any memory that may have been allocated to store * an error message, and spcprt() prints its contents. * * A setup routine, spcset(), computes intermediate values in the spcprm struct * from parameters in it that were supplied by the user. The struct always * needs to be set up by spcset() but it need not be called explicitly - refer * to the explanation of spcprm::flag. * * spcx2s() and spcs2x() implement the WCS spectral coordinate transformations. * In fact, they are high level driver routines for the lower level spectral * coordinate transformation routines described in spx.h. * * A number of routines are provided to aid in analysing or synthesising sets * of FITS spectral axis keywords: * * - spctype() checks a spectral CTYPEia keyword for validity and returns * information derived from it. * * - Spectral keyword analysis routine spcspxe() computes the values of the * X-type spectral variables for the S-type variables supplied. * * - Spectral keyword synthesis routine, spcxpse(), computes the S-type * variables for the X-types supplied. * * - Given a set of spectral keywords, a translation routine, spctrne(), * produces the corresponding set for the specified spectral CTYPEia. * * - spcaips() translates AIPS-convention spectral CTYPEia and VELREF * keyvalues. * * Spectral variable types - S, P, and X: * -------------------------------------- * A few words of explanation are necessary regarding spectral variable types * in FITS. * * Every FITS spectral axis has three associated spectral variables: * * S-type: the spectral variable in which coordinates are to be * expressed. Each S-type is encoded as four characters and is * linearly related to one of four basic types as follows: * * F: frequency * 'FREQ': frequency * 'AFRQ': angular frequency * 'ENER': photon energy * 'WAVN': wave number * 'VRAD': radio velocity * * W: wavelength in vacuo * 'WAVE': wavelength * 'VOPT': optical velocity * 'ZOPT': redshift * * A: wavelength in air * 'AWAV': wavelength in air * * V: velocity * 'VELO': relativistic velocity * 'BETA': relativistic beta factor * * The S-type forms the first four characters of the CTYPEia keyvalue, * and CRVALia and CDELTia are expressed as S-type quantities so that * they provide a first-order approximation to the S-type variable at * the reference point. * * Note that 'AFRQ', angular frequency, is additional to the variables * defined in WCS Paper III. * * P-type: the basic spectral variable (F, W, A, or V) with which the * S-type variable is associated (see list above). * * For non-grism axes, the P-type is encoded as the eighth character of * CTYPEia. * * X-type: the basic spectral variable (F, W, A, or V) for which the * spectral axis is linear, grisms excluded (see below). * * For non-grism axes, the X-type is encoded as the sixth character of * CTYPEia. * * Grisms: Grism axes have normal S-, and P-types but the axis is linear, * not in any spectral variable, but in a special "grism parameter". * The X-type spectral variable is either W or A for grisms in vacuo or * air respectively, but is encoded as 'w' or 'a' to indicate that an * additional transformation is required to convert to or from the * grism parameter. The spectral algorithm code for grisms also has a * special encoding in CTYPEia, either 'GRI' (in vacuo) or 'GRA' (in air). * * In the algorithm chain, the non-linear transformation occurs between the * X-type and the P-type variables; the transformation between P-type and * S-type variables is always linear. * * When the P-type and X-type variables are the same, the spectral axis is * linear in the S-type variable and the second four characters of CTYPEia * are blank. This can never happen for grism axes. * * As an example, correlating radio spectrometers always produce spectra that * are regularly gridded in frequency; a redshift scale on such a spectrum is * non-linear. The required value of CTYPEia would be 'ZOPT-F2W', where the * desired S-type is 'ZOPT' (redshift), the P-type is necessarily 'W' * (wavelength), and the X-type is 'F' (frequency) by the nature of the * instrument. * * Argument checking: * ------------------ * The input spectral values are only checked for values that would result in * floating point exceptions. In particular, negative frequencies and * wavelengths are allowed, as are velocities greater than the speed of * light. The same is true for the spectral parameters - rest frequency and * wavelength. * * Accuracy: * --------- * No warranty is given for the accuracy of these routines (refer to the * copyright notice); intending users must satisfy for themselves their * adequacy for the intended purpose. However, closure effectively to within * double precision rounding error was demonstrated by test routine tspc.c * which accompanies this software. * * * spcini() - Default constructor for the spcprm struct * ---------------------------------------------------- * spcini() sets all members of a spcprm struct to default values. It should * be used to initialize every spcprm struct. * * Given and returned: * spc struct spcprm* * Spectral transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null spcprm pointer passed. * * * spcfree() - Destructor for the spcprm struct * -------------------------------------------- * spcfree() frees any memory that may have been allocated to store an error * message in the spcprm struct. * * Given: * spc struct spcprm* * Spectral transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null spcprm pointer passed. * * * spcprt() - Print routine for the spcprm struct * ---------------------------------------------- * spcprt() prints the contents of a spcprm struct using wcsprintf(). Mainly * intended for diagnostic purposes. * * Given: * spc const struct spcprm* * Spectral transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null spcprm pointer passed. * * * spcset() - Setup routine for the spcprm struct * ---------------------------------------------- * spcset() sets up a spcprm struct according to information supplied within * it. * * Note that this routine need not be called directly; it will be invoked by * spcx2s() and spcs2x() if spcprm::flag is anything other than a predefined * magic value. * * Given and returned: * spc struct spcprm* * Spectral transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null spcprm pointer passed. * 2: Invalid spectral parameters. * * For returns > 1, a detailed error message is set in * spcprm::err if enabled, see wcserr_enable(). * * * spcx2s() - Transform to spectral coordinates * -------------------------------------------- * spcx2s() transforms intermediate world coordinates to spectral coordinates. * * Given and returned: * spc struct spcprm* * Spectral transformation parameters. * * Given: * nx int Vector length. * * sx int Vector stride. * * sspec int Vector stride. * * x const double[] * Intermediate world coordinates, in SI units. * * Returned: * spec double[] Spectral coordinates, in SI units. * * stat int[] Status return value status for each vector element: * 0: Success. * 1: Invalid value of x. * * Function return value: * int Status return value: * 0: Success. * 1: Null spcprm pointer passed. * 2: Invalid spectral parameters. * 3: One or more of the x coordinates were invalid, * as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * spcprm::err if enabled, see wcserr_enable(). * * * spcs2x() - Transform spectral coordinates * ----------------------------------------- * spcs2x() transforms spectral world coordinates to intermediate world * coordinates. * * Given and returned: * spc struct spcprm* * Spectral transformation parameters. * * Given: * nspec int Vector length. * * sspec int Vector stride. * * sx int Vector stride. * * spec const double[] * Spectral coordinates, in SI units. * * Returned: * x double[] Intermediate world coordinates, in SI units. * * stat int[] Status return value status for each vector element: * 0: Success. * 1: Invalid value of spec. * * Function return value: * int Status return value: * 0: Success. * 1: Null spcprm pointer passed. * 2: Invalid spectral parameters. * 4: One or more of the spec coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * spcprm::err if enabled, see wcserr_enable(). * * * spctype() - Spectral CTYPEia keyword analysis * --------------------------------------------- * spctype() checks whether a CTYPEia keyvalue is a valid spectral axis type * and if so returns information derived from it relating to the associated S-, * P-, and X-type spectral variables (see explanation above). * * The return arguments are guaranteed not be modified if CTYPEia is not a * valid spectral type; zero-pointers may be specified for any that are not of * interest. * * A deprecated form of this function, spctyp(), lacks the wcserr** parameter. * * Given: * ctype const char[9] * The CTYPEia keyvalue, (eight characters with null * termination). * * Returned: * stype char[] The four-letter name of the S-type spectral variable * copied or translated from ctype. If a non-zero * pointer is given, the array must accomodate a null- * terminated string of length 5. * * scode char[] The three-letter spectral algorithm code copied or * translated from ctype. Logarithmic ('LOG') and * tabular ('TAB') codes are also recognized. If a * non-zero pointer is given, the array must accomodate a * null-terminated string of length 4. * * sname char[] Descriptive name of the S-type spectral variable. * If a non-zero pointer is given, the array must * accomodate a null-terminated string of length 22. * * units char[] SI units of the S-type spectral variable. If a * non-zero pointer is given, the array must accomodate a * null-terminated string of length 8. * * ptype char* Character code for the P-type spectral variable * derived from ctype, one of 'F', 'W', 'A', or 'V'. * * xtype char* Character code for the X-type spectral variable * derived from ctype, one of 'F', 'W', 'A', or 'V'. * Also, 'w' and 'a' are synonymous to 'W' and 'A' for * grisms in vacuo and air respectively. Set to 'L' or * 'T' for logarithmic ('LOG') and tabular ('TAB') axes. * * restreq int* Multivalued flag that indicates whether rest * frequency or wavelength is required to compute * spectral variables for this CTYPEia: * 0: Not required. * 1: Required for the conversion between S- and * P-types (e.g. 'ZOPT-F2W'). * 2: Required for the conversion between P- and * X-types (e.g. 'BETA-W2V'). * 3: Required for the conversion between S- and * P-types, and between P- and X-types, but not * between S- and X-types (this applies only for * 'VRAD-V2F', 'VOPT-V2W', and 'ZOPT-V2W'). * Thus the rest frequency or wavelength is required for * spectral coordinate computations (i.e. between S- and * X-types) only if restreq%3 != 0. * * err struct wcserr ** * For function return values > 1, this struct will * contain a detailed error message. May be NULL if an * error message is not desired. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters (not a spectral * CTYPEia). * * * spcspxe() - Spectral keyword analysis * ------------------------------------ * spcspxe() analyses the CTYPEia and CRVALia FITS spectral axis keyword values * and returns information about the associated X-type spectral variable. * * A deprecated form of this function, spcspx(), lacks the wcserr** parameter. * * Given: * ctypeS const char[9] * Spectral axis type, i.e. the CTYPEia keyvalue, (eight * characters with null termination). For non-grism * axes, the character code for the P-type spectral * variable in the algorithm code (i.e. the eighth * character of CTYPEia) may be set to '?' (it will not * be reset). * * crvalS double Value of the S-type spectral variable at the reference * point, i.e. the CRVALia keyvalue, SI units. * * restfrq, * restwav double Rest frequency [Hz] and rest wavelength in vacuo [m], * only one of which need be given, the other should be * set to zero. Neither are required if the translation * is between wave-characteristic types, or between * velocity-characteristic types. E.g., required for * 'FREQ' -> 'ZOPT-F2W', but not required for * 'VELO-F2V' -> 'ZOPT-F2W'. * * Returned: * ptype char* Character code for the P-type spectral variable * derived from ctypeS, one of 'F', 'W', 'A', or 'V'. * * xtype char* Character code for the X-type spectral variable * derived from ctypeS, one of 'F', 'W', 'A', or 'V'. * Also, 'w' and 'a' are synonymous to 'W' and 'A' for * grisms in vacuo and air respectively; crvalX and dXdS * (see below) will conform to these. * * restreq int* Multivalued flag that indicates whether rest frequency * or wavelength is required to compute spectral * variables for this CTYPEia, as for spctype(). * * crvalX double* Value of the X-type spectral variable at the reference * point, SI units. * * dXdS double* The derivative, dX/dS, evaluated at the reference * point, SI units. Multiply the CDELTia keyvalue by * this to get the pixel spacing in the X-type spectral * coordinate. * * err struct wcserr ** * For function return values > 1, this struct will * contain a detailed error message. May be NULL if an * error message is not desired. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters. * * * spcxpse() - Spectral keyword synthesis * ------------------------------------- * spcxpse(), for the spectral axis type specified and the value provided for * the X-type spectral variable at the reference point, deduces the value of * the FITS spectral axis keyword CRVALia and also the derivative dS/dX which * may be used to compute CDELTia. See above for an explanation of the S-, * P-, and X-type spectral variables. * * A deprecated form of this function, spcxps(), lacks the wcserr** parameter. * * Given: * ctypeS const char[9] * The required spectral axis type, i.e. the CTYPEia * keyvalue, (eight characters with null termination). * For non-grism axes, the character code for the P-type * spectral variable in the algorithm code (i.e. the * eighth character of CTYPEia) may be set to '?' (it * will not be reset). * * crvalX double Value of the X-type spectral variable at the reference * point (N.B. NOT the CRVALia keyvalue), SI units. * * restfrq, * restwav double Rest frequency [Hz] and rest wavelength in vacuo [m], * only one of which need be given, the other should be * set to zero. Neither are required if the translation * is between wave-characteristic types, or between * velocity-characteristic types. E.g., required for * 'FREQ' -> 'ZOPT-F2W', but not required for * 'VELO-F2V' -> 'ZOPT-F2W'. * * Returned: * ptype char* Character code for the P-type spectral variable * derived from ctypeS, one of 'F', 'W', 'A', or 'V'. * * xtype char* Character code for the X-type spectral variable * derived from ctypeS, one of 'F', 'W', 'A', or 'V'. * Also, 'w' and 'a' are synonymous to 'W' and 'A' for * grisms; crvalX and cdeltX must conform to these. * * restreq int* Multivalued flag that indicates whether rest frequency * or wavelength is required to compute spectral * variables for this CTYPEia, as for spctype(). * * crvalS double* Value of the S-type spectral variable at the reference * point (i.e. the appropriate CRVALia keyvalue), SI * units. * * dSdX double* The derivative, dS/dX, evaluated at the reference * point, SI units. Multiply this by the pixel spacing * in the X-type spectral coordinate to get the CDELTia * keyvalue. * * err struct wcserr ** * For function return values > 1, this struct will * contain a detailed error message. May be NULL if an * error message is not desired. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters. * * * spctrne() - Spectral keyword translation * --------------------------------------- * spctrne() translates a set of FITS spectral axis keywords into the * corresponding set for the specified spectral axis type. For example, a * 'FREQ' axis may be translated into 'ZOPT-F2W' and vice versa. * * A deprecated form of this function, spctrn(), lacks the wcserr** parameter. * * Given: * ctypeS1 const char[9] * Spectral axis type, i.e. the CTYPEia keyvalue, (eight * characters with null termination). For non-grism * axes, the character code for the P-type spectral * variable in the algorithm code (i.e. the eighth * character of CTYPEia) may be set to '?' (it will not * be reset). * * crvalS1 double Value of the S-type spectral variable at the reference * point, i.e. the CRVALia keyvalue, SI units. * * cdeltS1 double Increment of the S-type spectral variable at the * reference point, SI units. * * restfrq, * restwav double Rest frequency [Hz] and rest wavelength in vacuo [m], * only one of which need be given, the other should be * set to zero. Neither are required if the translation * is between wave-characteristic types, or between * velocity-characteristic types. E.g., required for * 'FREQ' -> 'ZOPT-F2W', but not required for * 'VELO-F2V' -> 'ZOPT-F2W'. * * Given and returned: * ctypeS2 char[9] Required spectral axis type (eight characters with * null termination). The first four characters are * required to be given and are never modified. The * remaining four, the algorithm code, are completely * determined by, and must be consistent with, ctypeS1 * and the first four characters of ctypeS2. A non-zero * status value will be returned if they are inconsistent * (see below). However, if the final three characters * are specified as "???", or if just the eighth * character is specified as '?', the correct algorithm * code will be substituted (applies for grism axes as * well as non-grism). * * Returned: * crvalS2 double* Value of the new S-type spectral variable at the * reference point, i.e. the new CRVALia keyvalue, SI * units. * * cdeltS2 double* Increment of the new S-type spectral variable at the * reference point, i.e. the new CDELTia keyvalue, SI * units. * * err struct wcserr ** * For function return values > 1, this struct will * contain a detailed error message. May be NULL if an * error message is not desired. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters. * * A status value of 2 will be returned if restfrq or * restwav are not specified when required, or if ctypeS1 * or ctypeS2 are self-inconsistent, or have different * spectral X-type variables. * * * spcaips() - Translate AIPS-convention spectral keywords * ------------------------------------------------------- * spcaips() translates AIPS-convention spectral CTYPEia and VELREF keyvalues. * * Given: * ctypeA const char[9] * CTYPEia keyvalue possibly containing an * AIPS-convention spectral code (eight characters, need * not be null-terminated). * * velref int AIPS-convention VELREF code. It has the following * integer values: * 1: LSR kinematic, originally described simply as * "LSR" without distinction between the kinematic * and dynamic definitions. * 2: Barycentric, originally described as "HEL" * meaning heliocentric. * 3: Topocentric, originally described as "OBS" * meaning geocentric but widely interpreted as * topocentric. * AIPS++ extensions to VELREF are also recognized: * 4: LSR dynamic. * 5: Geocentric. * 6: Source rest frame. * 7: Galactocentric. * * For an AIPS 'VELO' axis, a radio convention velocity * (VRAD) is denoted by adding 256 to VELREF, otherwise * an optical velocity (VOPT) is indicated (this is not * applicable to 'FREQ' or 'FELO' axes). Setting velref * to 0 or 256 chooses between optical and radio velocity * without specifying a Doppler frame, provided that a * frame is encoded in ctypeA. If not, i.e. for * ctypeA = 'VELO', ctype will be returned as 'VELO'. * * VELREF takes precedence over CTYPEia in defining the * Doppler frame, e.g. * = ctypeA = 'VELO-HEL' = velref = 1 * * returns ctype = 'VOPT' with specsys set to 'LSRK'. * * Returned: * ctype char[9] Translated CTYPEia keyvalue, or a copy of ctypeA if no * translation was performed (in which case any trailing * blanks in ctypeA will be replaced with nulls). * * specsys char[9] Doppler reference frame indicated by VELREF or else * by CTYPEia with value corresponding to the SPECSYS * keyvalue in the FITS WCS standard. May be returned * blank if neither specifies a Doppler frame, e.g. * ctypeA = 'FELO' and velref%256 == 0. * * Function return value: * int Status return value: * -1: No translation required (not an error). * 0: Success. * 2: Invalid value of VELREF. * * * spcprm struct - Spectral transformation parameters * -------------------------------------------------- * The spcprm struct contains information required to transform spectral * coordinates. It consists of certain members that must be set by the user * ("given") and others that are set by the WCSLIB routines ("returned"). Some * of the latter are supplied for informational purposes while others are for * internal use only. * * int flag * (Given and returned) This flag must be set to zero whenever any of the * following spcprm structure members are set or changed: * * - spcprm::type, * - spcprm::code, * - spcprm::crval, * - spcprm::restfrq, * - spcprm::restwav, * - spcprm::pv[]. * * This signals the initialization routine, spcset(), to recompute the * returned members of the spcprm struct. spcset() will reset flag to * indicate that this has been done. * * char type[8] * (Given) Four-letter spectral variable type, e.g "ZOPT" for * CTYPEia = 'ZOPT-F2W'. (Declared as char[8] for alignment reasons.) * * char code[4] * (Given) Three-letter spectral algorithm code, e.g "F2W" for * CTYPEia = 'ZOPT-F2W'. * * double crval * (Given) Reference value (CRVALia), SI units. * * double restfrq * (Given) The rest frequency [Hz], and ... * * double restwav * (Given) ... the rest wavelength in vacuo [m], only one of which need be * given, the other should be set to zero. Neither are required if the * X and S spectral variables are both wave-characteristic, or both * velocity-characteristic, types. * * double pv[7] * (Given) Grism parameters for 'GRI' and 'GRA' algorithm codes: * - 0: G, grating ruling density. * - 1: m, interference order. * - 2: alpha, angle of incidence [deg]. * - 3: n_r, refractive index at the reference wavelength, lambda_r. * - 4: n'_r, dn/dlambda at the reference wavelength, lambda_r (/m). * - 5: epsilon, grating tilt angle [deg]. * - 6: theta, detector tilt angle [deg]. * * The remaining members of the spcprm struct are maintained by spcset() and * must not be modified elsewhere: * * double w[6] * (Returned) Intermediate values: * - 0: Rest frequency or wavelength (SI). * - 1: The value of the X-type spectral variable at the reference point * (SI units). * - 2: dX/dS at the reference point (SI units). * The remainder are grism intermediates. * * int isGrism * (Returned) Grism coordinates? * - 0: no, * - 1: in vacuum, * - 2: in air. * * int padding1 * (An unused variable inserted for alignment purposes only.) * * struct wcserr *err * (Returned) If enabled, when an error status is returned this structure * contains detailed information about the error, see wcserr_enable(). * * void *padding2 * (An unused variable inserted for alignment purposes only.) * int (*spxX2P)(SPX_ARGS) * (Returned) The first and ... * int (*spxP2S)(SPX_ARGS) * (Returned) ... the second of the pointers to the transformation * functions in the two-step algorithm chain X -> P -> S in the * pixel-to-spectral direction where the non-linear transformation is from * X to P. The argument list, SPX_ARGS, is defined in spx.h. * * int (*spxS2P)(SPX_ARGS) * (Returned) The first and ... * int (*spxP2X)(SPX_ARGS) * (Returned) ... the second of the pointers to the transformation * functions in the two-step algorithm chain S -> P -> X in the * spectral-to-pixel direction where the non-linear transformation is from * P to X. The argument list, SPX_ARGS, is defined in spx.h. * * * Global variable: const char *spc_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_SPC #define WCSLIB_SPC #include "spx.h" #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif extern const char *spc_errmsg[]; enum spc_errmsg_enum { SPCERR_NO_CHANGE = -1, /* No change. */ SPCERR_SUCCESS = 0, /* Success. */ SPCERR_NULL_POINTER = 1, /* Null spcprm pointer passed. */ SPCERR_BAD_SPEC_PARAMS = 2, /* Invalid spectral parameters. */ SPCERR_BAD_X = 3, /* One or more of x coordinates were invalid. */ SPCERR_BAD_SPEC = 4 /* One or more of the spec coordinates were invalid. */ }; struct spcprm { /* Initialization flag (see the prologue above). */ /*------------------------------------------------------------------------*/ int flag; /* Set to zero to force initialization. */ /* Parameters to be provided (see the prologue above). */ /*------------------------------------------------------------------------*/ char type[8]; /* Four-letter spectral variable type. */ char code[4]; /* Three-letter spectral algorithm code. */ double crval; /* Reference value (CRVALia), SI units. */ double restfrq; /* Rest frequency, Hz. */ double restwav; /* Rest wavelength, m. */ double pv[7]; /* Grism parameters: */ /* 0: G, grating ruling density. */ /* 1: m, interference order. */ /* 2: alpha, angle of incidence. */ /* 3: n_r, refractive index at lambda_r. */ /* 4: n'_r, dn/dlambda at lambda_r. */ /* 5: epsilon, grating tilt angle. */ /* 6: theta, detector tilt angle. */ /* Information derived from the parameters supplied. */ /*------------------------------------------------------------------------*/ double w[6]; /* Intermediate values. */ /* 0: Rest frequency or wavelength (SI). */ /* 1: CRVALX (SI units). */ /* 2: CDELTX/CDELTia = dX/dS (SI units). */ /* The remainder are grism intermediates. */ int isGrism; /* Grism coordinates? 1: vacuum, 2: air. */ int padding1; /* (Dummy inserted for alignment purposes.) */ /* Error handling */ /*------------------------------------------------------------------------*/ struct wcserr *err; /* Private */ /*------------------------------------------------------------------------*/ void *padding2; /* (Dummy inserted for alignment purposes.) */ int (*spxX2P)(SPX_ARGS); /* Pointers to the transformation functions */ int (*spxP2S)(SPX_ARGS); /* in the two-step algorithm chain in the */ /* pixel-to-spectral direction. */ int (*spxS2P)(SPX_ARGS); /* Pointers to the transformation functions */ int (*spxP2X)(SPX_ARGS); /* in the two-step algorithm chain in the */ /* spectral-to-pixel direction. */ }; /* Size of the spcprm struct in int units, used by the Fortran wrappers. */ #define SPCLEN (sizeof(struct spcprm)/sizeof(int)) int spcini(struct spcprm *spc); int spcfree(struct spcprm *spc); int spcprt(const struct spcprm *spc); int spcset(struct spcprm *spc); int spcx2s(struct spcprm *spc, int nx, int sx, int sspec, const double x[], double spec[], int stat[]); int spcs2x(struct spcprm *spc, int nspec, int sspec, int sx, const double spec[], double x[], int stat[]); int spctype(const char ctype[], char stype[], char scode[], char sname[], char units[], char *ptype, char *xtype, int *restreq, struct wcserr **err); int spcspxe(const char ctypeS[], double crvalS, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalX, double *dXdS, struct wcserr **err); int spcxpse(const char ctypeS[], double crvalX, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalS, double *dSdX, struct wcserr **err); int spctrne(const char ctypeS1[], double crvalS1, double cdeltS1, double restfrq, double restwav, char ctypeS2[], double *crvalS2, double *cdeltS2, struct wcserr **err); int spcaips(const char ctypeA[], int velref, char ctype[], char specsys[]); /* Deprecated. */ #define spcini_errmsg spc_errmsg #define spcprt_errmsg spc_errmsg #define spcset_errmsg spc_errmsg #define spcx2s_errmsg spc_errmsg #define spcs2x_errmsg spc_errmsg int spctyp(const char ctype[], char stype[], char scode[], char sname[], char units[], char *ptype, char *xtype, int *restreq); int spcspx(const char ctypeS[], double crvalS, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalX, double *dXdS); int spcxps(const char ctypeS[], double crvalX, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalS, double *dSdX); int spctrn(const char ctypeS1[], double crvalS1, double cdeltS1, double restfrq, double restwav, char ctypeS2[], double *crvalS2, double *cdeltS2); #ifdef __cplusplus } #endif #endif /* WCSLIB_SPC */ pywcs-1.12/wcslib/C/sph.c0000644001153600020070000002607012310355626017256 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: sph.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include "wcstrig.h" #include "sph.h" #define copysign(X, Y) ((Y) < 0.0 ? -fabs(X) : fabs(X)) #define tol 1.0e-5 /*--------------------------------------------------------------------------*/ int sphx2s( const double eul[5], int nphi, int ntheta, int spt, int sll, const double phi[], const double theta[], double lng[], double lat[]) { int mphi, mtheta, rowlen, rowoff; double cosphi, costhe, costhe3, costhe4, dlng, dphi, sinphi, sinthe, sinthe3, sinthe4, x, y, z; register int iphi, itheta; register const double *phip, *thetap; register double *latp, *lngp; if (ntheta > 0) { mphi = nphi; mtheta = ntheta; } else { mphi = 1; mtheta = 1; ntheta = nphi; } /* Check for a simple change in origin of longitude. */ if (eul[4] == 0.0) { if (eul[1] == 0.0) { dlng = fmod(eul[0] + 180.0 - eul[2], 360.0); lngp = lng; latp = lat; phip = phi; thetap = theta; for (itheta = 0; itheta < ntheta; itheta++) { for (iphi = 0; iphi < mphi; iphi++) { *lngp = *phip + dlng; *latp = *thetap; /* Normalize the celestial longitude. */ if (eul[0] >= 0.0) { if (*lngp < 0.0) *lngp += 360.0; } else { if (*lngp > 0.0) *lngp -= 360.0; } if (*lngp > 360.0) { *lngp -= 360.0; } else if (*lngp < -360.0) { *lngp += 360.0; } lngp += sll; latp += sll; phip += spt; thetap += spt; } } } else { dlng = fmod(eul[0] + eul[2], 360.0); lngp = lng; latp = lat; phip = phi; thetap = theta; for (itheta = 0; itheta < ntheta; itheta++) { for (iphi = 0; iphi < mphi; iphi++) { *lngp = dlng - *phip; *latp = -(*thetap); /* Normalize the celestial longitude. */ if (eul[0] >= 0.0) { if (*lngp < 0.0) *lngp += 360.0; } else { if (*lngp > 0.0) *lngp -= 360.0; } if (*lngp > 360.0) { *lngp -= 360.0; } else if (*lngp < -360.0) { *lngp += 360.0; } lngp += sll; latp += sll; phip += spt; thetap += spt; } } } return 0; } /* Do phi dependency. */ phip = phi; rowoff = 0; rowlen = nphi*sll; for (iphi = 0; iphi < nphi; iphi++, rowoff += sll, phip += spt) { dphi = *phip - eul[2]; lngp = lng + rowoff; for (itheta = 0; itheta < mtheta; itheta++) { *lngp = dphi; lngp += rowlen; } } /* Do theta dependency. */ thetap = theta; lngp = lng; latp = lat; for (itheta = 0; itheta < ntheta; itheta++, thetap += spt) { sincosd(*thetap, &sinthe, &costhe); costhe3 = costhe*eul[3]; costhe4 = costhe*eul[4]; sinthe3 = sinthe*eul[3]; sinthe4 = sinthe*eul[4]; for (iphi = 0; iphi < mphi; iphi++, lngp += sll, latp += sll) { dphi = *lngp; sincosd(dphi, &sinphi, &cosphi); /* Compute the celestial longitude. */ x = sinthe4 - costhe3*cosphi; if (fabs(x) < tol) { /* Rearrange formula to reduce roundoff errors. */ x = -cosd(*thetap + eul[1]) + costhe3*(1.0 - cosphi); } y = -costhe*sinphi; if (x != 0.0 || y != 0.0) { dlng = atan2d(y, x); } else { /* Change of origin of longitude. */ if (eul[1] < 90.0) { dlng = dphi + 180.0; } else { dlng = -dphi; } } *lngp = eul[0] + dlng; /* Normalize the celestial longitude. */ if (eul[0] >= 0.0) { if (*lngp < 0.0) *lngp += 360.0; } else { if (*lngp > 0.0) *lngp -= 360.0; } if (*lngp > 360.0) { *lngp -= 360.0; } else if (*lngp < -360.0) { *lngp += 360.0; } /* Compute the celestial latitude. */ if (fmod(dphi,180.0) == 0.0) { *latp = *thetap + cosphi*eul[1]; if (*latp > 90.0) *latp = 180.0 - *latp; if (*latp < -90.0) *latp = -180.0 - *latp; } else { z = sinthe3 + costhe4*cosphi; if (fabs(z) > 0.99) { /* Use an alternative formula for greater accuracy. */ *latp = copysign(acosd(sqrt(x*x+y*y)), z); } else { *latp = asind(z); } } } } return 0; } /*--------------------------------------------------------------------------*/ int sphs2x( const double eul[5], int nlng, int nlat, int sll, int spt, const double lng[], const double lat[], double phi[], double theta[]) { int mlat, mlng, rowlen, rowoff; double coslat, coslat3, coslat4, coslng, dlng, dphi, sinlat, sinlat3, sinlat4, sinlng, x, y, z; register int ilat, ilng; register const double *latp, *lngp; register double *phip, *thetap; if (nlat > 0) { mlng = nlng; mlat = nlat; } else { mlng = 1; mlat = 1; nlat = nlng; } /* Check for a simple change in origin of longitude. */ if (eul[4] == 0.0) { if (eul[1] == 0.0) { dphi = fmod(eul[2] - 180.0 - eul[0], 360.0); lngp = lng; latp = lat; phip = phi; thetap = theta; for (ilat = 0; ilat < nlat; ilat++) { for (ilng = 0; ilng < mlng; ilng++) { *phip = fmod(*lngp + dphi, 360.0); *thetap = *latp; /* Normalize the native longitude. */ if (*phip > 180.0) { *phip -= 360.0; } else if (*phip < -180.0) { *phip += 360.0; } phip += spt; thetap += spt; lngp += sll; latp += sll; } } } else { dphi = fmod(eul[2] + eul[0], 360.0); lngp = lng; latp = lat; phip = phi; thetap = theta; for (ilat = 0; ilat < nlat; ilat++) { for (ilng = 0; ilng < mlng; ilng++) { *phip = fmod(dphi - *lngp, 360.0); *thetap = -(*latp); /* Normalize the native longitude. */ if (*phip > 180.0) { *phip -= 360.0; } else if (*phip < -180.0) { *phip += 360.0; } phip += spt; thetap += spt; lngp += sll; latp += sll; } } } return 0; } /* Do lng dependency. */ lngp = lng; rowoff = 0; rowlen = nlng*spt; for (ilng = 0; ilng < nlng; ilng++, rowoff += spt, lngp += sll) { dlng = *lngp - eul[0]; phip = phi + rowoff; thetap = theta; for (ilat = 0; ilat < mlat; ilat++) { *phip = dlng; phip += rowlen; } } /* Do lat dependency. */ latp = lat; phip = phi; thetap = theta; for (ilat = 0; ilat < nlat; ilat++, latp += sll) { sincosd(*latp, &sinlat, &coslat); coslat3 = coslat*eul[3]; coslat4 = coslat*eul[4]; sinlat3 = sinlat*eul[3]; sinlat4 = sinlat*eul[4]; for (ilng = 0; ilng < mlng; ilng++, phip += spt, thetap += spt) { dlng = *phip; sincosd(dlng, &sinlng, &coslng); /* Compute the native longitude. */ x = sinlat4 - coslat3*coslng; if (fabs(x) < tol) { /* Rearrange formula to reduce roundoff errors. */ x = -cosd(*latp+eul[1]) + coslat3*(1.0 - coslng); } y = -coslat*sinlng; if (x != 0.0 || y != 0.0) { dphi = atan2d(y, x); } else { /* Change of origin of longitude. */ if (eul[1] < 90.0) { dphi = dlng - 180.0; } else { dphi = -dlng; } } *phip = fmod(eul[2] + dphi, 360.0); /* Normalize the native longitude. */ if (*phip > 180.0) { *phip -= 360.0; } else if (*phip < -180.0) { *phip += 360.0; } /* Compute the native latitude. */ if (fmod(dlng,180.0) == 0.0) { *thetap = *latp + coslng*eul[1]; if (*thetap > 90.0) *thetap = 180.0 - *thetap; if (*thetap < -90.0) *thetap = -180.0 - *thetap; } else { z = sinlat3 + coslat4*coslng; if (fabs(z) > 0.99) { /* Use an alternative formula for greater accuracy. */ *thetap = copysign(acosd(sqrt(x*x+y*y)), z); } else { *thetap = asind(z); } } } } return 0; } /*--------------------------------------------------------------------------*/ int sphdpa( int nfield, double lng0, double lat0, const double lng[], const double lat[], double dist[], double pa[]) { int i; double eul[5]; /* Set the Euler angles for the coordinate transformation. */ eul[0] = lng0; eul[1] = 90.0 - lat0; eul[2] = 0.0; eul[3] = cosd(eul[1]); eul[4] = sind(eul[1]); /* Transform field points to the new system. */ sphs2x(eul, nfield, 0, 1, 1, lng, lat, pa, dist); for (i = 0; i < nfield; i++) { /* Angular distance is obtained from latitude in the new frame. */ dist[i] = 90.0 - dist[i]; /* Position angle is obtained from longitude in the new frame. */ pa[i] = -pa[i]; if (pa[i] < -180.0) pa[i] += 360.0; } return 0; } /*--------------------------------------------------------------------------*/ int sphpad( int nfield, double lng0, double lat0, const double dist[], const double pa[], double lng[], double lat[]) { int i; double eul[5]; /* Set the Euler angles for the coordinate transformation. */ eul[0] = lng0; eul[1] = 90.0 - lat0; eul[2] = 0.0; eul[3] = cosd(eul[1]); eul[4] = sind(eul[1]); for (i = 0; i < nfield; i++) { /* Latitude in the new frame is obtained from angular distance. */ lat[i] = 90.0 - dist[i]; /* Longitude in the new frame is obtained from position angle. */ lng[i] = -pa[i]; } /* Transform field points to the old system. */ sphx2s(eul, nfield, 0, 1, 1, lng, lat, lng, lat); return 0; } pywcs-1.12/wcslib/C/sph.h0000644001153600020070000002333012310355626017257 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: sph.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the spherical coordinate * transformations used by the FITS World Coordinate System (WCS) standard. * Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of celestial coordinates in FITS", * Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077 (Paper II) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the sph routines * --------------------------- * The WCS spherical coordinate transformations are implemented via separate * functions, sphx2s() and sphs2x(), for the transformation in each direction. * * A utility function, sphdpa(), computes the angular distances and position * angles from a given point on the sky to a number of other points. sphpad() * does the complementary operation - computes the coordinates of points offset * by the given angular distances and position angles from a given point on the * sky. * * * sphx2s() - Rotation in the pixel-to-world direction * --------------------------------------------------- * sphx2s() transforms native coordinates of a projection to celestial * coordinates. * * Given: * eul const double[5] * Euler angles for the transformation: * 0: Celestial longitude of the native pole [deg]. * 1: Celestial colatitude of the native pole, or * native colatitude of the celestial pole [deg]. * 2: Native longitude of the celestial pole [deg]. * 3: cos(eul[1]) * 4: sin(eul[1]) * * nphi, * ntheta int Vector lengths. * * spt,sxy int Vector strides. * * phi,theta const double[] * Longitude and latitude in the native coordinate * system of the projection [deg]. * * Returned: * lng,lat double[] Celestial longitude and latitude [deg]. These may * refer to the same storage as phi and theta * respectively. * * Function return value: * int Status return value: * 0: Success. * * * sphs2x() - Rotation in the world-to-pixel direction * --------------------------------------------------- * sphs2x() transforms celestial coordinates to the native coordinates of a * projection. * * Given: * eul const double[5] * Euler angles for the transformation: * 0: Celestial longitude of the native pole [deg]. * 1: Celestial colatitude of the native pole, or * native colatitude of the celestial pole [deg]. * 2: Native longitude of the celestial pole [deg]. * 3: cos(eul[1]) * 4: sin(eul[1]) * * nlng,nlat int Vector lengths. * * sll,spt int Vector strides. * * lng,lat const double[] * Celestial longitude and latitude [deg]. * * Returned: * phi,theta double[] Longitude and latitude in the native coordinate system * of the projection [deg]. These may refer to the same * storage as lng and lat respectively. * * Function return value: * int Status return value: * 0: Success. * * * sphdpa() - Compute angular distance and position angle * ------------------------------------------------------ * sphdpa() computes the angular distance and generalized position angle (see * notes) from a "reference" point to a number of "field" points on the sphere. * The points must be specified consistently in any spherical coordinate * system. * * sphdpa() is complementary to sphpad(). * * Given: * nfield int The number of field points. * * lng0,lat0 double Spherical coordinates of the reference point [deg]. * * lng,lat const double[] * Spherical coordinates of the field points [deg]. * * Returned: * dist,pa double[] Angular distances and position angles [deg]. These * may refer to the same storage as lng and lat * respectively. * * Function return value: * int Status return value: * 0: Success. * * Notes: * sphdpa() uses sphs2x() to rotate coordinates so that the reference point * is at the north pole of the new system with the north pole of the old * system at zero longitude in the new. The Euler angles required by * sphs2x() for this rotation are * = eul[0] = lng0; = eul[1] = 90.0 - lat0; = eul[2] = 0.0; * * The angular distance and generalized position angle are readily obtained * from the longitude and latitude of the field point in the new system. * This applies even if the reference point is at one of the poles, in which * case the "position angle" returned is as would be computed for a reference * point at (lng0,+90-epsilon) or (lng0,-90+epsilon), in the limit as epsilon * goes to zero. * * It is evident that the coordinate system in which the two points are * expressed is irrelevant to the determination of the angular separation * between the points. However, this is not true of the generalized position * angle. * * The generalized position angle is here defined as the angle of * intersection of the great circle containing the reference and field points * with that containing the reference point and the pole. It has its normal * meaning when the the reference and field points are specified in * equatorial coordinates (right ascension and declination). * * Interchanging the reference and field points changes the position angle in * a non-intuitive way (because the sum of the angles of a spherical triangle * normally exceeds 180 degrees). * * The position angle is undefined if the reference and field points are * coincident or antipodal. This may be detected by checking for a distance * of 0 or 180 degrees (within rounding tolerance). sphdpa() will return an * arbitrary position angle in such circumstances. * * * sphpad() - Compute field points offset from a given point * --------------------------------------------------------- * sphpad() computes the coordinates of a set of points that are offset by the * specified angular distances and position angles from a given "reference" * point on the sky. The distances and position angles must be specified * consistently in any spherical coordinate system. * * sphpad() is complementary to sphdpa(). * * Given: * nfield int The number of field points. * * lng0,lat0 double Spherical coordinates of the reference point [deg]. * * dist,pa const double[] * Angular distances and position angles [deg]. * * Returned: * lng,lat double[] Spherical coordinates of the field points [deg]. * These may refer to the same storage as dist and pa * respectively. * * Function return value: * int Status return value: * 0: Success. * * Notes: * sphpad() is implemented analogously to sphdpa() although using sphx2s() * for the inverse transformation. In particular, when the reference point * is at one of the poles, "position angle" is interpreted as though the * reference point was at (lng0,+90-epsilon) or (lng0,-90+epsilon), in the * limit as epsilon goes to zero. * * Applying sphpad() with the distances and position angles computed by * sphdpa() should return the original field points. * *===========================================================================*/ #ifndef WCSLIB_SPH #define WCSLIB_SPH #ifdef __cplusplus extern "C" { #endif int sphx2s(const double eul[5], int nphi, int ntheta, int spt, int sxy, const double phi[], const double theta[], double lng[], double lat[]); int sphs2x(const double eul[5], int nlng, int nlat, int sll , int spt, const double lng[], const double lat[], double phi[], double theta[]); int sphdpa(int nfield, double lng0, double lat0, const double lng[], const double lat[], double dist[], double pa[]); int sphpad(int nfield, double lng0, double lat0, const double dist[], const double pa[], double lng[], double lat[]); #ifdef __cplusplus } #endif #endif /* WCSLIB_SPH */ pywcs-1.12/wcslib/C/spx.c0000644001153600020070000006123612310355626017301 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: spx.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "spx.h" /* Map status return value to message. */ const char *spx_errmsg[] = { "Success", "Null spxprm pointer passed", "Invalid spectral parameters", "Invalid spectral variable", "One or more of the inspec coordinates were invalid"}; /* Convenience macro for invoking wcserr_set(). */ #define SPX_ERRMSG(status) WCSERR_SET(status), spx_errmsg[status] #define C 2.99792458e8 #define h 6.6260755e-34 /*============================================================================ * Spectral cross conversions; given one spectral coordinate it computes all * the others, plus the required derivatives of each with respect to the * others. *===========================================================================*/ int specx(type, spec, restfrq, restwav, spx) const char *type; double spec, restfrq, restwav; struct spxprm *spx; { static const char *function = "specx"; register int k; int haverest; double beta, dwaveawav, gamma, n, s, t, u; struct wcserr **err; if (spx == 0x0) return SPXERR_NULL_POINTER; err = &(spx->err); haverest = 1; if (restfrq == 0.0) { if (restwav == 0.0) { /* No line rest frequency supplied. */ haverest = 0; /* Temporarily set a dummy value for conversions. */ spx->restwav = 1.0; } else { spx->restwav = restwav; } spx->restfrq = C/spx->restwav; } else { spx->restfrq = restfrq; spx->restwav = C/restfrq; } spx->err = 0x0; /* Convert to frequency. */ spx->wavetype = 0; spx->velotype = 0; if (strcmp(type, "FREQ") == 0) { if (spec == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable: frequency == 0"); } spx->freq = spec; spx->wavetype = 1; } else if (strcmp(type, "AFRQ") == 0) { if (spec == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable: frequency == 0"); } spx->freq = spec/(2.0*PI); spx->wavetype = 1; } else if (strcmp(type, "ENER") == 0) { if (spec == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable: frequency == 0"); } spx->freq = spec/h; spx->wavetype = 1; } else if (strcmp(type, "WAVN") == 0) { if (spec == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable: frequency == 0"); } spx->freq = spec*C; spx->wavetype = 1; } else if (strcmp(type, "VRAD") == 0) { spx->freq = spx->restfrq*(1.0 - spec/C); spx->velotype = 1; } else if (strcmp(type, "WAVE") == 0) { if (spec == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable: frequency == 0"); } spx->freq = C/spec; spx->wavetype = 1; } else if (strcmp(type, "VOPT") == 0) { s = 1.0 + spec/C; if (s == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable"); } spx->freq = spx->restfrq/s; spx->velotype = 1; } else if (strcmp(type, "ZOPT") == 0) { s = 1.0 + spec; if (s == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable"); } spx->freq = spx->restfrq/s; spx->velotype = 1; } else if (strcmp(type, "AWAV") == 0) { if (spec == 0.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable"); } s = 1.0/spec; s *= s; n = 2.554e8 / (0.41e14 - s); n += 294.981e8 / (1.46e14 - s); n += 1.000064328; spx->freq = C/(spec*n); spx->wavetype = 1; } else if (strcmp(type, "VELO") == 0) { beta = spec/C; if (fabs(beta) == 1.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable"); } spx->freq = spx->restfrq*(1.0 - beta)/sqrt(1.0 - beta*beta); spx->velotype = 1; } else if (strcmp(type, "BETA") == 0) { if (fabs(spec) == 1.0) { return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_VAR), "Invalid spectral variable"); } spx->freq = spx->restfrq*(1.0 - spec)/sqrt(1.0 - spec*spec); spx->velotype = 1; } else { /* Unrecognized type. */ return wcserr_set(WCSERR_SET(SPXERR_BAD_SPEC_PARAMS), "Unrecognized spectral type '%s'", type); } /* Convert frequency to the other spectral types. */ n = 1.0; for (k = 0; k < 4; k++) { s = n*spx->freq/C; s *= s; t = 0.41e14 - s; u = 1.46e14 - s; n = 1.000064328 + (2.554e8/t + 294.981e8/u); } dwaveawav = n - 2.0*s*(2.554e8/(t*t) + 294.981e8/(u*u)); s = spx->freq/spx->restfrq; spx->ener = spx->freq*h; spx->afrq = spx->freq*(2.0*PI); spx->wavn = spx->freq/C; spx->vrad = C*(1.0 - s); spx->wave = C/spx->freq; spx->awav = spx->wave/n; spx->vopt = C*(1.0/s - 1.0); spx->zopt = spx->vopt/C; spx->velo = C*(1.0 - s*s)/(1.0 + s*s); spx->beta = spx->velo/C; /* Compute the required derivatives. */ gamma = 1.0/sqrt(1.0 - spx->beta*spx->beta); spx->dfreqafrq = 1.0/(2.0*PI); spx->dafrqfreq = 1.0/spx->dfreqafrq; spx->dfreqener = 1.0/h; spx->denerfreq = 1.0/spx->dfreqener; spx->dfreqwavn = C; spx->dwavnfreq = 1.0/spx->dfreqwavn; spx->dfreqvrad = -spx->restfrq/C; spx->dvradfreq = 1.0/spx->dfreqvrad; spx->dfreqwave = -spx->freq/spx->wave; spx->dwavefreq = 1.0/spx->dfreqwave; spx->dfreqawav = spx->dfreqwave * dwaveawav; spx->dawavfreq = 1.0/spx->dfreqawav; spx->dfreqvelo = -gamma*spx->restfrq/(C + spx->velo); spx->dvelofreq = 1.0/spx->dfreqvelo; spx->dwavevopt = spx->restwav/C; spx->dvoptwave = 1.0/spx->dwavevopt; spx->dwavezopt = spx->restwav; spx->dzoptwave = 1.0/spx->dwavezopt; spx->dwaveawav = dwaveawav; spx->dawavwave = 1.0/spx->dwaveawav; spx->dwavevelo = gamma*spx->restwav/(C - spx->velo); spx->dvelowave = 1.0/spx->dwavevelo; spx->dawavvelo = spx->dwavevelo/dwaveawav; spx->dveloawav = 1.0/spx->dawavvelo; spx->dvelobeta = C; spx->dbetavelo = 1.0/spx->dvelobeta; /* Reset values if no line rest frequency was supplied. */ if (haverest) { spx->wavetype = 1; spx->velotype = 1; } else { spx->restfrq = 0.0; spx->restwav = 0.0; if (!spx->wavetype) { /* Don't have wave characteristic types. */ spx->freq = 0.0; spx->afrq = 0.0; spx->ener = 0.0; spx->wavn = 0.0; spx->wave = 0.0; spx->awav = 0.0; spx->dfreqwave = 0.0; spx->dwavefreq = 0.0; spx->dfreqawav = 0.0; spx->dawavfreq = 0.0; spx->dwaveawav = 0.0; spx->dawavwave = 0.0; } else { /* Don't have velocity types. */ spx->vrad = 0.0; spx->vopt = 0.0; spx->zopt = 0.0; spx->velo = 0.0; spx->beta = 0.0; } spx->dfreqvrad = 0.0; spx->dvradfreq = 0.0; spx->dfreqvelo = 0.0; spx->dvelofreq = 0.0; spx->dwavevopt = 0.0; spx->dvoptwave = 0.0; spx->dwavezopt = 0.0; spx->dzoptwave = 0.0; spx->dwavevelo = 0.0; spx->dvelowave = 0.0; spx->dawavvelo = 0.0; spx->dveloawav = 0.0; } return 0; } /*============================================================================ * Conversions between frequency and vacuum wavelength. *===========================================================================*/ int freqwave(dummy, nfreq, sfreq, swave, freq, wave, stat) double dummy; int nfreq, sfreq, swave; const double freq[]; double wave[]; int stat[]; { int status = 0; register int ifreq, *statp; register const double *freqp; register double *wavep; freqp = freq; wavep = wave; statp = stat; for (ifreq = 0; ifreq < nfreq; ifreq++) { if (*freqp != 0.0) { *wavep = C/(*freqp); *(statp++) = 0; } else { *(statp++) = 1; status = SPXERR_BAD_INSPEC_COORD; } freqp += sfreq; wavep += swave; } return status; } /*--------------------------------------------------------------------------*/ int wavefreq(dummy, nwave, swave, sfreq, wave, freq, stat) double dummy; int nwave, swave, sfreq; const double wave[]; double freq[]; int stat[]; { int status = 0; register int iwave, *statp; register const double *wavep; register double *freqp; wavep = wave; freqp = freq; statp = stat; for (iwave = 0; iwave < nwave; iwave++) { if (*wavep != 0.0) { *freqp = C/(*wavep); *(statp++) = 0; } else { *(statp++) = 1; status = SPXERR_BAD_INSPEC_COORD; } wavep += swave; freqp += sfreq; } return status; } /*============================================================================ * Conversions between frequency and air wavelength. *===========================================================================*/ int freqawav(dummy, nfreq, sfreq, sawav, freq, awav, stat) double dummy; int nfreq, sfreq, sawav; const double freq[]; double awav[]; int stat[]; { int status; if ((status = freqwave(dummy, nfreq, sfreq, sawav, freq, awav, stat))) { return status; } return waveawav(dummy, nfreq, sawav, sawav, awav, awav, stat); } /*--------------------------------------------------------------------------*/ int awavfreq(dummy, nawav, sawav, sfreq, awav, freq, stat) double dummy; int nawav, sawav, sfreq; const double awav[]; double freq[]; int stat[]; { int status; if ((status = awavwave(dummy, nawav, sawav, sfreq, awav, freq, stat))) { return status; } return wavefreq(dummy, nawav, sfreq, sfreq, freq, freq, stat); } /*============================================================================ * Conversions between frequency and relativistic velocity. *===========================================================================*/ int freqvelo(restfrq, nfreq, sfreq, svelo, freq, velo, stat) double restfrq; int nfreq, sfreq, svelo; const double freq[]; double velo[]; int stat[]; { double r, s; register int ifreq, *statp; register const double *freqp; register double *velop; r = restfrq*restfrq; freqp = freq; velop = velo; statp = stat; for (ifreq = 0; ifreq < nfreq; ifreq++) { s = *freqp * *freqp; *velop = C*(r - s)/(r + s); *(statp++) = 0; freqp += sfreq; velop += svelo; } return 0; } /*--------------------------------------------------------------------------*/ int velofreq(restfrq, nvelo, svelo, sfreq, velo, freq, stat) double restfrq; int nvelo, svelo, sfreq; const double velo[]; double freq[]; int stat[]; { int status = 0; double s; register int ivelo, *statp; register const double *velop; register double *freqp; velop = velo; freqp = freq; statp = stat; for (ivelo = 0; ivelo < nvelo; ivelo++) { s = C + *velop; if (s != 0.0) { *freqp = restfrq*sqrt((C - *velop)/s); *(statp++) = 0; } else { *(statp++) = 1; status = SPXERR_BAD_INSPEC_COORD; } velop += svelo; freqp += sfreq; } return status; } /*============================================================================ * Conversions between vacuum wavelength and air wavelength. *===========================================================================*/ int waveawav(dummy, nwave, swave, sawav, wave, awav, stat) double dummy; int nwave, swave, sawav; const double wave[]; double awav[]; int stat[]; { int status = 0; double n, s; register int iwave, k, *statp; register const double *wavep; register double *awavp; wavep = wave; awavp = awav; statp = stat; for (iwave = 0; iwave < nwave; iwave++) { if (*wavep != 0.0) { n = 1.0; for (k = 0; k < 4; k++) { s = n/(*wavep); s *= s; n = 2.554e8 / (0.41e14 - s); n += 294.981e8 / (1.46e14 - s); n += 1.000064328; } *awavp = (*wavep)/n; *(statp++) = 0; } else { *(statp++) = 1; status = SPXERR_BAD_INSPEC_COORD; } wavep += swave; awavp += sawav; } return status; } /*--------------------------------------------------------------------------*/ int awavwave(dummy, nawav, sawav, swave, awav, wave, stat) double dummy; int nawav, sawav, swave; const double awav[]; double wave[]; int stat[]; { int status = 0; double n, s; register int iawav, *statp; register const double *awavp; register double *wavep; awavp = awav; wavep = wave; statp = stat; for (iawav = 0; iawav < nawav; iawav++) { if (*awavp != 0.0) { s = 1.0/(*awavp); s *= s; n = 2.554e8 / (0.41e14 - s); n += 294.981e8 / (1.46e14 - s); n += 1.000064328; *wavep = (*awavp)*n; *(statp++) = 0; } else { *(statp++) = 1; status = SPXERR_BAD_INSPEC_COORD; } awavp += sawav; wavep += swave; } return status; } /*============================================================================ * Conversions between vacuum wavelength and relativistic velocity. *===========================================================================*/ int wavevelo(restwav, nwave, swave, svelo, wave, velo, stat) double restwav; int nwave, swave, svelo; const double wave[]; double velo[]; int stat[]; { double r, s; register int iwave, *statp; register const double *wavep; register double *velop; r = restwav*restwav; wavep = wave; velop = velo; statp = stat; for (iwave = 0; iwave < nwave; iwave++) { s = *wavep * *wavep; *velop = C*(s - r)/(s + r); *(statp++) = 0; wavep += swave; velop += svelo; } return 0; } /*--------------------------------------------------------------------------*/ int velowave(restwav, nvelo, svelo, swave, velo, wave, stat) double restwav; int nvelo, svelo, swave; const double velo[]; double wave[]; int stat[]; { int status = 0; double s; register int ivelo, *statp; register const double *velop; register double *wavep; velop = velo; wavep = wave; statp = stat; for (ivelo = 0; ivelo < nvelo; ivelo++) { s = C - *velop; if (s != 0.0) { *wavep = restwav*sqrt((C + *velop)/s); *(statp++) = 0; } else { *(statp++) = 1; status = SPXERR_BAD_INSPEC_COORD; } velop += svelo; wavep += swave; } return status; } /*============================================================================ * Conversions between air wavelength and relativistic velocity. *===========================================================================*/ int awavvelo(dummy, nawav, sawav, svelo, awav, velo, stat) double dummy; int nawav, sawav, svelo; const double awav[]; double velo[]; int stat[]; { int status; if ((status = awavwave(dummy, nawav, sawav, svelo, awav, velo, stat))) { return status; } return wavevelo(dummy, nawav, svelo, svelo, velo, velo, stat); } /*--------------------------------------------------------------------------*/ int veloawav(dummy, nvelo, svelo, sawav, velo, awav, stat) double dummy; int nvelo, svelo, sawav; const double velo[]; double awav[]; int stat[]; { int status; if ((status = velowave(dummy, nvelo, svelo, sawav, velo, awav, stat))) { return status; } return waveawav(dummy, nvelo, sawav, sawav, awav, awav, stat); } /*============================================================================ * Conversions between frequency and angular frequency. *===========================================================================*/ int freqafrq(dummy, nfreq, sfreq, safrq, freq, afrq, stat) double dummy; int nfreq, sfreq, safrq; const double freq[]; double afrq[]; int stat[]; { register int ifreq, *statp; register const double *freqp; register double *afrqp; freqp = freq; afrqp = afrq; statp = stat; for (ifreq = 0; ifreq < nfreq; ifreq++) { *afrqp = (*freqp)*(2.0*PI); *(statp++) = 0; freqp += sfreq; afrqp += safrq; } return 0; } /*--------------------------------------------------------------------------*/ int afrqfreq(dummy, nafrq, safrq, sfreq, afrq, freq, stat) double dummy; int nafrq, safrq, sfreq; const double afrq[]; double freq[]; int stat[]; { register int iafrq, *statp; register const double *afrqp; register double *freqp; afrqp = afrq; freqp = freq; statp = stat; for (iafrq = 0; iafrq < nafrq; iafrq++) { *freqp = (*afrqp)/(2.0*PI); *(statp++) = 0; afrqp += safrq; freqp += sfreq; } return 0; } /*============================================================================ * Conversions between frequency and energy. *===========================================================================*/ int freqener(dummy, nfreq, sfreq, sener, freq, ener, stat) double dummy; int nfreq, sfreq, sener; const double freq[]; double ener[]; int stat[]; { register int ifreq, *statp; register const double *freqp; register double *enerp; freqp = freq; enerp = ener; statp = stat; for (ifreq = 0; ifreq < nfreq; ifreq++) { *enerp = (*freqp)*h; *(statp++) = 0; freqp += sfreq; enerp += sener; } return 0; } /*--------------------------------------------------------------------------*/ int enerfreq(dummy, nener, sener, sfreq, ener, freq, stat) double dummy; int nener, sener, sfreq; const double ener[]; double freq[]; int stat[]; { register int iener, *statp; register const double *enerp; register double *freqp; enerp = ener; freqp = freq; statp = stat; for (iener = 0; iener < nener; iener++) { *freqp = (*enerp)/h; *(statp++) = 0; enerp += sener; freqp += sfreq; } return 0; } /*============================================================================ * Conversions between frequency and wave number. *===========================================================================*/ int freqwavn(dummy, nfreq, sfreq, swavn, freq, wavn, stat) double dummy; int nfreq, sfreq, swavn; const double freq[]; double wavn[]; int stat[]; { register int ifreq, *statp; register const double *freqp; register double *wavnp; freqp = freq; wavnp = wavn; statp = stat; for (ifreq = 0; ifreq < nfreq; ifreq++) { *wavnp = (*freqp)/C; *(statp++) = 0; freqp += sfreq; wavnp += swavn; } return 0; } /*--------------------------------------------------------------------------*/ int wavnfreq(dummy, nwavn, swavn, sfreq, wavn, freq, stat) double dummy; int nwavn, swavn, sfreq; const double wavn[]; double freq[]; int stat[]; { register int iwavn, *statp; register const double *wavnp; register double *freqp; wavnp = wavn; freqp = freq; statp = stat; for (iwavn = 0; iwavn < nwavn; iwavn++) { *freqp = (*wavnp)*C; *(statp++) = 0; wavnp += swavn; freqp += sfreq; } return 0; } /*============================================================================ * Conversions between frequency and radio velocity. *===========================================================================*/ int freqvrad(restfrq, nfreq, sfreq, svrad, freq, vrad, stat) double restfrq; int nfreq, sfreq, svrad; const double freq[]; double vrad[]; int stat[]; { double r; register int ifreq, *statp; register const double *freqp; register double *vradp; if (restfrq == 0.0) { return SPXERR_BAD_SPEC_PARAMS; } r = C/restfrq; freqp = freq; vradp = vrad; statp = stat; for (ifreq = 0; ifreq < nfreq; ifreq++) { *vradp = r*(restfrq - *freqp); *(statp++) = 0; freqp += sfreq; vradp += svrad; } return 0; } /*--------------------------------------------------------------------------*/ int vradfreq(restfrq, nvrad, svrad, sfreq, vrad, freq, stat) double restfrq; int nvrad, svrad, sfreq; const double vrad[]; double freq[]; int stat[]; { double r; register int ivrad, *statp; register const double *vradp; register double *freqp; r = restfrq/C; vradp = vrad; freqp = freq; statp = stat; for (ivrad = 0; ivrad < nvrad; ivrad++) { *freqp = r*(C - *vradp); *(statp++) = 0; vradp += svrad; freqp += sfreq; } return 0; } /*============================================================================ * Conversions between vacuum wavelength and optical velocity. *===========================================================================*/ int wavevopt(restwav, nwave, swave, svopt, wave, vopt, stat) double restwav; int nwave, swave, svopt; const double wave[]; double vopt[]; int stat[]; { double r; register int iwave, *statp; register const double *wavep; register double *voptp; if (restwav == 0.0) { return SPXERR_BAD_SPEC_PARAMS; } r = C/restwav; wavep = wave; voptp = vopt; statp = stat; for (iwave = 0; iwave < nwave; iwave++) { *voptp = r*(*wavep) - C; *(statp++) = 0; wavep += swave; voptp += svopt; } return 0; } /*--------------------------------------------------------------------------*/ int voptwave(restwav, nvopt, svopt, swave, vopt, wave, stat) double restwav; int nvopt, svopt, swave; const double vopt[]; double wave[]; int stat[]; { double r; register int ivopt, *statp; register const double *voptp; register double *wavep; r = restwav/C; voptp = vopt; wavep = wave; statp = stat; for (ivopt = 0; ivopt < nvopt; ivopt++) { *wavep = r*(C + *voptp); *(statp++) = 0; voptp += svopt; wavep += swave; } return 0; } /*============================================================================ * Conversions between vacuum wavelength and redshift. *===========================================================================*/ int wavezopt(restwav, nwave, swave, szopt, wave, zopt, stat) double restwav; int nwave, swave, szopt; const double wave[]; double zopt[]; int stat[]; { double r; register int iwave, *statp; register const double *wavep; register double *zoptp; if (restwav == 0.0) { return SPXERR_BAD_SPEC_PARAMS; } r = 1.0/restwav; wavep = wave; zoptp = zopt; statp = stat; for (iwave = 0; iwave < nwave; iwave++) { *zoptp = r*(*wavep) - 1.0; *(statp++) = 0; wavep += swave; zoptp += szopt; } return 0; } /*--------------------------------------------------------------------------*/ int zoptwave(restwav, nzopt, szopt, swave, zopt, wave, stat) double restwav; int nzopt, szopt, swave; const double zopt[]; double wave[]; int stat[]; { register int izopt, *statp; register const double *zoptp; register double *wavep; zoptp = zopt; wavep = wave; statp = stat; for (izopt = 0; izopt < nzopt; izopt++) { *wavep = restwav*(1.0 + *zoptp); *(statp++) = 0; zoptp += szopt; wavep += swave; } return 0; } /*============================================================================ * Conversions between relativistic velocity and beta (= v/c). *===========================================================================*/ int velobeta(dummy, nvelo, svelo, sbeta, velo, beta, stat) double dummy; int nvelo, svelo, sbeta; const double velo[]; double beta[]; int stat[]; { register int ivelo, *statp; register const double *velop; register double *betap; velop = velo; betap = beta; statp = stat; for (ivelo = 0; ivelo < nvelo; ivelo++) { *betap = (*velop)/C; *(statp++) = 0; velop += svelo; betap += sbeta; } return 0; } /*--------------------------------------------------------------------------*/ int betavelo(dummy, nbeta, sbeta, svelo, beta, velo, stat) double dummy; int nbeta, sbeta, svelo; const double beta[]; double velo[]; int stat[]; { register int ibeta, *statp; register const double *betap; register double *velop; betap = beta; velop = velo; statp = stat; for (ibeta = 0; ibeta < nbeta; ibeta++) { *velop = (*betap)*C; *(statp++) = 0; betap += sbeta; velop += svelo; } return 0; } pywcs-1.12/wcslib/C/spx.h0000644001153600020070000004712212310355626017304 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: spx.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the spectral coordinate systems * recognized by the FITS World Coordinate System (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the spx routines * --------------------------- * specx() is a scalar routine that, given one spectral variable (e.g. * frequency), computes all the others (e.g. wavelength, velocity, etc.) plus * the required derivatives of each with respect to the others. The results * are returned in the spxprm struct. * * The remaining routines are all vector conversions from one spectral * variable to another. The API of these functions only differ in whether the * rest frequency or wavelength need be supplied. * * Non-linear: * - freqwave() frequency -> vacuum wavelength * - wavefreq() vacuum wavelength -> frequency * * - freqawav() frequency -> air wavelength * - awavfreq() air wavelength -> frequency * * - freqvelo() frequency -> relativistic velocity * - velofreq() relativistic velocity -> frequency * * - waveawav() vacuum wavelength -> air wavelength * - awavwave() air wavelength -> vacuum wavelength * * - wavevelo() vacuum wavelength -> relativistic velocity * - velowave() relativistic velocity -> vacuum wavelength * * - awavvelo() air wavelength -> relativistic velocity * - veloawav() relativistic velocity -> air wavelength * * Linear: * - freqafrq() frequency -> angular frequency * - afrqfreq() angular frequency -> frequency * * - freqener() frequency -> energy * - enerfreq() energy -> frequency * * - freqwavn() frequency -> wave number * - wavnfreq() wave number -> frequency * * - freqvrad() frequency -> radio velocity * - vradfreq() radio velocity -> frequency * * - wavevopt() vacuum wavelength -> optical velocity * - voptwave() optical velocity -> vacuum wavelength * * - wavezopt() vacuum wavelength -> redshift * - zoptwave() redshift -> vacuum wavelength * * - velobeta() relativistic velocity -> beta (= v/c) * - betavelo() beta (= v/c) -> relativistic velocity * * These are the workhorse routines, to be used for fast transformations. * Conversions may be done "in place" by calling the routine with the output * vector set to the input. * * Argument checking: * ------------------ * The input spectral values are only checked for values that would result * in floating point exceptions. In particular, negative frequencies and * wavelengths are allowed, as are velocities greater than the speed of * light. The same is true for the spectral parameters - rest frequency and * wavelength. * * Accuracy: * --------- * No warranty is given for the accuracy of these routines (refer to the * copyright notice); intending users must satisfy for themselves their * adequacy for the intended purpose. However, closure effectively to within * double precision rounding error was demonstrated by test routine tspec.c * which accompanies this software. * * * specx() - Spectral cross conversions (scalar) * --------------------------------------------- * Given one spectral variable specx() computes all the others, plus the * required derivatives of each with respect to the others. * * Given: * type const char* * The type of spectral variable given by spec, FREQ, * AFRQ, ENER, WAVN, VRAD, WAVE, VOPT, ZOPT, AWAV, VELO, * or BETA (case sensitive). * * spec double The spectral variable given, in SI units. * * restfrq, * restwav double Rest frequency [Hz] or rest wavelength in vacuo [m], * only one of which need be given. The other should be * set to zero. If both are zero, only a subset of the * spectral variables can be computed, the remainder are * set to zero. Specifically, given one of FREQ, AFRQ, * ENER, WAVN, WAVE, or AWAV the others can be computed * without knowledge of the rest frequency. Likewise, * VRAD, VOPT, ZOPT, VELO, and BETA. * * Given and returned: * specs struct spxprm* * Data structure containing all spectral variables and * their derivatives, in SI units. * * Function return value: * int Status return value: * 0: Success. * 1: Null spxprm pointer passed. * 2: Invalid spectral parameters. * 3: Invalid spectral variable. * * For returns > 1, a detailed error message is set in * spxprm::err if enabled, see wcserr_enable(). * * freqafrq(), afrqfreq(), freqener(), enerfreq(), freqwavn(), wavnfreq(), * freqwave(), wavefreq(), freqawav(), awavfreq(), waveawav(), awavwave(), * velobeta(), and betavelo() implement vector conversions between wave-like * or velocity-like spectral types (i.e. conversions that do not need the rest * frequency or wavelength). They all have the same API. * * * freqafrq() - Convert frequency to angular frequency (vector) * ------------------------------------------------------------ * freqafrq() converts frequency to angular frequency. * * Given: * param double Ignored. * * nspec int Vector length. * * instep, * outstep int Vector strides. * * inspec const double[] * Input spectral variables, in SI units. * * Returned: * outspec double[] Output spectral variables, in SI units. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of inspec. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters. * 4: One or more of the inspec coordinates were * invalid, as indicated by the stat vector. * * * freqvelo(), velofreq(), freqvrad(), and vradfreq() implement vector * conversions between frequency and velocity spectral types. They all have * the same API. * * * freqvelo() - Convert frequency to relativistic velocity (vector) * ---------------------------------------------------------------- * freqvelo() converts frequency to relativistic velocity. * * Given: * param double Rest frequency [Hz]. * * nspec int Vector length. * * instep, * outstep int Vector strides. * * inspec const double[] * Input spectral variables, in SI units. * * Returned: * outspec double[] Output spectral variables, in SI units. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of inspec. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters. * 4: One or more of the inspec coordinates were * invalid, as indicated by the stat vector. * * * wavevelo(), velowave(), awavvelo(), veloawav(), wavevopt(), voptwave(), * wavezopt(), and zoptwave() implement vector conversions between wavelength * and velocity spectral types. They all have the same API. * * * wavevelo() - Conversions between wavelength and velocity types (vector) * ----------------------------------------------------------------------- * wavevelo() converts vacuum wavelength to relativistic velocity. * * Given: * param double Rest wavelength in vacuo [m]. * * nspec int Vector length. * * instep, * outstep int Vector strides. * * inspec const double[] * Input spectral variables, in SI units. * * Returned: * outspec double[] Output spectral variables, in SI units. * * stat int[] Status return value for each vector element: * 0: Success. * 1: Invalid value of inspec. * * Function return value: * int Status return value: * 0: Success. * 2: Invalid spectral parameters. * 4: One or more of the inspec coordinates were * invalid, as indicated by the stat vector. * * * spxprm struct - Spectral variables and their derivatives * -------------------------------------------------------- * The spxprm struct contains the value of all spectral variables and their * derivatives. It is used solely by specx() which constructs it from * information provided via its function arguments. * * This struct should be considered read-only, no members need ever be set nor * should ever be modified by the user. * * double restfrq * (Returned) Rest frequency [Hz]. * * double restwav * (Returned) Rest wavelength [m]. * * int wavetype * (Returned) True if wave types have been computed, and ... * * int velotype * (Returned) ... true if velocity types have been computed; types are * defined below. * * If one or other of spxprm::restfrq and spxprm::restwav is given * (non-zero) then all spectral variables may be computed. If both are * given, restfrq is used. If restfrq and restwav are both zero, only wave * characteristic xor velocity type spectral variables may be computed * depending on the variable given. These flags indicate what is * available. * * double freq * (Returned) Frequency [Hz] (wavetype). * * double afrq * (Returned) Angular frequency [rad/s] (wavetype). * * double ener * (Returned) Photon energy [J] (wavetype). * * double wavn * (Returned) Wave number [/m] (wavetype). * * double vrad * (Returned) Radio velocity [m/s] (velotype). * * double wave * (Returned) Vacuum wavelength [m] (wavetype). * * double vopt * (Returned) Optical velocity [m/s] (velotype). * * double zopt * (Returned) Redshift [dimensionless] (velotype). * * double awav * (Returned) Air wavelength [m] (wavetype). * * double velo * (Returned) Relativistic velocity [m/s] (velotype). * * double beta * (Returned) Relativistic beta [dimensionless] (velotype). * * double dfreqafrq * (Returned) Derivative of frequency with respect to angular frequency * [/rad] (constant, = 1 / 2*pi), and ... * double dafrqfreq * (Returned) ... vice versa [rad] (constant, = 2*pi, always available). * * double dfreqener * (Returned) Derivative of frequency with respect to photon energy * [/J/s] (constant, = 1/h), and ... * double denerfreq * (Returned) ... vice versa [Js] (constant, = h, Planck's constant, * always available). * * double dfreqwavn * (Returned) Derivative of frequency with respect to wave number [m/s] * (constant, = c, the speed of light in vacuuo), and ... * double dwavnfreq * (Returned) ... vice versa [s/m] (constant, = 1/c, always available). * * double dfreqvrad * (Returned) Derivative of frequency with respect to radio velocity [/m], * and ... * double dvradfreq * (Returned) ... vice versa [m] (wavetype && velotype). * * double dfreqwave * (Returned) Derivative of frequency with respect to vacuum wavelength * [/m/s], and ... * double dwavefreq * (Returned) ... vice versa [m s] (wavetype). * * double dfreqawav * (Returned) Derivative of frequency with respect to air wavelength, * [/m/s], and ... * double dawavfreq * (Returned) ... vice versa [m s] (wavetype). * * double dfreqvelo * (Returned) Derivative of frequency with respect to relativistic * velocity [/m], and ... * double dvelofreq * (Returned) ... vice versa [m] (wavetype && velotype). * * double dwavevopt * (Returned) Derivative of vacuum wavelength with respect to optical * velocity [s], and ... * double dvoptwave * (Returned) ... vice versa [/s] (wavetype && velotype). * * double dwavezopt * (Returned) Derivative of vacuum wavelength with respect to redshift [m], * and ... * double dzoptwave * (Returned) ... vice versa [/m] (wavetype && velotype). * * double dwaveawav * (Returned) Derivative of vacuum wavelength with respect to air * wavelength [dimensionless], and ... * double dawavwave * (Returned) ... vice versa [dimensionless] (wavetype). * * double dwavevelo * (Returned) Derivative of vacuum wavelength with respect to relativistic * velocity [s], and ... * double dvelowave * (Returned) ... vice versa [/s] (wavetype && velotype). * * double dawavvelo * (Returned) Derivative of air wavelength with respect to relativistic * velocity [s], and ... * double dveloawav * (Returned) ... vice versa [/s] (wavetype && velotype). * * double dvelobeta * (Returned) Derivative of relativistic velocity with respect to * relativistic beta [m/s] (constant, = c, the speed of light in vacuu0), * and ... * double dbetavelo * (Returned) ... vice versa [s/m] (constant, = 1/c, always available). * * struct wcserr *err * (Returned) If enabled, when an error status is returned this struct * contains detailed information about the error, see wcserr_enable(). * * void *padding * (An unused variable inserted for alignment purposes only.) * * Global variable: const char *spx_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_SPEC #define WCSLIB_SPEC #ifdef __cplusplus extern "C" { #endif #include "wcserr.h" extern const char *spx_errmsg[]; enum spx_errmsg { SPXERR_SUCCESS = 0, /* Success. */ SPXERR_NULL_POINTER = 1, /* Null spxprm pointer passed. */ SPXERR_BAD_SPEC_PARAMS = 2, /* Invalid spectral parameters. */ SPXERR_BAD_SPEC_VAR = 3, /* Invalid spectral variable. */ SPXERR_BAD_INSPEC_COORD = 4 /* One or more of the inspec coordinates were invalid. */ }; struct spxprm { double restfrq, restwav; /* Rest frequency [Hz] and wavelength [m]. */ int wavetype, velotype; /* True if wave/velocity types have been */ /* computed; types are defined below. */ /* Spectral variables computed by specx(). */ /*------------------------------------------------------------------------*/ double freq, /* wavetype: Frequency [Hz]. */ afrq, /* wavetype: Angular frequency [rad/s]. */ ener, /* wavetype: Photon energy [J]. */ wavn, /* wavetype: Wave number [/m]. */ vrad, /* velotype: Radio velocity [m/s]. */ wave, /* wavetype: Vacuum wavelength [m]. */ vopt, /* velotype: Optical velocity [m/s]. */ zopt, /* velotype: Redshift. */ awav, /* wavetype: Air wavelength [m]. */ velo, /* velotype: Relativistic velocity [m/s]. */ beta; /* velotype: Relativistic beta. */ /* Derivatives of spectral variables computed by specx(). */ /*------------------------------------------------------------------------*/ double dfreqafrq, dafrqfreq, /* Constant, always available. */ dfreqener, denerfreq, /* Constant, always available. */ dfreqwavn, dwavnfreq, /* Constant, always available. */ dfreqvrad, dvradfreq, /* wavetype && velotype. */ dfreqwave, dwavefreq, /* wavetype. */ dfreqawav, dawavfreq, /* wavetype. */ dfreqvelo, dvelofreq, /* wavetype && velotype. */ dwavevopt, dvoptwave, /* wavetype && velotype. */ dwavezopt, dzoptwave, /* wavetype && velotype. */ dwaveawav, dawavwave, /* wavetype. */ dwavevelo, dvelowave, /* wavetype && velotype. */ dawavvelo, dveloawav, /* wavetype && velotype. */ dvelobeta, dbetavelo; /* Constant, always available. */ /* Error handling */ /*------------------------------------------------------------------------*/ struct wcserr *err; /* Private */ /*------------------------------------------------------------------------*/ void *padding; /* (Dummy inserted for alignment purposes.) */ }; /* Size of the spxprm struct in int units, used by the Fortran wrappers. */ #define SPXLEN (sizeof(struct spxprm)/sizeof(int)) int specx(const char *type, double spec, double restfrq, double restwav, struct spxprm *specs); /* For use in declaring function prototypes, e.g. in spcprm. */ #define SPX_ARGS double param, int nspec, int instep, int outstep, \ const double inspec[], double outspec[], int stat[] int freqafrq(SPX_ARGS); int afrqfreq(SPX_ARGS); int freqener(SPX_ARGS); int enerfreq(SPX_ARGS); int freqwavn(SPX_ARGS); int wavnfreq(SPX_ARGS); int freqwave(SPX_ARGS); int wavefreq(SPX_ARGS); int freqawav(SPX_ARGS); int awavfreq(SPX_ARGS); int waveawav(SPX_ARGS); int awavwave(SPX_ARGS); int velobeta(SPX_ARGS); int betavelo(SPX_ARGS); int freqvelo(SPX_ARGS); int velofreq(SPX_ARGS); int freqvrad(SPX_ARGS); int vradfreq(SPX_ARGS); int wavevelo(SPX_ARGS); int velowave(SPX_ARGS); int awavvelo(SPX_ARGS); int veloawav(SPX_ARGS); int wavevopt(SPX_ARGS); int voptwave(SPX_ARGS); int wavezopt(SPX_ARGS); int zoptwave(SPX_ARGS); #ifdef __cplusplus } #endif #endif /* WCSLIB_SPEC */ pywcs-1.12/wcslib/C/tab.c0000644001153600020070000012074112310355626017232 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tab.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsprintf.h" #include "tab.h" const int TABSET = 137; /* Map status return value to message. */ const char *tab_errmsg[] = { "Success", "Null tabprm pointer passed", "Memory allocation failed", "Invalid tabular parameters", "One or more of the x coordinates were invalid", "One or more of the world coordinates were invalid"}; /* Convenience macro for invoking wcserr_set(). */ #define TAB_ERRMSG(status) WCSERR_SET(status), tab_errmsg[status] /*--------------------------------------------------------------------------*/ int tabini(int alloc, int M, const int K[], struct tabprm *tab) { static const char *function = "tabini"; int k, m, N; double *dp; struct wcserr **err; if (tab == 0x0) return TABERR_NULL_POINTER; /* Initialize error message handling. */ err = &(tab->err); if (tab->err && tab->flag != -1) { free(tab->err); } tab->err = 0x0; if (M <= 0) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "M must be positive, got %d", M); } /* Determine the total number of elements in the coordinate array. */ if (K) { N = M; for (m = 0; m < M; m++) { if (K[m] < 0) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Each element of K must be " "non-negative, got %d", K[m]); } N *= K[m]; } } else { /* Axis lengths as yet unknown. */ N = 0; } /* Initialize memory management. */ if (tab->flag == -1 || tab->m_flag != TABSET) { tab->m_flag = 0; tab->m_M = 0; tab->m_N = 0; tab->m_K = 0x0; tab->m_map = 0x0; tab->m_crval = 0x0; tab->m_index = 0x0; tab->m_indxs = 0x0; tab->m_coord = 0x0; } else { /* Clear any outstanding signals set by wcstab(). */ for (m = 0; m < tab->m_M; m++) { if (tab->m_indxs[m] == (double *)0x1) tab->m_indxs[m] = 0x0; } if (tab->m_coord == (double *)0x1) tab->m_coord = 0x0; } if (tab->flag == -1) { tab->sense = 0x0; tab->p0 = 0x0; tab->delta = 0x0; tab->extrema = 0x0; tab->set_M = 0; } /* Allocate memory for arrays if required. */ if (alloc || tab->K == 0x0 || tab->map == 0x0 || tab->crval == 0x0 || tab->index == 0x0 || tab->coord == 0x0) { /* Was sufficient allocated previously? */ if (tab->m_flag == TABSET && (tab->m_M < M || tab->m_N < N)) { /* No, free it. */ tabfree(tab); } if (alloc || tab->K == 0x0) { if (tab->m_K) { /* In case the caller fiddled with it. */ tab->K = tab->m_K; } else { if (!(tab->K = calloc(M, sizeof(int)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->m_flag = TABSET; tab->m_M = M; tab->m_K = tab->K; } } if (alloc || tab->map == 0x0) { if (tab->m_map) { /* In case the caller fiddled with it. */ tab->map = tab->m_map; } else { if (!(tab->map = calloc(M, sizeof(int)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->m_flag = TABSET; tab->m_M = M; tab->m_map = tab->map; } } if (alloc || tab->crval == 0x0) { if (tab->m_crval) { /* In case the caller fiddled with it. */ tab->crval = tab->m_crval; } else { if (!(tab->crval = calloc(M, sizeof(double)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->m_flag = TABSET; tab->m_M = M; tab->m_crval = tab->crval; } } if (alloc || tab->index == 0x0) { if (tab->m_index) { /* In case the caller fiddled with it. */ tab->index = tab->m_index; } else { if (!(tab->index = calloc(M, sizeof(double *)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->m_flag = TABSET; tab->m_M = M; tab->m_N = N; tab->m_index = tab->index; if (!(tab->m_indxs = calloc(M, sizeof(double *)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } /* Recall that calloc() initializes these pointers to zero. */ if (K) { for (m = 0; m < M; m++) { if (K[m]) { if (!(tab->index[m] = calloc(K[m], sizeof(double)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->m_indxs[m] = tab->index[m]; } } } } } if (alloc || tab->coord == 0x0) { if (tab->m_coord) { /* In case the caller fiddled with it. */ tab->coord = tab->m_coord; } else if (N) { if (!(tab->coord = calloc(N, sizeof(double)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->m_flag = TABSET; tab->m_M = M; tab->m_N = N; tab->m_coord = tab->coord; } } } tab->flag = 0; tab->M = M; /* Set defaults. */ for (m = 0; m < M; m++) { tab->map[m] = -1; tab->crval[m] = 0.0; if (K) { tab->K[m] = K[m]; if ((dp = tab->index[m])) { for (k = 0; k < K[m]; k++) { *(dp++) = k; } } } else { tab->K[m] = 0; } } /* Initialize the coordinate array. */ for (dp = tab->coord; dp < tab->coord + N; dp++) { *dp = UNDEFINED; } return 0; } /*--------------------------------------------------------------------------*/ int tabmem(struct tabprm *tab) { static const char *function = "tabmem"; int m, M, N; struct wcserr **err; if (tab == 0x0) return TABERR_NULL_POINTER; err = &(tab->err); if (tab->M == 0 || tab->K == 0x0) { /* Should have been set by this time. */ return wcserr_set(WCSERR_SET(TABERR_MEMORY), "Null pointers in tabprm struct"); } N = M = tab->M; for (m = 0; m < M; m++) { if (tab->K[m] < 0) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Each element of K must be " "non-negative, got %d", M); } N *= tab->K[m]; } if (tab->m_M == 0) { tab->m_M = M; } else if (tab->m_M < M) { /* Only possible if the user changed M. */ return wcserr_set(WCSERR_SET(TABERR_MEMORY), "tabprm struct inconsistent"); } if (tab->m_N == 0) { tab->m_N = N; } else if (tab->m_N < N) { /* Only possible if the user changed K[]. */ return wcserr_set(WCSERR_SET(TABERR_MEMORY), "tabprm struct inconsistent"); } if (tab->m_K == 0x0) { if ((tab->m_K = tab->K)) { tab->m_flag = TABSET; } } if (tab->m_map == 0x0) { if ((tab->m_map = tab->map)) { tab->m_flag = TABSET; } } if (tab->m_crval == 0x0) { if ((tab->m_crval = tab->crval)) { tab->m_flag = TABSET; } } if (tab->m_index == 0x0) { if ((tab->m_index = tab->index)) { tab->m_flag = TABSET; } } for (m = 0; m < tab->m_M; m++) { if (tab->m_indxs[m] == 0x0 || tab->m_indxs[m] == (double *)0x1) { if ((tab->m_indxs[m] = tab->index[m])) { tab->m_flag = TABSET; } } } if (tab->m_coord == 0x0 || tab->m_coord == (double *)0x1) { if ((tab->m_coord = tab->coord)) { tab->m_flag = TABSET; } } tab->flag = 0; return 0; } /*--------------------------------------------------------------------------*/ int tabcpy(int alloc, const struct tabprm *tabsrc, struct tabprm *tabdst) { static const char *function = "tabcpy"; int k, m, M, n, N, status; double *dstp, *srcp; struct wcserr **err; if (tabsrc == 0x0) return TABERR_NULL_POINTER; if (tabdst == 0x0) return TABERR_NULL_POINTER; err = &(tabdst->err); M = tabsrc->M; if (M <= 0) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "M must be positive, got %d", M); } if ((status = tabini(alloc, M, tabsrc->K, tabdst))) { return status; } N = M; for (m = 0; m < M; m++) { tabdst->map[m] = tabsrc->map[m]; tabdst->crval[m] = tabsrc->crval[m]; N *= tabsrc->K[m]; } for (m = 0; m < M; m++) { if ((srcp = tabsrc->index[m])) { dstp = tabdst->index[m]; for (k = 0; k < tabsrc->K[m]; k++) { *(dstp++) = *(srcp++); } } } srcp = tabsrc->coord; dstp = tabdst->coord; for (n = 0; n < N; n++) { *(dstp++) = *(srcp++); } return 0; } /*--------------------------------------------------------------------------*/ int tabfree(struct tabprm *tab) { int m; if (tab == 0x0) return TABERR_NULL_POINTER; if (tab->flag != -1) { /* Clear any outstanding signals set by wcstab(). */ for (m = 0; m < tab->m_M; m++) { if (tab->m_indxs[m] == (double *)0x1) tab->m_indxs[m] = 0x0; } if (tab->m_coord == (double *)0x1) tab->m_coord = 0x0; /* Free memory allocated by tabini(). */ if (tab->m_flag == TABSET) { if (tab->K == tab->m_K) tab->K = 0x0; if (tab->map == tab->m_map) tab->map = 0x0; if (tab->crval == tab->m_crval) tab->crval = 0x0; if (tab->index == tab->m_index) tab->index = 0x0; if (tab->coord == tab->m_coord) tab->coord = 0x0; if (tab->m_K) free(tab->m_K); if (tab->m_map) free(tab->m_map); if (tab->m_crval) free(tab->m_crval); if (tab->m_index) { for (m = 0; m < tab->m_M; m++) { if (tab->m_indxs[m]) free(tab->m_indxs[m]); } free(tab->m_index); free(tab->m_indxs); } if (tab->m_coord) free(tab->m_coord); } /* Free memory allocated by tabset(). */ if (tab->sense) free(tab->sense); if (tab->p0) free(tab->p0); if (tab->delta) free(tab->delta); if (tab->extrema) free(tab->extrema); } tab->m_flag = 0; tab->m_M = 0; tab->m_N = 0; tab->m_K = 0x0; tab->m_map = 0x0; tab->m_crval = 0x0; tab->m_index = 0x0; tab->m_indxs = 0x0; tab->m_coord = 0x0; tab->sense = 0x0; tab->p0 = 0x0; tab->delta = 0x0; tab->extrema = 0x0; tab->set_M = 0; if (tab->err) free(tab->err); tab->err = 0x0; tab->flag = 0; return 0; } /*--------------------------------------------------------------------------*/ int tabprt(const struct tabprm *tab) { char *cp, text[128]; int j, k, m, n, nd; double *dp; if (tab == 0x0) return TABERR_NULL_POINTER; if (tab->flag != TABSET) { wcsprintf("The tabprm struct is UNINITIALIZED.\n"); return 0; } wcsprintf(" flag: %d\n", tab->flag); wcsprintf(" M: %d\n", tab->M); /* Array dimensions. */ WCSPRINTF_PTR(" K: ", tab->K, "\n"); wcsprintf(" "); for (m = 0; m < tab->M; m++) { wcsprintf("%6d", tab->K[m]); } wcsprintf("\n"); /* Map vector. */ WCSPRINTF_PTR(" map: ", tab->map, "\n"); wcsprintf(" "); for (m = 0; m < tab->M; m++) { wcsprintf("%6d", tab->map[m]); } wcsprintf("\n"); /* Reference index value. */ WCSPRINTF_PTR(" crval: ", tab->crval, "\n"); wcsprintf(" "); for (m = 0; m < tab->M; m++) { wcsprintf(" %- 11.5g", tab->crval[m]); } wcsprintf("\n"); /* Index vectors. */ WCSPRINTF_PTR(" index: ", tab->index, "\n"); for (m = 0; m < tab->M; m++) { wcsprintf(" index[%d]: ", m); WCSPRINTF_PTR("", tab->index[m], ""); if (tab->index[m]) { for (k = 0; k < tab->K[m]; k++) { if (k%5 == 0) { wcsprintf("\n "); } wcsprintf(" %- 11.5g", tab->index[m][k]); } wcsprintf("\n"); } } /* Coordinate array. */ WCSPRINTF_PTR(" coord: ", tab->coord, "\n"); dp = tab->coord; for (n = 0; n < tab->nc; n++) { /* Array index. */ j = n; cp = text; for (m = 0; m < tab->M; m++) { nd = (tab->K[m] < 10) ? 1 : 2; sprintf(cp, ",%*d", nd, j % tab->K[m] + 1); j /= tab->K[m]; cp += strlen(cp); } wcsprintf(" (*%s)", text); for (m = 0; m < tab->M; m++) { wcsprintf(" %- 11.5g", *(dp++)); } wcsprintf("\n"); } wcsprintf(" nc: %d\n", tab->nc); WCSPRINTF_PTR(" sense: ", tab->sense, "\n"); if (tab->sense) { wcsprintf(" "); for (m = 0; m < tab->M; m++) { wcsprintf("%6d", tab->sense[m]); } wcsprintf("\n"); } WCSPRINTF_PTR(" p0: ", tab->p0, "\n"); if (tab->p0) { wcsprintf(" "); for (m = 0; m < tab->M; m++) { wcsprintf("%6d", tab->p0[m]); } wcsprintf("\n"); } WCSPRINTF_PTR(" delta: ", tab->delta, "\n"); if (tab->delta) { wcsprintf(" "); for (m = 0; m < tab->M; m++) { wcsprintf(" %- 11.5g", tab->delta[m]); } wcsprintf("\n"); } WCSPRINTF_PTR(" extrema: ", tab->extrema, "\n"); dp = tab->extrema; for (n = 0; n < tab->nc/tab->K[0]; n++) { /* Array index. */ j = n; cp = text; *cp = '\0'; for (m = 1; m < tab->M; m++) { nd = (tab->K[m] < 10) ? 1 : 2; sprintf(cp, ",%*d", nd, j % tab->K[m] + 1); j /= tab->K[m]; cp += strlen(cp); } wcsprintf(" (*,*%s)", text); for (m = 0; m < 2*tab->M; m++) { if (m == tab->M) wcsprintf("-> "); wcsprintf(" %- 11.5g", *(dp++)); } wcsprintf("\n"); } WCSPRINTF_PTR(" err: ", tab->err, "\n"); if (tab->err) { wcserr_prt(tab->err, " "); } /* Memory management. */ wcsprintf(" m_flag: %d\n", tab->m_flag); wcsprintf(" m_M: %d\n", tab->m_M); wcsprintf(" m_N: %d\n", tab->m_N); WCSPRINTF_PTR(" m_K: ", tab->m_K, ""); if (tab->m_K == tab->K) wcsprintf(" (= K)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_map: ", tab->m_map, ""); if (tab->m_map == tab->map) wcsprintf(" (= map)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_crval: ", tab->m_crval, ""); if (tab->m_crval == tab->crval) wcsprintf(" (= crval)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_index: ", tab->m_index, ""); if (tab->m_index == tab->index) wcsprintf(" (= index)"); wcsprintf("\n"); for (m = 0; m < tab->M; m++) { wcsprintf(" m_indxs[%d]: ", m); WCSPRINTF_PTR("", tab->m_indxs[m], ""); if (tab->m_indxs[m] == tab->index[m]) wcsprintf(" (= index[%d])", m); wcsprintf("\n"); } WCSPRINTF_PTR(" m_coord: ", tab->m_coord, ""); if (tab->m_coord == tab->coord) wcsprintf(" (= coord)"); wcsprintf("\n"); return 0; } /*--------------------------------------------------------------------------*/ int tabset(struct tabprm *tab) { static const char *function = "tabset"; int i, ic, k, *Km, m, M, ne; double *dcrd, *dmax, *dmin, dPsi, dval, *Psi; struct wcserr **err; if (tab == 0x0) return TABERR_NULL_POINTER; err = &(tab->err); /* Check the number of tabular coordinate axes. */ if ((M = tab->M) < 1) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: M must be positive, got %d", M); } /* Check the axis lengths. */ if (!tab->K) { return wcserr_set(WCSERR_SET(TABERR_MEMORY), "Null pointers in tabprm struct"); } tab->nc = 1; for (m = 0; m < M; m++) { if (tab->K[m] < 1) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Each element of K must be positive, " "got %d", tab->K[m]); } /* Number of coordinate vectors in the coordinate array. */ tab->nc *= tab->K[m]; } /* Check that the map vector is sensible. */ if (!tab->map) { return wcserr_set(WCSERR_SET(TABERR_MEMORY), "Null pointers in tabprm struct"); } for (m = 0; m < M; m++) { i = tab->map[m]; if (i < 0) { return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Each element of map must be " "non-negative, got %d", i); } } /* Check memory allocation for the remaining vectors. */ if (!tab->crval || !tab->index || !tab->coord) { return wcserr_set(WCSERR_SET(TABERR_MEMORY), "Null pointers in tabprm struct"); } /* Take memory if signalled to by wcstab(). */ for (m = 0; m < tab->m_M; m++) { if (tab->m_indxs[m] == (double *)0x1 && (tab->m_indxs[m] = tab->index[m])) { tab->m_flag = TABSET; } } if (tab->m_coord == (double *)0x1 && (tab->m_coord = tab->coord)) { tab->m_flag = TABSET; } /* Allocate memory for work vectors. */ if (tab->flag != TABSET || tab->set_M < M) { /* Free memory that may have been allocated previously. */ if (tab->sense) free(tab->sense); if (tab->p0) free(tab->p0); if (tab->delta) free(tab->delta); if (tab->extrema) free(tab->extrema); /* Allocate memory for internal arrays. */ if (!(tab->sense = calloc(M, sizeof(int)))) { return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } if (!(tab->p0 = calloc(M, sizeof(int)))) { free(tab->sense); return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } if (!(tab->delta = calloc(M, sizeof(double)))) { free(tab->sense); free(tab->p0); return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } ne = M * tab->nc * 2 / tab->K[0]; if (!(tab->extrema = calloc(ne, sizeof(double)))) { free(tab->sense); free(tab->p0); free(tab->delta); return wcserr_set(TAB_ERRMSG(TABERR_MEMORY)); } tab->set_M = M; } /* Check that the index vectors are monotonic. */ Km = tab->K; for (m = 0; m < M; m++, Km++) { tab->sense[m] = 0; if (*Km > 1) { if ((Psi = tab->index[m]) == 0x0) { /* Default indexing. */ tab->sense[m] = 1; } else { for (k = 0; k < *Km-1; k++) { switch (tab->sense[m]) { case 0: if (Psi[k] < Psi[k+1]) { /* Monotonic increasing. */ tab->sense[m] = 1; } else if (Psi[k] > Psi[k+1]) { /* Monotonic decreasing. */ tab->sense[m] = -1; } break; case 1: if (Psi[k] > Psi[k+1]) { /* Should be monotonic increasing. */ free(tab->sense); free(tab->p0); free(tab->delta); free(tab->extrema); return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Index vectors are not " "monotonically increasing"); } break; case -1: if (Psi[k] < Psi[k+1]) { /* Should be monotonic decreasing. */ free(tab->sense); free(tab->p0); free(tab->delta); free(tab->extrema); return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Index vectors are not " "monotonically decreasing"); } break; } } } if (tab->sense[m] == 0) { free(tab->sense); free(tab->p0); free(tab->delta); free(tab->extrema); return wcserr_set(WCSERR_SET(TABERR_BAD_PARAMS), "Invalid tabular parameters: Index vectors are not monotonic"); } } } /* Find the extremal values of the coordinate elements in each row. */ dcrd = tab->coord; dmin = tab->extrema; dmax = tab->extrema + M; for (ic = 0; ic < tab->nc; ic += tab->K[0]) { for (m = 0; m < M; m++, dcrd++) { if (tab->K[0] > 1) { /* Extrapolate a little before the start of the row. */ Psi = tab->index[0]; if (Psi == 0x0) { dPsi = 1.0; } else { dPsi = Psi[1] - Psi[0]; } dval = *dcrd; if (dPsi != 0.0) { dval -= 0.5 * (*(dcrd+M) - *dcrd)/dPsi; } *(dmax+m) = *(dmin+m) = dval; } else { *(dmax+m) = *(dmin+m) = *dcrd; } } dcrd -= M; for (i = 0; i < tab->K[0]; i++) { for (m = 0; m < M; m++, dcrd++) { if (*(dmax+m) < *dcrd) *(dmax+m) = *dcrd; if (*(dmin+m) > *dcrd) *(dmin+m) = *dcrd; if (tab->K[0] > 1 && i == tab->K[0]-1) { /* Extrapolate a little beyond the end of the row. */ Psi = tab->index[0]; if (Psi == 0x0) { dPsi = 1.0; } else { dPsi = Psi[i] - Psi[i-1]; } dval = *dcrd; if (dPsi != 0.0) { dval += 0.5 * (*dcrd - *(dcrd-M))/dPsi; } if (*(dmax+m) < dval) *(dmax+m) = dval; if (*(dmin+m) > dval) *(dmin+m) = dval; } } } dmin += 2*M; dmax += 2*M; } tab->flag = TABSET; return 0; } /*--------------------------------------------------------------------------*/ int tabx2s( struct tabprm *tab, int ncoord, int nelem, const double x[], double world[], int stat[]) { static const char *function = "tabx2s"; int i, iv, k, *Km, m, M, n, nv, offset, p1, status; double *coord, *Psi, psi_m, upsilon, wgt; register int *statp; register const double *xp; register double *wp; struct wcserr **err; if (tab == 0x0) return TABERR_NULL_POINTER; err = &(tab->err); /* Initialize if required. */ if (tab->flag != TABSET) { if ((status = tabset(tab))) return status; } /* This is used a lot. */ M = tab->M; status = 0; xp = x; wp = world; statp = stat; for (n = 0; n < ncoord; n++) { /* Determine the indexes. */ Km = tab->K; for (m = 0; m < M; m++, Km++) { /* N.B. psi_m and Upsilon_m are 1-relative FITS indexes. */ i = tab->map[m]; psi_m = *(xp+i) + tab->crval[m]; Psi = tab->index[m]; if (Psi == 0x0) { /* Default indexing is simple. */ upsilon = psi_m; } else { /* To ease confusion, decrement Psi so that we can use 1-relative C array indexing to match the 1-relative FITS indexing. */ Psi--; if (*Km == 1) { /* Index vector is degenerate. */ if (Psi[1]-0.5 <= psi_m && psi_m <= Psi[1]+0.5) { upsilon = psi_m; } else { *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_X)); goto next; } } else { /* Interpolate in the indexing vector. */ if (tab->sense[m] == 1) { /* Monotonic increasing index values. */ if (psi_m < Psi[1]) { if (Psi[1] - 0.5*(Psi[2]-Psi[1]) <= psi_m) { /* Allow minor extrapolation. */ k = 1; } else { /* Index is out of range. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_X)); goto next; } } else if (Psi[*Km] < psi_m) { if (psi_m <= Psi[*Km] + 0.5*(Psi[*Km]-Psi[*Km-1])) { /* Allow minor extrapolation. */ k = *Km - 1; } else { /* Index is out of range. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_X)); goto next; } } else { for (k = 1; k < *Km; k++) { if (psi_m < Psi[k]) { continue; } if (Psi[k] == psi_m && psi_m < Psi[k+1]) { break; } if (Psi[k] < psi_m && psi_m <= Psi[k+1]) { break; } } } } else { /* Monotonic decreasing index values. */ if (psi_m > Psi[1]) { if (Psi[1] + 0.5*(Psi[1]-Psi[2]) >= psi_m) { /* Allow minor extrapolation. */ k = 1; } else { /* Index is out of range. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_X)); goto next; } } else if (psi_m < Psi[*Km]) { if (Psi[*Km] - 0.5*(Psi[*Km-1]-Psi[*Km]) <= psi_m) { /* Allow minor extrapolation. */ k = *Km - 1; } else { /* Index is out of range. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_X)); goto next; } } else { for (k = 1; k < *Km; k++) { if (psi_m > Psi[k]) { continue; } if (Psi[k] == psi_m && psi_m > Psi[k+1]) { break; } if (Psi[k] > psi_m && psi_m >= Psi[k+1]) { break; } } } } upsilon = k + (psi_m - Psi[k]) / (Psi[k+1] - Psi[k]); } } if (upsilon < 0.5 || upsilon > *Km + 0.5) { /* Index out of range. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_X)); goto next; } /* Fiducial array indices and fractional offset. p1 is 1-relative while tab::p0 is 0-relative. */ p1 = (int)floor(upsilon); tab->p0[m] = p1 - 1; tab->delta[m] = upsilon - p1; if (p1 == 0) { tab->p0[m] += 1; tab->delta[m] -= 1.0; } else if (p1 == *Km && *Km > 1) { tab->p0[m] -= 1; tab->delta[m] += 1.0; } } /* Now interpolate in the coordinate array; the M-dimensional linear */ /* interpolation algorithm is described in Sect. 3.4 of WCS Paper IV. */ for (m = 0; m < M; m++) { i = tab->map[m]; *(wp+i) = 0.0; } /* Loop over the 2^M vertices surrounding P. */ nv = 1 << M; for (iv = 0; iv < nv; iv++) { /* Locate vertex in the coordinate array and compute its weight. */ offset = 0; wgt = 1.0; for (m = M-1; m >= 0; m--) { offset *= tab->K[m]; offset += tab->p0[m]; if (iv & (1 << m)) { if (tab->K[m] > 1) offset++; wgt *= tab->delta[m]; } else { wgt *= 1.0 - tab->delta[m]; } } if (wgt == 0.0) continue; /* Add the contribution from this vertex to each element. */ coord = tab->coord + offset*M; for (m = 0; m < M; m++) { i = tab->map[m]; *(wp+i) += *(coord++) * wgt; } if (wgt == 1.0) break; } *statp = 0; next: xp += nelem; wp += nelem; statp++; } return status; } /*--------------------------------------------------------------------------*/ int tabs2x( struct tabprm* tab, int ncoord, int nelem, const double world[], double x[], int stat[]) { static const char *function = "tabs2x"; int tabedge(struct tabprm *); int tabrow(struct tabprm *, const double *); int tabvox(struct tabprm *, const double *, int, double **, unsigned int *); int edge, i, ic, iv, k, *Km, M, m, n, nv, offset, status; double *dcrd, delta, *Psi, psi_m, **tabcoord, upsilon; register int *statp; register const double *wp; register double *xp; struct wcserr **err; if (tab == 0x0) return TABERR_NULL_POINTER; err = &(tab->err); /* Initialize if required. */ if (tab->flag != TABSET) { if ((status = tabset(tab))) return status; } /* This is used a lot. */ M = tab->M; if (M > 1) { nv = 1 << M; tabcoord = calloc(nv, sizeof(double *)); } status = 0; wp = world; xp = x; statp = stat; for (n = 0; n < ncoord; n++) { /* Locate this coordinate in the coordinate array. */ edge = 0; for (m = 0; m < M; m++) { tab->p0[m] = 0; } for (ic = 0; ic < tab->nc; ic++) { if (tab->p0[0] == 0) { /* New row, could it contain a solution? */ if (edge || tabrow(tab, wp)) { /* No, skip it. */ ic += tab->K[0]; tab->p0[1]++; edge = tabedge(tab); /* Because ic will be incremented when the loop is reentered. */ ic--; continue; } } if (M == 1) { /* Deal with the one-dimensional case separately for efficiency. */ if (*wp == tab->coord[0]) { tab->p0[0] = 0; tab->delta[0] = 0.0; break; } else if (ic < tab->nc - 1) { if (((tab->coord[ic] <= *wp && *wp <= tab->coord[ic+1]) || (tab->coord[ic] >= *wp && *wp >= tab->coord[ic+1])) && (tab->index[0] == 0x0 || tab->index[0][ic] != tab->index[0][ic+1])) { tab->p0[0] = ic; tab->delta[0] = (*wp - tab->coord[ic]) / (tab->coord[ic+1] - tab->coord[ic]); break; } } } else { /* Multi-dimensional tables are harder. */ if (!edge) { /* Addresses of the coordinates for each corner of the "voxel". */ for (iv = 0; iv < nv; iv++) { offset = 0; for (m = M-1; m >= 0; m--) { offset *= tab->K[m]; offset += tab->p0[m]; if ((iv & (1 << m)) && (tab->K[m] > 1)) offset++; } tabcoord[iv] = tab->coord + offset*M; } if (tabvox(tab, wp, 0, tabcoord, 0x0) == 0) { /* Found a solution. */ break; } } /* Next voxel. */ tab->p0[0]++; edge = tabedge(tab); } } if (ic == tab->nc) { /* Coordinate not found; allow minor extrapolation. */ if (M == 1) { /* Should there be a solution? */ if (tab->extrema[0] <= *wp && *wp <= tab->extrema[1]) { dcrd = tab->coord; for (i = 0; i < 2; i++) { if (i) dcrd += tab->K[0] - 2; delta = (*wp - *dcrd) / (*(dcrd+1) - *dcrd); if (i == 0) { if (-0.5 <= delta && delta <= 0.0) { tab->p0[0] = 0; tab->delta[0] = delta; ic = 0; break; } } else { if (1.0 <= delta && delta <= 1.5) { tab->p0[0] = tab->K[0] - 1; tab->delta[0] = delta - 1.0; ic = 0; } } } } } else { /* Multi-dimensional tables. */ /* >>> TBD <<< */ } } if (ic == tab->nc) { /* Coordinate not found. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_WORLD)); } else { /* Determine the intermediate world coordinates. */ Km = tab->K; for (m = 0; m < M; m++, Km++) { /* N.B. Upsilon_m and psi_m are 1-relative FITS indexes. */ upsilon = (tab->p0[m] + 1) + tab->delta[m]; if (upsilon < 0.5 || upsilon > *Km + 0.5) { /* Index out of range. */ *statp = 1; status = wcserr_set(TAB_ERRMSG(TABERR_BAD_WORLD)); } else { /* Do inverse lookup of the index vector. */ Psi = tab->index[m]; if (Psi == 0x0) { /* Default indexing. */ psi_m = upsilon; } else { /* Decrement Psi and use 1-relative C array indexing to match the 1-relative FITS indexing. */ Psi--; if (*Km == 1) { /* Degenerate index vector. */ psi_m = Psi[1]; } else { k = (int)(upsilon); psi_m = Psi[k]; if (k < *Km) { psi_m += (upsilon - k) * (Psi[k+1] - Psi[k]); } } } i = tab->map[m]; xp[i] = psi_m - tab->crval[m]; } } *statp = 0; } wp += nelem; xp += nelem; statp++; } if (M > 1) free(tabcoord); return status; } /*---------------------------------------------------------------------------- * Convenience routine to deal with of edge effects in tabprm::p0. *---------------------------------------------------------------------------*/ int tabedge(struct tabprm* tab) { int edge, *Km, m; edge = 0; Km = tab->K; for (m = 0; m < tab->M; m++, Km++) { if (tab->p0[m] == *Km) { /* p0 has been incremented beyond the end of the row, point it to the next one. */ tab->p0[m] = 0; tab->p0[m+1]++; } else if (tab->p0[m] == *Km - 1 && *Km > 1) { /* p0 is sitting at the end of a non-degenerate row. */ edge = 1; } } return edge; } /*---------------------------------------------------------------------------- * Quick test to see whether the world coordinate indicated by wp could lie * somewhere along (or near) the row of the image indexed by tabprm::p0. * Return 0 if so, 1 otherwise. * * tabprm::p0 selects a particular row of the image, p0[0] being ignored (i.e. * treated as zero). Adjacent rows that delimit a row of "voxels" are formed * by incrementing elements other than p0[0] in all binary combinations. N.B. * these are not the same as the voxels (pixels) that are indexed by, and * centred on, integral pixel coordinates in FITS. * * To see why it is necessary to examine the adjacent rows, consider the 2-D * case where the first world coordinate element is constant along each row. * If the first element of wp has value 0.5, and its value in the row indexed * by p0 has value 0, and in the next row it has value 1, then it is clear that * the solution lies in neither row but somewhere between them. Thus both rows * will be involved in finding the solution. * * tabprm::extrema is the address of the first element of a 1-D array that * records the minimum and maximum value of each element of the coordinate * vector in each row of the coordinate array, treated as though it were * defined as * * double extrema[K_M]...[K_2][2][M] * * The minimum is recorded in the first element of the compressed K_1 * dimension, then the maximum. *---------------------------------------------------------------------------*/ int tabrow(struct tabprm* tab, const double *wp) { int iv, M, m, nv, offset; unsigned int eq, gt, lt; const double tol = 1e-10; double *cp, w; M = tab->M; /* The number of corners in a "voxel". We need examine only half this number of rows. The extra factor of two will be used to select between the minimal and maximal values in each row. */ nv = 1 << M; eq = 0; lt = 0; gt = 0; for (iv = 0; iv < nv; iv++) { /* Find the index into tabprm::extrema for this row. */ offset = 0; for (m = M-1; m > 0; m--) { offset *= tab->K[m]; offset += tab->p0[m]; /* Select the row. */ if (iv & (1 << m)) { if (tab->K[m] > 1) offset++; } } /* The K_1 dimension has length 2 (see prologue). */ offset *= 2; /* Select the minimum on even numbered iterations, else the maximum. */ if (iv & 1) offset++; /* The last dimension has length M (see prologue). */ offset *= M; /* Address of the extremal elements (min or max) for this row. */ cp = tab->extrema + offset; /* For each coordinate element, we only need to find one row where its minimum value is less than that of wp, and one row where the maximum value is greater. That doesn't mean that there is a solution, only that there might be. */ for (m = 0; m < M; m++, cp++) { /* Apply the axis mapping. */ w = wp[tab->map[m]]; /* Finally the test itself; set bits in the bitmask. */ if (fabs(*cp - w) < tol) { eq |= (1 << m); } else if (*cp < w) { lt |= (1 << m); } else if (*cp > w) { gt |= (1 << m); } } /* Have all bits been switched on? */ if ((lt | eq) == nv-1 && (gt | eq) == nv-1) { /* A solution could lie within this row of voxels. */ return 0; } } /* No solution in this row. */ return 1; } /*---------------------------------------------------------------------------- * Does the world coordinate indicated by wp lie within the voxel indexed by * tabprm::p0? If so, do a binary chop of the interior of the voxel to find * it and return 0, with tabprm::delta set to the solution. Else return 1. * * As in tabrow(), a "voxel" is formed by incrementing the elements of * tabprm::p0 in all binary combinations. Note that these are not the same as * the voxels (pixels) that are indexed by, and centred on, integral pixel * coordinates in FITS. * * tabvox() calls itself recursively. When called from outside, level, being * the level of recursion, should be given as zero. tabcoord is an array * holding the addresses of the coordinates for each corner of the voxel. * vox is the address of a work array (vox2) used during recursive calls to * dissect the voxel. It is ignored when tabvox() is called from outside * (level == 0). * * It is assumed that the image dimensions are no greater than 16. ----------------------------------------------------------------------------*/ int tabvox( struct tabprm* tab, const double *wp, int level, double **tabcoord, unsigned int *vox) { int i, iv, jv, M, m, nv; unsigned int eq, et, gt, lt, vox2[16]; const double tol = 1e-10; double coord[16], *cp, dv, w, wgt; M = tab->M; /* The number of corners in a voxel. */ nv = 1 << M; dv = 1.0; for (i = 0; i < level; i++) { dv /= 2.0; } /* Could the coordinate lie within this voxel (level == 0) or sub-voxel (level > 0)? We use the fact that with linear interpolation the coordinate elements are extremal in a corner and test each one. */ lt = 0; gt = 0; eq = 0; for (iv = 0; iv < nv; iv++) { /* Select a corner of the sub-voxel. */ for (m = 0; m < M; m++) { coord[m] = 0.0; tab->delta[m] = level ? dv*vox[m] : 0.0; if (iv & (1 << m)) { tab->delta[m] += dv; } } /* Compute the coordinates of this corner of the sub-voxel by linear interpolation using the weighting algorithm described in Sect. 3.4 of WCS Paper IV. */ for (jv = 0; jv < nv; jv++) { /* Find the weight for this corner of the parent voxel. */ wgt = 1.0; for (m = 0; m < M; m++) { if (jv & (1 << m)) { wgt *= tab->delta[m]; } else { wgt *= 1.0 - tab->delta[m]; } } if (wgt == 0.0) continue; /* Add its contribution to each coordinate element. */ cp = tabcoord[jv]; for (m = 0; m < M; m++) { coord[m] += *(cp++) * wgt; } if (wgt == 1.0) break; } /* Coordinate elements are minimal or maximal in a corner. */ et = 0; for (m = 0; m < M; m++) { /* Apply the axis mapping. */ w = wp[tab->map[m]]; /* Finally the test itself; set bits in the bitmask. */ if (fabs(coord[m] - w) < tol) { et |= (1 << m); } else if (coord[m] < w) { lt |= (1 << m); } else if (coord[m] > w) { gt |= (1 << m); } } if (et == nv-1) { /* We've stumbled across a solution in this corner of the sub-voxel. */ return 0; } eq |= et; } /* Could the coordinate lie within this sub-voxel? */ if ((lt | eq) == nv-1 && (gt | eq) == nv-1) { /* Yes it could, but does it? */ /* Is it time to stop the recursion? */ if (level == 31) { /* We have a solution, squeeze out the last bit of juice. */ dv /= 2.0; for (m = 0; m < M; m++) { tab->delta[m] = dv * (2.0*vox[m] + 1.0); } return 0; } /* Subdivide the sub-voxel and try again for each subdivision. */ for (iv = 0; iv < nv; iv++) { /* Select the subdivision. */ for (m = 0; m < M; m++) { vox2[m] = level ? 2*vox[m] : 0; if (iv & (1 << m)) { vox2[m]++; } } /* Recurse. */ if (tabvox(tab, wp, level+1, tabcoord, vox2) == 0) { return 0; } } } /* No solution in this sub-voxel. */ return 1; } pywcs-1.12/wcslib/C/tab.h0000644001153600020070000005621112310355626017237 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tab.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement tabular coordinate systems as * defined by the FITS World Coordinate System (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (paper I) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the tab routines * --------------------------- * These routines implement the part of the FITS WCS standard that deals with * tabular coordinates, i.e. coordinates that are defined via a lookup table. * They define methods to be used for computing tabular world coordinates from * intermediate world coordinates (a linear transformation of image pixel * coordinates), and vice versa. They are based on the tabprm struct which * contains all information needed for the computations. The struct contains * some members that must be set by the user, and others that are maintained * by these routines, somewhat like a C++ class but with no encapsulation. * * tabini(), tabmem(), tabcpy(), and tabfree() are provided to manage the * tabprm struct, and another, tabprt(), to print its contents. * * A setup routine, tabset(), computes intermediate values in the tabprm struct * from parameters in it that were supplied by the user. The struct always * needs to be set up by tabset() but it need not be called explicitly - refer * to the explanation of tabprm::flag. * * tabx2s() and tabs2x() implement the WCS tabular coordinate transformations. * * Accuracy: * --------- * No warranty is given for the accuracy of these routines (refer to the * copyright notice); intending users must satisfy for themselves their * adequacy for the intended purpose. However, closure effectively to within * double precision rounding error was demonstrated by test routine ttab.c * which accompanies this software. * * * tabini() - Default constructor for the tabprm struct * ---------------------------------------------------- * tabini() allocates memory for arrays in a tabprm struct and sets all members * of the struct to default values. * * PLEASE NOTE: every tabprm struct should be initialized by tabini(), possibly * repeatedly. On the first invokation, and only the first invokation, the * flag member of the tabprm struct must be set to -1 to initialize memory * management, regardless of whether tabini() will actually be used to allocate * memory. * * Given: * alloc int If true, allocate memory unconditionally for arrays in * the tabprm struct. * * If false, it is assumed that pointers to these arrays * have been set by the user except if they are null * pointers in which case memory will be allocated for * them regardless. (In other words, setting alloc true * saves having to initalize these pointers to zero.) * * M int The number of tabular coordinate axes. * * K const int[] * Vector of length M whose elements (K_1, K_2,... K_M) * record the lengths of the axes of the coordinate array * and of each indexing vector. M and K[] are used to * determine the length of the various tabprm arrays and * therefore the amount of memory to allocate for them. * Their values are copied into the tabprm struct. * * It is permissible to set K (i.e. the address of the * array) to zero which has the same effect as setting * each element of K[] to zero. In this case no memory * will be allocated for the index vectors or coordinate * array in the tabprm struct. These together with the * K vector must be set separately before calling * tabset(). * * Given and returned: * tab struct tabprm* * Tabular transformation parameters. Note that, in * order to initialize memory management tabprm::flag * should be set to -1 when tab is initialized for the * first time (memory leaks may result if it had already * been initialized). * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * 2: Memory allocation failed. * 3: Invalid tabular parameters. * * For returns > 1, a detailed error message is set in * tabprm::err if enabled, see wcserr_enable(). * * * tabmem() - Acquire tabular memory * --------------------------------- * tabmem() takes control of memory allocated by the user for arrays in the * tabprm struct. * * Given and returned: * tab struct tabprm* * Tabular transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * 2: Memory allocation failed. * * For returns > 1, a detailed error message is set in * tabprm::err if enabled, see wcserr_enable(). * * * tabcpy() - Copy routine for the tabprm struct * --------------------------------------------- * tabcpy() does a deep copy of one tabprm struct to another, using tabini() to * allocate memory for its arrays if required. Only the "information to be * provided" part of the struct is copied; a call to tabset() is required to * set up the remainder. * * Given: * alloc int If true, allocate memory unconditionally for arrays in * the tabprm struct. * * If false, it is assumed that pointers to these arrays * have been set by the user except if they are null * pointers in which case memory will be allocated for * them regardless. (In other words, setting alloc true * saves having to initalize these pointers to zero.) * * tabsrc const struct tabprm* * Struct to copy from. * * Given and returned: * tabdst struct tabprm* * Struct to copy to. tabprm::flag should be set to -1 * if tabdst was not previously initialized (memory leaks * may result if it was previously initialized). * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * 2: Memory allocation failed. * * For returns > 1, a detailed error message is set in * tabprm::err (associated with tabdst) if enabled, see * wcserr_enable(). * * * tabfree() - Destructor for the tabprm struct * -------------------------------------------- * tabfree() frees memory allocated for the tabprm arrays by tabini(). * tabini() records the memory it allocates and tabfree() will only attempt to * free this. * * PLEASE NOTE: tabfree() must not be invoked on a tabprm struct that was not * initialized by tabini(). * * Returned: * tab struct tabprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * * * tabprt() - Print routine for the tabprm struct * ---------------------------------------------- * tabprt() prints the contents of a tabprm struct using wcsprintf(). Mainly * intended for diagnostic purposes. * * Given: * tab const struct tabprm* * Tabular transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * * * tabset() - Setup routine for the tabprm struct * ----------------------------------------------- * tabset() allocates memory for work arrays in the tabprm struct and sets up * the struct according to information supplied within it. * * Note that this routine need not be called directly; it will be invoked by * tabx2s() and tabs2x() if tabprm::flag is anything other than a predefined * magic value. * * Given and returned: * tab struct tabprm* * Tabular transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * 3: Invalid tabular parameters. * * For returns > 1, a detailed error message is set in * tabprm::err if enabled, see wcserr_enable(). * * * tabx2s() - Pixel-to-world transformation * ---------------------------------------- * tabx2s() transforms intermediate world coordinates to world coordinates * using coordinate lookup. * * Given and returned: * tab struct tabprm* * Tabular transformation parameters. * * Given: * ncoord, * nelem int The number of coordinates, each of vector length * nelem. * * x const double[ncoord][nelem] * Array of intermediate world coordinates, SI units. * * Returned: * world double[ncoord][nelem] * Array of world coordinates, in SI units. * * stat int[ncoord] * Status return value status for each coordinate: * 0: Success. * 1: Invalid intermediate world coordinate. * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * 3: Invalid tabular parameters. * 4: One or more of the x coordinates were invalid, * as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * tabprm::err if enabled, see wcserr_enable(). * * * tabs2x() - World-to-pixel transformation * ---------------------------------------- * tabs2x() transforms world coordinates to intermediate world coordinates. * * Given and returned: * tab struct tabprm* * Tabular transformation parameters. * * Given: * ncoord, * nelem int The number of coordinates, each of vector length * nelem. * world const double[ncoord][nelem] * Array of world coordinates, in SI units. * * Returned: * x double[ncoord][nelem] * Array of intermediate world coordinates, SI units. * stat int[ncoord] * Status return value status for each vector element: * 0: Success. * 1: Invalid world coordinate. * * Function return value: * int Status return value: * 0: Success. * 1: Null tabprm pointer passed. * 3: Invalid tabular parameters. * 5: One or more of the world coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * tabprm::err if enabled, see wcserr_enable(). * * * tabprm struct - Tabular transformation parameters * ------------------------------------------------- * The tabprm struct contains information required to transform tabular * coordinates. It consists of certain members that must be set by the user * ("given") and others that are set by the WCSLIB routines ("returned"). Some * of the latter are supplied for informational purposes while others are for * internal use only. * * int flag * (Given and returned) This flag must be set to zero whenever any of the * following tabprm structure members are set or changed: * * - tabprm::M (q.v., not normally set by the user), * - tabprm::K (q.v., not normally set by the user), * - tabprm::map, * - tabprm::crval, * - tabprm::index, * - tabprm::coord. * * This signals the initialization routine, tabset(), to recompute the * returned members of the tabprm struct. tabset() will reset flag to * indicate that this has been done. * * PLEASE NOTE: flag should be set to -1 when tabini() is called for the * first time for a particular tabprm struct in order to initialize memory * management. It must ONLY be used on the first initialization otherwise * memory leaks may result. * * int M * (Given or returned) Number of tabular coordinate axes. * * If tabini() is used to initialize the linprm struct (as would normally * be the case) then it will set M from the value passed to it as a * function argument. The user should not subsequently modify it. * * int *K * (Given or returned) Pointer to the first element of a vector of length * tabprm::M whose elements (K_1, K_2,... K_M) record the lengths of the * axes of the coordinate array and of each indexing vector. * * If tabini() is used to initialize the linprm struct (as would normally * be the case) then it will set K from the array passed to it as a * function argument. The user should not subsequently modify it. * * int *map * (Given) Pointer to the first element of a vector of length tabprm::M * that defines the association between axis m in the M-dimensional * coordinate array (1 <= m <= M) and the indices of the intermediate world * coordinate and world coordinate arrays, x[] and world[], in the argument * lists for tabx2s() and tabs2x(). * * When x[] and world[] contain the full complement of coordinate elements * in image-order, as will usually be the case, then map[m-1] == i-1 for * axis i in the N-dimensional image (1 <= i <= N). In terms of the FITS * keywords * * map[PVi_3a - 1] == i - 1. * * However, a different association may result if x[], for example, only * contains a (relevant) subset of intermediate world coordinate elements. * For example, if M == 1 for an image with N > 1, it is possible to fill * x[] with the relevant coordinate element with nelem set to 1. In this * case map[0] = 0 regardless of the value of i. * * double *crval * (Given) Pointer to the first element of a vector of length tabprm::M * whose elements contain the index value for the reference pixel for each * of the tabular coordinate axes. * * double **index * (Given) Pointer to the first element of a vector of length tabprm::M of * pointers to vectors of lengths (K_1, K_2,... K_M) of 0-relative indexes * (see tabprm::K). * * The address of any or all of these index vectors may be set to zero, * i.e. * = index[m] == 0; * * this is interpreted as default indexing, i.e. * = index[m][k] = k; * * double *coord * (Given) Pointer to the first element of the tabular coordinate array, * treated as though it were defined as * = double coord[K_M]...[K_2][K_1][M]; * * (see tabprm::K) i.e. with the M dimension varying fastest so that the * M elements of a coordinate vector are stored contiguously in memory. * * int nc * (Returned) Total number of coordinate vectors in the coordinate array * being the product K_1 * K_2 * ... * K_M (see tabprm::K). * * int padding * (An unused variable inserted for alignment purposes only.) * * int *sense * (Returned) Pointer to the first element of a vector of length tabprm::M * whose elements indicate whether the corresponding indexing vector is * monotonic increasing (+1), or decreasing (-1). * * int *p0 * (Returned) Pointer to the first element of a vector of length tabprm::M * of interpolated indices into the coordinate array such that Upsilon_m, * as defined in Paper III, is equal to (p0[m] + 1) + tabprm::delta[m]. * * double *delta * (Returned) Pointer to the first element of a vector of length tabprm::M * of interpolated indices into the coordinate array such that Upsilon_m, * as defined in Paper III, is equal to (tabprm::p0[m] + 1) + delta[m]. * * double *extrema * (Returned) Pointer to the first element of an array that records the * minimum and maximum value of each element of the coordinate vector in * each row of the coordinate array, treated as though it were defined as * = double extrema[K_M]...[K_2][2][M] * * (see tabprm::K). The minimum is recorded in the first element of the * compressed K_1 dimension, then the maximum. This array is used by the * inverse table lookup function, tabs2x(), to speed up table searches. * * struct wcserr *err * (Returned) If enabled, when an error status is returned this struct * contains detailed information about the error, see wcserr_enable(). * * int m_flag * (For internal use only.) * int m_M * (For internal use only.) * int m_N * (For internal use only.) * int set_M * (For internal use only.) * int m_K * (For internal use only.) * int m_map * (For internal use only.) * int m_crval * (For internal use only.) * int m_index * (For internal use only.) * int m_indxs * (For internal use only.) * int m_coord * (For internal use only.) * * * Global variable: const char *tab_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_TAB #define WCSLIB_TAB #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif extern const char *tab_errmsg[]; enum tab_errmsg_enum { TABERR_SUCCESS = 0, /* Success. */ TABERR_NULL_POINTER = 1, /* Null tabprm pointer passed. */ TABERR_MEMORY = 2, /* Memory allocation failed. */ TABERR_BAD_PARAMS = 3, /* Invalid tabular parameters. */ TABERR_BAD_X = 4, /* One or more of the x coordinates were invalid. */ TABERR_BAD_WORLD = 5 /* One or more of the world coordinates were invalid. */ }; struct tabprm { /* Initialization flag (see the prologue above). */ /*------------------------------------------------------------------------*/ int flag; /* Set to zero to force initialization. */ /* Parameters to be provided (see the prologue above). */ /*------------------------------------------------------------------------*/ int M; /* Number of tabular coordinate axes. */ int *K; /* Vector of length M whose elements */ /* (K_1, K_2,... K_M) record the lengths of */ /* the axes of the coordinate array and of */ /* each indexing vector. */ int *map; /* Vector of length M usually such that */ /* map[m-1] == i-1 for coordinate array */ /* axis m and image axis i (see above). */ double *crval; /* Vector of length M containing the index */ /* value for the reference pixel for each */ /* of the tabular coordinate axes. */ double **index; /* Vector of pointers to M indexing vectors */ /* of lengths (K_1, K_2,... K_M). */ double *coord; /* (1+M)-dimensional tabular coordinate */ /* array (see above). */ /* Information derived from the parameters supplied. */ /*------------------------------------------------------------------------*/ int nc; /* Number of coordinate vectors (of length */ /* M) in the coordinate array. */ int padding; /* (Dummy inserted for alignment purposes.) */ int *sense; /* Vector of M flags that indicate whether */ /* the Mth indexing vector is monotonic */ /* increasing, or else decreasing. */ int *p0; /* Vector of M indices. */ double *delta; /* Vector of M increments. */ double *extrema; /* (1+M)-dimensional array of coordinate */ /* extrema. */ /* Error handling */ /*------------------------------------------------------------------------*/ struct wcserr *err; /* Private - the remainder are for memory management. */ /*------------------------------------------------------------------------*/ int m_flag, m_M, m_N; int set_M; int *m_K, *m_map; double *m_crval, **m_index, **m_indxs, *m_coord; }; /* Size of the tabprm struct in int units, used by the Fortran wrappers. */ #define TABLEN (sizeof(struct tabprm)/sizeof(int)) int tabini(int alloc, int M, const int K[], struct tabprm *tab); int tabmem(struct tabprm *tab); int tabcpy(int alloc, const struct tabprm *tabsrc, struct tabprm *tabdst); int tabfree(struct tabprm *tab); int tabprt(const struct tabprm *tab); int tabset(struct tabprm *tab); int tabx2s(struct tabprm *tab, int ncoord, int nelem, const double x[], double world[], int stat[]); int tabs2x(struct tabprm *tab, int ncoord, int nelem, const double world[], double x[], int stat[]); /* Deprecated. */ #define tabini_errmsg tab_errmsg #define tabcpy_errmsg tab_errmsg #define tabfree_errmsg tab_errmsg #define tabprt_errmsg tab_errmsg #define tabset_errmsg tab_errmsg #define tabx2s_errmsg tab_errmsg #define tabs2x_errmsg tab_errmsg #ifdef __cplusplus } #endif #endif /* WCSLIB_TAB */ pywcs-1.12/wcslib/C/test/0000755001153600020070000000000012310355732017270 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/C/test/bth.keyrec0000644001153600020070000005362512310355626021266 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # WCSLIB 4.10 - an implementation of the FITS WCS standard. # Copyright (C) 1995-2012, Mark Calabretta # # This file is part of WCSLIB. # # WCSLIB is free software: you can redistribute it and/or modify it under the # terms of the GNU Lesser General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY # WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS # FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for # more details. # # You should have received a copy of the GNU Lesser General Public License # along with WCSLIB. If not, see . # # Correspondence concerning WCSLIB may be directed to: # Internet email: mcalabre@atnf.csiro.au # Postal address: Dr. Mark Calabretta # Australia Telescope National Facility, CSIRO # PO Box 76 # Epping NSW 1710 # AUSTRALIA # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: bth.keyrec,v 4.10 2012/02/05 23:41:44 cal103 Exp $ #----------------------------------------------------------------------------- # FITS header keyrecords used for testing by tbth1. # # Use 'tofits' (supplied) to convert this file to proper FITS format via # # tofits < bth.keyrec > bth.fits # # Lines in this file beginning with '#' are ignored by tofits. #----------------------------------------------------------------------------- XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 3330 / width of table in bytes NAXIS2 = 68 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 33 / number of fields in each row COMMENT wcsbth() ignores all of the above keywords except for TFIELDS which it COMMENT only considers to be advisory. In fact, TFIELDS here is incorrect COMMENT (deliberately) since WCS keywords are present below for column numbers COMMENT greater than 33. COMMENT WARNING WARNING WARNING COMMENT ------------------------- COMMENT This header has been developed for test purposes. It contains a mix COMMENT of WCS keywords whose presence within a single FITS header extends or COMMENT violates the FITS WCS standard. COMMENT COMMENT The main extension to the standard is the presence of image header COMMENT keywords in what is meant to be a binary table extension header. The COMMENT usage notes for wcsbth() in wcshdr.h explains how it interprets these COMMENT keywords. COMMENT COMMENT ----------------------------------------------------------------------- COMMENT ======================================================================= COMMENT COMMENT The primary image header keywords define a coordinate representation COMMENT using AIPS-convention WCS keywords. As it happens, no binary table COMMENT image array inherits these keywords and consequently they define an COMMENT "unattached" representation, one that is not associated with any COMMENT particular table column(s). Human intervention is required to form COMMENT such an association based on a priori knowledge. COMMENT COMMENT An old FITS WCS interpreter that only understood the AIPS convention COMMENT would most likely be confused by this header because NAXIS = 2 (above) COMMENT is fixed for a binary table. wcsbth() ignores NAXIS and deduces that COMMENT there are four coordinate axes by looking at the highest axis number COMMENT encoded in the WCS keywords themselves. COMMENT COMMENT An old FITS WCS interpreter also would not recognize the new WCSNAMEa COMMENT keyword, though its presence should not cause it any harm. It is set COMMENT here solely for identification purposes. COMMENT COMMENT This representation contains only standard image header keywords, but COMMENT their use in a binary table header is non-standard. COMMENT COMMENT ----------------------------------------------------------------------- COMMENT The following keyrecord is not part of the AIPS convention. WCSNAME = 'AIPS convention: TAN projection' / Name of this coordinate system CRPIX1 = 513.0 / Pixel coordinate of reference point CRPIX2 = 513.0 / Pixel coordinate of reference point CRPIX3 = 1025.0 / Pixel coordinate of reference point CRPIX4 = 1.0 / Pixel coordinate of reference point CDELT1 = -0.10 / x-scale CDELT2 = 0.10 / y-scale CROTA2 = 15.0 / Bulk image rotation CTYPE1 = 'RA---TAN' / Right ascension in a gnomonic projection CRVAL1 = 150.0 / Right ascension at the reference point CTYPE2 = 'DEC--TAN' / Declination in a gnomonic projection CRVAL2 = -30.0 / Declination at the reference point EPOCH = 2000.0 / Equinox of equatorial coordinates CDELT3 = 62.5e3 / Frequency scale CTYPE3 = 'FREQ ' / Frequency axis CRVAL3 = 1.3945e9 / Reference frequency VELREF = 258 / Barycentric radio velocity ALTRPIX = 0.0 / Alternate reference pixel (not handled) ALTRVAL = 0.0 / Alternate reference value (not handled) RESTFREQ= 1.42040575e9 / HI rest frequency CDELT4 = 1.0 / Stokes increment CTYPE4 = 'STOKES ' / Stokes convention axis (I, Q, U, V) CRVAL4 = 1.0 / Stokes I COMMENT ======================================================================= COMMENT COMMENT This coordinate representation utilizing a PCi_ja matrix expresses the COMMENT above AIPS convention header using standard WCS keywords. This set of COMMENT image header keywords with alternate representation 'I' is defined for COMMENT the purpose of inheritance (below) and so does not result in an COMMENT unattached representation as did the primary image header COMMENT representation above. COMMENT COMMENT This representation contains only standard image header keywords but COMMENT their use in a binary table header is non-standard. COMMENT COMMENT ----------------------------------------------------------------------- WCSAXESI= 4 / Number of coordinate axes CRPIX1I = 513 / Pixel coordinate of reference point CRPIX2I = 513 / Pixel coordinate of reference point CRPIX3I = 1025 / Pixel coordinate of reference point CRPIX4I = 1 / Pixel coordinate of reference point PC1_1I = 0.965925826289 / Coordinate transformation matrix element PC1_2I = 0.258819045103 / Coordinate transformation matrix element PC2_1I = -0.258819045103 / Coordinate transformation matrix element PC2_2I = 0.965925826289 / Coordinate transformation matrix element CDELT1I = -0.1 / [deg] Coordinate increment at reference point CDELT2I = 0.1 / [deg] Coordinate increment at reference point CDELT3I = 62500 / [Hz] Coordinate increment at reference point CDELT4I = 1 / Coordinate increment at reference point CUNIT1I = 'deg' / Units of coordinate increment and value CUNIT2I = 'deg' / Units of coordinate increment and value CUNIT3I = 'Hz' / Units of coordinate increment and value CTYPE1I = 'RA---TAN' / Right ascension, gnomonic projection CTYPE2I = 'DEC--TAN' / Declination, gnomonic projection CTYPE3I = 'FREQ' / Frequency (linear) CTYPE4I = 'STOKES' / Coordinate type code CRVAL1I = 150 / [deg] Coordinate value at reference point CRVAL2I = -30 / [deg] Coordinate value at reference point CRVAL3I = 1394500000 / [Hz] Coordinate value at reference point CRVAL4I = 1 / Coordinate value at reference point LONPOLEI= 180 / [deg] Native longitude of celestial pole LATPOLEI= -30 / [deg] Native latitude of celestial pole RESTFRQI= 1420405750 / [Hz] Line rest frequency RESTWAVI= 0 / [Hz] Line rest wavelength WCSNAMEI= 'AIPS convention: TAN projection' / Coordinate system title EQUINOXI= 2000 / [yr] Equinox of equatorial coordinates SPECSYSI= 'BARYCENT' / Reference frame of spectral coordinates COMMENT ======================================================================= COMMENT Binary table column 33 contains an image array, most of whose WCS COMMENT keywords would be inherited from the preceding image header keywords COMMENT with a = "I" provided that wcsbth() is invoked with an option that COMMENT allows it (i.e. by setting the WCSHDR_ALLIMG flag in its 'relax' COMMENT argument). COMMENT COMMENT Without full inheritance enabled, the presence of a single binary COMMENT table image array keyword, WCSN33I, would not be sufficient to cause COMMENT wcsbth() to create a wcsprm struct for this representation. However, COMMENT with inheritance enabled, WCSN33I is sufficient to trigger this COMMENT mechanism, in which case it overrides WCSNAMEI. COMMENT COMMENT Setting WCSHDR_AUXIMG alone only allows inheritance of the auxiliary COMMENT image header keywords. In this case it would not be sufficient to COMMENT cause wcsbth() to create a wcsprm struct for this representation COMMENT because there are no WCS keywords, either direct or inherited, that COMMENT allow the dimensionality of the coordinate system to be determined. COMMENT COMMENT The keyword is standard but such inheritance is non-standard. COMMENT ----------------------------------------------------------------------- WCSN33I = 'All WCS keywords inherited except for this one' / WCS title COMMENT ======================================================================= COMMENT Binary table column 44 is analogous to column 33 except with extra COMMENT binary table image array keywords that may override the image-header COMMENT equivalent if inheritance is enabled. COMMENT COMMENT wcsbth() would always create at least a 2D coordinate representation COMMENT for column 44, regardless of what other keywords were inherited. If COMMENT WCSHDR_ALLIMG was set, then a 4D representation would be constructed COMMENT from inherited keywords. WCSHDR_AUXIMG would not be sufficient for COMMENT this; however it would cause LONPOLEI and LATPOLEI to be inherited COMMENT (and four others) and these would affect the interpretation of the COMMENT coordinate system. COMMENT COMMENT The keywords are standard but such inheritance is non-standard. COMMENT ----------------------------------------------------------------------- WCSN44I = 'Most WCS keywords inherited' / WCS title 1CTY44I = 'RA---SIN' / Right ascension, orthographic projection 2CTY44I = 'DEC--SIN' / Declination, orthographic projection COMMENT ======================================================================= COMMENT Binary table keywords for the image array in column 77 with alternate COMMENT representation 'B'. COMMENT COMMENT This coordinate representation utilizing a PC (ijPCna) matrix COMMENT expresses the above gnomonic (TAN) projection as a slant zenithal COMMENT perspective projection (SZP) in order to test the reading of a number COMMENT of PVi_ma keywords. It also includes a linear time axis. COMMENT COMMENT This representation contains only standard keywords and usage. In COMMENT particular, it is is self-contained, i.e. no inheritance. COMMENT ----------------------------------------------------------------------- WCAX77B = 4 / Number of coordinate axes 1CRP77B = 513 / Pixel coordinate of reference point 2CRP77B = 513 / Pixel coordinate of reference point 3CRP77B = 1025 / Pixel coordinate of reference point 4CRP77B = 1 / Pixel coordinate of reference point 11PC77B = 0.866025404 / Coordinate transformation matrix element 12PC77B = 0.5 / Coordinate transformation matrix element 21PC77B = -0.5 / Coordinate transformation matrix element 22PC77B = 0.866025404 / Coordinate transformation matrix element 1CDE77B = -0.1 / [deg] Coordinate increment at reference point 2CDE77B = 0.1 / [deg] Coordinate increment at reference point 3CDE77B = -9.635265432e-06 / [m] Coordinate increment at reference point 4CDE77B = 1 / [s] Coordinate increment at reference point 1CUN77B = 'deg' / Units of coordinate increment and value 2CUN77B = 'deg' / Units of coordinate increment and value 3CUN77B = 'm' / Units of coordinate increment and value 4CUN77B = 's' / Units of coordinate increment and value 1CTY77B = 'RA---SZP' / Right ascension, slant zenithal perspective pro 2CTY77B = 'DEC--SZP' / Declination, slant zenithal perspective project 3CTY77B = 'WAVE-F2W' / Vacuum wavelength (linear in frequency) 4CTY77B = 'TIME' / Coordinate type code 1CRV77B = 150 / [deg] Coordinate value at reference point 2CRV77B = -30 / [deg] Coordinate value at reference point 3CRV77B = 0.214982042 / [m] Coordinate value at reference point 4CRV77B = -2000 / [s] Coordinate value at reference point 1V77_1B = 0 / [deg] Native longitude of the reference point 1V77_2B = 90 / [deg] Native latitude of the reference point 1V77_3B = 195 / [deg] alias for LONP77A (has precedence) 1V77_4B = -30 / [deg] alias for LATP77A (has precedence) 2V77_1B = 0 / SZP projection parameter 2V77_2B = 180 / SZP projection parameter 2V77_3B = 45 / SZP projection parameter 4S77_0B = 'UTC' / Coordinate transformation parameter LONP77B = 195 / [deg] Native longitude of celestial pole LATP77B = -30 / [deg] Native latitude of celestial pole RFRQ77B = 1420405750 / [Hz] Line rest frequency RWAV77B = 0.211061141 / [Hz] Line rest wavelength WCSN77B = 'St''d representation: SZP projection' / Coordinate system title 1CNA77B = 'Right ascension (J2000)' / Axis name for labelling purposes 2CNA77B = 'Declination (J2000)' / Axis name for labelling purposes 3CNA77B = 'Wavelength' / Axis name for labelling purposes 4CNA77B = 'Time offset' / Axis name for labelling purposes 3CRD77B = 1e-11 / [m] Random error in coordinate 3CSY77B = 1e-12 / [m] Systematic error in coordinate RADE77B = 'FK5' / Equatorial coordinate system EQUI77B = 2000 / [yr] Equinox of equatorial coordinates SPEC77B = 'BARYCENT' / Reference frame of spectral coordinates SOBS77B = 'TOPOCENT' / Reference frame of spectral observation VSYS77B = 1500 / [m/s] Velocity towards source SSRC77B = 'LSRK' / Reference frame of source redshift ZSOU77B = 0.0025 / Redshift of the source OBSGX77 = -4554231.9 / [m] ITRF observatory X-coordinate COMMENT OBSGEO-Y (below) should be inherited for OBSGY77. OBSGZ77 = -3454035.9 / [m] ITRF observatory Z-coordinate MJDOB77 = 35883.625 / [d] MJD of observation matching DOBS77 MJDA77 = 35883.7 / [d] MJD mid-observation matching DAVG77 DOBS77 = '1957-02-14T15:00:00' / ISO-8601 observation date matching MJDOB77 DAVG77 = '1957-02-14T16:48:00' / ISO-8601 mid-observation date matching MJDA77 COMMENT ======================================================================= COMMENT Pixel list keywords with axes in columns 8, 9 and 10 and alternate COMMENT representation 'P'. COMMENT COMMENT In the IRAF representation, if one CDi_ja (TCDn_ka) keyword is given COMMENT then the default is zero for any that are omitted. CDELTia (TCDLTna) COMMENT and CROTAn (TCROTna) keywords are included for informational purposes COMMENT only and otherwise are to be ignored. COMMENT COMMENT This representation uses the non-standard long form for some pixel COMMENT list keywords with non-blank alternate version specifier (these forms COMMENT are standard for a = ' ' only): COMMENT TCRPXna instead of TCRPna COMMENT TCDn_ka TCn_ka COMMENT TCDLTna TCDEna COMMENT TCUNIna TCUNna COMMENT TCTYPna TCTYna COMMENT TCRVLna TCRVna COMMENT TPVn_ma TVn_ma COMMENT TCNAMna TCNAna COMMENT TCRDEna TCRDna COMMENT TCSYEna TCSYna COMMENT Also, strictly speaking, alternate version codes are not defined for COMMENT TCROTn (e.g. TCROT9P below), and WCSNna should be TWCSna. However, COMMENT these are considered to be natural extensions that all FITS WCS COMMENT interpreters should support. Apart from that, this representation COMMENT contains standard keywords and usage. In particular, it is self- COMMENT contained, i.e. no inheritance. COMMENT ----------------------------------------------------------------------- TCRPX8P = 513 / Pixel coordinate of reference point TCRPX9P = 513 / Pixel coordinate of reference point TCRPX10P= 1025 / Pixel coordinate of reference point TCD8_8P = -0.08660254 / Coordinate transformation matrix element TCD8_9P = -0.05 / Coordinate transformation matrix element TCD9_8P = -0.05 / Coordinate transformation matrix element TCD9_9P = 0.08660254 / Coordinate transformation matrix element TC10_10P= -4.565153674e-5 / Coordinate transformation matrix element TCDLT8P = -0.10 / [deg] Coordinate increment at reference point TCDLT9P = 0.10 / [deg] Coordinate increment at reference point TCDLT10P= -4.565153674e-5 / Coordinate increment at reference point TCROT9P = 30.0 / [deg] Bulk image rotation TCUNI8P = 'deg' / Units of coordinate increment and value TCUNI9P = 'deg' / Units of coordinate increment and value TCTYP8P = 'RA---ZPN' / Right ascension, zenithal/azimuthal polynomial TCTYP9P = 'DEC--ZPN' / Declination, zenithal/azimuthal polynomial proj TCTYP10P= 'ZOPT-F2W' / Redshift (linear in frequency) TCRVL8P = 150 / [deg] Coordinate value at reference point TCRVL9P = -30 / [deg] Coordinate value at reference point TCRVL10P= 0.018577089 / Coordinate value at reference point TPV9_1P = 1 / ZPN projection parameter TPV9_3P = 0.333333333 / ZPN projection parameter TPV9_5P = 0.133333333 / ZPN projection parameter TPV9_7P = 0.053968254 / ZPN projection parameter TPV9_9P = 0.021869489 / ZPN projection parameter TPV9_11P= 0.008863236 / ZPN projection parameter TPV9_13P= 0.003592128 / ZPN projection parameter TPV9_15P= 0.001455834 / ZPN projection parameter TPV9_17P= 0.000590027 / ZPN projection parameter TPV9_19P= 0.000239129 / ZPN projection parameter LONP8P = 195 / [deg] Native longitude of celestial pole LATP8P = -30 / [deg] Native latitude of celestial pole RFRQ8P = 1420405750 / [Hz] Line rest frequency RWAV8P = 0.211061141 / [Hz] Line rest wavelength WCSN8P = 'IRAF representation: ZPN projection' / Coordinate system title TCNAM8P = 'Right ascension (J2000)' / Axis name for labelling purposes TCNAM9P = 'Declination (J2000)' / Axis name for labelling purposes TCNAM10P= 'Redshift' / Axis name for labelling purposes TCRDE10P= 5e-11 / Random error in coordinate TCSYE10P= 5e-12 / Systematic error in coordinate RADE8P = 'FK5' / Equatorial coordinate system EQUI8P = 2000 / [yr] Equinox of equatorial coordinates SPEC8P = 'BARYCENT' / Reference frame of spectral coordinates SOBS8P = 'TOPOCENT' / Reference frame of spectral observation VSYS8P = 1500 / [m/s] Velocity towards source SSRC8P = 'LSRK' / Reference frame of source redshift ZSOU8P = 0.00250000001174 / Redshift of the source COMMENT OBSGEO-X (below) should be inherited for OBSGX8. OBSGY8 = 2816758.3 / [m] ITRF observatory Y-coordinate OBSGZ8 = -3454035.9 / [m] ITRF observatory Z-coordinate MJDOB8 = 35883.625 / [d] MJD of observation matching DOBS8 MJDA8 = 35883.7 / [d] MJD mid-observation matching DAVG8 DOBS8 = '1957-02-14T15:00:00' / ISO-8601 observation date matching MJDOB8 DAVG8 = '1957-02-14T16:48:00' / ISO-8601 mid-observation date matching MJDA8 COMMENT ======================================================================= COMMENT COMMENT The following keywords have no alternates; they apply to each COMMENT coordinate representation, even that of the AIPS convention for COMMENT which, strictly, only the DATE-OBS keyword should be recognized. COMMENT COMMENT The keycomments for OBSGEO-Y and OBSGEO-Z have been omitted COMMENT deliberately for test purposes. COMMENT COMMENT ----------------------------------------------------------------------- OBSGEO-X= -4554231.9 / [m] ITRF observatory coordinates OBSGEO-Y= 2816758.3 / OBSGEO-Z= -3454035.9 MJD-OBS = 35883.625 / [d] MJD at start of observation (UTC) MJD-AVG = 35883.700 / [d] MJD mid-observation time (UTC) DATE-OBS= '1957-02-14T15:00:00'/ UTC date corresponding to MJD-OBS DATE-AVG= '1957-02-14T16:48:00'/ UTC date corresponding to MJD-AVG OBSGX99 = -4000000.0 / [m] ITRF observatory X-coordinate END pywcs-1.12/wcslib/C/test/pih.keyrec0000644001153600020070000005156712310355626021274 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # WCSLIB 4.10 - an implementation of the FITS WCS standard. # Copyright (C) 1995-2012, Mark Calabretta # # This file is part of WCSLIB. # # WCSLIB is free software: you can redistribute it and/or modify it under the # terms of the GNU Lesser General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY # WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS # FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for # more details. # # You should have received a copy of the GNU Lesser General Public License # along with WCSLIB. If not, see . # # Correspondence concerning WCSLIB may be directed to: # Internet email: mcalabre@atnf.csiro.au # Postal address: Dr. Mark Calabretta # Australia Telescope National Facility, CSIRO # PO Box 76 # Epping NSW 1710 # AUSTRALIA # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: pih.keyrec,v 4.10 2012/02/05 23:41:44 cal103 Exp $ #----------------------------------------------------------------------------- # FITS header keyrecords used for testing by tpih1, tpih2 and tfitshdr. # # Use 'tofits' (supplied) to convert this file to proper FITS format via # # tofits < bth.keyrec > bth.fits # # Lines in this file beginning with '#' are ignored by tofits. #----------------------------------------------------------------------------- SIMPLE = F / Standards-conformant FITS format? NO! BITPIX = -32 / IEEE single precision floating point NAXIS = 0 / No image data COMMENT WARNING WARNING WARNING COMMENT ------------------------- COMMENT This header has been developed for test purposes and as such contains COMMENT all standard WCS keywords. Combining certain of them (e.g. PCi_ja, COMMENT CDi_ja, and CROTAn) within a single FITS header violates certain WCS COMMENT standards. However, taken individually, each representation is legal, COMMENT except as indicated. COMMENT COMMENT The three alternate representations define essentially the same COMMENT coordinate system in three different ways. The older AIPS convention COMMENT is necessarily used for the primary representation because the COMMENT alternate version code (e.g. the "a" in CTYPEia) is not applicable in COMMENT that convention. COMMENT COMMENT For compatibility testing, the header also contains a number of non- COMMENT standard keywords and constructs: the AIPS keywords CROTAn, EPOCH, and COMMENT VELREF retrofitted with alternate version codes, and PROJPn, a COMMENT forerunner of PVi_ma. However, non-standard CD00i00j and PC00i00j COMMENT keywords, while recognized, are not included since they can only apply COMMENT to the primary representation which is used here to test the AIPS COMMENT convention. COMMENT COMMENT A simple TAN projection used in the primary representation is COMMENT expressed as an equivalent SZP projection in the "A" representation, COMMENT and approximated by a ZPN in the "I" representation. A bulk image COMMENT rotation of 15 deg applied by the defunct CROTAn keyword in the AIPS COMMENT convention is replaced in the alternates by an equivalent bulk image COMMENT rotation of 30 deg applied by the linear transformation matrix, COMMENT together with an effective bulk rotation of -15 deg applied by COMMENT LONPOLE (this is only possible for zenithal projections). COMMENT COMMENT Similarly, the spectral axis in the primary representation, a simple COMMENT linear frequency axis, is recast as non-linear wavelength and redshift COMMENT axes in the alternates. COMMENT COMMENT Although the parser handles free-format character string, integer, and COMMENT floating-point keyvalues (NOST 100-2.0, Sect. 5.2) most numeric values COMMENT in this header are given in the conventional fixed-format, with only COMMENT CROTA2I, EPOCHI, and VELREFI as exceptions for testing. Most string COMMENT values are free-format, only those in the "A" representation are fixed. COMMENT COMMENT ----------------------------------------------------------------------- COMMENT ----------------------------------------------------------------------- COMMENT Primary representation COMMENT ---------------------- COMMENT COMMENT In the AIPS convention CROTAn associated with the latitude axis COMMENT defines a bulk image rotation. Strictly speaking, the representation COMMENT here is illegal since it mixes new WCS keywords (WCSAXESa and COMMENT WCSNAMEa) with CROTAn, an older AIPS convention keyword. WCSAXES is COMMENT used here because setting NAXIS non-zero would require that this FITS COMMENT file contain a data section. COMMENT COMMENT Several PROJPn keyrecords (non-standard) are also included here for COMMENT test purposes; they were never part of the AIPS convention and only COMMENT appeared in early drafts of the WCS papers. Their values are not COMMENT actually used in the TAN projection. COMMENT COMMENT ----------------------------------------------------------------------- COMMENT The following two keyrecords are not part of the AIPS convention. WCSAXES = 4 / Four coordinate axes WCSNAME = 'AIPS convention: TAN projection' / Name of this coordinate system CRPIX1 = 513.0 / Pixel coordinate of reference point CRPIX2 = 513.0 / Pixel coordinate of reference point CRPIX3 = 1025.0 / Pixel coordinate of reference point CRPIX4 = 1.0 / Pixel coordinate of reference point CDELT1 = -0.10 / x-scale CDELT2 = 0.10 / y-scale CROTA2 = 15.0 / Bulk image rotation CTYPE1 = 'RA---TAN' / Right ascension in a gnomonic projection CRVAL1 = 150.0 / Right ascension at the reference point CTYPE2 = 'DEC--TAN' / Declination in a gnomonic projection CRVAL2 = -30.0 / Declination at the reference point EPOCH = 2000.0 / Equinox of equatorial coordinates CDELT3 = 62.5e3 / Frequency scale CTYPE3 = 'FREQ ' / Frequency axis CRVAL3 = 1.3945e9 / Reference frequency VELREF = 258 / Barycentric radio velocity ALTRPIX = 0.0 / Alternate reference pixel (not handled) ALTRVAL = 0.0 / Alternate reference value (not handled) RESTFREQ= 1.42040575e9 / HI rest frequency CDELT4 = 1.0 / Stokes increment CTYPE4 = 'STOKES ' / Stokes convention axis (I, Q, U, V) CRVAL4 = 1.0 / Stokes I COMMENT As explained above, the following keyrecords are non-standard. PROJP0 = 0.0 / Projection parameter (not used) PROJP1 = 0.0 / Projection parameter (not used) PROJP2 = 0.0 / Projection parameter (not used) COMMENT ----------------------------------------------------------------------- COMMENT Alternate representation 'A' COMMENT ---------------------------- COMMENT COMMENT This coordinate representation utilizing a PCi_ja matrix expresses the COMMENT above gnomonic (TAN) projection as a slant zenithal perspective COMMENT projection (SZP) in order to test the reading of a number of PVi_ma COMMENT keywords. It also includes a linear time axis. COMMENT COMMENT This representation contains only standard keywords and usage. COMMENT COMMENT ----------------------------------------------------------------------- WCSAXESA= 4 / Four coordinate axes WCSNAMEA= 'Standard representation: SZP projection' / Name of this system CRPIX1A = 513.0 / Pixel coordinate of reference point CRPIX2A = 513.0 / Pixel coordinate of reference point CRPIX3A = 1025.0 / Pixel coordinate of reference point CRPIX4A = 1.0 / Pixel coordinate of reference point PC1_1A = 0.866025404 / Linear transformation matrix element PC1_2A = 0.500000000 / Linear transformation matrix element PC2_1A = -0.500000000 / Linear transformation matrix element PC2_2A = 0.866025404 / Linear transformation matrix element CDELT1A = -0.10 / [deg] x-scale CUNIT1A = 'deg' / Degree units are required CTYPE1A = 'RA---SZP' / Right ascension in slant zenithal projection CRVAL1A = 150.0 / [deg] Right ascension at the reference point CNAME1A = 'Right ascension (J2000)' / Axis name for labelling purposes CDELT2A = 0.10 / [deg] y-scale CUNIT2A = 'deg' / Degree units are required CTYPE2A = 'DEC--SZP' / Declination in a slant zenithal projection CRVAL2A = -30.0 / [deg] Declination at the reference point CNAME2A = 'Declination (J2000)' / Axis name for labelling purposes PV1_1A = 0.0 / [deg] Native longitude of the reference point PV1_2A = 90.0 / [deg] Native latitude of the reference point PV1_3A = 195.0 / [deg] LONPOLEa by another name (precedence) PV1_4A = 999.0 / [deg] LATPOLEa by another name (precedence) PV2_1A = 0.0 / SZP distance, in spherical radii PV2_2A = 180.0 / [deg] SZP P-longitude PV2_3A = 45.0 / [deg] SZP P-latitude LONPOLEA= 195.0 / [deg] Native longitude of the NCP LATPOLEA= 999.0 / [deg] Native latitude of the NCP RADESYSA= 'FK5' / Mean equatorial coordinates, IAU 1984 system EQUINOXA= 2000.0 / [yr] Equinox of equatorial coordinates CDELT3A = -9.635265432e-6 / [m] Wavelength scale CUNIT3A = 'm' / Wavelength units CTYPE3A = 'WAVE-F2W' / Frequency axis expressed as wavelength CRVAL3A = 0.214982042 / [m] Reference wavelength CNAME3A = 'Wavelength' / Axis name for labelling purposes CRDER3A = 1.0e-11 / [m] Wavelength calibration, random error CSYER3A = 1.0e-12 / [m] Wavelength calibration, systematic error RESTFRQA= 1.42040575e9 / [Hz] HI rest frequency RESTWAVA= 0.211061141 / [m] HI rest wavelength SPECSYSA= 'BARYCENT' / Reference frame of spectral coordinates SSYSOBSA= 'TOPOCENT' / Reference frame of observation VELOSYSA= 1500.0 / [m/s] Bary-topo velocity towards the source SSYSSRCA= 'LSRK' / Reference frame of source redshift ZSOURCEA= 0.0025 / Redshift of the source CDELT4A = 1.0 / [s] Time scale CUNIT4A = 's' / Time units CTYPE4A = 'TIME''x''' / String value and comment containing quotes (') CRVAL4A = -2e3 / [s] Time at the reference point CNAME4A = 'Time offset' / Axis name for labelling purposes PS4_0A = 'UTC' / Time measurement system COMMENT ----------------------------------------------------------------------- COMMENT Alternate representation 'I' COMMENT ---------------------------- COMMENT COMMENT In the IRAF representation, if one CDi_ja keyword is given then the COMMENT default is zero for any that are omitted. CDELTia and CROTAn COMMENT keywords are included for informational purposes only and otherwise COMMENT are to be ignored. COMMENT COMMENT Strictly speaking, alternate version codes are not defined for CROTAn COMMENT (e.g. CROTA2I below), EPOCHa or VELREFa. The latter two should be COMMENT overridden by EQUINOXa and SPECSYSa even though they occur later in COMMENT the header. COMMENT COMMENT While encoding a TAN projection as SZP may be good for testing COMMENT purposes, approximating it by a zenithal polynomial projection (ZPN) COMMENT is even better! The polynomial coefficients are accurate to the COMMENT number of decimal places given (but don't ever do this in a real COMMENT header). COMMENT COMMENT ----------------------------------------------------------------------- WCSAXESI= 3 / Three coordinate axes WCSNAMEI= 'IRAF representation: ZPN projection' / Name of this coordinate system CRPIX1I = 513.0 / Pixel coordinate of reference point CRPIX2I = 513.0 / Pixel coordinate of reference point CRPIX3I = 1025.0 / Pixel coordinate of reference point CD1_1I = -0.086602540 / Linear transformation matrix element CD1_2I = -0.050000000 / Linear transformation matrix element CD2_1I = -0.050000000 / Linear transformation matrix element CD2_2I = 0.086602540 / Linear transformation matrix element CD3_3I = -4.565153674e-5 / Redshift scale CDELT1I = -0.10 / [deg] x-scale (informational) CUNIT1I = 'deg' / Degree units are required CTYPE1I = 'RA---ZPN' / Right ascension in slant zenithal projection CRVAL1I = 150.0 / [deg] Right ascension at the reference point CNAME1I = 'Right ascension (J2000)' / Axis name for labelling purposes CDELT2I = 0.10 / [deg] y-scale (informational) CUNIT2I = 'deg' / Degree units are required CTYPE2I = 'DEC--ZPN' / Declination in a slant zenithal projection CRVAL2I = -30.0 / [deg] Declination at the reference point CNAME2I = 'Declination (J2000)' / Axis name for labelling purposes PV2_1I = 1.000000000 / ZPN P1 coefficient for approximating TAN PV2_3I = 0.333333333 / ZPN P3 coefficient for approximating TAN PV2_5I = 0.133333333 / ZPN P5 coefficient for approximating TAN PV2_7I = 0.053968254 / ZPN P7 coefficient for approximating TAN PV2_9I = 0.021869489 / ZPN P9 coefficient for approximating TAN PV2_11I = 0.008863236 / ZPN P11 coefficient for approximating TAN PV2_13I = 0.003592128 / ZPN P13 coefficient for approximating TAN PV2_15I = 0.001455834 / ZPN P15 coefficient for approximating TAN PV2_17I = 0.000590027 / ZPN P17 coefficient for approximating TAN PV2_19I = 0.000239129 / ZPN P19 coefficient for approximating TAN LONPOLEI= 195.0 / [deg] Native longitude of the NCP LATPOLEI= 999.0 / [deg] Native latitude of the NCP RADESYSI= 'FK5' / Mean equatorial coordinates, IAU 1984 system EQUINOXI= 2000.0 / [yr] Equinox of equatorial coordinates CDELT3I = -4.565153674e-5 / Redshift scale (informational) CTYPE3I = 'ZOPT-F2W' / Frequency axis expressed as redshift CRVAL3I = 0.018577089 / Reference redshift CNAME3I = 'Redshift' / Axis name for labelling purposes CRDER3I = 5.0e-11 / Redshift calibration, random error CSYER3I = 5.0e-12 / Redshift calibration, systematic error RESTFRQI= 1.42040575e9 / [Hz] HI rest frequency RESTWAVI= 0.211061141 / [m] HI rest wavelength SSYSOBSI= 'TOPOCENT' / Reference frame of observation VELOSYSI= 1500.0 / [m/s] Bary-topo velocity towards the source SSYSSRCI= 'LSRK' / Reference frame of source redshift VSOURCEI= 748544.3 / [m/s] Apparent radial velocity of the source COMMENT As explained above, the following keyrecords are non-standard. CROTA2I = 30.0 / [deg] Bulk image rotation EPOCHI = 2000 / [yr] Equinox of equatorial coordinates VELREFI = 258 / Barycentric radio velocity COMMENT ----------------------------------------------------------------------- COMMENT COMMENT The following keywords have no alternates; they apply to each COMMENT coordinate representation, even that of the AIPS convention for COMMENT which, strictly, only the DATE-OBS keyword should be recognized. COMMENT COMMENT The keycomments for OBSGEO-Y and OBSGEO-Z have been omitted COMMENT deliberately for test purposes. COMMENT COMMENT ----------------------------------------------------------------------- OBSGEO-X= -4554231.9 / [m] ITRF observatory coordinates OBSGEO-Y= 2816758.3 / OBSGEO-Z= -3454035.9 MJD-OBS = 35883.625 / [d] MJD at start of observation (UTC) MJD-AVG = 35883.700 / [d] MJD mid-observation time (UTC) DATE-OBS= '1957-02-14T15:00:00'/ UTC date corresponding to MJD-OBS DATE-AVG= '1957-02-14T16:48:00'/ UTC date corresponding to MJD-AVG COMMENT ----------------------------------------------------------------------- COMMENT COMMENT The following look a little like WCS keywords but should be discarded: COMMENT COMMENT ----------------------------------------------------------------------- COMMENT CRPIXELS= 0.0 / Furphy, not CRPIXja PCATALOG= 0.0 / Furphy, not PCi_ja CDELTA = 0.0 / Furphy, not CDELTia CDI_JA = 0.0 / Furphy, not CDi_ja CUNITARY= 0.0 / Furphy, not CUNITia CTYPEXY = 0.0 / Furphy, not CTYPEia CRVALUE = 0.0 / Furphy, not CRVALia CNAME = 0.0 / Furphy, not CNAMEia PV1_1AL = 0.0 / Furphy, not PVi_ma PV02_1 = 0.0 / Furphy, not PVi_ma (leading zero on i) PV2_01 = 0.0 / Furphy, not PVi_ma (leading zero on m) PSEUDO = 0.0 / Furphy, not PSi_ma EPOCHAL = 0.0 / Furphy, not EPOCH VELREF1 = 0.0 / Furphy, not VELREF COMMENT ----------------------------------------------------------------------- COMMENT COMMENT The following illegal WCS keyrecords should be rejected by wcspih(): COMMENT COMMENT ----------------------------------------------------------------------- COMMENT CTYPE1 = 0.0 / Illegal, CTYPEia must be string type PV2_1 = '0.0' / Illegal, PVi_ma must be numeric PV2_1 = 0.0 / Illegal, "= " not in columns 9-10 EPOCH = '2000.0' / Illegal, EPOCH must be numeric COMMENT ----------------------------------------------------------------------- COMMENT COMMENT The following keyrecords are for testing fitshdr(): COMMENT COMMENT ----------------------------------------------------------------------- COMMENT NOVLSPEC=1 / Not a valid value specifier (no " " in col. 10) INT32 = 00000012345 / Not a 64-bit integer INT32 = -000000123456789 / Not a 64-bit integer INT32 = -2147483648 / Not a 64-bit integer (INT_MIN) INT32 = 2147483647 / Not a 64-bit integer (INT_MAX) INT32 = 0000000000000000000000000000000000012345 / Not a very long integer INT32 = -000000000000000000000000000123456789 / Not a very long integer INT64 = -2147483649 / 64-bit integer (INT_MIN - 1) INT64 = +2147483648 / 64-bit integer (INT_MAX + 1) INT64 = +100000000000000000 / 64-bit integer INT64 = -876543210987654321 / 64-bit integer INT64 = -9223372036854775808 / Not a very long integer (LONG_MIN) INT64 = +9223372036854775807 / Not a very long integer (LONG_MAX) INT64 = -000000000000000000000000000000876543210987654321 / 64-bit integer INTVL = -9223372036854775809 / Very long integer (LONG_MIN - 1) INTVL = +9223372036854775808 / Very long integer (LONG_MAX + 1) INTVL = -100000000000000000000000000000876543210987654321 / Very-long integer INTVL = +123456789012345678901234567890123456789012345678901234567890123456789 INTVL = 1234567890123456789012345678901234567890123456789012345678901234567890 COMPLEX = (137, -1) / An integer complex keyvalue COMPLEX = (10e5, -0.1) / A floating point complex keyvalue GOODSTR = '"G''DAY" ' / A valid string keyvalue BLANKS = ' ' / An all-blank string equals a single blank LONGSTR = 'The loooooongest possible non-continued string value, 68 characters.' CONTSTR = 'The quick brown & ' / Continued string, with & (will be stripped off) CONTINUE 'fox jumps over the' Relaxed handling of invalid keycomment CONTINUE ' lazy dog' PI = 3.14159265358929323 / [!?] is not a valid units specification CONTINUE 'Not a valid string continuation' COMMENT The following are all deliberate syntax errors: BadKey = 111 / Example of a syntax error, invalid keyword BADKEY! = 222 / Example of a syntax error, invalid keyword BAD KEY = 333 / Example of a syntax error, invalid keyword BADSTR = BAD / Example of a syntax error, invalid keyvalue BADSTR = "BAD" / Example of a syntax error, invalid keyvalue BADSTR = 'BAD' 'STR' / Example syntax error, invalid string keyvalue BADFLT = 49 + 94 / Example of a syntax error, invalid keyvalue BADFLT = 1D99 / Example of a syntax error, invalid keyvalue BADCOMM = 999 Example of a syntax error, invalid keycomment END = 'ILLEGAL' / Illegal END keyrecord END DANGLE1 Keyrecords following the END keyrecord should be ignored. DANGLE2 DANGLE3 pywcs-1.12/wcslib/C/test/tbth1.c0000644001153600020070000002024412310355626020462 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tbth1.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tbth1 tests wcsbth(), the WCS FITS parser for binary table headers, and * wcsfix(), which translates non-standard constructs. It reads a test header * and uses wcsprt() to print the resulting wcsprm structs. * * Input comes from file "bth.fits" using either fits_hdr2str() from CFITSIO * if the DO_CFITSIO preprocessor is defined, or read directly using fgets() * otherwise. * *---------------------------------------------------------------------------*/ #include #include #include #if defined HAVE_CFITSIO && defined DO_CFITSIO #include #endif #include #include #include int main() { char infile[] = "bth.fits"; char a, *hptr; short alts[1000][28]; int colsel[8], ctrl, ialt, iblock, icol, ifix, ikeyrec, iwcs, keysel, nkeyrec, nreject, nwcs, relax, stat[NWCSFIX], status; struct wcsprm *wcs; #if defined HAVE_CFITSIO && defined DO_CFITSIO char *header; fitsfile *fptr; #else char keyrec[81], header[288001]; int gotend, k; FILE *fptr; #endif /* Set line buffering in case stdout is redirected to a file, otherwise * stdout and stderr messages will be jumbled (stderr is unbuffered). */ setvbuf(stdout, NULL, _IOLBF, 0); printf("Testing WCSLIB parser for FITS binary table headers (tbth1.c)\n" "-------------------------------------------------------------\n\n"); /* Read in the FITS header, excluding COMMENT and HISTORY keyrecords. */ #if defined HAVE_CFITSIO && defined DO_CFITSIO status = 0; if (fits_open_file(&fptr, infile, READONLY, &status)) { fits_report_error(stderr, status); return 1; } if (fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status)) { fits_report_error(stderr, status); return 1; } fits_close_file(fptr, &status); #else if ((fptr = fopen(infile, "r")) == 0) { fprintf(stderr, "ERROR opening %s\n", infile); return 1; } k = 0; nkeyrec = 0; gotend = 0; for (iblock = 0; iblock < 100; iblock++) { for (ikeyrec = 0; ikeyrec < 36; ikeyrec++) { if (fgets(keyrec, 81, fptr) == 0) { break; } if (strncmp(keyrec, " ", 8) == 0) continue; if (strncmp(keyrec, "COMMENT ", 8) == 0) continue; if (strncmp(keyrec, "HISTORY ", 8) == 0) continue; strncpy(header+k, keyrec, 80); k += 80; nkeyrec++; if (strncmp(keyrec, "END ", 8) == 0) { /* An END keyrecord was read, but read the rest of the block. */ gotend = 1; } } if (gotend) break; } fclose(fptr); #endif fprintf(stderr, "Found %d non-comment header keyrecords.\n\n", nkeyrec); /* Parse the header, allowing all recognized non-standard WCS keywords and * usage. WCS keyrecords that are used are culled from the header, illegal * ones are reported. */ relax = WCSHDR_all; ctrl = -2; keysel = 0; colsel[0] = 0; fprintf(stderr, "\nIllegal-WCS header keyrecords rejected by wcsbth():\n"); if ((status = wcsbth(header, nkeyrec, relax, ctrl, keysel, colsel, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcsbth ERROR %d: %s.\n", status, wcs_errmsg[status]); } if (!nreject) fprintf(stderr, "(none)\n"); /* List the remaining keyrecords. */ printf("\n\nHeader keyrecords ignored by wcsbth():\n"); hptr = header; while (*hptr) { printf("%.80s\n", hptr); hptr += 80; } #if defined HAVE_CFITSIO && defined DO_CFITSIO free(header); #endif /* Summarize what was found. */ printf("\n\nExtracted %d coordinate description%s:\n", nwcs, (nwcs == 1) ? "" : "s"); printf("\n Unattached image header(s)"); status = wcsbdx(nwcs, &wcs, 0, alts); if (alts[0][27]) { printf(" with indices:\n -"); for (a = 'A'; a <= 'Z'; a++) { printf("%2c", a); } printf("\n "); for (ialt = 0; ialt < 27; ialt++) { if (alts[0][ialt] < 0) { printf(" -"); } else { printf("%2d", alts[0][ialt]); } } printf("\n"); } else { printf(": (none)\n"); } printf("\n Binary table image array(s)"); for (icol = 1; icol <= 999; icol++) { if (alts[icol][27]) { printf(" with indices:\n Col. -"); for (a = 'A'; a <= 'Z'; a++) { printf("%2c", a); } printf("\n"); for (icol = 1; icol <= 999; icol++) { for (ialt = 0; ialt < 27; ialt++) { if (alts[icol][ialt] >= 0) { printf("%5d: ", icol); for (ialt = 0; ialt < 27; ialt++) { if (alts[icol][ialt] < 0) { printf(" -"); } else { printf("%2d", alts[icol][ialt]); } } printf("\n"); break; } } } icol = 9999; } } if (icol < 9999) { printf(": (none)\n"); } printf("\n Pixel list(s)"); status = wcsbdx(nwcs, &wcs, 1, alts); for (icol = 1; icol <= 999; icol++) { if (alts[icol][27]) { printf(" with indices:\n Col. -"); for (a = 'A'; a <= 'Z'; a++) { printf("%2c", a); } printf("\n"); for (icol = 1; icol <= 999; icol++) { for (ialt = 0; ialt < 27; ialt++) { if (alts[icol][ialt] >= 0) { printf("%5d: ", icol); for (ialt = 0; ialt < 27; ialt++) { if (alts[icol][ialt] < 0) { printf(" -"); } else { printf("%2d", alts[icol][ialt]); } } printf("\n"); break; } } } icol = 9999; } } if (icol < 9999) { printf(": (none)\n"); } /* Fix non-standard usage and print each of the wcsprm structs. */ for (iwcs = 0; iwcs < nwcs; iwcs++) { printf("\n------------------------------------" "------------------------------------\n"); /* Fix non-standard WCS keyvalues. */ if ((status = wcsfix(7, 0, wcs+iwcs, stat))) { printf("wcsfix ERROR, status returns: ("); for (ifix = 0; ifix < NWCSFIX; ifix++) { printf(ifix ? ", %d" : "%d", stat[ifix]); } printf(")\n\n"); } if ((status = wcsset(wcs+iwcs))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); continue; } if ((status = wcsprt(wcs+iwcs))) { fprintf(stderr, "wcsprt ERROR %d: %s.\n", status, wcs_errmsg[status]); } } status = wcsvfree(&nwcs, &wcs); /* Do it again to check that wcsbth() can handle multiple invokations. */ printf("\nInvoking wcsbth() a second time on the same header...\n"); ctrl = 0; if ((status = wcsbth(header, nkeyrec, relax, 0, keysel, colsel, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcsbth ERROR %d: %s.\n", status, wcs_errmsg[status]); } else { printf("OK, extracted %d coordinate description%s.\n", nwcs, (nwcs == 1) ? "" : "s"); } return 0; } pywcs-1.12/wcslib/C/test/tcel1.c0000644001153600020070000002254212310355625020452 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tcel1.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tcel1 tests the spherical projection driver routines supplied with WCSLIB by * drawing native and celestial coordinate graticules for Bonne's projection. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include int main() { char text[80]; int ci, crval1, crval2, ilat, ilng, j, k, latpole, lonpole, stat[361], status; float xr[512], yr[512]; double lat[181], lng[361], phi[361], theta[361], x[361], y[361]; struct celprm native, celestial; printf( "Testing WCSLIB celestial coordinate transformation routines (tcel1.c)\n" "---------------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of cel status return values:\n"); for (status = 1; status <= 6; status++) { printf("%4d: %s.\n", status, cel_errmsg[status]); } printf("\n"); /* Initialize. */ celini(&native); /* Reference angles for the native graticule (in fact, the defaults). */ native.ref[0] = 0.0; native.ref[1] = 0.0; /* Set up Bonne's projection with conformal latitude at +35. */ strcpy(native.prj.code, "BON"); native.prj.pv[1] = 35.0; /* Celestial graticule. */ celini(&celestial); celestial.prj = native.prj; /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); /* Define pen colours. */ cpgscr(0, 0.0f, 0.0f, 0.0f); cpgscr(1, 1.0f, 1.0f, 0.0f); cpgscr(2, 1.0f, 1.0f, 1.0f); cpgscr(3, 0.5f, 0.5f, 0.8f); cpgscr(4, 0.8f, 0.5f, 0.5f); cpgscr(5, 0.8f, 0.8f, 0.8f); cpgscr(6, 0.5f, 0.5f, 0.8f); cpgscr(7, 0.8f, 0.5f, 0.5f); cpgscr(8, 0.3f, 0.5f, 0.3f); /* Define PGPLOT viewport. */ cpgenv(-180.0f, 180.0f, -90.0f, 140.0f, 1, -2); /* Loop over CRVAL2, LONPOLE, and LATPOLE with CRVAL1 incrementing by */ /* 15 degrees each time (it has an uninteresting effect). */ crval1 = -180; for (crval2 = -90; crval2 <= 90; crval2 += 30) { for (lonpole = -180; lonpole <= 180; lonpole += 30) { for (latpole = -1; latpole <= 1; latpole += 2) { /* For the celestial graticule, set the celestial coordinates of * the reference point of the projection (which for Bonne's * projection is at the intersection of the native equator and * prime meridian), the native longitude of the celestial pole, * and extra information needed to determine the celestial * latitude of the native pole. These correspond to FITS keywords * CRVAL1, CRVAL2, LONPOLE, and LATPOLE. */ celestial.ref[0] = (double)crval1; celestial.ref[1] = (double)crval2; celestial.ref[2] = (double)lonpole; celestial.ref[3] = (double)latpole; /* Skip invalid values of LONPOLE. */ if (celset(&celestial)) { continue; } /* Skip redundant values of LATPOLE. */ if (latpole == 1 && fabs(celestial.ref[3]) < 0.1) { continue; } /* Buffer PGPLOT output. */ cpgbbuf(); cpgeras(); /* Write a descriptive title. */ sprintf(text, "Bonne's projection (BON) - 15 degree graticule"); printf("\n%s\n", text); cpgtext(-180.0f, -100.0f, text); sprintf(text, "centred on celestial coordinates (%7.2f,%6.2f)", celestial.ref[0], celestial.ref[1]); printf("%s\n", text); cpgtext (-180.0f, -110.0f, text); sprintf(text, "with north celestial pole at native coordinates " "(%7.2f,%7.2f)", celestial.ref[2], celestial.ref[3]); printf("%s\n", text); cpgtext(-180.0f, -120.0f, text); /* Draw the native graticule faintly in the background. */ cpgsci(8); /* Draw native meridians of longitude. */ for (j = 0, ilat = -90; ilat <= 90; ilat++, j++) { lat[j] = (double)ilat; } for (ilng = -180; ilng <= 180; ilng += 15) { lng[0] = (double)ilng; if (ilng == -180) lng[0] = -179.99; if (ilng == 180) lng[0] = 179.99; /* Dash the longitude of the celestial pole. */ if ((ilng-lonpole)%360 == 0) { cpgsls(2); cpgslw(5); } cels2x(&native, 1, 181, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 181; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); cpgsls(1); cpgslw(1); } /* Draw native parallels of latitude. */ lng[0] = -179.99; lng[360] = 179.99; for (j = 1, ilng = -179; ilng < 180; ilng++, j++) { lng[j] = (double)ilng; } for (ilat = -90; ilat <= 90; ilat += 15) { lat[0] = (double)ilat; cels2x(&native, 361, 1, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 361; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); } /* Draw a colour-coded celestial coordinate graticule. */ ci = 1; /* Draw celestial meridians of longitude. */ for (j = 0, ilat = -90; ilat <= 90; ilat++, j++) { lat[j] = (double)ilat; } for (ilng = -180; ilng <= 180; ilng += 15) { lng[0] = (double)ilng; if (++ci > 7) ci = 2; cpgsci(ilng?ci:1); /* Dash the reference longitude. */ if ((ilng-crval1)%360 == 0) { cpgsls(2); cpgslw(5); } cels2x(&celestial, 1, 181, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 181; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } /* Test for discontinuities. */ if (j > 0) { if (fabs(x[j]-x[j-1]) > 4.0 || fabs(y[j]-y[j-1]) > 4.0) { if (k > 1) cpgline(k, xr, yr); k = 0; } } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); cpgsls(1); cpgslw(1); } /* Draw celestial parallels of latitude. */ for (j = 0, ilng = -180; ilng <= 180; ilng++, j++) { lng[j] = (double)ilng; } ci = 1; for (ilat = -90; ilat <= 90; ilat += 15) { lat[0] = (double)ilat; if (++ci > 7) ci = 2; cpgsci(ilat?ci:1); /* Dash the reference latitude. */ if (ilat == crval2) { cpgsls(2); cpgslw(5); } cels2x(&celestial, 361, 1, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 361; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } /* Test for discontinuities. */ if (j > 0) { if (fabs(x[j]-x[j-1]) > 4.0 || fabs(y[j]-y[j-1]) > 4.0) { if (k > 1) cpgline(k, xr, yr); k = 0; } } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); cpgsls(1); cpgslw(1); } /* Flush PGPLOT buffer. */ cpgebuf(); printf(" Type for next page: "); getc(stdin); /* Cycle through celestial longitudes. */ if ((crval1 += 15) > 180) crval1 = -180; /* Skip boring celestial latitudes. */ if (crval2 == 0) break; } if (crval2 == 0) break; } } cpgask(0); cpgend(); return 0; } pywcs-1.12/wcslib/C/test/tcel2.c0000644001153600020070000004355012310355625020455 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tcel2.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tcel2 thoroughly tests the WCSLIB celestial coordinate transformation * routines, particularly celset(), by plotting oblique test grids for a wide * variety of transformation parameters. A simple user interface provides * limited control of the path taken through this parameter space. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include #define nint(x) ((int)(x + (((x) > 0.0) ? 0.5 : -0.5))) int main() { char answer[16], ctrl, text[128]; int ci, crval1, crval1_j, crval2, crval2_i, first, ilat, ilng, iprj, j, k, latpole, lonpole, lonpole_i, lonpole_j, phi_p, stat[361], status; float xr[512], yr[512]; double alpha_p, lat[181], lng[361], phi[361], theta[361], x[361], y[361]; struct celprm native, celestial; printf( "Testing WCSLIB celestial coordinate transformation routines (tcel2.c)\n" "---------------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of cel status return values:\n"); for (status = 1; status <= 6; status++) { printf("%4d: %s.\n", status, cel_errmsg[status]); } printf("\n\nLegend (in the order drawn)\n---------------------------\n"); printf("Native graticule in dark green with the meridian containing the " "celestial\n pole (LONPOLE) thicker and in green. Also tagged " "beyond the perimeter.\n"); printf("Celestial graticule colour-coded, the direction of increasing " "celestial\n longitude and latitude is white -> blue -> red, " "with the equator and\n prime meridian in yellow.\n"); printf("Celestial meridian (CRVAL1) and parallel (CRVAL2) through the " "reference point\n is thicker and dashed.\n"); printf("Reference point of the projection (phi0,theta0) is marked with " "a green circle\n with red centre. It should coincide with the " "dashed celestial meridian and\n parallel.\n"); printf("Celestial pole (LONPOLE,LATPOLE) marked with a green circle with " "black centre.\n"); printf("Celestial prime meridian expected for \"change of origin\" case " "marked with\n an open yellow circle (where applicable). Should " "coincide with the prime\n meridian.\n"); printf("\n\n"); printf("Loop control; LONPOLE changes fastest, then CRVAL1, then CRVAL2\n" "---------------------------------------------------------------\n" " next: do next plot\n" " skip: skip past invalid values of LONPOLE\n" " break: break out of inner loop on LONPOLE\n" " continue: cycle through inner loop on LONPOLE\n"); printf(" proj: skip to next projection\n" " inc: LONPOLE++, preserving CRVAL1 & CRVAL2\n" " jump: CRVAL2++, preserving CRVAL1 & LONPOLE\n" " exit: terminate execution\n" " quit: terminate execution\n" "Capital letter kills query.\n"); printf("\n\n"); /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); /* Define pen colours. */ cpgscr( 0, 0.0f, 0.0f, 0.0f); /* Black */ cpgscr( 1, 1.0f, 1.0f, 0.0f); /* Yellow */ cpgscr( 2, 1.0f, 1.0f, 1.0f); /* White */ cpgscr( 3, 0.5f, 0.5f, 0.8f); /* Mauve */ cpgscr( 4, 0.8f, 0.5f, 0.5f); /* Pink */ cpgscr( 5, 0.8f, 0.8f, 0.8f); /* Grey */ cpgscr( 6, 0.5f, 0.5f, 0.8f); /* Mauve */ cpgscr( 7, 0.8f, 0.5f, 0.5f); /* Pink */ cpgscr( 8, 0.3f, 0.5f, 0.3f); /* Dark green */ cpgscr( 9, 0.0f, 1.0f, 0.0f); /* Green */ cpgscr(10, 1.0f, 0.0f, 0.0f); /* Red */ /* Define PGPLOT viewport. */ cpgenv(-195.0f, 195.0f, -195.0f, 195.0f, 1, -2); cpgsch(0.8f); ctrl = 'n'; for (iprj = 0; iprj < 4; iprj++) { /* Initialize. */ celini(&native); celini(&celestial); /* Reference coordinates for the native graticule. */ if (iprj == 0) { /* Set up a zenithal equidistant projection. */ strcpy(native.prj.code, "ARC"); native.ref[0] = 0.0; native.ref[1] = 90.0; native.ref[2] = 180.0; celestial.phi0 = 0.0; celestial.theta0 = 90.0; } else if (iprj == 1) { /* Set up a conic equidistant projection. */ strcpy(native.prj.code, "COD"); native.prj.pv[1] = 45.0; native.prj.pv[2] = 25.0; native.ref[0] = 0.0; native.ref[1] = 45.0; native.ref[2] = 180.0; celestial.phi0 = 60.0; celestial.theta0 = 45.0; } else if (iprj == 2) { /* Set up a Sanson-Flamsteed projection as Bonne's equatorial. */ strcpy(native.prj.code, "BON"); native.prj.pv[1] = 0.0; native.ref[0] = 0.0; native.ref[1] = 0.0; native.ref[2] = 0.0; celestial.phi0 = -30.0; celestial.theta0 = 0.0; } else if (iprj == 3) { /* Set up a polyconic projection. */ strcpy(native.prj.code, "PCO"); native.ref[0] = 0.0; native.ref[1] = 0.0; native.ref[2] = 0.0; celestial.phi0 = -60.0; celestial.theta0 = -90.0; } celestial.prj = native.prj; /* Loop over CRVAL2, CRVAL1 and LONPOLE. */ crval1_j = -180; crval2_i = 45; lonpole_i = 15; lonpole_j = -180; for (crval2 = -90; crval2 <= 90; crval2 += crval2_i) { for (crval1 = -180; crval1 <= 180; crval1 += 90) { first = 1; for (lonpole = -180; lonpole <= 180; lonpole += lonpole_i) { /* lonpole = 999; */ latpole = 999; /* if (crval2 < 0) latpole = -999; */ /* if (crval2 > 0) latpole = 999; */ if (ctrl == 'j' || ctrl == 'J') { /* Restore CRVAL1 and LONPOLE from last time. */ crval1 = crval1_j; lonpole = lonpole_j; } celestial.ref[0] = (double)crval1; celestial.ref[1] = (double)crval2; celestial.ref[2] = (double)lonpole; celestial.ref[3] = (double)latpole; /* Buffer PGPLOT output. */ cpgbbuf(); cpgeras(); cpgsci(2); /* Write parameter summary. */ sprintf(text, "(CRVAL1, CRVAL2, LONPOLE): (%+3.3d, %+2.2d, %+3.3d)", crval1, crval2, lonpole); cpgtext(-180.0f, 200.0f, text); /* Skip invalid values of LONPOLE. */ if (celset(&celestial)) { sprintf(text, "INVALID VALUE OF LONPOLE (= %+3.3d)", lonpole); cpgtext(-90.0f, 0.0f, text); sprintf(text, "%s projection, (\\gf\\d0\\u,\\gh\\d0\\u) = " "(%+3.3d, %+2.2d)", native.prj.code, nint(celestial.phi0), nint(celestial.theta0)); cpgtext(-180.0f, -200.0f, text); if (ctrl == 's' || ctrl == 'S') { cpgebuf(); continue; } goto skip; } /* Write parameters. */ sprintf(text, "%s projection, (\\gf\\d0\\u,\\gh\\d0\\u) = " "(%+3.3d, %+2.2d) - green circle with red centre", native.prj.code, nint(celestial.phi0), nint(celestial.theta0)); cpgtext(-180.0f, -200.0f, text); sprintf(text, "(CRVAL1, CRVAL2): (%+3.3d, %+2.2d) - dashed grid" " lines", nint(celestial.ref[0]), nint(celestial.ref[1])); cpgtext(-180.0f, -213.0f, text); sprintf(text, "(LONPOLE, LATPOLE): (%+3.3d, %+3.3d) -> " "(%+3.3d, %+2.2d) - open green circle", lonpole, latpole, nint(celestial.ref[2]), nint(celestial.ref[3])); cpgtext(-180.0f, -226.0f, text); sprintf(text, "(\\ga\\dp\\u, \\gd\\dp\\u): (%+3.3d, %+2.2d)", nint(celestial.euler[0]), nint(90.0-celestial.euler[1])); cpgtext(-180.0f, -239.0f, text); if (celestial.latpreq == 0) { sprintf(text, "(LATPOLE not required.)"); } else if (celestial.latpreq == 1) { sprintf(text, "(LATPOLE disambiguates.)"); } else if (celestial.latpreq == 2) { sprintf(text, "(LATPOLE IS DEFINITIVE.)"); } cpgtext(-40.0f, -239.0f, text); /* Draw the native graticule in the background (dark green). */ cpgsci(8); /* Draw native meridians of longitude. */ for (j = 0, ilat = -90; ilat <= 90; ilat++, j++) { lat[j] = (double)ilat; } phi_p = nint(celestial.ref[2]); for (ilng = -180; ilng <= 180; ilng += 15) { lng[0] = (double)ilng; if (ilng == -180) lng[0] = -179.99; if (ilng == 180) lng[0] = 179.99; /* Meridian containing the celestial pole (thick green). */ if (ilng == phi_p) { cpgslw(5); cpgsci(9); } cels2x(&native, 1, 181, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 181; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); cpgslw(1); cpgsci(8); } /* Draw native parallels of latitude. */ lng[0] = -179.99; lng[360] = 179.99; for (j = 1, ilng = -179; ilng < 180; ilng++, j++) { lng[j] = (double)ilng; } for (ilat = -90; ilat <= 90; ilat += 15) { lat[0] = (double)ilat; cels2x(&native, 361, 1, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 361; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); } /* Tag the longitude of the celestial pole. */ cpgslw(5); cpgsci(9); phi[0] = celestial.ref[2]; theta[0] = -90.0; theta[1] = -80.0; prjs2x(&(native.prj), 1, 2, 1, 1, phi, theta, x, y, stat); xr[0] = -x[0]; yr[0] = y[0]; xr[1] = -x[0] + (x[1] - x[0]); yr[1] = y[0] - (y[1] - y[0]); cpgline(2, xr, yr); /* Draw a colour-coded celestial coordinate graticule. */ ci = 1; /* Draw celestial meridians of longitude. */ for (j = 0, ilat = -90; ilat <= 90; ilat++, j++) { lat[j] = (double)ilat; } for (ilng = -180; ilng <= 180; ilng += 15) { lng[0] = (double)ilng; /* Cycle through colours with the prime meridian in yellow. */ if (++ci > 7) ci = 2; cpgsci(ilng?ci:1); /* Dash the reference longitude and make it thicker. */ if ((ilng-crval1)%360 == 0) { cpgsls(2); cpgslw(5); } cels2x(&celestial, 1, 181, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 181; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } /* Test for discontinuities. */ if (j > 0) { if (fabs(phi[j]-phi[j-1]) > 15.0) { if (k > 1) cpgline(k, xr, yr); k = 0; } } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); cpgsls(1); cpgslw(1); } /* Draw celestial parallels of latitude. */ for (j = 0, ilng = -180; ilng <= 180; ilng++, j++) { lng[j] = (double)ilng; } ci = 1; for (ilat = -90; ilat <= 90; ilat += 15) { lat[0] = (double)ilat; /* Cycle through colours with the prime meridian in yellow. */ if (++ci > 7) ci = 2; cpgsci(ilat?ci:1); /* Dash the reference latitude and make it thicker. */ if (ilat == crval2) { cpgsls(2); cpgslw(5); } cels2x(&celestial, 361, 1, 1, 1, lng, lat, phi, theta, x, y, stat); k = 0; for (j = 0; j < 361; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } /* Test for discontinuities. */ if (j > 0) { if (fabs(phi[j]-phi[j-1]) > 15.0) { if (k > 1) cpgline(k, xr, yr); k = 0; } } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); cpgsls(1); cpgslw(1); } /* Mark the fiducial point (green with red centre). */ phi[0] = celestial.phi0; theta[0] = celestial.theta0; prjs2x(&(native.prj), 1, 1, 1, 1, phi, theta, x, y, stat); xr[0] = -x[0]; yr[0] = y[0]; cpgslw(5); cpgsci(9); cpgpt1(xr[0], yr[0], 24); cpgpt1(xr[0], yr[0], 23); cpgsci(10); cpgpt1(xr[0], yr[0], 17); /* Mark the celestial pole. */ phi[0] = celestial.ref[2]; theta[0] = celestial.ref[3]; prjs2x(&(native.prj), 1, 1, 1, 1, phi, theta, x, y, stat); xr[0] = -x[0]; yr[0] = y[0]; cpgslw(5); cpgsci(9); cpgpt1(xr[0], yr[0], 24); cpgpt1(xr[0], yr[0], 23); cpgsci(0); cpgpt1(xr[0], yr[0], 17); /* Mark zero celestial longitude expected for "change of origin" * case with a thick yellow circle. */ if (celestial.euler[1] == 0.0 || celestial.euler[1] == 180.0) { if (celestial.theta0 == 90.0) { alpha_p = celestial.ref[0]; } else if (fabs(celestial.ref[1]) == 90.0) { alpha_p = celestial.ref[0]; } else if (celestial.euler[1] == 0.0) { alpha_p = celestial.ref[0] + celestial.ref[2] - celestial.phi0 - 180.0; } else { alpha_p = celestial.ref[0] - celestial.ref[2] + celestial.phi0; } if (celestial.euler[1] == 0.0) { phi[0] = celestial.euler[2] - alpha_p + 180.0; } else { phi[0] = celestial.euler[2] + alpha_p; } phi[0] = fmod(phi[0], 360.0); if (phi[0] < -180.0) { phi[0] += 360.0; } else if (phi[0] > 180.0) { phi[0] -= 360.0; } theta[0] = -45.0; prjs2x(&(native.prj), 1, 1, 1, 1, phi, theta, x, y, stat); xr[0] = -x[0]; yr[0] = y[0]; cpgslw(5); cpgsci(1); cpgpt1(xr[0], yr[0], 24); } cpgslw(1); /* Flush PGPLOT buffer. */ skip: cpgebuf(); if ((ctrl >= 'A' && ctrl <= 'Z') || ((ctrl == 'c' || ctrl == 'b' || ctrl == 'j') && !first)) { /* Keep going. */ } else { printf("Next, skip, break, continue, exit [%c]: ", ctrl); fgets(answer, 16, stdin); if (strchr("bBcCeEiIjJnNpPqQsS", (int)answer[0]) != 0) { ctrl = answer[0]; } } if (ctrl == 'i' || ctrl == 'I') { lonpole_i = 1; } else { lonpole_i = 15; } if (ctrl == 'P') { /* There's no point in skipping all projections. */ ctrl = 'p'; break; } if (ctrl == 'p') break; if (ctrl == 'b' || ctrl == 'B') break; if (ctrl == 'j' || ctrl == 'J') break; if (ctrl == 'e' || ctrl == 'E') goto end; if (ctrl == 'q' || ctrl == 'Q') goto end; first = 0; } if (ctrl == 'p') break; if (ctrl == 'j' || ctrl == 'J') break; } if (ctrl == 'p') break; if (ctrl == 'j' || ctrl == 'J') { /* Save CRVAL1 and LONPOLE for next time. */ crval1_j = crval1; lonpole_j = lonpole; /* Slow down CRVAL2. */ crval2_i = 1; } else { crval2_i = 45; } } } end: cpgask(0); cpgend(); return 0; } pywcs-1.12/wcslib/C/test/tfitshdr.c0000644001153600020070000002007712310355626021273 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tfitshdr.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tfitshdr tests fitshdr(), the FITS parser for image headers, by reading a * test header and printing the resulting fitskey structs. * * Input comes from file 'pih.fits' using either fits_hdr2str() from CFITSIO * if the DO_CFITSIO preprocessor is defined, or read directly using fgets() * otherwise. * * If the DO_WCSHDR preprocessor macro is defined, wcshdr() will be called * first to extract all WCS-related keyrecords from the input header before * passing it on to fitshdr(). * *---------------------------------------------------------------------------*/ #include #include #include #include #if defined HAVE_CFITSIO && defined DO_CFITSIO #include #endif #ifdef DO_WCSHDR #include #endif #include int main() { char infile[] = "pih.fits"; char text[80]; int i, j, k, nkeyrec, nkeyids, nreject, status; struct fitskey *keys, *kptr; struct fitskeyid keyids[8]; #if defined HAVE_CFITSIO && defined DO_CFITSIO char *header; fitsfile *fptr; #else char keyrec[81], header[288001]; int end; FILE *fptr; #endif #ifdef DO_WCSHDR struct wcsprm *wcs; int ctrl, nwcs, relax; #endif /* Set line buffering in case stdout is redirected to a file, otherwise * stdout and stderr messages will be jumbled (stderr is unbuffered). */ setvbuf(stdout, NULL, _IOLBF, 0); printf("Testing FITS image header parser (tfitshdr.c)\n" "---------------------------------------------\n\n"); /* Read in the FITS header. */ #if defined HAVE_CFITSIO && defined DO_CFITSIO status = 0; if (fits_open_file(&fptr, infile, READONLY, &status)) { fits_report_error(stderr, status); return 1; } if (fits_hdr2str(fptr, 0, NULL, 0, &header, &nkeyrec, &status)) { fits_report_error(stderr, status); return 1; } fits_close_file(fptr, &status); #else if ((fptr = fopen(infile, "r")) == 0) { printf("ERROR opening %s\n", infile); return 1; } k = 0; end = 0; nkeyrec = 0; for (j = 0; j < 100; j++) { for (i = 0; i < 36; i++) { if (fgets(keyrec, 81, fptr) == 0) { break; } strncpy(header+k, keyrec, 80); k += 80; nkeyrec++; if (strncmp(keyrec, "END ", 8) == 0) { /* An END keyrecord was read, but read the rest of the block. */ end = 1; } } if (end) break; } fclose(fptr); #endif printf("Found %d header keyrecords.\n", nkeyrec); #ifdef DO_WCSHDR /* Cull recognized, syntactically valid WCS keyrecords from the header. */ relax = WCSHDR_all; ctrl = -1; if ((status = wcspih(header, nkeyrec, relax, ctrl, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status, wcs_errmsg[status]); return 1; } /* Number remaining. */ nkeyrec = strlen(header) / 80; #endif /* Specific keywords to be located or culled. */ strcpy(keyids[0].name, "SIMPLE "); strcpy(keyids[1].name, "BITPIX "); strcpy(keyids[2].name, "NAXIS "); strcpy(keyids[3].name, "COMMENT "); strcpy(keyids[4].name, "HISTORY "); strcpy(keyids[5].name, " "); strcpy(keyids[6].name, "END "); nkeyids = 7; if (nkeyids) { printf("\nThe following keyrecords will not be listed:\n"); for (i = 0; i < nkeyids; i++) { printf(" \"%8s\"\n", keyids[i].name); } } /* Parse the header. */ if ((status = fitshdr(header, nkeyrec, nkeyids, keyids, &nreject, &keys))) { printf("fitskey ERROR %d: %s.\n", status, fitshdr_errmsg[status]); } #if defined HAVE_CFITSIO && defined DO_CFITSIO free(header); #endif /* Report the results. */ printf("\n%d header keyrecords parsed by fitshdr(), %d rejected:\n\n", nkeyrec, nreject); kptr = keys; for (i = 0; i < nkeyrec; i++, kptr++) { /* Skip syntactically valid keyrecords that were indexed. */ if (kptr->keyno < 0 && !kptr->status) continue; /* Basic keyrecord info. */ printf("%4d%5d %-8s%3d", kptr->keyno, kptr->status, kptr->keyword, kptr->type); /* Format the keyvalue for output. */ switch (abs(kptr->type)%10) { case 1: /* Logical. */ sprintf(text, "%c", kptr->keyvalue.i?'T':'F'); break; case 2: /* 32-bit signed integer. */ sprintf(text, "%d", kptr->keyvalue.i); break; case 3: /* 64-bit signed integer. */ #ifdef WCSLIB_INT64 sprintf(text, "%+lld", kptr->keyvalue.k); #else if (kptr->keyvalue.k[2]) { sprintf(text, "%+d%09d%09d", kptr->keyvalue.k[2], abs(kptr->keyvalue.k[1]), abs(kptr->keyvalue.k[0])); } else { sprintf(text, "%+d%09d", kptr->keyvalue.k[1], abs(kptr->keyvalue.k[0])); } #endif break; case 4: /* Very long integer. */ k = 0; for (j = 7; j > 0; j--) { if (kptr->keyvalue.l[j]) { k = j; break; } } sprintf(text, "%+d", kptr->keyvalue.l[k]); for (j = k-1; j >= 0; j--) { sprintf(text+strlen(text), "%09d", abs(kptr->keyvalue.l[j])); } break; case 5: /* Float. */ sprintf(text, "%+13.6e", kptr->keyvalue.f); break; case 6: /* Int complex. */ sprintf(text, "%.0f %.0f", kptr->keyvalue.c[0], kptr->keyvalue.c[1]); break; case 7: /* Float complex. */ sprintf(text, "%+13.6e %+13.6e", kptr->keyvalue.c[0], kptr->keyvalue.c[1]); break; case 8: /* String. */ sprintf(text, "\"%s\"", kptr->keyvalue.s); break; default: /* No value. */ *text = '\0'; break; } if (kptr->type > 0) { /* Keyvalue successfully extracted. */ printf(" %s", text); } else if (kptr->type < 0) { /* Syntax error of some type while extracting the keyvalue. */ printf(" (%s)", text); } /* Units? */ if (kptr->ulen) { printf(" %.*s", kptr->ulen-2, kptr->comment+1); } /* Comment text or reject keyrecord. */ printf("\n%s\n", kptr->comment); } /* Print indexes. */ printf("\n\nIndexes of selected keywords:\n"); for (i = 0; i < nkeyids; i++) { printf("%-8s%5d%5d%5d", keyids[i].name, keyids[i].count, keyids[i].idx[0], keyids[i].idx[1]); /* Print logical (SIMPLE) and integer (BITPIX, NAXIS) values. */ if (keyids[i].count) { kptr = keys + keyids[i].idx[0]; printf("%4d", kptr->type); if (kptr->type == 1) { printf("%5c", kptr->keyvalue.i?'T':'F'); } else if (kptr->type == 2) { printf("%5d", kptr->keyvalue.i); } } printf("\n"); } free(keys); return 0; } pywcs-1.12/wcslib/C/test/tlin.c0000644001153600020070000001023012310355625020377 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tlin.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tlin tests the linear transformation routines supplied with WCSLIB. * *---------------------------------------------------------------------------*/ #include #include #include #include int NAXIS = 5; int NCOORD = 2; int NELEM = 9; double CRPIX[5] = {256.0, 256.0, 64.0, 128.0, 1.0}; double PC[5][5] = {{ 1.0, 0.5, 0.0, 0.0, 0.0}, { 0.5, 1.0, 0.0, 0.0, 0.0}, { 0.0, 0.0, 1.0, 0.0, 0.0}, { 0.0, 0.0, 0.0, 1.0, 0.0}, { 0.0, 0.0, 0.0, 0.0, 1.0}}; double CDELT[5] = { 1.2, 2.3, 3.4, 4.5, 5.6}; double pix0[2][9] = {{303.0, 265.0, 112.4, 144.5, 28.2, 0.0, 0.0, 0.0, 0.0}, { 19.0, 57.0, 2.0, 15.0, 42.0, 0.0, 0.0, 0.0, 0.0}}; const double tol = 1.0e-13; int main() { int i, j, k, nFail, status; double img[2][9], *pcij, pix[2][9], resid, residmax; struct linprm lin; printf("Testing WCSLIB linear transformation routines (tlin.c)\n" "------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of lin status return values:\n"); for (status = 1; status <= 3; status++) { printf("%4d: %s.\n", status, lin_errmsg[status]); } lin.flag = -1; linini(1, NAXIS, &lin); pcij = lin.pc; for (i = 0; i < lin.naxis; i++) { lin.crpix[i] = CRPIX[i]; for (j = 0; j < lin.naxis; j++) { *(pcij++) = PC[i][j]; } lin.cdelt[i] = CDELT[i]; } for (k = 0; k < NCOORD; k++) { printf("\nPIX %d:", k+1); for (j = 0; j < NAXIS; j++) { printf("%14.8f", pix0[k][j]); } } printf("\n"); if ((status = linp2x(&lin, NCOORD, NELEM, pix0[0], img[0]))) { printf("linp2x ERROR %d\n", status); return 1; } for (k = 0; k < NCOORD; k++) { printf("\nIMG %d:", k+1); for (j = 0; j < NAXIS; j++) { printf("%14.8f", img[k][j]); } } printf("\n"); if ((status = linx2p(&lin, NCOORD, NELEM, img[0], pix[0]))) { printf("linx2p ERROR %d\n", status); return 1; } for (k = 0; k < NCOORD; k++) { printf("\nPIX %d:", k+1); for (j = 0; j < NAXIS; j++) { printf("%14.8f", pix[k][j]); } } printf("\n"); /* Check closure. */ nFail = 0; residmax = 0.0; for (k = 0; k < NCOORD; k++) { for (j = 0; j < NAXIS; j++) { resid = fabs(pix[k][j] - pix0[k][j]); if (residmax < resid) residmax = resid; if (resid > tol) nFail++; } } printf("\nlinp2x/linx2p: Maximum closure residual = %.1e pixel.\n", residmax); linfree(&lin); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } pywcs-1.12/wcslib/C/test/tlog.c0000644001153600020070000000737112310355625020412 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tlog.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tlog tests the logarithmic coordinate transformation routines for closure. * *---------------------------------------------------------------------------*/ #include #include #include #define NCRD 10000 const double tol = 1.0e-13; int main() { register int j, k; int nFail = 0, stat1[NCRD], stat2[NCRD], status; double logc[NCRD], resid, residmax, step, x0[NCRD], x1[NCRD]; double crval = 3.3; printf( "Testing closure of WCSLIB logarithmic coordinate routines (tlog.c)\n" "------------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of log status return values:\n"); for (status = 2; status <= 3; status++) { printf("%4d: %s.\n", status, log_errmsg[status]); } /* Construct a logarithmic axis and test closure. */ step = (40.0/NCRD) / 2.0; for (j = 0, k = -NCRD; j < NCRD; j++, k += 2) { x0[j] = k*step; } printf("\nLogarithmic range: %.1f to %.1f, step: %.4f\n", x0[0], x0[NCRD-1], x0[1] - x0[0]); /* Convert the first to the second. */ if ((status = logx2s(crval, NCRD, 1, 1, x0, logc, stat1))) { printf("logx2s ERROR %d: %s.\n", status, log_errmsg[status]); } /* Convert the second back to the first. */ if ((status = logs2x(crval, NCRD, 1, 1, logc, x1, stat2))) { printf("logs2x ERROR %d: %s.\n", status, log_errmsg[status]); } residmax = 0.0; /* Test closure. */ for (j = 0; j < NCRD; j++) { if (stat1[j]) { printf("logx2s: x =%20.12e -> log = ???, stat = %d\n", x0[j], stat1[j]); continue; } if (stat2[j]) { printf("logs2x: x =%20.12e -> log =%20.12e -> x = ???, stat = %d\n", x0[j], logc[j], stat2[j]); continue; } if (x0[j] == 0.0) { resid = fabs(x1[j] - x0[j]); } else { resid = fabs((x1[j] - x0[j]) / x0[j]); if (resid > residmax) residmax = resid; } if (resid > tol) { nFail++; printf("logx2s: x =%20.12e -> log =%20.12e ->\n x =%20.12e, " "resid =%20.12e\n", x0[j], logc[j], x1[j], resid); } } if (nFail) printf("\n"); printf("logx2s/logs2x: Maximum closure residual = %.1e\n", residmax); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } pywcs-1.12/wcslib/C/test/tofits.c0000644001153600020070000000470512310355625020753 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tofits.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tofits turns a list of FITS header keyrecords, one per line, into a proper * FITS header by padding them with blanks to 80 characters and stripping out * newline characters. It also pads the header to an integral number of 2880- * byte blocks if necessary. * * It operates as a filter, e.g.: * * tofits < infile > outfile * * Input lines beginning with '#' are treated as comments. * *===========================================================================*/ #include int main() { int c, i = 0, nkeyrec = 0; while ((c = getchar()) != EOF) { if (c == '\n') { /* Blank-fill the keyrecord. */ while (i++ < 80) { putchar(' '); } i = 0; nkeyrec++; } else if (c == '#' && i == 0) { /* Discard comments. */ while ((c = getchar()) != EOF) { if (c == '\n') break; } } else { putchar(c); i++; } } /* Pad to a multiple of 2880-bytes. */ if (nkeyrec %= 36) { while (nkeyrec++ < 36) { i = 0; while (i++ < 80) { putchar(' '); } } } return 0; } pywcs-1.12/wcslib/C/test/tpih1.c0000644001153600020070000001406312310355626020467 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tpih1.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tpih1 tests wcspih(), the WCS FITS parser for image headers, and wcsfix(), * which translates non-standard constructs. It reads a test header and uses * wcsprt() to print the resulting wcsprm structs. * * Input comes from file "pih.fits" using either fits_hdr2str() from CFITSIO * if the DO_CFITSIO preprocessor is defined, or read directly using fgets() * otherwise. * *---------------------------------------------------------------------------*/ #include #include #include #if defined HAVE_CFITSIO && defined DO_CFITSIO #include #endif #include #include #include #include int main() { char infile[] = "pih.fits"; char a, *hptr; int alts[27], ctrl, ialt, iblock, ifix, ikeyrec, iwcs, nkeyrec, nreject, nwcs, relax, stat[NWCSFIX], status; struct wcsprm *wcs; #if defined HAVE_CFITSIO && defined DO_CFITSIO char *header; fitsfile *fptr; #else char keyrec[81], header[288001]; int gotend, k; FILE *fptr; #endif /* Set line buffering in case stdout is redirected to a file, otherwise * stdout and stderr messages will be jumbled (stderr is unbuffered). */ setvbuf(stdout, NULL, _IOLBF, 0); printf("Testing WCSLIB parser for FITS image headers (tpih1.c)\n" "------------------------------------------------------\n\n"); /* Read in the FITS header, excluding COMMENT and HISTORY keyrecords. */ #if defined HAVE_CFITSIO && defined DO_CFITSIO status = 0; if (fits_open_file(&fptr, infile, READONLY, &status)) { fits_report_error(stderr, status); return 1; } if (fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status)) { fits_report_error(stderr, status); return 1; } fits_close_file(fptr, &status); #else if ((fptr = fopen(infile, "r")) == 0) { fprintf(stderr, "ERROR opening %s\n", infile); return 1; } k = 0; nkeyrec = 0; gotend = 0; for (iblock = 0; iblock < 100; iblock++) { for (ikeyrec = 0; ikeyrec < 36; ikeyrec++) { if (fgets(keyrec, 81, fptr) == 0) { break; } if (strncmp(keyrec, " ", 8) == 0) continue; if (strncmp(keyrec, "COMMENT ", 8) == 0) continue; if (strncmp(keyrec, "HISTORY ", 8) == 0) continue; strncpy(header+k, keyrec, 80); k += 80; nkeyrec++; if (strncmp(keyrec, "END ", 8) == 0) { /* An END keyrecord was read, but read the rest of the block. */ gotend = 1; } } if (gotend) break; } fclose(fptr); #endif fprintf(stderr, "Found %d non-comment header keyrecords.\n\n", nkeyrec); /* Parse the header, allowing all recognized non-standard WCS keywords and * usage. All WCS keyrecords are culled from the header, illegal ones are * reported. */ relax = WCSHDR_all; ctrl = -2; fprintf(stderr, "\nIllegal-WCS header keyrecords rejected by wcspih():\n"); if ((status = wcspih(header, nkeyrec, relax, ctrl, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status, wcs_errmsg[status]); } if (!nreject) fprintf(stderr, "(none)\n"); /* List the remaining keyrecords. */ printf("\n\nNon-WCS header keyrecords not used by wcspih():\n"); hptr = header; while (*hptr) { printf("%.80s\n", hptr); hptr += 80; } #if defined HAVE_CFITSIO && defined DO_CFITSIO free(header); #endif /* Summarize what was found. */ status = wcsidx(nwcs, &wcs, alts); printf("\n\nFound %d alternate coordinate descriptions with indices:\n ", nwcs); for (a = 'A'; a <= 'Z'; a++) { printf("%2c", a); } printf("\n"); for (ialt = 0; ialt < 27; ialt++) { if (alts[ialt] < 0) { printf(" -"); } else { printf("%2d", alts[ialt]); } } printf("\n"); /* Fix non-standard usage and print each of the wcsprm structs. The output * from wcsprt() will be written to an internal buffer and then printed just * to show that it can be done. */ wcsprintf_set(0x0); for (iwcs = 0; iwcs < nwcs; iwcs++) { wcsprintf("\n------------------------------------" "------------------------------------\n"); /* Fix non-standard WCS keyvalues. */ if ((status = wcsfix(7, 0, wcs+iwcs, stat))) { printf("wcsfix ERROR, status returns: ("); for (ifix = 0; ifix < NWCSFIX; ifix++) { printf(ifix ? ", %d" : "%d", stat[ifix]); } printf(")\n\n"); } if ((status = wcsset(wcs+iwcs))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); continue; } if ((status = wcsprt(wcs+iwcs))) { fprintf(stderr, "wcsprt ERROR %d: %s.\n", status, wcs_errmsg[status]); } } printf("%s", wcsprintf_buf()); status = wcsvfree(&nwcs, &wcs); return 0; } pywcs-1.12/wcslib/C/test/tpih2.c0000644001153600020070000001305112310355626020464 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tpih2.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tpih2 tests wcspih(), the WCS FITS parser for image headers, by reading a * test header and using pgsbox() to plot coordinate graticules for the * resulting wcsprm structs. * * Input comes from file "pih.fits" using either fits_hdr2str() from CFITSIO * if the DO_CFITSIO preprocessor is defined, or read directly using fgets() * otherwise. * *---------------------------------------------------------------------------*/ #include #include #include #include #if defined HAVE_CFITSIO && defined DO_CFITSIO #include #endif #include #include #include #include int main() { char infile[] = "pih.fits"; char devtyp[16], idents[3][80], nlcprm[1], opt[2]; int c0[] = {-1, -1, -1, -1, -1, -1, -1}; int i, ic, gcode[2], naxis[2], nkeyrec, nreject, nwcs, relax, status; float blc[2], trc[2]; double cache[257][4], grid1[1], grid2[1], nldprm[1]; struct wcsprm *wcs; nlfunc_t pgwcsl_; #if defined HAVE_CFITSIO && defined DO_CFITSIO char *header; fitsfile *fptr; #else char keyrec[81], header[28801]; int gotend, j, k; FILE *fptr; #endif /* Set line buffering in case stdout is redirected to a file, otherwise * stdout and stderr messages will be jumbled (stderr is unbuffered). */ setvbuf(stdout, NULL, _IOLBF, 0); printf("Testing WCSLIB parser for FITS image headers (tpih2.c)\n" "------------------------------------------------------\n\n"); /* Read in the FITS header, excluding COMMENT and HISTORY keyrecords. */ #if defined HAVE_CFITSIO && defined DO_CFITSIO status = 0; if (fits_open_file(&fptr, infile, READONLY, &status)) { fits_report_error(stderr, status); return 1; } if (fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status)) { fits_report_error(stderr, status); return 1; } fits_close_file(fptr, &status); #else if ((fptr = fopen(infile, "r")) == 0x0) { printf("ERROR opening %s\n", infile); return 1; } k = 0; nkeyrec = 0; gotend = 0; for (j = 0; j < 10; j++) { for (i = 0; i < 36; i++) { if (fgets(keyrec, 81, fptr) == 0) { break; } if (strncmp(keyrec, " ", 8) == 0) continue; if (strncmp(keyrec, "COMMENT ", 8) == 0) continue; if (strncmp(keyrec, "HISTORY ", 8) == 0) continue; strncpy(header+k, keyrec, 80); k += 80; nkeyrec++; if (strncmp(keyrec, "END ", 8) == 0) { /* An END keyrecord was read, but read the rest of the block. */ gotend = 1; } } if (gotend) break; } fclose(fptr); #endif fprintf(stderr, "Found %d non-comment header keyrecords.\n", nkeyrec); relax = WCSHDR_all; if ((status = wcspih(header, nkeyrec, relax, 2, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status, wcs_errmsg[status]); } #if defined HAVE_CFITSIO && defined DO_CFITSIO free(header); #endif /* Plot setup. */ naxis[0] = 1024; naxis[1] = 1024; blc[0] = 0.5f; blc[1] = 0.5f; trc[0] = naxis[0] + 0.5f; trc[1] = naxis[1] + 0.5f; strcpy(devtyp, "/XWINDOW"); cpgbeg(0, devtyp, 1, 1); cpgvstd(); cpgwnad(0.0f, 1.0f, 0.0f, 1.0f); cpgask(1); cpgpage(); /* Annotation. */ strcpy(idents[0], "Right ascension"); strcpy(idents[1], "Declination"); opt[0] = 'G'; opt[1] = 'E'; /* Compact lettering. */ cpgsch(0.8f); /* Draw full grid lines. */ cpgsci(1); gcode[0] = 2; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; for (i = 0; i < nwcs; i++) { if ((status = wcsset(wcs+i))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); continue; } /* Get WCSNAME out of the wcsprm struct. */ strcpy(idents[2], (wcs+i)->wcsname); printf("\n%s\n", idents[2]); /* Draw the celestial grid. The grid density is set for each world */ /* coordinate by specifying LABDEN = 1224. */ ic = -1; cpgsbox(blc, trc, idents, opt, 0, 1224, c0, gcode, 0.0, 0, grid1, 0, grid2, 0, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(wcs+i), nldprm, 256, &ic, cache, &status); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); } status = wcsvfree(&nwcs, &wcs); return 0; } pywcs-1.12/wcslib/C/test/tprj1.c0000644001153600020070000002306212310355625020500 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tprj1.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tproj1 tests spherical projections for closure. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include int projex(char pcode[4], struct prjprm *prj, int north, int south, double tol); int main() { int nFail = 0, status; const double tol = 1.0e-9; struct prjprm prj; printf( "Testing closure of WCSLIB spherical projection routines (tprj1.c)\n" "-----------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of prj status return values:\n"); for (status = 1; status <= 4; status++) { printf("%4d: %s.\n", status, prj_errmsg[status]); } printf("\n"); prjini(&prj); /* AZP: zenithal/azimuthal perspective. */ prj.pv[1] = 0.5; prj.pv[2] = 30.0; nFail += projex("AZP", &prj, 90, 5, tol); /* SZP: slant zenithal perspective. */ prj.pv[1] = 0.5; prj.pv[2] = 210.0; prj.pv[3] = 60.0; nFail += projex("SZP", &prj, 90, -90, tol); /* TAN: gnomonic. */ nFail += projex("TAN", &prj, 90, 5, tol); /* STG: stereographic. */ nFail += projex("STG", &prj, 90, -85, tol); /* SIN: orthographic/synthesis. */ prj.pv[1] = -0.3; prj.pv[2] = 0.5; nFail += projex("SIN", &prj, 90, 45, tol); /* ARC: zenithal/azimuthal equidistant. */ nFail += projex("ARC", &prj, 90, -90, tol); /* ZPN: zenithal/azimuthal polynomial. */ prj.pv[0] = 0.00000; prj.pv[1] = 0.95000; prj.pv[2] = -0.02500; prj.pv[3] = -0.15833; prj.pv[4] = 0.00208; prj.pv[5] = 0.00792; prj.pv[6] = -0.00007; prj.pv[7] = -0.00019; prj.pv[8] = 0.00000; prj.pv[9] = 0.00000; nFail += projex("ZPN", &prj, 90, 10, tol); /* ZEA: zenithal/azimuthal equal area. */ nFail += projex("ZEA", &prj, 90, -85, tol); /* AIR: Airy's zenithal projection. */ prj.pv[1] = 45.0; nFail += projex("AIR", &prj, 90, -85, tol); /* CYP: cylindrical perspective. */ prj.pv[1] = 3.0; prj.pv[2] = 0.8; nFail += projex("CYP", &prj, 90, -90, tol); /* CEA: cylindrical equal area. */ prj.pv[1] = 0.75; nFail += projex("CEA", &prj, 90, -90, tol); /* CAR: plate carree. */ nFail += projex("CAR", &prj, 90, -90, tol); /* MER: Mercator's. */ nFail += projex("MER", &prj, 85, -85, tol); /* SFL: Sanson-Flamsteed. */ nFail += projex("SFL", &prj, 90, -90, tol); /* PAR: parabolic. */ nFail += projex("PAR", &prj, 90, -90, tol); /* MOL: Mollweide's projection. */ nFail += projex("MOL", &prj, 90, -90, tol); /* AIT: Hammer-Aitoff. */ nFail += projex("AIT", &prj, 90, -90, tol); /* COP: conic perspective. */ prj.pv[1] = 60.0; prj.pv[2] = 15.0; nFail += projex("COP", &prj, 90, -25, tol); /* COE: conic equal area. */ prj.pv[1] = 60.0; prj.pv[2] = -15.0; nFail += projex("COE", &prj, 90, -90, tol); /* COD: conic equidistant. */ prj.pv[1] = -60.0; prj.pv[2] = 15.0; nFail += projex("COD", &prj, 90, -90, tol); /* COO: conic orthomorphic. */ prj.pv[1] = -60.0; prj.pv[2] = -15.0; nFail += projex("COO", &prj, 85, -90, tol); /* BON: Bonne's projection. */ prj.pv[1] = 30.0; nFail += projex("BON", &prj, 90, -90, tol); /* PCO: polyconic. */ nFail += projex("PCO", &prj, 90, -90, tol); /* TSC: tangential spherical cube. */ nFail += projex("TSC", &prj, 90, -90, tol); /* CSC: COBE quadrilateralized spherical cube. */ nFail += projex("CSC", &prj, 90, -90, 4.0e-2); /* QSC: quadrilateralized spherical cube. */ nFail += projex("QSC", &prj, 90, -90, tol); /* HPX: HEALPix projection. */ prj.pv[1] = 4.0; prj.pv[2] = 3.0; nFail += projex("HPX", &prj, 90, -90, tol); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } /*---------------------------------------------------------------------------- * projex() exercises the spherical projection routines. * * Given: * pcode[4] char Projection code. * north int Northern cutoff latitude, degrees. * south int Southern cutoff latitude, degrees. * tol double Reporting tolerance, degrees. * * Given and returned: * prj prjprm* Projection parameters. * * Function return value: * int Number of results exceeding reporting tolerance. *---------------------------------------------------------------------------*/ int projex( char pcode[4], struct prjprm *prj, int north, int south, double tol) { int lat, lng, nFail = 0, stat1[361], stat2[361], status; register int j; double dlat, dlatmx, dlng, dlngmx, dr, drmax; double lat1, lat2[361], lng1[361], lng2[361]; double r, theta; double x[361], x1[361], x2[361], y[361], y1[361], y2[361]; strcpy(prj->code, pcode); /* Uncomment the next line to test alternative initializations of */ /* projection parameters. */ /* prj->r0 = R2D; */ printf("Testing %s; latitudes%3d to%4d, reporting tolerance%8.1e deg.\n", prj->code, north, south, tol); dlngmx = 0.0; dlatmx = 0.0; prjset(prj); for (lat = north; lat >= south; lat--) { lat1 = (double)lat; for (j = 0, lng = -180; lng <= 180; lng++, j++) { lng1[j] = (double)lng; } if (prj->prjs2x(prj, 361, 1, 1, 1, lng1, &lat1, x, y, stat1) == 1) { printf(" %3s(S2X) ERROR 1: %s\n", pcode, prj_errmsg[1]); continue; } if (prj->prjx2s(prj, 361, 0, 1, 1, x, y, lng2, lat2, stat2) == 1) { printf(" %3s(X2S) ERROR 1: %s\n", pcode, prj_errmsg[1]); continue; } for (j = 0; j < 361; j++) { if (stat1[j]) continue; if (stat2[j]) { printf(" %3s(X2S): lng1 =%20.15f lat1 =%20.15f\n", pcode, lng1[j], lat1); printf(" x =%20.15f y =%20.15f ERROR%3d\n", x[j], y[j], stat2[j]); continue; } dlng = fabs(lng2[j] - lng1[j]); if (dlng > 180.0) dlng = fabs(dlng-360.0); if (abs(lat) != 90 && dlng > dlngmx) dlngmx = dlng; dlat = fabs(lat2[j] - lat1); if (dlat > dlatmx) dlatmx = dlat; if (dlat > tol) { nFail++; printf(" %3s: lng1 =%20.15f lat1 =%20.15f\n", pcode, lng1[j], lat1); printf(" x =%20.15f y =%20.15f\n", x[j], y[j]); printf(" lng2 =%20.15f lat2 =%20.15f\n", lng2[j], lat2[j]); } else if (abs(lat) != 90) { if (dlng > tol) { nFail++; printf(" %3s: lng1 =%20.15f lat1 =%20.15f\n", pcode, lng1[j], lat1); printf(" x =%20.15f y =%20.15f\n", x[j], y[j]); printf(" lng2 =%20.15f lat2 =%20.15f\n", lng2[j], lat2[j]); } } } } printf(" Maximum residual (sky): lng%8.1e lat%8.1e\n", dlngmx, dlatmx); /* Test closure at a point close to the reference point. */ r = 1.0; theta = -180.0; drmax = 0.0; for (j = 1; j <= 12; j++) { x1[0] = r*cosd(theta); y1[0] = r*sind(theta); if ((status = prj->prjx2s(prj, 1, 1, 1, 1, x1, y1, lng1, &lat1, stat2))) { printf(" %3s(X2S): x1 =%20.15f y1 =%20.15f ERROR%3d\n", pcode, x1[0], y1[0], status); } else if ((status = prj->prjs2x(prj, 1, 1, 1, 1, lng1, &lat1, x2, y2, stat1))) { printf(" %3s(S2X): x1 =%20.15f y1 =%20.15f\n", pcode, x1[0], y1[0]); printf(" lng =%20.15f lat =%20.15f ERROR%3d\n", lng1[0], lat1, status); } else { dr = sqrt((x2[0]-x1[0])*(x2[0]-x1[0]) + (y2[0]-y1[0])*(y2[0]-y1[0])); if (dr > drmax) drmax = dr; if (dr > tol) { nFail++; printf(" %3s: x1 =%20.15f y1 =%20.15f\n", pcode, x1[0], y1[0]); printf(" lng =%20.15f lat =%20.15f\n", lng1[0], lat1); printf(" x2 =%20.15f y2 =%20.15f\n", x2[0], y2[0]); } } r /= 10.0; theta += 15.0; } printf(" Maximum residual (ref): dR%8.1e\n", drmax); prjini(prj); return nFail; } pywcs-1.12/wcslib/C/test/tprj2.c0000644001153600020070000002654312310355625020510 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tprj2.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tproj2 tests projection routines by plotting test graticules using PGPLOT. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include int main() { void prjplt(); int status; char text[80], text1[80], text2[80]; struct prjprm prj; printf("Testing WCSLIB spherical projection routines (tprj2.c)\n" "------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of prj status return values:\n"); for (status = 1; status <= 4; status++) { printf("%4d: %s.\n", status, prj_errmsg[status]); } printf("\n"); /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); /* Define pen colours. */ cpgscr(0, 0.00f, 0.00f, 0.00f); cpgscr(1, 1.00f, 1.00f, 0.00f); cpgscr(2, 1.00f, 1.00f, 1.00f); cpgscr(3, 0.50f, 0.50f, 0.80f); cpgscr(4, 0.80f, 0.50f, 0.50f); cpgscr(5, 0.80f, 0.80f, 0.80f); cpgscr(6, 0.50f, 0.50f, 0.80f); cpgscr(7, 0.80f, 0.50f, 0.50f); cpgscr(8, 0.30f, 0.50f, 0.30f); strcpy(text1, "\n%s projection\n"); strcpy(text2, "\n%s projection\nParameters:"); prjini(&prj); /* AZP: zenithal/azimuthal perspective. */ prj.pv[1] = 2.0; prj.pv[2] = 30.0; printf(text2, "Zenithal/azimuthal perspective"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("AZP", 90, -90, &prj); /* SZP: slant zenithal perspective. */ prj.pv[1] = 2.0; prj.pv[2] = 210.0; prj.pv[3] = 60.0; printf(text2, "Slant zenithal perspective"); printf("%12.5f%12.5f%12.5f\n", prj.pv[1], prj.pv[2], prj.pv[3]); prjplt("SZP", 90, -90, &prj); /* TAN: gnomonic. */ printf(text1, "Gnomonic"); prjplt("TAN", 90, 5, &prj); /* STG: stereographic. */ printf(text1, "Stereographic"); prjplt("STG", 90, -85, &prj); /* SIN: orthographic. */ prj.pv[1] = -0.3; prj.pv[2] = 0.5; printf(text2, "Orthographic/synthesis"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("SIN", 90, -90, &prj); /* ARC: zenithal/azimuthal equidistant. */ printf(text1, "Zenithal/azimuthal equidistant"); prjplt("ARC", 90, -90, &prj); /* ZPN: zenithal/azimuthal polynomial. */ prj.pv[0] = 0.05000; prj.pv[1] = 0.95000; prj.pv[2] = -0.02500; prj.pv[3] = -0.15833; prj.pv[4] = 0.00208; prj.pv[5] = 0.00792; prj.pv[6] = -0.00007; prj.pv[7] = -0.00019; prj.pv[8] = 0.00000; prj.pv[9] = 0.00000; printf(text2, "Zenithal/azimuthal polynomial"); printf("%12.5f%12.5f%12.5f%12.5f%12.5f\n", prj.pv[0], prj.pv[1], prj.pv[2], prj.pv[3], prj.pv[4]); printf(" %12.5f%12.5f%12.5f%12.5f%12.5f\n", prj.pv[5], prj.pv[6], prj.pv[7], prj.pv[8], prj.pv[9]); prjplt("ZPN", 90, 10, &prj); /* ZEA: zenithal/azimuthal equal area. */ printf(text1, "Zenithal/azimuthal equal area"); prjplt("ZEA", 90, -90, &prj); /* AIR: Airy's zenithal projection. */ prj.pv[1] = 45.0; printf(text2, "Airy's zenithal"); printf("%12.5f\n", prj.pv[1]); prjplt("AIR", 90, -85, &prj); /* CYP: cylindrical perspective. */ prj.pv[1] = 3.0; prj.pv[2] = 0.8; printf(text2, "Cylindrical perspective"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("CYP", 90, -90, &prj); /* CEA: cylindrical equal area. */ prj.pv[1] = 0.75; printf(text2, "Cylindrical equal area"); printf("%12.5f\n", prj.pv[1]); prjplt("CEA", 90, -90, &prj); /* CAR: plate carree. */ printf(text1, "Plate carree"); prjplt("CAR", 90, -90, &prj); /* MER: Mercator's. */ printf(text1, "Mercator's"); prjplt("MER", 85, -85, &prj); /* SFL: Sanson-Flamsteed. */ printf(text1, "Sanson-Flamsteed (global sinusoid)"); prjplt("SFL", 90, -90, &prj); /* PAR: parabolic. */ printf(text1, "Parabolic"); prjplt("PAR", 90, -90, &prj); /* MOL: Mollweide's projection. */ printf(text1, "Mollweide's"); prjplt("MOL", 90, -90, &prj); /* AIT: Hammer-Aitoff. */ printf(text1, "Hammer-Aitoff"); prjplt("AIT", 90, -90, &prj); /* COP: conic perspective. */ prj.pv[1] = 60.0; prj.pv[2] = 15.0; printf(text2, "Conic perspective"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("COP", 90, -25, &prj); /* COE: conic equal area. */ prj.pv[1] = 60.0; prj.pv[2] = -15.0; printf(text2, "Conic equal area"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("COE", 90, -90, &prj); /* COD: conic equidistant. */ prj.pv[1] = -60.0; prj.pv[2] = 15.0; printf(text2, "Conic equidistant"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("COD", 90, -90, &prj); /* COO: conic orthomorphic. */ prj.pv[1] = -60.0; prj.pv[2] = -15.0; printf(text2, "Conic orthomorphic"); printf("%12.5f%12.5f\n", prj.pv[1], prj.pv[2]); prjplt("COO", 85, -90, &prj); /* BON: Bonne's projection. */ prj.pv[1] = 30.0; printf(text2, "Bonne's"); printf("%12.5f\n", prj.pv[1]); prjplt("BON", 90, -90, &prj); /* PCO: polyconic. */ printf(text1, "Polyconic"); prjplt("PCO", 90, -90, &prj); /* TSC: tangential spherical cube. */ printf(text1, "Tangential spherical cube"); prjplt("TSC", 90, -90, &prj); /* CSC: COBE quadrilateralized spherical cube. */ printf(text1, "COBE quadrilateralized spherical cube"); prjplt("CSC", 90, -90, &prj); /* QSC: quadrilateralized spherical cube. */ printf(text1, "Quadrilateralized spherical cube"); prjplt("QSC", 90, -90, &prj); /* HPX: HEALPix projection. */ prj.pv[1] = 4.0; prj.pv[2] = 3.0; printf(text1, "HEALPix"); prjplt("HPX", 90, -90, &prj); cpgask(0); cpgend(); return 0; } /*---------------------------------------------------------------------------- * PRJPLT draws a 15 degree coordinate graticule. * * Given: * pcode[4] char Projection mnemonic. * north int Northern cutoff latitude, degrees. * south int Southern cutoff latitude, degrees. * * Given and returned: * prj prjprm* Projection parameters. *---------------------------------------------------------------------------*/ void prjplt(pcode, north, south, prj) char pcode[4]; int north, south; struct prjprm *prj; { char text[80]; int ci, h, ilat, ilng, interrupted, len, stat[361]; register int j, k; float hx, hy, sx, sy, xr[512], yr[512]; double lat[361], lng[361], x[361], y[361]; strcpy(prj->code, pcode); printf("Plotting %s; latitudes%3d to%4d.\n", prj->code, north, south); cpgask(0); prjset(prj); if (prj->category == QUADCUBE) { /* Draw the perimeter of the quadcube projection. */ cpgenv(-335.0f, 65.0f, -200.0f, 200.0f, 1, -2); cpgsci(2); sprintf(text,"%s - 15 degree graticule", pcode); cpgtext(-340.0f, -220.0f, text); cpgsci(8); xr[0] = 45.0 + prj->x0; yr[0] = 45.0 - prj->y0; xr[1] = 45.0 + prj->x0; yr[1] = 3.0*45.0 - prj->y0; xr[2] = -45.0 + prj->x0; yr[2] = 3.0*45.0 - prj->y0; xr[3] = -45.0 + prj->x0; yr[3] = -3.0*45.0 - prj->y0; xr[4] = 45.0 + prj->x0; yr[4] = -3.0*45.0 - prj->y0; xr[5] = 45.0 + prj->x0; yr[5] = 45.0 - prj->y0; xr[6] = -7.0*45.0 + prj->x0; yr[6] = 45.0 - prj->y0; xr[7] = -7.0*45.0 + prj->x0; yr[7] = -45.0 - prj->y0; xr[8] = 45.0 + prj->x0; yr[8] = -45.0 - prj->y0; cpgline(9, xr, yr); } else { cpgenv(-200.0f, 200.0f, -200.0f, 200.0f, 1, -2); cpgsci(2); sprintf(text,"%s - 15 degree graticule", pcode); cpgtext(-240.0f, -220.0f, text); if (prj->category == HEALPIX) { /* Draw the perimeter of the HEALPix projection. */ cpgsci(8); h = (int)(prj->pv[1] + 0.5); sx = 180.0f / h; sy = sx * (int)(prj->pv[2] + 1.5) / 2.0f; hx = 180.0f + prj->x0; hy = sy - sx - prj->y0; cpgmove(hx, hy); for (j = 0; j < h; j++) { hx -= sx; hy += sx; cpgdraw(hx, hy); hx -= sx; hy -= sx; cpgdraw(hx, hy); } hx = 180.0f + prj->x0; hy = -sy + sx - prj->y0; k = ((int)prj->pv[2])%2 ? 1 : -1; if (k == -1) hy -= sx; cpgmove(hx, hy); for (j = 0; j < h; j++) { hx -= sx; hy -= k*sx; cpgdraw(hx, hy); hx -= sx; hy += k*sx; cpgdraw(hx, hy); } } } ci = 1; for (ilng = -180; ilng <= 180; ilng+=15) { if (++ci > 7) ci = 2; lng[0] = (double)ilng; cpgsci(ilng?ci:1); len = north - south + 1; for (j = 0, ilat = north; ilat >= south; ilat--, j++) { lat[j] = (double)ilat; } prj->prjs2x(prj, 1, len, 1, 1, lng, lat, x, y, stat); k = 0; for (j = 0; j < len; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } if (prj->category == QUADCUBE && j > 0) { if (fabs(x[j] - x[j-1]) > 2.0 || fabs(y[j] - y[j-1]) > 5.0) { if (k > 1) cpgline(k, xr, yr); k = 0; } } else if (prj->category == HEALPIX && ilng == 180) { if (x[j] > 180.0) { continue; } } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); } ci = 1; interrupted = (prj->category == QUADCUBE || prj->category == HEALPIX); for (ilat = -90; ilat <= 90; ilat += 15) { if (++ci > 7) ci = 2; if (ilat > north) continue; if (ilat < south) continue; lat[0] = (double)ilat; cpgsci(ilat?ci:1); for (j = 0, ilng = -180; ilng <= 180; ilng++, j++) { lng[j] = (double)ilng; } prj->prjs2x(prj, 361, 1, 1, 1, lng, lat, x, y, stat); k = 0; for (j = 0; j <= 360; j++) { if (stat[j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } if (interrupted && j > 0) { if (fabs(x[j] - x[j-1]) > 2.0 || fabs(y[j] - y[j-1]) > 5.0) { if (k > 1) cpgline(k, xr, yr); k = 0; } } xr[k] = -x[j]; yr[k] = y[j]; k++; } cpgline(k, xr, yr); } cpgsci(1); xr[0] = 0.0f; yr[0] = 0.0f; cpgpt(1, xr, yr, 21); cpgask(1); cpgpage(); prjini(prj); return; } pywcs-1.12/wcslib/C/test/tspc.c0000644001153600020070000003044512310355625020414 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tspc.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tspc tests the spectral transformation driver routines for closure. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include #define NSPEC 10001 const double tol = 1.0e-11; const double C = 2.99792458e8; int closure(const char[9], double, double, int, double, double, double); /* KPNO MARS spectrograph grism parameters. */ double mars[7] = {4.5e5, 1.0, 27.0, 1.765, -1.077e6, 3.0, 5.0}; int main() { char text[80]; int naxisj, nFail = 0, status; double cdeltX, crpixj, crvalX, restfrq, restwav, x1, x2; printf( "Testing closure of WCSLIB spectral transformation routines (tspc.c)\n" "-------------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of spc status return values:\n"); for (status = 1; status <= 4; status++) { printf("%4d: %s.\n", status, spc_errmsg[status]); } /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); naxisj = NSPEC; crpixj = naxisj/2 + 1; restfrq = 1420.40595e6; restwav = C/restfrq; x1 = 1.0e9; x2 = 2.0e9; cdeltX = (x2 - x1)/(naxisj - 1); crvalX = x1 + (crpixj - 1.0)*cdeltX; printf("\nLinear frequency axis, span: %.1f to %.1f (GHz), step: %.3f " "(kHz)\n---------------------------------------------------------" "-----------------\n", x1*1e-9, x2*1e-9, cdeltX*1e-3); nFail += closure("WAVE-F2W", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VOPT-F2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ZOPT-F2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AWAV-F2A", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VELO-F2V", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("BETA-F2V", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); restwav = 700.0e-9; restfrq = C/restwav; x1 = 300.0e-9; x2 = 900.0e-9; cdeltX = (x2 - x1)/(naxisj - 1); crvalX = x1 + (crpixj - 1.0)*cdeltX; printf("\nLinear vacuum wavelength axis, span: %.0f to %.0f (nm), " "step: %f (nm)\n---------------------------------------------" "-----------------------------\n", x1*1e9, x2*1e9, cdeltX*1e9); nFail += closure("FREQ-W2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AFRQ-W2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ENER-W2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVN-W2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VRAD-W2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AWAV-W2A", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VELO-W2V", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("BETA-W2V", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); printf("\nLinear air wavelength axis, span: %.0f to %.0f (nm), " "step: %f (nm)\n------------------------------------------" "--------------------------------\n", x1*1e9, x2*1e9, cdeltX*1e9); nFail += closure("FREQ-A2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AFRQ-A2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ENER-A2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVN-A2F", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VRAD-A2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVE-A2W", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VOPT-A2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ZOPT-A2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VELO-A2V", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("BETA-A2V", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); restfrq = 1420.40595e6; restwav = C/restfrq; x1 = -0.96*C; x2 = 0.96*C; cdeltX = (x2 - x1)/(naxisj - 1); crvalX = x1 + (crpixj - 1.0)*cdeltX; printf("\nLinear velocity axis, span: %.0f to %.0f m/s, step: %.0f " "(m/s)\n------------------------------------------------------" "--------------------\n", x1, x2, cdeltX); nFail += closure("FREQ-V2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AFRQ-V2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ENER-V2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVN-V2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VRAD-V2F", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVE-V2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VOPT-V2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ZOPT-V2W", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AWAV-V2A", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); restwav = 650.0e-9; restfrq = C/restwav; x1 = 300e-9; x2 = 1000e-9; cdeltX = (x2 - x1)/(naxisj - 1); crvalX = x1 + (crpixj - 1.0)*cdeltX; printf("\nVacuum wavelength grism axis, span: %.0f to %.0f (nm), " "step: %f (nm)\n--------------------------------------------" "------------------------------\n", x1*1e9, x2*1e9, cdeltX*1e9); nFail += closure("FREQ-GRI", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AFRQ-GRI", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ENER-GRI", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVN-GRI", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VRAD-GRI", restfrq, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("WAVE-GRI", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VOPT-GRI", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("ZOPT-GRI", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("AWAV-GRI", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VELO-GRI", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); nFail += closure("BETA-GRI", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); /* Reproduce Fig. 5 of Paper III. */ naxisj = 1700; crpixj = 719.8; crvalX = 7245.2e-10; cdeltX = 2.956e-10; restwav = 8500.0e-10; restfrq = C/restwav; x1 = crvalX + (1 - crpixj)*cdeltX; x2 = crvalX + (naxisj - crpixj)*cdeltX; mars[5] = 0.0; mars[6] = 0.0; printf("\nAir wavelength grism axis, span: %.0f to %.0f (nm), " "step: %f (nm)\n--------------------------------------------" "------------------------------\n", x1*1e9, x2*1e9, cdeltX*1e9); nFail += closure("AWAV-GRA", 0.0, 0.0, naxisj, crpixj, cdeltX, crvalX); nFail += closure("VELO-GRA", 0.0, restwav, naxisj, crpixj, cdeltX, crvalX); cpgask(0); cpgend(); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } /*--------------------------------------------------------------------------*/ int closure ( const char ctypeS[9], double restfrq, double restwav, int naxisj, double crpixj, double cdeltX, double crvalX) { char ptype, sname[32], title[80], units[8], xtype, ylab[80]; int nFail = 0, restreq, stat1[NSPEC], stat2[NSPEC], status; register int j; float tmp, x[NSPEC], xmin, xmax, y[NSPEC], ymax, ymin; double cdeltS, clos[NSPEC], crvalS, dSdX, resid, residmax, spec1[NSPEC], spec2[NSPEC]; struct spcprm spc; /* Get keyvalues for the required spectral axis type. */ if ((status = spcxps(ctypeS, crvalX, restfrq, restwav, &ptype, &xtype, &restreq, &crvalS, &dSdX))) { printf("ERROR %d from spcxps() for %s.\n", status, ctypeS); return 1; } cdeltS = cdeltX * dSdX; spcini(&spc); if (ctypeS[5] == 'G') { /* KPNO MARS spectrograph grism parameters. */ spc.pv[0] = mars[0]; spc.pv[1] = mars[1]; spc.pv[2] = mars[2]; spc.pv[3] = mars[3]; spc.pv[4] = mars[4]; spc.pv[5] = mars[5]; spc.pv[6] = mars[6]; } /* Construct the axis. */ for (j = 0; j < naxisj; j++) { spec1[j] = (j+1 - crpixj)*cdeltS; } printf("%4s (CRVALk+w) range: %13.6e to %13.6e, step: %13.6e\n", ctypeS, crvalS+spec1[0], crvalS+spec1[naxisj-1], cdeltS); /* Initialize. */ spc.flag = 0; spc.crval = crvalS; spc.restfrq = restfrq; spc.restwav = restwav; strncpy(spc.type, ctypeS, 4); spc.type[4] = '\0'; strcpy(spc.code, ctypeS+5); /* Convert the first to the second. */ if ((status = spcx2s(&spc, naxisj, 1, 1, spec1, spec2, stat1))) { printf("spcx2s ERROR %d: %s.\n", status, spc_errmsg[status]); } /* Convert the second back to the first. */ if ((status = spcs2x(&spc, naxisj, 1, 1, spec2, clos, stat2))) { printf("spcs2x ERROR %d: %s.\n", status, spc_errmsg[status]); } residmax = 0.0; /* Test closure. */ for (j = 0; j < naxisj; j++) { if (stat1[j]) { printf("%s: w =%20.12e -> %s = ???, stat = %d\n", ctypeS, spec1[j], spc.type, stat1[j]); continue; } if (stat2[j]) { printf("%s: w =%20.12e -> %s =%20.12e -> w = ???, stat = %d\n", ctypeS, spec1[j], spc.type, spec2[j], stat2[j]); continue; } resid = fabs((clos[j] - spec1[j])/cdeltS); if (resid > residmax) residmax = resid; if (resid > tol) { nFail++; printf("%s: w =%20.12e -> %s =%20.12e ->\n w =%20.12e, " "resid =%20.12e\n", ctypeS, spec1[j], spc.type, spec2[j], clos[j], resid); } } printf("%s: Maximum closure residual = %.1e pixel.\n", ctypeS, residmax); /* Draw graph. */ cpgbbuf(); cpgeras(); xmin = (float)(crvalS + spec1[0]); xmax = (float)(crvalS + spec1[naxisj-1]); ymin = (float)(spec2[0]) - xmin; ymax = ymin; for (j = 0; j < naxisj; j++) { x[j] = (float)(j+1); y[j] = (float)(spec2[j] - (crvalS + spec1[j])); if (y[j] > ymax) ymax = y[j]; if (y[j] < ymin) ymin = y[j]; } j = (int)crpixj + 1; if (y[j] < 0.0) { tmp = ymin; ymin = ymax; ymax = tmp; } cpgask(0); cpgenv(1.0f, (float)naxisj, ymin, ymax, 0, -1); cpgsci(1); cpgbox("ABNTS", 0.0f, 0, "BNTS", 0.0f, 0); spctyp(ctypeS, 0x0, 0x0, sname, units, 0x0, 0x0, 0x0); sprintf(ylab, "%s - correction [%s]", sname, units); sprintf(title, "%s: CRVALk + w [%s]", ctypeS, units); cpglab("Pixel coordinate", ylab, title); cpgaxis("N", 0.0f, ymax, (float)naxisj, ymax, xmin, xmax, 0.0f, 0, -0.5f, 0.0f, 0.5f, -0.5f, 0.0f); cpgaxis("N", (float)naxisj, ymin, (float)naxisj, ymax, (float)(ymin/cdeltS), (float)(ymax/cdeltS), 0.0f, 0, 0.5f, 0.0f, 0.5f, 0.1f, 0.0f); cpgmtxt("R", 2.2f, 0.5f, 0.5f, "Pixel offset"); cpgline(naxisj, x, y); cpgsci(7); cpgpt1((float)crpixj, 0.0f, 24); cpgebuf(); printf("Type for next page: "); (void)getchar(); printf("\n"); return nFail; } pywcs-1.12/wcslib/C/test/tsph.c0000644001153600020070000001063712310355626020423 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tsph.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tsph tests the spherical coordinate transformation routines for closure. * *---------------------------------------------------------------------------*/ #include #include #include #include #include int main() { int j, lat, lng, nFail = 0; double coslat, dlat, dlatmx, dlng, dlngmx, lng1[361], lng2[361], eul[5], lat1, lat2[361], phi[361], theta[361], zeta; const double tol = 1.0e-12; printf( "Testing closure of WCSLIB coordinate transformation routines (tsph.c)\n" "---------------------------------------------------------------------\n"); /* Set reference angles. */ eul[0] = 90.0; eul[1] = 30.0; eul[2] = -90.0; printf("\n%s\n%s%10.4f%10.4f%10.4f\n", "Celestial longitude and latitude of the native pole, and native", "longitude of the celestial pole (degrees):", eul[0], eul[1], eul[2]); eul[3] = cosd(eul[1]); eul[4] = sind(eul[1]); printf ("Reporting tolerance:%8.1e degrees of arc.\n", tol); dlngmx = 0.0; dlatmx = 0.0; for (lat = 90; lat >= -90; lat--) { lat1 = (double)lat; coslat = cosd(lat1); for (j = 0, lng = -180; lng <= 180; lng++, j++) { lng1[j] = (double)lng; } sphs2x(eul, 361, 1, 1, 1, lng1, &lat1, phi, theta); sphx2s(eul, 361, 0, 1, 1, phi, theta, lng2, lat2); for (j = 0; j <= 360; j++) { dlng = fabs(lng2[j] - lng1[j]); if (dlng > 180.0) dlng = fabs(dlng-360.0); dlng *= coslat; dlat = fabs(lat2[j]-lat1); if (dlng > dlngmx) dlngmx = dlng; if (dlat > dlatmx) dlatmx = dlat; if (dlng > tol || dlat > tol) { nFail++; printf("Unclosed: lng1 =%20.15f lat1 =%20.15f\n", lng1[j], lat1); printf(" phi =%20.15f theta =%20.15f\n", phi[j], theta[j]); printf(" lng2 =%20.15f lat2 =%20.15f\n", lng2[j], lat2[j]); } } } /* Test closure at points close to the pole. */ for (j = -1; j <= 1; j += 2) { zeta = 1.0; lng1[0] = -180.0; for (lat = 0; lat < 12; lat++) { lat1 = (double)j*(90.0 - zeta); sphs2x(eul, 1, 1, 1, 1, lng1, &lat1, phi, theta); sphx2s(eul, 1, 1, 1, 1, phi, theta, lng2, lat2); dlng = fabs(lng2[0] - lng1[0]); if (dlng > 180.0) dlng = fabs(dlng-360.0); dlng *= coslat; dlat = fabs(lat2[0]-lat1); if (dlng > dlngmx) dlngmx = dlng; if (dlat > dlatmx) dlatmx = dlat; if (dlng > tol || dlat > tol) { nFail++; printf("Unclosed: lng1 =%20.15f lat1 =%20.15f\n", lng1[0], lat1); printf(" phi =%20.15f theta =%20.15f\n", phi[0], theta[0]); printf(" lng2 =%20.15f lat2 =%20.15f\n", lng2[0], lat2[0]); } zeta /= 10.0; lng1[0] += 30.0; } } printf("\nsphs2x/sphx2s: Maximum closure residual = %.1e (lng), %.1e (lat) " "deg.\n", dlngmx, dlatmx); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } pywcs-1.12/wcslib/C/test/tsphdpa.c0000644001153600020070000000411412310355625021100 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tsphdpa.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tsphdpa tests sphdpa(). * *---------------------------------------------------------------------------*/ #include #include "sph.h" int main() { double dist, lat, lat0, lng, lng0, pa; printf("\nEnter reference (lng,lat): "); scanf("%lf%*[ , ]%lf", &lng0, &lat0); while (1) { printf("\nEnter field (lng,lat): "); scanf("%lf%*[ , ]%lf", &lng, &lat); sphdpa(1, lng0, lat0, &lng, &lat, &dist, &pa); printf("(%.4f,%.4f) - (%.4f,%.4f) -> (%.4f,%.4f) (dist,pa)\n", lng0, lat0, lng, lat, dist, pa); sphpad(1, lng0, lat0, &dist, &pa, &lng, &lat); printf("(%.4f,%.4f) + (%.4f,%.4f) -> (%.4f,%.4f) (lng,lat)\n", lng0, lat0, dist, pa, lng, lat); } return 0; } pywcs-1.12/wcslib/C/test/tspx.c0000644001153600020070000002207712310355625020443 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tspx.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tspx tests the spectral transformation routines for closure. * *---------------------------------------------------------------------------*/ #include #include #include #define NSPEC 9991 const double C = 2.99792458e8; const double tol = 1.0e-9; int closure(const char *from, const char *to, double parm, int (*fwd)(SPX_ARGS), int (*rev)(SPX_ARGS), const double spec1[], double spec2[]); int main() { int nFail = 0, stat[NSPEC], status; double restfrq, restwav, step; double awav[NSPEC], freq[NSPEC], spc1[NSPEC], spc2[NSPEC], velo[NSPEC], wave[NSPEC]; struct spxprm spx; register int j, k; printf( "Testing closure of WCSLIB spectral transformation routines (tspx.c)\n" "-------------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of spx status return values:\n"); for (status = 1; status <= 4; status++) { printf("%4d: %s.\n", status, spx_errmsg[status]); } restfrq = 1420.40595e6; restwav = C/restfrq; /* Exercise specx(). */ printf("\nTesting spectral cross-conversions (specx).\n\n"); if ((status = specx("VELO", 4.3e5, restfrq, restwav, &spx))) { printf("specx ERROR %d: %s.\n", status, spx_errmsg[status]); return 1; } printf(" restfrq:%20.12e\n", spx.restfrq); printf(" restwav:%20.12e\n", spx.restwav); printf(" wavetype:%3d\n", spx.wavetype); printf(" velotype:%3d\n", spx.velotype); printf("\n"); printf(" freq:%20.12e\n", spx.freq); printf(" afrq:%20.12e\n", spx.afrq); printf(" ener:%20.12e\n", spx.ener); printf(" wavn:%20.12e\n", spx.wavn); printf(" vrad:%20.12e\n", spx.vrad); printf(" wave:%20.12e\n", spx.wave); printf(" vopt:%20.12e\n", spx.vopt); printf(" zopt:%20.12e\n", spx.zopt); printf(" awav:%20.12e\n", spx.awav); printf(" velo:%20.12e\n", spx.velo); printf(" beta:%20.12e\n", spx.beta); printf("\n"); printf("dfreq/dafrq:%20.12e\n", spx.dfreqafrq); printf("dafrq/dfreq:%20.12e\n", spx.dafrqfreq); printf("dfreq/dener:%20.12e\n", spx.dfreqener); printf("dener/dfreq:%20.12e\n", spx.denerfreq); printf("dfreq/dwavn:%20.12e\n", spx.dfreqwavn); printf("dwavn/dfreq:%20.12e\n", spx.dwavnfreq); printf("dfreq/dvrad:%20.12e\n", spx.dfreqvrad); printf("dvrad/dfreq:%20.12e\n", spx.dvradfreq); printf("dfreq/dwave:%20.12e\n", spx.dfreqwave); printf("dwave/dfreq:%20.12e\n", spx.dwavefreq); printf("dfreq/dawav:%20.12e\n", spx.dfreqawav); printf("dawav/dfreq:%20.12e\n", spx.dawavfreq); printf("dfreq/dvelo:%20.12e\n", spx.dfreqvelo); printf("dvelo/dfreq:%20.12e\n", spx.dvelofreq); printf("dwave/dvopt:%20.12e\n", spx.dwavevopt); printf("dvopt/dwave:%20.12e\n", spx.dvoptwave); printf("dwave/dzopt:%20.12e\n", spx.dwavezopt); printf("dzopt/dwave:%20.12e\n", spx.dzoptwave); printf("dwave/dawav:%20.12e\n", spx.dwaveawav); printf("dawav/dwave:%20.12e\n", spx.dawavwave); printf("dwave/dvelo:%20.12e\n", spx.dwavevelo); printf("dvelo/dwave:%20.12e\n", spx.dvelowave); printf("dawav/dvelo:%20.12e\n", spx.dawavvelo); printf("dvelo/dawav:%20.12e\n", spx.dveloawav); printf("dvelo/dbeta:%20.12e\n", spx.dvelobeta); printf("dbeta/dvelo:%20.12e\n", spx.dbetavelo); printf("\n"); /* Construct a linear velocity spectrum. */ step = (2.0*C/NSPEC) / 2.0; for (j = 0, k = -NSPEC; j < NSPEC; j++, k += 2) { velo[j] = (k+1)*step; } printf("\nVelocity range: %.3f to %.3f km/s, step: %.3f km/s\n", velo[0]*1e-3, velo[NSPEC-1]*1e-3, (velo[1] - velo[0])*1e-3); /* Convert it to frequency. */ velofreq(restfrq, NSPEC, 1, 1, velo, freq, stat); /* Test closure of all two-way combinations. */ nFail += closure("freq", "afrq", 0.0, freqafrq, afrqfreq, freq, spc1); nFail += closure("afrq", "freq", 0.0, afrqfreq, freqafrq, spc1, spc2); nFail += closure("freq", "ener", 0.0, freqener, enerfreq, freq, spc1); nFail += closure("ener", "freq", 0.0, enerfreq, freqener, spc1, spc2); nFail += closure("freq", "wavn", 0.0, freqwavn, wavnfreq, freq, spc1); nFail += closure("wavn", "freq", 0.0, wavnfreq, freqwavn, spc1, spc2); nFail += closure("freq", "vrad", restfrq, freqvrad, vradfreq, freq, spc1); nFail += closure("vrad", "freq", restfrq, vradfreq, freqvrad, spc1, spc2); nFail += closure("freq", "wave", 0.0, freqwave, wavefreq, freq, wave); nFail += closure("wave", "freq", 0.0, wavefreq, freqwave, wave, spc2); nFail += closure("freq", "awav", 0.0, freqawav, awavfreq, freq, awav); nFail += closure("awav", "freq", 0.0, awavfreq, freqawav, awav, spc2); nFail += closure("freq", "velo", restfrq, freqvelo, velofreq, freq, velo); nFail += closure("velo", "freq", restfrq, velofreq, freqvelo, velo, spc2); nFail += closure("wave", "vopt", restwav, wavevopt, voptwave, wave, spc1); nFail += closure("vopt", "wave", restwav, voptwave, wavevopt, spc1, spc2); nFail += closure("wave", "zopt", restwav, wavezopt, zoptwave, wave, spc1); nFail += closure("zopt", "wave", restwav, zoptwave, wavezopt, spc1, spc2); nFail += closure("wave", "awav", 0.0, waveawav, awavwave, wave, spc1); nFail += closure("awav", "wave", 0.0, awavwave, waveawav, spc1, spc2); nFail += closure("wave", "velo", restwav, wavevelo, velowave, wave, spc1); nFail += closure("velo", "wave", restwav, velowave, wavevelo, spc1, spc2); nFail += closure("awav", "velo", restwav, awavvelo, veloawav, awav, spc1); nFail += closure("velo", "awav", restwav, veloawav, awavvelo, spc1, spc2); nFail += closure("velo", "beta", 0.0, velobeta, betavelo, velo, spc1); nFail += closure("beta", "velo", 0.0, betavelo, velobeta, spc1, spc2); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } /*--------------------------------------------------------------------------*/ int closure ( const char *from, const char *to, double parm, int (*fwd)(SPX_ARGS), int (*rev)(SPX_ARGS), const double spec1[], double spec2[]) { static char skip = '\0'; int nFail = 0, stat1[NSPEC], stat2[NSPEC], status; register int j; double clos[NSPEC], resid, residmax; /* Convert the first to the second. */ if ((status = fwd(parm, NSPEC, 1, 1, spec1, spec2, stat1))) { printf("%s%s ERROR %d: %s.\n", from, to, status, spx_errmsg[status]); } /* Convert the second back to the first. */ if ((status = rev(parm, NSPEC, 1, 1, spec2, clos, stat2))) { printf("%s%s ERROR %d: %s.\n", to, from, status, spx_errmsg[status]); } residmax = 0.0; /* Test closure. */ for (j = 0; j < NSPEC; j++) { if (stat1[j]) { printf("%c%s%s: %s = %.12e -> %s = ???, stat = %d\n", skip, from, to, from, spec1[j], to, stat1[j]); skip = '\0'; continue; } if (stat2[j]) { printf("%c%s%s: %s = %.12e -> %s = %.12e -> %s = ???, stat = %d\n", skip, to, from, from, spec1[j], to, spec2[j], from, stat2[j]); skip = '\0'; continue; } if (spec1[j] == 0.0) { resid = fabs(clos[j] - spec1[j]); } else { resid = fabs((clos[j] - spec1[j])/spec1[j]); if (resid > residmax) residmax = resid; } if (resid > tol) { nFail++; printf("%c%s%s: %s = %.12e -> %s = %.12e ->\n %s = %.12e, " "resid = %.1e\n", skip, from, to, from, spec1[j], to, spec2[j], from, clos[j], resid); skip = '\0'; } } printf("%s%s: Maximum closure residual = %.1e\n", from, to, residmax); if (residmax > tol) { printf("\n"); skip = '\0'; } else { skip = '\n'; } return nFail; } pywcs-1.12/wcslib/C/test/ttab1.c0000644001153600020070000002501012310355625020446 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: ttab1.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * ttab1 tests the -TAB routines for closure. * *---------------------------------------------------------------------------*/ #include #include #include /* Reporting tolerance. */ const double tol = 1.0e-8; int main() { char nl; int i, j, K[2], K1, K2, k, k1, k2, M, m, map[2], n, nFail = 0, stat0[128], stat1[128], status, status0, status1; double crpix, crval[2], epsilon, *index[1], psi_0, psi_1, resid, residmax, s[16], world[11][11][2], xt0[16], xt1[16], x0[11][11][2], x1[11][11][2], z; struct tabprm tab; printf( "Testing closure of WCSLIB tabular coordinate routines (ttab1.c)\n" "---------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of tab status return values:\n"); for (status = 1; status <= 5; status++) { printf("%4d: %s.\n", status, tab_errmsg[status]); } printf("\nReporting tolerance %5.1G.\n", tol); /* First a 1-dimensional table without index. */ printf("\nOne-dimensional test without index:\n"); M = 1; K[0] = 10; tab.flag = -1; tab.index = index; if ((status = tabini(1, M, K, &tab))) { printf("tabini ERROR %d: %s.\n", status, tab_errmsg[status]); return 1; } tab.M = M; tab.K[0] = K[0]; tab.map[0] = 0; tab.crval[0] = 0.0; tab.index[0] = 0x0; tab.coord[0] = 101.0; tab.coord[1] = 102.0; tab.coord[2] = 104.0; tab.coord[3] = 107.0; tab.coord[4] = 111.0; tab.coord[5] = 116.0; tab.coord[6] = 122.0; tab.coord[7] = 129.0; tab.coord[8] = 137.0; tab.coord[9] = 146.0; xt0[0] = 1.0; xt0[1] = 2.0; xt0[2] = 3.0; xt0[3] = 4.0; xt0[4] = 5.0; xt0[5] = 6.0; xt0[6] = 7.0; xt0[7] = 8.0; xt0[8] = 9.0; xt0[9] = 10.0; xt0[10] = 0.5; xt0[11] = 1.1; xt0[12] = 2.5; xt0[13] = 4.7; xt0[14] = 8.125; xt0[15] = 10.5; status0 = tabx2s(&tab, 16, 1, (double *)xt0, (double *)s, stat0); status1 = tabs2x(&tab, 16, 1, (double *)s, (double *)xt1, stat1); printf(" x -> s -> x\n"); for (i = 0; i < 16; i++) { printf("%8.5f%12.5f%9.5f", xt0[i], s[i], xt1[i]); if (stat0[i] || stat1[i]) { printf(" ERROR\n"); } else { printf("\n"); } if (i == 9) printf("\n"); } nl = 1; if (status0) { if (nl) printf("\n"); printf("tabx2s ERROR %d: %s.\n", status0, tab_errmsg[status0]); nl = 0; } if (status1) { if (nl) printf("\n"); printf("tabs2x ERROR %d: %s.\n", status1, tab_errmsg[status1]); } /* Test closure. */ nl = 1; residmax = 0.0; for (i = 0; i < 16; i++) { if (stat0[i]) { printf("\n tabx2s: x = %6.1f, stat = %d\n", xt0[i], stat0[i]); nl = 1; continue; } if (stat1[i]) { printf("\n tabs2x: s = %6.1f, stat = %d\n", s[i], stat1[i]); nl = 1; continue; } resid = fabs(xt1[i] - xt0[i]); if (resid > residmax) residmax = resid; if (resid > tol) { nFail++; if (nl) printf("\n"); printf(" Closure error:\n"); printf(" x = %20.15f\n", xt0[i]); printf(" -> s = %20.15f\n", s[i]); printf(" -> x = %20.15f\n", xt1[i]); nl = 0; } } tabfree(&tab); tab.index = 0x0; /* Now the 1-dimensional table from Sect. 6.2.3 of Paper III. */ printf("\n\nOne-dimensional test with index:\n"); M = 1; K[0] = 8; tab.flag = -1; if ((status = tabini(1, M, K, &tab))) { printf("tabini ERROR %d: %s.\n", status, tab_errmsg[status]); return 1; } tab.M = M; tab.K[0] = K[0]; tab.map[0] = 0; tab.crval[0] = 0.0; tab.index[0][0] = 0.0; tab.index[0][1] = 1.0; tab.index[0][2] = 1.0; tab.index[0][3] = 2.0; tab.index[0][4] = 2.0; tab.index[0][5] = 3.0; tab.index[0][6] = 3.0; tab.index[0][7] = 4.0; tab.coord[0] = 1997.84512; tab.coord[1] = 1997.84631; tab.coord[2] = 1993.28451; tab.coord[3] = 1993.28456; tab.coord[4] = 2001.59234; tab.coord[5] = 2001.59239; tab.coord[6] = 2002.18265; tab.coord[7] = 2002.18301; epsilon = 1e-3; crpix = 0.5; xt0[0] = 0.5 + epsilon - crpix; xt0[1] = 1.0 - crpix; xt0[2] = 1.5 - epsilon - crpix; xt0[3] = 1.5 + epsilon - crpix; xt0[4] = 2.0 - crpix; xt0[5] = 2.5 - epsilon - crpix; xt0[6] = 2.5 + epsilon - crpix; xt0[7] = 3.0 - crpix; xt0[8] = 3.5 - epsilon - crpix; xt0[9] = 3.5 + epsilon - crpix; xt0[10] = 4.0 - crpix; xt0[11] = 4.5 - epsilon - crpix; status0 = tabx2s(&tab, 12, 1, (double *)xt0, (double *)s, stat0); status1 = tabs2x(&tab, 12, 1, (double *)s, (double *)xt1, stat1); printf(" x -> time -> x\n"); for (i = 0; i < 12; i++) { printf("%8.5f%12.5f%9.5f", xt0[i], s[i], xt1[i]); if (stat0[i] || stat1[i]) { printf(" ERROR\n"); } else { printf("\n"); } } nl = 1; if (status0) { if (nl) printf("\n"); printf("tabx2s ERROR %d: %s.\n", status0, tab_errmsg[status0]); nl = 0; } if (status1) { if (nl) printf("\n"); printf("tabs2x ERROR %d: %s.\n", status1, tab_errmsg[status1]); } /* Test closure. */ nl = 1; residmax = 0.0; for (i = 0; i < 12; i++) { if (stat0[i]) { printf("\n tabx2s: x = %6.1f, stat = %d\n", xt0[i], stat0[i]); nl = 1; continue; } if (stat1[i]) { printf("\n tabs2x: s = %6.1f, stat = %d\n", s[i], stat1[i]); nl = 1; continue; } resid = fabs(xt1[i] - xt0[i]); if (resid > residmax) residmax = resid; if (resid > tol) { nFail++; if (nl) printf("\n"); printf(" Closure error:\n"); printf(" x = %20.15f\n", xt0[i]); printf(" -> s = %20.15f\n", s[i]); printf(" -> x = %20.15f\n", xt1[i]); nl = 0; } } tabfree(&tab); /* Now a 2-dimensional table. */ printf("\n\nTwo-dimensional test with index:\n"); M = 2; K[0] = K1 = 32; K[1] = K2 = 16; map[0] = 0; map[1] = 1; crval[0] = 4.0; crval[1] = -1.0; tab.flag = -1; if ((status = tabini(1, M, K, &tab))) { printf("tabini ERROR %d: %s.\n", status, tab_errmsg[status]); return 1; } /* Set up the tabprm struct. */ tab.M = M; for (m = 0; m < tab.M; m++) { tab.K[m] = K[m]; tab.map[m] = map[m]; tab.crval[m] = crval[m]; /* Construct a trivial 0-relative index. */ for (k = 0; k < tab.K[m]; k++) { tab.index[m][k] = (double)k; } } /* Construct a coordinate table. */ n = 0; z = 1.0 / (double)((K1-1) * (K2-1)); for (k2 = 0; k2 < K2; k2++) { for (k1 = 0; k1 < K1; k1++) { tab.coord[n++] = 3.0*k1*k2*z; tab.coord[n++] = -1.0*(K1-k1-1)*k2*z + 0.01*k1; } } /* Construct an array of intermediate world coordinates to transform. */ for (i = 0; i < 11; i++) { for (j = 0; j < 11; j++) { /* Compute psi_m within bounds... */ psi_0 = i*(K1-1)/10.0; psi_1 = j*(K2-1)/10.0; /* ...then compute x from it. */ x0[i][j][0] = psi_0 - crval[0]; x0[i][j][1] = psi_1 - crval[1]; } } /* Transform them to and fro. */ status0 = tabx2s(&tab, 121, 2, (double *)x0, (double *)world, stat0); status1 = tabs2x(&tab, 121, 2, (double *)world, (double *)x1, stat1); /* Print the results. */ printf(" x -> s -> x \n"); n = 0; for (i = 0; i < 11; i++) { for (j = 0; j < 11; j++, n++) { /* Print every sixth one only. */ if (n%6) continue; printf("(%4.1f,%4.1f) (%4.2f,%6.3f) (%4.1f,%4.1f)", x0[i][j][0], x0[i][j][1], world[i][j][0], world[i][j][1], x1[i][j][0], x1[i][j][1]); if (stat0[n] || stat1[n]) { printf(" ERROR\n"); } else { printf("\n"); } } } nl = 1; if (status0) { if (nl) printf("\n"); printf("tabx2s ERROR %d: %s.\n", status0, tab_errmsg[status0]); nl = 0; } if (status1) { if (nl) printf("\n"); printf("tabs2x ERROR %d: %s.\n", status1, tab_errmsg[status1]); } /* Check for closure. */ n = 0; nl = 1; residmax = 0.0; for (i = 0; i < 11; i++) { for (j = 0; j < 11; j++, n++) { if (stat0[n]) { printf(" tabx2s: x = (%6.1f,%6.1f), stat = %d\n", x0[i][j][0], x0[i][j][1], stat0[n]); nl = 1; continue; } if (stat1[n]) { printf(" tabs2x: s = (%6.1f,%6.1f), stat = %d\n", world[i][j][0], world[i][j][1], stat1[n]); nl = 1; continue; } for (m = 0; m < M; m++) { resid = fabs(x1[i][j][m] - x0[i][j][m]); if (resid > residmax) residmax = resid; if (resid > tol) { nFail++; if (nl) printf("\n"); printf(" Closure error:\n"); printf(" x = (%20.15f,%20.15f)\n", x0[i][j][0], x0[i][j][1]); printf(" -> w = (%20.15f,%20.15f)\n", world[i][j][0], world[i][j][1]); printf(" -> x = (%20.15f,%20.15f)\n", x1[i][j][0], x1[i][j][1]); nl = 0; break; } } } } printf("\ntabx2s/tabs2x: Maximum closure residual = %.1e\n", residmax); tabfree(&tab); if (nFail) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail); } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); } return nFail; } pywcs-1.12/wcslib/C/test/ttab2.c0000644001153600020070000001760112310355626020457 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: ttab2.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * ttab2 tests the -TAB routines using PGPLOT for graphical display. It * demonstrates the nature of linear interpolation in 2 dimensions by * contouring the interior a single 2 x 2 interpolation element as the values * in each corner change. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include #define K1 2 #define K2 2 /* Number of subdivisions on each side of the interpolation element. */ #define NP 128 int main() { /* Set up a 2 x 2 lookup table. */ const int M = 2; const int K[] = {K1, K2}; const int map[] = {0, 1}; const double crval[] = {0.0, 0.0}; char text[80]; int i, j, k, l, l1, l2, l3, lstep, m, stat[NP*NP], status; float array[NP][NP], clev[31], v0, v1, w; const float scl = 2.0f/(NP-1); float ltm[6]; double x[NP][NP][2], world[NP][NP][2]; struct tabprm tab; printf("Testing WCSLIB coordinate lookup table routines (ttab2.c)\n" "---------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of tab status return values:\n"); for (status = 1; status <= 5; status++) { printf("%4d: %s.\n", status, tab_errmsg[status]); } printf("\n"); /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); cpgvstd(); cpgsch(0.7f); /* The viewport is slightly oversized. */ cpgwnad(-0.65f, 1.65f, -0.65f, 1.65f); for (l = 0; l <= 30; l++) { clev[l] = 0.2f*(l-10); } ltm[0] = -scl*(1.0f + (NP-1)/4.0f); ltm[1] = scl; ltm[2] = 0.0f; ltm[3] = -scl*(1.0f + (NP-1)/4.0f); ltm[4] = 0.0f; ltm[5] = scl; /* Set up the lookup table. */ tab.flag = -1; if ((status = tabini(1, M, K, &tab))) { printf("tabini ERROR %d: %s.\n", status, tab_errmsg[status]); return 1; } tab.M = M; for (m = 0; m < tab.M; m++) { tab.K[m] = K[m]; tab.map[m] = map[m]; tab.crval[m] = crval[m]; for (k = 0; k < tab.K[m]; k++) { tab.index[m][k] = (double)k; } } /* Subdivide the interpolation element. */ for (i = 0; i < NP; i++) { for (j = 0; j < NP; j++) { x[i][j][0] = j*(K1-1.0)*scl - 0.5 - crval[0]; x[i][j][1] = i*(K2-1.0)*scl - 0.5 - crval[1]; } } /* The first coordinate element is static. */ tab.coord[0] = 0.0; tab.coord[2] = 0.0; tab.coord[4] = 0.0; tab.coord[6] = 0.0; /* (k1,k2) = (0,0). */ tab.coord[1] = 0.0; /* The second coordinate element varies in three of the corners. */ for (l3 = 0; l3 <= 100; l3 += 20) { /* (k1,k2) = (1,1). */ tab.coord[7] = 0.01 * l3; for (l2 = 0; l2 <= 100; l2 += 20) { /* (k1,k2) = (0,1). */ tab.coord[5] = 0.01 * l2; cpgpage(); for (l1 = 0; l1 <= 100; l1 += 2) { /* (k1,k2) = (1,0). */ tab.coord[3] = 0.01 * l1; /* Compute coordinates within the interpolation element. */ tab.flag = 0; if ((status = tabx2s(&tab, NP*NP, 2, (double *)x, (double *)world, stat))) { printf("tabx2s ERROR %d: %s.\n", status, tab_errmsg[status]); } /* Start a new plot. */ cpgbbuf(); cpgeras(); cpgsci(1); cpgslw(3); cpgbox("BCNST", 0.0f, 0, "BCNSTV", 0.0f, 0); cpgmtxt("T", 0.7f, 0.5f, 0.5f, "-TAB coordinates: " "linear interpolation / extrapolation in 2-D"); /* Draw the boundary of the interpolation element in red. */ cpgsci(2); cpgmove(-0.5f, 0.0f); cpgdraw( 1.5f, 0.0f); cpgmove( 1.0f, -0.5f); cpgdraw( 1.0f, 1.5f); cpgmove( 1.5f, 1.0f); cpgdraw(-0.5f, 1.0f); cpgmove( 0.0f, 1.5f); cpgdraw( 0.0f, -0.5f); /* Label the value of the coordinate element in each corner. */ sprintf(text, "%.1f", tab.coord[1]); cpgtext(-0.09f, -0.05f, text); sprintf(text, "%.2f", tab.coord[3]); cpgtext( 1.02f, -0.05f, text); sprintf(text, "%.1f", tab.coord[5]); cpgtext(-0.13f, 1.02f, text); sprintf(text, "%.1f", tab.coord[7]); cpgtext( 1.02f, 1.02f, text); cpgsci(1); /* Contour labelling: bottom. */ v0 = world[0][0][1]; v1 = world[0][NP-1][1]; if (v0 != v1) { lstep = (abs((int)((v1-v0)/0.2f)) < 10) ? 20 : 40; for (l = -200; l <= 300; l += lstep) { w = -0.5f + 2.0f * (l*0.01f - v0) / (v1 - v0); if (w < -0.5 || w > 1.5) continue; sprintf(text, "%4.1f", l*0.01f); cpgptxt(w+0.04f, -0.56f, 0.0f, 1.0f, text); } } /* Contour labelling: left. */ v0 = world[0][0][1]; v1 = world[NP-1][0][1]; if (v0 != v1) { lstep = (abs((int)((v1-v0)/0.2f)) < 10) ? 20 : 40; for (l = -200; l <= 300; l += lstep) { w = -0.5f + 2.0f * (l*0.01f - v0) / (v1 - v0); if (w < -0.5 || w > 1.5) continue; sprintf(text, "%4.1f", l*0.01f); cpgptxt(-0.52f, w-0.02f, 0.0f, 1.0f, text); } } /* Contour labelling: right. */ v0 = world[0][NP-1][1]; v1 = world[NP-1][NP-1][1]; if (v0 != v1) { lstep = (abs((int)((v1-v0)/0.2f)) < 10) ? 20 : 40; for (l = -200; l <= 300; l += lstep) { w = -0.5f + 2.0f * (l*0.01f - v0) / (v1 - v0); if (w < -0.5 || w > 1.5) continue; sprintf(text, "%.1f", l*0.01f); cpgptxt(1.52f, w-0.02f, 0.0f, 0.0f, text); } } /* Contour labelling: top. */ v0 = world[NP-1][0][1]; v1 = world[NP-1][NP-1][1]; if (v0 != v1) { lstep = (abs((int)((v1-v0)/0.2f)) < 10) ? 20 : 40; for (l = -200; l <= 300; l += lstep) { w = -0.5f + 2.0f * (l*0.01f - v0) / (v1 - v0); if (w < -0.5 || w > 1.5) continue; sprintf(text, "%4.1f", l*0.01f); cpgptxt(w+0.04f, 1.52f, 0.0f, 1.0f, text); } } /* Draw contours for the second coordinate element. */ for (i = 0; i < NP; i++) { for (j = 0; j < NP; j++) { array[i][j] = world[i][j][1]; } } cpgsci(4); cpgslw(2); cpgcont(array[0], NP, NP, 1, NP, 1, NP, clev, 10, ltm); cpgsci(7); cpgcont(array[0], NP, NP, 1, NP, 1, NP, clev+10, 1, ltm); cpgsci(5); cpgcont(array[0], NP, NP, 1, NP, 1, NP, clev+11, 20, ltm); cpgebuf(); } } } cpgend(); tabfree(&tab); return 0; } pywcs-1.12/wcslib/C/test/ttab3.c0000644001153600020070000001223112310355626020452 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: ttab3.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * ttab3 tests the -TAB routines using PGPLOT for graphical display. It * constructs a table that approximates Bonne's projection and uses it to * draw a graticule. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include #include #define K1 271 #define K2 235 int main() { /* Set up the lookup table. */ const int M = 2; const int K[] = {K1, K2}; const int map[] = {0, 1}; const double crval[] = {135.0, 95.0}; char text[80]; int ci, i, ilat, ilng, j, k, m, stat[K2][K1], status; float xr[361], yr[361]; double *dp, world[361][2], x[K1], xy[361][2], y[K2]; struct tabprm tab; struct prjprm prj; printf( "Testing WCSLIB inverse coordinate lookup table routines (ttab3.c)\n" "-----------------------------------------------------------------\n"); /* List status return messages. */ printf("\nList of tab status return values:\n"); for (status = 1; status <= 5; status++) { printf("%4d: %s.\n", status, tab_errmsg[status]); } printf("\n"); /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); cpgvstd(); cpgsch(0.7f); cpgwnad(-135.0f, 135.0f, -95.0f, 140.0f); cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgscr(0, 0.00f, 0.00f, 0.00f); cpgscr(1, 1.00f, 1.00f, 0.00f); cpgscr(2, 1.00f, 1.00f, 1.00f); cpgscr(3, 0.50f, 0.50f, 0.80f); cpgscr(4, 0.80f, 0.50f, 0.50f); cpgscr(5, 0.80f, 0.80f, 0.80f); cpgscr(6, 0.50f, 0.50f, 0.80f); cpgscr(7, 0.80f, 0.50f, 0.50f); cpgscr(8, 0.30f, 0.50f, 0.30f); /* Set up the lookup table. */ tab.flag = -1; if ((status = tabini(1, M, K, &tab))) { printf("tabini ERROR %d: %s.\n", status, tab_errmsg[status]); return 1; } tab.M = M; for (m = 0; m < tab.M; m++) { tab.K[m] = K[m]; tab.map[m] = map[m]; tab.crval[m] = crval[m]; for (k = 0; k < tab.K[m]; k++) { tab.index[m][k] = (double)k; } } /* Set up the lookup table to approximate Bonne's projection. */ for (i = 0; i < K1; i++) { x[i] = 135 - i; } for (j = 0; j < K2; j++) { y[j] = j - 95; } prjini(&prj); prj.pv[1] = 35.0; status = bonx2s(&prj, K1, K2, 1, 2, x, y, tab.coord, tab.coord+1, (int *)stat); dp = tab.coord; for (j = 0; j < K2; j++) { for (i = 0; i < K1; i++) { if (stat[j][i]) { *dp = 999.0; *(dp+1) = 999.0; } dp += 2; } } /* Draw meridians. */ ci = 1; for (ilng = -180; ilng <= 180; ilng += 15) { if (++ci > 7) ci = 2; cpgsci(ilng?ci:1); for (j = 0, ilat = -90; ilat <= 90; ilat++, j++) { world[j][0] = (double)ilng; world[j][1] = (double)ilat; } /* A fudge to account for the singularity at the poles. */ world[0][0] = 0.0; world[180][0] = 0.0; status = tabs2x(&tab, 181, 2, (double *)world, (double *)xy, (int *)stat); k = 0; for (j = 0; j < 181; j++) { if (stat[0][j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } xr[k] = xy[j][0]; yr[k] = xy[j][1]; k++; } cpgline(k, xr, yr); } /* Draw parallels. */ ci = 1; for (ilat = -75; ilat <= 75; ilat += 15) { if (++ci > 7) ci = 2; cpgsci(ilat?ci:1); for (j = 0, ilng = -180; ilng <= 180; ilng++, j++) { world[j][0] = (double)ilng; world[j][1] = (double)ilat; } status = tabs2x(&tab, 361, 2, (double *)world, (double *)xy, (int *)stat); k = 0; for (j = 0; j < 361; j++) { if (stat[0][j]) { if (k > 1) cpgline(k, xr, yr); k = 0; continue; } xr[k] = xy[j][0]; yr[k] = xy[j][1]; k++; } cpgline(k, xr, yr); } cpgend(); return 0; } pywcs-1.12/wcslib/C/test/tunits.c0000644001153600020070000001027712310355626020773 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tunits.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * tunits tests wcsulex(), wcsutrn(), and wcsunits() the FITS units * specification parser, translator and converter. * *---------------------------------------------------------------------------*/ #include #include #include #include #include int main() { char have[80], want[80]; int func, i, interactive, status; double offset, power, scale, units[WCSUNITS_NTYPE]; interactive = isatty(0); printf("Testing FITS unit specification parser (tunits.c)\n" "-------------------------------------------------\n"); if (interactive) printf("\nTo test wcsulex(), enter when prompted " "with \"Unit string (want):\".\n"); while (1) { if (interactive) printf("\nUnit string (have): "); if (!fgets(have, 80, stdin)) break; have[strlen(have)-1] = '\0'; if (!interactive) printf("\nUnit string (have): %s\n", have); if ((status = wcsutrn(7, have)) >= 0) { printf(" Translation: %s", have); if (status == 0) { printf("\n"); } else { printf(" (WARNING: %s)\n", wcsunits_errmsg[status]); } } if (interactive) printf("Unit string (want): "); if (!fgets(want, 80, stdin)) break; want[strlen(want)-1] = '\0'; if (*want) { if (!interactive) printf("Unit string (want): %s\n", want); if ((status = wcsutrn(7, want)) >= 0) { printf(" Translation: %s", want); if (status == 0) { printf("\n"); } else { printf(" (WARNING: %s)\n", wcsunits_errmsg[status]); } } printf("Conversion: \"%s\" -> \"%s\"\n", have, want); if ((status = wcsunits(have, want, &scale, &offset, &power))) { printf("wcsunits ERROR %d: %s.\n", status, wcsunits_errmsg[status]); continue; } printf(" = %s", (power == 1.0) ? "" : "("); if (scale == 1.0) { printf("value"); } else { printf("%.8g * value", scale); } if (offset != 0.0) { printf(" + %.8g", offset); } if (power == 1.0) { printf("\n"); } else { printf(")^%.8g\n", power); } } else { /* Parse the unit string. */ printf(" Parsing: \"%s\"\n", have); if ((status = wcsulex(have, &func, &scale, units))) { printf("wcsulex ERROR %d: %s.\n", status, wcsunits_errmsg[status]); continue; } printf("%15.8g *\n", scale); for (i = 0; i < WCSUNITS_NTYPE; i++) { if (units[i] != 0.0) { printf("%11.2f %s", units[i], wcsunits_types[i]); if (strlen(wcsunits_units[i])) { printf(" (%s)\n", wcsunits_units[i]); } else { printf("\n"); } } } } } printf("\n"); return 0; } pywcs-1.12/wcslib/C/test/twcs.c0000644001153600020070000003270212310355626020422 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility and: Michael Droetboom, Space Telescope Science Institute http://www.atnf.csiro.au/~mcalabre/index.html $Id: twcs.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * twcs tests wcss2p() and wcsp2s() for closure on an oblique 2-D slice through * a 4-D image with celestial, spectral and logarithmic coordinate axes. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include void parser(struct wcsprm *); int check_error(struct wcsprm *, int, int, char *); int test_errors(); /* Reporting tolerance. */ const double tol = 1.0e-10; /* In real life these would be encoded as FITS header keyrecords. */ const int NAXIS = 4; const double CRPIX[4] = { 513.0, 0.0, 0.0, 0.0}; const double PC[4][4] = {{ 1.1, 0.0, 0.0, 0.0}, { 0.0, 1.0, 0.0, 0.1}, { 0.0, 0.0, 1.0, 0.0}, { 0.0, 0.2, 0.0, 1.0}}; const double CDELT[4] = {-9.635265432e-6, 1.0, 0.1, -1.0}; char CTYPE[4][9] = {"WAVE-F2W", "XLAT-BON", "TIME-LOG", "XLON-BON"}; const double CRVAL[4] = {0.214982042, -30.0, 1.0, 150.0}; const double LONPOLE = 150.0; const double LATPOLE = 999.0; const double RESTFRQ = 1.42040575e9; const double RESTWAV = 0.0; int NPV = 3; struct pvcard PV[3]; /* Projection parameters are set in main(). */ int itest = 0; int main() { #define NELEM 9 char ok[] = "", mismatch[] = " (WARNING, mismatch)", *s; int i, k, lat, lng, nFail1 = 0, nFail2 = 0, stat[361], status; double freq, img[361][NELEM], lat1, lng1, phi[361], pixel1[361][NELEM], pixel2[361][NELEM], r, resid, residmax, theta[361], time, world1[361][NELEM], world2[361][NELEM]; struct wcsprm *wcs; printf("Testing closure of WCSLIB world coordinate transformation " "routines (twcs.c)\n" "----------------------------------------------------------" "-----------------\n"); /* List status return messages. */ printf("\nList of wcs status return values:\n"); for (status = 1; status <= 13; status++) { printf("%4d: %s.\n", status, wcs_errmsg[status]); } printf("\nSize of data types (bytes):\n"); printf(" char:%5"MODZ"u\n", sizeof(char)); printf(" short int:%5"MODZ"u\n", sizeof(short int)); printf(" int:%5"MODZ"u\n", sizeof(int)); printf(" long int:%5"MODZ"u\n", sizeof(long int)); printf(" float:%5"MODZ"u\n", sizeof(float)); printf(" double:%5"MODZ"u\n", sizeof(double)); printf(" char *:%5"MODZ"u\n", sizeof(char *)); printf(" char (*)[72]:%5"MODZ"u\n", sizeof(char (*)[72])); printf(" int *:%5"MODZ"u\n", sizeof(int *)); printf(" float *:%5"MODZ"u\n", sizeof(float *)); printf(" double *:%5"MODZ"u\n", sizeof(double *)); printf("struct pvcard *:%5"MODZ"u\n", sizeof(struct pvcard *)); printf("struct pscard *:%5"MODZ"u\n", sizeof(struct pscard *)); printf("\nSize of structs (bytes/ints):\n"); s = (sizeof(struct celprm) == sizeof(int)*CELLEN) ? ok : mismatch; printf(" celprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct celprm), CELLEN, s); s = (sizeof(struct fitskey) == sizeof(int)*KEYLEN) ? ok : mismatch; printf(" fitskey:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct fitskey), KEYLEN, s); s = (sizeof(struct fitskeyid) == sizeof(int)*KEYIDLEN) ? ok : mismatch; printf(" fitskeyid:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct fitskeyid), KEYIDLEN, s); s = (sizeof(struct linprm) == sizeof(int)*LINLEN) ? ok : mismatch; printf(" linprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct linprm), LINLEN, s); s = (sizeof(struct prjprm) == sizeof(int)*PRJLEN) ? ok : mismatch; printf(" prjprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct prjprm), PRJLEN, s); s = (sizeof(struct spcprm) == sizeof(int)*SPCLEN) ? ok : mismatch; printf(" spcprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct spcprm), SPCLEN, s); s = (sizeof(struct spxprm) == sizeof(int)*SPXLEN) ? ok : mismatch; printf(" spxprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct spxprm), SPXLEN, s); s = (sizeof(struct tabprm) == sizeof(int)*TABLEN) ? ok : mismatch; printf(" tabprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct tabprm), TABLEN, s); s = (sizeof(struct wcserr) == sizeof(int)*ERRLEN) ? ok : mismatch; printf(" wcserr:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct wcserr), ERRLEN, s); s = (sizeof(struct wcsprm) == sizeof(int)*WCSLEN) ? ok : mismatch; printf(" wcsprm:%5"MODZ"u /%4"MODZ"u%s\n", sizeof(struct wcsprm), WCSLEN, s); /* Set the PVi_ma keyvalues for the longitude axis. */ /*----------------------------------------------------------*/ /* For test purposes, these are set so that the fiducial */ /* native coordinates are at the native pole, i.e. so that */ /* (phi0,theta0) = (0,90), but without any fiducial offset, */ /* i.e. iwith PVi_0a == 0 (by default). */ /*----------------------------------------------------------*/ PV[0].i = 4; /* Longitude is on axis 4. */ PV[0].m = 1; /* Parameter number 1. */ PV[0].value = 0.0; /* Fiducial native longitude. */ PV[1].i = 4; /* Longitude is on axis 4. */ PV[1].m = 2; /* Parameter number 2. */ PV[1].value = 90.0; /* Fiducial native latitude. */ /* Set the PVi_m keyvaluess for the latitude axis. */ PV[2].i = 2; /* Latitude is on axis 2. */ PV[2].m = 1; /* Parameter number 1. */ PV[2].value = -30.0; /* PVi_1. */ /* The following routine simulates the actions of a FITS header parser. */ wcs = malloc(sizeof(struct wcsprm)); wcs->flag = -1; parser(wcs); printf("\nReporting tolerance %5.1g pixel.\n", tol); /* Initialize non-celestial world coordinates. */ time = 1.0; freq = 1.42040595e9 - 180.0 * 62500.0; for (k = 0; k < 361; k++) { world1[k][0] = 0.0; world1[k][1] = 0.0; world1[k][2] = 0.0; world1[k][3] = 0.0; world1[k][2] = time; time *= 1.01; world1[k][wcs->spec] = 2.99792458e8 / freq; freq += 62500.0; } residmax = 0.0; for (lat = 90; lat >= -90; lat--) { lat1 = (double)lat; for (lng = -180, k = 0; lng <= 180; lng++, k++) { lng1 = (double)lng; world1[k][wcs->lng] = lng1; world1[k][wcs->lat] = lat1; } if (wcss2p(wcs, 361, NELEM, world1[0], phi, theta, img[0], pixel1[0], stat)) { printf(" At wcss2p#1 with lat1 == %f\n", lat1); wcsperr(wcs, " "); continue; } if (wcsp2s(wcs, 361, NELEM, pixel1[0], img[0], phi, theta, world2[0], stat)) { printf(" At wcsp2s with lat1 == %f\n", lat1); wcsperr(wcs, " "); continue; } if (wcss2p(wcs, 361, NELEM, world2[0], phi, theta, img[0], pixel2[0], stat)) { printf(" At wcss2p#2 with lat1 == %f\n", lat1); wcsperr(wcs, " "); continue; } for (k = 0; k < 361; k++) { resid = 0.0; for (i = 0; i < NAXIS; i++) { r = pixel2[k][i] - pixel1[k][i]; resid += r*r; } resid = sqrt(resid); if (resid > residmax) residmax = resid; if (resid > tol) { nFail1++; printf("\nClosure error:\n" "world1:%18.12f%18.12f%18.12f%18.12f\n" "pixel1:%18.12f%18.12f%18.12f%18.12f\n" "world2:%18.12f%18.12f%18.12f%18.12f\n" "pixel2:%18.12f%18.12f%18.12f%18.12f\n", world1[k][0], world1[k][1], world1[k][2], world1[k][3], pixel1[k][0], pixel1[k][1], pixel1[k][2], pixel1[k][3], world2[k][0], world2[k][1], world2[k][2], world2[k][3], pixel2[k][0], pixel2[k][1], pixel2[k][2], pixel2[k][3]); } } } printf("wcsp2s/wcss2p: Maximum closure residual = %.1e pixel.\n", residmax); /* Test wcserr and wcsprintf() as well. */ nFail2 = 0; wcsprintf_set(stdout); wcsprintf("\n\nIGNORE messages marked with 'OK', they test wcserr " "(and wcsprintf):\n"); wcserr_enable(1); /* Test 1. */ wcs->pv[2].value = UNDEFINED; status = wcsset(wcs); nFail2 += check_error(wcs, status, WCSERR_BAD_PARAM, "Invalid parameter value"); nFail2 += test_errors(); if (nFail1 || nFail2) { if (nFail1) { printf("\nFAIL: %d closure residuals exceed reporting tolerance.\n", nFail1); } if (nFail2) { printf("FAIL: %d error messages differ from that expected.\n", nFail2); } } else { printf("\nPASS: All closure residuals are within reporting tolerance.\n"); printf("PASS: All error messages reported as expected.\n"); } /* Clean up. */ wcsfree(wcs); free(wcs); return nFail1 + nFail2; } /*--------------------------------------------------------------------------*/ void parser(wcs) struct wcsprm *wcs; { int i, j; double *pcij; /* In practice a parser would read the FITS header until it encountered */ /* the NAXIS keyword which must occur near the start, before any of the */ /* WCS keywords. It would then use wcsini() to allocate memory for */ /* arrays in the wcsprm struct and set default values. In this */ /* simulation the header keyvalues are set as global variables. */ wcsini(1, NAXIS, wcs); /* Now the parser scans the FITS header, identifying WCS keywords and */ /* loading their values into the appropriate elements of the wcsprm */ /* struct. */ for (j = 0; j < NAXIS; j++) { wcs->crpix[j] = CRPIX[j]; } pcij = wcs->pc; for (i = 0; i < NAXIS; i++) { for (j = 0; j < NAXIS; j++) { *(pcij++) = PC[i][j]; } } for (i = 0; i < NAXIS; i++) { wcs->cdelt[i] = CDELT[i]; } for (i = 0; i < NAXIS; i++) { strcpy(wcs->ctype[i], &CTYPE[i][0]); } for (i = 0; i < NAXIS; i++) { wcs->crval[i] = CRVAL[i]; } wcs->lonpole = LONPOLE; wcs->latpole = LATPOLE; wcs->restfrq = RESTFRQ; wcs->restwav = RESTWAV; wcs->npv = NPV; for (i = 0; i < NPV; i++) { wcs->pv[i] = PV[i]; } /* Extract information from the FITS header. */ if (wcsset(wcs)) { wcsperr(wcs, ""); } return; } /*--------------------------------------------------------------------------*/ int check_error(struct wcsprm *wcs, int status, int exstatus, char *exmsg) { const char *errmsg = (status ? (wcs->err)->msg : ""); wcsprintf("\nTest %d...\n", ++itest); if (status == exstatus && strcmp(errmsg, exmsg) == 0) { wcsperr(wcs, "OK: "); wcsprintf("...succeeded.\n"); } else { wcsprintf("Expected error %d: '%s', got\n", exstatus, exmsg); wcsperr(wcs, ""); wcsprintf("...failed.\n"); return 1; } return 0; } /*--------------------------------------------------------------------------*/ int test_errors() { const char *(multiple_cubeface[2]) = {"CUBEFACE", "CUBEFACE"}; const char *(projection_code[2]) = {"RA---FOO", "DEC--BAR"}; const char *(unmatched[2]) = {"RA---TAN", "FREQ-LOG"}; int i, nFail = 0, status; struct wcsprm wcs; /* Test 2. */ wcs.flag = -1; status = wcsini(1, -32, &wcs); nFail += check_error(&wcs, status, WCSERR_MEMORY, "naxis must be positive (got -32)"); /* Test 3. */ wcs.flag = 0; status = wcsini(1, 2, &wcs); nFail += check_error(&wcs, status, WCSERR_SUCCESS, ""); /* Test 4. */ for (i = 0; i < 2; i++) { strcpy(wcs.ctype[i], &multiple_cubeface[i][0]); } status = wcsset(&wcs); nFail += check_error(&wcs, status, WCSERR_BAD_CTYPE, "Multiple CUBEFACE axes (in CTYPE1 and CTYPE2)"); /* Test 5. */ wcs.flag = 0; status = wcsini(1, 2, &wcs); for (i = 0; i < 2; i++) { strcpy(wcs.ctype[i], &projection_code[i][0]); } status = wcsset(&wcs); nFail += check_error(&wcs, status, WCSERR_BAD_CTYPE, "Unrecognized projection code (FOO in CTYPE1)"); /* Test 6. */ wcs.flag = 0; status = wcsini(1, 2, &wcs); for (i = 0; i < 2; i++) { strcpy(wcs.ctype[i], &unmatched[i][0]); } status = wcsset(&wcs); nFail += check_error(&wcs, status, WCSERR_BAD_CTYPE, "Unmatched celestial axes"); return nFail; } pywcs-1.12/wcslib/C/test/twcsfix.c0000644001153600020070000001332512310355626021131 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: twcsfix.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * twcsfix tests the translation routines for non-standard WCS keyvalues, the * wcsfix() suite, and the spectral coordinate translation routine wcssptr(). * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include #include void parser(struct wcsprm *); const int NAXIS = 3; const double CRPIX[3] = {90.0, 90.0, 1.0}; const double PC[3][3] = {{ 1.0, 0.0, 0.0}, { 0.0, 1.0, 0.0}, { 0.0, 0.0, 1.0}}; const double CDELT[3] = {-1.0, 1.0, 19.68717093222}; char CUNIT[3][9] = {"ARCSEC", "ARCSEC", "KM/SEC"}; /* N.B. non-standard. */ char CTYPE[3][9] = {"RA---NCP", "DEC--NCP", "FELO-HEL"}; const double CRVAL[3] = {265.6220947090*3600.0, -28.98849996030*3600.0, 5569.27104}; const double RESTFRQ = 1.42040575e9; const double RESTWAV = 0.0; /* N.B. non-standard, corresponding to MJD 35884.04861111 */ const char DATEOBS[] = "1957/02/15 01:10:00"; /* For testing spcfix(). */ const int VELREF = 2; const char SPECSYS[] = "BARYCENT"; int main() { char ctypeS[9]; int i, stat[NWCSFIX], status; struct wcsprm wcs; struct wcserr info[NWCSFIX]; wcsprintf("Testing WCSLIB translator for non-standard usage (twcsfix.c)\n" "------------------------------------------------------------\n\n"); wcs.flag = -1; parser(&wcs); /* Note: to print the unfixed wcsprm struct using wcsprt() the struct would first have to be initialized by wcsset(). However, if the struct contains non-standard keyvalues then wcsset() will either fix them itself or else fail (e.g. for non-standard units). Thus, in general, wcsprt() cannot be used to print the unmodified struct. */ /* Fix non-standard WCS keyvalues. */ wcserr_enable(1); status = wcsfixi(7, 0, &wcs, stat, info); wcsprintf("wcsfix status returns: ("); for (i = 0; i < NWCSFIX; i++) { wcsprintf(i ? ", %d" : "%d", stat[i]); } wcsprintf(")\n"); for (i = 0; i < NWCSFIX; i++) { if (info[i].status < -1 || 0 < info[i].status) { wcsprintf("\n"); wcserr_prt(info+i, 0x0); } } if (status) { wcsprintf("\nwcsfix error %d", status); return 1; } /* Extract information from the FITS header. */ if (wcsset(&wcs)) { wcsprintf("\n"); wcserr_prt(wcs.err, 0x0); } wcsprintf("\n"); wcsprt(&wcs); wcsprintf("\n------------------------------------" "------------------------------------\n"); /* Should now have a 'VOPT-F2W' axis, translate it to frequency. */ strcpy(ctypeS, "FREQ-???"); i = -1; if (wcssptr(&wcs, &i, ctypeS)) { wcserr_prt(wcs.err, 0x0); return 1; } if (wcsset(&wcs)) { wcserr_prt(wcs.err, 0x0); return 1; } wcsprt(&wcs); wcsfree(&wcs); return 0; } /*--------------------------------------------------------------------------*/ void parser(wcs) struct wcsprm *wcs; { int i, j; double *pcij; /* In practice a parser would read the FITS header until it encountered */ /* the NAXIS keyword which must occur near the start, before any of the */ /* WCS keywords. It would then use wcsini() to allocate memory for */ /* arrays in the wcsprm struct and set default values. In this */ /* simulation the header keyvalues are set as global variables. */ wcsnpv(2); wcsini(1, NAXIS, wcs); /* Now the parser scans the FITS header, identifying WCS keywords and */ /* loading their values into the appropriate elements of the wcsprm */ /* struct. */ for (j = 0; j < NAXIS; j++) { wcs->crpix[j] = CRPIX[j]; } pcij = wcs->pc; for (i = 0; i < NAXIS; i++) { for (j = 0; j < NAXIS; j++) { *(pcij++) = PC[i][j]; } } for (i = 0; i < NAXIS; i++) { wcs->cdelt[i] = CDELT[i]; } for (i = 0; i < NAXIS; i++) { strcpy(wcs->cunit[i], &CUNIT[i][0]); } for (i = 0; i < NAXIS; i++) { strcpy(wcs->ctype[i], &CTYPE[i][0]); } for (i = 0; i < NAXIS; i++) { wcs->crval[i] = CRVAL[i]; } wcs->restfrq = RESTFRQ; wcs->restwav = RESTWAV; wcs->pv[0].i = -1; wcs->pv[0].m = -1; wcs->pv[0].value = -1.0; wcs->npv = 1; wcs->velref = VELREF; strcpy(wcs->dateobs, DATEOBS); strcpy(wcs->specsys, SPECSYS); return; } pywcs-1.12/wcslib/C/test/twcshdr.c0000644001153600020070000001333012310355626021114 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: twcshdr.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * twcshdr illustrates the steps required to read WCS information (including * -TAB coordinates) from a FITS header using the CFITSIO library * * Options: * -h: Uses wcshdo() to translate the wcsprm struct into a FITS header and * prints it. * * -p: Asks the user for a pixel coordinate which it transforms to world * coordinates and prints. * * -w: Asks the user for a world coordinate which it transforms to pixel * coordinates and prints. * * If none of the above options are specified it uses wcsprt() to print the * wcsprm struct itself. * * Input comes from a user-specified FITS file. * *===========================================================================*/ #include #include #include #include int main(int argc, char *argv[]) { char *header, *hptr; int dohdr = 0, dopixel = 0, doworld = 0; int i, nkeyrec, nreject, nwcs, stat[NWCSFIX], status = 0; double imgcrd[2], phi, pixcrd[2], theta, world[2]; fitsfile *fptr; struct wcsprm *wcs; /* Parse options. */ for (i = 1; i < argc && argv[i][0] == '-'; i++) { if (!argv[i][1]) break; switch (argv[i][1]) { case 'h': dohdr = 1; break; case 'p': dopixel = 1; break; case 'w': doworld = 1; break; default: fprintf(stderr, "Usage: twcshdr [-h | -p | -w] \n"); return 1; } } if (i != (argc-1)) { fprintf(stderr, "Usage: twcshdr [-h | -p | -w] \n"); return 1; } /* Open the FITS test file and read the primary header. */ fits_open_file(&fptr, argv[i], READONLY, &status); if ((status = fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status))) { fits_report_error(stderr, status); return 1; } /*-----------------------------------------------------------------------*/ /* Basic steps required to interpret a FITS WCS header, including -TAB. */ /*-----------------------------------------------------------------------*/ /* Parse the primary header of the FITS file. */ if ((status = wcspih(header, nkeyrec, WCSHDR_all, 2, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status,wcshdr_errmsg[status]); } /* Read coordinate arrays from the binary table extension. */ if ((status = fits_read_wcstab(fptr, wcs->nwtb, (wtbarr *)wcs->wtb, &status))) { fits_report_error(stderr, status); return 1; } /* Translate non-standard WCS keyvalues. */ if ((status = wcsfix(7, 0, wcs, stat))) { for (i = 0; i < NWCSFIX; i++) { if (stat[i] > 0) { fprintf(stderr, "wcsfix ERROR %d: %s.\n", status, wcsfix_errmsg[stat[i]]); } } return 1; } /*-----------------------------------------------------------------------*/ /* The wcsprm struct is now ready for use. */ /*-----------------------------------------------------------------------*/ /* Finished with the FITS file. */ fits_close_file(fptr, &status); free(header); /* Initialize the wcsprm struct, also taking control of memory allocated by * fits_read_wcstab(). */ if ((status = wcsset(wcs))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); return 1; } if (dohdr) { if ((status = wcshdo(WCSHDO_all, wcs+2, &nkeyrec, &header))) { return 1; } hptr = header; printf("\n\n"); for (i = 0; i < nkeyrec; i++, hptr += 80) { printf("%.80s\n", hptr); } free(header); } else if (dopixel) { while (1) { printf("Enter pixel coordinates: "); if (scanf("%lf%*[ ,]%lf", pixcrd, pixcrd+1) != wcs->naxis) break; status = wcsp2s(wcs, 1, 2, pixcrd, imgcrd, &phi, &theta, world, stat); printf(" (%20.15f, %20.15f) ->\n (%20.15f, %20.15f)\n\n", pixcrd[0], pixcrd[1], world[0], world[1]); } } else if (doworld) { while (1) { printf("Enter world coordinates: "); if (scanf("%lf%*[ ,]%lf", world, world+1) != wcs->naxis) break; status = wcss2p(wcs, 1, 2, world, &phi, &theta, imgcrd, pixcrd, stat); printf(" (%20.15f, %20.15f) ->\n (%20.15f, %20.15f)\n\n", world[0], world[1], pixcrd[0], pixcrd[1]); } } else { /* Print the struct. */ if ((status = wcsprt(wcs))) { return 1; } } /* Clean up. */ status = wcsvfree(&nwcs, &wcs); return 0; } pywcs-1.12/wcslib/C/test/twcsmix.c0000644001153600020070000005570012310355625021142 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: twcsmix.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * twcsmix tests wcsmix() for closure on the 1 degree celestial graticule for * a number of selected projections. Points with good solutions are marked * with a white dot on a graphical display of the projection while bad * solutions are flagged with a red circle. * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include void mixex(double, double, double, double); void id(struct wcsprm *, int *, double, double, double, double); void grdplt(struct wcsprm *, double, double, double, double); void parser(struct wcsprm *); /* Set to 1 to skip wcsmix(), primarily for debugging purposes. */ const int skip_wcsmix = 0; /* Reporting tolerance for mixex(). */ const double tol = 1.0e-9; /* In real life these would be encoded as FITS header keyrecords. */ const int NAXIS = 4; const double CRPIX[4] = { 513.0, 0.0, 0.0, 0.0}; const double PC[4][4] = {{ 1.1, 0.0, 0.0, 0.0}, { 0.0, 1.0, 0.0, 0.1}, { 0.0, 0.0, 1.0, 0.0}, { 0.0, 0.2, 0.0, 1.0}}; const double CDELT[4] = {-9.635265432e-6, 1.0, 1.0, -1.0}; /* The "xxx" is reset in main(). */ char CTYPE[4][9] = {"WAVE-F2W", "XLAT-xxx", "TIME ", "XLON-xxx"}; /* Will be reset in mixex(). */ double CRVAL[4] = {0.214982042, -30.0, -2e3, 150.0}; double LONPOLE = 150.0; double LATPOLE = 999.0; double RESTFRQ = 1.42040575e9; double RESTWAV = 0.0; int NPV; struct pvcard PV[10]; /* Projection parameters are set in main(). */ int main() { char text[80]; register int status; printf("Testing WCSLIB wcsmix() routine (twcsmix.c)\n" "-------------------------------------------\n"); /* List status return messages. */ printf("\nList of wcs status return values:\n"); for (status = 1; status <= 13; status++) { printf("%4d: %s.\n", status, wcs_errmsg[status]); } /* PGPLOT initialization. */ strcpy(text, "/xwindow"); cpgbeg(0, text, 1, 1); /* Define pen colours. */ cpgscr(0, 0.00f, 0.00f, 0.00f); cpgscr(1, 1.00f, 1.00f, 0.00f); cpgscr(2, 1.00f, 1.00f, 1.00f); cpgscr(3, 0.50f, 0.50f, 0.80f); cpgscr(4, 0.80f, 0.50f, 0.50f); cpgscr(5, 0.80f, 0.80f, 0.80f); cpgscr(6, 0.50f, 0.50f, 0.80f); cpgscr(7, 0.80f, 0.50f, 0.50f); cpgscr(8, 0.30f, 0.50f, 0.30f); cpgscr(9, 1.00f, 0.75f, 0.00f); /*----------------------------------------------------------*/ /* Set the PVi_m keyvalues for the longitude axis so that */ /* the fiducial native coordinates are at the native pole, */ /* i.e. (phi0,theta0) = (0,90), but without any fiducial */ /* offset. We do this as a test, and also so that all */ /* projections will be exercised with the same obliquity */ /* parameters. */ /*----------------------------------------------------------*/ PV[0].i = 4; /* Longitude is on axis 4. */ PV[0].m = 1; /* Parameter number 1. */ PV[0].value = 0.0; /* Fiducial native longitude. */ PV[1].i = 4; /* Longitude is on axis 4. */ PV[1].m = 2; /* Parameter number 2. */ PV[1].value = 90.0; /* Fiducial native latitude. */ /* Set the PVi_m keyvalues for the latitude axis. */ PV[2].i = 2; /* Latitude is on axis 2. */ PV[2].m = 1; /* Parameter number 1. */ PV[2].value = 0.0; /* PVi_1 (set below). */ PV[3].i = 2; /* Latitude is on axis 2. */ PV[3].m = 2; /* Parameter number 2. */ PV[3].value = 0.0; /* PVi_2 (set below). */ /* ARC: zenithal/azimuthal equidistant. */ strncpy(&CTYPE[1][5], "ARC", 3); strncpy(&CTYPE[3][5], "ARC", 3); NPV = 2; mixex(-190.0, 190.0, -190.0, 190.0); /* ZEA: zenithal/azimuthal equal area. */ strncpy(&CTYPE[1][5], "ZEA", 3); strncpy(&CTYPE[3][5], "ZEA", 3); NPV = 2; mixex(-120.0, 120.0, -120.0, 120.0); /* CYP: cylindrical perspective. */ strncpy(&CTYPE[1][5], "CYP", 3); strncpy(&CTYPE[3][5], "CYP", 3); NPV = 4; PV[2].value = 3.0; PV[3].value = 0.8; mixex(-170.0, 170.0, -170.0, 170.0); /* CEA: cylindrical equal area. */ strncpy(&CTYPE[1][5], "CEA", 3); strncpy(&CTYPE[3][5], "CEA", 3); NPV = 3; PV[2].value = 0.75; mixex(-200.0, 200.0, -200.0, 200.0); /* CAR: plate carree. */ strncpy(&CTYPE[1][5], "CAR", 3); strncpy(&CTYPE[3][5], "CAR", 3); NPV = 2; mixex(-210.0, 210.0, -210.0, 210.0); /* SFL: Sanson-Flamsteed. */ strncpy(&CTYPE[1][5], "SFL", 3); strncpy(&CTYPE[3][5], "SFL", 3); NPV = 2; mixex(-190.0, 190.0, -190.0, 190.0); /* PAR: parabolic. */ strncpy(&CTYPE[1][5], "PAR", 3); strncpy(&CTYPE[3][5], "PAR", 3); NPV = 2; mixex(-190.0, 190.0, -190.0, 190.0); /* MOL: Mollweide's projection. */ strncpy(&CTYPE[1][5], "MOL", 3); strncpy(&CTYPE[3][5], "MOL", 3); NPV = 2; mixex(-170.0, 170.0, -170.0, 170.0); /* AIT: Hammer-Aitoff. */ strncpy(&CTYPE[1][5], "AIT", 3); strncpy(&CTYPE[3][5], "AIT", 3); NPV = 2; mixex(-170.0, 170.0, -170.0, 170.0); /* COE: conic equal area. */ strncpy(&CTYPE[1][5], "COE", 3); strncpy(&CTYPE[3][5], "COE", 3); NPV = 4; PV[2].value = 60.0; PV[3].value = 15.0; mixex(-140.0, 140.0, -120.0, 160.0); /* COD: conic equidistant. */ strncpy(&CTYPE[1][5], "COD", 3); strncpy(&CTYPE[3][5], "COD", 3); NPV = 4; PV[2].value = 60.0; PV[3].value = 15.0; mixex(-200.0, 200.0, -180.0, 220.0); /* BON: Bonne's projection. */ strncpy(&CTYPE[1][5], "BON", 3); strncpy(&CTYPE[3][5], "BON", 3); NPV = 3; PV[2].value = 30.0; mixex(-160.0, 160.0, -160.0, 160.0); /* PCO: polyconic. */ strncpy(&CTYPE[1][5], "PCO", 3); strncpy(&CTYPE[3][5], "PCO", 3); NPV = 2; mixex(-190.0, 190.0, -190.0, 190.0); /* TSC: tangential spherical cube. */ strncpy(&CTYPE[1][5], "TSC", 3); strncpy(&CTYPE[3][5], "TSC", 3); NPV = 2; mixex(-340.0, 80.0, -210.0, 210.0); /* QSC: quadrilateralized spherical cube. */ strncpy(&CTYPE[1][5], "QSC", 3); strncpy(&CTYPE[3][5], "QSC", 3); NPV = 2; mixex(-340.0, 80.0, -210.0, 210.0); cpgend(); return 0; } /*---------------------------------------------------------------------------- * mixex() tests wcsmix(). *---------------------------------------------------------------------------*/ void mixex(imin, imax, jmin, jmax) double imax, imin, jmax, jmin; { int doid, lat, lng, wcslat, wcslng, stat, status; float ipt[1], jpt[1]; double lng1, lat1, phi, theta; double latspan[2], lngspan[2]; double img[4], pix1[4], pix2[4], pix3[4], world[4]; double pixlng, pixlat, *worldlat, *worldlng; struct wcsprm wcs; struct prjprm *wcsprj = &(wcs.cel.prj); /* This routine simulates the actions of a FITS header parser. */ wcs.flag = -1; parser(&wcs); /* Draw the coordinate graticule. */ grdplt(&wcs, imin, imax, jmin, jmax); if (skip_wcsmix) return; printf("Testing %s; reporting tolerance %5.1g deg.\n", wcsprj->code, tol); /* Cache frequently used values. */ wcslng = wcs.lng; wcslat = wcs.lat; worldlng = world + wcslng; worldlat = world + wcslat; world[0] = 0.0; world[1] = 0.0; world[2] = 0.0; world[3] = 0.0; world[wcs.spec] = 2.99792458e8 / RESTFRQ; for (lat = 90; lat >= -90; lat--) { lat1 = (double)lat; for (lng = -180; lng <= 180; lng+=15) { lng1 = (double)lng; *worldlng = lng1; *worldlat = lat1; if ((status = wcss2p(&wcs, 1, 4, world, &phi, &theta, img, pix1, &stat))) { printf("%3s(s2x): lng1 =%20.15f lat1 =%20.15f ERROR %3d\n", wcsprj->code, lng1, lat1, status); continue; } pixlng = pix1[wcslng]; pixlat = pix1[wcslat]; ipt[0] = pixlng; jpt[0] = pixlat; cpgpt(1, ipt, jpt, -1); lngspan[0] = lng1 - 9.3; if (lngspan[0] < -180.0) lngspan[0] = -180.0; lngspan[1] = lng1 + 4.1; if (lngspan[1] > 180.0) lngspan[1] = 180.0; latspan[0] = lat1 - 3.7; if (latspan[0] < -90.0) latspan[0] = -90.0; latspan[1] = lat1 + 7.2; if (latspan[1] > 90.0) latspan[1] = 90.0; doid = 1; pix2[wcslng] = pixlng; if ((status = wcsmix(&wcs, wcslng, 1, latspan, 1.0, 0, world, &phi, &theta, img, pix2))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" A: wcsmix ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if ((status = wcss2p(&wcs, 1, 0, world, &phi, &theta, img, pix3, &stat))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" A: wcss2p ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if (fabs(pix3[wcslng]-pixlng) > tol && (fabs(*worldlat-lat1) > tol || fabs(pix2[wcslat]-pixlat) > tol)) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" A: (lng2) =%20.15f lat2 =%20.15f\n", *worldlng, *worldlat); printf(" phi =%20.15f theta =%20.15f\n", phi, theta); printf(" (i2) =%20.15f j2 =%20.15f\n", pix2[wcslng], pix2[wcslat]); } pix2[wcslat] = pixlat; if ((status = wcsmix(&wcs, wcslat, 1, latspan, 1.0, 0, world, &phi, &theta, img, pix2))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" B: wcsmix ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if ((status = wcss2p(&wcs, 1, 0, world, &phi, &theta, img, pix3, &stat))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" B: wcss2p ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if (fabs(pix3[wcslat]-pixlat) > tol && (fabs(*worldlat-lat1) > tol || fabs(pix2[wcslng]-pixlng) > tol)) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" B: (lng2) =%20.15f lat2 =%20.15f\n", *worldlng, *worldlat); printf(" phi =%20.15f theta =%20.15f\n", phi, theta); printf(" i2 =%20.15f (j2) =%20.15f\n", pix2[wcslng], pix2[wcslat]); } *worldlat = lat1; pix2[wcslng] = pixlng; if ((status = wcsmix(&wcs, wcslng, 2, lngspan, 1.0, 0, world, &phi, &theta, img, pix2))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" C: wcsmix ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if ((status = wcss2p(&wcs, 1, 0, world, &phi, &theta, img, pix3, &stat))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" C: wcss2p ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if (fabs(pix3[wcslng]-pixlng) > tol && (fabs(*worldlng-lng1) > tol || fabs(pix2[wcslat]-pixlat) > tol)) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" C: lng2 =%20.15f (lat2) =%20.15f\n", *worldlng, *worldlat); printf(" phi =%20.15f theta =%20.15f\n", phi, theta); printf(" (i2) =%20.15f j2 =%20.15f\n", pix2[wcslng], pix2[wcslat]); } pix2[wcslat] = pixlat; if ((status = wcsmix(&wcs, wcslat, 2, lngspan, 1.0, 0, world, &phi, &theta, img, pix2))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" D: wcsmix ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if ((status = wcss2p(&wcs, 1, 0, world, &phi, &theta, img, pix3, &stat))) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" D: wcss2p ERROR %d: %s.\n", status, wcs_errmsg[status]); } else if (fabs(pix3[wcslat]-pixlat) > tol && (fabs(*worldlng-lng1) > tol || fabs(pix2[wcslng]-pixlng) > tol)) { id(&wcs, &doid, lng1, lat1, pixlng, pixlat); printf(" D: lng2 =%20.15f (lat2) =%20.15f\n", *worldlng, *worldlat); printf(" phi =%20.15f theta =%20.15f\n", phi, theta); printf(" i2 =%20.15f (j2) =%20.15f\n", pix2[wcslng], pix2[wcslat]); } } } wcsfree(&wcs); return; } /*--------------------------------------------------------------------------*/ void id(wcs, doid, lng1, lat1, pixlng, pixlat) struct wcsprm *wcs; int *doid; double lng1, lat1, pixlng, pixlat; { float ipt[1], jpt[1]; double phi, theta; struct celprm *wcscel = &(wcs->cel); struct prjprm *wcsprj = &(wcscel->prj); if (*doid) { /* Compute native coordinates. */ sphs2x(wcscel->euler, 1, 1, 1, 1, &lng1, &lat1, &phi, &theta); printf("\n%3s: lng1 =%20.15f lat1 =%20.15f\n", wcsprj->code, lng1, lat1); printf( " phi =%20.15f theta =%20.15f\n", phi, theta); printf( " i1 =%20.15f j1 =%20.15f\n", pixlng, pixlat); *doid = 0; cpgsci(9); ipt[0] = pixlng; jpt[0] = pixlat; cpgpt(1, ipt, jpt, 21); cpgsci(2); } return; } /*--------------------------------------------------------------------------*/ void grdplt(wcs, imin, imax, jmin, jmax) struct wcsprm *wcs; double imax, imin, jmax, jmin; { #define NELEM 9 char text[80]; int ci, ilat, ilng, j, k, stat[361]; float fimax, fimin, fjmax, fjmin, ir[1024], jr[1024]; double freq, img[361][NELEM], lat, lng, phi[361], pix[361][NELEM], step, theta[361], world[361][NELEM]; double *pixlat, *pixlng, *worldlat, *worldlng; struct wcsprm native; struct celprm *wcscel = &(wcs->cel); struct prjprm *wcsprj = &(wcscel->prj); struct prjprm *ntvprj = &(native.cel.prj); /* Initialize non-celestial world coordinates. */ freq = 1.42040595e9 - 180.0 * 62500.0; for (j = 0; j < 361; j++) { world[j][0] = 0.0; world[j][1] = 0.0; world[j][2] = 0.0; world[j][3] = 0.0; world[j][wcs->spec] = 2.99792458e8 / freq; freq += 62500.0; } /* Define PGPLOT viewport. */ fimax = (float)imax; fimin = (float)imin; fjmax = (float)jmax; fjmin = (float)jmin; cpgenv(fimin, fimax, fjmin, fjmax, 1, -2); /* Draw face boundaries of the quad-cube projections. */ if (wcsprj->category == QUADCUBE) { cpgsci(8); /* Draw the map boundary. */ for (j = 0; j < 9; j++) { img[j][0] = 0.0; img[j][1] = 0.0; img[j][2] = 0.0; img[j][3] = 0.0; } img[0][wcs->lng] = -wcsprj->w[0]; img[0][wcs->lat] = wcsprj->w[0]; img[1][wcs->lng] = -wcsprj->w[0]; img[1][wcs->lat] = wcsprj->w[0]*3.0; img[2][wcs->lng] = wcsprj->w[0]; img[2][wcs->lat] = wcsprj->w[0]*3.0; img[3][wcs->lng] = wcsprj->w[0]; img[3][wcs->lat] = -wcsprj->w[0]*3.0; img[4][wcs->lng] = -wcsprj->w[0]; img[4][wcs->lat] = -wcsprj->w[0]*3.0; img[5][wcs->lng] = -wcsprj->w[0]; img[5][wcs->lat] = wcsprj->w[0]; img[6][wcs->lng] = wcsprj->w[0]*7.0; img[6][wcs->lat] = wcsprj->w[0]; img[7][wcs->lng] = wcsprj->w[0]*7.0; img[7][wcs->lat] = -wcsprj->w[0]; img[8][wcs->lng] = -wcsprj->w[0]; img[8][wcs->lat] = -wcsprj->w[0]; linx2p(&(wcs->lin), 9, NELEM, img[0], pix[0]); for (j = 0; j < 9; j++) { ir[j] = pix[j][wcs->lng]; jr[j] = pix[j][wcs->lat]; } cpgline(9, ir, jr); } if (wcsprj->category == POLYCONIC) { step = 10.0; } else { step = 15.0; } /* Draw the native coordinate graticule faintly in the background. */ native.flag = -1; (void)wcscopy(1, wcs, &native); native.crval[wcs->lng] = 0.0; native.crval[wcs->lat] = 90.0; native.lonpole = 180.0; (void)wcsset(&native); cpgsci(8); /* Draw native meridians of longitude. */ for (ilng = -180; ilng <= 180; ilng += 15) { lng = (double)ilng; if (ilng == -180) lng = -179.99; if (ilng == 180) lng = 179.99; worldlng = world[0] + native.lng; worldlat = world[0] + native.lat; for (ilat = -90; ilat <= 90; ilat++) { *worldlng = lng; *worldlat = (double)ilat; worldlng += NELEM; worldlat += NELEM; } if (wcss2p(&native, 181, NELEM, world[0], phi, theta, img[0], pix[0], stat)) { continue; } k = 0; pixlng = pix[0] + native.lng; pixlat = pix[0] + native.lat; for (ilat = -90; ilat <= 90; ilat++) { if (ntvprj->category == QUADCUBE && k > 0) { if (fabs(*pixlng - ir[k-1]) > 2.0 || fabs(*pixlat - jr[k-1]) > 5.0) { if (k > 1) cpgline(k, ir, jr); k = 0; } } ir[k] = *pixlng; jr[k] = *pixlat; k++; pixlng += NELEM; pixlat += NELEM; } cpgline(k, ir, jr); } /* Draw native parallels of latitude. */ for (ilat = -90; ilat <= 90; ilat += 15) { lat = (double)ilat; worldlng = world[0] + native.lng; worldlat = world[0] + native.lat; for (ilng = -180; ilng <= 180; ilng++) { lng = (double)ilng; if (ilng == -180) lng = -179.99; if (ilng == 180) lng = 179.99; *worldlng = lng; *worldlat = lat; worldlng += NELEM; worldlat += NELEM; } if (wcss2p(&native, 361, NELEM, world[0], phi, theta, img[0], pix[0], stat)) { continue; } k = 0; pixlng = pix[0] + native.lng; pixlat = pix[0] + native.lat; for (ilng = -180; ilng <= 180; ilng++) { if (ntvprj->category == QUADCUBE && k > 0) { if (fabs(*pixlng - ir[k-1]) > 2.0 || fabs(*pixlat - jr[k-1]) > 5.0) { if (k > 1) cpgline(k, ir, jr); k = 0; } } ir[k] = *pixlng; jr[k] = *pixlat; k++; pixlng += NELEM; pixlat += NELEM; } cpgline(k, ir, jr); } /* Draw a colour-coded celestial coordinate graticule. */ ci = 1; /* Draw celestial meridians of longitude. */ for (ilng = -180; ilng <= 180; ilng += 15) { lng = (double)ilng; if (++ci > 7) ci = 2; cpgsci(ilng?ci:1); worldlng = world[0] + wcs->lng; worldlat = world[0] + wcs->lat; for (ilat = -90; ilat <= 90; ilat++) { lat = (double)ilat; *worldlng = lng; *worldlat = lat; worldlng += NELEM; worldlat += NELEM; } if (wcss2p(wcs, 181, NELEM, world[0], phi, theta, img[0], pix[0], stat)) { continue; } k = 0; pixlng = pix[0] + wcs->lng; pixlat = pix[0] + wcs->lat; for (ilat = -90; ilat <= 90; ilat++) { /* Test for discontinuities. */ if (k > 0) { if (fabs(*pixlng - ir[k-1]) > step || fabs(*pixlat - jr[k-1]) > step) { if (k > 1) cpgline(k, ir, jr); k = 0; } } ir[k] = *pixlng; jr[k] = *pixlat; k++; pixlng += NELEM; pixlat += NELEM; } cpgline(k, ir, jr); } /* Draw celestial parallels of latitude. */ ci = 1; for (ilat = -90; ilat <= 90; ilat += 15) { lat = (double)ilat; if (++ci > 7) ci = 2; cpgsci(ilat?ci:1); worldlng = world[0] + wcs->lng; worldlat = world[0] + wcs->lat; for (ilng = -180; ilng <= 180; ilng++) { lng = (double)ilng; *worldlng = lng; *worldlat = lat; worldlng += NELEM; worldlat += NELEM; } if (wcss2p(wcs, 361, NELEM, world[0], phi, theta, img[0], pix[0], stat)) { continue; } k = 0; pixlng = pix[0] + wcs->lng; pixlat = pix[0] + wcs->lat; for (ilng = -180; ilng <= 180; ilng++) { /* Test for discontinuities. */ if (k > 0) { if (fabs(*pixlng - ir[k-1]) > step || fabs(*pixlat - jr[k-1]) > step) { if (k > 1) cpgline(k, ir, jr); k = 0; } } ir[k] = *pixlng; jr[k] = *pixlat; k++; pixlng += NELEM; pixlat += NELEM; } cpgline(k, ir, jr); } /* Write a descriptive title. */ cpgsci(1); sprintf(text, "%s projection - 15 degree graticule", wcsprj->code); printf("\n\n%s\n", text); fjmin = jmin - 10.0; cpgtext(fimin, fjmin, text); sprintf(text, "centered on celestial coordinates (%6.2f,%6.2f)", wcscel->ref[0], wcscel->ref[1]); printf("%s\n", text); fjmin = jmin - 20.0; cpgtext(fimin, fjmin, text); sprintf(text, "with celestial pole at native coordinates (%7.2f,%7.2f)", wcscel->ref[2], wcscel->ref[3]); printf("%s\n", text); fjmin = jmin - 30.0; cpgtext(fimin, fjmin, text); cpgsci(2); return; } /*--------------------------------------------------------------------------*/ void parser(wcs) struct wcsprm *wcs; { int i, j, status; double *pcij; /* In practice a parser would read the FITS header until it encountered */ /* the NAXIS keyword which must occur near the start, before any of the */ /* WCS keywords. It would then use wcsini() to allocate memory for */ /* arrays in the wcsprm struct and set default values. In this */ /* simulation the header keyvalues are set as global variables. */ wcsini(1, NAXIS, wcs); /* Now the parser scans the FITS header, identifying WCS keywords and */ /* loading their values into the appropriate elements of the wcsprm */ /* struct. */ for (j = 0; j < NAXIS; j++) { wcs->crpix[j] = CRPIX[j]; } pcij = wcs->pc; for (i = 0; i < NAXIS; i++) { for (j = 0; j < NAXIS; j++) { *(pcij++) = PC[i][j]; } } for (i = 0; i < NAXIS; i++) { wcs->cdelt[i] = CDELT[i]; } for (i = 0; i < NAXIS; i++) { strcpy(wcs->ctype[i], &CTYPE[i][0]); } for (i = 0; i < NAXIS; i++) { wcs->crval[i] = CRVAL[i]; } wcs->lonpole = LONPOLE; wcs->latpole = LATPOLE; wcs->restfrq = RESTFRQ; wcs->restwav = RESTWAV; wcs->npv = NPV; for (i = 0; i < NPV; i++) { wcs->pv[i] = PV[i]; } /* Extract information from the FITS header. */ if ((status = wcsset(wcs))) { printf("wcsset ERROR%3d\n", status); } return; } pywcs-1.12/wcslib/C/test/twcssub.c0000644001153600020070000001272312310355626021135 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: twcssub.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * twcssub tests wcssub() which extracts the coordinate description for a * subimage from a wcsprm struct. * *---------------------------------------------------------------------------*/ #include #include #include #include /* In real life these would be encoded as FITS header keyrecords. */ const int NAXIS = 4; const double CRPIX[4] = { 1025.0, 64.0, 512.0, 513.0}; const double PC[4][4] = {{ 1.1, 0.0, 0.0, 0.0}, { 0.0, 1.0, 0.0, 0.0}, { 0.0, 0.0, 1.0, 0.1}, { 0.0, 0.0, 0.2, 1.0}}; const double CDELT[4] = {-9.2e-6, 10.0, 1.0, -1.0}; char CUNIT[4][16] = {"m", "s", "deg", "deg"}; char CTYPE[4][16] = {"WAVE-F2W", "TIME", "XLAT-SZP", "XLON-SZP"}; const double CRVAL[4] = {0.214982042, -2e3, -30.0, 150.0}; const double LONPOLE = 150.0; const double LATPOLE = 999.0; const double RESTFRQ = 1.42040575e9; const double RESTWAV = 0.0; char CNAME[4][16] = {"Wavelength", "Time", "Latitude", "Longitude"}; int NPS, NPV; struct pvcard PV[10]; struct pscard PS[10]; int main() { int axes[4], i, j, nsub, status; struct wcsprm wcs, wcsext; double *pcij; PV[0].i = 1; /* Frequency on axis 1. */ PV[0].m = 1; /* Parameter number 1. */ PV[0].value = -1.0; /* PV1_1. */ PV[1].i = 3; /* Latitude on axis 3. */ PV[1].m = 1; /* Parameter number 1. */ PV[1].value = 2.0; /* PV3_1. */ PV[2].i = 3; /* Latitude on axis 3. */ PV[2].m = 2; /* Parameter number 2. */ PV[2].value = 210.0; /* PV3_2. */ PV[3].i = 3; /* Latitude on axis 3. */ PV[3].m = 3; /* Parameter number 3. */ PV[3].value = 60.0; /* PV3_3. */ NPV = 4; PS[0].i = 2; /* Time on axis 2. */ PS[0].m = 1; /* Parameter number 1. */ strcpy(PS[0].value, "UTC"); /* PS2_1. */ NPS = 1; wcs.flag = -1; wcsini(1, NAXIS, &wcs); for (j = 0; j < NAXIS; j++) { wcs.crpix[j] = CRPIX[j]; } pcij = wcs.pc; for (i = 0; i < NAXIS; i++) { for (j = 0; j < NAXIS; j++) { *(pcij++) = PC[i][j]; } } for (i = 0; i < NAXIS; i++) { wcs.cdelt[i] = CDELT[i]; } for (i = 0; i < NAXIS; i++) { strcpy(wcs.cunit[i], &CUNIT[i][0]); strcpy(wcs.ctype[i], &CTYPE[i][0]); strcpy(wcs.cname[i], &CNAME[i][0]); } for (i = 0; i < NAXIS; i++) { wcs.crval[i] = CRVAL[i]; } wcs.lonpole = LONPOLE; wcs.latpole = LATPOLE; wcs.restfrq = RESTFRQ; wcs.restwav = RESTWAV; wcs.npv = NPV; for (i = 0; i < NPV; i++) { wcs.pv[i] = PV[i]; } wcs.nps = NPS; for (i = 0; i < NPS; i++) { wcs.ps[i] = PS[i]; } /* Initialize the wcsprm struct. */ wcserr_enable(1); (void) wcsset(&wcs); printf("Testing WCSLIB subimage extraction routine (twcssub.c)\n" "------------------------------------------------------\n"); printf("\nInitial contents of wcsprm struct:\n"); wcsprt(&wcs); /* Extract the coordinate description for a subimage and add a new axis. */ nsub = 4; wcsext.flag = -1; axes[0] = WCSSUB_LONGITUDE; axes[1] = WCSSUB_LATITUDE; axes[2] = -(WCSSUB_SPECTRAL | WCSSUB_STOKES); axes[3] = 0; printf("\n\nExtracted contents of wcsprm struct:\n"); if (wcssub(1, &wcs, &nsub, axes, &wcsext)) { wcsperr(&wcsext, ""); } else if (nsub == 0) { printf("None of the requested subimage axes were found.\n"); } else if (wcsset(&wcsext)) { wcsperr(&wcsext, ""); } else { wcsprt(&wcsext); } /* Set it up for failure by setting PC1_3 non-zero. */ *(wcs.pc+2) = 1.0; nsub = 2; axes[0] = 4; axes[1] = 3; status = wcssub(1, &wcs, &nsub, axes, &wcsext); if (status == WCSERR_NON_SEPARABLE) { printf("\n\nReceived wcssub status %d as expected for a non-separable " "subimage\ncoordinate system.\n", WCSERR_NON_SEPARABLE); } else { printf("\n\nERROR: expected wcssub status %d for a non-separable " "subimage coordinate\nsystem, but received status %d instead.\n", WCSERR_NON_SEPARABLE, status); } wcsfree(&wcs); wcsfree(&wcsext); return 0; } pywcs-1.12/wcslib/C/test/twcstab.c0000644001153600020070000003057712310355625021120 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: twcstab.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * twcstab tests wcstab() and also provides sample code for using it in * conjunction with wcspih() and fits_read_wcstab(). Although this example * and fits_read_wcstab() are based on the CFITSIO library, wcstab() itself * is completely independent of it. * * The input FITS file is constructed by create_input() from a list of header * keyrecords in wcstab.keyrec together with some hard-coded parameters. The * output fits file, wcstab.fits, is left for inspection. * *===========================================================================*/ #include #include #include #include #include #include int create_input(); int do_wcs_stuff(fitsfile *fptr, struct wcsprm *wcs); double lcprng(); int main() { char *header; int i, nkeyrec, nreject, nwcs, stat[NWCSFIX], status = 0; fitsfile *fptr; struct wcsprm *wcs; /* Set line buffering in case stdout is redirected to a file, otherwise * stdout and stderr messages will be jumbled (stderr is unbuffered). */ setvbuf(stdout, NULL, _IOLBF, 0); printf("Testing -TAB interpreter (twcstab.c)\n" "------------------------------------\n\n"); /* Create the input FITS test file. */ if (create_input()) { fprintf(stderr, "Failed to create FITS test file."); return 1; } /* Open the FITS test file and read the primary header. */ fits_open_file(&fptr, "wcstab.fits", READONLY, &status); if ((status = fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status))) { fits_report_error(stderr, status); return 1; } /*-----------------------------------------------------------------------*/ /* Basic steps required to interpret a FITS WCS header, including -TAB. */ /*-----------------------------------------------------------------------*/ /* Parse the primary header of the FITS file. */ if ((status = wcspih(header, nkeyrec, WCSHDR_all, 2, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status,wcshdr_errmsg[status]); } /* Read coordinate arrays from the binary table extension. */ if ((status = fits_read_wcstab(fptr, wcs->nwtb, (wtbarr *)wcs->wtb, &status))) { fits_report_error(stderr, status); return 1; } /* Translate non-standard WCS keyvalues. */ if ((status = wcsfix(7, 0, wcs, stat))) { for (i = 0; i < NWCSFIX; i++) { if (stat[i] > 0) { fprintf(stderr, "wcsfix ERROR %d: %s.\n", status, wcsfix_errmsg[stat[i]]); } } return 1; } /*-----------------------------------------------------------------------*/ /* The wcsprm struct is now ready for use. */ /*-----------------------------------------------------------------------*/ /* Do something with it. */ do_wcs_stuff(fptr, wcs); /* Finished with the FITS file. */ fits_close_file(fptr, &status); free(header); /* Clean up. */ status = wcsvfree(&nwcs, &wcs); return 0; } /*--------------------------------------------------------------------------*/ /* The celestial plane is 256 x 128 with the table indexed at every fourth */ /* pixel on each axis, but the image is rotated by 5 deg so the table needs */ /* to be a bit wider than 65 x 33. */ #define K1 70L #define K2 40L int create_input() { const double TWOPI = 2.0 * 3.14159265358979323846; /* These must match wcstab.keyrec. */ const char infile[] = "test/wcstab.keyrec"; const long NAXIS1 = 256; const long NAXIS2 = 128; const long NAXIS3 = 4; const char *ttype1[3] = {"CelCoords", "RAIndex", "DecIndex"}; const char *tform1[3] = {"5600E", "70E", "40E"}; const char *tunit1[3] = {"deg", "", ""}; const char *ttype2[4] = {"WaveIndex", "WaveCoord", "TimeIndex", "TimeCoord"}; const char *tform2[4] = {"8E", "8D", "8E", "8D"}; const char *tunit2[4] = {"", "m", "", "a"}; /* The remaining parameters may be chosen at will. */ float refval[] = {150.0f, -30.0f}; float span[] = {5.0f, (5.0f*K2)/K1}; float sigma[] = {0.10f, 0.05f}; double wcoord[] = {0.21106114, 0.21076437, 2.0e-6, 2.2e-6, 500.0e-9, 650.0e-9, 1.24e-9, 2.48e-9}; double windex[] = {0.5, 1.5, 1.5, 2.5, 2.5, 3.5, 3.5, 4.5}; double tcoord[] = {1997.84512, 1997.84631, 1993.28451, 1993.28456, 2001.59234, 2001.59239, 2002.18265, 2002.18301}; double tindex[] = {0.0, 1.0, 1.0, 2.0, 2.0, 3.0, 3.0, 4.0}; char keyrec[84]; int i, status; long dummy, firstelem, k1, k2, p1, p2, p3; float array[2*K1*K2], *fp, image[256]; double s, t, x1, x2, z, z1, z2; FILE *stream; fitsfile *fptr; /* Look for the input header keyrecords. */ if ((stream = fopen(infile+5, "r")) == 0x0) { if ((stream = fopen(infile, "r")) == 0x0) { printf("ERROR opening %s\n", infile); return 1; } } /* Create the FITS output file, deleting any pre-existing file. */ status = 0; fits_create_file(&fptr, "!wcstab.fits", &status); /* Convert header keyrecords to FITS. */ while (fgets(keyrec, 82, stream) != NULL) { /* Ignore meta-comments (copyright information, etc.). */ if (keyrec[0] == '#') continue; /* Strip off the newline. */ i = strlen(keyrec) - 1; if (keyrec[i] == '\n') keyrec[i] = '\0'; fits_write_record(fptr, keyrec, &status); } /* Create and write some phoney image data. */ firstelem = 1; for (p3 = 0; p3 < NAXIS3; p3++) { for (p2 = 0; p2 < NAXIS2; p2++) { fp = image; s = (p3 + 1) * cos(0.2 * p2); t = cos(0.8*p2); for (p1 = 0; p1 < NAXIS1; p1++) { /* Do not adjust your set! */ *(fp++) = sin(0.1*(p1+p2) + s) * cos(0.4*p1) * t; } fits_write_img_flt(fptr, 0L, firstelem, NAXIS1, image, &status); firstelem += NAXIS1; } } /* Add the first binary table extension. */ fits_create_tbl(fptr, BINARY_TBL, 1L, 3L, (char **)ttype1, (char **)tform1, (char **)tunit1, NULL, &status); /* Write EXTNAME and EXTVER near the top, after TFIELDS. */ fits_read_key_lng(fptr, "TFIELDS", &dummy, NULL, &status); fits_insert_key_str(fptr, "EXTNAME", "WCS-TABLE", "WCS Coordinate lookup table", &status); fits_insert_key_lng(fptr, "EXTVER", 1L, "Table number 1", &status); /* Write the TDIM1 keyrecord after TFORM1. */ fits_read_key_str(fptr, "TFORM1", keyrec, NULL, &status); sprintf(keyrec, "(2,%ld,%ld)", K1, K2); fits_insert_key_str(fptr, "TDIM1", keyrec, "Dimensions of 3-D array", &status); /* Plate carrée projection with a bit of noise for the sake of realism. */ fp = array; for (k2 = 0; k2 < K2; k2++) { for (k1 = 0; k1 < K1; k1++) { /* Box-Muller transformation: uniform -> normal distribution. */ x1 = lcprng(); x2 = lcprng(); if (x1 == 0.0) x1 = 1.0; z = sqrt(-2.0 * log(x1)); x2 *= TWOPI; z1 = z * cos(x2); z2 = z * sin(x2); *(fp++) = refval[0] + span[0] * (k1/(K1-1.0) - 0.5) + z1 * sigma[0]; *(fp++) = refval[1] + span[1] * (k2/(K2-1.0) - 0.5) + z2 * sigma[1]; } } fits_write_col_flt(fptr, 1, 1L, 1L, 2*K1*K2, array, &status); fp = array; for (k1 = 0; k1 < K1; k1++) { *(fp++) = 4.0f * k1; } fits_write_col_flt(fptr, 2, 1L, 1L, K1, array, &status); fp = array; for (k2 = 0; k2 < K2; k2++) { *(fp++) = 4.0f * k2; } fits_write_col_flt(fptr, 3, 1L, 1L, K2, array, &status); /* Add the second binary table extension. */ if (fits_create_tbl(fptr, BINARY_TBL, 1L, 4L, (char **)ttype2, (char **)tform2, (char **)tunit2, NULL, &status)) { fits_report_error(stderr, status); return 1; } /* Write EXTNAME and EXTVER near the top, after TFIELDS. */ fits_read_key_lng(fptr, "TFIELDS", &dummy, NULL, &status); fits_insert_key_str(fptr, "EXTNAME", "WCS-TABLE", "WCS Coordinate lookup table", &status); fits_insert_key_lng(fptr, "EXTVER", 2L, "Table number 2", &status); /* Write the TDIM2 keyrecord after TFORM2. */ fits_read_key_str(fptr, "TFORM2", keyrec, NULL, &status); fits_insert_key_str(fptr, "TDIM2", "(1,8)", "Dimensions of 2-D array", &status); /* Write the TDIM4 keyrecord after TFORM4. */ fits_read_key_str(fptr, "TFORM4", keyrec, NULL, &status); fits_insert_key_str(fptr, "TDIM4", "(1,8)", "Dimensions of 2-D array", &status); fits_write_col_dbl(fptr, 1, 1L, 1L, 8L, windex, &status); fits_write_col_dbl(fptr, 2, 1L, 1L, 8L, wcoord, &status); fits_write_col_dbl(fptr, 3, 1L, 1L, 8L, tindex, &status); fits_write_col_dbl(fptr, 4, 1L, 1L, 8L, tcoord, &status); fits_close_file(fptr, &status); if (status) { fits_report_error(stderr, status); return 1; } return 0; } /*--------------------------------------------------------------------------*/ /* A simple linear congruential pseudo-random number generator that produces * the same results on all systems so that the test output can be compared. * It produces a fixed sequence of uniformly distributed numbers in [0,1]. * Adapted from the example in Numerical Recipes in C. */ double lcprng() { static unsigned long next = 137UL; next = next * 1664525UL + 1013904223UL; return (double)(next % 1073741824UL) / 1073741823.0; } /*--------------------------------------------------------------------------*/ int do_wcs_stuff(fitsfile *fptr, struct wcsprm *wcs) { int i1, i2, i3, k, naxis1, naxis2, naxis3, stat[8], status; double phi[8], pixcrd[8][4], imgcrd[8][4], theta[8], world[8][4], x1, x2, x3; /* Initialize the wcsprm struct, also taking control of memory allocated by * fits_read_wcstab(). */ if ((status = wcsset(wcs))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); return 1; } /* Print the struct. */ if ((status = wcsprt(wcs))) return status; /* Compute coordinates in the corners. */ fits_read_key(fptr, TINT, "NAXIS1", &naxis1, NULL, &status); fits_read_key(fptr, TINT, "NAXIS2", &naxis2, NULL, &status); fits_read_key(fptr, TINT, "NAXIS3", &naxis3, NULL, &status); k = 0; x3 = 1.0f; for (i3 = 0; i3 < 2; i3++) { x2 = 0.5f; for (i2 = 0; i2 < 2; i2++) { x1 = 0.5f; for (i1 = 0; i1 < 2; i1++) { pixcrd[k][0] = x1; pixcrd[k][1] = x2; pixcrd[k][2] = x3; pixcrd[k][3] = 1.0f; k++; x1 = naxis1 + 0.5f; } x2 = naxis2 + 0.5f; } x3 = naxis3; } if ((status = wcsp2s(wcs, 8, 4, pixcrd[0], imgcrd[0], phi, theta, world[0], stat))) { fprintf(stderr, "\n\nwcsp2s ERROR %d: %s.\n", status, wcs_errmsg[status]); /* Invalid pixel coordinates. */ if (status == 8) status = 0; } if (status == 0) { printf("\n\nCorner world coordinates:\n" " Pixel World\n"); for (k = 0; k < 8; k++) { printf(" (%5.1f,%6.1f,%4.1f,%4.1f) -> (%7.3f,%8.3f,%9g,%11.5f)", pixcrd[k][0], pixcrd[k][1], pixcrd[k][2], pixcrd[k][3], world[k][0], world[k][1], world[k][2], world[k][3]); if (stat[k]) printf(" (BAD)"); printf("\n"); } } return 0; } pywcs-1.12/wcslib/C/test/units_test0000644001153600020070000000016112310355626021414 0ustar cslocumSTSCI\science00000000000000km/h m/ms JY/BEAM (kg/s^2)/beam KM/SEC m/s KM/H M/S log(MHZ) ln(/s) DEG ARCMINS ARCSEC sqrt(HZ^2) Jy Volts pywcs-1.12/wcslib/C/test/wcstab.keyrec0000644001153600020070000001605012310355626021763 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # # WCSLIB 4.10 - an implementation of the FITS WCS standard. # Copyright (C) 1995-2012, Mark Calabretta # # This file is part of WCSLIB. # # WCSLIB is free software: you can redistribute it and/or modify it under the # terms of the GNU Lesser General Public License as published by the Free # Software Foundation, either version 3 of the License, or (at your option) # any later version. # # WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY # WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS # FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for # more details. # # You should have received a copy of the GNU Lesser General Public License # along with WCSLIB. If not, see . # # Correspondence concerning WCSLIB may be directed to: # Internet email: mcalabre@atnf.csiro.au # Postal address: Dr. Mark Calabretta # Australia Telescope National Facility, CSIRO # PO Box 76 # Epping NSW 1710 # AUSTRALIA # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: wcstab.keyrec,v 4.10 2012/02/05 23:41:44 cal103 Exp $ #----------------------------------------------------------------------------- # List of FITS header keyrecords used by 'twcstab' to construct a FITS file # for testing wcstab() and fits_read_wcstab(). The coordinate arrays and # index vectors in the binary tables extensions are generated by twcstab # itself. # # Lines in this file beginning with '#' are ignored by twcstab. #----------------------------------------------------------------------------- SIMPLE = T / Standards-conformant FITS format BITPIX = -32 / IEEE single precision floating point NAXIS = 4 / Four image axes NAXIS1 = 256 / Length of 1st image axis - fastest varying NAXIS2 = 128 / Length of 2nd image axis NAXIS3 = 4 / Length of 3rd image axis NAXIS4 = 1 / Length of 4th image axis - slowest varying EXTEND = T / Binary table extensions contain lookup tables. COMMENT ----------------------------------------------------------------------- COMMENT Of the four -TAB coordinate axes, the first two celestial axes are COMMENT associated with a 2-D lookup table; the third spectral axis contains COMMENT a list of four wavelengths in the radio, infrared, optical, and x-ray COMMENT regimes; and the fourth time axis contains a list of observation COMMENT dates. Axes 3 and 4 are adapted from Table 11 of WCS Paper III. COMMENT COMMENT There are two separate bintables holding the -TAB arrays that differ COMMENT only in EXTVER. The first holds the 2-D celestial table, and the COMMENT second holds the two 1-D spectral and time coordinate tables. COMMENT ----------------------------------------------------------------------- WCSAXES = 4 / Four coordinate axes WCSNAME = '-TAB test file' / Name of this system CRPIX1 = 129.0 / Pixel coordinate of reference point CRPIX2 = 65.0 / Pixel coordinate of reference point PC1_1 = 0.996194698 / 5 deg rotation matrix element PC1_2 = 0.087155743 / 5 deg rotation matrix element PC2_1 = -0.087155743 / 5 deg rotation matrix element PC2_2 = 0.996194698 / 5 deg rotation matrix element CDELT1 = 1.0 / Index (psi_m) changes by one per pixel CDELT2 = 1.0 / Index (psi_m) changes by one per pixel CRVAL1 = 136.0 / Table index (Psi_m) at the reference point CRVAL2 = 76.0 / Table index (Psi_m) at the reference point CTYPE1 = 'RA---TAB' / Right ascension in lookup table CUNIT1 = 'deg' / Right ascension units CNAME1 = 'Right ascension (J2000)' / Axis name for labelling purposes PS1_0 = 'WCS-TABLE' / EXTNAME of bintable extension for -TAB arrays PV1_1 = 1 / EXTVER of bintable extension for -TAB arrays PV1_2 = 1 / EXTLEVEL of bintable extension for -TAB arrays PS1_1 = 'CelCoords' / Celestial coordinate array PS1_2 = 'RAIndex' / Right ascension index vector PV1_3 = 1 / Axis number in coordinate array CTYPE2 = 'DEC--TAB' / Declination in a slant zenithal projection CUNIT2 = 'deg' / Declination units CNAME2 = 'Declination (J2000)' / Axis name for labelling purposes PS2_0 = 'WCS-TABLE' / EXTNAME of bintable extension for -TAB arrays PV2_1 = 1 / EXTVER of bintable extension for -TAB arrays PV2_2 = 1 / EXTLEVEL of bintable extension for -TAB arrays PS2_1 = 'CelCoords' / Celestial coordinate array PS2_2 = 'DecIndex' / Declination index vector PV2_3 = 2 / Axis number in coordinate array RADESYS = 'FK5' / Mean equatorial coordinates, IAU 1984 system EQUINOX = 2000.0 / [yr] Equinox of equatorial coordinates CRPIX3 = 0.5 / Spectral bin initial edge of initial pixel CRPIX4 = 1.0 / Temporal bins are at begin/end time PC3_3 = 1.0 / Linear transformation matrix element PC3_4 = 0.0 / Linear transformation matrix element PC4_3 = 1.0 / Linear transformation matrix element PC4_4 = 1.0 / Linear transformation matrix element CDELT3 = 1.0 / Index (psi_m) changes by one per pixel CDELT4 = 1.0 / Index (psi_m) changes by one per pixel CRVAL3 = 0.5 / Table index (Psi_m) at the reference point CRVAL4 = 0.0 / Table index (Psi_m) at the reference point CTYPE3 = 'WAVE-TAB' / Wavelength axis by lookup table CUNIT3 = 'm' / Wavelength in metres CNAME3 = 'Wavelength' / Axis name for labelling purposes PS3_0 = 'WCS-TABLE' / EXTNAME of bintable extension for -TAB arrays PV3_1 = 2 / EXTVER of bintable extension for -TAB arrays PV3_2 = 1 / EXTLEVEL of bintable extension for -TAB arrays PS3_1 = 'WaveCoord' / Wavelength coordinate array PS3_2 = 'WaveIndex' / Wavelength index vector PV3_3 = 1 / Axis number in coordinate array CTYPE4 = 'TIME-TAB' / Time axis by lookup table CUNIT4 = 'a' / Time in years CNAME4 = 'Observation date' / Axis name for labelling purposes PS4_0 = 'WCS-TABLE' / EXTNAME of bintable extension for -TAB arrays PV4_1 = 2 / EXTVER of bintable extension for -TAB arrays PV4_2 = 1 / EXTLEVEL of bintable extension for -TAB arrays PS4_1 = 'TimeCoord' / Time coordinate array PS4_2 = 'TimeIndex' / Time index vector PV4_3 = 1 / Axis number in coordinate array END pywcs-1.12/wcslib/C/wcs.c0000644001153600020070000025161612310355626017266 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcs.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsprintf.h" #include "wcstrig.h" #include "wcsunits.h" #include "wcsutil.h" #include "lin.h" #include "log.h" #include "spc.h" #include "prj.h" #include "sph.h" #include "cel.h" #include "tab.h" #include "wcs.h" const int WCSSET = 137; /* Maximum number of PVi_ma and PSi_ma keywords. */ int NPVMAX = 64; int NPSMAX = 8; /* Map status return value to message. */ const char *wcs_errmsg[] = { "Success", "Null wcsprm pointer passed", "Memory allocation failed", "Linear transformation matrix is singular", "Inconsistent or unrecognized coordinate axis types", "Invalid parameter value", "Invalid coordinate transformation parameters", "Ill-conditioned coordinate transformation parameters", "One or more of the pixel coordinates were invalid", "One or more of the world coordinates were invalid", "Invalid world coordinate", "No solution found in the specified interval", "Invalid subimage specification", "Non-separable subimage coordinate system"}; /* Convenience macro for invoking wcserr_set(). */ #define WCS_ERRMSG(status) WCSERR_SET(status), wcs_errmsg[status] #ifndef signbit #define signbit(X) ((X) < 0.0 ? 1 : 0) #endif /* Internal helper functions, not for general use. */ static int wcs_types(struct wcsprm *); static int wcs_units(struct wcsprm *); /*--------------------------------------------------------------------------*/ int wcsnpv(int npvmax) { if (npvmax >= 0) NPVMAX = npvmax; return NPVMAX; } int wcsnps(int npsmax) { if (npsmax >= 0) NPSMAX = npsmax; return NPSMAX; } /*--------------------------------------------------------------------------*/ int wcsini(int alloc, int naxis, struct wcsprm *wcs) { static const char *function = "wcsini"; int i, j, k, status; double *cd; struct wcserr **err; if (wcs == 0x0) return WCSERR_NULL_POINTER; /* Initialize error message handling. */ err = &(wcs->err); if (wcs->flag != -1) { if (wcs->err) free(wcs->err); if (wcs->lin.err) free(wcs->lin.err); if (wcs->cel.err) free(wcs->cel.err); if (wcs->spc.err) free(wcs->spc.err); if (wcs->cel.prj.err) free(wcs->cel.prj.err); } wcs->err = 0x0; wcs->lin.err = 0x0; wcs->cel.err = 0x0; wcs->spc.err = 0x0; wcs->cel.prj.err = 0x0; /* Initialize pointers. */ if (wcs->flag == -1 || wcs->m_flag != WCSSET) { if (wcs->flag == -1) { wcs->types = 0x0; wcs->lin.flag = -1; wcs->tab = 0x0; } /* Initialize memory management. */ wcs->m_flag = 0; wcs->m_naxis = 0; wcs->m_crpix = 0x0; wcs->m_pc = 0x0; wcs->m_cdelt = 0x0; wcs->m_crval = 0x0; wcs->m_cunit = 0x0; wcs->m_ctype = 0x0; wcs->m_pv = 0x0; wcs->m_ps = 0x0; wcs->m_cd = 0x0; wcs->m_crota = 0x0; wcs->m_colax = 0x0; wcs->m_cname = 0x0; wcs->m_crder = 0x0; wcs->m_csyer = 0x0; wcs->m_tab = 0x0; wcs->m_wtb = 0x0; } if (naxis <= 0) { return wcserr_set(WCSERR_SET(WCSERR_MEMORY), "naxis must be positive (got %d)", naxis); } /* Allocate memory for arrays if required. */ if (alloc || wcs->crpix == 0x0 || wcs->pc == 0x0 || wcs->cdelt == 0x0 || wcs->crval == 0x0 || wcs->cunit == 0x0 || wcs->ctype == 0x0 || (NPVMAX && wcs->pv == 0x0) || (NPSMAX && wcs->ps == 0x0) || wcs->cd == 0x0 || wcs->crota == 0x0 || wcs->colax == 0x0 || wcs->cname == 0x0 || wcs->crder == 0x0 || wcs->csyer == 0x0) { /* Was sufficient allocated previously? */ if (wcs->m_flag == WCSSET && (wcs->m_naxis < naxis || wcs->npvmax < NPVMAX || wcs->npsmax < NPSMAX)) { /* No, free it. */ wcsfree(wcs); } if (alloc || wcs->crpix == 0x0) { if (wcs->m_crpix) { /* In case the caller fiddled with it. */ wcs->crpix = wcs->m_crpix; } else { if (!(wcs->crpix = calloc(naxis, sizeof(double)))) { return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_crpix = wcs->crpix; } } if (alloc || wcs->pc == 0x0) { if (wcs->m_pc) { /* In case the caller fiddled with it. */ wcs->pc = wcs->m_pc; } else { if (!(wcs->pc = calloc(naxis*naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_pc = wcs->pc; } } if (alloc || wcs->cdelt == 0x0) { if (wcs->m_cdelt) { /* In case the caller fiddled with it. */ wcs->cdelt = wcs->m_cdelt; } else { if (!(wcs->cdelt = calloc(naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_cdelt = wcs->cdelt; } } if (alloc || wcs->crval == 0x0) { if (wcs->m_crval) { /* In case the caller fiddled with it. */ wcs->crval = wcs->m_crval; } else { if (!(wcs->crval = calloc(naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_crval = wcs->crval; } } if (alloc || wcs->cunit == 0x0) { if (wcs->m_cunit) { /* In case the caller fiddled with it. */ wcs->cunit = wcs->m_cunit; } else { if (!(wcs->cunit = calloc(naxis, sizeof(char [72])))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_cunit = wcs->cunit; } } if (alloc || wcs->ctype == 0x0) { if (wcs->m_ctype) { /* In case the caller fiddled with it. */ wcs->ctype = wcs->m_ctype; } else { if (!(wcs->ctype = calloc(naxis, sizeof(char [72])))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_ctype = wcs->ctype; } } if (alloc || wcs->pv == 0x0) { if (wcs->m_pv) { /* In case the caller fiddled with it. */ wcs->pv = wcs->m_pv; } else { if (NPVMAX) { if (!(wcs->pv = calloc(NPVMAX, sizeof(struct pvcard)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } } else { wcs->pv = (struct pvcard *)0; } wcs->npvmax = NPVMAX; wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_pv = wcs->pv; } } if (alloc || wcs->ps == 0x0) { if (wcs->m_ps) { /* In case the caller fiddled with it. */ wcs->ps = wcs->m_ps; } else { if (NPSMAX) { if (!(wcs->ps = calloc(NPSMAX, sizeof(struct pscard)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } } else { wcs->ps = (struct pscard *)0; } wcs->npsmax = NPSMAX; wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_ps = wcs->ps; } } if (alloc || wcs->cd == 0x0) { if (wcs->m_cd) { /* In case the caller fiddled with it. */ wcs->cd = wcs->m_cd; } else { if (!(wcs->cd = calloc(naxis*naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_cd = wcs->cd; } } if (alloc || wcs->crota == 0x0) { if (wcs->m_crota) { /* In case the caller fiddled with it. */ wcs->crota = wcs->m_crota; } else { if (!(wcs->crota = calloc(naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_crota = wcs->crota; } } if (alloc || wcs->colax == 0x0) { if (wcs->m_colax) { /* In case the caller fiddled with it. */ wcs->colax = wcs->m_colax; } else { if (!(wcs->colax = calloc(naxis, sizeof(int)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_colax = wcs->colax; } } if (alloc || wcs->cname == 0x0) { if (wcs->m_cname) { /* In case the caller fiddled with it. */ wcs->cname = wcs->m_cname; } else { if (!(wcs->cname = calloc(naxis, sizeof(char [72])))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_cname = wcs->cname; } } if (alloc || wcs->crder == 0x0) { if (wcs->m_crder) { /* In case the caller fiddled with it. */ wcs->crder = wcs->m_crder; } else { if (!(wcs->crder = calloc(naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_crder = wcs->crder; } } if (alloc || wcs->csyer == 0x0) { if (wcs->m_csyer) { /* In case the caller fiddled with it. */ wcs->csyer = wcs->m_csyer; } else { if (!(wcs->csyer = calloc(naxis, sizeof(double)))) { wcsfree(wcs); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } wcs->m_flag = WCSSET; wcs->m_naxis = naxis; wcs->m_csyer = wcs->csyer; } } } wcs->flag = 0; wcs->naxis = naxis; /* Set defaults for the linear transformation. */ wcs->lin.crpix = wcs->crpix; wcs->lin.pc = wcs->pc; wcs->lin.cdelt = wcs->cdelt; wcs->lin.m_flag = 0; if ((status = linini(0, naxis, &(wcs->lin)))) { return wcserr_set(WCS_ERRMSG(status)); } /* CRVALia defaults to 0.0. */ for (i = 0; i < naxis; i++) { wcs->crval[i] = 0.0; } /* CUNITia and CTYPEia are blank by default. */ for (i = 0; i < naxis; i++) { memset(wcs->cunit[i], 0, 72); memset(wcs->ctype[i], 0, 72); } /* Set defaults for the celestial transformation parameters. */ wcs->lonpole = UNDEFINED; wcs->latpole = +90.0; /* Set defaults for the spectral transformation parameters. */ wcs->restfrq = 0.0; wcs->restwav = 0.0; /* Default parameter values. */ wcs->npv = 0; for (k = 0; k < wcs->npvmax; k++) { wcs->pv[k].i = 0; wcs->pv[k].m = 0; wcs->pv[k].value = 0.0; } wcs->nps = 0; for (k = 0; k < wcs->npsmax; k++) { wcs->ps[k].i = 0; wcs->ps[k].m = 0; memset(wcs->ps[k].value, 0, 72); } /* Defaults for alternate linear transformations. */ cd = wcs->cd; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++) { *(cd++) = 0.0; } } for (i = 0; i < naxis; i++) { wcs->crota[i] = 0.0; } wcs->altlin = 0; wcs->velref = 0; /* Defaults for auxiliary coordinate system information. */ memset(wcs->alt, 0, 4); wcs->alt[0] = ' '; wcs->colnum = 0; memset(wcs->wcsname, 0, 72); for (i = 0; i < naxis; i++) { wcs->colax[i] = 0; memset(wcs->cname[i], 0, 72); wcs->crder[i] = UNDEFINED; wcs->csyer[i] = UNDEFINED; } memset(wcs->radesys, 0, 72); wcs->equinox = UNDEFINED; memset(wcs->specsys, 0, 72); memset(wcs->ssysobs, 0, 72); wcs->velosys = UNDEFINED; memset(wcs->ssyssrc, 0, 72); wcs->zsource = UNDEFINED; wcs->obsgeo[0] = UNDEFINED; wcs->obsgeo[1] = UNDEFINED; wcs->obsgeo[2] = UNDEFINED; memset(wcs->dateobs, 0, 72); memset(wcs->dateavg, 0, 72); wcs->mjdobs = UNDEFINED; wcs->mjdavg = UNDEFINED; wcs->ntab = 0; wcs->tab = 0x0; wcs->nwtb = 0; wcs->wtb = 0x0; /* Reset derived values. */ strcpy(wcs->lngtyp, " "); strcpy(wcs->lattyp, " "); wcs->lng = -1; wcs->lat = -1; wcs->spec = -1; wcs->cubeface = -1; celini(&(wcs->cel)); spcini(&(wcs->spc)); return 0; } /*--------------------------------------------------------------------------*/ int wcssub( int alloc, const struct wcsprm *wcssrc, int *nsub, int axes[], struct wcsprm *wcsdst) { static const char *function = "wcssub"; char *c, ctypei[16]; int axis, cubeface, dealloc, dummy, i, itab, j, k, latitude, longitude, m, *map = 0x0, msub, naxis, npv, nps, other, spectral, status, stokes; const double *srcp; double *dstp; struct tabprm *tabp; struct wcserr **err; if (wcssrc == 0x0) return WCSERR_NULL_POINTER; err = &(wcsdst->err); if ((naxis = wcssrc->naxis) <= 0) { return wcserr_set(WCSERR_SET(WCSERR_MEMORY), "naxis must be positive (got %d)", naxis); } if (!(map = calloc(naxis, sizeof(int)))) { return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } if (nsub == 0x0) { nsub = &dummy; *nsub = naxis; } else if (*nsub == 0) { *nsub = naxis; } if ((dealloc = (axes == 0x0))) { /* Construct an index array. */ if (!(axes = calloc(naxis, sizeof(int)))) { free(map); return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } for (i = 0; i < naxis; i++) { axes[i] = i+1; } } /* So that we don't try to free an uninitialized pointer on cleanup. */ wcsdst->m_tab = 0x0; msub = 0; for (j = 0; j < *nsub; j++) { axis = axes[j]; if (abs(axis) > 0x1000) { /* Subimage extraction by type. */ k = abs(axis) & 0xFF; longitude = k & WCSSUB_LONGITUDE; latitude = k & WCSSUB_LATITUDE; cubeface = k & WCSSUB_CUBEFACE; spectral = k & WCSSUB_SPECTRAL; stokes = k & WCSSUB_STOKES; if ((other = (axis < 0))) { longitude = !longitude; latitude = !latitude; cubeface = !cubeface; spectral = !spectral; stokes = !stokes; } for (i = 0; i < naxis; i++) { strncpy (ctypei, (char *)(wcssrc->ctype + i), 8); ctypei[8] = '\0'; /* Find the last non-blank character. */ c = ctypei + 8; while (c-- > ctypei) { if (*c == ' ') *c = '\0'; if (*c != '\0') break; } if ( strcmp(ctypei, "RA") == 0 || strcmp(ctypei+1, "LON") == 0 || strcmp(ctypei+2, "LN") == 0 || strncmp(ctypei, "RA---", 5) == 0 || strncmp(ctypei+1, "LON-", 4) == 0 || strncmp(ctypei+2, "LN-", 3) == 0) { if (!longitude) { continue; } } else if ( strcmp(ctypei, "DEC") == 0 || strcmp(ctypei+1, "LAT") == 0 || strcmp(ctypei+2, "LT") == 0 || strncmp(ctypei, "DEC--", 5) == 0 || strncmp(ctypei+1, "LAT-", 4) == 0 || strncmp(ctypei+2, "LT-", 3) == 0) { if (!latitude) { continue; } } else if (strcmp(ctypei, "CUBEFACE") == 0) { if (!cubeface) { continue; } } else if (( strncmp(ctypei, "FREQ", 4) == 0 || strncmp(ctypei, "ENER", 4) == 0 || strncmp(ctypei, "WAVN", 4) == 0 || strncmp(ctypei, "VRAD", 4) == 0 || strncmp(ctypei, "WAVE", 4) == 0 || strncmp(ctypei, "VOPT", 4) == 0 || strncmp(ctypei, "ZOPT", 4) == 0 || strncmp(ctypei, "AWAV", 4) == 0 || strncmp(ctypei, "VELO", 4) == 0 || strncmp(ctypei, "BETA", 4) == 0) && (ctypei[4] == '\0' || ctypei[4] == '-')) { if (!spectral) { continue; } } else if (strcmp(ctypei, "STOKES") == 0) { if (!stokes) { continue; } } else if (!other) { continue; } /* This axis is wanted, but has it already been added? */ for (k = 0; k < msub; k++) { if (map[k] == i+1) { break; } } if (k == msub) map[msub++] = i+1; } } else if (0 < axis && axis <= naxis) { /* Check that the requested axis has not already been added. */ for (k = 0; k < msub; k++) { if (map[k] == axis) { break; } } if (k == msub) map[msub++] = axis; } else if (axis == 0) { /* Graft on a new axis. */ map[msub++] = 0; } else { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_SUBIMAGE)); goto cleanup; } } if ((*nsub = msub) == 0) { status = 0; goto cleanup; } for (i = 0; i < *nsub; i++) { axes[i] = map[i]; } /* Construct the inverse axis map: axes[i] == j means that output axis i+1 comes from input axis j, axes[i] == 0 means to create a new axis, map[i] == j means that input axis i+1 goes to output axis j, map[i] == 0 means that input axis i+1 is not used. */ for (i = 0; i < naxis; i++) { map[i] = 0; } for (i = 0; i < *nsub; i++) { if (axes[i] > 0) { map[axes[i]-1] = i+1; } } /* Check that the subimage coordinate system is separable. */ if (*nsub < naxis) { srcp = wcssrc->pc; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++) { if (*(srcp++) == 0.0 || j == i) continue; if ((map[i] == 0) != (map[j] == 0)) { status = wcserr_set(WCS_ERRMSG(WCSERR_NON_SEPARABLE)); goto cleanup; } } } } /* Initialize the destination. */ npv = NPVMAX; nps = NPSMAX; NPVMAX = 0; for (k = 0; k < wcssrc->npv; k++) { i = wcssrc->pv[k].i; if (i == 0 || (i > 0 && map[i-1])) { NPVMAX++; } } NPSMAX = 0; for (k = 0; k < wcssrc->nps; k++) { i = wcssrc->ps[k].i; if (i > 0 && map[i-1]) { NPSMAX++; } } status = wcsini(alloc, *nsub, wcsdst); NPVMAX = npv; NPSMAX = nps; if (status) { goto cleanup; } /* Linear transformation. */ srcp = wcssrc->crpix; dstp = wcsdst->crpix; for (j = 0; j < *nsub; j++, dstp++) { if (axes[j] > 0) { k = axes[j] - 1; *dstp = *(srcp+k); } } srcp = wcssrc->pc; dstp = wcsdst->pc; for (i = 0; i < *nsub; i++) { if (axes[i] > 0) { for (j = 0; j < *nsub; j++, dstp++) { if (axes[j] > 0) { k = (axes[i]-1)*naxis + (axes[j]-1); *dstp = *(srcp+k); } } } } srcp = wcssrc->cdelt; dstp = wcsdst->cdelt; for (i = 0; i < *nsub; i++, dstp++) { if (axes[i] > 0) { k = axes[i] - 1; *dstp = *(srcp+k); } } /* Coordinate reference value. */ srcp = wcssrc->crval; dstp = wcsdst->crval; for (i = 0; i < *nsub; i++, dstp++) { if (axes[i] > 0) { k = axes[i] - 1; *dstp = *(srcp+k); } } /* Coordinate units and type. */ for (i = 0; i < *nsub; i++) { if (axes[i] > 0) { k = axes[i] - 1; strncpy(wcsdst->cunit[i], wcssrc->cunit[k], 72); strncpy(wcsdst->ctype[i], wcssrc->ctype[k], 72); } } /* Celestial and spectral transformation parameters. */ wcsdst->lonpole = wcssrc->lonpole; wcsdst->latpole = wcssrc->latpole; wcsdst->restfrq = wcssrc->restfrq; wcsdst->restwav = wcssrc->restwav; /* Parameter values. */ npv = 0; for (k = 0; k < wcssrc->npv; k++) { i = wcssrc->pv[k].i; if (i == 0 || (i > 0 && map[i-1])) { /* i == 0 is a special code for the latitude axis. */ wcsdst->pv[npv] = wcssrc->pv[k]; wcsdst->pv[npv].i = map[i-1]; npv++; } } wcsdst->npv = npv; nps = 0; for (k = 0; k < wcssrc->nps; k++) { i = wcssrc->ps[k].i; if (i > 0 && map[i-1]) { wcsdst->ps[nps] = wcssrc->ps[k]; wcsdst->ps[nps].i = map[i-1]; nps++; } } wcsdst->nps = nps; /* Alternate linear transformations. */ srcp = wcssrc->cd; dstp = wcsdst->cd; for (i = 0; i < *nsub; i++) { if (axes[i] > 0) { for (j = 0; j < *nsub; j++, dstp++) { if (axes[j] > 0) { k = (axes[i]-1)*naxis + (axes[j]-1); *dstp = *(srcp+k); } } } } srcp = wcssrc->crota; dstp = wcsdst->crota; for (i = 0; i < *nsub; i++, dstp++) { if (axes[i] > 0) { k = axes[i] - 1; *dstp = *(srcp+k); } } wcsdst->altlin = wcssrc->altlin; wcsdst->velref = wcssrc->velref; /* Auxiliary coordinate system information. */ strncpy(wcsdst->alt, wcssrc->alt, 4); wcsdst->colnum = wcssrc->colnum; strncpy(wcsdst->wcsname, wcssrc->wcsname, 72); for (i = 0; i < *nsub; i++) { if (axes[i] > 0) { k = axes[i] - 1; wcsdst->colax[i] = wcssrc->colax[k]; strncpy(wcsdst->cname[i], wcssrc->cname[k], 72); wcsdst->crder[i] = wcssrc->crder[k]; wcsdst->csyer[i] = wcssrc->csyer[k]; } } strncpy(wcsdst->radesys, wcssrc->radesys, 72); wcsdst->equinox = wcssrc->equinox; strncpy(wcsdst->specsys, wcssrc->specsys, 72); strncpy(wcsdst->ssysobs, wcssrc->ssysobs, 72); wcsdst->velosys = wcssrc->velosys; strncpy(wcsdst->ssyssrc, wcssrc->ssyssrc, 72); wcsdst->zsource = wcssrc->zsource; wcsdst->obsgeo[0] = wcssrc->obsgeo[0]; wcsdst->obsgeo[1] = wcssrc->obsgeo[1]; wcsdst->obsgeo[2] = wcssrc->obsgeo[2]; strncpy(wcsdst->dateobs, wcssrc->dateobs, 72); strncpy(wcsdst->dateavg, wcssrc->dateavg, 72); wcsdst->mjdobs = wcssrc->mjdobs; wcsdst->mjdavg = wcssrc->mjdavg; /* Coordinate lookup tables; only copy what's needed. */ wcsdst->ntab = 0; for (itab = 0; itab < wcssrc->ntab; itab++) { /* Is this table wanted? */ for (m = 0; m < wcssrc->tab[itab].M; m++) { i = wcssrc->tab[itab].map[m]; if (map[i-1]) { wcsdst->ntab++; break; } } } if (wcsdst->ntab) { /* Allocate memory for tabprm structs. */ if (!(wcsdst->tab = calloc(wcsdst->ntab, sizeof(struct tabprm)))) { wcsdst->ntab = 0; status = wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); goto cleanup; } wcsdst->m_tab = wcsdst->tab; } tabp = wcsdst->tab; for (itab = 0; itab < wcssrc->ntab; itab++) { for (m = 0; m < wcssrc->tab[itab].M; m++) { i = wcssrc->tab[itab].map[m]; if (map[i-1]) { if ((status = tabcpy(1, wcssrc->tab + itab, tabp))) { wcserr_set(WCS_ERRMSG(status)); goto cleanup; } tabp++; break; } } } cleanup: if (map) free(map); if (dealloc) { free(axes); } if (status && wcsdst->m_tab) free(wcsdst->m_tab); return status; } /*--------------------------------------------------------------------------*/ int wcsfree(struct wcsprm *wcs) { int j; if (wcs == 0x0) return WCSERR_NULL_POINTER; if (wcs->flag == -1) { wcs->lin.flag = -1; } else { /* Free memory allocated by wcsini(). */ if (wcs->m_flag == WCSSET) { if (wcs->crpix == wcs->m_crpix) wcs->crpix = 0x0; if (wcs->pc == wcs->m_pc) wcs->pc = 0x0; if (wcs->cdelt == wcs->m_cdelt) wcs->cdelt = 0x0; if (wcs->crval == wcs->m_crval) wcs->crval = 0x0; if (wcs->cunit == wcs->m_cunit) wcs->cunit = 0x0; if (wcs->ctype == wcs->m_ctype) wcs->ctype = 0x0; if (wcs->pv == wcs->m_pv) wcs->pv = 0x0; if (wcs->ps == wcs->m_ps) wcs->ps = 0x0; if (wcs->cd == wcs->m_cd) wcs->cd = 0x0; if (wcs->crota == wcs->m_crota) wcs->crota = 0x0; if (wcs->colax == wcs->m_colax) wcs->colax = 0x0; if (wcs->cname == wcs->m_cname) wcs->cname = 0x0; if (wcs->crder == wcs->m_crder) wcs->crder = 0x0; if (wcs->csyer == wcs->m_csyer) wcs->csyer = 0x0; if (wcs->tab == wcs->m_tab) wcs->tab = 0x0; if (wcs->wtb == wcs->m_wtb) wcs->wtb = 0x0; if (wcs->m_crpix) free(wcs->m_crpix); if (wcs->m_pc) free(wcs->m_pc); if (wcs->m_cdelt) free(wcs->m_cdelt); if (wcs->m_crval) free(wcs->m_crval); if (wcs->m_cunit) free(wcs->m_cunit); if (wcs->m_ctype) free(wcs->m_ctype); if (wcs->m_pv) free(wcs->m_pv); if (wcs->m_ps) free(wcs->m_ps); if (wcs->m_cd) free(wcs->m_cd); if (wcs->m_crota) free(wcs->m_crota); if (wcs->m_colax) free(wcs->m_colax); if (wcs->m_cname) free(wcs->m_cname); if (wcs->m_crder) free(wcs->m_crder); if (wcs->m_csyer) free(wcs->m_csyer); /* Free memory allocated by wcstab(). */ if (wcs->m_tab) { for (j = 0; j < wcs->ntab; j++) { tabfree(wcs->m_tab + j); } free(wcs->m_tab); } if (wcs->m_wtb) free(wcs->m_wtb); } /* Free memory allocated by wcsset(). */ if (wcs->types) free(wcs->types); if (wcs->lin.crpix == wcs->m_crpix) wcs->lin.crpix = 0x0; if (wcs->lin.pc == wcs->m_pc) wcs->lin.pc = 0x0; if (wcs->lin.cdelt == wcs->m_cdelt) wcs->lin.cdelt = 0x0; } wcs->m_flag = 0; wcs->m_naxis = 0x0; wcs->m_crpix = 0x0; wcs->m_pc = 0x0; wcs->m_cdelt = 0x0; wcs->m_crval = 0x0; wcs->m_cunit = 0x0; wcs->m_ctype = 0x0; wcs->m_pv = 0x0; wcs->m_ps = 0x0; wcs->m_cd = 0x0; wcs->m_crota = 0x0; wcs->m_colax = 0x0; wcs->m_cname = 0x0; wcs->m_crder = 0x0; wcs->m_csyer = 0x0; wcs->ntab = 0; wcs->m_tab = 0x0; wcs->nwtb = 0; wcs->m_wtb = 0x0; wcs->types = 0x0; wcs->flag = 0; if (wcs->err) free(wcs->err); wcs->err = 0x0; linfree(&(wcs->lin)); celfree(&(wcs->cel)); spcfree(&(wcs->spc)); return 0; } /*--------------------------------------------------------------------------*/ int wcsprt(const struct wcsprm *wcs) { int i, j, k; struct wtbarr *wtbp; if (wcs == 0x0) return WCSERR_NULL_POINTER; if (wcs->flag != WCSSET) { wcsprintf("The wcsprm struct is UNINITIALIZED.\n"); return 0; } wcsprintf(" flag: %d\n", wcs->flag); wcsprintf(" naxis: %d\n", wcs->naxis); WCSPRINTF_PTR(" crpix: ", wcs->crpix, "\n"); wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" %- 11.5g", wcs->crpix[i]); } wcsprintf("\n"); /* Linear transformation. */ k = 0; WCSPRINTF_PTR(" pc: ", wcs->pc, "\n"); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" pc[%d][]:", i); for (j = 0; j < wcs->naxis; j++) { wcsprintf(" %- 11.5g", wcs->pc[k++]); } wcsprintf("\n"); } /* Coordinate increment at reference point. */ WCSPRINTF_PTR(" cdelt: ", wcs->cdelt, "\n"); wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" %- 11.5g", wcs->cdelt[i]); } wcsprintf("\n"); /* Coordinate value at reference point. */ WCSPRINTF_PTR(" crval: ", wcs->crval, "\n"); wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" %- 11.5g", wcs->crval[i]); } wcsprintf("\n"); /* Coordinate units and type. */ WCSPRINTF_PTR(" cunit: ", wcs->cunit, "\n"); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" \"%s\"\n", wcs->cunit[i]); } WCSPRINTF_PTR(" ctype: ", wcs->ctype, "\n"); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" \"%s\"\n", wcs->ctype[i]); } /* Celestial and spectral transformation parameters. */ if (undefined(wcs->lonpole)) { wcsprintf(" lonpole: UNDEFINED\n"); } else { wcsprintf(" lonpole: %9f\n", wcs->lonpole); } wcsprintf(" latpole: %9f\n", wcs->latpole); wcsprintf(" restfrq: %f\n", wcs->restfrq); wcsprintf(" restwav: %f\n", wcs->restwav); /* Parameter values. */ wcsprintf(" npv: %d\n", wcs->npv); wcsprintf(" npvmax: %d\n", wcs->npvmax); WCSPRINTF_PTR(" pv: ", wcs->pv, "\n"); for (i = 0; i < wcs->npv; i++) { wcsprintf(" %3d%4d %- 11.5g\n", (wcs->pv[i]).i, (wcs->pv[i]).m, (wcs->pv[i]).value); } wcsprintf(" nps: %d\n", wcs->nps); wcsprintf(" npsmax: %d\n", wcs->npsmax); WCSPRINTF_PTR(" ps: ", wcs->ps, "\n"); for (i = 0; i < wcs->nps; i++) { wcsprintf(" %3d%4d %s\n", (wcs->ps[i]).i, (wcs->ps[i]).m, (wcs->ps[i]).value); } /* Alternate linear transformations. */ k = 0; WCSPRINTF_PTR(" cd: ", wcs->cd, "\n"); if (wcs->cd) { for (i = 0; i < wcs->naxis; i++) { wcsprintf(" cd[%d][]:", i); for (j = 0; j < wcs->naxis; j++) { wcsprintf(" %- 11.5g", wcs->cd[k++]); } wcsprintf("\n"); } } WCSPRINTF_PTR(" crota: ", wcs->crota, "\n"); if (wcs->crota) { wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" %- 11.5g", wcs->crota[i]); } wcsprintf("\n"); } wcsprintf(" altlin: %d\n", wcs->altlin); wcsprintf(" velref: %d\n", wcs->velref); /* Auxiliary coordinate system information. */ wcsprintf(" alt: '%c'\n", wcs->alt[0]); wcsprintf(" colnum: %d\n", wcs->colnum); WCSPRINTF_PTR(" colax: ", wcs->colax, "\n"); if (wcs->colax) { wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { wcsprintf(" %5d", wcs->colax[i]); } wcsprintf("\n"); } if (wcs->wcsname[0] == '\0') { wcsprintf(" wcsname: UNDEFINED\n"); } else { wcsprintf(" wcsname: \"%s\"\n", wcs->wcsname); } WCSPRINTF_PTR(" cname: ", wcs->cname, "\n"); if (wcs->cname) { for (i = 0; i < wcs->naxis; i++) { if (wcs->cname[i][0] == '\0') { wcsprintf(" UNDEFINED\n"); } else { wcsprintf(" \"%s\"\n", wcs->cname[i]); } } } WCSPRINTF_PTR(" crder: ", wcs->crder, "\n"); if (wcs->crder) { wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { if (undefined(wcs->crder[i])) { wcsprintf(" UNDEFINED "); } else { wcsprintf(" %- 11.5g", wcs->crder[i]); } } wcsprintf("\n"); } WCSPRINTF_PTR(" csyer: ", wcs->csyer, "\n"); if (wcs->csyer) { wcsprintf(" "); for (i = 0; i < wcs->naxis; i++) { if (undefined(wcs->csyer[i])) { wcsprintf(" UNDEFINED "); } else { wcsprintf(" %- 11.5g", wcs->csyer[i]); } } wcsprintf("\n"); } if (wcs->radesys[0] == '\0') { wcsprintf(" radesys: UNDEFINED\n"); } else { wcsprintf(" radesys: \"%s\"\n", wcs->radesys); } if (undefined(wcs->equinox)) { wcsprintf(" equinox: UNDEFINED\n"); } else { wcsprintf(" equinox: %9f\n", wcs->equinox); } if (wcs->specsys[0] == '\0') { wcsprintf(" specsys: UNDEFINED\n"); } else { wcsprintf(" specsys: \"%s\"\n", wcs->specsys); } if (wcs->ssysobs[0] == '\0') { wcsprintf(" ssysobs: UNDEFINED\n"); } else { wcsprintf(" ssysobs: \"%s\"\n", wcs->ssysobs); } if (undefined(wcs->velosys)) { wcsprintf(" velosys: UNDEFINED\n"); } else { wcsprintf(" velosys: %9f\n", wcs->velosys); } if (wcs->ssyssrc[0] == '\0') { wcsprintf(" ssyssrc: UNDEFINED\n"); } else { wcsprintf(" ssyssrc: \"%s\"\n", wcs->ssyssrc); } if (undefined(wcs->zsource)) { wcsprintf(" zsource: UNDEFINED\n"); } else { wcsprintf(" zsource: %9f\n", wcs->zsource); } wcsprintf(" obsgeo: "); for (i = 0; i < 3; i++) { if (undefined(wcs->obsgeo[i])) { wcsprintf("UNDEFINED "); } else { wcsprintf("%- 11.5g ", wcs->obsgeo[i]); } } wcsprintf("\n"); if (wcs->dateobs[0] == '\0') { wcsprintf(" dateobs: UNDEFINED\n"); } else { wcsprintf(" dateobs: \"%s\"\n", wcs->dateobs); } if (wcs->dateavg[0] == '\0') { wcsprintf(" dateavg: UNDEFINED\n"); } else { wcsprintf(" dateavg: \"%s\"\n", wcs->dateavg); } if (undefined(wcs->mjdobs)) { wcsprintf(" mjdobs: UNDEFINED\n"); } else { wcsprintf(" mjdobs: %9f\n", wcs->mjdobs); } if (undefined(wcs->mjdavg)) { wcsprintf(" mjdavg: UNDEFINED\n"); } else { wcsprintf(" mjdavg: %9f\n", wcs->mjdavg); } wcsprintf(" ntab: %d\n", wcs->ntab); WCSPRINTF_PTR(" tab: ", wcs->tab, ""); if (wcs->tab != 0x0) wcsprintf(" (see below)"); wcsprintf("\n"); wcsprintf(" nwtb: %d\n", wcs->nwtb); WCSPRINTF_PTR(" wtb: ", wcs->wtb, ""); if (wcs->wtb != 0x0) wcsprintf(" (see below)"); wcsprintf("\n"); /* Derived values. */ WCSPRINTF_PTR(" types: ", wcs->types, "\n "); for (i = 0; i < wcs->naxis; i++) { wcsprintf("%5d", wcs->types[i]); } wcsprintf("\n"); wcsprintf(" lngtyp: \"%s\"\n", wcs->lngtyp); wcsprintf(" lattyp: \"%s\"\n", wcs->lattyp); wcsprintf(" lng: %d\n", wcs->lng); wcsprintf(" lat: %d\n", wcs->lat); wcsprintf(" spec: %d\n", wcs->spec); wcsprintf(" cubeface: %d\n", wcs->cubeface); WCSPRINTF_PTR(" err: ", wcs->err, "\n"); if (wcs->err) { wcserr_prt(wcs->err, " "); } wcsprintf(" lin: (see below)\n"); wcsprintf(" cel: (see below)\n"); wcsprintf(" spc: (see below)\n"); /* Memory management. */ wcsprintf(" m_flag: %d\n", wcs->m_flag); wcsprintf(" m_naxis: %d\n", wcs->m_naxis); WCSPRINTF_PTR(" m_crpix: ", wcs->m_crpix, ""); if (wcs->m_crpix == wcs->crpix) wcsprintf(" (= crpix)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_pc: ", wcs->m_pc, ""); if (wcs->m_pc == wcs->pc) wcsprintf(" (= pc)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_cdelt: ", wcs->m_cdelt, ""); if (wcs->m_cdelt == wcs->cdelt) wcsprintf(" (= cdelt)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_crval: ", wcs->m_crval, ""); if (wcs->m_crval == wcs->crval) wcsprintf(" (= crval)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_cunit: ", wcs->m_cunit, ""); if (wcs->m_cunit == wcs->cunit) wcsprintf(" (= cunit)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_ctype: ", wcs->m_ctype, ""); if (wcs->m_ctype == wcs->ctype) wcsprintf(" (= ctype)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_pv: ", wcs->m_pv, ""); if (wcs->m_pv == wcs->pv) wcsprintf(" (= pv)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_ps: ", wcs->m_ps, ""); if (wcs->m_ps == wcs->ps) wcsprintf(" (= ps)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_cd: ", wcs->m_cd, ""); if (wcs->m_cd == wcs->cd) wcsprintf(" (= cd)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_crota: ", wcs->m_crota, ""); if (wcs->m_crota == wcs->crota) wcsprintf(" (= crota)"); wcsprintf("\n"); wcsprintf("\n"); WCSPRINTF_PTR(" m_colax: ", wcs->m_colax, ""); if (wcs->m_colax == wcs->colax) wcsprintf(" (= colax)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_cname: ", wcs->m_cname, ""); if (wcs->m_cname == wcs->cname) wcsprintf(" (= cname)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_crder: ", wcs->m_crder, ""); if (wcs->m_crder == wcs->crder) wcsprintf(" (= crder)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_csyer: ", wcs->m_csyer, ""); if (wcs->m_csyer == wcs->csyer) wcsprintf(" (= csyer)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_tab: ", wcs->m_tab, ""); if (wcs->m_tab == wcs->tab) wcsprintf(" (= tab)"); wcsprintf("\n"); WCSPRINTF_PTR(" m_wtb: ", wcs->m_wtb, ""); if (wcs->m_wtb == wcs->wtb) wcsprintf(" (= wtb)"); wcsprintf("\n"); /* Tabular transformation parameters. */ if ((wtbp = wcs->wtb)) { for (j = 0; j < wcs->nwtb; j++, wtbp++) { wcsprintf("\n"); wcsprintf("wtb[%d].*\n", j); wcsprintf(" i: %d\n", wtbp->i); wcsprintf(" m: %d\n", wtbp->m); wcsprintf(" kind: %c\n", wtbp->kind); wcsprintf(" extnam: %s\n", wtbp->extnam); wcsprintf(" extver: %d\n", wtbp->extver); wcsprintf(" extlev: %d\n", wtbp->extlev); wcsprintf(" ttype: %s\n", wtbp->ttype); wcsprintf(" row: %ld\n", wtbp->row); wcsprintf(" ndim: %d\n", wtbp->ndim); WCSPRINTF_PTR(" dimlen: ", wtbp->dimlen, "\n"); WCSPRINTF_PTR(" arrayp: ", wtbp->arrayp, " -> "); WCSPRINTF_PTR("", *(wtbp->arrayp), "\n"); } } if (wcs->tab) { for (j = 0; j < wcs->ntab; j++) { wcsprintf("\n"); wcsprintf("tab[%d].*\n", j); tabprt(wcs->tab + j); } } /* Linear transformation parameters. */ wcsprintf("\n"); wcsprintf(" lin.*\n"); linprt(&(wcs->lin)); /* Celestial transformation parameters. */ wcsprintf("\n"); wcsprintf(" cel.*\n"); celprt(&(wcs->cel)); /* Spectral transformation parameters. */ wcsprintf("\n"); wcsprintf(" spc.*\n"); spcprt(&(wcs->spc)); return 0; } /*--------------------------------------------------------------------------*/ int wcsperr(const struct wcsprm *wcs, const char *prefix) { int j; if (wcs == 0x0) return WCSERR_NULL_POINTER; if (!wcserr_prt(wcs->err, prefix)) { wcserr_prt(wcs->lin.err, prefix); wcserr_prt(wcs->cel.err, prefix); wcserr_prt(wcs->cel.prj.err, prefix); wcserr_prt(wcs->spc.err, prefix); if (wcs->tab) { for (j = 0; j < wcs->ntab; j++) { wcserr_prt((wcs->tab + j)->err, prefix); } } } return 0; } /*--------------------------------------------------------------------------*/ int wcsset(struct wcsprm *wcs) { static const char *function = "wcsset"; char scode[4], stype[5]; int i, j, k, m, naxis, status; double lambda, rho; double *cd, *pc; struct celprm *wcscel = &(wcs->cel); struct prjprm *wcsprj = &(wcscel->prj); struct spcprm *wcsspc = &(wcs->spc); struct wcserr **err; if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); /* Determine axis types from CTYPEia. */ if ((status = wcs_types(wcs))) { return status; } /* Convert to canonical units. */ if ((status = wcs_units(wcs))) { return status; } /* Non-linear celestial axes present? */ if (wcs->lng >= 0 && wcs->types[wcs->lng] == 2200) { celini(wcscel); /* CRVALia, LONPOLEa, and LATPOLEa keyvalues. */ wcscel->ref[0] = wcs->crval[wcs->lng]; wcscel->ref[1] = wcs->crval[wcs->lat]; wcscel->ref[2] = wcs->lonpole; wcscel->ref[3] = wcs->latpole; /* PVi_ma keyvalues. */ for (k = 0; k < wcs->npv; k++) { i = wcs->pv[k].i - 1; m = wcs->pv[k].m; if (i == -1) { /* From a PROJPn keyword. */ i = wcs->lat; } if (i == wcs->lat) { /* PVi_ma associated with latitude axis. */ if (m < 30) { wcsprj->pv[m] = wcs->pv[k].value; } } else if (i == wcs->lng) { /* PVi_ma associated with longitude axis. */ switch (m) { case 0: wcscel->offset = (wcs->pv[k].value != 0.0); break; case 1: wcscel->phi0 = wcs->pv[k].value; break; case 2: wcscel->theta0 = wcs->pv[k].value; break; case 3: /* If present, overrides LONPOLEa. */ wcscel->ref[2] = wcs->pv[k].value; break; case 4: /* If present, overrides LATPOLEa. */ wcscel->ref[3] = wcs->pv[k].value; break; default: return wcserr_set(WCSERR_SET(WCSERR_BAD_COORD_TRANS), "PV%i_%i%s: Unrecognized coordinate transformation parameter", i+1, m, wcs->alt); break; } } } /* Do simple alias translations. */ if (strncmp(wcs->ctype[wcs->lng]+5, "GLS", 3) == 0) { wcscel->offset = 1; wcscel->phi0 = 0.0; wcscel->theta0 = wcs->crval[wcs->lat]; strcpy(wcsprj->code, "SFL"); } else if (strncmp(wcs->ctype[wcs->lng]+5, "NCP", 3) == 0) { /* Convert NCP to SIN. */ if (wcscel->ref[1] == 0.0) { return wcserr_set(WCSERR_SET(WCSERR_BAD_PARAM), "Invalid projection: NCP blows up on the equator"); } strcpy(wcsprj->code, "SIN"); wcsprj->pv[1] = 0.0; wcsprj->pv[2] = cosd(wcscel->ref[1])/sind(wcscel->ref[1]); } else { strncpy(wcsprj->code, wcs->ctype[wcs->lng]+5, 3); wcsprj->code[3] = '\0'; } /* Initialize the celestial transformation routines. */ wcsprj->r0 = 0.0; if ((status = celset(wcscel))) { return wcserr_set(WCS_ERRMSG(status+3)); } /* Update LONPOLE, LATPOLE, and PVi_ma keyvalues. */ wcs->lonpole = wcscel->ref[2]; wcs->latpole = wcscel->ref[3]; for (k = 0; k < wcs->npv; k++) { i = wcs->pv[k].i - 1; m = wcs->pv[k].m; if (i == wcs->lng) { switch (m) { case 1: wcs->pv[k].value = wcscel->phi0; break; case 2: wcs->pv[k].value = wcscel->theta0; break; case 3: wcs->pv[k].value = wcscel->ref[2]; break; case 4: wcs->pv[k].value = wcscel->ref[3]; break; } } } } /* Non-linear spectral axis present? */ if (wcs->spec >= 0 && wcs->types[wcs->spec] == 3300) { spcini(wcsspc); if ((status = spctype(wcs->ctype[wcs->spec], stype, scode, 0x0, 0x0, 0x0, 0x0, 0x0, err))) { return status; } strcpy(wcsspc->type, stype); strcpy(wcsspc->code, scode); /* CRVALia, RESTFRQa, and RESTWAVa keyvalues. */ wcsspc->crval = wcs->crval[wcs->spec]; wcsspc->restfrq = wcs->restfrq; wcsspc->restwav = wcs->restwav; /* PVi_ma keyvalues. */ for (k = 0; k < wcs->npv; k++) { i = wcs->pv[k].i - 1; m = wcs->pv[k].m; if (i == wcs->spec) { /* PVi_ma associated with grism axis. */ if (m < 7) { wcsspc->pv[m] = wcs->pv[k].value; } } } /* Initialize the spectral transformation routines. */ if ((status = spcset(wcsspc))) { return wcserr_set(WCS_ERRMSG(status+3)); } } /* Tabular axes present? */ for (j = 0; j < wcs->ntab; j++) { if ((status = tabset(wcs->tab + j))) { return wcserr_set(WCS_ERRMSG(status+3)); } } /* Initialize the linear transformation. */ naxis = wcs->naxis; wcs->altlin &= 7; if (wcs->altlin > 1 && !(wcs->altlin & 1)) { pc = wcs->pc; if (wcs->altlin & 2) { /* Copy CDi_ja to PCi_ja and reset CDELTia. */ cd = wcs->cd; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++) { *(pc++) = *(cd++); } wcs->cdelt[i] = 1.0; } } else if (wcs->altlin & 4) { /* Construct PCi_ja from CROTAia. */ if ((i = wcs->lng) >= 0 && (j = wcs->lat) >= 0) { rho = wcs->crota[j]; if (wcs->cdelt[i] == 0.0) { return wcserr_set(WCSERR_SET(WCSERR_SINGULAR_MTX), "Singular transformation matrix, CDELT%d is zero", i+1); } lambda = wcs->cdelt[j]/wcs->cdelt[i]; *(pc + i*naxis + i) = *(pc + j*naxis + j) = cosd(rho); *(pc + i*naxis + j) = *(pc + j*naxis + i) = sind(rho); *(pc + i*naxis + j) *= -lambda; *(pc + j*naxis + i) /= lambda; } } } wcs->lin.crpix = wcs->crpix; wcs->lin.pc = wcs->pc; wcs->lin.cdelt = wcs->cdelt; if ((status = linset(&(wcs->lin)))) { return wcserr_set(WCS_ERRMSG(status)); } /* Strip off trailing blanks and null-fill auxiliary string members. */ wcsutil_null_fill(4, wcs->alt); wcsutil_null_fill(72, wcs->wcsname); for (i = 0; i < naxis; i++) { wcsutil_null_fill(72, wcs->cname[i]); } wcsutil_null_fill(72, wcs->radesys); wcsutil_null_fill(72, wcs->specsys); wcsutil_null_fill(72, wcs->ssysobs); wcsutil_null_fill(72, wcs->ssyssrc); wcsutil_null_fill(72, wcs->dateobs); wcsutil_null_fill(72, wcs->dateavg); wcs->flag = WCSSET; return 0; } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int wcs_types(struct wcsprm *wcs) { static const char *function = "wcs_types"; const int nalias = 2; const char aliases [2][4] = {"NCP", "GLS"}; const char *alt = ""; char ctypei[16], pcode[4], requir[9], scode[4], specsys[9]; int i, j, m, naxis, *ndx = 0x0, type; struct wcserr **err; if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); /* Parse the CTYPEia keyvalues. */ pcode[0] = '\0'; requir[0] = '\0'; wcs->lng = -1; wcs->lat = -1; wcs->spec = -1; wcs->cubeface = -1; if (*(wcs->alt) != ' ') alt = wcs->alt; naxis = wcs->naxis; if (wcs->types) free(wcs->types); wcs->types = calloc(naxis, sizeof(int)); if (wcs->types == NULL) { return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } for (i = 0; i < naxis; i++) { /* Null fill. */ wcsutil_null_fill(72, wcs->ctype[i]); strncpy(ctypei, wcs->ctype[i], 15); ctypei[15] = '\0'; /* Check for early Paper IV syntax (e.g. '-SIP' used by Spitzer). */ if (strlen(ctypei) == 12 && ctypei[8] == '-') { /* Excise the "4-3-3" or "8-3"-form distortion code. */ ctypei[8] = '\0'; /* Remove trailing dashes from "8-3"-form codes. */ for (j = 7; j > 0; j--) { if (ctypei[j] != '-') break; ctypei[j] = '\0'; } } /* Logarithmic or tabular axis? */ wcs->types[i] = 0; if (strcmp(ctypei+4, "-LOG") == 0) { /* Logarithmic axis. */ wcs->types[i] = 400; } else if (strcmp(ctypei+4, "-TAB") == 0) { /* Tabular axis. */ wcs->types[i] = 500; } if (wcs->types[i]) { /* Could have -LOG or -TAB with celestial or spectral types. */ ctypei[4] = '\0'; /* Take care of things like 'FREQ-LOG' or 'RA---TAB'. */ for (j = 3; j >= 0; j--) { if (ctypei[j] != '-') break; ctypei[j] = '\0'; } } /* Translate AIPS spectral types for spctyp(). */ if (spcaips(ctypei, wcs->velref, ctypei, specsys) == 0) { strcpy(wcs->ctype[i], ctypei); if (wcs->specsys[0] == '\0') strcpy(wcs->specsys, specsys); } /* Process linear axes. */ if (!(strlen(ctypei) == 8 && ctypei[4] == '-') || (strlen(ctypei) > 8 && ctypei[8] == '-')) { /* Identify Stokes, celestial and spectral types. */ if (strcmp(ctypei, "STOKES") == 0) { /* STOKES axis. */ wcs->types[i] = 1100; } else if (strcmp(ctypei, "RA") == 0 || strcmp(ctypei+1, "LON") == 0 || strcmp(ctypei+2, "LN") == 0) { /* Longitude axis. */ if (wcs->lng < 0) wcs->lng = i; wcs->types[i] += 2000; } else if (strcmp(ctypei, "DEC") == 0 || strcmp(ctypei+1, "LAT") == 0 || strcmp(ctypei+2, "LT") == 0) { /* Latitude axis. */ if (wcs->lat < 0) wcs->lat = i; wcs->types[i] += 2001; } else if (strcmp(ctypei, "CUBEFACE") == 0) { /* CUBEFACE axis. */ if (wcs->cubeface == -1) { wcs->types[i] = 2102; wcs->cubeface = i; } else { /* Multiple CUBEFACE axes! */ return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Multiple CUBEFACE axes (in CTYPE%d%.1s and CTYPE%d%.1s)", wcs->cubeface+1, alt, i+1, alt); } } else if (spctyp(ctypei, 0x0, 0x0, 0x0, 0x0, 0x0, 0x0, 0x0) == 0) { /* Spectral axis. */ if (wcs->spec < 0) wcs->spec = i; wcs->types[i] += 3000; } continue; } /* CTYPEia is in "4-3" form; is it a recognized spectral type? */ if (spctyp(ctypei, 0x0, scode, 0x0, 0x0, 0x0, 0x0, 0x0) == 0) { /* Non-linear spectral axis found. */ wcs->types[i] = 3300; /* Check uniqueness. */ if (wcs->spec >= 0) { return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Multiple spectral axes (in CTYPE%d%.1s and CTYPE%d%.1s)", wcs->spec+1, alt, i+1, alt); } wcs->spec = i; continue; } /* Is it a recognized celestial projection? */ for (j = 0; j < prj_ncode; j++) { if (strncmp(ctypei+5, prj_codes[j], 3) == 0) break; } if (j == prj_ncode) { /* Not a standard projection code, maybe it's an alias. */ for (j = 0; j < nalias; j++) { if (strncmp(ctypei+5, aliases[j], 3) == 0) break; } if (j == nalias) { /* Not a recognized algorithm code of any type. */ wcs->types[i] = -1; return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Unrecognized projection code (%s in CTYPE%d%.1s)", ctypei+5, i+1, alt); } } /* Parse the celestial axis type. */ wcs->types[i] = 2200; if (*pcode == '\0') { /* The first of the two celestial axes. */ sprintf(pcode, "%.3s", ctypei+5); if (strncmp(ctypei, "RA--", 4) == 0) { wcs->lng = i; strcpy(wcs->lngtyp, "RA"); strcpy(wcs->lattyp, "DEC"); ndx = &wcs->lat; sprintf(requir, "DEC--%s", pcode); } else if (strncmp(ctypei, "DEC-", 4) == 0) { wcs->lat = i; strcpy(wcs->lngtyp, "RA"); strcpy(wcs->lattyp, "DEC"); ndx = &wcs->lng; sprintf(requir, "RA---%s", pcode); } else if (strncmp(ctypei+1, "LON", 3) == 0) { wcs->lng = i; sprintf(wcs->lngtyp, "%cLON", ctypei[0]); sprintf(wcs->lattyp, "%cLAT", ctypei[0]); ndx = &wcs->lat; sprintf(requir, "%s-%s", wcs->lattyp, pcode); } else if (strncmp(ctypei+1, "LAT", 3) == 0) { wcs->lat = i; sprintf(wcs->lngtyp, "%cLON", ctypei[0]); sprintf(wcs->lattyp, "%cLAT", ctypei[0]); ndx = &wcs->lng; sprintf(requir, "%s-%s", wcs->lngtyp, pcode); } else if (strncmp(ctypei+2, "LN", 2) == 0) { wcs->lng = i; sprintf(wcs->lngtyp, "%c%cLN", ctypei[0], ctypei[1]); sprintf(wcs->lattyp, "%c%cLT", ctypei[0], ctypei[1]); ndx = &wcs->lat; sprintf(requir, "%s-%s", wcs->lattyp, pcode); } else if (strncmp(ctypei+2, "LT", 2) == 0) { wcs->lat = i; sprintf(wcs->lngtyp, "%c%cLN", ctypei[0], ctypei[1]); sprintf(wcs->lattyp, "%c%cLT", ctypei[0], ctypei[1]); ndx = &wcs->lng; sprintf(requir, "%s-%s", wcs->lngtyp, pcode); } else { /* Unrecognized celestial type. */ wcs->types[i] = -1; wcs->lng = -1; wcs->lat = -1; return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Unrecognized celestial type (%5s in CTYPE%d%.1s)", ctypei, i+1, alt); } if (wcs->lat >= 0) wcs->types[i]++; } else { /* Looking for the complementary celestial axis. */ if (wcs->lat < 0) wcs->types[i]++; if (strncmp(ctypei, requir, 8) != 0) { /* Inconsistent projection types. */ wcs->lng = -1; wcs->lat = -1; return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Inconsistent " "projection types (expected %s, got %s in CTYPE%d%.1s)", requir, ctypei, i+1, alt); } *ndx = i; requir[0] = '\0'; } } /* Do we have a complementary pair of celestial axes? */ if (strcmp(requir, "")) { /* Unmatched celestial axis. */ wcs->lng = -1; wcs->lat = -1; return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Unmatched celestial axes"); } /* Table group numbers. */ for (j = 0; j < wcs->ntab; j++) { for (m = 0; m < wcs->tab[j].M; m++) { /* Get image axis number. */ i = wcs->tab[j].map[m]; type = (wcs->types[i] / 100) % 10; if (type != 5) { return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "Table parameters set for non-table axis type"); } wcs->types[i] += 10 * j; } } return 0; } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int wcs_units(struct wcsprm *wcs) { static const char *function = "wcs_units"; char ctype[9], units[16]; int i, j, naxis; double scale, offset, power; struct wcserr *uniterr = 0x0, **err; if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); naxis = wcs->naxis; for (i = 0; i < naxis; i++) { /* Use types set by wcs_types(). */ switch (wcs->types[i]/1000) { case 2: /* Celestial axis. */ strcpy(units, "deg"); break; case 3: /* Spectral axis. */ strncpy(ctype, wcs->ctype[i], 8); ctype[8] = '\0'; spctyp(ctype, 0x0, 0x0, 0x0, units, 0x0, 0x0, 0x0); break; default: continue; } /* Tabular axis, CDELTia and CRVALia relate to indices. */ if ((wcs->types[i]/100)%10 == 5) { continue; } wcsutil_null_fill(72, wcs->cunit[i]); if (wcs->cunit[i][0]) { if (wcsunitse(wcs->cunit[i], units, &scale, &offset, &power, &uniterr)) { wcserr_set(WCSERR_SET(WCSERR_BAD_COORD_TRANS), "In CUNIT%d%.1s: %s", i, (*wcs->alt)?wcs->alt:"", uniterr->msg); free(uniterr); return WCSERR_BAD_COORD_TRANS; } if (scale != 1.0) { wcs->cdelt[i] *= scale; wcs->crval[i] *= scale; for (j = 0; j < naxis; j++) { *(wcs->cd + i*naxis + j) *= scale; } strcpy(wcs->cunit[i], units); } } else { strcpy(wcs->cunit[i], units); } } return 0; } /*--------------------------------------------------------------------------*/ int wcsp2s( struct wcsprm *wcs, int ncoord, int nelem, const double pixcrd[], double imgcrd[], double phi[], double theta[], double world[], int stat[]) { static const char *function = "wcsp2s"; int bits, face, i, iso_x, iso_y, istat, *istatp, itab, k, m, nx, ny, *statp, status, type; double crvali, offset; register double *img, *wrl; struct celprm *wcscel = &(wcs->cel); struct prjprm *wcsprj = &(wcscel->prj); struct wcserr **err; /* Initialize if required. */ if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } /* Sanity check. */ if (ncoord < 1 || (ncoord > 1 && nelem < wcs->naxis)) { return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "ncoord and/or nelem inconsistent with the wcsprm"); } /* Apply pixel-to-world linear transformation. */ if ((status = linp2x(&(wcs->lin), ncoord, nelem, pixcrd, imgcrd))) { return wcserr_set(WCS_ERRMSG(status)); } /* Initialize status vectors. */ if (!(istatp = calloc(ncoord, sizeof(int)))) { return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } stat[0] = 0; wcsutil_setAli(ncoord, 1, stat); /* Convert intermediate world coordinates to world coordinates. */ for (i = 0; i < wcs->naxis; i++) { /* Extract the second digit of the axis type code. */ type = (wcs->types[i] / 100) % 10; if (type <= 1) { /* Linear or quantized coordinate axis. */ img = imgcrd + i; wrl = world + i; crvali = wcs->crval[i]; for (k = 0; k < ncoord; k++) { *wrl = *img + crvali; img += nelem; wrl += nelem; } } else if (wcs->types[i] == 2200) { /* Convert celestial coordinates; do we have a CUBEFACE axis? */ if (wcs->cubeface != -1) { /* Separation between faces. */ if (wcsprj->r0 == 0.0) { offset = 90.0; } else { offset = wcsprj->r0*PI/2.0; } /* Lay out faces in a plane. */ img = imgcrd; statp = stat; bits = (1 << i) | (1 << wcs->lat); for (k = 0; k < ncoord; k++, statp++) { face = (int)(*(img+wcs->cubeface) + 0.5); if (fabs(*(img+wcs->cubeface) - face) > 1e-10) { *statp |= bits; status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_PIX)); } else { *statp = 0; switch (face) { case 0: *(img+wcs->lat) += offset; break; case 1: break; case 2: *(img+i) += offset; break; case 3: *(img+i) += offset*2; break; case 4: *(img+i) += offset*3; break; case 5: *(img+wcs->lat) -= offset; break; default: *statp |= bits; status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_PIX)); } } img += nelem; } } /* Check for constant x and/or y. */ nx = ncoord; ny = 0; if ((iso_x = wcsutil_allEq(ncoord, nelem, imgcrd+i))) { nx = 1; ny = ncoord; } if ((iso_y = wcsutil_allEq(ncoord, nelem, imgcrd+wcs->lat))) { ny = 1; } /* Transform projection plane coordinates to celestial coordinates. */ if ((istat = celx2s(wcscel, nx, ny, nelem, nelem, imgcrd+i, imgcrd+wcs->lat, phi, theta, world+i, world+wcs->lat, istatp))) { if (istat == CELERR_BAD_PIX) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_PIX)); } else { status = wcserr_set(WCS_ERRMSG(istat+3)); goto cleanup; } } /* If x and y were both constant, replicate values. */ if (iso_x && iso_y) { wcsutil_setAll(ncoord, nelem, world+i); wcsutil_setAll(ncoord, nelem, world+wcs->lat); wcsutil_setAll(ncoord, 1, phi); wcsutil_setAll(ncoord, 1, theta); wcsutil_setAli(ncoord, 1, istatp); } if (istat == 5) { bits = (1 << i) | (1 << wcs->lat); wcsutil_setBit(ncoord, istatp, bits, stat); } } else if (type == 3 || type == 4) { /* Check for constant x. */ nx = ncoord; if ((iso_x = wcsutil_allEq(ncoord, nelem, imgcrd+i))) { nx = 1; } istat = 0; if (wcs->types[i] == 3300) { /* Spectral coordinates. */ istat = spcx2s(&(wcs->spc), nx, nelem, nelem, imgcrd+i, world+i, istatp); if (istat == SPCERR_BAD_X) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_PIX)); } else if (istat) { status = wcserr_set(WCS_ERRMSG(istat+3)); goto cleanup; } } else if (type == 4) { /* Logarithmic coordinates. */ istat = logx2s(wcs->crval[i], nx, nelem, nelem, imgcrd+i, world+i, istatp); if (istat == LOGERR_BAD_X) { if (*err == 0x0) { wcserr_set(WCS_ERRMSG(WCSERR_BAD_PIX)); } } else if (istat == LOGERR_BAD_LOG_REF_VAL) { wcserr_set(WCSERR_SET(WCSERR_BAD_PARAM), log_errmsg[istat]); goto cleanup; } } /* If x was constant, replicate values. */ if (iso_x) { wcsutil_setAll(ncoord, nelem, world+i); wcsutil_setAli(ncoord, 1, istatp); } if (istat == 3) { wcsutil_setBit(ncoord, istatp, 1 << i, stat); } } } /* Do tabular coordinates. */ for (itab = 0; itab < wcs->ntab; itab++) { istat = tabx2s(wcs->tab + itab, ncoord, nelem, imgcrd, world, istatp); if (istat == TABERR_BAD_X) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_PIX)); bits = 0; for (m = 0; m < wcs->tab[itab].M; m++) { bits |= 1 << wcs->tab[itab].map[m]; } wcsutil_setBit(ncoord, istatp, bits, stat); } else if (istat) { if (istat == TABERR_BAD_PARAMS) istat = WCSERR_BAD_PARAM; status = wcserr_set(WCS_ERRMSG(istat)); goto cleanup; } } /* Zero the unused world coordinate elements. */ for (i = wcs->naxis; i < nelem; i++) { world[i] = 0.0; wcsutil_setAll(ncoord, nelem, world+i); } cleanup: free(istatp); return status; } /*--------------------------------------------------------------------------*/ int wcss2p( struct wcsprm* wcs, int ncoord, int nelem, const double world[], double phi[], double theta[], double imgcrd[], double pixcrd[], int stat[]) { static const char *function = "wcss2p"; int bits, i, isolat, isolng, isospec, istat, *istatp, itab, k, m, nlat, nlng, nwrld, status, type; double crvali, offset; register const double *wrl; register double *img; struct celprm *wcscel = &(wcs->cel); struct prjprm *wcsprj = &(wcscel->prj); struct wcserr **err; /* Initialize if required. */ if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } /* Sanity check. */ if (ncoord < 1 || (ncoord > 1 && nelem < wcs->naxis)) { return wcserr_set(WCSERR_SET(WCSERR_BAD_CTYPE), "ncoord and/or nelem inconsistent with the wcsprm"); } /* Initialize status vectors. */ if (!(istatp = calloc(ncoord, sizeof(int)))) { return wcserr_set(WCS_ERRMSG(WCSERR_MEMORY)); } status = 0; stat[0] = 0; wcsutil_setAli(ncoord, 1, stat); /* Convert world coordinates to intermediate world coordinates. */ for (i = 0; i < wcs->naxis; i++) { /* Extract the second digit of the axis type code. */ type = (wcs->types[i] / 100) % 10; if (type <= 1) { /* Linear or quantized coordinate axis. */ wrl = world + i; img = imgcrd + i; crvali = wcs->crval[i]; for (k = 0; k < ncoord; k++) { *img = *wrl - crvali; wrl += nelem; img += nelem; } } else if (wcs->types[i] == 2200) { /* Celestial coordinates; check for constant lng and/or lat. */ nlng = ncoord; nlat = 0; if ((isolng = wcsutil_allEq(ncoord, nelem, world+i))) { nlng = 1; nlat = ncoord; } if ((isolat = wcsutil_allEq(ncoord, nelem, world+wcs->lat))) { nlat = 1; } /* Transform celestial coordinates to projection plane coordinates. */ if ((istat = cels2x(wcscel, nlng, nlat, nelem, nelem, world+i, world+wcs->lat, phi, theta, imgcrd+i, imgcrd+wcs->lat, istatp))) { if (istat == CELERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD)); } else { status = wcserr_set(WCS_ERRMSG(istat+3)); goto cleanup; } } /* If lng and lat were both constant, replicate values. */ if (isolng && isolat) { wcsutil_setAll(ncoord, nelem, imgcrd+i); wcsutil_setAll(ncoord, nelem, imgcrd+wcs->lat); wcsutil_setAll(ncoord, 1, phi); wcsutil_setAll(ncoord, 1, theta); wcsutil_setAli(ncoord, 1, istatp); } if (istat == CELERR_BAD_WORLD) { bits = (1 << i) | (1 << wcs->lat); wcsutil_setBit(ncoord, istatp, bits, stat); } /* Do we have a CUBEFACE axis? */ if (wcs->cubeface != -1) { /* Separation between faces. */ if (wcsprj->r0 == 0.0) { offset = 90.0; } else { offset = wcsprj->r0*PI/2.0; } /* Stack faces in a cube. */ img = imgcrd; for (k = 0; k < ncoord; k++) { if (*(img+wcs->lat) < -0.5*offset) { *(img+wcs->lat) += offset; *(img+wcs->cubeface) = 5.0; } else if (*(img+wcs->lat) > 0.5*offset) { *(img+wcs->lat) -= offset; *(img+wcs->cubeface) = 0.0; } else if (*(img+i) > 2.5*offset) { *(img+i) -= 3.0*offset; *(img+wcs->cubeface) = 4.0; } else if (*(img+i) > 1.5*offset) { *(img+i) -= 2.0*offset; *(img+wcs->cubeface) = 3.0; } else if (*(img+i) > 0.5*offset) { *(img+i) -= offset; *(img+wcs->cubeface) = 2.0; } else { *(img+wcs->cubeface) = 1.0; } img += nelem; } } } else if (type == 3 || type == 4) { /* Check for constancy. */ nwrld = ncoord; if ((isospec = wcsutil_allEq(ncoord, nelem, world+i))) { nwrld = 1; } istat = 0; if (wcs->types[i] == 3300) { /* Spectral coordinates. */ istat = spcs2x(&(wcs->spc), nwrld, nelem, nelem, world+i, imgcrd+i, istatp); if (istat == SPCERR_BAD_SPEC) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD)); } else if (istat) { status = wcserr_set(WCS_ERRMSG(istat+3)); goto cleanup; } } else if (type == 4) { /* Logarithmic coordinates. */ istat = logs2x(wcs->crval[i], nwrld, nelem, nelem, world+i, imgcrd+i, istatp); if (istat == LOGERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD)); } else if (istat == LOGERR_BAD_LOG_REF_VAL) { status = wcserr_set(WCSERR_SET(WCSERR_BAD_PARAM), log_errmsg[istat]); goto cleanup; } } /* If constant, replicate values. */ if (isospec) { wcsutil_setAll(ncoord, nelem, imgcrd+i); wcsutil_setAli(ncoord, 1, istatp); } if (istat == 4) { wcsutil_setBit(ncoord, istatp, 1 << i, stat); } } } /* Do tabular coordinates. */ for (itab = 0; itab < wcs->ntab; itab++) { istat = tabs2x(wcs->tab + itab, ncoord, nelem, world, imgcrd, istatp); if (istat == TABERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD)); bits = 0; for (m = 0; m < wcs->tab[itab].M; m++) { bits |= 1 << wcs->tab[itab].map[m]; } wcsutil_setBit(ncoord, istatp, bits, stat); } else if (istat) { if (istat == TABERR_BAD_PARAMS) istat = WCSERR_BAD_PARAM; status = wcserr_set(WCS_ERRMSG(istat)); goto cleanup; } } /* Zero the unused intermediate world coordinate elements. */ for (i = wcs->naxis; i < nelem; i++) { imgcrd[i] = 0.0; wcsutil_setAll(ncoord, nelem, imgcrd+i); } /* Apply world-to-pixel linear transformation. */ if ((istat = linx2p(&(wcs->lin), ncoord, nelem, imgcrd, pixcrd))) { status = wcserr_set(WCS_ERRMSG(istat)); goto cleanup; } cleanup: free(istatp); return status; } /*--------------------------------------------------------------------------*/ int wcsmix( struct wcsprm *wcs, int mixpix, int mixcel, const double vspan[2], double vstep, int viter, double world[], double phi[], double theta[], double imgcrd[], double pixcrd[]) { static const char *function = "wcsmix"; const int niter = 60; int crossed, istep, iter, j, k, nstep, retry, stat[1], status; const double tol = 1.0e-10; const double tol2 = 100.0*tol; double *worldlat, *worldlng; double lambda, span[2], step; double pixmix; double dlng, lng, lng0, lng0m, lng1, lng1m; double dlat, lat, lat0, lat0m, lat1, lat1m; double d, d0, d0m, d1, d1m, dx = 0.0; double dabs, dmin, lmin; double dphi, phi0, phi1; struct celprm *wcscel = &(wcs->cel); struct wcsprm wcs0; struct wcserr **err; /* Initialize if required. */ if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } worldlng = world + wcs->lng; worldlat = world + wcs->lat; /* Check vspan. */ if (vspan[0] <= vspan[1]) { span[0] = vspan[0]; span[1] = vspan[1]; } else { /* Swap them. */ span[0] = vspan[1]; span[1] = vspan[0]; } /* Check vstep. */ step = fabs(vstep); if (step == 0.0) { step = (span[1] - span[0])/10.0; if (step > 1.0 || step == 0.0) step = 1.0; } /* Check viter. */ nstep = viter; if (nstep < 5) { nstep = 5; } else if (nstep > 10) { nstep = 10; } /* Given pixel element. */ pixmix = pixcrd[mixpix]; /* Iterate on the step size. */ for (istep = 0; istep <= nstep; istep++) { if (istep) step /= 2.0; /* Iterate on the sky coordinate between the specified range. */ if (mixcel == 1) { /* Celestial longitude is given. */ /* Check whether the solution interval is a crossing interval. */ lat0 = span[0]; *worldlat = lat0; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = pixcrd[mixpix] - pixmix; dabs = fabs(d0); if (dabs < tol) return 0; lat1 = span[1]; *worldlat = lat1; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1 = pixcrd[mixpix] - pixmix; dabs = fabs(d1); if (dabs < tol) return 0; lmin = lat1; dmin = dabs; /* Check for a crossing point. */ if (signbit(d0) != signbit(d1)) { crossed = 1; dx = d1; } else { crossed = 0; lat0 = span[1]; } for (retry = 0; retry < 4; retry++) { /* Refine the solution interval. */ while (lat0 > span[0]) { lat0 -= step; if (lat0 < span[0]) lat0 = span[0]; *worldlat = lat0; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = pixcrd[mixpix] - pixmix; /* Check for a solution. */ dabs = fabs(d0); if (dabs < tol) return 0; /* Record the point of closest approach. */ if (dabs < dmin) { lmin = lat0; dmin = dabs; } /* Check for a crossing point. */ if (signbit(d0) != signbit(d1)) { crossed = 2; dx = d0; break; } /* Advance to the next subinterval. */ lat1 = lat0; d1 = d0; } if (crossed) { /* A crossing point was found. */ for (iter = 0; iter < niter; iter++) { /* Use regula falsi division of the interval. */ lambda = d0/(d0-d1); if (lambda < 0.1) { lambda = 0.1; } else if (lambda > 0.9) { lambda = 0.9; } dlat = lat1 - lat0; lat = lat0 + lambda*dlat; *worldlat = lat; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } /* Check for a solution. */ d = pixcrd[mixpix] - pixmix; dabs = fabs(d); if (dabs < tol) return 0; if (dlat < tol) { /* An artifact of numerical imprecision. */ if (dabs < tol2) return 0; /* Must be a discontinuity. */ break; } /* Record the point of closest approach. */ if (dabs < dmin) { lmin = lat; dmin = dabs; } if (signbit(d0) == signbit(d)) { lat0 = lat; d0 = d; } else { lat1 = lat; d1 = d; } } /* No convergence, must have been a discontinuity. */ if (crossed == 1) lat0 = span[1]; lat1 = lat0; d1 = dx; crossed = 0; } else { /* No crossing point; look for a tangent point. */ if (lmin == span[0]) break; if (lmin == span[1]) break; lat = lmin; lat0 = lat - step; if (lat0 < span[0]) lat0 = span[0]; lat1 = lat + step; if (lat1 > span[1]) lat1 = span[1]; *worldlat = lat0; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = fabs(pixcrd[mixpix] - pixmix); d = dmin; *worldlat = lat1; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1 = fabs(pixcrd[mixpix] - pixmix); for (iter = 0; iter < niter; iter++) { lat0m = (lat0 + lat)/2.0; *worldlat = lat0m; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0m = fabs(pixcrd[mixpix] - pixmix); if (d0m < tol) return 0; lat1m = (lat1 + lat)/2.0; *worldlat = lat1m; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1m = fabs(pixcrd[mixpix] - pixmix); if (d1m < tol) return 0; if (d0m < d && d0m <= d1m) { lat1 = lat; d1 = d; lat = lat0m; d = d0m; } else if (d1m < d) { lat0 = lat; d0 = d; lat = lat1m; d = d1m; } else { lat0 = lat0m; d0 = d0m; lat1 = lat1m; d1 = d1m; } } } } } else { /* Celestial latitude is given. */ /* Check whether the solution interval is a crossing interval. */ lng0 = span[0]; *worldlng = lng0; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = pixcrd[mixpix] - pixmix; dabs = fabs(d0); if (dabs < tol) return 0; lng1 = span[1]; *worldlng = lng1; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1 = pixcrd[mixpix] - pixmix; dabs = fabs(d1); if (dabs < tol) return 0; lmin = lng1; dmin = dabs; /* Check for a crossing point. */ if (signbit(d0) != signbit(d1)) { crossed = 1; dx = d1; } else { crossed = 0; lng0 = span[1]; } for (retry = 0; retry < 4; retry++) { /* Refine the solution interval. */ while (lng0 > span[0]) { lng0 -= step; if (lng0 < span[0]) lng0 = span[0]; *worldlng = lng0; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = pixcrd[mixpix] - pixmix; /* Check for a solution. */ dabs = fabs(d0); if (dabs < tol) return 0; /* Record the point of closest approach. */ if (dabs < dmin) { lmin = lng0; dmin = dabs; } /* Check for a crossing point. */ if (signbit(d0) != signbit(d1)) { crossed = 2; dx = d0; break; } /* Advance to the next subinterval. */ lng1 = lng0; d1 = d0; } if (crossed) { /* A crossing point was found. */ for (iter = 0; iter < niter; iter++) { /* Use regula falsi division of the interval. */ lambda = d0/(d0-d1); if (lambda < 0.1) { lambda = 0.1; } else if (lambda > 0.9) { lambda = 0.9; } dlng = lng1 - lng0; lng = lng0 + lambda*dlng; *worldlng = lng; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } /* Check for a solution. */ d = pixcrd[mixpix] - pixmix; dabs = fabs(d); if (dabs < tol) return 0; if (dlng < tol) { /* An artifact of numerical imprecision. */ if (dabs < tol2) return 0; /* Must be a discontinuity. */ break; } /* Record the point of closest approach. */ if (dabs < dmin) { lmin = lng; dmin = dabs; } if (signbit(d0) == signbit(d)) { lng0 = lng; d0 = d; } else { lng1 = lng; d1 = d; } } /* No convergence, must have been a discontinuity. */ if (crossed == 1) lng0 = span[1]; lng1 = lng0; d1 = dx; crossed = 0; } else { /* No crossing point; look for a tangent point. */ if (lmin == span[0]) break; if (lmin == span[1]) break; lng = lmin; lng0 = lng - step; if (lng0 < span[0]) lng0 = span[0]; lng1 = lng + step; if (lng1 > span[1]) lng1 = span[1]; *worldlng = lng0; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = fabs(pixcrd[mixpix] - pixmix); d = dmin; *worldlng = lng1; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1 = fabs(pixcrd[mixpix] - pixmix); for (iter = 0; iter < niter; iter++) { lng0m = (lng0 + lng)/2.0; *worldlng = lng0m; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0m = fabs(pixcrd[mixpix] - pixmix); if (d0m < tol) return 0; lng1m = (lng1 + lng)/2.0; *worldlng = lng1m; if ((status = wcss2p(wcs, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1m = fabs(pixcrd[mixpix] - pixmix); if (d1m < tol) return 0; if (d0m < d && d0m <= d1m) { lng1 = lng; d1 = d; lng = lng0m; d = d0m; } else if (d1m < d) { lng0 = lng; d0 = d; lng = lng1m; d = d1m; } else { lng0 = lng0m; d0 = d0m; lng1 = lng1m; d1 = d1m; } } } } } } /* Set cel0 to the unity transformation. */ wcs0 = *wcs; wcs0.cel.euler[0] = -90.0; wcs0.cel.euler[1] = 0.0; wcs0.cel.euler[2] = 90.0; wcs0.cel.euler[3] = 1.0; wcs0.cel.euler[4] = 0.0; /* No convergence, check for aberrant behaviour at a native pole. */ *theta = -90.0; for (j = 1; j <= 2; j++) { /* Could the celestial coordinate element map to a native pole? */ *phi = 0.0; *theta = -*theta; sphx2s(wcscel->euler, 1, 1, 1, 1, phi, theta, &lng, &lat); if (mixcel == 1) { if (fabs(fmod(*worldlng-lng, 360.0)) > tol) continue; if (lat < span[0]) continue; if (lat > span[1]) continue; *worldlat = lat; } else { if (fabs(*worldlat-lat) > tol) continue; if (lng < span[0]) lng += 360.0; if (lng > span[1]) lng -= 360.0; if (lng < span[0]) continue; if (lng > span[1]) continue; *worldlng = lng; } /* Is there a solution for the given pixel coordinate element? */ lng = *worldlng; lat = *worldlat; /* Feed native coordinates to wcss2p() with cel0 set to unity. */ *worldlng = -180.0; *worldlat = *theta; if ((status = wcss2p(&wcs0, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (wcs->err) free(wcs->err); wcs->err = wcs0.err; if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d0 = pixcrd[mixpix] - pixmix; /* Check for a solution. */ if (fabs(d0) < tol) { /* Recall saved world coordinates. */ *worldlng = lng; *worldlat = lat; return 0; } /* Search for a crossing interval. */ phi0 = -180.0; for (k = -179; k <= 180; k++) { phi1 = (double) k; *worldlng = phi1; if ((status = wcss2p(&wcs0, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (wcs->err) free(wcs->err); wcs->err = wcs0.err; if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } d1 = pixcrd[mixpix] - pixmix; /* Check for a solution. */ dabs = fabs(d1); if (dabs < tol) { /* Recall saved world coordinates. */ *worldlng = lng; *worldlat = lat; return 0; } /* Is it a crossing interval? */ if (signbit(d0) != signbit(d1)) break; phi0 = phi1; d0 = d1; } for (iter = 1; iter <= niter; iter++) { /* Use regula falsi division of the interval. */ lambda = d0/(d0-d1); if (lambda < 0.1) { lambda = 0.1; } else if (lambda > 0.9) { lambda = 0.9; } dphi = phi1 - phi0; *worldlng = phi0 + lambda*dphi; if ((status = wcss2p(&wcs0, 1, 0, world, phi, theta, imgcrd, pixcrd, stat))) { if (wcs->err) free(wcs->err); wcs->err = wcs0.err; if (status == WCSERR_BAD_WORLD) { status = wcserr_set(WCS_ERRMSG(WCSERR_BAD_WORLD_COORD)); } return status; } /* Check for a solution. */ d = pixcrd[mixpix] - pixmix; dabs = fabs(d); if (dabs < tol || (dphi < tol && dabs < tol2)) { /* Recall saved world coordinates. */ *worldlng = lng; *worldlat = lat; return 0; } if (signbit(d0) == signbit(d)) { phi0 = *worldlng; d0 = d; } else { phi1 = *worldlng; d1 = d; } } } /* No solution. */ return wcserr_set(WCS_ERRMSG(WCSERR_NO_SOLUTION)); } /*--------------------------------------------------------------------------*/ int wcssptr( struct wcsprm *wcs, int *i, char ctype[9]) { static const char *function = "wcssptr"; int j, status; double cdelt, crval; struct wcserr **err; /* Initialize if required. */ if (wcs == 0x0) return WCSERR_NULL_POINTER; err = &(wcs->err); if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } if ((j = *i) < 0) { if ((j = wcs->spec) < 0) { /* Look for a linear spectral axis. */ for (j = 0; j < wcs->naxis; j++) { if (wcs->types[j]/100 == 30) { break; } } if (j >= wcs->naxis) { /* No spectral axis. */ return wcserr_set(WCSERR_SET(WCSERR_BAD_SUBIMAGE), "No spectral axis found."); } } *i = j; } /* Translate the spectral axis. */ if (spctrne(wcs->ctype[j], wcs->crval[j], wcs->cdelt[j], wcs->restfrq, wcs->restwav, ctype, &crval, &cdelt, &(wcs->spc.err))) { return wcserr_set(WCS_ERRMSG(WCSERR_BAD_COORD_TRANS)); } /* Translate keyvalues. */ wcs->flag = 0; wcs->cdelt[j] = cdelt; wcs->crval[j] = crval; spctyp(ctype, 0x0, 0x0, 0x0, wcs->cunit[j], 0x0, 0x0, 0x0); strcpy(wcs->ctype[j], ctype); /* This keeps things tidy if the spectral axis is linear. */ spcini(&(wcs->spc)); return 0; } pywcs-1.12/wcslib/C/wcs.h0000644001153600020070000017546312310355626017300 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcs.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of celestial coordinates in FITS", * Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077 (Paper II) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the wcs routines * --------------------------- * These routines implement the FITS World Coordinate System (WCS) standard * which defines methods to be used for computing world coordinates from image * pixel coordinates, and vice versa. They are based on the wcsprm struct * which contains all information needed for the computations. The struct * contains some members that must be set by the user, and others that are * maintained by these routines, somewhat like a C++ class but with no * encapsulation. * * Three routines, wcsini(), wcssub(), and wcsfree() are provided to manage the * wcsprm struct and another, wcsprt(), to prints its contents. Refer to the * description of the wcsprm struct for an explanation of the anticipated usage * of these routines. wcscopy(), which does a deep copy of one wcsprm struct * to another, is defined as a preprocessor macro function that invokes * wcssub(). * * wcsperr() prints the error message(s) (if any) stored in a wcsprm struct, * and the linprm, celprm, prjprm, spcprm, and tabprm structs that it contains. * * A setup routine, wcsset(), computes intermediate values in the wcsprm struct * from parameters in it that were supplied by the user. The struct always * needs to be set up by wcsset() but this need not be called explicitly - * refer to the explanation of wcsprm::flag. * * wcsp2s() and wcss2p() implement the WCS world coordinate transformations. * In fact, they are high level driver routines for the WCS linear, * logarithmic, celestial, spectral and tabular transformation routines * described in lin.h, log.h, cel.h, spc.h and tab.h. * * Given either the celestial longitude or latitude plus an element of the * pixel coordinate a hybrid routine, wcsmix(), iteratively solves for the * unknown elements. * * wcssptr() translates the spectral axis in a wcsprm struct. For example, a * 'FREQ' axis may be translated into 'ZOPT-F2W' and vice versa. * * Quadcube projections: * --------------------- * The quadcube projections (TSC, CSC, QSC) may be represented in FITS in * either of two ways: * * a: The six faces may be laid out in one plane and numbered as follows: * = 0 = = 4 3 2 1 4 3 2 = = 5 * * Faces 2, 3 and 4 may appear on one side or the other (or both). The * world-to-pixel routines map faces 2, 3 and 4 to the left but the * pixel-to-world routines accept them on either side. * * b: The "COBE" convention in which the six faces are stored in a * three-dimensional structure using a CUBEFACE axis indexed from * 0 to 5 as above. * * These routines support both methods; wcsset() determines which is being * used by the presence or absence of a CUBEFACE axis in ctype[]. wcsp2s() * and wcss2p() translate the CUBEFACE axis representation to the single * plane representation understood by the lower-level WCSLIB projection * routines. * * * wcsini() - Default constructor for the wcsprm struct * ---------------------------------------------------- * wcsini() optionally allocates memory for arrays in a wcsprm struct and sets * all members of the struct to default values. Memory is allocated for up to * NPVMAX PVi_ma keywords or NPSMAX PSi_ma keywords per WCS representation. * These may be changed via wcsnpv() and wcsnps() before wcsini() is called. * * PLEASE NOTE: every wcsprm struct should be initialized by wcsini(), possibly * repeatedly. On the first invokation, and only the first invokation, * wcsprm::flag must be set to -1 to initialize memory management, regardless * of whether wcsini() will actually be used to allocate memory. * * Given: * alloc int If true, allocate memory unconditionally for the * crpix, etc. arrays. * * If false, it is assumed that pointers to these arrays * have been set by the user except if they are null * pointers in which case memory will be allocated for * them regardless. (In other words, setting alloc true * saves having to initalize these pointers to zero.) * * naxis int The number of world coordinate axes. This is used to * determine the length of the various wcsprm vectors and * matrices and therefore the amount of memory to * allocate for them. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Note that, in order to initialize memory management, * wcsprm::flag should be set to -1 when wcs is * initialized for the first time (memory leaks may * result if it had already been initialized). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * wcsnpv() - Memory allocation for PVi_ma * --------------------------------------- * wcsnpv() changes the value of NPVMAX (default 64). This global variable * controls the number of PVi_ma keywords that wcsini() should allocate space * for. * * PLEASE NOTE: This function is not thread-safe. * * Given: * n int Value of NPVMAX; ignored if < 0. * * Function return value: * int Current value of NPVMAX. * * * wcsnps() - Memory allocation for PSi_ma * --------------------------------------- * wcsnps() changes the values of NPSMAX (default 8). This global variable * controls the number of PSi_ma keywords that wcsini() should allocate space * for. * * PLEASE NOTE: This function is not thread-safe. * * Given: * n int Value of NPSMAX; ignored if < 0. * * Function return value: * int Current value of NPSMAX. * * * wcssub() - Subimage extraction routine for the wcsprm struct * ------------------------------------------------------------ * wcssub() extracts the coordinate description for a subimage from a wcsprm * struct. It does a deep copy, using wcsini() to allocate memory for its * arrays if required. Only the "information to be provided" part of the * struct is extracted; a call to wcsset() is required to set up the remainder. * * The world coordinate system of the subimage must be separable in the sense * that the world coordinates at any point in the subimage must depend only on * the pixel coordinates of the axes extracted. In practice, this means that * the PCi_ja matrix of the original image must not contain non-zero * off-diagonal terms that associate any of the subimage axes with any of the * non-subimage axes. * * Note that while the required elements of the tabprm array are extracted, the * wtbarr array is not. (Thus it is not appropriate to call wcssub() after * wcstab() but before filling the tabprm structs - refer to wcshdr.h.) * * wcssub() can also add axes to a wcsprm struct. The new axes will be created * using the defaults set by wcsini() which produce a simple, unnamed, linear * axis with world coordinate equal to the pixel coordinate. These default * values can be changed in before invoking wcsset(). * * Given: * alloc int If true, allocate memory for the crpix, etc. arrays in * the destination. Otherwise, it is assumed that * pointers to these arrays have been set by the user * except if they are null pointers in which case memory * will be allocated for them regardless. * * wcssrc const struct wcsprm* * Struct to extract from. * * Given and returned: * nsub int* * axes int[] Vector of length *nsub containing the image axis * numbers (1-relative) to extract. Order is * significant; axes[0] is the axis number of the input * image that corresponds to the first axis in the * subimage, etc. * * Use an axis number of 0 to create a new axis using * the defaults set by wcsini(). * * nsub (the pointer) may be set to zero, and so also may * nsub, to indicate the number of axes in the input * image; the number of axes will be returned if * nsub != 0x0. axes itself (the pointer) may be set to * zero to indicate the first *nsub axes in their * original order. * * Set both nsub and axes to zero to do a deep copy of * one wcsprm struct to another. * * Subimage extraction by coordinate axis type may be * done by setting the elements of axes[] to the * following special preprocessor macro values: * * WCSSUB_LONGITUDE: Celestial longitude. * WCSSUB_LATITUDE: Celestial latitude. * WCSSUB_CUBEFACE: Quadcube CUBEFACE axis. * WCSSUB_SPECTRAL: Spectral axis. * WCSSUB_STOKES: Stokes axis. * * Refer to the notes (below) for further usage examples. * * On return, *nsub will contain the number of axes in * the subimage; this may be zero if there were no axes * of the required type(s) (in which case no memory will * be allocated). axes[] will contain the axis numbers * that were extracted, or 0 for newly created axes. The * vector length must be sufficient to contain all axis * numbers. No checks are performed to verify that the * coordinate axes are consistent, this is done by * wcsset(). * * wcsdst struct wcsprm* * Struct describing the subimage. wcsprm::flag should * be set to -1 if wcsdst was not previously initialized * (memory leaks may result if it was previously * initialized). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 12: Invalid subimage specification. * 13: Non-separable subimage coordinate system. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * Notes: * Combinations of subimage axes of particular types may be extracted in the * same order as they occur in the input image by combining preprocessor * codes, for example * = *nsub = 1; = axes[0] = WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_SPECTRAL; * * would extract the longitude, latitude, and spectral axes in the same order * as the input image. If one of each were present, *nsub = 3 would be * returned. * * For convenience, WCSSUB_CELESTIAL is defined as the combination * WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_CUBEFACE. * * The codes may also be negated to extract all but the types specified, for * example * = *nsub = 4; = axes[0] = WCSSUB_LONGITUDE; = axes[1] = WCSSUB_LATITUDE; = axes[2] = WCSSUB_CUBEFACE; = axes[3] = -(WCSSUB_SPECTRAL | WCSSUB_STOKES); * * The last of these specifies all axis types other than spectral or Stokes. * Extraction is done in the order specified by axes[] a longitude axis (if * present) would be extracted first (via axes[0]) and not subsequently (via * axes[3]). Likewise for the latitude and cubeface axes in this example. * * From the foregoing, it is apparent that the value of *nsub returned may be * less than or greater than that given. However, it will never exceed the * number of axes in the input image (plus the number of newly-created axes * if any were specified on input). * * * wcscopy() macro - Copy routine for the wcsprm struct * ---------------------------------------------------- * wcscopy() does a deep copy of one wcsprm struct to another. As of * WCSLIB 3.6, it is implemented as a preprocessor macro that invokes * wcssub() with the nsub and axes pointers both set to zero. * * * wcsfree() - Destructor for the wcsprm struct * -------------------------------------------- * wcsfree() frees memory allocated for the wcsprm arrays by wcsini() and/or * wcsset(). wcsini() records the memory it allocates and wcsfree() will only * attempt to free this. * * PLEASE NOTE: wcsfree() must not be invoked on a wcsprm struct that was not * initialized by wcsini(). * * Returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * * * wcsprt() - Print routine for the wcsprm struct * ---------------------------------------------- * wcsprt() prints the contents of a wcsprm struct using wcsprintf(). Mainly * intended for diagnostic purposes. * * Given: * wcs const struct wcsprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * * * wcsperr() - Print error messages from a wcsprm struct * ----------------------------------------------------- * wcsperr() prints the error message(s), if any, stored in a wcsprm struct, * and the linprm, celprm, prjprm, spcprm, and tabprm structs that it contains. * If there are no errors then nothing is printed. It uses wcserr_prt(), q.v. * * Given: * wcs const struct wcsprm* * Coordinate transformation parameters. * * prefix const char * * If non-NULL, each output line will be prefixed with * this string. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * * * wcsset() - Setup routine for the wcsprm struct * ---------------------------------------------- * wcsset() sets up a wcsprm struct according to information supplied within * it (refer to the description of the wcsprm struct). * * wcsset() recognizes the NCP projection and converts it to the equivalent SIN * projection and likewise translates GLS into SFL. It also translates the * AIPS spectral types ('FREQ-LSR', 'FELO-HEL', etc.), possibly changing the * input header keywords wcsprm::ctype and/or wcsprm::specsys if necessary. * * Note that this routine need not be called directly; it will be invoked by * wcsp2s() and wcss2p() if the wcsprm::flag is anything other than a * predefined magic value. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * wcsp2s() - Pixel-to-world transformation * ---------------------------------------- * wcsp2s() transforms pixel coordinates to world coordinates. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Given: * ncoord, * nelem int The number of coordinates, each of vector length * nelem but containing wcs.naxis coordinate elements. * Thus nelem must equal or exceed the value of the * NAXIS keyword unless ncoord == 1, in which case nelem * is not used. * * pixcrd const double[ncoord][nelem] * Array of pixel coordinates. * * Returned: * imgcrd double[ncoord][nelem] * Array of intermediate world coordinates. For * celestial axes, imgcrd[][wcs.lng] and * imgcrd[][wcs.lat] are the projected x-, and * y-coordinates in pseudo "degrees". For spectral * axes, imgcrd[][wcs.spec] is the intermediate spectral * coordinate, in SI units. * * phi,theta double[ncoord] * Longitude and latitude in the native coordinate system * of the projection [deg]. * * world double[ncoord][nelem] * Array of world coordinates. For celestial axes, * world[][wcs.lng] and world[][wcs.lat] are the * celestial longitude and latitude [deg]. For * spectral axes, imgcrd[][wcs.spec] is the intermediate * spectral coordinate, in SI units. * * stat int[ncoord] * Status return value for each coordinate: * 0: Success. * 1+: A bit mask indicating invalid pixel coordinate * element(s). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * 8: One or more of the pixel coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * wcss2p() - World-to-pixel transformation * ---------------------------------------- * wcss2p() transforms world coordinates to pixel coordinates. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Given: * ncoord, * nelem int The number of coordinates, each of vector length nelem * but containing wcs.naxis coordinate elements. Thus * nelem must equal or exceed the value of the NAXIS * keyword unless ncoord == 1, in which case nelem is not * used. * * world const double[ncoord][nelem] * Array of world coordinates. For celestial axes, * world[][wcs.lng] and world[][wcs.lat] are the * celestial longitude and latitude [deg]. For spectral * axes, world[][wcs.spec] is the spectral coordinate, in * SI units. * * Returned: * phi,theta double[ncoord] * Longitude and latitude in the native coordinate * system of the projection [deg]. * * imgcrd double[ncoord][nelem] * Array of intermediate world coordinates. For * celestial axes, imgcrd[][wcs.lng] and * imgcrd[][wcs.lat] are the projected x-, and * y-coordinates in pseudo "degrees". For quadcube * projections with a CUBEFACE axis the face number is * also returned in imgcrd[][wcs.cubeface]. For * spectral axes, imgcrd[][wcs.spec] is the intermediate * spectral coordinate, in SI units. * * pixcrd double[ncoord][nelem] * Array of pixel coordinates. * * stat int[ncoord] * Status return value for each coordinate: * 0: Success. * 1+: A bit mask indicating invalid world coordinate * element(s). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * 9: One or more of the world coordinates were * invalid, as indicated by the stat vector. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * wcsmix() - Hybrid coordinate transformation * ------------------------------------------- * wcsmix(), given either the celestial longitude or latitude plus an element * of the pixel coordinate, solves for the remaining elements by iterating on * the unknown celestial coordinate element using wcss2p(). Refer also to the * notes below. * * Given and returned: * wcs struct wcsprm* * Indices for the celestial coordinates obtained * by parsing the wcsprm::ctype[]. * * Given: * mixpix int Which element of the pixel coordinate is given. * * mixcel int Which element of the celestial coordinate is given: * 1: Celestial longitude is given in * world[wcs.lng], latitude returned in * world[wcs.lat]. * 2: Celestial latitude is given in * world[wcs.lat], longitude returned in * world[wcs.lng]. * * vspan const double[2] * Solution interval for the celestial coordinate [deg]. * The ordering of the two limits is irrelevant. * Longitude ranges may be specified with any convenient * normalization, for example [-120,+120] is the same as * [240,480], except that the solution will be returned * with the same normalization, i.e. lie within the * interval specified. * * vstep const double * Step size for solution search [deg]. If zero, a * sensible, although perhaps non-optimal default will be * used. * * viter int If a solution is not found then the step size will be * halved and the search recommenced. viter controls how * many times the step size is halved. The allowed range * is 5 - 10. * * Given and returned: * world double[naxis] * World coordinate elements. world[wcs.lng] and * world[wcs.lat] are the celestial longitude and * latitude [deg]. Which is given and which returned * depends on the value of mixcel. All other elements * are given. * * Returned: * phi,theta double[naxis] * Longitude and latitude in the native coordinate * system of the projection [deg]. * * imgcrd double[naxis] * Image coordinate elements. imgcrd[wcs.lng] and * imgcrd[wcs.lat] are the projected x-, and * y-coordinates in pseudo "degrees". * * Given and returned: * pixcrd double[naxis] * Pixel coordinate. The element indicated by mixpix is * given and the remaining elements are returned. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * 10: Invalid world coordinate. * 11: No solution found in the specified interval. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * Notes: * Initially the specified solution interval is checked to see if it's a * "crossing" interval. If it isn't, a search is made for a crossing * solution by iterating on the unknown celestial coordinate starting at the * upper limit of the solution interval and decrementing by the specified * step size. A crossing is indicated if the trial value of the pixel * coordinate steps through the value specified. If a crossing interval is * found then the solution is determined by a modified form of "regula falsi" * division of the crossing interval. If no crossing interval was found * within the specified solution interval then a search is made for a * "non-crossing" solution as may arise from a point of tangency. The * process is complicated by having to make allowance for the discontinuities * that occur in all map projections. * * Once one solution has been determined others may be found by subsequent * invokations of wcsmix() with suitably restricted solution intervals. * * Note the circumstance that arises when the solution point lies at a native * pole of a projection in which the pole is represented as a finite curve, * for example the zenithals and conics. In such cases two or more valid * solutions may exist but wcsmix() only ever returns one. * * Because of its generality wcsmix() is very compute-intensive. For * compute-limited applications more efficient special-case solvers could be * written for simple projections, for example non-oblique cylindrical * projections. * * * wcssptr() - Spectral axis translation * ------------------------------------- * wcssptr() translates the spectral axis in a wcsprm struct. For example, a * 'FREQ' axis may be translated into 'ZOPT-F2W' and vice versa. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * i int* Index of the spectral axis (0-relative). If given < 0 * it will be set to the first spectral axis identified * from the ctype[] keyvalues in the wcsprm struct. * * ctype char[9] Desired spectral CTYPEia. Wildcarding may be used as * for the ctypeS2 argument to spctrn() as described in * the prologue of spc.h, i.e. if the final three * characters are specified as "???", or if just the * eighth character is specified as '?', the correct * algorithm code will be substituted and returned. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * 12: Invalid subimage specification (no spectral * axis). * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * wcsprm struct - Coordinate transformation parameters * ---------------------------------------------------- * The wcsprm struct contains information required to transform world * coordinates. It consists of certain members that must be set by the user * ("given") and others that are set by the WCSLIB routines ("returned"). * Some of the former are not actually required for transforming coordinates. * These are described as "auxiliary"; the struct simply provides a place to * store them, though they may be used by wcshdo() in constructing a FITS * header from a wcsprm struct. Some of the returned values are supplied for * informational purposes and others are for internal use only as indicated. * * In practice, it is expected that a WCS parser would scan the FITS header to * determine the number of coordinate axes. It would then use wcsini() to * allocate memory for arrays in the wcsprm struct and set default values. * Then as it reread the header and identified each WCS keyrecord it would load * the value into the relevant wcsprm array element. This is essentially what * wcspih() does - refer to the prologue of wcshdr.h. As the final step, * wcsset() is invoked, either directly or indirectly, to set the derived * members of the wcsprm struct. wcsset() strips off trailing blanks in all * string members and null-fills the character array. * * int flag * (Given and returned) This flag must be set to zero whenever any of the * following wcsprm struct members are set or changed: * * - wcsprm::naxis (q.v., not normally set by the user), * - wcsprm::crpix, * - wcsprm::pc, * - wcsprm::cdelt, * - wcsprm::crval, * - wcsprm::cunit, * - wcsprm::ctype, * - wcsprm::lonpole, * - wcsprm::latpole, * - wcsprm::restfrq, * - wcsprm::restwav, * - wcsprm::npv, * - wcsprm::pv, * - wcsprm::nps, * - wcsprm::ps, * - wcsprm::cd, * - wcsprm::crota, * - wcsprm::altlin. * * This signals the initialization routine, wcsset(), to recompute the * returned members of the celprm struct. celset() will reset flag to * indicate that this has been done. * * PLEASE NOTE: flag should be set to -1 when wcsini() is called for the * first time for a particular wcsprm struct in order to initialize memory * management. It must ONLY be used on the first initialization otherwise * memory leaks may result. * * int naxis * (Given or returned) Number of pixel and world coordinate elements. * * If wcsini() is used to initialize the linprm struct (as would normally * be the case) then it will set naxis from the value passed to it as a * function argument. The user should not subsequently modify it. * * double *crpix * (Given) Address of the first element of an array of double containing * the coordinate reference pixel, CRPIXja. * * double *pc * (Given) Address of the first element of the PCi_ja (pixel coordinate) * transformation matrix. The expected order is * = struct wcsprm wcs; = wcs.pc = {PC1_1, PC1_2, PC2_1, PC2_2}; * * This may be constructed conveniently from a 2-D array via * = double m[2][2] = {{PC1_1, PC1_2}, = {PC2_1, PC2_2}}; * * which is equivalent to * = double m[2][2]; = m[0][0] = PC1_1; = m[0][1] = PC1_2; = m[1][0] = PC2_1; = m[1][1] = PC2_2; * * The storage order for this 2-D array is the same as for the 1-D array, * whence * = wcs.pc = *m; * * would be legitimate. * * double *cdelt * (Given) Address of the first element of an array of double containing * the coordinate increments, CDELTia. * * double *crval * (Given) Address of the first element of an array of double containing * the coordinate reference values, CRVALia. * * char (*cunit)[72] * (Given) Address of the first element of an array of char[72] containing * the CUNITia keyvalues which define the units of measurement of the * CRVALia, CDELTia, and CDi_ja keywords. * * As CUNITia is an optional header keyword, cunit[][72] may be left blank * but otherwise is expected to contain a standard units specification as * defined by WCS Paper I. Utility function wcsutrn(), described in * wcsunits.h, is available to translate commonly used non-standard units * specifications but this must be done as a separate step before invoking * wcsset(). * * For celestial axes, if cunit[][72] is not blank, wcsset() uses * wcsunits() to parse it and scale cdelt[], crval[], and cd[][*] to * degrees. It then resets cunit[][72] to "deg". * * For spectral axes, if cunit[][72] is not blank, wcsset() uses wcsunits() * to parse it and scale cdelt[], crval[], and cd[][*] to SI units. It * then resets cunit[][72] accordingly. * * wcsset() ignores cunit[][72] for other coordinate types; cunit[][72] may * be used to label coordinate values. * * These variables accomodate the longest allowed string-valued FITS * keyword, being limited to 68 characters, plus the null-terminating * character. * * char (*ctype)[72] * (Given) Address of the first element of an array of char[72] containing * the coordinate axis types, CTYPEia. * * The ctype[][72] keyword values must be in upper case and there must be * zero or one pair of matched celestial axis types, and zero or one * spectral axis. The ctype[][72] strings should be padded with blanks on * the right and null-terminated so that they are at least eight characters * in length. * * These variables accomodate the longest allowed string-valued FITS * keyword, being limited to 68 characters, plus the null-terminating * character. * * double lonpole * (Given and returned) The native longitude of the celestial pole, phi_p, * given by LONPOLEa [deg] or by PVi_2a [deg] attached to the longitude * axis which takes precedence if defined, and ... * double latpole * (Given and returned) ... the native latitude of the celestial pole, * theta_p, given by LATPOLEa [deg] or by PVi_3a [deg] attached to the * longitude axis which takes precedence if defined. * * lonpole and latpole may be left to default to values set by wcsini() * (see celprm::ref), but in any case they will be reset by wcsset() to * the values actually used. Note therefore that if the wcsprm struct is * reused without resetting them, whether directly or via wcsini(), they * will no longer have their default values. * * double restfrq * (Given) The rest frequency [Hz], and/or ... * double restwav * (Given) ... the rest wavelength in vacuuo [m], only one of which need be * given, the other should be set to zero. * * int npv * (Given) The number of entries in the wcsprm::pv[] array. * * int npvmax * (Given or returned) The length of the wcsprm::pv[] array. * * npvmax will be set by wcsini() if it allocates memory for wcsprm::pv[], * otherwise it must be set by the user. See also wcsnpv(). * * struct pvcard *pv * (Given or returned) Address of the first element of an array of length * npvmax of pvcard structs. Set by wcsini() if it allocates memory for * pv[], otherwise it must be set by the user. See also wcsnpv(). * * As a FITS header parser encounters each PVi_ma keyword it should load it * into a pvcard struct in the array and increment npv. wcsset() * interprets these as required. * * Note that, if they were not given, wcsset() resets the entries for * PVi_1a, PVi_2a, PVi_3a, and PVi_4a for longitude axis i to match * phi_0 and theta_0 (the native longitude and latitude of the reference * point), LONPOLEa and LATPOLEa respectively. * * int nps * (Given) The number of entries in the wcsprm::ps[] array. * * int npsmax * (Given or returned) The length of the wcsprm::ps[] array. * * npsmax will be set by wcsini() if it allocates memory for wcsprm::ps[], * otherwise it must be set by the user. See also wcsnps(). * * struct pscard *ps * (Given or returned) Address of the first element of an array of length * npsmax of pscard structs. Set by wcsini() if it allocates memory for * ps[], otherwise it must be set by the user. See also wcsnps(). * * As a FITS header parser encounters each PSi_ma keyword it should load it * into a pscard struct in the array and increment nps. wcsset() * interprets these as required (currently no PSi_ma keyvalues are * recognized). * * double *cd * (Given) For historical compatibility, the wcsprm struct supports two * alternate specifications of the linear transformation matrix, those * associated with the CDi_ja keywords, and ... * double *crota * (Given) ... those associated with the CROTAia keywords. Although these * may not formally co-exist with PCi_ja, the approach taken here is simply * to ignore them if given in conjunction with PCi_ja. * * int altlin * (Given) altlin is a bit flag that denotes which of the PCi_ja, CDi_ja * and CROTAia keywords are present in the header: * * - Bit 0: PCi_ja is present. * * - Bit 1: CDi_ja is present. * * Matrix elements in the IRAF convention are * equivalent to the product CDi_ja = CDELTia * PCi_ja, but the * defaults differ from that of the PCi_ja matrix. If one or more * CDi_ja keywords are present then all unspecified CDi_ja default to * zero. If no CDi_ja (or CROTAia) keywords are present, then the * header is assumed to be in PCi_ja form whether or not any PCi_ja * keywords are present since this results in an interpretation of * CDELTia consistent with the original FITS specification. * * While CDi_ja may not formally co-exist with PCi_ja, it may co-exist * with CDELTia and CROTAia which are to be ignored. * * - Bit 2: CROTAia is present. * * In the AIPS convention, CROTAia may only be * associated with the latitude axis of a celestial axis pair. It * specifies a rotation in the image plane that is applied AFTER the * CDELTia; any other CROTAia keywords are ignored. * * CROTAia may not formally co-exist with PCi_ja. * * CROTAia and CDELTia may formally co-exist with CDi_ja but if so are to * be ignored. * * CDi_ja and CROTAia keywords, if found, are to be stored in the * wcsprm::cd and wcsprm::crota arrays which are dimensioned similarly to * wcsprm::pc and wcsprm::cdelt. FITS * header parsers should use the following procedure: * * - Whenever a PCi_ja keyword is encountered: altlin |= 1; * * - Whenever a CDi_ja keyword is encountered: altlin |= 2; * * - Whenever a CROTAia keyword is encountered: altlin |= 4; * * If none of these bits are set the PCi_ja representation results, i.e. * wcsprm::pc and wcsprm::cdelt will be used as given. * * These alternate specifications of the linear transformation matrix are * translated immediately to PCi_ja by wcsset() and are invisible to the * lower-level WCSLIB routines. In particular, wcsset() resets * wcsprm::cdelt to unity if CDi_ja is present (and no PCi_ja). * * If CROTAia are present but none is associated with the latitude axis * (and no PCi_ja or CDi_ja), then wcsset() reverts to a unity PCi_ja * matrix. * * int velref * (Given) AIPS velocity code VELREF, refer to spcaips(). * * char alt[4] * (Given, auxiliary) Character code for alternate coordinate descriptions * (i.e. the 'a' in keyword names such as CTYPEia). This is blank for the * primary coordinate description, or one of the 26 upper-case letters, * A-Z. * * An array of four characters is provided for alignment purposes, only the * first is used. * * int colnum * (Given, auxiliary) Where the coordinate representation is associated * with an image-array column in a FITS binary table, this variable may be * used to record the relevant column number. * * It should be set to zero for an image header or pixel list. * * int *colax * (Given, auxiliary) Address of the first element of an array of int * recording the column numbers for each axis in a pixel list. * * The array elements should be set to zero for an image header or image * array in a binary table. * * char (*cname)[72] * (Given, auxiliary) The address of the first element of an array of * char[72] containing the coordinate axis names, CNAMEia. * * These variables accomodate the longest allowed string-valued FITS * keyword, being limited to 68 characters, plus the null-terminating * character. * * double *crder * (Given, auxiliary) Address of the first element of an array of double * recording the random error in the coordinate value, CRDERia. * double *csyer * (Given, auxiliary) Address of the first element of an array of double * recording the systematic error in the coordinate value, CSYERia. * * char dateavg[72] * (Given, auxiliary) The date of a representative mid-point of the * observation in ISO format, yyyy-mm-ddThh:mm:ss. * char dateobs[72] * (Given, auxiliary) The date of the start of the observation unless * otherwise explained in the comment field of the DATE-OBS keyword, in * ISO format, yyyy-mm-ddThh:mm:ss. * * double equinox * (Given, auxiliary) The equinox associated with dynamical equatorial or * ecliptic coordinate systems, EQUINOXa (or EPOCH in older headers). Not * applicable to ICRS equatorial or ecliptic coordinates. * * double mjdavg * (Given, auxiliary) Modified Julian Date (MJD = JD - 2400000.5), MJD-AVG, * corresponding to DATE-AVG. * double mjdobs * (Given, auxiliary) Modified Julian Date (MJD = JD - 2400000.5), MJD-OBS, * corresponding to DATE-OBS. * * double obsgeo[3] * (Given, auxiliary) Location of the observer in a standard terrestrial * reference frame, OBSGEO-X, OBSGEO-Y, OBSGEO-Z [m]. * * char radesys[72] * (Given, auxiliary) The equatorial or ecliptic coordinate system type, * RADESYSa. * * char specsys[72] * (Given, auxiliary) Spectral reference frame (standard of rest), * SPECSYSa, and ... * char ssysobs[72] * (Given, auxiliary) ... the actual frame in which there is no * differential variation in the spectral coordinate across the * field-of-view, SSYSOBSa. * double velosys * (Given, auxiliary) The relative radial velocity [m/s] between the * observer and the selected standard of rest in the direction of the * celestial reference coordinate, VELOSYSa. * * double zsource * (Given, auxiliary) The redshift, ZSOURCEa, of the source, and ... * char ssyssrc[72] * (Given, auxiliary) ... the spectral reference frame (standard of rest) * in which this was measured, SSYSSRCa. * * double velangl * (Given, auxiliary) The angle [deg] that should be used to decompose an * observed velocity into radial and transverse components. * * char wcsname[72] * (Given, auxiliary) The name given to the coordinate representation, * WCSNAMEa. This variable accomodates the longest allowed string-valued * FITS keyword, being limited to 68 characters, plus the null-terminating * character. * * int ntab * (Given) See wcsprm::tab. * * int nwtb * (Given) See wcsprm::wtb. * * struct tabprm *tab * (Given) Address of the first element of an array of ntab tabprm structs * for which memory has been allocated. These are used to store tabular * transformation parameters. * * Although technically wcsprm::ntab and tab are "given", they will * normally be set by invoking wcstab(), whether directly or indirectly. * * The tabprm structs contain some members that must be supplied and others * that are derived. The information to be supplied comes primarily from * arrays stored in one or more FITS binary table extensions. These * arrays, referred to here as "wcstab arrays", are themselves located by * parameters stored in the FITS image header. * * struct wtbarr *wtb * (Given) Address of the first element of an array of nwtb wtbarr structs * for which memory has been allocated. These are used in extracting * wcstab arrays from a FITS binary table. * * Although technically wcsprm::nwtb and wtb are "given", they will * normally be set by invoking wcstab(), whether directly or indirectly. * * char lngtyp[8] * (Returned) Four-character WCS celestial longitude and ... * char lattyp[8] * (Returned) ... latitude axis types. e.g. "RA", "DEC", "GLON", "GLAT", * etc. extracted from 'RA--', 'DEC-', 'GLON', 'GLAT', etc. in the first * four characters of CTYPEia but with trailing dashes removed. (Declared * as char[8] for alignment reasons.) * * int lng * (Returned) Index for the longitude coordinate, and ... * int lat * (Returned) ... index for the latitude coordinate, and ... * int spec * (Returned) ... index for the spectral coordinate in the imgcrd[][] and * world[][] arrays in the API of wcsp2s(), wcss2p() and wcsmix(). * * These may also serve as indices into the pixcrd[][] array provided that * the PCi_ja matrix does not transpose axes. * * int cubeface * (Returned) Index into the pixcrd[][] array for the CUBEFACE axis. This * is used for quadcube projections where the cube faces are stored on a * separate axis (see wcs.h). * * int *types * (Returned) Address of the first element of an array of int containing a * four-digit type code for each axis. * * - First digit (i.e. 1000s): * - 0: Non-specific coordinate type. * - 1: Stokes coordinate. * - 2: Celestial coordinate (including CUBEFACE). * - 3: Spectral coordinate. * * - Second digit (i.e. 100s): * - 0: Linear axis. * - 1: Quantized axis (STOKES, CUBEFACE). * - 2: Non-linear celestial axis. * - 3: Non-linear spectral axis. * - 4: Logarithmic axis. * - 5: Tabular axis. * * - Third digit (i.e. 10s): * - 0: Group number, e.g. lookup table number, being an index into the * tabprm array (see above). * * - The fourth digit is used as a qualifier depending on the axis type. * * - For celestial axes: * - 0: Longitude coordinate. * - 1: Latitude coordinate. * - 2: CUBEFACE number. * * - For lookup tables: the axis number in a multidimensional table. * * CTYPEia in "4-3" form with unrecognized algorithm code will have its * type set to -1 and generate an error. * * void *padding * (An unused variable inserted for alignment purposes only.) * * struct linprm lin * (Returned) Linear transformation parameters (usage is described in the * prologue to lin.h). * * struct celprm cel * (Returned) Celestial transformation parameters (usage is described in * the prologue to cel.h). * * struct spcprm spc * (Returned) Spectral transformation parameters (usage is described in the * prologue to spc.h). * * struct wcserr *err * (Returned) If enabled, when an error status is returned this struct * contains detailed information about the error, see wcserr_enable(). * * void *m_padding * (For internal use only.) * int m_flag * (For internal use only.) * int m_naxis * (For internal use only.) * double *m_crpix * (For internal use only.) * double *m_pc * (For internal use only.) * double *m_cdelt * (For internal use only.) * double *m_crval * (For internal use only.) * char (*m_cunit)[72] * (For internal use only.) * char (*m_ctype)[72] * (For internal use only.) * struct pvcard *m_pv * (For internal use only.) * struct pscard *m_ps * (For internal use only.) * double *m_cd * (For internal use only.) * double *m_crota * (For internal use only.) * int *m_colax * (For internal use only.) * char (*m_cname)[72] * (For internal use only.) * double *m_crder * (For internal use only.) * double *m_csyer * (For internal use only.) * struct tabprm *m_tab * (For internal use only.) * struct wtbarr *m_wtb * (For internal use only.) * * * pscard struct - Store for PSi_ma keyrecords * ------------------------------------------- * The pscard struct is used to pass the parsed contents of PSi_ma keyrecords * to wcsset() via the wcsprm struct. * * All members of this struct are to be set by the user. * * int i * (Given) Axis number (1-relative), as in the FITS PSi_ma keyword. * * int m * (Given) Parameter number (non-negative), as in the FITS PSi_ma keyword. * * char value[72] * (Given) Parameter value. * * * pvcard struct - Store for PVi_ma keyrecords * ------------------------------------------- * The pvcard struct is used to pass the parsed contents of PVi_ma keyrecords * to wcsset() via the wcsprm struct. * * All members of this struct are to be set by the user. * * int i * (Given) Axis number (1-relative), as in the FITS PVi_ma keyword. If * i == 0, wcsset() will replace it with the latitude axis number. * * int m * (Given) Parameter number (non-negative), as in the FITS PVi_ma keyword. * * double value * (Given) Parameter value. * * * wtbarr struct - Extraction of coordinate lookup tables from BINTABLE * -------------------------------------------------------------------- * Function wcstab(), which is invoked automatically by wcspih(), sets up an * array of wtbarr structs to assist in extracting coordinate lookup tables * from a binary table extension (BINTABLE) and copying them into the tabprm * structs stored in wcsprm. Refer to the usage notes for wcspih() and * wcstab() in wcshdr.h, and also the prologue to tab.h. * * For C++ usage, because of a name space conflict with the wtbarr typedef * defined in CFITSIO header fitsio.h, the wtbarr struct is renamed to wtbarr_s * by preprocessor macro substitution with scope limited to wcs.h itself. * * int i * (Given) Image axis number. * * int m * (Given) wcstab array axis number for index vectors. * * int kind * (Given) Character identifying the wcstab array type: * - c: coordinate array, * - i: index vector. * * char extnam[72] * (Given) EXTNAME identifying the binary table extension. * * int extver * (Given) EXTVER identifying the binary table extension. * * int extlev * (Given) EXTLEV identifying the binary table extension. * * char ttype[72] * (Given) TTYPEn identifying the column of the binary table that contains * the wcstab array. * * long row * (Given) Table row number. * * int ndim * (Given) Expected dimensionality of the wcstab array. * * int *dimlen * (Given) Address of the first element of an array of int of length ndim * into which the wcstab array axis lengths are to be written. * * double **arrayp * (Given) Pointer to an array of double which is to be allocated by the * user and into which the wcstab array is to be written. * * * Global variable: const char *wcs_errmsg[] - Status return messages * ------------------------------------------------------------------ * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_WCS #define WCSLIB_WCS #include "lin.h" #include "cel.h" #include "spc.h" #include "tab.h" #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif #define WCSSUB_LONGITUDE 0x1001 #define WCSSUB_LATITUDE 0x1002 #define WCSSUB_CUBEFACE 0x1004 #define WCSSUB_CELESTIAL 0x1007 #define WCSSUB_SPECTRAL 0x1008 #define WCSSUB_STOKES 0x1010 extern const char *wcs_errmsg[]; enum wcs_errmsg_enum { WCSERR_SUCCESS = 0, /* Success. */ WCSERR_NULL_POINTER = 1, /* Null wcsprm pointer passed. */ WCSERR_MEMORY = 2, /* Memory allocation failed. */ WCSERR_SINGULAR_MTX = 3, /* Linear transformation matrix is singular. */ WCSERR_BAD_CTYPE = 4, /* Inconsistent or unrecognized coordinate axis types. */ WCSERR_BAD_PARAM = 5, /* Invalid parameter value. */ WCSERR_BAD_COORD_TRANS = 6, /* Invalid coordinate transformation parameters. */ WCSERR_ILL_COORD_TRANS = 7, /* Ill-conditioned coordinate transformation parameters. */ WCSERR_BAD_PIX = 8, /* One or more of the pixel coordinates were invalid. */ WCSERR_BAD_WORLD = 9, /* One or more of the world coordinates were invalid. */ WCSERR_BAD_WORLD_COORD = 10, /* Invalid world coordinate. */ WCSERR_NO_SOLUTION = 11, /* No solution found in the specified interval. */ WCSERR_BAD_SUBIMAGE = 12, /* Invalid subimage specification. */ WCSERR_NON_SEPARABLE = 13 /* Non-separable subimage coordinate system. */ }; /* Struct used for storing PVi_ma keywords. */ struct pvcard { int i; /* Axis number, as in PVi_ma (1-relative). */ int m; /* Parameter number, ditto (0-relative). */ double value; /* Parameter value. */ }; /* Struct used for storing PSi_ma keywords. */ struct pscard { int i; /* Axis number, as in PSi_ma (1-relative). */ int m; /* Parameter number, ditto (0-relative). */ char value[72]; /* Parameter value. */ }; /* For extracting wcstab arrays. Matches */ /* the wtbarr typedef defined in CFITSIO */ /* header fitsio.h. */ #ifdef __cplusplus #define wtbarr wtbarr_s /* See prologue above. */ #endif struct wtbarr { int i; /* Image axis number. */ int m; /* Array axis number for index vectors. */ int kind; /* wcstab array type. */ char extnam[72]; /* EXTNAME of binary table extension. */ int extver; /* EXTVER of binary table extension. */ int extlev; /* EXTLEV of binary table extension. */ char ttype[72]; /* TTYPEn of column containing the array. */ long row; /* Table row number. */ int ndim; /* Expected wcstab array dimensionality. */ int *dimlen; /* Where to write the array axis lengths. */ double **arrayp; /* Where to write the address of the array */ /* allocated to store the wcstab array. */ }; struct wcsprm { /* Initialization flag (see the prologue above). */ /*------------------------------------------------------------------------*/ int flag; /* Set to zero to force initialization. */ /* FITS header keyvalues to be provided (see the prologue above). */ /*------------------------------------------------------------------------*/ int naxis; /* Number of axes (pixel and coordinate). */ double *crpix; /* CRPIXja keyvalues for each pixel axis. */ double *pc; /* PCi_ja linear transformation matrix. */ double *cdelt; /* CDELTia keyvalues for each coord axis. */ double *crval; /* CRVALia keyvalues for each coord axis. */ char (*cunit)[72]; /* CUNITia keyvalues for each coord axis. */ char (*ctype)[72]; /* CTYPEia keyvalues for each coord axis. */ double lonpole; /* LONPOLEa keyvalue. */ double latpole; /* LATPOLEa keyvalue. */ double restfrq; /* RESTFRQa keyvalue. */ double restwav; /* RESTWAVa keyvalue. */ int npv; /* Number of PVi_ma keywords, and the */ int npvmax; /* number for which space was allocated. */ struct pvcard *pv; /* PVi_ma keywords for each i and m. */ int nps; /* Number of PSi_ma keywords, and the */ int npsmax; /* number for which space was allocated. */ struct pscard *ps; /* PSi_ma keywords for each i and m. */ /* Alternative header keyvalues (see the prologue above). */ /*------------------------------------------------------------------------*/ double *cd; /* CDi_ja linear transformation matrix. */ double *crota; /* CROTAia keyvalues for each coord axis. */ int altlin; /* Alternative representations */ /* Bit 0: PCi_ja is present, */ /* Bit 1: CDi_ja is present, */ /* Bit 2: CROTAia is present. */ int velref; /* AIPS velocity code, VELREF. */ /* Auxiliary coordinate system information, not used by WCSLIB. */ char alt[4]; int colnum; int *colax; char (*cname)[72]; double *crder; double *csyer; char dateavg[72]; char dateobs[72]; double equinox; double mjdavg; double mjdobs; double obsgeo[3]; char radesys[72]; char specsys[72]; char ssysobs[72]; double velosys; double zsource; char ssyssrc[72]; double velangl; char wcsname[72]; /* Coordinate lookup tables (see the prologue above). */ /*------------------------------------------------------------------------*/ int ntab; /* Number of separate tables. */ int nwtb; /* Number of wtbarr structs. */ struct tabprm *tab; /* Tabular transformation parameters. */ struct wtbarr *wtb; /* Array of wtbarr structs. */ /* Information derived from the FITS header keyvalues by wcsset(). */ /*------------------------------------------------------------------------*/ char lngtyp[8], lattyp[8]; /* Celestial axis types, e.g. RA, DEC. */ int lng, lat, spec; /* Longitude, latitude and spectral axis */ /* indices (0-relative). */ int cubeface; /* True if there is a CUBEFACE axis. */ int *types; /* Coordinate type codes for each axis. */ void *padding; /* (Dummy inserted for alignment purposes.) */ struct linprm lin; /* Linear transformation parameters. */ struct celprm cel; /* Celestial transformation parameters. */ struct spcprm spc; /* Spectral transformation parameters. */ /* Error handling */ /*------------------------------------------------------------------------*/ struct wcserr *err; /* Private - the remainder are for memory management. */ /*------------------------------------------------------------------------*/ void *m_padding; int m_flag, m_naxis; double *m_crpix, *m_pc, *m_cdelt, *m_crval; char (*m_cunit)[72], (*m_ctype)[72]; struct pvcard *m_pv; struct pscard *m_ps; double *m_cd, *m_crota; int *m_colax; char (*m_cname)[72]; double *m_crder, *m_csyer; struct tabprm *m_tab; struct wtbarr *m_wtb; }; /* Size of the wcsprm struct in int units, used by the Fortran wrappers. */ #define WCSLEN (sizeof(struct wcsprm)/sizeof(int)) int wcsnpv(int n); int wcsnps(int n); int wcsini(int alloc, int naxis, struct wcsprm *wcs); int wcssub(int alloc, const struct wcsprm *wcssrc, int *nsub, int axes[], struct wcsprm *wcsdst); int wcsfree(struct wcsprm *wcs); int wcsprt(const struct wcsprm *wcs); int wcsperr(const struct wcsprm *wcs, const char *prefix); int wcsset(struct wcsprm *wcs); int wcsp2s(struct wcsprm *wcs, int ncoord, int nelem, const double pixcrd[], double imgcrd[], double phi[], double theta[], double world[], int stat[]); int wcss2p(struct wcsprm *wcs, int ncoord, int nelem, const double world[], double phi[], double theta[], double imgcrd[], double pixcrd[], int stat[]); int wcsmix(struct wcsprm *wcs, int mixpix, int mixcel, const double vspan[], double vstep, int viter, double world[], double phi[], double theta[], double imgcrd[], double pixcrd[]); int wcssptr(struct wcsprm *wcs, int *i, char ctype[9]); /* Defined mainly for backwards compatibility, use wcssub() instead. */ #define wcscopy(alloc, wcssrc, wcsdst) wcssub(alloc, wcssrc, 0x0, 0x0, wcsdst) /* Deprecated. */ #define wcsini_errmsg wcs_errmsg #define wcssub_errmsg wcs_errmsg #define wcscopy_errmsg wcs_errmsg #define wcsfree_errmsg wcs_errmsg #define wcsprt_errmsg wcs_errmsg #define wcsset_errmsg wcs_errmsg #define wcsp2s_errmsg wcs_errmsg #define wcss2p_errmsg wcs_errmsg #define wcsmix_errmsg wcs_errmsg #ifdef __cplusplus #undef wtbarr } #endif #endif /* WCSLIB_WCS */ pywcs-1.12/wcslib/C/wcsbth.l0000644001153600020070000015346112310355626017774 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsbth.l,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcsbth.l is a Flex description file containing the definition of a lexical * scanner for parsing the WCS keyrecords for one or more image arrays and/or * pixel lists in a FITS binary table header. It can also handle primary image * and image extension headers. * * wcsbth.l requires Flex v2.5.4 or later. Refer to wcshdr.h for a description * of the user interface and operating notes. * * Implementation notes * -------------------- * wcsbth() may be invoked with an option that causes it to recognise the * image-header form of WCS keywords as defaults for each alternate coordinate * representation (up to 27). By design, with this option enabled wcsbth() can * also handle primary image and image extension headers, effectively treating * them as a single-column binary table though with WCS keywords of a different * form. * * NAXIS is always 2 for binary tables, it refers to the two-dimensional nature * of the table. Thus NAXIS does not count the number of image axes in either * image arrays or pixels lists and for the latter there is not even a formal * equivalent of WCSAXESa. Hence NAXIS is always ignored and a first pass * through the header is required to determine the number of images, the number * of alternate coordinate representations for each image (up to 27), and the * number of coordinate axes in each representation; this pass also counts the * number of iPVn_ma and iPSn_ma or TVk_ma and TSk_ma keywords in each * representation. * * On completion of the first pass, the association between column number and * axis number is defined for each representation of a pixel list. Memory is * allocated for an array of the required number of wcsprm structs and each of * these is initialized appropriately. These structs are filled in the second * pass. * * It is permissible for a scalar table column to contain degenerate (single- * point) image arrays and simultaneously form one axis of a pixel list. * * The parser does not check for duplicated keywords, for most keywords it * accepts the last encountered. * * wcsbth() does not currently handle the Green Bank convention. * *===========================================================================*/ /* Options. */ %option full %option never-interactive %option noyywrap %option outfile="wcsbth.c" %option prefix="wcsbth" /* Indices for parameterized keywords. */ I0 [0-9] I1 [1-9] I2 [1-9][0-9] I3 [1-9][0-9]{2} I4 [1-9][0-9]{3} /* Alternate coordinate system identifier. */ ALT [ A-Z] /* Keyvalue data types. */ INTEGER [+-]?[0-9]+ FLOAT [+-]?([0-9]+\.?[0-9]*|\.[0-9]+)([eE][+-]?[0-9]+)? STRING '([^']|'')*' /* Exclusive start states. */ %x CCCCCia iCCCna iCCCCn TCCCna TCCCCn %x CCi_ja ijCCna TCn_ka TCCn_ka %x CROTAi iCROTn TCROTn %x CCi_ma iCn_ma iCCn_ma TCn_ma TCCn_ma %x PROJPm %x CCCCCCCC CCCCCCCa %x CCCCna CCCCCna %x CCCCn CCCCCn %x VALUE INTEGER_VAL FLOAT_VAL STRING_VAL %x COMMENT DISCARD ERROR FLUSH %{ #include #include #include #include #include #include "wcs.h" #include "wcshdr.h" #include "wcsmath.h" /* Codes used for keyvalue data types. */ #define INTEGER 0 #define FLOAT 1 #define STRING 2 /* Bit masks used for keyword types: */ #define IMGAUX 0x1 /* Auxiliary image header, e.g. LONPOLEa or */ /* DATE-OBS. */ #define IMGAXIS 0x2 /* Image header with axis number, e.g. */ /* CTYPEia. */ #define IMGHEAD 0x3 /* Image header of either type. */ #define BIMGARR 0x4 /* Binary table image array with axis */ /* number, e.g. iCTYna. */ #define PIXLIST 0x8 /* Pixel list, e.g. TCTYna. */ #define BINTAB 0xC /* Shared binary table image array (without */ /* axis number) or pixel list, e.g. LONPna */ /* or OBSGXn. */ #define YY_DECL int wcsbth(char *header, int nkeyrec, int relax, int ctrl, \ int keysel, int *colsel, int *nreject, int *nwcs, \ struct wcsprm **wcs) #define YY_INPUT(inbuff, count, bufsize) \ { \ if (wcsbth_nkeyrec) { \ strncpy(inbuff, wcsbth_hdr, 80); \ inbuff[80] = '\n'; \ wcsbth_hdr += 80; \ wcsbth_nkeyrec--; \ count = 81; \ } else { \ count = YY_NULL; \ } \ } /* A convenience macro to get around incompatibilities between unput() and yyless(): put yytext followed by a blank back onto the input stream. */ #define WCSBTH_PUTBACK \ sprintf(stmp, "%s ", yytext); \ itmp = strlen(stmp); \ while (itmp) unput(stmp[--itmp]); /* These global variables are required by YY_INPUT. */ char *wcsbth_hdr; int wcsbth_nkeyrec; /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcsbth_abort_jmp_env; #define exit(status) longjmp(wcsbth_abort_jmp_env, status) /* Struct used internally for header bookkeeping. */ struct wcsbth_alts { int ncol, ialt, icol, imgherit; short int (*arridx)[27]; short int pixidx[27]; short int pad1; unsigned int *pixlist; unsigned char (*npv)[27]; unsigned char (*nps)[27]; unsigned char pixnpv[27]; unsigned char pixnps[27]; unsigned char pad2[2]; }; int wcsbth_pass1(int keytype, int i, int j, int n, int k, char a, char ptype, struct wcsbth_alts *alts); int wcsbth_init1(struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs); struct wcsprm *wcsbth_idx(struct wcsprm *wcs, struct wcsbth_alts *alts, int keytype, int n, char a); int wcsbth_colax(struct wcsprm *wcs, struct wcsbth_alts *alts, int k, char a); int wcsbth_epoch(void *wptr); int wcsbth_vsource(void *wptr); int wcsbth_final(struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs); %} %% /* Keyword indices, as used in the WCS papers, e.g. iVn_ma, TPn_ka. */ char a; int i, j, k, m, n; char *cptr, *errmsg, errtxt[80], exclude[1000], *extkey, *hptr, ptype, stmp[16]; int altlin, ialt, icol, incl, ipass, ipx, itmp, ix, jx, keytype, nsel, npass, status, valtype, voff; void *vptr, *wptr; struct wcsbth_alts alts; struct wcsprm *wcsp, wcstem; int (*special)(void *); int yylex_destroy(void); /* The data structures produced. */ *nwcs = 0; *wcs = 0x0; /* Parameters used to implement YY_INPUT. */ wcsbth_hdr = header; wcsbth_nkeyrec = nkeyrec; /* Our handle on the input stream. */ hptr = header; *nreject = 0; /* Keyword parameters. */ i = j = 0; n = k = 0; m = 0; a = ' '; /* Header bookkeeping. */ alts.ncol = 0; alts.arridx = 0x0; alts.pixlist = 0x0; alts.npv = 0x0; alts.nps = 0x0; for (ialt = 0; ialt < 27; ialt++) { alts.pixidx[ialt] = 0; alts.pixnpv[ialt] = 0; alts.pixnps[ialt] = 0; } /* For decoding the keyvalue. */ keytype = 0; valtype = -1; vptr = 0x0; /* For keywords that require special handling. */ altlin = 0; ptype = ' '; special = 0x0; /* Selection by column number. */ nsel = colsel ? colsel[0] : 0; incl = (nsel > 0); for (icol = 0; icol < 1000; icol++) { exclude[icol] = incl; } for (icol = 1; icol <= abs(nsel); icol++) { itmp = colsel[icol]; if (0 < itmp && itmp < 1000) { exclude[itmp] = !incl; } } exclude[0] = 0; /* Selection by keyword type. */ itmp = keysel; keysel = 0; if (itmp) { if (itmp & WCSHDR_IMGHEAD) keysel |= IMGHEAD; if (itmp & WCSHDR_BIMGARR) keysel |= BIMGARR; if (itmp & WCSHDR_PIXLIST) keysel |= PIXLIST; } if (keysel == 0) { keysel = IMGHEAD | BINTAB; } /* Control variables. */ ipass = 1; npass = 2; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcsbth_abort_jmp_env)) { return 4; } BEGIN(INITIAL); ^TFIELDS" = "" "*{INTEGER} { if (ipass == 1) { if (alts.ncol == 0) { sscanf(yytext, "TFIELDS = %d", &(alts.ncol)); BEGIN(FLUSH); } else { errmsg = "Duplicate or out-of-sequence TFIELDS keyword"; BEGIN(ERROR); } } else { BEGIN(FLUSH); } } ^WCSAXES{ALT}=" "" "*{INTEGER} { keytype = IMGAXIS; if (!(keytype & keysel)) { /* Ignore this key type. */ BEGIN(DISCARD); } else { if (relax & WCSHDR_ALLIMG) { if (ipass == 1) { sscanf(yytext, "WCSAXES%c= %d", &a, &i); wcsbth_pass1(IMGAXIS, i, 0, 0, 0, a, ' ', &alts); } BEGIN(FLUSH); } else if (relax & WCSHDR_reject) { errmsg = "Image-header keyword WCSAXESa in binary table"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } } ^WCAX{I1}{ALT}" = "" "*{INTEGER} | ^WCAX{I2}{ALT}" = "" "*{INTEGER} | ^WCAX{I3}{ALT}"= "" "*{INTEGER} { keytype = BIMGARR; /* Note that a blank in the sscanf() format string matches zero or more of them in the input. */ sscanf(yytext, "WCAX%d%c = %d", &n, &a, &i); if (!(keytype & keysel) || exclude[n]) { /* Ignore this key type or column. */ BEGIN(DISCARD); } else { if (ipass == 1) { wcsbth_pass1(BIMGARR, i, 0, n, 0, a, ' ', &alts); } BEGIN(FLUSH); } } ^WCST{I1}{ALT}" = "" "*{STRING} | ^WCST{I2}{ALT}" = "" "*{STRING} | ^WCST{I3}{ALT}"= "" "*{STRING} { /* Cross-reference supplier. */ keytype = BIMGARR; errmsg = "Cross-references are not currently implemented"; BEGIN(ERROR); } ^WCSX{I1}{ALT}" = "" "*{STRING} | ^WCSX{I2}{ALT}" = "" "*{STRING} | ^WCSX{I3}{ALT}"= "" "*{STRING} { /* Cross-reference consumer. */ keytype = BIMGARR; errmsg = "Cross-references are not currently implemented"; BEGIN(ERROR); } ^CRPIX { valtype = FLOAT; vptr = &(wcstem.crpix); extkey = "CRPIXja"; BEGIN(CCCCCia); } ^{I1}CRP | ^{I1}CRPX { valtype = FLOAT; vptr = &(wcstem.crpix); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { extkey = "jCRPXn"; BEGIN(iCCCCn); } } ^TCRP | ^TCRPX { valtype = FLOAT; vptr = &(wcstem.crpix); if (yyleng == 4) { BEGIN(TCCCna); } else { extkey = "TCRPXn"; BEGIN(TCCCCn); } } ^PC { valtype = FLOAT; vptr = &(wcstem.pc); altlin = 1; extkey = "PCi_ja"; BEGIN(CCi_ja); } ^{I2}PC { valtype = FLOAT; vptr = &(wcstem.pc); altlin = 1; sscanf(yytext, "%1d%1d", &i, &j); BEGIN(ijCCna); } ^TP | ^TPC { valtype = FLOAT; vptr = &(wcstem.pc); altlin = 1; if (yyleng == 2) { BEGIN(TCn_ka); } else { extkey = "TPCn_ka"; BEGIN(TCCn_ka); } } ^CD { valtype = FLOAT; vptr = &(wcstem.cd); altlin = 2; extkey = "CDi_ja"; BEGIN(CCi_ja); } ^{I2}CD { valtype = FLOAT; vptr = &(wcstem.cd); altlin = 2; sscanf(yytext, "%1d%1d", &i, &j); BEGIN(ijCCna); } ^TC | ^TCD { valtype = FLOAT; vptr = &(wcstem.cd); altlin = 2; if (yyleng == 2) { BEGIN(TCn_ka); } else { extkey = "TCDn_ka"; BEGIN(TCCn_ka); } } ^CDELT { valtype = FLOAT; vptr = &(wcstem.cdelt); extkey = "CDELTia"; BEGIN(CCCCCia); } ^{I1}CDE | ^{I1}CDLT { valtype = FLOAT; vptr = &(wcstem.cdelt); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { extkey = "iCDLTn"; BEGIN(iCCCCn); } } ^TCDE | ^TCDLT { valtype = FLOAT; vptr = &(wcstem.cdelt); if (yyleng == 4) { BEGIN(TCCCna); } else { extkey = "TCDLTn"; BEGIN(TCCCCn); } } ^CROTA { valtype = FLOAT; vptr = &(wcstem.crota); altlin = 4; extkey = "CROTAi"; BEGIN(CROTAi); } ^{I1}CROT { valtype = FLOAT; vptr = &(wcstem.crota); altlin = 4; sscanf(yytext, "%d", &i); extkey = "iCROTn"; BEGIN(iCROTn); } ^TCROT { valtype = FLOAT; vptr = &(wcstem.crota); altlin = 4; extkey = "TCROTn"; BEGIN(TCROTn); } ^CUNIT { valtype = STRING; vptr = &(wcstem.cunit); extkey = "CUNITia"; BEGIN(CCCCCia); } ^{I1}CUN | ^{I1}CUNI { valtype = STRING; vptr = &(wcstem.cunit); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { extkey = "iCUNIn"; BEGIN(iCCCCn); } } ^TCUN | ^TCUNI { valtype = STRING; vptr = &(wcstem.cunit); if (yyleng == 4) { BEGIN(TCCCna); } else { extkey = "TCUNIn"; BEGIN(TCCCCn); } } ^CTYPE { valtype = STRING; vptr = &(wcstem.ctype); extkey = "CTYPEia"; BEGIN(CCCCCia); } ^{I1}CTY | ^{I1}CTYP { valtype = STRING; vptr = &(wcstem.ctype); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { extkey = "iCTYPn"; BEGIN(iCCCCn); } } ^TCTY | ^TCTYP { valtype = STRING; vptr = &(wcstem.ctype); if (yyleng == 4) { BEGIN(TCCCna); } else { extkey = "TCTYPn"; BEGIN(TCCCCn); } } ^CRVAL { valtype = FLOAT; vptr = &(wcstem.crval); extkey = "CRVALia"; BEGIN(CCCCCia); } ^{I1}CRV | ^{I1}CRVL { valtype = FLOAT; vptr = &(wcstem.crval); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { extkey = "iCRVLn"; BEGIN(iCCCCn); } } ^TCRV | ^TCRVL { valtype = FLOAT; vptr = &(wcstem.crval); if (yyleng == 4) { BEGIN(TCCCna); } else { extkey = "TCRVLn"; BEGIN(TCCCCn); } } ^LONPOLE | ^LONP { valtype = FLOAT; vptr = &(wcstem.lonpole); if (yyleng == 7) { extkey = "LONPOLEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^LATPOLE | ^LATP { valtype = FLOAT; vptr = &(wcstem.latpole); if (yyleng == 7) { extkey = "LATPOLEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^RESTFRQ | ^RESTFREQ | ^RFRQ { valtype = FLOAT; vptr = &(wcstem.restfrq); if (yyleng == 8) { unput(' '); extkey = "RESTFREQ"; BEGIN(CCCCCCCa); } else if (yyleng == 7) { extkey = "RESTFRQa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^RESTWAV | ^RWAV { valtype = FLOAT; vptr = &(wcstem.restwav); if (yyleng == 7) { extkey = "RESTWAVa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^PV { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; extkey = "PVi_ma"; BEGIN(CCi_ma); } ^{I1}V | ^{I1}PV { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; sscanf(yytext, "%d", &i); if (yyleng == 2) { BEGIN(iCn_ma); } else { extkey = "iPVn_ma"; BEGIN(iCCn_ma); } } ^TV | ^TPV { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; if (yyleng == 2) { BEGIN(TCn_ma); } else { extkey = "TPVn_ma"; BEGIN(TCCn_ma); } } ^PROJP { valtype = FLOAT; vptr = &(wcstem.pv); ptype = 'v'; BEGIN(PROJPm); } ^PS { valtype = STRING; vptr = &(wcstem.ps); ptype = 's'; extkey = "PSi_ma"; BEGIN(CCi_ma); } ^{I1}S | ^{I1}PS { valtype = STRING; vptr = &(wcstem.ps); ptype = 's'; sscanf(yytext, "%d", &i); if (yyleng == 2) { BEGIN(iCn_ma); } else { extkey = "iPSn_ma"; BEGIN(iCCn_ma); } } ^TS | ^TPS { valtype = STRING; vptr = &(wcstem.ps); ptype = 's'; if (yyleng == 2) { BEGIN(TCn_ma); } else { extkey = "TPSn_ma"; BEGIN(TCCn_ma); } } ^CNAME { valtype = STRING; vptr = &(wcstem.cname); extkey = "CNAMEia"; BEGIN(CCCCCia); } ^{I1}CNA | ^{I1}CNAM { valtype = STRING; vptr = &(wcstem.cname); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "iCNAMn"; BEGIN(iCCCCn); } } ^TCNA | ^TCNAM { valtype = STRING; vptr = &(wcstem.cname); if (yyleng == 4) { BEGIN(TCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "TCNAMn"; BEGIN(TCCCCn); } } ^CRDER { valtype = FLOAT; vptr = &(wcstem.crder); extkey = "CRDERia"; BEGIN(CCCCCia); } ^{I1}CRD | ^{I1}CRDE { valtype = FLOAT; vptr = &(wcstem.crder); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "iCRDEn"; BEGIN(iCCCCn); } } ^TCRD | ^TCRDE { valtype = FLOAT; vptr = &(wcstem.crder); if (yyleng == 4) { BEGIN(TCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "TCRDEn"; BEGIN(TCCCCn); } } ^CSYER { valtype = FLOAT; vptr = &(wcstem.csyer); extkey = "CSYERia"; BEGIN(CCCCCia); } ^{I1}CSY | ^{I1}CSYE { valtype = FLOAT; vptr = &(wcstem.csyer); sscanf(yytext, "%d", &i); if (yyleng == 4) { BEGIN(iCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "iCSYEn"; BEGIN(iCCCCn); } } ^TCSY | ^TCSYE { valtype = FLOAT; vptr = &(wcstem.csyer); if (yyleng == 4) { BEGIN(TCCCna); } else { if (!(relax & WCSHDR_CNAMn)) vptr = 0x0; extkey = "TCSYEn"; BEGIN(TCCCCn); } } ^DATE-AVG | ^DAVG { valtype = STRING; vptr = wcstem.dateavg; if (yyleng == 8) { extkey = "DATE-AVG"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCn); } } ^DATE-OBS { valtype = STRING; vptr = wcstem.dateobs; extkey = "DATE-OBS"; BEGIN(CCCCCCCC); } ^DOBS{I1}" " | ^DOBS{I2}" " | ^DOBS{I3}" " { if (relax & WCSHDR_DOBSn) { valtype = STRING; vptr = wcstem.dateobs; yyless(4); BEGIN(CCCCn); } else { keytype = BINTAB; if (relax & WCSHDR_reject) { errmsg = "DOBSna keyword is non-standard"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } ^EPOCH{ALT}" " { sscanf(yytext, "EPOCH%c", &a); if (a == ' ' || (relax & WCSHDR_EPOCHa)) { valtype = FLOAT; vptr = &(wcstem.equinox); special = wcsbth_epoch; unput(a); extkey = "EPOCH"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "EPOCH keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } ^EQUINOX | ^EQUI { valtype = FLOAT; vptr = &(wcstem.equinox); if (yyleng == 7) { extkey = "EQUINOXa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^MJD-AVG" " | ^MJDA { valtype = FLOAT; vptr = &(wcstem.mjdavg); if (yyleng == 8) { extkey = "MJD-AVG"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCn); } } ^MJD-OBS" " | ^MJDOB { valtype = FLOAT; vptr = &(wcstem.mjdobs); if (yyleng == 8) { extkey = "MJD-OBS"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } ^OBSGEO-X | ^OBSGX { valtype = FLOAT; vptr = wcstem.obsgeo; if (yyleng == 8) { extkey = "OBSGEO-X"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } ^OBSGEO-Y | ^OBSGY { valtype = FLOAT; vptr = wcstem.obsgeo + 1; if (yyleng == 8) { extkey = "OBSGEO-Y"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } ^OBSGEO-Z | ^OBSGZ { valtype = FLOAT; vptr = wcstem.obsgeo + 2; if (yyleng == 8) { extkey = "OBSGEO-Z"; BEGIN(CCCCCCCC); } else { BEGIN(CCCCCn); } } ^RADESYS | ^RADE { valtype = STRING; vptr = wcstem.radesys; if (yyleng == 7) { extkey = "RADESYSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^RADECSYS { if (relax & WCSHDR_RADECSYS) { valtype = STRING; vptr = wcstem.radesys; unput(' '); extkey = "RADECSYS"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "RADECSYS keyword is non-standard"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } ^SPECSYS | ^SPEC { valtype = STRING; vptr = wcstem.specsys; if (yyleng == 7) { extkey = "SPECSYSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^SSYSOBS | ^SOBS { valtype = STRING; vptr = wcstem.ssysobs; if (yyleng == 7) { extkey = "SSYSOBSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^SSYSSRC | ^SSRC { valtype = STRING; vptr = wcstem.ssyssrc; if (yyleng == 7) { extkey = "SSYSSRCa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^VELOSYS | ^VSYS { valtype = FLOAT; vptr = &(wcstem.velosys); if (yyleng == 7) { extkey = "VELOSYSa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^VELANGL | ^VANG { valtype = FLOAT; vptr = &(wcstem.velangl); if (yyleng == 7) { extkey = "VELANGLa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^VELREF{ALT}" " { sscanf(yytext, "VELREF%c", &a); if (a == ' ' || (relax & WCSHDR_VELREFa)) { valtype = INTEGER; vptr = &(wcstem.velref); unput(a); extkey = "VELREF"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "VELREF keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } ^VSOURCE{ALT} { if (relax & WCSHDR_VSOURCE) { valtype = FLOAT; vptr = &(wcstem.zsource); special = wcsbth_vsource; yyless(7); extkey = "VSOURCEa"; BEGIN(CCCCCCCa); } else { keytype = IMGAUX; if (relax & WCSHDR_reject) { errmsg = "VSOURCEa keyword is deprecated"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } } ^VSOU{I1}{ALT}" " | ^VSOU{I2}{ALT}" " | ^VSOU{I3}{ALT} { if (relax & WCSHDR_VSOURCE) { valtype = FLOAT; vptr = &(wcstem.zsource); special = wcsbth_vsource; yyless(4); BEGIN(CCCCna); } else { keytype = BINTAB; if (relax & WCSHDR_reject) { errmsg = "VSOUna keyword is deprecated"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } } ^WCSNAME | ^WCSN | ^TWCS { valtype = STRING; vptr = wcstem.wcsname; if (yyleng == 7) { extkey = "WCSNAMEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^ZSOURCE | ^ZSOU { valtype = FLOAT; vptr = &(wcstem.zsource); if (yyleng == 7) { extkey = "ZSOURCEa"; BEGIN(CCCCCCCa); } else { BEGIN(CCCCna); } } ^END" "{77} { yyless(0); if (wcsbth_nkeyrec) { wcsbth_nkeyrec = 0; errmsg = "Keyrecords following the END keyrecord were ignored"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^. { yyless(0); BEGIN(DISCARD); } {I1}{ALT}" " | {I2}{ALT} { /* Image-header keyword. */ keytype = IMGAXIS; if (relax & WCSHDR_ALLIMG) { sscanf(yytext, "%d%c", &i, &a); BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } {I3} { /* Invalid axis number in image-header keyword. */ keytype = IMGAXIS; if (relax & WCSHDR_ALLIMG) { /* Will also be flagged by as invalid. */ sscanf(yytext, "%3d", &i); BEGIN(VALUE); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } {I1}" " | {I2}" " | {I3} | {I1}" " | {I2}" " | {I3} { if (vptr) { WCSBTH_PUTBACK; BEGIN((YY_START == iCCCCn) ? iCCCna : TCCCna); } else { keytype = (YY_START == iCCCCn) ? BIMGARR : PIXLIST; if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword is non-standard", extkey); BEGIN(ERROR); } else { BEGIN(DISCARD); } } } {I1}[A-Z]" " | {I2}[A-Z] | {I1}[A-Z]" " | {I2}[A-Z] { if (vptr && (relax & WCSHDR_LONGKEY)) { WCSBTH_PUTBACK; BEGIN((YY_START == iCCCCn) ? iCCCna : TCCCna); } else { keytype = (YY_START == iCCCna) ? BIMGARR : PIXLIST; if (relax & WCSHDR_reject) { errmsg = errtxt; if (!vptr) { sprintf(errmsg, "%s keyword is non-standard", extkey); } else { sprintf(errmsg, "%s keyword may not have an alternate version code", extkey); } BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } } . | . { BEGIN(DISCARD); } {I1}{ALT}" " | {I2}{ALT}" " | {I3}{ALT} | {I1}{ALT}" " | {I2}{ALT}" " | {I3}{ALT} { sscanf(yytext, "%d%c", &n, &a); if (YY_START == TCCCna) i = wcsbth_colax(*wcs, &alts, n, a); keytype = (YY_START == iCCCna) ? BIMGARR : PIXLIST; BEGIN(VALUE); } . | . { BEGIN(DISCARD); } {I1}_{I1}{ALT}" " | {I1}_{I2}{ALT}" " | {I2}_{I1}{ALT}" " | {I2}_{I2}{ALT} { /* Image-header keyword. */ if (relax & WCSHDR_ALLIMG) { sscanf(yytext, "%d_%d%c", &i, &j, &a); keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } {I1}_{I3}{ALT} | {I3}_{I1}{ALT} | {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I1} { /* Invalid axis number in image-header keyword. */ if (relax & WCSHDR_ALLIMG) { /* Will be flagged by as invalid. */ sscanf(yytext, "%d_%d", &i, &j); keytype = IMGAXIS; BEGIN(VALUE); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } {I0}{6} { /* This covers the defunct forms CD00i00j and PC00i00j. */ if (((relax & WCSHDR_PC00i00j) && (altlin == 1)) || ((relax & WCSHDR_CD00i00j) && (altlin == 2))) { sscanf(yytext, "%3d%3d", &i, &j); a = ' '; keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Defunct form of %si_ja keyword", (altlin==1) ? "PC" : "CD"); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . { BEGIN(DISCARD); } {I1}{ALT}" " | {I2}{ALT}" " | {I3}{ALT} { sscanf(yytext, "%d%c", &n, &a); keytype = BIMGARR; BEGIN(VALUE); } {I1}_{I1}{ALT}" " | {I1}_{I2}{ALT} | {I2}_{I1}{ALT} | {I1}_{I3} | {I2}_{I2} | {I3}_{I1} { if (relax & WCSHDR_LONGKEY) { WCSBTH_PUTBACK; BEGIN(TCn_ka); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword is non-standard", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . { BEGIN(DISCARD); } {I1}_{I1}{ALT}" " | {I1}_{I2}{ALT}" " | {I2}_{I1}{ALT}" " | {I1}_{I3}{ALT} | {I2}_{I2}{ALT} | {I3}_{I1}{ALT} { sscanf(yytext, "%d_%d%c", &n, &k, &a); i = wcsbth_colax(*wcs, &alts, n, a); j = wcsbth_colax(*wcs, &alts, k, a); keytype = PIXLIST; BEGIN(VALUE); } {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I1} { sscanf(yytext, "%d_%d", &n, &k); a = ' '; i = wcsbth_colax(*wcs, &alts, n, a); j = wcsbth_colax(*wcs, &alts, k, a); keytype = PIXLIST; BEGIN(VALUE); } . { BEGIN(DISCARD); } {I1}" " | {I2}" " { yyless(0); BEGIN(CCCCCia); } {I1}[A-Z]" " | {I2}[A-Z] { if (relax & WCSHDR_CROTAia) { yyless(0); BEGIN(CCCCCia); } else if (relax & WCSHDR_reject) { errmsg = "CROTAn keyword may not have an alternate version code"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . { BEGIN(DISCARD); } {I1}" " | {I2}" " | {I3} | {I1}" " | {I2}" " | {I3} { WCSBTH_PUTBACK; BEGIN((YY_START == iCROTn) ? iCCCna : TCCCna); } {I1}[A-Z]" " | {I2}[A-Z] | {I1}[A-Z]" " | {I2}[A-Z] { if (relax & WCSHDR_CROTAia) { WCSBTH_PUTBACK; BEGIN((YY_START == iCROTn) ? iCCCna : TCCCna); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword may not have an alternate version code", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . | . { BEGIN(DISCARD); } {ALT} | . { /* Image-header keyword. */ if (relax & (WCSHDR_AUXIMG | WCSHDR_ALLIMG)) { if (YY_START == CCCCCCCa) { sscanf(yytext, "%c", &a); } else { a = 0; unput(yytext[0]); } keytype = IMGAUX; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . { BEGIN(DISCARD); } {I1}{ALT}" " | {I2}{ALT}" " | {I3}{ALT} | {I1}{ALT}" " | {I2}{ALT} { sscanf(yytext, "%d%c", &n, &a); keytype = BINTAB; BEGIN(VALUE); } {I3} { sscanf(yytext, "%d", &n); a = ' '; keytype = BINTAB; BEGIN(VALUE); } . | . { BEGIN(DISCARD); } {I1}" " | {I2}" " | {I3}" " | {I4} | {I1}" " | {I2}" " | {I3} { sscanf(yytext, "%d", &n); a = 0; keytype = BINTAB; BEGIN(VALUE); } . | . { BEGIN(DISCARD); } {I1}_{I0}{ALT}" " | {I1}_{I2}{ALT}" " | {I2}_{I0}{ALT}" " | {I2}_{I2}{ALT} { /* Image-header keyword. */ if (relax & WCSHDR_ALLIMG) { sscanf(yytext, "%d_%d%c", &i, &m, &a); keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Image-header keyword %s in binary table", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } {I1}_{I3}{ALT} | {I3}_{I0}{ALT} | {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I0} { /* Invalid parameter in image-header keyword. */ if (relax & WCSHDR_ALLIMG) { /* Will be flagged by as invalid. */ sscanf(yytext, "%d_%d", &i, &m); keytype = IMGAXIS; BEGIN(VALUE); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . { BEGIN(DISCARD); } {I1}_{I0}{ALT}" " | {I1}_{I2}{ALT} | {I1}_{I3} | {I2}_{I0}{ALT} | {I2}_{I2} | {I3}_{I0} | {I1}_{I0}{ALT}" " | {I1}_{I2}{ALT} | {I1}_{I3} | {I2}_{I0}{ALT} | {I2}_{I2} | {I3}_{I0} { if (relax & WCSHDR_LONGKEY) { WCSBTH_PUTBACK; BEGIN((YY_START == iCCn_ma) ? iCn_ma : TCn_ma); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "%s keyword is non-standard", extkey); BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . | . { BEGIN(DISCARD); } {I1}_{I0}{ALT}" " | {I1}_{I2}{ALT}" " | {I1}_{I3}{ALT} | {I2}_{I0}{ALT}" " | {I2}_{I2}{ALT} | {I3}_{I0}{ALT} | {I1}_{I0}{ALT}" " | {I1}_{I2}{ALT}" " | {I1}_{I3}{ALT} | {I2}_{I0}{ALT}" " | {I2}_{I2}{ALT} | {I3}_{I0}{ALT} { sscanf(yytext, "%d_%d%c", &n, &m, &a); if (YY_START == TCn_ma) i = wcsbth_colax(*wcs, &alts, n, a); keytype = (YY_START == iCn_ma) ? BIMGARR : PIXLIST; BEGIN(VALUE); } {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I0} | {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I0} { /* Invalid combinations will be flagged by . */ sscanf(yytext, "%d_%d", &n, &m); a = ' '; if (YY_START == TCn_ma) i = wcsbth_colax(*wcs, &alts, n, a); keytype = (YY_START == iCn_ma) ? BIMGARR : PIXLIST; BEGIN(VALUE); } . | . { BEGIN(DISCARD); } {I0}" " { if (relax & WCSHDR_PROJPn) { sscanf(yytext, "%d", &m); i = 0; a = ' '; keytype = IMGAXIS; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = "PROJPn keyword is defunct"; BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } . { BEGIN(DISCARD); } =" "+ { /* Do checks on i, j, m, n, k. */ if (!(keytype & keysel)) { /* Selection by keyword type. */ BEGIN(DISCARD); } else if (exclude[n] || exclude[k]) { /* One or other column is not selected. */ if (k && (exclude[n] != exclude[k])) { /* For keywords such as TCn_ka, both columns must be excluded. User error, so return immediately. */ yylex_destroy(); return 3; } else { BEGIN(DISCARD); } } else if (i > 99 || j > 99 || m > 99 || n > 999 || k > 999) { if (relax & WCSHDR_reject) { errmsg = errtxt; if (i > 99 || j > 99) { sprintf(errmsg, "Axis number exceeds 99"); } else if (m > 99) { sprintf(errmsg, "Parameter number exceeds 99"); } else if (n > 999 || k > 999) { sprintf(errmsg, "Column number exceeds 999"); } BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } else if (ipass == 2 && npass == 3 && (keytype & BINTAB)) { /* Skip keyvalues that won't be inherited. */ BEGIN(FLUSH); } else if (ipass == 3 && (keytype & IMGHEAD)) { /* IMGHEAD keytypes are always dealt with on the second pass. */ BEGIN(FLUSH); } else if (vptr) { alts.icol = 0; alts.ialt = 0; voff = (char *)vptr - (char *)(&wcstem); if (valtype == INTEGER) { BEGIN(INTEGER_VAL); } else if (valtype == FLOAT) { BEGIN(FLOAT_VAL); } else if (valtype == STRING) { BEGIN(STRING_VAL); } else { errmsg = errtxt; sprintf(errmsg, "Internal parser ERROR, bad data type: %d", valtype); BEGIN(ERROR); } } else { errmsg = "Internal parser ERROR, null pointer"; BEGIN(ERROR); } } . { errmsg = "Invalid KEYWORD = VALUE syntax"; BEGIN(ERROR); } {INTEGER} { if (ipass == 1) { /* Do first-pass bookkeeping. */ wcsbth_pass1(keytype, i, j, n, k, a, ptype, &alts); BEGIN(FLUSH); } else { /* Update each coordinate representation. */ while ((wcsp = wcsbth_idx(*wcs, &alts, keytype, n, a))) { wptr = (void *)((char *)wcsp + voff); /* Read the keyvalue. */ if (special) { special(wptr); } else { sscanf(yytext, "%d", (int *)wptr); } } BEGIN(COMMENT); } } . { errmsg = "An integer value was expected"; BEGIN(ERROR); } {FLOAT} { if (ipass == 1) { /* Do first-pass bookkeeping. */ wcsbth_pass1(keytype, i, j, n, k, a, ptype, &alts); BEGIN(FLUSH); } else { /* Update each coordinate representation. */ while ((wcsp = wcsbth_idx(*wcs, &alts, keytype, n, a))) { wptr = (void *)((char *)wcsp + voff); /* Apply keyword parameterization. */ if (ptype == 'v') { ipx = wcsp->npv++; wcsp->pv[ipx].i = i; wcsp->pv[ipx].m = m; wptr = &(wcsp->pv[ipx].value); } else if (j) { /* Is the de-reference necessary? */ wptr = *((double **)wptr) + (i - 1)*(wcsp->naxis) + (j - 1); } else if (i) { wptr = *((double **)wptr) + (i - 1); } /* Read the keyvalue. */ if (special) { special(wptr); } else { sscanf(yytext, "%lf", (double *)wptr); } /* Flag the presence of PC, or CD and/or CROTA. */ if (altlin) { wcsp->altlin |= altlin; altlin = 0; } } BEGIN(COMMENT); } } . { errmsg = "A floating-point value was expected"; BEGIN(ERROR); } {STRING} { if (ipass == 1) { /* Do first-pass bookkeeping. */ wcsbth_pass1(keytype, i, j, n, k, a, ptype, &alts); BEGIN(FLUSH); } else { /* Update each coordinate representation. */ while ((wcsp = wcsbth_idx(*wcs, &alts, keytype, n, a))) { wptr = (void *)((char *)wcsp + voff); /* Apply keyword parameterization. */ if (ptype == 's') { ipx = wcsp->nps++; wcsp->ps[ipx].i = i; wcsp->ps[ipx].m = m; wptr = wcsp->ps[ipx].value; } else if (j) { wptr = *((char (**)[72])wptr) + (i - 1)*(wcsp->naxis) + (j - 1); } else if (i) { wptr = *((char (**)[72])wptr) + (i - 1); } /* Read the keyvalue. */ cptr = (char *)wptr; strcpy(cptr, yytext+1); /* Squeeze out repeated quotes. */ ix = 0; for (jx = 0; jx < 72; jx++) { if (ix < jx) { cptr[ix] = cptr[jx]; } if (cptr[jx] == '\0') { if (ix) cptr[ix-1] = '\0'; break; } else if (cptr[jx] == '\'' && cptr[jx+1] == '\'') { jx++; } ix++; } } BEGIN(COMMENT); } } . { errmsg = "A string value was expected"; BEGIN(ERROR); } " "*\/.* | " "* { BEGIN(FLUSH); } . { errmsg = "Malformed keycomment"; BEGIN(ERROR); } .* { if (ipass == npass) { if (ctrl < 0) { /* Preserve discards. */ if (hptr < wcsbth_hdr-80) { strncpy(hptr, wcsbth_hdr-80, 80); } hptr += 80; } else if (ctrl > 2) { fprintf(stderr, "%.80s\n Discarded.\n", wcsbth_hdr-80); } } BEGIN(FLUSH); } .* { (*nreject)++; if (ipass == npass) { if (ctrl == -1) { if (hptr < wcsbth_hdr-80) { /* Preserve rejects. */ strncpy(hptr, wcsbth_hdr-80, 80); } hptr += 80; } if (abs(ctrl) > 1) { fprintf(stderr, "%.80s\n%4d: %s.\n", wcsbth_hdr-80, *nreject, errmsg); } } BEGIN(FLUSH); } .*\n { /* Throw away the rest of the line and reset for the next one. */ i = j = 0; n = k = 0; m = 0; a = ' '; keytype = 0; valtype = -1; vptr = 0x0; altlin = 0; ptype = ' '; special = 0x0; BEGIN(INITIAL); } <> { /* End-of-input. */ if (ipass == 1) { if ((status = wcsbth_init1(&alts, nwcs, wcs)) || *nwcs == 0) { yylex_destroy(); return status; } if (alts.imgherit) npass = 3; if (abs(ctrl) > 2) { if (*nwcs == 1) { fprintf(stderr, "Found one coordinate representation.\n"); } else { fprintf(stderr, "Found %d coordinate representations.\n", *nwcs); } } } if (ipass++ < npass) { wcsbth_hdr = header; wcsbth_nkeyrec = nkeyrec; *nreject = 0; i = j = 0; k = n = 0; m = 0; a = ' '; keytype = 0; valtype = -1; vptr = 0x0; altlin = 0; ptype = ' '; special = 0x0; yyrestart(yyin); } else { yylex_destroy(); if (ctrl < 0) { *hptr = '\0'; } else if (ctrl == 1) { fprintf(stderr, "%d WCS keyrecords were rejected.\n", *nreject); } return wcsbth_final(&alts, nwcs, wcs); } } %% /*---------------------------------------------------------------------------- * Perform first-pass tasks: * * 1) Count the number of coordinate axes in each of the 27 possible alternate * image-header coordinate representations. Also count the number of PVi_ma * and PSi_ma keywords in each representation. * * 2) Determine the number of binary table columns that have an image array * with a coordinate representation (up to 999), and count the number of * coordinate axes in each of the 27 possible alternates. Also count the * number of iVn_ma and iSn_ma keywords in each representation. * * 3) Determine the number of alternate pixel list coordinate representations * (up to 27) and the table columns associated with each. Also count the * number of TVn_ma and TSn_ma keywords in each representation. * * In the first pass alts->arridx[icol][27] is used to determine the number of * axes in each of 27 possible image-header coordinate descriptions (icol == 0) * and each of the 27 possible coordinate representations for an image array in * each column. * * The elements of alts->pixlist[icol] are used as bit arrays to flag which of * the 27 possible pixel list coordinate representations are associated with * each table column. *---------------------------------------------------------------------------*/ int wcsbth_pass1( int keytype, int i, int j, int n, int k, char a, char ptype, struct wcsbth_alts *alts) { int ialt, icol, mask, ncol; if (a == 0) { /* Keywords such as DATE-OBS go along for the ride. */ return 0; } ncol = alts->ncol; /* Do we need to allocate memory for alts? */ if (alts->arridx == 0x0) { if (ncol == 0) { /* Can only happen if TFIELDS is missing or out-of-sequence. If n and k are both zero then we may be processing an image header so leave ncol alone - the array will be realloc'd later if required. */ if (n || k) { /* The header is mangled, assume the worst. */ ncol = 999; } } if (!(alts->arridx = calloc((1 + ncol)*27, sizeof(short int))) || !(alts->npv = calloc((1 + ncol)*27, sizeof(unsigned char))) || !(alts->nps = calloc((1 + ncol)*27, sizeof(unsigned char))) || !(alts->pixlist = calloc((1 + ncol), sizeof(unsigned int)))) { if (alts->arridx) free(alts->arridx); if (alts->npv) free(alts->npv); if (alts->nps) free(alts->nps); if (alts->pixlist) free(alts->pixlist); return 2; } alts->ncol = ncol; } else if (n > ncol || k > ncol) { /* Can only happen if TFIELDS or the WCS keyword is wrong; carry on. */ ncol = 999; if (!(alts->arridx = realloc(alts->arridx, 27*(1 + ncol)*sizeof(short int))) || !(alts->npv = realloc(alts->npv, 27*(1 + ncol)*sizeof(unsigned char))) || !(alts->nps = realloc(alts->nps, 27*(1 + ncol)*sizeof(unsigned char))) || !(alts->pixlist = realloc(alts->pixlist, (1 + ncol)*sizeof(unsigned int)))) { if (alts->arridx) free(alts->arridx); if (alts->npv) free(alts->npv); if (alts->nps) free(alts->nps); if (alts->pixlist) free(alts->pixlist); return 2; } /* Since realloc() doesn't initialize the extra memory. */ for (icol = (1 + alts->ncol); icol < (1 + ncol); icol++) { for (ialt = 0; ialt < 27; ialt++) { alts->arridx[icol][ialt] = 0; alts->npv[icol][ialt] = 0; alts->nps[icol][ialt] = 0; alts->pixlist[icol] = 0; } } alts->ncol = ncol; } ialt = 0; if (a != ' ') { ialt = a - 'A' + 1; } /* A BINTAB keytype such as LONPna, in conjunction with an IMGAXIS keytype causes a table column to be recognized as an image array. */ if (keytype & IMGHEAD || keytype & BIMGARR) { /* n == 0 is expected for IMGHEAD keywords. */ if (i == 0 && j == 0) { if (alts->arridx[n][ialt] == 0) { /* Flag that an auxiliary keyword was seen. */ alts->arridx[n][ialt] = -1; } } else { /* Record the maximum axis number found. */ if (alts->arridx[n][ialt] < i) { alts->arridx[n][ialt] = i; } if (alts->arridx[n][ialt] < j) { alts->arridx[n][ialt] = j; } } if (ptype == 'v') { alts->npv[n][ialt]++; } else if (ptype == 's') { alts->nps[n][ialt]++; } } /* BINTAB keytypes, which apply both to pixel lists as well as binary table image arrays, never contribute to recognizing a table column as a pixel list axis. A PIXLIST keytype is required for that. */ if (keytype == PIXLIST) { mask = 1 << ialt; /* n > 0 for PIXLIST keytypes. */ alts->pixlist[n] |= mask; if (k) alts->pixlist[k] |= mask; /* Used as a flag over all columns. */ alts->pixlist[0] |= mask; if (ptype == 'v') { alts->pixnpv[ialt]++; } else if (ptype == 's') { alts->pixnps[ialt]++; } } return 0; } /*---------------------------------------------------------------------------- * Perform initializations at the end of the first pass: * * 1) Determine the required number of wcsprm structs, allocate memory for * an array of them and initialize each one. *---------------------------------------------------------------------------*/ int wcsbth_init1( struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs) { int ialt, icol, inherit[27], ix, mask, ncol, npsmax, npvmax, status = 0; struct wcsprm *wcsp; if (alts->arridx == 0x0) { *nwcs = 0; return 0; } /* Determine the number of axes in each pixel list representation. */ ncol = alts->ncol; for (ialt = 0, mask = 1; ialt < 27; ialt++, mask <<= 1) { alts->pixidx[ialt] = 0; if (alts->pixlist[0] | mask) { for (icol = 1; icol <= ncol; icol++) { if (alts->pixlist[icol] & mask) { alts->pixidx[ialt]++; } } } } /* Find the total number of coordinate representations. */ *nwcs = 0; alts->imgherit = 0; for (ialt = 0; ialt < 27; ialt++) { inherit[ialt] = 0; for (icol = 1; icol <= ncol; icol++) { if (alts->arridx[icol][ialt] < 0) { /* No BIMGARR keytype but there's at least one BINTAB. */ if (alts->arridx[0][ialt] > 0) { /* There is an IMGAXIS keytype that we will inherit, so count this representation. */ alts->arridx[icol][ialt] = alts->arridx[0][ialt]; } else { alts->arridx[icol][ialt] = 0; } } if (alts->arridx[icol][ialt]) { if (alts->arridx[0][ialt]) { /* All IMGHEAD keywords are inherited for this ialt. */ inherit[ialt] = 1; if (alts->arridx[icol][ialt] < alts->arridx[0][ialt]) { /* The extra axes are also inherited. */ alts->arridx[icol][ialt] = alts->arridx[0][ialt]; } } (*nwcs)++; } } /* Count every "a" found in any IMGHEAD keyword... */ if (alts->arridx[0][ialt]) { if (inherit[ialt]) { /* ...but not if the IMGHEAD keywords will be inherited. */ alts->arridx[0][ialt] = 0; alts->imgherit = 1; } else { (*nwcs)++; } } /* We need a struct for every "a" found in a PIXLIST keyword. */ if (alts->pixidx[ialt]) { (*nwcs)++; } } if (*nwcs) { /* Allocate memory for the required number of wcsprm structs. */ if (!(*wcs = calloc(*nwcs, sizeof(struct wcsprm)))) { return 2; } /* Record the current values of NPVMAX and NPSMAX. */ npvmax = wcsnpv(-1); npsmax = wcsnps(-1); /* Initialize each wcsprm struct. */ wcsp = *wcs; *nwcs = 0; for (icol = 0; icol <= ncol; icol++) { for (ialt = 0; ialt < 27; ialt++) { if (alts->arridx[icol][ialt]) { /* Image-header representations that are not for inheritance (icol == 0) or binary table image array representations. */ wcsp->flag = -1; wcsnpv(alts->npv[icol][ialt]); wcsnps(alts->nps[icol][ialt]); if ((status = wcsini(1, (int)(alts->arridx[icol][ialt]), wcsp))) { wcsvfree(nwcs, wcs); break; } /* Record the alternate version code. */ if (ialt) { wcsp->alt[0] = 'A' + ialt - 1; } /* Record the table column number. */ wcsp->colnum = icol; /* On the second pass alts->arridx[icol][27] indexes the array of wcsprm structs. */ alts->arridx[icol][ialt] = (*nwcs)++; wcsp++; } else { /* Signal that this column has no WCS for this "a". */ alts->arridx[icol][ialt] = -1; } } } for (ialt = 0; ialt < 27; ialt++) { if (alts->pixidx[ialt]) { /* Pixel lists representations. */ wcsp->flag = -1; wcsnpv(alts->pixnpv[ialt]); wcsnps(alts->pixnps[ialt]); if ((status = wcsini(1, (int)(alts->pixidx[ialt]), wcsp))) { wcsvfree(nwcs, wcs); break; } /* Record the alternate version code. */ if (ialt) { wcsp->alt[0] = 'A' + ialt - 1; } /* Record the pixel list column numbers. */ mask = (1 << ialt); for (icol = 1, ix = 0; icol <= ncol; icol++) { if (alts->pixlist[icol] & mask) { wcsp->colax[ix++] = icol; } } /* alts->pixidx[] indexes the array of wcsprm structs. */ alts->pixidx[ialt] = (*nwcs)++; wcsp++; } else { /* Signal that this column is not a pixel list axis for this "a". */ alts->pixidx[ialt] = -1; } } /* Restore the original values of NPVMAX and NPSMAX. */ wcsnpv(npvmax); wcsnps(npsmax); } return status; } /*---------------------------------------------------------------------------- * Return a pointer to the next wcsprm struct for a particular column number * and alternate. *---------------------------------------------------------------------------*/ struct wcsprm *wcsbth_idx( struct wcsprm *wcs, struct wcsbth_alts *alts, int keytype, int n, char a) { const char as[] = " ABCDEFGHIJKLMNOPQRSTUVWXYZ"; int iwcs; if (!wcs) return 0x0; iwcs = -1; for (; iwcs < 0 && alts->ialt < 27; alts->ialt++) { /* Note that a == 0 applies to every alternate, otherwise this loop simply determines the appropriate value of alts->ialt. */ if (a && a != as[alts->ialt]) continue; if (keytype & (IMGHEAD | BIMGARR)) { for (; iwcs < 0 && alts->icol <= alts->ncol; alts->icol++) { /* Image header keywords, n == 0, apply to all columns, otherwise this loop simply determines the appropriate value of alts->icol. */ if (n && n != alts->icol) continue; iwcs = alts->arridx[alts->icol][alts->ialt]; } /* Break out of the loop to stop alts->ialt from being incremented. */ if (iwcs >= 0) break; /* Start from scratch for the next alts->ialt. */ alts->icol = 0; } if (keytype & (IMGAUX | PIXLIST)) { iwcs = alts->pixidx[alts->ialt]; } } return (iwcs >= 0) ? (wcs + iwcs) : 0x0; } /*---------------------------------------------------------------------------- * Return the axis number associated with the specified column number in a * particular pixel list coordinate representation. *---------------------------------------------------------------------------*/ int wcsbth_colax( struct wcsprm *wcs, struct wcsbth_alts *alts, int n, char a) { int ix; struct wcsprm *wcsp; if (!wcs) return 0; wcsp = wcs; if (a != ' ') { wcsp += alts->pixidx[a-'A'+1]; } for (ix = 0; ix < wcsp->naxis; ix++) { if (wcsp->colax[ix] == n) { return ++ix; } } return 0; } /*---------------------------------------------------------------------------- * Interpret EPOCH keywords. *---------------------------------------------------------------------------*/ int wcsbth_epoch(void *wptr) { double *equinox; /* If EQUINOXa is currently undefined then set it from EPOCHa. */ equinox = (double *)wptr; if (undefined(*equinox)) { sscanf(yytext, "%lf", equinox); } return 0; } /*---------------------------------------------------------------------------- * Interpret VSOURCE keywords. *---------------------------------------------------------------------------*/ int wcsbth_vsource(void *wptr) { double beta, c = 299792458.0, vsource, *zsource; /* If ZSOURCEa is currently undefined then set it from VSOURCEa. */ zsource = (double *)wptr; if (undefined(*zsource)) { sscanf(yytext, "%lf", &vsource); /* Convert relativistic Doppler velocity to redshift. */ beta = vsource/c; *zsource = (1.0 + beta)/sqrt(1.0 - beta*beta) - 1.0; } return 0; } /*---------------------------------------------------------------------------- * Tie up loose ends. *---------------------------------------------------------------------------*/ int wcsbth_final( struct wcsbth_alts *alts, int *nwcs, struct wcsprm **wcs) { int ialt, status; if (alts->arridx) free(alts->arridx); if (alts->npv) free(alts->npv); if (alts->nps) free(alts->nps); if (alts->pixlist) free(alts->pixlist); for (ialt = 0; ialt < *nwcs; ialt++) { /* Interpret -TAB header keywords. */ if ((status = wcstab(*wcs+ialt))) { wcsvfree(nwcs, wcs); return status; } } return 0; } pywcs-1.12/wcslib/C/wcserr.c0000644001153600020070000000733712310355626017776 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility Module author: Michael Droettboom http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcserr.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcserr.h" #include "wcsprintf.h" static int wcserr_enabled = 0; /*--------------------------------------------------------------------------*/ int wcserr_enable(int enable) { return wcserr_enabled = (enable ? 1 : 0); } /*--------------------------------------------------------------------------*/ int wcserr_prt( const struct wcserr *err, const char *prefix) { if (!wcserr_enabled) { wcsprintf("Error messaging is not enabled, use wcserr_enable().\n"); return 2; } if (err == 0x0) { return 0; } if (err->status) { if (prefix == 0x0) prefix = ""; if (err->status > 0) { wcsprintf("%sERROR %d in %s() at line %d of file %s:\n%s%s.\n", prefix, err->status, err->function, err->line_no, err->file, prefix, err->msg); } else { /* An informative message only. */ wcsprintf("%sINFORMATIVE message from %s() at line %d of file " "%s:\n%s%s.\n", prefix, err->function, err->line_no, err->file, prefix, err->msg); } } return 0; } /*--------------------------------------------------------------------------*/ int wcserr_clear( struct wcserr **err) { if (*err) free(*err); *err = 0x0; return 0; } /*--------------------------------------------------------------------------*/ int wcserr_set( struct wcserr **err, int status, const char *function, const char *file, int line_no, const char *format, ...) { va_list argp; if (!wcserr_enabled) return status; if (err == 0x0) { return status; } if (status) { if (*err == 0x0) { *err = calloc(1, sizeof(struct wcserr)); } (*err)->status = status; (*err)->function = function; (*err)->file = file; (*err)->line_no = line_no; va_start(argp, format); vsnprintf((*err)->msg, WCSERR_MSG_LENGTH, format, argp); va_end(argp); } else { if (*err) free(*err); *err = 0x0; } return status; } /*--------------------------------------------------------------------------*/ int wcserr_copy( const struct wcserr *src, struct wcserr *dst) { if (src == 0x0) { if (dst) { memset(dst, 0, sizeof(struct wcserr)); } return 0; } if (dst) { memcpy(dst, src, sizeof(struct wcserr)); } return src->status; } pywcs-1.12/wcslib/C/wcserr.h0000644001153600020070000002174212310355626017777 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility Module author: Michael Droettboom http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcserr.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * Summary of the wcserr routines * ------------------------------ * Most of the structs in WCSLIB contain a pointer to a wcserr struct as a * member. Functions in WCSLIB that return an error status code can also * allocate and set a detailed error message in this struct which also * identifies the function, source file, and line number where the error * occurred. * * For example: * = struct prjprm prj; = wcserr_enable(1); = if (prjini(&prj)) { = // Print the error message to stderr. = wcsprintf_set(stderr); = wcserr_prt(prj.err, 0x0); = } * * A number of utility functions used in managing the wcserr struct are for * internal use only. They are documented here solely as an aid to * understanding the code. They are not intended for external use - the API * may change without notice! * * * wcserr struct - Error message handling * -------------------------------------- * The wcserr struct contains the numeric error code, a textual description of * the error, and information about the function, source file, and line number * where the error was generated. * * int status * Numeric status code associated with the error, the meaning of which * depends on the function that generated it. See the documentation for * the particular function. * * int line_no * Line number where the error occurred as given by the __LINE__ * preprocessor macro. * * const char *function * Name of the function where the error occurred. * * const char *file * Name of the source file where the error occurred as given by the * __FILE__ preprocessor macro. * * char msg[WCSERR_MSG_LENGTH] * Informative error message. * * * wcserr_enable() - Enable/disable error messaging * ------------------------------------------------ * wcserr_enable() enables or disables wcserr error messaging. By default it * is disabled. * * PLEASE NOTE: This function is not thread-safe. * * Given: * enable int If true (non-zero), enable error messaging, else * disable it. * * Function return value: * int Status return value: * 0: Error messaging is disabled. * 1: Error messaging is enabled. * * * wcserr_prt() - Print a wcserr struct * ------------------------------------ * wcserr_prt() prints the error message (if any) contained in a wcserr struct. * It uses the wcsprintf() functions. * * Given: * err const struct wcserr* * The error object. If NULL, nothing is printed. * * prefix const char * * If non-NULL, each output line will be prefixed with * this string. * * Function return value: * int Status return value: * 0: Success. * 2: Error messaging is not enabled. * * * wcserr_clear() - Clear a wcserr struct * -------------------------------------- * wcserr_clear() clears the error (if any) contained in a wcserr struct. * * Given and returned: * err struct wcserr** * The error object. If NULL, nothing is done. Set to * NULL on return. * * Function return value: * int Status return value: * 0: Success. * * * wcserr_set() - Fill in the contents of an error object * ------------------------------------------------------ * INTERNAL USE ONLY. * * wcserr_set() fills a wcserr struct with information about an error. * * A convenience macro, WCSERR_SET, provides the source file and line number * information automatically. * * Given and returned: * err struct wcserr** * Error object. * * If err is NULL, returns the status code given without * setting an error message. * * If *err is NULL, allocates memory for a wcserr struct * (provided that status is non-zero). * * Given: * status int Numeric status code to set. If 0, then *err will be * deleted and *err will be returned as NULL. * * function const char * * Name of the function generating the error. This * must point to a constant string, i.e. in the * initialized read-only data section ("data") of the * executable. * * file const char * * Name of the source file generating the error. This * must point to a constant string, i.e. in the * initialized read-only data section ("data") of the * executable such as given by the __FILE__ preprocessor * macro. * * line_no int Line number in the source file generating the error * such as given by the __LINE__ preprocessor macro. * * format const char * * Format string of the error message. May contain * printf-style %-formatting codes. * * ... mixed The remaining variable arguments are applied (like * printf) to the format string to generate the error * message. * * Function return value: * int The status return code passed in. * * * wcserr_copy() - Copy an error object * ------------------------------------ * INTERNAL USE ONLY. * * wcserr_copy() copies one error object to another. Use of this function * should be avoided in general since the function, source file, and line * number information copied to the destination may lose its context. * * Given: * src const struct wcserr* * Source error object. If src is NULL, dst is cleared. * * Returned: * dst struct wcserr* * Destination error object. If NULL, no copy is made. * * Function return value: * int Numeric status code of the source error object. * * * WCSERR_SET() macro - Fill in the contents of an error object * ------------------------------------------------------------ * INTERNAL USE ONLY. * * WCSERR_SET() is a preprocessor macro that helps to fill in the argument list * of wcserr_set(). It takes status as an argument of its own and provides the * name of the source file and the line number at the point where invoked. It * assumes that the err and function arguments of wcserr_set() will be provided * by variables of the same names. * *===========================================================================*/ #ifndef WCSLIB_WCSERR #define WCSLIB_WCSERR #define WCSERR_MSG_LENGTH 160 struct wcserr { int status; /* Status code for the error. */ int line_no; /* Line number where the error occurred. */ const char *function; /* Function name. */ const char *file; /* Source file name. */ char msg[WCSERR_MSG_LENGTH]; /* Informative error message. */ }; /* Size of the wcserr struct in int units, used by the Fortran wrappers. */ #define ERRLEN (sizeof(struct wcserr)/sizeof(int)) int wcserr_enable(int enable); int wcserr_prt(const struct wcserr *err, const char *prefix); int wcserr_clear(struct wcserr **err); /* INTERNAL USE ONLY -------------------------------------------------------*/ int wcserr_set(struct wcserr **err, int status, const char *function, const char *file, int line_no, const char *format, ...); int wcserr_copy(const struct wcserr *src, struct wcserr *dst); /* Convenience macro for invoking wcserr_set(). */ #define WCSERR_SET(status) err, status, function, __FILE__, __LINE__ #endif /* WSCLIB_WCSERR */ pywcs-1.12/wcslib/C/wcsfix.c0000644001153600020070000005125612310355626017773 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsfix.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsutil.h" #include "sph.h" #include "wcs.h" #include "wcsunits.h" #include "wcsfix.h" extern const int WCSSET; /* Maximum number of coordinate axes that can be handled. */ #define NMAX 16 /* Map status return value to message. */ const char *wcsfix_errmsg[] = { "Success", "Null wcsprm pointer passed", "Memory allocation failed", "Linear transformation matrix is singular", "Inconsistent or unrecognized coordinate axis types", "Invalid parameter value", "Invalid coordinate transformation parameters", "Ill-conditioned coordinate transformation parameters", "All of the corner pixel coordinates are invalid", "Could not determine reference pixel coordinate", "Could not determine reference pixel value"}; /* Convenience macro for invoking wcserr_set(). */ #define WCSFIX_ERRMSG(status) WCSERR_SET(status), wcsfix_errmsg[status] /*--------------------------------------------------------------------------*/ int wcsfix(int ctrl, const int naxis[], struct wcsprm *wcs, int stat[]) { int status = 0; if ((stat[CDFIX] = cdfix(wcs)) > 0) { status = 1; } if ((stat[DATFIX] = datfix(wcs)) > 0) { status = 1; } if ((stat[UNITFIX] = unitfix(ctrl, wcs)) > 0) { status = 1; } if ((stat[SPCFIX] = spcfix(wcs)) > 0) { status = 1; } if ((stat[CELFIX] = celfix(wcs)) > 0) { status = 1; } if ((stat[CYLFIX] = cylfix(naxis, wcs)) > 0) { status = 1; } return status; } /*--------------------------------------------------------------------------*/ int wcsfixi(int ctrl, const int naxis[], struct wcsprm *wcs, int stat[], struct wcserr info[]) { int ifix, status = 0; struct wcserr err; /* Handling the status values returned from the sub-fixers is trickier than it might seem, especially considering that wcs->err may contain an error status on input which should be preserved if no translation errors occur. The simplest way seems to be to save a copy of wcs->err and clear it before each sub-fixer. The last real error to occur, excluding informative messages, is the one returned. To get informative messages from spcfix() it must precede celfix() and cylfix(). The latter call wcsset() which also translates AIPS-convention spectral axes. */ wcserr_copy(wcs->err, &err); for (ifix = CDFIX; ifix < NWCSFIX; ifix++) { /* Clear (delete) wcs->err. */ wcserr_clear(&(wcs->err)); switch (ifix) { case CDFIX: stat[ifix] = cdfix(wcs); break; case DATFIX: stat[ifix] = datfix(wcs); break; case UNITFIX: stat[ifix] = unitfix(ctrl, wcs); break; case SPCFIX: stat[ifix] = spcfix(wcs); break; case CELFIX: stat[ifix] = celfix(wcs); break; case CYLFIX: stat[ifix] = cylfix(naxis, wcs); break; default: continue; } if (stat[ifix] == FIXERR_NO_CHANGE) { /* No change => no message. */ wcserr_copy(0x0, info+ifix); } else if (stat[ifix] == FIXERR_SUCCESS) { /* Successful translation, but there may be an informative message. */ if (wcs->err && wcs->err->status < 0) { wcserr_copy(wcs->err, info+ifix); } else { wcserr_copy(0x0, info+ifix); } } else { /* An informative message or error message. */ wcserr_copy(wcs->err, info+ifix); if ((status = (stat[ifix] > 0))) { /* It was an error, replace the previous one. */ wcserr_copy(wcs->err, &err); } } } /* Restore the last error to occur. */ if (err.status) { wcserr_copy(&err, wcs->err); } else { wcserr_clear(&(wcs->err)); } return status; } /*--------------------------------------------------------------------------*/ int cdfix(struct wcsprm *wcs) { int i, k, naxis, status = FIXERR_NO_CHANGE; double *cd; if (wcs == 0x0) return FIXERR_NULL_POINTER; if ((wcs->altlin & 1) || !(wcs->altlin & 2)) { /* Either we have PCi_ja or there are no CDi_ja. */ return FIXERR_NO_CHANGE; } naxis = wcs->naxis; status = FIXERR_NO_CHANGE; for (i = 0; i < naxis; i++) { /* Row of zeros? */ cd = wcs->cd + i * naxis; for (k = 0; k < naxis; k++, cd++) { if (*cd != 0.0) goto next; } /* Column of zeros? */ cd = wcs->cd + i; for (k = 0; k < naxis; k++, cd += naxis) { if (*cd != 0.0) goto next; } cd = wcs->cd + i * (naxis + 1); *cd = 1.0; status = FIXERR_SUCCESS; next: ; } return status; } /*--------------------------------------------------------------------------*/ int datfix(struct wcsprm *wcs) { static const char *function = "datfix"; char orig_dateobs[72]; char *dateobs; int day, dd, hour = 0, jd, minute = 0, month, msec, n4, year; double mjdobs, sec = 0.0, t; struct wcserr **err; if (wcs == 0x0) return FIXERR_NULL_POINTER; err = &(wcs->err); dateobs = wcs->dateobs; strncpy(orig_dateobs, dateobs, 72); if (dateobs[0] == '\0') { if (undefined(wcs->mjdobs)) { /* No date information was provided. */ return FIXERR_NO_CHANGE; } else { /* Calendar date from MJD. */ jd = 2400001 + (int)wcs->mjdobs; n4 = 4*(jd + ((2*((4*jd - 17918)/146097)*3)/4 + 1)/2 - 37); dd = 10*(((n4-237)%1461)/4) + 5; year = n4/1461 - 4712; month = (2 + dd/306)%12 + 1; day = (dd%306)/10 + 1; sprintf(dateobs, "%.4d-%.2d-%.2d", year, month, day); /* Write time part only if non-zero. */ if ((t = wcs->mjdobs - (int)wcs->mjdobs) > 0.0) { t *= 24.0; hour = (int)t; t = 60.0 * (t - hour); minute = (int)t; sec = 60.0 * (t - minute); /* Round to 1ms. */ dd = 60000*(60*hour + minute) + (int)(1000*(sec+0.0005)); hour = dd / 3600000; dd -= 3600000 * hour; minute = dd / 60000; msec = dd - 60000 * minute; sprintf(dateobs+10, "T%.2d:%.2d:%.2d", hour, minute, msec/1000); /* Write fractions of a second only if non-zero. */ if (msec%1000) { sprintf(dateobs+19, ".%.3d", msec%1000); } } } } else { if (strlen(dateobs) < 8) { /* Can't be a valid date. */ return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: date string too short '%s'", dateobs); } /* Identify the date format. */ if (dateobs[4] == '-' && dateobs[7] == '-') { /* Standard year-2000 form: CCYY-MM-DD[Thh:mm:ss[.sss...]] */ if (sscanf(dateobs, "%4d-%2d-%2d", &year, &month, &day) < 3) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid date '%s'", dateobs); } if (dateobs[10] == 'T') { if (sscanf(dateobs+11, "%2d:%2d:%lf", &hour, &minute, &sec) < 3) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid time '%s'", dateobs+11); } } else if (dateobs[10] == ' ') { hour = 0; minute = 0; sec = 0.0; if (sscanf(dateobs+11, "%2d:%2d:%lf", &hour, &minute, &sec) == 3) { dateobs[10] = 'T'; } else { sprintf(dateobs+10, "T%.2d:%.2d:%04.1f", hour, minute, sec); } } } else if (dateobs[4] == '/' && dateobs[7] == '/') { /* Also allow CCYY/MM/DD[Thh:mm:ss[.sss...]] */ if (sscanf(dateobs, "%4d/%2d/%2d", &year, &month, &day) < 3) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid date '%s'", dateobs); } if (dateobs[10] == 'T') { if (sscanf(dateobs+11, "%2d:%2d:%lf", &hour, &minute, &sec) < 3) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid time '%s'", dateobs+11); } } else if (dateobs[10] == ' ') { hour = 0; minute = 0; sec = 0.0; if (sscanf(dateobs+11, "%2d:%2d:%lf", &hour, &minute, &sec) == 3) { dateobs[10] = 'T'; } else { sprintf(dateobs+10, "T%.2d:%.2d:%04.1f", hour, minute, sec); } } /* Looks ok, fix it up. */ dateobs[4] = '-'; dateobs[7] = '-'; } else { if (dateobs[2] == '/' && dateobs[5] == '/') { /* Old format date: DD/MM/YY, also allowing DD/MM/CCYY. */ if (sscanf(dateobs, "%2d/%2d/%4d", &day, &month, &year) < 3) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid date '%s'", dateobs); } } else if (dateobs[2] == '-' && dateobs[5] == '-') { /* Also recognize DD-MM-YY and DD-MM-CCYY */ if (sscanf(dateobs, "%2d-%2d-%4d", &day, &month, &year) < 3) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid date '%s'", dateobs); } } else { /* Not a valid date format. */ return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: invalid date '%s'", dateobs); } if (year < 100) year += 1900; /* Doesn't have a time. */ sprintf(dateobs, "%.4d-%.2d-%.2d", year, month, day); } /* Compute MJD. */ mjdobs = (double)((1461*(year - (12-month)/10 + 4712))/4 + (306*((month+9)%12) + 5)/10 - (3*((year - (12-month)/10 + 4900)/100))/4 + day - 2399904) + (hour + (minute + sec/60.0)/60.0)/24.0; if (undefined(wcs->mjdobs)) { wcs->mjdobs = mjdobs; } else { /* Check for consistency. */ if (fabs(mjdobs - wcs->mjdobs) > 0.5) { return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: inconsistent date '%s'", dateobs); } } } if (strncmp(orig_dateobs, dateobs, 72)) { wcserr_set(WCSERR_SET(FIXERR_DATE_FIX), "Changed '%s' to '%s'", orig_dateobs, dateobs); return FIXERR_SUCCESS; } return FIXERR_NO_CHANGE; } /*--------------------------------------------------------------------------*/ int unitfix(int ctrl, struct wcsprm *wcs) { int i, k, status = FIXERR_NO_CHANGE; char orig_unit[80], msg[WCSERR_MSG_LENGTH]; const char *function = "unitfix"; struct wcserr **err; if (wcs == 0x0) return FIXERR_NULL_POINTER; err = &(wcs->err); strcpy(msg, "Changed units: "); for (i = 0; i < wcs->naxis; i++) { strncpy(orig_unit, wcs->cunit[i], 80); if (wcsutrne(ctrl, wcs->cunit[i], &(wcs->err)) == 0) { k = strlen(msg); sprintf(msg+k, "'%s' -> '%s', ", orig_unit, wcs->cunit[i]); status = FIXERR_UNITS_ALIAS; } } if (status == FIXERR_UNITS_ALIAS) { k = strlen(msg) - 2; msg[k] = '\0'; wcserr_set(WCSERR_SET(FIXERR_UNITS_ALIAS), msg); status = FIXERR_SUCCESS; } return status; } /*--------------------------------------------------------------------------*/ int spcfix(struct wcsprm *wcs) { static const char *function = "spcfix"; char ctype[9], specsys[9]; int i, status; struct wcserr **err; if (wcs == 0x0) return FIXERR_NULL_POINTER; err = &(wcs->err); for (i = 0; i < wcs->naxis; i++) { /* Translate an AIPS-convention spectral type if present. */ status = spcaips(wcs->ctype[i], wcs->velref, ctype, specsys); if (status == 0) { /* An AIPS type was found but it may match what we already have. */ status = FIXERR_NO_CHANGE; /* Was specsys translated? */ if (wcs->specsys[0] == '\0' && *specsys) { strncpy(wcs->specsys, specsys, 9); wcserr_set(WCSERR_SET(FIXERR_SPC_UPDATE), "Changed SPECSYS to '%s'", specsys); status = FIXERR_SUCCESS; } /* Was ctype translated? Have to null-fill for comparing them. */ wcsutil_null_fill(9, wcs->ctype[i]); if (strncmp(wcs->ctype[i], ctype, 9)) { /* ctype was translated... */ if (status == FIXERR_SUCCESS) { /* ...and specsys was also. */ wcserr_set(WCSERR_SET(FIXERR_SPC_UPDATE), "Changed CTYPE%d from '%s' to '%s', and SPECSYS to '%s'", i+1, wcs->ctype[i], ctype, wcs->specsys); } else { wcserr_set(WCSERR_SET(FIXERR_SPC_UPDATE), "Changed CTYPE%d from '%s' to '%s'", i+1, wcs->ctype[i], ctype); status = FIXERR_SUCCESS; } strncpy(wcs->ctype[i], ctype, 9); } /* Tidy up. */ if (status == FIXERR_SUCCESS) { wcsutil_null_fill(72, wcs->ctype[i]); wcsutil_null_fill(72, wcs->specsys); } /* No need to check for others, wcsset() will fail if so. */ return status; } else if (status == SPCERR_BAD_SPEC_PARAMS) { /* An AIPS spectral type was found but with invalid velref. */ return wcserr_set(WCSERR_SET(FIXERR_BAD_PARAM), "Invalid parameter value: velref = %d", wcs->velref); } } return FIXERR_NO_CHANGE; } /*--------------------------------------------------------------------------*/ int celfix(struct wcsprm *wcs) { static const char *function = "celfix"; int k, status; struct celprm *wcscel = &(wcs->cel); struct prjprm *wcsprj = &(wcscel->prj); struct wcserr **err; if (wcs == 0x0) return FIXERR_NULL_POINTER; err = &(wcs->err); /* Initialize if required. */ if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } /* Was an NCP or GLS projection code translated? */ if (wcs->lat >= 0) { /* Check ctype. */ if (strcmp(wcs->ctype[wcs->lat]+5, "NCP") == 0) { strcpy(wcs->ctype[wcs->lng]+5, "SIN"); strcpy(wcs->ctype[wcs->lat]+5, "SIN"); if (wcs->npvmax < wcs->npv + 2) { /* Allocate space for two more PVi_ja keyvalues. */ if (wcs->m_flag == WCSSET && wcs->pv == wcs->m_pv) { if (!(wcs->pv = calloc(wcs->npv+2, sizeof(struct pvcard)))) { wcs->pv = wcs->m_pv; return wcserr_set(WCSFIX_ERRMSG(FIXERR_MEMORY)); } wcs->npvmax = wcs->npv + 2; wcs->m_flag = WCSSET; for (k = 0; k < wcs->npv; k++) { wcs->pv[k] = wcs->m_pv[k]; } if (wcs->m_pv) free(wcs->m_pv); wcs->m_pv = wcs->pv; } else { return wcserr_set(WCSFIX_ERRMSG(FIXERR_MEMORY)); } } wcs->pv[wcs->npv].i = wcs->lat + 1; wcs->pv[wcs->npv].m = 1; wcs->pv[wcs->npv].value = wcsprj->pv[1]; (wcs->npv)++; wcs->pv[wcs->npv].i = wcs->lat + 1; wcs->pv[wcs->npv].m = 2; wcs->pv[wcs->npv].value = wcsprj->pv[2]; (wcs->npv)++; return FIXERR_SUCCESS; } else if (strcmp(wcs->ctype[wcs->lat]+5, "GLS") == 0) { strcpy(wcs->ctype[wcs->lng]+5, "SFL"); strcpy(wcs->ctype[wcs->lat]+5, "SFL"); if (wcs->crval[wcs->lng] != 0.0 || wcs->crval[wcs->lat] != 0.0) { /* In the AIPS convention, setting the reference longitude and * latitude for GLS does not create an oblique graticule. A non-zero * reference longitude introduces an offset in longitude in the normal * way, whereas a non-zero reference latitude simply translates the * reference point (i.e. the map as a whole) to that latitude. This * might be effected by adjusting CRPIXja but that is complicated by * the linear transformation and instead is accomplished here by * setting theta_0. */ if (wcs->npvmax < wcs->npv + 2) { /* Allocate space for three more PVi_ja keyvalues. */ if (wcs->m_flag == WCSSET && wcs->pv == wcs->m_pv) { if (!(wcs->pv = calloc(wcs->npv+3, sizeof(struct pvcard)))) { wcs->pv = wcs->m_pv; return wcserr_set(WCSFIX_ERRMSG(FIXERR_MEMORY)); } wcs->npvmax = wcs->npv + 3; wcs->m_flag = WCSSET; for (k = 0; k < wcs->npv; k++) { wcs->pv[k] = wcs->m_pv[k]; } if (wcs->m_pv) free(wcs->m_pv); wcs->m_pv = wcs->pv; } else { return wcserr_set(WCSFIX_ERRMSG(FIXERR_MEMORY)); } } wcs->pv[wcs->npv].i = wcs->lng + 1; wcs->pv[wcs->npv].m = 0; wcs->pv[wcs->npv].value = 1.0; (wcs->npv)++; /* Note that the reference longitude is still zero. */ wcs->pv[wcs->npv].i = wcs->lng + 1; wcs->pv[wcs->npv].m = 1; wcs->pv[wcs->npv].value = 0.0; (wcs->npv)++; wcs->pv[wcs->npv].i = wcs->lng + 1; wcs->pv[wcs->npv].m = 2; wcs->pv[wcs->npv].value = wcs->crval[wcs->lat]; (wcs->npv)++; } return FIXERR_SUCCESS; } } return FIXERR_NO_CHANGE; } /*--------------------------------------------------------------------------*/ int cylfix(const int naxis[], struct wcsprm *wcs) { static const char *function = "cylfix"; unsigned short icnr, indx[NMAX], ncnr; int j, k, stat[4], status; double img[4][NMAX], lat, lng, phi[4], phi0, phimax, phimin, pix[4][NMAX], *pixj, theta[4], theta0, world[4][NMAX], x, y; struct wcserr **err; if (naxis == 0x0) return FIXERR_NO_CHANGE; if (wcs == 0x0) return FIXERR_NULL_POINTER; err = &(wcs->err); /* Initialize if required. */ if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } /* Check that we have a cylindrical projection. */ if (wcs->cel.prj.category != CYLINDRICAL) return FIXERR_NO_CHANGE; if (wcs->naxis < 2) return FIXERR_NO_CHANGE; /* Compute the native longitude in each corner of the image. */ ncnr = 1 << wcs->naxis; for (k = 0; k < NMAX; k++) { indx[k] = 1 << k; } phimin = 1.0e99; phimax = -1.0e99; for (icnr = 0; icnr < ncnr;) { /* Do four corners at a time. */ for (j = 0; j < 4; j++, icnr++) { pixj = pix[j]; for (k = 0; k < wcs->naxis; k++) { if (icnr & indx[k]) { *(pixj++) = naxis[k] + 0.5; } else { *(pixj++) = 0.5; } } } if (!(status = wcsp2s(wcs, 4, NMAX, pix[0], img[0], phi, theta, world[0], stat))) { for (j = 0; j < 4; j++) { if (phi[j] < phimin) phimin = phi[j]; if (phi[j] > phimax) phimax = phi[j]; } } } if (phimin > phimax) return status; /* Any changes needed? */ if (phimin >= -180.0 && phimax <= 180.0) return FIXERR_NO_CHANGE; /* Compute the new reference pixel coordinates. */ phi0 = (phimin + phimax) / 2.0; theta0 = 0.0; if ((status = prjs2x(&(wcs->cel.prj), 1, 1, 1, 1, &phi0, &theta0, &x, &y, stat))) { if (status == PRJERR_BAD_PARAM) { return wcserr_set(WCSFIX_ERRMSG(FIXERR_BAD_PARAM)); } return wcserr_set(WCSFIX_ERRMSG(FIXERR_NO_REF_PIX_COORD)); } for (k = 0; k < wcs->naxis; k++) { img[0][k] = 0.0; } img[0][wcs->lng] = x; img[0][wcs->lat] = y; if ((status = linx2p(&(wcs->lin), 1, 0, img[0], pix[0]))) { return wcserr_set(WCSFIX_ERRMSG(status)); } /* Compute celestial coordinates at the new reference pixel. */ if ((status = wcsp2s(wcs, 1, 0, pix[0], img[0], phi, theta, world[0], stat))) { if (wcs->err->status == WCSERR_BAD_PIX) { wcs->err->status = FIXERR_NO_REF_PIX_COORD; } return wcs->err->status; } /* Compute native coordinates of the celestial pole. */ lng = 0.0; lat = 90.0; (void)sphs2x(wcs->cel.euler, 1, 1, 1, 1, &lng, &lat, phi, theta); wcs->crpix[wcs->lng] = pix[0][wcs->lng]; wcs->crpix[wcs->lat] = pix[0][wcs->lat]; wcs->crval[wcs->lng] = world[0][wcs->lng]; wcs->crval[wcs->lat] = world[0][wcs->lat]; wcs->lonpole = phi[0] - phi0; return wcsset(wcs); } pywcs-1.12/wcslib/C/wcsfix.h0000644001153600020070000004105712310355626017776 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsfix.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of celestial coordinates in FITS", * Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077 (Paper II) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the wcsfix routines * ------------------------------ * Routines in this suite identify and translate various forms of non-standard * construct that are known to occur in FITS WCS headers. These range from the * translation of non-standard values for standard WCS keywords, to the repair * of malformed coordinate representations. * * Non-standard keyvalues: * ----------------------- * AIPS-convention celestial projection types, NCP and GLS, and spectral * types, 'FREQ-LSR', 'FELO-HEL', etc., set in CTYPEia are translated * on-the-fly by wcsset() but without modifying the relevant ctype[], pv[] or * specsys members of the wcsprm struct. That is, only the information * extracted from ctype[] is translated when wcsset() fills in wcsprm::cel * (celprm struct) or wcsprm::spc (spcprm struct). * * On the other hand, these routines do change the values of wcsprm::ctype[], * wcsprm::pv[], wcsprm::specsys and other wcsprm struct members as * appropriate to produce the same result as if the FITS header itself had * been translated. * * Auxiliary WCS header information not used directly by WCSLIB may also be * translated. For example, the older DATE-OBS date format (wcsprm::dateobs) * is recast to year-2000 standard form, and MJD-OBS (wcsprm::mjdobs) will be * deduced from it if not already set. * * Certain combinations of keyvalues that result in malformed coordinate * systems, as described in Sect. 7.3.4 of Paper I, may also be repaired. * These are handled by cylfix(). * * Non-standard keywords: * ---------------------- * The AIPS-convention CROTAn keywords are recognized as quasi-standard and * as such are accomodated by the wcsprm::crota[] and translated to * wcsprm::pc[][] by wcsset(). These are not dealt with here, nor are any * other non-standard keywords since these routines work only on the contents * of a wcsprm struct and do not deal with FITS headers per se. In * particular, they do not identify or translate CD00i00j, PC00i00j, PROJPn, * EPOCH, VELREF or VSOURCEa keywords; this may be done by the FITS WCS * header parser supplied with WCSLIB, refer to wcshdr.h. * * wcsfix() and wcsfixi() apply all of the corrections handled by the following * specific functions which may also be invoked separately: * * - cdfix(): Sets the diagonal element of the CDi_ja matrix to 1.0 if all * CDi_ja keywords associated with a particular axis are omitted. * * - datfix(): recast an older DATE-OBS date format in dateobs to year-2000 * standard form and derive mjdobs from it if not already set. * Alternatively, if mjdobs is set and dateobs isn't, then derive dateobs * from it. * * - unitfix(): translate some commonly used but non-standard unit strings in * the CUNITia keyvalues, e.g. 'DEG' -> 'deg'. * * - spcfix(): translate AIPS-convention spectral types, 'FREQ-LSR', * 'FELO-HEL', etc., in ctype[] as set from CTYPEia. * * - celfix(): translate AIPS-convention celestial projection types, NCP and * GLS, in ctype[] as set from CTYPEia. * * - cylfix(): fixes WCS keyvalues for malformed cylindrical projections that * suffer from the problem described in Sect. 7.3.4 of Paper I. * * * wcsfix() - Translate a non-standard WCS struct * ---------------------------------------------- * wcsfix() is identical to wcsfixi(), but lacks the info argument. * * * wcsfixi() - Translate a non-standard WCS struct * ----------------------------------------------- * wcsfix() applies all of the corrections handled separately by cdfix(), * datfix(), unitfix(), spcfix(), celfix(), and cylfix(). * * Given: * ctrl int Do potentially unsafe translations of non-standard * unit strings as described in the usage notes to * wcsutrn(). * * naxis const int [] * Image axis lengths. If this array pointer is set to * zero then cylfix() will not be invoked. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Returned: * stat int [NWCSFIX] * Status returns from each of the functions. Use the * preprocessor macros NWCSFIX to dimension this vector * and CDFIX, DATFIX, UNITFIX, SPCFIX, CELFIX, and CYLFIX * to access its elements. A status value of -2 is set * for functions that were not invoked. * * info struct wcserr [NWCSFIX] * Status messages from each of the functions. Use the * preprocessor macros NWCSFIX to dimension this vector * and CDFIX, DATFIX, UNITFIX, SPCFIX, CELFIX, and CYLFIX * to access its elements. * * Function return value: * int Status return value: * 0: Success. * 1: One or more of the translation functions * returned an error. * * * cdfix() - Fix erroneously omitted CDi_ja keywords * ------------------------------------------------- * cdfix() sets the diagonal element of the CDi_ja matrix to unity if all * CDi_ja keywords associated with a given axis were omitted. According to * Paper I, if any CDi_ja keywords at all are given in a FITS header then those * not given default to zero. This results in a singular matrix with an * intersecting row and column of zeros. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * -1: No change required (not an error). * 0: Success. * 1: Null wcsprm pointer passed. * * * datfix() - Translate DATE-OBS and derive MJD-OBS or vice versa * -------------------------------------------------------------- * datfix() translates the old DATE-OBS date format set in wcsprm::dateobs to * year-2000 standard form (yyyy-mm-ddThh:mm:ss) and derives MJD-OBS from it if * not already set. Alternatively, if wcsprm::mjdobs is set and * wcsprm::dateobs isn't, then datfix() derives wcsprm::dateobs from it. If * both are set but disagree by more than half a day then status 5 is returned. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. wcsprm::dateobs * and/or wcsprm::mjdobs may be changed. * * Function return value: * int Status return value: * -1: No change required (not an error). * 0: Success. * 1: Null wcsprm pointer passed. * 5: Invalid parameter value. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * Notes: * The MJD algorithms used by datfix() are from D.A. Hatcher, 1984, QJRAS, * 25, 53-55, as modified by P.T. Wallace for use in SLALIB subroutines CLDJ * and DJCL. * * * unitfix() - Correct aberrant CUNITia keyvalues * ---------------------------------------------- * unitfix() applies wcsutrn() to translate non-standard CUNITia keyvalues, * e.g. 'DEG' -> 'deg', also stripping off unnecessary whitespace. * * Given: * ctrl int Do potentially unsafe translations described in the * usage notes to wcsutrn(). * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * -1: No change required (not an error). * 0: Success (an alias was applied). * 1: Null wcsprm pointer passed. * * When units are translated (i.e. status 0), status -2 * is set in the wcserr struct to allow an informative * message to be returned. * * * spcfix() - Translate AIPS-convention spectral types * --------------------------------------------------- * spcfix() translates AIPS-convention spectral coordinate types, * '{FREQ,FELO,VELO}-{LSR,HEL,OBS}' (e.g. 'FREQ-OBS', 'FELO-HEL', 'VELO-LSR') * set in wcsprm::ctype[], subject to VELREF set in wcsprm::velref. * * Note that if wcs::specsys is already set then it will not be overridden. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. wcsprm::ctype[] * and/or wcsprm::specsys may be changed. * * Function return value: * int Status return value: * -1: No change required (not an error). * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * celfix() - Translate AIPS-convention celestial projection types * --------------------------------------------------------------- * celfix() translates AIPS-convention celestial projection types, NCP and * GLS, set in the ctype[] member of the wcsprm struct. * * Two additional pv[] keyvalues are created when translating NCP. If the * pv[] array was initially allocated by wcsini() then the array will be * expanded if necessary. Otherwise, error 2 will be returned if two empty * slots are not already available for use. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. wcsprm::ctype[] * and/or wcsprm::pv[] may be changed. * * Function return value: * int Status return value: * -1: No change required (not an error). * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * cylfix() - Fix malformed cylindrical projections * ------------------------------------------------ * cylfix() fixes WCS keyvalues for malformed cylindrical projections that * suffer from the problem described in Sect. 7.3.4 of Paper I. * * Given: * naxis const int [] * Image axis lengths. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters. * * Function return value: * int Status return value: * -1: No change required (not an error). * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * 8: All of the corner pixel coordinates are invalid. * 9: Could not determine reference pixel coordinate. * 10: Could not determine reference pixel value. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * Global variable: const char *wcsfix_errmsg[] - Status return messages * --------------------------------------------------------------------- * Error messages to match the status value returned from each function. * *===========================================================================*/ #ifndef WCSLIB_WCSFIX #define WCSLIB_WCSFIX #include "wcs.h" #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif #define CDFIX 0 #define DATFIX 1 #define UNITFIX 2 #define SPCFIX 3 #define CELFIX 4 #define CYLFIX 5 #define NWCSFIX 6 extern const char *wcsfix_errmsg[]; #define cylfix_errmsg wcsfix_errmsg enum wcsfix_errmsg_enum { FIXERR_DATE_FIX = -4, /* The date formatting has been fixed up. */ FIXERR_SPC_UPDATE = -3, /* Spectral axis type modified. */ FIXERR_UNITS_ALIAS = -2, /* Units alias translation. */ FIXERR_NO_CHANGE = -1, /* No change. */ FIXERR_SUCCESS = 0, /* Success. */ FIXERR_NULL_POINTER = 1, /* Null wcsprm pointer passed. */ FIXERR_MEMORY = 2, /* Memory allocation failed. */ FIXERR_SINGULAR_MTX = 3, /* Linear transformation matrix is singular. */ FIXERR_BAD_CTYPE = 4, /* Inconsistent or unrecognized coordinate axis types. */ FIXERR_BAD_PARAM = 5, /* Invalid parameter value. */ FIXERR_BAD_COORD_TRANS = 6, /* Invalid coordinate transformation parameters. */ FIXERR_ILL_COORD_TRANS = 7, /* Ill-conditioned coordinate transformation parameters. */ FIXERR_BAD_CORNER_PIX = 8, /* All of the corner pixel coordinates are invalid. */ FIXERR_NO_REF_PIX_COORD = 9, /* Could not determine reference pixel coordinate. */ FIXERR_NO_REF_PIX_VAL = 10 /* Could not determine reference pixel value. */ }; int wcsfix(int ctrl, const int naxis[], struct wcsprm *wcs, int stat[]); int wcsfixi(int ctrl, const int naxis[], struct wcsprm *wcs, int stat[], struct wcserr info[]); int cdfix(struct wcsprm *wcs); int datfix(struct wcsprm *wcs); int unitfix(int ctrl, struct wcsprm *wcs); int spcfix(struct wcsprm *wcs); int celfix(struct wcsprm *wcs); int cylfix(const int naxis[], struct wcsprm *wcs); #ifdef __cplusplus } #endif #endif /* WCSLIB_WCSFIX */ pywcs-1.12/wcslib/C/wcshdr.c0000644001153600020070000007377612310355626017775 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcshdr.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include "wcsutil.h" #include "wcsmath.h" #include "wcshdr.h" #include "tab.h" #include "wcs.h" extern const int WCSSET; /* Map status return value to message. */ const char *wcshdr_errmsg[] = { "Success", "Null wcsprm pointer passed", "Memory allocation failed", "Invalid column selection", "Fatal error returned by Flex parser", "Invalid tabular parameters"}; /* Convenience macro for invoking wcserr_set(). */ #define WCSHDR_ERRMSG(status) WCSERR_SET(status), wcshdr_errmsg[status] static void wcshdo_util(int, const char [], const char [], int, const char [], int, int, int, char, int, int [], char [], const char [], int *, char **, int *); /*--------------------------------------------------------------------------*/ int wcstab(struct wcsprm *wcs) { static const char *function = "wcstab"; char (*PSi_0a)[72] = 0x0, (*PSi_1a)[72] = 0x0, (*PSi_2a)[72] = 0x0; int *PVi_1a = 0x0, *PVi_2a = 0x0, *PVi_3a = 0x0, *tabax, *tabidx = 0x0; int getcrd, i, ip, itab, itabax, j, jtabax, m, naxis, ntabax, status; struct wtbarr *wtbp; struct tabprm *tabp; struct wcserr **err; if (wcs == 0x0) return WCSHDRERR_NULL_POINTER; err = &(wcs->err); /* Free memory previously allocated by wcstab(). */ if (wcs->flag != -1 && wcs->m_flag == WCSSET) { if (wcs->wtb == wcs->m_wtb) wcs->wtb = 0x0; if (wcs->tab == wcs->m_tab) wcs->tab = 0x0; if (wcs->m_wtb) free(wcs->m_wtb); if (wcs->m_tab) { for (j = 0; j < wcs->ntab; j++) { tabfree(wcs->m_tab + j); } free(wcs->m_tab); } } wcs->ntab = 0; wcs->nwtb = 0; wcs->wtb = 0x0; wcs->tab = 0x0; /* Determine the number of -TAB axes. */ naxis = wcs->naxis; if (!(tabax = calloc(naxis, sizeof(int)))) { return wcserr_set(WCSHDR_ERRMSG(WCSHDRERR_MEMORY)); } ntabax = 0; for (i = 0; i < naxis; i++) { /* Null fill. */ wcsutil_null_fill(72, wcs->ctype[i]); if (!strcmp(wcs->ctype[i]+4, "-TAB")) { tabax[i] = ntabax++; } else { tabax[i] = -1; } } if (ntabax == 0) { /* No lookup tables. */ status = 0; goto cleanup; } /* Collect information from the PSi_ma and PVi_ma keyvalues. */ if (!((PSi_0a = calloc(ntabax, sizeof(char[72]))) && (PVi_1a = calloc(ntabax, sizeof(int))) && (PVi_2a = calloc(ntabax, sizeof(int))) && (PSi_1a = calloc(ntabax, sizeof(char[72]))) && (PSi_2a = calloc(ntabax, sizeof(char[72]))) && (PVi_3a = calloc(ntabax, sizeof(int))) && (tabidx = calloc(ntabax, sizeof(int))))) { status = wcserr_set(WCSHDR_ERRMSG(WCSHDRERR_MEMORY)); goto cleanup; } for (itabax = 0; itabax < ntabax; itabax++) { /* Remember that calloc() zeroes allocated memory. */ PVi_1a[itabax] = 1; PVi_2a[itabax] = 1; PVi_3a[itabax] = 1; } for (ip = 0; ip < wcs->nps; ip++) { itabax = tabax[wcs->ps[ip].i - 1]; if (itabax >= 0) { switch (wcs->ps[ip].m) { case 0: /* EXTNAME. */ strcpy(PSi_0a[itabax], wcs->ps[ip].value); wcsutil_null_fill(72, PSi_0a[itabax]); break; case 1: /* TTYPEn for coordinate array. */ strcpy(PSi_1a[itabax], wcs->ps[ip].value); wcsutil_null_fill(72, PSi_1a[itabax]); break; case 2: /* TTYPEn for index vector. */ strcpy(PSi_2a[itabax], wcs->ps[ip].value); wcsutil_null_fill(72, PSi_2a[itabax]); break; } } } for (ip = 0; ip < wcs->npv; ip++) { itabax = tabax[wcs->pv[ip].i - 1]; if (itabax >= 0) { switch (wcs->pv[ip].m) { case 1: /* EXTVER. */ PVi_1a[itabax] = (int)(wcs->pv[ip].value + 0.5); break; case 2: /* EXTLEVEL. */ PVi_2a[itabax] = (int)(wcs->pv[ip].value + 0.5); break; case 3: /* Table axis number. */ PVi_3a[itabax] = (int)(wcs->pv[ip].value + 0.5); break; } } } /* Determine the number of independent tables. */ for (itabax = 0; itabax < ntabax; itabax++) { /* These have no defaults. */ if (!PSi_0a[itabax][0] || !PSi_1a[itabax][0]) { status = wcserr_set(WCSERR_SET(WCSHDRERR_BAD_TABULAR_PARAMS), "Invalid tabular parameters: PSi_0a and PSi_1a must be specified"); goto cleanup; } tabidx[itabax] = -1; for (jtabax = 0; jtabax < i; jtabax++) { /* EXTNAME, EXTVER, EXTLEVEL, and TTYPEn for the coordinate array */ /* must match for each axis of a multi-dimensional lookup table. */ if (strcmp(PSi_0a[itabax], PSi_0a[jtabax]) == 0 && strcmp(PSi_1a[itabax], PSi_1a[jtabax]) == 0 && PVi_1a[itabax] == PVi_1a[jtabax] && PVi_2a[itabax] == PVi_2a[jtabax]) { tabidx[itabax] = tabidx[jtabax]; break; } } if (jtabax == itabax) { tabidx[itabax] = wcs->ntab; wcs->ntab++; } } if (!(wcs->tab = calloc(wcs->ntab, sizeof(struct tabprm)))) { status = wcserr_set(WCSHDR_ERRMSG(WCSHDRERR_MEMORY)); goto cleanup; } wcs->m_tab = wcs->tab; /* Table dimensionality; find the largest axis number. */ for (itabax = 0; itabax < ntabax; itabax++) { tabp = wcs->tab + tabidx[itabax]; /* PVi_3a records the 1-relative table axis number. */ if (PVi_3a[itabax] > tabp->M) { tabp->M = PVi_3a[itabax]; } } for (itab = 0; itab < wcs->ntab; itab++) { if ((status = tabini(1, wcs->tab[itab].M, 0, wcs->tab + itab))) { if (status == 3) status = 5; wcserr_set(WCSHDR_ERRMSG(status)); goto cleanup; } } /* Copy parameters into the tabprm structs. */ for (i = 0; i < naxis; i++) { if ((itabax = tabax[i]) < 0) { /* Not a -TAB axis. */ continue; } /* PVi_3a records the 1-relative table axis number. */ m = PVi_3a[itabax] - 1; tabp = wcs->tab + tabidx[itabax]; tabp->map[m] = i; tabp->crval[m] = wcs->crval[i]; } /* Check for completeness. */ for (itab = 0; itab < wcs->ntab; itab++) { for (m = 0; m < wcs->tab[itab].M; m++) { if (wcs->tab[itab].map[m] < 0) { status = wcserr_set(WCSERR_SET(WCSHDRERR_BAD_TABULAR_PARAMS), "Invalid tabular parameters: the axis mapping is undefined"); goto cleanup; } } } /* Set up for reading the arrays; how many arrays are there? */ for (itabax = 0; itabax < ntabax; itabax++) { /* Does this -TAB axis have a non-degenerate index array? */ if (PSi_2a[itabax][0]) { wcs->nwtb++; } } /* Add one coordinate array for each table. */ wcs->nwtb += wcs->ntab; /* Allocate memory for structs to be returned. */ if (!(wcs->wtb = calloc(wcs->nwtb, sizeof(struct wtbarr)))) { wcs->nwtb = 0; status = wcserr_set(WCSHDR_ERRMSG(WCSHDRERR_MEMORY)); goto cleanup; } wcs->m_wtb = wcs->wtb; /* Set pointers for the index and coordinate arrays. */ wtbp = wcs->wtb; for (itab = 0; itab < wcs->ntab; itab++) { getcrd = 1; for (itabax = 0; itabax < ntabax; itabax++) { if (tabidx[itabax] != itab) continue; if (getcrd) { /* Coordinate array. */ wtbp->i = itabax + 1; wtbp->m = PVi_3a[itabax]; wtbp->kind = 'c'; strcpy(wtbp->extnam, PSi_0a[itabax]); wtbp->extver = PVi_1a[itabax]; wtbp->extlev = PVi_2a[itabax]; strcpy(wtbp->ttype, PSi_1a[itabax]); wtbp->row = 1L; wtbp->ndim = wcs->tab[itab].M + 1; wtbp->dimlen = wcs->tab[itab].K; wtbp->arrayp = &(wcs->tab[itab].coord); /* Signal for tabset() to take this memory. */ wcs->tab[itab].m_coord = (double *)0x1; wtbp++; getcrd = 0; } if (PSi_2a[itabax][0]) { /* Index array. */ wtbp->i = itabax + 1; wtbp->m = PVi_3a[itabax]; wtbp->kind = 'i'; m = wtbp->m - 1; strcpy(wtbp->extnam, PSi_0a[itabax]); wtbp->extver = PVi_1a[itabax]; wtbp->extlev = PVi_2a[itabax]; strcpy(wtbp->ttype, PSi_2a[itabax]); wtbp->row = 1L; wtbp->ndim = 1; wtbp->dimlen = wcs->tab[itab].K + m; wtbp->arrayp = wcs->tab[itab].index + m; /* Signal for tabset() to take this memory. */ wcs->tab[itab].m_indxs[m] = (double *)0x1; wtbp++; } } } status = 0; cleanup: if (tabax) free(tabax); if (tabidx) free(tabidx); if (PSi_0a) free(PSi_0a); if (PVi_1a) free(PVi_1a); if (PVi_2a) free(PVi_2a); if (PSi_1a) free(PSi_1a); if (PSi_2a) free(PSi_2a); if (PVi_3a) free(PVi_3a); if (status) { if (wcs->tab) free(wcs->tab); if (wcs->wtb) free(wcs->wtb); } return status; } /*--------------------------------------------------------------------------*/ int wcsidx(int nwcs, struct wcsprm **wcs, int alts[27]) { int a, iwcs; struct wcsprm *wcsp; for (a = 0; a < 27; a++) { alts[a] = -1; } if (wcs == 0x0) { return WCSHDRERR_NULL_POINTER; } wcsp = *wcs; for (iwcs = 0; iwcs < nwcs; iwcs++, wcsp++) { if (wcsp->colnum || wcsp->colax[0]) continue; if (wcsp->alt[0] == ' ') { a = 0; } else { a = wcsp->alt[0] - 'A' + 1; } alts[a] = iwcs; } return 0; } /*--------------------------------------------------------------------------*/ int wcsbdx(int nwcs, struct wcsprm **wcs, int type, short alts[1000][28]) { short *ip; int a, i, icol, iwcs; struct wcsprm *wcsp; for (ip = alts[0]; ip < alts[0] + 28*1000; ip++) { *ip = -1; } for (icol = 0; icol < 1000; icol++) { alts[icol][27] = 0; } if (wcs == 0x0) { return WCSHDRERR_NULL_POINTER; } wcsp = *wcs; for (iwcs = 0; iwcs < nwcs; iwcs++, wcsp++) { if (wcsp->alt[0] == ' ') { a = 0; } else { a = wcsp->alt[0] - 'A' + 1; } if (type) { /* Pixel list. */ if (wcsp->colax[0]) { for (i = 0; i < wcsp->naxis; i++) { alts[wcsp->colax[i]][a] = iwcs; alts[wcsp->colax[i]][27]++; } } else if (!wcsp->colnum) { alts[0][a] = iwcs; alts[0][27]++; } } else { /* Binary table image array. */ if (wcsp->colnum) { alts[wcsp->colnum][a] = iwcs; alts[wcsp->colnum][27]++; } else if (!wcsp->colax[0]) { alts[0][a] = iwcs; alts[0][27]++; } } } return 0; } /*--------------------------------------------------------------------------*/ int wcsvfree(int *nwcs, struct wcsprm **wcs) { int a, status = 0; struct wcsprm *wcsp; if (wcs == 0x0) { return WCSHDRERR_NULL_POINTER; } wcsp = *wcs; for (a = 0; a < *nwcs; a++, wcsp++) { status |= wcsfree(wcsp); } free(*wcs); *nwcs = 0; *wcs = 0x0; return status; } /*--------------------------------------------------------------------------*/ int wcshdo(int relax, struct wcsprm *wcs, int *nkeyrec, char **header) /* ::: CUBEFACE and STOKES handling? */ { static const char *function = "wcshdo"; char alt, comment[72], keyvalue[72], keyword[16], obsg[8] = "OBSG?", obsgeo[8] = "OBSGEO-?", ptype, xtype, xyz[] = "XYZ"; int bintab, col0, *colax, colnum, i, j, k, naxis, pixlist, primage, status = 0; struct wcserr **err; *nkeyrec = 0; *header = 0x0; if (wcs == 0x0) return WCSHDRERR_NULL_POINTER; err = &(wcs->err); if (wcs->flag != WCSSET) { if ((status = wcsset(wcs))) return status; } if ((naxis = wcs->naxis) == 0) { return 0; } /* These are mainly for convenience. */ alt = wcs->alt[0]; if (alt == ' ') alt = '\0'; colnum = wcs->colnum; colax = wcs->colax; primage = 0; bintab = 0; pixlist = 0; if (colnum) { bintab = 1; col0 = colnum; } else if (colax[0]) { pixlist = 1; col0 = colax[0]; } else { primage = 1; } /* WCS dimension. */ if (!pixlist) { sprintf(keyvalue, "%20d", naxis); wcshdo_util(relax, "WCSAXES", "WCAX", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Number of coordinate axes", nkeyrec, header, &status); } /* Reference pixel coordinates. */ for (j = 0; j < naxis; j++) { sprintf(keyvalue, "%20.12G", wcs->crpix[j]); wcshdo_util(relax, "CRPIX", "CRP", WCSHDO_CRPXna, "CRPX", 0, j+1, 0, alt, colnum, colax, keyvalue, "Pixel coordinate of reference point", nkeyrec, header, &status); } /* Linear transformation matrix. */ k = 0; for (i = 0; i < naxis; i++) { for (j = 0; j < naxis; j++, k++) { if (i == j) { if (wcs->pc[k] == 1.0) continue; } else { if (wcs->pc[k] == 0.0) continue; } sprintf(keyvalue, "%20.12G", wcs->pc[k]); wcshdo_util(relax, "PC", bintab ? "PC" : "P", WCSHDO_TPCn_ka, bintab ? 0x0 : "PC", i+1, j+1, 0, alt, colnum, colax, keyvalue, "Coordinate transformation matrix element", nkeyrec, header, &status); } } /* Coordinate increment at reference point. */ for (i = 0; i < naxis; i++) { sprintf(keyvalue, "%20.12G", wcs->cdelt[i]); comment[0] = '\0'; if (wcs->cunit[i][0]) sprintf(comment, "[%s] ", wcs->cunit[i]); strcat(comment, "Coordinate increment at reference point"); wcshdo_util(relax, "CDELT", "CDE", WCSHDO_CRPXna, "CDLT", i+1, 0, 0, alt, colnum, colax, keyvalue, comment, nkeyrec, header, &status); } /* Units of coordinate increment and reference value. */ for (i = 0; i < naxis; i++) { if (wcs->cunit[i][0] == '\0') continue; sprintf(keyvalue, "'%s'", wcs->cunit[i]); wcshdo_util(relax, "CUNIT", "CUN", WCSHDO_CRPXna, "CUNI", i+1, 0, 0, alt, colnum, colax, keyvalue, "Units of coordinate increment and value", nkeyrec, header, &status); } /* Coordinate type. */ for (i = 0; i < naxis; i++) { if (wcs->ctype[i][0] == '\0') continue; sprintf(keyvalue, "'%s'", wcs->ctype[i]); strcpy(comment, "Coordinate type code"); if (i == wcs->lng || i == wcs->lat) { if (strncmp(wcs->ctype[i], "RA--", 4) == 0) { strcpy(comment, "Right ascension, "); } else if (strncmp(wcs->ctype[i], "DEC-", 4) == 0) { strcpy(comment, "Declination, "); } else if (strncmp(wcs->ctype[i]+1, "LON", 3) == 0 || strncmp(wcs->ctype[i]+1, "LAT", 3) == 0) { switch (wcs->ctype[i][0]) { case 'G': strcpy(comment, "galactic "); break; case 'E': strcpy(comment, "ecliptic "); case 'H': strcpy(comment, "helioecliptic "); case 'S': strcpy(comment, "supergalactic "); } if (i == wcs->lng) { strcat(comment, "longitude, "); } else { strcat(comment, "latitude, "); } wcs->ctype[i][0] = toupper(wcs->ctype[i][0]); } strcat(comment, wcs->cel.prj.name); strcat(comment, " projection"); } else if (i == wcs->spec) { spctyp(wcs->ctype[i], 0x0, 0x0, comment, 0x0, &ptype, &xtype, 0x0); if (ptype == xtype) { strcat(comment, " (linear)"); } else { switch (xtype) { case 'F': strcat(comment, " (linear in frequency)"); break; case 'V': strcat(comment, " (linear in velocity)"); break; case 'W': strcat(comment, " (linear in wavelength)"); break; } } } wcshdo_util(relax, "CTYPE", "CTY", WCSHDO_CRPXna, "CTYP", i+1, 0, 0, alt, colnum, colax, keyvalue, comment, nkeyrec, header, &status); } /* Coordinate value at reference point. */ for (i = 0; i < naxis; i++) { sprintf(keyvalue, "%20.12G", wcs->crval[i]); comment[0] = '\0'; if (wcs->cunit[i][0]) sprintf(comment, "[%s] ", wcs->cunit[i]); strcat(comment, "Coordinate value at reference point"); wcshdo_util(relax, "CRVAL", "CRV", WCSHDO_CRPXna, "CRVL", i+1, 0, 0, alt, colnum, colax, keyvalue, comment, nkeyrec, header, &status); } /* Parameter values. */ for (k = 0; k < wcs->npv; k++) { sprintf(keyvalue, "%20.12G", (wcs->pv[k]).value); if ((wcs->pv[k]).i == (wcs->lng + 1)) { switch ((wcs->pv[k]).m) { case 1: strcpy(comment, "[deg] Native longitude of the reference point"); break; case 2: strcpy(comment, "[deg] Native latitude of the reference point"); break; case 3: if (primage) { sprintf(keyword, "LONPOLE%c", alt); } else if (bintab) { sprintf(keyword, "LONP%d%c", colnum, alt); } else { sprintf(keyword, "LONP%d%c", colax[(wcs->pv[k]).i - 1], alt); } sprintf(comment, "[deg] alias for %s (has precedence)", keyword); break; case 4: if (primage) { sprintf(keyword, "LATPOLE%c", alt); } else if (bintab) { sprintf(keyword, "LATP%d%c", colnum, alt); } else { sprintf(keyword, "LATP%d%c", colax[(wcs->pv[k]).i - 1], alt); } sprintf(comment, "[deg] alias for %s (has precedence)", keyword); break; } } else if ((wcs->pv[k]).i == (wcs->lat + 1)) { sprintf(comment, "%s projection parameter", wcs->cel.prj.code); } else { strcpy(comment, "Coordinate transformation parameter"); } wcshdo_util(relax, "PV", "V", WCSHDO_PVn_ma, "PV", wcs->pv[k].i, -1, wcs->pv[k].m, alt, colnum, colax, keyvalue, comment, nkeyrec, header, &status); } for (k = 0; k < wcs->nps; k++) { sprintf(keyvalue, "'%s'", (wcs->ps[k]).value); wcshdo_util(relax, "PS", "S", WCSHDO_PVn_ma, "PS", wcs->ps[k].i, -1, wcs->ps[k].m, alt, colnum, colax, keyvalue, "Coordinate transformation parameter", nkeyrec, header, &status); } /* Celestial and spectral transformation parameters. */ if (!undefined(wcs->lonpole)) { sprintf(keyvalue, "%20.12G", wcs->lonpole); wcshdo_util(relax, "LONPOLE", "LONP", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "[deg] Native longitude of celestial pole", nkeyrec, header, &status); } if (!undefined(wcs->latpole)) { sprintf(keyvalue, "%20.12G", wcs->latpole); wcshdo_util(relax, "LATPOLE", "LATP", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "[deg] Native latitude of celestial pole", nkeyrec, header, &status); } if (!undefined(wcs->restfrq)) { sprintf(keyvalue, "%20.12G", wcs->restfrq); wcshdo_util(relax, "RESTFRQ", "RFRQ", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "[Hz] Line rest frequency", nkeyrec, header, &status); } if (!undefined(wcs->restwav)) { sprintf(keyvalue, "%20.12G", wcs->restwav); wcshdo_util(relax, "RESTWAV", "RWAV", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "[Hz] Line rest wavelength", nkeyrec, header, &status); } /* Coordinate system title. */ if (wcs->wcsname[0]) { sprintf(keyvalue, "'%s'", wcs->wcsname); if (bintab) { wcshdo_util(relax, "WCSNAME", "WCSN", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Coordinate system title", nkeyrec, header, &status); } else { /* TWCS was a mistake. */ wcshdo_util(relax, "WCSNAME", "TWCS", WCSHDO_WCSNna, "WCSN", 0, 0, 0, alt, colnum, colax, keyvalue, "Coordinate system title", nkeyrec, header, &status); } } /* Coordinate axis title. */ if (wcs->cname) { for (i = 0; i < naxis; i++) { if (wcs->cname[i][0] == '\0') continue; sprintf(keyvalue, "'%s'", wcs->cname[i]); wcshdo_util(relax, "CNAME", "CNA", WCSHDO_CNAMna, "CNAM", i+1, 0, 0, alt, colnum, colax, keyvalue, "Axis name for labelling purposes", nkeyrec, header, &status); } } /* Random error in coordinate. */ if (wcs->crder) { for (i = 0; i < naxis; i++) { if (undefined(wcs->crder[i])) continue; sprintf(keyvalue, "%20.12G", wcs->crder[i]); comment[0] = '\0'; if (wcs->cunit[i][0]) sprintf(comment, "[%s] ", wcs->cunit[i]); strcat(comment, "Random error in coordinate"); wcshdo_util(relax, "CRDER", "CRD", WCSHDO_CNAMna, "CRDE", i+1, 0, 0, alt, colnum, colax, keyvalue, comment, nkeyrec, header, &status); } } /* Systematic error in coordinate. */ if (wcs->csyer) { for (i = 0; i < naxis; i++) { if (undefined(wcs->csyer[i])) continue; sprintf(keyvalue, "%20.12G", wcs->csyer[i]); comment[0] = '\0'; if (wcs->cunit[i][0]) sprintf(comment, "[%s] ", wcs->cunit[i]); strcat(comment, "Systematic error in coordinate"); wcshdo_util(relax, "CSYER", "CSY", WCSHDO_CNAMna, "CSYE", i+1, 0, 0, alt, colnum, colax, keyvalue, comment, nkeyrec, header, &status); } } /* Equatorial coordinate system type. */ if (wcs->radesys[0]) { sprintf(keyvalue, "'%s'", wcs->radesys); wcshdo_util(relax, "RADESYS", "RADE", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Equatorial coordinate system", nkeyrec, header, &status); } /* Equinox of equatorial coordinate system. */ if (!undefined(wcs->equinox)) { sprintf(keyvalue, "%20.12G", wcs->equinox); wcshdo_util(relax, "EQUINOX", "EQUI", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "[yr] Equinox of equatorial coordinates", nkeyrec, header, &status); } /* Reference frame of spectral coordinates. */ if (wcs->specsys[0]) { sprintf(keyvalue, "'%s'", wcs->specsys); wcshdo_util(relax, "SPECSYS", "SPEC", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Reference frame of spectral coordinates", nkeyrec, header, &status); } /* Reference frame of spectral observation. */ if (wcs->ssysobs[0]) { sprintf(keyvalue, "'%s'", wcs->ssysobs); wcshdo_util(relax, "SSYSOBS", "SOBS", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Reference frame of spectral observation", nkeyrec, header, &status); } /* Observer's velocity towards source. */ if (!undefined(wcs->velosys)) { sprintf(keyvalue, "%20.12G", wcs->velosys); wcshdo_util(relax, "VELOSYS", "VSYS", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "[m/s] Velocity towards source", nkeyrec, header, &status); } /* Reference frame of source redshift. */ if (wcs->ssyssrc[0]) { sprintf(keyvalue, "'%s'", wcs->ssyssrc); wcshdo_util(relax, "SSYSSRC", "SSRC", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Reference frame of source redshift", nkeyrec, header, &status); } /* Redshift of the source. */ if (!undefined(wcs->zsource)) { sprintf(keyvalue, "%20.12G", wcs->zsource); wcshdo_util(relax, "ZSOURCE", "ZSOU", 0, 0x0, 0, 0, 0, alt, colnum, colax, keyvalue, "Redshift of the source", nkeyrec, header, &status); } /* Observatory coordinates. */ for (k = 0; k < 3; k++) { if (undefined(wcs->obsgeo[k])) continue; sprintf(keyvalue, "%20.12G", wcs->obsgeo[k]); sprintf(comment, "[m] ITRF observatory %c-coordinate", xyz[k]); obsgeo[7] = xyz[k]; obsg[4] = xyz[k]; wcshdo_util(relax, obsgeo, obsg, 0, 0x0, 0, 0, 0, ' ', colnum, colax, keyvalue, comment, nkeyrec, header, &status); } /* MJD of observation. */ if (!undefined(wcs->mjdobs)) { sprintf(keyvalue, "%20.12G", wcs->mjdobs); strcpy(comment, "[d] MJD of observation"); if (wcs->dateobs[0]) { if (primage || (relax & 1) == 0) { sprintf(comment+22, " matching DATE-OBS"); } else { sprintf(comment+22, " matching DOBS%d", col0); } } wcshdo_util(relax, "MJD-OBS", "MJDOB", 0, 0x0, 0, 0, 0, ' ', colnum, colax, keyvalue, comment, nkeyrec, header, &status); } /* MJD mid-observation time. */ if (!undefined(wcs->mjdavg)) { sprintf(keyvalue, "%20.12G", wcs->mjdavg); strcpy(comment, "[d] MJD mid-observation"); if (wcs->dateavg[0]) { if (primage) { sprintf(comment+23, " matching DATE-AVG"); } else { sprintf(comment+23, " matching DAVG%d", col0); } } wcshdo_util(relax, "MJD-AVG", "MJDA", 0, 0x0, 0, 0, 0, ' ', colnum, colax, keyvalue, comment, nkeyrec, header, &status); } /* ISO-8601 date corresponding to MJD-OBS. */ if (wcs->dateobs[0]) { sprintf(keyvalue, "'%s'", wcs->dateobs); strcpy(comment, "ISO-8601 observation date"); if (!undefined(wcs->mjdobs)) { if (primage) { sprintf(comment+25, " matching MJD-OBS"); } else { sprintf(comment+25, " matching MJDOB%d", col0); } } if (relax & 1) { /* Allow DOBSn. */ wcshdo_util(relax, "DATE-OBS", "DOBS", WCSHDO_DOBSn, 0x0, 0, 0, 0, ' ', colnum, colax, keyvalue, comment, nkeyrec, header, &status); } else { /* Force DATE-OBS. */ wcshdo_util(relax, "DATE-OBS", 0x0, 0, 0x0, 0, 0, 0, ' ', 0, 0x0, keyvalue, comment, nkeyrec, header, &status); } } /* ISO-8601 date corresponding to MJD-OBS. */ if (wcs->dateavg[0]) { sprintf(keyvalue, "'%s'", wcs->dateavg); strcpy(comment, "ISO-8601 mid-observation date"); if (!undefined(wcs->mjdavg)) { if (primage) { sprintf(comment+29, " matching MJD-AVG"); } else { sprintf(comment+29, " matching MJDA%d", col0); } } wcshdo_util(relax, "DATE-AVG", "DAVG", 0, 0x0, 0, 0, 0, ' ', colnum, colax, keyvalue, comment, nkeyrec, header, &status); } if (status == WCSHDRERR_MEMORY) { wcserr_set(WCSHDR_ERRMSG(status)); } return status; } /*--------------------------------------------------------------------------*/ void wcshdo_util( int relax, const char pikey[], const char tbkey[], int level, const char tlkey[], int i, int j, int m, char alt, int btcol, int plcol[], char keyvalue[], const char keycomment[], int *nkeyrec, char **header, int *status) { char ch0, ch1, *hptr, keyword[16], *kptr; int nbyte, nc = 47, nv; if (*status) return; /* Reallocate memory in blocks of 2880 bytes. */ if ((*nkeyrec)%32 == 0) { nbyte = ((*nkeyrec)/32 + 1) * 2880; if (!(hptr = realloc(*header, nbyte))) { *status = WCSHDRERR_MEMORY; return; } *header = hptr; } /* Construct the keyword. */ if (alt == ' ') alt = '\0'; if (btcol) { /* Binary table image array. */ if (i > 0 && j) { if (j > 0) { sprintf(keyword, "%d%d%s%d%c", i, j, tbkey, btcol, alt); } else { sprintf(keyword, "%d%s%d_%d%c", i, tbkey, btcol, m, alt); } } else if (i > 0) { sprintf(keyword, "%d%s%d%c", i, tbkey, btcol, alt); } else if (j > 0) { sprintf(keyword, "%d%s%d%c", j, tbkey, btcol, alt); } else { sprintf(keyword, "%s%d%c", tbkey, btcol, alt); } if ((strlen(keyword) < 8) && tlkey && (relax & level)) { /* Use the long form. */ if (i > 0 && j) { if (j > 0) { sprintf(keyword, "%d%d%s%d%c", i, j, tlkey, btcol, alt); } else { sprintf(keyword, "%d%s%d_%d%c", i, tlkey, btcol, m, alt); } } else if (i > 0) { sprintf(keyword, "%d%s%d%c", i, tlkey, btcol, alt); } else if (j > 0) { sprintf(keyword, "%d%s%d%c", j, tlkey, btcol, alt); } else { sprintf(keyword, "%s%d%c", tlkey, btcol, alt); } } } else if (plcol && plcol[0]) { /* Pixel list. */ if (i > 0 && j) { if (j > 0) { sprintf(keyword, "T%s%d_%d%c", tbkey, plcol[i-1], plcol[j-1], alt); } else { sprintf(keyword, "T%s%d_%d%c", tbkey, plcol[i-1], m, alt); } } else if (i > 0) { sprintf(keyword, "T%s%d%c", tbkey, plcol[i-1], alt); } else if (j > 0) { sprintf(keyword, "T%s%d%c", tbkey, plcol[j-1], alt); } else { sprintf(keyword, "%s%d%c", tbkey, plcol[0], alt); } if ((strlen(keyword) < 8) && tlkey && (relax & level)) { /* Use the long form. */ if (i > 0 && j) { if (j > 0) { sprintf(keyword, "T%s%d_%d%c", tlkey, plcol[i-1], plcol[j-1], alt); } else { sprintf(keyword, "T%s%d_%d%c", tlkey, plcol[i-1], m, alt); } } else if (i > 0) { sprintf(keyword, "T%s%d%c", tlkey, plcol[i-1], alt); } else if (j > 0) { sprintf(keyword, "T%s%d%c", tlkey, plcol[j-1], alt); } else { sprintf(keyword, "%s%d%c", tlkey, plcol[0], alt); } } } else { if (i > 0 && j) { if (j > 0) { sprintf(keyword, "%s%d_%d%c", pikey, i, j, alt); } else { sprintf(keyword, "%s%d_%d%c", pikey, i, m, alt); } } else if (i > 0) { sprintf(keyword, "%s%d%c", pikey, i, alt); } else if (j > 0) { sprintf(keyword, "%s%d%c", pikey, j, alt); } else { sprintf(keyword, "%s%c", pikey, alt); } } /* Double-up single-quotes in the keyvalue. */ hptr = keyvalue + 1; while (*hptr) { if (*hptr == '\'') { kptr = hptr++; if (*hptr) { ch0 = *kptr; while (*kptr) { ch1 = *(++kptr); *kptr = ch0; ch0 = ch1; } } } hptr++; } if ((nv = strlen(keyvalue) > 20)) { /* Rob the keycomment to make space for the keyvalue. */ nc -= (nv - 20); } hptr = *header + (80 * ((*nkeyrec)++)); sprintf(hptr, "%-8.8s= %-20s / %-*.*s", keyword, keyvalue, nc, nc, keycomment); } pywcs-1.12/wcslib/C/wcshdr.h0000644001153600020070000015021612310355626017763 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcshdr.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * "Representations of celestial coordinates in FITS", * Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077 (Paper II) * * "Representations of spectral coordinates in FITS", * Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. * 2006, A&A, 446, 747 (Paper III) * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the wcshdr routines * ------------------------------ * Routines in this suite are aimed at extracting WCS information from a FITS * file. They provide the high-level interface between the FITS file and the * WCS coordinate transformation routines. * * Additionally, function wcshdo() is provided to write out the contents of a * wcsprm struct as a FITS header. * * Briefly, the anticipated sequence of operations is as follows: * * - 1: Open the FITS file and read the image or binary table header, e.g. * using CFITSIO routine fits_hdr2str(). * * - 2: Parse the header using wcspih() or wcsbth(); they will automatically * interpret 'TAB' header keywords using wcstab(). * * - 3: Allocate memory for, and read 'TAB' arrays from the binary table * extension, e.g. using CFITSIO routine fits_read_wcstab() - refer to * the prologue of getwcstab.h. wcsset() will automatically take * control of this allocated memory, in particular causing it to be * free'd by wcsfree(). * * - 4: Translate non-standard WCS usage using wcsfix(), see wcsfix.h. * * - 5: Initialize wcsprm struct(s) using wcsset() and calculate coordinates * using wcsp2s() and/or wcss2p(). Refer to the prologue of wcs.h for a * description of these and other high-level WCS coordinate * transformation routines. * * - 6: Clean up by freeing memory with wcsvfree(). * * In detail: * * - wcspih() is a high-level FITS WCS routine that parses an image header. It * returns an array of up to 27 wcsprm structs on each of which it invokes * wcstab(). * * - wcsbth() is the analogue of wcspih() for use with binary tables; it * handles image array and pixel list keywords. As an extension of the FITS * WCS standard, it also recognizes image header keywords which may be used * to provide default values via an inheritance mechanism. * * - wcstab() assists in filling in members of the wcsprm struct associated * with coordinate lookup tables ('TAB'). These are based on arrays stored * in a FITS binary table extension (BINTABLE) that are located by PVi_ma * keywords in the image header. * * - wcsidx() and wcsbdx() are utility routines that return the index for a * specified alternate coordinate descriptor in the array of wcsprm structs * returned by wcspih() or wcsbth(). * * - wcsvfree() deallocates memory for an array of wcsprm structs, such as * returned by wcspih() or wcsbth(). * * - wcshdo() writes out a wcsprm struct as a FITS header. * * * wcspih() - FITS WCS parser routine for image headers * ---------------------------------------------------- * wcspih() is a high-level FITS WCS routine that parses an image header, * either that of a primary HDU or of an image extension. All WCS keywords * defined in Papers I, II, and III are recognized, and also those used by the * AIPS convention and certain other keywords that existed in early drafts of * the WCS papers as explained in wcsbth() note 5. * * Given a character array containing a FITS image header, wcspih() identifies * and reads all WCS keywords for the primary coordinate representation and up * to 26 alternate representations. It returns this information as an array of * wcsprm structs. * * wcspih() invokes wcstab() on each of the wcsprm structs that it returns. * * Use wcsbth() in preference to wcspih() for FITS headers of unknown type; * wcsbth() can parse image headers as well as binary table and pixel list * headers. * * Given and returned: * header char[] Character array containing the (entire) FITS image * header from which to identify and construct the * coordinate representations, for example, as might be * obtained conveniently via the CFITSIO routine * fits_hdr2str(). * * Each header "keyrecord" (formerly "card image") * consists of exactly 80 7-bit ASCII printing characters * in the range 0x20 to 0x7e (which excludes NUL, BS, * TAB, LF, FF and CR) especially noting that the * keyrecords are NOT null-terminated. * * For negative values of ctrl (see below), header[] is * modified so that WCS keyrecords processed by wcspih() * are removed from it. * * Given: * nkeyrec int Number of keyrecords in header[]. * * relax int Degree of permissiveness: * 0: Recognize only FITS keywords defined by the * published WCS standard. * WCSHDR_all: Admit all recognized informal * extensions of the WCS standard. * Fine-grained control of the degree of permissiveness * is also possible as explained in wcsbth() note 5. * * ctrl int Error reporting and other control options for invalid * WCS and other header keyrecords: * 0: Do not report any rejected header keyrecords. * 1: Produce a one-line message stating the number * of WCS keyrecords rejected (nreject). * 2: Report each rejected keyrecord and the reason * why it was rejected. * 3: As above, but also report all non-WCS * keyrecords that were discarded, and the number * of coordinate representations (nwcs) found. * The report is written to stderr. * * For ctrl < 0, WCS keyrecords processed by wcspih() * are removed from header[]: * -1: Remove only valid WCS keyrecords whose values * were successfully extracted, nothing is * reported. * -2: Also remove WCS keyrecords that were rejected, * reporting each one and the reason that it was * rejected. * -3: As above, and also report the number of * coordinate representations (nwcs) found. * -11: Same as -1 but preserving the basic keywords * '{DATE,MJD}-{OBS,AVG}' and 'OBSGEO-{X,Y,Z}'. * If any keyrecords are removed from header[] it will * be null-terminated (NUL not being a legal FITS header * character), otherwise it will contain its original * complement of nkeyrec keyrecords and possibly not be * null-terminated. * * Returned: * nreject int* Number of WCS keywords rejected for syntax errors, * illegal values, etc. Keywords not recognized as WCS * keywords are simply ignored. Refer also to wcsbth() * note 5. * * nwcs int* Number of coordinate representations found. * * wcs struct wcsprm** * Pointer to an array of wcsprm structs containing up to * 27 coordinate representations. * * Memory for the array is allocated by wcspih() which * also invokes wcsini() for each struct to allocate * memory for internal arrays and initialize their * members to default values. Refer also to wcsbth() * note 8. Note that wcsset() is not invoked on these * structs. * * This allocated memory must be freed by the user, first * by invoking wcsfree() for each struct, and then by * freeing the array itself. A routine, wcsvfree(), is * provided to do this (see below). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 4: Fatal error returned by Flex parser. * * Notes: * Refer to wcsbth() notes 1, 2, 3, 5, 7, and 8. * * * wcsbth() - FITS WCS parser routine for binary table and image headers * --------------------------------------------------------------------- * wcsbth() is a high-level FITS WCS routine that parses a binary table header. * It handles image array and pixel list WCS keywords which may be present * together in one header. * * As an extension of the FITS WCS standard, wcsbth() also recognizes image * header keywords in a binary table header. These may be used to provide * default values via an inheritance mechanism discussed in note 5 (c.f. * WCSHDR_AUXIMG and WCSHDR_ALLIMG), or may instead result in wcsprm structs * that are not associated with any particular column. Thus wcsbth() can * handle primary image and image extension headers in addition to binary table * headers (it ignores NAXIS and does not rely on the presence of the TFIELDS * keyword). * * All WCS keywords defined in Papers I, II, and III are recognized, and also * those used by the AIPS convention and certain other keywords that existed in * early drafts of the WCS papers as explained in note 5 below. * * wcsbth() sets the colnum or colax[] members of the wcsprm structs that it * returns with the column number of an image array or the column numbers * associated with each pixel coordinate element in a pixel list. wcsprm * structs that are not associated with any particular column, as may be * derived from image header keywords, have colnum == 0. * * Note 6 below discusses the number of wcsprm structs returned by wcsbth(), * and the circumstances in which image header keywords cause a struct to be * created. See also note 9 concerning the number of separate images that may * be stored in a pixel list. * * The API to wcsbth() is similar to that of wcspih() except for the addition * of extra arguments that may be used to restrict its operation. Like * wcspih(), wcsbth() invokes wcstab() on each of the wcsprm structs that it * returns. * * Given and returned: * header char[] Character array containing the (entire) FITS binary * table, primary image, or image extension header from * which to identify and construct the coordinate * representations, for example, as might be obtained * conveniently via the CFITSIO routine fits_hdr2str(). * * Each header "keyrecord" (formerly "card image") * consists of exactly 80 7-bit ASCII printing * characters in the range 0x20 to 0x7e (which excludes * NUL, BS, TAB, LF, FF and CR) especially noting that * the keyrecords are NOT null-terminated. * * For negative values of ctrl (see below), header[] is * modified so that WCS keyrecords processed by wcsbth() * are removed from it. * * Given: * nkeyrec int Number of keyrecords in header[]. * * relax int Degree of permissiveness: * 0: Recognize only FITS keywords defined by the * published WCS standard. * WCSHDR_all: Admit all recognized informal * extensions of the WCS standard. * Fine-grained control of the degree of permissiveness * is also possible, as explained in note 5 below. * * ctrl int Error reporting and other control options for invalid * WCS and other header keyrecords: * 0: Do not report any rejected header keyrecords. * 1: Produce a one-line message stating the number * of WCS keyrecords rejected (nreject). * 2: Report each rejected keyrecord and the reason * why it was rejected. * 3: As above, but also report all non-WCS * keyrecords that were discarded, and the number * of coordinate representations (nwcs) found. * The report is written to stderr. * * For ctrl < 0, WCS keyrecords processed by wcsbth() * are removed from header[]: * -1: Remove only valid WCS keyrecords whose values * were successfully extracted, nothing is * reported. * -2: Also remove WCS keyrecords that were rejected, * reporting each one and the reason that it was * rejected. * -3: As above, and also report the number of * coordinate representations (nwcs) found. * -11: Same as -1 but preserving the basic keywords * '{DATE,MJD}-{OBS,AVG}' and 'OBSGEO-{X,Y,Z}'. * If any keyrecords are removed from header[] it will * be null-terminated (NUL not being a legal FITS header * character), otherwise it will contain its original * complement of nkeyrec keyrecords and possibly not be * null-terminated. * * keysel int Vector of flag bits that may be used to restrict the * keyword types considered: * WCSHDR_IMGHEAD: Image header keywords. * WCSHDR_BIMGARR: Binary table image array. * WCSHDR_PIXLIST: Pixel list keywords. * If zero, there is no restriction. * * Keywords such as EQUIna or RFRQna that are common to * binary table image arrays and pixel lists (including * WCSNna and TWCSna, as explained in note 4 below) are * selected by both WCSHDR_BIMGARR and WCSHDR_PIXLIST. * Thus if inheritance via WCSHDR_ALLIMG is enabled as * discussed in note 5 and one of these shared keywords * is present, then WCSHDR_IMGHEAD and WCSHDR_PIXLIST * alone may be sufficient to cause the construction of * coordinate descriptions for binary table image arrays. * * colsel int* Pointer to an array of table column numbers used to * restrict the keywords considered by wcsbth(). * * A null pointer may be specified to indicate that there * is no restriction. Otherwise, the magnitude of * cols[0] specifies the length of the array: * cols[0] > 0: the columns are included, * cols[0] < 0: the columns are excluded. * * For the pixel list keywords TPn_ka and TCn_ka (and * TPCn_ka and TCDn_ka if WCSHDR_LONGKEY is enabled), it * is an error for one column to be selected but not the * other. This is unlike the situation with invalid * keyrecords, which are simply rejected, because the * error is not intrinsic to the header itself but * arises in the way that it is processed. * * Returned: * nreject int* Number of WCS keywords rejected for syntax errors, * illegal values, etc. Keywords not recognized as WCS * keywords are simply ignored, refer also to note 5 * below. * * nwcs int* Number of coordinate representations found. * * wcs struct wcsprm** * Pointer to an array of wcsprm structs containing up * to 27027 coordinate representations, refer to note 6 * below. * * Memory for the array is allocated by wcsbth() which * also invokes wcsini() for each struct to allocate * memory for internal arrays and initialize their * members to default values. Refer also to note 8 * below. Note that wcsset() is not invoked on these * structs. * * This allocated memory must be freed by the user, first * by invoking wcsfree() for each struct, and then by * freeing the array itself. A routine, wcsvfree(), is * provided to do this (see below). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Invalid column selection. * 4: Fatal error returned by Flex parser. * * Notes: * 1: wcspih() determines the number of coordinate axes independently for * each alternate coordinate representation (denoted by the "a" value in * keywords like CTYPEia) from the higher of * * a: NAXIS, * b: WCSAXESa, * c: The highest axis number in any parameterized WCS keyword. The * keyvalue, as well as the keyword, must be syntactically valid * otherwise it will not be considered. * * If none of these keyword types is present, i.e. if the header only * contains auxiliary WCS keywords for a particular coordinate * representation, then no coordinate description is constructed for it. * * wcsbth() is similar except that it ignores the NAXIS keyword if given * an image header to process. * * The number of axes, which is returned as a member of the wcsprm * struct, may differ for different coordinate representations of the * same image. * * 2: wcspih() and wcsbth() enforce correct FITS "keyword = value" syntax * with regard to "= " occurring in columns 9 and 10. * * However, they do recognize free-format character (NOST 100-2.0, * Sect. 5.2.1), integer (Sect. 5.2.3), and floating-point values * (Sect. 5.2.4) for all keywords. * * 3: Where CROTAn, CDi_ja, and PCi_ja occur together in one header wcspih() * and wcsbth() treat them as described in the prologue to wcs.h. * * 4: WCS Paper I mistakenly defined the pixel list form of WCSNAMEa as * TWCSna instead of WCSNna; the 'T' is meant to substitute for the axis * number in the binary table form of the keyword - note that keywords * defined in WCS Papers II and III that are not parameterised by axis * number have identical forms for binary tables and pixel lists. * Consequently wcsbth() always treats WCSNna and TWCSna as equivalent. * * 5: wcspih() and wcsbth() interpret the "relax" argument as a vector of * flag bits to provide fine-grained control over what non-standard WCS * keywords to accept. The flag bits are subject to change in future and * should be set by using the preprocessor macros (see below) for the * purpose. * * - WCSHDR_none: Don't accept any extensions (not even those in the * errata). Treat non-conformant keywords in the same way as * non-WCS keywords in the header, i.e. simply ignore them. * * - WCSHDR_all: Accept all extensions recognized by the parser. * * - WCSHDR_reject: Reject non-standard keywords (that are not otherwise * accepted). A message will optionally be printed on stderr, as * determined by the ctrl argument, and nreject will be * incremented. * * This flag may be used to signal the presence of non-standard * keywords, otherwise they are simply passed over as though they * did not exist in the header. * * Useful for testing conformance of a FITS header to the WCS * standard. * * - WCSHDR_CROTAia: Accept CROTAia (wcspih()), * iCROTna (wcsbth()), * TCROTna (wcsbth()). * - WCSHDR_EPOCHa: Accept EPOCHa. * - WCSHDR_VELREFa: Accept VELREFa. * wcspih() always recognizes the AIPS-convention keywords, * CROTAn, EPOCH, and VELREF for the primary representation * (a = ' ') but alternates are non-standard. * * wcsbth() accepts EPOCHa and VELREFa only if WCSHDR_AUXIMG is * also enabled. * * - WCSHDR_CD00i00j: Accept CD00i00j (wcspih()). * - WCSHDR_PC00i00j: Accept PC00i00j (wcspih()). * - WCSHDR_PROJPn: Accept PROJPn (wcspih()). * These appeared in early drafts of WCS Paper I+II (before they * were split) and are equivalent to CDi_ja, PCi_ja, and PVi_ma * for the primary representation (a = ' '). PROJPn is * equivalent to PVi_ma with m = n <= 9, and is associated * exclusively with the latitude axis. * * - WCSHDR_RADECSYS: Accept RADECSYS. This appeared in early drafts of * WCS Paper I+II and was subsequently replaced by RADESYSa. * * wcsbth() accepts RADECSYS only if WCSHDR_AUXIMG is also * enabled. * * - WCSHDR_VSOURCE: Accept VSOURCEa or VSOUna (wcsbth()). This appeared * in early drafts of WCS Paper III and was subsequently dropped * in favour of ZSOURCEa and ZSOUna. * * wcsbth() accepts VSOURCEa only if WCSHDR_AUXIMG is also * enabled. * * - WCSHDR_DOBSn (wcsbth() only): Allow DOBSn, the column-specific analogue * of DATE-OBS. By an oversight this was never formally defined * in the standard. * * - WCSHDR_LONGKEY (wcsbth() only): Accept long forms of the alternate * binary table and pixel list WCS keywords, i.e. with "a" non- * blank. Specifically * # jCRPXna TCRPXna : jCRPXn jCRPna TCRPXn TCRPna CRPIXja # - TPCn_ka : - ijPCna - TPn_ka PCi_ja # - TCDn_ka : - ijCDna - TCn_ka CDi_ja # iCDLTna TCDLTna : iCDLTn iCDEna TCDLTn TCDEna CDELTia # iCUNIna TCUNIna : iCUNIn iCUNna TCUNIn TCUNna CUNITia # iCTYPna TCTYPna : iCTYPn iCTYna TCTYPn TCTYna CTYPEia # iCRVLna TCRVLna : iCRVLn iCRVna TCRVLn TCRVna CRVALia # iPVn_ma TPVn_ma : - iVn_ma - TVn_ma PVi_ma # iPSn_ma TPSn_ma : - iSn_ma - TSn_ma PSi_ma * * where the primary and standard alternate forms together with * the image-header equivalent are shown rightwards of the colon. * * The long form of these keywords could be described as quasi- * standard. TPCn_ka, iPVn_ma, and TPVn_ma appeared by mistake * in the examples in WCS Paper II and subsequently these and * also TCDn_ka, iPSn_ma and TPSn_ma were legitimized by the * errata to the WCS papers. * * Strictly speaking, the other long forms are non-standard and * in fact have never appeared in any draft of the WCS papers nor * in the errata. However, as natural extensions of the primary * form they are unlikely to be written with any other intention. * Thus it should be safe to accept them provided, of course, * that the resulting keyword does not exceed the 8-character * limit. * * If WCSHDR_CNAMn is enabled then also accept * # iCNAMna TCNAMna : --- iCNAna --- TCNAna CNAMEia # iCRDEna TCRDEna : --- iCRDna --- TCRDna CRDERia # iCSYEna TCSYEna : --- iCSYna --- TCSYna CSYERia * * Note that CNAMEia, CRDERia, CSYERia, and their variants are * not used by WCSLIB but are stored in the wcsprm struct as * auxiliary information. * * - WCSHDR_CNAMn (wcsbth() only): Accept iCNAMn, iCRDEn, iCSYEn, TCNAMn, * TCRDEn, and TCSYEn, i.e. with "a" blank. While non-standard, * these are the obvious analogues of iCTYPn, TCTYPn, etc. * * - WCSHDR_AUXIMG (wcsbth() only): Allow the image-header form of an * auxiliary WCS keyword with representation-wide scope to * provide a default value for all images. This default may be * overridden by the column-specific form of the keyword. * * For example, a keyword like EQUINOXa would apply to all image * arrays in a binary table, or all pixel list columns with * alternate representation "a" unless overridden by EQUIna. * * Specifically the keywords are: * # LATPOLEa for LATPna # LONPOLEa for LONPna # RESTFREQ for RFRQna # RESTFRQa for RFRQna # RESTWAVa for RWAVna * * whose keyvalues are actually used by WCSLIB, and also keywords * that provide auxiliary information that is simply stored in * the wcsprm struct: * # EPOCH - ... (No column-specific form.) # EPOCHa - ... Only if WCSHDR_EPOCHa is set. # EQUINOXa for EQUIna # RADESYSa for RADEna # RADECSYS for RADEna ... Only if WCSHDR_RADECSYS is set. # SPECSYSa for SPECna # SSYSOBSa for SOBSna # SSYSSRCa for SSRCna # VELOSYSa for VSYSna # VELANGLa for VANGna # VELREF - ... (No column-specific form.) # VELREFa - ... Only if WCSHDR_VELREFa is set. # VSOURCEa for VSOUna ... Only if WCSHDR_VSOURCE is set. # WCSNAMEa for WCSNna ... Or TWCSna (see below). # ZSOURCEa for ZSOUna * # DATE-AVG for DAVGn # DATE-OBS for DOBSn # MJD-AVG for MJDAn # MJD-OBS for MJDOBn # OBSGEO-X for OBSGXn # OBSGEO-Y for OBSGYn # OBSGEO-Z for OBSGZn * * where the image-header keywords on the left provide default * values for the column specific keywords on the right. * * Keywords in the last group, such as MJD-OBS, apply to all * alternate representations, so MJD-OBS would provide a default * value for all images in the header. * * This auxiliary inheritance mechanism applies to binary table * image arrays and pixel lists alike. Most of these keywords * have no default value, the exceptions being LONPOLEa and * LATPOLEa, and also RADESYSa and EQUINOXa which provide * defaults for each other. Thus the only potential difficulty * in using WCSHDR_AUXIMG is that of erroneously inheriting one * of these four keywords. * * Unlike WCSHDR_ALLIMG, the existence of one (or all) of these * auxiliary WCS image header keywords will not by itself cause a * wcsprm struct to be created for alternate representation "a". * This is because they do not provide sufficient information to * create a non-trivial coordinate representation when used in * conjunction with the default values of those keywords, such as * CTYPEia, that are parameterized by axis number. * * - WCSHDR_ALLIMG (wcsbth() only): Allow the image-header form of *all* * image header WCS keywords to provide a default value for all * image arrays in a binary table (n.b. not pixel list). This * default may be overridden by the column-specific form of the * keyword. * * For example, a keyword like CRPIXja would apply to all image * arrays in a binary table with alternate representation "a" * unless overridden by jCRPna. * * Specifically the keywords are those listed above for * WCSHDR_AUXIMG plus * # WCSAXESa for WCAXna * * which defines the coordinate dimensionality, and the following * keywords which are parameterized by axis number: * # CRPIXja for jCRPna # PCi_ja for ijPCna # CDi_ja for ijCDna # CDELTia for iCDEna # CROTAi for iCROTn # CROTAia - ... Only if WCSHDR_CROTAia is set. # CUNITia for iCUNna # CTYPEia for iCTYna # CRVALia for iCRVna # PVi_ma for iVn_ma # PSi_ma for iSn_ma * # CNAMEia for iCNAna # CRDERia for iCRDna # CSYERia for iCSYna * * where the image-header keywords on the left provide default * values for the column specific keywords on the right. * * This full inheritance mechanism only applies to binary table * image arrays, not pixel lists, because in the latter case * there is no well-defined association between coordinate axis * number and column number. * * Note that CNAMEia, CRDERia, CSYERia, and their variants are * not used by WCSLIB but are stored in the wcsprm struct as * auxiliary information. * * Note especially that at least one wcsprm struct will be * returned for each "a" found in one of the image header * keywords listed above: * * - If the image header keywords for "a" ARE NOT inherited by a * binary table, then the struct will not be associated with * any particular table column number and it is up to the user * to provide an association. * * - If the image header keywords for "a" ARE inherited by a * binary table image array, then those keywords are considered * to be "exhausted" and do not result in a separate wcsprm * struct. * * For example, to accept CD00i00j and PC00i00j and reject all other * extensions, use * = relax = WCSHDR_reject | WCSHDR_CD00i00j | WCSHDR_PC00i00j; * * The parser always treats EPOCH as subordinate to EQUINOXa if both are * present, and VSOURCEa is always subordinate to ZSOURCEa. * * Likewise, VELREF is subordinate to the formalism of WCS Paper III, see * spcaips(). * * Neither wcspih() nor wcsbth() currently recognize the AIPS-convention * keywords ALTRPIX or ALTRVAL which effectively define an alternative * representation for a spectral axis. * * 6: Depending on what flags have been set in its "relax" argument, * wcsbth() could return as many as 27027 wcsprm structs: * * - Up to 27 unattached representations derived from image header * keywords. * * - Up to 27 structs for each of up to 999 columns containing an image * arrays. * * - Up to 27 structs for a pixel list. * * Note that it is considered legitimate for a column to contain an image * array and also form part of a pixel list, and in particular that * wcsbth() does not check the TFORM keyword for a pixel list column to * check that it is scalar. * * In practice, of course, a realistic binary table header is unlikely to * contain more than a handful of images. * * In order for wcsbth() to create a wcsprm struct for a particular * coordinate representation, at least one WCS keyword that defines an * axis number must be present, either directly or by inheritance if * WCSHDR_ALLIMG is set. * * When the image header keywords for an alternate representation are * inherited by a binary table image array via WCSHDR_ALLIMG, those * keywords are considered to be "exhausted" and do not result in a * separate wcsprm struct. Otherwise they do. * * 7: Neither wcspih() nor wcsbth() check for duplicated keywords, in most * cases they accept the last encountered. * * 8: wcspih() and wcsbth() use wcsnpv() and wcsnps() (refer to the prologue * of wcs.h) to match the size of the pv[] and ps[] arrays in the wcsprm * structs to the number in the header. Consequently there are no unused * elements in the pv[] and ps[] arrays, indeed they will often be of * zero length. * * 9: The FITS WCS standard for pixel lists assumes that a pixel list * defines one and only one image, i.e. that each row of the binary table * refers to just one event, e.g. the detection of a single photon or * neutrino. * * In the absence of a formal mechanism for identifying the columns * containing pixel coordinates (as opposed to pixel values or ancillary * data recorded at the time the photon or neutrino was detected), * Paper I discusses how the WCS keywords themselves may be used to * identify them. * * In practice, however, pixel lists have been used to store multiple * images. Besides not specifying how to identify columns, the pixel * list convention is also silent on the method to be used to associate * table columns with image axes. * * wcsbth() simply collects all WCS keywords for a particular coordinate * representation (i.e. the "a" value in TCTYna) into one wcsprm struct. * However, these alternates need not be associated with the same table * columns and this allows a pixel list to contain up to 27 separate * images. As usual, if one of these representations happened to contain * more than two celestial axes, for example, then an error would result * when wcsset() is invoked on it. In this case the "colsel" argument * could be used to restrict the columns used to construct the * representation so that it only contained one pair of celestial axes. * * * wcstab() - Tabular construction routine * --------------------------------------- * wcstab() assists in filling in the information in the wcsprm struct relating * to coordinate lookup tables. * * Tabular coordinates ('TAB') present certain difficulties in that the main * components of the lookup table - the multidimensional coordinate array plus * an index vector for each dimension - are stored in a FITS binary table * extension (BINTABLE). Information required to locate these arrays is stored * in PVi_ma and PSi_ma keywords in the image header. * * wcstab() parses the PVi_ma and PSi_ma keywords associated with each 'TAB' * axis and allocates memory in the wcsprm struct for the required number of * tabprm structs. It sets as much of the tabprm struct as can be gleaned from * the image header, and also sets up an array of wtbarr structs (described in * the prologue of wcs.h) to assist in extracting the required arrays from the * BINTABLE extension(s). * * It is then up to the user to allocate memory for, and copy arrays from the * BINTABLE extension(s) into the tabprm structs. A CFITSIO routine, * fits_read_wcstab(), has been provided for this purpose, see getwcstab.h. * wcsset() will automatically take control of this allocated memory, in * particular causing it to be free'd by wcsfree(); the user must not attempt * to free it after wcsset() has been called. * * Note that wcspih() and wcsbth() automatically invoke wcstab() on each of the * wcsprm structs that they return. * * Given and returned: * wcs struct wcsprm* * Coordinate transformation parameters (see below). * * wcstab() sets ntab, tab, nwtb and wtb, allocating * memory for the tab and wtb arrays. This allocated * memory will be free'd automatically by wcsfree(). * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Invalid tabular parameters. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * * wcsidx() - Index alternate coordinate representations * ----------------------------------------------------- * wcsidx() returns an array of 27 indices for the alternate coordinate * representations in the array of wcsprm structs returned by wcspih(). For * the array returned by wcsbth() it returns indices for the unattached * (colnum == 0) representations derived from image header keywords - use * wcsbdx() for those derived from binary table image arrays or pixel lists * keywords. * * Given: * nwcs int Number of coordinate representations in the array. * * wcs const struct wcsprm** * Pointer to an array of wcsprm structs returned by * wcspih() or wcsbth(). * * Returned: * alts int[27] Index of each alternate coordinate representation in * the array: alts[0] for the primary, alts[1] for 'A', * etc., set to -1 if not present. * * For example, if there was no 'P' representation then * = alts['P'-'A'+1] == -1; * * Otherwise, the address of its wcsprm struct would be * = wcs + alts['P'-'A'+1]; * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * * * wcsbdx() - Index alternate coordinate representions * --------------------------------------------------- * wcsbdx() returns an array of 999 x 27 indices for the alternate coordinate * representions for binary table image arrays xor pixel lists in the array of * wcsprm structs returned by wcsbth(). Use wcsidx() for the unattached * representations derived from image header keywords. * * Given: * nwcs int Number of coordinate representations in the array. * * wcs const struct wcsprm** * Pointer to an array of wcsprm structs returned by * wcsbth(). * * type int Select the type of coordinate representation: * 0: binary table image arrays, * 1: pixel lists. * * Returned: * alts short[1000][28] * Index of each alternate coordinate represention in the * array: alts[col][0] for the primary, alts[col][1] for * 'A', to alts[col][26] for 'Z', where col is the * 1-relative column number, and col == 0 is used for * unattached image headers. Set to -1 if not present. * * alts[col][27] counts the number of coordinate * representations of the chosen type for each column. * * For example, if there was no 'P' represention for * column 13 then * = alts[13]['P'-'A'+1] == -1; * * Otherwise, the address of its wcsprm struct would be * = wcs + alts[13]['P'-'A'+1]; * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * * * wcsvfree() - Free the array of wcsprm structs * --------------------------------------------- * wcsvfree() frees the memory allocated by wcspih() or wcsbth() for the array * of wcsprm structs, first invoking wcsfree() on each of the array members. * * Given and returned: * nwcs int* Number of coordinate representations found; set to 0 * on return. * * wcs struct wcsprm** * Pointer to the array of wcsprm structs; set to 0 on * return. * * Function return value: * int Status return value: * 0: Success. * 1: Null wcsprm pointer passed. * * * wcshdo() - Write out a wcsprm struct as a FITS header * ----------------------------------------------------- * wcshdo() translates a wcsprm struct into a FITS header. If the colnum * member of the struct is non-zero then a binary table image array header will * be produced. Otherwise, if the colax[] member of the struct is set non-zero * then a pixel list header will be produced. Otherwise, a primary image or * image extension header will be produced. * * If the struct was originally constructed from a header, e.g. by wcspih(), * the output header will almost certainly differ in a number of respects: * * - The output header only contains WCS-related keywords. In particular, it * does not contain syntactically-required keywords such as SIMPLE, NAXIS, * BITPIX, or END. * * - Deprecated (e.g. CROTAn) or non-standard usage will be translated to * standard (this is partially dependent on whether wcsfix() was applied). * * - Quantities will be converted to the units used internally, basically SI * with the addition of degrees. * * - Floating-point quantities may be given to a different decimal precision. * * - Elements of the PCi_ja matrix will be written if and only if they differ * from the unit matrix. Thus, if the matrix is unity then no elements * will be written. * * - Additional keywords such as WCSAXESa, CUNITia, LONPOLEa and LATPOLEa may * appear. * * - The original keycomments will be lost, although wcshdo() tries hard to * write meaningful comments. * * - Keyword order may be changed. * * Keywords can be translated between the image array, binary table, and pixel * lists forms by manipulating the colnum or colax[] members of the wcsprm * struct. * * Given: * relax int Degree of permissiveness: * 0: Recognize only FITS keywords defined by the * published WCS standard. * -1: Admit all informal extensions of the WCS * standard. * Fine-grained control of the degree of permissiveness * is also possible as explained in the notes below. * * Given and returned: * wcs struct wcsprm* * Pointer to a wcsprm struct containing coordinate * transformation parameters. Will be initialized if * necessary. * * Returned: * nkeyrec int* Number of FITS header keyrecords returned in the * "header" array. * * header char** Pointer to an array of char holding the header. * Storage for the array is allocated by wcshdo() in * blocks of 2880 bytes (32 x 80-character keyrecords) * and must be free'd by the user to avoid memory leaks. * * Each keyrecord is 80 characters long and is *NOT* * null-terminated, so the first keyrecord starts at * (*header)[0], the second at (*header)[80], etc. * * Function return value: * int Status return value (associated with wcs_errmsg[]): * 0: Success. * 1: Null wcsprm pointer passed. * 2: Memory allocation failed. * 3: Linear transformation matrix is singular. * 4: Inconsistent or unrecognized coordinate axis * types. * 5: Invalid parameter value. * 6: Invalid coordinate transformation parameters. * 7: Ill-conditioned coordinate transformation * parameters. * * For returns > 1, a detailed error message is set in * wcsprm::err if enabled, see wcserr_enable(). * * Notes: * wcshdo() interprets the "relax" argument as a vector of flag bits to * provide fine-grained control over what non-standard WCS keywords to write. * The flag bits are subject to change in future and should be set by using * the preprocessor macros (see below) for the purpose. * * - WCSHDO_none: Don't use any extensions. * * - WCSHDO_all: Write all recognized extensions, equivalent to setting each * flag bit. * * - WCSHDO_safe: Write all extensions that are considered to be safe and * recommended. * * - WCSHDO_DOBSn: Write DOBSn, the column-specific analogue of DATE-OBS for * use in binary tables and pixel lists. WCS Paper III introduced * DATE-AVG and DAVGn but by an oversight DOBSn (the obvious analogy) * was never formally defined by the standard. The alternative to * using DOBSn is to write DATE-OBS which applies to the whole table. * This usage is considered to be safe and is recommended. * * - WCSHDO_TPCn_ka: WCS Paper I defined * * - TPn_ka and TCn_ka for pixel lists * * but WCS Paper II uses TPCn_ka in one example and subsequently the * errata for the WCS papers legitimized the use of * * - TPCn_ka and TCDn_ka for pixel lists * * provided that the keyword does not exceed eight characters. This * usage is considered to be safe and is recommended because of the * non-mnemonic terseness of the shorter forms. * * - WCSHDO_PVn_ma: WCS Paper I defined * * - iVn_ma and iSn_ma for bintables and * - TVn_ma and TSn_ma for pixel lists * * but WCS Paper II uses iPVn_ma and TPVn_ma in the examples and * subsequently the errata for the WCS papers legitimized the use of * * - iPVn_ma and iPSn_ma for bintables and * - TPVn_ma and TPSn_ma for pixel lists * * provided that the keyword does not exceed eight characters. This * usage is considered to be safe and is recommended because of the * non-mnemonic terseness of the shorter forms. * * - WCSHDO_CRPXna: For historical reasons WCS Paper I defined * * - jCRPXn, iCDLTn, iCUNIn, iCTYPn, and iCRVLn for bintables and * - TCRPXn, TCDLTn, TCUNIn, TCTYPn, and TCRVLn for pixel lists * * for use without an alternate version specifier. However, because * of the eight-character keyword constraint, in order to accommodate * column numbers greater than 99 WCS Paper I also defined * * - jCRPna, iCDEna, iCUNna, iCTYna and iCRVna for bintables and * - TCRPna, TCDEna, TCUNna, TCTYna and TCRVna for pixel lists * * for use with an alternate version specifier (the "a"). Like the * PC, CD, PV, and PS keywords there is an obvious tendency to * confuse these two forms for column numbers up to 99. It is very * unlikely that any parser would reject keywords in the first set * with a non-blank alternate version specifier so this usage is * considered to be safe and is recommended. * * - WCSHDO_CNAMna: WCS Papers I and III defined * * - iCNAna, iCRDna, and iCSYna for bintables and * - TCNAna, TCRDna, and TCSYna for pixel lists * * By analogy with the above, the long forms would be * * - iCNAMna, iCRDEna, and iCSYEna for bintables and * - TCNAMna, TCRDEna, and TCSYEna for pixel lists * * Note that these keywords provide auxiliary information only, none * of them are needed to compute world coordinates. This usage is * potentially unsafe and is not recommended at this time. * * - WCSHDO_WCSNna: In light of wcsbth() note 4, write WCSNna instead of * TWCSna for pixel lists. While wcsbth() treats WCSNna and TWCSna * as equivalent, other parsers may not. Consequently, this usage * is potentially unsafe and is not recommended at this time. * * * Global variable: const char *wcshdr_errmsg[] - Status return messages * --------------------------------------------------------------------- * Error messages to match the status value returned from each function. * Use wcs_errmsg[] for status returns from wcshdo(). * *===========================================================================*/ #ifndef WCSLIB_WCSHDR #define WCSLIB_WCSHDR #include "wcs.h" #ifdef __cplusplus extern "C" { #endif #define WCSHDR_none 0x00000000 #define WCSHDR_all 0x000FFFFF #define WCSHDR_reject 0x10000000 #define WCSHDR_CROTAia 0x00000001 #define WCSHDR_EPOCHa 0x00000002 #define WCSHDR_VELREFa 0x00000004 #define WCSHDR_CD00i00j 0x00000008 #define WCSHDR_PC00i00j 0x00000010 #define WCSHDR_PROJPn 0x00000020 #define WCSHDR_RADECSYS 0x00000040 #define WCSHDR_VSOURCE 0x00000080 #define WCSHDR_DOBSn 0x00000100 #define WCSHDR_LONGKEY 0x00000200 #define WCSHDR_CNAMn 0x00000400 #define WCSHDR_AUXIMG 0x00000800 #define WCSHDR_ALLIMG 0x00001000 #define WCSHDR_IMGHEAD 0x00010000 #define WCSHDR_BIMGARR 0x00020000 #define WCSHDR_PIXLIST 0x00040000 #define WCSHDO_none 0x00 #define WCSHDO_all 0xFF #define WCSHDO_safe 0x0F #define WCSHDO_DOBSn 0x01 #define WCSHDO_TPCn_ka 0x02 #define WCSHDO_PVn_ma 0x04 #define WCSHDO_CRPXna 0x08 #define WCSHDO_CNAMna 0x10 #define WCSHDO_WCSNna 0x20 extern const char *wcshdr_errmsg[]; enum wcshdr_errmsg_enum { WCSHDRERR_SUCCESS = 0, /* Success. */ WCSHDRERR_NULL_POINTER = 1, /* Null wcsprm pointer passed. */ WCSHDRERR_MEMORY = 2, /* Memory allocation failed. */ WCSHDRERR_BAD_COLUMN = 3, /* Invalid column selection. */ WCSHDRERR_PARSER = 4, /* Fatal error returned by Flex parser. */ WCSHDRERR_BAD_TABULAR_PARAMS = 5 /* Invalid tabular parameters. */ }; int wcspih(char *header, int nkeyrec, int relax, int ctrl, int *nreject, int *nwcs, struct wcsprm **wcs); int wcsbth(char *header, int nkeyrec, int relax, int ctrl, int keysel, int *colsel, int *nreject, int *nwcs, struct wcsprm **wcs); int wcstab(struct wcsprm *wcs); int wcsidx(int nwcs, struct wcsprm **wcs, int alts[27]); int wcsbdx(int nwcs, struct wcsprm **wcs, int type, short alts[1000][28]); int wcsvfree(int *nwcs, struct wcsprm **wcs); int wcshdo(int relax, struct wcsprm *wcs, int *nkeyrec, char **header); #ifdef __cplusplus } #endif #endif /* WCSLIB_WCSHDR */ pywcs-1.12/wcslib/C/wcslib.h0000644001153600020070000000414612310355626017754 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcslib.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. * * Summary of wcslib.h * ------------------- * This header file is provided purely for convenience. Use it to include all * of the separate WCSLIB headers. * *===========================================================================*/ #ifndef WCSLIB_WCSLIB #define WCSLIB_WCSLIB #include "cel.h" #include "fitshdr.h" #include "lin.h" #include "log.h" #include "prj.h" #include "spc.h" #include "sph.h" #include "spx.h" #include "tab.h" #include "wcs.h" #include "wcserr.h" #include "wcsfix.h" #include "wcshdr.h" #include "wcsmath.h" #include "wcsprintf.h" #include "wcstrig.h" #include "wcsunits.h" #include "wcsutil.h" #endif /* WCSLIB_WCSLIB */ pywcs-1.12/wcslib/C/wcsmath.h0000644001153600020070000000405112310355626020132 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsmath.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * Summary of wcsmath.h * -------------------- * Definition of mathematical constants used by WCSLIB. * *===========================================================================*/ #ifndef WCSLIB_WCSMATH #define WCSLIB_WCSMATH #ifdef PI #undef PI #endif #ifdef D2R #undef D2R #endif #ifdef R2D #undef R2D #endif #ifdef SQRT2 #undef SQRT2 #endif #ifdef SQRT2INV #undef SQRT2INV #endif #define PI 3.141592653589793238462643 #define D2R PI/180.0 #define R2D 180.0/PI #define SQRT2 1.4142135623730950488 #define SQRT2INV 1.0/SQRT2 #ifdef UNDEFINED #undef UNDEFINED #endif #define UNDEFINED 987654321.0e99 #define undefined(value) (value == UNDEFINED) #endif /* WCSLIB_WCSMATH */ pywcs-1.12/wcslib/C/wcspih.l0000644001153600020070000006260512310355626017776 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcspih.l,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcspih.l is a Flex description file containing the definition of a lexical * scanner for parsing the WCS keyrecords from a FITS primary image or image * extension header. * * wcspih.l requires Flex v2.5.4 or later. Refer to wcshdr.h for a description * of the user interface and operating notes. * * Implementation notes * -------------------- * Use of the WCSAXESa keyword is not mandatory. Its default value is "the * larger of NAXIS and the largest index of these keywords [i.e. CRPIXj, PCi_j * or CDi_j, CDELTi, CTYPEi, CRVALi, and CUNITi] found in the FITS header". * Consequently the definition of WCSAXESa effectively invalidates the use of * NAXIS for determining the number of coordinate axes and forces a preliminary * pass through the header to determine the "largest index" in headers where * WCSAXESa was omitted. * * Furthermore, since the use of WCSAXESa is optional, there is no way to * determine the number of coordinate representations (the "a" value) other * than by parsing all of the WCS keywords in the header; even if WCSAXESa was * specified for some representations it cannot be known in advance whether it * was specified for all of those present in the header. * * Hence the definition of WCSAXESa forces the scanner to be implemented in two * passes. The first pass is used to determine the number of coordinate * representations (up to 27) and the number of coordinate axes in each. * Effectively WCSAXESa is ignored unless it exceeds the "largest index" in * which case the keywords for the extra axes assume their default values. The * number of PVi_ma and PSi_ma keywords in each representation is also counted * in the first pass. * * On completion of the first pass, memory is allocated for an array of the * required number of wcsprm structs and each of these is initialized * appropriately. These structs are filled in the second pass. * * The parser does not check for duplicated keywords, it accepts the last * encountered. * *===========================================================================*/ /* Options. */ %option full %option never-interactive %option noyywrap %option outfile="wcspih.c" %option prefix="wcspih" /* Indices for parameterized keywords. */ I0 [0-9] I1 [1-9] I2 [1-9][0-9] I3 [1-9][0-9]{2} I4 [1-9][0-9]{3} /* Alternate coordinate system identifier. */ ALT [ A-Z] /* Keyvalue data types. */ INTEGER [+-]?[0-9]+ FLOAT [+-]?([0-9]+\.?[0-9]*|\.[0-9]+)([eE][+-]?[0-9]+)? STRING '([^']|'')*' /* Exclusive start states. */ %x CROTAi PROJPn %x CCCCCia CCi_ja CCi_ma CCCCCCCa CCCCCCCC %x VALUE %x INTEGER_VAL FLOAT_VAL STRING_VAL %x COMMENT %x DISCARD ERROR FLUSH %{ #include #include #include #include #include #include "wcs.h" #include "wcshdr.h" #include "wcsmath.h" #define INTEGER 0 #define FLOAT 1 #define STRING 2 #define YY_DECL int wcspih(char *header, int nkeyrec, int relax, int ctrl, \ int *nreject, int *nwcs, struct wcsprm **wcs) #define YY_INPUT(inbuff, count, bufsize) \ { \ if (wcspih_nkeyrec) { \ strncpy(inbuff, wcspih_hdr, 80); \ inbuff[80] = '\n'; \ wcspih_hdr += 80; \ wcspih_nkeyrec--; \ count = 81; \ } else { \ count = YY_NULL; \ } \ } /* These global variables are required by YY_INPUT. */ char *wcspih_hdr; int wcspih_nkeyrec; int wcspih_final(int alts[], double epoch[], double vsource[], int *nwcs, struct wcsprm **wcs); int wcspih_inits(int naxis, int alts[], int npv[], int nps[], int *nwcs, struct wcsprm **wcs); void wcspih_naxes(int naxis, int i, int j, char a, int alts[], int *npptr); /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcspih_abort_jmp_env; #define exit(status) longjmp(wcspih_abort_jmp_env, status) %} %% /* Keyword indices, as used in the WCS papers, e.g. PCi_ja, PVi_ma. */ char a; int i, j, m; char *cptr, *errmsg, errtxt[80], *hptr, *keep; int altlin, alts[27], ialt, idx, ipx, ix, jx, naxis, *npptr, nps[27], npv[27], pass, status, valtype, voff; double epoch[27], vsource[27]; void *vptr, *wptr; struct wcsprm *wcsp; int yylex_destroy(void); naxis = 0; for (ialt = 0; ialt < 27; ialt++) { alts[ialt] = 0; npv[ialt] = 0; nps[ialt] = 0; epoch[ialt] = UNDEFINED; vsource[ialt] = UNDEFINED; } /* Parameters used to implement YY_INPUT. */ wcspih_hdr = header; wcspih_nkeyrec = nkeyrec; /* Our handle on the input stream. */ hptr = header; keep = 0x0; *nreject = 0; /* Keyword parameters. */ i = j = m = 0; a = ' '; /* For decoding the keyvalue. */ valtype = -1; idx = -1; vptr = 0x0; /* For keywords that require special handling. */ altlin = 0; npptr = 0x0; /* The data structures produced. */ *nwcs = 0; *wcs = 0x0; pass = 1; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcspih_abort_jmp_env)) { return 3; } BEGIN(INITIAL); ^NAXIS" = "" "*{INTEGER} { if (pass == 1) { sscanf(yytext, "NAXIS = %d", &naxis); } if (naxis < 0) { errmsg = errtxt; sprintf(errmsg, "Negative value of NAXIS ignored: %d", naxis); naxis = 0; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^WCSAXES{ALT}=" "" "*{INTEGER} { if (pass == 1) { sscanf(yytext, "WCSAXES%c= %d", &a, &i); wcspih_naxes(naxis, i, 0, a, alts, 0); } BEGIN(FLUSH); } ^CRPIX { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crpix); BEGIN(CCCCCia); } ^PC { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->pc); altlin = 1; BEGIN(CCi_ja); } ^CD { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->cd); altlin = 2; BEGIN(CCi_ja); } ^CDELT { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->cdelt); BEGIN(CCCCCia); } ^CROTA { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crota); altlin = 4; BEGIN(CROTAi); } ^CUNIT { valtype = STRING; if (pass == 2) vptr = &((*wcs)->cunit); BEGIN(CCCCCia); } ^CTYPE { valtype = STRING; if (pass == 2) vptr = &((*wcs)->ctype); BEGIN(CCCCCia); } ^CRVAL { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crval); BEGIN(CCCCCia); } ^LONPOLE { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->lonpole); BEGIN(CCCCCCCa); } ^LATPOLE { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->latpole); BEGIN(CCCCCCCa); } ^RESTFRQ { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->restfrq); BEGIN(CCCCCCCa); } ^RESTFREQ { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->restfrq); unput(' '); BEGIN(CCCCCCCa); } ^RESTWAV { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->restwav); BEGIN(CCCCCCCa); } ^PV { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->pv); npptr = npv; BEGIN(CCi_ma); } ^PROJP { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->pv); npptr = npv; BEGIN(PROJPn); } ^PS { valtype = STRING; if (pass == 2) vptr = &((*wcs)->ps); npptr = nps; BEGIN(CCi_ma); } ^CNAME { valtype = STRING; if (pass == 2) vptr = &((*wcs)->cname); BEGIN(CCCCCia); } ^CRDER { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->crder); BEGIN(CCCCCia); } ^CSYER { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->csyer); BEGIN(CCCCCia); } ^DATE-AVG { valtype = STRING; if (pass == 2) vptr = (*wcs)->dateavg; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^DATE-OBS { valtype = STRING; if (pass == 2) vptr = (*wcs)->dateobs; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^EPOCH{ALT}" " { sscanf(yytext, "EPOCH%c", &a); if (a == ' ' || relax & WCSHDR_EPOCHa) { valtype = FLOAT; if (pass == 2) { vptr = epoch; if (a >= 'A') { vptr = (void *)((double *)vptr + alts[a-'A'+1]); } } unput(' '); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "EPOCH keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^EQUINOX { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->equinox); BEGIN(CCCCCCCa); } ^MJD-AVG" " { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->mjdavg); if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^MJD-OBS" " { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->mjdobs); if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^OBSGEO-X { valtype = FLOAT; if (pass == 2) vptr = (*wcs)->obsgeo; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^OBSGEO-Y { valtype = FLOAT; if (pass == 2) vptr = (*wcs)->obsgeo + 1; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^OBSGEO-Z { valtype = FLOAT; if (pass == 2) vptr = (*wcs)->obsgeo + 2; if (ctrl < -10) keep = wcspih_hdr - 80; BEGIN(CCCCCCCC); } ^RADESYS { valtype = STRING; if (pass == 2) vptr = (*wcs)->radesys; BEGIN(CCCCCCCa); } ^RADECSYS { if (relax & WCSHDR_RADECSYS) { valtype = STRING; if (pass == 2) vptr = (*wcs)->radesys; unput(' '); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "RADECSYS is non-standard, use RADESYSa"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^SPECSYS { valtype = STRING; if (pass == 2) vptr = (*wcs)->specsys; BEGIN(CCCCCCCa); } ^SSYSOBS { valtype = STRING; if (pass == 2) vptr = (*wcs)->ssysobs; BEGIN(CCCCCCCa); } ^SSYSSRC { valtype = STRING; if (pass == 2) vptr = (*wcs)->ssyssrc; BEGIN(CCCCCCCa); } ^VELANGL { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->velangl); BEGIN(CCCCCCCa); } ^VELOSYS { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->velosys); BEGIN(CCCCCCCa); } ^VELREF{ALT}" " { sscanf(yytext, "VELREF%c", &a); if (a == ' ' || relax & WCSHDR_VELREFa) { valtype = INTEGER; if (pass == 2) vptr = &((*wcs)->velref); unput(a); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "VELREF keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^VSOURCE{ALT} { sscanf(yytext, "VSOURCE%c", &a); if (relax & WCSHDR_VSOURCE) { valtype = FLOAT; if (pass == 2) { vptr = vsource; if (a >= 'A') { vptr = (void *)((double *)vptr + alts[a-'A'+1]); } } unput(' '); BEGIN(CCCCCCCa); } else if (relax & WCSHDR_reject) { errmsg = "Deprecated VSOURCEa keyword rejected"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^WCSNAME { valtype = STRING; if (pass == 2) vptr = (*wcs)->wcsname; BEGIN(CCCCCCCa); } ^ZSOURCE { valtype = FLOAT; if (pass == 2) vptr = &((*wcs)->zsource); BEGIN(CCCCCCCa); } ^END" "{77} { yyless(0); if (wcspih_nkeyrec) { wcspih_nkeyrec = 0; errmsg = "Keyrecords following the END keyrecord were ignored"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } ^. { BEGIN(DISCARD); } {I1}{ALT}" " | {I2}{ALT} { sscanf(yytext, "%d%c", &i, &a); idx = i - 1; BEGIN(VALUE); } {I3} { /* Invalid axis number will be caught by . */ sscanf(yytext, "%3d", &i); BEGIN(VALUE); } . { BEGIN(DISCARD); } {I1}_{I1}{ALT}" " | {I1}_{I2}{ALT}" " | {I2}_{I1}{ALT}" " | {I2}_{I2}{ALT} { sscanf(yytext, "%d_%d%c", &i, &j, &a); if (pass == 2) { wcsp = *wcs; if (a != ' ') { wcsp += alts[a-'A'+1]; } idx = (i-1)*(wcsp->naxis) + j - 1; } BEGIN(VALUE); } {I1}_{I3}{ALT} | {I3}_{I1}{ALT} | {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I1} { /* Invalid axis numbers will be caught by . */ sscanf(yytext, "%d_%d", &i, &j); BEGIN(VALUE); } {I0}{6} { /* This covers the defunct forms CD00i00j and PC00i00j. */ if (((relax & WCSHDR_PC00i00j) && (altlin == 1)) || ((relax & WCSHDR_CD00i00j) && (altlin == 2))) { sscanf(yytext, "%3d%3d", &i, &j); a = ' '; if (pass == 2) { idx = (i-1)*((*wcs)->naxis) + j - 1; } BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = errtxt; sprintf(errmsg, "Defunct form of %si_ja keyword", (altlin==1) ? "PC" : "CD"); BEGIN(ERROR); } else { BEGIN(DISCARD); } } . { BEGIN(DISCARD); } {I1}{ALT}" " | {I2}{ALT} { sscanf(yytext, "%d%c", &i, &a); if (a == ' ' || relax & WCSHDR_CROTAia) { idx = i - 1; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = "CROTAn keyword may not have an alternate version code"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } {I3} { sscanf(yytext, "%d", &i); a = ' '; idx = i - 1; BEGIN(VALUE); } . { BEGIN(DISCARD); } {ALT} | . { idx = -1; if (YY_START == CCCCCCCa) { sscanf(yytext, "%c", &a); } else { unput(yytext[0]); a = 0; } BEGIN(VALUE); } . { BEGIN(DISCARD); } {I1}_{I0}{ALT}" " | {I1}_{I2}{ALT}" " | {I2}_{I0}{ALT}" " | {I2}_{I2}{ALT} { sscanf(yytext, "%d_%d%c", &i, &m, &a); idx = -1; BEGIN(VALUE); } {I1}_{I3}{ALT} | {I3}_{I0}{ALT} | {I1}_{I4} | {I2}_{I3} | {I3}_{I2} | {I4}_{I0} { /* Invalid parameters will be caught by . */ sscanf(yytext, "%d_%d", &i, &m); BEGIN(VALUE); } . { BEGIN(DISCARD); } {I0}" " { if (relax & WCSHDR_PROJPn) { sscanf(yytext, "%d", &m); i = 0; a = ' '; idx = -1; BEGIN(VALUE); } else if (relax & WCSHDR_reject) { errmsg = "Defunct PROJPn keyword rejected"; BEGIN(ERROR); } else { BEGIN(DISCARD); } } . { BEGIN(DISCARD); } =" "+ { /* Do checks on i, j & m. */ if (i > 99 || j > 99 || m > 99) { if (relax & WCSHDR_reject) { errmsg = errtxt; if (i > 99 || j > 99) { sprintf(errmsg, "Axis number exceeds 99"); } else if (m > 99) { sprintf(errmsg, "Parameter number exceeds 99"); } BEGIN(ERROR); } else { /* Pretend we don't recognize it. */ BEGIN(DISCARD); } } else { if (valtype == INTEGER) { BEGIN(INTEGER_VAL); } else if (valtype == FLOAT) { BEGIN(FLOAT_VAL); } else if (valtype == STRING) { BEGIN(STRING_VAL); } else { errmsg = errtxt; sprintf(errmsg, "Internal parser ERROR, bad data type: %d", valtype); BEGIN(ERROR); } } } . { errmsg = "Invalid KEYWORD = VALUE syntax"; BEGIN(ERROR); } {INTEGER} { if (pass == 1) { wcspih_naxes(naxis, i, j, a, alts, npptr); BEGIN(FLUSH); } else { if (vptr) { /* Determine the coordinate representation. */ for (ialt = 0; ialt < *nwcs; ialt++) { /* The loop here is for keywords that apply */ /* to every alternate; these have a == 0. */ if (a >= 'A') { ialt = alts[a-'A'+1]; } wptr = vptr; if (ialt) { voff = (char *)(*wcs+ialt) - (char *)(*wcs); wptr = (void *)((char *)vptr + voff); } /* Apply keyword parameterization. */ if (idx >= 0) { wptr = *((int **)wptr) + idx; } /* Read the keyvalue. */ sscanf(yytext, "%d", (int *)wptr); if (a) break; } BEGIN(COMMENT); } else { errmsg = "Internal parser ERROR, null int pointer"; BEGIN(ERROR); } } } . { errmsg = "An integer value was expected"; BEGIN(ERROR); } {FLOAT} { if (pass == 1) { wcspih_naxes(naxis, i, j, a, alts, npptr); BEGIN(FLUSH); } else { if (vptr) { /* Determine the coordinate representation. */ for (ialt = 0; ialt < *nwcs; ialt++) { /* The loop here is for keywords like MJD-OBS that */ /* apply to every alternate; these have a == 0. */ if (a >= 'A') { ialt = alts[a-'A'+1]; } wptr = vptr; if (ialt) { voff = (char *)(*wcs+ialt) - (char *)(*wcs); wptr = (void *)((char *)vptr + voff); } /* Apply keyword parameterization. */ if (idx >= 0) { wptr = *((double **)wptr) + idx; } else if (npptr == npv) { ipx = (*wcs+ialt)->npv++; (*wcs+ialt)->pv[ipx].i = i; (*wcs+ialt)->pv[ipx].m = m; wptr = &((*wcs+ialt)->pv[ipx].value); } /* Read the keyvalue. */ sscanf(yytext, "%lf", (double *)wptr); /* Flag the presence of PCi_ja, or CDi_ja and/or CROTAia. */ if (altlin) { (*wcs+ialt)->altlin |= altlin; altlin = 0; } if (a) break; } BEGIN(COMMENT); } else { errmsg = "Internal parser ERROR, null float pointer"; BEGIN(ERROR); } } } . { errmsg = "A floating-point value was expected"; BEGIN(ERROR); } {STRING} { if (pass == 1) { wcspih_naxes(naxis, i, j, a, alts, npptr); BEGIN(FLUSH); } else { if (vptr) { /* Determine the coordinate representation. */ for (ialt = 0; ialt < *nwcs; ialt++) { /* The loop here is for keywords like DATE-OBS that */ /* apply to every alternate; these have a == 0. */ if (a >= 'A') { ialt = alts[a-'A'+1]; } wptr = vptr; if (ialt) { voff = (char *)(*wcs+ialt) - (char *)(*wcs); wptr = (void *)((char *)vptr + voff); } /* Apply keyword parameterization. */ if (idx >= 0) { wptr = *((char (**)[72])wptr) + idx; } else if (npptr == nps) { ipx = (*wcs+ialt)->nps++; (*wcs+ialt)->ps[ipx].i = i; (*wcs+ialt)->ps[ipx].m = m; wptr = (*wcs+ialt)->ps[ipx].value; } /* Read the keyvalue. */ cptr = (char *)wptr; strcpy(cptr, yytext+1); /* Squeeze out repeated quotes. */ ix = 0; for (jx = 0; jx < 72; jx++) { if (ix < jx) { cptr[ix] = cptr[jx]; } if (cptr[jx] == '\0') { if (ix) cptr[ix-1] = '\0'; break; } else if (cptr[jx] == '\'' && cptr[jx+1] == '\'') { jx++; } ix++; } if (a) break; } BEGIN(COMMENT); } else { errmsg = "Internal parser ERROR, null string pointer"; BEGIN(ERROR); } } } . { errmsg = "A string value was expected"; BEGIN(ERROR); } " "*\/.* | " "* { BEGIN(FLUSH); } . { errmsg = "Malformed keycomment"; BEGIN(ERROR); } .* { if (pass == 2) { if (ctrl < 0) { /* Preserve discards. */ keep = wcspih_hdr - 80; } else if (ctrl > 2) { fprintf(stderr, "%.80s\n Discarded.\n", wcspih_hdr-80); } } BEGIN(FLUSH); } .* { (*nreject)++; if (pass == 2) { if (ctrl%10 == -1) { /* Preserve rejects. */ keep = wcspih_hdr - 80; } if (abs(ctrl%10) > 1) { fprintf(stderr, "%.80s\n%4d: %s.\n", wcspih_hdr-80, *nreject, errmsg); } } BEGIN(FLUSH); } .*\n { if (pass == 2 && keep) { if (hptr < keep) { strncpy(hptr, keep, 80); } hptr += 80; } i = j = m = 0; a = ' '; valtype = -1; keep = 0x0; altlin = 0; npptr = 0x0; BEGIN(INITIAL); } <> { /* End-of-input. */ if (pass == 1) { if ((status = wcspih_inits(naxis, alts, npv, nps, nwcs, wcs)) || *nwcs == 0) { yylex_destroy(); return status; } if (abs(ctrl%10) > 2) { if (*nwcs == 1) { fprintf(stderr, "Found one coordinate representation.\n"); } else { fprintf(stderr, "Found %d coordinate representations.\n", *nwcs); } } wcspih_hdr = header; wcspih_nkeyrec = nkeyrec; *nreject = 0; pass = 2; i = j = m = 0; a = ' '; valtype = -1; yyrestart(yyin); } else { yylex_destroy(); if (ctrl < 0) { *hptr = '\0'; } else if (ctrl == 1) { fprintf(stderr, "%d WCS keyrecords were rejected.\n", *nreject); } return wcspih_final(alts, epoch, vsource, nwcs, wcs); } } %% /*---------------------------------------------------------------------------- * Determine the number of coordinate representations (up to 27) and the * number of coordinate axes in each, and count the number of PVi_ma and * PSi_ma keywords in each representation. *---------------------------------------------------------------------------*/ void wcspih_naxes(int naxis, int i, int j, char a, int alts[], int *npptr) { /* On the first pass alts[] is used to determine the number of axes */ /* for each of the 27 possible alternate coordinate descriptions. */ int ialt, *ip; if (a == 0) { return; } ialt = 0; if (a != ' ') { ialt = a - 'A' + 1; } ip = alts + ialt; if (*ip < naxis) { *ip = naxis; } /* i or j can be greater than naxis. */ if (*ip < i) { *ip = i; } if (*ip < j) { *ip = j; } if (npptr) { npptr[ialt]++; } } /*---------------------------------------------------------------------------- * Allocate memory for an array of the required number of wcsprm structs and * initialize each of them. *---------------------------------------------------------------------------*/ int wcspih_inits( int naxis, int alts[], int npv[], int nps[], int *nwcs, struct wcsprm **wcs) { int ialt, npsmax, npvmax, status = 0; struct wcsprm *wcsp; /* Find the number of coordinate descriptions. */ *nwcs = 0; for (ialt = 0; ialt < 27; ialt++) { if (alts[ialt]) (*nwcs)++; } if (!(*nwcs) && naxis) { /* NAXIS is non-zero but there were no WCS keywords with an alternate version code; create a default WCS with blank alternate version. */ wcspih_naxes(naxis, 0, 0, ' ', alts, 0x0); *nwcs = 1; } if (*nwcs) { /* Allocate memory for the required number of wcsprm structs. */ if (!(*wcs = calloc(*nwcs, sizeof(struct wcsprm)))) { return 2; } /* Record the current values of NPVMAX and NPSMAX. */ npvmax = wcsnpv(-1); npsmax = wcsnps(-1); /* Initialize each wcsprm struct. */ wcsp = *wcs; *nwcs = 0; for (ialt = 0; ialt < 27; ialt++) { if (alts[ialt]) { wcsp->flag = -1; wcsnpv(npv[ialt]); wcsnps(nps[ialt]); if ((status = wcsini(1, alts[ialt], wcsp))) { wcsvfree(nwcs, wcs); break; } /* Record the alternate version code. */ if (ialt) { wcsp->alt[0] = 'A' + ialt - 1; } /* On the second pass alts[] indexes the array of wcsprm structs. */ alts[ialt] = (*nwcs)++; wcsp++; } } /* Restore the original values of NPVMAX and NPSMAX. */ wcsnpv(npvmax); wcsnps(npsmax); } return status; } /*---------------------------------------------------------------------------- * Interpret special keywords encountered for each coordinate representation. *---------------------------------------------------------------------------*/ int wcspih_final( int alts[], double epoch[], double vsource[], int *nwcs, struct wcsprm **wcs) { int ialt, status; double beta, c = 299792458.0; for (ialt = 0; ialt < *nwcs; ialt++) { /* Check for EPOCH overriding EQUINOXa. */ if (undefined((*wcs+ialt)->equinox) && !undefined(epoch[ialt])) { /* Set EQUINOXa. */ (*wcs+ialt)->equinox = epoch[ialt]; } /* Check for VSOURCEa overriding ZSOURCEa. */ if (undefined((*wcs+ialt)->zsource) && !undefined(vsource[ialt])) { /* Convert relativistic Doppler velocity to redshift. */ beta = vsource[ialt]/c; (*wcs+ialt)->zsource = (1.0+beta)/sqrt(1.0 - beta*beta) - 1.0; } /* Interpret -TAB header keywords. */ if ((status = wcstab(*wcs+ialt))) { wcsvfree(nwcs, wcs); return status; } } return 0; } pywcs-1.12/wcslib/C/wcsprintf.c0000644001153600020070000000655412310355626020510 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsprintf.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include "wcsprintf.h" static FILE *wcsprintf_file = 0x0; static char *wcsprintf_buff = 0x0; static char *wcsprintf_bufp = 0x0; static size_t wcsprintf_size = 0; /*--------------------------------------------------------------------------*/ int wcsprintf_set(FILE *wcsout) { if (wcsout != 0x0) { /* Output to file. */ wcsprintf_file = wcsout; if (wcsprintf_buff != 0x0) { /* Release the buffer. */ free(wcsprintf_buff); wcsprintf_buff = 0x0; } } else { /* Output to buffer. */ if (wcsprintf_buff == 0x0) { /* Allocate a buffer. */ wcsprintf_buff = malloc(1024); if (wcsprintf_buff == NULL) { return 1; } wcsprintf_size = 1024; } /* Reset pointer to the start of the buffer. */ wcsprintf_bufp = wcsprintf_buff; *wcsprintf_bufp = '\0'; } return 0; } /*--------------------------------------------------------------------------*/ const char *wcsprintf_buf(void) { return wcsprintf_buff; } /*--------------------------------------------------------------------------*/ int wcsprintf(const char *format, ...) { int nbytes; size_t used; va_list arg_list; if (wcsprintf_buff == 0x0 && wcsprintf_file == 0x0) { /* Send output to stdout if wcsprintf_set() hasn't been called. */ wcsprintf_file = stdout; } va_start(arg_list, format); if (wcsprintf_file) { /* Output to file. */ nbytes = vfprintf(wcsprintf_file, format, arg_list); } else { /* Output to buffer. */ used = wcsprintf_bufp - wcsprintf_buff; if (wcsprintf_size - used < 128) { /* Expand the buffer. */ wcsprintf_size += 1024; wcsprintf_buff = realloc(wcsprintf_buff, wcsprintf_size); if (wcsprintf_buff == NULL) { return 1; } wcsprintf_bufp = wcsprintf_buff + used; } nbytes = vsprintf(wcsprintf_bufp, format, arg_list); wcsprintf_bufp += nbytes; } va_end(arg_list); return nbytes; } pywcs-1.12/wcslib/C/wcsprintf.h0000644001153600020070000001217312310355626020507 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsprintf.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. * * Summary of the wcsprintf routines * --------------------------------- * These routines allow diagnostic output from celprt(), linprt(), prjprt(), * spcprt(), tabprt(), wcsprt(), and wcserr_prt() to be redirected to a file or * captured in a string buffer. Those routines all use wcsprintf() for output. * * * wcsprintf() - Print function used by WCSLIB diagnostic routines * --------------------------------------------------------------- * wcsprintf() is used by the celprt(), linprt(), prjprt(), spcprt(), tabprt(), * wcsprt(), and wcserr_prt() routines. Its output may be redirected to a file * or string buffer via wcsprintf_set(). By default output goes to stdout. * * Given: * format char* Format string, passed to one of the printf(3) family * of stdio library functions. * * ... mixed Argument list matching format, as per printf(3). * * Function return value: * int Number of bytes written. * * * wcsprintf_set() - Set output disposition for wcsprintf() * -------------------------------------------------------- * wcsprintf_set() sets the output disposition for wcsprintf() which is used by * the celprt(), linprt(), prjprt(), spcprt(), tabprt(), wcsprt(), and * wcserr_prt() routines. * * Output goes to stdout by default if wcsprintf_set() has not been called. * * Given: * wcsout FILE* Pointer to an output stream that has been opened for * writing, e.g. by the fopen() stdio library function, * or one of the predefined stdio output streams - stdout * and stderr. If zero (NULL), output is written to an * internally-allocated string buffer, the address of * which may be obtained by wcsprintf_buf(). * * Function return value: * int Status return value: * 0: Success. * * * wcsprintf_buf() - Get the address of the internal string buffer * --------------------------------------------------------------- * wcsprintf_buf() returns the address of the internal string buffer created * when wcsprintf_set() is invoked with its FILE* argument set to zero. * * Function return value: * const char * * Address of the internal string buffer. The user may * free this buffer by calling wcsprintf_set() with a * valid FILE*, e.g. stdout. The free() stdlib library * function must NOT be invoked on this const pointer. * * * WCSPRINTF_PTR() macro - Print addresses in a consistent way * ----------------------------------------------------------- * WCSPRINTF_PTR() is a preprocessor macro used to print addresses in a * consistent way. * * On some systems the "%p" format descriptor renders a NULL pointer as the * string "0x0". On others, however, it produces "0" or even "(nil)". On * some systems a non-zero address is prefixed with "0x", on others, not. * * The WCSPRINTF_PTR() macro ensures that a NULL pointer is always rendered as * "0x0" and that non-zero addresses are prefixed with "0x" thus providing * consistency, for example, for comparing the output of test programs. * *===========================================================================*/ #ifndef WCSLIB_WCSPRINTF #define WCSLIB_WCSPRINTF #ifdef __cplusplus extern "C" { #endif #define WCSPRINTF_PTR(str1, ptr, str2) \ if (ptr) { \ wcsprintf("%s%#lx%s", (str1), (unsigned long)(ptr), (str2)); \ } else { \ wcsprintf("%s0x0%s", (str1), (str2)); \ } int wcsprintf_set(FILE *wcsout); int wcsprintf(const char *format, ...); const char *wcsprintf_buf(void); #ifdef __cplusplus } #endif #endif /* WCSLIB_WCSPRINTF */ pywcs-1.12/wcslib/C/wcstrig.c0000644001153600020070000001055612310355626020150 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcstrig.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include "wcsmath.h" #include "wcstrig.h" double cosd(angle) double angle; { int i; if (fmod(angle,90.0) == 0.0) { i = abs((int)floor(angle/90.0 + 0.5))%4; switch (i) { case 0: return 1.0; case 1: return 0.0; case 2: return -1.0; case 3: return 0.0; } } return cos(angle*D2R); } /*--------------------------------------------------------------------------*/ double sind(angle) double angle; { int i; if (fmod(angle,90.0) == 0.0) { i = abs((int)floor(angle/90.0 - 0.5))%4; switch (i) { case 0: return 1.0; case 1: return 0.0; case 2: return -1.0; case 3: return 0.0; } } return sin(angle*D2R); } /*--------------------------------------------------------------------------*/ void sincosd(double angle, double *s, double *c) { int i; if (fmod(angle,90.0) == 0.0) { i = abs((int)floor(angle/90.0 + 0.5))%4; switch (i) { case 0: *s = 0.0; *c = 1.0; return; case 1: *s = (angle > 0.0) ? 1.0 : -1.0; *c = 0.0; return; case 2: *s = 0.0; *c = -1.0; return; case 3: *s = (angle > 0.0) ? -1.0 : 1.0; *c = 0.0; return; } } #ifdef HAVE_SINCOS sincos(angle*D2R, s, c); #else *s = sin(angle*D2R); *c = cos(angle*D2R); #endif return; } /*--------------------------------------------------------------------------*/ double tand(angle) double angle; { double resid; resid = fmod(angle,360.0); if (resid == 0.0 || fabs(resid) == 180.0) { return 0.0; } else if (resid == 45.0 || resid == 225.0) { return 1.0; } else if (resid == -135.0 || resid == -315.0) { return -1.0; } return tan(angle*D2R); } /*--------------------------------------------------------------------------*/ double acosd(v) double v; { if (v >= 1.0) { if (v-1.0 < WCSTRIG_TOL) return 0.0; } else if (v == 0.0) { return 90.0; } else if (v <= -1.0) { if (v+1.0 > -WCSTRIG_TOL) return 180.0; } return acos(v)*R2D; } /*--------------------------------------------------------------------------*/ double asind(v) double v; { if (v <= -1.0) { if (v+1.0 > -WCSTRIG_TOL) return -90.0; } else if (v == 0.0) { return 0.0; } else if (v >= 1.0) { if (v-1.0 < WCSTRIG_TOL) return 90.0; } return asin(v)*R2D; } /*--------------------------------------------------------------------------*/ double atand(v) double v; { if (v == -1.0) { return -45.0; } else if (v == 0.0) { return 0.0; } else if (v == 1.0) { return 45.0; } return atan(v)*R2D; } /*--------------------------------------------------------------------------*/ double atan2d(y, x) double x, y; { if (y == 0.0) { if (x >= 0.0) { return 0.0; } else if (x < 0.0) { return 180.0; } } else if (x == 0.0) { if (y > 0.0) { return 90.0; } else if (y < 0.0) { return -90.0; } } return atan2(y,x)*R2D; } pywcs-1.12/wcslib/C/wcstrig.h0000644001153600020070000001425312310355626020153 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcstrig.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * Summary of the wcstrig routines * ------------------------------- * When dealing with celestial coordinate systems and spherical projections * (some moreso than others) it is often desirable to use an angular measure * that provides an exact representation of the latitude of the north or south * pole. The WCSLIB routines use the following trigonometric functions that * take or return angles in degrees: * * - cosd() * - sind() * - tand() * - acosd() * - asind() * - atand() * - atan2d() * - sincosd() * * These "trigd" routines are expected to handle angles that are a multiple of * 90 degrees returning an exact result. Some C implementations provide these * as part of a system library and in such cases it may (or may not!) be * preferable to use them. WCSLIB provides wrappers on the standard trig * functions based on radian measure, adding tests for multiples of 90 degrees. * * However, wcstrig.h also provides the choice of using preprocessor macro * implementations of the trigd functions that don't test for multiples of * 90 degrees (compile with -DWCSTRIG_MACRO). These are typically 20% faster * but may lead to problems near the poles. * * * cosd() - Cosine of an angle in degrees * -------------------------------------- * cosd() returns the cosine of an angle given in degrees. * * Given: * angle double [deg]. * * Function return value: * double Cosine of the angle. * * * sind() - Sine of an angle in degrees * ------------------------------------ * sind() returns the sine of an angle given in degrees. * * Given: * angle double [deg]. * * Function return value: * double Sine of the angle. * * * sincosd() - Sine and cosine of an angle in degrees * -------------------------------------------------- * sincosd() returns the sine and cosine of an angle given in degrees. * * Given: * angle double [deg]. * * Returned: * sin *double Sine of the angle. * * cos *double Cosine of the angle. * * Function return value: * void * * * tand() - Tangent of an angle in degrees * --------------------------------------- * tand() returns the tangent of an angle given in degrees. * * Given: * angle double [deg]. * * Function return value: * double Tangent of the angle. * * * acosd() - Inverse cosine, returning angle in degrees * ---------------------------------------------------- * acosd() returns the inverse cosine in degrees. * * Given: * x double in the range [-1,1]. * * Function return value: * double Inverse cosine of x [deg]. * * * asind() - Inverse sine, returning angle in degrees * -------------------------------------------------- * asind() returns the inverse sine in degrees. * * Given: * y double in the range [-1,1]. * * Function return value: * double Inverse sine of y [deg]. * * * atand() - Inverse tangent, returning angle in degrees * ----------------------------------------------------- * atand() returns the inverse tangent in degrees. * * Given: * s double * * Function return value: * double Inverse tangent of s [deg]. * * * atan2d() - Polar angle of (x,y), in degrees * ------------------------------------------- * atan2d() returns the polar angle, beta, in degrees, of polar coordinates * (rho,beta) corresponding Cartesian coordinates (x,y). It is equivalent to * the arg(x,y) function of WCS Paper II, though with transposed arguments. * * Given: * y double Cartesian y-coordinate. * * x double Cartesian x-coordinate. * * Function return value: * double Polar angle of (x,y) [deg]. * *===========================================================================*/ #ifndef WCSLIB_WCSTRIG #define WCSLIB_WCSTRIG #include #include "wcsconfig.h" #ifdef HAVE_SINCOS void sincos(double angle, double *sin, double *cos); #endif #ifdef __cplusplus extern "C" { #endif #ifdef WCSTRIG_MACRO /* Macro implementation of the trigd functions. */ #include "wcsmath.h" #define cosd(X) cos((X)*D2R) #define sind(X) sin((X)*D2R) #define tand(X) tan((X)*D2R) #define acosd(X) acos(X)*R2D #define asind(X) asin(X)*R2D #define atand(X) atan(X)*R2D #define atan2d(Y,X) atan2(Y,X)*R2D #ifdef HAVE_SINCOS #define sincosd(X,S,C) sincos((X)*D2R,(S),(C)) #else #define sincosd(X,S,C) *(S) = sin((X)*D2R); *(C) = cos((X)*D2R); #endif #else /* Use WCSLIB wrappers or native trigd functions. */ double cosd(double angle); double sind(double angle); void sincosd(double angle, double *sin, double *cos); double tand(double angle); double acosd(double x); double asind(double y); double atand(double s); double atan2d(double y, double x); /* Domain tolerance for asin() and acos() functions. */ #define WCSTRIG_TOL 1e-10 #endif /* WCSTRIG_MACRO */ #ifdef __cplusplus } #endif #endif /* WCSLIB_WCSTRIG */ pywcs-1.12/wcslib/C/wcsulex.l0000644001153600020070000004443512310355626020174 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsulex.l,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcsulex.l is a Flex description file containing the definition of a * recursive, multi-buffered lexical scanner that parses FITS units * specifications. * * It requires Flex v2.5.4 or later. * * Refer to wcsunits.h for a description of the user interface and operating * notes. * *===========================================================================*/ /* Options. */ %option full %option never-interactive %option noyywrap %option outfile="wcsulex.c" %option prefix="wcsulex" /* Exponents. */ INTEGER [+-]?[1-9][0-9]* FRAC {INTEGER}"/"[1-9][0-9]* FLOAT [+-]?([0-9]+\.?[0-9]*|\.[0-9]+) /* Metric prefixes. */ SUB3 [munpfazy] SUBPREFIX [dc]|{SUB3} SUP3 [kMGTPEZY] SUPPREFIX da|h|{SUP3} PREFIX {SUBPREFIX}|{SUPPREFIX} /* Basic and derived SI units. */ BASIC m|s|g|rad|sr|K|A|mol|cd DERIVED Hz|J|W|V|N|Pa|C|[Oo]hm|S|F|Wb|T|H|lm|lx SI_UNIT {BASIC}|{DERIVED} /* Additional recognized units: all metric prefixes allowed. */ ADD_ALL eV|Jy|R|G|barn /* Additional recognized units: only super-metric prefixes allowed. */ ADD_SUP a|yr|pc|bit|[bB]yte /* Additional recognized units: only sub-metric prefixes allowed. */ ADD_SUB mag /* Additional recognized units for which NO metric prefixes are allowed. */ GENERAL deg|arcmin|arcsec|mas|d|h|min|erg|Ry|u|D ASTRO [Aa]ngstrom|AU|lyr|beam|solRad|solMass|solLum|Sun DEVICE adu|bin|chan|count|ct|photon|ph|pixel|pix|voxel ADD_NONE {GENERAL}|{ASTRO}|{DEVICE} /* All additional recognized units. */ ADD_UNIT {ADD_ALL}|{ADD_SUP}|{ADD_SUB}|{ADD_NONE} /* Exclusive start states. */ %x PAREN PREFIX UNITS EXPON FLUSH %{ /* To get the prototype for fileno() from stdio.h when gcc is invoked with * -std=c89 (same as -ansi) or -std=c99 since we do not define YY_INPUT. */ #define _POSIX_SOURCE 1 #include #include #include #include #include "wcserr.h" #include "wcsmath.h" #include "wcsunits.h" #define YY_DECL int wcsulexe(const char unitstr[], int *func, double *scale, \ double units[], struct wcserr **err) /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcsulex_abort_jmp_env; #define exit(status) longjmp(wcsulex_abort_jmp_env, status) %} %% static const char *function = "wcsulexe"; int bracket = 0; int operator = 0; int paren = 0; int status = 0; int func_r, i, j; double dexp, expon, factor, factor_r, types[WCSUNITS_NTYPE]; YY_BUFFER_STATE buf; void add(double *factor, double types[], double *expon, double *scale, double units[]); int yylex_destroy(void); *func = 0; for (i = 0; i < WCSUNITS_NTYPE; i++) { units[i] = 0.0; types[i] = 0.0; } expon = 1.0; factor = 1.0; *scale = 1.0; yy_scan_string(unitstr); /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcsulex_abort_jmp_env)) { return wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error parsing '%s'", unitstr); } BEGIN(INITIAL); #ifdef DEBUG fprintf(stderr, "\n%s ->\n", unitstr); #endif ^" "+ { /* Pretend initial whitespace doesn't exist. */ yy_set_bol(1); } ^"[" { if (bracket++) { BEGIN(FLUSH); } else { yy_set_bol(1); } } ^10[0-9] { status = wcserr_set(WCSERR_SET(UNITSERR_BAD_NUM_MULTIPLIER), "Invalid exponent in '%s'", unitstr); BEGIN(FLUSH); } ^10 { factor = 10.0; BEGIN(EXPON); } ^log" "*"(" { *func = 1; unput('('); BEGIN(PAREN); } ^ln" "*"(" { *func = 2; unput('('); BEGIN(PAREN); } ^exp" "*"(" { *func = 3; unput('('); BEGIN(PAREN); } ^[*.] { /* Leading binary multiply. */ status = wcserr_set(WCSERR_SET(UNITSERR_DANGLING_BINOP), "Dangling binary operator in '%s'", unitstr); BEGIN(FLUSH); } " "+ /* Discard whitespace in INITIAL context. */ sqrt" "*"(" { expon /= 2.0; unput('('); BEGIN(PAREN); } "(" { /* Gather terms in parentheses. */ yyless(0); BEGIN(PAREN); } [*.] { if (operator++) { BEGIN(FLUSH); } } ^1"/" | "/" { if (operator++) { BEGIN(FLUSH); } else { expon *= -1.0; } } {SI_UNIT}|{ADD_UNIT} { operator = 0; yyless(0); BEGIN(UNITS); } {PREFIX}({SI_UNIT}|{ADD_ALL}) | {SUPPREFIX}{ADD_SUP} | {SUBPREFIX}{ADD_SUB} { operator = 0; yyless(0); BEGIN(PREFIX); } "]" { bracket = !bracket; BEGIN(FLUSH); } . { status = wcserr_set(WCSERR_SET(UNITSERR_BAD_INITIAL_SYMBOL), "Invalid symbol in INITIAL context in '%s'", unitstr); BEGIN(FLUSH); } "(" { paren++; operator = 0; yymore(); } ")" { paren--; if (paren) { /* Not balanced yet. */ yymore(); } else { /* Balanced; strip off the outer parentheses and recurse. */ yytext[yyleng-1] = '\0'; buf = YY_CURRENT_BUFFER; status = wcsulexe(yytext+1, &func_r, &factor_r, types, err); yy_switch_to_buffer(buf); if (func_r) { status = wcserr_set(WCSERR_SET(UNITSERR_FUNCTION_CONTEXT), "Function in invalid context in '%s'", unitstr); } if (status) { BEGIN(FLUSH); } else { factor *= factor_r; BEGIN(EXPON); } } } [^()]+ { yymore(); } d { factor = 1e-1; BEGIN(UNITS); } c { factor = 1e-2; BEGIN(UNITS); } m { factor = 1e-3; BEGIN(UNITS); } u { factor = 1e-6; BEGIN(UNITS); } n { factor = 1e-9; BEGIN(UNITS); } p { factor = 1e-12; BEGIN(UNITS); } f { factor = 1e-15; BEGIN(UNITS); } a { factor = 1e-18; BEGIN(UNITS); } z { factor = 1e-21; BEGIN(UNITS); } y { factor = 1e-24; BEGIN(UNITS); } da { factor = 1e+1; BEGIN(UNITS); } h { factor = 1e+2; BEGIN(UNITS); } k { factor = 1e+3; BEGIN(UNITS); } M { factor = 1e+6; BEGIN(UNITS); } G { factor = 1e+9; BEGIN(UNITS); } T { factor = 1e+12; BEGIN(UNITS); } P { factor = 1e+15; BEGIN(UNITS); } E { factor = 1e+18; BEGIN(UNITS); } Z { factor = 1e+21; BEGIN(UNITS); } Y { factor = 1e+24; BEGIN(UNITS); } . { /* Internal parser error. */ status = wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error parsing '%s'", unitstr); BEGIN(FLUSH); } A { /* Ampere. */ types[WCSUNITS_CHARGE] += 1.0; types[WCSUNITS_TIME] -= 1.0; BEGIN(EXPON); } a|yr { /* Year (annum). */ factor *= 31557600.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } adu { /* Analogue-to-digital converter units. */ types[WCSUNITS_COUNT] += 1.0; BEGIN(EXPON); } [Aa]ngstrom { /* Angstrom. */ factor *= 1e-10; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } arcmin { /* Minute of arc. */ factor /= 60.0; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } arcsec { /* Second of arc. */ factor /= 3600.0; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } AU { /* Astronomical unit. */ factor *= 1.49598e+11; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } barn { /* Barn. */ factor *= 1e-28; types[WCSUNITS_LENGTH] += 2.0; BEGIN(EXPON); } beam { /* Beam, as in Jy/beam. */ types[WCSUNITS_BEAM] += 1.0; BEGIN(EXPON); } bin { /* Bin (e.g. histogram). */ types[WCSUNITS_BIN] += 1.0; BEGIN(EXPON); } bit { /* Bit. */ types[WCSUNITS_BIT] += 1.0; BEGIN(EXPON); } [bB]yte { /* Byte. */ factor *= 8.0; types[WCSUNITS_BIT] += 1.0; BEGIN(EXPON); } C { /* Coulomb. */ types[WCSUNITS_CHARGE] += 1.0; BEGIN(EXPON); } cd { /* Candela. */ types[WCSUNITS_LUMINTEN] += 1.0; BEGIN(EXPON); } chan { /* Channel. */ types[WCSUNITS_BIN] += 1.0; BEGIN(EXPON); } count|ct { /* Count. */ types[WCSUNITS_COUNT] += 1.0; BEGIN(EXPON); } D { /* Debye. */ factor *= 1e-29 / 3.0; types[WCSUNITS_CHARGE] += 1.0; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } d { /* Day. */ factor *= 86400.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } deg { /* Degree. */ types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } erg { /* Erg. */ factor *= 1e-7; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } eV { /* Electron volt. */ factor *= 1.6021765e-19; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } F { /* Farad. */ types[WCSUNITS_MASS] -= 1.0; types[WCSUNITS_LENGTH] -= 2.0; types[WCSUNITS_TIME] += 3.0; types[WCSUNITS_CHARGE] += 2.0; BEGIN(EXPON); } G { /* Gauss. */ factor *= 1e-4; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } g { /* Gram. */ factor *= 1e-3; types[WCSUNITS_MASS] += 1.0; BEGIN(EXPON); } H { /* Henry. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] += 2.0; types[WCSUNITS_CHARGE] -= 2.0; BEGIN(EXPON); } h { /* Hour. */ factor *= 3600.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } Hz { /* Hertz. */ types[WCSUNITS_TIME] -= 1.0; BEGIN(EXPON); } J { /* Joule. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } Jy { /* Jansky. */ factor *= 1e-26; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } K { /* Kelvin. */ types[WCSUNITS_TEMPERATURE] += 1.0; BEGIN(EXPON); } lm { /* Lumen. */ types[WCSUNITS_LUMINTEN] += 1.0; types[WCSUNITS_SOLID_ANGLE] += 1.0; BEGIN(EXPON); } lx { /* Lux. */ types[WCSUNITS_LUMINTEN] += 1.0; types[WCSUNITS_SOLID_ANGLE] += 1.0; types[WCSUNITS_LENGTH] -= 2.0; BEGIN(EXPON); } lyr { /* Light year. */ factor *= 2.99792458e8 * 31557600.0; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } m { /* Metre. */ types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } mag { /* Stellar magnitude. */ types[WCSUNITS_MAGNITUDE] += 1.0; BEGIN(EXPON); } mas { /* Milli-arcsec. */ factor /= 3600e+3; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } min { /* Minute. */ factor *= 60.0; types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } mol { /* Mole. */ types[WCSUNITS_MOLE] += 1.0; BEGIN(EXPON); } N { /* Newton. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 1.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } [Oo]hm { /* Ohm. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 1.0; types[WCSUNITS_CHARGE] -= 2.0; BEGIN(EXPON); } Pa { /* Pascal. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] -= 1.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } pc { /* Parsec. */ factor *= 3.0857e16; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } photon|ph { /* Photon. */ types[WCSUNITS_COUNT] += 1.0; BEGIN(EXPON); } pixel|pix { /* Pixel. */ types[WCSUNITS_PIXEL] += 1.0; BEGIN(EXPON); } R { /* Rayleigh. */ factor *= 1e10 / (4.0 * PI); types[WCSUNITS_LENGTH] -= 2.0; types[WCSUNITS_TIME] -= 1.0; types[WCSUNITS_SOLID_ANGLE] -= 1.0; BEGIN(EXPON); } rad { /* Radian. */ factor *= 180.0 / PI; types[WCSUNITS_PLANE_ANGLE] += 1.0; BEGIN(EXPON); } Ry { /* Rydberg. */ factor *= 13.605692 * 1.6021765e-19; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 2.0; BEGIN(EXPON); } S { /* Siemen. */ types[WCSUNITS_MASS] -= 1.0; types[WCSUNITS_LENGTH] -= 2.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] += 2.0; BEGIN(EXPON); } s { /* Second. */ types[WCSUNITS_TIME] += 1.0; BEGIN(EXPON); } solLum { /* Solar luminosity. */ factor *= 3.8268e26; types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 3.0; BEGIN(EXPON); } solMass { /* Solar mass. */ factor *= 1.9891e30; types[WCSUNITS_MASS] += 1.0; BEGIN(EXPON); } solRad { /* Solar radius. */ factor *= 6.9599e8; types[WCSUNITS_LENGTH] += 1.0; BEGIN(EXPON); } sr { /* Steradian. */ types[WCSUNITS_SOLID_ANGLE] += 1.0; BEGIN(EXPON); } Sun { /* Sun (with respect to). */ types[WCSUNITS_SOLRATIO] += 1.0; BEGIN(EXPON); } T { /* Tesla. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } u { /* Unified atomic mass unit. */ factor *= 1.6605387e-27; types[WCSUNITS_MASS] += 1.0; BEGIN(EXPON); } V { /* Volt. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 1.0; types[WCSUNITS_TIME] -= 2.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } voxel { /* Voxel. */ types[WCSUNITS_VOXEL] += 1.0; BEGIN(EXPON); } W { /* Watt. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] -= 3.0; BEGIN(EXPON); } Wb { /* Weber. */ types[WCSUNITS_MASS] += 1.0; types[WCSUNITS_LENGTH] += 2.0; types[WCSUNITS_TIME] += 1.0; types[WCSUNITS_CHARGE] -= 1.0; BEGIN(EXPON); } . { /* Internal parser error. */ status = wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error parsing '%s'", unitstr); BEGIN(FLUSH); } " "*("**"|^) { /* Exponentiation. */ if (operator++) { BEGIN(FLUSH); } } " "*{INTEGER} { sscanf(yytext, " %d", &i); expon *= (double)i; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } " "*"("" "*{INTEGER}" "*")" { sscanf(yytext, " (%d)", &i); expon *= (double)i; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } " "*"("" "*{FRAC}" "*")" { sscanf(yytext, " (%d/%d)", &i, &j); expon *= (double)i / (double)j; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } " "*"("" "*{FLOAT}" "*")" { sscanf(yytext, " (%lf)", &dexp); expon *= dexp; add(&factor, types, &expon, scale, units); operator = 0; BEGIN(INITIAL); } " "*[.*]" "* { /* Multiply. */ if (operator++) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); BEGIN(INITIAL); } } " "*"(" { /* Multiply. */ if (operator) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); unput('('); BEGIN(INITIAL); } } " "+ { /* Multiply. */ if (operator) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); BEGIN(INITIAL); } } " "*"/"" "* { /* Divide. */ if (operator++) { BEGIN(FLUSH); } else { add(&factor, types, &expon, scale, units); expon = -1.0; BEGIN(INITIAL); } } " "*"]" { add(&factor, types, &expon, scale, units); bracket = !bracket; BEGIN(FLUSH); } . { status = wcserr_set(WCSERR_SET(UNITSERR_BAD_EXPON_SYMBOL), "Invalid symbol in EXPON context in '%s'", unitstr); BEGIN(FLUSH); } .* { /* Discard any remaining input. */ } <> { /* End-of-string. */ if (YY_START == EXPON) { add(&factor, types, &expon, scale, units); } yylex_destroy(); if (bracket) { status = wcserr_set(WCSERR_SET(UNITSERR_UNBAL_BRACKET), "Unbalanced bracket in '%s'", unitstr); } else if (paren) { status = wcserr_set(WCSERR_SET(UNITSERR_UNBAL_PAREN), "Unbalanced parenthesis in '%s'", unitstr); } else if (operator == 1) { status = wcserr_set(WCSERR_SET(UNITSERR_DANGLING_BINOP), "Dangling binary operator in '%s'", unitstr); } else if (operator) { status = wcserr_set(WCSERR_SET(UNITSERR_CONSEC_BINOPS), "Consecutive binary operators in '%s'", unitstr); #ifdef DEBUG } else { fprintf(stderr, "EOS\n"); #endif } if (status) { for (i = 0; i < WCSUNITS_NTYPE; i++) { units[i] = 0.0; *scale = 0.0; } } return status; } %% /*---------------------------------------------------------------------------- * Accumulate a term in a units specification and reset work variables. *---------------------------------------------------------------------------*/ void add( double *factor, double types[], double *expon, double *scale, double units[]) { int i; *scale *= pow(*factor, *expon); for (i = 0; i < WCSUNITS_NTYPE; i++) { units[i] += *expon * types[i]; types[i] = 0.0; } *expon = 1.0; *factor = 1.0; return; } pywcs-1.12/wcslib/C/wcsunits.c0000644001153600020070000001306312310355626020341 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsunits.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include "wcsunits.h" /* Map status return value to message. */ const char *wcsunits_errmsg[] = { "Success", "Invalid numeric multiplier", "Dangling binary operator", "Invalid symbol in INITIAL context", "Function in invalid context", "Invalid symbol in EXPON context", "Unbalanced bracket", "Unbalanced parenthesis", "Consecutive binary operators", "Internal parser error", "Non-conformant unit specifications", "Non-conformant functions", "Potentially unsafe translation"}; /* Unit types. */ const char *wcsunits_types[] = { "plane angle", "solid angle", "charge", "mole", "temperature", "luminous intensity", "mass", "length", "time", "beam", "bin", "bit", "count", "stellar magnitude", "pixel", "solar ratio", "voxel"}; const char *wcsunits_units[] = { "degree", "steradian", "Coulomb", "mole", "Kelvin", "candela", "kilogram", "metre", "second", "", "", "", "", "", "", "", ""}; const char *wcsunits_funcs[] = { "none", "log", "ln", "exp"}; /*--------------------------------------------------------------------------*/ int wcsunits( const char have[], const char want[], double *scale, double *offset, double *power) { return wcsunitse( have, want, scale, offset, power, 0x0); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int wcsunitse( const char have[], const char want[], double *scale, double *offset, double *power, struct wcserr **err) { static const char *function = "wcsunitse"; int func1, func2, i, status; double scale1, scale2, units1[WCSUNITS_NTYPE], units2[WCSUNITS_NTYPE]; if ((status = wcsulexe(have, &func1, &scale1, units1, err))) { return status; } if ((status = wcsulexe(want, &func2, &scale2, units2, err))) { return status; } /* Check conformance. */ for (i = 0; i < WCSUNITS_NTYPE; i++) { if (units1[i] != units2[i]) { return wcserr_set(WCSERR_SET(UNITSERR_BAD_UNIT_SPEC), "Mismatched units type '%s': have '%s', want '%s'", wcsunits_types[i], have, want); } } *scale = 0.0; *offset = 0.0; *power = 1.0; switch (func1) { case 0: /* No function. */ if (func2) { return wcserr_set(WCSERR_SET(UNITSERR_BAD_FUNCS), "Mismatched unit functions: have '%s' (%s), want '%s' (%s)", have, wcsunits_funcs[func1], want, wcsunits_funcs[func2]); } *scale = scale1 / scale2; break; case 1: /* log(). */ if (func2 == 1) { /* log(). */ *scale = 1.0; *offset = log10(scale1 / scale2); } else if (func2 == 2) { /* ln(). */ *scale = log(10.0); *offset = log(scale1 / scale2); } else { return wcserr_set(WCSERR_SET(UNITSERR_BAD_FUNCS), "Mismatched unit functions: have '%s' (%s), want '%s' (%s)", have, wcsunits_funcs[func1], want, wcsunits_funcs[func2]); } break; case 2: /* ln(). */ if (func2 == 1) { /* log(). */ *scale = 1.0 / log(10.0); *offset = log(scale1 / scale2); } else if (func2 == 2) { /* ln(). */ *scale = 1.0; *offset = log(scale1 / scale2); } else { return wcserr_set(WCSERR_SET(UNITSERR_BAD_FUNCS), "Mismatched unit functions: have '%s' (%s), want '%s' (%s)", have, wcsunits_funcs[func1], want, wcsunits_funcs[func2]); } break; case 3: /* exp(). */ if (func2 != 3) { return wcserr_set(WCSERR_SET(UNITSERR_BAD_FUNCS), "Mismatched unit functions: have '%s' (%s), want '%s' (%s)", have, wcsunits_funcs[func1], want, wcsunits_funcs[func2]); } *scale = 1.0; *power = scale1 / scale2; break; default: /* Internal parser error. */ return wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units parser error"); } return 0; } /*--------------------------------------------------------------------------*/ int wcsutrn(int ctrl, char unitstr[]) { return wcsutrne(ctrl, unitstr, 0x0); } /*--------------------------------------------------------------------------*/ int wcsulex(const char unitstr[], int *func, double *scale, double units[]) { return wcsulexe(unitstr, func, scale, units, 0x0); } pywcs-1.12/wcslib/C/wcsunits.h0000644001153600020070000004114612310355626020351 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsunits.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * WCSLIB 4.10 - C routines that implement the FITS World Coordinate System * (WCS) standard. Refer to * * "Representations of world coordinates in FITS", * Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061 (Paper I) * * The Flexible Image Transport System (FITS), a data format widely used in * astronomy for data interchange and archive, is described in * * "Definition of The Flexible Image Transport System (FITS)", * Hanisch, R.J., Farris, A., Greisen, E.W., et al. 2001, A&A, 376, 359 * * which formalizes NOST 100-2.0, a document produced by the NASA/Science * Office of Standards and Technology, see http://fits.gsfc.nasa.gov. * * Refer to the README file provided with WCSLIB for an overview of the * library. * * * Summary of the wcsunits routines * -------------------------------- * Routines in this suite deal with units specifications and conversions: * * - wcsunitse(): given two unit specifications, derive the conversion from * one to the other. * * - wcsutrne(): translates certain commonly used but non-standard unit * strings. It is intended to be called before wcsulexe() which only * handles standard FITS units specifications. * * - wcsulexe(): parses a standard FITS units specification of arbitrary * complexity, deriving the conversion to canonical units. * * * wcsunitse() - FITS units specification conversion * ------------------------------------------------- * wcsunitse() derives the conversion from one system of units to another. * * A deprecated form of this function, wcsunits(), lacks the wcserr** * parameter. * * Given: * have const char [] * FITS units specification to convert from (null- * terminated), with or without surrounding square * brackets (for inline specifications); text following * the closing bracket is ignored. * * want const char [] * FITS units specification to convert to (null- * terminated), with or without surrounding square * brackets (for inline specifications); text following * the closing bracket is ignored. * * Returned: * scale, * offset, * power double* Convert units using * = pow(scale*value + offset, power); * * Normally offset is zero except for log() or ln() * conversions, e.g. "log(MHz)" to "ln(Hz)". Likewise, * power is normally unity except for exp() conversions, * e.g. "exp(ms)" to "exp(/Hz)". Thus conversions * ordinarily consist of * = value *= scale; * * err struct wcserr ** * If enabled, for function return values > 1, this * struct will contain a detailed error message, see * wcserr_enable(). May be NULL if an error message is * not desired. * * Function return value: * int Status return value: * 0: Success. * 1-9: Status return from wcsulexe(). * 10: Non-conformant unit specifications. * 11: Non-conformant functions. * * scale is zeroed on return if an error occurs. * * * wcsutrne() - Translation of non-standard unit specifications * ------------------------------------------------------------ * wcsutrne() translates certain commonly used but non-standard unit strings, * e.g. "DEG", "MHZ", "KELVIN", that are not recognized by wcsulexe(), refer to * the notes below for a full list. Compounds are also recognized, e.g. * "JY/BEAM" and "KM/SEC/SEC". Extraneous embedded blanks are removed. * * A deprecated form of this function, wcsutrn(), lacks the wcserr** parameter. * * Given: * ctrl int Although "S" is commonly used to represent seconds, * its translation to "s" is potentially unsafe since the * standard recognizes "S" formally as Siemens, however * rarely that may be used. The same applies to "H" for * hours (Henry), and "D" for days (Debye). This * bit-flag controls what to do in such cases: * 1: Translate "S" to "s". * 2: Translate "H" to "h". * 4: Translate "D" to "d". * Thus ctrl == 0 doesn't do any unsafe translations, * whereas ctrl == 7 does all of them. * * Given and returned: * unitstr char [] Null-terminated character array containing the units * specification to be translated. * * Inline units specifications in the a FITS header * keycomment are also handled. If the first non-blank * character in unitstr is '[' then the unit string is * delimited by its matching ']'. Blanks preceding '[' * will be stripped off, but text following the closing * bracket will be preserved without modification. * * err struct wcserr ** * If enabled, for function return values > 1, this * struct will contain a detailed error message, see * wcserr_enable(). May be NULL if an error message is * not desired. * * Function return value: * int Status return value: * -1: No change was made, other than stripping blanks * (not an error). * 0: Success. * 9: Internal parser error. * 12: Potentially unsafe translation, whether applied * or not (see notes). * * Notes: * Translation of non-standard unit specifications: apart from leading and * trailing blanks, a case-sensitive match is required for the aliases listed * below, in particular the only recognized aliases with metric prefixes are * "KM", "KHZ", "MHZ", and "GHZ". Potentially unsafe translations of "D", * "H", and "S", shown in parentheses, are optional. * = Unit Recognized aliases = ---- ------------------------------------------------------------- = Angstrom angstrom = arcmin arcmins, ARCMIN, ARCMINS = arcsec arcsecs, ARCSEC, ARCSECS = beam BEAM = byte Byte = d day, days, (D), DAY, DAYS = deg degree, degrees, DEG, DEGREE, DEGREES = GHz GHZ = h hr, (H), HR = Hz hz, HZ = kHz KHZ = Jy JY = K kelvin, kelvins, Kelvin, Kelvins, KELVIN, KELVINS = km KM = m metre, meter, metres, meters, M, METRE, METER, METRES, METERS = min MIN = MHz MHZ = Ohm ohm = Pa pascal, pascals, Pascal, Pascals, PASCAL, PASCALS = pixel pixels, PIXEL, PIXELS = rad radian, radians, RAD, RADIAN, RADIANS = s sec, second, seconds, (S), SEC, SECOND, SECONDS = V volt, volts, Volt, Volts, VOLT, VOLTS = yr year, years, YR, YEAR, YEARS * * The aliases "angstrom", "ohm", and "Byte" for (Angstrom, Ohm, and byte) * are recognized by wcsulexe() itself as an unofficial extension of the * standard, but they are converted to the standard form here. * * * wcsulexe() - FITS units specification parser * -------------------------------------------- * wcsulexe() parses a standard FITS units specification of arbitrary * complexity, deriving the scale factor required to convert to canonical * units - basically SI with degrees and "dimensionless" additions such as * byte, pixel and count. * * A deprecated form of this function, wcsulex(), lacks the wcserr** parameter. * * Given: * unitstr const char [] * Null-terminated character array containing the units * specification, with or without surrounding square * brackets (for inline specifications); text following * the closing bracket is ignored. * * Returned: * func int* Special function type, see note 4: * 0: None * 1: log() ...base 10 * 2: ln() ...base e * 3: exp() * * scale double* Scale factor for the unit specification; multiply a * value expressed in the given units by this factor to * convert it to canonical units. * * units double[WCSUNITS_NTYPE] * A units specification is decomposed into powers of 16 * fundamental unit types: angle, mass, length, time, * count, pixel, etc. Preprocessor macro WCSUNITS_NTYPE * is defined to dimension this vector, and others such * WCSUNITS_PLANE_ANGLE, WCSUNITS_LENGTH, etc. to access * its elements. * * Corresponding character strings, wcsunits_types[] and * wcsunits_units[], are predefined to describe each * quantity and its canonical units. * * err struct wcserr ** * If enabled, for function return values > 1, this * struct will contain a detailed error message, see * wcserr_enable(). May be NULL if an error message is * not desired. * * Function return value: * int Status return value: * 0: Success. * 1: Invalid numeric multiplier. * 2: Dangling binary operator. * 3: Invalid symbol in INITIAL context. * 4: Function in invalid context. * 5: Invalid symbol in EXPON context. * 6: Unbalanced bracket. * 7: Unbalanced parenthesis. * 8: Consecutive binary operators. * 9: Internal parser error. * * scale and units[] are zeroed on return if an error * occurs. * * Notes: * 1: wcsulexe() is permissive in accepting whitespace in all contexts in a * units specification where it does not create ambiguity (e.g. not * between a metric prefix and a basic unit string), including in strings * like "log (m ** 2)" which is formally disallowed. * * 2: Supported extensions: * - "angstrom" (OGIP usage) is allowed in addition to "Angstrom". * - "ohm" (OGIP usage) is allowed in addition to "Ohm". * - "Byte" (common usage) is allowed in addition to "byte". * * 3: Table 6 of WCS Paper I lists eleven units for which metric prefixes are * allowed. However, in this implementation only prefixes greater than * unity are allowed for "a" (annum), "yr" (year), "pc" (parsec), "bit", * and "byte", and only prefixes less than unity are allowed for "mag" * (stellar magnitude). * * Metric prefix "P" (peta) is specifically forbidden for "a" (annum) to * avoid confusion with "Pa" (Pascal, not peta-annum). Note that metric * prefixes are specifically disallowed for "h" (hour) and "d" (day) so * that "ph" (photons) cannot be interpreted as pico-hours, nor "cd" * (candela) as centi-days. * * 4: Function types log(), ln() and exp() may only occur at the start of the * units specification. The scale and units[] returned for these refers * to the string inside the function "argument", e.g. to "MHz" in log(MHz) * for which a scale of 1e6 will be returned. * * * Global variable: const char *wcsunits_errmsg[] - Status return messages * ----------------------------------------------------------------------- * Error messages to match the status value returned from each function. * * * Global variable: const char *wcsunits_types[] - Names of physical quantities * ---------------------------------------------------------------------------- * Names for physical quantities to match the units vector returned by * wcsulexe(): * - 0: plane angle * - 1: solid angle * - 2: charge * - 3: mole * - 4: temperature * - 5: luminous intensity * - 6: mass * - 7: length * - 8: time * - 9: beam * - 10: bin * - 11: bit * - 12: count * - 13: stellar magnitude * - 14: pixel * - 15: solar ratio * - 16: voxel * * * Global variable: const char *wcsunits_units[] - Names of units * -------------------------------------------------------------- * Names for the units (SI) to match the units vector returned by wcsulexe(): * - 0: degree * - 1: steradian * - 2: Coulomb * - 3: mole * - 4: Kelvin * - 5: candela * - 6: kilogram * - 7: metre * - 8: second * * The remainder are dimensionless. *===========================================================================*/ #ifndef WCSLIB_WCSUNITS #define WCSLIB_WCSUNITS #include "wcserr.h" #ifdef __cplusplus extern "C" { #endif extern const char *wcsunits_errmsg[]; enum wcsunits_errmsg_enum { UNITSERR_SUCCESS = 0, /* Success. */ UNITSERR_BAD_NUM_MULTIPLIER = 1, /* Invalid numeric multiplier. */ UNITSERR_DANGLING_BINOP = 2, /* Dangling binary operator. */ UNITSERR_BAD_INITIAL_SYMBOL = 3, /* Invalid symbol in INITIAL context. */ UNITSERR_FUNCTION_CONTEXT = 4, /* Function in invalid context. */ UNITSERR_BAD_EXPON_SYMBOL = 5, /* Invalid symbol in EXPON context. */ UNITSERR_UNBAL_BRACKET = 6, /* Unbalanced bracket. */ UNITSERR_UNBAL_PAREN = 7, /* Unbalanced parenthesis. */ UNITSERR_CONSEC_BINOPS = 8, /* Consecutive binary operators. */ UNITSERR_PARSER_ERROR = 9, /* Internal parser error. */ UNITSERR_BAD_UNIT_SPEC = 10, /* Non-conformant unit specifications. */ UNITSERR_BAD_FUNCS = 11, /* Non-conformant functions. */ UNITSERR_UNSAFE_TRANS = 12 /* Potentially unsafe translation. */ }; extern const char *wcsunits_types[]; extern const char *wcsunits_units[]; #define WCSUNITS_PLANE_ANGLE 0 #define WCSUNITS_SOLID_ANGLE 1 #define WCSUNITS_CHARGE 2 #define WCSUNITS_MOLE 3 #define WCSUNITS_TEMPERATURE 4 #define WCSUNITS_LUMINTEN 5 #define WCSUNITS_MASS 6 #define WCSUNITS_LENGTH 7 #define WCSUNITS_TIME 8 #define WCSUNITS_BEAM 9 #define WCSUNITS_BIN 10 #define WCSUNITS_BIT 11 #define WCSUNITS_COUNT 12 #define WCSUNITS_MAGNITUDE 13 #define WCSUNITS_PIXEL 14 #define WCSUNITS_SOLRATIO 15 #define WCSUNITS_VOXEL 16 #define WCSUNITS_NTYPE 17 int wcsunitse(const char have[], const char want[], double *scale, double *offset, double *power, struct wcserr **err); int wcsutrne(int ctrl, char unitstr[], struct wcserr **err); int wcsulexe(const char unitstr[], int *func, double *scale, double units[], struct wcserr **err); /* Deprecated. */ int wcsunits(const char have[], const char want[], double *scale, double *offset, double *power); int wcsutrn(int ctrl, char unitstr[]); int wcsulex(const char unitstr[], int *func, double *scale, double units[]); #ifdef __cplusplus } #endif #endif /* WCSLIB_WCSUNITS */ pywcs-1.12/wcslib/C/wcsutil.c0000644001153600020070000001020212310355626020144 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsutil.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include "wcsutil.h" /*--------------------------------------------------------------------------*/ void wcsutil_blank_fill(int n, char c[]) { int k; for (k = strlen(c); k < n; k++) { c[k] = ' '; } return; } /*--------------------------------------------------------------------------*/ void wcsutil_null_fill(int n, char c[]) { int j, k; if (n <= 0) return; /* Null-fill the string. */ *(c+n-1) = '\0'; for (j = 0; j < n; j++) { if (c[j] == '\0') { for (k = j+1; k < n; k++) { c[k] = '\0'; } break; } } for (k = j-1; k > 0; k--) { if (c[k] != ' ') break; c[k] = '\0'; } return; } /*--------------------------------------------------------------------------*/ int wcsutil_allEq(int nvec, int nelem, const double *first) { double v0; const double *vp; if (nvec <= 0 || nelem <= 0) return 0; v0 = *first; for (vp = first+nelem; vp < first + nvec*nelem; vp += nelem) { if (*vp != v0) return 0; } return 1; } /*--------------------------------------------------------------------------*/ void wcsutil_setAll(int nvec, int nelem, double *first) { double v0, *vp; if (nvec <= 0 || nelem <= 0) return; v0 = *first; for (vp = first+nelem; vp < first + nvec*nelem; vp += nelem) { *vp = v0; } } /*--------------------------------------------------------------------------*/ void wcsutil_setAli(int nvec, int nelem, int *first) { int v0, *vp; if (nvec <= 0 || nelem <= 0) return; v0 = *first; for (vp = first+nelem; vp < first + nvec*nelem; vp += nelem) { *vp = v0; } } /*--------------------------------------------------------------------------*/ void wcsutil_setBit(int nelem, const int *sel, int bits, int *array) { int *arrp; if (bits == 0 || nelem <= 0) return; if (sel == 0x0) { /* All elements selected. */ for (arrp = array; arrp < array + nelem; arrp++) { *arrp |= bits; } } else { /* Some elements selected. */ for (arrp = array; arrp < array + nelem; arrp++) { if (*(sel++)) *arrp |= bits; } } } /*--------------------------------------------------------------------------*/ char *wcsutil_fptr2str(int (*func)(), char hext[]) { unsigned char *p = (unsigned char *)(&func); char *t = hext; int i, *(ip[2]), j[2], le = 1, gotone = 0; /* Test for little-endian addresses. */ ip[0] = j; ip[1] = j + 1; if ((unsigned char *)ip[0] < (unsigned char *)ip[1]) { /* Little-endian, reverse it. */ p += sizeof(func) - 1; le = -1; } sprintf(t, "0x0"); t += 2; for (i = 0; i < sizeof(func); i++) { /* Skip leading zeroes. */ if (*p) gotone = 1; if (gotone) { sprintf(t, "%02x", *p); t += 2; } p += le; } return hext; } pywcs-1.12/wcslib/C/wcsutil.h0000644001153600020070000001702512310355626020163 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsutil.h,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * Summary of the wcsutil routines * ------------------------------- * Simple utility functions for internal use only by WCSLIB. They are * documented here solely as an aid to understanding the code. They are not * intended for external use - the API may change without notice! * * * wcsutil_blank_fill() - Fill a character string with blanks * ---------------------------------------------------------- * INTERNAL USE ONLY. * * wcsutil_blank_fill() pads a character string with blanks starting with the * terminating NULL character. * * Used by the Fortran wrapper functions in translating C character strings * into Fortran CHARACTER variables. * * Given: * n int Length of the character array, c[]. * * Given and returned: * c char[] The character string. It will not be null-terminated * on return. * * Function return value: * void * * * wcsutil_null_fill() - Fill a character string with NULLs * -------------------------------------------------------- * INTERNAL USE ONLY. * * wcsutil_null_fill() strips off trailing blanks and pads the character array * holding the string with NULL characters. * * Used mainly to make character strings intelligible in the GNU debugger which * prints the rubbish following the terminating NULL, obscuring the valid part * of the string. * * Given: * n int Number of characters. * * Given and returned: * c char[] The character string. * * Function return value: * void * * * wcsutil_allEq() - Test for equality of a particular vector element * ------------------------------------------------------------------ * INTERNAL USE ONLY. * * wcsutil_allEq() tests for equality of a particular element in a set of * vectors. * * Given: * nvec int The number of vectors. * * nelem int The length of each vector. * * first const double* * Pointer to the first element to test in the array. * The elements tested for equality are * = *first == *(first + nelem) = == *(first + nelem*2) = : = == *(first + nelem*(nvec-1)); * * The array might be dimensioned as * = double v[nvec][nelem]; * * Function return value: * int Status return value: * 0: Not all equal. * 1: All equal. * * * wcsutil_setAll() - Set a particular vector element * -------------------------------------------------- * INTERNAL USE ONLY. * * wcsutil_setAll() sets the value of a particular element in a set of vectors. * * Given: * nvec int The number of vectors. * * nelem int The length of each vector. * * Given and returned: * first double* Pointer to the first element in the array, the value * of which is used to set the others * = *(first + nelem) = *first; = *(first + nelem*2) = *first; = : = *(first + nelem*(nvec-1)) = *first; * * The array might be dimensioned as * = double v[nvec][nelem]; * * Function return value: * void * * * wcsutil_setAli() - Set a particular vector element * -------------------------------------------------- * INTERNAL USE ONLY. * * wcsutil_setAli() sets the value of a particular element in a set of vectors. * * Given: * nvec int The number of vectors. * * nelem int The length of each vector. * * Given and returned: * first int* Pointer to the first element in the array, the value * of which is used to set the others * = *(first + nelem) = *first; = *(first + nelem*2) = *first; = : = *(first + nelem*(nvec-1)) = *first; * * The array might be dimensioned as * = int v[nvec][nelem]; * * Function return value: * void * * * wcsutil_setBit() - Set bits in selected elements of an array * ------------------------------------------------------------ * INTERNAL USE ONLY. * * wcsutil_setBit() sets bits in selected elements of an array. * * Given: * nelem int Number of elements in the array. * * sel const int* * Address of a selection array of length nelem. May * be specified as the null pointer in which case all * elements are selected. * * bits int Bit mask. * * Given and returned: * array int* Address of the array of length nelem. * * Function return value: * void * * * wcsutil_fptr2str() - Translate pointer-to-function to string * ------------------------------------------------------------ * INTERNAL USE ONLY. * * wcsutil_fptr2str() translates a pointer-to-function to hexadecimal string * representation for output. It is used by the various routines that print * the contents of WCSLIB structs. Note that it is not strictly legal to * type-pun a function pointer to void*. * * See stackoverflow.com/questions/2741683/how-to-format-a-function-pointer * * Given: * fptr int (*)() Pointer to function. * * Returned: * hext char[] Null-terminated string. Should be at least 19 bytes * in size to accomodate a 64-bit address (16 bytes in * hex), plus the leading "0x" and trailing '\0'. * * Function return value: * char * The address of hext. * *===========================================================================*/ #ifndef WCSLIB_WCSUTIL #define WCSLIB_WCSUTIL void wcsutil_blank_fill(int n, char c[]); void wcsutil_null_fill (int n, char c[]); int wcsutil_allEq (int nvec, int nelem, const double *first); void wcsutil_setAll(int nvec, int nelem, double *first); void wcsutil_setAli(int nvec, int nelem, int *first); void wcsutil_setBit(int nelem, const int *sel, int bits, int *array); char *wcsutil_fptr2str(int (*func)(), char hext[]); #endif /* WCSLIB_WCSUTIL */ pywcs-1.12/wcslib/C/wcsutrn.l0000644001153600020070000001506512310355626020204 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsutrn.l,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *============================================================================= * * wcsutrn.l is a Flex description file containing the definition of a lexical * scanner that translates non-standard FITS units specifications. * * It requires Flex v2.5.4 or later. * * Refer to wcsunits.h for a description of the user interface and operating * notes. * *===========================================================================*/ /* Options. */ %option full %option never-interactive %option noyywrap %option outfile="wcsutrn.c" %option prefix="wcsutrn" /* Exclusive start states. */ %x NEXT FLUSH %{ /* To get the prototype for fileno() from stdio.h when gcc is invoked with * -std=c89 (same as -ansi) or -std=c99 since we do not define YY_INPUT. */ #define _POSIX_SOURCE 1 #include #include #include #include #include "wcserr.h" #include "wcsunits.h" #define YY_DECL int wcsutrne(int ctrl, char unitstr[], struct wcserr **err) /* Used in preempting the call to exit() by yy_fatal_error(). */ jmp_buf wcsutrn_abort_jmp_env; #define exit(status) longjmp(wcsutrn_abort_jmp_env, status) %} %% static const char *function = "wcsutrne"; char orig[80], subs[80]; int bracket = 0; int unsafe = 0; int status = -1; YY_BUFFER_STATE inbuff; int yylex_destroy(void); *orig = '\0'; *subs = '\0'; inbuff = yy_scan_string(unitstr); *unitstr = '\0'; /* Return here via longjmp() invoked by yy_fatal_error(). */ if (setjmp(wcsutrn_abort_jmp_env)) { return wcserr_set(WCSERR_SET(UNITSERR_PARSER_ERROR), "Internal units translator error parsing '%s'", unitstr); } BEGIN(INITIAL); #ifdef DEBUG fprintf(stderr, "\n%s ->\n", unitstr); #endif ^" "*"[" { /* Looks like a keycomment. */ strcat(unitstr, "["); bracket = 1; } " "+ /* Discard leading whitespace. */ [^A-Za-z] { /* Non-alphabetic character. */ strcat(unitstr, yytext); if (bracket && *yytext == ']') { BEGIN(FLUSH); } } angstrom { strcpy(orig, yytext); strcpy(subs, "Angstrom"); BEGIN(NEXT); } arcmins|ARCMINS? { strcpy(orig, yytext); strcpy(subs, "arcmin"); BEGIN(NEXT); } arcsecs|ARCSECS? { strcpy(orig, yytext); strcpy(subs, "arcsec"); BEGIN(NEXT); } BEAM { strcpy(orig, yytext); strcpy(subs, "beam"); BEGIN(NEXT); } Byte { strcpy(orig, yytext); strcpy(subs, "byte"); BEGIN(NEXT); } days?|DAYS? { strcpy(orig, yytext); strcpy(subs, "d"); BEGIN(NEXT); } D { unsafe = 1; strcpy(orig, yytext); strcpy(subs, (ctrl & 4) ? "d" : "D"); BEGIN(NEXT); } degrees?|DEG|DEGREES? { strcpy(orig, yytext); strcpy(subs, "deg"); BEGIN(NEXT); } GHZ { strcpy(orig, yytext); strcpy(subs, "GHz"); BEGIN(NEXT); } hr|HR { strcpy(orig, yytext); strcpy(subs, "h"); BEGIN(NEXT); } H { unsafe = 1; strcpy(orig, yytext); strcpy(subs, (ctrl & 2) ? "h" : "H"); BEGIN(NEXT); } hz|HZ { strcpy(orig, yytext); strcpy(subs, "Hz"); BEGIN(NEXT); } KHZ { strcpy(orig, yytext); strcpy(subs, "kHz"); BEGIN(NEXT); } JY { strcpy(orig, yytext); strcpy(subs, "Jy"); BEGIN(NEXT); } [kK]elvins?|KELVINS? { strcpy(orig, yytext); strcpy(subs, "K"); BEGIN(NEXT); } KM { strcpy(orig, yytext); strcpy(subs, "km"); BEGIN(NEXT); } metres?|meters?|M|METRES?|METERS? { strcpy(orig, yytext); strcpy(subs, "m"); BEGIN(NEXT); } MIN { strcpy(orig, yytext); strcpy(subs, "min"); BEGIN(NEXT); } MHZ { strcpy(orig, yytext); strcpy(subs, "MHz"); BEGIN(NEXT); } Ohm { strcpy(orig, yytext); strcpy(subs, "ohm"); BEGIN(NEXT); } [pP]ascals?|PASCALS? { strcpy(orig, yytext); strcpy(subs, "Pa"); BEGIN(NEXT); } pixels|PIXELS? { strcpy(orig, yytext); strcpy(subs, "pixel"); BEGIN(NEXT); } radians?|RAD|RADIANS? { strcpy(orig, yytext); strcpy(subs, "rad"); BEGIN(NEXT); } sec|seconds?|SEC|SECONDS? { strcpy(orig, yytext); strcpy(subs, "s"); BEGIN(NEXT); } S { unsafe = 1; strcpy(orig, yytext); strcpy(subs, (ctrl & 1) ? "s" : "S"); BEGIN(NEXT); } [vV]olts?|VOLTS? { strcpy(orig, yytext); strcpy(subs, "V"); BEGIN(NEXT); } years?|YR|YEARS? { strcpy(orig, yytext); strcpy(subs, "yr"); BEGIN(NEXT); } [A-Za-z]+ { /* Not a recognized alias. */ strcpy(orig, yytext); strcpy(subs, orig); BEGIN(NEXT); } [A-Za-z]+ { /* Reject the alias match. */ strcat(orig, yytext); strcpy(subs, orig); } " "+[^A-Za-z] { /* Discard separating whitespace. */ unput(yytext[yyleng-1]); } " "+[A-Za-z] { /* Compress separating whitespace. */ strcat(unitstr, subs); strcat(unitstr, " "); if (strcmp(orig, subs)) status = 0; unput(yytext[yyleng-1]); *subs = '\0'; BEGIN(INITIAL); } . { /* Copy anything else unchanged. */ strcat(unitstr, subs); if (strcmp(orig, subs)) status = 0; unput(*yytext); *subs = '\0'; BEGIN(INITIAL); } .* { /* Copy out remaining input. */ strcat(unitstr, yytext); } <> { /* End-of-string. */ if (*subs) { strcat(unitstr, subs); if (strcmp(orig, subs)) status = 0; } yylex_destroy(); if (unsafe) { return wcserr_set(WCSERR_SET(UNITSERR_UNSAFE_TRANS), "Unsafe unit translation in '%s'", unitstr); } return status; } %% pywcs-1.12/wcslib/CHANGES0000644001153600020070000020427412310355626017135 0ustar cslocumSTSCI\science00000000000000WCSLIB version 4.10 (2012/02/06) -------------------------------- * C library - datfix() and spcfix() now return informative messages when dates and AIPS-convention spectral axes are translated (changes contributed by Michael Droettboom). spcaips() now returns an error status for invalid values of VELREF. - wcssub() has been augmented with the ability to add new axes onto a wcsprm struct. WCSLIB version 4.9 (2012/01/24) ------------------------------- * C library - Fixes to wcsfixi() for collecting the messages properly in the info array (from Michael Droettboom). - Handle certain malformed date strings more gracefully in datfix(). - Make informative messages printed by wcserr_prt() a bit more informative. WCSLIB version 4.8.4 (2011/12/05) --------------------------------- * C library - Fixed the pseudo-random number generator in twcstab.c - gcc 4.6 with '-O2' baulked at testing for signed integer overflow. * Installation - In configure.ac, the Fortran compiler's libraries must be added to the link list when checking for the PGPLOT libraries since gcc is driving the linker. Likewise in C/GNUmakefile when linking test programs that use PGPLOT. - Use 'make CHECK=nopgplot check' to run only the non-graphical tests (even if PGPLOT is available). - After compiling and running the tests, 'make check' now summarizes the non-graphical test results and stops if any failed. WCSLIB version 4.8.3 (2011/11/17) --------------------------------- * C library - Minor generalization of the wcserr diagnostics to allow the return of informative messages which are associated with negative status values. wcserr_prt() will now recognize and print them as such. Added wcserr_clear() to reset (clear) a wcserr struct. - Modified unitfix() to return an informative message if a units alias is applied, and wcsfixi() to allow such messages to be propagated through the info array (from Michael Droettboom). - Modified twcsfix.c to use wcserr diagnostics, in particular to report units alias translations. * Fortran wrappers - In wcsfix_(), interpret *naxis == 0 as meaning naxis == 0x0, thus causing cylfix() to be skipped. - Modified twcsfix.f to reflect changes made to twcsfix.c. WCSLIB version 4.8.2 (2011/10/04) --------------------------------- * Installation - Changes for Debian package generation contributed by Ole Streicher: - Corrections to 'configure' reported by 'lintian'. - Generate man pages for the utility programs and install them. WCSLIB version 4.8.1 (2011/09/19) --------------------------------- * Installation - Set SONAME in the sharable library in accordance with tldp.org/HOWTO/Program-Library-HOWTO/shared-libraries.html (reported by Ole Streicher, Debian package maintainer). The sharable library will again be installed with full release number and with a symbolic link from SONAME pointing to it. If defined, SHRLN will point to SONAME. WCSLIB version 4.8 (2011/08/15) ------------------------------- * C library - New error diagnostics mechanism contributed by Michael Droettboom: Most functions that return a numeric status (error) code now also write a detailed error message to a wcserr struct attached to the passed-in *prm struct. See wcserr.h for more information. Functions that didn't have a *prm struct as an argument have no direct way to return an error message. Therefore, these functions now have duplicate versions with the suffix "e" that take an additional "struct wcserr *" parameter. These functions are: spcspx() -> spcspxe() spctrn() -> spctrne() spctyp() -> spctype() spcxps() -> spcxpse() wcsulex() -> wcsulexe() wcsunits() -> wcsunitse() wcsutrn() -> wcsutrne() A new function wcsfixi() was added which is identical to wcsfix() but in addition stores all of the detailed textual messages about the fixes that were performed. - In wcssub(), ensure that wcstab->m_tab has been initialized before trying to free it on status return 12 or 13 (reported by Hans Terlow). - Bug fixes: - In sphx2s() and sphs2x() for the case where |eul[1]| = 180.0. - For parsing AIPS-convention VELREF in wcsbth(). - In spcaips() for translating AIPS-convention CTYPEia without Doppler frame. - Non-graphical test programs now simply report "PASS" if they satisfy the reporting tolerance for closure residuals, etc. Their full output is reported otherwise. Run 'make MODE=interactive check' to revert to the previous behaviour of reporting the full output for tests that succeed. - Eliminated compiler warnings about type-punning of pointer-to- function. * Fortran wrappers Extensive modifications to track the new error handling mechanism in the C library. * Installation - configure now prefers gfortran over g77 if available. - Don't rely on "." being in the PATH if config.status needs to be run in the pgsbox and utils makefile (reported by Peter Teuben). WCSLIB version 4.7 (2011/02/07) ------------------------------- * C library - Bug fix in celset() for interpreting LATPOLEa when LONPOLEa = phi0. Crept in at version 4.4. - Fixed the bounds test on y in hpxx2s() (HEALPix projection) for unconventional values of H and K. In hpxx2s() and hpxs2x(), corrected the offset of the southern polar half-facets for even K. In hpxs2x(), put the phi = 180 meridian in the expected place. - Bug fixes in tabx2s() and tabs2x() for default indexes (reported by David Berry). In tabs2x(), if no solution is found then do minor extrapolation past the ends of each row (1-D case only). Sped up tabs2x() by about 50%. - New functions wcsprintf(), wcsprintf_set(), and wcsprintf_buf(), declared in wcsprintf.h, provide control over the disposition of output from celprt(), linprt(), prjprt(), spcprt(), tabprt(), and wcsprt() routines. Prompted by Michael Droettboom, with an initial implementation. * Fortran wrappers - In the various test programs, used EQUIVALENCEs to ensure that the CEL, LIN, PRJ, etc. arrays are aligned on a DOUBLE PRECISION boundary. * PGSBOX - Bug fix for the case where NG1 == 0 and GRID1(0) < 0, and likewise for NG2 and GRID2. * Utilities - In wcsware, added a '-w' option to convert world coordinates obtained from stdin to pixel coordinates using wcss2p(). Allow multiple sets of input coordinates with the '-x' and '-w' options and report the value of the intermediate world coordinates. * User manual - Fixed list formatting for function return values < 0 or > 9. - New section for wcsprintf() and related routines. * Installation - Changes prompted by Sébastien Fabbro for the Gentoo Linux package: a) autoconf updates, b) respect LDFLAGS when building the shared library, c) install documentation, d) recognise DESTDIR for doing a staged installation. - As of this release, the minor WCSLIB version number (second field) will be incremented if and only if a change is made that affects the library itself, not the documentation or utilities. The version number on the installed libraries and header files will omit the patch number (third field). WCSLIB version 4.6.3 (2010/11/24) --------------------------------- * C library - Bug fix in wcsbth() for handling the inheritance of image header keywords (uncovered by valgrind, reported by Jim Lewis). WCSLIB version 4.6.2 (2010/11/22) --------------------------------- * C library - Fixed a memory leak in wcsbth.l (reported by Jim Lewis). WCSLIB version 4.6.1 (2010/11/18) --------------------------------- * Fortran wrappers - Fixed typos in cel_f.c, celget[cdi] -> celgt[cdi]. WCSLIB version 4.6 (2010/11/16) ------------------------------- * C library - In wcsulex.l and wcsutrn.l, stdlib.h must be included explicitly before the redefinition of exit() - most versions of flex do include it upfront but some don't (reported by Peter Williams). * Fortran wrappers - Changes intended to avert nuisance compiler warnings that could potentially obscure warnings indicative of a genuine problem: - To stop messages about unused variables when the relevant compiler option is set, e.g. 'g77 -Wunused', the various *_ERRMSG arrays defined in the Fortran include files and (formerly) initialized therein via DATA statements, e.g. PRJ_ERRMSG in prj.inc, have now been placed into COMMON blocks with names such as PRJ_DATA, and are initialized via DATA statements in BLOCK DATA subprograms defined in separate files, e.g. prj_data.f. - To stop messages about subroutines being invoked with inconsistent argument lists if the relevant compiler option is not set, e.g. 'g77 -Wno-globals', the C wrapper functions that take 'void *' arguments now have separate forms for INTEGER, DOUBLE PRECISION, and CHARACTER arguments that simply invoke the generic function. Application code must be modified to take advantage of this. * User manual - In the section on the Fortran wrappers in the manual, warn about the need for the INTEGER array holding a data structure to be aligned on a DOUBLE PRECISION boundary. WCSLIB version 4.5.6 (2010/10/28) --------------------------------- * Installation - Fixed the search for CFITSIO and PGPLOT library and include directories. WCSLIB version 4.5.5 (2010/10/14) --------------------------------- * Installation - Build the PGSBOX sharable library. WCSLIB version 4.5.4 (2010/09/28) --------------------------------- * C library - In wcshdo(), according to the FITS standard, "Letters in the exponential form ('E' or 'D') shall be upper case" (reported by Michael Droettboom). WCSLIB version 4.5.3 (2010/09/23) --------------------------------- * Utilities - Various improvements to wcsgrid: correct the scaling set via cpgwnad(); label angles other than RA,Dec in decimal degrees; draw the projection boundary for projections other than zenithals. WCSLIB version 4.5.2 (2010/09/23) --------------------------------- * C library - Fixed the translation of GLS to SFL in wcsset() and celfix() when the reference longitude is non-zero - it introduces an offset in longitude in the normal way. (This undoes part of the change applied in version 4.4.) WCSLIB version 4.5.1 (2010/08/12) --------------------------------- * C library - New utility function, sphpad(), computes the coordinates of points offset by given angular distances and position angles from a given point on the sky (complementary to sphdpa()). * Fortran wrappers - New wrapper function: - SPHPAD for sphpad(). WCSLIB version 4.5 (2010/07/16) ------------------------------- * C library - Fixed the interpretation of VELREF when translating AIPS-convention spectral types. Such translation is now handled by a new special- purpose function, spcaips(). The wcsprm struct has been augmented with an entry for velref which is filled by wcspih() and wcsbth(). Previously, selection by VELREF of the radio or optical velocity convention for type VELO was not properly handled. * Fortran wrappers - New wrapper function: - SPCAIPS for spcaips(). - Changed spc.inc, spc_f.c, wcs.inc and wcs_f.c to track VELREF changes. - Declared functions external in the include files to avoid compiler warnings about unused variables (if the particular option is set). * Utilities - Added a '-q' option to fitshdr to quit after a specified number of HDUs. WCSLIB version 4.4.4 (2009/09/14) --------------------------------- * Installation - Added more configure options for controlling the build: --disable-fortran, --disable-utils, --without-cfitsio, and --without-pgplot. WCSLIB version 4.4.3 (2009/09/03) --------------------------------- * C library - Set wave number units to "/m" in spctyp(), was "1/m" which is not strictly legal and wasn't handled by wcsulex() (reported by Hans Terlow). Also fixed a number of units specifications in the prologue of spx.h to conform with Paper I usage. - In wcsulex(), allow unit strings like "1/m" in addition to "/m", provided that the superfluous "1" is the first non-blank character in the expression, or parenthesised sub-expression. - In wcssptr(), ensure that i is always reset if given < 0. * User manual - Augmented the list of FITS WCS and related software in the manual. WCSLIB version 4.4.2 (2009/08/13) --------------------------------- * C library - In sphx2s() and sphs2x(), handle the case where |eul[1]| = 180.0 separately for speed and accuracy. This change also fixes a rare and subtle bug in cels2x() that occurs when celprm::isolat is set and the magnitude of the first latitude in the lat[] vector exceeds 90 deg (reported by Hans Terlouw). * Installation - Fix relating to creation of symlinks when installing the libraries. WCSLIB version 4.4.1 (2009/08/11) --------------------------------- * Installation - Fixes for installation of the CHANGES file and for the creation of a symbolic link for the sharable library if one already exists. WCSLIB version 4.4 (2009/08/10) ------------------------------- * C library - Creation of WCSLIB user manual from the header file prologues using a special-purpose parser, doxextr, and sed scripts to generate input for doxygen. This required minor formatting changes to all prologues plus miscellaneous changes such as naming of arguments in function prototypes. - Bug fix in wcsset() that affected handling of PROJPn (deprecated) and PVi_ma attached to the longitude (not latitude) axis. Guard against long strings when copying the projection code. In wcs_types(), allow for early Paper IV distortion codes (e.g. "RA---TAN-SIP") when parsing CTYPEia. - Use sincos() whereever possible for a ~15% speedup (patches for cel.c, prj.c and sph.c supplied by Michael Droettboom). configure checks for, and uses it automatically if available. - Fixed the translation of GLS to SFL in wcsset() and celfix() when the reference longitude and latitude are non-zero. (In the AIPS convention, this simply translates the reference point, i.e. the map as a whole, to those coordinates without creating an oblique grid.) - Bug fix in prjoff(), a utility function used by the prj routines. It forces (x,y) = (0,0) at (phi_0,theta_0) when the latter are set by PVi_[012]a attached to the longitude (not latitude) axis. Rarely used in practice. - New utility function, sphdpa(), computes the distance and position angle from a point on the sphere to a set of field points. - In sphx2s() and sphx2s(), handle a simple change in origin of longitude using a short-cut calculation for speed and accuracy. Similarly in celset(), check whether phip == phi0 when computing latp and if so use a short-cut that ensures latp == 90.0 (exactly) if lat0 == theta0. The resulting spherical rotation then becomes a simple change in origin of longitude. In particular, these changes should assist PGSBOX in drawing grid lines of +/-180 longitude, to prevent flip-flopping between one and the other. - wcsbth() & wcspih(): resolved an inconsistency between the documentation and code by renamimg WCSHDR_VSOURCEa as WCSHDR_VSOURCE. - Flex code: moved declaration of helper functions out of global scope. - Fixed the call to wcss2p() in twcshdr (in a section of code not usually exercised). * Fortran wrappers - New wrapper functions: - WCSBTH for wcsbth(), - WCSBDX for wcsbdx(), - CDFIX for cdfix(), - SPHDPA for sphdpa(). - Updated WCSLEN (in wcs.inc) and added WCS_COLAX and WCS_VELANGL to match changes to wcsprm made in v4.3 with corresponding changes to the wrapper functions. Likewise updated TABLEN (in tab.inc) for changes to tabprm, and added CEL_LATPREQ for celprm. - Struct lengths (WCSLEN, PRJLEN, etc.) are now long enough to accomodate 64-bit machines. - Updated the flag bits for the RELAX argument in wcshdr.inc to reflect changes to wcshdr.h made in v4.3. Renamed WCSHDR_VSOURCEa to WCSHDR_VSOURCE for consistency with the C library. * PGSBOX - Improved grid labelling, particularly in minimizing the number of fields required in sexagesimal labels. * Utilities - New utility program: - wcsware extracts the WCS keywords for an image from the specified FITS file, constructs wcsprm structs for each coordinate representation found, and performs a variety of operations using them. - Old utility programs (first appeared in 4.3 but were not recorded): - HPXcvt reorganises HEALPix data into a 2-D FITS image with HPX coordinate system. - wcsgrid extracts the WCS keywords for an image from the specified FITS file and uses pgsbox() to plot a 2-D coordinate graticule for each alternate representation found. - fitshdr lists headers from a FITS file specified on the command line, or else on stdin, printing them as 80-character keyrecords without trailing blanks. * Installation - New configure options, --with-pgplotinc, --with-pgplotlib, --with-cfitsioinc and --with-cfitsiolib allow additional directories to be added to the library and include file search path. - Miscellaneous fixes and improvements to the installation process. - Generate a metadata file for pkg-config. - Added 'make MODE=interactive check' to run the test programs in interactive mode rather than batch. - Merged the separate CHANGES files for C, Fortran and PGSBOX into one (this), with a new section for utilities. WCSLIB version 4.3.3 (2009/04/30) --------------------------------- * C library - fitshdr.l, wcsbth.l, and wcspih.l: use setjmp/longjmp to preempt the call to exit() which is hard-coded in function yy_fatal_error() supplied by flex. - wcspih.l: if NAXIS is non-zero but there were no WCS keywords at all in the header then create a default WCS with blank alternate version. WCSLIB version 4.3.2 (2009/03/16) --------------------------------- * C library - utils/GNUmakefile: create BINDIR if necessary prior to installing utilities. WCSLIB version 4.3.1 (2008/09/08) --------------------------------- * Installation - Top-level GNUmakefile: install header files. WCSLIB version 4.3 (2007/12/27) ------------------------------- * C library - A new general WCS header parser wcsbth() handles binary table image arrays and pixel lists as well as image array headers. Added "colax" to the wcsprm struct to record the column numbers for each axis in a pixel list. - New function wcsbdx() is the analog of wcsidx() for the array of wcsprm structs returned by wcsbth(). - New function wcshdo() writes out a wcsprm struct as a FITS header. - Changes to wcspih(): - Bug fix, check for a == 0 (indication of a keyword that applies to all alternates) in internal helper function wcspih_naxes() (reported by Craig Markwardt). - Added a new ctrl option to remove valid WCS keyrecords except for those with a more general role, namely {DATE,MJD}-{OBS,AVG} and OBSGEO-{X,Y,Z} (suggested by Jim Lewis). - Added a rule for VELANGLa. Also added "velangl" to the wcsprm struct. - Do checks on the i, k & m keyword parameters in . - Fixed the test for repeated blanks in the NAXIS and WCSAXES patterns. - Fixed three rules to allow m == 0. - Reworked the implementation notes in the prologue. - The flex scanners, fitshdr.l, wcsbth.l, wcspih.l, wcsulex.l, and wcsutrn.l, invoke yylex_destroy() before returning to avoid a 16kiB memory leak. This was reported by several people, however it may be problematic depending on the version of flex used - version 2.5.9 or later is required. If this is not available, C sources pre- generated by flex 2.5.33 will be used. - In wcs.c, don't define the signbit macro if already defined (for MacOSX). - In wcs.h, documented wtbarr namespace issues in C++. - In wcsset(), always set wcsprm.cunit[i], if possible (primarily for use by wcshdo()). - In wcsfix.c, parenthesised a boolean expression that was otherwise incorrect. - Fixed an obscure floating point rounding error in celset() that appeared with -O2 optimization in gcc v3.3.5 (Linux). - prjset() now correctly propagates the status value returned by the specific projection-setting functions (reported by Bill Pence). - Bug fix in hpxx2s(), also added bounds checking. Minor efficiencies in carx2s() and merx2s(). - In the various functions that print the contents of the structs, use the "%p" printf conversion specifier to print addresses rather than casting the pointer to int and using "#x". The latter does not work on 64-bit machines where sizeof(int) != sizeof(void*). - Reorganized the various structs to get alignment on 64-bit machines. - All header file prologues now reference the README file for an overview of the library. - Miscellaneous portability fixes for 64-bit, MacOSX, OSF compiler, etc. - Elimination of compiler warnings, e.g. parenthesised assignments used as truth values (a favourite gcc gripe!), etc. - Process flex descriptions using a newer version of flex, primarily for MacOSX. However, the processed files are now only used when flex 2.5.9 or later is not available. - Removed WCSLIB 2.x backwards-compatibility measures from lin.h, prj.h, prj.c, and sph.h. * Fortran wrappers - (No substantive changes.) * PGSBOX - Miscellaneous improvements to PGSBOX. * General - Switched licensing to LGPL 3.0. - In comment text, replaced use of the obsolete term "card" with "keyrecord" which consists of a "keyword", "keyvalue", and "keycomment". * Installation - General improvements to the installation process: autoconf-related portability improvements, particularly relating to Fortran name mangling; makefile rules for building the shared library, for processing flex descriptions; don't rely on "." being in the PATH when running tests. WCSLIB version 4.2 (2005/09/23) ------------------------------- * C library - Brought the installation process under control of GNU autoconf, the top-level makefile now builds and tests everything, and the C library has a config.h in which WCS_INT64 is set. Added an INSTALL file. - Merged the FORTRAN, C and PGSBOX READMEs into one top-level README. - Extensions for -TAB coordinate handling: in tabx2s() and tabs2x(), allow extrapolation by half a cell at either end of the index and coordinate tables; fits_read_wcstab() (in getwcstab.{h,c}) allows TDIMn to be omitted for 1-D lookup tables for which it has the form '(1,K)', i.e. describing a degenerate 2-D array; wcsprt() now prints the wtbarr structs in wcsprm. - Bug fixes for -TAB coordinate handling: in tabx2s() and tabs2x() the incorrect indexing variable, m instead of i, was used for tab->crval[]; wcsp2s() and wcss2p() returned prematurely in the tabular coordinate loop; in wcstab(), removed an extraneous assignment to wtbp->kind for index arrays. - In wcsp2s() and wcss2p(), elements of the stat[] vector that had been set were being reset incorrectly to zero. The stat[] values are now set as flag bits for each coordinate element. - Added cdfix() to the wcsfix() suite to fix erroneously omitted CDi_ja cards. - PGSBOX is now compiled into a separate object library, and is installed alongside WCSLIB. - Eliminated several instances of non-ANSI C library functions and header files and some residual K&R C usage. The Sun C compiler complained about const int definitions of initializers used in variable declarations in some of the test programs; changed these to preprocessor macros. * Fortran wrappers - Fixed handling of 64-bit integer keyvalues in keyget_(). - Fixed output formatting of 64-bit integer keyvalues in tfitshdr.f. - Fixed minor syntax errors in twcsfix.f and tpih1.f reported by the Sun Fortran compiler. - The output of each test program now identifies the source file. * PGSBOX - (No substantive changes.) WCSLIB version 4.1 (2005/08/31) ------------------------------- * C library Summary of added functionality: - -TAB coordinate axes are now fully implemented in the WCSLIB driver functions (in wcs.{h,c}); multiple -TAB axes are supported. A new function, wcstab(), which is automatically invoked by wcspih(), parses -TAB-related header cards and sets up structs for a separate routine that reads the necessary arrays from a FITS binary table extension. An implementation of this routine in CFITSIO, fits_read_wcstab(), is provided. Note however that the interface of this function is experimental, and the code itself must be considered beta-release in WCSLIB 4.1. - Units specifications, either from CNAMEia or inline comments (with brackets), of arbitrary complexity are now fully implemented via a parser, wcsulex(), and converter, wcsunits(). This is invoked automatically by wcsset(). - Translators for non-standard WCS constructs are provided. These cover date formats, units specifications, defunct celestial projection types, AIPS spectral axis types, and the repair of malformed cylindrical coordinate systems. - wcspih() now has options to remove the WCS cards it has processed from the header and a new generic FITS header parser, fitshdr(), may be used to parse the remaining non-WCS cards. In addition to the more basic types, it handles 64-bit and 'very long' (70 digit) integer keyvalues, and also continued string keyvalues. It also does keyword matching and extracts units specifications in inline comments. - -LOG coordinates are now implemented independently of spectral coordinate types. Multiple -LOG axes are supported. - New function wcssptr() translates the spectral axis in a wcsprm struct to the required type. - The README file now gives an introduction to, and complete overview of, WCSLIB. It provides a point of entry to programming with WCSLIB. Complete descriptions and usage notes for all functions are contained in the header files. - The FORTRAN wrappers and test programs are now completely up-to-date with respect to the C implementation. - All code, including the FORTRAN wrappers, PGSBOX, and all test programs, now pass 'purify' without memory leaks, uninitialized memory reads, memory access violations, or other memory faults. Change notes: - Added options to wcspih() to remove WCS cards from the input header leaving only non-WCS cards behind. Modified test programs tpih1.c and tpih2.c to use CFITSIO optionally via preprocessor macro DO_CFITSIO. - New function wcstab() in wcshdr.{h,c} parses -TAB-related header cards and sets up structs for a separate routine that reads the necessary arrays from a FITS binary table extension. New test/demo program twcstab.c using header defined in wcstab.cards. - CFITSIO implementation, fits_read_wcstab() in getwcstab.{h,c}, of a function, independent of WCSLIB, for extracting arrays from a binary table as required in constructing -TAB coordinates. - New units specification parser, wcsulex() in wcsunits.h and wcsulex.l, and converter, wcsunits() in wcsunits.{h,c}. New test/demo program tunits.c. - New parser for non-standard units specifications, wcsutrn() in wcsunits.h and wcsutrn.l, also tested by tunits.c. - New functions datfix(), unitfix() (which applies wcsutrn()), celfix(), and spcfix() join cylfix() in wcsfix.{h,c} to translate various forms of non-standard or quasi-standard FITS WCS keyvalues in a wcsprm struct. wcsfix() applies all of these in sequence. New test/demo program twcsfix.c, with wcsfix() also now invoked by tpih1.c. - New generic FITS header parser, fitshdr() in fitshdr.{h,l}. New test/demo program tfitshdr.c uses wcs.cards with extra non-WCS cards added. - -LOG coordinates are now treated as a coordinate type separate from spectral coordinates, implemented via log.{h,c} and test program tlog.c. The logarithmic functions were removed from spx.{h,c}, and spc.c. - Extensive changes to wcs.{h,c} to support multiple -TAB and -LOG coordinate axes and units conversion. Substantially changed the test program, twcs.c, to test the more general functionality. - New function wcssptr() in wcs.{h,c} translates the spectral axis in a wcsprm struct. - Added DATE-AVG to wcsprm. Also ntab, tab, nwtb, and wtb required for -TAB implementation. Define struct wtbarr. - Added a types[] member to the wcsprm struct to identify axis coordinate types using a four-digit code. - Use memset() in wcsini() to null-fill character arrays in the wcsprm struct so that they don't appear to be padded with garbage when displayed by gdb. - Do alias translation for AIPS-convention spectral types in wcsset() using spctyp(). If wcsset() finds a CTYPEia in "4-3" form with an unrecognized algorithm code it now returns an error rather than assume that it's a linear axis. wcsset() now also resets lonpole and latpole to the values actually used. - Modified spctyp() to translate AIPS-convention spectral ctypes, and modified the argument list to return the parsed spectral type and algorithm code. The return arguments will not be modified if CTYPEia is not a valid spectral type; zero-pointers may be specified for any that are not of interest. Removed the external const variables, spc_codes and spc_ncode, as their function is now fulfilled by spctyp(). - Fixed a bug in spctrn() in resolving ctypeS2 wildcarding. - Added latpreq member to the celprm struct, set by celset() to indicate how LATPOLE is used. Augmented tcel2.c to report it. - New function tabmem() in tab.{h,c} takes control of user-allocated memory. - tabini() allows K == 0 and also K[m] == 0 to initialize partially the tabprm struct (for wcstab()). It now does fine-grained bookkeeping of memory allocation for the index arrays and allocates each individually. tabprm.index[] == 0x0 is recognized as default indexing in tabset(), tabx2s() and tabs2x(). - The *prt() functions report parameters to an extra decimal place. - tabprt() prints the array index for elements of the coordinate and index vectors. - Set the 0th element in all *_errmsg arrays to "Success". - Extracted string utility functions used by WCSLIB into wcsutil.{h,c}. - Removed support for K&R C. * Fortran wrappers - The FORTRAN wrappers and test programs are now completely up-to-date with respect to the C implementation. - New include files, wrappers, and test programs: fitshdr.inc, fitshdr_f.c, getwcstab.inc, getwcstab_f.c, log.inc, log_f.c, sph.inc, tab.inc, tab_f.c, tfitshdr.f, tlog.f, ttab1.f, ttab2.f, ttab3.f, tunits.f, twcsfix.f, twcstab.f, wcsfix.inc, wcsfix_f.c, wcsunits.inc, wcsunits_f.c. - Updates to reflect changes to the C library and test programs: cel.inc, cel_f.c, prj.inc, spc.inc, spc_f.c, spx.inc, spx_f.c, tlin.f, tpih1.f, tpih2.f, tprj1.f, tprj2.f, tspc.f, tsph.f, tspx.f, twcs.f, twcsmix.f, twcssub.f, wcs.inc, wcs_f.c, wcshdr.inc, wcshdr_f.c. - Added *_ERRMSG arrays containing status messages to all include files. - Removed support for K&R C. * PGSBOX - Fixed a subtle though benign memory fault identified by 'purify'. - Reset LATPOLE in the COE example in cpgtest.f when drawing the second (native) grid because it will have been set to a non-default value by wcsset() when the first grid was drawn; set wcs.flag to -1 before wcsinit() and call wcsfree() at the end. Similarly for pgtest.f. WCSLIB version 4.0 (2005/02/07) ------------------------------- * C library - Implemented tabular coordinates (-TAB). New files: tab.h and tab.c, and test programs ttab[123].c. These have not been incorporated into the higher-level (wcs.h) functions at this stage. - New spectral functions: spchek() checks a spectral algorithm code for legitimacy; from the spectral keywords given, spcspx() derives the corresponding CRVALi and CDELTi keywords for the underlying P-, and X-type spectral coordinates; spcxps() does the opposite; spctrn() combines spcspx() and spcxps() to translate one set of spectral keywords into another, e.g. 'FREQ' -> 'ZOPT-F2W'. - Implemented the HEALPix (HPX) projection in the prj functions. - Added a new function, wcsidx(), to return an array that indexes the alternate coordinate descriptions found by wcspih() (suggested by Bill Pence, NASA/Goddard). Modified tpih1.c to exercise it. - In wcsp2s() and wcss2p(), check that nelem equals or exceeds wcs.naxis; emphasised this in the usage notes for these functions in tab.h (suggested by Bill Pence, NASA/Goddard). - Moved the macros used for UNDEFINED values and the corresponding macro test function, undefined(), to wcsmath.h for general use. Previously, UNDEFINED values were only used internally, but they are now visible in some of the structs, particularly values of undefined auxiliary header cards in the wcsprm struct. - Remove const from the double args in the specx() prototype in spx.h to match the definition in spx.c (reported by Bryan Irby, NASA/Goddard). - Fixed the interaction between the FLAVOUR and PGPLOTLIB definitions in the C and FORTRAN Makefiles by introducing a separate variable, DO_PLOTS, to control whether to exercise test programs that require PGPLOT (reported by Bill Pence, NASA/Goddard). * Fortran wrappers - New wrapper defined in wcshdr_f.c: wcsidx_(). Modified test program tpih1.f to use it. * PGSBOX - (No substantive changes.) * General - Changed the copyright notice in all library routines from LGPL to GPL as recommended by the FSF (http://www.gnu.org/licenses/why-not- lgpl.html). * Installation - General improvements to the installation process: fixed the interaction between the FLAVOUR and PGPLOTLIB definitions in the Makefile by introducing a separate variable, DO_PLOTS, to control whether to exercise test programs that require PGPLOT (reported by Bill Pence, NASA/Goddard). Added an "install" target to the Makefile. WCSLIB version 3.6 (2004/08/25) ------------------------------- * C library - New service routine, wcssub() extracts the coordinate description for a subimage from a wcsprm struct. wcscopy() is now implemented as a preprocessor macro that invokes wcssub(). New test program, twcssub.c, tests wcssub(). - In wcspih(): 1) Fixed handling of string-valued keywords where the inline comment contains a single-quote character ('). 2) Fixed the address arithmetic for EPOCH and VELREF. 3) Translate VSOURCEa into ZSOURCEa if required. 4) Recognize SSYSSRCa. 5) Support free-format string keyvalues, as well as integer and floating-point keyvalues; documented this in the prologue of wcshdr.h. 6) Allow header cards without inline comments. 7) Fixed function prototyping in wcspih.l (i.e. ANSI and non-ANSI forms were potentially mixed). 8) Catch an unhandled newline character on the END card that was echoed to stdout. 9) In error messages, print "ERROR" (uppercase) - POSIX standard. - Modified wcs.cards to explain and test free-format keyvalues, and also augmented the inline comment on illegal WCS cards that are to be rejected, and WCS-like cards to be discarded. Added a header card with no inline comment. - Removed vsource from the wcsprm struct and added ssyssrc. - In wcsini(), fixed a problem with memory management for wcs.pv when NPVMAX is zero; likewise for wcs.ps and NPSMAX. - In wcsprt(), don't print auxiliary coordinate system information in arrays with zero address. - In wcss2p(), status == 9 (one or more invalid world coordinates) was not returned appropriately. - Renamed twcs1.c to twcs.c, and twcs2.c to twcsmix.c. - "Error status/code/number" is now referred to consistently as the "status return value". - Some vestiges of K&R C were removed: preprocessor definition of const, and K&R function prototypes. * Fortran wrappers - New wrapper defined in wcs_f.c: wcssub_(). New test program, twcssub.f. - Renamed twcs1.f to twcs.f, and twcs2.f to twcsmix.f. * PGSBOX - (No substantive changes.) * Installation - Worked over the C, FORTRAN, and PGSBOX makefiles, in particular to make them all consistent. WCSLIB version 3.5 (2004/06/28) ------------------------------- * C library - WCSLIB now provides a function, wcspih() implemented as a Flex description, that parses a FITS image header, either that of a primary HDU or an image extension. Given a character array containing the header it identifies and reads all WCS cards for the primary coordinate description and up to 26 alternate descriptions and returns this information as an array of wcsprm structs. A service routine, wcsvfree(), is provided to free the memory allocated by wcspih(). The relevant header file for these functions is wcshdr.h. Test programs, tpih1 and tpih2, are provided to verify wcspih. The first simply prints the contents of the structs using wcsprt(). The second uses cpgsbox() to draw coordinate graticules. A FITS WCS test header has been developed to provide input to these test programs. It is implemented as a list of card images, wcs.cards, one card per line, together with a program, tofits, that compiles these into a valid FITS file. tpih1 uses its own code to read this, whereas tpih2 uses the fits_hdr2str() function from CFITSIO. - Removed twcsprt, tpih exercises wcsprt() much more thoroughly than twcsprt ever did. Modified twcs1 to print the size of the various structs as twcsprt used to. - Although they are not used in any coordinate calculations, the wcsprm struct now provides data members for storing all of the auxiliary FITS WCS header cards defined in Papers I, II, and III, such as WCSNAMEa, EQUINOXa, and CNAMEia. Members are also provided for storing the alternate descriptor code (the "a" in CTYPEia), and the binary table column number. These are supported by the high level WCSLIB routines, wcsini(), wcscopy(), wcsfree(), and wcsprt(). Refer to wcs.h for details. - The number of PVi_ma cards for which wcsini() allocates memory is now set by a global variable, NPVMAX (previously a C-preprocessor macro). This defaults to 64 but may be changed by a new function, wcsnpv(). The wcsprm struct contains a new member, npvmax, that records the value of this number at the time the struct was initialized. This is in addition to npv which records the actual number of cards that were encountered. Similarly, NPSMAX (default 8) is used for the number of PSi_ma cards, and it may be changed via wcsnps(). The axis number, i, in the pvcard struct used for storing PVi_ma cards may now be set to 0 to indicate the latitude axis. - calloc() is now used in place of malloc() in allocating memory for arrays, and inclusion of malloc.h has been replaced with stdlib.h for all platforms. wcsfree() checks that wcs.flag != -1 before testing wcs.m_flag when freeing memory allocated by wcsini() in case the struct is uninitialized. Similarly for linfree(). - In prj.h, renamed C-preprocessor macros INI, PRT, SET, X2S and S2X to PRJINI, PRJPRT, PRJSET, PRJX2S and PRJS2X to reduce the likelihood of namespace clashes. Similarly in spc.h. Also, in prj.c, changed the name of helper routine offset() to prjoff() to reduce the likelihood of global namespace conflicts. - In line with bonx2s() and bons2x(), bonset() now recognizes the equatorial case of Bonne's projection as Sanson-Flamsteed, mainly so that the auxiliary information in the prjprm struct more accurately reflects the truth. Modified tcel2 to exercise this by using an equatorial Bonne projection in place of the Hammer-Aitov. - zpns2x() used prj.w[0] for bounds checking, though this had not been set by zpnset() for polynomials of degree N < 3. Consequently, bounds checking for N < 3 was unreliable (reported by David Berry, STARLINK). - Changed some variable names in tscs2x(), cscx2s(), cscs2x(), qscx2s(), and qscs2x() to match Paper II, and likewise changed some inequality tests in qscs2x() without changing the results. - Minor tidying up of output formatting in prjprt(). - Added the alternate version code to FITS WCS keywords mentioned in comments, e.g. CTYPEi changed to CTYPEia. * Fortran wrappers - New wrappers defined in wcshdr_f.c: wcspih_() and wcsvfree_(), and also a new service function, wcsvcopy_(). New test programs, TPIH1 and TPIH2, being analogues of tpih1 and tpih2. Removed TWCSPRT. - In wcs_f.c, new wrappers wcsnpv_() and wcsnps_(); modified wcsput_() and wcsget_() to handle new members of the wcsprm struct. Also modified wcsput_() to null-fill all char[] members of the wcsprm struct, and likewise wcsget_() to blank-fill them. - Modified wcs.inc to support changes to the wcsprm struct. * PGSBOX - In PGSBOX, increased the dimension of the WORLD and XY vectors from 2 to 9 to accomodate higher-dimensional coordinate representations of up to 9 elements. Similarly for pgwcsl(). The assumption (presently) is that the first two world, and pixel, coordinate elements are the relevant ones; the others are all set to zero when pgwcsl() initializes and otherwise ignored. Assigned some variables in DATA to stop compiler messages about uninitialized variables. - Generalized the Makefile, bringing it into line with the WCSLIB Makefile, and adding separate targets for compiling and running the test programs. The default target now simply compiles pgsbox.c and cpgsbox.c. A separate target compiles pgwcsl.c and inserts it into ../C/libwcs.a. WCSLIB version 3.4 (2004/02/11) ------------------------------- * C library - In aitx2s(), apply the boundary condition 0.5 <= Z^2 <= 1 given after Eq. (109) in WCS Paper II to detect outlying pixels. - Fixed several special-case bugs in celset(): 1) For theta_0 = 90, in substituting the default value for phi_p (LONPOLE), a) for the special case when delta_0 = 90, celset() provided the wrong value (180 instead of 0), b) celset() neglected to add phi_0 (normally 0). 2) For theta_0 != 90, a) for the special case when delta_0 = -90, celset() incorrectly computed delta_p (as theta_0 instead of -theta_0), b) for the special case when delta_p = +90 (or -90), celset() neglected to subtract (or add) phi_0 (normally 0). 3) For |delta_0| = 90, celset() incorrectly allowed the particular, invalid, value of phi_p (LONPOLE) that put the other pole at the fiducial point. 4) For theta_0 = 0, delta_0 = 0 LATPOLE determines delta_p completely. For LATPOLE > 90 celset() now sets delta_p to 90, and for LATPOLE < -90 it sets it to -90. - Additional refinements in celset(): 1) cel->ref[2] is normalized in the range [-180,180]. 2) Account for rounding error in the computation of delta_p. - sphx2s() and sphs2x() incorrectly handled the "change in the origin of longitude" special case that arises when delta_p = -90, in the even more restrictive case where |theta| = 90 also; it applied Eq. (3) instead of Eq. (4) of Paper II. - Added a new test program, tcel2.c, to exercise celset() more thoroughly. Renamed the original tcel.c to tcel1.c and modified the Makefile to suit. * Fortran wrappers - (No changes.) * PGSBOX - (No substantive changes.) WCSLIB version 3.3 (2003/10/21) ------------------------------- * C library - In celset(), the default value for phi_p (LONPOLE) is phi_p = phi_0 + ((delta_0 < theta_0) ? 180.0 : 0.0) Previously phi_0 (which is normally zero) was not added (reported by David Berry, STARLINK). - wcsprt() and linprt() now check that the structs have been initialized. - In wcsini(), when the wcsprm flag is -1 also set the linprm flag to -1 to force initialization of the memory managed by linset(). - wcsset() now explicitly initializes the celprm and spcprm structs via celini() and spcini(). - Fixed syntax errors in the macro definitions of linrev_errmsg and linfwd_errmsg. - In Makefile, added the -ansi option to gcc to force it to behave like a strict ANSI C compiler, specifically in setting the __STDC__ preprocessor macro. * Fortran wrappers - (No changes.) * PGSBOX - PGSBOX now recognizes status returns -1, -2, and -3 from NLFUNC for opcodes +2 and +1 which cause it to accept the returned (x,y) coordinates but not consider them as one end of a crossing segment for labelling world coordinate 1, 2, or both. - PGSBOX now takes care not to lose vertical tick marks (and hence labels) at the left or right edge of the frame. Likewise for horizontal tick marks at the top or bottom edge of the frame. - Tightened up the test in PGSBOX for cycles in angle to catch the case where the coordinate value spans a full 360 degrees. - PGSBOX will no longer accept frame crossings that are too oblique; floating point rounding errors may cause grid lines that should otherwise track along the frame to weave down it from side-to-side resulting in spurious crossing points. - Fixed a bug in pgwcsl_() for processing simple linear coordinates. - pgwcsl_() now returns error -2 if the latitude is outside -90 to +90 for opcodes +2 and +1. - Amended the translation of status return codes from WCSLIB in pgwcsl_(). - Provided a header file for pgwcsl_() (mainly for C++ usage). - Added extra test plots to PGTEST and cpgtest. - Added extra functionality to the Makefile. WCSLIB version 3.2 (2003/09/09) ------------------------------- * C library - Added the facility of setting the flag member of a wcsprm struct to -1 before calling wcsini() for the first time in order to initialize memory management. Likewise for linprm and linini(). - Renamed wcscpy() to wcscopy() to avoid a conflict with the Posix "wide character string" function of the same name (wchar.h). In particular, this is used by the GNU C++ string class. - The higher level functions (wcs, cel, spc) no longer return prematurely if some of the input coordinate values are invalid. - All functions now test whether a null pointer for the particular struct (wcsprm, celprm, etc.) has been passed to them. - Function return codes have been rationalized into a consistent set within each of the wcs, cel, lin, prj, spc, and spx suites of functions. Error messages to match these error codes are now encoded in a single character array, e.g. wcs_errmsg and prj_errmsg, instead of a separate array for each function. Macro definitions for the older character arrays (e.g. wcsini_errmsg) have been provided for backward compatibility. - Declared prj_stat as extern in prj.h. * Fortran wrappers - (No changes.) * PGSBOX - Added an ENTRY point, PGLBOX, that provides a simplified interface to PGSBOX for linear axes without having to specify an NLFUNC or the associated parameters. WCSLIB version 3.1 (2003/04/29) ------------------------------- * C library - Added "global" and "divergent" prjprm struct informational members to record whether the projection is capable of mapping the whole sphere, and whether it is divergent in latitude. - Function cylfix() provided to fix WCS FITS header cards for malformed cylindrical projections (c.f. Paper II, Sect. 7.3.4). - Added support for CUNITi cards to wcsprm (but not currently implemented). - Added macro implementations of the trigd functions to wcstrig.h, enabled if WCSTRIG_MACRO is defined. - Improved printing of the WCSLIB structs. - Added macro definitions for the lengths of the WCSLIB structs measured in sizeof(int) units (mainly for the FORTRAN wrappers). * Fortran wrappers - FORTRAN is now supported via a set of wrappers on the C library. Refer to the README file. * PGSBOX WCSLIB version 3.0 beta release (2003/04/01) -------------------------------------------- * C library - Fully vectorized function interfaces (C preprocessor macros are available to implement the scalar interfaces of the proj.c, sph.c, and lin.c routines from WCSLIB 2.x). - Implementation of Paper II, Sect. 2.5: User-specified (phi0, theta0). - Implementation of Paper III (excluding "-TAB"). - Memory management is now implemented in the upper-level (wcs.c) routines. - New extensible design should accomodate Paper IV (and any other) without further change to the function interfaces. * PGSBOX - Added a C wrapper function, cpgsbox(), and C test/demo program, cpgtest, that duplicates PGTEST and serves as a C coding template. - Added calendar date axes. - Sped up the max/min search - if only tickmarks are required there is no need to search the interior of the image. - Return margin widths in CACHE(,NC). - Fixed a buglet that caused ticks at the frame edges to be skipped. - Return error 3 if CACHE overflows. - Adapted PGWCSL for WCSLIB 3.x - it is now a C function (for interfacing to WCSLIB) with a FORTRAN-like interface (for PGSBOX). WCSLIB version 2.9 (2002/04/03) ------------------------------- * C library - Fixed a bug with alias translation in wcsset(). - Added a conditional compilation directive to lin.c for Apple's MacOS X. * Fortran library - Fixed CUBEFACE handling in WCSSET. WCSLIB version 2.8 (2001/11/16) ------------------------------- * C library - Added support for the SZP projection with szpset(), szpfwd() and szprev(), and generalized AZP with support for the tilt parameter, gamma. - Added phi0 to the prjprm struct, this is set by the projection initialization routines along with theta0. - Fixed a problem in wcsmix() caused by numerical imprecision that could cause it not to recognize when convergence was reached; break out of the loop early if a discontinuity is detected. - Clarified the usage of vspan in the prologue to wcsmix(). - Fixed comments relating to LATPOLE in the prologue to cel.c and tcel.c, and replaced references to LONGPOLE with LONPOLE. - Augmented the error reports in twcs2. - Modified projex() in tproj1 and prjplt() in tproj2 to make use of the information stored in the prjprm struct. * Fortran library - Added support for the SZP projection with SZPSET, SZPFWD and SZPREV, and generalized AZP with support for the tilt parameter, gamma. - Changed the call sequence to PRJSET to return PHI0 along with THETA0. - Fixed a problem in WCSMIX caused by numerical imprecision that could cause it not to recognize when convergence was reached; break out of the loop early if a discontinuity is detected. - Clarified the usage of VSPAN in the prologue to WCSMIX. - Fixed comments relating to LATPOLE in the prologue to CEL and TCEL, and replaced references to LONGPOLE with LONPOLE. - Augmented the error reports in TWCS2. - Modified PROJEX in TPROJ1 and PRJPLT in TPROJ2 to use the generic driver routines PRJSET, PRJFWD and PRJREV. PRJPLT also now uses the projection type encoded in PRJ(11). WCSLIB version 2.7 (2001/02/19) ------------------------------- * C library - Added generic driver routines prjset(), prjfwd() and prjrev(). These invoke specific projection routines via the pointer-to- function elements, prjfwd and prjrev, transferred to the prjprm struct from celprm. - Added code (3-letter projection code) and theta0 (reference latitude) elements to prjprm. - The projection code for the Sanson-Flamsteed projection is now SFL. The upper-level routines, wcsset(), wcsfwd(), and wcsrev(), recognize GLS as an alias for this. - wcsset() now recognizes 'xyLN/xyLT' axis pairs. - Two bugs in the translation from NCP to SIN in wcsfwd() and wcsrev() were fixed: (1) the projection parameter was computed incorrectly and (2) they did not honour prj->flag set to -1 to disable strict bounds checking. - A bug in wcsmix() was fixed - it was relying on the wcsprm struct to have been initialized beforehand. - The test programs now use the cpgplot interface to PGPLOT, the old tpgc.c and tpgf.f wrappers have been removed. * Fortran library - Added generic driver routines PRJSET, PRJFWD and PRJREV. These are keyed to specific projection routines via the value of PRJ(11) which now differs for each projection. - The projection code for the Sanson-Flamsteed projection is now SFL. The upper-level routines, WCSSET, WCSFWD, and WCSREV, recognize GLS as an alias for this. - WCSSET now recognizes 'xyLN/xyLT' axis pairs. - A bug in the translation from NCP to SIN in WCSFWD and WCSREV was fixed; they did not honour PRJ(11) set to -1 to disable strict bounds checking. - A bug in WCSMIX was fixed - it was relying on the WCS array to have been initialized beforehand. WCSLIB version 2.6 (2000/05/10) ------------------------------- * C library - Check for invalid (x,y) in zearev(). - In wcsmath.h, guard against prior definition of PI and other preprocessor variables. * Fortran library - Check for invalid (X,Y) in ZEAREV. - Declare COSD and SIND in WCSFWD and WCSREV, reported by Clive Page (cgp@star.le.ac.uk). WCSLIB version 2.5 (1999/12/14) ------------------------------- * C library - Added copyright notice to header files and prefixed include guard names with "WCSLIB_". - Fixed cube face handling in wcsfwd() and wcsrev() (reported by Doug Mink, CfA). Allow more general face layout in the inverse quadcube projections. - Fixed the problem in wcsmix() where it failed to find a valid solution when the solution point lay at a native pole of a projection in which the pole is represented as a finite interval. However, wcsmix() will only ever return one solution even when two or more valid solutions may exist. - wcsmix() now accepts viter in the range 5 - 10, the specified value will be pushed up or down into this range if necessary. - The projection routines for AZP, TAN, SIN, ZPN, and COP now return error 2 if (phi,theta) correspond to the overlapped (far) side of the projection. This strict bounds checking can be switched off by setting prj->flag to -1 (rather than 0) when the projections are initialized. - The upper level routines, wcsset(), wcsfwd(), wcsrev(), and wcsmix(), now recognize the NCP projection and convert it to the equivalent SIN projection. The lower level routines do not recognize NCP. - Extracted definitions of mathematical constants (PI etc.) from proj.h into wcsmath.h in order to avoid conflicts with their definition in math.h in some systems (such as Linux). - Describe the two alternate representations of the quadcube projections (i.e. faces laid out or stacked) in the prologue of wcs.c. * Fortran library - Fixed cube face handling in WCSFWD and WCSREV, reported by Doug Mink (dmink@cfa.harvard.edu). Allow more general face layout in the inverse quadcube projections. - Fixed the problem in WCSMIX where it failed to find a valid solution when the solution point lay at a native pole of a projection in which the pole is represented as a finite interval. However, WCSMIX will only ever return one solution even when two or more valid solutions may exist. - WCSMIX now accepts VITER in the range 5 - 10, the specified value will be pushed up or down into this range if necessary. - The projection routines for AZP, TAN, SIN, ZPN, and COP now return error 2 if (phi,theta) correspond to the overlapped (far) side of the projection. This strict bounds checking can be switched off by setting PRJ(11) to -1 (rather than 0) when the projections are initialized. - The upper level routines, WCSSET, WCSFWD, WCSREV, and WCSMIX, now recognize the NCP projection and convert it to the equivalent SIN projection. The lower level routines do not recognize NCP. - Describe the two alternate representations of the quadcube projections (i.e. faces laid out or stacked) in the prologue of wcs.f. WCSLIB version 2.4 (1996/09/23) ------------------------------- * C library - In sinrev(), cscrev(), qscrev(), and tscrev(), return error 2 if (x,y) do not lie within the perimeter of the projection. In sinrev(), stop the computation of phi for the "synthesis" projection being applied to the pure "orthographic" case (reported by David Berry, STARLINK). - (Internal change) Renamed variables l <-> m in the quadcube projections to accord with standard usage (and revised WCS draft paper). * Fortran library - In SINREV, CSCREV, QSCREV, and TSCREV, return error 2 if (X,Y) do not lie within the perimeter of the projection. In SINREV, stop the computation of PHI for the "synthesis" projection being applied to the pure "orthographic" case. Reported by David Berry (dsb@ast.man.ac.uk). - (Internal change) Renamed variables L <-> M in the quadcube projections to accord with standard usage (and revised WCS draft paper). - (Internal change) Stopped PRJ(11) doing double service in any projection. It is now set and tested for a specific magic value rather than simply being non-zero. WCSLIB version 2.3 (1996/06/24) ------------------------------- * C library - Fixed two bugs in zpnset(). The first led to an incorrect determination of the degree of the polynomial and would mainly have affected the efficiency of zpnrev(). The second affected the determination of the boundary of the projection but would only have been significant for projections with a point of inflection between 9 and 10 degrees of the pole. Reported by David Berry, STARLINK. - Replaced usage of alloca() in lin.c with malloc() and free() for portability as suggested by Klaus Banse, ESO (kbanse@eso.org). - Allow for C implementations that provide their own versions of cosd(), sind(), tand(), acosd(), asind(), atand(), and atan2d(). From Klaus Banse, ESO (kbanse@eso.org). - Implemented the CUBEFACE axis for quadcube projections. - Made all function prototypes const-correct. - Adapted the header files to C++ usage. - Added a new test program, twcs1, to verify closure of wcsfwd() and wcsrev(). The old twcs test program is now called twcs2. - Added external arrays of error messages indexed by function return value. For example, extern const char *wcsmix_errmsg[] for wcsmix(). Messages for the many proj.c functions are in prjfwd_errmsg[], etc. * Fortran library - Implemented the CUBEFACE axis for quadcube projections. - Added a new test program, TWCS1, to verify closure of WCSFWD and WCSREV. The old TWCS test program is now called TWCS2. WCSLIB version 2.2 (1996/01/18) ------------------------------- * C library - Amended the projection equations for the conics (COP, COD, COE, COO) and Bonne's projection (BON) to correctly handle southern hemisphere projections with PROJP1 < 0 (reported by Lindsay Davis, NOAO). Revised tproj1 and tproj2 to test such cases. * Fortran library - Amended the projection equations for the conics (COP, COD, COE, COO) and Bonne's projection (BON) to correctly handle southern hemisphere projections with PROJP1 < 0 (reported by Lindsay Davis, NOAO). Revised TPROJ1 and TPROJ2 to test such cases. - Increased the dimension of the WCS array from WCS(0:2) to WCS(0:3) to allow for future handling of the CUBEFACE keyword - WCS(3) will store an index to the CUBEFACE axis. This affects the call sequences of WCSSET, WCSFWD, WCSREV, and WCSMIX. WCSLIB version 2.1 (1995/11/17) ------------------------------- * C library The main change of interest to programmers is that of changed argument lists for wcsfwd() and wcsrev() as described below. - The WCS linear transformations are now implemented in WCSLIB, complete with matrix inverter. The new files are lin.c, lin.h, and test program tlin.c. - Given either the celestial longitude or latitude plus an element of the pixel coordinate a new routine, wcsmix(), solves for the remaining elements by iterating on the unknown celestial coordinate element using wcsfwd(). - The high level driver routines wcsfwd(), wcsrev(), and wcsmix() now apply the full WCS algorithm chain (except for pixel regularization table), including parsing the CTYPEn header cards and computing non- celestial elements of the world coordinate. This required a change to their argument lists which now more closely reflect the sequence of algorithms applied. A new routine, wcsset(), parses the CTYPEn. - The high level driver routines of WCSLIB 1.0 are available as intermediate level drivers celset(), celfwd(), and celrev(), but note that their argument lists have been extended to return native coordinates. The related struct is now called celprm instead of wcsprm. - The reference point for conic projections is now at the midpoint of the standard parallels. The FITS header cards PROJP1 and PROJP2 now give the half-sum (midpoint) and half-difference of the latitudes of the standard parallels; previously they gave the latitudes of the standard parallels themselves. The change is reflected in this release of WCSLIB. - A bug in celset() (formerly wcsset()) that misapplied WCS draft equations 7 has been fixed (thanks to Rick Ebert IPAC/JPL and Lindsey Davis, NOAO for reporting this). This affected the computation of Euler angles for the celestial coordinate transformation for those projections that have their reference point away from the native pole. In investigating this a deficiency with the formalism was discovered that led to the introduction of a LATPOLE FITS header card which may be used to disambiguate where CRVAL1, CRVAL2, and LONGPOLE do not uniquely determine the latitude of the native pole. The celprm struct (formerly wcsprm) has been extended to accomodate LATPOLE. - Default values of LONGPOLE and LATPOLE are now supported and their use is recommended where appropriate. - Numerical precision was being lost near the native poles in the SIN, AIR, and QSC projections and this has been recovered (reported by Lindsey Davis, NOAO). Floating underflows in CSC are now avoided. - Numerical precision was also lost in certain circumstances in the spherical coordinate transformation routines and this has been fixed. - The test programs have been enhanced in various ways and the library has been validated on an SGI machine using both 32-bit and 64-bit compilers. * Fortran library The main change of interest to programmers is that of changed call sequences for WCSFWD and WCSREV as described below. - The WCS linear transformations are now implemented in WCSLIB, complete with matrix inverter. The new files are lin.f and test program tlin.f. - Given either the celestial longitude or latitude plus an element of the pixel coordinate a new routine, WCSMIX, solves for the remaining elements by iterating on the unknown celestial coordinate element using WCSFWD. - The high level driver routines WCSFWD, WCSREV, and WCSMIX now apply the full WCS algorithm chain (except for pixel regularization table), including parsing the CTYPEn header cards and computing non- celestial elements of the world coordinate. This required a change to their call sequences which now more closely reflect the sequence of algorithms applied. A new routine, WCSSET, parses the CTYPEn. - The high level driver routines of WCSLIB 1.0 are available as intermediate level drivers CELSET, CELFWD, and CELREV, but note that their call sequences have been extended to return native coordinates. The related parameter array is now called CEL instead of WCS. - The reference point for conic projections is now at the midpoint of the standard parallels. The FITS header cards PROJP1 and PROJP2 now give the half-sum (midpoint) and half-difference of the latitudes of the standard parallels; previously they gave the latitudes of the standard parallels themselves. The change is reflected in this release of WCSLIB. - A bug in CELSET (formerly WCSSET) that misapplied WCS draft equations 7 has been fixed (thanks to Rick Ebert IPAC/JPL and Lindsey Davis, NOAO for reporting this). This affected the computation of Euler angles for the celestial coordinate transformation for those projections that have their reference point away from the native pole. In investigating this a deficiency with the formalism was discovered that led to the introduction of a LATPOLE FITS header card which may be used to disambiguate where CRVAL1, CRVAL2, and LONGPOLE do not uniquely determine the latitude of the native pole. The CEL parameter array (formerly WCS) has been extended to accomodate LATPOLE as CEL(4), and the flag variable is now CEL(5) (formerly WCS(4)). - Default values of LONGPOLE and LATPOLE are now supported and their use is recommended where appropriate. - Numerical precision was being lost near the native poles in the SIN, AIR, and QSC projections and this has been recovered (reported by Lindsey Davis, NOAO). Floating underflows in CSC are now avoided. - Numerical precision was also lost in certain circumstances in the spherical coordinate transformation routines and this has been fixed. - The test programs have been enhanced in various ways and the library has been validated on an SGI machine using both 32-bit and 64-bit compilers. WCSLIB version 1.0 (1995/01/31) ------------------------------- * C library Initial release. * Fortran library Initial release. ------------------------------------------------------------------------ $Id: CHANGES,v 4.10 2012/02/05 23:41:45 cal103 Exp $ pywcs-1.12/wcslib/config/0000755001153600020070000000000012310355732017374 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/config/config.guess0000755001153600020070000012675512310355626021736 0ustar cslocumSTSCI\science00000000000000#! /bin/sh # Attempt to guess a canonical system name. # Copyright (C) 1992, 1993, 1994, 1995, 1996, 1997, 1998, 1999, # 2000, 2001, 2002, 2003, 2004, 2005, 2006, 2007, 2008, 2009, 2010, # 2011 Free Software Foundation, Inc. timestamp='2011-10-01' # This file is free software; you can redistribute it and/or modify it # under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, but # WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. 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The system name ranges from "MiNT" over "FreeMiNT" # to the lowercase version "mint" (or "freemint"). Finally # the system name "TOS" denotes a system which is actually not # MiNT. But MiNT is downward compatible to TOS, so this should # be no problem. atarist[e]:*MiNT:*:* | atarist[e]:*mint:*:* | atarist[e]:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; atari*:*MiNT:*:* | atari*:*mint:*:* | atarist[e]:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; *falcon*:*MiNT:*:* | *falcon*:*mint:*:* | *falcon*:*TOS:*:*) echo m68k-atari-mint${UNAME_RELEASE} exit ;; milan*:*MiNT:*:* | milan*:*mint:*:* | *milan*:*TOS:*:*) echo m68k-milan-mint${UNAME_RELEASE} exit ;; hades*:*MiNT:*:* | hades*:*mint:*:* | *hades*:*TOS:*:*) echo m68k-hades-mint${UNAME_RELEASE} exit ;; *:*MiNT:*:* | *:*mint:*:* | *:*TOS:*:*) echo m68k-unknown-mint${UNAME_RELEASE} exit ;; m68k:machten:*:*) echo m68k-apple-machten${UNAME_RELEASE} exit ;; powerpc:machten:*:*) echo powerpc-apple-machten${UNAME_RELEASE} exit ;; RISC*:Mach:*:*) echo mips-dec-mach_bsd4.3 exit ;; RISC*:ULTRIX:*:*) echo mips-dec-ultrix${UNAME_RELEASE} exit ;; VAX*:ULTRIX*:*:*) echo vax-dec-ultrix${UNAME_RELEASE} exit ;; 2020:CLIX:*:* | 2430:CLIX:*:*) echo clipper-intergraph-clix${UNAME_RELEASE} exit ;; mips:*:*:UMIPS | mips:*:*:RISCos) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #ifdef __cplusplus #include /* for printf() prototype */ int main (int argc, char *argv[]) { #else int main (argc, argv) int argc; char *argv[]; { #endif #if defined (host_mips) && defined (MIPSEB) #if defined (SYSTYPE_SYSV) printf ("mips-mips-riscos%ssysv\n", argv[1]); exit (0); #endif #if defined (SYSTYPE_SVR4) printf ("mips-mips-riscos%ssvr4\n", argv[1]); exit (0); #endif #if defined (SYSTYPE_BSD43) || defined(SYSTYPE_BSD) printf ("mips-mips-riscos%sbsd\n", argv[1]); exit (0); #endif #endif exit (-1); } EOF $CC_FOR_BUILD -o $dummy $dummy.c && dummyarg=`echo "${UNAME_RELEASE}" | sed -n 's/\([0-9]*\).*/\1/p'` && SYSTEM_NAME=`$dummy $dummyarg` && { echo "$SYSTEM_NAME"; exit; } echo mips-mips-riscos${UNAME_RELEASE} exit ;; Motorola:PowerMAX_OS:*:*) echo powerpc-motorola-powermax exit ;; Motorola:*:4.3:PL8-*) echo powerpc-harris-powermax exit ;; Night_Hawk:*:*:PowerMAX_OS | Synergy:PowerMAX_OS:*:*) echo powerpc-harris-powermax exit ;; Night_Hawk:Power_UNIX:*:*) echo powerpc-harris-powerunix exit ;; m88k:CX/UX:7*:*) echo m88k-harris-cxux7 exit ;; m88k:*:4*:R4*) echo m88k-motorola-sysv4 exit ;; m88k:*:3*:R3*) echo m88k-motorola-sysv3 exit ;; AViiON:dgux:*:*) # DG/UX returns AViiON for all architectures UNAME_PROCESSOR=`/usr/bin/uname -p` if [ $UNAME_PROCESSOR = mc88100 ] || [ $UNAME_PROCESSOR = mc88110 ] then if [ ${TARGET_BINARY_INTERFACE}x = m88kdguxelfx ] || \ [ ${TARGET_BINARY_INTERFACE}x = x ] then echo m88k-dg-dgux${UNAME_RELEASE} else echo m88k-dg-dguxbcs${UNAME_RELEASE} fi else echo i586-dg-dgux${UNAME_RELEASE} fi exit ;; M88*:DolphinOS:*:*) # DolphinOS (SVR3) echo m88k-dolphin-sysv3 exit ;; M88*:*:R3*:*) # Delta 88k system running SVR3 echo m88k-motorola-sysv3 exit ;; XD88*:*:*:*) # Tektronix XD88 system running UTekV (SVR3) echo m88k-tektronix-sysv3 exit ;; Tek43[0-9][0-9]:UTek:*:*) # Tektronix 4300 system running UTek (BSD) echo m68k-tektronix-bsd exit ;; *:IRIX*:*:*) echo mips-sgi-irix`echo ${UNAME_RELEASE}|sed -e 's/-/_/g'` exit ;; ????????:AIX?:[12].1:2) # AIX 2.2.1 or AIX 2.1.1 is RT/PC AIX. echo romp-ibm-aix # uname -m gives an 8 hex-code CPU id exit ;; # Note that: echo "'`uname -s`'" gives 'AIX ' i*86:AIX:*:*) echo i386-ibm-aix exit ;; ia64:AIX:*:*) if [ -x /usr/bin/oslevel ] ; then IBM_REV=`/usr/bin/oslevel` else IBM_REV=${UNAME_VERSION}.${UNAME_RELEASE} fi echo ${UNAME_MACHINE}-ibm-aix${IBM_REV} exit ;; *:AIX:2:3) if grep bos325 /usr/include/stdio.h >/dev/null 2>&1; then eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #include main() { if (!__power_pc()) exit(1); puts("powerpc-ibm-aix3.2.5"); exit(0); } EOF if $CC_FOR_BUILD -o $dummy $dummy.c && SYSTEM_NAME=`$dummy` then echo "$SYSTEM_NAME" else echo rs6000-ibm-aix3.2.5 fi elif grep bos324 /usr/include/stdio.h >/dev/null 2>&1; then echo rs6000-ibm-aix3.2.4 else echo rs6000-ibm-aix3.2 fi exit ;; *:AIX:*:[4567]) IBM_CPU_ID=`/usr/sbin/lsdev -C -c processor -S available | sed 1q | awk '{ print $1 }'` if /usr/sbin/lsattr -El ${IBM_CPU_ID} | grep ' POWER' >/dev/null 2>&1; then IBM_ARCH=rs6000 else IBM_ARCH=powerpc fi if [ -x /usr/bin/oslevel ] ; then IBM_REV=`/usr/bin/oslevel` else IBM_REV=${UNAME_VERSION}.${UNAME_RELEASE} fi echo ${IBM_ARCH}-ibm-aix${IBM_REV} exit ;; *:AIX:*:*) echo rs6000-ibm-aix exit ;; ibmrt:4.4BSD:*|romp-ibm:BSD:*) echo romp-ibm-bsd4.4 exit ;; ibmrt:*BSD:*|romp-ibm:BSD:*) # covers RT/PC BSD and echo romp-ibm-bsd${UNAME_RELEASE} # 4.3 with uname added to exit ;; # report: romp-ibm BSD 4.3 *:BOSX:*:*) echo rs6000-bull-bosx exit ;; DPX/2?00:B.O.S.:*:*) echo m68k-bull-sysv3 exit ;; 9000/[34]??:4.3bsd:1.*:*) echo m68k-hp-bsd exit ;; hp300:4.4BSD:*:* | 9000/[34]??:4.3bsd:2.*:*) echo m68k-hp-bsd4.4 exit ;; 9000/[34678]??:HP-UX:*:*) HPUX_REV=`echo ${UNAME_RELEASE}|sed -e 's/[^.]*.[0B]*//'` case "${UNAME_MACHINE}" in 9000/31? ) HP_ARCH=m68000 ;; 9000/[34]?? ) HP_ARCH=m68k ;; 9000/[678][0-9][0-9]) if [ -x /usr/bin/getconf ]; then sc_cpu_version=`/usr/bin/getconf SC_CPU_VERSION 2>/dev/null` sc_kernel_bits=`/usr/bin/getconf SC_KERNEL_BITS 2>/dev/null` case "${sc_cpu_version}" in 523) HP_ARCH="hppa1.0" ;; # CPU_PA_RISC1_0 528) HP_ARCH="hppa1.1" ;; # CPU_PA_RISC1_1 532) # CPU_PA_RISC2_0 case "${sc_kernel_bits}" in 32) HP_ARCH="hppa2.0n" ;; 64) HP_ARCH="hppa2.0w" ;; '') HP_ARCH="hppa2.0" ;; # HP-UX 10.20 esac ;; esac fi if [ "${HP_ARCH}" = "" ]; then eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #define _HPUX_SOURCE #include #include int main () { #if defined(_SC_KERNEL_BITS) long bits = sysconf(_SC_KERNEL_BITS); #endif long cpu = sysconf (_SC_CPU_VERSION); switch (cpu) { case CPU_PA_RISC1_0: puts ("hppa1.0"); break; case CPU_PA_RISC1_1: puts ("hppa1.1"); break; case CPU_PA_RISC2_0: #if defined(_SC_KERNEL_BITS) switch (bits) { case 64: puts ("hppa2.0w"); break; case 32: puts ("hppa2.0n"); break; default: puts ("hppa2.0"); break; } break; #else /* !defined(_SC_KERNEL_BITS) */ puts ("hppa2.0"); break; #endif default: puts ("hppa1.0"); break; } exit (0); } EOF (CCOPTS= $CC_FOR_BUILD -o $dummy $dummy.c 2>/dev/null) && HP_ARCH=`$dummy` test -z "$HP_ARCH" && HP_ARCH=hppa fi ;; esac if [ ${HP_ARCH} = "hppa2.0w" ] then eval $set_cc_for_build # hppa2.0w-hp-hpux* has a 64-bit kernel and a compiler generating # 32-bit code. hppa64-hp-hpux* has the same kernel and a compiler # generating 64-bit code. GNU and HP use different nomenclature: # # $ CC_FOR_BUILD=cc ./config.guess # => hppa2.0w-hp-hpux11.23 # $ CC_FOR_BUILD="cc +DA2.0w" ./config.guess # => hppa64-hp-hpux11.23 if echo __LP64__ | (CCOPTS= $CC_FOR_BUILD -E - 2>/dev/null) | grep -q __LP64__ then HP_ARCH="hppa2.0w" else HP_ARCH="hppa64" fi fi echo ${HP_ARCH}-hp-hpux${HPUX_REV} exit ;; ia64:HP-UX:*:*) HPUX_REV=`echo ${UNAME_RELEASE}|sed -e 's/[^.]*.[0B]*//'` echo ia64-hp-hpux${HPUX_REV} exit ;; 3050*:HI-UX:*:*) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #include int main () { long cpu = sysconf (_SC_CPU_VERSION); /* The order matters, because CPU_IS_HP_MC68K erroneously returns true for CPU_PA_RISC1_0. CPU_IS_PA_RISC returns correct results, however. */ if (CPU_IS_PA_RISC (cpu)) { switch (cpu) { case CPU_PA_RISC1_0: puts ("hppa1.0-hitachi-hiuxwe2"); break; case CPU_PA_RISC1_1: puts ("hppa1.1-hitachi-hiuxwe2"); break; case CPU_PA_RISC2_0: puts ("hppa2.0-hitachi-hiuxwe2"); break; default: puts ("hppa-hitachi-hiuxwe2"); break; } } else if (CPU_IS_HP_MC68K (cpu)) puts ("m68k-hitachi-hiuxwe2"); else puts ("unknown-hitachi-hiuxwe2"); exit (0); } EOF $CC_FOR_BUILD -o $dummy $dummy.c && SYSTEM_NAME=`$dummy` && { echo "$SYSTEM_NAME"; exit; } echo unknown-hitachi-hiuxwe2 exit ;; 9000/7??:4.3bsd:*:* | 9000/8?[79]:4.3bsd:*:* ) echo hppa1.1-hp-bsd exit ;; 9000/8??:4.3bsd:*:*) echo hppa1.0-hp-bsd exit ;; *9??*:MPE/iX:*:* | *3000*:MPE/iX:*:*) echo hppa1.0-hp-mpeix exit ;; hp7??:OSF1:*:* | hp8?[79]:OSF1:*:* ) echo hppa1.1-hp-osf exit ;; hp8??:OSF1:*:*) echo hppa1.0-hp-osf exit ;; i*86:OSF1:*:*) if [ -x /usr/sbin/sysversion ] ; then echo ${UNAME_MACHINE}-unknown-osf1mk else echo ${UNAME_MACHINE}-unknown-osf1 fi exit ;; parisc*:Lites*:*:*) echo hppa1.1-hp-lites exit ;; C1*:ConvexOS:*:* | convex:ConvexOS:C1*:*) echo c1-convex-bsd exit ;; C2*:ConvexOS:*:* | convex:ConvexOS:C2*:*) if getsysinfo -f scalar_acc then echo c32-convex-bsd else echo c2-convex-bsd fi exit ;; C34*:ConvexOS:*:* | convex:ConvexOS:C34*:*) echo c34-convex-bsd exit ;; C38*:ConvexOS:*:* | convex:ConvexOS:C38*:*) echo c38-convex-bsd exit ;; C4*:ConvexOS:*:* | convex:ConvexOS:C4*:*) echo c4-convex-bsd exit ;; CRAY*Y-MP:*:*:*) echo ymp-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*[A-Z]90:*:*:*) echo ${UNAME_MACHINE}-cray-unicos${UNAME_RELEASE} \ | sed -e 's/CRAY.*\([A-Z]90\)/\1/' \ -e y/ABCDEFGHIJKLMNOPQRSTUVWXYZ/abcdefghijklmnopqrstuvwxyz/ \ -e 's/\.[^.]*$/.X/' exit ;; CRAY*TS:*:*:*) echo t90-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*T3E:*:*:*) echo alphaev5-cray-unicosmk${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; CRAY*SV1:*:*:*) echo sv1-cray-unicos${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; *:UNICOS/mp:*:*) echo craynv-cray-unicosmp${UNAME_RELEASE} | sed -e 's/\.[^.]*$/.X/' exit ;; F30[01]:UNIX_System_V:*:* | F700:UNIX_System_V:*:*) FUJITSU_PROC=`uname -m | tr 'ABCDEFGHIJKLMNOPQRSTUVWXYZ' 'abcdefghijklmnopqrstuvwxyz'` FUJITSU_SYS=`uname -p | tr 'ABCDEFGHIJKLMNOPQRSTUVWXYZ' 'abcdefghijklmnopqrstuvwxyz' | sed -e 's/\///'` FUJITSU_REL=`echo ${UNAME_RELEASE} | sed -e 's/ /_/'` echo "${FUJITSU_PROC}-fujitsu-${FUJITSU_SYS}${FUJITSU_REL}" exit ;; 5000:UNIX_System_V:4.*:*) FUJITSU_SYS=`uname -p | tr 'ABCDEFGHIJKLMNOPQRSTUVWXYZ' 'abcdefghijklmnopqrstuvwxyz' | sed -e 's/\///'` FUJITSU_REL=`echo ${UNAME_RELEASE} | tr 'ABCDEFGHIJKLMNOPQRSTUVWXYZ' 'abcdefghijklmnopqrstuvwxyz' | sed -e 's/ /_/'` echo "sparc-fujitsu-${FUJITSU_SYS}${FUJITSU_REL}" exit ;; i*86:BSD/386:*:* | i*86:BSD/OS:*:* | *:Ascend\ Embedded/OS:*:*) echo ${UNAME_MACHINE}-pc-bsdi${UNAME_RELEASE} exit ;; sparc*:BSD/OS:*:*) echo sparc-unknown-bsdi${UNAME_RELEASE} exit ;; *:BSD/OS:*:*) echo ${UNAME_MACHINE}-unknown-bsdi${UNAME_RELEASE} exit ;; *:FreeBSD:*:*) UNAME_PROCESSOR=`/usr/bin/uname -p` case ${UNAME_PROCESSOR} in amd64) echo x86_64-unknown-freebsd`echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'` ;; *) echo ${UNAME_PROCESSOR}-unknown-freebsd`echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'` ;; esac exit ;; i*:CYGWIN*:*) echo ${UNAME_MACHINE}-pc-cygwin exit ;; *:MINGW*:*) echo ${UNAME_MACHINE}-pc-mingw32 exit ;; i*:windows32*:*) # uname -m includes "-pc" on this system. echo ${UNAME_MACHINE}-mingw32 exit ;; i*:PW*:*) echo ${UNAME_MACHINE}-pc-pw32 exit ;; *:Interix*:*) case ${UNAME_MACHINE} in x86) echo i586-pc-interix${UNAME_RELEASE} exit ;; authenticamd | genuineintel | EM64T) echo x86_64-unknown-interix${UNAME_RELEASE} exit ;; IA64) echo ia64-unknown-interix${UNAME_RELEASE} exit ;; esac ;; [345]86:Windows_95:* | [345]86:Windows_98:* | [345]86:Windows_NT:*) echo i${UNAME_MACHINE}-pc-mks exit ;; 8664:Windows_NT:*) echo x86_64-pc-mks exit ;; i*:Windows_NT*:* | Pentium*:Windows_NT*:*) # How do we know it's Interix rather than the generic POSIX subsystem? # It also conflicts with pre-2.0 versions of AT&T UWIN. Should we # UNAME_MACHINE based on the output of uname instead of i386? echo i586-pc-interix exit ;; i*:UWIN*:*) echo ${UNAME_MACHINE}-pc-uwin exit ;; amd64:CYGWIN*:*:* | x86_64:CYGWIN*:*:*) echo x86_64-unknown-cygwin exit ;; p*:CYGWIN*:*) echo powerpcle-unknown-cygwin exit ;; prep*:SunOS:5.*:*) echo powerpcle-unknown-solaris2`echo ${UNAME_RELEASE}|sed -e 's/[^.]*//'` exit ;; *:GNU:*:*) # the GNU system echo `echo ${UNAME_MACHINE}|sed -e 's,[-/].*$,,'`-unknown-gnu`echo ${UNAME_RELEASE}|sed -e 's,/.*$,,'` exit ;; *:GNU/*:*:*) # other systems with GNU libc and userland echo ${UNAME_MACHINE}-unknown-`echo ${UNAME_SYSTEM} | sed 's,^[^/]*/,,' | tr '[A-Z]' '[a-z]'``echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'`-gnu exit ;; i*86:Minix:*:*) echo ${UNAME_MACHINE}-pc-minix exit ;; alpha:Linux:*:*) case `sed -n '/^cpu model/s/^.*: \(.*\)/\1/p' < /proc/cpuinfo` in EV5) UNAME_MACHINE=alphaev5 ;; EV56) UNAME_MACHINE=alphaev56 ;; PCA56) UNAME_MACHINE=alphapca56 ;; PCA57) UNAME_MACHINE=alphapca56 ;; EV6) UNAME_MACHINE=alphaev6 ;; EV67) UNAME_MACHINE=alphaev67 ;; EV68*) UNAME_MACHINE=alphaev68 ;; esac objdump --private-headers /bin/sh | grep -q ld.so.1 if test "$?" = 0 ; then LIBC="libc1" ; else LIBC="" ; fi echo ${UNAME_MACHINE}-unknown-linux-gnu${LIBC} exit ;; arm*:Linux:*:*) eval $set_cc_for_build if echo __ARM_EABI__ | $CC_FOR_BUILD -E - 2>/dev/null \ | grep -q __ARM_EABI__ then echo ${UNAME_MACHINE}-unknown-linux-gnu else if echo __ARM_PCS_VFP | $CC_FOR_BUILD -E - 2>/dev/null \ | grep -q __ARM_PCS_VFP then echo ${UNAME_MACHINE}-unknown-linux-gnueabi else echo ${UNAME_MACHINE}-unknown-linux-gnueabihf fi fi exit ;; avr32*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; cris:Linux:*:*) echo cris-axis-linux-gnu exit ;; crisv32:Linux:*:*) echo crisv32-axis-linux-gnu exit ;; frv:Linux:*:*) echo frv-unknown-linux-gnu exit ;; hexagon:Linux:*:*) echo hexagon-unknown-linux-gnu exit ;; i*86:Linux:*:*) LIBC=gnu eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #ifdef __dietlibc__ LIBC=dietlibc #endif EOF eval `$CC_FOR_BUILD -E $dummy.c 2>/dev/null | grep '^LIBC'` echo "${UNAME_MACHINE}-pc-linux-${LIBC}" exit ;; ia64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; m32r*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; m68*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; mips:Linux:*:* | mips64:Linux:*:*) eval $set_cc_for_build sed 's/^ //' << EOF >$dummy.c #undef CPU #undef ${UNAME_MACHINE} #undef ${UNAME_MACHINE}el #if defined(__MIPSEL__) || defined(__MIPSEL) || defined(_MIPSEL) || defined(MIPSEL) CPU=${UNAME_MACHINE}el #else #if defined(__MIPSEB__) || defined(__MIPSEB) || defined(_MIPSEB) || defined(MIPSEB) CPU=${UNAME_MACHINE} #else CPU= #endif #endif EOF eval `$CC_FOR_BUILD -E $dummy.c 2>/dev/null | grep '^CPU'` test x"${CPU}" != x && { echo "${CPU}-unknown-linux-gnu"; exit; } ;; or32:Linux:*:*) echo or32-unknown-linux-gnu exit ;; padre:Linux:*:*) echo sparc-unknown-linux-gnu exit ;; parisc64:Linux:*:* | hppa64:Linux:*:*) echo hppa64-unknown-linux-gnu exit ;; parisc:Linux:*:* | hppa:Linux:*:*) # Look for CPU level case `grep '^cpu[^a-z]*:' /proc/cpuinfo 2>/dev/null | cut -d' ' -f2` in PA7*) echo hppa1.1-unknown-linux-gnu ;; PA8*) echo hppa2.0-unknown-linux-gnu ;; *) echo hppa-unknown-linux-gnu ;; esac exit ;; ppc64:Linux:*:*) echo powerpc64-unknown-linux-gnu exit ;; ppc:Linux:*:*) echo powerpc-unknown-linux-gnu exit ;; s390:Linux:*:* | s390x:Linux:*:*) echo ${UNAME_MACHINE}-ibm-linux exit ;; sh64*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; sh*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; sparc:Linux:*:* | sparc64:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; tile*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; vax:Linux:*:*) echo ${UNAME_MACHINE}-dec-linux-gnu exit ;; x86_64:Linux:*:*) echo x86_64-unknown-linux-gnu exit ;; xtensa*:Linux:*:*) echo ${UNAME_MACHINE}-unknown-linux-gnu exit ;; i*86:DYNIX/ptx:4*:*) # ptx 4.0 does uname -s correctly, with DYNIX/ptx in there. # earlier versions are messed up and put the nodename in both # sysname and nodename. echo i386-sequent-sysv4 exit ;; i*86:UNIX_SV:4.2MP:2.*) # Unixware is an offshoot of SVR4, but it has its own version # number series starting with 2... # I am not positive that other SVR4 systems won't match this, # I just have to hope. -- rms. # Use sysv4.2uw... so that sysv4* matches it. echo ${UNAME_MACHINE}-pc-sysv4.2uw${UNAME_VERSION} exit ;; i*86:OS/2:*:*) # If we were able to find `uname', then EMX Unix compatibility # is probably installed. echo ${UNAME_MACHINE}-pc-os2-emx exit ;; i*86:XTS-300:*:STOP) echo ${UNAME_MACHINE}-unknown-stop exit ;; i*86:atheos:*:*) echo ${UNAME_MACHINE}-unknown-atheos exit ;; i*86:syllable:*:*) echo ${UNAME_MACHINE}-pc-syllable exit ;; i*86:LynxOS:2.*:* | i*86:LynxOS:3.[01]*:* | i*86:LynxOS:4.[02]*:*) echo i386-unknown-lynxos${UNAME_RELEASE} exit ;; i*86:*DOS:*:*) echo ${UNAME_MACHINE}-pc-msdosdjgpp exit ;; i*86:*:4.*:* | i*86:SYSTEM_V:4.*:*) UNAME_REL=`echo ${UNAME_RELEASE} | sed 's/\/MP$//'` if grep Novell /usr/include/link.h >/dev/null 2>/dev/null; then echo ${UNAME_MACHINE}-univel-sysv${UNAME_REL} else echo ${UNAME_MACHINE}-pc-sysv${UNAME_REL} fi exit ;; i*86:*:5:[678]*) # UnixWare 7.x, OpenUNIX and OpenServer 6. case `/bin/uname -X | grep "^Machine"` in *486*) UNAME_MACHINE=i486 ;; *Pentium) UNAME_MACHINE=i586 ;; *Pent*|*Celeron) UNAME_MACHINE=i686 ;; esac echo ${UNAME_MACHINE}-unknown-sysv${UNAME_RELEASE}${UNAME_SYSTEM}${UNAME_VERSION} exit ;; i*86:*:3.2:*) if test -f /usr/options/cb.name; then UNAME_REL=`sed -n 's/.*Version //p' /dev/null >/dev/null ; then UNAME_REL=`(/bin/uname -X|grep Release|sed -e 's/.*= //')` (/bin/uname -X|grep i80486 >/dev/null) && UNAME_MACHINE=i486 (/bin/uname -X|grep '^Machine.*Pentium' >/dev/null) \ && UNAME_MACHINE=i586 (/bin/uname -X|grep '^Machine.*Pent *II' >/dev/null) \ && UNAME_MACHINE=i686 (/bin/uname -X|grep '^Machine.*Pentium Pro' >/dev/null) \ && UNAME_MACHINE=i686 echo ${UNAME_MACHINE}-pc-sco$UNAME_REL else echo ${UNAME_MACHINE}-pc-sysv32 fi exit ;; pc:*:*:*) # Left here for compatibility: # uname -m prints for DJGPP always 'pc', but it prints nothing about # the processor, so we play safe by assuming i586. # Note: whatever this is, it MUST be the same as what config.sub # prints for the "djgpp" host, or else GDB configury will decide that # this is a cross-build. echo i586-pc-msdosdjgpp exit ;; Intel:Mach:3*:*) echo i386-pc-mach3 exit ;; paragon:*:*:*) echo i860-intel-osf1 exit ;; i860:*:4.*:*) # i860-SVR4 if grep Stardent /usr/include/sys/uadmin.h >/dev/null 2>&1 ; then echo i860-stardent-sysv${UNAME_RELEASE} # Stardent Vistra i860-SVR4 else # Add other i860-SVR4 vendors below as they are discovered. echo i860-unknown-sysv${UNAME_RELEASE} # Unknown i860-SVR4 fi exit ;; mini*:CTIX:SYS*5:*) # "miniframe" echo m68010-convergent-sysv exit ;; mc68k:UNIX:SYSTEM5:3.51m) echo m68k-convergent-sysv exit ;; M680?0:D-NIX:5.3:*) echo m68k-diab-dnix exit ;; M68*:*:R3V[5678]*:*) test -r /sysV68 && { echo 'm68k-motorola-sysv'; exit; } ;; 3[345]??:*:4.0:3.0 | 3[34]??A:*:4.0:3.0 | 3[34]??,*:*:4.0:3.0 | 3[34]??/*:*:4.0:3.0 | 4400:*:4.0:3.0 | 4850:*:4.0:3.0 | SKA40:*:4.0:3.0 | SDS2:*:4.0:3.0 | SHG2:*:4.0:3.0 | S7501*:*:4.0:3.0) OS_REL='' test -r /etc/.relid \ && OS_REL=.`sed -n 's/[^ ]* [^ ]* \([0-9][0-9]\).*/\1/p' < /etc/.relid` /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4.3${OS_REL}; exit; } /bin/uname -p 2>/dev/null | /bin/grep entium >/dev/null \ && { echo i586-ncr-sysv4.3${OS_REL}; exit; } ;; 3[34]??:*:4.0:* | 3[34]??,*:*:4.0:*) /bin/uname -p 2>/dev/null | grep 86 >/dev/null \ && { echo i486-ncr-sysv4; 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*:SINIX-*:*:*) if uname -p 2>/dev/null >/dev/null ; then UNAME_MACHINE=`(uname -p) 2>/dev/null` echo ${UNAME_MACHINE}-sni-sysv4 else echo ns32k-sni-sysv fi exit ;; PENTIUM:*:4.0*:*) # Unisys `ClearPath HMP IX 4000' SVR4/MP effort # says echo i586-unisys-sysv4 exit ;; *:UNIX_System_V:4*:FTX*) # From Gerald Hewes . # How about differentiating between stratus architectures? -djm echo hppa1.1-stratus-sysv4 exit ;; *:*:*:FTX*) # From seanf@swdc.stratus.com. echo i860-stratus-sysv4 exit ;; i*86:VOS:*:*) # From Paul.Green@stratus.com. echo ${UNAME_MACHINE}-stratus-vos exit ;; *:VOS:*:*) # From Paul.Green@stratus.com. echo hppa1.1-stratus-vos exit ;; mc68*:A/UX:*:*) echo m68k-apple-aux${UNAME_RELEASE} exit ;; news*:NEWS-OS:6*:*) echo mips-sony-newsos6 exit ;; R[34]000:*System_V*:*:* | R4000:UNIX_SYSV:*:* | R*000:UNIX_SV:*:*) if [ -d /usr/nec ]; then echo mips-nec-sysv${UNAME_RELEASE} else echo mips-unknown-sysv${UNAME_RELEASE} fi exit ;; BeBox:BeOS:*:*) # BeOS running on hardware made by Be, PPC only. echo powerpc-be-beos exit ;; 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echo '#endif') | \ (CCOPTS= $CC_FOR_BUILD -E - 2>/dev/null) | \ grep IS_64BIT_ARCH >/dev/null then UNAME_PROCESSOR="x86_64" fi fi ;; unknown) UNAME_PROCESSOR=powerpc ;; esac echo ${UNAME_PROCESSOR}-apple-darwin${UNAME_RELEASE} exit ;; *:procnto*:*:* | *:QNX:[0123456789]*:*) UNAME_PROCESSOR=`uname -p` if test "$UNAME_PROCESSOR" = "x86"; then UNAME_PROCESSOR=i386 UNAME_MACHINE=pc fi echo ${UNAME_PROCESSOR}-${UNAME_MACHINE}-nto-qnx${UNAME_RELEASE} exit ;; *:QNX:*:4*) echo i386-pc-qnx exit ;; NEO-?:NONSTOP_KERNEL:*:*) echo neo-tandem-nsk${UNAME_RELEASE} exit ;; NSE-?:NONSTOP_KERNEL:*:*) echo nse-tandem-nsk${UNAME_RELEASE} exit ;; NSR-?:NONSTOP_KERNEL:*:*) echo nsr-tandem-nsk${UNAME_RELEASE} exit ;; *:NonStop-UX:*:*) echo mips-compaq-nonstopux exit ;; BS2000:POSIX*:*:*) echo bs2000-siemens-sysv exit ;; DS/*:UNIX_System_V:*:*) echo ${UNAME_MACHINE}-${UNAME_SYSTEM}-${UNAME_RELEASE} exit ;; *:Plan9:*:*) # "uname -m" is not consistent, so use $cputype instead. 386 # is converted to i386 for consistency with other x86 # operating systems. if test "$cputype" = "386"; then UNAME_MACHINE=i386 else UNAME_MACHINE="$cputype" fi echo ${UNAME_MACHINE}-unknown-plan9 exit ;; *:TOPS-10:*:*) echo pdp10-unknown-tops10 exit ;; *:TENEX:*:*) echo pdp10-unknown-tenex exit ;; KS10:TOPS-20:*:* | KL10:TOPS-20:*:* | TYPE4:TOPS-20:*:*) echo pdp10-dec-tops20 exit ;; XKL-1:TOPS-20:*:* | TYPE5:TOPS-20:*:*) echo pdp10-xkl-tops20 exit ;; *:TOPS-20:*:*) echo pdp10-unknown-tops20 exit ;; *:ITS:*:*) echo pdp10-unknown-its exit ;; SEI:*:*:SEIUX) echo mips-sei-seiux${UNAME_RELEASE} exit ;; *:DragonFly:*:*) echo ${UNAME_MACHINE}-unknown-dragonfly`echo ${UNAME_RELEASE}|sed -e 's/[-(].*//'` exit ;; *:*VMS:*:*) UNAME_MACHINE=`(uname -p) 2>/dev/null` case "${UNAME_MACHINE}" in A*) echo alpha-dec-vms ; exit ;; I*) echo ia64-dec-vms ; exit ;; V*) echo vax-dec-vms ; exit ;; esac ;; *:XENIX:*:SysV) echo i386-pc-xenix exit ;; i*86:skyos:*:*) echo ${UNAME_MACHINE}-pc-skyos`echo ${UNAME_RELEASE}` | sed -e 's/ .*$//' exit ;; i*86:rdos:*:*) echo ${UNAME_MACHINE}-pc-rdos exit ;; i*86:AROS:*:*) echo ${UNAME_MACHINE}-pc-aros exit ;; esac #echo '(No uname command or uname output not recognized.)' 1>&2 #echo "${UNAME_MACHINE}:${UNAME_SYSTEM}:${UNAME_RELEASE}:${UNAME_VERSION}" 1>&2 eval $set_cc_for_build cat >$dummy.c < # include #endif main () { #if defined (sony) #if defined (MIPSEB) /* BFD wants "bsd" instead of "newsos". Perhaps BFD should be changed, I don't know.... */ printf ("mips-sony-bsd\n"); exit (0); #else #include printf ("m68k-sony-newsos%s\n", #ifdef NEWSOS4 "4" #else "" #endif ); exit (0); #endif #endif #if defined (__arm) && defined (__acorn) && defined (__unix) printf ("arm-acorn-riscix\n"); exit (0); #endif #if defined (hp300) && !defined (hpux) printf ("m68k-hp-bsd\n"); exit (0); #endif #if defined (NeXT) #if !defined (__ARCHITECTURE__) #define __ARCHITECTURE__ "m68k" #endif int version; version=`(hostinfo | sed -n 's/.*NeXT Mach \([0-9]*\).*/\1/p') 2>/dev/null`; if (version < 4) printf ("%s-next-nextstep%d\n", __ARCHITECTURE__, version); else printf ("%s-next-openstep%d\n", __ARCHITECTURE__, version); exit (0); #endif #if defined (MULTIMAX) || defined (n16) #if defined (UMAXV) printf ("ns32k-encore-sysv\n"); exit (0); #else #if defined (CMU) printf ("ns32k-encore-mach\n"); exit (0); #else printf ("ns32k-encore-bsd\n"); exit (0); #endif #endif #endif #if defined (__386BSD__) printf ("i386-pc-bsd\n"); exit (0); #endif #if defined (sequent) #if defined (i386) printf ("i386-sequent-dynix\n"); exit (0); #endif #if defined (ns32000) printf ("ns32k-sequent-dynix\n"); exit (0); #endif #endif #if defined (_SEQUENT_) struct utsname un; uname(&un); if (strncmp(un.version, "V2", 2) == 0) { printf ("i386-sequent-ptx2\n"); exit (0); } if (strncmp(un.version, "V1", 2) == 0) { /* XXX is V1 correct? */ printf ("i386-sequent-ptx1\n"); exit (0); } printf ("i386-sequent-ptx\n"); exit (0); #endif #if defined (vax) # if !defined (ultrix) # include # if defined (BSD) # if BSD == 43 printf ("vax-dec-bsd4.3\n"); exit (0); # else # if BSD == 199006 printf ("vax-dec-bsd4.3reno\n"); exit (0); # else printf ("vax-dec-bsd\n"); exit (0); # endif # endif # else printf ("vax-dec-bsd\n"); exit (0); # endif # else printf ("vax-dec-ultrix\n"); exit (0); # endif #endif #if defined (alliant) && defined (i860) printf ("i860-alliant-bsd\n"); exit (0); #endif exit (1); } EOF $CC_FOR_BUILD -o $dummy $dummy.c 2>/dev/null && SYSTEM_NAME=`$dummy` && { echo "$SYSTEM_NAME"; exit; } # Apollos put the system type in the environment. test -d /usr/apollo && { echo ${ISP}-apollo-${SYSTYPE}; exit; } # Convex versions that predate uname can use getsysinfo(1) if [ -x /usr/convex/getsysinfo ] then case `getsysinfo -f cpu_type` in c1*) echo c1-convex-bsd exit ;; c2*) if getsysinfo -f scalar_acc then echo c32-convex-bsd else echo c2-convex-bsd fi exit ;; c34*) echo c34-convex-bsd exit ;; c38*) echo c38-convex-bsd exit ;; c4*) echo c4-convex-bsd exit ;; esac fi cat >&2 < in order to provide the needed information to handle your system. config.guess timestamp = $timestamp uname -m = `(uname -m) 2>/dev/null || echo unknown` uname -r = `(uname -r) 2>/dev/null || echo unknown` uname -s = `(uname -s) 2>/dev/null || echo unknown` uname -v = `(uname -v) 2>/dev/null || echo unknown` /usr/bin/uname -p = `(/usr/bin/uname -p) 2>/dev/null` /bin/uname -X = `(/bin/uname -X) 2>/dev/null` hostinfo = `(hostinfo) 2>/dev/null` /bin/universe = `(/bin/universe) 2>/dev/null` /usr/bin/arch -k = `(/usr/bin/arch -k) 2>/dev/null` /bin/arch = `(/bin/arch) 2>/dev/null` /usr/bin/oslevel = `(/usr/bin/oslevel) 2>/dev/null` /usr/convex/getsysinfo = `(/usr/convex/getsysinfo) 2>/dev/null` UNAME_MACHINE = ${UNAME_MACHINE} UNAME_RELEASE = ${UNAME_RELEASE} UNAME_SYSTEM = ${UNAME_SYSTEM} UNAME_VERSION = ${UNAME_VERSION} EOF exit 1 # Local variables: # eval: (add-hook 'write-file-hooks 'time-stamp) # time-stamp-start: "timestamp='" # time-stamp-format: "%:y-%02m-%02d" # time-stamp-end: "'" # End: pywcs-1.12/wcslib/config/config.sub0000755001153600020070000010503412310355626021364 0ustar cslocumSTSCI\science00000000000000#! /bin/sh # Configuration validation subroutine script. # Copyright (C) 1992, 1993, 1994, 1995, 1996, 1997, 1998, 1999, # 2000, 2001, 2002, 2003, 2004, 2005, 2006, 2007, 2008, 2009, 2010, # 2011 Free Software Foundation, Inc. timestamp='2011-09-09' # This file is (in principle) common to ALL GNU software. # The presence of a machine in this file suggests that SOME GNU software # can handle that machine. It does not imply ALL GNU software can. # # This file is free software; you can redistribute it and/or modify # it under the terms of the GNU General Public License as published by # the Free Software Foundation; either version 2 of the License, or # (at your option) any later version. # # This program is distributed in the hope that it will be useful, # but WITHOUT ANY WARRANTY; without even the implied warranty of # MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program; if not, write to the Free Software # Foundation, Inc., 51 Franklin Street - Fifth Floor, Boston, MA # 02110-1301, USA. # # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # Please send patches to . Submit a context # diff and a properly formatted GNU ChangeLog entry. # # Configuration subroutine to validate and canonicalize a configuration type. # Supply the specified configuration type as an argument. # If it is invalid, we print an error message on stderr and exit with code 1. # Otherwise, we print the canonical config type on stdout and succeed. # You can get the latest version of this script from: # http://git.savannah.gnu.org/gitweb/?p=config.git;a=blob_plain;f=config.sub;hb=HEAD # This file is supposed to be the same for all GNU packages # and recognize all the CPU types, system types and aliases # that are meaningful with *any* GNU software. # Each package is responsible for reporting which valid configurations # it does not support. The user should be able to distinguish # a failure to support a valid configuration from a meaningless # configuration. # The goal of this file is to map all the various variations of a given # machine specification into a single specification in the form: # CPU_TYPE-MANUFACTURER-OPERATING_SYSTEM # or in some cases, the newer four-part form: # CPU_TYPE-MANUFACTURER-KERNEL-OPERATING_SYSTEM # It is wrong to echo any other type of specification. me=`echo "$0" | sed -e 's,.*/,,'` usage="\ Usage: $0 [OPTION] CPU-MFR-OPSYS $0 [OPTION] ALIAS Canonicalize a configuration name. Operation modes: -h, --help print this help, then exit -t, --time-stamp print date of last modification, then exit -v, --version print version number, then exit Report bugs and patches to ." version="\ GNU config.sub ($timestamp) Copyright (C) 1992, 1993, 1994, 1995, 1996, 1997, 1998, 1999, 2000, 2001, 2002, 2003, 2004, 2005, 2006, 2007, 2008, 2009, 2010, 2011 Free Software Foundation, Inc. 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We also ### recognize some manufacturers as not being operating systems, so we ### can provide default operating systems below. case $os in -sun*os*) # Prevent following clause from handling this invalid input. ;; -dec* | -mips* | -sequent* | -encore* | -pc532* | -sgi* | -sony* | \ -att* | -7300* | -3300* | -delta* | -motorola* | -sun[234]* | \ -unicom* | -ibm* | -next | -hp | -isi* | -apollo | -altos* | \ -convergent* | -ncr* | -news | -32* | -3600* | -3100* | -hitachi* |\ -c[123]* | -convex* | -sun | -crds | -omron* | -dg | -ultra | -tti* | \ -harris | -dolphin | -highlevel | -gould | -cbm | -ns | -masscomp | \ -apple | -axis | -knuth | -cray | -microblaze) os= basic_machine=$1 ;; -bluegene*) os=-cnk ;; -sim | -cisco | -oki | -wec | -winbond) os= basic_machine=$1 ;; -scout) ;; -wrs) os=-vxworks basic_machine=$1 ;; -chorusos*) os=-chorusos basic_machine=$1 ;; -chorusrdb) os=-chorusrdb basic_machine=$1 ;; -hiux*) os=-hiuxwe2 ;; -sco6) os=-sco5v6 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco5) os=-sco3.2v5 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco4) os=-sco3.2v4 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco3.2.[4-9]*) os=`echo $os | sed -e 's/sco3.2./sco3.2v/'` basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco3.2v[4-9]*) # Don't forget version if it is 3.2v4 or newer. basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco5v6*) # Don't forget version if it is 3.2v4 or newer. basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -sco*) os=-sco3.2v2 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -udk*) basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -isc) os=-isc2.2 basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -clix*) basic_machine=clipper-intergraph ;; -isc*) basic_machine=`echo $1 | sed -e 's/86-.*/86-pc/'` ;; -lynx*) os=-lynxos ;; -ptx*) basic_machine=`echo $1 | sed -e 's/86-.*/86-sequent/'` ;; -windowsnt*) os=`echo $os | sed -e 's/windowsnt/winnt/'` ;; -psos*) os=-psos ;; -mint | -mint[0-9]*) basic_machine=m68k-atari os=-mint ;; esac # Decode aliases for certain CPU-COMPANY combinations. case $basic_machine in # Recognize the basic CPU types without company name. # Some are omitted here because they have special meanings below. 1750a | 580 \ | a29k \ | alpha | alphaev[4-8] | alphaev56 | alphaev6[78] | alphapca5[67] \ | alpha64 | alpha64ev[4-8] | alpha64ev56 | alpha64ev6[78] | alpha64pca5[67] \ | am33_2.0 \ | arc | arm | arm[bl]e | arme[lb] | armv[2345] | armv[345][lb] | avr | avr32 \ | be32 | be64 \ | bfin \ | c4x | clipper \ | d10v | d30v | dlx | dsp16xx \ | fido | fr30 | frv \ | h8300 | h8500 | hppa | hppa1.[01] | hppa2.0 | hppa2.0[nw] | hppa64 \ | hexagon \ | i370 | i860 | i960 | ia64 \ | ip2k | iq2000 \ | le32 | le64 \ | lm32 \ | m32c | m32r | m32rle | m68000 | m68k | m88k \ | maxq | mb | microblaze | mcore | mep | metag \ | mips | mipsbe | mipseb | mipsel | mipsle \ | mips16 \ | mips64 | mips64el \ | mips64octeon | mips64octeonel \ | mips64orion | mips64orionel \ | mips64r5900 | mips64r5900el \ | mips64vr | mips64vrel \ | mips64vr4100 | mips64vr4100el \ | mips64vr4300 | mips64vr4300el \ | mips64vr5000 | mips64vr5000el \ | mips64vr5900 | mips64vr5900el \ | mipsisa32 | mipsisa32el \ | mipsisa32r2 | mipsisa32r2el \ | mipsisa64 | mipsisa64el \ | mipsisa64r2 | mipsisa64r2el \ | mipsisa64sb1 | mipsisa64sb1el \ | mipsisa64sr71k | mipsisa64sr71kel \ | mipstx39 | mipstx39el \ | mn10200 | mn10300 \ | moxie \ | mt \ | msp430 \ | nds32 | nds32le | nds32be \ | nios | nios2 \ | ns16k | ns32k \ | open8 \ | or32 \ | pdp10 | pdp11 | pj | pjl \ | powerpc | powerpc64 | powerpc64le | powerpcle \ | pyramid \ | rx \ | score \ | sh | sh[1234] | sh[24]a | sh[24]aeb | sh[23]e | sh[34]eb | sheb | shbe | shle | sh[1234]le | sh3ele \ | sh64 | sh64le \ | sparc | sparc64 | sparc64b | sparc64v | sparc86x | sparclet | sparclite \ | sparcv8 | sparcv9 | sparcv9b | sparcv9v \ | spu \ | tahoe | tic4x | tic54x | tic55x | tic6x | tic80 | tron \ | ubicom32 \ | v850 | v850e | v850e1 | v850e2 | v850es | v850e2v3 \ | we32k \ | x86 | xc16x | xstormy16 | xtensa \ | z8k | z80) basic_machine=$basic_machine-unknown ;; c54x) basic_machine=tic54x-unknown ;; c55x) basic_machine=tic55x-unknown ;; c6x) basic_machine=tic6x-unknown ;; m6811 | m68hc11 | m6812 | m68hc12 | picochip) # Motorola 68HC11/12. basic_machine=$basic_machine-unknown os=-none ;; m88110 | m680[12346]0 | m683?2 | m68360 | m5200 | v70 | w65 | z8k) ;; ms1) basic_machine=mt-unknown ;; strongarm | thumb | xscale) basic_machine=arm-unknown ;; xscaleeb) basic_machine=armeb-unknown ;; xscaleel) basic_machine=armel-unknown ;; # We use `pc' rather than `unknown' # because (1) that's what they normally are, and # (2) the word "unknown" tends to confuse beginning users. i*86 | x86_64) basic_machine=$basic_machine-pc ;; # Object if more than one company name word. *-*-*) echo Invalid configuration \`$1\': machine \`$basic_machine\' not recognized 1>&2 exit 1 ;; # Recognize the basic CPU types with company name. 580-* \ | a29k-* \ | alpha-* | alphaev[4-8]-* | alphaev56-* | alphaev6[78]-* \ | alpha64-* | alpha64ev[4-8]-* | alpha64ev56-* | alpha64ev6[78]-* \ | alphapca5[67]-* | alpha64pca5[67]-* | arc-* \ | arm-* | armbe-* | armle-* | armeb-* | armv*-* \ | avr-* | avr32-* \ | be32-* | be64-* \ | bfin-* | bs2000-* \ | c[123]* | c30-* | [cjt]90-* | c4x-* \ | clipper-* | craynv-* | cydra-* \ | d10v-* | d30v-* | dlx-* \ | elxsi-* \ | f30[01]-* | f700-* | fido-* | fr30-* | frv-* | fx80-* \ | h8300-* | h8500-* \ | hppa-* | hppa1.[01]-* | hppa2.0-* | hppa2.0[nw]-* | hppa64-* \ | hexagon-* \ | i*86-* | i860-* | i960-* | ia64-* \ | ip2k-* | iq2000-* \ | le32-* | le64-* \ | lm32-* \ | m32c-* | m32r-* | m32rle-* \ | m68000-* | m680[012346]0-* | m68360-* | m683?2-* | m68k-* \ | m88110-* | m88k-* | maxq-* | mcore-* | metag-* | microblaze-* \ | mips-* | mipsbe-* | mipseb-* | mipsel-* | mipsle-* \ | mips16-* \ | mips64-* | mips64el-* \ | mips64octeon-* | mips64octeonel-* \ | mips64orion-* | mips64orionel-* \ | mips64r5900-* | mips64r5900el-* \ | mips64vr-* | mips64vrel-* \ | mips64vr4100-* | mips64vr4100el-* \ | mips64vr4300-* | mips64vr4300el-* \ | mips64vr5000-* | mips64vr5000el-* \ | mips64vr5900-* | mips64vr5900el-* \ | mipsisa32-* | mipsisa32el-* \ | mipsisa32r2-* | mipsisa32r2el-* \ | mipsisa64-* | mipsisa64el-* \ | mipsisa64r2-* | mipsisa64r2el-* \ | mipsisa64sb1-* | mipsisa64sb1el-* \ | mipsisa64sr71k-* | mipsisa64sr71kel-* \ | mipstx39-* | mipstx39el-* \ | mmix-* \ | mt-* \ | msp430-* \ | nds32-* | nds32le-* | nds32be-* \ | nios-* | nios2-* \ | none-* | np1-* | ns16k-* | ns32k-* \ | open8-* \ | orion-* \ | pdp10-* | pdp11-* | pj-* | pjl-* | pn-* | power-* \ | powerpc-* | powerpc64-* | powerpc64le-* | powerpcle-* \ | pyramid-* \ | romp-* | rs6000-* | rx-* \ | sh-* | sh[1234]-* | sh[24]a-* | sh[24]aeb-* | sh[23]e-* | sh[34]eb-* | sheb-* | shbe-* \ | shle-* | sh[1234]le-* | sh3ele-* | sh64-* | sh64le-* \ | sparc-* | sparc64-* | sparc64b-* | sparc64v-* | sparc86x-* | sparclet-* \ | sparclite-* \ | sparcv8-* | sparcv9-* | sparcv9b-* | sparcv9v-* | sv1-* | sx?-* \ | tahoe-* \ | tic30-* | tic4x-* | tic54x-* | tic55x-* | tic6x-* | tic80-* \ | tile*-* \ | tron-* \ | ubicom32-* \ | v850-* | v850e-* | v850e1-* | v850es-* | v850e2-* | v850e2v3-* \ | vax-* \ | we32k-* \ | x86-* | x86_64-* | xc16x-* | xps100-* \ | xstormy16-* | xtensa*-* \ | ymp-* \ | z8k-* | z80-*) ;; # Recognize the basic CPU types without company name, with glob match. xtensa*) basic_machine=$basic_machine-unknown ;; # Recognize the various machine names and aliases which stand # for a CPU type and a company and sometimes even an OS. 386bsd) basic_machine=i386-unknown os=-bsd ;; 3b1 | 7300 | 7300-att | att-7300 | pc7300 | safari | unixpc) basic_machine=m68000-att ;; 3b*) basic_machine=we32k-att ;; a29khif) basic_machine=a29k-amd os=-udi ;; abacus) basic_machine=abacus-unknown ;; adobe68k) basic_machine=m68010-adobe os=-scout ;; alliant | fx80) basic_machine=fx80-alliant ;; altos | altos3068) basic_machine=m68k-altos ;; am29k) basic_machine=a29k-none os=-bsd ;; amd64) basic_machine=x86_64-pc ;; amd64-*) basic_machine=x86_64-`echo $basic_machine | sed 's/^[^-]*-//'` ;; amdahl) basic_machine=580-amdahl os=-sysv ;; amiga | amiga-*) basic_machine=m68k-unknown ;; amigaos | amigados) basic_machine=m68k-unknown os=-amigaos ;; amigaunix | amix) basic_machine=m68k-unknown os=-sysv4 ;; apollo68) basic_machine=m68k-apollo os=-sysv ;; apollo68bsd) basic_machine=m68k-apollo os=-bsd ;; aros) basic_machine=i386-pc os=-aros ;; aux) basic_machine=m68k-apple os=-aux ;; balance) basic_machine=ns32k-sequent os=-dynix ;; blackfin) basic_machine=bfin-unknown os=-linux ;; blackfin-*) basic_machine=bfin-`echo $basic_machine | sed 's/^[^-]*-//'` os=-linux ;; bluegene*) basic_machine=powerpc-ibm os=-cnk ;; c54x-*) basic_machine=tic54x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c55x-*) basic_machine=tic55x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c6x-*) basic_machine=tic6x-`echo $basic_machine | sed 's/^[^-]*-//'` ;; c90) basic_machine=c90-cray os=-unicos ;; cegcc) basic_machine=arm-unknown os=-cegcc ;; convex-c1) basic_machine=c1-convex os=-bsd ;; convex-c2) basic_machine=c2-convex os=-bsd ;; convex-c32) basic_machine=c32-convex os=-bsd ;; convex-c34) basic_machine=c34-convex os=-bsd ;; convex-c38) basic_machine=c38-convex os=-bsd ;; cray | j90) basic_machine=j90-cray os=-unicos ;; craynv) basic_machine=craynv-cray os=-unicosmp ;; cr16 | cr16-*) basic_machine=cr16-unknown os=-elf ;; crds | unos) basic_machine=m68k-crds ;; crisv32 | crisv32-* | etraxfs*) basic_machine=crisv32-axis ;; cris | cris-* | etrax*) basic_machine=cris-axis ;; crx) basic_machine=crx-unknown os=-elf ;; da30 | da30-*) basic_machine=m68k-da30 ;; decstation | decstation-3100 | pmax | pmax-* | pmin | dec3100 | decstatn) basic_machine=mips-dec ;; decsystem10* | dec10*) basic_machine=pdp10-dec os=-tops10 ;; decsystem20* | dec20*) basic_machine=pdp10-dec os=-tops20 ;; delta | 3300 | motorola-3300 | motorola-delta \ | 3300-motorola | delta-motorola) basic_machine=m68k-motorola ;; delta88) basic_machine=m88k-motorola os=-sysv3 ;; dicos) basic_machine=i686-pc os=-dicos ;; djgpp) basic_machine=i586-pc os=-msdosdjgpp ;; dpx20 | dpx20-*) basic_machine=rs6000-bull os=-bosx ;; dpx2* | dpx2*-bull) basic_machine=m68k-bull os=-sysv3 ;; ebmon29k) basic_machine=a29k-amd os=-ebmon ;; elxsi) basic_machine=elxsi-elxsi os=-bsd ;; encore | umax | mmax) basic_machine=ns32k-encore ;; es1800 | OSE68k | ose68k | ose | OSE) basic_machine=m68k-ericsson os=-ose ;; fx2800) basic_machine=i860-alliant ;; genix) basic_machine=ns32k-ns ;; gmicro) basic_machine=tron-gmicro os=-sysv ;; go32) basic_machine=i386-pc os=-go32 ;; h3050r* | hiux*) basic_machine=hppa1.1-hitachi os=-hiuxwe2 ;; h8300hms) basic_machine=h8300-hitachi os=-hms ;; h8300xray) basic_machine=h8300-hitachi os=-xray ;; h8500hms) basic_machine=h8500-hitachi os=-hms ;; harris) basic_machine=m88k-harris os=-sysv3 ;; hp300-*) basic_machine=m68k-hp ;; hp300bsd) basic_machine=m68k-hp os=-bsd ;; hp300hpux) basic_machine=m68k-hp os=-hpux ;; hp3k9[0-9][0-9] | hp9[0-9][0-9]) basic_machine=hppa1.0-hp ;; hp9k2[0-9][0-9] | hp9k31[0-9]) basic_machine=m68000-hp ;; hp9k3[2-9][0-9]) basic_machine=m68k-hp ;; hp9k6[0-9][0-9] | hp6[0-9][0-9]) basic_machine=hppa1.0-hp ;; hp9k7[0-79][0-9] | hp7[0-79][0-9]) basic_machine=hppa1.1-hp ;; hp9k78[0-9] | hp78[0-9]) # FIXME: really hppa2.0-hp basic_machine=hppa1.1-hp ;; hp9k8[67]1 | hp8[67]1 | hp9k80[24] | hp80[24] | hp9k8[78]9 | hp8[78]9 | hp9k893 | hp893) # FIXME: really hppa2.0-hp basic_machine=hppa1.1-hp ;; hp9k8[0-9][13679] | hp8[0-9][13679]) basic_machine=hppa1.1-hp ;; hp9k8[0-9][0-9] | hp8[0-9][0-9]) basic_machine=hppa1.0-hp ;; hppa-next) os=-nextstep3 ;; hppaosf) basic_machine=hppa1.1-hp os=-osf ;; hppro) basic_machine=hppa1.1-hp os=-proelf ;; i370-ibm* | ibm*) basic_machine=i370-ibm ;; # I'm not sure what "Sysv32" means. Should this be sysv3.2? i*86v32) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-sysv32 ;; i*86v4*) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-sysv4 ;; i*86v) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-sysv ;; i*86sol2) basic_machine=`echo $1 | sed -e 's/86.*/86-pc/'` os=-solaris2 ;; i386mach) basic_machine=i386-mach os=-mach ;; i386-vsta | vsta) basic_machine=i386-unknown os=-vsta ;; iris | iris4d) basic_machine=mips-sgi case $os in -irix*) ;; *) os=-irix4 ;; esac ;; isi68 | isi) basic_machine=m68k-isi os=-sysv ;; m68knommu) basic_machine=m68k-unknown os=-linux ;; m68knommu-*) basic_machine=m68k-`echo $basic_machine | sed 's/^[^-]*-//'` os=-linux ;; m88k-omron*) basic_machine=m88k-omron ;; magnum | m3230) basic_machine=mips-mips os=-sysv ;; merlin) basic_machine=ns32k-utek os=-sysv ;; microblaze) basic_machine=microblaze-xilinx ;; mingw32) basic_machine=i386-pc os=-mingw32 ;; mingw32ce) basic_machine=arm-unknown os=-mingw32ce ;; miniframe) basic_machine=m68000-convergent ;; *mint | -mint[0-9]* | *MiNT | *MiNT[0-9]*) basic_machine=m68k-atari os=-mint ;; mips3*-*) basic_machine=`echo $basic_machine | sed -e 's/mips3/mips64/'` ;; mips3*) basic_machine=`echo $basic_machine | sed -e 's/mips3/mips64/'`-unknown ;; monitor) basic_machine=m68k-rom68k os=-coff ;; morphos) basic_machine=powerpc-unknown os=-morphos ;; msdos) basic_machine=i386-pc os=-msdos ;; ms1-*) basic_machine=`echo $basic_machine | sed -e 's/ms1-/mt-/'` ;; mvs) basic_machine=i370-ibm os=-mvs ;; nacl) basic_machine=le32-unknown os=-nacl ;; ncr3000) basic_machine=i486-ncr os=-sysv4 ;; netbsd386) basic_machine=i386-unknown os=-netbsd ;; netwinder) basic_machine=armv4l-rebel os=-linux ;; news | news700 | news800 | news900) basic_machine=m68k-sony os=-newsos ;; news1000) basic_machine=m68030-sony os=-newsos ;; news-3600 | risc-news) basic_machine=mips-sony os=-newsos ;; necv70) basic_machine=v70-nec os=-sysv ;; next | m*-next ) basic_machine=m68k-next case $os in -nextstep* ) ;; -ns2*) os=-nextstep2 ;; *) os=-nextstep3 ;; esac ;; nh3000) basic_machine=m68k-harris os=-cxux ;; nh[45]000) basic_machine=m88k-harris os=-cxux ;; nindy960) basic_machine=i960-intel os=-nindy ;; mon960) basic_machine=i960-intel os=-mon960 ;; nonstopux) basic_machine=mips-compaq os=-nonstopux ;; np1) basic_machine=np1-gould ;; neo-tandem) basic_machine=neo-tandem ;; nse-tandem) basic_machine=nse-tandem ;; nsr-tandem) basic_machine=nsr-tandem ;; op50n-* | op60c-*) basic_machine=hppa1.1-oki os=-proelf ;; openrisc | openrisc-*) basic_machine=or32-unknown ;; os400) basic_machine=powerpc-ibm os=-os400 ;; OSE68000 | ose68000) basic_machine=m68000-ericsson os=-ose ;; os68k) basic_machine=m68k-none os=-os68k ;; pa-hitachi) basic_machine=hppa1.1-hitachi os=-hiuxwe2 ;; paragon) basic_machine=i860-intel os=-osf ;; parisc) basic_machine=hppa-unknown os=-linux ;; parisc-*) basic_machine=hppa-`echo $basic_machine | sed 's/^[^-]*-//'` os=-linux ;; pbd) basic_machine=sparc-tti ;; pbb) basic_machine=m68k-tti ;; pc532 | pc532-*) basic_machine=ns32k-pc532 ;; pc98) basic_machine=i386-pc ;; pc98-*) basic_machine=i386-`echo $basic_machine | sed 's/^[^-]*-//'` ;; pentium | p5 | k5 | k6 | nexgen | viac3) basic_machine=i586-pc ;; pentiumpro | p6 | 6x86 | athlon | athlon_*) basic_machine=i686-pc ;; pentiumii | pentium2 | pentiumiii | pentium3) basic_machine=i686-pc ;; pentium4) basic_machine=i786-pc ;; pentium-* | p5-* | k5-* | k6-* | nexgen-* | viac3-*) basic_machine=i586-`echo $basic_machine | sed 's/^[^-]*-//'` ;; pentiumpro-* | p6-* | 6x86-* | athlon-*) basic_machine=i686-`echo $basic_machine | sed 's/^[^-]*-//'` ;; pentiumii-* | pentium2-* | pentiumiii-* | pentium3-*) basic_machine=i686-`echo $basic_machine | sed 's/^[^-]*-//'` ;; pentium4-*) basic_machine=i786-`echo $basic_machine | sed 's/^[^-]*-//'` ;; pn) basic_machine=pn-gould ;; power) basic_machine=power-ibm ;; ppc | ppcbe) basic_machine=powerpc-unknown ;; ppc-* | ppcbe-*) basic_machine=powerpc-`echo $basic_machine | sed 's/^[^-]*-//'` ;; ppcle | powerpclittle | ppc-le | powerpc-little) basic_machine=powerpcle-unknown ;; ppcle-* | powerpclittle-*) basic_machine=powerpcle-`echo $basic_machine | sed 's/^[^-]*-//'` ;; ppc64) basic_machine=powerpc64-unknown ;; ppc64-*) basic_machine=powerpc64-`echo $basic_machine | sed 's/^[^-]*-//'` ;; ppc64le | powerpc64little | ppc64-le | powerpc64-little) basic_machine=powerpc64le-unknown ;; ppc64le-* | powerpc64little-*) basic_machine=powerpc64le-`echo $basic_machine | sed 's/^[^-]*-//'` ;; ps2) basic_machine=i386-ibm ;; pw32) basic_machine=i586-unknown os=-pw32 ;; rdos) basic_machine=i386-pc os=-rdos ;; rom68k) basic_machine=m68k-rom68k os=-coff ;; rm[46]00) basic_machine=mips-siemens ;; rtpc | rtpc-*) basic_machine=romp-ibm ;; s390 | s390-*) basic_machine=s390-ibm ;; s390x | s390x-*) basic_machine=s390x-ibm ;; sa29200) basic_machine=a29k-amd os=-udi ;; sb1) basic_machine=mipsisa64sb1-unknown ;; sb1el) basic_machine=mipsisa64sb1el-unknown ;; sde) basic_machine=mipsisa32-sde os=-elf ;; sei) basic_machine=mips-sei os=-seiux ;; sequent) basic_machine=i386-sequent ;; sh) basic_machine=sh-hitachi os=-hms ;; sh5el) basic_machine=sh5le-unknown ;; sh64) basic_machine=sh64-unknown ;; sparclite-wrs | simso-wrs) basic_machine=sparclite-wrs os=-vxworks ;; sps7) basic_machine=m68k-bull os=-sysv2 ;; spur) basic_machine=spur-unknown ;; st2000) basic_machine=m68k-tandem ;; stratus) basic_machine=i860-stratus os=-sysv4 ;; strongarm-* | thumb-*) basic_machine=arm-`echo $basic_machine | sed 's/^[^-]*-//'` ;; sun2) basic_machine=m68000-sun ;; sun2os3) basic_machine=m68000-sun os=-sunos3 ;; sun2os4) basic_machine=m68000-sun os=-sunos4 ;; sun3os3) basic_machine=m68k-sun os=-sunos3 ;; sun3os4) basic_machine=m68k-sun os=-sunos4 ;; sun4os3) basic_machine=sparc-sun os=-sunos3 ;; sun4os4) basic_machine=sparc-sun os=-sunos4 ;; sun4sol2) basic_machine=sparc-sun os=-solaris2 ;; sun3 | sun3-*) basic_machine=m68k-sun ;; sun4) basic_machine=sparc-sun ;; sun386 | sun386i | roadrunner) basic_machine=i386-sun ;; sv1) basic_machine=sv1-cray os=-unicos ;; symmetry) basic_machine=i386-sequent os=-dynix ;; t3e) basic_machine=alphaev5-cray os=-unicos ;; t90) basic_machine=t90-cray os=-unicos ;; tile*) basic_machine=$basic_machine-unknown os=-linux-gnu ;; tx39) basic_machine=mipstx39-unknown ;; tx39el) basic_machine=mipstx39el-unknown ;; toad1) basic_machine=pdp10-xkl os=-tops20 ;; tower | tower-32) basic_machine=m68k-ncr ;; tpf) basic_machine=s390x-ibm os=-tpf ;; udi29k) basic_machine=a29k-amd os=-udi ;; ultra3) basic_machine=a29k-nyu os=-sym1 ;; v810 | necv810) basic_machine=v810-nec os=-none ;; vaxv) basic_machine=vax-dec os=-sysv ;; vms) basic_machine=vax-dec os=-vms ;; vpp*|vx|vx-*) basic_machine=f301-fujitsu ;; vxworks960) basic_machine=i960-wrs os=-vxworks ;; vxworks68) basic_machine=m68k-wrs os=-vxworks ;; vxworks29k) basic_machine=a29k-wrs os=-vxworks ;; w65*) basic_machine=w65-wdc os=-none ;; w89k-*) basic_machine=hppa1.1-winbond os=-proelf ;; xbox) basic_machine=i686-pc os=-mingw32 ;; xps | xps100) basic_machine=xps100-honeywell ;; xscale-* | xscalee[bl]-*) basic_machine=`echo $basic_machine | sed 's/^xscale/arm/'` ;; ymp) basic_machine=ymp-cray os=-unicos ;; z8k-*-coff) basic_machine=z8k-unknown os=-sim ;; z80-*-coff) basic_machine=z80-unknown os=-sim ;; none) basic_machine=none-none os=-none ;; # Here we handle the default manufacturer of certain CPU types. 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See the # GNU General Public License for more details. # # You should have received a copy of the GNU General Public License # along with this program; if not, write to the Free Software # Foundation, Inc., 59 Temple Place - Suite 330, Boston, MA 02111-1307, USA. # As a special exception to the GNU General Public License, if you # distribute this file as part of a program that contains a # configuration script generated by Autoconf, you may include it under # the same distribution terms that you use for the rest of that program. # This script byte-compiles all `.el' files which are part of its # arguments, using GNU Emacs, and put the resulting `.elc' files into # the current directory, so disregarding the original directories used # in `.el' arguments. # # This script manages in such a way that all Emacs LISP files to # be compiled are made visible between themselves, in the event # they require or load-library one another. if test $# = 0; then echo 1>&2 "No files given to $0" exit 1 fi if test -z "$EMACS" || test "$EMACS" = "t"; then # Value of "t" means we are running in a shell under Emacs. # Just assume Emacs is called "emacs". 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(exit 0); exit pywcs-1.12/wcslib/config/install-sh0000755001153600020070000002017412310355626021406 0ustar cslocumSTSCI\science00000000000000#!/bin/sh # install - install a program, script, or datafile scriptversion=2003-09-24.23 # This originates from X11R5 (mit/util/scripts/install.sh), which was # later released in X11R6 (xc/config/util/install.sh) with the # following copyright and license. # # Copyright (C) 1994 X Consortium # # Permission is hereby granted, free of charge, to any person obtaining a copy # of this software and associated documentation files (the "Software"), to # deal in the Software without restriction, including without limitation the # rights to use, copy, modify, merge, publish, distribute, sublicense, and/or # sell copies of the Software, and to permit persons to whom the Software is # furnished to do so, subject to the following conditions: # # The above copyright notice and this permission notice shall be included in # all copies or substantial portions of the Software. # # THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR # IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY, # FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE # X CONSORTIUM BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER LIABILITY, WHETHER IN # AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM, OUT OF OR IN CONNEC- # TION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE SOFTWARE. # # Except as contained in this notice, the name of the X Consortium shall not # be used in advertising or otherwise to promote the sale, use or other deal- # ings in this Software without prior written authorization from the X Consor- # tium. # # # FSF changes to this file are in the public domain. # # Calling this script install-sh is preferred over install.sh, to prevent # `make' implicit rules from creating a file called install from it # when there is no Makefile. # # This script is compatible with the BSD install script, but was written # from scratch. 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Now check whether nonexistent headers # can be detected and how. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include _ACEOF if { (ac_try="$ac_cpp conftest.$ac_ext" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_cpp conftest.$ac_ext") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } >/dev/null && { test -z "$ac_c_preproc_warn_flag$ac_c_werror_flag" || test ! -s conftest.err }; then # Broken: success on invalid input. continue else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 # Passes both tests. ac_preproc_ok=: break fi rm -f conftest.err conftest.$ac_ext done # Because of `break', _AC_PREPROC_IFELSE's cleaning code was skipped. rm -f conftest.err conftest.$ac_ext if $ac_preproc_ok; then break fi done ac_cv_prog_CPP=$CPP fi CPP=$ac_cv_prog_CPP else ac_cv_prog_CPP=$CPP fi { echo "$as_me:$LINENO: result: $CPP" >&5 echo "${ECHO_T}$CPP" >&6; } ac_preproc_ok=false for ac_c_preproc_warn_flag in '' yes do # Use a header file that comes with gcc, so configuring glibc # with a fresh cross-compiler works. # Prefer to if __STDC__ is defined, since # exists even on freestanding compilers. # On the NeXT, cc -E runs the code through the compiler's parser, # not just through cpp. "Syntax error" is here to catch this case. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #ifdef __STDC__ # include #else # include #endif Syntax error _ACEOF if { (ac_try="$ac_cpp conftest.$ac_ext" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_cpp conftest.$ac_ext") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } >/dev/null && { test -z "$ac_c_preproc_warn_flag$ac_c_werror_flag" || test ! -s conftest.err }; then : else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 # Broken: fails on valid input. continue fi rm -f conftest.err conftest.$ac_ext # OK, works on sane cases. 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then { echo "$as_me:$LINENO: result: $CC" >&5 echo "${ECHO_T}$CC" >&6; } else { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi fi fi if test -z "$CC"; then # Extract the first word of "cc", so it can be a program name with args. set dummy cc; ac_word=$2 { echo "$as_me:$LINENO: checking for $ac_word" >&5 echo $ECHO_N "checking for $ac_word... $ECHO_C" >&6; } if test "${ac_cv_prog_CC+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test -n "$CC"; then ac_cv_prog_CC="$CC" # Let the user override the test. else ac_prog_rejected=no as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if { test -f "$as_dir/$ac_word$ac_exec_ext" && $as_test_x "$as_dir/$ac_word$ac_exec_ext"; }; then if test "$as_dir/$ac_word$ac_exec_ext" = "/usr/ucb/cc"; then ac_prog_rejected=yes continue fi ac_cv_prog_CC="cc" echo "$as_me:$LINENO: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS if test $ac_prog_rejected = yes; then # We found a bogon in the path, so make sure we never use it. set dummy $ac_cv_prog_CC shift if test $# != 0; then # We chose a different compiler from the bogus one. # However, it has the same basename, so the bogon will be chosen # first if we set CC to just the basename; use the full file name. shift ac_cv_prog_CC="$as_dir/$ac_word${1+' '}$@" fi fi fi fi CC=$ac_cv_prog_CC if test -n "$CC"; then { echo "$as_me:$LINENO: result: $CC" >&5 echo "${ECHO_T}$CC" >&6; } else { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi fi if test -z "$CC"; then if test -n "$ac_tool_prefix"; then for ac_prog in cl.exe do # Extract the first word of "$ac_tool_prefix$ac_prog", so it can be a program name with args. set dummy $ac_tool_prefix$ac_prog; ac_word=$2 { echo "$as_me:$LINENO: checking for $ac_word" >&5 echo $ECHO_N "checking for $ac_word... $ECHO_C" >&6; } if test "${ac_cv_prog_CC+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test -n "$CC"; then ac_cv_prog_CC="$CC" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if { test -f "$as_dir/$ac_word$ac_exec_ext" && $as_test_x "$as_dir/$ac_word$ac_exec_ext"; }; then ac_cv_prog_CC="$ac_tool_prefix$ac_prog" echo "$as_me:$LINENO: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi CC=$ac_cv_prog_CC if test -n "$CC"; then { echo "$as_me:$LINENO: result: $CC" >&5 echo "${ECHO_T}$CC" >&6; } else { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi test -n "$CC" && break done fi if test -z "$CC"; then ac_ct_CC=$CC for ac_prog in cl.exe do # Extract the first word of "$ac_prog", so it can be a program name with args. set dummy $ac_prog; ac_word=$2 { echo "$as_me:$LINENO: checking for $ac_word" >&5 echo $ECHO_N "checking for $ac_word... $ECHO_C" >&6; } if test "${ac_cv_prog_ac_ct_CC+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test -n "$ac_ct_CC"; then ac_cv_prog_ac_ct_CC="$ac_ct_CC" # Let the user override the test. else as_save_IFS=$IFS; 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If you think this configuration is useful to you, please write to autoconf@gnu.org." >&5 echo "$as_me: WARNING: In the future, Autoconf will not detect cross-tools whose name does not start with the host triplet. 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echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } { (ac_try="$ac_compiler -V >&5" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compiler -V >&5") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } { echo "$as_me:$LINENO: checking whether we are using the GNU C compiler" >&5 echo $ECHO_N "checking whether we are using the GNU C compiler... $ECHO_C" >&6; } if test "${ac_cv_c_compiler_gnu+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ int main () { #ifndef __GNUC__ choke me #endif ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_compiler_gnu=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_compiler_gnu=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_cv_c_compiler_gnu=$ac_compiler_gnu fi { echo "$as_me:$LINENO: result: $ac_cv_c_compiler_gnu" >&5 echo "${ECHO_T}$ac_cv_c_compiler_gnu" >&6; } GCC=`test $ac_compiler_gnu = yes && echo yes` ac_test_CFLAGS=${CFLAGS+set} ac_save_CFLAGS=$CFLAGS { echo "$as_me:$LINENO: checking whether $CC accepts -g" >&5 echo $ECHO_N "checking whether $CC accepts -g... $ECHO_C" >&6; } if test "${ac_cv_prog_cc_g+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_save_c_werror_flag=$ac_c_werror_flag ac_c_werror_flag=yes ac_cv_prog_cc_g=no CFLAGS="-g" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_cc_g=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 CFLAGS="" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then : else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_c_werror_flag=$ac_save_c_werror_flag CFLAGS="-g" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_cc_g=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_c_werror_flag=$ac_save_c_werror_flag fi { echo "$as_me:$LINENO: result: $ac_cv_prog_cc_g" >&5 echo "${ECHO_T}$ac_cv_prog_cc_g" >&6; } if test "$ac_test_CFLAGS" = set; then CFLAGS=$ac_save_CFLAGS elif test $ac_cv_prog_cc_g = yes; then if test "$GCC" = yes; then CFLAGS="-g -O2" else CFLAGS="-g" fi else if test "$GCC" = yes; then CFLAGS="-O2" else CFLAGS= fi fi { echo "$as_me:$LINENO: checking for $CC option to accept ISO C89" >&5 echo $ECHO_N "checking for $CC option to accept ISO C89... $ECHO_C" >&6; } if test "${ac_cv_prog_cc_c89+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_prog_cc_c89=no ac_save_CC=$CC cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #include #include /* Most of the following tests are stolen from RCS 5.7's src/conf.sh. */ struct buf { int x; }; FILE * (*rcsopen) (struct buf *, struct stat *, int); static char *e (p, i) char **p; int i; { return p[i]; } static char *f (char * (*g) (char **, int), char **p, ...) { char *s; va_list v; va_start (v,p); s = g (p, va_arg (v,int)); va_end (v); return s; } /* OSF 4.0 Compaq cc is some sort of almost-ANSI by default. It has function prototypes and stuff, but not '\xHH' hex character constants. These don't provoke an error unfortunately, instead are silently treated as 'x'. The following induces an error, until -std is added to get proper ANSI mode. Curiously '\x00'!='x' always comes out true, for an array size at least. It's necessary to write '\x00'==0 to get something that's true only with -std. */ int osf4_cc_array ['\x00' == 0 ? 1 : -1]; /* IBM C 6 for AIX is almost-ANSI by default, but it replaces macro parameters inside strings and character constants. */ #define FOO(x) 'x' int xlc6_cc_array[FOO(a) == 'x' ? 1 : -1]; int test (int i, double x); struct s1 {int (*f) (int a);}; struct s2 {int (*f) (double a);}; int pairnames (int, char **, FILE *(*)(struct buf *, struct stat *, int), int, int); int argc; char **argv; int main () { return f (e, argv, 0) != argv[0] || f (e, argv, 1) != argv[1]; ; return 0; } _ACEOF for ac_arg in '' -qlanglvl=extc89 -qlanglvl=ansi -std \ -Ae "-Aa -D_HPUX_SOURCE" "-Xc -D__EXTENSIONS__" do CC="$ac_save_CC $ac_arg" rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_cc_c89=$ac_arg else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext test "x$ac_cv_prog_cc_c89" != "xno" && break done rm -f conftest.$ac_ext CC=$ac_save_CC fi # AC_CACHE_VAL case "x$ac_cv_prog_cc_c89" in x) { echo "$as_me:$LINENO: result: none needed" >&5 echo "${ECHO_T}none needed" >&6; } ;; xno) { echo "$as_me:$LINENO: result: unsupported" >&5 echo "${ECHO_T}unsupported" >&6; } ;; *) CC="$CC $ac_cv_prog_cc_c89" { echo "$as_me:$LINENO: result: $ac_cv_prog_cc_c89" >&5 echo "${ECHO_T}$ac_cv_prog_cc_c89" >&6; } ;; esac ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu case $ac_cv_prog_cc_stdc in no) ac_cv_prog_cc_c99=no; ac_cv_prog_cc_c89=no ;; *) { echo "$as_me:$LINENO: checking for $CC option to accept ISO C99" >&5 echo $ECHO_N "checking for $CC option to accept ISO C99... $ECHO_C" >&6; } if test "${ac_cv_prog_cc_c99+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_prog_cc_c99=no ac_save_CC=$CC cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #include #include #include // Check varargs macros. These examples are taken from C99 6.10.3.5. #define debug(...) fprintf (stderr, __VA_ARGS__) #define showlist(...) puts (#__VA_ARGS__) #define report(test,...) ((test) ? puts (#test) : printf (__VA_ARGS__)) static void test_varargs_macros (void) { int x = 1234; int y = 5678; debug ("Flag"); debug ("X = %d\n", x); showlist (The first, second, and third items.); report (x>y, "x is %d but y is %d", x, y); } // Check long long types. #define BIG64 18446744073709551615ull #define BIG32 4294967295ul #define BIG_OK (BIG64 / BIG32 == 4294967297ull && BIG64 % BIG32 == 0) #if !BIG_OK your preprocessor is broken; #endif #if BIG_OK #else your preprocessor is broken; #endif static long long int bignum = -9223372036854775807LL; static unsigned long long int ubignum = BIG64; struct incomplete_array { int datasize; double data[]; }; struct named_init { int number; const wchar_t *name; double average; }; typedef const char *ccp; static inline int test_restrict (ccp restrict text) { // See if C++-style comments work. // Iterate through items via the restricted pointer. // Also check for declarations in for loops. for (unsigned int i = 0; *(text+i) != '\0'; ++i) continue; return 0; } // Check varargs and va_copy. static void test_varargs (const char *format, ...) { va_list args; va_start (args, format); va_list args_copy; va_copy (args_copy, args); const char *str; int number; float fnumber; while (*format) { switch (*format++) { case 's': // string str = va_arg (args_copy, const char *); break; case 'd': // int number = va_arg (args_copy, int); break; case 'f': // float fnumber = va_arg (args_copy, double); break; default: break; } } va_end (args_copy); va_end (args); } int main () { // Check bool. _Bool success = false; // Check restrict. if (test_restrict ("String literal") == 0) success = true; char *restrict newvar = "Another string"; // Check varargs. test_varargs ("s, d' f .", "string", 65, 34.234); test_varargs_macros (); // Check flexible array members. struct incomplete_array *ia = malloc (sizeof (struct incomplete_array) + (sizeof (double) * 10)); ia->datasize = 10; for (int i = 0; i < ia->datasize; ++i) ia->data[i] = i * 1.234; // Check named initializers. struct named_init ni = { .number = 34, .name = L"Test wide string", .average = 543.34343, }; ni.number = 58; int dynamic_array[ni.number]; dynamic_array[ni.number - 1] = 543; // work around unused variable warnings return (!success || bignum == 0LL || ubignum == 0uLL || newvar[0] == 'x' || dynamic_array[ni.number - 1] != 543); ; return 0; } _ACEOF for ac_arg in '' -std=gnu99 -c99 -qlanglvl=extc99 do CC="$ac_save_CC $ac_arg" rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_cc_c99=$ac_arg else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext test "x$ac_cv_prog_cc_c99" != "xno" && break done rm -f conftest.$ac_ext CC=$ac_save_CC fi # AC_CACHE_VAL case "x$ac_cv_prog_cc_c99" in x) { echo "$as_me:$LINENO: result: none needed" >&5 echo "${ECHO_T}none needed" >&6; } ;; xno) { echo "$as_me:$LINENO: result: unsupported" >&5 echo "${ECHO_T}unsupported" >&6; } ;; *) CC="$CC $ac_cv_prog_cc_c99" { echo "$as_me:$LINENO: result: $ac_cv_prog_cc_c99" >&5 echo "${ECHO_T}$ac_cv_prog_cc_c99" >&6; } ;; esac if test "x$ac_cv_prog_cc_c99" != xno; then ac_cv_prog_cc_stdc=$ac_cv_prog_cc_c99 else { echo "$as_me:$LINENO: checking for $CC option to accept ISO C89" >&5 echo $ECHO_N "checking for $CC option to accept ISO C89... $ECHO_C" >&6; } if test "${ac_cv_prog_cc_c89+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_prog_cc_c89=no ac_save_CC=$CC cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #include #include /* Most of the following tests are stolen from RCS 5.7's src/conf.sh. */ struct buf { int x; }; FILE * (*rcsopen) (struct buf *, struct stat *, int); static char *e (p, i) char **p; int i; { return p[i]; } static char *f (char * (*g) (char **, int), char **p, ...) { char *s; va_list v; va_start (v,p); s = g (p, va_arg (v,int)); va_end (v); return s; } /* OSF 4.0 Compaq cc is some sort of almost-ANSI by default. It has function prototypes and stuff, but not '\xHH' hex character constants. These don't provoke an error unfortunately, instead are silently treated as 'x'. The following induces an error, until -std is added to get proper ANSI mode. Curiously '\x00'!='x' always comes out true, for an array size at least. It's necessary to write '\x00'==0 to get something that's true only with -std. */ int osf4_cc_array ['\x00' == 0 ? 1 : -1]; /* IBM C 6 for AIX is almost-ANSI by default, but it replaces macro parameters inside strings and character constants. */ #define FOO(x) 'x' int xlc6_cc_array[FOO(a) == 'x' ? 1 : -1]; int test (int i, double x); struct s1 {int (*f) (int a);}; struct s2 {int (*f) (double a);}; int pairnames (int, char **, FILE *(*)(struct buf *, struct stat *, int), int, int); int argc; char **argv; int main () { return f (e, argv, 0) != argv[0] || f (e, argv, 1) != argv[1]; ; return 0; } _ACEOF for ac_arg in '' -qlanglvl=extc89 -qlanglvl=ansi -std \ -Ae "-Aa -D_HPUX_SOURCE" "-Xc -D__EXTENSIONS__" do CC="$ac_save_CC $ac_arg" rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_cc_c89=$ac_arg else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext test "x$ac_cv_prog_cc_c89" != "xno" && break done rm -f conftest.$ac_ext CC=$ac_save_CC fi # AC_CACHE_VAL case "x$ac_cv_prog_cc_c89" in x) { echo "$as_me:$LINENO: result: none needed" >&5 echo "${ECHO_T}none needed" >&6; } ;; xno) { echo "$as_me:$LINENO: result: unsupported" >&5 echo "${ECHO_T}unsupported" >&6; } ;; *) CC="$CC $ac_cv_prog_cc_c89" { echo "$as_me:$LINENO: result: $ac_cv_prog_cc_c89" >&5 echo "${ECHO_T}$ac_cv_prog_cc_c89" >&6; } ;; esac if test "x$ac_cv_prog_cc_c89" != xno; then ac_cv_prog_cc_stdc=$ac_cv_prog_cc_c89 else ac_cv_prog_cc_stdc=no fi fi ;; esac { echo "$as_me:$LINENO: checking for $CC option to accept ISO Standard C" >&5 echo $ECHO_N "checking for $CC option to accept ISO Standard C... $ECHO_C" >&6; } if test "${ac_cv_prog_cc_stdc+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 fi case $ac_cv_prog_cc_stdc in no) { echo "$as_me:$LINENO: result: unsupported" >&5 echo "${ECHO_T}unsupported" >&6; } ;; '') { echo "$as_me:$LINENO: result: none needed" >&5 echo "${ECHO_T}none needed" >&6; } ;; *) { echo "$as_me:$LINENO: result: $ac_cv_prog_cc_stdc" >&5 echo "${ECHO_T}$ac_cv_prog_cc_stdc" >&6; } ;; esac { echo "$as_me:$LINENO: checking for an ANSI C-conforming const" >&5 echo $ECHO_N "checking for an ANSI C-conforming const... $ECHO_C" >&6; } if test "${ac_cv_c_const+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ int main () { /* FIXME: Include the comments suggested by Paul. */ #ifndef __cplusplus /* Ultrix mips cc rejects this. */ typedef int charset[2]; const charset cs; /* SunOS 4.1.1 cc rejects this. */ char const *const *pcpcc; char **ppc; /* NEC SVR4.0.2 mips cc rejects this. */ struct point {int x, y;}; static struct point const zero = {0,0}; /* AIX XL C 1.02.0.0 rejects this. It does not let you subtract one const X* pointer from another in an arm of an if-expression whose if-part is not a constant expression */ const char *g = "string"; pcpcc = &g + (g ? g-g : 0); /* HPUX 7.0 cc rejects these. */ ++pcpcc; ppc = (char**) pcpcc; pcpcc = (char const *const *) ppc; { /* SCO 3.2v4 cc rejects this. */ char *t; char const *s = 0 ? (char *) 0 : (char const *) 0; *t++ = 0; if (s) return 0; } { /* Someone thinks the Sun supposedly-ANSI compiler will reject this. */ int x[] = {25, 17}; const int *foo = &x[0]; ++foo; } { /* Sun SC1.0 ANSI compiler rejects this -- but not the above. */ typedef const int *iptr; iptr p = 0; ++p; } { /* AIX XL C 1.02.0.0 rejects this saying "k.c", line 2.27: 1506-025 (S) Operand must be a modifiable lvalue. */ struct s { int j; const int *ap[3]; }; struct s *b; b->j = 5; } { /* ULTRIX-32 V3.1 (Rev 9) vcc rejects this */ const int foo = 10; if (!foo) return 0; } return !cs[0] && !zero.x; #endif ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_c_const=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_c_const=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_c_const" >&5 echo "${ECHO_T}$ac_cv_c_const" >&6; } if test $ac_cv_c_const = no; then cat >>confdefs.h <<\_ACEOF #define const _ACEOF fi { echo "$as_me:$LINENO: checking for grep that handles long lines and -e" >&5 echo $ECHO_N "checking for grep that handles long lines and -e... $ECHO_C" >&6; } if test "${ac_cv_path_GREP+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else # Extract the first word of "grep ggrep" to use in msg output if test -z "$GREP"; then set dummy grep ggrep; ac_prog_name=$2 if test "${ac_cv_path_GREP+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_path_GREP_found=false # Loop through the user's path and test for each of PROGNAME-LIST as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH$PATH_SEPARATOR/usr/xpg4/bin do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_prog in grep ggrep; do for ac_exec_ext in '' $ac_executable_extensions; do ac_path_GREP="$as_dir/$ac_prog$ac_exec_ext" { test -f "$ac_path_GREP" && $as_test_x "$ac_path_GREP"; } || continue # Check for GNU ac_path_GREP and select it if it is found. # Check for GNU $ac_path_GREP case `"$ac_path_GREP" --version 2>&1` in *GNU*) ac_cv_path_GREP="$ac_path_GREP" ac_path_GREP_found=:;; *) ac_count=0 echo $ECHO_N "0123456789$ECHO_C" >"conftest.in" while : do cat "conftest.in" "conftest.in" >"conftest.tmp" mv "conftest.tmp" "conftest.in" cp "conftest.in" "conftest.nl" echo 'GREP' >> "conftest.nl" "$ac_path_GREP" -e 'GREP$' -e '-(cannot match)-' < "conftest.nl" >"conftest.out" 2>/dev/null || break diff "conftest.out" "conftest.nl" >/dev/null 2>&1 || break ac_count=`expr $ac_count + 1` if test $ac_count -gt ${ac_path_GREP_max-0}; then # Best one so far, save it but keep looking for a better one ac_cv_path_GREP="$ac_path_GREP" ac_path_GREP_max=$ac_count fi # 10*(2^10) chars as input seems more than enough test $ac_count -gt 10 && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out;; esac $ac_path_GREP_found && break 3 done done done IFS=$as_save_IFS fi GREP="$ac_cv_path_GREP" if test -z "$GREP"; then { { echo "$as_me:$LINENO: error: no acceptable $ac_prog_name could be found in $PATH$PATH_SEPARATOR/usr/xpg4/bin" >&5 echo "$as_me: error: no acceptable $ac_prog_name could be found in $PATH$PATH_SEPARATOR/usr/xpg4/bin" >&2;} { (exit 1); exit 1; }; } fi else ac_cv_path_GREP=$GREP fi fi { echo "$as_me:$LINENO: result: $ac_cv_path_GREP" >&5 echo "${ECHO_T}$ac_cv_path_GREP" >&6; } GREP="$ac_cv_path_GREP" { echo "$as_me:$LINENO: checking for egrep" >&5 echo $ECHO_N "checking for egrep... $ECHO_C" >&6; } if test "${ac_cv_path_EGREP+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if echo a | $GREP -E '(a|b)' >/dev/null 2>&1 then ac_cv_path_EGREP="$GREP -E" else # Extract the first word of "egrep" to use in msg output if test -z "$EGREP"; then set dummy egrep; ac_prog_name=$2 if test "${ac_cv_path_EGREP+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_path_EGREP_found=false # Loop through the user's path and test for each of PROGNAME-LIST as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH$PATH_SEPARATOR/usr/xpg4/bin do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_prog in egrep; do for ac_exec_ext in '' $ac_executable_extensions; do ac_path_EGREP="$as_dir/$ac_prog$ac_exec_ext" { test -f "$ac_path_EGREP" && $as_test_x "$ac_path_EGREP"; } || continue # Check for GNU ac_path_EGREP and select it if it is found. # Check for GNU $ac_path_EGREP case `"$ac_path_EGREP" --version 2>&1` in *GNU*) ac_cv_path_EGREP="$ac_path_EGREP" ac_path_EGREP_found=:;; *) ac_count=0 echo $ECHO_N "0123456789$ECHO_C" >"conftest.in" while : do cat "conftest.in" "conftest.in" >"conftest.tmp" mv "conftest.tmp" "conftest.in" cp "conftest.in" "conftest.nl" echo 'EGREP' >> "conftest.nl" "$ac_path_EGREP" 'EGREP$' < "conftest.nl" >"conftest.out" 2>/dev/null || break diff "conftest.out" "conftest.nl" >/dev/null 2>&1 || break ac_count=`expr $ac_count + 1` if test $ac_count -gt ${ac_path_EGREP_max-0}; then # Best one so far, save it but keep looking for a better one ac_cv_path_EGREP="$ac_path_EGREP" ac_path_EGREP_max=$ac_count fi # 10*(2^10) chars as input seems more than enough test $ac_count -gt 10 && break done rm -f conftest.in conftest.tmp conftest.nl conftest.out;; esac $ac_path_EGREP_found && break 3 done done done IFS=$as_save_IFS fi EGREP="$ac_cv_path_EGREP" if test -z "$EGREP"; then { { echo "$as_me:$LINENO: error: no acceptable $ac_prog_name could be found in $PATH$PATH_SEPARATOR/usr/xpg4/bin" >&5 echo "$as_me: error: no acceptable $ac_prog_name could be found in $PATH$PATH_SEPARATOR/usr/xpg4/bin" >&2;} { (exit 1); exit 1; }; } fi else ac_cv_path_EGREP=$EGREP fi fi fi { echo "$as_me:$LINENO: result: $ac_cv_path_EGREP" >&5 echo "${ECHO_T}$ac_cv_path_EGREP" >&6; } EGREP="$ac_cv_path_EGREP" { echo "$as_me:$LINENO: checking for ANSI C header files" >&5 echo $ECHO_N "checking for ANSI C header files... $ECHO_C" >&6; } if test "${ac_cv_header_stdc+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #include #include int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_header_stdc=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_header_stdc=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $ac_cv_header_stdc = yes; then # SunOS 4.x string.h does not declare mem*, contrary to ANSI. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "memchr" >/dev/null 2>&1; then : else ac_cv_header_stdc=no fi rm -f -r conftest* fi if test $ac_cv_header_stdc = yes; then # ISC 2.0.2 stdlib.h does not declare free, contrary to ANSI. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "free" >/dev/null 2>&1; then : else ac_cv_header_stdc=no fi rm -f -r conftest* fi if test $ac_cv_header_stdc = yes; then # /bin/cc in Irix-4.0.5 gets non-ANSI ctype macros unless using -ansi. if test "$cross_compiling" = yes; then : else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #if ((' ' & 0x0FF) == 0x020) # define ISLOWER(c) ('a' <= (c) && (c) <= 'z') # define TOUPPER(c) (ISLOWER(c) ? 'A' + ((c) - 'a') : (c)) #else # define ISLOWER(c) \ (('a' <= (c) && (c) <= 'i') \ || ('j' <= (c) && (c) <= 'r') \ || ('s' <= (c) && (c) <= 'z')) # define TOUPPER(c) (ISLOWER(c) ? ((c) | 0x40) : (c)) #endif #define XOR(e, f) (((e) && !(f)) || (!(e) && (f))) int main () { int i; for (i = 0; i < 256; i++) if (XOR (islower (i), ISLOWER (i)) || toupper (i) != TOUPPER (i)) return 2; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then : else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) ac_cv_header_stdc=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi fi fi { echo "$as_me:$LINENO: result: $ac_cv_header_stdc" >&5 echo "${ECHO_T}$ac_cv_header_stdc" >&6; } if test $ac_cv_header_stdc = yes; then cat >>confdefs.h <<\_ACEOF #define STDC_HEADERS 1 _ACEOF fi # On IRIX 5.3, sys/types and inttypes.h are conflicting. for ac_header in sys/types.h sys/stat.h stdlib.h string.h memory.h strings.h \ inttypes.h stdint.h unistd.h do as_ac_Header=`echo "ac_cv_header_$ac_header" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $ac_header" >&5 echo $ECHO_N "checking for $ac_header... $ECHO_C" >&6; } if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default #include <$ac_header> _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then eval "$as_ac_Header=yes" else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 eval "$as_ac_Header=no" fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi ac_res=`eval echo '${'$as_ac_Header'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_Header'}'` = yes; then cat >>confdefs.h <<_ACEOF #define `echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done { echo "$as_me:$LINENO: checking for size_t" >&5 echo $ECHO_N "checking for size_t... $ECHO_C" >&6; } if test "${ac_cv_type_size_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef size_t ac__type_new_; int main () { if ((ac__type_new_ *) 0) return 0; if (sizeof (ac__type_new_)) return 0; ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_type_size_t=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_type_size_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_type_size_t" >&5 echo "${ECHO_T}$ac_cv_type_size_t" >&6; } if test $ac_cv_type_size_t = yes; then : else cat >>confdefs.h <<_ACEOF #define size_t unsigned int _ACEOF fi if test "x$ac_cv_prog_cc_stdc" = xno -o \ "x$ac_cv_c_const" = xno -o \ "x$ac_cv_type_size_t" = xno; then { { echo "$as_me:$LINENO: error: ------------------------------------------------------- An ANSI standard C library is required to build WCSLIB. ERROR: WCSLIB configuration failure. -------------------------------------------------------" >&5 echo "$as_me: error: ------------------------------------------------------- An ANSI standard C library is required to build WCSLIB. ERROR: WCSLIB configuration failure. -------------------------------------------------------" >&2;} { (exit 1); exit 1; }; } fi # Check for data types (suggested by autoscan - off_t is only required by # fitshdr). { echo "$as_me:$LINENO: checking for off_t" >&5 echo $ECHO_N "checking for off_t... $ECHO_C" >&6; } if test "${ac_cv_type_off_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef off_t ac__type_new_; int main () { if ((ac__type_new_ *) 0) return 0; if (sizeof (ac__type_new_)) return 0; ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_type_off_t=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_type_off_t=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_type_off_t" >&5 echo "${ECHO_T}$ac_cv_type_off_t" >&6; } if test $ac_cv_type_off_t = yes; then : else cat >>confdefs.h <<_ACEOF #define off_t long int _ACEOF fi { echo "$as_me:$LINENO: checking for int8_t" >&5 echo $ECHO_N "checking for int8_t... $ECHO_C" >&6; } if test "${ac_cv_c_int8_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_c_int8_t=no for ac_type in 'int8_t' 'int' 'long int' \ 'long long int' 'short int' 'signed char'; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(0 < ($ac_type) (((($ac_type) 1 << (8 - 2)) - 1) * 2 + 1))]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(($ac_type) (((($ac_type) 1 << (8 - 2)) - 1) * 2 + 1) < ($ac_type) (((($ac_type) 1 << (8 - 2)) - 1) * 2 + 2))]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then : else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 case $ac_type in int8_t) ac_cv_c_int8_t=yes ;; *) ac_cv_c_int8_t=$ac_type ;; esac fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$ac_cv_c_int8_t" != no && break done fi { echo "$as_me:$LINENO: result: $ac_cv_c_int8_t" >&5 echo "${ECHO_T}$ac_cv_c_int8_t" >&6; } case $ac_cv_c_int8_t in #( no|yes) ;; #( *) cat >>confdefs.h <<_ACEOF #define int8_t $ac_cv_c_int8_t _ACEOF ;; esac { echo "$as_me:$LINENO: checking for int16_t" >&5 echo $ECHO_N "checking for int16_t... $ECHO_C" >&6; } if test "${ac_cv_c_int16_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_c_int16_t=no for ac_type in 'int16_t' 'int' 'long int' \ 'long long int' 'short int' 'signed char'; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(0 < ($ac_type) (((($ac_type) 1 << (16 - 2)) - 1) * 2 + 1))]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(($ac_type) (((($ac_type) 1 << (16 - 2)) - 1) * 2 + 1) < ($ac_type) (((($ac_type) 1 << (16 - 2)) - 1) * 2 + 2))]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then : else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 case $ac_type in int16_t) ac_cv_c_int16_t=yes ;; *) ac_cv_c_int16_t=$ac_type ;; esac fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$ac_cv_c_int16_t" != no && break done fi { echo "$as_me:$LINENO: result: $ac_cv_c_int16_t" >&5 echo "${ECHO_T}$ac_cv_c_int16_t" >&6; } case $ac_cv_c_int16_t in #( no|yes) ;; #( *) cat >>confdefs.h <<_ACEOF #define int16_t $ac_cv_c_int16_t _ACEOF ;; esac { echo "$as_me:$LINENO: checking for int32_t" >&5 echo $ECHO_N "checking for int32_t... $ECHO_C" >&6; } if test "${ac_cv_c_int32_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_c_int32_t=no for ac_type in 'int32_t' 'int' 'long int' \ 'long long int' 'short int' 'signed char'; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(0 < ($ac_type) (((($ac_type) 1 << (32 - 2)) - 1) * 2 + 1))]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(($ac_type) (((($ac_type) 1 << (32 - 2)) - 1) * 2 + 1) < ($ac_type) (((($ac_type) 1 << (32 - 2)) - 1) * 2 + 2))]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then : else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 case $ac_type in int32_t) ac_cv_c_int32_t=yes ;; *) ac_cv_c_int32_t=$ac_type ;; esac fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$ac_cv_c_int32_t" != no && break done fi { echo "$as_me:$LINENO: result: $ac_cv_c_int32_t" >&5 echo "${ECHO_T}$ac_cv_c_int32_t" >&6; } case $ac_cv_c_int32_t in #( no|yes) ;; #( *) cat >>confdefs.h <<_ACEOF #define int32_t $ac_cv_c_int32_t _ACEOF ;; esac { echo "$as_me:$LINENO: checking for uint8_t" >&5 echo $ECHO_N "checking for uint8_t... $ECHO_C" >&6; } if test "${ac_cv_c_uint8_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_c_uint8_t=no for ac_type in 'uint8_t' 'unsigned int' 'unsigned long int' \ 'unsigned long long int' 'unsigned short int' 'unsigned char'; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(($ac_type) -1 >> (8 - 1) == 1)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then case $ac_type in uint8_t) ac_cv_c_uint8_t=yes ;; *) ac_cv_c_uint8_t=$ac_type ;; esac else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$ac_cv_c_uint8_t" != no && break done fi { echo "$as_me:$LINENO: result: $ac_cv_c_uint8_t" >&5 echo "${ECHO_T}$ac_cv_c_uint8_t" >&6; } case $ac_cv_c_uint8_t in #( no|yes) ;; #( *) cat >>confdefs.h <<\_ACEOF #define _UINT8_T 1 _ACEOF cat >>confdefs.h <<_ACEOF #define uint8_t $ac_cv_c_uint8_t _ACEOF ;; esac { echo "$as_me:$LINENO: checking for uint16_t" >&5 echo $ECHO_N "checking for uint16_t... $ECHO_C" >&6; } if test "${ac_cv_c_uint16_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_c_uint16_t=no for ac_type in 'uint16_t' 'unsigned int' 'unsigned long int' \ 'unsigned long long int' 'unsigned short int' 'unsigned char'; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(($ac_type) -1 >> (16 - 1) == 1)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then case $ac_type in uint16_t) ac_cv_c_uint16_t=yes ;; *) ac_cv_c_uint16_t=$ac_type ;; esac else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$ac_cv_c_uint16_t" != no && break done fi { echo "$as_me:$LINENO: result: $ac_cv_c_uint16_t" >&5 echo "${ECHO_T}$ac_cv_c_uint16_t" >&6; } case $ac_cv_c_uint16_t in #( no|yes) ;; #( *) cat >>confdefs.h <<_ACEOF #define uint16_t $ac_cv_c_uint16_t _ACEOF ;; esac { echo "$as_me:$LINENO: checking for uint32_t" >&5 echo $ECHO_N "checking for uint32_t... $ECHO_C" >&6; } if test "${ac_cv_c_uint32_t+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_c_uint32_t=no for ac_type in 'uint32_t' 'unsigned int' 'unsigned long int' \ 'unsigned long long int' 'unsigned short int' 'unsigned char'; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { static int test_array [1 - 2 * !(($ac_type) -1 >> (32 - 1) == 1)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then case $ac_type in uint32_t) ac_cv_c_uint32_t=yes ;; *) ac_cv_c_uint32_t=$ac_type ;; esac else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext test "$ac_cv_c_uint32_t" != no && break done fi { echo "$as_me:$LINENO: result: $ac_cv_c_uint32_t" >&5 echo "${ECHO_T}$ac_cv_c_uint32_t" >&6; } case $ac_cv_c_uint32_t in #( no|yes) ;; #( *) cat >>confdefs.h <<\_ACEOF #define _UINT32_T 1 _ACEOF cat >>confdefs.h <<_ACEOF #define uint32_t $ac_cv_c_uint32_t _ACEOF ;; esac # Check for ANSI C headers. { echo "$as_me:$LINENO: checking for ANSI C header files" >&5 echo $ECHO_N "checking for ANSI C header files... $ECHO_C" >&6; } if test "${ac_cv_header_stdc+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #include #include int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_header_stdc=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_header_stdc=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext if test $ac_cv_header_stdc = yes; then # SunOS 4.x string.h does not declare mem*, contrary to ANSI. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "memchr" >/dev/null 2>&1; then : else ac_cv_header_stdc=no fi rm -f -r conftest* fi if test $ac_cv_header_stdc = yes; then # ISC 2.0.2 stdlib.h does not declare free, contrary to ANSI. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include _ACEOF if (eval "$ac_cpp conftest.$ac_ext") 2>&5 | $EGREP "free" >/dev/null 2>&1; then : else ac_cv_header_stdc=no fi rm -f -r conftest* fi if test $ac_cv_header_stdc = yes; then # /bin/cc in Irix-4.0.5 gets non-ANSI ctype macros unless using -ansi. if test "$cross_compiling" = yes; then : else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #include #if ((' ' & 0x0FF) == 0x020) # define ISLOWER(c) ('a' <= (c) && (c) <= 'z') # define TOUPPER(c) (ISLOWER(c) ? 'A' + ((c) - 'a') : (c)) #else # define ISLOWER(c) \ (('a' <= (c) && (c) <= 'i') \ || ('j' <= (c) && (c) <= 'r') \ || ('s' <= (c) && (c) <= 'z')) # define TOUPPER(c) (ISLOWER(c) ? ((c) | 0x40) : (c)) #endif #define XOR(e, f) (((e) && !(f)) || (!(e) && (f))) int main () { int i; for (i = 0; i < 256; i++) if (XOR (islower (i), ISLOWER (i)) || toupper (i) != TOUPPER (i)) return 2; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then : else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) ac_cv_header_stdc=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi fi fi { echo "$as_me:$LINENO: result: $ac_cv_header_stdc" >&5 echo "${ECHO_T}$ac_cv_header_stdc" >&6; } if test $ac_cv_header_stdc = yes; then cat >>confdefs.h <<\_ACEOF #define STDC_HEADERS 1 _ACEOF fi for ac_header in ctype.h errno.h limits.h math.h setjmp.h stdarg.h stdio.h \ stdlib.h string.h do as_ac_Header=`echo "ac_cv_header_$ac_header" | $as_tr_sh` if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then { echo "$as_me:$LINENO: checking for $ac_header" >&5 echo $ECHO_N "checking for $ac_header... $ECHO_C" >&6; } if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 fi ac_res=`eval echo '${'$as_ac_Header'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } else # Is the header compilable? { echo "$as_me:$LINENO: checking $ac_header usability" >&5 echo $ECHO_N "checking $ac_header usability... $ECHO_C" >&6; } cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default #include <$ac_header> _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_header_compiler=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_header_compiler=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext { echo "$as_me:$LINENO: result: $ac_header_compiler" >&5 echo "${ECHO_T}$ac_header_compiler" >&6; } # Is the header present? { echo "$as_me:$LINENO: checking $ac_header presence" >&5 echo $ECHO_N "checking $ac_header presence... $ECHO_C" >&6; } cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include <$ac_header> _ACEOF if { (ac_try="$ac_cpp conftest.$ac_ext" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_cpp conftest.$ac_ext") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } >/dev/null && { test -z "$ac_c_preproc_warn_flag$ac_c_werror_flag" || test ! -s conftest.err }; then ac_header_preproc=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_header_preproc=no fi rm -f conftest.err conftest.$ac_ext { echo "$as_me:$LINENO: result: $ac_header_preproc" >&5 echo "${ECHO_T}$ac_header_preproc" >&6; } # So? What about this header? case $ac_header_compiler:$ac_header_preproc:$ac_c_preproc_warn_flag in yes:no: ) { echo "$as_me:$LINENO: WARNING: $ac_header: accepted by the compiler, rejected by the preprocessor!" >&5 echo "$as_me: WARNING: $ac_header: accepted by the compiler, rejected by the preprocessor!" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: proceeding with the compiler's result" >&5 echo "$as_me: WARNING: $ac_header: proceeding with the compiler's result" >&2;} ac_header_preproc=yes ;; no:yes:* ) { echo "$as_me:$LINENO: WARNING: $ac_header: present but cannot be compiled" >&5 echo "$as_me: WARNING: $ac_header: present but cannot be compiled" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: check for missing prerequisite headers?" >&5 echo "$as_me: WARNING: $ac_header: check for missing prerequisite headers?" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: see the Autoconf documentation" >&5 echo "$as_me: WARNING: $ac_header: see the Autoconf documentation" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: section \"Present But Cannot Be Compiled\"" >&5 echo "$as_me: WARNING: $ac_header: section \"Present But Cannot Be Compiled\"" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: proceeding with the preprocessor's result" >&5 echo "$as_me: WARNING: $ac_header: proceeding with the preprocessor's result" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: in the future, the compiler will take precedence" >&5 echo "$as_me: WARNING: $ac_header: in the future, the compiler will take precedence" >&2;} ( cat <<\_ASBOX ## ------------------------------------- ## ## Report this to mcalabre@atnf.csiro.au ## ## ------------------------------------- ## _ASBOX ) | sed "s/^/$as_me: WARNING: /" >&2 ;; esac { echo "$as_me:$LINENO: checking for $ac_header" >&5 echo $ECHO_N "checking for $ac_header... $ECHO_C" >&6; } if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else eval "$as_ac_Header=\$ac_header_preproc" fi ac_res=`eval echo '${'$as_ac_Header'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } fi if test `eval echo '${'$as_ac_Header'}'` = yes; then cat >>confdefs.h <<_ACEOF #define `echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done if test "x$ac_cv_header_stdc" = xno; then { { echo "$as_me:$LINENO: error: ------------------------------------------------------------------- An ANSI standard C library is required to build WCSLIB. One of the ANSI C header files it requires is missing or unusable. ERROR: WCSLIB configuration failure. -------------------------------------------------------------------" >&5 echo "$as_me: error: ------------------------------------------------------------------- An ANSI standard C library is required to build WCSLIB. One of the ANSI C header files it requires is missing or unusable. ERROR: WCSLIB configuration failure. -------------------------------------------------------------------" >&2;} { (exit 1); exit 1; }; } fi # Checks for ANSI C library functions (suggested by autoscan - fseeko and # stat are only required by fitshdr). { echo "$as_me:$LINENO: checking for floor in -lm" >&5 echo $ECHO_N "checking for floor in -lm... $ECHO_C" >&6; } if test "${ac_cv_lib_m_floor+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lm $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char floor (); int main () { return floor (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_m_floor=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_m_floor=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_m_floor" >&5 echo "${ECHO_T}$ac_cv_lib_m_floor" >&6; } if test $ac_cv_lib_m_floor = yes; then cat >>confdefs.h <<_ACEOF #define HAVE_LIBM 1 _ACEOF LIBS="-lm $LIBS" fi { echo "$as_me:$LINENO: checking for _LARGEFILE_SOURCE value needed for large files" >&5 echo $ECHO_N "checking for _LARGEFILE_SOURCE value needed for large files... $ECHO_C" >&6; } if test "${ac_cv_sys_largefile_source+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include int main () { return fseeko (stdin, 0, 0) && (fseeko) (stdin, 0, 0); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_sys_largefile_source=no; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #define _LARGEFILE_SOURCE 1 #include int main () { return fseeko (stdin, 0, 0) && (fseeko) (stdin, 0, 0); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_sys_largefile_source=1; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext ac_cv_sys_largefile_source=unknown break done fi { echo "$as_me:$LINENO: result: $ac_cv_sys_largefile_source" >&5 echo "${ECHO_T}$ac_cv_sys_largefile_source" >&6; } case $ac_cv_sys_largefile_source in #( no | unknown) ;; *) cat >>confdefs.h <<_ACEOF #define _LARGEFILE_SOURCE $ac_cv_sys_largefile_source _ACEOF ;; esac rm -f -r conftest* # We used to try defining _XOPEN_SOURCE=500 too, to work around a bug # in glibc 2.1.3, but that breaks too many other things. # If you want fseeko and ftello with glibc, upgrade to a fixed glibc. if test $ac_cv_sys_largefile_source != unknown; then cat >>confdefs.h <<\_ACEOF #define HAVE_FSEEKO 1 _ACEOF fi for ac_header in stdlib.h do as_ac_Header=`echo "ac_cv_header_$ac_header" | $as_tr_sh` if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then { echo "$as_me:$LINENO: checking for $ac_header" >&5 echo $ECHO_N "checking for $ac_header... $ECHO_C" >&6; } if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 fi ac_res=`eval echo '${'$as_ac_Header'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } else # Is the header compilable? { echo "$as_me:$LINENO: checking $ac_header usability" >&5 echo $ECHO_N "checking $ac_header usability... $ECHO_C" >&6; } cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default #include <$ac_header> _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_header_compiler=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_header_compiler=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext { echo "$as_me:$LINENO: result: $ac_header_compiler" >&5 echo "${ECHO_T}$ac_header_compiler" >&6; } # Is the header present? 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{ echo "$as_me:$LINENO: checking $ac_header usability" >&5 echo $ECHO_N "checking $ac_header usability... $ECHO_C" >&6; } cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default #include <$ac_header> _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_header_compiler=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_header_compiler=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext { echo "$as_me:$LINENO: result: $ac_header_compiler" >&5 echo "${ECHO_T}$ac_header_compiler" >&6; } # Is the header present? { echo "$as_me:$LINENO: checking $ac_header presence" >&5 echo $ECHO_N "checking $ac_header presence... $ECHO_C" >&6; } cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include <$ac_header> _ACEOF if { (ac_try="$ac_cpp conftest.$ac_ext" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_cpp conftest.$ac_ext") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } >/dev/null && { test -z "$ac_c_preproc_warn_flag$ac_c_werror_flag" || test ! -s conftest.err }; then ac_header_preproc=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_header_preproc=no fi rm -f conftest.err conftest.$ac_ext { echo "$as_me:$LINENO: result: $ac_header_preproc" >&5 echo "${ECHO_T}$ac_header_preproc" >&6; } # So? What about this header? case $ac_header_compiler:$ac_header_preproc:$ac_c_preproc_warn_flag in yes:no: ) { echo "$as_me:$LINENO: WARNING: $ac_header: accepted by the compiler, rejected by the preprocessor!" >&5 echo "$as_me: WARNING: $ac_header: accepted by the compiler, rejected by the preprocessor!" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: proceeding with the compiler's result" >&5 echo "$as_me: WARNING: $ac_header: proceeding with the compiler's result" >&2;} ac_header_preproc=yes ;; no:yes:* ) { echo "$as_me:$LINENO: WARNING: $ac_header: present but cannot be compiled" >&5 echo "$as_me: WARNING: $ac_header: present but cannot be compiled" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: check for missing prerequisite headers?" >&5 echo "$as_me: WARNING: $ac_header: check for missing prerequisite headers?" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: see the Autoconf documentation" >&5 echo "$as_me: WARNING: $ac_header: see the Autoconf documentation" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: section \"Present But Cannot Be Compiled\"" >&5 echo "$as_me: WARNING: $ac_header: section \"Present But Cannot Be Compiled\"" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: proceeding with the preprocessor's result" >&5 echo "$as_me: WARNING: $ac_header: proceeding with the preprocessor's result" >&2;} { echo "$as_me:$LINENO: WARNING: $ac_header: in the future, the compiler will take precedence" >&5 echo "$as_me: WARNING: $ac_header: in the future, the compiler will take precedence" >&2;} ( cat <<\_ASBOX ## ------------------------------------- ## ## Report this to mcalabre@atnf.csiro.au ## ## ------------------------------------- ## _ASBOX ) | sed "s/^/$as_me: WARNING: /" >&2 ;; esac { echo "$as_me:$LINENO: checking for $ac_header" >&5 echo $ECHO_N "checking for $ac_header... $ECHO_C" >&6; } if { as_var=$as_ac_Header; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else eval "$as_ac_Header=\$ac_header_preproc" fi ac_res=`eval echo '${'$as_ac_Header'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } fi if test `eval echo '${'$as_ac_Header'}'` = yes; then cat >>confdefs.h <<_ACEOF #define `echo "HAVE_$ac_header" | $as_tr_cpp` 1 _ACEOF fi done { echo "$as_me:$LINENO: checking for GNU libc compatible realloc" >&5 echo $ECHO_N "checking for GNU libc compatible realloc... $ECHO_C" >&6; } if test "${ac_cv_func_realloc_0_nonnull+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test "$cross_compiling" = yes; then ac_cv_func_realloc_0_nonnull=no else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #if defined STDC_HEADERS || defined HAVE_STDLIB_H # include #else char *realloc (); #endif int main () { return ! realloc (0, 0); ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_func_realloc_0_nonnull=yes else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) ac_cv_func_realloc_0_nonnull=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi fi { echo "$as_me:$LINENO: result: $ac_cv_func_realloc_0_nonnull" >&5 echo "${ECHO_T}$ac_cv_func_realloc_0_nonnull" >&6; } if test $ac_cv_func_realloc_0_nonnull = yes; then cat >>confdefs.h <<\_ACEOF #define HAVE_REALLOC 1 _ACEOF else cat >>confdefs.h <<\_ACEOF #define HAVE_REALLOC 0 _ACEOF case " $LIBOBJS " in *" realloc.$ac_objext "* ) ;; *) LIBOBJS="$LIBOBJS realloc.$ac_objext" ;; esac cat >>confdefs.h <<\_ACEOF #define realloc rpl_realloc _ACEOF fi { echo "$as_me:$LINENO: checking for function prototypes" >&5 echo $ECHO_N "checking for function prototypes... $ECHO_C" >&6; } if test "$ac_cv_prog_cc_c89" != no; then { echo "$as_me:$LINENO: result: yes" >&5 echo "${ECHO_T}yes" >&6; } cat >>confdefs.h <<\_ACEOF #define PROTOTYPES 1 _ACEOF cat >>confdefs.h <<\_ACEOF #define __PROTOTYPES 1 _ACEOF else { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi { echo "$as_me:$LINENO: checking whether setvbuf arguments are reversed" >&5 echo $ECHO_N "checking whether setvbuf arguments are reversed... $ECHO_C" >&6; } if test "${ac_cv_func_setvbuf_reversed+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_func_setvbuf_reversed=no cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include # ifdef PROTOTYPES int (setvbuf) (FILE *, int, char *, size_t); # endif int main () { char buf; return setvbuf (stdout, _IOLBF, &buf, 1); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include # ifdef PROTOTYPES int (setvbuf) (FILE *, int, char *, size_t); # endif int main () { char buf; return setvbuf (stdout, &buf, _IOLBF, 1); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then # It compiles and links either way, so it must not be declared # with a prototype and most likely this is a K&R C compiler. # Try running it. if test "$cross_compiling" = yes; then : # Assume setvbuf is not reversed when cross-compiling. else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { /* This call has the arguments reversed. A reversed system may check and see that the address of buf is not _IOLBF, _IONBF, or _IOFBF, and return nonzero. */ char buf; if (setvbuf (stdout, _IOLBF, &buf, 1) != 0) return 1; putchar ('\r'); return 0; /* Non-reversed systems SEGV here. */ ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_func_setvbuf_reversed=yes else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi ac_cv_func_setvbuf_reversed=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_func_setvbuf_reversed" >&5 echo "${ECHO_T}$ac_cv_func_setvbuf_reversed" >&6; } if test $ac_cv_func_setvbuf_reversed = yes; then cat >>confdefs.h <<\_ACEOF #define SETVBUF_REVERSED 1 _ACEOF fi { echo "$as_me:$LINENO: checking whether lstat dereferences a symlink specified with a trailing slash" >&5 echo $ECHO_N "checking whether lstat dereferences a symlink specified with a trailing slash... $ECHO_C" >&6; } if test "${ac_cv_func_lstat_dereferences_slashed_symlink+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else rm -f conftest.sym conftest.file echo >conftest.file if test "$as_ln_s" = "ln -s" && ln -s conftest.file conftest.sym; then if test "$cross_compiling" = yes; then ac_cv_func_lstat_dereferences_slashed_symlink=no else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { struct stat sbuf; /* Linux will dereference the symlink and fail. That is better in the sense that it means we will not have to compile and use the lstat wrapper. */ return lstat ("conftest.sym/", &sbuf) == 0; ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_func_lstat_dereferences_slashed_symlink=yes else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) ac_cv_func_lstat_dereferences_slashed_symlink=no fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi else # If the `ln -s' command failed, then we probably don't even # have an lstat function. ac_cv_func_lstat_dereferences_slashed_symlink=no fi rm -f conftest.sym conftest.file fi { echo "$as_me:$LINENO: result: $ac_cv_func_lstat_dereferences_slashed_symlink" >&5 echo "${ECHO_T}$ac_cv_func_lstat_dereferences_slashed_symlink" >&6; } test $ac_cv_func_lstat_dereferences_slashed_symlink = yes && cat >>confdefs.h <<_ACEOF #define LSTAT_FOLLOWS_SLASHED_SYMLINK 1 _ACEOF if test $ac_cv_func_lstat_dereferences_slashed_symlink = no; then case " $LIBOBJS " in *" lstat.$ac_objext "* ) ;; *) LIBOBJS="$LIBOBJS lstat.$ac_objext" ;; esac fi { echo "$as_me:$LINENO: checking whether stat accepts an empty string" >&5 echo $ECHO_N "checking whether stat accepts an empty string... $ECHO_C" >&6; } if test "${ac_cv_func_stat_empty_string_bug+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test "$cross_compiling" = yes; then ac_cv_func_stat_empty_string_bug=yes else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { struct stat sbuf; return stat ("", &sbuf) == 0; ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_func_stat_empty_string_bug=no else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) ac_cv_func_stat_empty_string_bug=yes fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi fi { echo "$as_me:$LINENO: result: $ac_cv_func_stat_empty_string_bug" >&5 echo "${ECHO_T}$ac_cv_func_stat_empty_string_bug" >&6; } if test $ac_cv_func_stat_empty_string_bug = yes; then case " $LIBOBJS " in *" stat.$ac_objext "* ) ;; *) LIBOBJS="$LIBOBJS stat.$ac_objext" ;; esac cat >>confdefs.h <<_ACEOF #define HAVE_STAT_EMPTY_STRING_BUG 1 _ACEOF fi for ac_func in vprintf do as_ac_var=`echo "ac_cv_func_$ac_func" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $ac_func" >&5 echo $ECHO_N "checking for $ac_func... $ECHO_C" >&6; } if { as_var=$as_ac_var; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Define $ac_func to an innocuous variant, in case declares $ac_func. For example, HP-UX 11i declares gettimeofday. */ #define $ac_func innocuous_$ac_func /* System header to define __stub macros and hopefully few prototypes, which can conflict with char $ac_func (); below. Prefer to if __STDC__ is defined, since exists even on freestanding compilers. */ #ifdef __STDC__ # include #else # include #endif #undef $ac_func /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char $ac_func (); /* The GNU C library defines this for functions which it implements to always fail with ENOSYS. Some functions are actually named something starting with __ and the normal name is an alias. */ #if defined __stub_$ac_func || defined __stub___$ac_func choke me #endif int main () { return $ac_func (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then eval "$as_ac_var=yes" else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 eval "$as_ac_var=no" fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext fi ac_res=`eval echo '${'$as_ac_var'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_var'}'` = yes; then cat >>confdefs.h <<_ACEOF #define `echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF { echo "$as_me:$LINENO: checking for _doprnt" >&5 echo $ECHO_N "checking for _doprnt... $ECHO_C" >&6; } if test "${ac_cv_func__doprnt+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Define _doprnt to an innocuous variant, in case declares _doprnt. For example, HP-UX 11i declares gettimeofday. */ #define _doprnt innocuous__doprnt /* System header to define __stub macros and hopefully few prototypes, which can conflict with char _doprnt (); below. Prefer to if __STDC__ is defined, since exists even on freestanding compilers. */ #ifdef __STDC__ # include #else # include #endif #undef _doprnt /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char _doprnt (); /* The GNU C library defines this for functions which it implements to always fail with ENOSYS. Some functions are actually named something starting with __ and the normal name is an alias. */ #if defined __stub__doprnt || defined __stub____doprnt choke me #endif int main () { return _doprnt (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_func__doprnt=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_func__doprnt=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_func__doprnt" >&5 echo "${ECHO_T}$ac_cv_func__doprnt" >&6; } if test $ac_cv_func__doprnt = yes; then cat >>confdefs.h <<\_ACEOF #define HAVE_DOPRNT 1 _ACEOF fi fi done for ac_func in floor memset pow sqrt strchr strstr do as_ac_var=`echo "ac_cv_func_$ac_func" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $ac_func" >&5 echo $ECHO_N "checking for $ac_func... $ECHO_C" >&6; } if { as_var=$as_ac_var; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Define $ac_func to an innocuous variant, in case declares $ac_func. For example, HP-UX 11i declares gettimeofday. */ #define $ac_func innocuous_$ac_func /* System header to define __stub macros and hopefully few prototypes, which can conflict with char $ac_func (); below. Prefer to if __STDC__ is defined, since exists even on freestanding compilers. */ #ifdef __STDC__ # include #else # include #endif #undef $ac_func /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char $ac_func (); /* The GNU C library defines this for functions which it implements to always fail with ENOSYS. Some functions are actually named something starting with __ and the normal name is an alias. */ #if defined __stub_$ac_func || defined __stub___$ac_func choke me #endif int main () { return $ac_func (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then eval "$as_ac_var=yes" else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 eval "$as_ac_var=no" fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext fi ac_res=`eval echo '${'$as_ac_var'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_var'}'` = yes; then cat >>confdefs.h <<_ACEOF #define `echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done # System libraries that may be required by WCSLIB itself. # SunOS, extra maths functions. { echo "$as_me:$LINENO: checking for cosd in -lsunmath" >&5 echo $ECHO_N "checking for cosd in -lsunmath... $ECHO_C" >&6; } if test "${ac_cv_lib_sunmath_cosd+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lsunmath $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char cosd (); int main () { return cosd (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_sunmath_cosd=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_sunmath_cosd=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_sunmath_cosd" >&5 echo "${ECHO_T}$ac_cv_lib_sunmath_cosd" >&6; } if test $ac_cv_lib_sunmath_cosd = yes; then LIBS="-lsunmath $LIBS" fi # See if we can find sincos(). for ac_func in sincos do as_ac_var=`echo "ac_cv_func_$ac_func" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $ac_func" >&5 echo $ECHO_N "checking for $ac_func... $ECHO_C" >&6; } if { as_var=$as_ac_var; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Define $ac_func to an innocuous variant, in case declares $ac_func. For example, HP-UX 11i declares gettimeofday. */ #define $ac_func innocuous_$ac_func /* System header to define __stub macros and hopefully few prototypes, which can conflict with char $ac_func (); below. Prefer to if __STDC__ is defined, since exists even on freestanding compilers. */ #ifdef __STDC__ # include #else # include #endif #undef $ac_func /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char $ac_func (); /* The GNU C library defines this for functions which it implements to always fail with ENOSYS. Some functions are actually named something starting with __ and the normal name is an alias. */ #if defined __stub_$ac_func || defined __stub___$ac_func choke me #endif int main () { return $ac_func (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then eval "$as_ac_var=yes" else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 eval "$as_ac_var=no" fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext fi ac_res=`eval echo '${'$as_ac_var'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_var'}'` = yes; then cat >>confdefs.h <<_ACEOF #define `echo "HAVE_$ac_func" | $as_tr_cpp` 1 _ACEOF fi done # Check the size and availability of integer data types. { echo "$as_me:$LINENO: checking for int" >&5 echo $ECHO_N "checking for int... $ECHO_C" >&6; } if test "${ac_cv_type_int+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_new_; int main () { if ((ac__type_new_ *) 0) return 0; if (sizeof (ac__type_new_)) return 0; ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_type_int=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_type_int=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_type_int" >&5 echo "${ECHO_T}$ac_cv_type_int" >&6; } # The cast to long int works around a bug in the HP C Compiler # version HP92453-01 B.11.11.23709.GP, which incorrectly rejects # declarations like `int a3[[(sizeof (unsigned char)) >= 0]];'. # This bug is HP SR number 8606223364. { echo "$as_me:$LINENO: checking size of int" >&5 echo $ECHO_N "checking size of int... $ECHO_C" >&6; } if test "${ac_cv_sizeof_int+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test "$cross_compiling" = yes; then # Depending upon the size, compute the lo and hi bounds. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) >= 0)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_lo=0 ac_mid=0 while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) <= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=$ac_mid; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo=`expr $ac_mid + 1` if test $ac_lo -le $ac_mid; then ac_lo= ac_hi= break fi ac_mid=`expr 2 '*' $ac_mid + 1` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) < 0)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=-1 ac_mid=-1 while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) >= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_lo=$ac_mid; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_hi=`expr '(' $ac_mid ')' - 1` if test $ac_mid -le $ac_hi; then ac_lo= ac_hi= break fi ac_mid=`expr 2 '*' $ac_mid` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo= ac_hi= fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext # Binary search between lo and hi bounds. while test "x$ac_lo" != "x$ac_hi"; do ac_mid=`expr '(' $ac_hi - $ac_lo ')' / 2 + $ac_lo` cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) <= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=$ac_mid else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo=`expr '(' $ac_mid ')' + 1` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done case $ac_lo in ?*) ac_cv_sizeof_int=$ac_lo;; '') if test "$ac_cv_type_int" = yes; then { { echo "$as_me:$LINENO: error: cannot compute sizeof (int) See \`config.log' for more details." >&5 echo "$as_me: error: cannot compute sizeof (int) See \`config.log' for more details." >&2;} { (exit 77); exit 77; }; } else ac_cv_sizeof_int=0 fi ;; esac else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef int ac__type_sizeof_; static long int longval () { return (long int) (sizeof (ac__type_sizeof_)); } static unsigned long int ulongval () { return (long int) (sizeof (ac__type_sizeof_)); } #include #include int main () { FILE *f = fopen ("conftest.val", "w"); if (! f) return 1; if (((long int) (sizeof (ac__type_sizeof_))) < 0) { long int i = longval (); if (i != ((long int) (sizeof (ac__type_sizeof_)))) return 1; fprintf (f, "%ld\n", i); } else { unsigned long int i = ulongval (); if (i != ((long int) (sizeof (ac__type_sizeof_)))) return 1; fprintf (f, "%lu\n", i); } return ferror (f) || fclose (f) != 0; ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_sizeof_int=`cat conftest.val` else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) if test "$ac_cv_type_int" = yes; then { { echo "$as_me:$LINENO: error: cannot compute sizeof (int) See \`config.log' for more details." >&5 echo "$as_me: error: cannot compute sizeof (int) See \`config.log' for more details." >&2;} { (exit 77); exit 77; }; } else ac_cv_sizeof_int=0 fi fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi rm -f conftest.val fi { echo "$as_me:$LINENO: result: $ac_cv_sizeof_int" >&5 echo "${ECHO_T}$ac_cv_sizeof_int" >&6; } cat >>confdefs.h <<_ACEOF #define SIZEOF_INT $ac_cv_sizeof_int _ACEOF { echo "$as_me:$LINENO: checking for long int" >&5 echo $ECHO_N "checking for long int... $ECHO_C" >&6; } if test "${ac_cv_type_long_int+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_new_; int main () { if ((ac__type_new_ *) 0) return 0; if (sizeof (ac__type_new_)) return 0; ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_type_long_int=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_type_long_int=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_type_long_int" >&5 echo "${ECHO_T}$ac_cv_type_long_int" >&6; } # The cast to long int works around a bug in the HP C Compiler # version HP92453-01 B.11.11.23709.GP, which incorrectly rejects # declarations like `int a3[[(sizeof (unsigned char)) >= 0]];'. # This bug is HP SR number 8606223364. { echo "$as_me:$LINENO: checking size of long int" >&5 echo $ECHO_N "checking size of long int... $ECHO_C" >&6; } if test "${ac_cv_sizeof_long_int+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test "$cross_compiling" = yes; then # Depending upon the size, compute the lo and hi bounds. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) >= 0)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_lo=0 ac_mid=0 while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) <= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=$ac_mid; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo=`expr $ac_mid + 1` if test $ac_lo -le $ac_mid; then ac_lo= ac_hi= break fi ac_mid=`expr 2 '*' $ac_mid + 1` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) < 0)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=-1 ac_mid=-1 while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) >= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_lo=$ac_mid; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_hi=`expr '(' $ac_mid ')' - 1` if test $ac_mid -le $ac_hi; then ac_lo= ac_hi= break fi ac_mid=`expr 2 '*' $ac_mid` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo= ac_hi= fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext # Binary search between lo and hi bounds. while test "x$ac_lo" != "x$ac_hi"; do ac_mid=`expr '(' $ac_hi - $ac_lo ')' / 2 + $ac_lo` cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) <= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=$ac_mid else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo=`expr '(' $ac_mid ')' + 1` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done case $ac_lo in ?*) ac_cv_sizeof_long_int=$ac_lo;; '') if test "$ac_cv_type_long_int" = yes; then { { echo "$as_me:$LINENO: error: cannot compute sizeof (long int) See \`config.log' for more details." >&5 echo "$as_me: error: cannot compute sizeof (long int) See \`config.log' for more details." >&2;} { (exit 77); exit 77; }; } else ac_cv_sizeof_long_int=0 fi ;; esac else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long int ac__type_sizeof_; static long int longval () { return (long int) (sizeof (ac__type_sizeof_)); } static unsigned long int ulongval () { return (long int) (sizeof (ac__type_sizeof_)); } #include #include int main () { FILE *f = fopen ("conftest.val", "w"); if (! f) return 1; if (((long int) (sizeof (ac__type_sizeof_))) < 0) { long int i = longval (); if (i != ((long int) (sizeof (ac__type_sizeof_)))) return 1; fprintf (f, "%ld\n", i); } else { unsigned long int i = ulongval (); if (i != ((long int) (sizeof (ac__type_sizeof_)))) return 1; fprintf (f, "%lu\n", i); } return ferror (f) || fclose (f) != 0; ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_sizeof_long_int=`cat conftest.val` else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) if test "$ac_cv_type_long_int" = yes; then { { echo "$as_me:$LINENO: error: cannot compute sizeof (long int) See \`config.log' for more details." >&5 echo "$as_me: error: cannot compute sizeof (long int) See \`config.log' for more details." >&2;} { (exit 77); exit 77; }; } else ac_cv_sizeof_long_int=0 fi fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi rm -f conftest.val fi { echo "$as_me:$LINENO: result: $ac_cv_sizeof_long_int" >&5 echo "${ECHO_T}$ac_cv_sizeof_long_int" >&6; } cat >>confdefs.h <<_ACEOF #define SIZEOF_LONG_INT $ac_cv_sizeof_long_int _ACEOF { echo "$as_me:$LINENO: checking for long long int" >&5 echo $ECHO_N "checking for long long int... $ECHO_C" >&6; } if test "${ac_cv_type_long_long_int+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_new_; int main () { if ((ac__type_new_ *) 0) return 0; if (sizeof (ac__type_new_)) return 0; ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_type_long_long_int=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_type_long_long_int=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_type_long_long_int" >&5 echo "${ECHO_T}$ac_cv_type_long_long_int" >&6; } # The cast to long int works around a bug in the HP C Compiler # version HP92453-01 B.11.11.23709.GP, which incorrectly rejects # declarations like `int a3[[(sizeof (unsigned char)) >= 0]];'. # This bug is HP SR number 8606223364. { echo "$as_me:$LINENO: checking size of long long int" >&5 echo $ECHO_N "checking size of long long int... $ECHO_C" >&6; } if test "${ac_cv_sizeof_long_long_int+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test "$cross_compiling" = yes; then # Depending upon the size, compute the lo and hi bounds. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) >= 0)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_lo=0 ac_mid=0 while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) <= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=$ac_mid; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo=`expr $ac_mid + 1` if test $ac_lo -le $ac_mid; then ac_lo= ac_hi= break fi ac_mid=`expr 2 '*' $ac_mid + 1` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) < 0)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=-1 ac_mid=-1 while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) >= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_lo=$ac_mid; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_hi=`expr '(' $ac_mid ')' - 1` if test $ac_mid -le $ac_hi; then ac_lo= ac_hi= break fi ac_mid=`expr 2 '*' $ac_mid` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo= ac_hi= fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext # Binary search between lo and hi bounds. while test "x$ac_lo" != "x$ac_hi"; do ac_mid=`expr '(' $ac_hi - $ac_lo ')' / 2 + $ac_lo` cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_sizeof_; int main () { static int test_array [1 - 2 * !(((long int) (sizeof (ac__type_sizeof_))) <= $ac_mid)]; test_array [0] = 0 ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_hi=$ac_mid else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_lo=`expr '(' $ac_mid ')' + 1` fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext done case $ac_lo in ?*) ac_cv_sizeof_long_long_int=$ac_lo;; '') if test "$ac_cv_type_long_long_int" = yes; then { { echo "$as_me:$LINENO: error: cannot compute sizeof (long long int) See \`config.log' for more details." >&5 echo "$as_me: error: cannot compute sizeof (long long int) See \`config.log' for more details." >&2;} { (exit 77); exit 77; }; } else ac_cv_sizeof_long_long_int=0 fi ;; esac else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default typedef long long int ac__type_sizeof_; static long int longval () { return (long int) (sizeof (ac__type_sizeof_)); } static unsigned long int ulongval () { return (long int) (sizeof (ac__type_sizeof_)); } #include #include int main () { FILE *f = fopen ("conftest.val", "w"); if (! f) return 1; if (((long int) (sizeof (ac__type_sizeof_))) < 0) { long int i = longval (); if (i != ((long int) (sizeof (ac__type_sizeof_)))) return 1; fprintf (f, "%ld\n", i); } else { unsigned long int i = ulongval (); if (i != ((long int) (sizeof (ac__type_sizeof_)))) return 1; fprintf (f, "%lu\n", i); } return ferror (f) || fclose (f) != 0; ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then ac_cv_sizeof_long_long_int=`cat conftest.val` else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) if test "$ac_cv_type_long_long_int" = yes; then { { echo "$as_me:$LINENO: error: cannot compute sizeof (long long int) See \`config.log' for more details." >&5 echo "$as_me: error: cannot compute sizeof (long long int) See \`config.log' for more details." >&2;} { (exit 77); exit 77; }; } else ac_cv_sizeof_long_long_int=0 fi fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi rm -f conftest.val fi { echo "$as_me:$LINENO: result: $ac_cv_sizeof_long_long_int" >&5 echo "${ECHO_T}$ac_cv_sizeof_long_long_int" >&6; } cat >>confdefs.h <<_ACEOF #define SIZEOF_LONG_LONG_INT $ac_cv_sizeof_long_long_int _ACEOF # 64-bit integer data type; use long long int preferentially since that # accords with "%lld" formatting used in fitshdr.l, e.g. # int size_t long int long long int # --- ------ -------- ------------- # gcc x86: 32 32 32 64 # gcc x86_64: 32 64 64 64 if test "x$ac_cv_sizeof_long_long_int" = x8; then cat >>confdefs.h <<\_ACEOF #define WCSLIB_INT64 long long int _ACEOF elif test "x$ac_cv_sizeof_long_int" = x8; then cat >>confdefs.h <<\_ACEOF #define WCSLIB_INT64 long int _ACEOF elif test "x$ac_cv_sizeof_int" = x8; then cat >>confdefs.h <<\_ACEOF #define WCSLIB_INT64 int _ACEOF fi # Does printf() have the z modifier for size_t type? Important for 64-bit. { echo "$as_me:$LINENO: checking for printf z format modifier for size_t type" >&5 echo $ECHO_N "checking for printf z format modifier for size_t type... $ECHO_C" >&6; } if test "$cross_compiling" = yes; then cat >>confdefs.h <<\_ACEOF #define MODZ "" _ACEOF { echo "$as_me:$LINENO: result: assumed not" >&5 echo "${ECHO_T}assumed not" >&6; } else cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ $ac_includes_default int main () { char buf[64]; if (sprintf(buf, "%zu", (size_t)1) != 1) return 1; else if (strcmp(buf, "1")) return 2; ; return 0; } _ACEOF rm -f conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { ac_try='./conftest$ac_exeext' { (case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_try") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); }; }; then cat >>confdefs.h <<\_ACEOF #define MODZ "z" _ACEOF { echo "$as_me:$LINENO: result: yes" >&5 echo "${ECHO_T}yes" >&6; } else echo "$as_me: program exited with status $ac_status" >&5 echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ( exit $ac_status ) cat >>confdefs.h <<\_ACEOF #define MODZ "" _ACEOF { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi rm -f core *.core core.conftest.* gmon.out bb.out conftest$ac_exeext conftest.$ac_objext conftest.$ac_ext fi # Starting values, may be augmented later. SUBDIRS="C" TSTDIRS="C" INSTDIR="C" # Ways of specifying the Fortran compiler, in order of precedence: # configure --enable-fortran= # F77= configure ...bash # # Ways of disabling Fortran: # configure --disable-fortran # configure --enable-fortran=no # F77=no configure ...bash # Check whether --enable-fortran was given. if test "${enable_fortran+set}" = set; then enableval=$enable_fortran; fi # Check whether --enable-fortran was given. if test "${enable_fortran+set}" = set; then enableval=$enable_fortran; fi if test "x$enable_fortran" != x -a "x$enable_fortran" != xyes ; then F77="$enable_fortran" fi if test "x$F77" = xno ; then F77= { echo "$as_me:$LINENO: WARNING: Compilation of Fortran wrappers and PGSBOX disabled" >&5 echo "$as_me: WARNING: Compilation of Fortran wrappers and PGSBOX disabled" >&2;} else if test "x$F77" = x ; then # Look for a Fortran compiler. ac_ext=f ac_compile='$F77 -c $FFLAGS conftest.$ac_ext >&5' ac_link='$F77 -o conftest$ac_exeext $FFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_f77_compiler_gnu if test -n "$ac_tool_prefix"; then for ac_prog in gfortran g77 f77 ifort xlf frt pgf77 fl32 af77 fort77 f90 \ xlf90 pgf90 epcf90 f95 fort xlf95 lf95 g95 do # Extract the first word of "$ac_tool_prefix$ac_prog", so it can be a program name with args. set dummy $ac_tool_prefix$ac_prog; ac_word=$2 { echo "$as_me:$LINENO: checking for $ac_word" >&5 echo $ECHO_N "checking for $ac_word... $ECHO_C" >&6; } if test "${ac_cv_prog_F77+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test -n "$F77"; then ac_cv_prog_F77="$F77" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if { test -f "$as_dir/$ac_word$ac_exec_ext" && $as_test_x "$as_dir/$ac_word$ac_exec_ext"; }; then ac_cv_prog_F77="$ac_tool_prefix$ac_prog" echo "$as_me:$LINENO: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi F77=$ac_cv_prog_F77 if test -n "$F77"; then { echo "$as_me:$LINENO: result: $F77" >&5 echo "${ECHO_T}$F77" >&6; } else { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi test -n "$F77" && break done fi if test -z "$F77"; then ac_ct_F77=$F77 for ac_prog in gfortran g77 f77 ifort xlf frt pgf77 fl32 af77 fort77 f90 \ xlf90 pgf90 epcf90 f95 fort xlf95 lf95 g95 do # Extract the first word of "$ac_prog", so it can be a program name with args. set dummy $ac_prog; ac_word=$2 { echo "$as_me:$LINENO: checking for $ac_word" >&5 echo $ECHO_N "checking for $ac_word... $ECHO_C" >&6; } if test "${ac_cv_prog_ac_ct_F77+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test -n "$ac_ct_F77"; then ac_cv_prog_ac_ct_F77="$ac_ct_F77" # Let the user override the test. else as_save_IFS=$IFS; IFS=$PATH_SEPARATOR for as_dir in $PATH do IFS=$as_save_IFS test -z "$as_dir" && as_dir=. for ac_exec_ext in '' $ac_executable_extensions; do if { test -f "$as_dir/$ac_word$ac_exec_ext" && $as_test_x "$as_dir/$ac_word$ac_exec_ext"; }; then ac_cv_prog_ac_ct_F77="$ac_prog" echo "$as_me:$LINENO: found $as_dir/$ac_word$ac_exec_ext" >&5 break 2 fi done done IFS=$as_save_IFS fi fi ac_ct_F77=$ac_cv_prog_ac_ct_F77 if test -n "$ac_ct_F77"; then { echo "$as_me:$LINENO: result: $ac_ct_F77" >&5 echo "${ECHO_T}$ac_ct_F77" >&6; } else { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi test -n "$ac_ct_F77" && break done if test "x$ac_ct_F77" = x; then F77="" else case $cross_compiling:$ac_tool_warned in yes:) { echo "$as_me:$LINENO: WARNING: In the future, Autoconf will not detect cross-tools whose name does not start with the host triplet. If you think this configuration is useful to you, please write to autoconf@gnu.org." >&5 echo "$as_me: WARNING: In the future, Autoconf will not detect cross-tools whose name does not start with the host triplet. If you think this configuration is useful to you, please write to autoconf@gnu.org." >&2;} ac_tool_warned=yes ;; esac F77=$ac_ct_F77 fi fi # Provide some information about the compiler. echo "$as_me:$LINENO: checking for Fortran 77 compiler version" >&5 ac_compiler=`set X $ac_compile; echo $2` { (ac_try="$ac_compiler --version >&5" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compiler --version >&5") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } { (ac_try="$ac_compiler -v >&5" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compiler -v >&5") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } { (ac_try="$ac_compiler -V >&5" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compiler -V >&5") 2>&5 ac_status=$? echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } rm -f a.out # If we don't use `.F' as extension, the preprocessor is not run on the # input file. (Note that this only needs to work for GNU compilers.) ac_save_ext=$ac_ext ac_ext=F { echo "$as_me:$LINENO: checking whether we are using the GNU Fortran 77 compiler" >&5 echo $ECHO_N "checking whether we are using the GNU Fortran 77 compiler... $ECHO_C" >&6; } if test "${ac_cv_f77_compiler_gnu+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF program main #ifndef __GNUC__ choke me #endif end _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_f77_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_compiler_gnu=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_compiler_gnu=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_cv_f77_compiler_gnu=$ac_compiler_gnu fi { echo "$as_me:$LINENO: result: $ac_cv_f77_compiler_gnu" >&5 echo "${ECHO_T}$ac_cv_f77_compiler_gnu" >&6; } ac_ext=$ac_save_ext ac_test_FFLAGS=${FFLAGS+set} ac_save_FFLAGS=$FFLAGS FFLAGS= { echo "$as_me:$LINENO: checking whether $F77 accepts -g" >&5 echo $ECHO_N "checking whether $F77 accepts -g... $ECHO_C" >&6; } if test "${ac_cv_prog_f77_g+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else FFLAGS=-g cat >conftest.$ac_ext <<_ACEOF program main end _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_f77_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_f77_g=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_prog_f77_g=no fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_prog_f77_g" >&5 echo "${ECHO_T}$ac_cv_prog_f77_g" >&6; } if test "$ac_test_FFLAGS" = set; then FFLAGS=$ac_save_FFLAGS elif test $ac_cv_prog_f77_g = yes; then if test "x$ac_cv_f77_compiler_gnu" = xyes; then FFLAGS="-g -O2" else FFLAGS="-g" fi else if test "x$ac_cv_f77_compiler_gnu" = xyes; then FFLAGS="-O2" else FFLAGS= fi fi G77=`test $ac_compiler_gnu = yes && echo yes` ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu fi if test "x$F77" = x; then { echo "$as_me:$LINENO: WARNING: ------------------------------------------------------------------ Fortran compiler not found, will skip Fortran wrappers and PGSBOX. ------------------------------------------------------------------" >&5 echo "$as_me: WARNING: ------------------------------------------------------------------ Fortran compiler not found, will skip Fortran wrappers and PGSBOX. ------------------------------------------------------------------" >&2;} # Best guess at Fortran name mangling for use if a compiler does ever # become available. cat >>confdefs.h <<\_ACEOF #define F77_FUNC(name,NAME) name ## _ _ACEOF else if test "x$ac_cv_f77_compiler_gnu" = xyes ; then if test "x$F77" = xg77 -o "x$F77" = xf77 ; then # Not recognized by gfortran. FFLAGS="$FFLAGS -Wno-globals" fi fi { echo "$as_me:$LINENO: checking whether $F77 accepts -I" >&5 echo $ECHO_N "checking whether $F77 accepts -I... $ECHO_C" >&6; } ac_ext=f ac_compile='$F77 -c $FFLAGS conftest.$ac_ext >&5' ac_link='$F77 -o conftest$ac_exeext $FFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_f77_compiler_gnu FFLAGS_save=$FFLAGS FFLAGS=-I. cat >conftest.$ac_ext <<_ACEOF program main end _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_f77_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then FFLAGS="$FFLAGS_save -I."; { echo "$as_me:$LINENO: result: yes" >&5 echo "${ECHO_T}yes" >&6; } else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 FFLAGS="$FFLAGS_save"; { echo "$as_me:$LINENO: result: no" >&5 echo "${ECHO_T}no" >&6; } fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_ext=c ac_cpp='$CPP $CPPFLAGS' ac_compile='$CC -c $CFLAGS $CPPFLAGS conftest.$ac_ext >&5' ac_link='$CC -o conftest$ac_exeext $CFLAGS $CPPFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_c_compiler_gnu # Libraries required by the Fortran compiler itself (sets FLIBS). # Required by utilities and test programs written in C that link to # Fortran object modules such as pgsbox. ac_ext=f ac_compile='$F77 -c $FFLAGS conftest.$ac_ext >&5' ac_link='$F77 -o conftest$ac_exeext $FFLAGS $LDFLAGS conftest.$ac_ext $LIBS >&5' ac_compiler_gnu=$ac_cv_f77_compiler_gnu { echo "$as_me:$LINENO: checking how to get verbose linking output from $F77" >&5 echo $ECHO_N "checking how to get verbose linking output from $F77... $ECHO_C" >&6; } if test "${ac_cv_prog_f77_v+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else cat >conftest.$ac_ext <<_ACEOF program main end _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_f77_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_prog_f77_v= # Try some options frequently used verbose output for ac_verb in -v -verbose --verbose -V -\#\#\#; do cat >conftest.$ac_ext <<_ACEOF program main end _ACEOF # Compile and link our simple test program by passing a flag (argument # 1 to this macro) to the Fortran compiler in order to get # "verbose" output that we can then parse for the Fortran linker # flags. ac_save_FFLAGS=$FFLAGS FFLAGS="$FFLAGS $ac_verb" eval "set x $ac_link" shift echo "$as_me:$LINENO: $*" >&5 ac_f77_v_output=`eval $ac_link 5>&1 2>&1 | grep -v 'Driving:'` echo "$ac_f77_v_output" >&5 FFLAGS=$ac_save_FFLAGS rm -f -r conftest* # On HP/UX there is a line like: "LPATH is: /foo:/bar:/baz" where # /foo, /bar, and /baz are search directories for the Fortran linker. # Here, we change these into -L/foo -L/bar -L/baz (and put it first): ac_f77_v_output="`echo $ac_f77_v_output | grep 'LPATH is:' | sed 's,.*LPATH is\(: *[^ ]*\).*,\1,;s,: */, -L/,g'` $ac_f77_v_output" # FIXME: we keep getting bitten by quoted arguments; a more general fix # that detects unbalanced quotes in FLIBS should be implemented # and (ugh) tested at some point. case $ac_f77_v_output in # If we are using xlf then replace all the commas with spaces. *xlfentry*) ac_f77_v_output=`echo $ac_f77_v_output | sed 's/,/ /g'` ;; # With Intel ifc, ignore the quoted -mGLOB_options_string stuff (quoted # $LIBS confuse us, and the libraries appear later in the output anyway). *mGLOB_options_string*) ac_f77_v_output=`echo $ac_f77_v_output | sed 's/"-mGLOB[^"]*"/ /g'` ;; # Portland Group compiler has singly- or doubly-quoted -cmdline argument # Singly-quoted arguments were reported for versions 5.2-4 and 6.0-4. # Doubly-quoted arguments were reported for "PGF90/x86 Linux/x86 5.0-2". *-cmdline\ * | *-ignore\ * | *-def\ *) ac_f77_v_output=`echo $ac_f77_v_output | sed "\ s/-cmdline *'[^']*'/ /g; s/-cmdline *\"[^\"]*\"/ /g s/-ignore *'[^']*'/ /g; s/-ignore *\"[^\"]*\"/ /g s/-def *'[^']*'/ /g; s/-def *\"[^\"]*\"/ /g"` ;; # If we are using Cray Fortran then delete quotes. *cft90*) ac_f77_v_output=`echo $ac_f77_v_output | sed 's/"//g'` ;; esac # look for -l* and *.a constructs in the output for ac_arg in $ac_f77_v_output; do case $ac_arg in [\\/]*.a | ?:[\\/]*.a | -[lLRu]*) ac_cv_prog_f77_v=$ac_verb break 2 ;; esac done done if test -z "$ac_cv_prog_f77_v"; then { echo "$as_me:$LINENO: WARNING: cannot determine how to obtain linking information from $F77" >&5 echo "$as_me: WARNING: cannot determine how to obtain linking information from $F77" >&2;} fi else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 { echo "$as_me:$LINENO: WARNING: compilation failed" >&5 echo "$as_me: WARNING: compilation failed" >&2;} fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext fi { echo "$as_me:$LINENO: result: $ac_cv_prog_f77_v" >&5 echo "${ECHO_T}$ac_cv_prog_f77_v" >&6; } { echo "$as_me:$LINENO: checking for Fortran 77 libraries of $F77" >&5 echo $ECHO_N "checking for Fortran 77 libraries of $F77... $ECHO_C" >&6; } if test "${ac_cv_f77_libs+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else if test "x$FLIBS" != "x"; then ac_cv_f77_libs="$FLIBS" # Let the user override the test. else cat >conftest.$ac_ext <<_ACEOF program main end _ACEOF # Compile and link our simple test program by passing a flag (argument # 1 to this macro) to the Fortran compiler in order to get # "verbose" output that we can then parse for the Fortran linker # flags. ac_save_FFLAGS=$FFLAGS FFLAGS="$FFLAGS $ac_cv_prog_f77_v" eval "set x $ac_link" shift echo "$as_me:$LINENO: $*" >&5 ac_f77_v_output=`eval $ac_link 5>&1 2>&1 | grep -v 'Driving:'` echo "$ac_f77_v_output" >&5 FFLAGS=$ac_save_FFLAGS rm -f -r conftest* # On HP/UX there is a line like: "LPATH is: /foo:/bar:/baz" where # /foo, /bar, and /baz are search directories for the Fortran linker. # Here, we change these into -L/foo -L/bar -L/baz (and put it first): ac_f77_v_output="`echo $ac_f77_v_output | grep 'LPATH is:' | sed 's,.*LPATH is\(: *[^ ]*\).*,\1,;s,: */, -L/,g'` $ac_f77_v_output" # FIXME: we keep getting bitten by quoted arguments; a more general fix # that detects unbalanced quotes in FLIBS should be implemented # and (ugh) tested at some point. case $ac_f77_v_output in # If we are using xlf then replace all the commas with spaces. *xlfentry*) ac_f77_v_output=`echo $ac_f77_v_output | sed 's/,/ /g'` ;; 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grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_sys_largefile_source=1; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext ac_cv_sys_largefile_source=unknown break done fi { echo "$as_me:$LINENO: result: $ac_cv_sys_largefile_source" >&5 echo "${ECHO_T}$ac_cv_sys_largefile_source" >&6; } case $ac_cv_sys_largefile_source in #( no | unknown) ;; *) cat >>confdefs.h <<_ACEOF #define _LARGEFILE_SOURCE $ac_cv_sys_largefile_source _ACEOF ;; esac rm -f -r conftest* # We used to try defining _XOPEN_SOURCE=500 too, to work around a bug # in glibc 2.1.3, but that breaks too many other things. # If you want fseeko and ftello with glibc, upgrade to a fixed glibc. if test $ac_cv_sys_largefile_source != unknown; then cat >>confdefs.h <<\_ACEOF #define HAVE_FSEEKO 1 _ACEOF fi # Check whether --enable-largefile was given. if test "${enable_largefile+set}" = set; then enableval=$enable_largefile; fi if test "$enable_largefile" != no; then { echo "$as_me:$LINENO: checking for special C compiler options needed for large files" >&5 echo $ECHO_N "checking for special C compiler options needed for large files... $ECHO_C" >&6; } if test "${ac_cv_sys_largefile_CC+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_cv_sys_largefile_CC=no if test "$GCC" != yes; then ac_save_CC=$CC while :; do # IRIX 6.2 and later do not support large files by default, # so use the C compiler's -n32 option if that helps. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext CC="$CC -n32" rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_sys_largefile_CC=' -n32'; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext break done CC=$ac_save_CC rm -f conftest.$ac_ext fi fi { echo "$as_me:$LINENO: result: $ac_cv_sys_largefile_CC" >&5 echo "${ECHO_T}$ac_cv_sys_largefile_CC" >&6; } if test "$ac_cv_sys_largefile_CC" != no; then CC=$CC$ac_cv_sys_largefile_CC fi { echo "$as_me:$LINENO: checking for _FILE_OFFSET_BITS value needed for large files" >&5 echo $ECHO_N "checking for _FILE_OFFSET_BITS value needed for large files... $ECHO_C" >&6; } if test "${ac_cv_sys_file_offset_bits+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_sys_file_offset_bits=no; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #define _FILE_OFFSET_BITS 64 #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_sys_file_offset_bits=64; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_cv_sys_file_offset_bits=unknown break done fi { echo "$as_me:$LINENO: result: $ac_cv_sys_file_offset_bits" >&5 echo "${ECHO_T}$ac_cv_sys_file_offset_bits" >&6; } case $ac_cv_sys_file_offset_bits in #( no | unknown) ;; *) cat >>confdefs.h <<_ACEOF #define _FILE_OFFSET_BITS $ac_cv_sys_file_offset_bits _ACEOF ;; esac rm -f -r conftest* if test $ac_cv_sys_file_offset_bits = unknown; then { echo "$as_me:$LINENO: checking for _LARGE_FILES value needed for large files" >&5 echo $ECHO_N "checking for _LARGE_FILES value needed for large files... $ECHO_C" >&6; } if test "${ac_cv_sys_large_files+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else while :; do cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_sys_large_files=no; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #define _LARGE_FILES 1 #include /* Check that off_t can represent 2**63 - 1 correctly. We can't simply define LARGE_OFF_T to be 9223372036854775807, since some C++ compilers masquerading as C compilers incorrectly reject 9223372036854775807. */ #define LARGE_OFF_T (((off_t) 1 << 62) - 1 + ((off_t) 1 << 62)) int off_t_is_large[(LARGE_OFF_T % 2147483629 == 721 && LARGE_OFF_T % 2147483647 == 1) ? 1 : -1]; #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { ; return 0; } _ACEOF rm -f conftest.$ac_objext if { (ac_try="$ac_compile" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_compile") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest.$ac_objext; then ac_cv_sys_large_files=1; break else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 fi rm -f core conftest.err conftest.$ac_objext conftest.$ac_ext ac_cv_sys_large_files=unknown break done fi { echo "$as_me:$LINENO: result: $ac_cv_sys_large_files" >&5 echo "${ECHO_T}$ac_cv_sys_large_files" >&6; } case $ac_cv_sys_large_files in #( no | unknown) ;; *) cat >>confdefs.h <<_ACEOF #define _LARGE_FILES $ac_cv_sys_large_files _ACEOF ;; esac rm -f -r conftest* fi fi # Extra places to look for third-party libraries and header files. LIBDIRS= # Check whether --with-cfitsio was given. if test "${with_cfitsio+set}" = set; then withval=$with_cfitsio; fi if test "x$with_cfitsio" = xno ; then { echo "$as_me:$LINENO: WARNING: CFITSIO disabled" >&5 echo "$as_me: WARNING: CFITSIO disabled" >&2;} else # Check whether --with-cfitsiolib was given. if test "${with_cfitsiolib+set}" = set; then withval=$with_cfitsiolib; fi if test "x$with_cfitsiolib" != x ; then LIBDIRS="$LIBDIRS $with_cfitsiolib" fi # Check whether --with-cfitsioinc was given. if test "${with_cfitsioinc+set}" = set; then withval=$with_cfitsioinc; fi if test "x$with_cfitsioinc" != x ; then CFITSIO_INCDIRS="$with_cfitsioinc" fi CFITSIO_INCDIRS="$CFITSIO_INCDIRS \ /usr/local/cfitsio/include \ /local/cfitsio/include" LIBDIRS="$LIBDIRS \ /usr/local/cfitsio/lib \ /local/cfitsio/lib" fi # Check whether --with-pgplot was given. if test "${with_pgplot+set}" = set; then withval=$with_pgplot; fi if test "x$with_pgplot" = xno ; then { echo "$as_me:$LINENO: WARNING: PGPLOT disabled" >&5 echo "$as_me: WARNING: PGPLOT disabled" >&2;} else # Check whether --with-pgplotlib was given. if test "${with_pgplotlib+set}" = set; then withval=$with_pgplotlib; fi if test "x$with_pgplotlib" != x ; then LIBDIRS="$LIBDIRS $with_pgplotlib" fi # Check whether --with-pgplotinc was given. if test "${with_pgplotinc+set}" = set; then withval=$with_pgplotinc; fi if test "x$with_pgplotinc" != x ; then PGPLOT_INCDIRS="$with_pgplotinc" fi PGPLOT_INCDIRS="$PGPLOT_INCDIRS \ /usr/local/pgplot/include \ /local/pgplot/include" LIBDIRS="$LIBDIRS \ /usr/local/pgplot/lib \ /local/pgplot/lib" fi if test "x$with_cfitsio" != xno -o \ "x$with_pgplot" != xno ; then LIBDIRS="$LIBDIRS \ /usr/local/lib \ /local/lib \ /opt/local/lib \ /opt/SUNWspro/lib \ /sw/lib" for LIBDIR in $LIBDIRS ; do as_ac_File=`echo "ac_cv_file_$LIBDIR" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $LIBDIR" >&5 echo $ECHO_N "checking for $LIBDIR... $ECHO_C" >&6; } if { as_var=$as_ac_File; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else test "$cross_compiling" = yes && { { echo "$as_me:$LINENO: error: cannot check for file existence when cross compiling" >&5 echo "$as_me: error: cannot check for file existence when cross compiling" >&2;} { (exit 1); exit 1; }; } if test -r "$LIBDIR"; then eval "$as_ac_File=yes" else eval "$as_ac_File=no" fi fi ac_res=`eval echo '${'$as_ac_File'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_File'}'` = yes; then LDFLAGS="$LDFLAGS -L$LIBDIR" else continue fi done # Generic include directories. INCDIRS="/usr/local/include \ /local/include \ /opt/local/include \ /sw/include \ /local \ /usr/include" # CFITSIO. if test "x$with_cfitsio" != xno ; then # Search for CFITSIO. for INCDIR in $CFITSIO_INCDIRS $INCDIRS ; do as_ac_File=`echo "ac_cv_file_$INCDIR/cfitsio/fitsio.h" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $INCDIR/cfitsio/fitsio.h" >&5 echo $ECHO_N "checking for $INCDIR/cfitsio/fitsio.h... $ECHO_C" >&6; } if { as_var=$as_ac_File; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else test "$cross_compiling" = yes && { { echo "$as_me:$LINENO: error: cannot check for file existence when cross compiling" >&5 echo "$as_me: error: cannot check for file existence when cross compiling" >&2;} { (exit 1); exit 1; }; } if test -r "$INCDIR/cfitsio/fitsio.h"; then eval "$as_ac_File=yes" else eval "$as_ac_File=no" fi fi ac_res=`eval echo '${'$as_ac_File'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_File'}'` = yes; then CFITSIOINC="-I$INCDIR/cfitsio"; break fi as_ac_File=`echo "ac_cv_file_$INCDIR/fitsio.h" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $INCDIR/fitsio.h" >&5 echo $ECHO_N "checking for $INCDIR/fitsio.h... $ECHO_C" >&6; } if { as_var=$as_ac_File; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else test "$cross_compiling" = yes && { { echo "$as_me:$LINENO: error: cannot check for file existence when cross compiling" >&5 echo "$as_me: error: cannot check for file existence when cross compiling" >&2;} { (exit 1); exit 1; }; } if test -r "$INCDIR/fitsio.h"; then eval "$as_ac_File=yes" else eval "$as_ac_File=no" fi fi ac_res=`eval echo '${'$as_ac_File'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_File'}'` = yes; then CFITSIOINC="-I$INCDIR"; break fi done { echo "$as_me:$LINENO: checking for recv in -lsocket" >&5 echo $ECHO_N "checking for recv in -lsocket... $ECHO_C" >&6; } if test "${ac_cv_lib_socket_recv+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lsocket $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char recv (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return recv (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_socket_recv=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_socket_recv=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_socket_recv" >&5 echo "${ECHO_T}$ac_cv_lib_socket_recv" >&6; } if test $ac_cv_lib_socket_recv = yes; then CFITSIOLIB="-lsocket" fi { echo "$as_me:$LINENO: checking for ffopen in -lcfitsio" >&5 echo $ECHO_N "checking for ffopen in -lcfitsio... $ECHO_C" >&6; } if test "${ac_cv_lib_cfitsio_ffopen+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lcfitsio $CFITSIOLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char ffopen (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return ffopen (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_cfitsio_ffopen=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_cfitsio_ffopen=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_cfitsio_ffopen" >&5 echo "${ECHO_T}$ac_cv_lib_cfitsio_ffopen" >&6; } if test $ac_cv_lib_cfitsio_ffopen = yes; then CFITSIOLIB="-lcfitsio $CFITSIOLIB" fi if test "x$CFITSIOINC" = x -o "x$CFITSIOLIB" = x; then { echo "$as_me:$LINENO: WARNING: CFITSIO not found, skipping CFITSIO-dependent tests." >&5 echo "$as_me: WARNING: CFITSIO not found, skipping CFITSIO-dependent tests." >&2;} else { echo "$as_me:$LINENO: CFITSIO appears to be available." >&5 echo "$as_me: CFITSIO appears to be available." >&6;} cat >>confdefs.h <<\_ACEOF #define HAVE_CFITSIO 1 _ACEOF # Check for fits_read_wcstab, present in CFITSIO 3.004beta and later. { echo "$as_me:$LINENO: checking for fits_read_wcstab in -lcfitsio" >&5 echo $ECHO_N "checking for fits_read_wcstab in -lcfitsio... $ECHO_C" >&6; } if test "${ac_cv_lib_cfitsio_fits_read_wcstab+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lcfitsio $CFITSIOLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char fits_read_wcstab (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return fits_read_wcstab (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_cfitsio_fits_read_wcstab=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_cfitsio_fits_read_wcstab=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_cfitsio_fits_read_wcstab" >&5 echo "${ECHO_T}$ac_cv_lib_cfitsio_fits_read_wcstab" >&6; } if test $ac_cv_lib_cfitsio_fits_read_wcstab = yes; then GETWCSTAB= else GETWCSTAB=getwcstab.o fi if test "x$GETWCSTAB" != x ; then { echo "$as_me:$LINENO: WARNING: fits_read_wcstab not found in CFITSIO, will use getwcstab.c to compile test programs." >&5 echo "$as_me: WARNING: fits_read_wcstab not found in CFITSIO, will use getwcstab.c to compile test programs." >&2;} fi fi fi # PGPLOT. if test "x$F77" != x -a "x$with_pgplot" != xno ; then # Search for PGPLOT. for INCDIR in $PGPLOT_INCDIRS $INCDIRS ; do as_ac_File=`echo "ac_cv_file_$INCDIR/pgplot/cpgplot.h" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $INCDIR/pgplot/cpgplot.h" >&5 echo $ECHO_N "checking for $INCDIR/pgplot/cpgplot.h... $ECHO_C" >&6; } if { as_var=$as_ac_File; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else test "$cross_compiling" = yes && { { echo "$as_me:$LINENO: error: cannot check for file existence when cross compiling" >&5 echo "$as_me: error: cannot check for file existence when cross compiling" >&2;} { (exit 1); exit 1; }; } if test -r "$INCDIR/pgplot/cpgplot.h"; then eval "$as_ac_File=yes" else eval "$as_ac_File=no" fi fi ac_res=`eval echo '${'$as_ac_File'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_File'}'` = yes; then PGPLOTINC="-I$INCDIR/pgplot"; break fi as_ac_File=`echo "ac_cv_file_$INCDIR/cpgplot.h" | $as_tr_sh` { echo "$as_me:$LINENO: checking for $INCDIR/cpgplot.h" >&5 echo $ECHO_N "checking for $INCDIR/cpgplot.h... $ECHO_C" >&6; } if { as_var=$as_ac_File; eval "test \"\${$as_var+set}\" = set"; }; then echo $ECHO_N "(cached) $ECHO_C" >&6 else test "$cross_compiling" = yes && { { echo "$as_me:$LINENO: error: cannot check for file existence when cross compiling" >&5 echo "$as_me: error: cannot check for file existence when cross compiling" >&2;} { (exit 1); exit 1; }; } if test -r "$INCDIR/cpgplot.h"; then eval "$as_ac_File=yes" else eval "$as_ac_File=no" fi fi ac_res=`eval echo '${'$as_ac_File'}'` { echo "$as_me:$LINENO: result: $ac_res" >&5 echo "${ECHO_T}$ac_res" >&6; } if test `eval echo '${'$as_ac_File'}'` = yes; then PGPLOTINC="-I$INCDIR"; break fi done # FLIBS (found above via AC_F77_LIBRARY_LDFLAGS) only helps if PGPLOT was # built using the same Fortran compiler that we are using here. # PGPLOT compiled by the SUN Fortran compiler but linked with something # else. { echo "$as_me:$LINENO: checking for iand_ in -lM77" >&5 echo $ECHO_N "checking for iand_ in -lM77... $ECHO_C" >&6; } if test "${ac_cv_lib_M77_iand_+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lM77 $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char iand_ (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return iand_ (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_M77_iand_=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_M77_iand_=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_M77_iand_" >&5 echo "${ECHO_T}$ac_cv_lib_M77_iand_" >&6; } if test $ac_cv_lib_M77_iand_ = yes; then PGPLOTLIB="-lM77 $PGPLOTLIB" fi { echo "$as_me:$LINENO: checking for f77_init in -lF77" >&5 echo $ECHO_N "checking for f77_init in -lF77... $ECHO_C" >&6; } if test "${ac_cv_lib_F77_f77_init+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lF77 $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char f77_init (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return f77_init (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_F77_f77_init=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_F77_f77_init=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_F77_f77_init" >&5 echo "${ECHO_T}$ac_cv_lib_F77_f77_init" >&6; } if test $ac_cv_lib_F77_f77_init = yes; then PGPLOTLIB="-lF77 $PGPLOTLIB" fi if test "x$F77" != xg77; then # For PGPLOT compiled with g77 but linked with something else. { echo "$as_me:$LINENO: checking for main in -lfrtbegin" >&5 echo $ECHO_N "checking for main in -lfrtbegin... $ECHO_C" >&6; } if test "${ac_cv_lib_frtbegin_main+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lfrtbegin $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return main (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_frtbegin_main=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_frtbegin_main=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_frtbegin_main" >&5 echo "${ECHO_T}$ac_cv_lib_frtbegin_main" >&6; } if test $ac_cv_lib_frtbegin_main = yes; then PGPLOTLIB="-lfrtbegin $PGPLOTLIB" fi { echo "$as_me:$LINENO: checking for gerror_ in -lg2c" >&5 echo $ECHO_N "checking for gerror_ in -lg2c... $ECHO_C" >&6; } if test "${ac_cv_lib_g2c_gerror_+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lg2c $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char gerror_ (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return gerror_ (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_g2c_gerror_=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_g2c_gerror_=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_g2c_gerror_" >&5 echo "${ECHO_T}$ac_cv_lib_g2c_gerror_" >&6; } if test $ac_cv_lib_g2c_gerror_ = yes; then PGPLOTLIB="-lg2c $PGPLOTLIB" fi fi if test "x$F77" != xgfortran; then # For PGPLOT compiled with gfortran but linked with something else. # Note that if gfortran itself is driving the linker it can be harmful # to add -lgfortran to the link list without also adding -lgfortranbegin. # Doing so stops gfortran from adding -lgfortranbegin which is needed to # resolve "main". { echo "$as_me:$LINENO: checking for _gfortran_abort in -lgfortran" >&5 echo $ECHO_N "checking for _gfortran_abort in -lgfortran... $ECHO_C" >&6; } if test "${ac_cv_lib_gfortran__gfortran_abort+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lgfortran $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char _gfortran_abort (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return _gfortran_abort (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_gfortran__gfortran_abort=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_gfortran__gfortran_abort=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_gfortran__gfortran_abort" >&5 echo "${ECHO_T}$ac_cv_lib_gfortran__gfortran_abort" >&6; } if test $ac_cv_lib_gfortran__gfortran_abort = yes; then PGPLOTLIB="-lgfortran $PGPLOTLIB" fi fi # Search for X11 includes and libraries. { echo "$as_me:$LINENO: checking for X" >&5 echo $ECHO_N "checking for X... $ECHO_C" >&6; } # Check whether --with-x was given. if test "${with_x+set}" = set; then withval=$with_x; fi # $have_x is `yes', `no', `disabled', or empty when we do not yet know. if test "x$with_x" = xno; then # The user explicitly disabled X. have_x=disabled else case $x_includes,$x_libraries in #( *\'*) { { echo "$as_me:$LINENO: error: Cannot use X directory names containing '" >&5 echo "$as_me: error: Cannot use X directory names containing '" >&2;} { (exit 1); exit 1; }; };; #( *,NONE | NONE,*) if test "${ac_cv_have_x+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else # One or both of the vars are not set, and there is no cached value. ac_x_includes=no ac_x_libraries=no rm -f -r conftest.dir if mkdir conftest.dir; then cd conftest.dir cat >Imakefile <<'_ACEOF' incroot: @echo incroot='${INCROOT}' usrlibdir: @echo usrlibdir='${USRLIBDIR}' libdir: @echo libdir='${LIBDIR}' _ACEOF if (export CC; ${XMKMF-xmkmf}) >/dev/null 2>/dev/null && test -f Makefile; then # GNU make sometimes prints "make[1]: Entering...", which would confuse us. for ac_var in incroot usrlibdir libdir; do eval "ac_im_$ac_var=\`\${MAKE-make} $ac_var 2>/dev/null | sed -n 's/^$ac_var=//p'\`" done # Open Windows xmkmf reportedly sets LIBDIR instead of USRLIBDIR. for ac_extension in a so sl dylib la dll; do if test ! -f "$ac_im_usrlibdir/libX11.$ac_extension" && test -f "$ac_im_libdir/libX11.$ac_extension"; then ac_im_usrlibdir=$ac_im_libdir; break fi done # Screen out bogus values from the imake configuration. They are # bogus both because they are the default anyway, and because # using them would break gcc on systems where it needs fixed includes. case $ac_im_incroot in /usr/include) ac_x_includes= ;; *) test -f "$ac_im_incroot/X11/Xos.h" && ac_x_includes=$ac_im_incroot;; esac case $ac_im_usrlibdir in /usr/lib | /lib) ;; *) test -d "$ac_im_usrlibdir" && ac_x_libraries=$ac_im_usrlibdir ;; esac fi cd .. rm -f -r conftest.dir fi # Standard set of common directories for X headers. # Check X11 before X11Rn because it is often a symlink to the current release. ac_x_header_dirs=' /usr/X11/include /usr/X11R6/include /usr/X11R5/include /usr/X11R4/include /usr/include/X11 /usr/include/X11R6 /usr/include/X11R5 /usr/include/X11R4 /usr/local/X11/include /usr/local/X11R6/include /usr/local/X11R5/include /usr/local/X11R4/include /usr/local/include/X11 /usr/local/include/X11R6 /usr/local/include/X11R5 /usr/local/include/X11R4 /usr/X386/include /usr/x386/include /usr/XFree86/include/X11 /usr/include /usr/local/include /usr/unsupported/include /usr/athena/include /usr/local/x11r5/include /usr/lpp/Xamples/include /usr/openwin/include /usr/openwin/share/include' if test "$ac_x_includes" = no; then # Guess where to find include files, by looking for Xlib.h. # First, try using that file with no special directory specified. cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include _ACEOF if { (ac_try="$ac_cpp conftest.$ac_ext" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_cpp conftest.$ac_ext") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } >/dev/null && { test -z "$ac_c_preproc_warn_flag$ac_c_werror_flag" || test ! -s conftest.err }; then # We can compile using X headers with no special include directory. ac_x_includes= else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 for ac_dir in $ac_x_header_dirs; do if test -r "$ac_dir/X11/Xlib.h"; then ac_x_includes=$ac_dir break fi done fi rm -f conftest.err conftest.$ac_ext fi # $ac_x_includes = no if test "$ac_x_libraries" = no; then # Check for the libraries. # See if we find them without any special options. # Don't add to $LIBS permanently. ac_save_LIBS=$LIBS LIBS="-lX11 $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ #include #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { XrmInitialize () ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then LIBS=$ac_save_LIBS # We can link X programs with no special library path. ac_x_libraries= else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 LIBS=$ac_save_LIBS for ac_dir in `echo "$ac_x_includes $ac_x_header_dirs" | sed s/include/lib/g` do # Don't even attempt the hair of trying to link an X program! for ac_extension in a so sl dylib la dll; do if test -r "$ac_dir/libX11.$ac_extension"; then ac_x_libraries=$ac_dir break 2 fi done done fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext fi # $ac_x_libraries = no case $ac_x_includes,$ac_x_libraries in #( no,* | *,no | *\'*) # Didn't find X, or a directory has "'" in its name. ac_cv_have_x="have_x=no";; #( *) # Record where we found X for the cache. ac_cv_have_x="have_x=yes\ ac_x_includes='$ac_x_includes'\ ac_x_libraries='$ac_x_libraries'" esac fi ;; #( *) have_x=yes;; esac eval "$ac_cv_have_x" fi # $with_x != no if test "$have_x" != yes; then { echo "$as_me:$LINENO: result: $have_x" >&5 echo "${ECHO_T}$have_x" >&6; } no_x=yes else # If each of the values was on the command line, it overrides each guess. test "x$x_includes" = xNONE && x_includes=$ac_x_includes test "x$x_libraries" = xNONE && x_libraries=$ac_x_libraries # Update the cache value to reflect the command line values. ac_cv_have_x="have_x=yes\ ac_x_includes='$x_includes'\ ac_x_libraries='$x_libraries'" { echo "$as_me:$LINENO: result: libraries $x_libraries, headers $x_includes" >&5 echo "${ECHO_T}libraries $x_libraries, headers $x_includes" >&6; } fi if test "x$no_x" = x; then if test "x$ac_x_libraries" != x ; then # Not needed for systems that keep the X11 libraries in /usr/lib. LDFLAGS="$LDFLAGS -L$ac_x_libraries" fi PGPLOTLIB="-lX11 $PGPLOTLIB" fi # It is possible that other libraries may be required depending on what # graphics drivers were installed with PGPLOT. { echo "$as_me:$LINENO: checking for deflate in -lz" >&5 echo $ECHO_N "checking for deflate in -lz... $ECHO_C" >&6; } if test "${ac_cv_lib_z_deflate+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lz $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char deflate (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return deflate (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_z_deflate=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_z_deflate=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_z_deflate" >&5 echo "${ECHO_T}$ac_cv_lib_z_deflate" >&6; } if test $ac_cv_lib_z_deflate = yes; then PGPLOTLIB="-lz $PGPLOTLIB" fi { echo "$as_me:$LINENO: checking for png_error in -lpng" >&5 echo $ECHO_N "checking for png_error in -lpng... $ECHO_C" >&6; } if test "${ac_cv_lib_png_png_error+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lpng $PGPLOTLIB $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. Use char because int might match the return type of a GCC builtin and then its argument prototype would still apply. */ #ifdef __cplusplus extern "C" #endif char png_error (); #ifdef F77_DUMMY_MAIN # ifdef __cplusplus extern "C" # endif int F77_DUMMY_MAIN() { return 1; } #endif int main () { return png_error (); ; return 0; } _ACEOF rm -f conftest.$ac_objext conftest$ac_exeext if { (ac_try="$ac_link" case "(($ac_try" in *\"* | *\`* | *\\*) ac_try_echo=\$ac_try;; *) ac_try_echo=$ac_try;; esac eval "echo \"\$as_me:$LINENO: $ac_try_echo\"") >&5 (eval "$ac_link") 2>conftest.er1 ac_status=$? grep -v '^ *+' conftest.er1 >conftest.err rm -f conftest.er1 cat conftest.err >&5 echo "$as_me:$LINENO: \$? = $ac_status" >&5 (exit $ac_status); } && { test -z "$ac_c_werror_flag" || test ! -s conftest.err } && test -s conftest$ac_exeext && $as_test_x conftest$ac_exeext; then ac_cv_lib_png_png_error=yes else echo "$as_me: failed program was:" >&5 sed 's/^/| /' conftest.$ac_ext >&5 ac_cv_lib_png_png_error=no fi rm -f core conftest.err conftest.$ac_objext conftest_ipa8_conftest.oo \ conftest$ac_exeext conftest.$ac_ext LIBS=$ac_check_lib_save_LIBS fi { echo "$as_me:$LINENO: result: $ac_cv_lib_png_png_error" >&5 echo "${ECHO_T}$ac_cv_lib_png_png_error" >&6; } if test $ac_cv_lib_png_png_error = yes; then PGPLOTLIB="-lpng $PGPLOTLIB" fi { echo "$as_me:$LINENO: checking for pgbeg_ in -lpgplot" >&5 echo $ECHO_N "checking for pgbeg_ in -lpgplot... $ECHO_C" >&6; } if test "${ac_cv_lib_pgplot_pgbeg_+set}" = set; then echo $ECHO_N "(cached) $ECHO_C" >&6 else ac_check_lib_save_LIBS=$LIBS LIBS="-lpgplot $PGPLOTLIB $FLIBS $LIBS $LIBS" cat >conftest.$ac_ext <<_ACEOF /* confdefs.h. */ _ACEOF cat confdefs.h >>conftest.$ac_ext cat >>conftest.$ac_ext <<_ACEOF /* end confdefs.h. */ /* Override any GCC internal prototype to avoid an error. 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AC_PROG_LN_S AC_PROG_INSTALL AC_MSG_NOTICE([End of primary configuration. ]) # The following are required to build utilities and test programs. # ---------------------------------------------------------------- AC_MSG_NOTICE([Looking for libraries etc. for utilities and test suite...]) # Check for other quasi-standard header files. AC_CHECK_HEADERS([unistd.h]) # Large file support. AC_FUNC_FSEEKO AC_SYS_LARGEFILE # Extra places to look for third-party libraries and header files. LIBDIRS= AC_ARG_WITH([cfitsio], [AS_HELP_STRING([--without-cfitsio], [eschew CFITSIO])], []) if test "x$with_cfitsio" = xno ; then AC_MSG_WARN([CFITSIO disabled]) else AC_ARG_WITH([cfitsiolib], [AS_HELP_STRING([--with-cfitsiolib=DIR], [directory containing cfitsio library])], []) if test "x$with_cfitsiolib" != x ; then LIBDIRS="$LIBDIRS $with_cfitsiolib" fi AC_ARG_WITH([cfitsioinc], [AS_HELP_STRING([--with-cfitsioinc=DIR], [directory containing cfitsio header files])], []) if test "x$with_cfitsioinc" != x ; then CFITSIO_INCDIRS="$with_cfitsioinc" fi CFITSIO_INCDIRS="$CFITSIO_INCDIRS \ /usr/local/cfitsio/include \ /local/cfitsio/include" LIBDIRS="$LIBDIRS \ /usr/local/cfitsio/lib \ /local/cfitsio/lib" fi AC_ARG_WITH([pgplot], [AS_HELP_STRING([--without-pgplot], [eschew PGPLOT])], []) if test "x$with_pgplot" = xno ; then AC_MSG_WARN([PGPLOT disabled]) else AC_ARG_WITH([pgplotlib], [AS_HELP_STRING([--with-pgplotlib=DIR], [directory containing pgplot library])], []) if test "x$with_pgplotlib" != x ; then LIBDIRS="$LIBDIRS $with_pgplotlib" fi AC_ARG_WITH([pgplotinc], [AS_HELP_STRING([--with-pgplotinc=DIR], [directory containing pgplot header files])], []) if test "x$with_pgplotinc" != x ; then PGPLOT_INCDIRS="$with_pgplotinc" fi PGPLOT_INCDIRS="$PGPLOT_INCDIRS \ /usr/local/pgplot/include \ /local/pgplot/include" LIBDIRS="$LIBDIRS \ /usr/local/pgplot/lib \ /local/pgplot/lib" fi if test "x$with_cfitsio" != xno -o \ "x$with_pgplot" != xno ; then LIBDIRS="$LIBDIRS \ /usr/local/lib \ /local/lib \ /opt/local/lib \ /opt/SUNWspro/lib \ /sw/lib" for LIBDIR in $LIBDIRS ; do AC_CHECK_FILE([$LIBDIR], [LDFLAGS="$LDFLAGS -L$LIBDIR"], [continue]) done # Generic include directories. INCDIRS="/usr/local/include \ /local/include \ /opt/local/include \ /sw/include \ /local \ /usr/include" # CFITSIO. if test "x$with_cfitsio" != xno ; then # Search for CFITSIO. for INCDIR in $CFITSIO_INCDIRS $INCDIRS ; do AC_CHECK_FILE([$INCDIR/cfitsio/fitsio.h], [CFITSIOINC="-I$INCDIR/cfitsio"; break]) AC_CHECK_FILE([$INCDIR/fitsio.h], [CFITSIOINC="-I$INCDIR"; break]) done AC_CHECK_LIB([socket], [recv], [CFITSIOLIB="-lsocket"], [], [$LIBS]) AC_CHECK_LIB([cfitsio], [ffopen], [CFITSIOLIB="-lcfitsio $CFITSIOLIB"], [], [$CFITSIOLIB $LIBS]) if test "x$CFITSIOINC" = x -o "x$CFITSIOLIB" = x; then AC_MSG_WARN([CFITSIO not found, skipping CFITSIO-dependent tests.]) else AC_MSG_NOTICE([CFITSIO appears to be available.]) AC_DEFINE([HAVE_CFITSIO], [1], [Define to 1 if CFITSIO is available.]) # Check for fits_read_wcstab, present in CFITSIO 3.004beta and later. AC_CHECK_LIB([cfitsio], [fits_read_wcstab], [GETWCSTAB=], [GETWCSTAB=getwcstab.o], [$CFITSIOLIB $LIBS]) if test "x$GETWCSTAB" != x ; then AC_MSG_WARN([fits_read_wcstab not found in CFITSIO, will use getwcstab.c to compile test programs.]) fi fi fi # PGPLOT. if test "x$F77" != x -a "x$with_pgplot" != xno ; then # Search for PGPLOT. for INCDIR in $PGPLOT_INCDIRS $INCDIRS ; do AC_CHECK_FILE([$INCDIR/pgplot/cpgplot.h], [PGPLOTINC="-I$INCDIR/pgplot"; break]) AC_CHECK_FILE([$INCDIR/cpgplot.h], [PGPLOTINC="-I$INCDIR"; break]) done # FLIBS (found above via AC_F77_LIBRARY_LDFLAGS) only helps if PGPLOT was # built using the same Fortran compiler that we are using here. # PGPLOT compiled by the SUN Fortran compiler but linked with something # else. AC_CHECK_LIB([M77], [iand_], [PGPLOTLIB="-lM77 $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) AC_CHECK_LIB([F77], [f77_init], [PGPLOTLIB="-lF77 $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) if test "x$F77" != xg77; then # For PGPLOT compiled with g77 but linked with something else. AC_CHECK_LIB([frtbegin], [main], [PGPLOTLIB="-lfrtbegin $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) AC_CHECK_LIB([g2c], [gerror_], [PGPLOTLIB="-lg2c $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) fi if test "x$F77" != xgfortran; then # For PGPLOT compiled with gfortran but linked with something else. # Note that if gfortran itself is driving the linker it can be harmful # to add -lgfortran to the link list without also adding -lgfortranbegin. # Doing so stops gfortran from adding -lgfortranbegin which is needed to # resolve "main". AC_CHECK_LIB([gfortran], [_gfortran_abort], [PGPLOTLIB="-lgfortran $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) fi # Search for X11 includes and libraries. AC_PATH_X if test "x$no_x" = x; then if test "x$ac_x_libraries" != x ; then # Not needed for systems that keep the X11 libraries in /usr/lib. LDFLAGS="$LDFLAGS -L$ac_x_libraries" fi PGPLOTLIB="-lX11 $PGPLOTLIB" fi # It is possible that other libraries may be required depending on what # graphics drivers were installed with PGPLOT. AC_CHECK_LIB([z], [deflate], [PGPLOTLIB="-lz $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) AC_CHECK_LIB([png], [png_error], [PGPLOTLIB="-lpng $PGPLOTLIB"], [], [$PGPLOTLIB $LIBS]) AC_CHECK_LIB([pgplot], [pgbeg_], [PGPLOTLIB="-lpgplot $PGPLOTLIB"], [], [$PGPLOTLIB $FLIBS $LIBS]) AC_CHECK_LIB([cpgplot], [cpgbeg], [PGPLOTLIB="-lcpgplot $PGPLOTLIB"], [PGPLOTLIB=], [$PGPLOTLIB $FLIBS $LIBS]) # Only need the PGPLOT include file to build PGSBOX. if test "x$PGPLOTINC" != x; then SUBDIRS="$SUBDIRS pgsbox" INSTDIR="pgsbox" fi # Also need the PGPLOT library to build pgtest and cpgtest. if test "x$PGPLOTLIB" = x; then AC_MSG_WARN([PGPLOT not found, skipping PGPLOT-dependent tests.]) else AC_MSG_NOTICE([PGPLOT appears to be available.]) TSTDIRS="$TSTDIRS pgsbox" fi fi fi # Utilities are compiled last since they need the libraries. # Ways of disabling them: # configure --disable-utils # configure --enable-utils=no AC_ARG_ENABLE([utils], [AS_HELP_STRING([--disable-utils], [don't build the WCS utilities])], []) if test "x$enable_utils" != xno ; then SUBDIRS="$SUBDIRS utils" INSTDIR="$INSTDIR utils" else AC_MSG_WARN([Compilation of WCS utilities disabled]) fi AC_SUBST([CFITSIOINC]) AC_SUBST([CFITSIOLIB]) AC_SUBST([GETWCSTAB]) AC_SUBST([PGPLOTINC]) AC_SUBST([PGPLOTLIB]) AC_SUBST([SUBDIRS]) AC_SUBST([TSTDIRS]) AC_SUBST([INSTDIR]) AC_MSG_NOTICE([End of auxiliary configuration. ]) # Do it. AC_MSG_NOTICE([Configuring files...]) AC_CONFIG_FILES([makedefs wcslib.pc]) AC_CONFIG_HEADERS([wcsconfig.h wcsconfig_f77.h wcsconfig_tests.h wcsconfig_utils.h]) AC_OUTPUT pywcs-1.12/wcslib/COPYING0000644001153600020070000010451312310355626017170 0ustar cslocumSTSCI\science00000000000000 GNU GENERAL PUBLIC LICENSE Version 3, 29 June 2007 Copyright (C) 2007 Free Software Foundation, Inc. Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. Preamble The GNU General Public License is a free, copyleft license for software and other kinds of works. The licenses for most software and other practical works are designed to take away your freedom to share and change the works. By contrast, the GNU General Public License is intended to guarantee your freedom to share and change all versions of a program--to make sure it remains free software for all its users. 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Copyright (C) This program is free software: you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program. If not, see . Also add information on how to contact you by electronic and paper mail. If the program does terminal interaction, make it output a short notice like this when it starts in an interactive mode: Copyright (C) This program comes with ABSOLUTELY NO WARRANTY; for details type `show w'. This is free software, and you are welcome to redistribute it under certain conditions; type `show c' for details. 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But first, please read . pywcs-1.12/wcslib/COPYING.LESSER0000644001153600020070000001672512310355626020173 0ustar cslocumSTSCI\science00000000000000 GNU LESSER GENERAL PUBLIC LICENSE Version 3, 29 June 2007 Copyright (C) 2007 Free Software Foundation, Inc. Everyone is permitted to copy and distribute verbatim copies of this license document, but changing it is not allowed. This version of the GNU Lesser General Public License incorporates the terms and conditions of version 3 of the GNU General Public License, supplemented by the additional permissions listed below. 0. Additional Definitions. As used herein, "this License" refers to version 3 of the GNU Lesser General Public License, and the "GNU GPL" refers to version 3 of the GNU General Public License. "The Library" refers to a covered work governed by this License, other than an Application or a Combined Work as defined below. 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If the Library as you received it specifies that a proxy can decide whether future versions of the GNU Lesser General Public License shall apply, that proxy's public statement of acceptance of any version is permanent authorization for you to choose that version for the Library. pywcs-1.12/wcslib/doxygen/0000755001153600020070000000000012310355732017604 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/doxygen/Bonne.gif0000644001153600020070000002221412310355626021337 0ustar cslocumSTSCI\science00000000000000GIF87a ëòÿÿÿÿÿffÿÿff3™3, ëþºÜþ0ÊI«½8ëÍ»ÿ`(Ždižhª®lë¾p,Ïtmßx®ï|ïÿÀ ¢@,„È™±˜,-‡Œ‚€Ø¬:‰‚èÐhÝ Ž##Ëìš5åìBÜ °Ï*ÜxÔ[¸>n¿¯`r{kotZ xyƒ{‚j} tp}†ˆ šš‹Id–He–o››Q“žAD ¡o¶·¶[¥>G¥¤™š ‰ªP°I » d·m˶½Mb¾ ­˜‡ÄƱÉÍ€c¢B³ÙàÜÃoÊÚ3èÜŹ£Zбä¾Áå×— ïí9dá“Ç,‚!6S~Aß>~»´Á†Õ®yG†-88þ†] 1 ã!Q‰eT¬æ0Ü%súq›ПÌs—èÄ‚ÍæÔ,ViÑWšN˜1÷JˆÃÎ,¡[H>2ÍÁS 0VBFN°I’ª=k*2ÞS6a#étkP±u* ÏO£@p—Q´Z,™´%uñ­ëÖ„SWvl‘«‹GÞ¼H[@z à/öXMÙK‰qÞ4é°0% 3©êts¹F›;;ù,¨ž§ ¹ùœ;kjt»ì–÷P+aÙLÛ©%²m—qQª2…áĹR­yr§¯>pþ¾HŽsÌÎt@È?,>Aq’éÅNXæÇ‘•H#¬ÐO¥ú‘ìóØÙHAŠ%Š£¨Ù—¸ ! 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Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: doxextr.l,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * * doxextr.l is a Flex description file containing a lexical scanner definition * used to extract comments from the prologue of WCSLIB header files and * produce mark-up for doxygen. It relies on strict formatting of comments * in the header file. * * Header sections are: * - SUMMARY: Introduced by '* Summary of the {NAME} ' * where {NAME} is the name of the header file without .h suffix. * * - FUNCTION: Introduced by '* {NAME}() - ' * where {NAME} is the name of the function. * * - STRUCTURE: Introduced by '* {NAME} struct - ' or '* {NAME} union - ' * where {NAME} is the name of the struct or union. * * - DEFINE: Introduced by '* {NAME} define - ' or '* {NAME}() macro - ' * where {NAME} is the name of the preprocessor definition. * * - VARIABLE: Introduced by '* Global variable: {NAME} - ' * where {NAME} is the name of a global variable. * * It requires Flex v2.5.4 or later. * *===========================================================================*/ /* Options. */ /* %option full */ %option never-interactive %option nounput %option noyywrap %option outfile="doxextr.c" %option prefix="doxextr" /* Indentation levels. */ I " " IT {I}{5} ID {I}{10} /* Patterns. */ NAME [a-zA-Z_][a-zA-Z_0-9]* /* Optional whitespace. */ WS0 " "* /* Required whitespace. */ WS1 " "+ /* Sequence of non-whitespace characters. */ NWS [^ ]+ /* Hyphen. */ DASH {WS1}-{WS1} /* Exclusive start states. */ %x PROLOG BODY %x DEFINE FUNCTION STRUCTURE SUMMARY VARIABLE %x DEFMARK FILEMARK FNMARK STRUCTMARK UNIONMARK VARMARK %x BRIEF NOTES PARAM RETURN STRUCTVAR TABLEROW %x FLUSH PRINTE PRINTF %{ #include #include #include #define TABLE 1 #define VERBATIM 2 %} %% const int id = 24; char *(func[128]), listype[8], *(proto[128]), name[32], *param, text[128]; int ifunc, ilist, indent, listndt[8], lmore, nfunc, pass1, pcont, plist, section, special, subsection, td; void listitem(int indent, char listype[8], int listndt[8], int *ilist); void endlist(int isItem, int indent, char listype[8], int listndt[8], int *ilist); void endspecial(int *special); void printe(const char *text, const char *name); ilist = 0; listndt[0] = -1; listype[0] = '-'; lmore = 0; *name = '\0'; nfunc = 0; pass1 = 1; pcont = 0; plist = 0; section = PROLOG; special = 0; subsection = 0; td = 0; BEGIN(PROLOG); \n {} ^\/ | ^{WS1} | ^\*=+ { /* Copyright notice. */ BEGIN(FLUSH); } <*>^\*{WS0}\n\*{WS0}\n { /* Consecutive blank lines denoting the end of a section. */ if (pass1) { BEGIN(FLUSH); } else if (section != BODY) { if (section != PROLOG) { endlist(0, 0, listype, listndt, &ilist); endspecial(&special); printf("*/\n"); section = PROLOG; } BEGIN(PROLOG); } } <*>^\*=+\*\/ { /* End of prologue. */ if (pass1) { section = BODY; BEGIN(FLUSH); } else { if (section != PROLOG) { endlist(0, 0, listype, listndt, &ilist); endspecial(&special); printf("*/\n"); } return 0; } } <*>{WS0}-+\n { /* Discard underlining. */ } <*>^\*{WS0}\n { if (!pass1) { endspecial(&special); lmore = yyleng; yymore(); } } <*>^\*" " { /* First-level prologue indentation. */ if (pass1) { BEGIN(FLUSH); } else { endspecial(&special); lmore = yyleng; yymore(); } } <*>^-/\n { /* Horizontal rule. */ if (!pass1) { printf("*
\n"); } BEGIN(FLUSH); } <*>^#{WS0} { /* HTML table. */ if (pass1) { BEGIN(FLUSH); } else { if (special != TABLE) { endspecial(&special); printf("*
\n"); special = TABLE; } printf("* \n"); printf("*%s", yytext+lmore+1); td = 0; BEGIN(TABLEROW); } } <*>^=/\n | <*>^=" ".* { /* Verbatim text (code). */ if (!pass1) { if (special != VERBATIM) { endspecial(&special); printf("* @code\n"); special = VERBATIM; } printf(" %s\n", yytext+lmore+1); } BEGIN(FLUSH); } "Summary of the"{WS1} | "Summary of"{WS1} { /* The next token will be the file name. */ section = SUMMARY; BEGIN(FILEMARK); } {NAME}"()"{DASH} { /* Description of a function API. */ section = FUNCTION; subsection = 0; yyless(lmore); BEGIN(FNMARK); } {NAME}{WS1}struct{DASH} { /* Description of structure members. */ section = STRUCTURE; subsection = 0; yyless(lmore); BEGIN(STRUCTMARK); } {NAME}{WS1}union{DASH} { /* Description of union members. */ section = STRUCTURE; subsection = 0; yyless(lmore); BEGIN(UNIONMARK); } Global" "variable:" ".*{DASH} { /* Description of global variable. */ section = VARIABLE; yyless(lmore+17); BEGIN(VARMARK); } {NAME}("()")*{WS1}(define|macro){DASH} { /* Description of preprocessor definition. */ section = DEFINE; yyless(lmore); BEGIN(DEFMARK); } . { BEGIN(FLUSH); } {NAME} { printf("/** @file %s.h\n*\n", yytext); BEGIN(FLUSH); } [A-Z].{1,50}: { /* Sub-section header. */ endlist(0, 0, listype, listndt, &ilist); printf("*\n* %*s @n\n", yyleng-(lmore+1), yytext+lmore); BEGIN(FLUSH); } {WS1}"- " | {WS1}/{NWS}:\[^:] { /* Unnumbered list item. */ lmore -= 2; indent = yyleng - lmore; if (yytext[yyleng-2] == '-') { /* The two-character pattern was matched. */ indent -= 2; } endlist(1, indent, listype, listndt, &ilist); if (lmore) printf("*\n"); if (indent > listndt[ilist]) { ilist++; listndt[ilist] = indent; listype[ilist] = 'U'; printf("%-*s<%cL>\n", indent, "*", listype[ilist]); } printf("%-*s
  • ", indent, "*"); BEGIN(PRINTE); } {WS1} { lmore -= 2; indent = yyleng - lmore; endlist(0, indent, listype, listndt, &ilist); yymore(); BEGIN(PRINTE); } . { endlist(0, 0, listype, listndt, &ilist); yymore(); BEGIN(PRINTE); } {NAME} { strcpy(name, yytext); for (ifunc = 0; ifunc < nfunc; ifunc++) { if (strcmp(yytext, func[ifunc]) == 0) { printf("\n/** @fn %s\n*\n", proto[ifunc]); break; } } if (ifunc == nfunc) { printf("\n/** @fn %s\n*\n", yytext); } } "()"{DASH} { BEGIN(BRIEF); } Given: { printf("*\n"); subsection = PARAM; param = "in"; BEGIN(FLUSH); } "Given and returned:" { printf("*\n"); subsection = PARAM; param = "in,out"; BEGIN(FLUSH); } Returned: { printf("*\n"); subsection = PARAM; param = "out"; BEGIN(FLUSH); } "Function return value:" { printf("*\n"); subsection = RETURN; BEGIN(FLUSH); } "Notes:" { printf("*\n* @b Notes: @n\n"); subsection = NOTES; ilist = 0; BEGIN(FLUSH); } {I} { if (!subsection || subsection == NOTES) { /* Lists in the function prologue or notes section. */ lmore = yyleng; yymore(); } if (subsection) BEGIN(subsection); } . { yymore(); BEGIN(PRINTE); } [a-zA-Z].{17}" ".* | "..."" "{7}.{8}" ".* { if (pcont) { printf("%s\n%-*s", strtok(yytext, " "), id, "*"); pcont = 0; } else { sprintf(text, "* @param[%s] %s ", param, strtok(yytext, " ")); printf("%-24s", text); } printe(yytext+20, name); plist = 0; BEGIN(FLUSH); } ({NAME},)+{WS0} { if (pcont) { printf("%s", yytext); } else { printf("* @param[%s] %s", param, yytext); pcont = 1; } plist = 0; BEGIN(FLUSH); } {NAME}(,{NAME})? { if (pcont) { pcont = 0; } else { printf("* @param[%s] ", param); } printf("%s\n", yytext); plist = 0; BEGIN(FLUSH); } {IT}[a-z].* { pcont = 0; printe(yytext+20, name); BEGIN(FLUSH); } {IT}[a-z].{6}" ".* { /* Function return type. */ printf("* @return "); printe(yytext+20, name); plist = 0; BEGIN(FLUSH); } {IT}[a-z].* { /* Function return type. */ printf("* @return\n"); plist = 0; BEGIN(FLUSH); } {ID}" "[-1].*:{WS1}.* { /* Status return value, less than 0 or greater than 9. */ if (lmore > 2) printf("* @n\n"); printf("%-*s- ", id, "*"); printe(yytext+(id-3), name); plist = 1; BEGIN(FLUSH); } {ID}" ".*:{WS1}.* { /* List of parameter or status return values. */ if (lmore > 2) printf("* @n\n"); printf("%-*s- ", id, "*"); printe(yytext+(id-2), name); plist = 1; BEGIN(FLUSH); } {ID}" ".* { /* List of parameter or status return values. */ if (lmore > 2) printf("* @n\n"); printf("* "); printe(yytext, name); BEGIN(FLUSH); } {ID}.* { /* List of parameter or status return values. */ if (plist) { printf("%-*s.\n", id, "*"); plist = 0; } else if (lmore > 2) { printf("* @n\n"); } printf("* "); printe(yytext, name); BEGIN(FLUSH); } {WS0}-" " | {WS0}[1-9a-z]:" " { /* List item. */ lmore -= 4; indent = yyleng - lmore; if (yytext[yyleng-2] == '-') { /* The two-character pattern was matched. */ indent -= 2; } else { /* The three-character pattern was matched. */ indent -= 3; } endlist(1, indent, listype, listndt, &ilist); if (lmore) printf("*\n"); listitem(indent, listype, listndt, &ilist); BEGIN(PRINTE); } {WS1} { lmore -= 4; indent = yyleng - lmore; endlist(0, indent, listype, listndt, &ilist); yymore(); BEGIN(PRINTE); } . { endlist(0, 4, listype, listndt, &ilist); yymore(); BEGIN(PRINTE); } {NAME} { strcpy(name, yytext); printf("\n/** @struct %s\n*\n", yytext); } {WS1}struct{DASH} { BEGIN(BRIEF); } {NAME} { strcpy(name, yytext); printf("\n/** @union %s\n*\n", yytext); } {WS1}union{DASH} { BEGIN(BRIEF); } {I}(char|int|long|double|struct{WS1}{NAME}|union) { endlist(0, 0, listype, listndt, &ilist); printf("*/\n"); printf("\n/** @var %s", yytext+lmore+2); BEGIN(STRUCTVAR); } {I}{I}{WS0}-" " | {I}{I}{WS0}[0-9a-z]:" " { /* Start of list. */ lmore -= 2; indent = yyleng - lmore; if (yytext[yyleng-2] == '-') { /* The two-character pattern was matched. */ indent -= 2; } else { /* The three-character pattern was matched. */ indent -= 3; } endlist(1, indent, listype, listndt, &ilist); if (lmore) printf("*\n"); listitem(indent, listype, listndt, &ilist); BEGIN(PRINTE); } {WS1} { lmore -= 2; indent = yyleng - lmore; endlist(0, indent, listype, listndt, &ilist); yymore(); BEGIN(PRINTE); } . { endlist(0, 0, listype, listndt, &ilist); yymore(); BEGIN(PRINTE); } (\*{WS1}|{WS1}\*?) { printf("%s", yytext); } {NAME}, { printf("%s::%s\n*\n* (See next ...)\n", name, yytext); BEGIN(FLUSH); } {NAME} { printf("%s::%s\n*\n", name, yytext); BEGIN(FLUSH); } "(*"{NAME}")" { printf("(*%s::%s\n*\n", name, yytext+2); BEGIN(FLUSH); } .*{DASH} { printf("\n/** @var %.*s\n*\n", yyleng-3, yytext); BEGIN(BRIEF); } . { yymore(); BEGIN(PRINTE); } {NAME} { strcpy(name, yytext); printf("\n/** @def %s\n*\n", yytext); } ("()")*{WS1}(define|macro){DASH} { BEGIN(BRIEF); } . { yymore(); BEGIN(PRINTE); } . { if (!td) { printf("
    • %s", yytext); td = 0; } \n { if (td) printf("\n"); td = 0; printf("* \n"); yyless(0); BEGIN(FLUSH); } ^(void|int|double){WS1}{NAME}{WS0}\([^)]* { proto[nfunc] = malloc((yyleng+2)*sizeof(char)); sprintf(proto[nfunc], "%s)", yytext); func[nfunc] = malloc(16*sizeof(char)); strtok(yytext, " "); strcpy(func[nfunc], strtok(0x0, " (")); nfunc++; BEGIN(FLUSH); } ^. { BEGIN(FLUSH); } \n {} .* { printf("* @brief %s.\n*\n", yytext); BEGIN(FLUSH); } .* { printe(yytext, name); BEGIN(FLUSH); } .* { printf("%s\n", yytext); BEGIN(FLUSH); } .*\n { /* Throw away the rest of the line and begin the next cycle. */ lmore = 0; BEGIN(section); } <> { if (pass1) { lmore = 0; *name = '\0'; pass1 = 0; section = PROLOG; subsection = 0; BEGIN(PROLOG); rewind(yyin); yyrestart(yyin); } else { printf("*/\n"); return 0; } } %% /*---------------------------------------------------------------------------- * Output a list item, starting a new list if necessary. *---------------------------------------------------------------------------*/ void listitem( int indent, char listype[8], int listndt[8], int *ilist) { if (indent > listndt[*ilist]) { (*ilist)++; listndt[*ilist] = indent; if (yytext[yyleng-2] == '-') { listype[*ilist] = 'U'; } else { listype[*ilist] = 'O'; } if (yytext[yyleng-3] == 'a') { printf("%-*s\n", indent, "*"); } else { printf("%-*s<%cL>\n", indent, "*", listype[*ilist]); } } printf("%-*s
  • ", indent, "*"); } /*---------------------------------------------------------------------------- * Finish any lists. *---------------------------------------------------------------------------*/ void endlist( int isItem, int indent, char listype[8], int listndt[8], int *ilist) { /* Plain text at the same level of indentation as an item tag signals */ /* end-of-list. */ while (*ilist && (indent < listndt[*ilist] || (indent == listndt[*ilist] && !isItem))) { printf("%-*s\n", listndt[*ilist], "*", listype[*ilist]); (*ilist)--; } } /*---------------------------------------------------------------------------- * Finish tables or code sections. *---------------------------------------------------------------------------*/ void endspecial( int *special) { if (*special) { if (*special == TABLE) { printf("*
    • "); td = 1; } printf("%s", yytext); } " "{2,} { printf("
    \n"); } else if (*special == VERBATIM) { printf("* @endcode\n"); } *special = 0; } } /*---------------------------------------------------------------------------- * Print text with name escaped by '%' to prevent a document reference. *---------------------------------------------------------------------------*/ void printe(const char *text, const char *name) { char *cp; int len; if ((len = strlen(name))) { while ((cp = strstr(text, name))) { if (cp > text && (*(cp-1) == '_' || ('a' <= *(cp-1) && *(cp-1) <= 'z') || ('A' <= *(cp-1) && *(cp-1) <= 'Z'))) { /* Not a match. */ printf("%.*s", cp-text+len, text); } else { if (*(cp+len) == ':' && *(cp+len+1) == ':') { // Allow references to struct members. printf("%.*s", cp-text+len, text); } else { // Disallow a reference and use bold font. printf("%.*s@b %%%s", cp-text, text, name); } } text = cp + len; } } printf("%s\n", text); } /*--------------------------------------------------------------------------*/ int main(int argc, char *argv[]) { /* Check inputs. */ if (argc != 2) { fprintf(stderr, "Usage: doxextr
    \n"); return 1; } /* Check accessibility of the input file. */ if (access(argv[1], R_OK) == -1) { perror(argv[1]); return 1; } if ((yyin = fopen(argv[1], "r")) == NULL) { perror(argv[1]); return 1; } /* Set line buffering in case stdout is redirected to a file, otherwise * stdout and stderr messages will be jumbled (stderr is unbuffered). */ setvbuf(stdout, NULL, _IOLBF, 0); return yylex(); } pywcs-1.12/wcslib/doxygen/doxextr.sed0000644001153600020070000000340312310355626022000 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|("given")|(given)|g s|("returned")|(returned)|g s|(Given)|(Given)|g s|(Given & returned)|(Given \& returned)|g s|(Returned)|(Returned)|g /^\*/s|"|\"|g # All standard. s|BITPIX|&|g s|CDELTia|CDELTia|g s|CNAMEia|CNAMEia|g s|\([^_]\)COMMENT|\1COMMENT|g s|CRDERia|CRDERia|g s|CRPIXja|CRPIXja|g s|CRVALia|CRVALia|g s|CSYERia|CSYERia|g s|CTYPEia|CTYPEia|g s|CUNITia|CUNITia|g s|DATE-AVG|&|g s|DATE-OBS|&|g s|END|&|g s|EQUINOXa|EQUINOXa|g s|EXTLEV|&|g s|EXTNAME|&|g s|EXTVER|&|g s|HISTORY|&|g s|LATPOLEa|LATPOLEa|g s|LONPOLEa|LONPOLEa|g s|MJD-AVG|&|g s|MJD-OBS|&|g s|NAXIS|&|g s|OBSGEO-[XYZ]|&|g s|RADESYSa|RADESYSa|g s|RESTFRQa|RESTFRQa|g s|RESTWAVa|RESTWAVa|g s|SIMPLE|&|g s|SPECSYSa|SPECSYSa|g s|SSYSOBSa|SSYSOBSa|g s|SSYSSRCa|SSYSSRCa|g s|TTYPEn|TTYPEn|g s|VELOSYSa|VELOSYSa|g s|WCSAXESa|WCSAXESa|g s|WCSNAMEa|WCSNAMEa|g s|VELANGLa|VELANGLa|g s|ZSOURCEa|ZSOURCEa|g s|PCi_ja|PCi_ja|g s|CDi_ja|CDi_ja|g s|PSi_ma|PSi_ma|g s|PVi_ma|PVi_ma|g s|PLEASE NOTE:|&|g # To prevent " -> " above. s||
      |g s|-||g pywcs-1.12/wcslib/doxygen/Doxyfile0000644001153600020070000014427512310355626021331 0ustar cslocumSTSCI\science00000000000000# Doxyfile 1.5.1 # This file describes the settings to be used by the documentation system # doxygen (www.doxygen.org) for a project # # All text after a hash (#) is considered a comment and will be ignored # The format is: # TAG = value [value, ...] # For lists items can also be appended using: # TAG += value [value, ...] # Values that contain spaces should be placed between quotes (" ") #--------------------------------------------------------------------------- # Project related configuration options #--------------------------------------------------------------------------- # The PROJECT_NAME tag is a single word (or a sequence of words surrounded # by quotes) that should identify the project. PROJECT_NAME = "WCSLIB 4.10" # The PROJECT_NUMBER tag can be used to enter a project or revision number. # This could be handy for archiving the generated documentation or # if some version control system is used. PROJECT_NUMBER = # The OUTPUT_DIRECTORY tag is used to specify the (relative or absolute) # base path where the generated documentation will be put. # If a relative path is entered, it will be relative to the location # where doxygen was started. If left blank the current directory will be used. OUTPUT_DIRECTORY = # If the CREATE_SUBDIRS tag is set to YES, then doxygen will create # 4096 sub-directories (in 2 levels) under the output directory of each output # format and will distribute the generated files over these directories. # Enabling this option can be useful when feeding doxygen a huge amount of # source files, where putting all generated files in the same directory would # otherwise cause performance problems for the file system. CREATE_SUBDIRS = NO # The OUTPUT_LANGUAGE tag is used to specify the language in which all # documentation generated by doxygen is written. Doxygen will use this # information to generate all constant output in the proper language. # The default language is English, other supported languages are: # Afrikaans, Arabic, Brazilian, Catalan, Chinese, Chinese-Traditional, # Croatian, Czech, Danish, Dutch, Finnish, French, German, Greek, Hungarian, # Italian, Japanese, Japanese-en (Japanese with English messages), Korean, # Korean-en, Lithuanian, Norwegian, Polish, Portuguese, Romanian, Russian, # Serbian, Slovak, Slovene, Spanish, Swedish, and Ukrainian. OUTPUT_LANGUAGE = English # This tag can be used to specify the encoding used in the generated output. # The encoding is not always determined by the language that is chosen, # but also whether or not the output is meant for Windows or non-Windows users. # In case there is a difference, setting the USE_WINDOWS_ENCODING tag to YES # forces the Windows encoding (this is the default for the Windows binary), # whereas setting the tag to NO uses a Unix-style encoding (the default for # all platforms other than Windows). USE_WINDOWS_ENCODING = NO # If the BRIEF_MEMBER_DESC tag is set to YES (the default) Doxygen will # include brief member descriptions after the members that are listed in # the file and class documentation (similar to JavaDoc). # Set to NO to disable this. BRIEF_MEMBER_DESC = YES # If the REPEAT_BRIEF tag is set to YES (the default) Doxygen will prepend # the brief description of a member or function before the detailed description. # Note: if both HIDE_UNDOC_MEMBERS and BRIEF_MEMBER_DESC are set to NO, the # brief descriptions will be completely suppressed. REPEAT_BRIEF = NO # This tag implements a quasi-intelligent brief description abbreviator # that is used to form the text in various listings. Each string # in this list, if found as the leading text of the brief description, will be # stripped from the text and the result after processing the whole list, is # used as the annotated text. Otherwise, the brief description is used as-is. # If left blank, the following values are used ("$name" is automatically # replaced with the name of the entity): "The $name class" "The $name widget" # "The $name file" "is" "provides" "specifies" "contains" # "represents" "a" "an" "the" ABBREVIATE_BRIEF = # If the ALWAYS_DETAILED_SEC and REPEAT_BRIEF tags are both set to YES then # Doxygen will generate a detailed section even if there is only a brief # description. ALWAYS_DETAILED_SEC = NO # If the INLINE_INHERITED_MEMB tag is set to YES, doxygen will show all # inherited members of a class in the documentation of that class as if those # members were ordinary class members. Constructors, destructors and assignment # operators of the base classes will not be shown. INLINE_INHERITED_MEMB = NO # If the FULL_PATH_NAMES tag is set to YES then Doxygen will prepend the full # path before files name in the file list and in the header files. If set # to NO the shortest path that makes the file name unique will be used. FULL_PATH_NAMES = NO # If the FULL_PATH_NAMES tag is set to YES then the STRIP_FROM_PATH tag # can be used to strip a user-defined part of the path. Stripping is # only done if one of the specified strings matches the left-hand part of # the path. The tag can be used to show relative paths in the file list. # If left blank the directory from which doxygen is run is used as the # path to strip. STRIP_FROM_PATH = # The STRIP_FROM_INC_PATH tag can be used to strip a user-defined part of # the path mentioned in the documentation of a class, which tells # the reader which header file to include in order to use a class. # If left blank only the name of the header file containing the class # definition is used. Otherwise one should specify the include paths that # are normally passed to the compiler using the -I flag. STRIP_FROM_INC_PATH = # If the SHORT_NAMES tag is set to YES, doxygen will generate much shorter # (but less readable) file names. This can be useful is your file systems # doesn't support long names like on DOS, Mac, or CD-ROM. SHORT_NAMES = NO # If the JAVADOC_AUTOBRIEF tag is set to YES then Doxygen # will interpret the first line (until the first dot) of a JavaDoc-style # comment as the brief description. If set to NO, the JavaDoc # comments will behave just like the Qt-style comments (thus requiring an # explicit @brief command for a brief description. JAVADOC_AUTOBRIEF = NO # The MULTILINE_CPP_IS_BRIEF tag can be set to YES to make Doxygen # treat a multi-line C++ special comment block (i.e. a block of //! or /// # comments) as a brief description. This used to be the default behaviour. # The new default is to treat a multi-line C++ comment block as a detailed # description. Set this tag to YES if you prefer the old behaviour instead. MULTILINE_CPP_IS_BRIEF = NO # If the DETAILS_AT_TOP tag is set to YES then Doxygen # will output the detailed description near the top, like JavaDoc. # If set to NO, the detailed description appears after the member # documentation. DETAILS_AT_TOP = NO # If the INHERIT_DOCS tag is set to YES (the default) then an undocumented # member inherits the documentation from any documented member that it # re-implements. INHERIT_DOCS = YES # If the SEPARATE_MEMBER_PAGES tag is set to YES, then doxygen will produce # a new page for each member. If set to NO, the documentation of a member will # be part of the file/class/namespace that contains it. SEPARATE_MEMBER_PAGES = NO # The TAB_SIZE tag can be used to set the number of spaces in a tab. # Doxygen uses this value to replace tabs by spaces in code fragments. TAB_SIZE = 8 # This tag can be used to specify a number of aliases that acts # as commands in the documentation. An alias has the form "name=value". # For example adding "sideeffect=\par Side Effects:\n" will allow you to # put the command \sideeffect (or @sideeffect) in the documentation, which # will result in a user-defined paragraph with heading "Side Effects:". # You can put \n's in the value part of an alias to insert newlines. ALIASES = # Set the OPTIMIZE_OUTPUT_FOR_C tag to YES if your project consists of C # sources only. Doxygen will then generate output that is more tailored for C. # For instance, some of the names that are used will be different. The list # of all members will be omitted, etc. OPTIMIZE_OUTPUT_FOR_C = YES # Set the OPTIMIZE_OUTPUT_JAVA tag to YES if your project consists of Java # sources only. Doxygen will then generate output that is more tailored for Java. # For instance, namespaces will be presented as packages, qualified scopes # will look different, etc. OPTIMIZE_OUTPUT_JAVA = NO # If you use STL classes (i.e. std::string, std::vector, etc.) but do not want to # include (a tag file for) the STL sources as input, then you should # set this tag to YES in order to let doxygen match functions declarations and # definitions whose arguments contain STL classes (e.g. func(std::string); v.s. # func(std::string) {}). This also make the inheritance and collaboration # diagrams that involve STL classes more complete and accurate. BUILTIN_STL_SUPPORT = NO # If member grouping is used in the documentation and the DISTRIBUTE_GROUP_DOC # tag is set to YES, then doxygen will reuse the documentation of the first # member in the group (if any) for the other members of the group. By default # all members of a group must be documented explicitly. DISTRIBUTE_GROUP_DOC = NO # Set the SUBGROUPING tag to YES (the default) to allow class member groups of # the same type (for instance a group of public functions) to be put as a # subgroup of that type (e.g. under the Public Functions section). Set it to # NO to prevent subgrouping. Alternatively, this can be done per class using # the \nosubgrouping command. SUBGROUPING = YES #--------------------------------------------------------------------------- # Build related configuration options #--------------------------------------------------------------------------- # If the EXTRACT_ALL tag is set to YES doxygen will assume all entities in # documentation are documented, even if no documentation was available. # Private class members and static file members will be hidden unless # the EXTRACT_PRIVATE and EXTRACT_STATIC tags are set to YES EXTRACT_ALL = YES # If the EXTRACT_PRIVATE tag is set to YES all private members of a class # will be included in the documentation. EXTRACT_PRIVATE = NO # If the EXTRACT_STATIC tag is set to YES all static members of a file # will be included in the documentation. EXTRACT_STATIC = NO # If the EXTRACT_LOCAL_CLASSES tag is set to YES classes (and structs) # defined locally in source files will be included in the documentation. # If set to NO only classes defined in header files are included. EXTRACT_LOCAL_CLASSES = NO # This flag is only useful for Objective-C code. When set to YES local # methods, which are defined in the implementation section but not in # the interface are included in the documentation. # If set to NO (the default) only methods in the interface are included. EXTRACT_LOCAL_METHODS = NO # If the HIDE_UNDOC_MEMBERS tag is set to YES, Doxygen will hide all # undocumented members of documented classes, files or namespaces. # If set to NO (the default) these members will be included in the # various overviews, but no documentation section is generated. # This option has no effect if EXTRACT_ALL is enabled. HIDE_UNDOC_MEMBERS = NO # If the HIDE_UNDOC_CLASSES tag is set to YES, Doxygen will hide all # undocumented classes that are normally visible in the class hierarchy. # If set to NO (the default) these classes will be included in the various # overviews. This option has no effect if EXTRACT_ALL is enabled. HIDE_UNDOC_CLASSES = NO # If the HIDE_FRIEND_COMPOUNDS tag is set to YES, Doxygen will hide all # friend (class|struct|union) declarations. # If set to NO (the default) these declarations will be included in the # documentation. HIDE_FRIEND_COMPOUNDS = NO # If the HIDE_IN_BODY_DOCS tag is set to YES, Doxygen will hide any # documentation blocks found inside the body of a function. # If set to NO (the default) these blocks will be appended to the # function's detailed documentation block. HIDE_IN_BODY_DOCS = NO # The INTERNAL_DOCS tag determines if documentation # that is typed after a \internal command is included. If the tag is set # to NO (the default) then the documentation will be excluded. # Set it to YES to include the internal documentation. INTERNAL_DOCS = NO # If the CASE_SENSE_NAMES tag is set to NO then Doxygen will only generate # file names in lower-case letters. If set to YES upper-case letters are also # allowed. This is useful if you have classes or files whose names only differ # in case and if your file system supports case sensitive file names. Windows # and Mac users are advised to set this option to NO. CASE_SENSE_NAMES = YES # If the HIDE_SCOPE_NAMES tag is set to NO (the default) then Doxygen # will show members with their full class and namespace scopes in the # documentation. If set to YES the scope will be hidden. HIDE_SCOPE_NAMES = NO # If the SHOW_INCLUDE_FILES tag is set to YES (the default) then Doxygen # will put a list of the files that are included by a file in the documentation # of that file. SHOW_INCLUDE_FILES = YES # If the INLINE_INFO tag is set to YES (the default) then a tag [inline] # is inserted in the documentation for inline members. INLINE_INFO = YES # If the SORT_MEMBER_DOCS tag is set to YES (the default) then doxygen # will sort the (detailed) documentation of file and class members # alphabetically by member name. If set to NO the members will appear in # declaration order. SORT_MEMBER_DOCS = NO # If the SORT_BRIEF_DOCS tag is set to YES then doxygen will sort the # brief documentation of file, namespace and class members alphabetically # by member name. If set to NO (the default) the members will appear in # declaration order. SORT_BRIEF_DOCS = NO # If the SORT_BY_SCOPE_NAME tag is set to YES, the class list will be # sorted by fully-qualified names, including namespaces. If set to # NO (the default), the class list will be sorted only by class name, # not including the namespace part. # Note: This option is not very useful if HIDE_SCOPE_NAMES is set to YES. # Note: This option applies only to the class list, not to the # alphabetical list. SORT_BY_SCOPE_NAME = NO # The GENERATE_TODOLIST tag can be used to enable (YES) or # disable (NO) the todo list. This list is created by putting \todo # commands in the documentation. GENERATE_TODOLIST = YES # The GENERATE_TESTLIST tag can be used to enable (YES) or # disable (NO) the test list. This list is created by putting \test # commands in the documentation. GENERATE_TESTLIST = YES # The GENERATE_BUGLIST tag can be used to enable (YES) or # disable (NO) the bug list. This list is created by putting \bug # commands in the documentation. GENERATE_BUGLIST = YES # The GENERATE_DEPRECATEDLIST tag can be used to enable (YES) or # disable (NO) the deprecated list. This list is created by putting # \deprecated commands in the documentation. GENERATE_DEPRECATEDLIST= YES # The ENABLED_SECTIONS tag can be used to enable conditional # documentation sections, marked by \if sectionname ... \endif. ENABLED_SECTIONS = # The MAX_INITIALIZER_LINES tag determines the maximum number of lines # the initial value of a variable or define consists of for it to appear in # the documentation. If the initializer consists of more lines than specified # here it will be hidden. Use a value of 0 to hide initializers completely. # The appearance of the initializer of individual variables and defines in the # documentation can be controlled using \showinitializer or \hideinitializer # command in the documentation regardless of this setting. MAX_INITIALIZER_LINES = 30 # Set the SHOW_USED_FILES tag to NO to disable the list of files generated # at the bottom of the documentation of classes and structs. If set to YES the # list will mention the files that were used to generate the documentation. SHOW_USED_FILES = NO # If the sources in your project are distributed over multiple directories # then setting the SHOW_DIRECTORIES tag to YES will show the directory hierarchy # in the documentation. The default is NO. SHOW_DIRECTORIES = NO # The FILE_VERSION_FILTER tag can be used to specify a program or script that # doxygen should invoke to get the current version for each file (typically from the # version control system). Doxygen will invoke the program by executing (via # popen()) the command , where is the value of # the FILE_VERSION_FILTER tag, and is the name of an input file # provided by doxygen. Whatever the program writes to standard output # is used as the file version. See the manual for examples. FILE_VERSION_FILTER = #--------------------------------------------------------------------------- # configuration options related to warning and progress messages #--------------------------------------------------------------------------- # The QUIET tag can be used to turn on/off the messages that are generated # by doxygen. Possible values are YES and NO. If left blank NO is used. QUIET = NO # The WARNINGS tag can be used to turn on/off the warning messages that are # generated by doxygen. Possible values are YES and NO. If left blank # NO is used. WARNINGS = YES # If WARN_IF_UNDOCUMENTED is set to YES, then doxygen will generate warnings # for undocumented members. If EXTRACT_ALL is set to YES then this flag will # automatically be disabled. WARN_IF_UNDOCUMENTED = YES # If WARN_IF_DOC_ERROR is set to YES, doxygen will generate warnings for # potential errors in the documentation, such as not documenting some # parameters in a documented function, or documenting parameters that # don't exist or using markup commands wrongly. WARN_IF_DOC_ERROR = YES # This WARN_NO_PARAMDOC option can be abled to get warnings for # functions that are documented, but have no documentation for their parameters # or return value. If set to NO (the default) doxygen will only warn about # wrong or incomplete parameter documentation, but not about the absence of # documentation. WARN_NO_PARAMDOC = YES # The WARN_FORMAT tag determines the format of the warning messages that # doxygen can produce. The string should contain the $file, $line, and $text # tags, which will be replaced by the file and line number from which the # warning originated and the warning text. Optionally the format may contain # $version, which will be replaced by the version of the file (if it could # be obtained via FILE_VERSION_FILTER) WARN_FORMAT = "$file:$line: $text" # The WARN_LOGFILE tag can be used to specify a file to which warning # and error messages should be written. If left blank the output is written # to stderr. WARN_LOGFILE = #--------------------------------------------------------------------------- # configuration options related to the input files #--------------------------------------------------------------------------- # The INPUT tag can be used to specify the files and/or directories that contain # documented source files. You may enter file names like "myfile.cpp" or # directories like "/usr/src/myproject". Separate the files or directories # with spaces. INPUT = . ../C # If the value of the INPUT tag contains directories, you can use the # FILE_PATTERNS tag to specify one or more wildcard pattern (like *.cpp # and *.h) to filter out the source-files in the directories. If left # blank the following patterns are tested: # *.c *.cc *.cxx *.cpp *.c++ *.java *.ii *.ixx *.ipp *.i++ *.inl *.h *.hh *.hxx # *.hpp *.h++ *.idl *.odl *.cs *.php *.php3 *.inc *.m *.mm *.py FILE_PATTERNS = *.h # The RECURSIVE tag can be used to turn specify whether or not subdirectories # should be searched for input files as well. Possible values are YES and NO. # If left blank NO is used. RECURSIVE = NO # The EXCLUDE tag can be used to specify files and/or directories that should # excluded from the INPUT source files. This way you can easily exclude a # subdirectory from a directory tree whose root is specified with the INPUT tag. EXCLUDE = getwcstab.h wcsutil.h ../C/wcslib.h # The EXCLUDE_SYMLINKS tag can be used select whether or not files or # directories that are symbolic links (a Unix filesystem feature) are excluded # from the input. EXCLUDE_SYMLINKS = NO # If the value of the INPUT tag contains directories, you can use the # EXCLUDE_PATTERNS tag to specify one or more wildcard patterns to exclude # certain files from those directories. Note that the wildcards are matched # against the file with absolute path, so to exclude all test directories # for example use the pattern */test/* EXCLUDE_PATTERNS = # The EXAMPLE_PATH tag can be used to specify one or more files or # directories that contain example code fragments that are included (see # the \include command). EXAMPLE_PATH = # If the value of the EXAMPLE_PATH tag contains directories, you can use the # EXAMPLE_PATTERNS tag to specify one or more wildcard pattern (like *.cpp # and *.h) to filter out the source-files in the directories. If left # blank all files are included. EXAMPLE_PATTERNS = # If the EXAMPLE_RECURSIVE tag is set to YES then subdirectories will be # searched for input files to be used with the \include or \dontinclude # commands irrespective of the value of the RECURSIVE tag. # Possible values are YES and NO. If left blank NO is used. EXAMPLE_RECURSIVE = NO # The IMAGE_PATH tag can be used to specify one or more files or # directories that contain image that are included in the documentation (see # the \image command). IMAGE_PATH = . # The INPUT_FILTER tag can be used to specify a program that doxygen should # invoke to filter for each input file. Doxygen will invoke the filter program # by executing (via popen()) the command , where # is the value of the INPUT_FILTER tag, and is the name of an # input file. Doxygen will then use the output that the filter program writes # to standard output. If FILTER_PATTERNS is specified, this tag will be # ignored. INPUT_FILTER = # The FILTER_PATTERNS tag can be used to specify filters on a per file pattern # basis. Doxygen will compare the file name with each pattern and apply the # filter if there is a match. The filters are a list of the form: # pattern=filter (like *.cpp=my_cpp_filter). See INPUT_FILTER for further # info on how filters are used. If FILTER_PATTERNS is empty, INPUT_FILTER # is applied to all files. FILTER_PATTERNS = # If the FILTER_SOURCE_FILES tag is set to YES, the input filter (if set using # INPUT_FILTER) will be used to filter the input files when producing source # files to browse (i.e. when SOURCE_BROWSER is set to YES). FILTER_SOURCE_FILES = NO #--------------------------------------------------------------------------- # configuration options related to source browsing #--------------------------------------------------------------------------- # If the SOURCE_BROWSER tag is set to YES then a list of source files will # be generated. Documented entities will be cross-referenced with these sources. # Note: To get rid of all source code in the generated output, make sure also # VERBATIM_HEADERS is set to NO. SOURCE_BROWSER = NO # Setting the INLINE_SOURCES tag to YES will include the body # of functions and classes directly in the documentation. INLINE_SOURCES = NO # Setting the STRIP_CODE_COMMENTS tag to YES (the default) will instruct # doxygen to hide any special comment blocks from generated source code # fragments. Normal C and C++ comments will always remain visible. STRIP_CODE_COMMENTS = YES # If the REFERENCED_BY_RELATION tag is set to YES (the default) # then for each documented function all documented # functions referencing it will be listed. REFERENCED_BY_RELATION = YES # If the REFERENCES_RELATION tag is set to YES (the default) # then for each documented function all documented entities # called/used by that function will be listed. REFERENCES_RELATION = YES # If the REFERENCES_LINK_SOURCE tag is set to YES (the default) # and SOURCE_BROWSER tag is set to YES, then the hyperlinks from # functions in REFERENCES_RELATION and REFERENCED_BY_RELATION lists will # link to the source code. Otherwise they will link to the documentstion. REFERENCES_LINK_SOURCE = YES # If the USE_HTAGS tag is set to YES then the references to source code # will point to the HTML generated by the htags(1) tool instead of doxygen # built-in source browser. The htags tool is part of GNU's global source # tagging system (see http://www.gnu.org/software/global/global.html). You # will need version 4.8.6 or higher. USE_HTAGS = NO # If the VERBATIM_HEADERS tag is set to YES (the default) then Doxygen # will generate a verbatim copy of the header file for each class for # which an include is specified. Set to NO to disable this. VERBATIM_HEADERS = YES #--------------------------------------------------------------------------- # configuration options related to the alphabetical class index #--------------------------------------------------------------------------- # If the ALPHABETICAL_INDEX tag is set to YES, an alphabetical index # of all compounds will be generated. Enable this if the project # contains a lot of classes, structs, unions or interfaces. ALPHABETICAL_INDEX = NO # If the alphabetical index is enabled (see ALPHABETICAL_INDEX) then # the COLS_IN_ALPHA_INDEX tag can be used to specify the number of columns # in which this list will be split (can be a number in the range [1..20]) COLS_IN_ALPHA_INDEX = 5 # In case all classes in a project start with a common prefix, all # classes will be put under the same header in the alphabetical index. # The IGNORE_PREFIX tag can be used to specify one or more prefixes that # should be ignored while generating the index headers. IGNORE_PREFIX = #--------------------------------------------------------------------------- # configuration options related to the HTML output #--------------------------------------------------------------------------- # If the GENERATE_HTML tag is set to YES (the default) Doxygen will # generate HTML output. GENERATE_HTML = YES # The HTML_OUTPUT tag is used to specify where the HTML docs will be put. # If a relative path is entered the value of OUTPUT_DIRECTORY will be # put in front of it. If left blank `html' will be used as the default path. HTML_OUTPUT = ../html # The HTML_FILE_EXTENSION tag can be used to specify the file extension for # each generated HTML page (for example: .htm,.php,.asp). If it is left blank # doxygen will generate files with .html extension. HTML_FILE_EXTENSION = .html # The HTML_HEADER tag can be used to specify a personal HTML header for # each generated HTML page. If it is left blank doxygen will generate a # standard header. HTML_HEADER = # The HTML_FOOTER tag can be used to specify a personal HTML footer for # each generated HTML page. If it is left blank doxygen will generate a # standard footer. HTML_FOOTER = # The HTML_STYLESHEET tag can be used to specify a user-defined cascading # style sheet that is used by each HTML page. It can be used to # fine-tune the look of the HTML output. If the tag is left blank doxygen # will generate a default style sheet. Note that doxygen will try to copy # the style sheet file to the HTML output directory, so don't put your own # stylesheet in the HTML output directory as well, or it will be erased! HTML_STYLESHEET = # If the HTML_ALIGN_MEMBERS tag is set to YES, the members of classes, # files or namespaces will be aligned in HTML using tables. If set to # NO a bullet list will be used. HTML_ALIGN_MEMBERS = YES # If the GENERATE_HTMLHELP tag is set to YES, additional index files # will be generated that can be used as input for tools like the # Microsoft HTML help workshop to generate a compressed HTML help file (.chm) # of the generated HTML documentation. GENERATE_HTMLHELP = NO # If the GENERATE_HTMLHELP tag is set to YES, the CHM_FILE tag can # be used to specify the file name of the resulting .chm file. You # can add a path in front of the file if the result should not be # written to the html output directory. CHM_FILE = # If the GENERATE_HTMLHELP tag is set to YES, the HHC_LOCATION tag can # be used to specify the location (absolute path including file name) of # the HTML help compiler (hhc.exe). If non-empty doxygen will try to run # the HTML help compiler on the generated index.hhp. HHC_LOCATION = # If the GENERATE_HTMLHELP tag is set to YES, the GENERATE_CHI flag # controls if a separate .chi index file is generated (YES) or that # it should be included in the master .chm file (NO). GENERATE_CHI = NO # If the GENERATE_HTMLHELP tag is set to YES, the BINARY_TOC flag # controls whether a binary table of contents is generated (YES) or a # normal table of contents (NO) in the .chm file. BINARY_TOC = NO # The TOC_EXPAND flag can be set to YES to add extra items for group members # to the contents of the HTML help documentation and to the tree view. TOC_EXPAND = NO # The DISABLE_INDEX tag can be used to turn on/off the condensed index at # top of each HTML page. The value NO (the default) enables the index and # the value YES disables it. DISABLE_INDEX = NO # This tag can be used to set the number of enum values (range [1..20]) # that doxygen will group on one line in the generated HTML documentation. ENUM_VALUES_PER_LINE = 4 # If the GENERATE_TREEVIEW tag is set to YES, a side panel will be # generated containing a tree-like index structure (just like the one that # is generated for HTML Help). For this to work a browser that supports # JavaScript, DHTML, CSS and frames is required (for instance Mozilla 1.0+, # Netscape 6.0+, Internet explorer 5.0+, or Konqueror). Windows users are # probably better off using the HTML help feature. GENERATE_TREEVIEW = NO # If the treeview is enabled (see GENERATE_TREEVIEW) then this tag can be # used to set the initial width (in pixels) of the frame in which the tree # is shown. TREEVIEW_WIDTH = 250 #--------------------------------------------------------------------------- # configuration options related to the LaTeX output #--------------------------------------------------------------------------- # If the GENERATE_LATEX tag is set to YES (the default) Doxygen will # generate Latex output. GENERATE_LATEX = YES # The LATEX_OUTPUT tag is used to specify where the LaTeX docs will be put. # If a relative path is entered the value of OUTPUT_DIRECTORY will be # put in front of it. If left blank `latex' will be used as the default path. LATEX_OUTPUT = latex # The LATEX_CMD_NAME tag can be used to specify the LaTeX command name to be # invoked. If left blank `latex' will be used as the default command name. LATEX_CMD_NAME = latex # The MAKEINDEX_CMD_NAME tag can be used to specify the command name to # generate index for LaTeX. If left blank `makeindex' will be used as the # default command name. MAKEINDEX_CMD_NAME = makeindex # If the COMPACT_LATEX tag is set to YES Doxygen generates more compact # LaTeX documents. This may be useful for small projects and may help to # save some trees in general. COMPACT_LATEX = YES # The PAPER_TYPE tag can be used to set the paper type that is used # by the printer. Possible values are: a4, a4wide, letter, legal and # executive. If left blank a4wide will be used. PAPER_TYPE = a4wide # The EXTRA_PACKAGES tag can be to specify one or more names of LaTeX # packages that should be included in the LaTeX output. EXTRA_PACKAGES = latexsym # The LATEX_HEADER tag can be used to specify a personal LaTeX header for # the generated latex document. The header should contain everything until # the first chapter. If it is left blank doxygen will generate a # standard header. Notice: only use this tag if you know what you are doing! LATEX_HEADER = # If the PDF_HYPERLINKS tag is set to YES, the LaTeX that is generated # is prepared for conversion to pdf (using ps2pdf). The pdf file will # contain links (just like the HTML output) instead of page references # This makes the output suitable for online browsing using a pdf viewer. PDF_HYPERLINKS = YES # If the USE_PDFLATEX tag is set to YES, pdflatex will be used instead of # plain latex in the generated Makefile. Set this option to YES to get a # higher quality PDF documentation. USE_PDFLATEX = YES # If the LATEX_BATCHMODE tag is set to YES, doxygen will add the \\batchmode. # command to the generated LaTeX files. This will instruct LaTeX to keep # running if errors occur, instead of asking the user for help. # This option is also used when generating formulas in HTML. LATEX_BATCHMODE = NO # If LATEX_HIDE_INDICES is set to YES then doxygen will not # include the index chapters (such as File Index, Compound Index, etc.) # in the output. LATEX_HIDE_INDICES = NO #--------------------------------------------------------------------------- # configuration options related to the RTF output #--------------------------------------------------------------------------- # If the GENERATE_RTF tag is set to YES Doxygen will generate RTF output # The RTF output is optimized for Word 97 and may not look very pretty with # other RTF readers or editors. GENERATE_RTF = NO # The RTF_OUTPUT tag is used to specify where the RTF docs will be put. # If a relative path is entered the value of OUTPUT_DIRECTORY will be # put in front of it. If left blank `rtf' will be used as the default path. RTF_OUTPUT = rtf # If the COMPACT_RTF tag is set to YES Doxygen generates more compact # RTF documents. This may be useful for small projects and may help to # save some trees in general. COMPACT_RTF = NO # If the RTF_HYPERLINKS tag is set to YES, the RTF that is generated # will contain hyperlink fields. The RTF file will # contain links (just like the HTML output) instead of page references. # This makes the output suitable for online browsing using WORD or other # programs which support those fields. # Note: wordpad (write) and others do not support links. RTF_HYPERLINKS = NO # Load stylesheet definitions from file. Syntax is similar to doxygen's # config file, i.e. a series of assignments. You only have to provide # replacements, missing definitions are set to their default value. RTF_STYLESHEET_FILE = # Set optional variables used in the generation of an rtf document. # Syntax is similar to doxygen's config file. RTF_EXTENSIONS_FILE = #--------------------------------------------------------------------------- # configuration options related to the man page output #--------------------------------------------------------------------------- # If the GENERATE_MAN tag is set to YES (the default) Doxygen will # generate man pages GENERATE_MAN = NO # The MAN_OUTPUT tag is used to specify where the man pages will be put. # If a relative path is entered the value of OUTPUT_DIRECTORY will be # put in front of it. If left blank `man' will be used as the default path. MAN_OUTPUT = man # The MAN_EXTENSION tag determines the extension that is added to # the generated man pages (default is the subroutine's section .3) MAN_EXTENSION = .3 # If the MAN_LINKS tag is set to YES and Doxygen generates man output, # then it will generate one additional man file for each entity # documented in the real man page(s). These additional files # only source the real man page, but without them the man command # would be unable to find the correct page. The default is NO. MAN_LINKS = NO #--------------------------------------------------------------------------- # configuration options related to the XML output #--------------------------------------------------------------------------- # If the GENERATE_XML tag is set to YES Doxygen will # generate an XML file that captures the structure of # the code including all documentation. GENERATE_XML = NO # The XML_OUTPUT tag is used to specify where the XML pages will be put. # If a relative path is entered the value of OUTPUT_DIRECTORY will be # put in front of it. If left blank `xml' will be used as the default path. XML_OUTPUT = xml # The XML_SCHEMA tag can be used to specify an XML schema, # which can be used by a validating XML parser to check the # syntax of the XML files. XML_SCHEMA = # The XML_DTD tag can be used to specify an XML DTD, # which can be used by a validating XML parser to check the # syntax of the XML files. XML_DTD = # If the XML_PROGRAMLISTING tag is set to YES Doxygen will # dump the program listings (including syntax highlighting # and cross-referencing information) to the XML output. Note that # enabling this will significantly increase the size of the XML output. XML_PROGRAMLISTING = YES #--------------------------------------------------------------------------- # configuration options for the AutoGen Definitions output #--------------------------------------------------------------------------- # If the GENERATE_AUTOGEN_DEF tag is set to YES Doxygen will # generate an AutoGen Definitions (see autogen.sf.net) file # that captures the structure of the code including all # documentation. Note that this feature is still experimental # and incomplete at the moment. GENERATE_AUTOGEN_DEF = NO #--------------------------------------------------------------------------- # configuration options related to the Perl module output #--------------------------------------------------------------------------- # If the GENERATE_PERLMOD tag is set to YES Doxygen will # generate a Perl module file that captures the structure of # the code including all documentation. Note that this # feature is still experimental and incomplete at the # moment. GENERATE_PERLMOD = NO # If the PERLMOD_LATEX tag is set to YES Doxygen will generate # the necessary Makefile rules, Perl scripts and LaTeX code to be able # to generate PDF and DVI output from the Perl module output. PERLMOD_LATEX = NO # If the PERLMOD_PRETTY tag is set to YES the Perl module output will be # nicely formatted so it can be parsed by a human reader. This is useful # if you want to understand what is going on. On the other hand, if this # tag is set to NO the size of the Perl module output will be much smaller # and Perl will parse it just the same. PERLMOD_PRETTY = YES # The names of the make variables in the generated doxyrules.make file # are prefixed with the string contained in PERLMOD_MAKEVAR_PREFIX. # This is useful so different doxyrules.make files included by the same # Makefile don't overwrite each other's variables. PERLMOD_MAKEVAR_PREFIX = #--------------------------------------------------------------------------- # Configuration options related to the preprocessor #--------------------------------------------------------------------------- # If the ENABLE_PREPROCESSING tag is set to YES (the default) Doxygen will # evaluate all C-preprocessor directives found in the sources and include # files. ENABLE_PREPROCESSING = YES # If the MACRO_EXPANSION tag is set to YES Doxygen will expand all macro # names in the source code. If set to NO (the default) only conditional # compilation will be performed. Macro expansion can be done in a controlled # way by setting EXPAND_ONLY_PREDEF to YES. MACRO_EXPANSION = YES # If the EXPAND_ONLY_PREDEF and MACRO_EXPANSION tags are both set to YES # then the macro expansion is limited to the macros specified with the # PREDEFINED and EXPAND_AS_DEFINED tags. EXPAND_ONLY_PREDEF = YES # If the SEARCH_INCLUDES tag is set to YES (the default) the includes files # in the INCLUDE_PATH (see below) will be search if a #include is found. SEARCH_INCLUDES = YES # The INCLUDE_PATH tag can be used to specify one or more directories that # contain include files that are not input files but should be processed by # the preprocessor. INCLUDE_PATH = # You can use the INCLUDE_FILE_PATTERNS tag to specify one or more wildcard # patterns (like *.h and *.hpp) to filter out the header-files in the # directories. If left blank, the patterns specified with FILE_PATTERNS will # be used. INCLUDE_FILE_PATTERNS = # The PREDEFINED tag can be used to specify one or more macro names that # are defined before the preprocessor is started (similar to the -D option of # gcc). The argument of the tag is a list of macros of the form: name # or name=definition (no spaces). If the definition and the = are # omitted =1 is assumed. To prevent a macro definition from being # undefined via #undef or recursively expanded use the := operator # instead of the = operator. PREDEFINED = # If the MACRO_EXPANSION and EXPAND_ONLY_PREDEF tags are set to YES then # this tag can be used to specify a list of macro names that should be expanded. # The macro definition that is found in the sources will be used. # Use the PREDEFINED tag if you want to use a different macro definition. EXPAND_AS_DEFINED = # If the SKIP_FUNCTION_MACROS tag is set to YES (the default) then # doxygen's preprocessor will remove all function-like macros that are alone # on a line, have an all uppercase name, and do not end with a semicolon. Such # function macros are typically used for boiler-plate code, and will confuse # the parser if not removed. 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SEARCHENGINE = NO pywcs-1.12/wcslib/doxygen/fitshdr.sed0000644001153600020070000000043012310355626021743 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} /^\*/s| fitskey| #fitskey|g s|CONTINUE|&|g s|END|&|g s|ABCD.*89-_|&|g s|"= "|''= ''|g s|'='|'='|g s|'/'|'/'|g s|'&'|'\&'|g s|(')|(')|g pywcs-1.12/wcslib/doxygen/fitshdr_extras.dox0000644001153600020070000000306612310355626023360 0ustar cslocumSTSCI\science00000000000000/** @def FITSHDR_KEYWORD * @brief Flag bit indicating illegal keyword syntax. * * Bit mask for the status flag bit-vector returned by fitshdr() indicating * illegal keyword syntax. */ /** @def FITSHDR_KEYVALUE * @brief Flag bit indicating illegal keyvalue syntax. * * Bit mask for the status flag bit-vector returned by fitshdr() indicating * illegal keyvalue syntax. */ /** @def FITSHDR_COMMENT * @brief Flag bit indicating illegal keycomment syntax. * * Bit mask for the status flag bit-vector returned by fitshdr() indicating * illegal keycomment syntax. */ /** @def FITSHDR_KEYREC * @brief Flag bit indicating illegal keyrecord. * * Bit mask for the status flag bit-vector returned by fitshdr() indicating * an illegal keyrecord, e.g. an END keyrecord with trailing text. */ /** @def FITSHDR_CARD * @brief Deprecated. * * @deprecated Added for backwards compatibility, use FITSHDR_KEYREC * instead. */ /** @def FITSHDR_TRAILER * @brief Flag bit indicating keyrecord following a valid END keyrecord. * * Bit mask for the status flag bit-vector returned by fitshdr() indicating * a keyrecord following a valid END keyrecord. */ /** @typedef int64 * @brief 64-bit signed integer data type. * * 64-bit signed integer data type defined via preprocessor macro WCSLIB_INT64 * which may be defined in wcsconfig.h. For example * * @code * #define WCSLIB_INT64 long long int * @endcode * * This is typedef'd in fitshdr.h as * * @code * #ifdef WCSLIB_INT64 * typedef WCSLIB_INT64 int64; * #else * typedef int int64[3]; * #endif * @endcode * * See fitskey::type. */ pywcs-1.12/wcslib/doxygen/getwcstab.sed0000644001153600020070000000015012310355626022262 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} /^\*/s| wtbarr| #wtbarr|g /^\*/s| #wtbarr_s| wtbarr_s|g s|'TAB'|'TAB'|g pywcs-1.12/wcslib/doxygen/GNUmakefile0000644001153600020070000000443112310355626021662 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile for building the documentation for WCSLIB 4.10 # # Summary of the main targets # --------------------------- # build: Invoke 'doxygen' etc. to compile the documentation. # clean: Delete rubbish files. # cleaner (distclean or realclean): clean, and also delete intermediate # files. # cleanest: cleaner, and also delete the generated documentation. # # Notes: # 1) If you need to make changes then preferably modify ../makedefs.in # instead and re-run configure. # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: GNUmakefile,v 4.10 2012/02/05 23:41:45 cal103 Exp $ #----------------------------------------------------------------------------- # Get configure settings. include ../makedefs DOXHDRS := $(notdir $(wildcard ../C/*.h)) DOXMARX := $(DOXHDRS:.h=.dox) EXTRADOX := mainpage.dox $(wildcard *_extras.dox) # Pattern rules #-------------- %.dox : ../C/%.h doxextr doxextr.sed %.sed Doxyfile -@ echo '' @ if [ -f $*.sed ] ; then \ echo "doxextr $< | sed -f $*.sed | sed -f doxextr.sed > $@" ; \ ./doxextr $< | sed -f $*.sed | sed -f doxextr.sed > $@ ; \ else \ echo "doxextr $< | sed -f doxextr.sed > $@" ; \ ./doxextr $< | sed -f doxextr.sed > $@ ; \ fi %.c : %.l -@ echo '' -@ $(RM) $@ $(FLEX) $(FLFLAGS) -t $< | sed -e 's/^[ ]*#/#/' > $@ % : %.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) -o $@ $< # Don't fret if there's no specific sed script. %.sed : ; # Static rules #------------- .PHONY : all clean cleaner cleanest distclean html pdf realclean build : doxextr html pdf html : ../html/index.html pdf : ../wcslib.pdf ../wcslib.pdf : latex/refman.tex $(MAKE) -C latex refman.pdf -@ $(RM) $@ mv latex/refman.pdf $@ ../html/index.html latex/refman.tex : doxextr wcslib.h -@ echo '' doxygen wcslib.h : $(DOXMARX) $(EXTRADOX) @ cat ../C/wcslib.h *.dox > $@ clean : - $(RM) core cleaner distclean realclean : clean - $(RM) doxextr wcslib.h - $(RM) $(DOXMARX) - $(RM) wcslib.tag - $(RM) -r ./latex cleanest : cleaner - $(RM) -r ../html ../wcslib.pdf GNUmakefile : ../makedefs ; ../makedefs : ../makedefs.in cd .. && ./config.status pywcs-1.12/wcslib/doxygen/lin.sed0000644001153600020070000000005112310355626021061 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} /^\*/s| linprm| #linprm|g pywcs-1.12/wcslib/doxygen/lin_extras.dox0000644001153600020070000000343512310355626022477 0ustar cslocumSTSCI\science00000000000000/** @def LINLEN * @brief Size of the #linprm struct in @a int units. * * Size of the #linprm struct in @a int units, used by the Fortran wrappers. */ /** @def linini_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @def lincpy_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @def linfree_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @def linprt_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @def linset_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @def linp2x_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @def linx2p_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #lin_errmsg directly now * instead. */ /** @fn matinv(int n, const double mat[], double inv[]) * * @brief Matrix inversion. * * @b %matinv() performs matrix inversion using LU-triangular factorization * with scaled partial pivoting. * * @param[in] n Order of the matrix (\f$n \times n\f$). * * @param[in] mat Matrix to be inverted, stored as mat[\f$i n + j\f$] * where \f$i\f$ and \f$j\f$ are the row and column * indices respectively. * * @param[out] inv Inverse of mat with the same storage convention. * * @return Status return value: * - 0: Success. * - 2: Memory allocation failed. * - 3: Singular matrix. */ pywcs-1.12/wcslib/doxygen/mainpage.dox0000644001153600020070000013202612310355626022107 0ustar cslocumSTSCI\science00000000000000/** @mainpage WCSLIB 4.10 and PGSBOX 4.10 @image html Bonne.gif "Bonne's projection" @section contents Contents - @subpage intro - @subpage software - @subpage overview - @subpage structs - @subpage memory - @subpage diagnostics - @subpage vector - @subpage threads - @subpage testing - @subpage fortran - @subpage pgsbox @section copyright Copyright @verbatim WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA @endverbatim */ /** @page intro Introduction WCSLIB is a C library, supplied with a full set of Fortran wrappers, that implements the "World Coordinate System" (WCS) standard in FITS (Flexible Image Transport System). It also includes a @ref software "PGPLOT"-based routine, @ref pgsbox "PGSBOX", for drawing general curvilinear coordinate graticules and a number of utility programs. The FITS data format is widely used within the international astronomical community, from the radio to gamma-ray regimes, for data interchange and archive, and also increasingly as an online format. It is described in - "Definition of The Flexible Image Transport System (FITS)", FITS Standard, Version 3.0, 2008 July 10. available from the FITS Support Office at http://fits.gsfc.nasa.gov. The FITS WCS standard is described in - "Representations of world coordinates in FITS" (Paper I), Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061-1075 - "Representations of celestial coordinates in FITS" (Paper II), Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077-1122 - "Representations of spectral coordinates in FITS" (Paper III), Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. 2006, A&A, 446, 747 - "Mapping on the HEALPix Grid" (HPX), Calabretta, M.R., & Roukema, B.F. 2007, MNRAS, 381, 865 Reprints of all published papers may be obtained from NASA's Astrophysics Data System (ADS), http://adsabs.harvard.edu/. Reprints of Papers I, II (+HPX) and III are available from http://www.atnf.csiro.au/~mcalabre/. This site also includes errata and supplementary material for Papers I, II and III. Additional information on all aspects of FITS and its various software implementations may be found at the FITS Support Office http://fits.gsfc.nasa.gov. */ /** @page software FITS-WCS and related software Several implementations of the FITS WCS standards are available: - The @ref overview "WCSLIB" software distribution (i.e. this library) may be obtained from http://www.atnf.csiro.au/~mcalabre/WCS/. The remainder of this manual describes its use. - @b wcstools, developed by Doug Mink, may be obtained from http://tdc-www.harvard.edu/software/wcstools/. - @b AST, developed by David Berry within the U.K. Starlink project, http://www.starlink.ac.uk/ast/ and now supported by JAC, Hawaii http://starlink.jach.hawaii.edu/starlink/. @n@n A useful utility for experimenting with FITS WCS descriptions (similar to @a wcsgrid) is also provided; go to the above site and then look at the section entitled "FITS-WCS Plotting Demo". - @b SolarSoft, http://sohowww.nascom.nasa.gov/solarsoft/, primarily an IDL-based system for analysis of Solar physics data, contains a module written by Bill Thompson oriented towards Solar coordinate systems, including spectral, http://sohowww.nascom.nasa.gov/solarsoft/gen/idl/wcs/. - The IDL Astronomy Library, http://idlastro.gsfc.nasa.gov/, contains an independent implementation of FITS-WCS in IDL by Rick Balsano, Wayne Landsman and others. See http://idlastro.gsfc.nasa.gov/contents.html#C5. Python wrappers to @ref overview "WCSLIB" are provided by - The Kapteyn Package http://www.astro.rug.nl/software/kapteyn/ by Hans Terlouw and Martin Vogelaar. - pywcs, http://stsdas.stsci.edu/astrolib/pywcs/ by Michael Droettboom. Java is supported via - CADC/CCDA Java Native Interface (JNI) bindings to @ref overview "WCSLIB" 4.2 http://www.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/cadc/source/ by Patrick Dowler. Recommended WCS-aware FITS image viewers: - Bill Joye's DS9, http://hea-www.harvard.edu/RD/ds9/, and - Fv by Pan Chai, http://heasarc.gsfc.nasa.gov/ftools/fv/. both handle 2-D images. Currently (2012/01/24) I know of no image viewers that handle 1-D spectra properly nor multi-dimensional data, not even multi-dimensional data with only two non-degenerate image axes (please inform me if you know otherwise). Pre-built @ref overview "WCSLIB" packages are available, generally a little behind the main release (this list will probably be out-of-date by the time you read it, best do a web search): - Fedora (RPM), https://admin.fedoraproject.org/pkgdb/packages/name/wcslib. - Fresh Ports (RPM), http://www.freshports.org/astro/wcslib/. - Gentoo, http://packages.gentoo.org/package/sci-astronomy/wcslib. - RPM (general) http://v2.www.rpmseek.com/cat/Libraries.html?hl=com&cx=591:W. Bill Pence's general FITS IO library, CFITSIO is available from http://heasarc.gsfc.nasa.gov/fitsio/. It is used optionally by some of the high-level WCSLIB test programs and is required by two of the utility programs. PGPLOT, Tim Pearson's Fortran plotting package on which @ref pgsbox "PGSBOX" is based, also used by some of the WCSLIB self-test suite and a utility program, is available from http://astro.caltech.edu/~tjp/pgplot/. */ /** @page overview Overview of WCSLIB WCSLIB is documented in the prologues of its header files which provide a detailed description of the purpose of each function and its interface (this material is, of course, used to generate the doxygen manual). Here we explain how the library as a whole is structured. We will normally refer to WCSLIB 'routines', meaning C functions or Fortran 'subroutines', though the latter are actually wrappers implemented in C. WCSLIB is layered software, each layer depends only on those beneath; understanding WCSLIB first means understanding its stratigraphy. There are essentially three levels, though some intermediate levels exist within these: - The top layer consists of routines that provide the connection between FITS files and the high-level WCSLIB data structures, the main function being to parse a FITS header, extract WCS information, and copy it into a wcsprm struct. The lexical parsers among these are implemented as Flex descriptions (source files with .l suffix) and the C code generated from these by Flex is included in the source distribution. - wcshdr.h,c -- Routines for constructing wcsprm data structures from information in a FITS header and conversely for writing a wcsprm struct out as a FITS header. - wcspih.l -- Flex implementation of wcspih(), a lexical parser for WCS "keyrecords" in an image header. A @b @e keyrecord (formerly called "card image") consists of a @b @e keyword, its value - the @b @e keyvalue - and an optional comment, the @b @e keycomment. - wcsbth.l -- Flex implementation of wcsbth() which parses binary table image array and pixel list headers in addition to image array headers. - getwcstab.h,c -- Implementation of a -TAB binary table reader in @ref software "CFITSIO". . @n A generic FITS header parser is also provided to handle non-WCS keyrecords that are ignored by wcspih(): - fitshdr.h,l -- Generic FITS header parser (not WCS-specific). . @n The philosophy adopted for dealing with non-standard WCS usage is to translate it at this level so that the middle- and low-level routines need only deal with standard constructs: - wcsfix.h,c -- Translator for non-standard FITS WCS constructs (uses wcsutrne()). - wcsutrn.l -- Lexical translator for non-standard units specifications. . @n As a concrete example, within this layer the @c CTYPEia keyvalues would be extracted from a FITS header and copied into the @a ctype[] array within a wcsprm struct. None of the header keyrecords are interpreted. - The middle layer analyses the WCS information obtained from the FITS header by the top-level routines, identifying the separate steps of the WCS algorithm chain for each of the coordinate axes in the image. It constructs the various data structures on which the low-level routines are based and invokes them in the correct sequence. Thus the wcsprm struct is essentially the glue that binds together the low-level routines into a complete coordinate description. - wcs.h,c -- Driver routines for the low-level routines. - wcsunits.h,c -- Unit conversions (uses wcsulexe()). - wcsulex.l -- Lexical parser for units specifications. . @n To continue the above example, within this layer the @a ctype[] keyvalues in a wcsprm struct are analysed to determine the nature of the coordinate axes in the image. - Applications programmers who use the top- and middle-level routines generally need know nothing about the low-level routines. These are essentially mathematical in nature and largely independent of FITS itself. The mathematical formulae and algorithms cited in the WCS Papers, for example the spherical projection equations of Paper II and the lookup-table methods of Paper III, are implemented by the routines in this layer, some of which serve to aggregate others: - cel.h,c -- Celestial coordinate transformations, combines prj.h,c and sph.h,c. - spc.h,c -- Spectral coordinate transformations, combines transformations from spx.h,c. . @n The remainder of the routines in this level are independent of everything other than the grass-roots mathematical functions: - lin.h,c -- Linear transformation matrix. - log.h,c -- Logarithmic coordinates. - prj.h,c -- Spherical projection equations. - sph.h,c -- Spherical coordinate transformations. - spx.h,c -- Basic spectral transformations. - tab.h,c -- Coordinate lookup tables. . @n As the routines within this layer are quite generic, some, principally the implementation of the spherical projection equations, have been used in other packages (AST, wcstools) that provide their own implementations of the functionality of the top and middle-level routines. - At the grass-roots level there are a number of mathematical and utility routines. @n@n When dealing with celestial coordinate systems it is often desirable to use an angular measure that provides an exact representation of the latitude of the north or south pole. The WCSLIB routines use the following trigonometric functions that take or return angles in degrees: - cosd(), sind(), sincosd(), tand(), acosd(), asind(), atand(), atan2d() . @n These "trigd" routines are expected to handle angles that are a multiple of @f$90^\circ@f$ returning an exact result. Some C implementations provide these as part of a system library and in such cases it may (or may not!) be preferable to use them. wcstrig.c provides wrappers on the standard trig functions based on radian measure, adding tests for multiples of @f$90^\circ@f$. @n@n However, wcstrig.h also provides the choice of using preprocessor macro implementations of the trigd functions that don't test for multiples of @f$90^\circ@f$ (compile with @c -DWCSTRIG_MACRO). These are typically 20% faster but may lead to problems near the poles. - wcsmath.h -- Defines mathematical and other constants. - wcstrig.h,c -- Various implementations of trigd functions. - wcsutil.h,c -- Simple utility functions for string manipulation, etc. used by WCSLIB. Complementary to the C library, a set of wrappers are provided that allow all WCSLIB C functions to be called by Fortran programs, see below. Plotting of coordinate graticules is one of the more important requirements of a world coordinate system. WCSLIB provides a @ref software "PGPLOT"-based subroutine, @ref pgsbox "PGSBOX" (Fortran), which handles general curvilinear coordinates via a user-supplied function - @c PGWCSL provides the interface to WCSLIB. A C wrapper, @a cpgsbox(), is also provided, see below. Several utility programs are distributed with WCSLIB: - @a wcsgrid extracts the WCS keywords for an image from the specified FITS file and uses @a cpgsbox() to plot a 2-D coordinate graticule for it. It requires WCSLIB, @ref pgsbox "PGSBOX" and @ref software "CFITSIO". - @a wcsware extracts the WCS keywords for an image from the specified FITS file and constructs wcsprm structs for each coordinate representation found. The structs may then be printed or used to transform pixel coordinates to world coordinates. It requires WCSLIB and @ref software "CFITSIO". - @a HPXcvt reorganises HEALPix data into a 2-D FITS image with HPX coordinate system. The input data may be stored in a FITS file as a primary image or image extension, or as a binary table extension. Both NESTED and RING pixel indices are supported. It uses @ref software "CFITSIO". - @a fitshdr lists headers from a FITS file specified on the command line, or else on stdin, printing them as 80-character keyrecords without trailing blanks. It is independent of WCSLIB. */ /** @page structs WCSLIB data structures The WCSLIB routines are based on data structures specific to them: wcsprm for the wcs.h,c routines, celprm for cel.h,c, and likewise spcprm, linprm, prjprm and tabprm, with struct definitions contained in the corresponding header files: wcs.h, cel.h, etc. The structs store the parameters that define a coordinate transformation and also intermediate values derived from those parameters. As a high-level object, the wcsprm struct contains linprm, tabprm, spcprm, and celprm structs, and in turn the celprm struct contains a prjprm struct. Hence the wcsprm struct contains everything needed for a complete coordinate description. Applications programmers who use the top- and middle-level routines generally only need to pass wcsprm structs from one routine that fills them to another that uses them. However, since these structs are fundamental to WCSLIB it is worthwhile knowing something about the way they work. Three basic operations apply to all WCSLIB structs: - Initialize. Each struct has a specific initialization routine, e.g. wcsini(), celini(), spcini(), etc. These allocate memory (if required) and set all struct members to default values. - Fill in the required values. Each struct has members whose values must be provided. For example, for wcsprm these values correspond to FITS WCS header keyvalues as are provided by the top-level header parsing routine, wcspih(). - Compute intermediate values. Specific setup routines, e.g. wcsset(), celset(), spcset(), etc., compute intermediate values from the values provided. In particular, wcsset() analyses the FITS WCS keyvalues provided, fills the required values in the lower-level structs contained in wcsprm, and invokes the setup routine for each of them. Each struct contains a @a flag member that records its setup state. This is cleared by the initialization routine and checked by the routines that use the struct; they will invoke the setup routine automatically if necessary, hence it need not be invoked specifically by the application programmer. However, if any of the required values in a struct are changed then either the setup routine must be invoked on it, or else the @a flag must be zeroed to signal that the struct needs to be reset. The initialization routine may be invoked repeatedly on a struct if it is desired to reuse it. However, the @a flag member of structs that contain allocated memory (wcsprm, linprm and tabprm) must be set to -1 before the first initialization to initialize memory management, but not subsequently or else memory leaks will result. Each struct has one or more service routines: to do deep copies from one to another, to print its contents, and to free allocated memory. Refer to the header files for a detailed description. */ /** @page memory Memory management The initialization routines for certain of the WCSLIB data structures allocate memory for some of their members: - wcsini() optionally allocates memory for the @a crpix, @a pc, @a cdelt, @a crval, @a cunit, @a ctype, @a pv, @a ps, @a cd, @a crota, @a colax, @a cname, @a crder, and @a csyer arrays in the wcsprm struct (using linini() for certain of these). Note that wcsini() does not allocate memory for the @a tab array - refer to the usage notes for wcstab() in wcshdr.h. If the @a pc matrix is not unity, wcsset() (via linset()) also allocates memory for the @a piximg and @a imgpix arrays. - linini(): optionally allocates memory for the @a crpix, @a pc, and @a cdelt arrays in the linprm struct. If the @a pc matrix is not unity, linset() also allocates memory for the @a piximg and @a imgpix arrays. Typically these would be used by wcsini() and wcsset(). - tabini(): optionally allocates memory for the @a K, @a map, @a crval, @a index, and @a coord arrays (including the arrays referenced by @a index[]) in the tabprm struct. tabmem() takes control of any of these arrays that may have been allocated by the user, specifically in that tabfree() will then free it. tabset() also allocates memory for the @a sense, @a p0, @a delta and @a extrema arrays. The caller may load data into these arrays but must not modify the struct members (i.e. the pointers) themselves or else memory leaks will result. wcsini() maintains a record of memory it has allocated and this is used by wcsfree() which wcsini() uses to free any memory that it may have allocated on a previous invokation. Thus it is not necessary for the caller to invoke wcsfree() separately if wcsini() is invoked repeatedly on the same wcsprm struct. Likewise, wcsset() deallocates memory that it may have allocated on a previous invokation. The same comments apply to linini(), linfree(), and linset() and to tabini(), tabfree(), and tabset(). A memory leak will result if a wcsprm, linprm or tabprm struct goes out of scope before the memory has been @a free'd, either by the relevant routine, wcsfree(), linfree() or tabfree(), or otherwise. Likewise, if one of these structs itself has been @a malloc'd and the allocated memory is not @a free'd when the memory for the struct is @a free'd. A leak may also arise if the caller interferes with the array pointers in the "private" part of these structs. Beware of making a shallow copy of a wcsprm, linprm or tabprm struct by assignment; any changes made to allocated memory in one would be reflected in the other, and if the memory allocated for one was @a free'd the other would reference unallocated memory. Use the relevant routine instead to make a deep copy: wcssub(), lincpy() or tabcpy(). */ /** @page diagnostics Diagnostic output All @ref overview "WCSLIB" functions return a status value, each of which is associated with a fixed error message which may be used for diagnostic output. For example @verbatim int status; struct wcsprm wcs; ... if ((status = wcsset(&wcs)) { fprintf(stderr, "ERROR %d from wcsset(): %s.\n", status, wcs_errmsg[status]); return status; } @endverbatim This might produce output like @verbatim ERROR 5 from wcsset(): Invalid parameter value. @endverbatim The error messages are provided as global variables with names of the form @a cel_errmsg, @a prj_errmsg, etc. by including the relevant header file. As of version 4.8, courtesy of Michael Droettboom @ref software "(pywcs)", WCSLIB has a second error messaging system which provides more detailed information about errors, including the function, source file, and line number where the error occurred. For example, @verbatim struct wcsprm wcs; /* Enable wcserr and send messages to stderr. */ wcserr_enable(1); wcsprintf_set(stderr); ... if (wcsset(&wcs) { wcsperr(&wcs); return wcs.err->status; } @endverbatim In this example, if an error was generated in one of the prjset() functions, wcsperr() would print an error traceback starting with wcsset(), then celset(), and finally the particular projection-setting function that generated the error. For each of them it would print the status return value, function name, source file, line number, and an error message which may be more specific and informative than the general error messages reported in the first example. For example, in response to a deliberately generated error, the @c twcs test program, which tests wcserr among other things, produces a traceback similar to this: @verbatim ERROR 5 in wcsset() at line 1564 of file wcs.c: Invalid parameter value. ERROR 2 in celset() at line 196 of file cel.c: Invalid projection parameters. ERROR 2 in bonset() at line 5727 of file prj.c: Invalid parameters for Bonne's projection. @endverbatim Each of the @ref structs "structs" in @ref overview "WCSLIB" includes a pointer, called @a err, to a wcserr struct. When an error occurs, a struct is allocated and error information stored in it. The wcserr pointers and the @ref memory "memory" allocated for them are managed by the routines that manage the various structs such as wcsini() and wcsfree(). wcserr messaging is an opt-in system enabled via wcserr_enable(), as in the example above. If enabled, when an error occurs it is the user's responsibility to free the memory allocated for the error message using wcsfree(), celfree(), prjfree(), etc. Failure to do so before the struct goes out of scope will result in memory leaks (if execution continues beyond the error). */ /** @page vector Vector API WCSLIB's API is vector-oriented. At the least, this allows the function call overhead to be amortised by spreading it over multiple coordinate transformations. However, vector computations may provide an opportunity for caching intermediate calculations and this can produce much more significant efficiencies. For example, many of the spherical projection equations are partially or fully separable in the mathematical sense, i.e. @f$ (x,y) = f(\phi) g(\theta) @f$, so if @f$ \theta @f$ was invariant for a set of coordinate transformations then @f$ g(\theta) @f$ would only need to be computed once. Depending on the circumstances, this may well lead to speedups of a factor of two or more. WCSLIB has two different categories of vector API: - Certain steps in the WCS algorithm chain operate on coordinate vectors as a whole rather than particular elements of it. For example, the linear transformation takes one or more pixel coordinate vectors, multiples by the transformation matrix, and returns whole intermediate world coordinate vectors. @n The routines that implement these steps, wcsp2s(), wcss2p(), linp2x(), linx2p(), tabx2s(), and tabs2x(), accept and return two-dimensional arrays, i.e. a number of coordinate vectors. Because WCSLIB permits these arrays to contain unused elements, three parameters are needed to describe them: - @a naxis: the number of coordinate elements, as per the FITS @c NAXIS or @c WCSAXES keyvalues, - @a ncoord: the number of coordinate vectors, - @a nelem: the total number of elements in each vector, unused as well as used. Clearly, @a nelem must equal or exceed @a naxis. (Note that when @a ncoord is unity, @a nelem is irrelevant and so is ignored. It may be set to 0.) . @a ncoord and @a nelem are specified as function arguments while @a naxis is provided as a member of the wcsprm (or linprm) struct. @n For example, wcss2p() accepts an array of world coordinate vectors, world[ncoord][nelem]. In the following example, @a naxis = 4, @a ncoord = 5, and @a nelem = 7: @verbatim s1 x1 y1 t1 u u u s2 x2 y2 t2 u u u s3 x3 y3 t3 u u u s4 x4 y4 t4 u u u s5 x5 y5 t5 u u u @endverbatim where @a u indicates unused array elements, and the array is laid out in memory as @verbatim s1 x1 y1 t1 u u u s2 x2 y2 ... @endverbatim @b Note that the stat[] vector returned by routines in this category is of length @a ncoord, as are the intermediate phi[] and theta[] vectors returned by wcsp2s() and wcss2p(). @n @b Note also that the function prototypes for routines in this category have to declare these two-dimensional arrays as one-dimensional vectors in order to avoid warnings from the C compiler about declaration of "incomplete types". This was considered preferable to declaring them as simple pointers-to-double which gives no indication that storage is associated with them. - Other steps in the WCS algorithm chain typically operate only on a part of the coordinate vector. For example, a spectral transformation operates on only one element of an intermediate world coordinate that may also contain celestial coordinate elements. In the above example, spcx2s() might operate only on the @a s (spectral) coordinate elements. @n Routines like spcx2s() and celx2s() that implement these steps accept and return one-dimensional vectors in which the coordinate element of interest is specified via a starting address, a length, and a stride. To continue the previous example, the starting address for the spectral elements is @a s1, the length is 5, and the stride is 7. @section lengths Vector lengths Routines such as spcx2s() and celx2s() accept and return either one coordinate vector, or a pair of coordinate vectors (one-dimensional C arrays). As explained above, the coordinate elements of interest are usually embedded in a two-dimensional array and must be selected by specifying a starting point, length and stride through the array. For routines such as spcx2s() that operate on a single element of each coordinate vector these parameters have a straightforward interpretation. However, for routines such as celx2s() that operate on a pair of elements in each coordinate vector, WCSLIB allows these parameters to be specified independently for each input vector, thereby providing a much more general interpretation than strictly needed to traverse an array. This is best described by illustration. The following diagram describes the situation for cels2x(), as a specific example, with nlng = 5, and nlat = 3: @verbatim lng[0] lng[1] lng[2] lng[3] lng[4] ------ ------ ------ ------ ------ lat[0] | x,y[0] x,y[1] x,y[2] x,y[3] x,y[4] lat[1] | x,y[5] x,y[6] x,y[7] x,y[8] x,y[9] lat[2] | x,y[10] x,y[11] x,y[12] x,y[13] x,y[14] @endverbatim In this case, while only 5 longitude elements and 3 latitude elements are specified, the world-to-pixel routine would calculate nlng * nlat = 15 (x,y) coordinate pairs. It is the responsibility of the caller to ensure that sufficient space has been allocated in all of the output arrays, in this case phi[], theta[], x[], y[] and stat[]. Vector computation will often be required where neither @a lng nor @a lat is constant. This is accomplished by setting @a nlat = 0 which is interpreted to mean nlat = nlng but only the matrix diagonal is to be computed. Thus, for nlng = 3 and nlat = 0 only three (x,y) coordinate pairs are computed: @verbatim lng[0] lng[1] lng[2] ------ ------ ------ lat[0] | x,y[0] lat[1] | x,y[1] lat[2] | x,y[2] @endverbatim Note how this differs from nlng = 3, nlat = 1: @verbatim lng[0] lng[1] lng[2] ------ ------ ------ lat[0] | x,y[0] x,y[1] x,y[2] @endverbatim The situation for celx2s() is similar; the x-coordinate (like @a lng) varies fastest. Similar comments can be made for all routines that accept arguments specifying vector length(s) and stride(s). (tabx2s() and tabs2x() do not fall into this category because the @c -TAB algorithm is fully N-dimensional so there is no way to know in advance how many coordinate elements may be involved.) The reason that WCSLIB allows this generality is related to the aforementioned opportunities that vector computations may provide for caching intermediate calculations and the significant efficiencies that can result. The high-level routines, wcsp2s() and wcss2p(), look for opportunities to collapse a set of coordinate transformations where one of the coordinate elements is invariant, and the low-level routines take advantage of such to cache intermediate calculations. @section strides Vector strides As explained above, the vector stride arguments allow the caller to specify that successive elements of a vector are not contiguous in memory. This applies equally to vectors given to, or returned from a function. As a further example consider the following two arrangements in memory of the elements of four (x,y) coordinate pairs together with an @a s coordinate element (e.g. spectral): - x1 x2 x3 x4 y1 y2 y3 y4 s1 s2 s3 s4 @n the address of x[] is @a x1, its stride is 1, and length 4, @n the address of y[] is @a y1, its stride is 1, and length 4, @n the address of s[] is @a s1, its stride is 1, and length 4. - x1 y1 s1 x2 y2 s2 x3 y3 s3 x4 y4 s4 @n the address of x[] is @a x1, its stride is 3, and length 4, @n the address of y[] is @a y1, its stride is 3, and length 4, @n the address of s[] is @a s1, its stride is 3, and length 4. For routines such as cels2x(), each of the pair of input vectors is assumed to have the same stride. Each of the output vectors also has the same stride, though it may differ from the input stride. For example, for cels2x() the input lng[] and lat[] vectors each have vector stride @a sll, while the x[] and y[] output vectors have stride @a sxy. However, the intermediate phi[] and theta[] arrays each have unit stride, as does the stat[] vector. If the vector length is 1 then the stride is irrelevant and so ignored. It may be set to 0. */ /** @page threads Thread-safety With the following exceptions WCSLIB 4.10 is thread-safe: - The C code generated by Flex is not re-entrant. Flex does have the capacity for producing re-entrant scanners but they have a different API. This may be handled by a compile-time option in future but in the meantime calls to the header parsers should be serialized via a mutex. - The low-level functions wcsnpv() and wcsnps() are not thread-safe but within the library itself they are only used by the Flex scanners wcspih() and wcsbth(). They would rarely need to be used by application programmers. - Diagnostic functions that print the contents of the various structs, namely celprt(), linprt(), prjprt(), spcprt(), tabprt(), wcsprt(), and wcsperr() use printf() which is thread-safe by the POSIX requirement on @c stdio. However, this is only at the function level. Where multiple threads invoke these functions simultaneously their output is likely to be interleaved. - wcserr_enable() sets a static variable and so is not thread-safe. However, this facility is not intended to be used dynamically. If detailed error messages are required, enable wcserr when execution starts and don't change it. */ /** @page testing Example code, testing and verification WCSLIB has an extensive test suite that also provides programming templates as well as demonstrations. Test programs, with names that indicate the main WCSLIB routine under test, reside in @c ./{C,Fortran}/test and each contains a brief description of its purpose. The high- and middle-level test programs are more instructive for applications programming, while the low-level tests are vital for verifying the integrity of the mathematical routines. - High level: @n @a twcstab provides an example of high-level applications programming using WCSLIB and @ref software "CFITSIO". It constructs an input FITS test file, specifically for testing TAB coordinates, partly using @c wcstab.keyrec, and then extracts the coordinate description from it following the steps outlined in wcshdr.h. @n@n @a tpih1 and @a tpih2 verify wcspih(). The first prints the contents of the structs returned by wcspih() using wcsprt() and the second uses @a cpgsbox() to draw coordinate graticules. Input for these comes from a FITS WCS test header implemented as a list of keyrecords, @c wcs.keyrec, one keyrecord per line, together with a program, @a tofits, that compiles these into a valid FITS file. @n@n @a tfitshdr also uses @c wcs.keyrec to test the generic FITS header parsing routine. @n@n @a twcsfix sets up a wcsprm struct containing various non-standard constructs and then invokes wcsfix() to translate them all to standard usage. - Middle level: @n @a twcs tests closure of wcss2p() and wcsp2s() for a number of selected projections. @a twcsmix verifies wcsmix() on the @f$1^\circ@f$ grid of celestial longitude and latitude for a number of selected projections. It plots a test grid for each projection and indicates the location of successful and failed solutions. @a twcssub tests the extraction of a coordinate description for a subimage from a wcsprm struct by wcssub(). @n@n @a tunits tests wcsutrne(), wcsunitse() and wcsulexe(), the units specification translator, converter and parser, either interactively or using a list of units specifications contained in units_test. - Low level: @n @a tlin, @a tlog, @a tprj1, @a tsph, @a tspc, @a tspc, and ttab1 test "closure" of the respective routines. Closure tests apply the forward and reverse transformations in sequence and compare the result with the original value. Ideally, the result should agree exactly, but because of floating point rounding errors there is usually a small discrepancy so it is only required to agree within a "closure tolerance". @n@n @a tprj1 tests for closure separately for longitude and latitude except at the poles where it only tests for closure in latitude. Note that closure in longitude does not deal with angular displacements on the sky. This is appropriate for many projections such as the cylindricals where circumpolar parallels are projected at the same length as the equator. On the other hand, @a tsph does test for closure in angular displacement. @n@n The tolerance for reporting closure discrepancies is set at @f$10^{-10}@f$ degree for most projections; this is slightly less than 3 microarcsec. The worst case closure figure is reported for each projection and this is usually better than the reporting tolerance by several orders of magnitude. @a tprj1 and @a tsph test closure at all points on the @f$1^\circ@f$ grid of native longitude and latitude and to within @f$5^\circ@f$ of any latitude of divergence for those projections that cannot represent the full sphere. Closure is also tested at a sequence of points close to the reference point (@a tprj1) or pole (@a tsph). @n@n Closure has been verified at all test points for SUN workstations. However, non-closure may be observed for other machines near native latitude @f$-90^\circ@f$ for the zenithal, cylindrical and conic equal area projections (ZEA, CEA and COE), and near divergent latitudes of projections such as the azimuthal perspective and stereographic projections (AZP and STG). Rounding errors may also carry points between faces of the quad-cube projections (CSC, QSC, and TSC). Although such excursions may produce long lists of non-closure points, this is not necessarily indicative of a fundamental problem. @n@n Note that the inverse of the COBE quad-qube projection (CSC) is a polynomial approximation and its closure tolerance is intrinsically poor. @n@n Although tests for closure help to verify the internal consistency of the routines they do not verify them in an absolute sense. This is partly addressed by @a tcel1, @a tcel2, @a tprj2, @a ttab2 and @a ttab3 which plot graticules for visual inspection of scaling, orientation, and other macroscopic characteristics of the projections. */ /** @page fortran WCSLIB Fortran wrappers The Fortran subdirectory contains wrappers, written in C, that allow Fortran programs to use WCSLIB. A prerequisite for using the wrappers is an understanding of the usage of the associated C routines, in particular the data structures they are based on. The principle difficulty in creating the wrappers was the need to manage these C structs from within Fortran, particularly as they contain pointers to allocated memory, pointers to C functions, and other structs that themselves contain similar entities. To this end, routines have been provided to set and retrieve values of the various structs, for example @c WCSPUT and @c WCSGET for the wcsprm struct, and @c CELPUT and @c CELGET for the celprm struct. These must be used in conjunction with wrappers on the routines provided to manage the structs in C, for example @c WCSINI, @c WCSSUB, @c WCSCOPY, @c WCSFREE, and @c WCSPRT which wrap wcsini(), wcssub(), wcscopy(), wcsfree(), and wcsprt(). The various @c *PUT and @c *GET routines are based on codes defined in Fortran include files (*.inc), if your Fortran compiler does not support the @c INCLUDE statement then you will need to include these manually wherever necessary. Codes are defined as parameters with names like @c WCS_CRPIX which refers to wcsprm::crpix (if your Fortran compiler does not support long symbolic names then you will need to rename these). The include files also contain parameters, such as @c WCSLEN, that define the length of an @c INTEGER array that must be declared to hold the struct. This length may differ for different platforms depending on how the C compiler aligns data within the structs. A test program for the C library, @a twcs, prints the size of the struct in sizeof(int) units and the values in the Fortran include files must equal or exceed these. On some platforms, such as Suns, it is important that the start of the @c INTEGER array be aligned on a @c DOUBLE @c PRECISION boundary, otherwise a @c BUS error may result. This may be achieved via an @c EQUIVALENCE with a @c DOUBLE @c PRECISION variable, or by sequencing variables in a @c COMMON block so that the @c INTEGER array follows immediately after a @c DOUBLE @c PRECISION variable. The @c *PUT routines set only one element of an array at a time; the final one or two integer arguments of these routines specify 1-relative array indices (N.B. not 0-relative as in C). The one exception is the prjprm::pv array. The @c *PUT routines also reset the @a flag element to signal that the struct needs to be reinitialized. Therefore, if you wanted to set wcsprm::flag itself to -1 prior to the first call to @c WCSINI, for example, then that @c WCSPUT must be the last one before the call. The @c *GET routines retrieve whole arrays at a time and expect array arguments of the appropriate length where necessary. Note that they do not initialize the structs. A basic coding fragment is @verbatim INTEGER LNGIDX, STATUS CHARACTER CTYPE1*72 INCLUDE 'wcs.inc' * WCSLEN is defined as a parameter in wcs.inc. INTEGER WCS(WCSLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS, DUMMY) * Allocate memory and set default values for 2 axes. STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) STATUS = WCSINI (2, WCS) * Set CRPIX1, and CRPIX2; WCS_CRPIX is defined in wcs.inc. STATUS = WCSPUT (WCS, WCS_CRPIX, 512D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 512D0, 2, 0) * Set PC1_2 to 5.0 (I = 1, J = 2). STATUS = WCSPUT (WCS, WCS_PC, 5D0, 1, 2) * Set CTYPE1 to 'RA---SIN'; N.B. must be given as CHARACTER*72. CTYPE1 = 'RA---SIN' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE1, 1, 0) * Set PV1_3 to -1.0 (I = 1, M = 3). STATUS = WCSPUT (WCS, WCS_PV, -1D0, 1, 3) etc. * Initialize. STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN CALL FLUSH(6) STATUS = WCSPERR(WCS, CHAR(0)) ENDIF * Find the "longitude" axis. STATUS = WCSGET (WCS, WCS_LNG, LNGIDX) * Free memory. STATUS = WCSFREE (WCS) @endverbatim Refer to the various Fortran test programs for further programming examples. In particular, @a twcs and @a twcsmix show how to retrieve elements of the celprm and prjprm structs contained within the wcsprm struct. Note that the data type of the third argument to the @c *PUT and @c *GET routines differs depending on the data type of the corresponding C struct member, be it @a int, @a double, or @a char[]. It is essential that the Fortran data type match that of the C struct for @a int and @a double types, and be a @c CHARACTER variable of the correct length for @a char[] types. Compilers (e.g. g77) may warn of inconsistent usage of this argument but this can (usually) be safely ignored. If these warnings become annoying, type-specific variants are provided for each of the @c *PUT routines, @c *PTI, @c *PTD, and @c *PTC for @a int, @a double, or @a char[] and likewise @c *GTI, @c *GTD, and @c *GTC for the @c *GET routines. When calling wrappers for C functions that print to @a stdout, such as @c WCSPRT, and @c WCSPERR, or that may print to @a stderr, such as @c WCSPIH, @c WCSBTH, @c WCSULEXE, or @c WCSUTRNE, it may be necessary to flush the Fortran I/O buffers beforehand so that the output appears in the correct order. The wrappers for these functions do call @c fflush(NULL), but depending on the particular system, this may not succeed in flushing the Fortran I/O buffers. Most Fortran compilers provide the non-standard intrinsic @c FLUSH(), which is called with unit number 6 to flush @a stdout (as in the example above), and unit 0 for @a stderr. A basic assumption made by the wrappers is that an @c INTEGER variable is no less than half the size of a @c DOUBLE @c PRECISION. */ /** @page pgsbox PGSBOX @c PGSBOX, which is provided as a separate part of WCSLIB, is a @ref software "PGPLOT" routine (PGPLOT being a Fortran graphics library) that draws and labels curvilinear coordinate grids. Example @c PGSBOX grids can be seen at http://www.atnf.csiro.au/~mcalabre/WCS/PGSBOX/index.html. The prologue to pgsbox.f contains usage instructions. pgtest.f and cpgtest.c serve as test and demonstration programs in Fortran and C and also as well- documented examples of usage. @c PGSBOX requires a separate routine, @c EXTERNAL @c NLFUNC, to define the coordinate transformation. Fortran subroutine @c PGCRFN (pgcrfn.f) is provided to define separable pairs of non-linear coordinate systems. Linear, logarithmic and power-law axis types are currently defined; further types may be added as required. A C function, @a pgwcsl_(), with Fortran-like interface defines an @c NLFUNC that interfaces to WCSLIB 4.x for @c PGSBOX to draw celestial coordinate grids. @ref software "PGPLOT" is implemented as a Fortran library with a set of C wrapper routines that are generated by a software tool. However, @c PGSBOX has a more complicated interface than any of the standard PGPLOT routines, especially in having an @c EXTERNAL function in its argument list. Consequently, @c PGSBOX is implemented in Fortran but with a hand-coded C wrapper, @a cpgsbox(). As an example, in this suite the C test/demo program, @a cpgtest, calls the C wrapper, @a cpgsbox(), passing it a pointer to @a pgwcsl_(). In turn, @a cpgsbox() calls @c PGSBOX, which invokes @a pgwcsl_() as an @c EXTERNAL subroutine. In this sequence, a complicated C struct defined by @a cpgtest is passed through @c PGSBOX to @a pgwcsl_() as an @c INTEGER array. While there are no formal standards for calling Fortran from C, there are some fairly well established conventions. Nevertheless, it's possible that you may need to modify the code if you use a combination of Fortran and C compilers with linkage conventions that differ from that of the GNU compilers, gcc and g77. */ /* Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: mainpage.dox,v 4.10 2012/02/05 23:41:45 cal103 Exp $ */ pywcs-1.12/wcslib/doxygen/prj.sed0000644001153600020070000000272012310355626021077 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|PVi_\([0-4]\)a|PVi_\1a|g s| prjprm| #prjprm|g s|???set()|&|g s|???x2s()|&|g s|???s2x()|&|g s|AIR|&|g s|AIT|&|g s|ARC|&|g s|AZP|&|g s|BON|&|g s|CAR|&|g s|CEA|&|g s|COD|&|g s|COE|&|g s|COO|&|g s|COP|&|g s|CSC|&|g s|CYP|&|g s|HPX|&|g s|MER|&|g s|MOL|&|g s|PAR|&|g s|PCO|&|g s|QSC|&|g s|SFL|&|g s|SIN|&|g s|STG|&|g s|SZP|&|g s|TAN|&|g s|TSC|&|g s|ZEA|&|g s|ZPN|&|g s| i | i |g s|carree|car\ée|g s|\[-90,90\]|@f$[-90^\\circ,90^\\circ]@f$|g s|\[-180,180\]|@f$[-180^\\circ,180^\\circ]@f$|g s|180/pi|@f$180^\\circ/\\pi@f$|g s|\([1-9][0-9]*\) degrees|@f$\1^\\circ@f$|g s| 1 degree | @f$1^\\circ@f$ degree |g s| 1E-10 degree | @f$0^\\circ.0000000001@f$ |g s| phi\([ .]\)| @f$\\phi@f$\1|g s| phi, | @f$\\phi@f$, |g s| theta\([ .]\)| @f$\\theta@f$\1|g s| theta, | @f$\\theta@f$, |g s|phi_0|@f$\\phi_0@f$|g s|theta_0|@f$\\theta_0@f$|g s|(phi,theta)|@f$(\\phi,\\theta)@f$|g s|(x,y)|@f$(x,y)@f$|g s| x, | @f$x@f$,|g s| x\([ .]\)| @f$x@f$\1|g s| y, | @f$y@f$,|g s| y\([ .]\)| @f$y@f$\1|g pywcs-1.12/wcslib/doxygen/prj_extras.dox0000644001153600020070000007616412310355626022521 0ustar cslocumSTSCI\science00000000000000/** @fn int azpset(struct prjprm *prj) * * @brief Set up a #prjprm struct for * the zenithal/azimuthal perspective (AZP) * projection. * * @b %azpset() sets up a #prjprm struct for * a zenithal/azimuthal perspective (AZP) * projection. * * See prjset() for a description of the API. */ /** @fn int azpx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * zenithal/azimuthal perspective (AZP) * projection. * * @b %azpx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal perspective (AZP) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int azps2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * zenithal/azimuthal perspective (AZP) * projection. * * @b %azps2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal perspective (AZP) * projection. * * See prjs2x() for a description of the API. */ /** @fn int szpset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * slant zenithal perspective (SZP) * projection. * * @b %szpset() sets up a #prjprm struct for * a slant zenithal perspective (SZP) * projection. * * See prjset() for a description of the API. */ /** @fn int szpx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * slant zenithal perspective (SZP) * projection. * * @b %szpx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a slant zenithal perspective (SZP) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int szps2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * slant zenithal perspective (SZP) * projection. * * @b %szps2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a slant zenithal perspective (SZP) * projection. * * See prjs2x() for a description of the API. */ /** @fn int tanset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * gnomonic (TAN) * projection. * * @b %tanset() sets up a #prjprm struct for * a gnomonic (TAN) * projection. * * See prjset() for a description of the API. */ /** @fn int tanx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * gnomonic (TAN) * projection. * * @b %tanx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a gnomonic (TAN) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int tans2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * gnomonic (TAN) * projection. * * @b %tans2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a gnomonic (TAN) * projection. * * See prjs2x() for a description of the API. */ /** @fn int stgset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * stereographic (STG) * projection. * * @b %stgset() sets up a #prjprm struct for * a stereographic (STG) * projection. * * See prjset() for a description of the API. */ /** @fn int stgx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * stereographic (STG) * projection. * * @b %stgx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a stereographic (STG) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int stgs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * stereographic (STG) * projection. * * @b %stgs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a stereographic (STG) * projection. * * See prjs2x() for a description of the API. */ /** @fn int sinset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * orthographic/synthesis (SIN) * projection. * * @b %stgset() sets up a #prjprm struct for * an orthographic/synthesis (SIN) * projection. * * See prjset() for a description of the API. */ /** @fn int sinx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * orthographic/synthesis (SIN) * projection. * * @b %sinx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * an orthographic/synthesis (SIN) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int sins2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * orthographic/synthesis (SIN) * projection. * * @b %sins2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * an orthographic/synthesis (SIN) * projection. * * See prjs2x() for a description of the API. */ /** @fn int arcset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * zenithal/azimuthal equidistant (ARC) * projection. * * @b %arcset() sets up a #prjprm struct for * a zenithal/azimuthal equidistant (ARC) * projection. * * See prjset() for a description of the API. */ /** @fn int arcx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * zenithal/azimuthal equidistant (ARC) * projection. * * @b %arcx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal equidistant (ARC) * projection to native spherical * coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int arcs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * zenithal/azimuthal equidistant (ARC) * projection. * * @b %arcs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal equidistant (ARC) * projection. * * See prjs2x() for a description of the API. */ /** @fn int zpnset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * zenithal/azimuthal polynomial (ZPN) * projection. * * @b %zpnset() sets up a #prjprm struct for * a zenithal/azimuthal polynomial (ZPN) * projection. * * See prjset() for a description of the API. */ /** @fn int zpnx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * zenithal/azimuthal polynomial (ZPN) * projection. * * @b %zpnx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal polynomial (ZPN) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int zpns2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * zenithal/azimuthal polynomial (ZPN) * projection. * * @b %zpns2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal polynomial (ZPN) * projection. * * See prjs2x() for a description of the API. */ /** @fn int zeaset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * zenithal/azimuthal equal area (ZEA) * projection. * * @b %zeaset() sets up a #prjprm struct for * a zenithal/azimuthal equal area (ZEA) * projection. * * See prjset() for a description of the API. */ /** @fn int zeax2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * zenithal/azimuthal equal area (ZEA) * projection. * * @b %zeax2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal equal area (ZEA) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int zeas2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * zenithal/azimuthal equal area (ZEA) * projection. * * @b %zeas2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a zenithal/azimuthal equal area (ZEA) * projection. * * See prjs2x() for a description of the API. */ /** @fn int airset(struct prjprm *prj) * * @brief Set up a #prjprm struct for * Airy's (AIR) * projection. * * @b %airset() sets up a #prjprm struct for * an Airy (AIR) * projection. * * See prjset() for a description of the API. */ /** @fn int airx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for * Airy's (AIR) * projection. * * @b %airx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * an Airy (AIR) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int airs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for * Airy's (AIR) * projection. * * @b %airs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * an Airy (AIR) * projection. * * See prjs2x() for a description of the API. */ /** @fn int cypset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * cylindrical perspective (CYP) * projection. * * @b %cypset() sets up a #prjprm struct for * a cylindrical perspective (CYP) * projection. * * See prjset() for a description of the API. */ /** @fn int cypx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * cylindrical perspective (CYP) * projection. * * @b %cypx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a cylindrical perspective (CYP) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int cyps2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * cylindrical perspective (CYP) * projection. * * @b %cyps2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a cylindrical perspective (CYP) * projection. * * See prjs2x() for a description of the API. */ /** @fn int ceaset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * cylindrical equal area (CEA) * projection. * * @b %ceaset() sets up a #prjprm struct for * a cylindrical equal area (CEA) * projection. * * See prjset() for a description of the API. */ /** @fn int ceax2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * cylindrical equal area (CEA) * projection. * * @b %ceax2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a cylindrical equal area (CEA) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int ceas2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * cylindrical equal area (CEA) * projection. * * @b %ceas2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a cylindrical equal area (CEA) * projection. * * See prjs2x() for a description of the API. */ /** @fn int carset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * plate carrée (CAR) * projection. * * @b %carset() sets up a #prjprm struct for * a plate carrée (CAR) * projection. * * See prjset() for a description of the API. */ /** @fn int carx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * plate carrée (CAR) * projection. * * @b %carx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a plate carrée (CAR) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int cars2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * plate carrée (CAR) * projection. * * @b %cars2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a plate carrée (CAR) * projection. * * See prjs2x() for a description of the API. */ /** @fn int merset(struct prjprm *prj) * * @brief Set up a #prjprm struct for * Mercator's (MER) * projection. * * @b %merset() sets up a #prjprm struct for * a Mercator (MER) * projection. * * See prjset() for a description of the API. */ /** @fn int merx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for * Mercator's (MER) * projection. * * @b %merx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a Mercator (MER) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int mers2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for * Mercator's (MER) * projection. * * @b %mers2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a Mercator (MER) * projection. * * See prjs2x() for a description of the API. */ /** @fn int sflset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * Sanson-Flamsteed (SFL) * projection. * * @b %sflset() sets up a #prjprm struct for * a Sanson-Flamsteed (SFL) * projection. * * See prjset() for a description of the API. */ /** @fn int sflx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * Sanson-Flamsteed (SFL) * projection. * * @b %sflx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a Sanson-Flamsteed (SFL) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int sfls2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * Sanson-Flamsteed (SFL) * projection. * * @b %sfls2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a Sanson-Flamsteed (SFL) * projection. * * See prjs2x() for a description of the API. */ /** @fn int parset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * parabolic (PAR) * projection. * * @b %parset() sets up a #prjprm struct for * a parabolic (PAR) * projection. * * See prjset() for a description of the API. */ /** @fn int parx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * parabolic (PAR) * projection. * * @b %parx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a parabolic (PAR) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int pars2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * parabolic (PAR) * projection. * * @b %pars2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a parabolic (PAR) * projection. * * See prjs2x() for a description of the API. */ /** @fn int molset(struct prjprm *prj) * * @brief Set up a #prjprm struct for * Mollweide's (MOL) * projection. * * @b %molset() sets up a #prjprm struct for * a Mollweide (MOL) * projection. * * See prjset() for a description of the API. */ /** @fn int molx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for * Mollweide's (MOL) * projection. * * @b %molx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a Mollweide (MOL) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int mols2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for * Mollweide's (MOL) * projection. * * @b %mols2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a Mollweide (MOL) * projection. * * See prjs2x() for a description of the API. */ /** @fn int aitset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * Hammer-Aitoff (AIT) * projection. * * @b %aitset() sets up a #prjprm struct for * a Hammer-Aitoff (AIT) * projection. * * See prjset() for a description of the API. */ /** @fn int aitx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * Hammer-Aitoff (AIT) * projection. * * @b %aitx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a Hammer-Aitoff (AIT) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int aits2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * Hammer-Aitoff (AIT) * projection. * * @b %aits2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a Hammer-Aitoff (AIT) * projection. * * See prjs2x() for a description of the API. */ /** @fn int copset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * conic perspective (COP) * projection. * * @b %copset() sets up a #prjprm struct for * a conic perspective (COP) * projection. * * See prjset() for a description of the API. */ /** @fn int copx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * conic perspective (COP) * projection. * * @b %copx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic perspective (COP) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int cops2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * conic perspective (COP) * projection. * * @b %cops2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic perspective (COP) * projection. * * See prjs2x() for a description of the API. */ /** @fn int coeset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * conic equal area (COE) * projection. * * @b %coeset() sets up a #prjprm struct for * a conic equal area (COE) * projection. * * See prjset() for a description of the API. */ /** @fn int coex2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * conic equal area (COE) * projection. * * @b %coex2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic equal area (COE) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int coes2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * conic equal area (COE) * projection. * * @b %coes2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic equal area (COE) * projection. * * See prjs2x() for a description of the API. */ /** @fn int codset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * conic equidistant (COD) * projection. * * @b %codset() sets up a #prjprm struct for * a conic equidistant (COD) * projection. * * See prjset() for a description of the API. */ /** @fn int codx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * conic equidistant (COD) * projection. * * @b %codx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic equidistant (COD) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int cods2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * conic equidistant (COD) * projection. * * @b %cods2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic equidistant (COD) * projection. * * See prjs2x() for a description of the API. */ /** @fn int cooset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * conic orthomorphic (COO) * projection. * * @b %cooset() sets up a #prjprm struct for * a conic orthomorphic (COO) * projection. * * See prjset() for a description of the API. */ /** @fn int coox2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * conic orthomorphic (COO) * projection. * * @b %coox2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic orthomorphic (COO) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int coos2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * conic orthomorphic (COO) * projection. * * @b %coos2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a conic orthomorphic (COO) * projection. * * See prjs2x() for a description of the API. */ /** @fn int bonset(struct prjprm *prj) * * @brief Set up a #prjprm struct for * Bonne's (BON) * projection. * * @b %bonset() sets up a #prjprm struct for * a Bonne (BON) * projection. * * See prjset() for a description of the API. */ /** @fn int bonx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for * Bonne's (BON) * projection. * * @b %bonx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a Bonne (BON) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int bons2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for * Bonne's (BON) * projection. * * @b %bons2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a Bonne (BON) * projection. * * See prjs2x() for a description of the API. */ /** @fn int pcoset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * polyconic (PCO) * projection. * * @b %pcoset() sets up a #prjprm struct for * a polyconic (PCO) * projection. * * See prjset() for a description of the API. */ /** @fn int pcox2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * polyconic (PCO) * projection. * * @b %pcox2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a polyconic (PCO) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int pcos2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * polyconic (PCO) * projection. * * @b %pcos2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a polyconic (PCO) * projection. * * See prjs2x() for a description of the API. */ /** @fn int tscset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * tangential spherical cube (TSC) * projection. * * @b %tscset() sets up a #prjprm struct for * a tangential spherical cube (TSC) * projection. * * See prjset() for a description of the API. */ /** @fn int tscx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * tangential spherical cube (TSC) * projection. * * @b %tscx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a tangential spherical cube (TSC) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int tscs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * tangential spherical cube (TSC) * projection. * * @b %tscs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a tangential spherical cube (TSC) * projection. * * See prjs2x() for a description of the API. */ /** @fn int cscset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * COBE spherical cube (CSC) * projection. * * @b %cscset() sets up a #prjprm struct for * a COBE spherical cube (CSC) * projection. * * See prjset() for a description of the API. */ /** @fn int cscx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * COBE spherical cube (CSC) * projection. * * @b %cscx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a COBE spherical cube (CSC) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int cscs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * COBE spherical cube (CSC) * projection. * * @b %cscs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a COBE spherical cube (CSC) * projection. * * See prjs2x() for a description of the API. */ /** @fn int qscset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * quadrilateralized spherical cube (QSC) * projection. * * @b %qscset() sets up a #prjprm struct for * a quadrilateralized spherical cube (QSC) * projection. * * See prjset() for a description of the API. */ /** @fn int qscx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * quadrilateralized spherical cube (QSC) * projection. * * @b %qscx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a quadrilateralized spherical cube (QSC) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int qscs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * quadrilateralized spherical cube (QSC) * projection. * * @b %qscs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a quadrilateralized spherical cube (QSC) * projection. * * See prjs2x() for a description of the API. */ /** @fn int hpxset(struct prjprm *prj) * * @brief Set up a #prjprm struct for the * HEALPix (HPX) * projection. * * @b %hpxset() sets up a #prjprm struct for * a HEALPix (HPX) * projection. * * See prjset() for a description of the API. */ /** @fn int hpxx2s(PRJX2S_ARGS) * * @brief Cartesian-to-spherical transformation for the * HEALPix (HPX) * projection. * * @b %hpxx2s() deprojects Cartesian \f$(x,y)\f$ coordinates in the plane of * a HEALPix (HPX) * projection to native spherical coordinates \f$(\phi,\theta)\f$. * * See prjx2s() for a description of the API. */ /** @fn int hpxs2x(PRJS2X_ARGS) * * @brief Spherical-to-Cartesian transformation for the * HEALPix (HPX) * projection. * * @b %hpxs2x() projects native spherical coordinates \f$(\phi,\theta)\f$ to * Cartesian \f$(x,y)\f$ coordinates in the plane of * a HEALPix (HPX) * projection. * * See prjs2x() for a description of the API. */ /** @var const int ZENITHAL * @brief Identifier for zenithal/azimuthal projections. * * Identifier for zenithal/azimuthal projections, see prjprm::category. */ /** @var const int CYLINDRICAL * @brief Identifier for cylindrical projections. * * Identifier for cylindrical projections, see prjprm::category. */ /** @var const int PSEUDOCYLINDRICAL * @brief Identifier for pseudocylindrical projections. * * Identifier for pseudocylindrical projections, see prjprm::category. */ /** @var const int CONVENTIONAL * @brief Identifier for conventional projections. * * Identifier for conventional projections, see prjprm::category. */ /** @var const int CONIC * @brief Identifier for conic projections. * * Identifier for conic projections, see prjprm::category. */ /** @var const int POLYCONIC * @brief Identifier for polyconic projections. * * Identifier for polyconic projections, see prjprm::category. */ /** @var const int QUADCUBE * @brief Identifier for quadcube projections. * * Identifier for quadcube projections, see prjprm::category. */ /** @var const int HEALPIX * @brief Identifier for the HEALPix projection. * * Identifier for the HEALPix projection, see prjprm::category. */ /** @var const char prj_categories[9][32] * @brief Projection categories. * * Names of the projection categories, all in lower-case except for "HEALPix". * * Provided for information only, not used by the projection routines. */ /** @var const int prj_ncode * @brief The number of recognized three-letter projection codes. * * The number of recognized three-letter projection codes (currently 27), * see #prj_codes. */ /** @var const char prj_codes[27][4] * @brief Recognized three-letter projection codes. * * List of all recognized three-letter projection codes (currently 27), e.g. * SIN, TAN, etc. */ /** @def PVN * @brief Total number of projection parameters. * * The total number of projection parameters numbered 0 to PVN-1. */ /** @def PRJX2S_ARGS * @brief For use in declaring deprojection function prototypes. * * Preprocessor macro used for declaring deprojection function prototypes. */ /** @def PRJS2X_ARGS * @brief For use in declaring projection function prototypes. * * Preprocessor macro used for declaring projection function prototypes. */ /** @def PRJLEN * @brief Size of the #prjprm struct in @a int units. * * Size of the #prjprm struct in @a int units, used by the Fortran wrappers. */ /** @def prjini_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #prj_errmsg directly now * instead. */ /** @def prjprt_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #prj_errmsg directly now * instead. */ /** @def prjset_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #prj_errmsg directly now * instead. */ /** @def prjx2s_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #prj_errmsg directly now * instead. */ /** @def prjs2x_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #prj_errmsg directly now * instead. */ pywcs-1.12/wcslib/doxygen/README0000644001153600020070000000272412310355626020473 0ustar cslocumSTSCI\science00000000000000Overview of generation of the WCSLIB manual using doxygen --------------------------------------------------------- Documentation is extracted from the C header files using a flex scanner, doxextr (see ./doxextr.l). doxextr relies on strict adherence to a set of formatting rules in order to minimize the amount of doxygen markup required in the C source files. doxextr extracts information from the header files and applies doxygen markup to it. This is passed through a generic sed filter, doxexr.sed, and possibly also a specific sed filter, e.g. prj.sed for prj.h, which applies additional doxygen markup, mainly for fonts and formulae. The makefile rule that drives this process writes the output to a set of files with names of the form *.dox, e.g. prj.dox. Additional doxygen markup may also be provided via files in this directory with names of the form *_extras.dox, e.g. prj_extras.dox. These are maintained manually. Similarly, the main page and explanatory sections of the manual are maintained in mainpage.dox. The makefile rule concatenates ../C/wcslib.h and all of the .dox files in this directory onto ./wcslib.h for input to doxygen which is told via its configuration file, Doxyfile, to ignore ../C/wcslib.h. This subterfuge is necessary to avoid spurious file references in the generated latex manual. Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: README,v 4.10 2012/02/05 23:41:45 cal103 Exp $ pywcs-1.12/wcslib/doxygen/spc.sed0000644001153600020070000000236612310355626021077 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|CTYPEn|CTYPEn|g s|VELREF|&|g s|'AFRQ'|'AFRQ'|g s|'AWAV'|'AWAV'|g s|'BETA'|'BETA'|g s|'ENER'|'ENER'|g s|'FREQ'|'FREQ'|g s|'FELO'|'FELO'|g s|'VELO'|'VELO'|g s|'VOPT'|'VOPT'|g s|'VRAD'|'VRAD'|g s|'WAVE'|'WAVE'|g s|'WAVN'|'WAVN'|g s|'ZOPT'|'ZOPT'|g s|'VELO-F2V'|&|g s|'ZOPT-F2W'|&|g s|'VRAD-V2F'|&|g s|'VOPT-V2W'|&|g s|'ZOPT-V2W'|&|g s|'BETA-W2V'|&|g s|'LOG'|'LOG'|g s|'TAB'|'TAB'|g s|'GRA'|'GRA'|g s|'GRI'|'GRI'|g s|X -> P -> S|@f$X\\leadsto P\\rightarrow S@f$|g s|S -> P -> X|@f$S\\rightarrow P\\leadsto X@f$|g s| \([PSX]\)\([ -.:]\)| @f$\1@f$\2|g s| S | @f$S@f$ |g s| G, | @f$G@f$, |g s| m, | @f$m@f$, |g s|alpha|@f$\\alpha@f$|g s|n_r|@f$n_r@f$|g s|n'_r|@f$n'_r@f$|g s|epsilon|@f$\\epsilon@f$|g s|theta|@f$\\theta@f$|g s|lambda_r|@f$\\lambda_r@f$|g s|dn/dlambda|@f$dn/d\\lambda@f$|g s|dX/dS|@f$dX/dS@f$|g s|dS/dX|@f$dS/dX@f$|g s|restreq%3 != 0|\\code & \\endcode|g pywcs-1.12/wcslib/doxygen/spc_extras.dox0000644001153600020070000000150112310355626022472 0ustar cslocumSTSCI\science00000000000000/** @def SPCLEN * @brief Size of the spcprm struct in @a int units. * * Size of the spcprm struct in @a int units, used by the Fortran wrappers. */ /** @def spcini_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #spc_errmsg directly now * instead. */ /** @def spcprt_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #spc_errmsg directly now * instead. */ /** @def spcset_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #spc_errmsg directly now * instead. */ /** @def spcx2s_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #spc_errmsg directly now * instead. */ /** @def spcs2x_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #spc_errmsg directly now * instead. */ pywcs-1.12/wcslib/doxygen/sph.sed0000644001153600020070000000066112310355626021100 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|dist and pa|dist and pa| s|lng and lat|lng and lat| s|phi and theta|phi and theta| s|\([1-9][0-9]*\) degrees|@f$\1^\\circ@f$|g s|(lng0,+90-epsilon)|@f$(\\alpha_0,+90^\\circ-\\epsilon)@f$| s|(lng0,-90+epsilon)|@f$(\\alpha_0,-90^\\circ+\\epsilon)@f$| s| 0 or | @f$0^\\circ@f$ or | s| epsilon| @f$\\epsilon@f$|g s|cos(|@f$cos@f$(|g s|sin(|@f$sin@f$(|g pywcs-1.12/wcslib/doxygen/spx.sed0000644001153600020070000000105312310355626021114 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|AFRQ|&|g s|AWAV|&|g s|BETA|&|g s|ENER|&|g s|FREQ|&|g s|VELO|&|g s|VOPT|&|g s|VRAD|&|g s|WAVE|&|g s|WAVN|&|g s|ZOPT|&|g s|velotype)|velotype)|g s|(wavetype|(wavetype|g s|= 1 / 2\*pi|@f$= 1 / 2 \\pi@f$|g s|= 2\*pi|@f$= 2 \\pi@f$|g s|= c,|@f$= c@f$,|g s|= 1/c|@f$= 1/c@f$|g s|= h,|@f$= h@f$,|g s|= 1/h|@f$= 1/h@f$|g s|= v/c|@f$\\beta = v/c@f$|g pywcs-1.12/wcslib/doxygen/spx_extras.dox0000644001153600020070000001171412310355626022526 0ustar cslocumSTSCI\science00000000000000/** @fn int afrqfreq(SPX_ARGS) * @brief Convert angular frequency to frequency (vector). * * @b %afrqfreq() converts angular frequency to frequency. * * See freqafrq() for a description of the API. */ /** @fn int freqener(SPX_ARGS) * @brief Convert frequency to photon energy (vector). * * @b %freqener() converts frequency to photon energy. * * See freqafrq() for a description of the API. */ /** @fn int enerfreq(SPX_ARGS) * @brief Convert photon energy to frequency (vector). * * @b %enerfreq() converts photon energy to frequency. * * See freqafrq() for a description of the API. */ /** @fn int freqwavn(SPX_ARGS) * @brief Convert frequency to wave number (vector). * * @b %freqwavn() converts frequency to wave number. * * See freqafrq() for a description of the API. */ /** @fn int wavnfreq(SPX_ARGS) * @brief Convert wave number to frequency (vector). * * @b %wavnfreq() converts wave number to frequency. * * See freqafrq() for a description of the API. */ /** @fn int freqwave(SPX_ARGS) * @brief Convert frequency to vacuum wavelength (vector). * * @b %freqwave() converts frequency to vacuum wavelength. * * See freqafrq() for a description of the API. */ /** @fn int wavefreq(SPX_ARGS) * @brief Convert vacuum wavelength to frequency (vector). * * @b %wavefreq() converts vacuum wavelength to frequency. * * See freqafrq() for a description of the API. */ /** @fn int freqawav(SPX_ARGS) * @brief Convert frequency to air wavelength (vector). * * @b %freqawav() converts frequency to air wavelength. * * See freqafrq() for a description of the API. */ /** @fn int awavfreq(SPX_ARGS) * @brief Convert air wavelength to frequency (vector). * * @b %awavfreq() converts air wavelength to frequency. * * See freqafrq() for a description of the API. */ /** @fn int waveawav(SPX_ARGS) * @brief Convert vacuum wavelength to air wavelength (vector). * * @b %waveawav() converts vacuum wavelength to air wavelength. * * See freqafrq() for a description of the API. */ /** @fn int awavwave(SPX_ARGS) * @brief Convert air wavelength to vacuum wavelength (vector). * * @b %awavwave() converts air wavelength to vacuum wavelength. * * See freqafrq() for a description of the API. */ /** @fn int velobeta(SPX_ARGS) * @brief Convert relativistic velocity to relativistic beta (vector). * * @b %velobeta() converts relativistic velocity to relativistic beta. * * See freqafrq() for a description of the API. */ /** @fn int betavelo(SPX_ARGS) * @brief Convert relativistic beta to relativistic velocity (vector). * * @b %betavelo() converts relativistic beta to relativistic velocity. * * See freqafrq() for a description of the API. */ /** @fn int velofreq(SPX_ARGS) * @brief Convert relativistic velocity to frequency (vector). * * @b %velofreq() converts relativistic velocity to frequency. * * See freqvelo() for a description of the API. */ /** @fn int freqvrad(SPX_ARGS) * @brief Convert frequency to radio velocity (vector). * * @b %freqvrad() converts frequency to radio velocity. * * See freqvelo() for a description of the API. */ /** @fn int vradfreq(SPX_ARGS) * @brief Convert radio velocity to frequency (vector). * * @b %vradfreq() converts radio velocity to frequency. * * See freqvelo() for a description of the API. */ /** @fn int velowave(SPX_ARGS) * @brief Convert relativistic velocity to vacuum wavelength (vector). * * @b %velowave() converts relativistic velocity to vacuum wavelength. * * See freqvelo() for a description of the API. */ /** @fn int awavvelo(SPX_ARGS) * @brief Convert air wavelength to relativistic velocity (vector). * * @b %awavvelo() converts air wavelength to relativistic velocity. * * See freqvelo() for a description of the API. */ /** @fn int veloawav(SPX_ARGS) * @brief Convert relativistic velocity to air wavelength (vector). * * @b %veloawav() converts relativistic velocity to air wavelength. * * See freqvelo() for a description of the API. */ /** @fn int wavevopt(SPX_ARGS) * @brief Convert vacuum wavelength to optical velocity (vector). * * @b %wavevopt() converts vacuum wavelength to optical velocity. * * See freqvelo() for a description of the API. */ /** @fn int voptwave(SPX_ARGS) * @brief Convert optical velocity to vacuum wavelength (vector). * * @b %voptwave() converts optical velocity to vacuum wavelength. * * See freqvelo() for a description of the API. */ /** @fn int wavezopt(SPX_ARGS) * @brief Convert vacuum wavelength to redshift (vector). * * @b %wavevopt() converts vacuum wavelength to redshift. * * See freqvelo() for a description of the API. */ /** @fn int zoptwave(SPX_ARGS) * @brief Convert redshift to vacuum wavelength (vector). * * @b %zoptwave() converts redshift to vacuum wavelength. * * See freqvelo() for a description of the API. */ /** @def SPX_ARGS * @brief For use in declaring spectral conversion function prototypes. * * Preprocessor macro used for declaring spectral conversion function * prototypes. */ /** @def SPXLEN * @brief Size of the spxprm struct in @a int units. * * Size of the spxprm struct in @a int units, used by the Fortran wrappers. */ pywcs-1.12/wcslib/doxygen/tab.sed0000644001153600020070000000036512310355626021055 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|PVi_\([0-4]\)a|PVi_\1a|g s| <= | @f$\\leq@f$ |g s|(K_1, K_2,... K_M)|@f$&@f$|g s| K_1 \* K_2 \* ... \* K_M |@f$K_1 K_2 \\ldots K_M@f$|g s| compressed K_1 | compressed @f$K_1@f$ |g s|Upsilon_m|@f$\\&@f$|g pywcs-1.12/wcslib/doxygen/tab_extras.dox0000644001153600020070000000212412310355626022455 0ustar cslocumSTSCI\science00000000000000/** @def TABLEN * @brief Size of the tabprm struct in @a int units. * * Size of the tabprm struct in @a int units, used by the Fortran wrappers. */ /** @def tabini_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ /** @def tabcpy_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ /** @def tabfree_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ /** @def tabprt_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ /** @def tabset_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ /** @def tabx2s_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ /** @def tabs2x_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #tab_errmsg directly now * instead. */ pywcs-1.12/wcslib/doxygen/wcs.sed0000644001153600020070000000200512310355626021074 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|CROTAia|CROTAia|g s|EPOCH|&|g s|VELREF|&|g s|PVi_\([0-4]\)a|PVi_\1a|g s|'a'|'a'|g s|axis i |axis i |g s|\([^_]\)CUBEFACE|\1CUBEFACE|g s|\([^_]\)STOKES|\1STOKES|g s|'RA--'|'RA--'|g s|'DEC-'|'DEC-'|g s|'GLON'|'GLON'|g s|'GLAT'|'GLAT'|g s|CSC|&|g s|GLS|&|g s|NCP|&|g s|QSC|&|g s|SFL|&|g s|SIN|&|g s|TSC|&|g s|'FREQ'|'FREQ'|g s|'FELO-HEL'|&|g s|'FREQ-LSR'|&|g s|'ZOPT-F2W'|&|g s|yyyy-mm-ddThh:mm:ss|yyyy-mm-ddThh:mm:ss|g s|(phi_0,theta_0)|@f$(\\phi_0,\\theta_0)@f$| s|phi_p|@f$\\phi_{\\mathrm p}@f$|g s|theta_p|@f$\\theta_{\\mathrm p}@f$|g s| x-| @f$x@f$-|g s| y-| @f$y@f$-|g s/altlin |= [124];/\\code & \\endcode/ pywcs-1.12/wcslib/doxygen/wcs_extras.dox0000644001153600020070000000525112310355626022507 0ustar cslocumSTSCI\science00000000000000/** @def WCSSUB_LONGITUDE * @brief Mask for extraction of longitude axis by wcssub(). * * Mask to use for extracting the longitude axis when sub-imaging, refer to the * axes argument of wcssub(). */ /** @def WCSSUB_LATITUDE * @brief Mask for extraction of latitude axis by wcssub(). * * Mask to use for extracting the latitude axis when sub-imaging, refer to the * axes argument of wcssub(). */ /** @def WCSSUB_CUBEFACE * @brief Mask for extraction of CUBEFACE axis by wcssub(). * * Mask to use for extracting the CUBEFACE axis when * sub-imaging, refer to the axes argument of wcssub(). */ /** @def WCSSUB_CELESTIAL * @brief Mask for extraction of celestial axes by wcssub(). * * Mask to use for extracting the celestial axes (longitude, latitude and * cubeface) when sub-imaging, refer to the axes argument of * wcssub(). */ /** @def WCSSUB_SPECTRAL * @brief Mask for extraction of spectral axis by wcssub(). * * Mask to use for extracting the spectral axis when sub-imaging, refer to the * axes argument of wcssub(). */ /** @def WCSSUB_STOKES * @brief Mask for extraction of STOKES axis by wcssub(). * * Mask to use for extracting the STOKES axis when sub-imaging, * refer to the axes argument of wcssub(). */ /** @def WCSLEN * @brief Size of the wcsprm struct in int units. * * Size of the wcsprm struct in @a int units, used by the Fortran wrappers. */ /** @def wcsini_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcssub_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcscopy_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcsfree_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcsprt_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcsset_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcsp2s_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcss2p_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ /** @def wcsmix_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcs_errmsg directly now * instead. */ pywcs-1.12/wcslib/doxygen/wcsfix.sed0000644001153600020070000000143512310355626021611 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|CD00i00j|&|g s|EPOCH|&|g s|PC00i00j|&|g s|PROJPn|&|g s|VELREF|&|g s|VSOURCEa|&|g s|GLS|&|g s|NCP|&|g s|SIN|&|g s|FREQ\([^-]\)|FREQ\1|g s|FELO\([^-]\)|FELO\1|g s|VELO\([^-]\)|VELO\1|g s|\([^-]\)OBS|\1OBS|g s|\([^-]\)LSR|\1LSR|g s|\([^-]\)HEL|\1HEL|g s|'VELO-OBS'|&|g s|'FELO-HEL'|&|g s|'FREQ-LSR'|&|g s|'DEG'|'DEG'|g s|'deg'|'deg'|g s|CLDJ|&|g s|DJCL|&|g s|yyyy-mm-ddThh:mm:ss|yyyy-mm-ddThh:mm:ss|g pywcs-1.12/wcslib/doxygen/wcsfix_extras.dox0000644001153600020070000000262112310355626023214 0ustar cslocumSTSCI\science00000000000000/** @def CDFIX * @brief Index of cdfix() status value in vector returned by wcsfix(). * * Index of the status value returned by cdfix() in the status * vector returned by wcsfix(). */ /** @def DATFIX * @brief Index of datfix() status value in vector returned by wcsfix(). * * Index of the status value returned by datfix() in the status vector * returned by wcsfix(). */ /** @def UNITFIX * @brief Index of unitfix() status value in vector returned by wcsfix(). * * Index of the status value returned by unitfix() in the status vector * returned by wcsfix(). */ /** @def CELFIX * @brief Index of celfix() status value in vector returned by wcsfix(). * * Index of the status value returned by celfix() in the status vector * returned by wcsfix(). */ /** @def SPCFIX * @brief Index of spcfix() status value in vector returned by wcsfix(). * * Index of the status value returned by spcfix() in the status vector * returned by wcsfix(). */ /** @def CYLFIX * @brief Index of cylfix() status value in vector returned by wcsfix(). * * Index of the status value returned by cylfix() in the status vector * returned by wcsfix(). */ /** @def NWCSFIX * @brief Number of elements in the status vector returned by wcsfix(). * * Number of elements in the status vector returned by wcsfix(). */ /** @def cylfix_errmsg * @brief Deprecated. * @deprecated Added for backwards compatibility, use #wcsfix_errmsg directly * now instead. */ pywcs-1.12/wcslib/doxygen/wcshdr.sed0000644001153600020070000001260712310355626021603 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} # All standard. s|\([ >]\)CROTAi|\1CROTAi|g s|\([ >]\)DAVGn|\1DAVGn|g s|\([ >]\)EQUIna|\1EQUIna|g s|\([ >]\)LATPna|\1LATPna|g s|\([ >]\)LONPna|\1LONPna|g s|\([ >]\)MJDAn|\1MJDAn|g s|\([ >]\)MJDOBn|\1MJDOBn|g s|\([ >]\)OBSGXn|\1OBSGXn|g s|\([ >]\)OBSGYn|\1OBSGYn|g s|\([ >]\)OBSGZn|\1OBSGZn|g s|\([ >]\)RADEna|\1RADEna|g s|\([ >]\)RFRQna|\1RFRQna|g s|\([ >]\)RWAVna|\1RWAVna|g s|\([ >]\)SOBSna|\1SOBSna|g s|\([ >]\)SPECna|\1SPECna|g s|\([ >]\)SSRCna|\1SSRCna|g s|\([ >]\)TCDEna|\1TCDEna|g s|\([ >]\)TCDLTn|\1TCDLTn|g s|\([ >]\)TCNAna|\1TCNAna|g s|\([ >]\)TCRDna|\1TCRDna|g s|\([ >]\)TCRPXn|\1TCRPXn|g s|\([ >]\)TCRPna|\1TCRPna|g s|\([ >]\)TCRVLn|\1TCRVLn|g s|\([ >]\)TCRVna|\1TCRVna|g s|\([ >]\)TCSYna|\1TCSYna|g s|\([ >]\)TCTYPn|\1TCTYPn|g s|\([ >]\)TCTYna|\1TCTYna|g s|\([ >]\)TCUNIn|\1TCUNIn|g s|\([ >]\)TCUNna|\1TCUNna|g s|\([ >]\)TCn_ka|\1TCn_ka|g s|\([ >]\)TFIELDS|\1TFIELDS|g s|\([ >]\)TFORM|\1TFORM|g s|\([ >]\)TPn_ka|\1TPn_ka|g s|\([ >]\)TSn_ma|\1TSn_ma|g s|\([ >]\)TVn_ma|\1TVn_ma|g s|\([ >]\)TWCSna|\1TWCSna|g s|\([ >]\)VANGna|\1VANGna|g s|\([ >]\)VSYSna|\1VSYSna|g s|\([ >]\)WCAXna|\1WCAXna|g s|\([ >]\)WCSNna|\1WCSNna|g s|\([ >]\)iCDEna|\1iCDEna|g s|\([ >]\)iCDLTn|\1iCDLTn|g s|\([ >]\)iCNAna|\1iCNAna|g s|\([ >]\)iCRDna|\1iCRDna|g s|\([ >]\)iCROTn|\1iCROTn|g s|\([ >]\)iCRVLn|\1iCRVLn|g s|\([ >]\)iCRVna|\1iCRVna|g s|\([ >]\)iCSYna|\1iCSYna|g s|\([ >]\)iCTYPn|\1iCTYPn|g s|\([ >]\)iCTYna|\1iCTYna|g s|\([ >]\)iCUNIn|\1iCUNIn|g s|\([ >]\)iCUNna|\1iCUNna|g s|\([ >]\)iSn_ma|\1iSn_ma|g s|\([ >]\)iVn_ma|\1iVn_ma|g s|\([ >]\)ijCDna|\1ijCDna|g s|\([ >]\)ijPCna|\1ijPCna|g s|\([ >]\)jCRPXn|\1jCRPXn|g s|\([ >]\)jCRPna|\1jCRPna|g #\([ >]\)All\1non-standard or deprecated. s|\([ >]\)ALTRPIX|\1ALTRPIX|g s|\([ >]\)ALTRVAL|\1ALTRVAL|g s|\([ >]\)CD00i00j|\1CD00i00j|g s|\([ >]\)CROTAia|\1CROTAia|g s|\([ >]\)CROTAn|\1CROTAn|g s|\([ >]\)DOBSn|\1DOBSn|g s|\([ >]\)EPOCHa|\1EPOCHa|g s|\([ >]\)EPOCH|\1EPOCH|g s|\([ >]\)PC00i00j|\1PC00i00j|g s|\([ >]\)PROJPn|\1PROJPn|g s|\([ >]\)RADECSYS|\1RADECSYS|g s|\([ >]\)RESTFREQ|\1RESTFREQ|g s|\([ >]\)TCDLTna|\1TCDLTna|g s|\([ >]\)TCDn_ka|\1TCDn_ka|g s|\([ >]\)TCNAMn|\1TCNAMn|g s|\([ >]\)TCNAMna|\1TCNAMna|g s|\([ >]\)TCRDEn|\1TCRDEn|g s|\([ >]\)TCRDEna|\1TCRDEna|g s|\([ >]\)TCROTna|\1TCROTna|g s|\([ >]\)TCRPXna|\1TCRPXna|g s|\([ >]\)TCRVLna|\1TCRVLna|g s|\([ >]\)TCSYEn|\1TCSYEn|g s|\([ >]\)TCSYEna|\1TCSYEna|g s|\([ >]\)TCTYPn|\1TCTYPn|g s|\([ >]\)TCTYPna|\1TCTYPna|g s|\([ >]\)TCUNIna|\1TCUNIna|g s|\([ >]\)TPCn_ka|\1TPCn_ka|g s|\([ >]\)TPSn_ma|\1TPSn_ma|g s|\([ >]\)TPVn_ma|\1TPVn_ma|g s|\([ >]\)VELREFa|\1VELREFa|g s|\([ >]\)VELREF|\1VELREF|g s|\([ >]\)VSOURCEa|\1VSOURCEa|g s|\([ >]\)VSOUna|\1VSOUna|g s|\([ >]\)ZSOUna|\1ZSOUna|g s|\([ >]\)iCDLTna|\1iCDLTna|g s|\([ >]\)iCNAMn|\1iCNAMn|g s|\([ >]\)iCNAMna|\1iCNAMna|g s|\([ >]\)iCRDEn|\1iCRDEn|g s|\([ >]\)iCRDEna|\1iCRDEna|g s|\([ >]\)iCROTna|\1iCROTna|g s|\([ >]\)iCRVLna|\1iCRVLna|g s|\([ >]\)iCSYEn|\1iCSYEn|g s|\([ >]\)iCSYEna|\1iCSYEna|g s|\([ >]\)iCTYPn|\1iCTYPn|g s|\([ >]\)iCTYPna|\1iCTYPna|g s|\([ >]\)iCUNIna|\1iCUNIna|g s|\([ >]\)iPSn_ma|\1iPSn_ma|g s|\([ >]\)iPVn_ma|\1iPVn_ma|g s|\([ >]\)jCRPXna|\1jCRPXna|g s|'TAB'|'TAB'|g s|'T'|'T'|g s|'{DATE,MJD}-|'{DATE,MJD}-|g s|{OBS,AVG}'|{OBS,AVG}'|g s|'OBSGEO-|'OBSGEO-|g s|{X,Y,Z}'|{X,Y,Z}'|g s|WCSHDR_|#&|g s|WCSHDO_|#&|g /^\*/s|tabprm|#&|g /^\*/s|wcsprm|#&|g /^\*/s|wtbarr|#&|g s|fits_hdr2str()|&|g s|m = n <= 9|m = n @f$\\le@f$ 9| s| ARE NOT | are not | s| ARE | are | s|"relax"|relax| pywcs-1.12/wcslib/doxygen/wcshdr_extras.dox0000644001153600020070000002202412310355626023202 0ustar cslocumSTSCI\science00000000000000/** @def WCSHDR_none * @brief Bit mask for wcspih() and wcsbth() - reject all extensions. * * Bit mask for the relax argument of wcspih() and wcsbth() - reject * all extensions. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_all * @brief Bit mask for wcspih() and wcsbth() - accept all extensions. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * all extensions. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_reject * @brief Bit mask for wcspih() and wcsbth() - reject non-standard keywords. * * Bit mask for the relax argument of wcspih() and wcsbth() - reject * non-standard keywords. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_CROTAia * @brief Bit mask for wcspih() and wcsbth() - accept CROTAia, * iCROTna, TCROTna. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * CROTAia, iCROTna, TCROTna. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_EPOCHa * @brief Bit mask for wcspih() and wcsbth() - accept EPOCHa. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * EPOCHa. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_VELREFa * @brief Bit mask for wcspih() and wcsbth() - accept VELREFa. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * VELREFa. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_CD00i00j * @brief Bit mask for wcspih() and wcsbth() - accept * CD00i00j. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * CD00i00j. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_PC00i00j * @brief Bit mask for wcspih() and wcsbth() - accept * PC00i00j. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * PC00i00j. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_PROJPn * @brief Bit mask for wcspih() and wcsbth() - accept PROJPn. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * PROJPn. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_RADECSYS * @brief Bit mask for wcspih() and wcsbth() - accept RADECSYS. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * RADECSYS. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_VSOURCE * @brief Bit mask for wcspih() and wcsbth() - accept VSOURCEa. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * VSOURCEa. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_DOBSn * @brief Bit mask for wcspih() and wcsbth() - accept DOBSn. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * DOBSn. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_LONGKEY * @brief Bit mask for wcspih() and wcsbth() - accept long forms of the * alternate binary table and pixel list WCS keywords. * * Bit mask for the relax argument of wcspih() and wcsbth() - * accept long forms of the alternate binary table and pixel list WCS keywords. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_CNAMn * @brief Bit mask for wcspih() and wcsbth() - accept * iCNAMn, TCNAMn, * iCRDEn, TCRDEn, * iCSYEn, TCSYEn. * * Bit mask for the relax argument of wcspih() and wcsbth() - accept * iCNAMn, TCNAMn, * iCRDEn, TCRDEn, * iCSYEn, TCSYEn. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_AUXIMG * @brief Bit mask for wcspih() and wcsbth() - allow the image-header form of * an auxiliary WCS keyword to provide a default value for all images. * * Bit mask for the relax argument of wcspih() and wcsbth() - * allow the image-header form of an auxiliary WCS keyword with * representation-wide scope to provide a default value for all images. * * Refer to wcsbth() note 5. */ /** @def WCSHDR_ALLIMG * @brief Bit mask for wcspih() and wcsbth() - allow the image-header form of * all image header WCS keywords to provide a default value for all * images. * * Bit mask for the relax argument of wcspih() and wcsbth() - * allow the image-header form of all image header WCS keywords to * provide a default value for all image arrays in a binary table (n.b. not * pixel list). * * Refer to wcsbth() note 5. */ /** @def WCSHDR_IMGHEAD * @brief Bit mask for wcsbth() - restrict to image header keywords only. * * Bit mask for the keysel argument of wcsbth() - * restrict keyword types considered to image header keywords only. */ /** @def WCSHDR_BIMGARR * @brief Bit mask for wcsbth() - restrict to binary table image array keywords * only. * * Bit mask for the keysel argument of wcsbth() - * restrict keyword types considered to binary table image array keywords only. */ /** @def WCSHDR_PIXLIST * @brief Bit mask for wcsbth() - restrict to pixel list keywords only. * * Bit mask for the keysel argument of wcsbth() - * restrict keyword types considered to pixel list keywords only. */ /** @def WCSHDO_none * @brief Bit mask for wcshdo() - don't write any extensions. * * Bit mask for the relax argument of wcshdo() - * don't write any extensions. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_all * @brief Bit mask for wcshdo() - write all extensions. * * Bit mask for the relax argument of wcshdo() - * write all extensions. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_safe * @brief Bit mask for wcshdo() - write safe extensions only. * * Bit mask for the relax argument of wcshdo() - * write only extensions that are considered safe. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_DOBSn * @brief Bit mask for wcshdo() - write DOBSn. * * Bit mask for the relax argument of wcshdo() - write * DOBSn, the column-specific analogue of DATE-OBS for * use in binary tables and pixel lists. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_TPCn_ka * @brief Bit mask for wcshdo() - write TPCn_ka. * * Bit mask for the relax argument of wcshdo() - write * TPCn_ka * if less than eight characters instead of * TPn_ka. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_PVn_ma * @brief Bit mask for wcshdo() - write * iPVn_ma, TPVn_ma, * iPSn_ma, TPSn_ma. * * Bit mask for the relax argument of wcshdo() - write * iPVn_ma, TPVn_ma, * iPSn_ma, TPSn_ma, * if less than eight characters instead of * iVn_ma, TVn_ma, * iSn_ma, TSn_ma. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_CRPXna * @brief Bit mask for wcshdo() - write * jCRPXna, TCRPXna, * iCDLTna, TCDLTna, * iCUNIna, TCUNIna, * iCTYPna, TCTYPna, * iCRVLna, TCRVLna. * * Bit mask for the relax argument of wcshdo() - write * jCRPXna, TCRPXna, * iCDLTna, TCDLTna, * iCUNIna, TCUNIna, * iCTYPna, TCTYPna, * iCRVLna, TCRVLna, * if less than eight characters instead of * jCRPna, TCRPna, * iCDEna, TCDEna, * iCUNna, TCUNna, * iCTYna, TCTYna, * iCRVna, TCRVna. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_CNAMna * @brief Bit mask for wcshdo() - write * iCNAMna, TCNAMna, * iCRDEna, TCRDEna, * iCSYEna, TCSYEna. * * Bit mask for the relax argument of wcshdo() - write * iCNAMna, TCNAMna, * iCRDEna, TCRDEna, * iCSYEna, TCSYEna, * if less than eight characters instead of * iCNAna, TCNAna, * iCRDna, TCRDna, * iCSYna, TCSYna. * * Refer to the notes for wcshdo(). */ /** @def WCSHDO_WCSNna * @brief Bit mask for wcshdo() - write WCSNna instead of * TWCSna * * Bit mask for the relax argument of wcshdo() - * write WCSNna instead of TWCSna. * * Refer to the notes for wcshdo(). */ pywcs-1.12/wcslib/doxygen/wcsmath_extras.dox0000644001153600020070000000135612310355626023363 0ustar cslocumSTSCI\science00000000000000/** @def D2R * @brief Degrees to radians conversion factor. * * Factor @f$\pi/180^\circ@f$ to convert from degrees to radians. */ /** @def R2D * @brief Radians to degrees conversion factor. * * Factor @f$180^\circ/\pi@f$ to convert from radians to degrees. */ /** @def SQRT2 * @f$\sqrt{2}@f$, used only by molset() (MOL projection). */ /** @def SQRT2INV * @f$1/\sqrt{2}@f$, used only by qscx2s() (QSC projection). */ /** @def UNDEFINED * @brief Value used to indicate an undefined quantity. * * Value used to indicate an undefined quantity (noting that NaNs cannot be * used portably). */ /** @def undefined * @brief Macro used to test for an undefined quantity. * * Macro used to test for an undefined value. */ pywcs-1.12/wcslib/doxygen/wcstrig.sed0000644001153600020070000000027512310355626021771 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|90 degrees|@f$90^\\circ@f$|g s| x-| @f$x@f$-|g s| y-| @f$y@f$-|g s| beta| @f$\\beta@f$|g s| (x,y)| @f$(x,y)@f$|g s|(rho,beta)|@f$(\\rho,\\beta)@f$|g s|arg(x,y)|@f$\\&@f$|g pywcs-1.12/wcslib/doxygen/wcstrig_extras.dox0000644001153600020070000000045212310355626023373 0ustar cslocumSTSCI\science00000000000000/** @def WCSTRIG_TOL * @brief Domain tolerance for asin() and acos() functions. * * Domain tolerance for the asin() and acos() functions to allow for floating * point rounding errors. * * If @f$v@f$ lies in the range @f$1 < |v| < 1 + WCSTRIG\_TOL@f$ then it will * be treated as @f$|v| == 1@f$. */ pywcs-1.12/wcslib/doxygen/wcsunits.sed0000644001153600020070000000014312310355626022160 0ustar cslocumSTSCI\science00000000000000/^[^*]/{p;d;} s|offset is|offset is| s|power is|power is| s|1e6|@f$10^6@f$| pywcs-1.12/wcslib/doxygen/wcsunits_extras.dox0000644001153600020070000001015512310355626023571 0ustar cslocumSTSCI\science00000000000000/** @def WCSUNITS_PLANE_ANGLE * @brief Array index for plane angle units type. * * Array index for plane angle units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_SOLID_ANGLE * @brief Array index for solid angle units type. * * Array index for solid angle units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_CHARGE * @brief Array index for charge units type. * * Array index for charge units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_MOLE * @brief Array index for mole units type. * * Array index for mole ("gram molecular weight") units in the units * array returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_TEMPERATURE * @brief Array index for temperature units type. * * Array index for temperature units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_LUMINTEN * @brief Array index for luminous intensity units type. * * Array index for luminous intensity units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_MASS * @brief Array index for mass units type. * * Array index for mass units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_LENGTH * @brief Array index for length units type. * * Array index for length units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_TIME * @brief Array index for time units type. * * Array index for time units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_BEAM * @brief Array index for beam units type. * * Array index for beam units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_BIN * @brief Array index for bin units type. * * Array index for bin units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_BIT * @brief Array index for bit units type. * * Array index for bit units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_COUNT * @brief Array index for count units type. * * Array index for count units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_MAGNITUDE * @brief Array index for stellar magnitude units type. * * Array index for stellar magnitude units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_PIXEL * @brief Array index for pixel units type. * * Array index for pixel units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_SOLRATIO * @brief Array index for solar mass ratio units type. * * Array index for solar mass ratio units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_VOXEL * @brief Array index for voxel units type. * * Array index for voxel units in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ /** @def WCSUNITS_NTYPE * @brief Number of entries in the units array. * * Number of entries in the units array * returned by wcsulex(), and the #wcsunits_types[] and #wcsunits_units[] * global variables. */ pywcs-1.12/wcslib/flavours0000644001153600020070000001045412310355626017721 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # Makefile overrides for various combinations of architecture, operating # system and compiler. Used for development and testing only, not required # for building WCSLIB. # # Variables like CC and CFLAGS are exported into the environment so that they # will be seen by 'configure'. Thus, normal usage is as follows: # # make distclean # make FLAVOUR=Linux configure # make # # Reminder: add '-d' to FLFLAGS for debugging. # # $Id: flavours,v 4.10 2012/02/05 23:41:45 cal103 Exp $ #----------------------------------------------------------------------------- # The list of FLAVOURs can be set on the command line. F := $(shell echo $(FLAVOURS) | tr a-z A-Z) ifeq "$F" "" F := FLAVOURS := "" endif ifeq "$F" "LINUX" override FLAVOURS := "" Linux Linuxp endif ifeq "$F" "SUN" override FLAVOURS := "" SUN/GNU SUN/GNU3 SUN/GNUp SUN/ANSI endif ifeq "$F" "PURE" override FLAVOURS := SUN/Pure SUN/Quant endif F := # Various C standards handled by features.h in Linux. FEATURES := ifeq "$(notdir $(shell pwd))" "utils" # To get off_t for fseeko() usage in fitshdr when gcc is invoked with the # -std=c89 (same as -ansi) or the -std=c99 options. FEATURES := -D_XOPEN_SOURCE endif # Linux with gcc/gfortran (also works for Darwin). ifeq "$(FLAVOUR)" "Linux" F := $(FLAVOUR) export CC := gcc -std=c89 -pedantic export CPPFLAGS := $(FEATURES) export CFLAGS := -g -O0 -Wall -Wpadded -Wno-long-long export FFLAGS := -g -O0 -fimplicit-none -Wall -I. VALGRIND := valgrind -v --leak-check=yes endif ifeq "$(FLAVOUR)" "Linuxp" F := $(FLAVOUR) export CC := gcc -std=c89 -pedantic export CPPFLAGS := $(FEATURES) export CFLAGS := -pg -g -O -Wall -Wpadded -Wno-long-long export FFLAGS := -pg -a -g -O -fimplicit-none -Wall -I. export LDFLAGS := -pg -g $(filter -L%, $(LDFLAGS)) override EXTRA_CLEAN := gmon.out bb.out endif # Solaris with gcc/gfortran 4.x (lynx). ifeq "$(FLAVOUR)" "SUN/GNU" F := $(FLAVOUR) export CC := gcc -std=c89 export CPPFLAGS := $(FEATURES) export CFLAGS := -g -Wall -Wpadded -Wno-long-long export F77 := gfortran export FFLAGS := -g -fimplicit-none -Wall -I. LD := gcc endif ifeq "$(FLAVOUR)" "SUN/GNU3" F := $(FLAVOUR) export CC := gcc-3.1.1 -std=c89 export CPPFLAGS := $(FEATURES) export CFLAGS := -g -Wall -Wpadded -Wno-long-long export F77 := g77-3.1.1 export FFLAGS := -g -Wimplicit -Wunused -Wno-globals -I. LD := gcc-3.1.1 endif ifeq "$(FLAVOUR)" "SUN/GNUp" F := $(FLAVOUR) export CC := gcc -std=c89 -pedantic export CPPFLAGS := $(FEATURES) export CFLAGS := -pg -a -g -O -Wall -Wpadded -Wno-long-long export FFLAGS := -pg -a -g -O -fimplicit-none -Wall -I. export LDFLAGS := -pg -a -g $(filter -L%, $(LDFLAGS)) override EXTRA_CLEAN := gmon.out bb.out endif # Solaris with SUN cc/f77. ifeq "$(FLAVOUR)" "SUN/ANSI" F := $(FLAVOUR) WCSTRIG := NATIVE export CC := cc export CFLAGS := -g -I/usr/local/include export F77 := f77 export FFLAGS := -g -erroff=WDECL_LOCAL_NOTUSED LD := f77 endif # Purify and quantify in Solaris. ifeq "$(FLAVOUR)" "SUN/Pure" F := $(FLAVOUR) WCSTRIG := NATIVE export CC := purify gcc export CFLAGS := -g export F77 := purify gcc export FFLAGS := -g -Wimplicit -Wno-globals -I. export LDFLAGS := $(filter -L%, $(LDFLAGS)) override EXTRA_CLEAN := *_pure_p*.[ao] *.pcv .pure ../C/*_pure_p*.[ao] endif ifeq "$(FLAVOUR)" "SUN/Quant" F := $(FLAVOUR) WCSTRIG := NATIVE export CC := quantify gcc export CFLAGS := -g export F77 := quantify gcc export FFLAGS := -g -Wimplicit -Wno-globals -I. export LDFLAGS := $(filter -L%, $(LDFLAGS)) override EXTRA_CLEAN := *_pure_q*.[ao] .pure endif ifneq "$F" "$(FLAVOUR)" override FLAVOUR := unrecognised endif # gmake uses FC in place of configure's F77. ifdef F77 FC := $(F77) endif ifndef TIMER TIMER := date +"%a %Y/%m/%d %X %z, executing on $$HOST" endif ifdef FLAVOUR TIMER := $(TIMER) ; echo " with $(FLAVOUR) FLAVOUR." endif show :: -@ echo 'For code development...' -@ echo ' FLAVOURS := $(FLAVOURS)' -@ echo ' FLAVOUR := $(FLAVOUR)' -@ echo ' VALGRIND := $(VALGRIND)' -@ echo ' EXTRA_CLEAN := $(EXTRA_CLEAN)' -@ echo '' pywcs-1.12/wcslib/Fortran/0000755001153600020070000000000012310355732017542 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/Fortran/cel.inc0000644001153600020070000000611012310355626021000 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: cel.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL CELFREE, CELGET, CELGTC, CELGTD, CELGTI, CELINI, CELPRT, : CELPTC, CELPTD, CELPTI, CELPUT, CELS2X, CELSET, CELX2S INTEGER CELFREE, CELGET, CELGTC, CELGTD, CELGTI, CELINI, CELPRT, : CELPTC, CELPTD, CELPTI, CELPUT, CELS2X, CELSET, CELX2S * Length of the CELPRM data structure (INTEGER array) on 64-bit * machines. Only needs to be 144 on 32-bit machines. INTEGER CELLEN PARAMETER (CELLEN = 150) * Codes for CEL data structure elements used by CELPUT and CELGET. INTEGER CEL_FLAG, CEL_OFFSET, CEL_PHI0, CEL_PRJ, CEL_REF, : CEL_THETA0 PARAMETER (CEL_FLAG = 100) PARAMETER (CEL_OFFSET = 101) PARAMETER (CEL_PHI0 = 102) PARAMETER (CEL_THETA0 = 103) PARAMETER (CEL_REF = 104) PARAMETER (CEL_PRJ = 105) * Codes for CEL data structure elements used by CELGET (only). INTEGER CEL_ERR, CEL_EULER, CEL_ISOLAT, CEL_LATPRQ PARAMETER (CEL_EULER = 200) PARAMETER (CEL_LATPRQ = 201) PARAMETER (CEL_ISOLAT = 202) PARAMETER (CEL_ERR = 203) * Error codes and messages. INTEGER CELERR_BAD_COORD_TRANS, CELERR_BAD_PARAM, : CELERR_BAD_PIX, CELERR_BAD_WORLD, : CELERR_ILL_COORD_TRANS, CELERR_NULL_POINTER, : CELERR_SUCCESS PARAMETER (CELERR_SUCCESS = 0) PARAMETER (CELERR_NULL_POINTER = 1) PARAMETER (CELERR_BAD_PARAM = 2) PARAMETER (CELERR_BAD_COORD_TRANS = 3) PARAMETER (CELERR_ILL_COORD_TRANS = 4) PARAMETER (CELERR_BAD_PIX = 5) PARAMETER (CELERR_BAD_WORLD = 6) CHARACTER CEL_ERRMSG(0:6)*80 COMMON /CEL_DATA/ CEL_ERRMSG pywcs-1.12/wcslib/Fortran/cel_f.c0000644001153600020070000001525712310355626020772 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: cel_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include /* Fortran name mangling. */ #include #define celini_ F77_FUNC(celini, CELINI) #define celput_ F77_FUNC(celput, CELPUT) #define celget_ F77_FUNC(celget, CELGET) #define celfree_ F77_FUNC(celfree, CELFREE) #define celprt_ F77_FUNC(celprt, CELPRT) #define celset_ F77_FUNC(celset, CELSET) #define celx2s_ F77_FUNC(celx2s, CELX2S) #define cels2x_ F77_FUNC(cels2x, CELS2X) #define celptc_ F77_FUNC(celptc, CELPTC) #define celptd_ F77_FUNC(celptd, CELPTD) #define celpti_ F77_FUNC(celpti, CELPTI) #define celgtc_ F77_FUNC(celgtc, CELGTC) #define celgtd_ F77_FUNC(celgtd, CELGTD) #define celgti_ F77_FUNC(celgti, CELGTI) #define CEL_FLAG 100 #define CEL_OFFSET 101 #define CEL_PHI0 102 #define CEL_THETA0 103 #define CEL_REF 104 #define CEL_PRJ 105 #define CEL_EULER 200 #define CEL_LATPRQ 201 #define CEL_ISOLAT 202 #define CEL_ERR 203 /*--------------------------------------------------------------------------*/ int celini_(int *cel) { return celini((struct celprm *)cel); } /*--------------------------------------------------------------------------*/ int celput_(int *cel, const int *what, const void *value, const int *i) { int k; int *icelp; const int *ivalp; const double *dvalp; struct celprm *celp; /* Cast pointers. */ celp = (struct celprm *)cel; ivalp = (const int *)value; dvalp = (const double *)value; celp->flag = 0; switch (*what) { case CEL_FLAG: celp->flag = *ivalp; break; case CEL_OFFSET: celp->offset = *ivalp; break; case CEL_PHI0: celp->phi0 = *dvalp; break; case CEL_THETA0: celp->theta0 = *dvalp; break; case CEL_REF: celp->ref[*i-1] = *dvalp; break; case CEL_PRJ: k = (int *)(&(celp->prj)) - (int *)celp; icelp = cel + k; for (k = 0; k < PRJLEN; k++) { *(icelp++) = *(ivalp++); } break; default: return 1; } return 0; } int celptc_(int *cel, const int *what, const char *value, const int *i) { return celput_(cel, what, value, i); } int celptd_(int *cel, const int *what, const double *value, const int *i) { return celput_(cel, what, value, i); } int celpti_(int *cel, const int *what, const int *value, const int *i) { return celput_(cel, what, value, i); } /*--------------------------------------------------------------------------*/ int celget_(const int *cel, const int *what, void *value) { int k; int *ivalp; double *dvalp; const int *icelp; const struct celprm *celp; /* Cast pointers. */ celp = (const struct celprm *)cel; ivalp = (int *)value; dvalp = (double *)value; switch (*what) { case CEL_FLAG: *ivalp = celp->flag; break; case CEL_OFFSET: *ivalp = celp->offset; break; case CEL_PHI0: *dvalp = celp->phi0; break; case CEL_THETA0: *dvalp = celp->theta0; break; case CEL_REF: for (k = 0; k < 4; k++) { *(dvalp++) = celp->ref[k]; } break; case CEL_PRJ: icelp = (int *)(&(celp->prj)); for (k = 0; k < PRJLEN; k++) { *(ivalp++) = *(icelp++); } break; case CEL_EULER: for (k = 0; k < 5; k++) { *(dvalp++) = celp->euler[k]; } break; case CEL_LATPRQ: *ivalp = celp->latpreq; break; case CEL_ISOLAT: *ivalp = celp->isolat; break; case CEL_ERR: /* Copy the contents of the wcserr struct. */ if (celp->err) { icelp = (int *)(celp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(icelp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; default: return 1; } return 0; } int celgtc_(const int *cel, const int *what, char *value) { return celget_(cel, what, value); } int celgtd_(const int *cel, const int *what, double *value) { return celget_(cel, what, value); } int celgti_(const int *cel, const int *what, int *value) { return celget_(cel, what, value); } /*--------------------------------------------------------------------------*/ int celfree_(int *cel) { return celfree((struct celprm *)cel); } /*--------------------------------------------------------------------------*/ int celprt_(int *cel) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling CELPRT in the Fortran code. */ fflush(NULL); return celprt((struct celprm *)cel); } /*--------------------------------------------------------------------------*/ int celset_(int *cel) { return celset((struct celprm *)cel); } /*--------------------------------------------------------------------------*/ int celx2s_( int *cel, const int *nx, const int *ny, const int *sxy, const int *sll, const double x[], const double y[], double phi[], double theta[], double lng[], double lat[], int stat[]) { return celx2s((struct celprm *)cel, *nx, *ny, *sxy, *sll, x, y, phi, theta, lng, lat, stat); } /*--------------------------------------------------------------------------*/ int cels2x_( int *cel, const int *nlng, const int *nlat, const int *sll, const int *sxy, const double lng[], const double lat[], double phi[], double theta[], double x[], double y[], int stat[]) { return cels2x((struct celprm *)cel, *nlng, *nlat, *sll, *sxy, lng, lat, phi, theta, x, y, stat); } pywcs-1.12/wcslib/Fortran/fitshdr.inc0000644001153600020070000000515712310355626021712 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: fitshdr.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL FITSHDR, FREEKEYS, KEYGET, KEYIDGET, KEYIDGTC, KEYIDGTI, : KEYIDPTC, KEYIDPUT INTEGER FITSHDR, FREEKEYS, KEYGET, KEYIDGET, KEYIDGTC, KEYIDGTI, : KEYIDPTC, KEYIDPUT * Length of FITSKEY and FITSKEYID data structures (INTEGER arrays) * on 64-bit machines. These are the same for 32-bit machines. INTEGER KEYLEN, KEYIDLEN PARAMETER (KEYLEN = 48) PARAMETER (KEYIDLEN = 6) * Codes for KEYID data structure elements used by KEYIDPUT/GET. INTEGER KEYID_COUNT, KEYID_IDX, KEYID_NAME PARAMETER (KEYID_NAME = 100) PARAMETER (KEYID_COUNT = 101) PARAMETER (KEYID_IDX = 102) * Codes for KEY data structure elements used by KEYGET. INTEGER KEY_COMMENT, KEY_KEYID, KEY_KEYNO, KEY_KEYVALUE, : KEY_KEYWORD, KEY_STATUS, KEY_TYPE, KEY_ULEN PARAMETER (KEY_KEYNO = 200) PARAMETER (KEY_KEYID = 201) PARAMETER (KEY_STATUS = 202) PARAMETER (KEY_KEYWORD = 203) PARAMETER (KEY_TYPE = 204) PARAMETER (KEY_KEYVALUE = 205) PARAMETER (KEY_ULEN = 206) PARAMETER (KEY_COMMENT = 207) CHARACTER FITSHDR_ERRMSG(0:2)*80 COMMON /FITSHDR_DATA/ FITSHDR_ERRMSG pywcs-1.12/wcslib/Fortran/fitshdr_f.c0000644001153600020070000001465112310355626021667 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: fitshdr_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include /* Fortran name mangling. */ #include #define keyidput_ F77_FUNC(keyidput, KEYIDPUT) #define keyidget_ F77_FUNC(keyidget, KEYIDGET) #define keyget_ F77_FUNC(keyget, KEYGET) #define fitshdr_ F77_FUNC(fitshdr, FITSHDR) #define freekeys_ F77_FUNC(freekeys, FREEKEYS) #define keyidptc_ F77_FUNC(keyidptc, KEYIDPTC) #define keyidgtc_ F77_FUNC(keyidgtc, KEYIDGTC) #define keyidgti_ F77_FUNC(keyidgti, KEYIDGTI) #define KEYID_NAME 100 #define KEYID_COUNT 101 #define KEYID_IDX 102 #define KEY_KEYNO 200 #define KEY_KEYID 201 #define KEY_STATUS 202 #define KEY_KEYWORD 203 #define KEY_TYPE 204 #define KEY_KEYVALUE 205 #define KEY_ULEN 206 #define KEY_COMMENT 207 /*--------------------------------------------------------------------------*/ int keyidput_(int *keyid, const int *i, const int *what, const void *value) { const char *cvalp; struct fitskeyid *kidp; /* Cast pointers. */ kidp = (struct fitskeyid *)keyid + *i; cvalp = (const char *)value; switch (*what) { case KEYID_NAME: strncpy(kidp->name, cvalp, 12); wcsutil_null_fill(12, kidp->name); break; default: return 1; } return 0; } int keyidptc_(int *keyid, const int *i, const int *what, const char *value) { return keyidput_(keyid, i, what, value); } /*--------------------------------------------------------------------------*/ int keyidget_(const int *keyid, const int *i, const int *what, void *value) { char *cvalp; int *ivalp; const struct fitskeyid *keyidp; /* Cast pointers. */ keyidp = (const struct fitskeyid *)keyid + *i; cvalp = (char *)value; ivalp = (int *)value; switch (*what) { case KEYID_NAME: strncpy(cvalp, keyidp->name, 12); wcsutil_blank_fill(12, cvalp); break; case KEYID_COUNT: *ivalp = keyidp->count; break; case KEYID_IDX: *(ivalp++) = keyidp->idx[0]; *(ivalp++) = keyidp->idx[1]; break; default: return 1; } return 0; } int keyidgtc_(const int *keyid, const int *i, const int *what, char *value) { return keyidget_(keyid, i, what, value); } int keyidgti_(const int *keyid, const int *i, const int *what, int *value) { return keyidget_(keyid, i, what, value); } /*--------------------------------------------------------------------------*/ int keyget_( const int *keys, const int *i, const int *what, void *value, int *nc) { char *cvalp, text[32]; int *ivalp, j; double *dvalp; const struct fitskey *keyp; /* Cast pointers. */ keyp = *((const struct fitskey **)keys) + *i; cvalp = (char *)value; ivalp = (int *)value; dvalp = (double *)value; *nc = 1; switch (*what) { case KEY_KEYNO: *ivalp = keyp->keyno; break; case KEY_KEYID: *ivalp = keyp->keyid; break; case KEY_STATUS: *ivalp = keyp->status; break; case KEY_KEYWORD: *nc = strlen(keyp->keyword); strncpy(cvalp, keyp->keyword, 12); wcsutil_blank_fill(12, cvalp); break; case KEY_TYPE: *ivalp = keyp->type; break; case KEY_KEYVALUE: switch (abs(keyp->type)%10) { case 1: case 2: /* Logical and 32-bit integer. */ *ivalp = keyp->keyvalue.i; break; case 3: /* 64-bit integer. */ *nc = 3; #ifdef WCSLIB_INT64 sprintf(text, "%28.27lld", keyp->keyvalue.k); sscanf(text+1, "%9d%9d%9d", ivalp+2, ivalp+1, ivalp); if (*text == '-') { ivalp[0] *= -1; ivalp[1] *= -1; ivalp[2] *= -1; } #else *(ivalp++) = keyp->keyvalue.k[0]; *(ivalp++) = keyp->keyvalue.k[1]; *(ivalp++) = keyp->keyvalue.k[2]; #endif break; case 4: /* Very long integer. */ *nc = 8; for (j = 0; j < 8; j++) { *(ivalp++) = keyp->keyvalue.l[j]; } break; case 5: /* Floating point. */ *dvalp = keyp->keyvalue.f; break; case 6: case 7: /* Integer complex and floating point complex. */ *nc = 2; *(dvalp++) = keyp->keyvalue.c[0]; *(dvalp++) = keyp->keyvalue.c[1]; break; case 8: /* String or part of a continued string. */ *nc = strlen(keyp->keyvalue.s); strncpy(cvalp, keyp->keyvalue.s, 72); wcsutil_blank_fill(72, cvalp); break; default: /* No value. */ break; } break; case KEY_ULEN: *ivalp = keyp->ulen; break; case KEY_COMMENT: *nc = strlen(keyp->comment); strncpy(cvalp, keyp->comment, 84); wcsutil_blank_fill(84, cvalp); break; default: return 1; } return 0; } /*--------------------------------------------------------------------------*/ int fitshdr_( const char header[], const int *nkeyrec, const int *nkeyids, int *keyids, int *nreject, iptr keys) { return fitshdr(header, *nkeyrec, *nkeyids, (struct fitskeyid *)keyids, nreject, (struct fitskey **)keys); } /*--------------------------------------------------------------------------*/ int freekeys_(int *keys) { free(*((struct fitskey **)keys)); *keys = 0; return 0; } pywcs-1.12/wcslib/Fortran/getwcstab.inc0000644001153600020070000000266512310355626022233 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: getwcstab.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL FTWCST INTEGER FTWCST pywcs-1.12/wcslib/Fortran/getwcstab_f.c0000644001153600020070000000406112310355626022201 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: getwcstab_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include /* Fortran name mangling. */ #include #define ftwcst_ F77_FUNC(ftwcst, FTWCST) /* CFITSIO global variable defined by/for the FITSIO wrappers that maps * Fortran unit numbers to fitsfile *; see f77_wrap.h and f77_wrap1.c. */ extern fitsfile *gFitsFiles[]; /*--------------------------------------------------------------------------*/ int ftwcst_( int *unit, int *nwtb, int *wtb, int *status) { /* *wtb is meant to hold a pointer to a wtbarr struct. On 64-bit machines sizeof(void *) = 2 * sizeof(int) = sizeof(long). */ long wtbp = *((long *)wtb); return fits_read_wcstab(gFitsFiles[*unit], *nwtb, (void *)wtbp, status); } pywcs-1.12/wcslib/Fortran/GNUmakefile0000644001153600020070000002340212310355626021617 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile for building the WCSLIB 4.10 FORTRAN wrappers. # # Summary of the main targets # --------------------------- # build: Build the library # # clean: Delete intermediate object files. # # cleaner: clean, and also delete the test executables. # # cleanest (distclean, or realclean): cleaner, and also delete the # object library. # # check (or test): Compile and run the test programs. By default they are # executed in batch mode, and non-graphical tests only report # "PASS" on success. Use # # make MODE=interactive check # # to run them interactively with full diagnostic output. To skip # graphical tests even if PGPLOT is available, use # # make CHECK=nopgplot check # # tests: Compile the test programs (but don't run them). # # Notes: # 1) If you need to make changes then preferably modify ../makedefs.in # instead and re-run configure. # # 2) This makefile assumes that the WCSLIB 4.10 sources reside in ../C # (as in the distribution kit). # # 3) twcstab assumes that ../C/wcstab.fits has already been generated by # the corresponding C test program. # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: GNUmakefile,v 4.10 2012/02/05 23:41:44 cal103 Exp $ #----------------------------------------------------------------------------- # Get configure settings. include ../makedefs MODULES := $(patsubst %.c,%.o,$(filter-out getwcstab_f.c,$(wildcard *.c))) MODULES += $(patsubst %.f,%.o,$(wildcard *.f)) ifdef GETWCSTAB FGETWCSTAB := ../C/getwcstab.o endif WCSLIB := ../C/$(WCSLIB) # Build the sharable library? ifneq "$(SHRLIB)" "" PICLIB := ../C/libwcs-PIC.a SHRLIB := ../C/$(SHRLIB) endif CPPFLAGS += -I.. -I../C vpath %.h ..:../C vpath %.in .. # For building and exercising the test suite # ------------------------------------------ # Test programs that don't require CFITSIO or PGPLOT. TEST_N := tlin tlog tprj1 tsph tspx ttab1 twcs twcssub tpih1 tfitshdr tunits \ twcsfix # Test programs that require CFITSIO (they don't need PGPLOT). TEST_C := twcstab # Test programs that require PGPLOT but not PGSBOX. TEST_P := tspc tprj2 tcel1 ttab2 ttab3 twcsmix # Test programs that require PGPLOT and PGSBOX. TEST_B := tpih2 TESTS := $(TEST_N) # Add test programs that require CFITSIO if we have it. ifneq "$(CFITSIOINC)" "" ifneq "$(CFITSIOLIB)" "" TESTS += $(TEST_C) endif endif # Add test programs that require PGPLOT if we have it. ifneq "$(CHECK)" "nopgplot" ifneq "$(PGPLOTINC)" "" ifneq "$(PGPLOTLIB)" "" TESTS += $(TEST_P) $(TEST_B) endif endif endif PGSBOXLIB := ../pgsbox/libpgsbox-$(LIBVER).a PGPLOTLIB := $(PGPLOTLIB) # Pattern rules #-------------- $(WCSLIB)(%.o) : %.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) -c $< $(AR) r $(WCSLIB) $% -@ $(RM) $% $(WCSLIB)(%.o) : %.f -@ echo '' $(FC) $(FFLAGS) -c $< $(AR) r $(WCSLIB) $% -@ $(RM) $% $(PICLIB)(%.o) : %.c -@ echo '' $(CC) $(CPPFLAGS) $(SHRFLAGS) -c $< $(AR) r $(PICLIB) $% -@ $(RM) $% $(PICLIB)(%.o) : %.f -@ echo '' $(FC) $(FFLAGS) $(SHRFLAGS) -c $< $(AR) r $(PICLIB) $% -@ $(RM) $% %.i : %.c -@ echo '' -@ $(RM) $@ $(CPP) $(CPPFLAGS) $(CFLAGS) $< > $@ %.d : %.c -@ echo '' -@ $(CPP) $(CPPFLAGS) $(CFLAGS) $< | \ sed -n -e 's|^# 1 "\([^/].*\.h\)".*|\1|p' | \ sort -u %.o : %.f -@ echo '' $(FC) $(FFLAGS) -c $< run_% : % -@ echo '' -@ $(TIMER) @ if [ '$(MODE)' = interactive -o '$(VALGRIND)' ] ; then \ printf 'Press to run $<: ' ; \ read DUMMY ; \ fi ; \ if [ '$(VALGRIND)' ] ; then \ if [ '$<' = tunits ] ; then \ $(VALGRIND) ./$< < test/units_test ; \ else \ $(VALGRIND) ./$< ; \ fi ; \ else \ if [ '$(filter $<, $(TEST_N) $(TEST_C))' ] ; then \ if [ '$<' = tunits ] ; then \ if [ '$(MODE)' = interactive ] ; then \ ./$< < ../C/test/units_test 2>&1 | tee $<.out ; \ else \ ./$< < ../C/test/units_test > $<.out 2>&1 ; \ fi ; \ else \ if [ '$(MODE)' = interactive ] ; then \ ./$< < /dev/null 2>&1 | tee $<.out ; \ else \ ./$< < /dev/null > $<.out 2>&1 ; \ fi ; \ fi ; \ if grep 'PASS:' $<.out > /dev/null ; then \ if [ '$(MODE)' != interactive ] ; then \ head -2 $<.out ; \ grep 'PASS:' $<.out ; \ fi ; \ echo 'PASS: Fortran/$<' >> test_results ; \ elif [ -f 'test/$<.out' ] ; then \ trap 'rm -f run_test.tmp' 0 1 2 3 15 ; \ sed -e 's/0x[0-9a-f][0-9a-f][0-9a-f]*/0x
      /g' $<.out > \ run_test.tmp ; \ mv -f run_test.tmp $<.out ; \ if cmp -s $<.out test/$<.out ; then \ if [ '$(MODE)' != interactive ] ; then \ head -2 $<.out ; \ echo 'PASS: Output agrees with Fortran/test/$<.out' ; \ fi ; \ echo 'PASS: Fortran/$<' >> test_results ; \ else \ if [ '$(MODE)' != interactive ] ; then \ cat $<.out ; \ fi ; \ echo '' ; \ echo 'FAIL: Output disagrees with Fortran/test/$<.out' ; \ echo 'FAIL: Fortran/$<' >> test_results ; \ fi ; \ elif [ '$(MODE)' != interactive ] ; then \ cat $<.out ; \ echo 'FAIL: Fortran/$<' >> test_results ; \ fi ; \ elif [ '$(MODE)' = interactive ] ; then \ ./$< ; \ else \ if [ '$<' = tcel2 ] ; then \ echo N | ./$< ; \ else \ ./$< < /dev/null 2>&1 ; \ fi ; \ fi ; \ fi -@ echo '' # Static and static pattern rules #-------------------------------- .PHONY : build check clean cleaner cleanest distclean install lib realclean \ test tests build : lib lib : $(WCSLIB) $(SHRLIB) $(WCSLIB) :: -@ echo '' $(MAKE) -C ../C lib $(WCSLIB) :: $(MODULES:%=$(WCSLIB)(%)) -@ echo '' $(RANLIB) $(WCSLIB) $(SHRLIB) : $(PICLIB) -@ echo '' -@ $(RM) -r tmp mkdir tmp && \ cd tmp && \ trap 'cd .. ; $(RM) -r tmp' 0 1 2 3 15 ; \ $(AR) x ../$(PICLIB) && \ $(SHRLD) $(LDFLAGS) -o $(@F) *.o && \ mv $(@F) ../../C $(PICLIB) : $(MODULES:%.o=$(PICLIB)(%.o)) ; install : build $(MAKE) -C ../C install $(INSTALL) -m 444 *.inc $(INCDIR) clean : - $(RM) -r *.o *.i a.out t*.out core fort.* *.dSYM $(EXTRA_CLEAN) cleaner : clean - $(RM) .gdb_history - $(RM) $(TEST_N) - $(RM) $(TEST_P) tpih2 twcstab - $(RM) tofits pih.fits test_results cleanest distclean realclean : cleaner - $(RM) $(WCSLIB) $(PICLIB) $(SHRLIB) check test : tests $(TESTS:%=run_%) tests : $(TESTS) $(TEST_N) : % : test/%.f $(WCSLIB) -@ echo '' $(FC) $(FFLAGS) $(LDFLAGS) -o $@ $< $(WCSLIB) $(LIBS) -@ $(RM) $@.o $(TEST_P) : % : test/%.f $(WCSLIB) -@ echo '' $(FC) $(FFLAGS) $(LDFLAGS) -o $@ $< $(WCSLIB) $(PGPLOTLIB) $(LIBS) -@ $(RM) $@.o tpih2 : % : test/%.f $(PGSBOXLIB) $(WCSLIB) -@ echo '' $(FC) $(FFLAGS) $(LDFLAGS) -o $@ $< $(PGSBOXLIB) $(WCSLIB) \ $(PGPLOTLIB) $(LIBS) -@ $(RM) $@.o twcstab : test/twcstab.f getwcstab_f.o getwcstab.inc $(FGETWCSTAB) \ $(WCSLIB) -@ echo '' $(FC) $(FFLAGS) $(LDFLAGS) -o $@ $< getwcstab_f.o \ $(FGETWCSTAB) $(CFITSIOLIB) $(WCSLIB) $(LIBS) -@ $(RM) $@.o getwcstab_f.o : getwcstab_f.c getwcstab.h -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) $(CFITSIOINC) -c $< ../C/getwcstab.o :: -@ echo '' $(MAKE) -C ../C getwcstab.o $(PGSBOXLIB) : -@ echo '' $(MAKE) -C ../pgsbox lib tofits : ../C/test/tofits.c $(CC) $(CFLAGS) -o $@ $< pih.fits : ../C/test/pih.keyrec tofits sed '/^BADKEYREC/q' $< | ./tofits > $@ GNUmakefile : ../makedefs ; ../makedefs ../wcsconfig.h ../wcsconfig_f77.h : makedefs.in wcsconfig.h.in \ wcsconfig_f77.h.in ../config.status -@ $(RM) ../wcsconfig.h ../wcsconfig_f77.h cd .. && ./config.status show :: -@ echo ' MODULES := $(MODULES)' # Dependencies (use the %.d pattern rule to list them) #----------------------------------------------------- $(WCSLIB)(cel_f.o) : cel.h prj.h wcserr.h wcsconfig_f77.h $(WCSLIB)(fitshdr_f.o) : fitshdr.h wcsconfig.h wcsconfig_f77.h wcsutil.h $(WCSLIB)(getwcstab_f.o): getwcstab.h wcsconfig_f77.h $(WCSLIB)(lin_f.o) : lin.h wcsconfig_f77.h wcserr.h $(WCSLIB)(log_f.o) : log.h wcsconfig_f77.h $(WCSLIB)(prj_f.o) : prj.h wcsconfig_f77.h wcserr.h $(WCSLIB)(spc_f.o) : spc.h spx.h wcsconfig_f77.h wcserr.h wcsutil.h $(WCSLIB)(sph_f.o) : sph.h wcsconfig_f77.h $(WCSLIB)(spx_f.o) : spx.h wcsconfig_f77.h wcserr.h $(WCSLIB)(tab_f.o) : tab.h wcsconfig_f77.h wcserr.h $(WCSLIB)(wcs_f.o) : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h \ wcsconfig_f77.h wcserr.h wcsutil.h $(WCSLIB)(wcsfix_f.o) : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h \ wcsconfig_f77.h wcserr.h wcsfix.h $(WCSLIB)(wcshdr_f.o) : cel.h lin.h prj.h spc.h spx.h tab.h wcs.h \ wcsconfig_f77.h wcserr.h wcshdr.h $(WCSLIB)(wcsunits_f.o) : wcsconfig_f77.h wcserr.h wcsunits.h wcsutil.h tcel1 : cel.inc prj.inc tfitshdr: fitshdr.inc wcshdr.inc tlin : lin.inc tlog : log.inc tpih1 : wcs.inc wcsfix.inc wcshdr.inc tpih2 : wcs.inc wcshdr.inc tprj1 : prj.inc tprj2 : prj.inc tspc : spc.inc spx.inc tspx : spx.inc ttab1 : tab.inc ttab2 : tab.inc ttab3 : prj.inc tab.inc tunits : wcsunits.inc twcs : cel.inc prj.inc wcs.inc wcserr.inc wcsmath.inc twcsfix : wcs.inc wcsfix.inc wcsunits.inc twcsmix : cel.inc lin.inc prj.inc wcs.inc twcssub : wcs.inc twcstab : getwcstab.inc wcs.inc wcsfix.inc wcshdr.inc run_tfitshdr run_tpih1 run_tpih2: pih.fits run_twcstab: ../C/wcstab.fits pywcs-1.12/wcslib/Fortran/lin.inc0000644001153600020070000000540312310355626021023 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: lin.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL LINCPY, LINFREE, LINGET, LINGTD, LINGTI, LININI, LINP2X, : LINPRT, LINPTD, LINPTI, LINPUT, LINSET, LINX2P INTEGER LINCPY, LINFREE, LINGET, LINGTD, LINGTI, LININI, LINP2X, : LINPRT, LINPTD, LINPTI, LINPUT, LINSET, LINX2P * Length of the LINPRM data structure (INTEGER array) on 64-bit * machines. Only needs to be 18 on 32-bit machines. INTEGER LINLEN PARAMETER (LINLEN = 28) * Codes for LIN data structure elements used by LINPUT and LINGET. INTEGER LIN_CDELT, LIN_CRPIX, LIN_FLAG, LIN_NAXIS, LIN_PC PARAMETER (LIN_FLAG = 100) PARAMETER (LIN_NAXIS = 101) PARAMETER (LIN_CRPIX = 102) PARAMETER (LIN_PC = 103) PARAMETER (LIN_CDELT = 104) * Codes for LIN data structure elements used by LINGET (only). INTEGER LIN_ERR, LIN_IMGPIX, LIN_PIXIMG, LIN_UNITY PARAMETER (LIN_PIXIMG = 200) PARAMETER (LIN_IMGPIX = 201) PARAMETER (LIN_UNITY = 202) PARAMETER (LIN_ERR = 203) * Error codes and messages. INTEGER LINERR_MEMORY, LINERR_NULL_POINTER, LINERR_SINGULAR_MTX, : LINERR_SUCCESS PARAMETER (LINERR_SUCCESS = 0) PARAMETER (LINERR_NULL_POINTER = 1) PARAMETER (LINERR_MEMORY = 2) PARAMETER (LINERR_SINGULAR_MTX = 3) CHARACTER LIN_ERRMSG(0:3)*80 COMMON /LIN_DATA/ LIN_ERRMSG pywcs-1.12/wcslib/Fortran/lin_f.c0000644001153600020070000001554312310355626021007 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: lin_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include /* Fortran name mangling. */ #include #define linini_ F77_FUNC(linini, LININI) #define lincpy_ F77_FUNC(lincpy, LINCPY) #define linput_ F77_FUNC(linput, LINPUT) #define linget_ F77_FUNC(linget, LINGET) #define linfree_ F77_FUNC(linfree, LINFREE) #define linprt_ F77_FUNC(linprt, LINPRT) #define linset_ F77_FUNC(linset, LINSET) #define linp2x_ F77_FUNC(linp2x, LINP2X) #define linx2p_ F77_FUNC(linx2p, LINX2P) #define linptd_ F77_FUNC(linptd, LINPTD) #define linpti_ F77_FUNC(linpti, LINPTI) #define lingtd_ F77_FUNC(lingtd, LINGTD) #define lingti_ F77_FUNC(lingti, LINGTI) #define LIN_FLAG 100 #define LIN_NAXIS 101 #define LIN_CRPIX 102 #define LIN_PC 103 #define LIN_CDELT 104 #define LIN_PIXIMG 200 #define LIN_IMGPIX 201 #define LIN_UNITY 202 #define LIN_ERR 203 /*--------------------------------------------------------------------------*/ int linini_(const int *naxis, int *lin) { return linini(1, *naxis, (struct linprm *)lin); } /*--------------------------------------------------------------------------*/ int lincpy_(const int *linsrc, int *lindst) { return lincpy(1, (const struct linprm *)linsrc, (struct linprm *)lindst); } /*--------------------------------------------------------------------------*/ int linput_( int *lin, const int *what, const void *value, const int *i, const int *j) { int i0, j0, k; const int *ivalp; const double *dvalp; struct linprm *linp; /* Cast pointers. */ linp = (struct linprm *)lin; ivalp = (const int *)value; dvalp = (const double *)value; /* Convert 1-relative FITS axis numbers to 0-relative C array indices. */ i0 = *i - 1; j0 = *j - 1; linp->flag = 0; switch (*what) { case LIN_FLAG: linp->flag = *ivalp; break; case LIN_NAXIS: linp->naxis = *ivalp; break; case LIN_CRPIX: linp->crpix[i0] = *dvalp; break; case LIN_PC: k = (i0)*(linp->naxis) + (j0); *(linp->pc+k) = *dvalp; break; case LIN_CDELT: linp->cdelt[i0] = *dvalp; break; default: return 1; } return 0; } int linptd_( int *lin, const int *what, const double *value, const int *i, const int *j) { return linput_(lin, what, value, i, j); } int linpti_( int *lin, const int *what, const int *value, const int *i, const int *j) { return linput_(lin, what, value, i, j); } /*--------------------------------------------------------------------------*/ int linget_(const int *lin, const int *what, void *value) { int i, j, k, naxis; int *ivalp; double *dvalp; const int *ilinp; const double *dlinp; const struct linprm *linp; /* Cast pointers. */ linp = (const struct linprm *)lin; ivalp = (int *)value; dvalp = (double *)value; naxis = linp->naxis; switch (*what) { case LIN_FLAG: *ivalp = linp->flag; break; case LIN_NAXIS: *ivalp = naxis; break; case LIN_CRPIX: for (i = 0; i < naxis; i++) { *(dvalp++) = linp->crpix[i]; } break; case LIN_PC: /* C row-major to FORTRAN column-major. */ for (j = 0; j < naxis; j++) { dlinp = linp->pc + j; for (i = 0; i < naxis; i++) { *(dvalp++) = *dlinp; dlinp += naxis; } } break; case LIN_CDELT: for (i = 0; i < naxis; i++) { *(dvalp++) = linp->cdelt[i]; } break; case LIN_PIXIMG: /* C row-major to FORTRAN column-major. */ for (j = 0; j < naxis; j++) { dlinp = linp->piximg + j; for (i = 0; i < naxis; i++) { *(dvalp++) = *dlinp; dlinp += naxis; } } break; case LIN_IMGPIX: /* C row-major to FORTRAN column-major. */ for (j = 0; j < naxis; j++) { dlinp = linp->imgpix + j; for (i = 0; i < naxis; i++) { *(dvalp++) = *dlinp; dlinp += naxis; } } break; case LIN_UNITY: *ivalp = linp->unity; break; case LIN_ERR: /* Copy the contents of the wcserr struct. */ if (linp->err) { ilinp = (int *)(linp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(ilinp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; default: return 1; } return 0; } int lingtd_(const int *lin, const int *what, double *value) { return linget_(lin, what, value); } int lingti_(const int *lin, const int *what, int *value) { return linget_(lin, what, value); } /*--------------------------------------------------------------------------*/ int linfree_(int *lin) { return linfree((struct linprm *)lin); } /*--------------------------------------------------------------------------*/ int linprt_(int *lin) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling LINPRT in the Fortran code. */ fflush(NULL); return linprt((struct linprm *)lin); } /*--------------------------------------------------------------------------*/ int linset_(int *lin) { return linset((struct linprm *)lin); } /*--------------------------------------------------------------------------*/ int linp2x_( int *lin, const int *ncoord, const int *nelem, const double pixcrd[], double imgcrd[]) { return linp2x((struct linprm *)lin, *ncoord, *nelem, pixcrd, imgcrd); } /*--------------------------------------------------------------------------*/ int linx2p_( int *lin, const int *ncoord, const int *nelem, const double imgcrd[], double pixcrd[]) { return linx2p((struct linprm *)lin, *ncoord, *nelem, imgcrd, pixcrd); } pywcs-1.12/wcslib/Fortran/log.inc0000644001153600020070000000360512310355626021024 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: log.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL LOGS2X, LOGX2S INTEGER LOGS2X, LOGX2S * Error codes and messages. INTEGER LOGERR_BAD_LOG_REF_VAL, LOGERR_BAD_WORLD, LOGERR_BAD_X, : LOGERR_NULL_POINTER, LOGERR_SUCCESS PARAMETER (LOGERR_SUCCESS = 0) PARAMETER (LOGERR_NULL_POINTER = 1) PARAMETER (LOGERR_BAD_LOG_REF_VAL = 2) PARAMETER (LOGERR_BAD_X = 3) PARAMETER (LOGERR_BAD_WORLD = 4) CHARACTER LOG_ERRMSG(0:3)*80 COMMON /LOG_DATA/ LOG_ERRMSG pywcs-1.12/wcslib/Fortran/log_f.c0000644001153600020070000000412412310355626020777 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: log_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include /* Fortran name mangling. */ #include #define logx2s_ F77_FUNC(logx2s, LOGX2S) #define logs2x_ F77_FUNC(logs2x, LOGS2X) /*--------------------------------------------------------------------------*/ int logx2s_( const double *crval, const int *nx, const int *sx, const int *slogc, const double x[], double logc[], int stat[]) { return logx2s(*crval, *nx, *sx, *slogc, x, logc, stat); } /*--------------------------------------------------------------------------*/ int logs2x_( const double *crval, const int *nlogc, const int *slogc, const int *sx, const double logc[], double x[], int stat[]) { return logs2x(*crval, *nlogc, *slogc, *sx, logc, x, stat); } pywcs-1.12/wcslib/Fortran/prj.inc0000644001153600020070000001346012310355626021036 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: prj.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL PRJFREE, PRJGET, PRJGTC, PRJGTD, PRJGTI, PRJINI, PRJPRT, : PRJPTC, PRJPTD, PRJPTI, PRJPUT, PRJS2X, PRJSET, PRJX2S INTEGER PRJFREE, PRJGET, PRJGTC, PRJGTD, PRJGTI, PRJINI, PRJPRT, : PRJPTC, PRJPTD, PRJPTI, PRJPUT, PRJS2X, PRJSET, PRJX2S EXTERNAL AZPSET, AZPX2S, AZPS2X, SFLSET, SFLX2S, SFLS2X, : SZPSET, SZPX2S, SZPS2X, PARSET, PARX2S, PARS2X, : TANSET, TANX2S, TANS2X, MOLSET, MOLX2S, MOLS2X, : STGSET, STGX2S, STGS2X, AITSET, AITX2S, AITS2X, : SINSET, SINX2S, SINS2X, COPSET, COPX2S, COPS2X, : ARCSET, ARCX2S, ARCS2X, COESET, COEX2S, COES2X, : ZPNSET, ZPNX2S, ZPNS2X, CODSET, CODX2S, CODS2X, : ZEASET, ZEAX2S, ZEAS2X, COOSET, COOX2S, COOS2X, : AIRSET, AIRX2S, AIRS2X, BONSET, BONX2S, BONS2X, : CYPSET, CYPX2S, CYPS2X, PCOSET, PCOX2S, PCOS2X, : CEASET, CEAX2S, CEAS2X, TSCSET, TSCX2S, TSCS2X, : CARSET, CARX2S, CARS2X, CSCSET, CSCX2S, CSCS2X, : MERSET, MERX2S, MERS2X, QSCSET, QSCX2S, QSCS2X INTEGER AZPSET, AZPX2S, AZPS2X, SFLSET, SFLX2S, SFLS2X, : SZPSET, SZPX2S, SZPS2X, PARSET, PARX2S, PARS2X, : TANSET, TANX2S, TANS2X, MOLSET, MOLX2S, MOLS2X, : STGSET, STGX2S, STGS2X, AITSET, AITX2S, AITS2X, : SINSET, SINX2S, SINS2X, COPSET, COPX2S, COPS2X, : ARCSET, ARCX2S, ARCS2X, COESET, COEX2S, COES2X, : ZPNSET, ZPNX2S, ZPNS2X, CODSET, CODX2S, CODS2X, : ZEASET, ZEAX2S, ZEAS2X, COOSET, COOX2S, COOS2X, : AIRSET, AIRX2S, AIRS2X, BONSET, BONX2S, BONS2X, : CYPSET, CYPX2S, CYPS2X, PCOSET, PCOX2S, PCOS2X, : CEASET, CEAX2S, CEAS2X, TSCSET, TSCX2S, TSCS2X, : CARSET, CARX2S, CARS2X, CSCSET, CSCX2S, CSCS2X, : MERSET, MERX2S, MERS2X, QSCSET, QSCX2S, QSCS2X * Length of the PRJPRM data structure (INTEGER array) on 64-bit * machines. Only needs to be 116 on 32-bit machines. INTEGER PRJLEN PARAMETER (PRJLEN = 120) * Number of projection parameters supported by WCSLIB, 0 to PVN-1. INTEGER PRJ_PVN PARAMETER (PRJ_PVN = 30) * Codes for PRJ data structure elements used by PRJPUT and PRJGET. INTEGER PRJ_BOUNDS, PRJ_CODE, PRJ_FLAG, PRJ_PHI0, PRJ_PV, : PRJ_R0, PRJ_THETA0 PARAMETER (PRJ_FLAG = 100) PARAMETER (PRJ_CODE = 101) PARAMETER (PRJ_R0 = 102) PARAMETER (PRJ_PV = 103) PARAMETER (PRJ_PHI0 = 104) PARAMETER (PRJ_THETA0 = 105) PARAMETER (PRJ_BOUNDS = 106) * Codes for PRJ data structure elements used by PRJGET (only). INTEGER PRJ_CATEGORY, PRJ_CONFORMAL, PRJ_ERR, PRJ_GLOBAL, : PRJ_DIVERGENT, PRJ_EQUIAREAL, PRJ_N, PRJ_NAME, : PRJ_PVRANGE, PRJ_SIMPLEZEN, PRJ_W, PRJ_X0, PRJ_Y0 PARAMETER (PRJ_NAME = 200) PARAMETER (PRJ_CATEGORY = 201) PARAMETER (PRJ_PVRANGE = 202) PARAMETER (PRJ_SIMPLEZEN = 203) PARAMETER (PRJ_EQUIAREAL = 204) PARAMETER (PRJ_CONFORMAL = 205) PARAMETER (PRJ_GLOBAL = 206) PARAMETER (PRJ_DIVERGENT = 207) PARAMETER (PRJ_X0 = 208) PARAMETER (PRJ_Y0 = 209) PARAMETER (PRJ_ERR = 210) PARAMETER (PRJ_W = 211) PARAMETER (PRJ_N = 212) * Projection categories. INTEGER PRJ_CONIC, PRJ_CONVENTIONAL, PRJ_CYLINDRICAL, : PRJ_HEALPIX, PRJ_POLYCONIC, PRJ_PSEUDOCYLINDRICAL, : PRJ_QUADCUBE, PRJ_ZENITHAL PARAMETER (PRJ_ZENITHAL = 1) PARAMETER (PRJ_CYLINDRICAL = 2) PARAMETER (PRJ_PSEUDOCYLINDRICAL = 3) PARAMETER (PRJ_CONVENTIONAL = 4) PARAMETER (PRJ_CONIC = 5) PARAMETER (PRJ_POLYCONIC = 6) PARAMETER (PRJ_QUADCUBE = 7) PARAMETER (PRJ_HEALPIX = 8) * Error codes and messages. INTEGER PRJERR_BAD_PARAM, PRJERR_BAD_PIX, PRJERR_BAD_WORLD, : PRJERR_NULL_POINTER, PRJERR_SUCCESS PARAMETER (PRJERR_SUCCESS = 0) PARAMETER (PRJERR_NULL_POINTER = 1) PARAMETER (PRJERR_BAD_PARAM = 2) PARAMETER (PRJERR_BAD_PIX = 3) PARAMETER (PRJERR_BAD_WORLD = 4) CHARACTER PRJ_ERRMSG(0:4)*80 COMMON /PRJ_DATA/ PRJ_ERRMSG pywcs-1.12/wcslib/Fortran/prj_f.c0000644001153600020070000002013012310355626021004 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: prj_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include /* Fortran name mangling. */ #include #define prjini_ F77_FUNC(prjini, PRJINI) #define prjput_ F77_FUNC(prjput, PRJPUT) #define prjget_ F77_FUNC(prjget, PRJGET) #define prjfree_ F77_FUNC(prjfree, PRJFREE) #define prjprt_ F77_FUNC(prjprt, PRJPRT) #define prjptc_ F77_FUNC(prjptc, PRJPTC) #define prjptd_ F77_FUNC(prjptd, PRJPTD) #define prjpti_ F77_FUNC(prjpti, PRJPTI) #define prjgtc_ F77_FUNC(prjgtc, PRJGTC) #define prjgtd_ F77_FUNC(prjgtd, PRJGTD) #define prjgti_ F77_FUNC(prjgti, PRJGTI) #define PRJ_FLAG 100 #define PRJ_CODE 101 #define PRJ_R0 102 #define PRJ_PV 103 #define PRJ_PHI0 104 #define PRJ_THETA0 105 #define PRJ_BOUNDS 106 #define PRJ_NAME 200 #define PRJ_CATEGORY 201 #define PRJ_PVRANGE 202 #define PRJ_SIMPLEZEN 203 #define PRJ_EQUIAREAL 204 #define PRJ_CONFORMAL 205 #define PRJ_GLOBAL 206 #define PRJ_DIVERGENT 207 #define PRJ_X0 208 #define PRJ_Y0 209 #define PRJ_ERR 210 #define PRJ_W 211 #define PRJ_N 212 /*--------------------------------------------------------------------------*/ int prjini_(int *prj) { return prjini((struct prjprm *)prj); } /*--------------------------------------------------------------------------*/ int prjput_(int *prj, const int *what, const void *value, const int *m) { const char *cvalp; const int *ivalp; const double *dvalp; struct prjprm *prjp; /* Cast pointers. */ prjp = (struct prjprm *)prj; cvalp = (const char *)value; ivalp = (const int *)value; dvalp = (const double *)value; prjp->flag = 0; switch (*what) { case PRJ_FLAG: prjp->flag = *ivalp; break; case PRJ_CODE: strncpy(prjp->code, cvalp, 3); prjp->code[3] = '\0'; break; case PRJ_R0: prjp->r0 = *dvalp; break; case PRJ_PV: prjp->pv[*m] = *dvalp; break; case PRJ_PHI0: prjp->phi0 = *dvalp; break; case PRJ_THETA0: prjp->theta0 = *dvalp; break; case PRJ_BOUNDS: prjp->bounds = *ivalp; break; default: return 1; } return 0; } int prjptc_(int *prj, const int *what, const char *value, const int *m) { return prjput_(prj, what, value, m); } int prjptd_(int *prj, const int *what, const double *value, const int *m) { return prjput_(prj, what, value, m); } int prjpti_(int *prj, const int *what, const int *value, const int *m) { return prjput_(prj, what, value, m); } /*--------------------------------------------------------------------------*/ int prjget_(const int *prj, const int *what, void *value) { int k, m; char *cvalp; int *ivalp; double *dvalp; const int *iprjp; const struct prjprm *prjp; /* Cast pointers. */ prjp = (const struct prjprm *)prj; cvalp = (char *)value; ivalp = (int *)value; dvalp = (double *)value; switch (*what) { case PRJ_FLAG: *ivalp = prjp->flag; break; case PRJ_CODE: strncpy(cvalp, prjp->code, 3); break; case PRJ_R0: *dvalp = prjp->r0; break; case PRJ_PV: for (m = 0; m < PVN; m++) { *(dvalp++) = prjp->pv[m]; } break; case PRJ_PHI0: *dvalp = prjp->phi0; break; case PRJ_THETA0: *dvalp = prjp->theta0; break; case PRJ_BOUNDS: *ivalp = prjp->bounds; break; case PRJ_NAME: strncpy(cvalp, prjp->name, 40); break; case PRJ_CATEGORY: *ivalp = prjp->category; break; case PRJ_PVRANGE: *ivalp = prjp->pvrange; break; case PRJ_SIMPLEZEN: *ivalp = prjp->simplezen; break; case PRJ_EQUIAREAL: *ivalp = prjp->equiareal; break; case PRJ_CONFORMAL: *ivalp = prjp->conformal; break; case PRJ_GLOBAL: *ivalp = prjp->global; break; case PRJ_DIVERGENT: *ivalp = prjp->divergent; break; case PRJ_X0: *dvalp = prjp->x0; break; case PRJ_Y0: *dvalp = prjp->y0; break; case PRJ_ERR: /* Copy the contents of the wcserr struct. */ if (prjp->err) { iprjp = (int *)(prjp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(iprjp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; case PRJ_W: for (m = 0; m < 10; m++) { *(dvalp++) = prjp->w[m]; } break; case PRJ_N: *ivalp = prjp->n; break; default: return 1; } return 0; } int prjgtc_(const int *prj, const int *what, char *value) { return prjget_(prj, what, value); } int prjgtd_(const int *prj, const int *what, double *value) { return prjget_(prj, what, value); } int prjgti_(const int *prj, const int *what, int *value) { return prjget_(prj, what, value); } /*--------------------------------------------------------------------------*/ int prjfree_(int *prj) { return prjfree((struct prjprm *)prj); } /*--------------------------------------------------------------------------*/ int prjprt_(int *prj) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling PRJPRT in the Fortran code. */ fflush(NULL); return prjprt((struct prjprm *)prj); } /*--------------------------------------------------------------------------*/ #define PRJSET_FWRAP(pcode, PCODE) \ int F77_FUNC(pcode##set, PCODE##SET)(int *prj) \ {return prjset((struct prjprm *)prj);} #define PRJS2X_FWRAP(pcode, PCODE) \ int F77_FUNC(pcode##s2x, PCODE##S2X)( \ int *prj, \ const int *nphi, \ const int *ntheta, \ const int *spt, \ const int *sxy, \ const double phi[], \ const double theta[], \ double x[], \ double y[], \ int stat[]) \ {return prj##s2x((struct prjprm *)prj, *nphi, *ntheta, *spt, *sxy, \ phi, theta, x, y, stat);} #define PRJX2S_FWRAP(pcode, PCODE) \ int F77_FUNC(pcode##x2s, PRJ##X2S)( \ int *prj, \ const int *nx, \ const int *ny, \ const int *sxy, \ const int *spt, \ const double x[], \ const double y[], \ double phi[], \ double theta[], \ int stat[]) \ {return pcode##x2s((struct prjprm *)prj, *nx, *ny, *sxy, *spt, x, y, \ phi, theta, stat);} #define PRJ_FWRAP(pcode, PCODE) \ PRJSET_FWRAP(pcode, PCODE) \ PRJS2X_FWRAP(pcode, PCODE) \ PRJX2S_FWRAP(pcode, PCODE) PRJ_FWRAP(prj, PRJ) PRJ_FWRAP(azp, AZP) PRJ_FWRAP(szp, SZP) PRJ_FWRAP(tan, TAN) PRJ_FWRAP(stg, STG) PRJ_FWRAP(sin, SIN) PRJ_FWRAP(arc, ARC) PRJ_FWRAP(zpn, ZPN) PRJ_FWRAP(zea, ZEA) PRJ_FWRAP(air, AIR) PRJ_FWRAP(cyp, CYP) PRJ_FWRAP(cea, CEA) PRJ_FWRAP(car, CAR) PRJ_FWRAP(mer, MER) PRJ_FWRAP(sfl, SFL) PRJ_FWRAP(par, PAR) PRJ_FWRAP(mol, MOL) PRJ_FWRAP(ait, AIT) PRJ_FWRAP(cop, COP) PRJ_FWRAP(coe, COE) PRJ_FWRAP(cod, COD) PRJ_FWRAP(coo, COO) PRJ_FWRAP(bon, BON) PRJ_FWRAP(pco, PCO) PRJ_FWRAP(tsc, TSC) PRJ_FWRAP(csc, CSC) PRJ_FWRAP(qsc, QSC) PRJ_FWRAP(hpx, HPX) pywcs-1.12/wcslib/Fortran/spc.inc0000644001153600020070000000623212310355626021027 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: spc.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL SPCAIPS, SPCFREE, SPCGET, SPCGTC, SPCGTD, SPCGTI, : SPCINI, SPCPRT, SPCPTC, SPCPTD, SPCPTI, SPCPUT, SPCS2X, : SPCSET, SPCSPXE, SPCTRNE, SPCTYPE, SPCX2S, SPCXPSE INTEGER SPCAIPS, SPCFREE, SPCGET, SPCGTC, SPCGTD, SPCGTI, : SPCINI, SPCPRT, SPCPTC, SPCPTD, SPCPTI, SPCPUT, SPCS2X, : SPCSET, SPCSPXE, SPCTRNE, SPCTYPE, SPCX2S, SPCXPSE * Deprecated functions. EXTERNAL SPCSPX, SPCTRN, SPCTYP, SPCXPS INTEGER SPCSPX, SPCTRN, SPCTYP, SPCXPS * Length of the SPCPRM data structure (INTEGER array) on 64-bit * machines. Only needs to be 44 on 32-bit machines. INTEGER SPCLEN PARAMETER (SPCLEN = 50) * Codes for SPC data structure elements used by SPCPUT and SPCGET. INTEGER SPC_CODE, SPC_CRVAL, SPC_FLAG, SPC_PV, SPC_RESTFRQ, : SPC_RESTWAV, SPC_TYPE PARAMETER (SPC_FLAG = 100) PARAMETER (SPC_TYPE = 101) PARAMETER (SPC_CODE = 102) PARAMETER (SPC_CRVAL = 103) PARAMETER (SPC_RESTFRQ = 104) PARAMETER (SPC_RESTWAV = 105) PARAMETER (SPC_PV = 106) * Codes for SPC data structure elements used by SPCGET (only). INTEGER SPC_ERR, SPC_ISGRISM, SPC_W PARAMETER (SPC_W = 200) PARAMETER (SPC_ISGRISM = 201) PARAMETER (SPC_ERR = 202) * Error codes and messages. INTEGER SPCERR_BAD_SPEC, SPCERR_BAD_SPEC_PARAMS, SPCERR_BAD_X, : SPCERR_NULL_POINTER, SPCERR_SUCCESS PARAMETER (SPCERR_SUCCESS = 0) PARAMETER (SPCERR_NULL_POINTER = 1) PARAMETER (SPCERR_BAD_SPEC_PARAMS = 2) PARAMETER (SPCERR_BAD_X = 3) PARAMETER (SPCERR_BAD_SPEC = 4) CHARACTER SPC_ERRMSG(0:4)*80 COMMON /SPC_DATA/ SPC_ERRMSG pywcs-1.12/wcslib/Fortran/spc_f.c0000644001153600020070000002636712310355626021020 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: spc_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include #include /* Fortran name mangling. */ #include #define spcini_ F77_FUNC(spcini, SPCINI) #define spcput_ F77_FUNC(spcput, SPCPUT) #define spcget_ F77_FUNC(spcget, SPCGET) #define spcfree_ F77_FUNC(spcfree, SPCFREE) #define spcprt_ F77_FUNC(spcprt, SPCPRT) #define spcset_ F77_FUNC(spcset, SPCSET) #define spcx2s_ F77_FUNC(spcx2s, SPCX2S) #define spcs2x_ F77_FUNC(spcs2x, SPCS2X) #define spctype_ F77_FUNC(spctype, SPCTYPE) #define spcspxe_ F77_FUNC(spcspxe, SPCSPXE) #define spcxpse_ F77_FUNC(spcxpse, SPCXPSE) #define spctrne_ F77_FUNC(spctrne, SPCTRNE) #define spcaips_ F77_FUNC(spcaips, SPCAIPS) #define spcptc_ F77_FUNC(spcptc, SPCPTC) #define spcptd_ F77_FUNC(spcptd, SPCPTD) #define spcpti_ F77_FUNC(spcpti, SPCPTI) #define spcgtc_ F77_FUNC(spcgtc, SPCGTC) #define spcgtd_ F77_FUNC(spcgtd, SPCGTD) #define spcgti_ F77_FUNC(spcgti, SPCGTI) /* Deprecated. */ #define spctyp_ F77_FUNC(spctyp, SPCTYP) #define spcspx_ F77_FUNC(spcspx, SPCSPX) #define spcxps_ F77_FUNC(spcxps, SPCXPS) #define spctrn_ F77_FUNC(spctrn, SPCTRN) #define SPC_FLAG 100 #define SPC_TYPE 101 #define SPC_CODE 102 #define SPC_CRVAL 103 #define SPC_RESTFRQ 104 #define SPC_RESTWAV 105 #define SPC_PV 106 #define SPC_W 200 #define SPC_ISGRISM 201 #define SPC_ERR 202 /*--------------------------------------------------------------------------*/ int spcini_(int *spc) { return spcini((struct spcprm *)spc); } /*--------------------------------------------------------------------------*/ int spcput_(int *spc, const int *what, const void *value, const int *m) { const char *cvalp; const int *ivalp; const double *dvalp; struct spcprm *spcp; /* Cast pointers. */ spcp = (struct spcprm *)spc; cvalp = (const char *)value; ivalp = (const int *)value; dvalp = (const double *)value; spcp->flag = 0; switch (*what) { case SPC_FLAG: spcp->flag = *ivalp; break; case SPC_TYPE: strncpy(spcp->type, cvalp, 4); spcp->type[4] = '\0'; break; case SPC_CODE: strncpy(spcp->code, cvalp, 3); spcp->code[3] = '\0'; break; case SPC_CRVAL: spcp->crval = *dvalp; break; case SPC_RESTFRQ: spcp->restfrq = *dvalp; break; case SPC_RESTWAV: spcp->restwav = *dvalp; break; case SPC_PV: spcp->pv[*m] = *dvalp; break; default: return 1; } return 0; } int spcptc_(int *spc, const int *what, const char *value, const int *m) { return spcput_(spc, what, value, m); } int spcptd_(int *spc, const int *what, const double *value, const int *m) { return spcput_(spc, what, value, m); } int spcpti_(int *spc, const int *what, const int *value, const int *m) { return spcput_(spc, what, value, m); } /*--------------------------------------------------------------------------*/ int spcget_(const int *spc, const int *what, void *value) { int k, m; char *cvalp; int *ivalp; double *dvalp; const int *ispcp; const struct spcprm *spcp; /* Cast pointers. */ spcp = (const struct spcprm *)spc; cvalp = (char *)value; ivalp = (int *)value; dvalp = (double *)value; switch (*what) { case SPC_FLAG: *ivalp = spcp->flag; break; case SPC_TYPE: strncpy(cvalp, spcp->type, 4); break; case SPC_CODE: strncpy(cvalp, spcp->code, 3); break; case SPC_CRVAL: *dvalp = spcp->crval; break; case SPC_RESTFRQ: *dvalp = spcp->restfrq; break; case SPC_RESTWAV: *dvalp = spcp->restwav; break; case SPC_PV: for (m = 0; m < 7; m++) { *(dvalp++) = spcp->pv[m]; } break; case SPC_W: for (m = 0; m < 6; m++) { *(dvalp++) = spcp->w[m]; } break; case SPC_ISGRISM: *ivalp = spcp->isGrism; break; case SPC_ERR: /* Copy the contents of the wcserr struct. */ if (spcp->err) { ispcp = (int *)(spcp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(ispcp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; default: return 1; } return 0; } int spcgtc_(const int *spc, const int *what, char *value) { return spcget_(spc, what, value); } int spcgtd_(const int *spc, const int *what, double *value) { return spcget_(spc, what, value); } int spcgti_(const int *spc, const int *what, int *value) { return spcget_(spc, what, value); } /*--------------------------------------------------------------------------*/ int spcfree_(int *spc) { return spcfree((struct spcprm *)spc); } /*--------------------------------------------------------------------------*/ int spcprt_(int *spc) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling SPCPRT in the Fortran code. */ fflush(NULL); return spcprt((struct spcprm *)spc); } /*--------------------------------------------------------------------------*/ int spcset_(int *spc) { return spcset((struct spcprm *)spc); } /*--------------------------------------------------------------------------*/ int spcx2s_( int *spc, const int *nx, const int *sspec, const int *sx, const double x[], double spec[], int stat[]) { return spcx2s((struct spcprm *)spc, *nx, *sx, *sspec, x, spec, stat); } /*--------------------------------------------------------------------------*/ int spcs2x_( int *spc, const int *nspec, const int *sspec, const int *sx, const double spec[], double x[], int stat[]) { return spcs2x((struct spcprm *)spc, *nspec, *sspec, *sx, spec, x, stat); } /*--------------------------------------------------------------------------*/ int spctype_( const char ctypei[8], char stype[4], char scode[3], char sname[21], char units[7], char ptype[1], char xtype[1], int *restreq, iptr err) { char ctypei_[9], scode_[4], sname_[22], stype_[5], units_[8]; int status; strncpy(ctypei_, ctypei, 8); ctypei_[8] = '\0'; status = spctype(ctypei_, stype_, scode_, sname_, units_, ptype, xtype, restreq, (struct wcserr **)err); wcsutil_blank_fill( 5, stype_); wcsutil_blank_fill( 4, scode_); wcsutil_blank_fill(22, sname_); wcsutil_blank_fill( 8, units_); strncpy(stype, stype_, 4); strncpy(scode, scode_, 3); strncpy(sname, sname_, 21); strncpy(units, units_, 7); return status; } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spctyp_( const char ctypei[8], char stype[4], char scode[3], char sname[21], char units[7], char ptype[1], char xtype[1], int *restreq) { return spctype_(ctypei, stype, scode, sname, units, ptype, xtype, restreq, 0x0); } /*--------------------------------------------------------------------------*/ int spcspxe_( const char ctypeS[8], const double *crvalS, const double *restfrq, const double *restwav, char ptype[1], char xtype[1], int *restreq, double *crvalX, double *dXdS, iptr err) { char ctypeS_[9]; strncpy(ctypeS_, ctypeS, 8); ctypeS_[8] = '\0'; return spcspxe(ctypeS_, *crvalS, *restfrq, *restwav, ptype, xtype, restreq, crvalX, dXdS, (struct wcserr **)err); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spcspx_( const char ctypeS[8], const double *crvalS, const double *restfrq, const double *restwav, char ptype[1], char xtype[1], int *restreq, double *crvalX, double *dXdS) { return spcspxe_(ctypeS, crvalS, restfrq, restwav, ptype, xtype, restreq, crvalX, dXdS, 0x0); } /*--------------------------------------------------------------------------*/ int spcxpse_( const char ctypeS[8], const double *crvalX, const double *restfrq, const double *restwav, char ptype[1], char xtype[1], int *restreq, double *crvalS, double *dSdX, iptr err) { char ctypeS_[9]; strncpy(ctypeS_, ctypeS, 8); ctypeS_[8] = '\0'; return spcxpse(ctypeS_, *crvalX, *restfrq, *restwav, ptype, xtype, restreq, crvalS, dSdX, (struct wcserr **)err); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spcxps_( const char ctypeS[8], const double *crvalX, const double *restfrq, const double *restwav, char ptype[1], char xtype[1], int *restreq, double *crvalS, double *dSdX) { return spcxpse_(ctypeS, crvalX, restfrq, restwav, ptype, xtype, restreq, crvalS, dSdX, 0x0); } /*--------------------------------------------------------------------------*/ int spctrne_( const char ctypeS1[8], const double *crvalS1, const double *cdeltS1, const double *restfrq, const double *restwav, char ctypeS2[8], double *crvalS2, double *cdeltS2, iptr err) { int status; char ctypeS1_[9], ctypeS2_[9]; strncpy(ctypeS1_, ctypeS1, 8); ctypeS1_[8] = '\0'; status = spctrne(ctypeS1_, *crvalS1, *cdeltS1, *restfrq, *restwav, ctypeS2_, crvalS2, cdeltS2, (struct wcserr **)err); wcsutil_blank_fill(9, ctypeS2_); strncpy(ctypeS2, ctypeS2_, 8); return status; } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int spctrn_( const char ctypeS1[8], const double *crvalS1, const double *cdeltS1, const double *restfrq, const double *restwav, char ctypeS2[8], double *crvalS2, double *cdeltS2) { return spctrne_(ctypeS1, crvalS1, cdeltS1, restfrq, restwav, ctypeS2, crvalS2, cdeltS2, 0x0); } /*--------------------------------------------------------------------------*/ int spcaips_( const char ctypeA[8], int *velref, char ctype[8], char specsys[8]) { int status; char ctypeA_[9], ctype_[9], specsys_[9]; strncpy(ctypeA_, ctypeA, 8); ctypeA_[8] = '\0'; status = spcaips(ctypeA_, *velref, ctype_, specsys_); wcsutil_blank_fill(9, ctype_); strncpy(ctype, ctype_, 8); wcsutil_blank_fill(9, specsys_); strncpy(specsys, specsys_, 8); return status; } pywcs-1.12/wcslib/Fortran/sph.inc0000644001153600020070000000273712310355626021042 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: sph.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL SPHDPA, SPHPAD, SPHS2X, SPHX2S INTEGER SPHDPA, SPHPAD, SPHS2X, SPHX2S pywcs-1.12/wcslib/Fortran/sph_f.c0000644001153600020070000000556212310355626021017 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: sph_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include /* Fortran name mangling. */ #include #define sphx2s_ F77_FUNC(sphx2s, SPHX2S) #define sphs2x_ F77_FUNC(sphs2x, SPHS2X) #define sphdpa_ F77_FUNC(sphdpa, SPHDPA) #define sphpad_ F77_FUNC(sphpad, SPHPAD) /*--------------------------------------------------------------------------*/ int sphx2s_( const double eul[5], const int *nphi, const int *ntheta, const int *spt, const int *sll, const double phi[], const double theta[], double lng[], double lat[]) { return sphx2s(eul, *nphi, *ntheta, *spt, *sll, phi, theta, lng, lat); } /*--------------------------------------------------------------------------*/ int sphs2x_( const double eul[5], const int *nlng, const int *nlat, const int *sll, const int *spt, const double lng[], const double lat[], double phi[], double theta[]) { return sphs2x(eul, *nlng, *nlat, *sll, *spt, lng, lat, phi, theta); } /*--------------------------------------------------------------------------*/ int sphdpa_( const int *nfield, const double *lng0, const double *lat0, const double lng[], const double lat[], double dist[], double pa[]) { return sphdpa(*nfield, *lng0, *lat0, lng, lat, dist, pa); } /*--------------------------------------------------------------------------*/ int sphpad_( const int *nfield, const double *lng0, const double *lat0, const double dist[], const double pa[], double lng[], double lat[]) { return sphpad(*nfield, *lng0, *lat0, dist, pa, lng, lat); } pywcs-1.12/wcslib/Fortran/spx.inc0000644001153600020070000001270112310355626021052 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: spx.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL SPECX, SPXGET, SPXGTI, : FREQAFRQ, AFRQFREQ, FREQENER, ENERFREQ, : FREQWAVN, WAVNFREQ, FREQVRAD, VRADFREQ, : FREQWAVE, WAVEFREQ, FREQAWAV, AWAVFREQ, : FREQVELO, VELOFREQ, WAVEVOPT, VOPTWAVE, : WAVEZOPT, ZOPTWAVE, WAVEAWAV, AWAVWAVE, : WAVEVELO, VELOWAVE, AWAVVELO, VELOAWAV, : VELOBETA, BETAVELO INTEGER SPECX, SPXGET, SPXGTI, : FREQAFRQ, AFRQFREQ, FREQENER, ENERFREQ, : FREQWAVN, WAVNFREQ, FREQVRAD, VRADFREQ, : FREQWAVE, WAVEFREQ, FREQAWAV, AWAVFREQ, : FREQVELO, VELOFREQ, WAVEVOPT, VOPTWAVE, : WAVEZOPT, ZOPTWAVE, WAVEAWAV, AWAVWAVE, : WAVEVELO, VELOWAVE, AWAVVELO, VELOAWAV, : VELOBETA, BETAVELO * Spectral data structure. INTEGER SPX_WAVETYPE, SPX_VELOTYPE DOUBLE PRECISION : SPX_RESTFRQ, SPX_RESTWAV, SPX_TYPES, : SPX_FREQ, SPX_AFRQ, SPX_ENER, SPX_WAVN, : SPX_VRAD, SPX_WAVE, SPX_VOPT, SPX_ZOPT, : SPX_AWAV, SPX_VELO, SPX_BETA, : SPX_DFREQAFRQ, SPX_DAFRQFREQ, SPX_DFREQENER, : SPX_DENERFREQ, SPX_DFREQWAVN, SPX_DWAVNFREQ, : SPX_DFREQVRAD, SPX_DVRADFREQ, SPX_DFREQWAVE, : SPX_DWAVEFREQ, SPX_DFREQAWAV, SPX_DAWAVFREQ, : SPX_DFREQVELO, SPX_DVELOFREQ, SPX_DWAVEVOPT, : SPX_DVOPTWAVE, SPX_DWAVEZOPT, SPX_DZOPTWAVE, : SPX_DWAVEAWAV, SPX_DAWAVWAVE, SPX_DWAVEVELO, : SPX_DVELOWAVE, SPX_DAWAVVELO, SPX_DVELOAWAV, : SPX_DVELOBETA, SPX_DBETAVELO * Direct equivalences into the data structure (not indexing codes). DOUBLE PRECISION SPX(40) EQUIVALENCE (SPX( 1), SPX_RESTFRQ) EQUIVALENCE (SPX( 2), SPX_RESTWAV) EQUIVALENCE (SPX( 3), SPX_TYPES) EQUIVALENCE (SPX( 4), SPX_FREQ) EQUIVALENCE (SPX( 5), SPX_AFRQ) EQUIVALENCE (SPX( 6), SPX_ENER) EQUIVALENCE (SPX( 7), SPX_WAVN) EQUIVALENCE (SPX( 8), SPX_VRAD) EQUIVALENCE (SPX( 9), SPX_WAVE) EQUIVALENCE (SPX(10), SPX_VOPT) EQUIVALENCE (SPX(11), SPX_ZOPT) EQUIVALENCE (SPX(12), SPX_AWAV) EQUIVALENCE (SPX(13), SPX_VELO) EQUIVALENCE (SPX(14), SPX_BETA) EQUIVALENCE (SPX(15), SPX_DFREQAFRQ) EQUIVALENCE (SPX(16), SPX_DAFRQFREQ) EQUIVALENCE (SPX(17), SPX_DFREQENER) EQUIVALENCE (SPX(18), SPX_DENERFREQ) EQUIVALENCE (SPX(19), SPX_DFREQWAVN) EQUIVALENCE (SPX(20), SPX_DWAVNFREQ) EQUIVALENCE (SPX(21), SPX_DFREQVRAD) EQUIVALENCE (SPX(22), SPX_DVRADFREQ) EQUIVALENCE (SPX(23), SPX_DFREQWAVE) EQUIVALENCE (SPX(24), SPX_DWAVEFREQ) EQUIVALENCE (SPX(25), SPX_DFREQAWAV) EQUIVALENCE (SPX(26), SPX_DAWAVFREQ) EQUIVALENCE (SPX(27), SPX_DFREQVELO) EQUIVALENCE (SPX(28), SPX_DVELOFREQ) EQUIVALENCE (SPX(29), SPX_DWAVEVOPT) EQUIVALENCE (SPX(30), SPX_DVOPTWAVE) EQUIVALENCE (SPX(31), SPX_DWAVEZOPT) EQUIVALENCE (SPX(32), SPX_DZOPTWAVE) EQUIVALENCE (SPX(33), SPX_DWAVEAWAV) EQUIVALENCE (SPX(34), SPX_DAWAVWAVE) EQUIVALENCE (SPX(35), SPX_DWAVEVELO) EQUIVALENCE (SPX(36), SPX_DVELOWAVE) EQUIVALENCE (SPX(37), SPX_DAWAVVELO) EQUIVALENCE (SPX(38), SPX_DVELOAWAV) EQUIVALENCE (SPX(39), SPX_DVELOBETA) EQUIVALENCE (SPX(40), SPX_DBETAVELO) INTEGER SPXI(2) EQUIVALENCE (SPXI, SPX_TYPES) EQUIVALENCE (SPXI(1), SPX_WAVETYPE) EQUIVALENCE (SPXI(2), SPX_VELOTYPE) * Codes for SPX data structure elements used by SPXGET (only). INTEGER SPX_ERR PARAMETER (SPX_ERR = 200) * Error codes and messages. INTEGER SPXERR_BAD_INSPEC_COORD, SPXERR_BAD_SPEC_PARAMS, : SPXERR_BAD_SPEC_VAR, SPXERR_NULL_POINTER, SPXERR_SUCCESS PARAMETER (SPXERR_SUCCESS = 0) PARAMETER (SPXERR_NULL_POINTER = 1) PARAMETER (SPXERR_BAD_SPEC_PARAMS = 2) PARAMETER (SPXERR_BAD_SPEC_VAR = 3) PARAMETER (SPXERR_BAD_INSPEC_COORD = 4) CHARACTER SPX_ERRMSG(0:4)*80 COMMON /SPX_DATA/ SPX_ERRMSG pywcs-1.12/wcslib/Fortran/spx_f.c0000644001153600020070000000743012310355626021033 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: spx_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include /* Fortran name mangling. */ #include #define spxget_ F77_FUNC(spxget, SPXGET) #define specx_ F77_FUNC(specx, SPECX) #define SPX_ERR 200 /*--------------------------------------------------------------------------*/ int spxget_(const int *spx, const int *what, void *value) { int k; int *ivalp; const int *ispxp; const struct spxprm *spxp; /* Cast pointers. */ spxp = (const struct spxprm *)spx; ivalp = (int *)value; switch (*what) { case SPX_ERR: /* Copy the contents of the wcserr struct. */ if (spxp->err) { ispxp = (int *)(spxp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(ispxp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; default: return 1; } return 0; } int spxgti_(const int *spx, const int *what, int *value) { return spxget_(spx, what, value); } /*--------------------------------------------------------------------------*/ int specx_( const char *type, const double *spec, const double *restfrq, const double *restwav, double *specs) { char stype[5]; strncpy(stype, type, 4); stype[4] = '\0'; return specx(stype, *spec, *restfrq, *restwav, (struct spxprm *)specs); } /*--------------------------------------------------------------------------*/ #define SPX_FWRAP(scode, SCODE) \ int F77_FUNC(scode, SCODE)( \ const double *rest, \ const int *n1, \ const int *s1, \ const int *s2, \ const double spec1[], \ double spec2[], \ int stat[]) \ {return scode(*rest, *n1, *s1, *s2, spec1, spec2, stat);} SPX_FWRAP(freqafrq, FREQAFRQ) SPX_FWRAP(afrqfreq, AFRQFREQ) SPX_FWRAP(freqener, FREQENER) SPX_FWRAP(enerfreq, ENERFREQ) SPX_FWRAP(freqwavn, FREQWAVN) SPX_FWRAP(wavnfreq, WAVNFREQ) SPX_FWRAP(freqvrad, FREQVRAD) SPX_FWRAP(vradfreq, VRADFREQ) SPX_FWRAP(freqwave, FREQWAVE) SPX_FWRAP(wavefreq, WAVEFREQ) SPX_FWRAP(freqawav, FREQAWAV) SPX_FWRAP(awavfreq, AWAVFREQ) SPX_FWRAP(freqvelo, FREQVELO) SPX_FWRAP(velofreq, VELOFREQ) SPX_FWRAP(wavevopt, WAVEVOPT) SPX_FWRAP(voptwave, VOPTWAVE) SPX_FWRAP(wavezopt, WAVEZOPT) SPX_FWRAP(zoptwave, ZOPTWAVE) SPX_FWRAP(waveawav, WAVEAWAV) SPX_FWRAP(awavwave, AWAVWAVE) SPX_FWRAP(wavevelo, WAVEVELO) SPX_FWRAP(velowave, VELOWAVE) SPX_FWRAP(awavvelo, AWAVVELO) SPX_FWRAP(veloawav, VELOAWAV) SPX_FWRAP(velobeta, VELOBETA) SPX_FWRAP(betavelo, BETAVELO) pywcs-1.12/wcslib/Fortran/tab.inc0000644001153600020070000000613512310355626021012 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tab.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL TABCPY, TABFREE, TABGET, TABGTD, TABGTI, TABINI, TABMEM, : TABPRT, TABPTD, TABPTI, TABPUT, TABS2X, TABSET, TABX2S INTEGER TABCPY, TABFREE, TABGET, TABGTD, TABGTI, TABINI, TABMEM, : TABPRT, TABPTD, TABPTI, TABPUT, TABS2X, TABSET, TABX2S * Length of the TABPRM data structure (INTEGER array) on 64-bit * machines. Only needs to be 24 on 32-bit machines. INTEGER TABLEN PARAMETER (TABLEN = 40) * Codes for TAB data structure elements used by TABPUT and TABGET. INTEGER TAB_COORD, TAB_CRVAL, TAB_FLAG, TAB_INDEX, TAB_K, TAB_M, : TAB_MAP PARAMETER (TAB_FLAG = 100) PARAMETER (TAB_M = 101) PARAMETER (TAB_K = 102) PARAMETER (TAB_MAP = 103) PARAMETER (TAB_CRVAL = 104) PARAMETER (TAB_INDEX = 105) PARAMETER (TAB_COORD = 106) * Codes for TAB data structure elements used by TABGET (only). INTEGER TAB_DELTA, TAB_ERR, TAB_EXTREMA, TAB_NC, TAB_P0, : TAB_SENSE PARAMETER (TAB_NC = 200) PARAMETER (TAB_SENSE = 201) PARAMETER (TAB_P0 = 202) PARAMETER (TAB_DELTA = 203) PARAMETER (TAB_EXTREMA = 204) PARAMETER (TAB_ERR = 205) * Error codes and messages. INTEGER TABERR_BAD_PARAMS, TABERR_BAD_WORLD, TABERR_BAD_X, : TABERR_MEMORY, TABERR_NULL_POINTER, TABERR_SUCCESS PARAMETER (TABERR_SUCCESS = 0) PARAMETER (TABERR_NULL_POINTER = 1) PARAMETER (TABERR_MEMORY = 2) PARAMETER (TABERR_BAD_PARAMS = 3) PARAMETER (TABERR_BAD_X = 4) PARAMETER (TABERR_BAD_WORLD = 5) CHARACTER TAB_ERRMSG(0:5)*80 COMMON /TAB_DATA/ TAB_ERRMSG pywcs-1.12/wcslib/Fortran/tab_f.c0000644001153600020070000001671512310355626020775 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: tab_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include /* Fortran name mangling. */ #include #define tabini_ F77_FUNC(tabini, TABINI) #define tabmem_ F77_FUNC(tabmem, TABMEM) #define tabcpy_ F77_FUNC(tabcpy, TABCPY) #define tabput_ F77_FUNC(tabput, TABPUT) #define tabget_ F77_FUNC(tabget, TABGET) #define tabfree_ F77_FUNC(tabfree, TABFREE) #define tabprt_ F77_FUNC(tabprt, TABPRT) #define tabset_ F77_FUNC(tabset, TABSET) #define tabx2s_ F77_FUNC(tabx2s, TABX2S) #define tabs2x_ F77_FUNC(tabs2x, TABS2X) #define tabptd_ F77_FUNC(tabptd, TABPTD) #define tabpti_ F77_FUNC(tabpti, TABPTI) #define tabgtd_ F77_FUNC(tabgtd, TABGTD) #define tabgti_ F77_FUNC(tabgti, TABGTI) #define TAB_FLAG 100 #define TAB_M 101 #define TAB_K 102 #define TAB_MAP 103 #define TAB_CRVAL 104 #define TAB_INDEX 105 #define TAB_COORD 106 #define TAB_NC 200 #define TAB_SENSE 201 #define TAB_P0 202 #define TAB_DELTA 203 #define TAB_EXTREMA 204 #define TAB_ERR 205 /*--------------------------------------------------------------------------*/ int tabini_(const int *M, const int *K, int *tab) { return tabini(1, *M, K, (struct tabprm *)tab); } /*--------------------------------------------------------------------------*/ int tabmem_(int *tab) { return tabmem((struct tabprm *)tab); } /*--------------------------------------------------------------------------*/ int tabcpy_(const int *tabsrc, int *tabdst) { return tabcpy(1, (const struct tabprm *)tabsrc, (struct tabprm *)tabdst); } /*--------------------------------------------------------------------------*/ int tabput_( int *tab, const int *what, const void *value, const int *m, const int *k) { int k0, m0; const int *ivalp; const double *dvalp; struct tabprm *tabp; /* Cast pointers. */ tabp = (struct tabprm *)tab; ivalp = (const int *)value; dvalp = (const double *)value; /* Convert 1-relative FITS axis numbers to 0-relative C array indices. */ m0 = *m - 1; k0 = *k - 1; tabp->flag = 0; switch (*what) { case TAB_FLAG: tabp->flag = *ivalp; break; case TAB_M: tabp->M = *ivalp; break; case TAB_K: tabp->K[m0] = *ivalp; break; case TAB_MAP: tabp->map[m0] = *ivalp; break; case TAB_CRVAL: tabp->crval[m0] = *dvalp; break; case TAB_INDEX: tabp->index[m0][k0] = *dvalp; break; case TAB_COORD: tabp->coord[m0] = *dvalp; break; default: return 1; } return 0; } int tabptd_(int *tab, const int *what, const double *value, const int *m, const int *k) { return tabput_(tab, what, value, m, k); } int tabpti_(int *tab, const int *what, const int *value, const int *m, const int *k) { return tabput_(tab, what, value, m, k); } /*--------------------------------------------------------------------------*/ int tabget_(const int *tab, const int *what, void *value) { int i, k, m, n; int *ivalp; double *dvalp; const int *itabp; const struct tabprm *tabp; /* Cast pointers. */ tabp = (const struct tabprm *)tab; ivalp = (int *)value; dvalp = (double *)value; switch (*what) { case TAB_FLAG: *ivalp = tabp->flag; break; case TAB_M: *ivalp = tabp->M; break; case TAB_K: for (m = 0; m < tabp->M; m++) { *(ivalp++) = tabp->K[m]; } break; case TAB_MAP: for (m = 0; m < tabp->M; m++) { *(ivalp++) = tabp->map[m]; } break; case TAB_CRVAL: for (m = 0; m < tabp->M; m++) { *(dvalp++) = tabp->crval[m]; } break; case TAB_INDEX: for (m = 0; m < tabp->M; m++) { for (k = 0; k < tabp->K[m]; k++) { *(dvalp++) = tabp->index[m][k]; } } break; case TAB_COORD: /* Don't rely on tabprm.nc being set. */ n = tabp->M; for (m = 0; m < tabp->M; m++) { n *= tabp->K[m]; } for (i = 0; i < n; i++) { *(dvalp++) = tabp->coord[i]; } break; case TAB_NC: *ivalp = tabp->nc; break; case TAB_SENSE: for (m = 0; m < tabp->M; m++) { *(ivalp++) = tabp->sense[m]; } break; case TAB_P0: for (m = 0; m < tabp->M; m++) { *(ivalp++) = tabp->p0[m]; } break; case TAB_DELTA: for (m = 0; m < tabp->M; m++) { *(dvalp++) = tabp->delta[m]; } break; case TAB_EXTREMA: n = 2 * tabp->M; for (m = 1; m < tabp->M; m++) { n *= tabp->K[m]; } for (i = 0; i < n; i++) { *(dvalp++) = tabp->extrema[i]; } break; case TAB_ERR: /* Copy the contents of the wcserr struct. */ if (tabp->err) { itabp = (int *)(tabp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(itabp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; default: return 1; } return 0; } int tabgtd_(const int *tab, const int *what, double *value) { return tabget_(tab, what, value); } int tabgti_(const int *tab, const int *what, int *value) { return tabget_(tab, what, value); } /*--------------------------------------------------------------------------*/ int tabfree_(int *tab) { return tabfree((struct tabprm *)tab); } /*--------------------------------------------------------------------------*/ int tabprt_(const int *tab) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling TABPRT in the Fortran code. */ fflush(NULL); return tabprt((const struct tabprm *)tab); } /*--------------------------------------------------------------------------*/ int tabset_(int *tab) { return tabset((struct tabprm *)tab); } /*--------------------------------------------------------------------------*/ int tabx2s_( int *tab, const int *ncoord, const int *nelem, const double x[], double world[], int stat[]) { return tabx2s((struct tabprm *)tab, *ncoord, *nelem, x, world, stat); } /*--------------------------------------------------------------------------*/ int tabs2x_( struct tabprm* tab, const int *ncoord, const int *nelem, const double world[], double x[], int stat[]) { return tabs2x((struct tabprm *)tab, *ncoord, *nelem, world, x, stat); } pywcs-1.12/wcslib/Fortran/test/0000755001153600020070000000000012310355732020521 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/Fortran/test/tcel1.f0000644001153600020070000002637712310355626021721 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tcel1.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TCEL1 *----------------------------------------------------------------------- * * tcel1 tests the spherical projection driver routines supplied with * WCSLIB by drawing native and celestial coordinate graticules for * Bonne's projection. * *----------------------------------------------------------------------- INTEGER CI, CRVAL1, CRVAL2, ILAT, ILNG, J, K, LATPOL, LNGPOL, : STAT(361), STATUS REAL XR(512), YR(512) DOUBLE PRECISION LAT(181), LNG(361), PHI(361), REF(4), THETA(361), : X(361), Y(361) CHARACTER TEXT*72 * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary, done here using a equivalences. * Failure to do this may result in mysterious "bus errors". INCLUDE 'cel.inc' INCLUDE 'prj.inc' INTEGER CEL(CELLEN) INTEGER NTV(CELLEN) INTEGER PRJ(PRJLEN) DOUBLE PRECISION DUMMY1, DUMMY2, DUMMY3 EQUIVALENCE (CEL,DUMMY1), (NTV,DUMMY2), (PRJ,DUMMY3) *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing WCSLIB celestial coordinate transformation ', : 'routines (tcel1.f)',/, : '---------------------------------------------------', : '------------------') * Initialize. STATUS = CELINI (NTV) * Reference angles for the native graticule (in fact, the defaults). STATUS = CELPUT (NTV, CEL_REF, 0D0, 1) STATUS = CELPUT (NTV, CEL_REF, 0D0, 2) * Set up Bonne's projection with conformal latitude at +35. STATUS = CELGET (NTV, CEL_PRJ, PRJ) STATUS = PRJPUT (PRJ, PRJ_CODE, 'BON', 0) STATUS = PRJPUT (PRJ, PRJ_PV, 35D0, 1) STATUS = CELPUT (NTV, CEL_PRJ, PRJ, 0) * Celestial graticule. STATUS = CELINI (CEL) STATUS = CELPUT (CEL, CEL_PRJ, PRJ, 0) * PGPLOT initialization. CALL PGBEG (0, '/xwindow', 1, 1) * Define pen colours. CALL PGSCR (0, 0.00, 0.00, 0.00) CALL PGSCR (1, 1.00, 1.00, 0.00) CALL PGSCR (2, 1.00, 1.00, 1.00) CALL PGSCR (3, 0.50, 0.50, 0.80) CALL PGSCR (4, 0.80, 0.50, 0.50) CALL PGSCR (5, 0.80, 0.80, 0.80) CALL PGSCR (6, 0.50, 0.50, 0.80) CALL PGSCR (7, 0.80, 0.50, 0.50) CALL PGSCR (8, 0.30, 0.50, 0.30) * Define PGPLOT viewport. CALL PGENV (-180.0, 180.0, -90.0, 140.0, 1, -2) * Loop over CRVAL2, LONPOLE, and LATPOLE with CRVAL1 incrementing by * 15 degrees each time (it has an uninteresting effect). CRVAL1 = -180 DO 190 CRVAL2 = -90, 90, 30 DO 180 LNGPOL = -180, 180, 30 DO 170 LATPOL = -1, 1, 2 * For the celestial graticule, set the celestial * coordinates of the reference point of the projection * (which for Bonne's projection is at the intersection of * the native equator and prime meridian), the native * longitude of the celestial pole, and extra information * needed to determine the celestial latitude of the native * pole. These correspond to FITS keywords CRVAL1, CRVAL2, * LONPOLE, and LATPOLE. STATUS = CELPUT (CEL, CEL_FLAG, 0, 0) STATUS = CELPUT (CEL, CEL_REF, DBLE(CRVAL1), 1) STATUS = CELPUT (CEL, CEL_REF, DBLE(CRVAL2), 2) STATUS = CELPUT (CEL, CEL_REF, DBLE(LNGPOL), 3) STATUS = CELPUT (CEL, CEL_REF, DBLE(LATPOL), 4) * Skip invalid values of LONPOLE. STATUS = CELSET (CEL) IF (STATUS.NE.0) GO TO 170 * Skip redundant values of LATPOLE. STATUS = CELGET (CEL, CEL_REF, REF) IF (LATPOL.EQ.1 .AND. ABS(REF(4)).LT.0.1D0) GO TO 170 * Buffer PGPLOT output. CALL PGBBUF () CALL PGERAS () * Write a descriptive title. TEXT = 'Bonne''s projection (BON) - 15 degree graticule' WRITE (*, '(/,A)') TEXT CALL PGTEXT (-180.0, -100.0, TEXT) WRITE (TEXT, 20) REF(1), REF(2) 20 FORMAT ('centred on celestial coordinates (',F7.2,',',F6.2, : ')') WRITE (*, '(A)') TEXT CALL PGTEXT (-180.0, -110.0, TEXT) WRITE (TEXT, 30) REF(3), REF(4) 30 FORMAT ('with north celestial pole at native coordinates (', : F7.2,',',F7.2,')') WRITE (*, '(A)') TEXT CALL PGTEXT (-180.0, -120.0, TEXT) * Draw the native graticule faintly in the background. CALL PGSCI (8) * Draw native meridians of longitude. J = 1 DO 40 ILAT = -90, 90 LAT(J) = DBLE(ILAT) J = J + 1 40 CONTINUE DO 60 ILNG = -180, 180, 15 LNG(1) = DBLE(ILNG) IF (ILNG.EQ.-180) LNG(1) = -179.99D0 IF (ILNG.EQ.+180) LNG(1) = +179.99D0 * Dash the longitude of the celestial pole. IF (MOD(ILNG-LNGPOL,360).EQ.0) THEN CALL PGSLS (2) CALL PGSLW (5) END IF STATUS = CELS2X (NTV, 1, 181, 1, 1, LNG, LAT, PHI, THETA, : X, Y, STAT) K = 0 DO 50 J = 1, 181 IF (STAT(J).NE.0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 GO TO 50 END IF K = K + 1 XR(K) = -X(J) YR(K) = Y(J) 50 CONTINUE CALL PGLINE (K, XR, YR) CALL PGSLS (1) CALL PGSLW (1) 60 CONTINUE * Draw native parallels of latitude. LNG(1) = -179.99D0 LNG(361) = +179.99D0 J = 2 ILNG = -179 DO 70 ILNG = -179, 180 LNG(J) = DBLE(ILNG) J = J + 1 70 CONTINUE DO 90 ILAT = -90, 90, 15 LAT(1) = DBLE(ILAT) STATUS = CELS2X (NTV, 361, 1, 1, 1, LNG, LAT, PHI, THETA, : X, Y, STAT) K = 0 DO 80 J = 1, 361 IF (STAT(J).NE.0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 GO TO 80 END IF K = K + 1 XR(K) = -X(J) YR(K) = Y(J) 80 CONTINUE CALL PGLINE (K, XR, YR) 90 CONTINUE * Draw a colour-coded celestial coordinate graticule. CI = 1 * Draw celestial meridians of longitude. J = 1 DO 100 ILAT = -90, 90 LAT(J) = DBLE(ILAT) J = J + 1 100 CONTINUE DO 120 ILNG = -180, 180, 15 LNG(1) = DBLE(ILNG) CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILNG.EQ.0) THEN CALL PGSCI (1) ELSE CALL PGSCI (CI) END IF * Dash the reference longitude. IF (MOD(ILNG-CRVAL1,360).EQ.0) THEN CALL PGSLS (2) CALL PGSLW (5) END IF STATUS = CELS2X (CEL, 1, 181, 1, 1, LNG, LAT, PHI, THETA, : X, Y, STAT) K = 0 DO 110 J = 1, 181 IF (STAT(J).NE.0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 GO TO 110 END IF * Test for discontinuities. IF (J.GT.1) THEN IF (ABS(X(J) - X(J-1)).GT.4D0 .OR. : ABS(Y(J) - Y(J-1)).GT.4D0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 END IF END IF K = K + 1 XR(K) = -X(J) YR(K) = Y(J) 110 CONTINUE CALL PGLINE (K, XR, YR) CALL PGSLS (1) CALL PGSLW (1) 120 CONTINUE * Draw celestial parallels of latitude. J = 1 DO 130 ILNG = -180, 180 LNG(J) = DBLE(ILNG) J = J + 1 130 CONTINUE CI = 1 DO 150 ILAT = -90, 90, 15 LAT(1) = DBLE(ILAT) CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILAT.EQ.0) THEN CALL PGSCI (1) ELSE CALL PGSCI (CI) END IF * Dash the reference latitude. IF (ILAT.EQ.CRVAL2) THEN CALL PGSLS (2) CALL PGSLW (5) END IF STATUS = CELS2X (CEL, 361, 1, 1, 1, LNG, LAT, PHI, THETA, : X, Y, STAT) K = 0 DO 140 J = 1, 361 IF (STAT(J).NE.0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 GO TO 140 END IF * Test for discontinuities. IF (J.GT.1) THEN IF (ABS(X(J) - X(J-1)).GT.4D0 .OR. : ABS(Y(J) - Y(J-1)).GT.4D0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 END IF END IF K = K + 1 XR(K) = -X(J) YR(K) = Y(J) 140 CONTINUE CALL PGLINE (K, XR, YR) CALL PGSLS (1) CALL PGSLW (1) 150 CONTINUE * Flush PGPLOT buffer. CALL PGEBUF () WRITE (*, '(A,$)') ' Type for next page: ' READ (*, *, END=160) * Cycle through celestial longitudes. 160 CRVAL1 = CRVAL1 + 15 IF (CRVAL1.GT.180) CRVAL1 = -180 * Skip boring celestial latitudes. IF (CRVAL2.EQ.0) GO TO 190 170 CONTINUE 180 CONTINUE 190 CONTINUE CALL PGASK (0) CALL PGEND END pywcs-1.12/wcslib/Fortran/test/tfitshdr.f0000644001153600020070000002340612310355626022526 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tfitshdr.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TFITSHDR *----------------------------------------------------------------------- * * TFITSHDR tests FITSHDR, the FITS parser for image headers, by reading * a test header and printing the resulting fitskey structs. * * Input comes from file 'pih.fits'. * * WCSHDR is called first to extract all WCS-related keyrecords from the * input header before passing it on to FITSHDR. * * KEYS, which is meant to hold a pointer, is declared as an array of * length 2 to accomodate 64-bit machines for which sizeof(void *) = * 2*sizeof(int). *----------------------------------------------------------------------- LOGICAL GOTEND INTEGER CTRL, I, IERR, IVAL(8), J, K, KEYNO, KEYS(2), KEYTYP, : KTYP, NC, NKEYRC, NKEYID, NREJECT, NWCS, RELAX, STATUS, : ULEN, WCSP DOUBLE PRECISION FVAL(2) CHARACTER KEYREC*80, CVAL*72, HEADER*288001, KEYWRD*12, INFILE*9, : TEXT*84 INCLUDE 'wcshdr.inc' INCLUDE 'fitshdr.inc' INTEGER KEYIDS(KEYIDLEN,8) DATA INFILE /'pih.fits'/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing FITS image header parser (tfitshdr.f)',/, : '---------------------------------------------',/) * Open the FITS WCS test header for formatted, direct I/O. OPEN (UNIT=1, FILE=INFILE, FORM='FORMATTED', ACCESS='DIRECT', : RECL=80, IOSTAT=IERR) IF (IERR.NE.0) THEN WRITE (*, 20) IERR, INFILE 20 FORMAT ('ERROR',I3,' opening ',A) GO TO 999 END IF * Read in the FITS header, excluding COMMENT and HISTORY keyrecords. K = 1 NKEYRC = 0 GOTEND = .FALSE. DO 50 J = 0, 100 DO 40 I = 1, 36 READ (1, '(A80)', REC=36*J+I, IOSTAT=IERR) KEYREC IF (IERR.NE.0) THEN WRITE (*, 30) IERR 30 FORMAT ('ERROR',I3,' reading header.') GO TO 999 END IF HEADER(K:) = KEYREC K = K + 80 NKEYRC = NKEYRC + 1 IF (KEYREC(:8).EQ.'END ') THEN * An END keyrecord was read, read the rest of the block. GOTEND = .TRUE. END IF 40 CONTINUE IF (GOTEND) GO TO 60 50 CONTINUE 60 CLOSE (UNIT=1) HEADER(K:K) = CHAR (0) WRITE (*, 70) NKEYRC 70 FORMAT ('Found',I4,' header keyrecords.') * Cull all recognized, syntactically valid WCS keyrecords from the * header. RELAX = WCSHDR_all CTRL = -1 * WCSPIH will allocate memory for NWCS intialized WCSPRM structs. IERR = WCSPIH (HEADER, NKEYRC, RELAX, CTRL, NREJECT, NWCS, WCSP) IF (IERR.NE.0) THEN WRITE (*, 80) IERR 80 FORMAT ('WCSPIH ERROR',I2,'.') GO TO 999 END IF * Number remaining. DO 90 I = 1, 288001, 80 IF (HEADER(I:I).EQ.CHAR(0)) GO TO 100 90 CONTINUE 100 NKEYRC = I / 80 * Specific keywords to be located or culled. IERR = KEYIDPUT (KEYIDS, 0, KEYID_NAME, 'SIMPLE ') IERR = KEYIDPUT (KEYIDS, 1, KEYID_NAME, 'BITPIX ') IERR = KEYIDPUT (KEYIDS, 2, KEYID_NAME, 'NAXIS ') IERR = KEYIDPUT (KEYIDS, 3, KEYID_NAME, 'COMMENT ') IERR = KEYIDPUT (KEYIDS, 4, KEYID_NAME, 'HISTORY ') IERR = KEYIDPUT (KEYIDS, 5, KEYID_NAME, ' ') IERR = KEYIDPUT (KEYIDS, 6, KEYID_NAME, 'END ') NKEYID = 7 IF (NKEYID.GT.0) THEN WRITE (*, '(/,A)') : 'The following keyrecords will not be listed:' DO 120 I = 0, NKEYID-1 IERR = KEYIDGET (KEYIDS, I, KEYID_NAME, TEXT) WRITE (*, 110) TEXT 110 FORMAT (' "',A8,'"') 120 CONTINUE END IF * Parse the header. IERR = FITSHDR (HEADER, NKEYRC, NKEYID, KEYIDS, NREJECT, KEYS) IF (IERR.NE.0) THEN WRITE (*, 130) IERR 130 FORMAT ('FITSKEY ERROR',I2) END IF * Report the results. WRITE (*, 140) NKEYRC, NREJECT 140 FORMAT(/,I3,' header keyrecords parsed by FITSHDR,',I3, : ' rejected:',/) DO 200 I = 0, NKEYRC-1 * Skip syntactically valid keyrecords that were indexed. IERR = KEYGET (KEYS, I, KEY_KEYNO, KEYNO, NC) IERR = KEYGET (KEYS, I, KEY_STATUS, STATUS, NC) IF (KEYNO.LT.0 .AND. STATUS.EQ.0) GO TO 200 * Basic keyrecord info. IERR = KEYGET (KEYS, I, KEY_KEYWORD, KEYWRD, NC) IERR = KEYGET (KEYS, I, KEY_TYPE, KEYTYP, NC) WRITE (*, '(I4,I5,2X,A,I3,$)') KEYNO, STATUS, KEYWRD(:8), : KEYTYP * Format the keyvalue for output. KTYP = MOD(ABS(KEYTYP),10) IF (KTYP.EQ.1) THEN * Logical. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, IVAL, NC) IF (IVAL(1).EQ.0) THEN TEXT = 'F' ELSE TEXT = 'T' END IF ELSE IF (KTYP.EQ.2) THEN * 32-bit signed integer. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, IVAL, NC) WRITE (TEXT, '(I11)') IVAL(1) ELSE IF (KTYP.EQ.3) THEN * 64-bit signed integer. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, IVAL, NC) IF (IVAL(3).NE.0) THEN WRITE (TEXT, '(SP,I11,SS,2I9.9)') IVAL(3), ABS(IVAL(2)), : ABS(IVAL(1)) ELSE WRITE (TEXT, '(SP,I11,SS,I9.9)') IVAL(2), ABS(IVAL(1)) END IF ELSE IF (KTYP.EQ.4) THEN * Very long integer. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, IVAL, NC) K = 0 DO 150 J = 8, 2, -1 IF (IVAL(J).NE.0) THEN K = J GO TO 160 END IF 150 CONTINUE 160 WRITE (TEXT, '(SP,I11)') IVAL(K) NC = 12 DO 170 J = K-1, 1, -1 WRITE (TEXT(NC:), '(I9.9)') ABS(IVAL(J)) NC = NC + 9 170 CONTINUE ELSE IF (KTYP.EQ.5) THEN * Float. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, FVAL, NC) WRITE (TEXT, '(SP,1PE13.6)') FVAL(1) ELSE IF (KTYP.EQ.6) THEN * Int complex. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, FVAL, NC) WRITE (TEXT, '(2I11)') NINT(FVAL(1)), NINT(FVAL(2)) ELSE IF (KTYP.EQ.7) THEN * Float complex. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, FVAL, NC) WRITE (TEXT, '(SP,1P,E13.6,2X,E13.6)') FVAL ELSE IF (KTYP.EQ.8) THEN * String. IERR = KEYGET (KEYS, I, KEY_KEYVALUE, CVAL, NC) TEXT = '"' // CVAL(:NC) // '"' ELSE * No value. TEXT = '' END IF * Account for Fortran's abysmal formatting control. IF (ABS(KEYTYP).EQ.2 .OR. : ABS(KEYTYP).EQ.3 .OR. : ABS(KEYTYP).EQ.4 .OR. : ABS(KEYTYP).EQ.6) THEN * Squeeze out leading blanks. DO 180 J = 1, 84 IF (TEXT(J:J).NE.' ') THEN TEXT = TEXT(J:) GO TO 190 END IF 180 CONTINUE END IF 190 NC = LNBLNK(TEXT) IF (KEYTYP.GT.0) THEN * Keyvalue successfully extracted. WRITE (*, '(2X,A,$)') TEXT(:NC) ELSE IF (KEYTYP.LT.0) THEN * Syntax error of some type while extracting the keyvalue. WRITE (*, '(2X,A,$)') '(' // TEXT(:NC) // ')' END IF * Units? IERR = KEYGET (KEYS, I, KEY_ULEN, ULEN, NC) IERR = KEYGET (KEYS, I, KEY_COMMENT, TEXT, NC) IF (ULEN.GT.0) THEN WRITE (*, '(X,A,$)') TEXT(2:ULEN-2) END IF * Comment text or reject keyrecord. WRITE (*, '(/,A)') TEXT(:NC) 200 CONTINUE * Print indexes. WRITE (*, '(//,A)') 'Indexes of selected keywords:' DO 210 I = 0, NKEYID-1 IERR = KEYIDGET (KEYIDS, I, KEYID_NAME, TEXT) IERR = KEYIDGET (KEYIDS, I, KEYID_COUNT, NC) IERR = KEYIDGET (KEYIDS, I, KEYID_IDX, IVAL) WRITE (*, '(A8,3I5,$)') TEXT, NC, IVAL(1), IVAL(2) * Print logical (SIMPLE) and integer (BITPIX, NAXIS) values. IF (NC.GT.0) THEN IERR = KEYGET (KEYS, IVAL(1), KEY_TYPE, KEYTYP, NC) WRITE (*, '(I4,$)') KEYTYP IF (KEYTYP.EQ.1) THEN IERR = KEYGET (KEYS, I, KEY_KEYVALUE, IVAL, NC) IF (IVAL(1).EQ.0) THEN WRITE (*, '(4X,A,$)') 'F' ELSE WRITE (*, '(4X,A,$)') 'T' END IF ELSE IF (KEYTYP.EQ.2) THEN IERR = KEYGET (KEYS, I, KEY_KEYVALUE, IVAL, NC) WRITE (*, '(I5,$)') IVAL(1) END IF END IF WRITE (*, '()') 210 CONTINUE IERR = FREEKEYS(KEYS) 999 CONTINUE END pywcs-1.12/wcslib/Fortran/test/tlin.f0000644001153600020070000001167012310355626021645 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tlin.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TLIN *----------------------------------------------------------------------- * * TLIN tests the linear transformation routines supplied with WCSLIB. * *----------------------------------------------------------------------- DOUBLE PRECISION TOL PARAMETER (TOL = 1D-13) INTEGER NAXIS, NCOORD, NELEM PARAMETER (NAXIS = 5, NCOORD = 2, NELEM = 9) INTEGER I, J, K, NFAIL, STATUS DOUBLE PRECISION CDELT(NAXIS), CRPIX(NAXIS), IMG(NELEM,2), : PC(NAXIS,NAXIS), PIX0(NELEM,2), PIX(NELEM,2), RESID, : RESIDMAX * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'lin.inc' INTEGER LIN(LINLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (LIN,DUMMY) DATA (CRPIX(I), I=1,NAXIS) : /256D0, 256D0, 64D0, 128D0, 1D0/ DATA ((PC(I,J),J=1,NAXIS),I=1,NAXIS) : / 1.0D0, 0.5D0, 0D0, 0D0, 0D0, : 0.5D0, 1.0D0, 0D0, 0D0, 0D0, : 0.0D0, 0.0D0, 1D0, 0D0, 0D0, : 0.0D0, 0.0D0, 0D0, 1D0, 0D0, : 0.0D0, 0.0D0, 0D0, 0D0, 1D0/ DATA (CDELT(I), I=1,NAXIS) : / 1.2D0, 2.3D0, 3.4D0, 4.5D0, 5.6D0/ DATA ((PIX0(I,J), I=1,NAXIS), J=1,2) : /303.0D0, 265.0D0, 112.4D0, 144.5D0, 28.2D0, : 19.0D0, 57.0D0, 2.0D0, 15.0D0, 42.0D0/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ( : 'Testing WCSLIB linear transformation routines (tlin.f)',/, : '------------------------------------------------------') STATUS = LINPUT (LIN, LIN_FLAG, -1, 0, 0) STATUS = LININI (NAXIS, LIN) DO 30 I = 1, NAXIS STATUS = LINPUT (LIN, LIN_CRPIX, CRPIX(I), I, 0) DO 20 J = 1, NAXIS STATUS = LINPUT (LIN, LIN_PC, PC(I,J), I, J) 20 CONTINUE STATUS = LINPUT (LIN, LIN_CDELT, CDELT(I), I, 0) 30 CONTINUE WRITE (*, *) DO 50 K = 1, NCOORD WRITE (*, 40) K, (PIX0(J,K), J=1,NAXIS) 40 FORMAT ('PIX',I2,':',10F14.8) 50 CONTINUE STATUS = LINP2X (LIN, NCOORD, NELEM, PIX0, IMG) IF (STATUS.NE.0) THEN WRITE (*, 60) STATUS 60 FORMAT ('LINP2X ERROR',I3) GO TO 999 END IF WRITE (*, *) DO 80 K = 1, NCOORD WRITE (*, 70) K, (IMG(J,K), J=1,NAXIS) 70 FORMAT ('IMG',I2,':',10F14.8) 80 CONTINUE STATUS = LINX2P (LIN, NCOORD, NELEM, IMG, PIX) IF (STATUS.NE.0) THEN WRITE (*, 90) STATUS 90 FORMAT ('LINX2P ERROR',I3) GO TO 999 END IF WRITE (*, *) DO 100 K = 1, NCOORD WRITE (*, 40) K, (PIX(J,K), J=1,NAXIS) 100 CONTINUE * Check closure. NFAIL = 0 RESIDMAX = 0D0 DO 120 K = 1, NCOORD DO 110 J = 1, NAXIS RESID = ABS(PIX(j,k) - PIX0(j,k)) IF (RESIDMAX.LT.RESID) RESIDMAX = RESID IF (RESID.GT.TOL) NFAIL = NFAIL + 1 110 CONTINUE 120 CONTINUE WRITE (*, 130) RESIDMAX 130 FORMAT (/,'LINP2X/LINX2P: Maximum closure residual =',1PE8.1, : ' pixel.') IF (NFAIL.NE.0) THEN WRITE (*, 140) NFAIL 140 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 150) 150 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF 999 STATUS = LINFREE(LIN) END pywcs-1.12/wcslib/Fortran/test/tlog.f0000644001153600020070000001045512310355626021644 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tlog.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TLOG *----------------------------------------------------------------------- * * TLOG tests the logarithmic coordinate transformation routines for * closure. * *----------------------------------------------------------------------- DOUBLE PRECISION TOL PARAMETER (TOL = 1D-13) INTEGER NCRD PARAMETER (NCRD = 10000) INTEGER J, K, NFAIL, STAT1(NCRD), STAT2(NCRD), STATUS DOUBLE PRECISION CRVAL, LOGC(NCRD), RESID, RESMAX, STEP, : X0(NCRD), X1(NCRD) DATA CRVAL /3.3D0/ INCLUDE 'log.inc' *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing closure of WCSLIB logarithmic coordinate ', : 'routines (tlog.f)',/, : '-------------------------------------------------', : '-----------------') * Construct a logarithmic axis and test closure. STEP = (40D0/NCRD) / 2D0 K = -NCRD DO 20 J = 1, NCRD X0(J) = K*STEP K = K + 2 20 CONTINUE WRITE (*, 30) X0(1), X0(NCRD), X0(2) - X0(1) 30 FORMAT (/,'Logarithmic range:',F6.1,' to',F5.1,', step:',F7.4) * Convert the first to the second. STATUS = LOGX2S(CRVAL, NCRD, 1, 1, X0, LOGC, STAT1) IF (STATUS.NE.0) THEN WRITE (*, 40) STATUS 40 FORMAT ('LOGX2S ERROR',I2,'.') END IF * Convert the second back to the first. STATUS = LOGS2X(CRVAL, NCRD, 1, 1, LOGC, X1, STAT2) IF (STATUS.NE.0) THEN WRITE (*, 50) STATUS 50 FORMAT ('LOGS2X ERROR',I2,'.') END IF * Test closure. NFAIL = 0 RESMAX = 0D0 DO 90 J = 1, NCRD IF (STAT1(J).NE.0) THEN WRITE (*, 60) X0(J), STAT1(J) 60 FORMAT ('LOGX2S: X =',1PE20.12,' -> log = ???, stat =',I2,'.') GO TO 90 END IF IF (STAT2(J).NE.0) THEN WRITE (*, 70) X0(J), LOGC(J), STAT2(J) 70 FORMAT ('LOGS2X: x =',1PE20.12,' -> log =',1PE20.12, : ' -> x = ???, stat =',I2) GO TO 90 END IF IF (X0(J).EQ.0D0) THEN RESID = ABS(X1(J) - X0(J)) ELSE RESID = ABS((X1(J) - X0(J)) / X0(J)) IF (RESID.GT.RESMAX) RESMAX = RESID END IF IF (RESID.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 80) X0(J), LOGC(J), X1(J), RESID 80 FORMAT ('LOGX2S: x =',1PE20.12,' -> log =',1PE20.12,' ->',/, : ' x =',1PE20.12,', resid =',1PE20.12) END IF 90 CONTINUE IF (RESMAX.GT.TOL) THEN WRITE (*, *) END IF WRITE (*, 100) RESMAX 100 FORMAT ('LOGX2S/LOGS2X: Maximum closure residual =',1PE8.1) IF (NFAIL.NE.0) THEN WRITE (*, 110) NFAIL 110 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 120) 120 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF END pywcs-1.12/wcslib/Fortran/test/tpih1.f0000644001153600020070000001425112310355626021722 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tpih1.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TPIH1 *----------------------------------------------------------------------- * * TPIH1 tests WCSPIH, the WCS FITS parser for image headers, and WCSFIX, * which translates non-standard constructs. It reads a test header and * uses WCSPRT to print the resulting WCSPRM structs. * * Input comes from file 'pih.fits'. * * WCSP, which is meant to hold an address, is declared as an INTEGER * array of length 2 to accomodate 64-bit machines for which * sizeof(void *) = 2*sizeof(int). *----------------------------------------------------------------------- LOGICAL GOTEND INTEGER ALTS(0:26), CTRL, I, IERR, J, K, NKEYRC, NREJECT, NWCS, : RELAX, WCSP(2) CHARACTER CALTS(0:26)*2, KEYREC*80, HEADER*288001, INFILE*9 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcshdr.inc' INCLUDE 'wcs.inc' INCLUDE 'wcsfix.inc' INTEGER WCS(WCSLEN), STAT(WCSFIX_NWCS) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS,DUMMY) DATA INFILE /'pih.fits'/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ( : 'Testing WCSLIB parser for FITS image headers (tpih1.f)',/, : '------------------------------------------------------',/) * Open the FITS WCS test header for formatted, direct I/O. OPEN (UNIT=1, FILE=INFILE, FORM='FORMATTED', ACCESS='DIRECT', : RECL=80, IOSTAT=IERR) IF (IERR.NE.0) THEN WRITE (*, 20) IERR, INFILE 20 FORMAT ('ERROR',I3,' opening ',A) GO TO 999 END IF * Read in the FITS header, excluding COMMENT and HISTORY keyrecords. K = 1 NKEYRC = 0 GOTEND = .FALSE. DO 50 J = 0, 100 DO 40 I = 1, 36 READ (1, '(A80)', REC=36*J+I, IOSTAT=IERR) KEYREC IF (IERR.NE.0) THEN WRITE (*, 30) IERR 30 FORMAT ('ERROR',I3,' reading header.') GO TO 999 END IF IF (KEYREC(:8).EQ.' ') GO TO 40 IF (KEYREC(:8).EQ.'COMMENT ') GO TO 40 IF (KEYREC(:8).EQ.'HISTORY ') GO TO 40 HEADER(K:) = KEYREC K = K + 80 NKEYRC = NKEYRC + 1 IF (KEYREC(:8).EQ.'END ') THEN * An END keyrecord was read, read the rest of the block. GOTEND = .TRUE. END IF 40 CONTINUE IF (GOTEND) GO TO 60 50 CONTINUE 60 CLOSE (UNIT=1) HEADER(K:K) = CHAR (0) WRITE (*, 70) NKEYRC 70 FORMAT ('Found',I4,' non-comment header keyrecords.',/) * Cull all WCS keyrecords from the header but report illegal ones. WRITE (*, 80) 80 FORMAT (/,'Illegal-WCS header keyrecords rejected by wcspih():') RELAX = WCSHDR_all CTRL = -2 * WCSPIH will allocate memory for NWCS intialized WCSPRM structs. CALL FLUSH(6) IERR = WCSPIH (HEADER, NKEYRC, RELAX, CTRL, NREJECT, NWCS, WCSP) IF (IERR.NE.0) THEN WRITE (*, 90) IERR 90 FORMAT ('WCSPIH ERROR',I2,'.') GO TO 999 END IF * List keyrecords that were not consumed by WCSPIH. WRITE (*, 100) 100 FORMAT (//,'Non-WCS header keyrecords not used by WCSPIH:') DO 110 I = 1, 288001, 80 IF (HEADER(I:I).EQ.CHAR(0)) GO TO 120 WRITE (*, '(A)') HEADER(I:I+79) 110 CONTINUE 120 IERR = WCSIDX (NWCS, WCSP, ALTS) WRITE (*, 130) 130 FORMAT (//,'Index of alternate coordinate descriptions found:',/, : ' A B C D E F G H I J K L M N O P Q R S T U V W X Y Z') DO 140 I = 0, 26 IF (ALTS(I).LT.0) THEN CALTS(I) = ' -' ELSE WRITE (CALTS(I), '(I2)') ALTS(I) END IF 140 CONTINUE WRITE (*, '(27A)') CALTS DO 190 I = 0, NWCS-1 WRITE (*, 150) 150 FORMAT (/,'------------------------------------', : '------------------------------------') * Copy into our WCSPRM struct. IERR = WCSVCOPY (WCSP, I, WCS) * Fix non-standard WCS keyvalues. IERR = WCSFIX (7, 0, WCS, STAT) IF (IERR.NE.0) THEN WRITE (*, 160) (STAT(J), J=1,WCSFIX_NWCS) 160 FORMAT ('WCSFIX ERROR, status returns: (',(I2,:,','),')',/) END IF IERR = WCSSET (WCS) IF (IERR.NE.0) THEN WRITE (*, 170) IERR 170 FORMAT ('WCSSET ERROR',I2,'.') GO TO 190 END IF CALL FLUSH(6) IERR = WCSPRT (WCS) IF (IERR.NE.0) THEN WRITE (*, 180) IERR 180 FORMAT ('WCSPRT ERROR',I2,'.') GO TO 190 END IF * Free memory (doesn't free memory allocated by WCSPIH). IERR = WCSFREE (WCS) 190 CONTINUE * Free the memory allocated by WCSPIH. IERR = WCSVFREE (NWCS, WCSP) 999 CONTINUE END pywcs-1.12/wcslib/Fortran/test/tpih2.f0000644001153600020070000001420012310355626021715 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tpih2.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TPIH2 *----------------------------------------------------------------------- * * TPIH2 tests WCSPIH, the WCS FITS parser for image headers, by reading * a test header and using PGSBOX to plot coordinate graticules for the * resulting WCSPRM structs. * * Input comes from file 'pih.fits'. * * WCSP, which is meant to hold an address, is declared as an INTEGER * array of length 2 to accomodate 64-bit machines for which * sizeof(void *) = 2*sizeof(int). *----------------------------------------------------------------------- LOGICAL GOTEND INTEGER C0(7), GCODE(2), I, IC, IERR, J, K, NAXIS(2), : NKEYRC, NREJECT, NWCS, RELAX, WCSP(2) REAL BLC(2), TRC(2) DOUBLE PRECISION CACHE(4,0:256), NLDPRM(8) CHARACTER KEYREC*80, DEVTYP*16, HEADER*28801, IDENTS(3)*80, : INFILE*9, NLCPRM(1)*1, OPT(2)*1, WCSNAME*72 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcshdr.inc' INCLUDE 'wcs.inc' INTEGER WCS(WCSLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS,DUMMY) EXTERNAL PGWCSL DATA INFILE /'pih.fits'/ DATA C0 /7*-1/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ( : 'Testing WCSLIB parser for FITS image headers (tpih2.f)',/, : '------------------------------------------------------',/) * Open the FITS WCS test header for formatted, direct I/O. OPEN (UNIT=1, FILE=INFILE, FORM='FORMATTED', ACCESS='DIRECT', : RECL=80, IOSTAT=IERR) IF (IERR.NE.0) THEN WRITE (*, 20) IERR, INFILE 20 FORMAT ('ERROR',I3,' opening ',A) GO TO 999 END IF * Read in the FITS header, excluding COMMENT and HISTORY keyrecords. K = 1 NKEYRC = 0 GOTEND = .FALSE. DO 50 J = 0, 100 DO 40 I = 1, 36 READ (1, '(A80)', REC=36*J+I, IOSTAT=IERR) KEYREC IF (IERR.NE.0) THEN WRITE (*, 30) IERR 30 FORMAT ('ERROR',I3,' reading header.') GO TO 999 END IF IF (KEYREC(:8).EQ.' ') GO TO 40 IF (KEYREC(:8).EQ.'COMMENT ') GO TO 40 IF (KEYREC(:8).EQ.'HISTORY ') GO TO 40 HEADER(K:) = KEYREC K = K + 80 NKEYRC = NKEYRC + 1 IF (KEYREC(:8).EQ.'END ') THEN * An END keyrecord was read, read the rest of the block. GOTEND = .TRUE. END IF 40 CONTINUE IF (GOTEND) GO TO 60 50 CONTINUE 60 CLOSE (UNIT=1) HEADER(K:K) = CHAR (0) WRITE (*, 70) NKEYRC 70 FORMAT ('Found',I4,' non-comment header keyrecords.') * WCSPIH will allocate memory for an array of NWCS intialized WCSPRM * structs. This array will be returned via a "pointer", WCSP, that * may be passed to WCSVCOPY to extract a particular struct. RELAX = WCSHDR_all IERR = WCSPIH (HEADER, NKEYRC, RELAX, 3, NREJECT, NWCS, WCSP) IF (IERR.NE.0) THEN WRITE (*, 80) IERR 80 FORMAT ('WCSPIH ERROR',I2,'.') GO TO 999 END IF * Plot setup. NAXIS(1) = 1024 NAXIS(2) = 1024 BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = NAXIS(1) + 0.5 TRC(2) = NAXIS(2) + 0.5 DEVTYP = '/XWINDOW' CALL PGBEG(0, DEVTYP, 1, 1) CALL PGVSTD() CALL PGWNAD(0.0, 1.0, 0.0, 1.0) CALL PGASK(1) CALL PGPAGE() * Annotation. IDENTS(1) = 'Right ascension' IDENTS(2) = 'Declination' OPT(1) = 'G' OPT(2) = 'E' * Compact lettering. CALL PGSCH(0.8) * Draw full grid lines. CALL PGSCI(1) GCODE(1) = 2 GCODE(2) = 2 DO 100 I = 0, NWCS-1 * Copy into our WCSPRM struct. IERR = WCSVCOPY (WCSP, I, WCS) IERR = WCSSET (WCS) IF (IERR.NE.0) THEN WRITE (*, 90) IERR 90 FORMAT ('WCSSET ERROR',I2,'.') GO TO 999 END IF * Get WCSNAME out of the WCSPRM struct. IERR = WCSGET (WCS, WCS_WCSNAME, WCSNAME) IDENTS(3) = WCSNAME WRITE (*, '(/,A)') WCSNAME * Draw the celestial grid. The grid density is set for each * world coordinate by specifying LABDEN = 1224. IC = -1 CALL PGSBOX(BLC, TRC, IDENTS, OPT, 0, 1224, C0, GCODE, 0D0, 0, : 0D0, 0, 0D0, 0, PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, NLDPRM, : 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE() * Free memory (doesn't free memory allocated by WCSPIH). IERR = WCSFREE (WCS) 100 CONTINUE * Free the memory allocated by WCSPIH. IERR = WCSVFREE (NWCS, WCSP) 999 CONTINUE END pywcs-1.12/wcslib/Fortran/test/tprj1.f0000644001153600020070000002624112310355626021737 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tprj1.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TPRJ1 *----------------------------------------------------------------------- * * TPRJ1 tests forward and reverse spherical projections for closure. * *----------------------------------------------------------------------- INCLUDE 'prj.inc' INTEGER J, K, NFAIL, PROJEX, STATUS DOUBLE PRECISION PV(0:29) DOUBLE PRECISION PI PARAMETER (PI = 3.141592653589793238462643D0) DOUBLE PRECISION TOL PARAMETER (TOL = 1D-9) *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing closure of WCSLIB spherical projection ', : 'routines (tprj1.f)',/, : '-----------------------------------------------', : '------------------') WRITE (*, '(/,A)') 'List of prj status return values:' DO 40 STATUS = 1, 4 DO 30 K = 80, 1, -1 IF (PRJ_ERRMSG(STATUS)(K:K).NE.' ') THEN WRITE(*, 20) STATUS, PRJ_ERRMSG(STATUS)(:K) 20 FORMAT(I4,': ',A,'.') GO TO 40 END IF 30 CONTINUE 40 CONTINUE WRITE(*, '()') DO 50 J = 0, 29 PV(J) = 0D0 50 CONTINUE NFAIL = 0 * AZP: zenithal/azimuthal perspective. PV(1) = 0.5D0 PV(2) = 30D0 NFAIL = NFAIL + PROJEX ('AZP', PV, 90, 5, TOL) * SZP: slant zenithal perspective. PV(1) = 0.5D0 PV(2) = 210D0 PV(3) = 60D0 NFAIL = NFAIL + PROJEX ('SZP', PV, 90, -90, TOL) * TAN: gnomonic. NFAIL = NFAIL + PROJEX ('TAN', PV, 90, 5, TOL) * STG: stereographic. NFAIL = NFAIL + PROJEX ('STG', PV, 90, -85, TOL) * SIN: orthographic/synthesis. PV(1) = -0.3D0 PV(2) = 0.5D0 NFAIL = NFAIL + PROJEX ('SIN', PV, 90, 45, TOL) * ARC: zenithal/azimuthal equidistant. NFAIL = NFAIL + PROJEX ('ARC', PV, 90, -90, TOL) * ZPN: zenithal/azimuthal polynomial. PV(0) = 0.00000D0 PV(1) = 0.95000D0 PV(2) = -0.02500D0 PV(3) = -0.15833D0 PV(4) = 0.00208D0 PV(5) = 0.00792D0 PV(6) = -0.00007D0 PV(7) = -0.00019D0 PV(8) = 0.00000D0 PV(9) = 0.00000D0 NFAIL = NFAIL + PROJEX ('ZPN', PV, 90, 10, TOL) * ZEA: zenithal/azimuthal equal area. NFAIL = NFAIL + PROJEX ('ZEA', PV, 90, -85, TOL) * AIR: Airy's zenithal projection. PV(1) = 45D0 NFAIL = NFAIL + PROJEX ('AIR', PV, 90, -85, TOL) * CYP: cylindrical perspective. PV(1) = 3.0D0 PV(2) = 0.8D0 NFAIL = NFAIL + PROJEX ('CYP', PV, 90, -90, TOL) * CEA: cylindrical equal area. PV(1) = 0.75D0 NFAIL = NFAIL + PROJEX ('CEA', PV, 90, -90, TOL) * CAR: plate carree. NFAIL = NFAIL + PROJEX ('CAR', PV, 90, -90, TOL) * MER: Mercator's. NFAIL = NFAIL + PROJEX ('MER', PV, 85, -85, TOL) * SFL: Sanson-Flamsteed. NFAIL = NFAIL + PROJEX ('SFL', PV, 90, -90, TOL) * PAR: parabolic. NFAIL = NFAIL + PROJEX ('PAR', PV, 90, -90, TOL) * MOL: Mollweide's projection. NFAIL = NFAIL + PROJEX ('MOL', PV, 90, -90, TOL) * AIT: Hammer-Aitoff. NFAIL = NFAIL + PROJEX ('AIT', PV, 90, -90, TOL) * COP: conic perspective. PV(1) = 60D0 PV(2) = 15D0 NFAIL = NFAIL + PROJEX ('COP', PV, 90, -25, TOL) * COE: conic equal area. PV(1) = 60D0 PV(2) = -15D0 NFAIL = NFAIL + PROJEX ('COE', PV, 90, -90, TOL) * COD: conic equidistant. PV(1) = -60D0 PV(2) = 15D0 NFAIL = NFAIL + PROJEX ('COD', PV, 90, -90, TOL) * COO: conic orthomorphic. PV(1) = -60D0 PV(2) = -15D0 NFAIL = NFAIL + PROJEX ('COO', PV, 85, -90, TOL) * BON: Bonne's projection. PV(1) = 30D0 NFAIL = NFAIL + PROJEX ('BON', PV, 90, -90, TOL) * PCO: polyconic. NFAIL = NFAIL + PROJEX ('PCO', PV, 90, -90, TOL) * TSC: tangential spherical cube. NFAIL = NFAIL + PROJEX ('TSC', PV, 90, -90, TOL) * CSC: COBE quadrilateralized spherical cube. NFAIL = NFAIL + PROJEX ('CSC', PV, 90, -90, 4D-2) * QSC: quadrilateralized spherical cube. NFAIL = NFAIL + PROJEX ('QSC', PV, 90, -90, TOL) * HPX: HEALPix projection. PV(1) = 4D0 PV(2) = 3D0 NFAIL = NFAIL + PROJEX ('HPX', PV, 90, -90, TOL) IF (NFAIL.NE.0) THEN WRITE (*, 60) NFAIL 60 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 70) 70 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF END *----------------------------------------------------------------------- INTEGER FUNCTION PROJEX (PCODE, PV, NORTH, SOUTH, TOL) *----------------------------------------------------------------------- * PROJEX exercises the spherical projection routines. * * Given: * PCODE C*3 Projection code. * PV D(0:29) Projection parameters. * NORTH I Northern cutoff latitude, degrees. * SOUTH I Southern cutoff latitude, degrees. * TOL D Reporting tolerance, degrees. *----------------------------------------------------------------------- INTEGER J, LAT, LNG, NFAIL, NORTH, SOUTH, STAT1(361), : STAT2(361), STATUS DOUBLE PRECISION DLAT, DLATMX, DLNG, DLNGMX, DR, DRMAX, LAT1, : LAT2(361), LNG1(361), LNG2(361), PV(0:29), R, THETA, : TOL, X(361), X1(361), X2(361), Y(361), Y1(361), Y2(361) CHARACTER PCODE*3 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'prj.inc' INTEGER PRJ(PRJLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (PRJ,DUMMY) DOUBLE PRECISION D2R, PI PARAMETER (PI = 3.141592653589793238462643D0) PARAMETER (D2R = PI/180D0) *----------------------------------------------------------------------- STATUS = PRJINI(PRJ) DO 10 J = 0, 29 STATUS = PRJPUT (PRJ, PRJ_PV, PV(J), J) 10 CONTINUE STATUS = PRJPUT (PRJ, PRJ_CODE, PCODE, 0) * Uncomment the next line to test alternative initializations of * projection parameters. * STATUS = PRJPUT (PRJ, PRJ_R0, 180D0/PI, 0) WRITE (*, 20) PCODE, NORTH, SOUTH, TOL 20 FORMAT ('Testing ',A3,'; latitudes',I3,' to',I4, : ', reporting tolerance',1PG8.1,' deg.') NFAIL = 0 DLNGMX = 0D0 DLATMX = 0D0 DO 80 LAT = NORTH, SOUTH, -1 LAT1 = DBLE(LAT) J = 1 DO 30 LNG = -180, 180 LNG1(J) = DBLE(LNG) J = J + 1 30 CONTINUE STATUS = PRJS2X (PRJ, 361, 1, 1, 1, LNG1, LAT1, X, Y, STAT1) IF (STATUS.EQ.1) THEN WRITE (*, 40) PCODE, STATUS 40 FORMAT (3X,A3,'(S2X) ERROR',I2) GO TO 80 END IF STATUS = PRJX2S (PRJ, 361, 0, 1, 1, X, Y, LNG2, LAT2, STAT2) IF (STATUS.EQ.1) THEN WRITE (*, 50) PCODE, STATUS 50 FORMAT (3X,A3,'(X2S) ERROR',I2) GO TO 80 END IF LNG = -180 DO 70 J = 1, 361 IF (STAT1(J).NE.0) GO TO 70 IF (STAT2(J).NE.0) THEN WRITE (*, 55) PCODE, LNG1(J), LAT1, X(J), Y(J), STAT2(J) 55 FORMAT (3X,A3,'(X2S): lng1 =',F20.15,' lat1 =',F20.15,/, : ' x =',F20.15,' y =',F20.15, : ' ERROR',I3) GO TO 70 END IF DLNG = ABS(LNG2(J) - LNG1(J)) IF (DLNG.GT.180D0) DLNG = ABS(DLNG-360D0) IF (ABS(LAT).NE.90 .AND. DLNG.GT.DLNGMX) DLNGMX = DLNG DLAT = ABS(LAT2(J) - LAT1) IF (DLAT.GT.DLATMX) DLATMX = DLAT IF (DLAT.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 60) PCODE, LNG1(J), LAT1, X(J), Y(J), LNG2(J), : LAT2(J) 60 FORMAT (8X,A3,': lng1 =',F20.15,' lat1 =',F20.15,/, : 8X,' x =',F20.15,' y =',F20.15,/, : 8X,' lng2 =',F20.15,' lat2 =',F20.15) ELSE IF (ABS(LAT).NE.90) THEN IF (DLNG.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 60) PCODE, LNG1(J), LAT1, X(J), Y(J), : LNG2(J), LAT2(J) END IF END IF 70 CONTINUE 80 CONTINUE WRITE (*, 90) DLNGMX, DLATMX 90 FORMAT (13X,'Maximum residual (sky): lng',1P,E8.1,' lat',E8.1) * Test closure at points close to the reference point. R = 1.0 THETA = -180D0 DRMAX = 0D0 DO 140 J = 1, 12 X1(1) = R*COS(THETA*D2R) Y1(1) = R*SIN(THETA*D2R) STATUS = PRJX2S (PRJ, 1, 1, 1, 1, X1, Y1, LNG1, LAT1, STAT2) IF (STATUS.NE.0) THEN WRITE (*, 100) PCODE, X1(1), Y1(1), STATUS 100 FORMAT (8X,A3,'(X2S): x1 =',F20.15,' y1 =',F20.15, : ' ERROR',I3) GO TO 130 END IF STATUS = PRJS2X (PRJ, 1, 1, 1, 1, LNG1, LAT1, X2, Y2, STAT1) IF (STATUS.NE.0) THEN WRITE (*, 110) PCODE, X1(1), Y1(1), LNG1(1), LAT1, STATUS 110 FORMAT (3X,A3,': x1 =',F20.15,' y1 =',F20.15,/, : 3X,' lng =',F20.15,' lat =',F20.15,' ERROR', : I3) GO TO 130 END IF DR = SQRT((X2(1)-X1(1))**2 + (Y2(1)-Y1(1))**2) IF (DR.GT.DRMAX) DRMAX = DR IF (DR.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 120) PCODE, X1(1), Y1(1), LNG1(1), LAT1, X2(1), : Y2(1) 120 FORMAT (8X,A3,': x1 =',F20.15,' y1 =',F20.15,/, : 8X,' lng =',F20.15,' lat =',F20.15,/, : 8X,' x2 =',F20.15,' y2 =',F20.15) END IF 130 R = R/10D0 THETA = THETA + 15D0 140 CONTINUE WRITE (*, 150) DRMAX 150 FORMAT (13X,'Maximum residual (ref): dR',1PE8.1) PROJEX = NFAIL END pywcs-1.12/wcslib/Fortran/test/tprj2.f0000644001153600020070000003064112310355626021737 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tprj2.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TPRJ2 *----------------------------------------------------------------------- * * TPRJ2 tests projection routines by plotting test graticules using * PGPLOT. * *----------------------------------------------------------------------- INTEGER J DOUBLE PRECISION PV(0:29) DOUBLE PRECISION PI PARAMETER (PI = 3.141592653589793238462643D0) *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ( : 'Testing WCSLIB spherical projection routines (tprj2.f)',/, : '------------------------------------------------------') DO 20 J = 0, 29 PV(J) = 0D0 20 CONTINUE * PGPLOT initialization. CALL PGBEG (0, '/xwindow', 1, 1) * Define pen colours. CALL PGSCR (0, 0.00, 0.00, 0.00) CALL PGSCR (1, 1.00, 1.00, 0.00) CALL PGSCR (2, 1.00, 1.00, 1.00) CALL PGSCR (3, 0.50, 0.50, 0.80) CALL PGSCR (4, 0.80, 0.50, 0.50) CALL PGSCR (5, 0.80, 0.80, 0.80) CALL PGSCR (6, 0.50, 0.50, 0.80) CALL PGSCR (7, 0.80, 0.50, 0.50) CALL PGSCR (8, 0.30, 0.50, 0.30) 30 FORMAT(/,A,' projection') 40 FORMAT(/,A,' projection',/,'Parameters:',5F12.5,/,5F12.5) * AZP: zenithal/azimuthal perspective. PV(1) = 2D0 PV(2) = 30D0 WRITE (*, 40) 'Zenithal/azimuthal perspective', (PV(J), J=1,2) CALL PRJPLT ('AZP', 90, -90, PV) * SZP: zenithal/azimuthal perspective. PV(1) = 2D0 PV(2) = 210D0 PV(3) = 60D0 WRITE (*, 40) 'Slant zenithal perspective', (PV(J), J=1,3) CALL PRJPLT ('SZP', 90, -90, PV) * TAN: gnomonic. WRITE (*, 30) 'Gnomonic' CALL PRJPLT ('TAN', 90, 5, PV) * STG: stereographic. WRITE (*, 30) 'Stereographic' CALL PRJPLT ('STG', 90, -85, PV) * SIN: orthographic. PV(1) = -0.3D0 PV(2) = 0.5D0 WRITE (*, 40) 'Orthographic/synthesis', (PV(J), J=1,2) CALL PRJPLT ('SIN', 90, -90, PV) * ARC: zenithal/azimuthal equidistant. WRITE (*, 30) 'Zenithal/azimuthal equidistant' CALL PRJPLT ('ARC', 90, -90, PV) * ZPN: zenithal/azimuthal polynomial. PV(0) = 0.05000D0 PV(1) = 0.95000D0 PV(2) = -0.02500D0 PV(3) = -0.15833D0 PV(4) = 0.00208D0 PV(5) = 0.00792D0 PV(6) = -0.00007D0 PV(7) = -0.00019D0 PV(8) = 0.00000D0 PV(9) = 0.00000D0 WRITE (*, 40) 'Zenithal/azimuthal polynomial', (PV(J), J=0,9) CALL PRJPLT ('ZPN', 90, 10, PV) * ZEA: zenithal/azimuthal equal area. WRITE (*, 30) 'Zenithal/azimuthal equal area' CALL PRJPLT ('ZEA', 90, -90, PV) * AIR: Airy's zenithal projection. PV(1) = 45D0 WRITE (*, 40) 'Airy''s zenithal', PV(1) CALL PRJPLT ('AIR', 90, -85, PV) * CYP: cylindrical perspective. PV(1) = 3.0D0 PV(2) = 0.8D0 WRITE (*, 40) 'Cylindrical perspective', (PV(J), J=1,2) CALL PRJPLT ('CYP', 90, -90, PV) * CEA: cylindrical equal area. PV(1) = 0.75D0 WRITE (*, 40) 'Cylindrical equal area', PV(1) CALL PRJPLT ('CEA', 90, -90, PV) * CAR: plate carree. WRITE (*, 30) 'Plate carree' CALL PRJPLT ('CAR', 90, -90, PV) * MER: Mercator's. WRITE (*, 30) 'Mercator''s' CALL PRJPLT ('MER', 85, -85, PV) * SFL: Sanson-Flamsteed. WRITE (*, 30) 'Sanson-Flamsteed (global sinusoid)' CALL PRJPLT ('SFL', 90, -90, PV) * PAR: parabolic. WRITE (*, 30) 'Parabolic' CALL PRJPLT ('PAR', 90, -90, PV) * MOL: Mollweide's projection. WRITE (*, 30) 'Mollweide''s' CALL PRJPLT ('MOL', 90, -90, PV) * AIT: Hammer-Aitoff. WRITE (*, 30) 'Hammer-Aitoff' CALL PRJPLT ('AIT', 90, -90, PV) * COP: conic perspective. PV(1) = 60D0 PV(2) = 15D0 WRITE (*, 40) 'Conic perspective', (PV(J), J=1,2) CALL PRJPLT ('COP', 90, -25, PV) * COE: conic equal area. PV(1) = 60D0 PV(2) = -15D0 WRITE (*, 40) 'Conic equal area', (PV(J), J=1,2) CALL PRJPLT ('COE', 90, -90, PV) * COD: conic equidistant. PV(1) = -60D0 PV(2) = 15D0 WRITE (*, 40) 'Conic equidistant', (PV(J), J=1,2) CALL PRJPLT ('COD', 90, -90, PV) * COO: conic orthomorphic. PV(1) = -60D0 PV(2) = -15D0 WRITE (*, 40) 'Conic orthomorphic', (PV(J), J=1,2) CALL PRJPLT ('COO', 85, -90, PV) * BON: Bonne's projection. PV(1) = 30D0 WRITE (*, 40) 'Bonne''s', PV(1) CALL PRJPLT ('BON', 90, -90, PV) * PCO: polyconic. WRITE (*, 30) 'Polyconic' CALL PRJPLT ('PCO', 90, -90, PV) * TSC: tangential spherical cube. WRITE (*, 30) 'Tangential spherical cube' CALL PRJPLT ('TSC', 90, -90, PV) * CSC: COBE quadrilateralized spherical cube. WRITE (*, 30) 'COBE quadrilateralized spherical cube' CALL PRJPLT ('CSC', 90, -90, PV) * QSC: quadrilateralized spherical cube. WRITE (*, 30) 'Quadrilateralized spherical cube' CALL PRJPLT ('QSC', 90, -90, PV) * HPX: HEALPix projection. PV(1) = 4D0 PV(2) = 3D0 WRITE (*, 40) 'HEALPix', (PV(J), J=1,2) CALL PRJPLT ('HPX', 90, -90, PV) CALL PGASK (0) CALL PGEND END SUBROUTINE PRJPLT (PCODE, NORTH, SOUTH, PV) *----------------------------------------------------------------------- * PRJPLT draws a 15 degree coordinate graticule. * * Given: * PCODE C*3 Projection code. * NORTH I Northern cutoff latitude, degrees. * SOUTH I Southern cutoff latitude, degrees. * PV D(0:29) Projection parameters. *----------------------------------------------------------------------- LOGICAL CUBIC, HEALPX, INTRRP INTEGER CI, H, ILAT, ILNG, J, K, LEN, NORTH, SOUTH, STAT(361), : STATUS REAL HX, HY, SX, SY, XR(512), YR(512) DOUBLE PRECISION LAT(361), LNG(361), PV(0:29), X(361), X0, Y(361), : Y0 CHARACTER PCODE*3 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'prj.inc' INTEGER PRJ(PRJLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (PRJ,DUMMY) *----------------------------------------------------------------------- STATUS = PRJINI(PRJ) DO 10 J = 0, 29 STATUS = PRJPUT (PRJ, PRJ_PV, PV(J), J) 10 CONTINUE STATUS = PRJPUT (PRJ, PRJ_CODE, PCODE, 0) WRITE (*, 20) PCODE, NORTH, SOUTH 20 FORMAT ('Plotting ',A3,'; latitudes',I3,' to',I4,'.') CALL PGASK (0) STATUS = PRJSET(PRJ) STATUS = PRJGET (PRJ, PRJ_CATEGORY, J) CUBIC = J.EQ.PRJ_QUADCUBE HEALPX = J.EQ.PRJ_HEALPIX IF (CUBIC) THEN * Draw the perimeter of the quadcube projection. CALL PGENV (-335.0, 65.0, -200.0, 200.0, 1, -2) CALL PGSCI (2) CALL PGTEXT (-340.0, -220.0, PCODE // ' - 15 degree graticule') CALL PGSCI (8) STATUS = PRJGET (PRJ, PRJ_X0, X0) STATUS = PRJGET (PRJ, PRJ_Y0, Y0) XR(1) = 45.0 + X0 YR(1) = 45.0 - Y0 XR(2) = 45.0 + X0 YR(2) = 3.0*45.0 - Y0 XR(3) = -45.0 + X0 YR(3) = 3.0*45.0 - Y0 XR(4) = -45.0 + X0 YR(4) = -3.0*45.0 - Y0 XR(5) = 45.0 + X0 YR(5) = -3.0*45.0 - Y0 XR(6) = 45.0 + X0 YR(6) = 45.0 - Y0 XR(7) = -7.0*45.0 + X0 YR(7) = 45.0 - Y0 XR(8) = -7.0*45.0 + X0 YR(8) = -45.0 - Y0 XR(9) = 45.0 + X0 YR(9) = -45.0 - Y0 CALL PGLINE (9, XR, YR) ELSE CALL PGENV (-200.0, 200.0, -200.0, 200.0, 1, -2) CALL PGSCI (2) CALL PGTEXT (-240.0, -220.0, PCODE//' - 15 degree graticule') IF (HEALPX) THEN * Draw the perimeter of the HEALPix projection. CALL PGSCI (8) H = NINT(PV(1)) SX = 180.0 / H SY = SX * NINT(PV(2) + 1D0) / 2.0 STATUS = PRJGET (PRJ, PRJ_X0, X0) STATUS = PRJGET (PRJ, PRJ_Y0, Y0) HX = 180.0 + X0 HY = SY - SX - Y0 CALL PGMOVE (HX, HY) DO 30 J = 1, H HX = HX - SX HY = HY + SX CALL PGDRAW (HX, HY) HX = HX - SX HY = HY - SX CALL PGDRAW (HX, HY) 30 CONTINUE HX = 180.0 + X0 HY = -SY + SX - Y0 IF (MOD(INT(PV(2)),2).EQ.1) THEN K = 1 ELSE K = -1 HY = HY - SX END IF CALL PGMOVE (HX, HY) DO 40 J = 1, H HX = HX - SX HY = HY - K*SX CALL PGDRAW (HX, HY) HX = HX - SX HY = HY + K*SX CALL PGDRAW (HX, HY) 40 CONTINUE END IF END IF CI = 1 DO 70 ILNG = -180, 180, 15 CI = CI + 1 IF (CI.GT.7) CI = 2 LNG(1) = DBLE(ILNG) IF (ILNG.EQ.0) THEN CALL PGSCI (1) ELSE CALL PGSCI (CI) END IF J = 1 DO 50 ILAT = NORTH, SOUTH, -1 LAT(J) = DBLE(ILAT) J = J + 1 50 CONTINUE LEN = NORTH - SOUTH + 1 STATUS = PRJS2X (PRJ, 1, LEN, 1, 1, LNG, LAT, X, Y, STAT) K = 0 DO 60 J = 1, LEN IF (STAT(J).NE.0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 GO TO 60 END IF IF (CUBIC .AND. J.GT.0) THEN IF (ABS(X(J) - X(J-1)).GT.2D0 .OR. : ABS(Y(J) - Y(J-1)).GT.5D0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 END IF ELSE IF (HEALPX .AND. ILNG.EQ.180) THEN IF (X(J).GT.180D0) GO TO 60 END IF K = K + 1 XR(K) = -X(J) YR(K) = Y(J) 60 CONTINUE CALL PGLINE (K, XR, YR) 70 CONTINUE CI = 1 INTRRP = CUBIC .OR. HEALPX DO 100 ILAT = -90, 90, 15 CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILAT.GT.NORTH) GO TO 100 IF (ILAT.LT.SOUTH) GO TO 100 LAT(1) = DBLE(ILAT) IF (ILAT.EQ.0) THEN CALL PGSCI (1) ELSE CALL PGSCI (CI) END IF ILNG = -180 DO 80 J = 1, 361 LNG(J) = DBLE(ILNG) ILNG = ILNG + 1 80 CONTINUE STATUS = PRJS2X (PRJ, 361, 1, 1, 1, LNG, LAT, X, Y, STAT) K = 0 DO 90 J = 1, 361 IF (STAT(J).NE.0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 GO TO 90 END IF IF (INTRRP .AND. J.GT.0) THEN IF (ABS(X(J) - X(J-1)).GT.2D0 .OR. : ABS(Y(J) - Y(J-1)).GT.5D0) THEN IF (K.GT.1) CALL PGLINE (K, XR, YR) K = 0 END IF END IF K = K + 1 XR(K) = -X(J) YR(K) = Y(J) 90 CONTINUE CALL PGLINE (K, XR, YR) 100 CONTINUE CALL PGSCI(1) XR(1) = 0.0 YR(1) = 0.0 CALL PGPT (1, XR, YR, 21) CALL PGASK (1) CALL PGPAGE() RETURN END pywcs-1.12/wcslib/Fortran/test/tspc.f0000644001153600020070000004023712310355626021651 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tspc.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TSPC *----------------------------------------------------------------------- * * TSPC tests the spectral transformation driver routines for closure. * *----------------------------------------------------------------------- * Maximum length of spectral axis - see CLOSURE. INTEGER NSPEC PARAMETER (NSPEC = 10001) INTEGER CLOSURE, NAXISJ, NFAIL DOUBLE PRECISION C, CDELTX, CRPIXJ, CRVALX, MARS(0:6), RESTFRQ, : RESTWAV, X1, X2 COMMON /SPECTRO/ MARS DATA C /2.99792458D8/ * KPNO MARS spectrograph grism parameters. DATA MARS /4.5D5, 1D0, 27D0, 1.765D0, -1.077D6, 3D0, 5D0/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing closure of WCSLIB spectral transformation ', : 'routines (tspc.f)',/, : '--------------------------------------------------', : '-----------------') NFAIL = 0 * PGPLOT initialization. CALL PGBEG (0, '/xwindow', 1, 1) NAXISJ = NSPEC CRPIXJ = NAXISJ/2 + 1 RESTFRQ = 1420.40595D6 RESTWAV = C/RESTFRQ X1 = 1D9 X2 = 2D9 CDELTX = (X2 - X1)/(NAXISJ - 1) CRVALX = X1 + (CRPIXJ - 1.0)*CDELTX WRITE (*, 20) X1*1D-9, X2*1D-9, CDELTX*1D-3 20 FORMAT (/,'Linear frequency axis, span:',F4.1,' to',F4.1, : ' (GHz), step:',F8.3,' (kHz)',/,'---------------------', : '-----------------------------------------------------') NFAIL = NFAIL + CLOSURE('WAVE-F2W', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VOPT-F2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ZOPT-F2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AWAV-F2A', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VELO-F2V', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('BETA-F2V', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) RESTWAV = 700D-9 RESTFRQ = C/RESTWAV X1 = 300D-9 X2 = 900D-9 CDELTX = (X2 - X1)/(NAXISJ - 1) CRVALX = X1 + (CRPIXJ - 1D0)*CDELTX WRITE (*, 30) INT(X1*1D9), INT(X2*1D9), CDELTX*1D9 30 FORMAT (/,'Linear vacuum wavelength axis, span:',I4,' to',I4, : ' (nm), step:',F9.6,' (nm)',/,'----------------------', : '----------------------------------------------------') NFAIL = NFAIL + CLOSURE('FREQ-W2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AFRQ-W2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ENER-W2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVN-W2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VRAD-W2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AWAV-W2A', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VELO-W2V', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('BETA-W2V', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) WRITE (*, 40) INT(X1*1D9), INT(X2*1D9), CDELTX*1D9 40 FORMAT (/,'Linear air wavelength axis, span:',I4,' to',I4, : ' (nm), step:',F9.6,' (nm)',/,'----------------------', : '----------------------------------------------------') NFAIL = NFAIL + CLOSURE('FREQ-A2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AFRQ-A2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ENER-A2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVN-A2F', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VRAD-A2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVE-A2W', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VOPT-A2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ZOPT-A2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VELO-A2V', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('BETA-A2V', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) RESTFRQ = 1420.40595D6 RESTWAV = C/RESTFRQ X1 = -0.96D0*C X2 = 0.96D0*C CDELTX = (X2 - X1)/(NAXISJ - 1) CRVALX = X1 + (CRPIXJ - 1D0)*CDELTX WRITE (*, 50) INT(X1), INT(X2), INT(CDELTX) 50 FORMAT (/,'Linear velocity axis, span:',I11,' to',I10, : ' m/s, step:',I6,' (m/s)',/,'-----------------------', : '---------------------------------------------------') NFAIL = NFAIL + CLOSURE('FREQ-V2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AFRQ-V2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ENER-V2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVN-V2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VRAD-V2F', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVE-V2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VOPT-V2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ZOPT-V2W', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AWAV-V2A', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) RESTWAV = 650D-9 RESTFRQ = C/RESTWAV X1 = 300D-9 X2 = 1000D-9 CDELTX = (X2 - X1)/(NAXISJ - 1) CRVALX = X1 + (CRPIXJ - 1D0)*CDELTX WRITE (*, 60) INT(X1*1D9), INT(X2*1D9), CDELTX*1D9 60 FORMAT (/,'Vacuum wavelength grism axis, span:',I4,' to',I5, : ' (nm), step:',F9.6,' (nm)',/,'----------------------', : '----------------------------------------------------') NFAIL = NFAIL + CLOSURE('FREQ-GRI', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AFRQ-GRI', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ENER-GRI', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVN-GRI', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VRAD-GRI', RESTFRQ, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('WAVE-GRI', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VOPT-GRI', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('ZOPT-GRI', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('AWAV-GRI', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VELO-GRI', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('BETA-GRI', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) * Reproduce Fig. 5 of Paper III. NAXISJ = 1700 CRPIXJ = 719.8D0 CRVALX = 7245.2D-10 CDELTX = 2.956D-10 RESTWAV = 8500D-10 RESTFRQ = C/RESTWAV X1 = CRVALX + (1 - CRPIXJ)*CDELTX X2 = CRVALX + (NAXISJ - CRPIXJ)*CDELTX MARS(5) = 0D0 MARS(6) = 0D0 WRITE (*, 70) INT(X1*1D9), INT(X2*1D9), CDELTX*1D9 70 FORMAT (/,'Air wavelength grism axis, span:',I4,' to',I5, : ' (nm), step:',F9.6,' (nm)',/,'----------------------', : '----------------------------------------------------') NFAIL = NFAIL + CLOSURE('AWAV-GRA', 0D0, 0D0, NAXISJ, CRPIXJ, : CDELTX, CRVALX) NFAIL = NFAIL + CLOSURE('VELO-GRA', 0D0, RESTWAV, NAXISJ, CRPIXJ, : CDELTX, CRVALX) CALL PGASK(0) CALL PGEND() IF (NFAIL.NE.0) THEN WRITE (*, 80) NFAIL 80 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 90) 90 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF END *======================================================================= INTEGER FUNCTION CLOSURE (CTYPES, RESTFRQ, RESTWAV, NAXISJ, : CRPIXJ, CDELTX, CRVALX) INTEGER NSPEC PARAMETER (NSPEC = 10001) INTEGER J, NAXISJ, NFAIL, RESTREQ, STAT1(NSPEC), STAT2(NSPEC), : STATUS REAL TMP, X(NSPEC), XMIN, XMAX, Y(NSPEC), YMAX, YMIN DOUBLE PRECISION CDELTS, CDELTX, CLOS(NSPEC), CRPIXJ, CRVALS, : CRVALX, DSDX, MARS(0:6), RESID, RESIDMAX, RESTFRQ, : RESTWAV, SPEC1(NSPEC), SPEC2(NSPEC), TOL CHARACTER CTYPES*8, PTYPE, SCODE*3, SNAME*21, STYPE*4, TITLE*80, : UNITS*7, XTYPE, YLAB*80 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'spx.inc' INCLUDE 'spc.inc' INTEGER SPC(SPCLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (SPC,DUMMY) COMMON /SPECTRO/ MARS DATA TOL /1D-11/ *----------------------------------------------------------------------- * Get keyvalues for the required spectral axis type. STATUS = SPCXPS (CTYPES, CRVALX, RESTFRQ, RESTWAV, PTYPE, XTYPE, : RESTREQ, CRVALS, DSDX) IF (STATUS.NE.0) THEN WRITE (*, 5) STATUS, CTYPES 5 FORMAT ('ERROR',I2,' from SPCXPS for',A,'.') RETURN END IF CDELTS = CDELTX * DSDX STATUS = SPCINI(SPC) IF (CTYPES(6:6).EQ.'G') THEN * KPNO MARS spectrograph grism parameters. STATUS = SPCPUT (SPC, SPC_PV, MARS(0), 0) STATUS = SPCPUT (SPC, SPC_PV, MARS(1), 1) STATUS = SPCPUT (SPC, SPC_PV, MARS(2), 2) STATUS = SPCPUT (SPC, SPC_PV, MARS(3), 3) STATUS = SPCPUT (SPC, SPC_PV, MARS(4), 4) STATUS = SPCPUT (SPC, SPC_PV, MARS(5), 5) STATUS = SPCPUT (SPC, SPC_PV, MARS(6), 6) END IF * Construct the axis. DO 10 J = 1, NAXISJ SPEC1(J) = (J - CRPIXJ)*CDELTS 10 CONTINUE WRITE (*, 20) CTYPES, CRVALS+SPEC1(1), CRVALS+SPEC1(NAXISJ), : CDELTS 20 FORMAT (A,' (CRVALk+w) range: ',1PE13.6,' to ',1PE13.6,', step: ', : 1PE13.6) * Initialize. STATUS = SPCPUT (SPC, SPC_FLAG, 0, 0) STATUS = SPCPUT (SPC, SPC_CRVAL, CRVALS, 0) STATUS = SPCPUT (SPC, SPC_RESTFRQ, RESTFRQ, 0) STATUS = SPCPUT (SPC, SPC_RESTWAV, RESTWAV, 0) STATUS = SPCPUT (SPC, SPC_TYPE, CTYPES, 0) STATUS = SPCPUT (SPC, SPC_CODE, CTYPES(6:8), 0) * Convert the first to the second. STATUS = SPCX2S(SPC, NAXISJ, 1, 1, SPEC1, SPEC2, STAT1) IF (STATUS.NE.0) THEN WRITE (*, 30) STATUS 30 FORMAT ('SPCX2S ERROR',I2,'.') RETURN END IF * Convert the second back to the first. STATUS = SPCS2X(SPC, NAXISJ, 1, 1, SPEC2, CLOS, STAT2) IF (STATUS.NE.0) THEN WRITE (*, 40) STATUS 40 FORMAT ('SPCS2X ERROR',I2,'.') RETURN END IF * Test closure. NFAIL = 0 RESIDMAX = 0D0 STATUS = SPCGET (SPC, SPC_TYPE, STYPE, 0) DO 80 J = 1, NAXISJ IF (STAT1(J).NE.0) THEN WRITE (*, 50) CTYPES, SPEC1(J), STYPE, STAT1(J) 50 FORMAT (A,': w =',1PE20.12,' -> ',A,' = ???, stat = ',I2) GO TO 80 END IF IF (STAT2(J).NE.0) THEN WRITE (*, 60) CTYPES, SPEC1(J), STYPE, SPEC2(J), STAT2(J) 60 FORMAT (A,': w =',1PE20.12,' -> ',A,' =',1PE20.12, : ' -> w = ???, stat = ',I2) GO TO 80 END IF RESID = ABS((CLOS(J) - SPEC1(J))/CDELTS) IF (RESID.GT.RESIDMAX) RESIDMAX = RESID IF (RESID.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 70) CTYPES, SPEC1(J), STYPE, SPEC2(J), CLOS(J), : RESID 70 FORMAT (A,': w =',1PE20.12,' -> ',A,' =',1PE20.12,' ->',/, : ' w =',1PE20.12,', resid =',1PE8.1) END IF 80 CONTINUE WRITE (*, 90) CTYPES, RESIDMAX 90 FORMAT (A,': Maximum closure residual =',1PE8.1,' pixel') * Draw graph. CALL PGBBUF() CALL PGERAS() XMIN = REAL(CRVALS + SPEC1(1)) XMAX = REAL(CRVALS + SPEC1(NAXISJ)) YMIN = REAL(SPEC2(1)) - XMIN YMAX = YMIN DO 100 J = 1, NAXISJ X(J) = REAL(J) Y(J) = REAL(SPEC2(J) - (CRVALS + SPEC1(J))) IF (Y(J).GT.YMAX) YMAX = Y(J) IF (Y(J).LT.YMIN) YMIN = Y(J) 100 CONTINUE J = INT(CRPIXJ+1) IF (Y(J).LT.0D0) then TMP = YMIN YMIN = YMAX YMAX = TMP END IF CALL PGASK(0) CALL PGENV(1.0, REAL(NAXISJ), YMIN, YMAX, 0, -1) CALL PGSCI(1) CALL PGBOX('ABNTS', 0.0, 0, 'BNTS', 0.0, 0) STATUS = SPCTYP (CTYPES, STYPE, SCODE, SNAME, UNITS, PTYPE, XTYPE, : RESTREQ) DO 110 J = 21, 1, -1 IF (SNAME(J:J).NE.' ') GO TO 120 110 CONTINUE 120 YLAB = SNAME(:J) // ' - correction ' // UNITS TITLE = CTYPES // ': CRVALk + w ' // UNITS CALL PGLAB('Pixel coordinate', YLAB, TITLE) CALL PGAXIS('N', 0.0, YMAX, REAL(NAXISJ), YMAX, XMIN, XMAX, 0.0, : 0, -0.5, 0.0, 0.5, -0.5, 0.0) CALL PGAXIS('N', REAL(NAXISJ), ymin, REAL(NAXISJ), YMAX, : REAL(YMIN/CDELTS), REAL(YMAX/CDELTS), 0.0, 0, 0.5, : 0.0, 0.5, 0.1, 0.0) CALL PGMTXT('R', 2.2, 0.5, 0.5, 'Pixel offset') CALL PGLINE(NAXISJ, X, Y) CALL PGSCI(7) CALL PGPT1(REAL(CRPIXJ), 0.0, 24) CALL PGEBUF() WRITE (*, '(A,$)') 'Type for next page: ' READ (*, *, END=130) 130 WRITE (*, *) CLOSURE = NFAIL END pywcs-1.12/wcslib/Fortran/test/tsph.f0000644001153600020070000001211112310355626021644 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tsph.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TSPH *----------------------------------------------------------------------- * * TSPH tests the forward and reverse spherical coordinate transformation * routines for closure. * *----------------------------------------------------------------------- INTEGER J, LAT, LNG, NFAIL, SPHS2X, SPHX2S, STATUS DOUBLE PRECISION COSLAT, DLAT, DLATMX, DLNG, DLNGMX, LNG1(361), : LNG2(361), EUL(5), LAT1, LAT2(361), PHI(361), : THETA(361), TOL, ZETA PARAMETER (TOL = 1D-12) DOUBLE PRECISION D2R, PI PARAMETER (PI = 3.141592653589793238462643D0) PARAMETER (D2R = PI/180D0) *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing closure of WCSLIB coordinate transformation ', : 'routines (tsph.f)',/, : '----------------------------------------------------', : '-----------------') * Set reference angles. EUL(1) = 90D0 EUL(2) = 30D0 EUL(3) = -90D0 WRITE (*, 20) (EUL(J),J=1,3) 20 FORMAT (/,'Celestial longitude and latitude of the native pole, ', : 'and native',/,'longitude of the celestial pole ', : '(degrees):',3F10.4) EUL(4) = COS(EUL(2)*D2R) EUL(5) = SIN(EUL(2)*D2R) WRITE (*, 30) TOL 30 FORMAT ('Reporting tolerance:',1PG8.1,' degrees of arc.') NFAIL = 0 DLNGMX = 0D0 DLATMX = 0D0 DO 70 LAT = 90, -90, -1 LAT1 = DBLE(LAT) COSLAT = COS(LAT1*D2R) J = 1 DO 40 LNG = -180, 180 LNG1(J) = DBLE(LNG) J = J + 1 40 CONTINUE STATUS = SPHS2X (EUL, 361, 1, 1, 1, LNG1, LAT1, PHI, THETA) STATUS = SPHX2S (EUL, 361, 0, 1, 1, PHI, THETA, LNG2, LAT2) DO 60 J = 1, 361 DLNG = ABS(LNG2(J) - LNG1(J)) IF (DLNG.GT.180D0) DLNG = ABS(DLNG-360D0) DLNG = DLNG*COSLAT DLAT = ABS(LAT2(J)-LAT1) IF (DLNG.GT.DLNGMX) DLNGMX = DLNG IF (DLAT.GT.DLATMX) DLATMX = DLAT IF (DLNG.GT.TOL .OR. DLAT.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 50) LNG1(J), LAT1, PHI(J), THETA(J), LNG2(J), : LAT2(J) 50 FORMAT ('Unclosed: LNG1 =',F20.15,' LAT1 =',F20.15,/, : ' PHI =',F20.15,' THETA =',F20.15,/, : ' LNG2 =',F20.15,' LAT2 =',F20.15) END IF 60 CONTINUE 70 CONTINUE * Test closure at points close to the pole. DO 90 J = -1, 1, 2 ZETA = 1D0 LNG1(1) = -180D0 DO 80 LAT = 1, 12 LAT1 = DBLE(J)*(90D0 - ZETA) STATUS = SPHS2X (EUL, 1, 1, 1, 1, LNG1, LAT1, PHI, THETA) STATUS = SPHX2S (EUL, 1, 1, 1, 1, PHI, THETA, LNG2, LAT2) DLNG = ABS(LNG2(1) - LNG1(1)) IF (DLNG.GT.180D0) DLNG = ABS(DLNG-360D0) DLNG = DLNG*COSLAT DLAT = ABS(LAT2(1)-LAT1) IF (DLNG.GT.DLNGMX) DLNGMX = DLNG IF (DLAT.GT.DLATMX) DLATMX = DLAT IF (DLNG.GT.TOL .OR. DLAT.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 50) LNG1(1), LAT1, PHI(1), THETA(1), LNG2(1), : LAT2(1) END IF ZETA = ZETA/10D0 LNG1(1) = LNG1(1) + 30D0 80 CONTINUE 90 CONTINUE WRITE (*, 100) DLNGMX, DLATMX 100 FORMAT (/,'SPHS2X/SPHX2S: Maximum closure residual =',1P,E8.1, : ' (lng)',E8.1,' (lat) deg.') IF (NFAIL.NE.0) THEN WRITE (*, 110) NFAIL 110 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 120) 120 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF END pywcs-1.12/wcslib/Fortran/test/tspx.f0000644001153600020070000002436112310355626021676 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tspx.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TSPX *----------------------------------------------------------------------- * * TSPEC tests the spectral transformation routines for closure. * *----------------------------------------------------------------------- * Length of spectral axis - see CLOSURE. INTEGER NSPEC PARAMETER (NSPEC = 9991) INTEGER CLOSURE, J, K, NFAIL, STAT(NSPEC), STATUS DOUBLE PRECISION AWAV(NSPEC), C, FREQ(NSPEC), RESTFRQ, RESTWAV, : SPC1(NSPEC), SPC2(NSPEC), STEP, VELO(NSPEC), WAVE(NSPEC) INCLUDE 'spx.inc' DATA C /2.99792458D8/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing closure of WCSLIB spectral transformation ', : 'routines (tspx.f)',/, : '--------------------------------------------------', : '-----------------') RESTFRQ = 1420.40595D6 RESTWAV = C/RESTFRQ * Exercise SPECX. WRITE (*, 20) 20 FORMAT (/,'Testing spectral cross-conversions (specx).',/) STATUS = SPECX('VELO', 4.3D5, RESTFRQ, RESTWAV, SPX) WRITE (*, 30) SPX(1), SPX(2), SPXI(1), SPXI(2), (SPX(J), J=4,14) 30 FORMAT (' restfrq:',1PE20.12,/,' restwav:',1PE20.12,/, : ' wavetype:',I3,/, ' velotype:',I3,//, : ' freq:',1PE20.12,/,' afrq:',1PE20.12,/, : ' ener:',1PE20.12,/,' wavn:',1PE20.12,/, : ' vrad:',1PE20.12,/,' wave:',1PE20.12,/, : ' vopt:',1PE20.12,/,' zopt:',1PE20.12,/, : ' awav:',1PE20.12,/,' velo:',1PE20.12,/, : ' beta:',1PE20.12,/) WRITE (*, 40) (SPX(J), J=15,40) 40 FORMAT ('dfreq/dafrq:',1PE20.12,/,'dafrq/dfreq:',1PE20.12,/, : 'dfreq/dener:',1PE20.12,/,'dener/dfreq:',1PE20.12,/, : 'dfreq/dwavn:',1PE20.12,/,'dwavn/dfreq:',1PE20.12,/, : 'dfreq/dvrad:',1PE20.12,/,'dvrad/dfreq:',1PE20.12,/, : 'dfreq/dwave:',1PE20.12,/,'dwave/dfreq:',1PE20.12,/, : 'dfreq/dawav:',1PE20.12,/,'dawav/dfreq:',1PE20.12,/, : 'dfreq/dvelo:',1PE20.12,/,'dvelo/dfreq:',1PE20.12,/, : 'dwave/dvopt:',1PE20.12,/,'dvopt/dwave:',1PE20.12,/, : 'dwave/dzopt:',1PE20.12,/,'dzopt/dwave:',1PE20.12,/, : 'dwave/dawav:',1PE20.12,/,'dawav/dwave:',1PE20.12,/, : 'dwave/dvelo:',1PE20.12,/,'dvelo/dwave:',1PE20.12,/, : 'dawav/dvelo:',1PE20.12,/,'dvelo/dawav:',1PE20.12,/, : 'dvelo/dbeta:',1PE20.12,/,'dbeta/dvelo:',1PE20.12,/) * Construct a linear velocity spectrum. STEP = (2D0*C/NSPEC) / 2D0 K = -NSPEC DO 50 J = 1, NSPEC VELO(J) = (K+1)*STEP K = K + 2 50 CONTINUE WRITE (*, 60) VELO(1)*1D-3, VELO(NSPEC)*1D-3, : (VELO(2) - VELO(1))*1D-3 60 FORMAT (/,'Velocity range:',F12.3,' to',F11.3,' km/s, step:', : F7.3,' km/s') * Convert it to frequency. STATUS = VELOFREQ(RESTFRQ, NSPEC, 1, 1, VELO, FREQ, STAT) * Test closure of all two-way combinations. NFAIL = 0 NFAIL = NFAIL + CLOSURE ('freq', 'afrq', 0D0, : FREQAFRQ, AFRQFREQ, FREQ, SPC1) NFAIL = NFAIL + CLOSURE ('afrq', 'freq', 0D0, : AFRQFREQ, FREQAFRQ, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('freq', 'ener', 0D0, : FREQENER, ENERFREQ, FREQ, SPC1) NFAIL = NFAIL + CLOSURE ('ener', 'freq', 0D0, : ENERFREQ, FREQENER, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('freq', 'wavn', 0D0, : FREQWAVN, WAVNFREQ, FREQ, SPC1) NFAIL = NFAIL + CLOSURE ('wavn', 'freq', 0D0, : WAVNFREQ, FREQWAVN, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('freq', 'vrad', RESTFRQ, : FREQVRAD, VRADFREQ, FREQ, SPC1) NFAIL = NFAIL + CLOSURE ('vrad', 'freq', RESTFRQ, : VRADFREQ, FREQVRAD, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('freq', 'wave', 0D0, : FREQWAVE, WAVEFREQ, FREQ, WAVE) NFAIL = NFAIL + CLOSURE ('wave', 'freq', 0D0, : WAVEFREQ, FREQWAVE, WAVE, SPC2) NFAIL = NFAIL + CLOSURE ('freq', 'awav', 0D0, : FREQAWAV, AWAVFREQ, FREQ, AWAV) NFAIL = NFAIL + CLOSURE ('awav', 'freq', 0D0, : AWAVFREQ, FREQAWAV, AWAV, SPC2) NFAIL = NFAIL + CLOSURE ('freq', 'velo', RESTFRQ, : FREQVELO, VELOFREQ, FREQ, VELO) NFAIL = NFAIL + CLOSURE ('velo', 'freq', RESTFRQ, : VELOFREQ, FREQVELO, VELO, SPC2) NFAIL = NFAIL + CLOSURE ('wave', 'vopt', RESTWAV, : WAVEVOPT, VOPTWAVE, WAVE, SPC1) NFAIL = NFAIL + CLOSURE ('vopt', 'wave', RESTWAV, : VOPTWAVE, WAVEVOPT, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('wave', 'zopt', RESTWAV, : WAVEZOPT, ZOPTWAVE, WAVE, SPC1) NFAIL = NFAIL + CLOSURE ('zopt', 'wave', RESTWAV, : ZOPTWAVE, WAVEZOPT, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('wave', 'awav', 0D0, : WAVEAWAV, AWAVWAVE, WAVE, SPC1) NFAIL = NFAIL + CLOSURE ('awav', 'wave', 0D0, : AWAVWAVE, WAVEAWAV, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('wave', 'velo', RESTWAV, : WAVEVELO, VELOWAVE, WAVE, SPC1) NFAIL = NFAIL + CLOSURE ('velo', 'wave', RESTWAV, : VELOWAVE, WAVEVELO, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('awav', 'velo', RESTWAV, : AWAVVELO, VELOAWAV, AWAV, SPC1) NFAIL = NFAIL + CLOSURE ('velo', 'awav', RESTWAV, : VELOAWAV, AWAVVELO, SPC1, SPC2) NFAIL = NFAIL + CLOSURE ('velo', 'beta', 0D0, : VELOBETA, BETAVELO, VELO, SPC1) NFAIL = NFAIL + CLOSURE ('beta', 'velo', 0D0, : BETAVELO, VELOBETA, SPC1, SPC2) IF (NFAIL.NE.0) THEN WRITE (*, 70) NFAIL 70 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 80) 80 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF END *======================================================================= INTEGER FUNCTION CLOSURE (FROM, TO, PARM, FWD, REV, SPEC1, SPEC2) INTEGER NSPEC PARAMETER (NSPEC = 9991) LOGICAL SKIP INTEGER J, NFAIL, STAT1(NSPEC), STAT2(NSPEC), STATUS DOUBLE PRECISION CLOS(NSPEC), PARM, RESID, RESIDMAX, SPEC1(NSPEC), : SPEC2(NSPEC), TOL CHARACTER FROM*(*), TO*(*) PARAMETER (TOL = 1D-9) INTEGER FWD, REV EXTERNAL FWD, REV SAVE SKIP DATA SKIP/.FALSE./ *----------------------------------------------------------------------- * Convert the first to the second. STATUS = FWD(PARM, NSPEC, 1, 1, SPEC1, SPEC2, STAT1) IF (STATUS.NE.0) THEN WRITE (*, 10) FROM, TO, STATUS 10 FORMAT (A,A,' ERROR',I2,'.') END IF * Convert the second back to the first. STATUS = REV(PARM, NSPEC, 1, 1, SPEC2, CLOS, STAT2) IF (STATUS.NE.0) THEN WRITE (*, 10) TO, FROM, STATUS END IF * Test closure. NFAIL = 0 RESIDMAX = 0.0 DO 50 J = 1, NSPEC IF (STAT1(J).NE.0) THEN IF (SKIP) WRITE (*, *) WRITE (*, 20) FROM, TO, FROM, SPEC1(J), TO, STAT1(J) 20 FORMAT (A,A,': ',A,' =',1PE19.12,' -> ',A, : ' = ???, stat = ',I2) SKIP = .FALSE. GO TO 50 END IF IF (STAT2(J).NE.0) THEN IF (SKIP) WRITE (*, *) WRITE (*, 30) TO, FROM, FROM, SPEC1(J), TO, SPEC2(J), FROM, : STAT2(J) 30 FORMAT (A,A,': ',A,' =',1PE19.12,' -> ',A,' =',1PE19.12, : ' -> ',A,' = ???, stat = ',I2) SKIP = .FALSE. GO TO 50 END IF IF (SPEC1(J).EQ.0.0) THEN RESID = ABS(CLOS(J) - SPEC1(J)) ELSE RESID = ABS((CLOS(J) - SPEC1(J))/SPEC1(J)) IF (RESID.GT.RESIDMAX) RESIDMAX = RESID END IF IF (RESID.GT.TOL) THEN NFAIL = NFAIL + 1 IF (SKIP) WRITE (*, *) WRITE (*, 40) FROM, TO, FROM, SPEC1(J), TO, SPEC2(J), FROM, : CLOS(J), RESID 40 FORMAT (A,A,': ',A,' =',1PE19.12,' -> ',A,' =',1PE19.12, : ' ->',/,' ',A,' =',1PE19.12,', resid =', : 1PE8.1) SKIP = .FALSE. END IF 50 CONTINUE WRITE (*, 60) FROM, TO, RESIDMAX 60 FORMAT (A,A,': Maximum closure residual =',1PE8.1) IF (RESIDMAX.GT.TOL) THEN WRITE (*, *) SKIP = .FALSE. ELSE SKIP = .TRUE. END IF CLOSURE = NFAIL END pywcs-1.12/wcslib/Fortran/test/ttab1.f0000644001153600020070000002170512310355626021712 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: ttab1.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TTAB1 *----------------------------------------------------------------------- * * TTAB1 tests the -TAB routines for closure. * *----------------------------------------------------------------------- DOUBLE PRECISION TOL PARAMETER (TOL = 1D-8) INTEGER K1, K2, M PARAMETER (M = 2, K1 = 32, K2 = 16) INTEGER K(2), MAP(2) DOUBLE PRECISION CRVAL(2) DATA K /K1, K2/ DATA MAP /0, 1/ DATA CRVAL /1D0, -1D0/ INTEGER I, IK, IK1, IK2, IM, J, N, NFAIL, STAT0(128), : STAT1(128), STATUS DOUBLE PRECISION CRPIX4, EPSILON, RESID, RESIDMAX, TIME(12), : WORLD(M,11,11), XT0(12), XT1(12), X0(M,11,11), : X1(M,11,11), Z * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'tab.inc' INTEGER TAB(TABLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (TAB,DUMMY) *----------------------------------------------------------------------- WRITE (*, 10) TOL 10 FORMAT ('Testing closure of WCSLIB tabular coordinate routines ', : '(ttab1.f)',/, : '------------------------------------------------------', : '---------',//, : 'Reporting tolerance',1PG8.1,'.') * First a 1-dimensional table from Sect. 6.2.3 of Paper III. WRITE (*, '(/,A)') 'One-dimensional test:' STATUS = TABPUT (TAB, TAB_FLAG, -1, 0, 0) STATUS = TABINI (M, K, TAB) IF (STATUS.NE.0) THEN WRITE (*, 20) STATUS 20 FORMAT ('TABINI ERROR',I2,'.') GO TO 999 END IF STATUS = TABPUT (TAB, TAB_M, 1, 0, 0) STATUS = TABPUT (TAB, TAB_K, 8, 1, 0) STATUS = TABPUT (TAB, TAB_MAP, 0, 1, 0) STATUS = TABPUT (TAB, TAB_CRVAL, 0D0, 1, 0) STATUS = TABPUT (TAB, TAB_INDEX, 0D0, 1, 1) STATUS = TABPUT (TAB, TAB_INDEX, 1D0, 1, 2) STATUS = TABPUT (TAB, TAB_INDEX, 1D0, 1, 3) STATUS = TABPUT (TAB, TAB_INDEX, 2D0, 1, 4) STATUS = TABPUT (TAB, TAB_INDEX, 2D0, 1, 5) STATUS = TABPUT (TAB, TAB_INDEX, 3D0, 1, 6) STATUS = TABPUT (TAB, TAB_INDEX, 3D0, 1, 7) STATUS = TABPUT (TAB, TAB_INDEX, 4D0, 1, 8) STATUS = TABPUT (TAB, TAB_COORD, 1997.84512D0, 1, 0) STATUS = TABPUT (TAB, TAB_COORD, 1997.84631D0, 2, 0) STATUS = TABPUT (TAB, TAB_COORD, 1993.28451D0, 3, 0) STATUS = TABPUT (TAB, TAB_COORD, 1993.28456D0, 4, 0) STATUS = TABPUT (TAB, TAB_COORD, 2001.59234D0, 5, 0) STATUS = TABPUT (TAB, TAB_COORD, 2001.59239D0, 6, 0) STATUS = TABPUT (TAB, TAB_COORD, 2002.18265D0, 7, 0) STATUS = TABPUT (TAB, TAB_COORD, 2002.18301D0, 8, 0) EPSILON = 1D-3 CRPIX4 = 0.5 XT0(1) = 0.5 + EPSILON - CRPIX4 XT0(2) = 1.0 - CRPIX4 XT0(3) = 1.5 - EPSILON - CRPIX4 XT0(4) = 1.5 + EPSILON - CRPIX4 XT0(5) = 2.0 - CRPIX4 XT0(6) = 2.5 - EPSILON - CRPIX4 XT0(7) = 2.5 + EPSILON - CRPIX4 XT0(8) = 3.0 - CRPIX4 XT0(9) = 3.5 - EPSILON - CRPIX4 XT0(10) = 3.5 + EPSILON - CRPIX4 XT0(11) = 4.0 - CRPIX4 XT0(12) = 4.5 - EPSILON - CRPIX4 STATUS = TABX2S (TAB, 12, 1, XT0, TIME, STAT0) IF (STATUS.NE.0) THEN WRITE (*, 30) STATUS 30 FORMAT ('TABX2S ERROR',I2,'.') END IF STATUS = TABS2X (TAB, 12, 1, TIME, XT1, STAT1) IF (STATUS.NE.0) THEN WRITE (*, 40) STATUS 40 FORMAT ('TABX2S ERROR',I2,'.') END IF WRITE (*, 50) 50 FORMAT (' x -> time -> x') DO 70 I = 1, 12 WRITE (*, 60) XT0(I), TIME(I), XT1(I) 60 FORMAT (F8.5,F12.5,F9.5) 70 CONTINUE WRITE (*, '(/)') * Test closure. NFAIL = 0 RESIDMAX = 0D0 DO 110 I = 1, 12 IF (STAT0(I).NE.0) THEN WRITE (*, 80) XT0(I), STAT0(I) 80 FORMAT (' TABX2S: X =',F7.1,', STAT =',I2) GO TO 110 END IF IF (STAT1(I).NE.0) THEN WRITE (*, 90) TIME(I), STAT1(I) 90 FORMAT (' TABS2X: T =',F7.1,', STAT =',I2) GO TO 110 END IF RESID = ABS(XT1(I) - XT0(I)) IF (RESID.GT.RESIDMAX) RESIDMAX = RESID IF (RESID.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 100) XT0(I), TIME(I), XT1(I) 100 FORMAT (' Closure error:',/,' X = ',F20.15,/, : ' -> T = ',F20.15,/,' -> X = ',F20.15) END IF 110 CONTINUE STATUS = TABFREE (TAB) * Now a 2-dimensional table. WRITE (*, '(A)') 'Two-dimensional test:' STATUS = TABPUT (TAB, TAB_FLAG, -1, 0, 0) STATUS = TABINI (M, K, TAB) IF (STATUS.NE.0) THEN WRITE (*, 120) STATUS 120 FORMAT ('TABINI ERROR',I2,'.') GO TO 999 END IF STATUS = TABPUT (TAB, TAB_M, M, 0, 0) DO 140 IM = 1, M STATUS = TABPUT (TAB, TAB_K, K(IM), IM, 0) STATUS = TABPUT (TAB, TAB_MAP, MAP(IM), IM, 0) STATUS = TABPUT (TAB, TAB_CRVAL, CRVAL(IM), IM, 0) DO 130 IK = 1, K(IM) STATUS = TABPUT (TAB, TAB_INDEX, DBLE(IK-1), IM, IK) 130 CONTINUE 140 CONTINUE N = 0 Z = 1D0 / ((K1-1) * (K2-1)) DO 160 IK2 = 0, K2-1 DO 150 IK1 = 0, K1-1 N = N + 1 STATUS = TABPUT (TAB, TAB_COORD, 3D0*IK1*IK2*Z, N, 0) N = N + 1 STATUS = TABPUT (TAB, TAB_COORD, -1D0*(K1-IK1-1)*IK2*Z + : 0.01*IK1, N, 0) 150 CONTINUE 160 CONTINUE DO 180 I = 1, 11 DO 170 J = 1, 11 X0(1,J,I) = (J-1)*(K1-1)/10D0 - CRVAL(1) X0(2,J,I) = (I-1)*(K2-1)/10D0 - CRVAL(2) 170 CONTINUE 180 CONTINUE STATUS = TABX2S (TAB, 121, 2, X0, WORLD, STAT0) IF (STATUS.NE.0) THEN WRITE (*, 190) STATUS 190 FORMAT ('TABX2S ERROR',I2,'.') END IF STATUS = TABS2X (TAB, 121, 2, WORLD, X1, STAT1) IF (STATUS.NE.0) THEN WRITE (*, 200) STATUS 200 FORMAT ('TABX2S ERROR',I2,'.') END IF * Test closure. N = 0 RESIDMAX = 0D0 DO 260 I = 1, 11 DO 250 J = 1, 11 N = N + 1 IF (STAT0(N).NE.0) THEN WRITE (*, 210) X0(1,J,I), X0(2,J,I), STAT0(N) 210 FORMAT (' TABX2S: X = (',F6.1,',',F6.1,'), STAT =',I2) GO TO 250 END IF IF (STAT1(N).NE.0) THEN WRITE (*, 220) WORLD(1,J,I), WORLD(2,J,I), STAT1(N) 220 FORMAT (' TABS2X: S = (',F6.1,',',F6.1,'), STAT =',I2) GO TO 250 END IF DO 240 IM = 1, M RESID = ABS(X1(IM,J,I) - X0(IM,J,I)) IF (RESID.GT.RESIDMAX) RESIDMAX = RESID IF (RESID.GT.TOL) THEN NFAIL = NFAIL + 1 WRITE (*, 230) X0(1,J,I), X0(2,J,I), WORLD(1,J,I), : WORLD(2,J,I), X1(1,J,I), X1(2,J,I) 230 FORMAT (' Closure error:',/, : ' X = (',F20.15,',',F20.15,')',/, : ' -> W = (',F20.15,',',F20.15,')',/, : ' -> X = (',F20.15,',',F20.15,')') GO TO 250 END IF 240 CONTINUE 250 CONTINUE 260 CONTINUE WRITE (*, 270) RESIDMAX 270 FORMAT (/,'TABX2S/TABS2X: Maximum closure residual =',1PE8.1) IF (NFAIL.NE.0) THEN WRITE (*, 280) NFAIL 280 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') ELSE WRITE (*, 290) 290 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.') END IF 999 STATUS = TABFREE (TAB) END pywcs-1.12/wcslib/Fortran/test/ttab2.f0000644001153600020070000002242612310355626021714 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: ttab2.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TTAB2 *----------------------------------------------------------------------- * * TTAB2 tests the -TAB routines using PGPLOT for graphical display. It * demonstrates the nature of linear interpolation in 2 dimensions by * contouring the interior a single 2 x 2 interpolation element as the * values in each corner change. * *----------------------------------------------------------------------- * Set up a 2 x 2 lookup table. INTEGER K1, K2, M PARAMETER (M = 2, K1 = 2, K2 = 2) INTEGER K(2), MAP(2) DOUBLE PRECISION CRVAL(2) DATA K /K1, K2/ DATA MAP /0, 1/ DATA CRVAL /0D0, 0D0/ * Number of subdivisions on each side of the interpolation element. INTEGER NP REAL SCL PARAMETER (NP = 128) PARAMETER (SCL = 2.0/(NP-1)) INTEGER I, IM, IK, J, L, L1, L2, L3, LSTEP, STAT(NP*NP), STATUS REAL ARRAY(NP,NP), CLEV(-10:20), LTM(6), V0, V1, W DOUBLE PRECISION X(M,NP,NP), WORLD(M,NP,NP) CHARACTER TEXT*80 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'tab.inc' INTEGER TAB(TABLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (TAB,DUMMY) *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ( : 'Testing WCSLIB coordinate lookup table routines (ttab2.f)',/, : '---------------------------------------------------------') * PGPLOT initialization. CALL PGBEG (0, '/xwindow', 1, 1) CALL PGVSTD () CALL PGSCH (0.7) * The viewport is slightly oversized. CALL PGWNAD (-0.65, 1.65, -0.65, 1.65) DO 20 L = -10, 20 CLEV(L) = 0.2*L 20 CONTINUE LTM(1) = -SCL*(1.0 + (NP-1)/4.0) LTM(2) = SCL LTM(3) = 0.0 LTM(4) = -SCL*(1.0 + (NP-1)/4.0) LTM(5) = 0.0 LTM(6) = SCL * Set up the lookup table. STATUS = TABPUT (TAB, TAB_FLAG, -1, 0, 0) STATUS = TABINI(M, K, TAB) IF (STATUS.NE.0) THEN WRITE (*, 30) STATUS 30 FORMAT ('TABINI ERROR',I2,'.') GO TO 999 END IF STATUS = TABPUT (TAB, TAB_M, M, 0, 0) DO 50 IM = 1, M STATUS = TABPUT (TAB, TAB_K, K(IM), IM, 0) STATUS = TABPUT (TAB, TAB_MAP, MAP(IM), IM, 0) STATUS = TABPUT (TAB, TAB_CRVAL, CRVAL(IM), IM, 0) DO 40 IK = 1, K(IM) STATUS = TABPUT (TAB, TAB_INDEX, DBLE(IK-1), IM, IK) 40 CONTINUE 50 CONTINUE * Subdivide the interpolation element. DO 70 I = 1, NP DO 60 J = 1, NP X(1,J,I) = (J-1)*(K1-1.0)*SCL - 0.5 - CRVAL(1) X(2,J,I) = (I-1)*(K2-1.0)*SCL - 0.5 - CRVAL(2) 60 CONTINUE 70 CONTINUE * The first coordinate element is static. STATUS = TABPUT (TAB, TAB_COORD, 0D0, 1, 0) STATUS = TABPUT (TAB, TAB_COORD, 0D0, 3, 0) STATUS = TABPUT (TAB, TAB_COORD, 0D0, 5, 0) STATUS = TABPUT (TAB, TAB_COORD, 0D0, 7, 0) * (k1,k2) = (1,1). STATUS = TABPUT (TAB, TAB_COORD, 0D0, 2, 0) * The second coordinate element varies in three of the corners. DO 170 L3 = 0, 100, 20 * (k1,k2) = (2,2). STATUS = TABPUT (TAB, TAB_COORD, 0.01D0*L3, 8, 0) DO 160 L2 = 0, 100, 20 * (k1,k2) = (1,2). STATUS = TABPUT (TAB, TAB_COORD, 0.01D0*L2, 6, 0) CALL PGPAGE () DO 150 L1 = 0, 100, 2 * (k1,k2) = (2,1). STATUS = TABPUT (TAB, TAB_COORD, 0.01D0*L1, 4, 0) * Compute coordinates within the interpolation element. STATUS = TABX2S (TAB, NP*NP, 2, X, WORLD, STAT) IF (STATUS.NE.0) THEN WRITE (*, 80) STATUS 80 FORMAT ('TABX2S ERROR',I2,'.') END IF * Start a new plot. CALL PGBBUF () CALL PGERAS () CALL PGSCI (1) CALL PGSLW (3) CALL PGBOX ('BCNST', 0.0, 0, 'BCNSTV', 0.0, 0) CALL PGMTXT ('T', 0.7, 0.5, 0.5, '-TAB coordinates: ' // : 'linear interpolation / extrapolation in 2-D') * Draw the boundary of the interpolation element in red. CALL PGSCI (2) CALL PGMOVE (-0.5, 0.0) CALL PGDRAW ( 1.5, 0.0) CALL PGMOVE ( 1.0, -0.5) CALL PGDRAW ( 1.0, 1.5) CALL PGMOVE ( 1.5, 1.0) CALL PGDRAW (-0.5, 1.0) CALL PGMOVE ( 0.0, 1.5) CALL PGDRAW ( 0.0, -0.5) * Label the value of the coordinate element in each corner. WRITE (TEXT, '(F3.1)') 0.0 CALL PGTEXT (-0.09, -0.05, TEXT) WRITE (TEXT, '(F4.2)') 0.01*L1 CALL PGTEXT ( 1.02, -0.05, TEXT) WRITE (TEXT, '(F3.1)') 0.01*L2 CALL PGTEXT (-0.13, 1.02, TEXT) WRITE (TEXT, '(F3.1)') 0.01*L3 CALL PGTEXT ( 1.02, 1.02, TEXT) CALL PGSCI (1) * Contour labelling: bottom. V0 = WORLD(2,1,1) V1 = WORLD(2,NP,1) IF (V0.NE.V1) THEN IF (ABS(INT((V1-V0)/0.2)).LT.10) THEN LSTEP = 20 ELSE LSTEP = 40 END IF DO 90 L = -200, 300, LSTEP W = -0.5 + 2.0*(L*0.01 - V0)/(V1 - V0) IF (W.LT.-0.5 .OR. W.GT.1.5) GO TO 90 WRITE (TEXT, '(F4.1)') L*0.01 CALL PGPTXT (W+0.04, -0.56, 0.0, 1.0, TEXT) 90 CONTINUE END IF * Contour labelling: left. V0 = WORLD(2,1,1) V1 = WORLD(2,1,NP) IF (V0.NE.V1) THEN IF (ABS(INT((V1-V0)/0.2)).LT.10) THEN LSTEP = 20 ELSE LSTEP = 40 END IF DO 100 L = -200, 300, LSTEP W = -0.5 + 2.0*(L*0.01 - V0)/(V1 - V0) IF (W.LT.-0.5 .OR. W.GT.1.5) GO TO 100 WRITE (TEXT, '(F4.1)') L*0.01 CALL PGPTXT (-0.52, W-0.02, 0.0, 1.0, TEXT) 100 CONTINUE END IF * Contour labelling: right. V0 = WORLD(2,NP,1) V1 = WORLD(2,NP,NP) IF (V0.NE.V1) THEN IF (ABS(INT((V1-V0)/0.2)).LT.10) THEN LSTEP = 20 ELSE LSTEP = 40 END IF DO 110 L = -200, 300, LSTEP W = -0.5 + 2.0*(L*0.01 - V0)/(V1 - V0) IF (W.LT.-0.5 .OR. W.GT.1.5) GO TO 110 WRITE (TEXT, '(F3.1)') L*0.01 CALL PGPTXT (1.52, W-0.02, 0.0, 0.0, TEXT) 110 CONTINUE END IF * Contour labelling: top. V0 = WORLD(2,1,NP) V1 = WORLD(2,NP,NP) IF (V0.NE.V1) THEN IF (ABS(INT((V1-V0)/0.2)).LT.10) THEN LSTEP = 20 ELSE LSTEP = 40 END IF DO 120 L = -200, 300, LSTEP W = -0.5 + 2.0*(L*0.01 - V0)/(V1 - V0) IF (W.LT.-0.5 .OR. W.GT.1.5) GO TO 120 WRITE (TEXT, '(F3.1)') L*0.01 CALL PGPTXT (W+0.04, 1.52, 0.0, 1.0, TEXT) 120 CONTINUE END IF * Draw contours for the second coordinate element. DO 140 I = 1, NP DO 130 J = 1, NP ARRAY(J,I) = WORLD(2,J,I) 130 CONTINUE 140 CONTINUE CALL PGSLW (2) CALL PGSCI (4) CALL PGCONT (ARRAY, NP, NP, 1, NP, 1, NP, CLEV(-10), 10, : LTM) CALL PGSCI (7) CALL PGCONT (ARRAY, NP, NP, 1, NP, 1, NP, CLEV(0), 1, LTM) CALL PGSCI (5) CALL PGCONT (ARRAY, NP, NP, 1, NP, 1, NP, CLEV(1), 20, LTM) CALL PGEBUF () 150 CONTINUE 160 CONTINUE 170 CONTINUE CALL PGEND () 999 STATUS = TABFREE (TAB) END pywcs-1.12/wcslib/Fortran/test/ttab3.f0000644001153600020070000001444012310355626021712 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: ttab3.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TTAB3 *----------------------------------------------------------------------- * * TTAB3 tests the -TAB routines using PGPLOT for graphical display. It * constructs a table that approximates Bonne's projection and uses it to * draw a graticule. * *----------------------------------------------------------------------- * Set up the lookup table. INTEGER K1, K2, M PARAMETER (M = 2, K1 = 271, K2 = 235) INTEGER K(M), MAP(M) DOUBLE PRECISION CRVAL(M) DATA K /K1, K2/ DATA MAP /0, 1/ DATA CRVAL /135D0, 95D0/ INTEGER CI, I, IK, ILAT, ILNG, IM, J, STAT(K1,K2), STATUS REAL XR(361), YR(361) DOUBLE PRECISION COORD(M,K1,K2), WORLD(M,361), X(K1), XY(M,361), : Y(K2) * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary, done here using equivalences. * Failure to do this may result in mysterious "bus errors". INCLUDE 'prj.inc' INCLUDE 'tab.inc' INTEGER PRJ(PRJLEN), TAB(TABLEN) DOUBLE PRECISION DUMMY1, DUMMY2 EQUIVALENCE (PRJ,DUMMY1), (TAB,DUMMY2) *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing WCSLIB inverse coordinate lookup table ', : 'routines (ttab3.f)',/, : '-----------------------------------------------', : '------------------',/) * PGPLOT initialization. CALL PGBEG (0, '/xwindow', 1, 1) CALL PGVSTD () CALL PGSCH (0.7) CALL PGWNAD (-135.0, 135.0, -95.0, 140.0) CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGSCR (0, 0.00, 0.00, 0.00) CALL PGSCR (1, 1.00, 1.00, 0.00) CALL PGSCR (2, 1.00, 1.00, 1.00) CALL PGSCR (3, 0.50, 0.50, 0.80) CALL PGSCR (4, 0.80, 0.50, 0.50) CALL PGSCR (5, 0.80, 0.80, 0.80) CALL PGSCR (6, 0.50, 0.50, 0.80) CALL PGSCR (7, 0.80, 0.50, 0.50) CALL PGSCR (8, 0.30, 0.50, 0.30) * Set up the lookup table. STATUS = TABPUT (TAB, TAB_FLAG, -1, 0, 0) STATUS = TABINI(M, K, TAB) IF (STATUS.NE.0) THEN WRITE (*, 20) STATUS 20 FORMAT ('TABINI ERROR',I2,'.') GO TO 999 END IF STATUS = TABPUT (TAB, TAB_M, M, 0, 0) DO 40 IM = 1, M STATUS = TABPUT (TAB, TAB_K, K(IM), IM, 0) STATUS = TABPUT (TAB, TAB_MAP, MAP(IM), IM, 0) STATUS = TABPUT (TAB, TAB_CRVAL, CRVAL(IM), IM, 0) DO 30 IK = 1, K(IM) STATUS = TABPUT (TAB, TAB_INDEX, DBLE(IK-1), IM, IK) 30 CONTINUE 40 CONTINUE * Set up the lookup table to approximate Bonne's projection. DO 50 I = 1, K1 X(I) = 136 - I 50 CONTINUE DO 60 J = 1, K2 Y(J) = J - 96 60 CONTINUE STATUS = PRJINI (PRJ) STATUS = PRJPUT (PRJ, PRJ_PV, 35D0, 1) STATUS = BONX2S (PRJ, K1, K2, 1, 2, X, Y, COORD(1,1,1), : COORD(2,1,1), STAT) IK = 1 DO 80 J = 1, K2 DO 70 I = 1, K1 IF (STAT(I,J).NE.0) THEN COORD(1,I,J) = 999D0 COORD(2,I,J) = 999D0 END IF STATUS = TABPUT (TAB, TAB_COORD, COORD(1,I,J), IK, 0) STATUS = TABPUT (TAB, TAB_COORD, COORD(2,I,J), IK+1, 0) IK = IK + 2 70 CONTINUE 80 CONTINUE * Draw meridians. CI = 1 DO 110 ILNG = -180, 180, 15 CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILNG.NE.0) THEN CALL PGSCI (CI) ELSE CALL PGSCI (1) END IF J = 0 DO 90 ILAT = -90, 90 J = J + 1 WORLD(1,J) = DBLE(ILNG) WORLD(2,J) = DBLE(ILAT) 90 CONTINUE * A fudge to account for the singularity at the poles. WORLD(1,1) = 0D0 WORLD(1,181) = 0D0 STATUS = TABS2X (TAB, 181, 2, WORLD, XY, STAT) IK = 0 DO 100 J = 1, 181 IF (STAT(J,1).NE.0) THEN IF (IK.GT.1) CALL PGLINE (K, XR, YR) IK = 0 GO TO 100 END IF IK = IK + 1 XR(IK) = XY(1,J) YR(IK) = XY(2,J) 100 CONTINUE CALL PGLINE (IK, XR, YR) 110 CONTINUE * Draw parallels. CI = 1 DO 140 ILAT = -75, 75, 15 CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILAT.NE.0) THEN CALL PGSCI (CI) ELSE CALL PGSCI (1) END IF J = 0 DO 120 ILNG = -180, 180 J = J + 1 WORLD(1,J) = DBLE(ILNG) WORLD(2,J) = DBLE(ILAT) 120 CONTINUE STATUS = TABS2X (TAB, 361, 2, WORLD, XY, STAT) IK = 0 DO 130 J = 1, 361 IF (STAT(J,1).NE.0) THEN IF (IK.GT.1) CALL PGLINE (IK, XR, YR) IK = 0 GO TO 130 END IF IK = IK + 1 XR(IK) = XY(1,J) YR(IK) = XY(2,J) 130 CONTINUE CALL PGLINE (IK, XR, YR) 140 CONTINUE CALL PGEND () 999 STATUS = TABFREE (TAB) END pywcs-1.12/wcslib/Fortran/test/tunits.f0000644001153600020070000001266112310355626022226 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: tunits.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TUNITS *----------------------------------------------------------------------- * * TUNITS tests WCSULEX, WCSUTRN, and WCSUNITS the FITS units * specification parser, translator and converter. * *----------------------------------------------------------------------- INCLUDE 'wcsunits.inc' LOGICAL INTRCT INTEGER FUNC, I, NC, STATUS DOUBLE PRECISION OFFSET, POWER, SCALE, UNITS(WCSUNITS_NTYPE) CHARACTER HAVE*80, WANT*80 *----------------------------------------------------------------------- INTRCT = ISATTY(5) WRITE (*, 10) 10 FORMAT ('Testing FITS unit specification parser (tunits.f)',/, : '-------------------------------------------------') IF (INTRCT) WRITE (*, 20) 20 FORMAT (/,'To test WCSULEX, enter when prompted with "Unit ', : 'string (want):".') 30 CONTINUE IF (INTRCT) WRITE (*, '(/,A,$)') 'Unit string (have): ' READ (*, '(A)', END=999) HAVE NC = LNBLNK(HAVE) IF (.NOT.INTRCT) WRITE (*, 40) HAVE(:NC) 40 FORMAT (/,'Unit string (have): ',A) STATUS = WCSUTRN(7, HAVE) IF (STATUS.GE.0) THEN NC = LNBLNK(HAVE) WRITE (*, 50) HAVE(:NC) 50 FORMAT (' Translation: ',A,$) IF (STATUS.EQ.0) THEN WRITE (*, '()') ELSE NC = LNBLNK(WCSUNITS_ERRMSG(STATUS)) WRITE (*, 60) WCSUNITS_ERRMSG(STATUS)(:NC) 60 FORMAT (' (WARNING: ',A,')') END IF END IF IF (INTRCT) WRITE (*, '(A,$)') 'Unit string (want): ' READ (*, '(A)', END=999) WANT IF (WANT.NE.' ') THEN NC = LNBLNK(WANT) IF (.NOT.INTRCT) WRITE (*, 70) WANT(:NC) 70 FORMAT ('Unit string (want): ',A) STATUS = WCSUTRN(7, WANT) IF (STATUS.GE.0) THEN NC = LNBLNK(WANT) WRITE (*, 50) WANT(:NC) IF (STATUS.EQ.0) THEN WRITE (*, '()') ELSE NC = LNBLNK(WCSUNITS_ERRMSG(STATUS)) WRITE (*, 60) WCSUNITS_ERRMSG(STATUS)(:NC) END IF END IF WRITE (*, 80) HAVE(:LNBLNK(HAVE)), WANT(:LNBLNK(WANT)) 80 FORMAT ('Conversion: "',A,'" -> "',A,'"') STATUS = WCSUNITS (HAVE, WANT, SCALE, OFFSET, POWER) IF (STATUS.NE.0) THEN NC = LNBLNK(WCSUNITS_ERRMSG(STATUS)) WRITE (*, 90) STATUS, WCSUNITS_ERRMSG(STATUS)(:NC) 90 FORMAT ('WCSUNITS ERROR',I3,': ',A) GO TO 30 END IF IF (POWER.EQ.1D0) THEN WRITE (*, '(A,$)') ' = ' ELSE WRITE (*, '(A,$)') ' = (' END IF IF (SCALE.EQ.1.0) THEN WRITE (*, '(A,$)') 'value' ELSE WRITE (*, '(1PG14.8,A,$)') SCALE, ' * value' END IF IF (OFFSET.NE.0D0) THEN WRITE (*, '(A,1PG14.8,$)') ' + ', OFFSET END IF IF (POWER.EQ.1D0) THEN WRITE (*, '()') ELSE WRITE (*, '(A,1PG12.6)') ')^', POWER END IF ELSE * Parse the unit string. NC = LNBLNK(HAVE) WRITE (*, '(A,A,A)') ' Parsing: "', HAVE(:NC), '"' STATUS = WCSULEX (HAVE, FUNC, SCALE, UNITS) IF (STATUS.NE.0) THEN NC = LNBLNK(WCSUNITS_ERRMSG(STATUS)) WRITE (*, 100) STATUS, WCSUNITS_ERRMSG(STATUS)(:NC) 100 FORMAT ('WCSULEX ERROR',I3,': ',A,'.') GO TO 30 END IF WRITE (*, '(1PG15.8,A)') SCALE, ' *' DO 110 I = 1, WCSUNITS_NTYPE IF (UNITS(I).NE.0.0) THEN NC = LNBLNK(WCSUNITS_TYPES(I)) WRITE (*, '(F11.2,X,A,$)') UNITS(I), : WCSUNITS_TYPES(I)(:NC) IF (WCSUNITS_UNITS(I).NE.' ') THEN NC = LNBLNK(WCSUNITS_UNITS(I)) WRITE (*, '(A,A,A)') ' (', WCSUNITS_UNITS(I)(:NC),')' ELSE WRITE (*, '()') END IF END IF 110 CONTINUE END IF GO TO 30 999 WRITE (*, '()') END pywcs-1.12/wcslib/Fortran/test/twcs.f0000644001153600020070000003466212310355626021665 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: twcs.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TWCS *----------------------------------------------------------------------- * * TWCS1 tests WCSS2P and WCSP2S for closure on an oblique 2-D slice * through a 4-D image with celestial, spectral and logarithmic * coordinate axes. * *----------------------------------------------------------------------- INCLUDE 'cel.inc' INCLUDE 'prj.inc' INCLUDE 'wcs.inc' INCLUDE 'wcserr.inc' INCLUDE 'wcsmath.inc' DOUBLE PRECISION TOL PARAMETER (TOL = 1D-10) INTEGER NELEM PARAMETER (NELEM = 9) INTEGER CHECK_ERROR, ETEST, I, J, K, LAT, LATIDX, LNG, LNGIDX, : NFAIL1, NFAIL2, SPCIDX, STAT(0:360), STATUS, : TEST_ERRORS DOUBLE PRECISION FREQ, IMG(NELEM,0:360), LAT1, LNG1, PHI(0:360), : PIXEL1(NELEM,0:360), PIXEL2(NELEM,0:360), R, RESID, : RESMAX, THETA(0:360), TIME, WORLD1(NELEM,0:360), : WORLD2(NELEM,0:360) * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INTEGER WCS(WCSLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS,DUMMY) * Number of axes. INTEGER N PARAMETER (N = 4) * WCS header parameters. INTEGER NAXIS, NPV, PVI(3), PVM(3) DOUBLE PRECISION CDELT(N), CRPIX(N), CRVAL(N), LATPOLE, LONPOLE, : PC(N,N), PV(3), RESTFRQ, RESTWAV CHARACTER CTYPE(N)*72 COMMON /HEADER/ NAXIS, NPV, CRPIX, PC, CDELT, CRVAL, LONPOLE, : LATPOLE, RESTFRQ, RESTWAV, PVI, PVM, PV COMMON /HEADCH/ CTYPE DATA NAXIS /N/ DATA (CRPIX(J), J=1,N) : /513D0, 0D0, 0D0, 0D0/ DATA ((PC(I,J),J=1,N),I=1,N) : /1.1D0, 0D0, 0D0, 0D0, : 0D0, 1.0D0, 0D0, 0.1D0, : 0D0, 0D0, 1.0D0, 0D0, : 0D0, 0.2D0, 0D0, 1.0D0/ DATA (CDELT(I), I=1,N) : /-9.635265432D-6, 1D0, 0.1D0, -1D0/ DATA (CTYPE(I), I=1,N) : /'WAVE-F2W', 'XLAT-BON', 'TIME-LOG', 'XLON-BON'/ DATA (CRVAL(I), I=1,N) : /0.214982042D0, -30D0, 1D0, 150D0/ DATA LONPOLE /150D0/ DATA LATPOLE /999D0/ DATA RESTFRQ /1.42040575D9/ DATA RESTWAV /0D0/ * Set PVi_m keyvalues for the longitude axis (I = 4). For test * purposes, these are set so that the fiducial native coordinates * are at the native pole, i.e. so that (phi0,theta0) = (0,90), but * without any fiducial offset, i.e. iwith PVi_0a == 0 (by default). DATA NPV /3/ DATA (PVI(K), PVM(K), PV(K), K=1,2) : /4, 1, 0D0, : 4, 2, 90D0/ * PVi_m keyvalues for the latitude axis (I = 2). DATA PVI(3), PVM(3), PV(3) : /2, 1, -30D0/ * For the wcserr tests. COMMON /ERRTST/ ETEST DATA ETEST /0/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing closure of WCSLIB world coordinate ', : 'transformation routines (twcs.f)',/, : '-------------------------------------------', : '--------------------------------') * This routine simulates the actions of a FITS header parser. STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) CALL PARSER (WCS) WRITE (*, 20) TOL 20 FORMAT (/,'Reporting tolerance',1PG8.1,' pixel.') * Get indices. STATUS = WCSGET (WCS, WCS_LNG, LNGIDX) STATUS = WCSGET (WCS, WCS_LAT, LATIDX) STATUS = WCSGET (WCS, WCS_SPEC, SPCIDX) * Initialize non-celestial world coordinates. TIME = 1D0 FREQ = 1.42040595D9 - 180D0 * 62500D0 DO 30 K = 0, 360 WORLD1(1,K) = 0D0 WORLD1(2,K) = 0D0 WORLD1(3,K) = 0D0 WORLD1(4,K) = 0D0 WORLD1(3,K) = TIME TIME = 1.01D0 * TIME WORLD1(SPCIDX,K) = 2.99792458D8 / FREQ FREQ = FREQ + 62500D0 30 CONTINUE NFAIL1 = 0 RESMAX = 0D0 DO 110 LAT = 90, -90, -1 LAT1 = DBLE(LAT) K = 0 DO 40 LNG = -180, 180 LNG1 = DBLE(LNG) WORLD1(LNGIDX,K) = LNG1 WORLD1(LATIDX,K) = LAT1 K = K + 1 40 CONTINUE STATUS = WCSS2P (WCS, 361, NELEM, WORLD1, PHI, THETA, IMG, : PIXEL1, STAT) IF (STATUS.NE.0) THEN WRITE (*, 50) STATUS, LAT1 50 FORMAT (3X,'WCSS2P(1) ERROR',I3,' (LAT1 =',F20.15, ')') GO TO 110 END IF STATUS = WCSP2S (WCS, 361, NELEM, PIXEL1, IMG, PHI, THETA, : WORLD2, STAT) IF (STATUS.NE.0) THEN WRITE (*, 60) STATUS, LAT1 60 FORMAT (3X,'WCSP2S ERROR',I3,' (LAT1 =',F20.15, ')') GO TO 110 END IF STATUS = WCSS2P (WCS, 361, NELEM, WORLD2, PHI, THETA, IMG, : PIXEL2, STAT) IF (STATUS.NE.0) THEN WRITE (*, 70) STATUS, LAT1 70 FORMAT (3X,'WCSS2P(2) ERROR',I3,' (LAT1 =',F20.15, ')') GO TO 110 END IF DO 100 K = 0, 360 RESID = 0D0 DO 80 I = 1, NAXIS R = PIXEL2(I,K) - PIXEL1(I,K) RESID = RESID + R*R 80 CONTINUE RESID = SQRT(RESID) IF (RESID.GT.RESMAX) RESMAX = RESID IF (RESID.GT.TOL) THEN NFAIL1 = NFAIL1 + 1 WRITE (*, 90) (WORLD1(I,K), I=1,NAXIS), : (PIXEL1(I,K), I=1,NAXIS), : (WORLD2(I,K), I=1,NAXIS), : (PIXEL2(I,K), I=1,NAXIS) 90 FORMAT (/,'Closure error:',/, : 'world1:',4F18.12,/, : 'pixel1:',4F18.12,/, : 'world2:',4F18.12,/, : 'pixel2:',4F18.12) END IF LNG1 = LNG1 + 1D0 100 CONTINUE 110 CONTINUE WRITE (*, 120) RESMAX 120 FORMAT ('WCSP2S/WCSS2P: Maximum closure residual =',1P,G8.1, : ' pixel.') * Test WCSERR. WRITE (*, 130) 130 FORMAT (//,'IGNORE messages marked with ''OK'', they test ', : 'WCSERR: ') STATUS = WCSERR_ENABLE(1) * Test 1. STATUS = WCSPUT (WCS, WCS_PV, UNDEFINED, PVI(3), PVM(3)) STATUS = WCSSET (WCS) NFAIL2 = CHECK_ERROR (WCS, STATUS, WCSERR_BAD_PARAM, : 'Invalid parameter value') NFAIL2 = NFAIL2 + TEST_ERRORS() IF (NFAIL1.NE.0 .OR. NFAIL2.NE.0) THEN IF (NFAIL1.NE.0) THEN WRITE (*, 140) NFAIL1 140 FORMAT (/,'FAIL:',I5,' closure residuals exceed reporting ', : 'tolerance.') END IF IF (NFAIL2.NE.0) THEN WRITE (*, 150) NFAIL2 150 FORMAT ('FAIL:',I5,' error messages differ from that ', : 'expected.') END IF ELSE WRITE (*, 160) 160 FORMAT (/,'PASS: All closure residuals are within reporting ', : 'tolerance.',/,'PASS: All error messages reported as ', : 'expected.') END IF * Clean up. STATUS = WCSFREE(WCS) END *----------------------------------------------------------------------- SUBROUTINE PARSER (WCS) *----------------------------------------------------------------------- * In practice a parser would read the FITS header until it encountered * the NAXIS keyword which must occur near the start, before any of the * WCS keywords. It would then use WCSINI to allocate memory for arrays * in the WCSPRM "data structure" and set default values. * * In this simulation the header keyvalues are set in the main program in * variables passed in COMMON. *----------------------------------------------------------------------- * Number of axes. INTEGER N PARAMETER (N = 4) INTEGER I, J, K, NAXIS, NPV, PVI(3), PVM(3), STATUS, WCS(*) DOUBLE PRECISION CDELT(N), CRPIX(N), CRVAL(N), LATPOLE, LONPOLE, : PC(N,N), PV(3), RESTFRQ, RESTWAV CHARACTER CTYPE(N)*72 INCLUDE 'wcs.inc' COMMON /HEADER/ NAXIS, NPV, CRPIX, PC, CDELT, CRVAL, LONPOLE, : LATPOLE, RESTFRQ, RESTWAV, PVI, PVM, PV COMMON /HEADCH/ CTYPE *----------------------------------------------------------------------- STATUS = WCSINI (NAXIS, WCS) DO 20 I = 1, NAXIS STATUS = WCSPUT (WCS, WCS_CRPIX, CRPIX(I), I, 0) DO 10 J = 1, NAXIS STATUS = WCSPUT (WCS, WCS_PC, PC(I,J), I, J) 10 CONTINUE STATUS = WCSPUT (WCS, WCS_CDELT, CDELT(I), I, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(I), I, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, CRVAL(I), I, 0) 20 CONTINUE STATUS = WCSPUT (WCS, WCS_LONPOLE, LONPOLE, 0, 0) STATUS = WCSPUT (WCS, WCS_LATPOLE, LATPOLE, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTFRQ, RESTFRQ, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTWAV, RESTWAV, 0, 0) DO 30 K = 1, NPV STATUS = WCSPUT (WCS, WCS_PV, PV(K), PVI(K), PVM(K)) 30 CONTINUE * Extract information from the FITS header. STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN WRITE (*, 40) STATUS 40 FORMAT ('WCSSET ERROR',I3) END IF END *----------------------------------------------------------------------- INTEGER FUNCTION TEST_ERRORS() *----------------------------------------------------------------------- INTEGER CHECK_ERROR, ETEST, NFAIL, STATUS * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcs.inc' INTEGER WCS(WCSLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS,DUMMY) COMMON /ERRTST/ ETEST *----------------------------------------------------------------------- NFAIL = 0 * Test 2. STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) STATUS = WCSINI (-32, WCS) NFAIL = NFAIL + CHECK_ERROR (WCS, STATUS, WCSERR_MEMORY, : 'naxis must be positive (got -32)') * Test 3. STATUS = WCSPUT (WCS, WCS_FLAG, 0, 0, 0) STATUS = WCSINI (2, WCS) NFAIL = NFAIL + CHECK_ERROR (WCS, STATUS, WCSERR_SUCCESS, ' ') * Test 4. STATUS = WCSPUT (WCS, WCS_CTYPE, 'CUBEFACE', 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, 'CUBEFACE', 2, 0) STATUS = WCSSET (WCS) NFAIL = NFAIL + CHECK_ERROR (WCS, STATUS, WCSERR_BAD_CTYPE, : 'Multiple CUBEFACE axes (in CTYPE1 and CTYPE2)') * Test 5. STATUS = WCSPUT (WCS, WCS_FLAG, 0, 0, 0) STATUS = WCSINI (2, WCS) STATUS = WCSPUT (WCS, WCS_CTYPE, 'RA---FOO', 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, 'DEC--BAR', 2, 0) STATUS = WCSSET (WCS) NFAIL = NFAIL + CHECK_ERROR (WCS, STATUS, WCSERR_BAD_CTYPE, : 'Unrecognized projection code (FOO in CTYPE1)') * Test 6. STATUS = WCSPUT (WCS, WCS_FLAG, 0, 0, 0) STATUS = WCSINI (2, WCS) STATUS = WCSPUT (WCS, WCS_CTYPE, 'RA---TAN', 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, 'FREQ-LOG', 2, 0) STATUS = WCSSET (WCS) NFAIL = NFAIL + CHECK_ERROR (WCS, STATUS, WCSERR_BAD_CTYPE, : 'Unmatched celestial axes') STATUS = WCSFREE(WCS) TEST_ERRORS = NFAIL END *----------------------------------------------------------------------- INTEGER FUNCTION CHECK_ERROR(WCS, STATUS, EXSTATUS, EXMSG) *----------------------------------------------------------------------- INCLUDE 'wcs.inc' INCLUDE 'wcserr.inc' INTEGER EXSTATUS, ILEN, ISTAT, ETEST, STATUS, WCS(WCSLEN) CHARACTER ERRMSG*(WCSERR_MSG_LENGTH), EXMSG*(*) * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary. As a dummy argument, WCS should * already be aligned. WCSERR is aligned here using an equivalence. * Failure to do this may result in mysterious "bus errors". INTEGER WCSERR(ERRLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCSERR,DUMMY) COMMON /ERRTST/ ETEST *----------------------------------------------------------------------- IF (STATUS.NE.0) THEN ISTAT = WCSGET (WCS, WCS_ERR, WCSERR) ISTAT = WCSERR_GET (WCSERR, WCSERR_MSG, ERRMSG) ELSE ERRMSG = ' ' END IF ETEST = ETEST + 1 WRITE (*, 10) ETEST 10 FORMAT (/,'Test ',I2,'...') IF (STATUS.EQ.EXSTATUS .AND. ERRMSG.EQ.EXMSG) THEN CALL FLUSH(6) ISTAT = WCSPERR (WCS, 'OK: '//CHAR(0)) WRITE (*, *) '...succeeded.' CHECK_ERROR = 0 ELSE WRITE (*, 20) EXSTATUS, EXMSG(:ILEN(EXMSG)) 20 FORMAT ('Expected error ',I2,': ''',A,''', got') CALL FLUSH(6) ISTAT = WCSPERR (WCS, CHAR(0)) WRITE (*, *) '...failed.' CHECK_ERROR = 1 END IF END *----------------------------------------------------------------------- INTEGER FUNCTION ILEN(STRING) *----------------------------------------------------------------------- CHARACTER STRING*(*) *----------------------------------------------------------------------- DO 10 ILEN = LEN(STRING), 1, -1 IF (STRING(ILEN:ILEN).NE. ' ') RETURN 10 CONTINUE ILEN = 0 END pywcs-1.12/wcslib/Fortran/test/twcsfix.f0000644001153600020070000001553112310355626022366 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: twcsfix.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TWCSFIX *----------------------------------------------------------------------- * * TWCSFIX tests the translation routines for non-standard WCS keyvalues, * the WCSFIX suite, and the spectral coordinate translation routine * WCSPTR. * *----------------------------------------------------------------------- DOUBLE PRECISION TOL PARAMETER (TOL = 1D-10) * CUNITia is set to arcsec below as an additional test. DOUBLE PRECISION DEC, RA PARAMETER (RA = 265.62209470900D0 * 3600D0) PARAMETER (DEC = -28.98849996030D0 * 3600D0) * Number of axes. INTEGER N PARAMETER (N = 3) INTEGER I, J, NAXIS DOUBLE PRECISION CDELT(N), CRPIX(N), CRVAL(N), PC(N,N), RESTFRQ, : RESTWAV CHARACTER CTYPE(N)*72, CUNIT(N)*72, DATEOBS*72 COMMON /HEADER/ CRPIX, PC, CDELT, CRVAL, RESTFRQ, RESTWAV, NAXIS COMMON /HEADCH/ CTYPE, CUNIT, DATEOBS * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcs.inc' INCLUDE 'wcsfix.inc' INTEGER STAT(WCSFIX_NWCS), STATUS CHARACTER CTYPES*8 INTEGER WCS(WCSLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS,DUMMY) DATA NAXIS /N/ DATA (CRPIX(J), J=1,N) : /90D0, 90D0, 1D0/ DATA ((PC(I,J),J=1,N),I=1,N) : /1D0, 0D0, 0D0, : 0D0, 1D0, 0D0, : 0D0, 0D0, 1D0/ DATA (CDELT(I), I=1,N) : /-1D0, 1D0, 19.68717093222D0/ DATA (CUNIT(I), I=1,N) : /'ARCSEC', 'ARCSEC', 'KM/SEC'/ DATA (CTYPE(I), I=1,N) : /'RA---NCP', 'DEC--NCP', 'FELO-HEL'/ DATA (CRVAL(I), I=1,N) : /RA, DEC, 5569.27104D0/ DATA RESTFRQ /1.42040575D9/ DATA RESTWAV /0D0/ * N.B. non-standard, corresponding to MJD 35884.04861111 DATA DATEOBS /'1957/02/15 01:10:00'/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing WCSLIB translator for non-standard usage ', : '(twcsfix.f)',/, : '-------------------------------------------------', : '-----------',/) * This routine simulates the actions of a FITS header parser. STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) CALL PARSER (WCS) * Fix non-standard WCS keyvalues. STATUS = WCSFIX (7, 0, WCS, STAT) WRITE (*, 20) (STAT(I), I=1,WCSFIX_NWCS) 20 FORMAT ('WCSFIX status returns: (',I2,5(',',I2),')',/) IF (STATUS.NE.0) THEN WRITE (*, 30) STATUS 30 FORMAT ('WCSFIX ERROR',I2,'.') GO TO 999 END IF * Extract information from the FITS header. STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN WRITE (*, 40) STATUS 40 FORMAT (/,'WCSSET ERROR',I2,'.') END IF CALL FLUSH(6) STATUS = WCSPRT (WCS) WRITE (*, 50) 50 FORMAT (/,'------------------------------------', : '------------------------------------') * Should now have a 'VOPT-F2W' axis, translate it to frequency. CTYPES = 'FREQ-???' I = -1 STATUS = WCSSPTR (WCS, I, CTYPES) IF (STATUS.NE.0) THEN WRITE (*, 60) STATUS 60 FORMAT ('WCSPTR ERROR',I2,'.') GO TO 999 END IF STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN WRITE (*, 70) STATUS 70 FORMAT ('WCSSET ERROR',I2,'.') GO TO 999 END IF CALL FLUSH(6) STATUS = WCSPRT (WCS) STATUS = WCSFREE (WCS) 999 CONTINUE END *----------------------------------------------------------------------- SUBROUTINE PARSER (WCS) *----------------------------------------------------------------------- * In practice a parser would read the FITS header until it encountered * the NAXIS keyword which must occur near the start, before any of the * WCS keywords. It would then use WCSINI to allocate memory for arrays * in the WCSPRM "data structure" and set default values. * * In this simulation the header keyvalues are set in the main program in * variables passed in COMMON. *----------------------------------------------------------------------- * Number of axes. INTEGER N PARAMETER (N = 3) INTEGER I, J, NAXIS, STATUS, WCS(*) DOUBLE PRECISION CDELT(N), CRPIX(N), CRVAL(N), : PC(N,N), RESTFRQ, RESTWAV CHARACTER CTYPE(N)*72, CUNIT(N)*72, DATEOBS*72 COMMON /HEADER/ CRPIX, PC, CDELT, CRVAL, RESTFRQ, RESTWAV, NAXIS COMMON /HEADCH/ CTYPE, CUNIT, DATEOBS INCLUDE 'wcsunits.inc' INCLUDE 'wcs.inc' *----------------------------------------------------------------------- STATUS = WCSNPV (2) STATUS = WCSINI (NAXIS, WCS) DO 20 I = 1, NAXIS STATUS = WCSPUT (WCS, WCS_CRPIX, CRPIX(I), I, 0) DO 10 J = 1, NAXIS STATUS = WCSPUT (WCS, WCS_PC, PC(I,J), I, J) 10 CONTINUE STATUS = WCSPUT (WCS, WCS_CDELT, CDELT(I), I, 0) STATUS = WCSPUT (WCS, WCS_CUNIT, CUNIT(I), I, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(I), I, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, CRVAL(I), I, 0) 20 CONTINUE STATUS = WCSPUT (WCS, WCS_RESTFRQ, RESTFRQ, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTWAV, RESTWAV, 0, 0) STATUS = WCSPUT (WCS, WCS_NPV, 1, 0, 0) STATUS = WCSPUT (WCS, WCS_PV, -1D0, -1, -1) STATUS = WCSPUT (WCS, WCS_DATEOBS, DATEOBS, 0, 0) RETURN END pywcs-1.12/wcslib/Fortran/test/twcsmix.f0000644001153600020070000006470512310355626022404 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: twcsmix.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TWCS2 *----------------------------------------------------------------------- * * TWCS2 tests WCSMIX for closure on the 1 degree celestial graticule for * a number of selected projections. Points with good solutions are * marked with a white dot on a graphical display of the projection while * bad solutions are flagged with a red circle. * *----------------------------------------------------------------------- * Number of axes. INTEGER N PARAMETER (N = 4) INTEGER I, J, K, NAXIS, NPV, PVI(4), PVM(4) DOUBLE PRECISION CDELT(N), CRPIX(N), CRVAL(N), LATPOLE, LONPOLE, : PC(N,N), PV(4), RESTFRQ, RESTWAV CHARACTER CTYPE(N)*72 DOUBLE PRECISION TOL PARAMETER (TOL = 1D-9) COMMON /HEADER/ NAXIS, NPV, CRPIX, PC, CDELT, CRVAL, LONPOLE, : LATPOLE, RESTFRQ, RESTWAV, PVI, PVM, PV COMMON /HEADCH/ CTYPE DATA NAXIS /N/ DATA (CRPIX(J), J=1,N) : /513D0, 0D0, 0D0, 0D0/ DATA ((PC(I,J),J=1,N),I=1,N) : /1.1D0, 0D0, 0D0, 0D0, : 0D0, 1.0D0, 0D0, 0.1D0, : 0D0, 0D0, 1.0D0, 0D0, : 0D0, 0.2D0, 0D0, 1.0D0/ DATA (CDELT(I), I=1,N) : /-9.635265432D-6, 1D0, 1D0, -1D0/ DATA (CTYPE(I), I=1,N) : /'WAVE-F2W', 'XLAT-xxx ', 'TIME ', 'XLON-xxx '/ DATA (CRVAL(I), I=1,N) : /0.214982042D0, -30D0, -2D3, 150D0/ DATA LONPOLE /150D0/ DATA LATPOLE /999D0/ DATA RESTFRQ /1.42040575D9/ DATA RESTWAV /0D0/ * Set PVi_m keyvalues for the longitude axis (I = 4) so that the * fiducial native coordinates are at the native pole, i.e. * (phi0,theta0) = (0,90), but without any fiducial offset. We do * this as a test, and also so that all projections will be * exercised with the same obliquity parameters. DATA (PVI(K), PVM(K), PV(K), K=1,2) : /4, 1, 0D0, : 4, 2, 90D0/ * PVi_m keyvalues for the latitude axis (I = 2). Value may be reset * below. DATA (PVI(K), PVM(K), PV(K), K=3,4) : /2, 1, 0D0, : 2, 2, 0D0/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing WCSLIB wcsmix routine (twcsmix.f)',/, : '-----------------------------------------') * PGPLOT initialization. CALL PGBEG (0, '/xwindow', 1, 1) * Define pen colours. CALL PGSCR (0, 0.00, 0.00, 0.00) CALL PGSCR (1, 1.00, 1.00, 0.00) CALL PGSCR (2, 1.00, 1.00, 1.00) CALL PGSCR (3, 0.50, 0.50, 0.80) CALL PGSCR (4, 0.80, 0.50, 0.50) CALL PGSCR (5, 0.80, 0.80, 0.80) CALL PGSCR (6, 0.50, 0.50, 0.80) CALL PGSCR (7, 0.80, 0.50, 0.50) CALL PGSCR (8, 0.30, 0.50, 0.30) CALL PGSCR (9, 1.00, 0.75, 0.00) * ARC: zenithal/azimuthal equidistant. CTYPE(2)(6:8) = 'ARC' CTYPE(4)(6:8) = 'ARC' NPV = 2 CALL MIXEX (TOL, -190.0, 190.0, -190.0, 190.0) * ZEA: zenithal/azimuthal equal area. CTYPE(2)(6:8) = 'ZEA' CTYPE(4)(6:8) = 'ZEA' NPV = 2 CALL MIXEX (TOL, -120.0, 120.0, -120.0, 120.0) * CYP: cylindrical perspective. CTYPE(2)(6:8) = 'CYP' CTYPE(4)(6:8) = 'CYP' NPV = 4 PV(3) = 3D0 PV(4) = 0.8D0 CALL MIXEX (TOL, -170.0, 170.0, -170.0, 170.0) * CEA: cylindrical equal area. CTYPE(2)(6:8) = 'CEA' CTYPE(4)(6:8) = 'CEA' NPV = 3 PV(3) = 0.75D0 CALL MIXEX (TOL, -200.0, 200.0, -200.0, 200.0) * CAR: plate carree. CTYPE(2)(6:8) = 'CAR' CTYPE(4)(6:8) = 'CAR' NPV = 2 CALL MIXEX (TOL, -210.0, 210.0, -210.0, 210.0) * SFL: Sanson-Flamsteed. CTYPE(2)(6:8) = 'SFL' CTYPE(4)(6:8) = 'SFL' NPV = 2 CALL MIXEX (TOL, -190.0, 190.0, -190.0, 190.0) * PAR: parabolic. CTYPE(2)(6:8) = 'PAR' CTYPE(4)(6:8) = 'PAR' NPV = 2 CALL MIXEX (TOL, -190.0, 190.0, -190.0, 190.0) * MOL: Mollweide's projection. CTYPE(2)(6:8) = 'MOL' CTYPE(4)(6:8) = 'MOL' NPV = 2 CALL MIXEX (TOL, -170.0, 170.0, -170.0, 170.0) * AIT: Hammer-Aitoff. CTYPE(2)(6:8) = 'AIT' CTYPE(4)(6:8) = 'AIT' NPV = 2 CALL MIXEX (TOL, -170.0, 170.0, -170.0, 170.0) * COE: conic equal area. CTYPE(2)(6:8) = 'COE' CTYPE(4)(6:8) = 'COE' NPV = 4 PV(3) = 60D0 PV(4) = 15D0 CALL MIXEX (TOL, -140.0, 140.0, -120.0, 160.0) * COD: conic equidistant. CTYPE(2)(6:8) = 'COD' CTYPE(4)(6:8) = 'COD' NPV = 4 PV(3) = 60D0 PV(4) = 15D0 CALL MIXEX (TOL, -200.0, 200.0, -180.0, 220.0) * BON: Bonne's projection. CTYPE(2)(6:8) = 'BON' CTYPE(4)(6:8) = 'BON' NPV = 3 PV(3) = 30D0 CALL MIXEX (TOL, -160.0, 160.0, -160.0, 160.0) * PCO: polyconic. CTYPE(2)(6:8) = 'PCO' CTYPE(4)(6:8) = 'PCO' NPV = 2 CALL MIXEX (TOL, -190.0, 190.0, -190.0, 190.0) * TSC: tangential spherical cube. CTYPE(2)(6:8) = 'TSC' CTYPE(4)(6:8) = 'TSC' NPV = 2 CALL MIXEX (TOL, -340.0, 80.0, -210.0, 210.0) * QSC: quadrilateralized spherical cube. CTYPE(2)(6:8) = 'QSC' CTYPE(4)(6:8) = 'QSC' NPV = 2 CALL MIXEX (TOL, -340.0, 80.0, -210.0, 210.0) CALL PGEND () END *----------------------------------------------------------------------- SUBROUTINE MIXEX (TOL, IMIN, IMAX, JMIN, JMAX) *----------------------------------------------------------------------- * MIXEX tests WCSMIX. * * Given: * TOL D Reporting tolerance, degrees. *----------------------------------------------------------------------- INTEGER DOID, ILAT, ILNG, LATIDX, LNGIDX, SPCIDX, STAT, STATUS REAL IMAX, IMIN, IPT(1), JMAX, JMIN, JPT(1) DOUBLE PRECISION IMG(4), LAT1, LATSPN(2), LNGSPN(2), LNG1, PHI, : PIX1(4), PIX2(4), PIX3(4), PIXLAT, PIXLNG, THETA, TOL, : WORLD(4) CHARACTER PCODE*3 * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary, done here using equivalences. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcs.inc' INCLUDE 'cel.inc' INCLUDE 'prj.inc' INTEGER CEL(CELLEN), PRJ(PRJLEN), WCS(WCSLEN) DOUBLE PRECISION DUMMY1, DUMMY2, DUMMY3 EQUIVALENCE (CEL,DUMMY1), (PRJ,DUMMY2), (WCS,DUMMY3) *----------------------------------------------------------------------- * This routine simulates the actions of a FITS header parser. STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) CALL PARSER (WCS) * Draw the coordinate graticule. CALL GRDPLT(WCS, IMIN, IMAX, JMIN, JMAX) STATUS = WCSGET (WCS, WCS_CEL, CEL) STATUS = CELGET (CEL, CEL_PRJ, PRJ) STATUS = PRJGET (PRJ, PRJ_CODE, PCODE) WRITE (*, 10) PCODE, TOL 10 FORMAT ('Testing ',A,'; reporting tolerance',1PG8.1,' deg.') STATUS = WCSGET (WCS, WCS_LNG, LNGIDX) STATUS = WCSGET (WCS, WCS_LAT, LATIDX) STATUS = WCSGET (WCS, WCS_SPEC, SPCIDX) WORLD(1) = 0D0 WORLD(2) = 0D0 WORLD(3) = 0D0 WORLD(4) = 0D0 WORLD(SPCIDX) = 2.99792458D8 / 1.42040595D9 DO 80 ILAT = 90, -90, -1 LAT1 = DBLE(ILAT) DO 70 ILNG = -180, 180, 15 LNG1 = DBLE(ILNG) WORLD(LNGIDX) = LNG1 WORLD(LATIDX) = LAT1 STATUS = WCSS2P (WCS, 1, 4, WORLD, PHI, THETA, IMG, PIX1, : STAT) IF (STATUS.NE.0) THEN WRITE (*, 20) PCODE, LNG1, LAT1, STATUS 20 FORMAT (A3,': LNG1 =',F20.15,' LAT1 =',F20.15, : ' ERROR',I3) GO TO 70 END IF PIXLNG = PIX1(LNGIDX) PIXLAT = PIX1(LATIDX) IPT(1) = PIXLNG JPT(1) = PIXLAT CALL PGPT (1, IPT, JPT, -1) LNGSPN(1) = LNG1 - 9.3D0 IF (LNGSPN(1).LT.-180D0) LNGSPN(1) = -180D0 LNGSPN(2) = LNG1 + 4.1D0 IF (LNGSPN(2).GT. 180D0) LNGSPN(2) = 180D0 LATSPN(1) = LAT1 - 3.7D0 IF (LATSPN(1).LT. -90D0) LATSPN(1) = -90D0 LATSPN(2) = LAT1 + 7.2D0 IF (LATSPN(2).GT. 90D0) LATSPN(2) = 90D0 DOID = 1 PIX2(LNGIDX) = PIXLNG STATUS = WCSMIX (WCS, LNGIDX, 1, LATSPN, 1D0, 0, WORLD, : PHI, THETA, IMG, PIX2) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' A: WCSMIX ERROR', STATUS ELSE STATUS = WCSS2P (WCS, 1, 0, WORLD, PHI, THETA, IMG, PIX3, : STAT) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' A: WCSS2P ERROR', STATUS ELSE IF (ABS(PIX3(LNGIDX)-PIXLNG).GT.TOL .AND. : (ABS(WORLD(LATIDX)- LAT1).GT.TOL .OR. : ABS(PIX2(LATIDX)-PIXLAT).GT.TOL)) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, 30) WORLD(LNGIDX), WORLD(LATIDX), PHI, : THETA, PIX2(LNGIDX), PIX2(LATIDX) 30 FORMAT (' A: (LNG2) =',F20.15,' LAT2 =',F20.15,/, : ' PHI =',F20.15,' THETA =',F20.15,/, : ' (I2) =',F20.15,' J2 =',F20.15) END IF END IF PIX2(LATIDX) = PIXLAT STATUS = WCSMIX (WCS, LATIDX, 1, LATSPN, 1D0, 0, WORLD, : PHI, THETA, IMG, PIX2) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' B: WCSMIX ERROR', STATUS ELSE STATUS = WCSS2P (WCS, 1, 0, WORLD, PHI, THETA, IMG, PIX3, : STAT) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' B: WCSS2P ERROR', STATUS ELSE IF (ABS(PIX3(LATIDX)-PIXLAT).GT.TOL .AND. : (ABS(WORLD(LATIDX)- LAT1).GT.TOL .OR. : ABS(PIX2(LNGIDX)-PIXLNG).GT.TOL)) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, 40) WORLD(LNGIDX), WORLD(LATIDX), PHI, : THETA, PIX2(LNGIDX), PIX2(LATIDX) 40 FORMAT (' B: (LNG2) =',F20.15,' LAT2 =',F20.15,/, : ' PHI =',F20.15,' THETA =',F20.15,/, : ' I2 =',F20.15,' (J2) =',F20.15) END IF END IF WORLD(LATIDX) = LAT1 PIX2(LNGIDX) = PIXLNG STATUS = WCSMIX (WCS, LNGIDX, 2, LNGSPN, 1D0, 0, WORLD, : PHI, THETA, IMG, PIX2) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' C: WCSMIX ERROR', STATUS ELSE STATUS = WCSS2P (WCS, 1, 0, WORLD, PHI, THETA, IMG, PIX3, : STAT) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' C: WCSS2P ERROR', STATUS ELSE IF (ABS(PIX3(LNGIDX)-PIXLNG).GT.TOL .AND. : (ABS(WORLD(LNGIDX)- LNG1).GT.TOL .OR. : ABS(PIX2(LATIDX)-PIXLAT).GT.TOL)) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, 50) WORLD(LNGIDX), WORLD(LATIDX), PHI, : THETA, PIX2(LNGIDX), PIX2(LATIDX) 50 FORMAT (' C: LNG2 =',F20.15,' (LAT2) =',F20.15,/, : ' PHI =',F20.15,' THETA =',F20.15,/, : ' (I2) =',F20.15,' J2 =',F20.15) END IF END IF PIX2(LATIDX) = PIXLAT STATUS = WCSMIX (WCS, LATIDX, 2, LNGSPN, 1D0, 0, WORLD, : PHI, THETA, IMG, PIX2) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' D: WCSMIX ERROR', STATUS ELSE STATUS = WCSS2P (WCS, 1, 0, WORLD, PHI, THETA, IMG, PIX3, : STAT) IF (STATUS.NE.0) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, '(A,I2)') ' D: WCSS2P ERROR', STATUS ELSE IF (ABS(PIX3(LATIDX)-PIXLAT).GT.TOL .AND. : (ABS(WORLD(LNGIDX)- LNG1).GT.TOL .OR. : ABS(PIX2(LNGIDX)-PIXLNG).GT.TOL)) THEN CALL ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) WRITE (*, 60) WORLD(LNGIDX), WORLD(LATIDX), PHI, : THETA, PIX2(LNGIDX), PIX2(LATIDX) 60 FORMAT (' D: LNG2 =',F20.15,' (LAT2) =',F20.15,/, : ' PHI =',F20.15,' THETA =',F20.15,/, : ' I2 =',F20.15,' (J2) =',F20.15) END IF END IF 70 CONTINUE 80 CONTINUE STATUS = WCSFREE (WCS) RETURN END *----------------------------------------------------------------------- SUBROUTINE ID (WCS, DOID, LNG1, LAT1, PIXLNG, PIXLAT) *----------------------------------------------------------------------- INTEGER DOID, STATUS REAL IPT(1), JPT(1) DOUBLE PRECISION EULER(5), LNG1, LAT1, PHI, PIXLAT, PIXLNG, THETA CHARACTER PCODE*3 * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary. As a dummy argument, WCS should * already be aligned. The others are aligned here using * equivalences. Failure to do this may result in mysterious "bus * errors". INCLUDE 'wcs.inc' INCLUDE 'cel.inc' INCLUDE 'prj.inc' INTEGER CEL(CELLEN), PRJ(PRJLEN), WCS(WCSLEN) DOUBLE PRECISION DUMMY1, DUMMY2 EQUIVALENCE (CEL,DUMMY1), (PRJ,DUMMY2) *----------------------------------------------------------------------- IF (DOID.NE.0) THEN * Compute native coordinates. STATUS = WCSGET (WCS, WCS_CEL, CEL) STATUS = CELGET (CEL, CEL_EULER, EULER) CALL SPHS2X (EULER, 1, 1, 1, 1, LNG1, LAT1, PHI, THETA) STATUS = CELGET (CEL, CEL_PRJ, PRJ) STATUS = PRJGET (PRJ, PRJ_CODE, PCODE) WRITE (*, 10) PCODE, LNG1, LAT1, PHI, THETA, PIXLNG, PIXLAT 10 FORMAT (/,A3,': LNG1 =',F20.15,' LAT1 =',F20.15,/, : ' PHI =',F20.15,' THETA =',F20.15,/, : ' I1 =',F20.15,' J1 =',F20.15) DOID = 0 CALL PGSCI (9) IPT(1) = PIXLNG JPT(1) = PIXLAT CALL PGPT (1, IPT, JPT, 21) CALL PGSCI (2) END IF RETURN END *----------------------------------------------------------------------- SUBROUTINE GRDPLT (WCS, IMIN, IMAX, JMIN, JMAX) *----------------------------------------------------------------------- * Number of axes. INTEGER N, NELEM PARAMETER (N = 4, NELEM = 9) LOGICAL CUBIC INTEGER CATEG, CI, ILAT, ILNG, J, K, LATIDX, LNGIDX, SPCIDX, : STAT(0:360), STATUS REAL IMAX, IMIN, JMAX, JMIN, IR(0:1023), JR(0:1023) DOUBLE PRECISION FREQ, IMG(NELEM,0:360), LAT, LNG, PHI(0:360), : PIX(NELEM,0:360), REF(4), STEP, THETA(0:360), W(10), : WORLD(NELEM,0:360) CHARACTER PCODE*3, TEXT*80 * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary. As a dummy argument, WCS should * already be aligned. The others are aligned here using * equivalences. Failure to do this may result in mysterious "bus * errors". INCLUDE 'wcs.inc' INCLUDE 'cel.inc' INCLUDE 'prj.inc' INCLUDE 'lin.inc' INTEGER CEL(CELLEN), LIN(LINLEN), PRJ(PRJLEN), WCS(WCSLEN) INTEGER NATIVE(WCSLEN) DOUBLE PRECISION DUMMY1, DUMMY2, DUMMY3, DUMMY4 EQUIVALENCE (CEL,DUMMY1), (LIN,DUMMY2), (PRJ,DUMMY3), : (NATIVE,DUMMY4) *----------------------------------------------------------------------- * Initialize non-celestial world coordinates. STATUS = WCSGET (WCS, WCS_LNG, LNGIDX) STATUS = WCSGET (WCS, WCS_LAT, LATIDX) STATUS = WCSGET (WCS, WCS_SPEC, SPCIDX) FREQ = 1.42040595D9 - 180D0 * 62500D0 DO 10 J = 0, 360 WORLD(1,J) = 0D0 WORLD(2,J) = 0D0 WORLD(3,J) = 0D0 WORLD(4,J) = 0D0 WORLD(SPCIDX,J) = 2.99792458D8 / FREQ FREQ = FREQ + 62500D0 10 CONTINUE * Define PGPLOT viewport. CALL PGENV (IMIN, IMAX, JMIN, JMAX, 1, -2) STATUS = WCSGET (WCS, WCS_CEL, CEL) STATUS = CELGET (CEL, CEL_PRJ, PRJ) STATUS = PRJGET (PRJ, PRJ_CATEGORY, CATEG) CUBIC = CATEG.EQ.7 IF (CUBIC) THEN * Some sort of quad-cube projection. CALL PGSCI (8) * Draw the map boundary. DO 20 J = 0, 8 IMG(1,J) = 0D0 IMG(2,J) = 0D0 IMG(3,J) = 0D0 IMG(4,J) = 0D0 20 CONTINUE STATUS = PRJGET (PRJ, PRJ_W, W) IMG(LNGIDX,0) = -W(1) IMG(LATIDX,0) = W(1) IMG(LNGIDX,1) = -W(1) IMG(LATIDX,1) = W(1)*3D0 IMG(LNGIDX,2) = W(1) IMG(LATIDX,2) = W(1)*3D0 IMG(LNGIDX,3) = W(1) IMG(LATIDX,3) = -W(1)*3D0 IMG(LNGIDX,4) = -W(1) IMG(LATIDX,4) = -W(1)*3D0 IMG(LNGIDX,5) = -W(1) IMG(LATIDX,5) = W(1) IMG(LNGIDX,6) = W(1)*7D0 IMG(LATIDX,6) = W(1) IMG(LNGIDX,7) = W(1)*7D0 IMG(LATIDX,7) = -W(1) IMG(LNGIDX,8) = -W(1) IMG(LATIDX,8) = -W(1) STATUS = WCSGET (WCS, WCS_LIN, LIN) STATUS = LINX2P (LIN, 9, NELEM, IMG, PIX) DO 30 J = 0, 8 IR(J) = PIX(LNGIDX,J) JR(J) = PIX(LATIDX,J) 30 CONTINUE CALL PGLINE (9, IR, JR) END IF IF (CATEG.EQ.6) THEN * Polyconic. STEP = 10D0 ELSE STEP = 15D0 END IF * Draw the native coordinate graticule faintly in the background. STATUS = WCSPUT (NATIVE, WCS_FLAG, -1, 0, 0) STATUS = WCSCOPY (WCS, NATIVE) STATUS = WCSPUT (NATIVE, WCS_CRVAL, 0D0, LNGIDX, 0) STATUS = WCSPUT (NATIVE, WCS_CRVAL, 90D0, LATIDX, 0) STATUS = WCSPUT (NATIVE, WCS_LONPOLE, 180D0, 0, 0) STATUS = WCSSET (NATIVE) CALL PGSCI (8) * Draw native meridians of longitude. DO 60 ILNG = -180, 180, 15 LNG = DBLE(ILNG) IF (ILNG.EQ.-180) LNG = -179.99D0 IF (ILNG.EQ.+180) LNG = +179.99D0 J = 0 DO 40 ILAT = -90, 90 WORLD(LNGIDX,J) = LNG WORLD(LATIDX,J) = DBLE(ILAT) J = J + 1 40 CONTINUE STATUS = WCSS2P (NATIVE, 181, NELEM, WORLD, PHI, THETA, IMG, : PIX, STAT) IF (STATUS.NE.0) GO TO 60 J = 0 K = 0 DO 50 ILAT = -90, 90 IF (CUBIC .AND. K.GT.0) THEN IF (ABS(PIX(LNGIDX,J)-IR(K-1)).GT.2D0 .OR. : ABS(PIX(LATIDX,J)-JR(K-1)).GT.5D0) THEN IF (K.GT.1) CALL PGLINE (K, IR, JR) K = 0 END IF END IF IR(K) = PIX(LNGIDX,J) JR(K) = PIX(LATIDX,J) J = J + 1 K = K + 1 50 CONTINUE CALL PGLINE (K, IR, JR) 60 CONTINUE * Draw native parallels of latitude. DO 90 ILAT = -90, 90, 15 LAT = DBLE(ILAT) J = 0 DO 70 ILNG = -180, 180 LNG = DBLE(ILNG) IF (ILNG.EQ.-180) LNG = -179.99D0 IF (ILNG.EQ.+180) LNG = +179.99D0 WORLD(LNGIDX,J) = LNG WORLD(LATIDX,J) = LAT J = J + 1 70 CONTINUE STATUS = WCSS2P (NATIVE, 361, NELEM, WORLD, PHI, THETA, IMG, : PIX, STAT) IF (STATUS.NE.0) GO TO 90 J = 0 K = 0 DO 80 ILNG = -180, 180 IF (CUBIC .AND. K.GT.0) THEN IF (ABS(PIX(LNGIDX,J)-IR(K-1)).GT.2D0 .OR. : ABS(PIX(LATIDX,J)-JR(K-1)).GT.5D0) THEN IF (K.GT.1) CALL PGLINE (K, IR, JR) K = 0 END IF END IF IR(K) = PIX(LNGIDX,J) JR(K) = PIX(LATIDX,J) J = J + 1 K = K + 1 80 CONTINUE CALL PGLINE (K, IR, JR) 90 CONTINUE STATUS = WCSFREE (NATIVE) * Draw a colour-coded celestial coordinate graticule. CI = 1 * Draw celestial meridians of longitude. DO 120 ILNG = -180, 180, 15 LNG = DBLE(ILNG) CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILNG.NE.0) THEN CALL PGSCI (CI) ELSE CALL PGSCI (1) END IF J = 0 DO 100 ILAT = -90, 90 LAT = DBLE(ILAT) WORLD(LNGIDX,J) = LNG WORLD(LATIDX,J) = LAT J = J + 1 100 CONTINUE STATUS = WCSS2P (WCS, 181, NELEM, WORLD, PHI, THETA, IMG, PIX, : STAT) IF (STATUS.NE.0) GO TO 120 J = 0 K = 0 DO 110 ILAT = -90, 90 * Test for discontinuities. IF (K.GT.0) THEN IF (ABS(PIX(LNGIDX,J)-IR(K-1)).GT.STEP .OR. : ABS(PIX(LATIDX,J)-JR(K-1)).GT.STEP) THEN IF (K.GT.1) CALL PGLINE (K, IR, JR) K = 0 END IF END IF IR(K) = PIX(LNGIDX,J) JR(K) = PIX(LATIDX,J) J = J + 1 K = K + 1 110 CONTINUE CALL PGLINE (K, IR, JR) 120 CONTINUE * Draw celestial parallels of latitude. CI = 1 DO 150 ILAT = -90, 90, 15 LAT = DBLE(ILAT) CI = CI + 1 IF (CI.GT.7) CI = 2 IF (ILAT.NE.0) THEN CALL PGSCI (CI) ELSE CALL PGSCI (1) END IF J = 0 DO 130 ILNG = -180, 180 WORLD(LNGIDX,J) = DBLE(ILNG) WORLD(LATIDX,J) = LAT J = J + 1 130 CONTINUE STATUS = WCSS2P (WCS, 361, NELEM, WORLD, PHI, THETA, IMG, PIX, : STAT) IF (STATUS.NE.0) GO TO 150 J = 0 K = 0 DO 140 ILNG = -180, 180 * Test for discontinuities. IF (K.GT.0) THEN IF (ABS(PIX(LNGIDX,J)-IR(K-1)).GT.STEP .OR. : ABS(PIX(LATIDX,J)-JR(K-1)).GT.STEP) THEN IF (K.GT.1) CALL PGLINE (K, IR, JR) K = 0 END IF END IF IR(K) = PIX(LNGIDX,J) JR(K) = PIX(LATIDX,J) J = J + 1 K = K + 1 140 CONTINUE CALL PGLINE (K, IR, JR) 150 CONTINUE * Write a descriptive title. CALL PGSCI (1) STATUS = PRJGET (PRJ, PRJ_CODE, PCODE) TEXT = PCODE // ' projection - 15 degree graticule' WRITE (*, '(//,A)') TEXT CALL PGTEXT (IMIN, JMIN-10.0, TEXT) STATUS = CELGET (CEL, CEL_REF, REF) WRITE (TEXT, 160) REF(1), REF(2) 160 FORMAT ('centered on celestial coordinates (',F6.2,',',F6.2,')') WRITE (*, '(A)') TEXT CALL PGTEXT (IMIN, JMIN-20.0, TEXT) WRITE (TEXT, 170) REF(3), REF(4) 170 FORMAT ('with celestial pole at native coordinates (',F7.2, : ',',F7.2,')') WRITE (*, '(A)') TEXT CALL PGTEXT (IMIN, JMIN-30.0, TEXT) CALL PGSCI (2) RETURN END *----------------------------------------------------------------------- SUBROUTINE PARSER (WCS) *----------------------------------------------------------------------- * In practice a parser would read the FITS header until it encountered * the NAXIS keyword which must occur near the start, before any of the * WCS keywords. It would then use WCSINI to allocate memory for arrays * in the WCSPRM "data structure" and set default values. * * In this simulation the header keyvalues are set in the main program in * variables passed in COMMON. *----------------------------------------------------------------------- * Number of axes. INTEGER N PARAMETER (N = 4) INTEGER I, J, K, NAXIS, NPV, PVI(4), PVM(4), STATUS, WCS(*) DOUBLE PRECISION CDELT(N), CRPIX(N), CRVAL(N), LATPOLE, LONPOLE, : PC(N,N), PV(4), RESTFRQ, RESTWAV CHARACTER CTYPE(N)*72 INCLUDE 'wcs.inc' COMMON /HEADER/ NAXIS, NPV, CRPIX, PC, CDELT, CRVAL, LONPOLE, : LATPOLE, RESTFRQ, RESTWAV, PVI, PVM, PV COMMON /HEADCH/ CTYPE *----------------------------------------------------------------------- STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) STATUS = WCSINI (NAXIS, WCS) DO 20 I = 1, NAXIS STATUS = WCSPUT (WCS, WCS_CRPIX, CRPIX(I), I, 0) DO 10 J = 1, NAXIS STATUS = WCSPUT (WCS, WCS_PC, PC(I,J), I, J) 10 CONTINUE STATUS = WCSPUT (WCS, WCS_CDELT, CDELT(I), I, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(I), I, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, CRVAL(I), I, 0) 20 CONTINUE STATUS = WCSPUT (WCS, WCS_LONPOLE, LONPOLE, 0, 0) STATUS = WCSPUT (WCS, WCS_LATPOLE, LATPOLE, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTFRQ, RESTFRQ, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTWAV, RESTWAV, 0, 0) DO 30 K = 1, NPV STATUS = WCSPUT (WCS, WCS_PV, PV(K), PVI(K), PVM(K)) 30 CONTINUE * Extract information from the FITS header. STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN WRITE (*, 40) STATUS 40 FORMAT ('WCSSET ERROR',I3) END IF RETURN END pywcs-1.12/wcslib/Fortran/test/twcssub.f0000644001153600020070000001500112310355626022361 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: twcssub.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TWCSSUB *----------------------------------------------------------------------- * * TWCSSUB tests WCSSUB which extracts the coordinate description for a * subimage from a wcsprm struct. * *----------------------------------------------------------------------- * Number of axes. INTEGER NAXIS PARAMETER (NAXIS = 4) INTEGER AXES(NAXIS), I, J, K, NPS, NPV, NSUB, PSI(10), PSM(10), : PVI(10), PVM(10), STATUS DOUBLE PRECISION CDELT(NAXIS), CRPIX(NAXIS), CRVAL(NAXIS), : LATPOLE, LONPOLE, PC(NAXIS,NAXIS), PV(10), RESTFRQ, : RESTWAV CHARACTER CNAME(NAXIS)*72, CTYPE(NAXIS)*72, CUNIT(NAXIS)*72, : PS(10)*72 * On some systems, such as Sun Sparc, the structs MUST be aligned * on a double precision boundary, done here using equivalences. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcs.inc' INCLUDE 'wcserr.inc' INTEGER WCS(WCSLEN), WCSEXT(WCSLEN) DOUBLE PRECISION DUMMY1, DUMMY2 EQUIVALENCE (WCS,DUMMY1), (WCSEXT,DUMMY2) DATA (CRPIX(J), J=1,NAXIS) : / 1025D0, 64D0, 512D0, 513D0/ DATA ((PC(I,J),J=1,NAXIS),I=1,NAXIS) : / 1.1D0, 0D0, 0D0, 0D0, : 0D0, 1.0D0, 0D0, 0D0, : 0D0, 0D0, 1.0D0, 0.1D0, : 0D0, 0D0, 0.2D0, 1.0D0/ DATA (CDELT(I), I=1,NAXIS) : /-9.2D-6, 10D0, 1D0, -1D0/ DATA (CUNIT(I), I=1,NAXIS) : /'m', 's', 'deg', 'deg'/ DATA (CTYPE(I), I=1,NAXIS) : /'WAVE-F2W', 'TIME', 'XLAT-SZP', 'XLON-SZP'/ DATA (CRVAL(I), I=1,NAXIS) : /0.214982042D0, -2D3, -30D0, 150D0/ DATA LONPOLE /150D0/ DATA LATPOLE /999D0/ DATA RESTFRQ /1.42040575D9/ DATA RESTWAV /0D0/ DATA (CNAME(I), I=1,NAXIS) : /'Wavelength', 'Time', 'Latitude', 'Longitude'/ PARAMETER (NPV = 4) DATA (PVI(K), PVM(K), PV(K), K=1,NPV) : /1, 1, -1D0, : 3, 1, 2D0, : 3, 2, 210D0, : 3, 3, 60D0/ PARAMETER (NPS = 1) DATA (PSI(K), PSM(K), PS(K), K=1,NPS) : /2, 1, 'UTC'/ *----------------------------------------------------------------------- STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) STATUS = WCSINI (NAXIS, WCS) DO 20 I = 1, NAXIS STATUS = WCSPUT (WCS, WCS_CRPIX, CRPIX(I), I, 0) DO 10 J = 1, NAXIS STATUS = WCSPUT (WCS, WCS_PC, PC(I,J), I, J) 10 CONTINUE STATUS = WCSPUT (WCS, WCS_CDELT, CDELT(I), I, 0) STATUS = WCSPUT (WCS, WCS_CUNIT, CUNIT(I), I, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(I), I, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, CRVAL(I), I, 0) STATUS = WCSPUT (WCS, WCS_CNAME, CNAME(I), I, 0) 20 CONTINUE STATUS = WCSPUT (WCS, WCS_LONPOLE, LONPOLE, 0, 0) STATUS = WCSPUT (WCS, WCS_LATPOLE, LATPOLE, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTFRQ, RESTFRQ, 0, 0) STATUS = WCSPUT (WCS, WCS_RESTWAV, RESTWAV, 0, 0) DO 30 K = 1, NPV STATUS = WCSPUT (WCS, WCS_PV, PV(K), PVI(K), PVM(K)) 30 CONTINUE DO 40 K = 1, NPS STATUS = WCSPUT (WCS, WCS_PS, PS(K), PSI(K), PSM(K)) 40 CONTINUE * Extract information from the FITS header. STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN WRITE (*, 50) STATUS 50 FORMAT ('WCSSET ERROR',I3,'.') GO TO 999 END IF WRITE (*, 60) 60 FORMAT ( : 'Testing WCSLIB subimage extraction subroutine (twcssub.f)',/, : '---------------------------------------------------------',//, : 'Initial contents of wcsprm struct:') CALL FLUSH(6) STATUS = WCSPRT (WCS) * Extract the coordinate description for a subimage and add an axis. NSUB = 4 AXES(1) = WCSSUB_LONGITUDE AXES(2) = WCSSUB_LATITUDE AXES(3) = -(WCSSUB_SPECTRAL + WCSSUB_STOKES) AXES(4) = 0 WRITE (6, 70) 70 FORMAT (//,'Extracted contents of wcsprm struct:') STATUS = WCSPUT (WCSEXT, WCS_FLAG, -1, 0, 0) STATUS = WCSSUB (WCS, NSUB, AXES, WCSEXT) CALL FLUSH(6) IF (STATUS.NE.0) THEN STATUS = WCSPERR (WCSEXT, CHAR(0)) ELSE STATUS = WCSSET (WCSEXT) IF (STATUS.NE.0) THEN STATUS = WCSPERR (WCSEXT, CHAR(0)) ELSE STATUS = WCSPRT (WCSEXT) END IF END IF * Set it up for failure by setting PC1_3 non-zero. STATUS = WCSPUT (WCS, WCS_PC, 1D0, 1, 3) NSUB = 2 AXES(1) = 4 AXES(2) = 3 STATUS = WCSSUB(WCS, NSUB, AXES, WCSEXT) IF (STATUS.EQ.WCSERR_NON_SEPARABLE) THEN WRITE (6, 80) WCSERR_NON_SEPARABLE 80 FORMAT (//,'Received wcssub status',I3,' as expected for a ' : 'non-separable subimage',/,'coordinate system.') ELSE WRITE (6, 90) WCSERR_NON_SEPARABLE, STATUS 90 FORMAT (//,'ERROR: expected wcssub status',I3,' for a non-', : 'separable subimage coordinate',/,'system, but received ', : 'status',I3,' instead.') END IF STATUS = WCSFREE (WCSEXT) 999 STATUS = WCSFREE (WCS) END pywcs-1.12/wcslib/Fortran/test/twcstab.f0000644001153600020070000001423312310355626022344 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: twcstab.f,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= PROGRAM TWCSTAB *----------------------------------------------------------------------- * * TWCSTAB tests WCSTAB and also provides sample code for using it in * conjunction with WCSPIH and FTWCST. Although this example and FTWCST * are based on the CFITSIO library, WCSTAB itself is completely * independent of it. * * We assume that the input file, ../C/wcstab.fits, has already been * generated by running the C version of twcstab. * * WCSP and WTB, which are meant to hold addresses, are declared as * INTEGER arrays of length 2 to accomodate 64-bit machines for which * sizeof(void *) = 2*sizeof(int). *======================================================================= LOGICAL GOTEND INTEGER BLOKSZ, I, J, K, IERR, IUNIT, NKEYRC, NREJECT, NWCS, : NWTB, STATUS, WCSP(2), WTB(2) CHARACTER KEYREC*80, HEADER*28801, INFILE*16 * On some systems, such as Sun Sparc, the struct MUST be aligned * on a double precision boundary, done here using an equivalence. * Failure to do this may result in mysterious "bus errors". INCLUDE 'wcs.inc' INCLUDE 'wcshdr.inc' INCLUDE 'wcsfix.inc' INCLUDE 'getwcstab.inc' INTEGER STAT(WCSFIX_NWCS) INTEGER WCS(WCSLEN) DOUBLE PRECISION DUMMY EQUIVALENCE (WCS,DUMMY) DATA INFILE /'../C/wcstab.fits'/ *----------------------------------------------------------------------- WRITE (*, 10) 10 FORMAT ('Testing WCSTAB and associated routines (twcstab.f)',/, : '--------------------------------------------------',/) * Open the FITS test file. IUNIT = 1 STATUS = 0 CALL FTOPEN (IUNIT, INFILE, 0, BLOKSZ, STATUS) IF (STATUS.NE.0) THEN CALL FLUSH(6) CALL FTRPRT ('STDERR', STATUS) GO TO 999 END IF * Read the primary header; unfortunately there is no FITSIO * equivalent of CFITSIO's fits_hdr2str() so do it the long way. OPEN (UNIT=1, FILE=INFILE, FORM='FORMATTED', ACCESS='DIRECT', : RECL=80, IOSTAT=IERR) IF (IERR.NE.0) THEN WRITE (*, 20) IERR, INFILE 20 FORMAT ('ERROR',I3,' opening ',A) GO TO 999 END IF * Read in the FITS header, excluding COMMENT and HISTORY keyrecords. K = 1 NKEYRC = 0 GOTEND = .FALSE. DO 50 J = 0, 100 DO 40 I = 1, 36 READ (1, '(A80)', REC=36*J+I, IOSTAT=IERR) KEYREC IF (IERR.NE.0) THEN WRITE (*, 30) IERR 30 FORMAT ('ERROR',I3,' reading header.') GO TO 999 END IF IF (KEYREC(:8).EQ.' ') GO TO 40 IF (KEYREC(:8).EQ.'COMMENT ') GO TO 40 IF (KEYREC(:8).EQ.'HISTORY ') GO TO 40 HEADER(K:) = KEYREC K = K + 80 NKEYRC = NKEYRC + 1 IF (KEYREC(:8).EQ.'END ') THEN * An END keyrecord was read, read the rest of the block. GOTEND = .TRUE. END IF 40 CONTINUE IF (GOTEND) GO TO 60 50 CONTINUE 60 CLOSE (UNIT=1) *----------------------------------------------------------------------- * Basic steps required to interpret a FITS WCS header, including -TAB. *----------------------------------------------------------------------- * Parse the primary header of the FITS file. STATUS = WCSPIH (HEADER, NKEYRC, WCSHDR_all, 2, NREJECT, NWCS, : WCSP) IF (STATUS.NE.0) THEN WRITE (*, 70) STATUS, WCSHDR_ERRMSG(STATUS) 70 FORMAT ('WCSPIH ERROR',I2,A) GO TO 999 END IF * Copy into our WCSPRM struct. IERR = WCSVCOPY (WCSP, 0, WCS) * Read coordinate arrays from the binary table extension. STATUS = WCSGET (WCS, WCS_NWTB, NWTB) STATUS = WCSGET (WCS, WCS_WTB, WTB) STATUS = FTWCST (IUNIT, NWTB, WTB, STATUS) IF (STATUS.NE.0) THEN CALL FLUSH(6) CALL FTRPRT ('STDERR', STATUS) GO TO 999 END IF * Fix non-standard WCS keyvalues. STATUS = WCSFIX (7, 0, WCS, STAT) IF (STATUS.NE.0) THEN WRITE (*, 80) (STAT(I), I=1,WCSFIX_NWCS) 80 FORMAT ('WCSFIX ERROR, status returns: ',10(I2,:,',')) GO TO 999 END IF *----------------------------------------------------------------------- * The wcsprm struct is now ready for use. *----------------------------------------------------------------------- * Finished with the FITS file. CALL FTCLOS (IUNIT, STATUS) * Initialize the wcsprm struct, taking memory allocated by FTWCST. IF (STATUS.EQ.0) STATUS = WCSSET (WCS) IF (STATUS.NE.0) THEN WRITE (*, 90) STATUS, WCS_ERRMSG(STATUS) 90 FORMAT ('WCSSET ERROR',I2,A) GO TO 998 END IF * Do something with it. CALL FLUSH(6) STATUS = WCSPRT (WCS) * Clean up. 998 STATUS = WCSFREE (WCS) STATUS = WCSVFREE (NWCS, WCSP) 999 CONTINUE END pywcs-1.12/wcslib/Fortran/wcs.inc0000644001153600020070000001506612310355626021043 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcs.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL WCSCOPY, WCSFREE, WCSGET, WCSGTC, WCSGTD, WCSGTI, : WCSINI, WCSMIX, WCSNPS, WCSNPV, WCSP2S, WCSPERR, WCSPRT, : WCSSPTR, WCSPTC, WCSPTD, WCSPTI, WCSPUT, WCSS2P, WCSSET, : WCSSUB INTEGER WCSCOPY, WCSFREE, WCSGET, WCSGTC, WCSGTD, WCSGTI, : WCSINI, WCSMIX, WCSNPS, WCSNPV, WCSP2S, WCSPERR, WCSPRT, : WCSSPTR, WCSPTC, WCSPTD, WCSPTI, WCSPUT, WCSS2P, WCSSET, : WCSSUB * Length of the WCSPRM data structure (INTEGER array) on 64-bit * machines. Only needs to be 416 on 32-bit machines. INTEGER WCSLEN PARAMETER (WCSLEN = 474) * Codes for WCS data structure elements used by WCSPUT and WCSGET. INTEGER WCS_ALT, WCS_ALTLIN, WCS_CD, WCS_CDELT, WCS_CNAME, : WCS_COLAX, WCS_COLNUM, WCS_CRDER, WCS_CROTA, WCS_CRPIX, : WCS_CRVAL, WCS_CSYER, WCS_CTYPE, WCS_CUNIT, WCS_DATEAVG, : WCS_DATEOBS, WCS_EQUINOX, WCS_FLAG, WCS_LATPOLE, : WCS_LONPOLE, WCS_MJDAVG, WCS_MJDOBS, WCS_NAXIS, WCS_NPS, : WCS_NPSMAX, WCS_NPV, WCS_NPVMAX, WCS_OBSGEO, WCS_PC, : WCS_PS, WCS_PV, WCS_RADESYS, WCS_RESTFRQ, WCS_RESTWAV, : WCS_SPECSYS, WCS_SSYSOBS, WCS_SSYSSRC, WCS_VELANGL, : WCS_VELOSYS, WCS_VELREF, WCS_WCSNAME, WCS_ZSOURCE PARAMETER (WCS_FLAG = 100) PARAMETER (WCS_NAXIS = 101) PARAMETER (WCS_CRPIX = 102) PARAMETER (WCS_PC = 103) PARAMETER (WCS_CDELT = 104) PARAMETER (WCS_CRVAL = 105) PARAMETER (WCS_CUNIT = 106) PARAMETER (WCS_CTYPE = 107) PARAMETER (WCS_LONPOLE = 108) PARAMETER (WCS_LATPOLE = 109) PARAMETER (WCS_RESTFRQ = 110) PARAMETER (WCS_RESTWAV = 111) PARAMETER (WCS_NPV = 112) PARAMETER (WCS_NPVMAX = 113) PARAMETER (WCS_PV = 114) PARAMETER (WCS_NPS = 115) PARAMETER (WCS_NPSMAX = 116) PARAMETER (WCS_PS = 117) PARAMETER (WCS_CD = 118) PARAMETER (WCS_CROTA = 119) PARAMETER (WCS_ALTLIN = 120) PARAMETER (WCS_VELREF = 121) PARAMETER (WCS_ALT = 122) PARAMETER (WCS_COLNUM = 123) PARAMETER (WCS_COLAX = 124) PARAMETER (WCS_CNAME = 125) PARAMETER (WCS_CRDER = 126) PARAMETER (WCS_CSYER = 127) PARAMETER (WCS_DATEAVG = 128) PARAMETER (WCS_DATEOBS = 129) PARAMETER (WCS_EQUINOX = 130) PARAMETER (WCS_MJDAVG = 131) PARAMETER (WCS_MJDOBS = 132) PARAMETER (WCS_OBSGEO = 133) PARAMETER (WCS_RADESYS = 134) PARAMETER (WCS_SPECSYS = 135) PARAMETER (WCS_SSYSOBS = 136) PARAMETER (WCS_VELOSYS = 137) PARAMETER (WCS_ZSOURCE = 138) PARAMETER (WCS_SSYSSRC = 139) PARAMETER (WCS_VELANGL = 140) PARAMETER (WCS_WCSNAME = 141) * Codes for WCS data structure elements used by WCSGET (only). INTEGER WCS_CEL, WCS_CUBEFACE, WCS_ERR, WCS_LAT, WCS_LATTYP, : WCS_LIN, WCS_LNG, WCS_LNGTYP, WCS_NTAB, WCS_NWTB, : WCS_SPC, WCS_SPEC, WCS_TAB, WCS_TYPES, WCS_WTB PARAMETER (WCS_NTAB = 200) PARAMETER (WCS_NWTB = 201) PARAMETER (WCS_TAB = 202) PARAMETER (WCS_WTB = 203) PARAMETER (WCS_LNGTYP = 204) PARAMETER (WCS_LATTYP = 205) PARAMETER (WCS_LNG = 206) PARAMETER (WCS_LAT = 207) PARAMETER (WCS_SPEC = 208) PARAMETER (WCS_CUBEFACE = 209) PARAMETER (WCS_TYPES = 210) PARAMETER (WCS_LIN = 211) PARAMETER (WCS_CEL = 212) PARAMETER (WCS_SPC = 213) PARAMETER (WCS_ERR = 214) * Flag bits for the AXES argument. INTEGER WCSSUB_CELESTIAL, WCSSUB_CUBEFACE, WCSSUB_LATITUDE, : WCSSUB_LONGITUDE, WCSSUB_SPECTRAL, WCSSUB_STOKES PARAMETER (WCSSUB_LONGITUDE = 4096 + 1) PARAMETER (WCSSUB_LATITUDE = 4096 + 2) PARAMETER (WCSSUB_CUBEFACE = 4096 + 4) PARAMETER (WCSSUB_CELESTIAL = 4096 + 7) PARAMETER (WCSSUB_SPECTRAL = 4096 + 8) PARAMETER (WCSSUB_STOKES = 4096 + 16) * Error codes and messages. INTEGER WCSERR_BAD_COORD_TRANS, WCSERR_BAD_CTYPE, : WCSERR_BAD_PARAM, WCSERR_BAD_PIX, WCSERR_BAD_SUBIMAGE, : WCSERR_BAD_WORLD, WCSERR_BAD_WORLD_COORD, : WCSERR_ILL_COORD_TRANS, WCSERR_MEMORY, : WCSERR_NON_SEPARABLE, WCSERR_NO_SOLUTION, : WCSERR_NULL_POINTER, WCSERR_SINGULAR_MTX, WCSERR_SUCCESS PARAMETER (WCSERR_SUCCESS = 0) PARAMETER (WCSERR_NULL_POINTER = 1) PARAMETER (WCSERR_MEMORY = 2) PARAMETER (WCSERR_SINGULAR_MTX = 3) PARAMETER (WCSERR_BAD_CTYPE = 4) PARAMETER (WCSERR_BAD_PARAM = 5) PARAMETER (WCSERR_BAD_COORD_TRANS = 6) PARAMETER (WCSERR_ILL_COORD_TRANS = 7) PARAMETER (WCSERR_BAD_PIX = 8) PARAMETER (WCSERR_BAD_WORLD = 9) PARAMETER (WCSERR_BAD_WORLD_COORD = 10) PARAMETER (WCSERR_NO_SOLUTION = 11) PARAMETER (WCSERR_BAD_SUBIMAGE = 12) PARAMETER (WCSERR_NON_SEPARABLE = 13) CHARACTER WCS_ERRMSG(0:13)*80 COMMON /WCS_DATA/ WCS_ERRMSG pywcs-1.12/wcslib/Fortran/wcs_f.c0000644001153600020070000004361212310355626021017 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcs_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include /* Fortran name mangling. */ #include #define wcsnpv_ F77_FUNC(wcsnpv, WCSNPV) #define wcsnps_ F77_FUNC(wcsnps, WCSNPS) #define wcsini_ F77_FUNC(wcsini, WCSINI) #define wcssub_ F77_FUNC(wcssub, WCSSUB) #define wcscopy_ F77_FUNC(wcscopy, WCSCOPY) #define wcsput_ F77_FUNC(wcsput, WCSPUT) #define wcsget_ F77_FUNC(wcsget, WCSGET) #define wcsfree_ F77_FUNC(wcsfree, WCSFREE) #define wcsprt_ F77_FUNC(wcsprt, WCSPRT) #define wcsperr_ F77_FUNC(wcsperr, WCSPERR) #define wcsset_ F77_FUNC(wcsset, WCSSET) #define wcsp2s_ F77_FUNC(wcsp2s, WCSP2S) #define wcss2p_ F77_FUNC(wcss2p, WCSS2P) #define wcsmix_ F77_FUNC(wcsmix, WCSMIX) #define wcssptr_ F77_FUNC(wcssptr, WCSSPTR) #define wcsptc_ F77_FUNC(wcsptc, WCSPTC) #define wcsptd_ F77_FUNC(wcsptd, WCSPTD) #define wcspti_ F77_FUNC(wcspti, WCSPTI) #define wcsgtc_ F77_FUNC(wcsgtc, WCSGTC) #define wcsgtd_ F77_FUNC(wcsgtd, WCSGTD) #define wcsgti_ F77_FUNC(wcsgti, WCSGTI) #define WCS_FLAG 100 #define WCS_NAXIS 101 #define WCS_CRPIX 102 #define WCS_PC 103 #define WCS_CDELT 104 #define WCS_CRVAL 105 #define WCS_CUNIT 106 #define WCS_CTYPE 107 #define WCS_LONPOLE 108 #define WCS_LATPOLE 109 #define WCS_RESTFRQ 110 #define WCS_RESTWAV 111 #define WCS_NPV 112 #define WCS_NPVMAX 113 #define WCS_PV 114 #define WCS_NPS 115 #define WCS_NPSMAX 116 #define WCS_PS 117 #define WCS_CD 118 #define WCS_CROTA 119 #define WCS_ALTLIN 120 #define WCS_VELREF 121 #define WCS_ALT 122 #define WCS_COLNUM 123 #define WCS_COLAX 124 #define WCS_CNAME 125 #define WCS_CRDER 126 #define WCS_CSYER 127 #define WCS_DATEAVG 128 #define WCS_DATEOBS 129 #define WCS_EQUINOX 130 #define WCS_MJDAVG 131 #define WCS_MJDOBS 132 #define WCS_OBSGEO 133 #define WCS_RADESYS 134 #define WCS_SPECSYS 135 #define WCS_SSYSOBS 136 #define WCS_VELOSYS 137 #define WCS_ZSOURCE 138 #define WCS_SSYSSRC 139 #define WCS_VELANGL 140 #define WCS_WCSNAME 141 #define WCS_NTAB 200 #define WCS_NWTB 201 #define WCS_TAB 202 #define WCS_WTB 203 #define WCS_LNGTYP 204 #define WCS_LATTYP 205 #define WCS_LNG 206 #define WCS_LAT 207 #define WCS_SPEC 208 #define WCS_CUBEFACE 209 #define WCS_TYPES 210 #define WCS_LIN 211 #define WCS_CEL 212 #define WCS_SPC 213 #define WCS_ERR 214 /*--------------------------------------------------------------------------*/ int wcsnpv_(int *npvmax) { return wcsnpv(*npvmax); } int wcsnps_(int *npsmax) { return wcsnps(*npsmax); } /*--------------------------------------------------------------------------*/ int wcsini_(const int *naxis, int *wcs) { return wcsini(1, *naxis, (struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int wcssub_(const int *wcssrc, int *nsub, int axes[], int *wcsdst) { return wcssub(1, (const struct wcsprm *)wcssrc, nsub, axes, (struct wcsprm *)wcsdst); } /*--------------------------------------------------------------------------*/ int wcscopy_(const int *wcssrc, int *wcsdst) { return wcscopy(1, (const struct wcsprm *)wcssrc, (struct wcsprm *)wcsdst); } /*--------------------------------------------------------------------------*/ int wcsput_( int *wcs, const int *what, const void *value, const int *i, const int *j) { int i0, j0, k; const char *cvalp; const int *ivalp; const double *dvalp; struct wcsprm *wcsp; /* Cast pointers. */ wcsp = (struct wcsprm *)wcs; cvalp = (const char *)value; ivalp = (const int *)value; dvalp = (const double *)value; /* Convert 1-relative FITS axis numbers to 0-relative C array indices. */ i0 = *i - 1; j0 = *j - 1; wcsp->flag = 0; switch (*what) { case WCS_FLAG: wcsp->flag = *ivalp; break; case WCS_NAXIS: wcsp->naxis = *ivalp; break; case WCS_CRPIX: wcsp->crpix[i0] = *dvalp; break; case WCS_PC: k = (i0)*(wcsp->naxis) + (j0); *(wcsp->pc+k) = *dvalp; break; case WCS_CDELT: wcsp->cdelt[i0] = *dvalp; break; case WCS_CRVAL: wcsp->crval[i0] = *dvalp; break; case WCS_CUNIT: strncpy(wcsp->cunit[i0], cvalp, 72); wcsutil_null_fill(72, wcsp->cunit[i0]); break; case WCS_CTYPE: strncpy(wcsp->ctype[i0], cvalp, 72); wcsutil_null_fill(72, wcsp->ctype[i0]); break; case WCS_LONPOLE: wcsp->lonpole = *dvalp; break; case WCS_LATPOLE: wcsp->latpole = *dvalp; break; case WCS_RESTFRQ: wcsp->restfrq = *dvalp; break; case WCS_RESTWAV: wcsp->restwav = *dvalp; break; case WCS_NPV: case WCS_NPVMAX: return 1; break; case WCS_PV: (wcsp->pv + wcsp->npv)->i = *i; (wcsp->pv + wcsp->npv)->m = *j; (wcsp->pv + wcsp->npv)->value = *dvalp; (wcsp->npv)++; break; case WCS_NPS: case WCS_NPSMAX: return 1; break; case WCS_PS: (wcsp->ps + wcsp->nps)->i = *i; (wcsp->ps + wcsp->nps)->m = *j; strncpy((wcsp->ps + wcsp->nps)->value, cvalp, 72); wcsutil_null_fill(72, (wcsp->ps + wcsp->nps)->value); (wcsp->nps)++; break; case WCS_CD: k = (i0)*(wcsp->naxis) + (j0); *(wcsp->cd+k) = *dvalp; break; case WCS_CROTA: wcsp->crota[i0] = *dvalp; break; case WCS_ALTLIN: wcsp->altlin = *ivalp; break; case WCS_VELREF: wcsp->velref = *ivalp; break; case WCS_ALT: wcsp->alt[0] = cvalp[0]; wcsutil_null_fill(4, wcsp->alt); break; case WCS_COLNUM: wcsp->colnum = *ivalp; break; case WCS_COLAX: wcsp->colax[i0] = *ivalp; break; case WCS_CNAME: strncpy(wcsp->cname[i0], cvalp, 72); wcsutil_null_fill(72, wcsp->cname[i0]); break; case WCS_CRDER: wcsp->crder[i0] = *dvalp; break; case WCS_CSYER: wcsp->csyer[i0] = *dvalp; break; case WCS_DATEAVG: strncpy(wcsp->dateavg, cvalp, 72); wcsutil_null_fill(72, wcsp->dateavg); break; case WCS_DATEOBS: strncpy(wcsp->dateobs, cvalp, 72); wcsutil_null_fill(72, wcsp->dateobs); break; case WCS_EQUINOX: wcsp->equinox = *dvalp; break; case WCS_MJDAVG: wcsp->mjdavg = *dvalp; break; case WCS_MJDOBS: wcsp->mjdobs = *dvalp; break; case WCS_OBSGEO: wcsp->obsgeo[i0] = *dvalp; break; case WCS_RADESYS: strncpy(wcsp->radesys, cvalp, 72); wcsutil_null_fill(72, wcsp->radesys); break; case WCS_SPECSYS: strncpy(wcsp->specsys, cvalp, 72); wcsutil_null_fill(72, wcsp->specsys); break; case WCS_SSYSOBS: strncpy(wcsp->ssysobs, cvalp, 72); wcsutil_null_fill(72, wcsp->ssysobs); break; case WCS_VELOSYS: wcsp->velosys = *dvalp; break; case WCS_ZSOURCE: wcsp->zsource = *dvalp; break; case WCS_SSYSSRC: strncpy(wcsp->ssyssrc, cvalp, 72); wcsutil_null_fill(72, wcsp->ssyssrc); break; case WCS_VELANGL: wcsp->velangl = *dvalp; break; case WCS_WCSNAME: strncpy(wcsp->wcsname, cvalp, 72); wcsutil_null_fill(72, wcsp->wcsname); break; default: return 1; } return 0; } int wcsptc_(int *wcs, const int *what, const char *value, const int *i, const int *j) { return wcsput_(wcs, what, value, i, j); } int wcsptd_(int *wcs, const int *what, const double *value, const int *i, const int *j) { return wcsput_(wcs, what, value, i, j); } int wcspti_(int *wcs, const int *what, const int *value, const int *i, const int *j) { return wcsput_(wcs, what, value, i, j); } /*--------------------------------------------------------------------------*/ int wcsget_(const int *wcs, const int *what, void *value) { int i, j, k, naxis; char *cvalp; int *ivalp; double *dvalp; const int *iwcsp; const double *dwcsp; const struct wcsprm *wcsp; /* Cast pointers. */ wcsp = (const struct wcsprm *)wcs; cvalp = (char *)value; ivalp = (int *)value; dvalp = (double *)value; naxis = wcsp->naxis; switch (*what) { case WCS_FLAG: *ivalp = wcsp->flag; break; case WCS_NAXIS: *ivalp = naxis; break; case WCS_CRPIX: for (i = 0; i < naxis; i++) { *(dvalp++) = wcsp->crpix[i]; } break; case WCS_PC: /* C row-major to FORTRAN column-major. */ for (j = 0; j < naxis; j++) { dwcsp = wcsp->pc + j; for (i = 0; i < naxis; i++) { *(dvalp++) = *dwcsp; dwcsp += naxis; } } break; case WCS_CDELT: for (i = 0; i < naxis; i++) { *(dvalp++) = wcsp->cdelt[i]; } break; case WCS_CRVAL: for (i = 0; i < naxis; i++) { *(dvalp++) = wcsp->crval[i]; } break; case WCS_CUNIT: for (i = 0; i < naxis; i++) { strncpy(cvalp, wcsp->cunit[i], 72); wcsutil_blank_fill(72, cvalp); cvalp += 72; } break; case WCS_CTYPE: for (i = 0; i < naxis; i++) { strncpy(cvalp, wcsp->ctype[i], 72); wcsutil_blank_fill(72, cvalp); cvalp += 72; } break; case WCS_LONPOLE: *dvalp = wcsp->lonpole; break; case WCS_LATPOLE: *dvalp = wcsp->latpole; break; case WCS_RESTFRQ: *dvalp = wcsp->restfrq; break; case WCS_RESTWAV: *dvalp = wcsp->restwav; break; case WCS_NPV: *ivalp = wcsp->npv; break; case WCS_NPVMAX: *ivalp = wcsp->npvmax; break; case WCS_PV: for (k = 0; k < wcsp->npv; k++) { *(dvalp++) = (wcsp->pv + k)->i; *(dvalp++) = (wcsp->pv + k)->m; *(dvalp++) = (wcsp->pv + k)->value; } break; case WCS_NPS: *ivalp = wcsp->nps; break; case WCS_NPSMAX: *ivalp = wcsp->npsmax; break; case WCS_PS: for (k = 0; k < wcsp->nps; k++) { *(dvalp++) = (wcsp->ps + k)->i; *(dvalp++) = (wcsp->ps + k)->m; cvalp += 2*sizeof(double); strncpy(cvalp, (wcsp->ps + k)->value, 72); wcsutil_blank_fill(72, cvalp); cvalp += 72; } break; case WCS_CD: /* C row-major to FORTRAN column-major. */ for (j = 0; j < naxis; j++) { dwcsp = wcsp->cd + j; for (i = 0; i < naxis; i++) { *(dvalp++) = *dwcsp; dwcsp += naxis; } } break; case WCS_CROTA: for (i = 0; i < naxis; i++) { *(dvalp++) = wcsp->crota[i]; } break; case WCS_ALTLIN: *ivalp = wcsp->altlin; break; case WCS_VELREF: *ivalp = wcsp->velref; break; case WCS_ALT: strncpy(cvalp, wcsp->alt, 4); wcsutil_blank_fill(4, cvalp); break; case WCS_COLNUM: *ivalp = wcsp->colnum; break; case WCS_COLAX: for (i = 0; i < naxis; i++) { *(ivalp++) = wcsp->colax[i]; } break; case WCS_CNAME: for (i = 0; i < naxis; i++) { strncpy(cvalp, wcsp->cname[i], 72); wcsutil_blank_fill(72, cvalp); cvalp += 72; } break; case WCS_CRDER: for (i = 0; i < naxis; i++) { *(dvalp++) = wcsp->crder[i]; } break; case WCS_CSYER: for (i = 0; i < naxis; i++) { *(dvalp++) = wcsp->csyer[i]; } break; case WCS_DATEAVG: strncpy(cvalp, wcsp->dateavg, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_DATEOBS: strncpy(cvalp, wcsp->dateobs, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_EQUINOX: *dvalp = wcsp->equinox; break; case WCS_MJDAVG: *dvalp = wcsp->mjdavg; break; case WCS_MJDOBS: *dvalp = wcsp->mjdobs; break; case WCS_OBSGEO: for (i = 0; i < 3; i++) { *(dvalp++) = wcsp->obsgeo[i]; } break; case WCS_RADESYS: strncpy(cvalp, wcsp->radesys, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_SPECSYS: strncpy(cvalp, wcsp->specsys, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_SSYSOBS: strncpy(cvalp, wcsp->ssysobs, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_VELOSYS: *dvalp = wcsp->velosys; break; case WCS_ZSOURCE: *dvalp = wcsp->zsource; break; case WCS_SSYSSRC: strncpy(cvalp, wcsp->ssyssrc, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_VELANGL: *dvalp = wcsp->velangl; break; case WCS_WCSNAME: strncpy(cvalp, wcsp->wcsname, 72); wcsutil_blank_fill(72, cvalp); break; case WCS_NTAB: *ivalp = wcsp->ntab; break; case WCS_NWTB: *ivalp = wcsp->nwtb; break; case WCS_TAB: *(void **)value = wcsp->tab; break; case WCS_WTB: *(void **)value = wcsp->wtb; break; case WCS_LNGTYP: strncpy(cvalp, wcsp->lngtyp, 4); wcsutil_blank_fill(4, cvalp); break; case WCS_LATTYP: strncpy(cvalp, wcsp->lattyp, 4); wcsutil_blank_fill(4, cvalp); break; case WCS_LNG: *ivalp = wcsp->lng + 1; break; case WCS_LAT: *ivalp = wcsp->lat + 1; break; case WCS_SPEC: *ivalp = wcsp->spec + 1; break; case WCS_CUBEFACE: *ivalp = wcsp->cubeface; break; case WCS_TYPES: for (i = 0; i < naxis; i++) { *(ivalp++) = wcsp->types[i]; } break; case WCS_LIN: /* Copy the contents of the linprm struct. */ iwcsp = (int *)(&(wcsp->lin)); for (k = 0; k < LINLEN; k++) { *(ivalp++) = *(iwcsp++); } break; case WCS_CEL: /* Copy the contents of the celprm struct. */ iwcsp = (int *)(&(wcsp->cel)); for (k = 0; k < CELLEN; k++) { *(ivalp++) = *(iwcsp++); } break; case WCS_SPC: /* Copy the contents of the spcprm struct. */ iwcsp = (int *)(&(wcsp->spc)); for (k = 0; k < SPCLEN; k++) { *(ivalp++) = *(iwcsp++); } break; case WCS_ERR: /* Copy the contents of the wcserr struct. */ if (wcsp->err) { iwcsp = (int *)(wcsp->err); for (k = 0; k < ERRLEN; k++) { *(ivalp++) = *(iwcsp++); } } else { for (k = 0; k < ERRLEN; k++) { *(ivalp++) = 0; } } break; default: return 1; } return 0; } int wcsgtc_(const int *wcs, const int *what, char *value) { return wcsget_(wcs, what, value); } int wcsgtd_(const int *wcs, const int *what, double *value) { return wcsget_(wcs, what, value); } int wcsgti_(const int *wcs, const int *what, int *value) { return wcsget_(wcs, what, value); } /*--------------------------------------------------------------------------*/ int wcsfree_(int *wcs) { return wcsfree((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int wcsprt_(int *wcs) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling WCSPRT in the Fortran code. */ fflush(NULL); return wcsprt((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ /* prefix should be null-terminated, or else of length 72 in which case * trailing blanks are not significant. */ int wcsperr_(int *wcs, const char prefix[72]) { char prefix_[72]; int i; strncpy(prefix_, prefix, 72); if (prefix_[71] == ' ') { for (i = 70; i >= 0; i--) { if (prefix_[i] != ' ') break; prefix_[i] = '\0'; } } else { prefix_[71] = '\0'; } /* This may or may not force the Fortran I/O buffers to be flushed. */ /* If not, try CALL FLUSH(6) before calling WCSPERR in the Fortran code. */ fflush(NULL); return wcsperr((struct wcsprm *)wcs, prefix_); } /*--------------------------------------------------------------------------*/ int wcsset_(int *wcs) { return wcsset((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int wcsp2s_( int *wcs, const int *ncoord, const int *nelem, const double pixcrd[], double imgcrd[], double phi[], double theta[], double world[], int stat[]) { return wcsp2s((struct wcsprm *)wcs, *ncoord, *nelem, pixcrd, imgcrd, phi, theta, world, stat); } /*--------------------------------------------------------------------------*/ int wcss2p_( int* wcs, const int *ncoord, const int *nelem, const double world[], double phi[], double theta[], double imgcrd[], double pixcrd[], int stat[]) { return wcss2p((struct wcsprm *)wcs, *ncoord, *nelem, world, phi, theta, imgcrd, pixcrd, stat); } /*--------------------------------------------------------------------------*/ int wcsmix_( int *wcs, const int *mixpix, const int *mixcel, const double vspan[2], const double *vstep, int *viter, double world[], double phi[], double theta[], double imgcrd[], double pixcrd[]) { return wcsmix((struct wcsprm *)wcs, *mixpix-1, *mixcel, vspan, *vstep, *viter, world, phi, theta, imgcrd, pixcrd); } /*--------------------------------------------------------------------------*/ int wcssptr_(struct wcsprm *wcs, int *i, char ctype[9]) { int status = wcssptr(wcs, i, ctype); wcsutil_blank_fill(9, ctype); return status; } pywcs-1.12/wcslib/Fortran/wcsfix.inc0000644001153600020070000000561212310355626021546 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcsfix.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL CDFIX, CELFIX, CYLFIX, DATFIX, SPCFIX, UNITFIX, WCSFIX INTEGER CDFIX, CELFIX, CYLFIX, DATFIX, SPCFIX, UNITFIX, WCSFIX * Flag bits for the RELAX argument. INTEGER WCSFIX_CD, WCSFIX_CEL, WCSFIX_CYL, WCSFIX_DAT, : WCSFIX_NWCS, WCSFIX_SPC, WCSFIX_UNIT PARAMETER (WCSFIX_CD = 1) PARAMETER (WCSFIX_DAT = 2) PARAMETER (WCSFIX_UNIT = 3) PARAMETER (WCSFIX_CEL = 4) PARAMETER (WCSFIX_SPC = 5) PARAMETER (WCSFIX_CYL = 6) PARAMETER (WCSFIX_NWCS = 6) * Error codes and messages. INTEGER FIXERR_BAD_COORD_TRANS, FIXERR_BAD_CORNER_PIX, : FIXERR_BAD_CTYPE, FIXERR_BAD_PARAM, : FIXERR_ILL_COORD_TRANS, FIXERR_MEMORY, FIXERR_NO_CHANGE, : FIXERR_NO_REF_PIX_COORD, FIXERR_NO_REF_PIX_VAL, : FIXERR_NULL_POINTER, FIXERR_SINGULAR_MTX, FIXERR_SUCCESS PARAMETER (FIXERR_NO_CHANGE = -1) PARAMETER (FIXERR_SUCCESS = 0) PARAMETER (FIXERR_NULL_POINTER = 1) PARAMETER (FIXERR_MEMORY = 2) PARAMETER (FIXERR_SINGULAR_MTX = 3) PARAMETER (FIXERR_BAD_CTYPE = 4) PARAMETER (FIXERR_BAD_PARAM = 5) PARAMETER (FIXERR_BAD_COORD_TRANS = 6) PARAMETER (FIXERR_ILL_COORD_TRANS = 7) PARAMETER (FIXERR_BAD_CORNER_PIX = 8) PARAMETER (FIXERR_NO_REF_PIX_COORD = 9) PARAMETER (FIXERR_NO_REF_PIX_VAL = 10) CHARACTER WCSFIX_ERRMSG(0:10)*80 COMMON /WCSFIX_DATA/ WCSFIX_ERRMSG pywcs-1.12/wcslib/Fortran/wcsfix_f.c0000644001153600020070000000560412310355626021525 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsfix_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include /* Fortran name mangling. */ #include #define wcsfix_ F77_FUNC(wcsfix, WCSFIX) #define cdfix_ F77_FUNC(cdfix, CDFIX) #define datfix_ F77_FUNC(datfix, DATFIX) #define unitfix_ F77_FUNC(unitfix, UNITFIX) #define celfix_ F77_FUNC(celfix, CELFIX) #define spcfix_ F77_FUNC(spcfix, SPCFIX) #define cylfix_ F77_FUNC(cylfix, CYLFIX) /*--------------------------------------------------------------------------*/ int wcsfix_(int *ctrl, const int naxis[], int *wcs, int stat[]) { if (*naxis == 0) naxis = 0x0; return wcsfix(*ctrl, naxis, (struct wcsprm *)wcs, stat); } /*--------------------------------------------------------------------------*/ int cdfix_(int *wcs) { return cdfix((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int datfix_(int *wcs) { return datfix((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int unitfix_(int *ctrl, int *wcs) { return unitfix(*ctrl, (struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int celfix_(int *wcs) { return celfix((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int spcfix_(int *wcs) { return spcfix((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int cylfix_(const int naxis[], int *wcs) { return cylfix(naxis, (struct wcsprm *)wcs); } pywcs-1.12/wcslib/Fortran/wcshdr.inc0000644001153600020070000000643112310355626021535 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcshdr.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL WCSBDX, WCSBTH, WCSIDX, WCSPIH, WCSTAB, WCSVCOPY, : WCSVFREE INTEGER WCSBDX, WCSBTH, WCSIDX, WCSPIH, WCSTAB, WCSVCOPY, : WCSVFREE * Flag bits for the RELAX argument. INTEGER WCSHDR_all, WCSHDR_ALLIMG, WCSHDR_AUXIMG, : WCSHDR_BIMGARR, WCSHDR_CD00i00j, WCSHDR_CNAMn, : WCSHDR_CROTAia, WCSHDR_DOBSn, WCSHDR_EPOCHa, : WCSHDR_IMGHEAD, WCSHDR_LONGKEY, WCSHDR_none, : WCSHDR_PC00i00j, WCSHDR_PIXLIST, WCSHDR_PROJPn, : WCSHDR_RADECSYS, WCSHDR_reject, WCSHDR_VELREFa, : WCSHDR_VSOURCE PARAMETER (WCSHDR_none = 0) PARAMETER (WCSHDR_all = 2**20 - 1) PARAMETER (WCSHDR_reject = 2**28) PARAMETER (WCSHDR_CROTAia = 2**0) PARAMETER (WCSHDR_EPOCHa = 2**1) PARAMETER (WCSHDR_VELREFa = 2**2) PARAMETER (WCSHDR_CD00i00j = 2**3) PARAMETER (WCSHDR_PC00i00j = 2**4) PARAMETER (WCSHDR_PROJPn = 2**5) PARAMETER (WCSHDR_RADECSYS = 2**6) PARAMETER (WCSHDR_VSOURCE = 2**7) PARAMETER (WCSHDR_DOBSn = 2**8) PARAMETER (WCSHDR_LONGKEY = 2**9) PARAMETER (WCSHDR_CNAMn = 2**10) PARAMETER (WCSHDR_AUXIMG = 2**11) PARAMETER (WCSHDR_ALLIMG = 2**12) PARAMETER (WCSHDR_IMGHEAD = 2**16) PARAMETER (WCSHDR_BIMGARR = 2**17) PARAMETER (WCSHDR_PIXLIST = 2**18) * Error codes and messages. INTEGER WCSHDRERR_BAD_TABULAR_PARAMS, WCSHDRERR_MEMORY, : WCSHDRERR_NULL_POINTER, WCSHDRERR_PARSER, : WCSHDRERR_SUCCESS PARAMETER (WCSHDRERR_SUCCESS = 0) PARAMETER (WCSHDRERR_NULL_POINTER = 1) PARAMETER (WCSHDRERR_MEMORY = 2) PARAMETER (WCSHDRERR_BAD_TABULAR_PARAMS = 3) PARAMETER (WCSHDRERR_PARSER = 4) CHARACTER WCSHDR_ERRMSG(0:3)*80 COMMON /WCSHDR_DATA/ WCSHDR_ERRMSG pywcs-1.12/wcslib/Fortran/wcshdr_f.c0000644001153600020070000001036212310355626021511 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcshdr_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include /* Fortran name mangling. */ #include #define wcspih_ F77_FUNC(wcspih, WCSPIH) #define wcsbth_ F77_FUNC(wcsbth, WCSBTH) #define wcstab_ F77_FUNC(wcstab, WCSTAB) #define wcsidx_ F77_FUNC(wcsidx, WCSIDX) #define wcsbdx_ F77_FUNC(wcsbdx, WCSBDX) #define wcsvcopy_ F77_FUNC(wcsvcopy, WCSVCOPY) #define wcsvfree_ F77_FUNC(wcsvfree, WCSVFREE) /*--------------------------------------------------------------------------*/ int wcspih_( char header[], const int *nkeys, const int *relax, const int *ctrl, int *nreject, int *nwcs, iptr wcsp) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling WCSPIH in the Fortran code. */ fflush(NULL); return wcspih(header, *nkeys, *relax, *ctrl, nreject, nwcs, (struct wcsprm **)wcsp); } /*--------------------------------------------------------------------------*/ int wcsbth_( char header[], const int *nkeys, const int *relax, const int *ctrl, const int *keysel, int *colsel, int *nreject, int *nwcs, iptr wcsp) { /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling WCSBTH in the Fortran code. */ fflush(NULL); return wcsbth(header, *nkeys, *relax, *ctrl, *keysel, colsel, nreject, nwcs, (struct wcsprm **)wcsp); } /*--------------------------------------------------------------------------*/ int wcstab_(int *wcs) { return wcstab((struct wcsprm *)wcs); } /*--------------------------------------------------------------------------*/ int wcsidx_(int *nwcs, iptr wcsp, int alts[27]) { return wcsidx(*nwcs, (struct wcsprm **)wcsp, alts); } /*--------------------------------------------------------------------------*/ int wcsbdx_(int *nwcs, iptr wcsp, int *type, short alts[1000][28]) { return wcsbdx(*nwcs, (struct wcsprm **)wcsp, *type, alts); } /*--------------------------------------------------------------------------*/ int wcsvcopy_(const iptr wcspp, const int *i, int *wcs) { struct wcsprm *wcsdst, *wcssrc; /* Do a shallow copy. */ wcssrc = *((struct wcsprm **)wcspp) + *i; wcsdst = (struct wcsprm *)wcs; *wcsdst = *wcssrc; /* Don't take memory. */ wcsdst->m_flag = 0; wcsdst->m_naxis = 0; wcsdst->m_crpix = 0x0; wcsdst->m_pc = 0x0; wcsdst->m_cdelt = 0x0; wcsdst->m_cunit = 0x0; wcsdst->m_ctype = 0x0; wcsdst->m_crval = 0x0; wcsdst->m_pv = 0x0; wcsdst->m_ps = 0x0; wcsdst->m_cd = 0x0; wcsdst->m_crota = 0x0; wcsdst->m_cname = 0x0; wcsdst->m_crder = 0x0; wcsdst->m_csyer = 0x0; wcsdst->m_wtb = 0x0; wcsdst->m_tab = 0x0; return 0; } /*--------------------------------------------------------------------------*/ int wcsvfree_(int *nwcs, iptr wcspp) { return wcsvfree(nwcs, (struct wcsprm **)wcspp); } pywcs-1.12/wcslib/Fortran/wcsunits.inc0000644001153600020070000001020612310355626022115 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * WCSLIB 4.10 - an implementation of the FITS WCS standard. * Copyright (C) 1995-2012, Mark Calabretta * * This file is part of WCSLIB. * * WCSLIB is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * WCSLIB is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with WCSLIB. If not, see http://www.gnu.org/licenses. * * Correspondence concerning WCSLIB may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcsunits.inc,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *======================================================================= * Functions. EXTERNAL WCSULEXE, WCSUNITSE, WCSUTRNE INTEGER WCSULEXE, WCSUNITSE, WCSUTRNE * Deprecated functions. EXTERNAL WCSULEX, WCSUNITS, WCSUTRN INTEGER WCSULEX, WCSUNITS, WCSUTRN * Array indices. INTEGER WCSUNITS_BEAM, WCSUNITS_BIN, WCSUNITS_BIT, : WCSUNITS_CHARGE, WCSUNITS_COUNT, WCSUNITS_LENGTH, : WCSUNITS_LUMINTEN, WCSUNITS_MAGNITUDE, WCSUNITS_MASS, : WCSUNITS_MOLE, WCSUNITS_NTYPE, WCSUNITS_PIXEL, : WCSUNITS_PLANE_ANGLE, WCSUNITS_SOLID_ANGLE, : WCSUNITS_SOLRATIO, WCSUNITS_TEMPERATURE, WCSUNITS_TIME, : WCSUNITS_VOXEL PARAMETER (WCSUNITS_PLANE_ANGLE = 1) PARAMETER (WCSUNITS_SOLID_ANGLE = 2) PARAMETER (WCSUNITS_CHARGE = 3) PARAMETER (WCSUNITS_MOLE = 4) PARAMETER (WCSUNITS_TEMPERATURE = 5) PARAMETER (WCSUNITS_LUMINTEN = 6) PARAMETER (WCSUNITS_MASS = 7) PARAMETER (WCSUNITS_LENGTH = 8) PARAMETER (WCSUNITS_TIME = 9) PARAMETER (WCSUNITS_BEAM = 10) PARAMETER (WCSUNITS_BIN = 11) PARAMETER (WCSUNITS_BIT = 12) PARAMETER (WCSUNITS_COUNT = 13) PARAMETER (WCSUNITS_MAGNITUDE = 14) PARAMETER (WCSUNITS_PIXEL = 15) PARAMETER (WCSUNITS_SOLRATIO = 16) PARAMETER (WCSUNITS_VOXEL = 17) PARAMETER (WCSUNITS_NTYPE = 17) CHARACTER WCSUNITS_ERRMSG(0:12)*40, : WCSUNITS_TYPES(WCSUNITS_NTYPE)*18, : WCSUNITS_UNITS(WCSUNITS_NTYPE)*9 * Error codes and messages. INTEGER UNITSERR_BAD_EXPON_SYMBOL, UNITSERR_BAD_FUNCS, : UNITSERR_BAD_INITIAL_SYMBOL, : UNITSERR_BAD_NUM_MULTIPLIER, UNITSERR_BAD_UNIT_SPEC, : UNITSERR_CONSEC_BINOPS, UNITSERR_DANGLING_BINOP, : UNITSERR_FUNCTION_CONTEXT, UNITSERR_PARSER_ERROR, : UNITSERR_SUCCESS, UNITSERR_UNBAL_BRACKET, : UNITSERR_UNBAL_PAREN, UNITSERR_UNSAFE_TRANS PARAMETER (UNITSERR_SUCCESS = 0) PARAMETER (UNITSERR_BAD_NUM_MULTIPLIER = 1) PARAMETER (UNITSERR_DANGLING_BINOP = 2) PARAMETER (UNITSERR_BAD_INITIAL_SYMBOL = 3) PARAMETER (UNITSERR_FUNCTION_CONTEXT = 4) PARAMETER (UNITSERR_BAD_EXPON_SYMBOL = 5) PARAMETER (UNITSERR_UNBAL_BRACKET = 6) PARAMETER (UNITSERR_UNBAL_PAREN = 7) PARAMETER (UNITSERR_CONSEC_BINOPS = 8) PARAMETER (UNITSERR_PARSER_ERROR = 9) PARAMETER (UNITSERR_BAD_UNIT_SPEC = 10) PARAMETER (UNITSERR_BAD_FUNCS = 11) PARAMETER (UNITSERR_UNSAFE_TRANS = 12) COMMON /WCSUNITS_DATA/ WCSUNITS_ERRMSG, WCSUNITS_TYPES, : WCSUNITS_UNITS pywcs-1.12/wcslib/Fortran/wcsunits_f.c0000644001153600020070000000770012310355626022100 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsunits_f.c,v 4.10 2012/02/05 23:41:44 cal103 Exp $ *===========================================================================*/ #include #include #include #include /* Fortran name mangling. */ #include #define wcsunitse_ F77_FUNC(wcsunitse, WCSUNITSE) #define wcsutrne_ F77_FUNC(wcsutrne, WCSUTRNE) #define wcsulexe_ F77_FUNC(wcsulexe, WCSULEXE) /* Deprecated. */ #define wcsunits_ F77_FUNC(wcsunits, WCSUNITS) #define wcsutrn_ F77_FUNC(wcsutrn, WCSUTRN) #define wcsulex_ F77_FUNC(wcsulex, WCSULEX) /*--------------------------------------------------------------------------*/ int wcsunitse_( const char have[72], const char want[72], double *scale, double *offset, double *power, iptr err) { char have_[72], want_[72]; strncpy(have_, have, 72); strncpy(want_, want, 72); have_[71] = '\0'; want_[71] = '\0'; return wcsunitse(have_, want_, scale, offset, power, (struct wcserr **)err); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int wcsunits_( const char have[72], const char want[72], double *scale, double *offset, double *power) { return wcsunitse_(have, want, scale, offset, power, 0x0); } /*--------------------------------------------------------------------------*/ int wcsutrne_( const int *ctrl, char unitstr[72], iptr err) { int status; char unitstr_[72]; strncpy(unitstr_, unitstr, 72); unitstr_[71] = '\0'; /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling WCSUTRNE in the Fortran code. */ fflush(NULL); status = wcsutrne(*ctrl, unitstr_, (struct wcserr **)err); wcsutil_blank_fill(72, unitstr_); strncpy(unitstr, unitstr_, 72); return status; } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int wcsutrn_( const int *ctrl, char unitstr[72]) { return wcsutrne_(ctrl, unitstr, 0x0); } /*--------------------------------------------------------------------------*/ int wcsulexe_( const char unitstr[72], int *func, double *scale, double units[WCSUNITS_NTYPE], iptr err) { char unitstr_[72]; strncpy(unitstr_, unitstr, 72); unitstr_[71] = '\0'; /* This may or may not force the Fortran I/O buffers to be flushed. If * not, try CALL FLUSH(6) before calling WCSULEXE in the Fortran code. */ fflush(NULL); return wcsulexe(unitstr_, func, scale, units, (struct wcserr **)err); } /* : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : : */ int wcsulex_( const char unitstr[72], int *func, double *scale, double units[WCSUNITS_NTYPE]) { return wcsulexe_(unitstr, func, scale, units, 0x0); } pywcs-1.12/wcslib/GNUmakefile0000644001153600020070000001451212310355626020206 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile for building WCSLIB 4.10 # # Summary of the main targets # --------------------------- # all: Do 'make all' in each subdirectory (excluding ./doxygen). # check: Do 'make check' in each subdirectory (compile and run tests). # tests: Do 'make tests' in each subdirectory (compile test programs but # don't run them). # install: Do 'make install' in each subdirectory. # clean: Recursively delete intermediate files produced as part of the # build, e.g. object modules, core dumps, etc. # cleaner: Recursively clean, and also delete test executables, test # input and output, and intermediates produced in compiling the # programmers' manual. # distclean (or realclean): Recursively delete all platform-dependent files # generated during the build, preserving only the programmers' # manual and man pages (which are normally provided pre-built). # It is the one to use between builds for multiple platforms. # cleanest: Like distclean, but deletes everything that can be regenerated # from the source files, including the programmers' manual and # man pages, but excluding 'configure'. # show: Print the values of important variables used in this and the # other makefiles. # writable: Run chmod recursively to make all sources writable. # # Notes: # 1) If you need to make changes then preferably modify makedefs.in instead. # # 2) Refer also to the makefiles in subdirectories, particularly # C/GNUmakefile. # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: GNUmakefile,v 4.10 2012/02/05 23:41:45 cal103 Exp $ #----------------------------------------------------------------------------- # Get configure settings. include makedefs ifeq "$(CHECK)" "nopgplot" TSTDIRS := $(filter-out pgsbox,$(TSTDIRS)) endif .PHONY : build check chmod clean cleaner cleanest distclean install \ realclean show tests writable build : -@ for DIR in $(SUBDIRS) ; do \ echo '' ; \ $(TIMER) ; \ $(MAKE) -k -C $$DIR build ; \ done check tests :: show -@ echo '' -@ $(TIMER) @ for DIR in $(SUBDIRS) ; do \ echo '' ; \ $(MAKE) -i -C $$DIR cleaner ; \ done -@ echo '' @ for DIR in $(TSTDIRS) ; do \ echo '' ; \ $(TIMER) ; \ $(MAKE) -k -C $$DIR $@ ; \ done check :: -@ echo '' -@ echo 'Summary of results for non-graphical tests' -@ echo '------------------------------------------' -@ cat ./*/test_results @ if grep 'FAIL:' ./*/test_results > /dev/null ; then \ exit 1 ; \ else \ exit 0 ; \ fi install : @ for DIR in $(INSTDIR) ; do \ $(MAKE) -k -C $$DIR $@ ; \ done $(INSTALL) -m 444 wcsconfig.h wcsconfig_f77.h $(INCDIR) - if [ ! -d "$(DOCDIR)" ] ; then \ $(INSTALL) -d -m 2775 $(DOCDIR) ; \ fi $(INSTALL) -m 444 CHANGES COPYING* README $(DOCDIR) - if [ ! -d "$(PDFDIR)" ] ; then \ $(INSTALL) -d -m 2775 $(PDFDIR) ; \ fi $(INSTALL) -m 444 wcslib.pdf $(PDFDIR) - if [ ! -d "$(HTMLDIR)/html" ] ; then \ $(INSTALL) -d -m 2775 $(HTMLDIR)/html ; \ fi $(INSTALL) -m 444 html/* $(HTMLDIR)/html if [ ! -d "$(LIBDIR)/pkgconfig" ] ; then \ $(INSTALL) -d -m 2775 $(LIBDIR)/pkgconfig ; \ fi $(INSTALL) -m 444 wcslib.pc $(LIBDIR)/pkgconfig/wcslib.pc clean cleaner : for DIR in $(SUBDIRS) doxygen ; do \ $(MAKE) -C $$DIR $@ ; \ done cleanest distclean realclean : for DIR in $(SUBDIRS) doxygen ; do \ $(MAKE) -C $$DIR $@ ; \ done - $(RM) *.log - $(RM) -r autom4te.cache autoscan.log - $(RM) confdefs.h conftest.* - $(RM) config.log config.status configure.lineno - $(RM) makedefs wcslib.pc - $(RM) wcsconfig.h wcsconfig_*.h - $(RM) wcslib-*.tar.gz show :: -@ echo 'Subdirectories to be built...' -@ echo ' SUBDIRS := $(SUBDIRS)' -@ echo ' TSTDIRS := $(TSTDIRS)' -@ echo '' writable : chmod -R u+w . GNUmakefile : makedefs ; makedefs : makedefs.in config.status -@ echo '' -@ $(TIMER) ./config.status config.status : configure -@ echo '' -@ $(TIMER) -@ echo '' -@ echo "Environment variables that affect 'configure':" -@ echo " CC = $${CC-(undefined)}" -@ echo " CFLAGS = $${CFLAGS-(undefined)}" -@ echo " CPP = $${CPP-(undefined)}" -@ echo " CPPFLAGS = $${CPPFLAGS-(undefined)}" -@ echo " F77 = $${F77-(undefined)}" -@ echo " FFLAGS = $${FFLAGS-(undefined)}" -@ echo " LDFLAGS = $${LDFLAGS-(undefined)}" -@ echo '' ./configure --no-create #----------------------------------------------------------------------------- # These are for code management. .PHONY : dist dist : $(MAKE) -C doxygen cleanest build $(MAKE) -C utils man $(MAKE) distclean -@ echo $(WCSLIBPKG)/C/RCS > wcslib.X -@ echo $(WCSLIBPKG)/C/flexed/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/C/test/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/doxygen/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/Fortran/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/Fortran/test/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/makedefs >> wcslib.X -@ echo $(WCSLIBPKG)/other >> wcslib.X -@ echo $(WCSLIBPKG)/pgsbox/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/TODO >> wcslib.X -@ echo $(WCSLIBPKG)/utils/RCS >> wcslib.X -@ echo $(WCSLIBPKG)/wcslib.T >> wcslib.X -@ echo $(WCSLIBPKG)/wcslib.X >> wcslib.X rm -f $(WCSLIBPKG).tar.bz2 tar cf - -C .. -X wcslib.X $(WCSLIBPKG) | \ tar t | \ grep -v '/$$' | \ sort > wcslib.T rm -f wcslib.X tar cvf $(WCSLIBPKG).tar -C .. -T wcslib.T rm -f wcslib.T bzip2 $(WCSLIBPKG).tar chmod 444 $(WCSLIBPKG).tar.bz2 install_dist : cp -fp $(WCSLIBPKG).tar.bz2 /nfs/ftp/software/wcslib/ mv -f $(WCSLIBPKG).tar.bz2 ../wcslib-releases/ (cd /nfs/ftp/software/wcslib/ && \ rm -f wcslib.tar.bz2 && \ ln -s $(WCSLIBPKG).tar.bz2 wcslib.tar.bz2) cp -fp CHANGES wcslib.pdf ~/public_html/WCS/ rsync --archive --delete html/ ~/public_html/WCS/wcslib/ configure : configure.ac -@ echo '' -@ $(TIMER) autoconf # Code development overrides must be included specifically before 'configure' # generates makedefs. -include flavours pywcs-1.12/wcslib/html/0000755001153600020070000000000012310355732017073 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/html/annotated.html0000644001153600020070000000636612310355626021753 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Structures

      Data Structures

      Here are the data structures with brief descriptions:
      celprmCelestial transformation parameters
      fitskeyKeyword/value information
      fitskeyidKeyword indexing
      linprmLinear transformation parameters
      prjprmProjection parameters
      pscardStore for PSi_ma keyrecords
      pvcardStore for PVi_ma keyrecords
      spcprmSpectral transformation parameters
      spxprmSpectral variables and their derivatives
      tabprmTabular transformation parameters
      wcserrError message handling
      wcsprmCoordinate transformation parameters
      wtbarrExtraction of coordinate lookup tables from BINTABLE
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
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      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/cel_8h.html0000644001153600020070000010775712310355626021146 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: cel.h File Reference

      cel.h File Reference

      #include "prj.h"
      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  celprm
       Celestial transformation parameters. More...

      Defines

      #define CELLEN   (sizeof(struct celprm)/sizeof(int))
       Size of the celprm struct in int units.
      #define celini_errmsg   cel_errmsg
       Deprecated.
      #define celprt_errmsg   cel_errmsg
       Deprecated.
      #define celset_errmsg   cel_errmsg
       Deprecated.
      #define celx2s_errmsg   cel_errmsg
       Deprecated.
      #define cels2x_errmsg   cel_errmsg
       Deprecated.

      Enumerations

      enum  cel_errmsg_enum {
        CELERR_SUCCESS = 0, CELERR_NULL_POINTER = 1, CELERR_BAD_PARAM = 2, CELERR_BAD_COORD_TRANS = 3,
        CELERR_ILL_COORD_TRANS = 4, CELERR_BAD_PIX = 5, CELERR_BAD_WORLD = 6
      }

      Functions

      int celini (struct celprm *cel)
       Default constructor for the celprm struct.
      int celfree (struct celprm *cel)
       Destructor for the celprm struct.
      int celprt (const struct celprm *cel)
       Print routine for the celprm struct.
      int celset (struct celprm *cel)
       Setup routine for the celprm struct.
      int celx2s (struct celprm *cel, int nx, int ny, int sxy, int sll, const double x[], const double y[], double phi[], double theta[], double lng[], double lat[], int stat[])
       Pixel-to-world celestial transformation.
      int cels2x (struct celprm *cel, int nlng, int nlat, int sll, int sxy, const double lng[], const double lat[], double phi[], double theta[], double x[], double y[], int stat[])
       World-to-pixel celestial transformation.

      Variables

      const char * cel_errmsg []

      Detailed Description

      These routines implement the part of the FITS World Coordinate System (WCS) standard that deals with celestial coordinates. They define methods to be used for computing celestial world coordinates from intermediate world coordinates (a linear transformation of image pixel coordinates), and vice versa. They are based on the celprm struct which contains all information needed for the computations. This struct contains some elements that must be set by the user, and others that are maintained by these routines, somewhat like a C++ class but with no encapsulation.

      Routine celini() is provided to initialize the celprm struct with default values, celfree() reclaims any memory that may have been allocated to store an error message, and celprt() prints its contents.

      A setup routine, celset(), computes intermediate values in the celprm struct from parameters in it that were supplied by the user. The struct always needs to be set up by celset() but it need not be called explicitly - refer to the explanation of celprm::flag.

      celx2s() and cels2x() implement the WCS celestial coordinate transformations. In fact, they are high level driver routines for the lower level spherical coordinate rotation and projection routines described in sph.h and prj.h.

      Define Documentation

      #define CELLEN   (sizeof(struct celprm)/sizeof(int))

      Size of the celprm struct in int units, used by the Fortran wrappers.

      #define celini_errmsg   cel_errmsg

      Deprecated:
      Added for backwards compatibility, use cel_errmsg directly now instead.

      #define celprt_errmsg   cel_errmsg

      Deprecated:
      Added for backwards compatibility, use cel_errmsg directly now instead.

      #define celset_errmsg   cel_errmsg

      Deprecated:
      Added for backwards compatibility, use cel_errmsg directly now instead.

      #define celx2s_errmsg   cel_errmsg

      Deprecated:
      Added for backwards compatibility, use cel_errmsg directly now instead.

      #define cels2x_errmsg   cel_errmsg

      Deprecated:
      Added for backwards compatibility, use cel_errmsg directly now instead.

      Enumeration Type Documentation

      enum cel_errmsg_enum

      Enumerator:
      CELERR_SUCCESS 
      CELERR_NULL_POINTER 
      CELERR_BAD_PARAM 
      CELERR_BAD_COORD_TRANS 
      CELERR_ILL_COORD_TRANS 
      CELERR_BAD_PIX 
      CELERR_BAD_WORLD 

      Function Documentation

      int celini ( struct celprm *  cel  ) 

      celini() sets all members of a celprm struct to default values. It should be used to initialize every celprm struct.

      Parameters:
      [out] cel Celestial transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null celprm pointer passed.

      int celfree ( struct celprm *  cel  ) 

      celfree() frees any memory that may have been allocated to store an error message in the celprm struct.

      Parameters:
      [in] cel Celestial transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null celprm pointer passed.

      int celprt ( const struct celprm *  cel  ) 

      celprt() prints the contents of a celprm struct using wcsprintf(). Mainly intended for diagnostic purposes.

      Parameters:
      [in] cel Celestial transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null celprm pointer passed.

      int celset ( struct celprm *  cel  ) 

      celset() sets up a celprm struct according to information supplied within it.

      Note that this routine need not be called directly; it will be invoked by celx2s() and cels2x() if celprm::flag is anything other than a predefined magic value.

      Parameters:
      [in,out] cel Celestial transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null celprm pointer passed.
      • 2: Invalid projection parameters.
      • 3: Invalid coordinate transformation parameters.
      • 4: Ill-conditioned coordinate transformation parameters.
      For returns > 1, a detailed error message is set in celprm::err if enabled, see wcserr_enable().

      int celx2s ( struct celprm *  cel,
      int  nx,
      int  ny,
      int  sxy,
      int  sll,
      const double  x[],
      const double  y[],
      double  phi[],
      double  theta[],
      double  lng[],
      double  lat[],
      int  stat[] 
      )

      celx2s() transforms $(x,y)$ coordinates in the plane of projection to celestial coordinates $(\alpha,\delta)$.

      Parameters:
      [in,out] cel Celestial transformation parameters.
      [in] nx,ny Vector lengths.
      [in] sxy,sll Vector strides.
      [in] x,y Projected coordinates in pseudo "degrees".
      [out] phi,theta Longitude and latitude $(\phi,\theta)$ in the native coordinate system of the projection [deg].
      [out] lng,lat Celestial longitude and latitude $(\alpha,\delta)$ of the projected point [deg].
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of $(x,y)$.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null celprm pointer passed.
      • 2: Invalid projection parameters.
      • 3: Invalid coordinate transformation parameters.
      • 4: Ill-conditioned coordinate transformation parameters.
      • 5: One or more of the $(x,y)$ coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in celprm::err if enabled, see wcserr_enable().

      int cels2x ( struct celprm *  cel,
      int  nlng,
      int  nlat,
      int  sll,
      int  sxy,
      const double  lng[],
      const double  lat[],
      double  phi[],
      double  theta[],
      double  x[],
      double  y[],
      int  stat[] 
      )

      cels2x() transforms celestial coordinates $(\alpha,\delta)$ to $(x,y)$ coordinates in the plane of projection.

      Parameters:
      [in,out] cel Celestial transformation parameters.
      [in] nlng,nlat Vector lengths.
      [in] sll,sxy Vector strides.
      [in] lng,lat Celestial longitude and latitude $(\alpha,\delta)$ of the projected point [deg].
      [out] phi,theta Longitude and latitude $(\phi,\theta)$ in the native coordinate system of the projection [deg].
      [out] x,y Projected coordinates in pseudo "degrees".
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of $(\alpha,\delta)$.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null celprm pointer passed.
      • 2: Invalid projection parameters.
      • 3: Invalid coordinate transformation parameters.
      • 4: Ill-conditioned coordinate transformation parameters.
      • 6: One or more of the $(\alpha,\delta)$ coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in celprm::err if enabled, see wcserr_enable().

      Variable Documentation

      const char* cel_errmsg[]

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/deprecated.html0000644001153600020070000003471412310355626022074 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Deprecated List

      Deprecated List

      Global celini_errmsg
      Added for backwards compatibility, use cel_errmsg directly now instead.

      Global celprt_errmsg
      Added for backwards compatibility, use cel_errmsg directly now instead.

      Global celset_errmsg
      Added for backwards compatibility, use cel_errmsg directly now instead.

      Global celx2s_errmsg
      Added for backwards compatibility, use cel_errmsg directly now instead.

      Global cels2x_errmsg
      Added for backwards compatibility, use cel_errmsg directly now instead.

      Global FITSHDR_CARD
      Added for backwards compatibility, use FITSHDR_KEYREC instead.

      Global linini_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global lincpy_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global linfree_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global linprt_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global linset_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global linp2x_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global linx2p_errmsg
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Global prjini_errmsg
      Added for backwards compatibility, use prj_errmsg directly now instead.

      Global prjprt_errmsg
      Added for backwards compatibility, use prj_errmsg directly now instead.

      Global prjset_errmsg
      Added for backwards compatibility, use prj_errmsg directly now instead.

      Global prjx2s_errmsg
      Added for backwards compatibility, use prj_errmsg directly now instead.

      Global prjs2x_errmsg
      Added for backwards compatibility, use prj_errmsg directly now instead.

      Global spcini_errmsg
      Added for backwards compatibility, use spc_errmsg directly now instead.

      Global spcprt_errmsg
      Added for backwards compatibility, use spc_errmsg directly now instead.

      Global spcset_errmsg
      Added for backwards compatibility, use spc_errmsg directly now instead.

      Global spcx2s_errmsg
      Added for backwards compatibility, use spc_errmsg directly now instead.

      Global spcs2x_errmsg
      Added for backwards compatibility, use spc_errmsg directly now instead.

      Global tabini_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global tabcpy_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global tabfree_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global tabprt_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global tabset_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global tabx2s_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global tabs2x_errmsg
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Global wcsini_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcssub_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcscopy_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcsfree_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcsprt_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcsset_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcsp2s_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcss2p_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global wcsmix_errmsg
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Global cylfix_errmsg
      Added for backwards compatibility, use wcsfix_errmsg directly now instead.
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
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      File List

      Here is a list of all files with brief descriptions:
      cel.h [code]
      fitshdr.h [code]
      getwcstab.h [code]
      lin.h [code]
      log.h [code]
      prj.h [code]
      spc.h [code]
      sph.h [code]
      spx.h [code]
      tab.h [code]
      wcs.h [code]
      wcserr.h [code]
      wcsfix.h [code]
      wcshdr.h [code]
      wcslib.h [code]
      wcsmath.h [code]
      wcsprintf.h [code]
      wcstrig.h [code]
      wcsunits.h [code]
      wcsutil.h [code]
      Generated on Mon Feb 6 10:41:58 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/fitshdr_8h-source.html0000644001153600020070000014123112310355626023325 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: fitshdr.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/fitshdr_8h.html0000644001153600020070000005472712310355626022044 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: fitshdr.h File Reference

      fitshdr.h File Reference

      #include "wcsconfig.h"

      Go to the source code of this file.

      Data Structures

      struct  fitskeyid
       Keyword indexing. More...
      struct  fitskey
       Keyword/value information. More...

      Defines

      #define FITSHDR_KEYWORD   0x01
       Flag bit indicating illegal keyword syntax.
      #define FITSHDR_KEYVALUE   0x02
       Flag bit indicating illegal keyvalue syntax.
      #define FITSHDR_COMMENT   0x04
       Flag bit indicating illegal keycomment syntax.
      #define FITSHDR_KEYREC   0x08
       Flag bit indicating illegal keyrecord.
      #define FITSHDR_CARD   0x08
       Deprecated.
      #define FITSHDR_TRAILER   0x10
       Flag bit indicating keyrecord following a valid END keyrecord.
      #define KEYIDLEN   (sizeof(struct fitskeyid)/sizeof(int))
      #define KEYLEN   (sizeof(struct fitskey)/sizeof(int))

      Typedefs

      typedef int int64 [3]
       64-bit signed integer data type.

      Functions

      int fitshdr (const char header[], int nkeyrec, int nkeyids, struct fitskeyid keyids[], int *nreject, struct fitskey **keys)
       FITS header parser routine.

      Variables

      const char * fitshdr_errmsg []
       Status return messages.

      Detailed Description

      fitshdr() is a generic FITS header parser provided to handle keyrecords that are ignored by the WCS header parsers, wcspih() and wcsbth(). Typically the latter may be set to remove WCS keyrecords from a header leaving fitshdr() to handle the remainder.

      Define Documentation

      #define FITSHDR_KEYWORD   0x01

      Bit mask for the status flag bit-vector returned by fitshdr() indicating illegal keyword syntax.

      #define FITSHDR_KEYVALUE   0x02

      Bit mask for the status flag bit-vector returned by fitshdr() indicating illegal keyvalue syntax.

      #define FITSHDR_COMMENT   0x04

      Bit mask for the status flag bit-vector returned by fitshdr() indicating illegal keycomment syntax.

      #define FITSHDR_KEYREC   0x08

      Bit mask for the status flag bit-vector returned by fitshdr() indicating an illegal keyrecord, e.g. an END keyrecord with trailing text.

      #define FITSHDR_CARD   0x08

      Deprecated:
      Added for backwards compatibility, use FITSHDR_KEYREC instead.

      #define FITSHDR_TRAILER   0x10

      Bit mask for the status flag bit-vector returned by fitshdr() indicating a keyrecord following a valid END keyrecord.

      #define KEYIDLEN   (sizeof(struct fitskeyid)/sizeof(int))

      #define KEYLEN   (sizeof(struct fitskey)/sizeof(int))

      Typedef Documentation

      int64

      64-bit signed integer data type defined via preprocessor macro WCSLIB_INT64 which may be defined in wcsconfig.h. For example

         #define WCSLIB_INT64 long long int

      This is typedef'd in fitshdr.h as

         #ifdef WCSLIB_INT64
     typedef WCSLIB_INT64 int64;
   #else
     typedef int int64[3];
   #endif

      See fitskey::type.

      Function Documentation

      int fitshdr ( const char  header[],
      int  nkeyrec,
      int  nkeyids,
      struct fitskeyid  keyids[],
      int *  nreject,
      struct fitskey **  keys 
      )

      fitshdr() parses a character array containing a FITS header, extracting all keywords and their values into an array of fitskey structs.

      Parameters:
      [in] header Character array containing the (entire) FITS header, for example, as might be obtained conveniently via the CFITSIO routine fits_hdr2str().
      Each header "keyrecord" (formerly "card image") consists of exactly 80 7-bit ASCII printing characters in the range 0x20 to 0x7e (which excludes NUL, BS, TAB, LF, FF and CR) especially noting that the keyrecords are NOT null-terminated.
      [in] nkeyrec Number of keyrecords in header[].
      [in] nkeyids Number of entries in keyids[].
      [in,out] keyids While all keywords are extracted from the header, keyids[] provides a convienient way of indexing them. The fitskeyid struct contains three members; fitskeyid::name must be set by the user while fitskeyid::count and fitskeyid::name are returned by fitshdr(). All matched keywords will have their fitskey::keyno member negated.
      [out] nreject Number of header keyrecords rejected for syntax errors.
      [out] keys Pointer to an array of nkeyrec fitskey structs containing all keywords and keyvalues extracted from the header.
      Memory for the array is allocated by fitshdr() and this must be freed by the user by invoking free() on the array.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null fitskey pointer passed.
      • 2: Memory allocation failed.
      • 3: Fatal error returned by Flex parser.
      Notes:
      1. Keyword parsing is done in accordance with the syntax defined by NOST 100-2.0, noting the following points in particular:

        1. Sect. 5.1.2.1 specifies that keywords be left-justified in columns 1-8, blank-filled with no embedded spaces, composed only of the ASCII characters ABCDEFGHJKLMNOPQRSTUVWXYZ0123456789-_

          fitshdr() accepts any characters in columns 1-8 but flags keywords that do not conform to standard syntax.

        2. Sect. 5.1.2.2 defines the "value indicator" as the characters ''= '' occurring in columns 9 and 10. If these are absent then the keyword has no value and columns 9-80 may contain any ASCII text (but see note 2 for CONTINUE keyrecords). This is copied to the comment member of the fitskey struct.

        3. Sect. 5.1.2.3 states that a keyword may have a null (undefined) value if the value/comment field, columns 11-80, consists entirely of spaces, possibly followed by a comment.

        4. Sect. 5.1.1 states that trailing blanks in a string keyvalue are not significant and the parser always removes them. A string containing nothing but blanks will be replaced with a single blank.

          Sect. 5.2.1 also states that a quote character (') in a string value is to be represented by two successive quote characters and the parser removes the repeated quote.

        5. The parser recognizes free-format character (NOST 100-2.0, Sect. 5.2.1), integer (Sect. 5.2.3), and floating-point values (Sect. 5.2.4) for all keywords.

        6. Sect. 5.2.3 offers no comment on the size of an integer keyvalue except indirectly in limiting it to 70 digits. The parser will translates an integer keyvalue to a 32-bit signed integer if it lies in the range -2147483648 to +2147483647, otherwise it interprets it as a 64-bit signed integer if possible, or else a "very long" integer (see fitskey::type).

        7. END not followed by 77 blanks is not considered to be a legitimate end keyrecord.

      2. The parser supports a generalization of the OGIP Long String Keyvalue Convention (v1.0) whereby strings may be continued onto successive header keyrecords. A keyrecord contains a segment of a continued string if and only if

        1. it contains the pseudo-keyword CONTINUE,

        2. columns 9 and 10 are both blank,

        3. columns 11 to 80 contain what would be considered a valid string keyvalue, including optional keycomment, if column 9 had contained '=',

        4. the previous keyrecord contained either a valid string keyvalue or a valid CONTINUE keyrecord.

        If any of these conditions is violated, the keyrecord is considered in isolation.

        Syntax errors in keycomments in a continued string are treated more permissively than usual; the '/' delimiter may be omitted provided that parsing of the string keyvalue is not compromised. However, the FITSHDR_COMMENT status bit will be set for the keyrecord (see fitskey::status).

        As for normal strings, trailing blanks in a continued string are not significant.

        In the OGIP convention "the '&' character is used as the last non-blank character of the string to indicate that the string is (probably) continued on the following keyword". This additional syntax is not required by fitshdr(), but if '&' does occur as the last non-blank character of a continued string keyvalue then it will be removed, along with any trailing blanks. However, blanks that occur before the '&' will be preserved.

      Variable Documentation

      const char * fitshdr_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
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K_M)$ \form#60:$\leq$ \form#61:$K_1 K_2 \ldots K_M$ \form#62:$\Upsilon_m$ \form#63:$K_1$ \form#64:$\le$ \form#65:$\pi/180^\circ$ \form#66:$\sqrt{2}$ \form#67:$1/\sqrt{2}$ \form#68:$\beta$ \form#69:$(\rho,\beta)$ \form#70:$\arg(x,y)$ \form#71:$v$ \form#72:$1 < |v| < 1 + WCSTRIG\_TOL$ \form#73:$|v| == 1$ \form#74:$10^6$ pywcs-1.12/wcslib/html/fortran.html0000644001153600020070000002134212310355626021440 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: WCSLIB Fortran wrappers

      WCSLIB Fortran wrappers

      The Fortran subdirectory contains wrappers, written in C, that allow Fortran programs to use WCSLIB.

      A prerequisite for using the wrappers is an understanding of the usage of the associated C routines, in particular the data structures they are based on. The principle difficulty in creating the wrappers was the need to manage these C structs from within Fortran, particularly as they contain pointers to allocated memory, pointers to C functions, and other structs that themselves contain similar entities.

      To this end, routines have been provided to set and retrieve values of the various structs, for example WCSPUT and WCSGET for the wcsprm struct, and CELPUT and CELGET for the celprm struct. These must be used in conjunction with wrappers on the routines provided to manage the structs in C, for example WCSINI, WCSSUB, WCSCOPY, WCSFREE, and WCSPRT which wrap wcsini(), wcssub(), wcscopy(), wcsfree(), and wcsprt().

      The various *PUT and *GET routines are based on codes defined in Fortran include files (*.inc), if your Fortran compiler does not support the INCLUDE statement then you will need to include these manually wherever necessary. Codes are defined as parameters with names like WCS_CRPIX which refers to wcsprm::crpix (if your Fortran compiler does not support long symbolic names then you will need to rename these).

      The include files also contain parameters, such as WCSLEN, that define the length of an INTEGER array that must be declared to hold the struct. This length may differ for different platforms depending on how the C compiler aligns data within the structs. A test program for the C library, twcs, prints the size of the struct in sizeof(int) units and the values in the Fortran include files must equal or exceed these. On some platforms, such as Suns, it is important that the start of the INTEGER array be aligned on a DOUBLE PRECISION boundary, otherwise a BUS error may result. This may be achieved via an EQUIVALENCE with a DOUBLE PRECISION variable, or by sequencing variables in a COMMON block so that the INTEGER array follows immediately after a DOUBLE PRECISION variable.

      The *PUT routines set only one element of an array at a time; the final one or two integer arguments of these routines specify 1-relative array indices (N.B. not 0-relative as in C). The one exception is the prjprm::pv array.

      The *PUT routines also reset the flag element to signal that the struct needs to be reinitialized. Therefore, if you wanted to set wcsprm::flag itself to -1 prior to the first call to WCSINI, for example, then that WCSPUT must be the last one before the call.

      The *GET routines retrieve whole arrays at a time and expect array arguments of the appropriate length where necessary. Note that they do not initialize the structs.

      A basic coding fragment is

            INTEGER   LNGIDX, STATUS
      CHARACTER CTYPE1*72

      INCLUDE 'wcs.inc'

*     WCSLEN is defined as a parameter in wcs.inc.
      INTEGER   WCS(WCSLEN)
      DOUBLE PRECISION DUMMY
      EQUIVALENCE (WCS, DUMMY)

*     Allocate memory and set default values for 2 axes.
      STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0)
      STATUS = WCSINI (2, WCS)

*     Set CRPIX1, and CRPIX2; WCS_CRPIX is defined in wcs.inc.
      STATUS = WCSPUT (WCS, WCS_CRPIX, 512D0, 1, 0)
      STATUS = WCSPUT (WCS, WCS_CRPIX, 512D0, 2, 0)

*     Set PC1_2 to 5.0 (I = 1, J = 2).
      STATUS = WCSPUT (WCS, WCS_PC, 5D0, 1, 2)

*     Set CTYPE1 to 'RA---SIN'; N.B. must be given as CHARACTER*72.
      CTYPE1 = 'RA---SIN'
      STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE1, 1, 0)

*     Set PV1_3 to -1.0 (I = 1, M = 3).
      STATUS = WCSPUT (WCS, WCS_PV, -1D0, 1, 3)

      etc.

*     Initialize.
      STATUS = WCSSET (WCS)
      IF (STATUS.NE.0) THEN
        CALL FLUSH(6)
        STATUS = WCSPERR(WCS, CHAR(0))
      ENDIF

*     Find the "longitude" axis.
      STATUS = WCSGET (WCS, WCS_LNG, LNGIDX)

*     Free memory.
      STATUS = WCSFREE (WCS)

      Refer to the various Fortran test programs for further programming examples. In particular, twcs and twcsmix show how to retrieve elements of the celprm and prjprm structs contained within the wcsprm struct.

      Note that the data type of the third argument to the *PUT and *GET routines differs depending on the data type of the corresponding C struct member, be it int, double, or char[]. It is essential that the Fortran data type match that of the C struct for int and double types, and be a CHARACTER variable of the correct length for char[] types. Compilers (e.g. g77) may warn of inconsistent usage of this argument but this can (usually) be safely ignored. If these warnings become annoying, type-specific variants are provided for each of the *PUT routines, *PTI, *PTD, and *PTC for int, double, or char[] and likewise *GTI, *GTD, and *GTC for the *GET routines.

      When calling wrappers for C functions that print to stdout, such as WCSPRT, and WCSPERR, or that may print to stderr, such as WCSPIH, WCSBTH, WCSULEXE, or WCSUTRNE, it may be necessary to flush the Fortran I/O buffers beforehand so that the output appears in the correct order. The wrappers for these functions do call fflush(NULL), but depending on the particular system, this may not succeed in flushing the Fortran I/O buffers. Most Fortran compilers provide the non-standard intrinsic FLUSH(), which is called with unit number 6 to flush stdout (as in the example above), and unit 0 for stderr.

      A basic assumption made by the wrappers is that an INTEGER variable is no less than half the size of a DOUBLE PRECISION.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/functions.html0000644001153600020070000000733112310355626021777 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - a -

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      pywcs-1.12/wcslib/html/functions_0x62.html0000644001153600020070000000667612310355626022571 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - b -

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      pywcs-1.12/wcslib/html/functions_0x63.html0000644001153600020070000001320112310355626022550 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - c -

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/functions_0x64.html0000644001153600020070000001436212310355626022562 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - d -

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/functions_0x65.html0000644001153600020070000001113512310355626022556 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - e -

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      pywcs-1.12/wcslib/html/functions_0x66.html0000644001153600020070000001020212310355626022551 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - f -

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/functions_0x67.html0000644001153600020070000000654012310355626022564 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - g -

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/functions_0x69.html0000644001153600020070000001024012310355626022556 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
      Here is a list of all struct and union fields with links to the structures/unions they belong to:

      - i -

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/functions_0x6b.html0000644001153600020070000000763712310355626022647 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Data Fields
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      getwcstab.h File Reference

      #include <fitsio.h>

      Go to the source code of this file.

      Data Structures

      struct  wtbarr
       Extraction of coordinate lookup tables from BINTABLE. More...

      Functions

      int fits_read_wcstab (fitsfile *fptr, int nwtb, wtbarr *wtb, int *status)
       FITS 'TAB' table reading routine.

      Detailed Description

      fits_read_wcstab(), an implementation of a FITS table reading routine for 'TAB' coordinates, is provided for CFITSIO programmers. It has been incorporated into CFITSIO as of v3.006 with the definitions in this file, getwcstab.h, moved into fitsio.h.

      fits_read_wcstab() is not included in the WCSLIB object library but the source code is presented here as it may be useful for programmers using an older version of CFITSIO than 3.006, or as a programming template for non-CFITSIO programmers.

      Function Documentation

      int fits_read_wcstab ( fitsfile *  fptr,
      int  nwtb,
      wtbarr *  wtb,
      int *  status 
      )

      fits_read_wcstab() extracts arrays from a binary table required in constructing 'TAB' coordinates.

      Parameters:
      [in] fptr Pointer to the file handle returned, for example, by the fits_open_file() routine in CFITSIO.
      [in] nwtb Number of arrays to be read from the binary table(s).
      [in,out] wtb Address of the first element of an array of wtbarr typedefs. This wtbarr typedef is defined to match the wtbarr struct defined in WCSLIB. An array of such structs returned by the WCSLIB function wcstab() as discussed in the notes below.
      [out] status CFITSIO status value.
      Returns:
      CFITSIO status value.
      Notes:
      In order to maintain WCSLIB and CFITSIO as independent libraries it is not permissible for any CFITSIO library code to include WCSLIB header files, or vice versa. However, the CFITSIO function fits_read_wcstab() accepts an array of wtbarr structs defined in wcs.h within WCSLIB.

      The problem therefore is to define the wtbarr struct within fitsio.h without including wcs.h, especially noting that wcs.h will often (but not always) be included together with fitsio.h in an applications program that uses fits_read_wcstab().

      The solution adopted is for WCSLIB to define "struct wtbarr" while fitsio.h defines "typedef wtbarr" as an untagged struct with identical members. This allows both wcs.h and fitsio.h to define a wtbarr data type without conflict by virtue of the fact that structure tags and typedef names share different name spaces in C; Appendix A, Sect. A11.1 (p227) of the K&R ANSI edition states that:

      Identifiers fall into several name spaces that do not interfere with one another; the same identifier may be used for different purposes, even in the same scope, if the uses are in different name spaces. These classes are: objects, functions, typedef names, and enum constants; labels; tags of structures, unions, and enumerations; and members of each structure or union individually.

      Therefore, declarations within WCSLIB look like 

            struct wtbarr *w;

      while within CFITSIO they are simply 

            wtbarr *w;

      As suggested by the commonality of the names, these are really the same aggregate data type. However, in passing a (struct wtbarr *) to fits_read_wcstab() a cast to (wtbarr *) is formally required.

      When using WCSLIB and CFITSIO together in C++ the situation is complicated by the fact that typedefs and structs share the same namespace; C++ Annotated Reference Manual, Sect. 7.1.3 (p105). In that case the wtbarr struct in wcs.h is renamed by preprocessor macro substitution to wtbarr_s to distinguish it from the typedef defined in fitsio.h. However, the scope of this macro substitution is limited to wcs.h itself and CFITSIO programmer code, whether in C++ or C, should always use the wtbarr typedef.

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      Here is a list of all functions, variables, defines, enums, and typedefs with links to the files they belong to:

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      Generated on Mon Feb 6 10:41:58 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/index.html0000644001153600020070000000612012310355626021071 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: WCSLIB 4.10 and PGSBOX 4.10

      WCSLIB 4.10 and PGSBOX 4.10

      Bonne.gif

      Bonne's projection

      Contents

      Copyright

        WCSLIB 4.10 - an implementation of the FITS WCS standard.
  Copyright (C) 1995-2012, Mark Calabretta

  WCSLIB is free software: you can redistribute it and/or modify it under the
  terms of the GNU Lesser General Public License as published by the Free
  Software Foundation, either version 3 of the License, or (at your option)
  any later version.

  WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY
  WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS
  FOR A PARTICULAR PURPOSE.  See the GNU Lesser General Public License for
  more details.

  You should have received a copy of the GNU Lesser General Public License
  along with WCSLIB.  If not, see <http://www.gnu.org/licenses/>.

  Correspondence concerning WCSLIB may be directed to:
    Internet email: mcalabre@atnf.csiro.au
    Postal address: Dr. Mark Calabretta
                    Australia Telescope National Facility, CSIRO
                    PO Box 76
                    Epping NSW 1710
                    AUSTRALIA
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/intro.html0000644001153600020070000000626212310355626021124 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Introduction

      Introduction

      WCSLIB is a C library, supplied with a full set of Fortran wrappers, that implements the "World Coordinate System" (WCS) standard in FITS (Flexible Image Transport System). It also includes a PGPLOT-based routine, PGSBOX, for drawing general curvilinear coordinate graticules and a number of utility programs.

      The FITS data format is widely used within the international astronomical community, from the radio to gamma-ray regimes, for data interchange and archive, and also increasingly as an online format. It is described in

      • "Definition of The Flexible Image Transport System (FITS)", FITS Standard, Version 3.0, 2008 July 10.

      available from the FITS Support Office at http://fits.gsfc.nasa.gov.

      The FITS WCS standard is described in

      • "Representations of world coordinates in FITS" (Paper I), Greisen, E.W., & Calabretta, M.R. 2002, A&A, 395, 1061-1075

      • "Representations of celestial coordinates in FITS" (Paper II), Calabretta, M.R., & Greisen, E.W. 2002, A&A, 395, 1077-1122

      • "Representations of spectral coordinates in FITS" (Paper III), Greisen, E.W., Calabretta, M.R., Valdes, F.G., & Allen, S.L. 2006, A&A, 446, 747

      • "Mapping on the HEALPix Grid" (HPX), Calabretta, M.R., & Roukema, B.F. 2007, MNRAS, 381, 865

      Reprints of all published papers may be obtained from NASA's Astrophysics Data System (ADS), http://adsabs.harvard.edu/. Reprints of Papers I, II (+HPX) and III are available from http://www.atnf.csiro.au/~mcalabre/. This site also includes errata and supplementary material for Papers I, II and III.

      Additional information on all aspects of FITS and its various software implementations may be found at the FITS Support Office http://fits.gsfc.nasa.gov.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/lin_8h-source.html0000644001153600020070000014305412310355626022451 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: lin.h Source File
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      pywcs-1.12/wcslib/html/lin_8h.html0000644001153600020070000012313212310355626021146 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: lin.h File Reference

      lin.h File Reference

      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  linprm
       Linear transformation parameters. More...

      Defines

      #define LINLEN   (sizeof(struct linprm)/sizeof(int))
       Size of the linprm struct in int units.
      #define linini_errmsg   lin_errmsg
       Deprecated.
      #define lincpy_errmsg   lin_errmsg
       Deprecated.
      #define linfree_errmsg   lin_errmsg
       Deprecated.
      #define linprt_errmsg   lin_errmsg
       Deprecated.
      #define linset_errmsg   lin_errmsg
       Deprecated.
      #define linp2x_errmsg   lin_errmsg
       Deprecated.
      #define linx2p_errmsg   lin_errmsg
       Deprecated.

      Enumerations

      enum  lin_errmsg_enum { LINERR_SUCCESS = 0, LINERR_NULL_POINTER = 1, LINERR_MEMORY = 2, LINERR_SINGULAR_MTX = 3 }

      Functions

      int linini (int alloc, int naxis, struct linprm *lin)
       Default constructor for the linprm struct.
      int lincpy (int alloc, const struct linprm *linsrc, struct linprm *lindst)
       Copy routine for the linprm struct.
      int linfree (struct linprm *lin)
       Destructor for the linprm struct.
      int linprt (const struct linprm *lin)
       Print routine for the linprm struct.
      int linset (struct linprm *lin)
       Setup routine for the linprm struct.
      int linp2x (struct linprm *lin, int ncoord, int nelem, const double pixcrd[], double imgcrd[])
       Pixel-to-world linear transformation.
      int linx2p (struct linprm *lin, int ncoord, int nelem, const double imgcrd[], double pixcrd[])
       World-to-pixel linear transformation.
      int matinv (int n, const double mat[], double inv[])
       Matrix inversion.

      Variables

      const char * lin_errmsg []
       Status return messages.

      Detailed Description

      These routines apply the linear transformation defined by the FITS WCS standard. They are based on the linprm struct which contains all information needed for the computations. The struct contains some members that must be set by the user, and others that are maintained by these routines, somewhat like a C++ class but with no encapsulation.

      Three routines, linini(), lincpy(), and linfree() are provided to manage the linprm struct, and another, linprt(), prints its contents.

      A setup routine, linset(), computes intermediate values in the linprm struct from parameters in it that were supplied by the user. The struct always needs to be set up by linset() but need not be called explicitly - refer to the explanation of linprm::flag.

      linp2x() and linx2p() implement the WCS linear transformations.

      An auxiliary matrix inversion routine, matinv(), is included. It uses LU-triangular factorization with scaled partial pivoting.

      Define Documentation

      #define LINLEN   (sizeof(struct linprm)/sizeof(int))

      Size of the linprm struct in int units, used by the Fortran wrappers.

      #define linini_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      #define lincpy_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      #define linfree_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      #define linprt_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      #define linset_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      #define linp2x_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      #define linx2p_errmsg   lin_errmsg

      Deprecated:
      Added for backwards compatibility, use lin_errmsg directly now instead.

      Enumeration Type Documentation

      enum lin_errmsg_enum

      Enumerator:
      LINERR_SUCCESS 
      LINERR_NULL_POINTER 
      LINERR_MEMORY 
      LINERR_SINGULAR_MTX 

      Function Documentation

      int linini ( int  alloc,
      int  naxis,
      struct linprm *  lin 
      )

      linini() allocates memory for arrays in a linprm struct and sets all members of the struct to default values.

      PLEASE NOTE: every linprm struct should be initialized by linini(), possibly repeatedly. On the first invokation, and only the first invokation, linprm::flag must be set to -1 to initialize memory management, regardless of whether linini() will actually be used to allocate memory.

      Parameters:
      [in] alloc If true, allocate memory unconditionally for arrays in the linprm struct.
      If false, it is assumed that pointers to these arrays have been set by the user except if they are null pointers in which case memory will be allocated for them regardless. (In other words, setting alloc true saves having to initalize these pointers to zero.)
      [in] naxis The number of world coordinate axes, used to determine array sizes.
      [in,out] lin Linear transformation parameters. Note that, in order to initialize memory management linprm::flag should be set to -1 when lin is initialized for the first time (memory leaks may result if it had already been initialized).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.
      • 2: Memory allocation failed.
      For returns > 1, a detailed error message is set in linprm::err if enabled, see wcserr_enable().

      int lincpy ( int  alloc,
      const struct linprm *  linsrc,
      struct linprm *  lindst 
      )

      lincpy() does a deep copy of one linprm struct to another, using linini() to allocate memory for its arrays if required. Only the "information to be provided" part of the struct is copied; a call to linset() is required to initialize the remainder.

      Parameters:
      [in] alloc If true, allocate memory for the crpix, pc, and cdelt arrays in the destination. Otherwise, it is assumed that pointers to these arrays have been set by the user except if they are null pointers in which case memory will be allocated for them regardless.
      [in] linsrc Struct to copy from.
      [in,out] lindst Struct to copy to. linprm::flag should be set to -1 if lindst was not previously initialized (memory leaks may result if it was previously initialized).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.
      • 2: Memory allocation failed.
      For returns > 1, a detailed error message is set in linprm::err if enabled, see wcserr_enable().

      int linfree ( struct linprm *  lin  ) 

      linfree() frees memory allocated for the linprm arrays by linini() and/or linset(). linini() keeps a record of the memory it allocates and linfree() will only attempt to free this.

      PLEASE NOTE: linfree() must not be invoked on a linprm struct that was not initialized by linini().

      Parameters:
      [in] lin Linear transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.

      int linprt ( const struct linprm *  lin  ) 

      linprt() prints the contents of a linprm struct using wcsprintf(). Mainly intended for diagnostic purposes.

      Parameters:
      [in] lin Linear transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.

      int linset ( struct linprm *  lin  ) 

      linset(), if necessary, allocates memory for the linprm::piximg and linprm::imgpix arrays and sets up the linprm struct according to information supplied within it - refer to the explanation of linprm::flag.

      Note that this routine need not be called directly; it will be invoked by linp2x() and linx2p() if the linprm::flag is anything other than a predefined magic value.

      Parameters:
      [in,out] lin Linear transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.
      • 2: Memory allocation failed.
      • 3: PCi_ja matrix is singular.
      For returns > 1, a detailed error message is set in linprm::err if enabled, see wcserr_enable().

      int linp2x ( struct linprm *  lin,
      int  ncoord,
      int  nelem,
      const double  pixcrd[],
      double  imgcrd[] 
      )

      linp2x() transforms pixel coordinates to intermediate world coordinates.

      Parameters:
      [in,out] lin Linear transformation parameters.
      [in] ncoord,nelem The number of coordinates, each of vector length nelem but containing lin.naxis coordinate elements.
      [in] pixcrd Array of pixel coordinates.
      [out] imgcrd Array of intermediate world coordinates.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.
      • 2: Memory allocation failed.
      • 3: PCi_ja matrix is singular.
      For returns > 1, a detailed error message is set in linprm::err if enabled, see wcserr_enable().

      int linx2p ( struct linprm *  lin,
      int  ncoord,
      int  nelem,
      const double  imgcrd[],
      double  pixcrd[] 
      )

      linx2p() transforms intermediate world coordinates to pixel coordinates.

      Parameters:
      [in,out] lin Linear transformation parameters.
      [in] ncoord,nelem The number of coordinates, each of vector length nelem but containing lin.naxis coordinate elements.
      [in] imgcrd Array of intermediate world coordinates.
      [out] pixcrd Array of pixel coordinates. Status return value:
      • 0: Success.
      • 1: Null linprm pointer passed.
      • 2: Memory allocation failed.
      • 3: PCi_ja matrix is singular.
      For returns > 1, a detailed error message is set in linprm::err if enabled, see wcserr_enable().

      matinv ( int  n,
      const double  mat[],
      double  inv[] 
      )

      matinv() performs matrix inversion using LU-triangular factorization with scaled partial pivoting.

      Parameters:
      [in] n Order of the matrix ($n \times n$).
      [in] mat Matrix to be inverted, stored as mat[$i n + j$] where $i$ and $j$ are the row and column indices respectively.
      [out] inv Inverse of mat with the same storage convention.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Memory allocation failed.
      • 3: Singular matrix.

      Variable Documentation

      const char * lin_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/log_8h-source.html0000644001153600020070000004465412310355626022456 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: log.h Source File
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      pywcs-1.12/wcslib/html/log_8h.html0000644001153600020070000003324512310355626021152 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: log.h File Reference

      log.h File Reference

      Go to the source code of this file.

      Enumerations

      enum  log_errmsg_enum {
        LOGERR_SUCCESS = 0, LOGERR_NULL_POINTER = 1, LOGERR_BAD_LOG_REF_VAL = 2, LOGERR_BAD_X = 3,
        LOGERR_BAD_WORLD = 4
      }

      Functions

      int logx2s (double crval, int nx, int sx, int slogc, const double x[], double logc[], int stat[])
       Transform to logarithmic coordinates.
      int logs2x (double crval, int nlogc, int slogc, int sx, const double logc[], double x[], int stat[])
       Transform logarithmic coordinates.

      Variables

      const char * log_errmsg []
       Status return messages.

      Detailed Description

      These routines implement the part of the FITS WCS standard that deals with logarithmic coordinates. They define methods to be used for computing logarithmic world coordinates from intermediate world coordinates (a linear transformation of image pixel coordinates), and vice versa.

      logx2s() and logs2x() implement the WCS logarithmic coordinate transformations.

      Argument checking:
      The input log-coordinate values are only checked for values that would result in floating point exceptions and the same is true for the log-coordinate reference value.

      Accuracy:
      No warranty is given for the accuracy of these routines (refer to the copyright notice); intending users must satisfy for themselves their adequacy for the intended purpose. However, closure effectively to within double precision rounding error was demonstrated by test routine tlog.c which accompanies this software.

      Enumeration Type Documentation

      enum log_errmsg_enum

      Enumerator:
      LOGERR_SUCCESS 
      LOGERR_NULL_POINTER 
      LOGERR_BAD_LOG_REF_VAL 
      LOGERR_BAD_X 
      LOGERR_BAD_WORLD 

      Function Documentation

      int logx2s ( double  crval,
      int  nx,
      int  sx,
      int  slogc,
      const double  x[],
      double  logc[],
      int  stat[] 
      )

      logx2s() transforms intermediate world coordinates to logarithmic coordinates.

      Parameters:
      [in,out] crval Log-coordinate reference value (CRVALia).
      [in] nx Vector length.
      [in] sx Vector stride.
      [in] slogc Vector stride.
      [in] x Intermediate world coordinates, in SI units.
      [out] logc Logarithmic coordinates, in SI units.
      [out] stat Status return value status for each vector element:
      • 0: Success.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid log-coordinate reference value.

      int logs2x ( double  crval,
      int  nlogc,
      int  slogc,
      int  sx,
      const double  logc[],
      double  x[],
      int  stat[] 
      )

      logs2x() transforms logarithmic world coordinates to intermediate world coordinates.

      Parameters:
      [in,out] crval Log-coordinate reference value (CRVALia).
      [in] nlogc Vector length.
      [in] slogc Vector stride.
      [in] sx Vector stride.
      [in] logc Logarithmic coordinates, in SI units.
      [out] x Intermediate world coordinates, in SI units.
      [out] stat Status return value status for each vector element:
      • 0: Success.
      • 1: Invalid value of logc.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid log-coordinate reference value.
      • 4: One or more of the world-coordinate values are incorrect, as indicated by the stat vector.

      Variable Documentation

      const char * log_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/memory.html0000644001153600020070000002120012310355626021266 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Memory management

      Memory management

      The initialization routines for certain of the WCSLIB data structures allocate memory for some of their members:

      • wcsini() optionally allocates memory for the crpix, pc, cdelt, crval, cunit, ctype, pv, ps, cd, crota, colax, cname, crder, and csyer arrays in the wcsprm struct (using linini() for certain of these). Note that wcsini() does not allocate memory for the tab array - refer to the usage notes for wcstab() in wcshdr.h. If the pc matrix is not unity, wcsset() (via linset()) also allocates memory for the piximg and imgpix arrays.

      • linini(): optionally allocates memory for the crpix, pc, and cdelt arrays in the linprm struct. If the pc matrix is not unity, linset() also allocates memory for the piximg and imgpix arrays. Typically these would be used by wcsini() and wcsset().

      • tabini(): optionally allocates memory for the K, map, crval, index, and coord arrays (including the arrays referenced by index[]) in the tabprm struct. tabmem() takes control of any of these arrays that may have been allocated by the user, specifically in that tabfree() will then free it. tabset() also allocates memory for the sense, p0, delta and extrema arrays.

      The caller may load data into these arrays but must not modify the struct members (i.e. the pointers) themselves or else memory leaks will result.

      wcsini() maintains a record of memory it has allocated and this is used by wcsfree() which wcsini() uses to free any memory that it may have allocated on a previous invokation. Thus it is not necessary for the caller to invoke wcsfree() separately if wcsini() is invoked repeatedly on the same wcsprm struct. Likewise, wcsset() deallocates memory that it may have allocated on a previous invokation. The same comments apply to linini(), linfree(), and linset() and to tabini(), tabfree(), and tabset().

      A memory leak will result if a wcsprm, linprm or tabprm struct goes out of scope before the memory has been free'd, either by the relevant routine, wcsfree(), linfree() or tabfree(), or otherwise. Likewise, if one of these structs itself has been malloc'd and the allocated memory is not free'd when the memory for the struct is free'd. A leak may also arise if the caller interferes with the array pointers in the "private" part of these structs.

      Beware of making a shallow copy of a wcsprm, linprm or tabprm struct by assignment; any changes made to allocated memory in one would be reflected in the other, and if the memory allocated for one was free'd the other would reference unallocated memory. Use the relevant routine instead to make a deep copy: wcssub(), lincpy() or tabcpy().

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/overview.html0000644001153600020070000003030612310355626021633 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Overview of WCSLIB

      Overview of WCSLIB

      WCSLIB is documented in the prologues of its header files which provide a detailed description of the purpose of each function and its interface (this material is, of course, used to generate the doxygen manual). Here we explain how the library as a whole is structured. We will normally refer to WCSLIB 'routines', meaning C functions or Fortran 'subroutines', though the latter are actually wrappers implemented in C.

      WCSLIB is layered software, each layer depends only on those beneath; understanding WCSLIB first means understanding its stratigraphy. There are essentially three levels, though some intermediate levels exist within these:

      • The top layer consists of routines that provide the connection between FITS files and the high-level WCSLIB data structures, the main function being to parse a FITS header, extract WCS information, and copy it into a wcsprm struct. The lexical parsers among these are implemented as Flex descriptions (source files with .l suffix) and the C code generated from these by Flex is included in the source distribution.
        • wcshdr.h,c -- Routines for constructing wcsprm data structures from information in a FITS header and conversely for writing a wcsprm struct out as a FITS header.
        • wcspih.l -- Flex implementation of wcspih(), a lexical parser for WCS "keyrecords" in an image header. A keyrecord (formerly called "card image") consists of a keyword, its value - the keyvalue - and an optional comment, the keycomment.
        • wcsbth.l -- Flex implementation of wcsbth() which parses binary table image array and pixel list headers in addition to image array headers.
        • getwcstab.h,c -- Implementation of a -TAB binary table reader in CFITSIO.

        A generic FITS header parser is also provided to handle non-WCS keyrecords that are ignored by wcspih():
        • fitshdr.h,l -- Generic FITS header parser (not WCS-specific).

        The philosophy adopted for dealing with non-standard WCS usage is to translate it at this level so that the middle- and low-level routines need only deal with standard constructs:
        • wcsfix.h,c -- Translator for non-standard FITS WCS constructs (uses wcsutrne()).
        • wcsutrn.l -- Lexical translator for non-standard units specifications.

        As a concrete example, within this layer the CTYPEia keyvalues would be extracted from a FITS header and copied into the ctype[] array within a wcsprm struct. None of the header keyrecords are interpreted.

      • The middle layer analyses the WCS information obtained from the FITS header by the top-level routines, identifying the separate steps of the WCS algorithm chain for each of the coordinate axes in the image. It constructs the various data structures on which the low-level routines are based and invokes them in the correct sequence. Thus the wcsprm struct is essentially the glue that binds together the low-level routines into a complete coordinate description.
        • wcs.h,c -- Driver routines for the low-level routines.
        • wcsunits.h,c -- Unit conversions (uses wcsulexe()).
        • wcsulex.l -- Lexical parser for units specifications.

        To continue the above example, within this layer the ctype[] keyvalues in a wcsprm struct are analysed to determine the nature of the coordinate axes in the image.

      • Applications programmers who use the top- and middle-level routines generally need know nothing about the low-level routines. These are essentially mathematical in nature and largely independent of FITS itself. The mathematical formulae and algorithms cited in the WCS Papers, for example the spherical projection equations of Paper II and the lookup-table methods of Paper III, are implemented by the routines in this layer, some of which serve to aggregate others:
        • cel.h,c -- Celestial coordinate transformations, combines prj.h,c and sph.h,c.
        • spc.h,c -- Spectral coordinate transformations, combines transformations from spx.h,c.

        The remainder of the routines in this level are independent of everything other than the grass-roots mathematical functions:
        • lin.h,c -- Linear transformation matrix.
        • log.h,c -- Logarithmic coordinates.
        • prj.h,c -- Spherical projection equations.
        • sph.h,c -- Spherical coordinate transformations.
        • spx.h,c -- Basic spectral transformations.
        • tab.h,c -- Coordinate lookup tables.

        As the routines within this layer are quite generic, some, principally the implementation of the spherical projection equations, have been used in other packages (AST, wcstools) that provide their own implementations of the functionality of the top and middle-level routines.

      • At the grass-roots level there are a number of mathematical and utility routines.

        When dealing with celestial coordinate systems it is often desirable to use an angular measure that provides an exact representation of the latitude of the north or south pole. The WCSLIB routines use the following trigonometric functions that take or return angles in degrees:
        These "trigd" routines are expected to handle angles that are a multiple of $90^\circ$ returning an exact result. Some C implementations provide these as part of a system library and in such cases it may (or may not!) be preferable to use them. wcstrig.c provides wrappers on the standard trig functions based on radian measure, adding tests for multiples of $90^\circ$.

        However, wcstrig.h also provides the choice of using preprocessor macro implementations of the trigd functions that don't test for multiples of $90^\circ$ (compile with -DWCSTRIG_MACRO). These are typically 20% faster but may lead to problems near the poles.
        • wcsmath.h -- Defines mathematical and other constants.
        • wcstrig.h,c -- Various implementations of trigd functions.
        • wcsutil.h,c -- Simple utility functions for string manipulation, etc. used by WCSLIB.

      Complementary to the C library, a set of wrappers are provided that allow all WCSLIB C functions to be called by Fortran programs, see below.

      Plotting of coordinate graticules is one of the more important requirements of a world coordinate system. WCSLIB provides a PGPLOT-based subroutine, PGSBOX (Fortran), which handles general curvilinear coordinates via a user-supplied function - PGWCSL provides the interface to WCSLIB. A C wrapper, cpgsbox(), is also provided, see below.

      Several utility programs are distributed with WCSLIB:

      • wcsgrid extracts the WCS keywords for an image from the specified FITS file and uses cpgsbox() to plot a 2-D coordinate graticule for it. It requires WCSLIB, PGSBOX and CFITSIO.

      • wcsware extracts the WCS keywords for an image from the specified FITS file and constructs wcsprm structs for each coordinate representation found. The structs may then be printed or used to transform pixel coordinates to world coordinates. It requires WCSLIB and CFITSIO.

      • HPXcvt reorganises HEALPix data into a 2-D FITS image with HPX coordinate system. The input data may be stored in a FITS file as a primary image or image extension, or as a binary table extension. Both NESTED and RING pixel indices are supported. It uses CFITSIO.

      • fitshdr lists headers from a FITS file specified on the command line, or else on stdin, printing them as 80-character keyrecords without trailing blanks. It is independent of WCSLIB.
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/pages.html0000644001153600020070000000223112310355626021060 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Page Index

      Related Pages

      Here is a list of all related documentation pages:
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/pgsbox.html0000644001153600020070000000667412310355626021302 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: PGSBOX

      PGSBOX

      PGSBOX, which is provided as a separate part of WCSLIB, is a PGPLOT routine (PGPLOT being a Fortran graphics library) that draws and labels curvilinear coordinate grids. Example PGSBOX grids can be seen at http://www.atnf.csiro.au/~mcalabre/WCS/PGSBOX/index.html.

      The prologue to pgsbox.f contains usage instructions. pgtest.f and cpgtest.c serve as test and demonstration programs in Fortran and C and also as well- documented examples of usage.

      PGSBOX requires a separate routine, EXTERNAL NLFUNC, to define the coordinate transformation. Fortran subroutine PGCRFN (pgcrfn.f) is provided to define separable pairs of non-linear coordinate systems. Linear, logarithmic and power-law axis types are currently defined; further types may be added as required. A C function, pgwcsl_(), with Fortran-like interface defines an NLFUNC that interfaces to WCSLIB 4.x for PGSBOX to draw celestial coordinate grids.

      PGPLOT is implemented as a Fortran library with a set of C wrapper routines that are generated by a software tool. However, PGSBOX has a more complicated interface than any of the standard PGPLOT routines, especially in having an EXTERNAL function in its argument list. Consequently, PGSBOX is implemented in Fortran but with a hand-coded C wrapper, cpgsbox().

      As an example, in this suite the C test/demo program, cpgtest, calls the C wrapper, cpgsbox(), passing it a pointer to pgwcsl_(). In turn, cpgsbox() calls PGSBOX, which invokes pgwcsl_() as an EXTERNAL subroutine. In this sequence, a complicated C struct defined by cpgtest is passed through PGSBOX to pgwcsl_() as an INTEGER array.

      While there are no formal standards for calling Fortran from C, there are some fairly well established conventions. Nevertheless, it's possible that you may need to modify the code if you use a combination of Fortran and C compilers with linkage conventions that differ from that of the GNU compilers, gcc and g77.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/prj_8h-source.html0000644001153600020070000031330212310355626022455 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: prj.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/prj_8h.html0000644001153600020070000055020112310355626021160 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: prj.h File Reference

      prj.h File Reference

      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  prjprm
       Projection parameters. More...

      Defines

      #define PVN   30
       Total number of projection parameters.
      #define PRJX2S_ARGS
       For use in declaring deprojection function prototypes.
      #define PRJS2X_ARGS
       For use in declaring projection function prototypes.
      #define PRJLEN   (sizeof(struct prjprm)/sizeof(int))
       Size of the prjprm struct in int units.
      #define prjini_errmsg   prj_errmsg
       Deprecated.
      #define prjprt_errmsg   prj_errmsg
       Deprecated.
      #define prjset_errmsg   prj_errmsg
       Deprecated.
      #define prjx2s_errmsg   prj_errmsg
       Deprecated.
      #define prjs2x_errmsg   prj_errmsg
       Deprecated.

      Enumerations

      enum  prj_errmsg_enum {
        PRJERR_SUCCESS = 0, PRJERR_NULL_POINTER = 1, PRJERR_BAD_PARAM = 2, PRJERR_BAD_PIX = 3,
        PRJERR_BAD_WORLD = 4
      }

      Functions

      int prjini (struct prjprm *prj)
       Default constructor for the prjprm struct.
      int prjfree (struct prjprm *prj)
       Destructor for the prjprm struct.
      int prjprt (const struct prjprm *prj)
       Print routine for the prjprm struct.
      int prjset (struct prjprm *prj)
       Generic setup routine for the prjprm struct.
      int prjx2s (PRJX2S_ARGS)
       Generic Cartesian-to-spherical deprojection.
      int prjs2x (PRJS2X_ARGS)
       Generic spherical-to-Cartesian projection.
      int azpset (struct prjprm *prj)
       Set up a prjprm struct for the zenithal/azimuthal perspective (AZP) projection.
      int azpx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the zenithal/azimuthal perspective (AZP) projection.
      int azps2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the zenithal/azimuthal perspective (AZP) projection.
      int szpset (struct prjprm *prj)
       Set up a prjprm struct for the slant zenithal perspective (SZP) projection.
      int szpx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the slant zenithal perspective (SZP) projection.
      int szps2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the slant zenithal perspective (SZP) projection.
      int tanset (struct prjprm *prj)
       Set up a prjprm struct for the gnomonic (TAN) projection.
      int tanx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the gnomonic (TAN) projection.
      int tans2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the gnomonic (TAN) projection.
      int stgset (struct prjprm *prj)
       Set up a prjprm struct for the stereographic (STG) projection.
      int stgx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the stereographic (STG) projection.
      int stgs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the stereographic (STG) projection.
      int sinset (struct prjprm *prj)
       Set up a prjprm struct for the orthographic/synthesis (SIN) projection.
      int sinx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the orthographic/synthesis (SIN) projection.
      int sins2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the orthographic/synthesis (SIN) projection.
      int arcset (struct prjprm *prj)
       Set up a prjprm struct for the zenithal/azimuthal equidistant (ARC) projection.
      int arcx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the zenithal/azimuthal equidistant (ARC) projection.
      int arcs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the zenithal/azimuthal equidistant (ARC) projection.
      int zpnset (struct prjprm *prj)
       Set up a prjprm struct for the zenithal/azimuthal polynomial (ZPN) projection.
      int zpnx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the zenithal/azimuthal polynomial (ZPN) projection.
      int zpns2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the zenithal/azimuthal polynomial (ZPN) projection.
      int zeaset (struct prjprm *prj)
       Set up a prjprm struct for the zenithal/azimuthal equal area (ZEA) projection.
      int zeax2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the zenithal/azimuthal equal area (ZEA) projection.
      int zeas2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the zenithal/azimuthal equal area (ZEA) projection.
      int airset (struct prjprm *prj)
       Set up a prjprm struct for Airy's (AIR) projection.
      int airx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for Airy's (AIR) projection.
      int airs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for Airy's (AIR) projection.
      int cypset (struct prjprm *prj)
       Set up a prjprm struct for the cylindrical perspective (CYP) projection.
      int cypx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the cylindrical perspective (CYP) projection.
      int cyps2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the cylindrical perspective (CYP) projection.
      int ceaset (struct prjprm *prj)
       Set up a prjprm struct for the cylindrical equal area (CEA) projection.
      int ceax2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the cylindrical equal area (CEA) projection.
      int ceas2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the cylindrical equal area (CEA) projection.
      int carset (struct prjprm *prj)
       Set up a prjprm struct for the plate carrée (CAR) projection.
      int carx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the plate carrée (CAR) projection.
      int cars2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the plate carrée (CAR) projection.
      int merset (struct prjprm *prj)
       Set up a prjprm struct for Mercator's (MER) projection.
      int merx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for Mercator's (MER) projection.
      int mers2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for Mercator's (MER) projection.
      int sflset (struct prjprm *prj)
       Set up a prjprm struct for the Sanson-Flamsteed (SFL) projection.
      int sflx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the Sanson-Flamsteed (SFL) projection.
      int sfls2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the Sanson-Flamsteed (SFL) projection.
      int parset (struct prjprm *prj)
       Set up a prjprm struct for the parabolic (PAR) projection.
      int parx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the parabolic (PAR) projection.
      int pars2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the parabolic (PAR) projection.
      int molset (struct prjprm *prj)
       Set up a prjprm struct for Mollweide's (MOL) projection.
      int molx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for Mollweide's (MOL) projection.
      int mols2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for Mollweide's (MOL) projection.
      int aitset (struct prjprm *prj)
       Set up a prjprm struct for the Hammer-Aitoff (AIT) projection.
      int aitx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the Hammer-Aitoff (AIT) projection.
      int aits2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the Hammer-Aitoff (AIT) projection.
      int copset (struct prjprm *prj)
       Set up a prjprm struct for the conic perspective (COP) projection.
      int copx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the conic perspective (COP) projection.
      int cops2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the conic perspective (COP) projection.
      int coeset (struct prjprm *prj)
       Set up a prjprm struct for the conic equal area (COE) projection.
      int coex2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the conic equal area (COE) projection.
      int coes2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the conic equal area (COE) projection.
      int codset (struct prjprm *prj)
       Set up a prjprm struct for the conic equidistant (COD) projection.
      int codx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the conic equidistant (COD) projection.
      int cods2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the conic equidistant (COD) projection.
      int cooset (struct prjprm *prj)
       Set up a prjprm struct for the conic orthomorphic (COO) projection.
      int coox2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the conic orthomorphic (COO) projection.
      int coos2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the conic orthomorphic (COO) projection.
      int bonset (struct prjprm *prj)
       Set up a prjprm struct for Bonne's (BON) projection.
      int bonx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for Bonne's (BON) projection.
      int bons2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for Bonne's (BON) projection.
      int pcoset (struct prjprm *prj)
       Set up a prjprm struct for the polyconic (PCO) projection.
      int pcox2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the polyconic (PCO) projection.
      int pcos2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the polyconic (PCO) projection.
      int tscset (struct prjprm *prj)
       Set up a prjprm struct for the tangential spherical cube (TSC) projection.
      int tscx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the tangential spherical cube (TSC) projection.
      int tscs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the tangential spherical cube (TSC) projection.
      int cscset (struct prjprm *prj)
       Set up a prjprm struct for the COBE spherical cube (CSC) projection.
      int cscx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the COBE spherical cube (CSC) projection.
      int cscs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the COBE spherical cube (CSC) projection.
      int qscset (struct prjprm *prj)
       Set up a prjprm struct for the quadrilateralized spherical cube (QSC) projection.
      int qscx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the quadrilateralized spherical cube (QSC) projection.
      int qscs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the quadrilateralized spherical cube (QSC) projection.
      int hpxset (struct prjprm *prj)
       Set up a prjprm struct for the HEALPix (HPX) projection.
      int hpxx2s (PRJX2S_ARGS)
       Cartesian-to-spherical transformation for the HEALPix (HPX) projection.
      int hpxs2x (PRJS2X_ARGS)
       Spherical-to-Cartesian transformation for the HEALPix (HPX) projection.

      Variables

      const char * prj_errmsg []
       Status return messages.
      const int CONIC
       Identifier for conic projections.
      const int CONVENTIONAL
       Identifier for conventional projections.
      const int CYLINDRICAL
       Identifier for cylindrical projections.
      const int POLYCONIC
       Identifier for polyconic projections.
      const int PSEUDOCYLINDRICAL
       Identifier for pseudocylindrical projections.
      const int QUADCUBE
       Identifier for quadcube projections.
      const int ZENITHAL
       Identifier for zenithal/azimuthal projections.
      const int HEALPIX
       Identifier for the HEALPix projection.
      const char prj_categories [9][32]
       Projection categories.
      const int prj_ncode
       The number of recognized three-letter projection codes.
      const char prj_codes [27][4]
       Recognized three-letter projection codes.

      Detailed Description

      These routines implement the spherical map projections defined by the FITS WCS standard. They are based on the prjprm struct which contains all information needed for the computations. The struct contains some members that must be set by the user, and others that are maintained by these routines, somewhat like a C++ class but with no encapsulation.

      Routine prjini() is provided to initialize the prjprm struct with default values, prjfree() reclaims any memory that may have been allocated to store an error message, and prjprt() prints its contents.

      Setup routines for each projection with names of the form ???set(), where "???" is the down-cased three-letter projection code, compute intermediate values in the prjprm struct from parameters in it that were supplied by the user. The struct always needs to be set by the projection's setup routine but that need not be called explicitly - refer to the explanation of prjprm::flag.

      Each map projection is implemented via separate functions for the spherical projection, ???s2x(), and deprojection, ???x2s().

      A set of driver routines, prjset(), prjx2s(), and prjs2x(), provides a generic interface to the specific projection routines which they invoke via pointers-to-functions stored in the prjprm struct.

      In summary, the routines are:

      Argument checking (projection routines):
      The values of $\phi$ and $\theta$ (the native longitude and latitude) normally lie in the range $[-180^\circ,180^\circ]$ for $\phi$, and $[-90^\circ,90^\circ]$ for $\theta$. However, all projection routines will accept any value of $\phi$ and will not normalize it.

      The projection routines do not explicitly check that $\theta$ lies within the range $[-90^\circ,90^\circ]$. They do check for any value of $\theta$ that produces an invalid argument to the projection equations (e.g. leading to division by zero). The projection routines for AZP, SZP, TAN, SIN, ZPN, and COP also return error 2 if $(\phi,\theta)$ corresponds to the overlapped (far) side of the projection but also return the corresponding value of $(x,y)$. This strict bounds checking may be relaxed at any time by setting prjprm::bounds to 0 (rather than 1); the projections need not be reinitialized.

      Argument checking (deprojection routines):
      Error checking on the projected coordinates $(x,y)$ is limited to that required to ascertain whether a solution exists. Where a solution does exist no check is made that the value of $\phi$ and $\theta$ obtained lie within the ranges $[-180^\circ,180^\circ]$ for $\phi$, and $[-90^\circ,90^\circ]$ for $\theta$.

      Accuracy:
      No warranty is given for the accuracy of these routines (refer to the copyright notice); intending users must satisfy for themselves their adequacy for the intended purpose. However, closure to a precision of at least $0^\circ.0000000001$ of longitude and latitude has been verified for typical projection parameters on the $1^\circ$ degree graticule of native longitude and latitude (to within $5^\circ$ of any latitude where the projection may diverge). Refer to the tprj1.c and tprj2.c test routines that accompany this software.

      Define Documentation

      #define PVN   30

      The total number of projection parameters numbered 0 to PVN-1.

      #define PRJX2S_ARGS

      Value:

      struct prjprm *prj, int nx, int ny, int sxy, int spt, \
const double x[], const double y[], double phi[], double theta[], int stat[]
      Preprocessor macro used for declaring deprojection function prototypes.

      #define PRJS2X_ARGS

      Value:

      struct prjprm *prj, int nx, int ny, int sxy, int spt, \
const double phi[], const double theta[], double x[], double y[], int stat[]
      Preprocessor macro used for declaring projection function prototypes.

      #define PRJLEN   (sizeof(struct prjprm)/sizeof(int))

      Size of the prjprm struct in int units, used by the Fortran wrappers.

      #define prjini_errmsg   prj_errmsg

      Deprecated:
      Added for backwards compatibility, use prj_errmsg directly now instead.

      #define prjprt_errmsg   prj_errmsg

      Deprecated:
      Added for backwards compatibility, use prj_errmsg directly now instead.

      #define prjset_errmsg   prj_errmsg

      Deprecated:
      Added for backwards compatibility, use prj_errmsg directly now instead.

      #define prjx2s_errmsg   prj_errmsg

      Deprecated:
      Added for backwards compatibility, use prj_errmsg directly now instead.

      #define prjs2x_errmsg   prj_errmsg

      Deprecated:
      Added for backwards compatibility, use prj_errmsg directly now instead.

      Enumeration Type Documentation

      enum prj_errmsg_enum

      Enumerator:
      PRJERR_SUCCESS 
      PRJERR_NULL_POINTER 
      PRJERR_BAD_PARAM 
      PRJERR_BAD_PIX 
      PRJERR_BAD_WORLD 

      Function Documentation

      int prjini ( struct prjprm *  prj  ) 

      prjini() sets all members of a prjprm struct to default values. It should be used to initialize every prjprm struct.

      Parameters:
      [out] prj Projection parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null prjprm pointer passed.

      int prjfree ( struct prjprm *  prj  ) 

      prjfree() frees any memory that may have been allocated to store an error message in the prjprm struct.

      Parameters:
      [in] prj Projection parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null prjprm pointer passed.

      int prjprt ( const struct prjprm *  prj  ) 

      prjprt() prints the contents of a prjprm struct using wcsprintf(). Mainly intended for diagnostic purposes.

      Parameters:
      [in] prj Projection parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null prjprm pointer passed.

      int prjset ( struct prjprm *  prj  ) 

      prjset() sets up a prjprm struct according to information supplied within it.

      Note that this routine need not be called directly; it will be invoked by prjx2s() and prjs2x() if prj.flag is anything other than a predefined magic value.

      The one important distinction between prjset() and the setup routines for the specific projections is that the projection code must be defined in the prjprm struct in order for prjset() to identify the required projection. Once prjset() has initialized the prjprm struct, prjx2s() and prjs2x() use the pointers to the specific projection and deprojection routines contained therein.

      Parameters:
      [in,out] prj Projection parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null prjprm pointer passed.
      • 2: Invalid projection parameters.
      For returns > 1, a detailed error message is set in prjprm::err if enabled, see wcserr_enable().

      int prjx2s ( PRJX2S_ARGS   ) 

      Deproject Cartesian $(x,y)$ coordinates in the plane of projection to native spherical coordinates $(\phi,\theta)$.

      The projection is that specified by prjprm::code.

      Parameters:
      [in,out] prj Projection parameters.
      [in] nx,ny Vector lengths.
      [in] sxy,spt Vector strides.
      [in] x,y Projected coordinates.
      [out] phi,theta Longitude and latitude $(\phi,\theta)$ of the projected point in native spherical coordinates [deg].
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of $(x,y)$.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null prjprm pointer passed.
      • 2: Invalid projection parameters.
      • 3: One or more of the $(x,y)$ coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in prjprm::err if enabled, see wcserr_enable().

      int prjs2x ( PRJS2X_ARGS   ) 

      Project native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of projection.

      The projection is that specified by prjprm::code.

      Parameters:
      [in,out] prj Projection parameters.
      [in] nphi,ntheta Vector lengths.
      [in] spt,sxy Vector strides.
      [in] phi,theta Longitude and latitude $(\phi,\theta)$ of the projected point in native spherical coordinates [deg].
      [out] x,y Projected coordinates.
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of $(\phi,\theta)$.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null prjprm pointer passed.
      • 2: Invalid projection parameters.
      • 4: One or more of the $(\phi,\theta)$ coordinates were, invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in prjprm::err if enabled, see wcserr_enable().

      int azpset ( struct prjprm *  prj  ) 

      azpset() sets up a prjprm struct for a zenithal/azimuthal perspective (AZP) projection.

      See prjset() for a description of the API.

      int azpx2s ( PRJX2S_ARGS   ) 

      azpx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal perspective (AZP) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int azps2x ( PRJS2X_ARGS   ) 

      azps2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal perspective (AZP) projection.

      See prjs2x() for a description of the API.

      int szpset ( struct prjprm *  prj  ) 

      szpset() sets up a prjprm struct for a slant zenithal perspective (SZP) projection.

      See prjset() for a description of the API.

      int szpx2s ( PRJX2S_ARGS   ) 

      szpx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a slant zenithal perspective (SZP) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int szps2x ( PRJS2X_ARGS   ) 

      szps2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a slant zenithal perspective (SZP) projection.

      See prjs2x() for a description of the API.

      int tanset ( struct prjprm *  prj  ) 

      tanset() sets up a prjprm struct for a gnomonic (TAN) projection.

      See prjset() for a description of the API.

      int tanx2s ( PRJX2S_ARGS   ) 

      tanx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a gnomonic (TAN) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int tans2x ( PRJS2X_ARGS   ) 

      tans2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a gnomonic (TAN) projection.

      See prjs2x() for a description of the API.

      int stgset ( struct prjprm *  prj  ) 

      stgset() sets up a prjprm struct for a stereographic (STG) projection.

      See prjset() for a description of the API.

      int stgx2s ( PRJX2S_ARGS   ) 

      stgx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a stereographic (STG) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int stgs2x ( PRJS2X_ARGS   ) 

      stgs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a stereographic (STG) projection.

      See prjs2x() for a description of the API.

      int sinset ( struct prjprm *  prj  ) 

      stgset() sets up a prjprm struct for an orthographic/synthesis (SIN) projection.

      See prjset() for a description of the API.

      int sinx2s ( PRJX2S_ARGS   ) 

      sinx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of an orthographic/synthesis (SIN) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int sins2x ( PRJS2X_ARGS   ) 

      sins2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of an orthographic/synthesis (SIN) projection.

      See prjs2x() for a description of the API.

      int arcset ( struct prjprm *  prj  ) 

      arcset() sets up a prjprm struct for a zenithal/azimuthal equidistant (ARC) projection.

      See prjset() for a description of the API.

      int arcx2s ( PRJX2S_ARGS   ) 

      arcx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal equidistant (ARC) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int arcs2x ( PRJS2X_ARGS   ) 

      arcs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal equidistant (ARC) projection.

      See prjs2x() for a description of the API.

      int zpnset ( struct prjprm *  prj  ) 

      zpnset() sets up a prjprm struct for a zenithal/azimuthal polynomial (ZPN) projection.

      See prjset() for a description of the API.

      int zpnx2s ( PRJX2S_ARGS   ) 

      zpnx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal polynomial (ZPN) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int zpns2x ( PRJS2X_ARGS   ) 

      zpns2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal polynomial (ZPN) projection.

      See prjs2x() for a description of the API.

      int zeaset ( struct prjprm *  prj  ) 

      zeaset() sets up a prjprm struct for a zenithal/azimuthal equal area (ZEA) projection.

      See prjset() for a description of the API.

      int zeax2s ( PRJX2S_ARGS   ) 

      zeax2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal equal area (ZEA) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int zeas2x ( PRJS2X_ARGS   ) 

      zeas2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a zenithal/azimuthal equal area (ZEA) projection.

      See prjs2x() for a description of the API.

      int airset ( struct prjprm *  prj  ) 

      airset() sets up a prjprm struct for an Airy (AIR) projection.

      See prjset() for a description of the API.

      int airx2s ( PRJX2S_ARGS   ) 

      airx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of an Airy (AIR) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int airs2x ( PRJS2X_ARGS   ) 

      airs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of an Airy (AIR) projection.

      See prjs2x() for a description of the API.

      int cypset ( struct prjprm *  prj  ) 

      cypset() sets up a prjprm struct for a cylindrical perspective (CYP) projection.

      See prjset() for a description of the API.

      int cypx2s ( PRJX2S_ARGS   ) 

      cypx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a cylindrical perspective (CYP) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int cyps2x ( PRJS2X_ARGS   ) 

      cyps2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a cylindrical perspective (CYP) projection.

      See prjs2x() for a description of the API.

      int ceaset ( struct prjprm *  prj  ) 

      ceaset() sets up a prjprm struct for a cylindrical equal area (CEA) projection.

      See prjset() for a description of the API.

      int ceax2s ( PRJX2S_ARGS   ) 

      ceax2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a cylindrical equal area (CEA) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int ceas2x ( PRJS2X_ARGS   ) 

      ceas2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a cylindrical equal area (CEA) projection.

      See prjs2x() for a description of the API.

      int carset ( struct prjprm *  prj  ) 

      carset() sets up a prjprm struct for a plate carrée (CAR) projection.

      See prjset() for a description of the API.

      int carx2s ( PRJX2S_ARGS   ) 

      carx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a plate carrée (CAR) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int cars2x ( PRJS2X_ARGS   ) 

      cars2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a plate carrée (CAR) projection.

      See prjs2x() for a description of the API.

      int merset ( struct prjprm *  prj  ) 

      merset() sets up a prjprm struct for a Mercator (MER) projection.

      See prjset() for a description of the API.

      int merx2s ( PRJX2S_ARGS   ) 

      merx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a Mercator (MER) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int mers2x ( PRJS2X_ARGS   ) 

      mers2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a Mercator (MER) projection.

      See prjs2x() for a description of the API.

      int sflset ( struct prjprm *  prj  ) 

      sflset() sets up a prjprm struct for a Sanson-Flamsteed (SFL) projection.

      See prjset() for a description of the API.

      int sflx2s ( PRJX2S_ARGS   ) 

      sflx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a Sanson-Flamsteed (SFL) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int sfls2x ( PRJS2X_ARGS   ) 

      sfls2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a Sanson-Flamsteed (SFL) projection.

      See prjs2x() for a description of the API.

      int parset ( struct prjprm *  prj  ) 

      parset() sets up a prjprm struct for a parabolic (PAR) projection.

      See prjset() for a description of the API.

      int parx2s ( PRJX2S_ARGS   ) 

      parx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a parabolic (PAR) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int pars2x ( PRJS2X_ARGS   ) 

      pars2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a parabolic (PAR) projection.

      See prjs2x() for a description of the API.

      int molset ( struct prjprm *  prj  ) 

      molset() sets up a prjprm struct for a Mollweide (MOL) projection.

      See prjset() for a description of the API.

      int molx2s ( PRJX2S_ARGS   ) 

      molx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a Mollweide (MOL) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int mols2x ( PRJS2X_ARGS   ) 

      mols2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a Mollweide (MOL) projection.

      See prjs2x() for a description of the API.

      int aitset ( struct prjprm *  prj  ) 

      aitset() sets up a prjprm struct for a Hammer-Aitoff (AIT) projection.

      See prjset() for a description of the API.

      int aitx2s ( PRJX2S_ARGS   ) 

      aitx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a Hammer-Aitoff (AIT) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int aits2x ( PRJS2X_ARGS   ) 

      aits2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a Hammer-Aitoff (AIT) projection.

      See prjs2x() for a description of the API.

      int copset ( struct prjprm *  prj  ) 

      copset() sets up a prjprm struct for a conic perspective (COP) projection.

      See prjset() for a description of the API.

      int copx2s ( PRJX2S_ARGS   ) 

      copx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a conic perspective (COP) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int cops2x ( PRJS2X_ARGS   ) 

      cops2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a conic perspective (COP) projection.

      See prjs2x() for a description of the API.

      int coeset ( struct prjprm *  prj  ) 

      coeset() sets up a prjprm struct for a conic equal area (COE) projection.

      See prjset() for a description of the API.

      int coex2s ( PRJX2S_ARGS   ) 

      coex2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a conic equal area (COE) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int coes2x ( PRJS2X_ARGS   ) 

      coes2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a conic equal area (COE) projection.

      See prjs2x() for a description of the API.

      int codset ( struct prjprm *  prj  ) 

      codset() sets up a prjprm struct for a conic equidistant (COD) projection.

      See prjset() for a description of the API.

      int codx2s ( PRJX2S_ARGS   ) 

      codx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a conic equidistant (COD) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int cods2x ( PRJS2X_ARGS   ) 

      cods2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a conic equidistant (COD) projection.

      See prjs2x() for a description of the API.

      int cooset ( struct prjprm *  prj  ) 

      cooset() sets up a prjprm struct for a conic orthomorphic (COO) projection.

      See prjset() for a description of the API.

      int coox2s ( PRJX2S_ARGS   ) 

      coox2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a conic orthomorphic (COO) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int coos2x ( PRJS2X_ARGS   ) 

      coos2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a conic orthomorphic (COO) projection.

      See prjs2x() for a description of the API.

      int bonset ( struct prjprm *  prj  ) 

      bonset() sets up a prjprm struct for a Bonne (BON) projection.

      See prjset() for a description of the API.

      int bonx2s ( PRJX2S_ARGS   ) 

      bonx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a Bonne (BON) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int bons2x ( PRJS2X_ARGS   ) 

      bons2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a Bonne (BON) projection.

      See prjs2x() for a description of the API.

      int pcoset ( struct prjprm *  prj  ) 

      pcoset() sets up a prjprm struct for a polyconic (PCO) projection.

      See prjset() for a description of the API.

      int pcox2s ( PRJX2S_ARGS   ) 

      pcox2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a polyconic (PCO) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int pcos2x ( PRJS2X_ARGS   ) 

      pcos2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a polyconic (PCO) projection.

      See prjs2x() for a description of the API.

      int tscset ( struct prjprm *  prj  ) 

      tscset() sets up a prjprm struct for a tangential spherical cube (TSC) projection.

      See prjset() for a description of the API.

      int tscx2s ( PRJX2S_ARGS   ) 

      tscx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a tangential spherical cube (TSC) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int tscs2x ( PRJS2X_ARGS   ) 

      tscs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a tangential spherical cube (TSC) projection.

      See prjs2x() for a description of the API.

      int cscset ( struct prjprm *  prj  ) 

      cscset() sets up a prjprm struct for a COBE spherical cube (CSC) projection.

      See prjset() for a description of the API.

      int cscx2s ( PRJX2S_ARGS   ) 

      cscx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a COBE spherical cube (CSC) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int cscs2x ( PRJS2X_ARGS   ) 

      cscs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a COBE spherical cube (CSC) projection.

      See prjs2x() for a description of the API.

      int qscset ( struct prjprm *  prj  ) 

      qscset() sets up a prjprm struct for a quadrilateralized spherical cube (QSC) projection.

      See prjset() for a description of the API.

      int qscx2s ( PRJX2S_ARGS   ) 

      qscx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a quadrilateralized spherical cube (QSC) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int qscs2x ( PRJS2X_ARGS   ) 

      qscs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a quadrilateralized spherical cube (QSC) projection.

      See prjs2x() for a description of the API.

      int hpxset ( struct prjprm *  prj  ) 

      hpxset() sets up a prjprm struct for a HEALPix (HPX) projection.

      See prjset() for a description of the API.

      int hpxx2s ( PRJX2S_ARGS   ) 

      hpxx2s() deprojects Cartesian $(x,y)$ coordinates in the plane of a HEALPix (HPX) projection to native spherical coordinates $(\phi,\theta)$.

      See prjx2s() for a description of the API.

      int hpxs2x ( PRJS2X_ARGS   ) 

      hpxs2x() projects native spherical coordinates $(\phi,\theta)$ to Cartesian $(x,y)$ coordinates in the plane of a HEALPix (HPX) projection.

      See prjs2x() for a description of the API.

      Variable Documentation

      const char * prj_errmsg[]

      Error messages to match the status value returned from each function.

      const int CONIC

      Identifier for conic projections, see prjprm::category.

      const int CONVENTIONAL

      Identifier for conventional projections, see prjprm::category.

      const int CYLINDRICAL

      Identifier for cylindrical projections, see prjprm::category.

      const int POLYCONIC

      Identifier for polyconic projections, see prjprm::category.

      const int PSEUDOCYLINDRICAL

      Identifier for pseudocylindrical projections, see prjprm::category.

      const int QUADCUBE

      Identifier for quadcube projections, see prjprm::category.

      const int ZENITHAL

      Identifier for zenithal/azimuthal projections, see prjprm::category.

      const int HEALPIX

      Identifier for the HEALPix projection, see prjprm::category.

      const char prj_categories[9][32]

      Names of the projection categories, all in lower-case except for "HEALPix".

      Provided for information only, not used by the projection routines.

      const int prj_ncode

      The number of recognized three-letter projection codes (currently 27), see prj_codes.

      const char prj_codes[27][4]

      List of all recognized three-letter projection codes (currently 27), e.g. SIN, TAN, etc.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/software.html0000644001153600020070000001341012310355626021614 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: FITS-WCS and related software

      FITS-WCS and related software

      Several implementations of the FITS WCS standards are available:

      • AST, developed by David Berry within the U.K. Starlink project, http://www.starlink.ac.uk/ast/ and now supported by JAC, Hawaii http://starlink.jach.hawaii.edu/starlink/.

        A useful utility for experimenting with FITS WCS descriptions (similar to wcsgrid) is also provided; go to the above site and then look at the section entitled "FITS-WCS Plotting Demo".

      Python wrappers to WCSLIB are provided by

      Java is supported via

      Recommended WCS-aware FITS image viewers:

      both handle 2-D images.

      Currently (2012/01/24) I know of no image viewers that handle 1-D spectra properly nor multi-dimensional data, not even multi-dimensional data with only two non-degenerate image axes (please inform me if you know otherwise).

      Pre-built WCSLIB packages are available, generally a little behind the main release (this list will probably be out-of-date by the time you read it, best do a web search):

      Bill Pence's general FITS IO library, CFITSIO is available from http://heasarc.gsfc.nasa.gov/fitsio/. It is used optionally by some of the high-level WCSLIB test programs and is required by two of the utility programs.

      PGPLOT, Tim Pearson's Fortran plotting package on which PGSBOX is based, also used by some of the WCSLIB self-test suite and a utility program, is available from http://astro.caltech.edu/~tjp/pgplot/.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/spc_8h-source.html0000644001153600020070000030375112310355626022456 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: spc.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/spc_8h.html0000644001153600020070000024355512310355626021165 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: spc.h File Reference

      spc.h File Reference

      #include "spx.h"
      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  spcprm
       Spectral transformation parameters. More...

      Defines

      #define SPCLEN   (sizeof(struct spcprm)/sizeof(int))
       Size of the spcprm struct in int units.
      #define spcini_errmsg   spc_errmsg
       Deprecated.
      #define spcprt_errmsg   spc_errmsg
       Deprecated.
      #define spcset_errmsg   spc_errmsg
       Deprecated.
      #define spcx2s_errmsg   spc_errmsg
       Deprecated.
      #define spcs2x_errmsg   spc_errmsg
       Deprecated.

      Enumerations

      enum  spc_errmsg_enum {
        SPCERR_NO_CHANGE = -1, SPCERR_SUCCESS = 0, SPCERR_NULL_POINTER = 1, SPCERR_BAD_SPEC_PARAMS = 2,
        SPCERR_BAD_X = 3, SPCERR_BAD_SPEC = 4
      }

      Functions

      int spcini (struct spcprm *spc)
       Default constructor for the spcprm struct.
      int spcfree (struct spcprm *spc)
       Destructor for the spcprm struct.
      int spcprt (const struct spcprm *spc)
       Print routine for the spcprm struct.
      int spcset (struct spcprm *spc)
       Setup routine for the spcprm struct.
      int spcx2s (struct spcprm *spc, int nx, int sx, int sspec, const double x[], double spec[], int stat[])
       Transform to spectral coordinates.
      int spcs2x (struct spcprm *spc, int nspec, int sspec, int sx, const double spec[], double x[], int stat[])
       Transform spectral coordinates.
      int spctype (const char ctype[], char stype[], char scode[], char sname[], char units[], char *ptype, char *xtype, int *restreq, struct wcserr **err)
       Spectral CTYPEia keyword analysis.
      int spcspxe (const char ctypeS[], double crvalS, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalX, double *dXdS, struct wcserr **err)
       Spectral keyword analysis.
      int spcxpse (const char ctypeS[], double crvalX, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalS, double *dSdX, struct wcserr **err)
       Spectral keyword synthesis.
      int spctrne (const char ctypeS1[], double crvalS1, double cdeltS1, double restfrq, double restwav, char ctypeS2[], double *crvalS2, double *cdeltS2, struct wcserr **err)
       Spectral keyword translation.
      int spcaips (const char ctypeA[], int velref, char ctype[], char specsys[])
       Translate AIPS-convention spectral keywords.
      int spctyp (const char ctype[], char stype[], char scode[], char sname[], char units[], char *ptype, char *xtype, int *restreq)
      int spcspx (const char ctypeS[], double crvalS, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalX, double *dXdS)
      int spcxps (const char ctypeS[], double crvalX, double restfrq, double restwav, char *ptype, char *xtype, int *restreq, double *crvalS, double *dSdX)
      int spctrn (const char ctypeS1[], double crvalS1, double cdeltS1, double restfrq, double restwav, char ctypeS2[], double *crvalS2, double *cdeltS2)

      Variables

      const char * spc_errmsg []
       Status return messages.

      Detailed Description

      These routines implement the part of the FITS WCS standard that deals with spectral coordinates. They define methods to be used for computing spectral world coordinates from intermediate world coordinates (a linear transformation of image pixel coordinates), and vice versa. They are based on the spcprm struct which contains all information needed for the computations. The struct contains some members that must be set by the user, and others that are maintained by these routines, somewhat like a C++ class but with no encapsulation.

      Routine spcini() is provided to initialize the spcprm struct with default values, spcfree() reclaims any memory that may have been allocated to store an error message, and spcprt() prints its contents.

      A setup routine, spcset(), computes intermediate values in the spcprm struct from parameters in it that were supplied by the user. The struct always needs to be set up by spcset() but it need not be called explicitly - refer to the explanation of spcprm::flag.

      spcx2s() and spcs2x() implement the WCS spectral coordinate transformations. In fact, they are high level driver routines for the lower level spectral coordinate transformation routines described in spx.h.

      A number of routines are provided to aid in analysing or synthesising sets of FITS spectral axis keywords:

      • spctype() checks a spectral CTYPEia keyword for validity and returns information derived from it.

      • Spectral keyword analysis routine spcspxe() computes the values of the $X$-type spectral variables for the $S$-type variables supplied.

      • Spectral keyword synthesis routine, spcxpse(), computes the $S$-type variables for the $X$-types supplied.

      • Given a set of spectral keywords, a translation routine, spctrne(), produces the corresponding set for the specified spectral CTYPEia.

      • spcaips() translates AIPS-convention spectral CTYPEia and VELREF keyvalues.

      Spectral variable types - $S$, $P$, and $X$:
      A few words of explanation are necessary regarding spectral variable types in FITS.

      Every FITS spectral axis has three associated spectral variables:

      $S$-type: the spectral variable in which coordinates are to be expressed. Each $S$-type is encoded as four characters and is linearly related to one of four basic types as follows:

      F: frequency 'FREQ': frequency 'AFRQ': angular frequency 'ENER': photon energy 'WAVN': wave number 'VRAD': radio velocity

      W: wavelength in vacuo 'WAVE': wavelength 'VOPT': optical velocity 'ZOPT': redshift

      A: wavelength in air 'AWAV': wavelength in air

      V: velocity 'VELO': relativistic velocity 'BETA': relativistic beta factor

      The $S$-type forms the first four characters of the CTYPEia keyvalue, and CRVALia and CDELTia are expressed as $S$-type quantities so that they provide a first-order approximation to the $S$-type variable at the reference point.

      Note that 'AFRQ', angular frequency, is additional to the variables defined in WCS Paper III.

      $P$-type: the basic spectral variable (F, W, A, or V) with which the $S$-type variable is associated (see list above).

      For non-grism axes, the $P$-type is encoded as the eighth character of CTYPEia.

      $X$-type: the basic spectral variable (F, W, A, or V) for which the spectral axis is linear, grisms excluded (see below).

      For non-grism axes, the $X$-type is encoded as the sixth character of CTYPEia.

      Grisms: Grism axes have normal $S$-, and $P$-types but the axis is linear, not in any spectral variable, but in a special "grism parameter". The $X$-type spectral variable is either W or A for grisms in vacuo or air respectively, but is encoded as 'w' or 'a' to indicate that an additional transformation is required to convert to or from the grism parameter. The spectral algorithm code for grisms also has a special encoding in CTYPEia, either 'GRI' (in vacuo) or 'GRA' (in air).

      In the algorithm chain, the non-linear transformation occurs between the $X$-type and the $P$-type variables; the transformation between $P$-type and $S$-type variables is always linear.

      When the $P$-type and $X$-type variables are the same, the spectral axis is linear in the $S$-type variable and the second four characters of CTYPEia are blank. This can never happen for grism axes.

      As an example, correlating radio spectrometers always produce spectra that are regularly gridded in frequency; a redshift scale on such a spectrum is non-linear. The required value of CTYPEia would be 'ZOPT-F2W', where the desired $S$-type is 'ZOPT' (redshift), the $P$-type is necessarily 'W' (wavelength), and the $X$-type is 'F' (frequency) by the nature of the instrument.

      Argument checking:
      The input spectral values are only checked for values that would result in floating point exceptions. In particular, negative frequencies and wavelengths are allowed, as are velocities greater than the speed of light. The same is true for the spectral parameters - rest frequency and wavelength.

      Accuracy:
      No warranty is given for the accuracy of these routines (refer to the copyright notice); intending users must satisfy for themselves their adequacy for the intended purpose. However, closure effectively to within double precision rounding error was demonstrated by test routine tspc.c which accompanies this software.

      Define Documentation

      #define SPCLEN   (sizeof(struct spcprm)/sizeof(int))

      Size of the spcprm struct in int units, used by the Fortran wrappers.

      #define spcini_errmsg   spc_errmsg

      Deprecated:
      Added for backwards compatibility, use spc_errmsg directly now instead.

      #define spcprt_errmsg   spc_errmsg

      Deprecated:
      Added for backwards compatibility, use spc_errmsg directly now instead.

      #define spcset_errmsg   spc_errmsg

      Deprecated:
      Added for backwards compatibility, use spc_errmsg directly now instead.

      #define spcx2s_errmsg   spc_errmsg

      Deprecated:
      Added for backwards compatibility, use spc_errmsg directly now instead.

      #define spcs2x_errmsg   spc_errmsg

      Deprecated:
      Added for backwards compatibility, use spc_errmsg directly now instead.

      Enumeration Type Documentation

      enum spc_errmsg_enum

      Enumerator:
      SPCERR_NO_CHANGE 
      SPCERR_SUCCESS 
      SPCERR_NULL_POINTER 
      SPCERR_BAD_SPEC_PARAMS 
      SPCERR_BAD_X 
      SPCERR_BAD_SPEC 

      Function Documentation

      int spcini ( struct spcprm *  spc  ) 

      spcini() sets all members of a spcprm struct to default values. It should be used to initialize every spcprm struct.

      Parameters:
      [in,out] spc Spectral transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spcprm pointer passed.

      int spcfree ( struct spcprm *  spc  ) 

      spcfree() frees any memory that may have been allocated to store an error message in the spcprm struct.

      Parameters:
      [in] spc Spectral transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spcprm pointer passed.

      int spcprt ( const struct spcprm *  spc  ) 

      spcprt() prints the contents of a spcprm struct using wcsprintf(). Mainly intended for diagnostic purposes.

      Parameters:
      [in] spc Spectral transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spcprm pointer passed.

      int spcset ( struct spcprm *  spc  ) 

      spcset() sets up a spcprm struct according to information supplied within it.

      Note that this routine need not be called directly; it will be invoked by spcx2s() and spcs2x() if spcprm::flag is anything other than a predefined magic value.

      Parameters:
      [in,out] spc Spectral transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spcprm pointer passed.
      • 2: Invalid spectral parameters.
      For returns > 1, a detailed error message is set in spcprm::err if enabled, see wcserr_enable().

      int spcx2s ( struct spcprm *  spc,
      int  nx,
      int  sx,
      int  sspec,
      const double  x[],
      double  spec[],
      int  stat[] 
      )

      spcx2s() transforms intermediate world coordinates to spectral coordinates.

      Parameters:
      [in,out] spc Spectral transformation parameters.
      [in] nx Vector length.
      [in] sx Vector stride.
      [in] sspec Vector stride.
      [in] x Intermediate world coordinates, in SI units.
      [out] spec Spectral coordinates, in SI units.
      [out] stat Status return value status for each vector element:
      • 0: Success.
      • 1: Invalid value of x.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spcprm pointer passed.
      • 2: Invalid spectral parameters.
      • 3: One or more of the x coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in spcprm::err if enabled, see wcserr_enable().

      int spcs2x ( struct spcprm *  spc,
      int  nspec,
      int  sspec,
      int  sx,
      const double  spec[],
      double  x[],
      int  stat[] 
      )

      spcs2x() transforms spectral world coordinates to intermediate world coordinates.

      Parameters:
      [in,out] spc Spectral transformation parameters.
      [in] nspec Vector length.
      [in] sspec Vector stride.
      [in] sx Vector stride.
      [in] spec Spectral coordinates, in SI units.
      [out] x Intermediate world coordinates, in SI units.
      [out] stat Status return value status for each vector element:
      • 0: Success.
      • 1: Invalid value of spec.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spcprm pointer passed.
      • 2: Invalid spectral parameters.
      • 4: One or more of the spec coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in spcprm::err if enabled, see wcserr_enable().

      int spctype ( const char  ctype[],
      char  stype[],
      char  scode[],
      char  sname[],
      char  units[],
      char *  ptype,
      char *  xtype,
      int *  restreq,
      struct wcserr **  err 
      )

      spctype() checks whether a CTYPEia keyvalue is a valid spectral axis type and if so returns information derived from it relating to the associated $S$-, $P$-, and $X$-type spectral variables (see explanation above).

      The return arguments are guaranteed not be modified if CTYPEia is not a valid spectral type; zero-pointers may be specified for any that are not of interest.

      A deprecated form of this function, spctyp(), lacks the wcserr** parameter.

      Parameters:
      [in] ctype The CTYPEia keyvalue, (eight characters with null termination).
      [out] stype The four-letter name of the $S$-type spectral variable copied or translated from ctype. If a non-zero pointer is given, the array must accomodate a null- terminated string of length 5.
      [out] scode The three-letter spectral algorithm code copied or translated from ctype. Logarithmic ('LOG') and tabular ('TAB') codes are also recognized. If a non-zero pointer is given, the array must accomodate a null-terminated string of length 4.
      [out] sname Descriptive name of the $S$-type spectral variable. If a non-zero pointer is given, the array must accomodate a null-terminated string of length 22.
      [out] units SI units of the $S$-type spectral variable. If a non-zero pointer is given, the array must accomodate a null-terminated string of length 8.
      [out] ptype Character code for the $P$-type spectral variable derived from ctype, one of 'F', 'W', 'A', or 'V'.
      [out] xtype Character code for the $X$-type spectral variable derived from ctype, one of 'F', 'W', 'A', or 'V'. Also, 'w' and 'a' are synonymous to 'W' and 'A' for grisms in vacuo and air respectively. Set to 'L' or 'T' for logarithmic ('LOG') and tabular ('TAB') axes.
      [out] restreq Multivalued flag that indicates whether rest frequency or wavelength is required to compute spectral variables for this CTYPEia:
      • 0: Not required.
      • 1: Required for the conversion between $S$- and $P$-types (e.g. 'ZOPT-F2W').
      • 2: Required for the conversion between $P$- and $X$-types (e.g. 'BETA-W2V').
      • 3: Required for the conversion between $S$- and $P$-types, and between $P$- and $X$-types, but not between $S$- and $X$-types (this applies only for 'VRAD-V2F', 'VOPT-V2W', and 'ZOPT-V2W').
      Thus the rest frequency or wavelength is required for spectral coordinate computations (i.e. between $S$- and $X$-types) only if 
       restreq%3 != 0
      .
      [out] err For function return values > 1, this struct will contain a detailed error message. May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters (not a spectral CTYPEia).

      int spcspxe ( const char  ctypeS[],
      double  crvalS,
      double  restfrq,
      double  restwav,
      char *  ptype,
      char *  xtype,
      int *  restreq,
      double *  crvalX,
      double *  dXdS,
      struct wcserr **  err 
      )

      spcspxe() analyses the CTYPEia and CRVALia FITS spectral axis keyword values and returns information about the associated $X$-type spectral variable.

      A deprecated form of this function, spcspx(), lacks the wcserr** parameter.

      Parameters:
      [in] ctypeS Spectral axis type, i.e. the CTYPEia keyvalue, (eight characters with null termination). For non-grism axes, the character code for the $P$-type spectral variable in the algorithm code (i.e. the eighth character of CTYPEia) may be set to '?' (it will not be reset).
      [in] crvalS Value of the $S$-type spectral variable at the reference point, i.e. the CRVALia keyvalue, SI units.
      [in] restfrq,restwav Rest frequency [Hz] and rest wavelength in vacuo [m], only one of which need be given, the other should be set to zero. Neither are required if the translation is between wave-characteristic types, or between velocity-characteristic types. E.g., required for 'FREQ' -> 'ZOPT-F2W', but not required for 'VELO-F2V' -> 'ZOPT-F2W'.
      [out] ptype Character code for the $P$-type spectral variable derived from ctypeS, one of 'F', 'W', 'A', or 'V'.
      [out] xtype Character code for the $X$-type spectral variable derived from ctypeS, one of 'F', 'W', 'A', or 'V'. Also, 'w' and 'a' are synonymous to 'W' and 'A' for grisms in vacuo and air respectively; crvalX and dXdS (see below) will conform to these.
      [out] restreq Multivalued flag that indicates whether rest frequency or wavelength is required to compute spectral variables for this CTYPEia, as for spctype().
      [out] crvalX Value of the $X$-type spectral variable at the reference point, SI units.
      [out] dXdS The derivative, $dX/dS$, evaluated at the reference point, SI units. Multiply the CDELTia keyvalue by this to get the pixel spacing in the $X$-type spectral coordinate.
      [out] err For function return values > 1, this struct will contain a detailed error message. May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters.

      int spcxpse ( const char  ctypeS[],
      double  crvalX,
      double  restfrq,
      double  restwav,
      char *  ptype,
      char *  xtype,
      int *  restreq,
      double *  crvalS,
      double *  dSdX,
      struct wcserr **  err 
      )

      spcxpse(), for the spectral axis type specified and the value provided for the $X$-type spectral variable at the reference point, deduces the value of the FITS spectral axis keyword CRVALia and also the derivative $dS/dX$ which may be used to compute CDELTia. See above for an explanation of the $S$-, $P$-, and $X$-type spectral variables.

      A deprecated form of this function, spcxps(), lacks the wcserr** parameter.

      Parameters:
      [in] ctypeS The required spectral axis type, i.e. the CTYPEia keyvalue, (eight characters with null termination). For non-grism axes, the character code for the $P$-type spectral variable in the algorithm code (i.e. the eighth character of CTYPEia) may be set to '?' (it will not be reset).
      [in] crvalX Value of the $X$-type spectral variable at the reference point (N.B. NOT the CRVALia keyvalue), SI units.
      [in] restfrq,restwav Rest frequency [Hz] and rest wavelength in vacuo [m], only one of which need be given, the other should be set to zero. Neither are required if the translation is between wave-characteristic types, or between velocity-characteristic types. E.g., required for 'FREQ' -> 'ZOPT-F2W', but not required for 'VELO-F2V' -> 'ZOPT-F2W'.
      [out] ptype Character code for the $P$-type spectral variable derived from ctypeS, one of 'F', 'W', 'A', or 'V'.
      [out] xtype Character code for the $X$-type spectral variable derived from ctypeS, one of 'F', 'W', 'A', or 'V'. Also, 'w' and 'a' are synonymous to 'W' and 'A' for grisms; crvalX and cdeltX must conform to these.
      [out] restreq Multivalued flag that indicates whether rest frequency or wavelength is required to compute spectral variables for this CTYPEia, as for spctype().
      [out] crvalS Value of the $S$-type spectral variable at the reference point (i.e. the appropriate CRVALia keyvalue), SI units.
      [out] dSdX The derivative, $dS/dX$, evaluated at the reference point, SI units. Multiply this by the pixel spacing in the $X$-type spectral coordinate to get the CDELTia keyvalue.
      [out] err For function return values > 1, this struct will contain a detailed error message. May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters.

      int spctrne ( const char  ctypeS1[],
      double  crvalS1,
      double  cdeltS1,
      double  restfrq,
      double  restwav,
      char  ctypeS2[],
      double *  crvalS2,
      double *  cdeltS2,
      struct wcserr **  err 
      )

      spctrne() translates a set of FITS spectral axis keywords into the corresponding set for the specified spectral axis type. For example, a 'FREQ' axis may be translated into 'ZOPT-F2W' and vice versa.

      A deprecated form of this function, spctrn(), lacks the wcserr** parameter.

      Parameters:
      [in] ctypeS1 Spectral axis type, i.e. the CTYPEia keyvalue, (eight characters with null termination). For non-grism axes, the character code for the $P$-type spectral variable in the algorithm code (i.e. the eighth character of CTYPEia) may be set to '?' (it will not be reset).
      [in] crvalS1 Value of the $S$-type spectral variable at the reference point, i.e. the CRVALia keyvalue, SI units.
      [in] cdeltS1 Increment of the $S$-type spectral variable at the reference point, SI units.
      [in] restfrq,restwav Rest frequency [Hz] and rest wavelength in vacuo [m], only one of which need be given, the other should be set to zero. Neither are required if the translation is between wave-characteristic types, or between velocity-characteristic types. E.g., required for 'FREQ' -> 'ZOPT-F2W', but not required for 'VELO-F2V' -> 'ZOPT-F2W'.
      [in,out] ctypeS2 Required spectral axis type (eight characters with null termination). The first four characters are required to be given and are never modified. The remaining four, the algorithm code, are completely determined by, and must be consistent with, ctypeS1 and the first four characters of ctypeS2. A non-zero status value will be returned if they are inconsistent (see below). However, if the final three characters are specified as "???", or if just the eighth character is specified as '?', the correct algorithm code will be substituted (applies for grism axes as well as non-grism).
      [out] crvalS2 Value of the new $S$-type spectral variable at the reference point, i.e. the new CRVALia keyvalue, SI units.
      [out] cdeltS2 Increment of the new $S$-type spectral variable at the reference point, i.e. the new CDELTia keyvalue, SI units.
      [out] err For function return values > 1, this struct will contain a detailed error message. May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters.
      A status value of 2 will be returned if restfrq or restwav are not specified when required, or if ctypeS1 or ctypeS2 are self-inconsistent, or have different spectral $X$-type variables.

      int spcaips ( const char  ctypeA[],
      int  velref,
      char  ctype[],
      char  specsys[] 
      )

      spcaips() translates AIPS-convention spectral CTYPEia and VELREF keyvalues.

      Parameters:
      [in] ctypeA CTYPEia keyvalue possibly containing an AIPS-convention spectral code (eight characters, need not be null-terminated).
      [in] velref AIPS-convention VELREF code. It has the following integer values:
      • 1: LSR kinematic, originally described simply as "LSR" without distinction between the kinematic and dynamic definitions.
      • 2: Barycentric, originally described as "HEL" meaning heliocentric.
      • 3: Topocentric, originally described as "OBS" meaning geocentric but widely interpreted as topocentric.
      AIPS++ extensions to VELREF are also recognized:
      • 4: LSR dynamic.
      • 5: Geocentric.
      • 6: Source rest frame.
      • 7: Galactocentric.
      For an AIPS 'VELO' axis, a radio convention velocity (VRAD) is denoted by adding 256 to VELREF, otherwise an optical velocity (VOPT) is indicated (this is not applicable to 'FREQ' or 'FELO' axes). Setting velref to 0 or 256 chooses between optical and radio velocity without specifying a Doppler frame, provided that a frame is encoded in ctypeA. If not, i.e. for ctypeA = 'VELO', ctype will be returned as 'VELO'.
      VELREF takes precedence over CTYPEia in defining the Doppler frame, e.g. 
                                ctypeA = 'VELO-HEL'
                          velref = 1

      returns ctype = 'VOPT' with specsys set to 'LSRK'.
      [out] ctype Translated CTYPEia keyvalue, or a copy of ctypeA if no translation was performed (in which case any trailing blanks in ctypeA will be replaced with nulls).
      [out] specsys Doppler reference frame indicated by VELREF or else by CTYPEia with value corresponding to the SPECSYS keyvalue in the FITS WCS standard. May be returned blank if neither specifies a Doppler frame, e.g. ctypeA = 'FELO' and velref256 == 0.
      Returns:
      Status return value:
      • -1: No translation required (not an error).
      • 0: Success.
      • 2: Invalid value of VELREF.

      int spctyp ( const char  ctype[],
      char  stype[],
      char  scode[],
      char  sname[],
      char  units[],
      char *  ptype,
      char *  xtype,
      int *  restreq 
      )

      int spcspx ( const char  ctypeS[],
      double  crvalS,
      double  restfrq,
      double  restwav,
      char *  ptype,
      char *  xtype,
      int *  restreq,
      double *  crvalX,
      double *  dXdS 
      )

      int spcxps ( const char  ctypeS[],
      double  crvalX,
      double  restfrq,
      double  restwav,
      char *  ptype,
      char *  xtype,
      int *  restreq,
      double *  crvalS,
      double *  dSdX 
      )

      int spctrn ( const char  ctypeS1[],
      double  crvalS1,
      double  cdeltS1,
      double  restfrq,
      double  restwav,
      char  ctypeS2[],
      double *  crvalS2,
      double *  cdeltS2 
      )

      Variable Documentation

      const char * spc_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/sph_8h-source.html0000644001153600020070000006474712310355626022474 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: sph.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/sph_8h.html0000644001153600020070000005224612310355626021165 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: sph.h File Reference

      sph.h File Reference

      Go to the source code of this file.

      Functions

      int sphx2s (const double eul[5], int nphi, int ntheta, int spt, int sxy, const double phi[], const double theta[], double lng[], double lat[])
       Rotation in the pixel-to-world direction.
      int sphs2x (const double eul[5], int nlng, int nlat, int sll, int spt, const double lng[], const double lat[], double phi[], double theta[])
       Rotation in the world-to-pixel direction.
      int sphdpa (int nfield, double lng0, double lat0, const double lng[], const double lat[], double dist[], double pa[])
       Compute angular distance and position angle.
      int sphpad (int nfield, double lng0, double lat0, const double dist[], const double pa[], double lng[], double lat[])
       Compute field points offset from a given point.

      Detailed Description

      The WCS spherical coordinate transformations are implemented via separate functions, sphx2s() and sphs2x(), for the transformation in each direction.

      A utility function, sphdpa(), computes the angular distances and position angles from a given point on the sky to a number of other points. sphpad() does the complementary operation - computes the coordinates of points offset by the given angular distances and position angles from a given point on the sky.

      Function Documentation

      int sphx2s ( const double  eul[5],
      int  nphi,
      int  ntheta,
      int  spt,
      int  sxy,
      const double  phi[],
      const double  theta[],
      double  lng[],
      double  lat[] 
      )

      sphx2s() transforms native coordinates of a projection to celestial coordinates.

      Parameters:
      [in] eul Euler angles for the transformation:
      • 0: Celestial longitude of the native pole [deg].
      • 1: Celestial colatitude of the native pole, or native colatitude of the celestial pole [deg].
      • 2: Native longitude of the celestial pole [deg].
      • 3: $cos$(eul[1])
      • 4: $sin$(eul[1])
      [in] nphi,ntheta Vector lengths.
      [in] spt,sxy Vector strides.
      [in] phi,theta Longitude and latitude in the native coordinate system of the projection [deg].
      [out] lng,lat Celestial longitude and latitude [deg]. These may refer to the same storage as phi and theta respectively.
      Returns:
      Status return value:
      • 0: Success.

      int sphs2x ( const double  eul[5],
      int  nlng,
      int  nlat,
      int  sll,
      int  spt,
      const double  lng[],
      const double  lat[],
      double  phi[],
      double  theta[] 
      )

      sphs2x() transforms celestial coordinates to the native coordinates of a projection.

      Parameters:
      [in] eul Euler angles for the transformation:
      • 0: Celestial longitude of the native pole [deg].
      • 1: Celestial colatitude of the native pole, or native colatitude of the celestial pole [deg].
      • 2: Native longitude of the celestial pole [deg].
      • 3: $cos$(eul[1])
      • 4: $sin$(eul[1])
      [in] nlng,nlat Vector lengths.
      [in] sll,spt Vector strides.
      [in] lng,lat Celestial longitude and latitude [deg].
      [out] phi,theta Longitude and latitude in the native coordinate system of the projection [deg]. These may refer to the same storage as lng and lat respectively.
      Returns:
      Status return value:
      • 0: Success.

      int sphdpa ( int  nfield,
      double  lng0,
      double  lat0,
      const double  lng[],
      const double  lat[],
      double  dist[],
      double  pa[] 
      )

      sphdpa() computes the angular distance and generalized position angle (see notes) from a "reference" point to a number of "field" points on the sphere. The points must be specified consistently in any spherical coordinate system.

      sphdpa() is complementary to sphpad().

      Parameters:
      [in] nfield The number of field points.
      [in] lng0,lat0 Spherical coordinates of the reference point [deg].
      [in] lng,lat Spherical coordinates of the field points [deg].
      [out] dist,pa Angular distances and position angles [deg]. These may refer to the same storage as lng and lat respectively.
      Returns:
      Status return value:
      • 0: Success.
      Notes:
      sphdpa() uses sphs2x() to rotate coordinates so that the reference point is at the north pole of the new system with the north pole of the old system at zero longitude in the new. The Euler angles required by sphs2x() for this rotation are 
            eul[0] = lng0;
      eul[1] = 90.0 - lat0;
      eul[2] =  0.0;

      The angular distance and generalized position angle are readily obtained from the longitude and latitude of the field point in the new system. This applies even if the reference point is at one of the poles, in which case the "position angle" returned is as would be computed for a reference point at $(\alpha_0,+90^\circ-\epsilon)$ or $(\alpha_0,-90^\circ+\epsilon)$, in the limit as $\epsilon$ goes to zero.

      It is evident that the coordinate system in which the two points are expressed is irrelevant to the determination of the angular separation between the points. However, this is not true of the generalized position angle.

      The generalized position angle is here defined as the angle of intersection of the great circle containing the reference and field points with that containing the reference point and the pole. It has its normal meaning when the the reference and field points are specified in equatorial coordinates (right ascension and declination).

      Interchanging the reference and field points changes the position angle in a non-intuitive way (because the sum of the angles of a spherical triangle normally exceeds $180^\circ$).

      The position angle is undefined if the reference and field points are coincident or antipodal. This may be detected by checking for a distance of $0^\circ$ or $180^\circ$ (within rounding tolerance). sphdpa() will return an arbitrary position angle in such circumstances.

      int sphpad ( int  nfield,
      double  lng0,
      double  lat0,
      const double  dist[],
      const double  pa[],
      double  lng[],
      double  lat[] 
      )

      sphpad() computes the coordinates of a set of points that are offset by the specified angular distances and position angles from a given "reference" point on the sky. The distances and position angles must be specified consistently in any spherical coordinate system.

      sphpad() is complementary to sphdpa().

      Parameters:
      [in] nfield The number of field points.
      [in] lng0,lat0 Spherical coordinates of the reference point [deg].
      [in] dist,pa Angular distances and position angles [deg].
      [out] lng,lat Spherical coordinates of the field points [deg]. These may refer to the same storage as dist and pa respectively.
      Returns:
      Status return value:
      • 0: Success.
      Notes:
      sphpad() is implemented analogously to sphdpa() although using sphx2s() for the inverse transformation. In particular, when the reference point is at one of the poles, "position angle" is interpreted as though the reference point was at $(\alpha_0,+90^\circ-\epsilon)$ or $(\alpha_0,-90^\circ+\epsilon)$, in the limit as $\epsilon$ goes to zero.

      Applying sphpad() with the distances and position angles computed by sphdpa() should return the original field points.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/spx_8h-source.html0000644001153600020070000017622512310355626022507 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: spx.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/spx_8h.html0000644001153600020070000015465612310355626021215 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: spx.h File Reference

      spx.h File Reference

      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  spxprm
       Spectral variables and their derivatives. More...

      Defines

      #define SPXLEN   (sizeof(struct spxprm)/sizeof(int))
       Size of the spxprm struct in int units.
      #define SPX_ARGS
       For use in declaring spectral conversion function prototypes.

      Enumerations

      enum  spx_errmsg {
        SPXERR_SUCCESS = 0, SPXERR_NULL_POINTER = 1, SPXERR_BAD_SPEC_PARAMS = 2, SPXERR_BAD_SPEC_VAR = 3,
        SPXERR_BAD_INSPEC_COORD = 4
      }

      Functions

      int specx (const char *type, double spec, double restfrq, double restwav, struct spxprm *specs)
       Spectral cross conversions (scalar).
      int freqafrq (SPX_ARGS)
       Convert frequency to angular frequency (vector).
      int afrqfreq (SPX_ARGS)
       Convert angular frequency to frequency (vector).
      int freqener (SPX_ARGS)
       Convert frequency to photon energy (vector).
      int enerfreq (SPX_ARGS)
       Convert photon energy to frequency (vector).
      int freqwavn (SPX_ARGS)
       Convert frequency to wave number (vector).
      int wavnfreq (SPX_ARGS)
       Convert wave number to frequency (vector).
      int freqwave (SPX_ARGS)
       Convert frequency to vacuum wavelength (vector).
      int wavefreq (SPX_ARGS)
       Convert vacuum wavelength to frequency (vector).
      int freqawav (SPX_ARGS)
       Convert frequency to air wavelength (vector).
      int awavfreq (SPX_ARGS)
       Convert air wavelength to frequency (vector).
      int waveawav (SPX_ARGS)
       Convert vacuum wavelength to air wavelength (vector).
      int awavwave (SPX_ARGS)
       Convert air wavelength to vacuum wavelength (vector).
      int velobeta (SPX_ARGS)
       Convert relativistic velocity to relativistic beta (vector).
      int betavelo (SPX_ARGS)
       Convert relativistic beta to relativistic velocity (vector).
      int freqvelo (SPX_ARGS)
       Convert frequency to relativistic velocity (vector).
      int velofreq (SPX_ARGS)
       Convert relativistic velocity to frequency (vector).
      int freqvrad (SPX_ARGS)
       Convert frequency to radio velocity (vector).
      int vradfreq (SPX_ARGS)
       Convert radio velocity to frequency (vector).
      int wavevelo (SPX_ARGS)
       Conversions between wavelength and velocity types (vector).
      int velowave (SPX_ARGS)
       Convert relativistic velocity to vacuum wavelength (vector).
      int awavvelo (SPX_ARGS)
       Convert air wavelength to relativistic velocity (vector).
      int veloawav (SPX_ARGS)
       Convert relativistic velocity to air wavelength (vector).
      int wavevopt (SPX_ARGS)
       Convert vacuum wavelength to optical velocity (vector).
      int voptwave (SPX_ARGS)
       Convert optical velocity to vacuum wavelength (vector).
      int wavezopt (SPX_ARGS)
       Convert vacuum wavelength to redshift (vector).
      int zoptwave (SPX_ARGS)
       Convert redshift to vacuum wavelength (vector).

      Variables

      const char * spx_errmsg []

      Detailed Description

      specx() is a scalar routine that, given one spectral variable (e.g. frequency), computes all the others (e.g. wavelength, velocity, etc.) plus the required derivatives of each with respect to the others. The results are returned in the spxprm struct.

      The remaining routines are all vector conversions from one spectral variable to another. The API of these functions only differ in whether the rest frequency or wavelength need be supplied.

      Non-linear:

      Linear:

      These are the workhorse routines, to be used for fast transformations. Conversions may be done "in place" by calling the routine with the output vector set to the input.

      Argument checking:
      The input spectral values are only checked for values that would result in floating point exceptions. In particular, negative frequencies and wavelengths are allowed, as are velocities greater than the speed of light. The same is true for the spectral parameters - rest frequency and wavelength.

      Accuracy:
      No warranty is given for the accuracy of these routines (refer to the copyright notice); intending users must satisfy for themselves their adequacy for the intended purpose. However, closure effectively to within double precision rounding error was demonstrated by test routine tspec.c which accompanies this software.

      Define Documentation

      #define SPXLEN   (sizeof(struct spxprm)/sizeof(int))

      Size of the spxprm struct in int units, used by the Fortran wrappers.

      #define SPX_ARGS

      Value:

      double param, int nspec, int instep, int outstep, \
    const double inspec[], double outspec[], int stat[]
      Preprocessor macro used for declaring spectral conversion function prototypes.

      Enumeration Type Documentation

      enum spx_errmsg

      Enumerator:
      SPXERR_SUCCESS 
      SPXERR_NULL_POINTER 
      SPXERR_BAD_SPEC_PARAMS 
      SPXERR_BAD_SPEC_VAR 
      SPXERR_BAD_INSPEC_COORD 

      Function Documentation

      int specx ( const char *  type,
      double  spec,
      double  restfrq,
      double  restwav,
      struct spxprm *  specs 
      )

      Given one spectral variable specx() computes all the others, plus the required derivatives of each with respect to the others.

      Parameters:
      [in] type The type of spectral variable given by spec, FREQ, AFRQ, ENER, WAVN, VRAD, WAVE, VOPT, ZOPT, AWAV, VELO, or BETA (case sensitive).
      [in] spec The spectral variable given, in SI units.
      [in] restfrq,restwav Rest frequency [Hz] or rest wavelength in vacuo [m], only one of which need be given. The other should be set to zero. If both are zero, only a subset of the spectral variables can be computed, the remainder are set to zero. Specifically, given one of FREQ, AFRQ, ENER, WAVN, WAVE, or AWAV the others can be computed without knowledge of the rest frequency. Likewise, VRAD, VOPT, ZOPT, VELO, and BETA.
      [in,out] specs Data structure containing all spectral variables and their derivatives, in SI units.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null spxprm pointer passed.
      • 2: Invalid spectral parameters.
      • 3: Invalid spectral variable.
      For returns > 1, a detailed error message is set in spxprm::err if enabled, see wcserr_enable().
      freqafrq(), afrqfreq(), freqener(), enerfreq(), freqwavn(), wavnfreq(), freqwave(), wavefreq(), freqawav(), awavfreq(), waveawav(), awavwave(), velobeta(), and betavelo() implement vector conversions between wave-like or velocity-like spectral types (i.e. conversions that do not need the rest frequency or wavelength). They all have the same API.

      int freqafrq ( SPX_ARGS   ) 

      freqafrq() converts frequency to angular frequency.

      Parameters:
      [in] param Ignored.
      [in] nspec Vector length.
      [in] instep,outstep Vector strides.
      [in] inspec Input spectral variables, in SI units.
      [out] outspec Output spectral variables, in SI units.
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of inspec.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters.
      • 4: One or more of the inspec coordinates were invalid, as indicated by the stat vector.

      int afrqfreq ( SPX_ARGS   ) 

      afrqfreq() converts angular frequency to frequency.

      See freqafrq() for a description of the API.

      int freqener ( SPX_ARGS   ) 

      freqener() converts frequency to photon energy.

      See freqafrq() for a description of the API.

      int enerfreq ( SPX_ARGS   ) 

      enerfreq() converts photon energy to frequency.

      See freqafrq() for a description of the API.

      int freqwavn ( SPX_ARGS   ) 

      freqwavn() converts frequency to wave number.

      See freqafrq() for a description of the API.

      int wavnfreq ( SPX_ARGS   ) 

      wavnfreq() converts wave number to frequency.

      See freqafrq() for a description of the API.

      int freqwave ( SPX_ARGS   ) 

      freqwave() converts frequency to vacuum wavelength.

      See freqafrq() for a description of the API.

      int wavefreq ( SPX_ARGS   ) 

      wavefreq() converts vacuum wavelength to frequency.

      See freqafrq() for a description of the API.

      int freqawav ( SPX_ARGS   ) 

      freqawav() converts frequency to air wavelength.

      See freqafrq() for a description of the API.

      int awavfreq ( SPX_ARGS   ) 

      awavfreq() converts air wavelength to frequency.

      See freqafrq() for a description of the API.

      int waveawav ( SPX_ARGS   ) 

      waveawav() converts vacuum wavelength to air wavelength.

      See freqafrq() for a description of the API.

      int awavwave ( SPX_ARGS   ) 

      awavwave() converts air wavelength to vacuum wavelength.

      See freqafrq() for a description of the API.

      int velobeta ( SPX_ARGS   ) 

      velobeta() converts relativistic velocity to relativistic beta.

      See freqafrq() for a description of the API.

      int betavelo ( SPX_ARGS   ) 

      betavelo() converts relativistic beta to relativistic velocity.

      See freqafrq() for a description of the API.

      int freqvelo ( SPX_ARGS   ) 

      freqvelo() converts frequency to relativistic velocity.

      Parameters:
      [in] param Rest frequency [Hz].
      [in] nspec Vector length.
      [in] instep,outstep Vector strides.
      [in] inspec Input spectral variables, in SI units.
      [out] outspec Output spectral variables, in SI units.
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of inspec.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters.
      • 4: One or more of the inspec coordinates were invalid, as indicated by the stat vector.

      int velofreq ( SPX_ARGS   ) 

      velofreq() converts relativistic velocity to frequency.

      See freqvelo() for a description of the API.

      int freqvrad ( SPX_ARGS   ) 

      freqvrad() converts frequency to radio velocity.

      See freqvelo() for a description of the API.

      int vradfreq ( SPX_ARGS   ) 

      vradfreq() converts radio velocity to frequency.

      See freqvelo() for a description of the API.

      int wavevelo ( SPX_ARGS   ) 

      wavevelo() converts vacuum wavelength to relativistic velocity.

      Parameters:
      [in] param Rest wavelength in vacuo [m].
      [in] nspec Vector length.
      [in] instep,outstep Vector strides.
      [in] inspec Input spectral variables, in SI units.
      [out] outspec Output spectral variables, in SI units.
      [out] stat Status return value for each vector element:
      • 0: Success.
      • 1: Invalid value of inspec.
      Returns:
      Status return value:
      • 0: Success.
      • 2: Invalid spectral parameters.
      • 4: One or more of the inspec coordinates were invalid, as indicated by the stat vector.

      int velowave ( SPX_ARGS   ) 

      velowave() converts relativistic velocity to vacuum wavelength.

      See freqvelo() for a description of the API.

      int awavvelo ( SPX_ARGS   ) 

      awavvelo() converts air wavelength to relativistic velocity.

      See freqvelo() for a description of the API.

      int veloawav ( SPX_ARGS   ) 

      veloawav() converts relativistic velocity to air wavelength.

      See freqvelo() for a description of the API.

      int wavevopt ( SPX_ARGS   ) 

      wavevopt() converts vacuum wavelength to optical velocity.

      See freqvelo() for a description of the API.

      int voptwave ( SPX_ARGS   ) 

      voptwave() converts optical velocity to vacuum wavelength.

      See freqvelo() for a description of the API.

      int wavezopt ( SPX_ARGS   ) 

      wavevopt() converts vacuum wavelength to redshift.

      See freqvelo() for a description of the API.

      int zoptwave ( SPX_ARGS   ) 

      zoptwave() converts redshift to vacuum wavelength.

      See freqvelo() for a description of the API.

      Variable Documentation

      const char* spx_errmsg[]

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structcelprm.html0000644001153600020070000004174112310355626022521 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: celprm Struct Reference

      celprm Struct Reference

      Celestial transformation parameters. More...

      #include <cel.h>


      Data Fields

      int flag
      int offset
      double phi0
      double theta0
      double ref [4]
      struct prjprm prj
      double euler [5]
      int latpreq
      int isolat
      struct wcserr * err
      void * padding

      Detailed Description

      The celprm struct contains information required to transform celestial coordinates. It consists of certain members that must be set by the user (given) and others that are set by the WCSLIB routines (returned). Some of the latter are supplied for informational purposes and others are for internal use only.

      Returned celprm struct members must not be modified by the user.

      Field Documentation

      int celprm::flag

      (Given and returned) This flag must be set to zero whenever any of the following celprm struct members are set or changed:

      This signals the initialization routine, celset(), to recompute the returned members of the celprm struct. celset() will reset flag to indicate that this has been done.

      int celprm::offset

      (Given) If true (non-zero), an offset will be applied to $(x,y)$ to force $(x,y)$ = (0,0) at the fiducial point, ($\phi_0$,$\theta_0$). Default is 0 (false).

      double celprm::phi0

      (Given) The native longitude, $\phi_0$ [deg], and ...

      double celprm::theta0

      (Given) ... the native latitude, $\theta_0$ [deg], of the fiducial point, i.e. the point whose celestial coordinates are given in celprm::ref[1:2]. If undefined (set to a magic value by prjini()) the initialization routine, celset(), will set this to a projection-specific default.

      double celprm::ref

      (Given) The first pair of values should be set to the celestial longitude and latitude of the fiducial point [deg] - typically right ascension and declination. These are given by the CRVALia keywords in FITS.

      (Given and returned) The second pair of values are the native longitude, $\phi_{\mathrm p}$ [deg], and latitude, $\theta_{\mathrm p}$ [deg], of the celestial pole (the latter is the same as the celestial latitude of the native pole, $\delta_{\mathrm p}$) and these are given by the FITS keywords LONPOLEa and LATPOLEa (or by PVi_2a and PVi_3a attached to the longitude axis which take precedence if defined).

      LONPOLEa defaults to $\phi_0$ (see above) if the celestial latitude of the fiducial point of the projection is greater than or equal to the native latitude, otherwise $\phi_0$ + 180 [deg]. (This is the condition for the celestial latitude to increase in the same direction as the native latitude at the fiducial point.) ref[2] may be set to UNDEFINED (from wcsmath.h) or 999.0 to indicate that the correct default should be substituted.

      $\theta_{\mathrm p}$, the native latitude of the celestial pole (or equally the celestial latitude of the native pole, $\delta_{\mathrm p}$) is often determined uniquely by CRVALia and LONPOLEa in which case LATPOLEa is ignored. However, in some circumstances there are two valid solutions for $\theta_{\mathrm p}$ and LATPOLEa is used to choose between them. LATPOLEa is set in ref[3] and the solution closest to this value is used to reset ref[3]. It is therefore legitimate, for example, to set ref[3] to +90.0 to choose the more northerly solution - the default if the LATPOLEa keyword is omitted from the FITS header. For the special case where the fiducial point of the projection is at native latitude zero, its celestial latitude is zero, and LONPOLEa = $\pm$ 90.0 then the celestial latitude of the native pole is not determined by the first three reference values and LATPOLEa specifies it completely.

      The returned value, celprm::latpreq, specifies how LATPOLEa was actually used.

      struct prjprm celprm::prj [read]

      (Given and returned) Projection parameters described in the prologue to prj.h.

      double celprm::euler

      (Returned) Euler angles and associated intermediaries derived from the coordinate reference values. The first three values are the $Z$-, $X$-, and $Z'$-Euler angles [deg], and the remaining two are the cosine and sine of the $X$-Euler angle.

      int celprm::latpreq

      (Returned) For informational purposes, this indicates how the LATPOLEa keyword was used

      • 0: Not required, $\theta_{\mathrm p}$ (== $\delta_{\mathrm p}$) was determined uniquely by the CRVALia and LONPOLEa keywords.
      • 1: Required to select between two valid solutions of $\theta_{\mathrm p}$.
      • 2: $\theta_{\mathrm p}$ was specified solely by LATPOLEa.

      int celprm::isolat

      (Returned) True if the spherical rotation preserves the magnitude of the latitude, which occurs iff the axes of the native and celestial coordinates are coincident. It signals an opportunity to cache intermediate calculations common to all elements in a vector computation.

      struct wcserr * celprm::err [read]

      (Returned) If enabled, when an error status is returned this struct contains detailed information about the error, see wcserr_enable().

      void *padding (An unused variable inserted for alignment purposes only.)

      Global variable: const char *cel_errmsg[] - Status return messages Status messages to match the status value returned from each function.

      void* celprm::padding

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structfitskey.html0000644001153600020070000005257712310355626022726 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: fitskey Struct Reference

      fitskey Struct Reference

      Keyword/value information. More...

      #include <fitshdr.h>


      Data Fields

      int keyno
      int keyid
      int status
      char keyword [12]
      int type
      int padding
      union {
         int   i
         int64   k
         int   l [8]
         double   f
         double   c [2]
         char   s [72]
      } keyvalue
      int ulen
      char comment [84]

      Detailed Description

      fitshdr() returns an array of fitskey structs, each of which contains the result of parsing one FITS header keyrecord. All members of the fitskey struct are returned by fitshdr(), none are given by the user.

      Field Documentation

      int fitskey::keyno

      (Returned) Keyrecord number (1-relative) in the array passed as input to fitshdr(). This will be negated if the keyword matched any specified in the keyids[] index.

      int fitskey::keyid

      (Returned) Index into the first entry in keyids[] with which the keyrecord matches, else -1.

      int fitskey::status

      (Returned) Status flag bit-vector for the header keyrecord employing the following bit masks defined as preprocessor macros:

      • FITSHDR_KEYWORD: Illegal keyword syntax.
      • FITSHDR_KEYVALUE: Illegal keyvalue syntax.
      • FITSHDR_COMMENT: Illegal keycomment syntax.
      • FITSHDR_KEYREC: Illegal keyrecord, e.g. an END keyrecord with trailing text.
      • FITSHDR_TRAILER: Keyrecord following a valid END keyrecord.

      The header keyrecord is syntactically correct if no bits are set.

      char fitskey::keyword

      (Returned) Keyword name, null-filled for keywords of less than eight characters (trailing blanks replaced by nulls).

      Use 

              sprintf(dst, "%.8s", keyword)

      to copy it to a character array with null-termination, or 

              sprintf(dst, "%8.8s", keyword)

      to blank-fill to eight characters followed by null-termination.

      int fitskey::type

      (Returned) Keyvalue data type:

      • 0: No keyvalue.
      • 1: Logical, represented as int.
      • 2: 32-bit signed integer.
      • 3: 64-bit signed integer (see below).
      • 4: Very long integer (see below).
      • 5: Floating point (stored as double).
      • 6: Integer complex (stored as double[2]).
      • 7: Floating point complex (stored as double[2]).
      • 8: String.
      • 8+10*n: Continued string (described below and in fitshdr() note 2).

      A negative type indicates that a syntax error was encountered when attempting to parse a keyvalue of the particular type.

      Comments on particular data types:

      • 64-bit signed integers lie in the range 
                    (-9223372036854775808 <= int64 <  -2147483648) ||
                     (+2147483647 <  int64 <= +9223372036854775807)

        A native 64-bit data type may be defined via preprocessor macro WCSLIB_INT64 defined in wcsconfig.h, e.g. as 'long long int'; this will be typedef'd to 'int64' here. If WCSLIB_INT64 is not set, then int64 is typedef'd to int[3] instead and fitskey::keyvalue is to be computed as 

                    ((keyvalue.k[2]) * 1000000000 +
              keyvalue.k[1]) * 1000000000 +
              keyvalue.k[0]

        and may reported via 

                     if (keyvalue.k[2]) {
               printf("%d%09d%09d", keyvalue.k[2], abs(keyvalue.k[1]),
                                    abs(keyvalue.k[0]));
             } else {
               printf("%d%09d", keyvalue.k[1], abs(keyvalue.k[0]));
             }

        where keyvalue.k[0] and keyvalue.k[1] range from -999999999 to +999999999.

      • Very long integers, up to 70 decimal digits in length, are encoded in keyvalue.l as an array of int[8], each of which stores 9 decimal digits. fitskey::keyvalue is to be computed as 
                    (((((((keyvalue.l[7]) * 1000000000 +
                   keyvalue.l[6]) * 1000000000 +
                   keyvalue.l[5]) * 1000000000 +
                   keyvalue.l[4]) * 1000000000 +
                   keyvalue.l[3]) * 1000000000 +
                   keyvalue.l[2]) * 1000000000 +
                   keyvalue.l[1]) * 1000000000 +
                   keyvalue.l[0]

      • Continued strings are not reconstructed, they remain split over successive fitskey structs in the keys[] array returned by fitshdr(). fitskey::keyvalue data type, 8 + 10n, indicates the segment number, n, in the continuation.

      int fitskey::padding

      (An unused variable inserted for alignment purposes only.)

      int fitskey::i

      (Returned) Logical (fitskey::type == 1) and 32-bit signed integer (fitskey::type == 2) data types in the fitskey::keyvalue union.

      int64 fitskey::k

      (Returned) 64-bit signed integer (fitskey::type == 3) data type in the fitskey::keyvalue union.

      int fitskey::l

      (Returned) Very long integer (fitskey::type == 4) data type in the fitskey::keyvalue union.

      double fitskey::f

      (Returned) Floating point (fitskey::type == 5) data type in the fitskey::keyvalue union.

      double fitskey::c

      (Returned) Integer and floating point complex (fitskey::type == 6 || 7) data types in the fitskey::keyvalue union.

      char fitskey::s

      (Returned) Null-terminated string (fitskey::type == 8) data type in the fitskey::keyvalue union.

      union fitskey::keyvalue

      (Returned) A union comprised of

      used by the fitskey struct to contain the value associated with a keyword.

      int fitskey::ulen

      (Returned) Where a keycomment contains a units string in the standard form, e.g. [m/s], the ulen member indicates its length, inclusive of square brackets. Otherwise ulen is zero.

      char fitskey::comment

      (Returned) Keycomment, i.e. comment associated with the keyword or, for keyrecords rejected because of syntax errors, the compete keyrecord itself with null-termination.

      Comments are null-terminated with trailing spaces removed. Leading spaces are also removed from keycomments (i.e. those immediately following the '/' character), but not from COMMENT or HISTORY keyrecords or keyrecords without a value indicator (''= '' in columns 9-80).

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structfitskeyid.html0000644001153600020070000001203512310355626023224 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: fitskeyid Struct Reference

      fitskeyid Struct Reference

      Keyword indexing. More...

      #include <fitshdr.h>


      Data Fields

      char name [12]
      int count
      int idx [2]

      Detailed Description

      fitshdr() uses the fitskeyid struct to return indexing information for specified keywords. The struct contains three members, the first of which, fitskeyid::name, must be set by the user with the remainder returned by fitshdr().

      Field Documentation

      char fitskeyid::name

      (Given) Name of the required keyword. This is to be set by the user; the '.' character may be used for wildcarding. Trailing blanks will be replaced with nulls.

      int fitskeyid::count

      (Returned) The number of matches found for the keyword.

      int fitskeyid::idx

      (Returned) Indices into keys[], the array of fitskey structs returned by fitshdr(). Note that these are 0-relative array indices, not keyrecord numbers.

      If the keyword is found in the header the first index will be set to the array index of its first occurrence, otherwise it will be set to -1.

      If multiples of the keyword are found, the second index will be set to the array index of its last occurrence, otherwise it will be set to -1.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structlinprm.html0000644001153600020070000004337012310355626022540 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: linprm Struct Reference

      linprm Struct Reference

      Linear transformation parameters. More...

      #include <lin.h>


      Data Fields

      int flag
      int naxis
      double * crpix
      double * pc
      double * cdelt
      double * piximg
      double * imgpix
      int unity
      int padding
      struct wcserr * err
      int i_naxis
      int m_flag
      int m_naxis
      int m_padding
      double * m_crpix
      double * m_pc
      double * m_cdelt
      void * padding2

      Detailed Description

      The linprm struct contains all of the information required to perform a linear transformation. It consists of certain members that must be set by the user (given) and others that are set by the WCSLIB routines (returned).

      Field Documentation

      int linprm::flag

      (Given and returned) This flag must be set to zero whenever any of the following members of the linprm struct are set or modified:

      This signals the initialization routine, linset(), to recompute the returned members of the linprm struct. linset() will reset flag to indicate that this has been done.

      PLEASE NOTE: flag should be set to -1 when linini() is called for the first time for a particular linprm struct in order to initialize memory management. It must ONLY be used on the first initialization otherwise memory leaks may result.

      int linprm::naxis

      (Given or returned) Number of pixel and world coordinate elements.

      If linini() is used to initialize the linprm struct (as would normally be the case) then it will set naxis from the value passed to it as a function argument. The user should not subsequently modify it.

      double * linprm::crpix

      (Given) Pointer to the first element of an array of double containing the coordinate reference pixel, CRPIXja.

      double * linprm::pc

      (Given) Pointer to the first element of the PCi_ja (pixel coordinate) transformation matrix. The expected order is 

              struct linprm lin;
        lin.pc = {PC1_1, PC1_2, PC2_1, PC2_2};

      This may be constructed conveniently from a 2-D array via 

              double m[2][2] = {{PC1_1, PC1_2},
                          {PC2_1, PC2_2}};

      which is equivalent to 

              double m[2][2];
        m[0][0] = PC1_1;
        m[0][1] = PC1_2;
        m[1][0] = PC2_1;
        m[1][1] = PC2_2;

      The storage order for this 2-D array is the same as for the 1-D array, whence 

              lin.pc = *m;

      would be legitimate.

      double * linprm::cdelt

      (Given) Pointer to the first element of an array of double containing the coordinate increments, CDELTia.

      double * linprm::piximg

      (Returned) Pointer to the first element of the matrix containing the product of the CDELTia diagonal matrix and the PCi_ja matrix.

      double * linprm::imgpix

      (Returned) Pointer to the first element of the inverse of the linprm::piximg matrix.

      int linprm::unity

      (Returned) True if the linear transformation matrix is unity.

      int linprm::padding

      (An unused variable inserted for alignment purposes only.)

      struct wcserr * linprm::err [read]

      (Returned) If enabled, when an error status is returned this struct contains detailed information about the error, see wcserr_enable().

      int linprm::i_naxis

      (For internal use only.)

      int linprm::m_flag

      (For internal use only.)

      int linprm::m_naxis

      (For internal use only.)

      int linprm::m_padding

      (For internal use only.)

      double * linprm::m_crpix

      (For internal use only.)

      double * linprm::m_pc

      (For internal use only.)

      double * linprm::m_cdelt

      (For internal use only.) void *padding2 (For internal use only.)

      void* linprm::padding2

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structprjprm.html0000644001153600020070000005771112310355626022555 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: prjprm Struct Reference

      prjprm Struct Reference

      Projection parameters. More...

      #include <prj.h>


      Data Fields

      int flag
      char code [4]
      double r0
      double pv [PVN]
      double phi0
      double theta0
      int bounds
      char name [40]
      int category
      int pvrange
      int simplezen
      int equiareal
      int conformal
      int global
      int divergent
      double x0
      double y0
      struct wcserr * err
      void * padding
      double w [10]
      int m
      int n
      int(* prjx2s )(PRJX2S_ARGS)
      int(* prjs2x )(PRJS2X_ARGS)

      Detailed Description

      The prjprm struct contains all information needed to project or deproject native spherical coordinates. It consists of certain members that must be set by the user (given) and others that are set by the WCSLIB routines (returned). Some of the latter are supplied for informational purposes while others are for internal use only.

      Field Documentation

      int prjprm::flag

      (Given and returned) This flag must be set to zero whenever any of the following prjprm struct members are set or changed:

      This signals the initialization routine (prjset() or ???set()) to recompute the returned members of the prjprm struct. flag will then be reset to indicate that this has been done.

      Note that flag need not be reset when prjprm::bounds is changed.

      char prjprm::code

      (Given) Three-letter projection code defined by the FITS standard.

      double prjprm::r0

      (Given) The radius of the generating sphere for the projection, a linear scaling parameter. If this is zero, it will be reset to its default value of $180^\circ/\pi$ (the value for FITS WCS).

      double prjprm::pv

      (Given) Projection parameters. These correspond to the PVi_ma keywords in FITS, so pv[0] is PVi_0a, pv[1] is PVi_1a, etc., where i denotes the latitude-like axis. Many projections use pv[1] (PVi_1a), some also use pv[2] (PVi_2a) and SZP uses pv[3] (PVi_3a). ZPN is currently the only projection that uses any of the others.

      Usage of the pv[] array as it applies to each projection is described in the prologue to each trio of projection routines in prj.c.

      double prjprm::phi0

      (Given) The native longitude, $\phi_0$ [deg], and ...

      double prjprm::theta0

      (Given) ... the native latitude, $\theta_0$ [deg], of the reference point, i.e. the point $(x,y)$ = (0,0). If undefined (set to a magic value by prjini()) the initialization routine will set this to a projection-specific default.

      int prjprm::bounds

      (Given) Controls strict bounds checking for the AZP, SZP, TAN, SIN, ZPN, and COP projections; set to zero to disable checking.

      The remaining members of the prjprm struct are maintained by the setup routines and must not be modified elsewhere:

      char prjprm::name

      (Returned) Long name of the projection.

      Provided for information only, not used by the projection routines.

      int prjprm::category

      (Returned) Projection category matching the value of the relevant global variable:

      • ZENITHAL,
      • CYLINDRICAL,
      • PSEUDOCYLINDRICAL,
      • CONVENTIONAL,
      • CONIC,
      • POLYCONIC,
      • QUADCUBE, and
      • HEALPIX.

      The category name may be identified via the prj_categories character array, e.g. 

              struct prjprm prj;
          ...
        printf("%s\n", prj_categories[prj.category]);

      Provided for information only, not used by the projection routines.

      int prjprm::pvrange

      (Returned) Range of projection parameter indices: 100 times the first allowed index plus the number of parameters, e.g. TAN is 0 (no parameters), SZP is 103 (1 to 3), and ZPN is 30 (0 to 29).

      Provided for information only, not used by the projection routines.

      int prjprm::simplezen

      (Returned) True if the projection is a radially-symmetric zenithal projection.

      Provided for information only, not used by the projection routines.

      int prjprm::equiareal

      (Returned) True if the projection is equal area.

      Provided for information only, not used by the projection routines.

      int prjprm::conformal

      (Returned) True if the projection is conformal.

      Provided for information only, not used by the projection routines.

      int prjprm::global

      (Returned) True if the projection can represent the whole sphere in a finite, non-overlapped mapping.

      Provided for information only, not used by the projection routines.

      int prjprm::divergent

      (Returned) True if the projection diverges in latitude.

      Provided for information only, not used by the projection routines.

      double prjprm::x0

      (Returned) The offset in $x$,and ...

      double prjprm::y0

      (Returned) ... the offset in $y$ used to force $(x,y)$ = (0,0) at ($\phi_0$,$\theta_0$).

      struct wcserr * prjprm::err [read]

      (Returned) If enabled, when an error status is returned this struct contains detailed information about the error, see wcserr_enable().

      void *padding (An unused variable inserted for alignment purposes only.)

      void* prjprm::padding

      double prjprm::w

      (Returned) Intermediate floating-point values derived from the projection parameters, cached here to save recomputation.

      Usage of the w[] array as it applies to each projection is described in the prologue to each trio of projection routines in prj.c.

      int prjprm::m

      int prjprm::n

      (Returned) Intermediate integer value (used only for the ZPN and HPX projections).

      prjprm::prjx2s

      (Returned) Pointer to the projection ...

      prjprm::prjs2x

      (Returned) ... and deprojection routines.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structpscard.html0000644001153600020070000001037412310355626022511 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: pscard Struct Reference

      pscard Struct Reference

      Store for PSi_ma keyrecords. More...

      #include <wcs.h>


      Data Fields

      int i
      int m
      char value [72]

      Detailed Description

      The pscard struct is used to pass the parsed contents of PSi_ma keyrecords to wcsset() via the wcsprm struct.

      All members of this struct are to be set by the user.

      Field Documentation

      int pscard::i

      (Given) Axis number (1-relative), as in the FITS PSi_ma keyword.

      int pscard::m

      (Given) Parameter number (non-negative), as in the FITS PSi_ma keyword.

      char pscard::value

      (Given) Parameter value.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structpvcard.html0000644001153600020070000001065512310355626022516 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: pvcard Struct Reference

      pvcard Struct Reference

      Store for PVi_ma keyrecords. More...

      #include <wcs.h>


      Data Fields

      int i
      int m
      double value

      Detailed Description

      The pvcard struct is used to pass the parsed contents of PVi_ma keyrecords to wcsset() via the wcsprm struct.

      All members of this struct are to be set by the user.

      Field Documentation

      int pvcard::i

      (Given) Axis number (1-relative), as in the FITS PVi_ma keyword. If i == 0, wcsset() will replace it with the latitude axis number.

      int pvcard::m

      (Given) Parameter number (non-negative), as in the FITS PVi_ma keyword.

      double pvcard::value

      (Given) Parameter value.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structs.html0000644001153600020070000001527712310355626021506 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: WCSLIB data structures

      WCSLIB data structures

      The WCSLIB routines are based on data structures specific to them: wcsprm for the wcs.h,c routines, celprm for cel.h,c, and likewise spcprm, linprm, prjprm and tabprm, with struct definitions contained in the corresponding header files: wcs.h, cel.h, etc. The structs store the parameters that define a coordinate transformation and also intermediate values derived from those parameters. As a high-level object, the wcsprm struct contains linprm, tabprm, spcprm, and celprm structs, and in turn the celprm struct contains a prjprm struct. Hence the wcsprm struct contains everything needed for a complete coordinate description.

      Applications programmers who use the top- and middle-level routines generally only need to pass wcsprm structs from one routine that fills them to another that uses them. However, since these structs are fundamental to WCSLIB it is worthwhile knowing something about the way they work.

      Three basic operations apply to all WCSLIB structs:

      • Initialize. Each struct has a specific initialization routine, e.g. wcsini(), celini(), spcini(), etc. These allocate memory (if required) and set all struct members to default values.

      • Fill in the required values. Each struct has members whose values must be provided. For example, for wcsprm these values correspond to FITS WCS header keyvalues as are provided by the top-level header parsing routine, wcspih().

      • Compute intermediate values. Specific setup routines, e.g. wcsset(), celset(), spcset(), etc., compute intermediate values from the values provided. In particular, wcsset() analyses the FITS WCS keyvalues provided, fills the required values in the lower-level structs contained in wcsprm, and invokes the setup routine for each of them.

      Each struct contains a flag member that records its setup state. This is cleared by the initialization routine and checked by the routines that use the struct; they will invoke the setup routine automatically if necessary, hence it need not be invoked specifically by the application programmer. However, if any of the required values in a struct are changed then either the setup routine must be invoked on it, or else the flag must be zeroed to signal that the struct needs to be reset.

      The initialization routine may be invoked repeatedly on a struct if it is desired to reuse it. However, the flag member of structs that contain allocated memory (wcsprm, linprm and tabprm) must be set to -1 before the first initialization to initialize memory management, but not subsequently or else memory leaks will result.

      Each struct has one or more service routines: to do deep copies from one to another, to print its contents, and to free allocated memory. Refer to the header files for a detailed description.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structspcprm.html0000644001153600020070000004325312310355626022543 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: spcprm Struct Reference

      spcprm Struct Reference

      Spectral transformation parameters. More...

      #include <spc.h>


      Data Fields

      int flag
      char type [8]
      char code [4]
      double crval
      double restfrq
      double restwav
      double pv [7]
      double w [6]
      int isGrism
      int padding1
      struct wcserr * err
      void * padding2
      int(* spxX2P )(SPX_ARGS)
      int(* spxP2S )(SPX_ARGS)
      int(* spxS2P )(SPX_ARGS)
      int(* spxP2X )(SPX_ARGS)

      Detailed Description

      The spcprm struct contains information required to transform spectral coordinates. It consists of certain members that must be set by the user (given) and others that are set by the WCSLIB routines (returned). Some of the latter are supplied for informational purposes while others are for internal use only.

      Field Documentation

      int spcprm::flag

      (Given and returned) This flag must be set to zero whenever any of the following spcprm structure members are set or changed:

      This signals the initialization routine, spcset(), to recompute the returned members of the spcprm struct. spcset() will reset flag to indicate that this has been done.

      char spcprm::type

      (Given) Four-letter spectral variable type, e.g "ZOPT" for CTYPEia = 'ZOPT-F2W'. (Declared as char[8] for alignment reasons.)

      char spcprm::code

      (Given) Three-letter spectral algorithm code, e.g "F2W" for CTYPEia = 'ZOPT-F2W'.

      double spcprm::crval

      (Given) Reference value (CRVALia), SI units.

      double spcprm::restfrq

      (Given) The rest frequency [Hz], and ...

      double spcprm::restwav

      (Given) ... the rest wavelength in vacuo [m], only one of which need be given, the other should be set to zero. Neither are required if the $X$ and $S$ spectral variables are both wave-characteristic, or both velocity-characteristic, types.

      double spcprm::pv

      (Given) Grism parameters for 'GRI' and 'GRA' algorithm codes:

      • 0: $G$, grating ruling density.
      • 1: $m$, interference order.
      • 2: $\alpha$, angle of incidence [deg].
      • 3: $n_r$, refractive index at the reference wavelength, $\lambda_r$.
      • 4: $n'_r$, $dn/d\lambda$ at the reference wavelength, $\lambda_r$ (/m).
      • 5: $\epsilon$, grating tilt angle [deg].
      • 6: $\theta$, detector tilt angle [deg].

      The remaining members of the spcprm struct are maintained by spcset() and must not be modified elsewhere:

      double spcprm::w

      (Returned) Intermediate values:

      • 0: Rest frequency or wavelength (SI).
      • 1: The value of the $X$-type spectral variable at the reference point (SI units).
      • 2: $dX/dS$ at the reference point (SI units).
      The remainder are grism intermediates.

      int spcprm::isGrism

      (Returned) Grism coordinates?

      • 0: no,
      • 1: in vacuum,
      • 2: in air.

      int spcprm::padding1

      (An unused variable inserted for alignment purposes only.)

      struct wcserr * spcprm::err [read]

      (Returned) If enabled, when an error status is returned this structure contains detailed information about the error, see wcserr_enable().

      void *padding2 (An unused variable inserted for alignment purposes only.)

      void* spcprm::padding2

      spcprm::spxX2P

      (Returned) The first and ...

      spcprm::spxP2S

      (Returned) ... the second of the pointers to the transformation functions in the two-step algorithm chain $X\leadsto P\rightarrow S$ in the pixel-to-spectral direction where the non-linear transformation is from $X$ to $P$. The argument list, SPX_ARGS, is defined in spx.h.

      spcprm::spxS2P

      (Returned) The first and ...

      spcprm::spxP2X

      (Returned) ... the second of the pointers to the transformation functions in the two-step algorithm chain $S\rightarrow P\leadsto X$ in the spectral-to-pixel direction where the non-linear transformation is from $P$ to $X$. The argument list, SPX_ARGS, is defined in spx.h.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structspxprm.html0000644001153600020070000010663212310355626022571 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: spxprm Struct Reference

      spxprm Struct Reference

      Spectral variables and their derivatives. More...

      #include <spx.h>


      Data Fields

      double restfrq
      double restwav
      int wavetype
      int velotype
      double freq
      double afrq
      double ener
      double wavn
      double vrad
      double wave
      double vopt
      double zopt
      double awav
      double velo
      double beta
      double dfreqafrq
      double dafrqfreq
      double dfreqener
      double denerfreq
      double dfreqwavn
      double dwavnfreq
      double dfreqvrad
      double dvradfreq
      double dfreqwave
      double dwavefreq
      double dfreqawav
      double dawavfreq
      double dfreqvelo
      double dvelofreq
      double dwavevopt
      double dvoptwave
      double dwavezopt
      double dzoptwave
      double dwaveawav
      double dawavwave
      double dwavevelo
      double dvelowave
      double dawavvelo
      double dveloawav
      double dvelobeta
      double dbetavelo
      struct wcserr * err
      void * padding

      Detailed Description

      The spxprm struct contains the value of all spectral variables and their derivatives. It is used solely by specx() which constructs it from information provided via its function arguments.

      This struct should be considered read-only, no members need ever be set nor should ever be modified by the user.

      Field Documentation

      double spxprm::restfrq

      (Returned) Rest frequency [Hz].

      double spxprm::restwav

      (Returned) Rest wavelength [m].

      int spxprm::wavetype

      (Returned) True if wave types have been computed, and ...

      int spxprm::velotype

      (Returned) ... true if velocity types have been computed; types are defined below.

      If one or other of spxprm::restfrq and spxprm::restwav is given (non-zero) then all spectral variables may be computed. If both are given, restfrq is used. If restfrq and restwav are both zero, only wave characteristic xor velocity type spectral variables may be computed depending on the variable given. These flags indicate what is available.

      double spxprm::freq

      (Returned) Frequency [Hz] (wavetype).

      double spxprm::afrq

      (Returned) Angular frequency [rad/s] (wavetype).

      double spxprm::ener

      (Returned) Photon energy [J] (wavetype).

      double spxprm::wavn

      (Returned) Wave number [/m] (wavetype).

      double spxprm::vrad

      (Returned) Radio velocity [m/s] (velotype).

      double spxprm::wave

      (Returned) Vacuum wavelength [m] (wavetype).

      double spxprm::vopt

      (Returned) Optical velocity [m/s] (velotype).

      double spxprm::zopt

      (Returned) Redshift [dimensionless] (velotype).

      double spxprm::awav

      (Returned) Air wavelength [m] (wavetype).

      double spxprm::velo

      (Returned) Relativistic velocity [m/s] (velotype).

      double spxprm::beta

      (Returned) Relativistic beta [dimensionless] (velotype).

      double spxprm::dfreqafrq

      (Returned) Derivative of frequency with respect to angular frequency [/rad] (constant, $= 1 / 2 \pi$), and ...

      double spxprm::dafrqfreq

      (Returned) ... vice versa [rad] (constant, $= 2 \pi$, always available).

      double spxprm::dfreqener

      (Returned) Derivative of frequency with respect to photon energy [/J/s] (constant, $= 1/h$), and ...

      double spxprm::denerfreq

      (Returned) ... vice versa [Js] (constant, $= h$, Planck's constant, always available).

      double spxprm::dfreqwavn

      (Returned) Derivative of frequency with respect to wave number [m/s] (constant, $= c$, the speed of light in vacuuo), and ...

      double spxprm::dwavnfreq

      (Returned) ... vice versa [s/m] (constant, $= 1/c$, always available).

      double spxprm::dfreqvrad

      (Returned) Derivative of frequency with respect to radio velocity [/m], and ...

      double spxprm::dvradfreq

      (Returned) ... vice versa [m] (wavetype && velotype).

      double spxprm::dfreqwave

      (Returned) Derivative of frequency with respect to vacuum wavelength [/m/s], and ...

      double spxprm::dwavefreq

      (Returned) ... vice versa [m s] (wavetype).

      double spxprm::dfreqawav

      (Returned) Derivative of frequency with respect to air wavelength, [/m/s], and ...

      double spxprm::dawavfreq

      (Returned) ... vice versa [m s] (wavetype).

      double spxprm::dfreqvelo

      (Returned) Derivative of frequency with respect to relativistic velocity [/m], and ...

      double spxprm::dvelofreq

      (Returned) ... vice versa [m] (wavetype && velotype).

      double spxprm::dwavevopt

      (Returned) Derivative of vacuum wavelength with respect to optical velocity [s], and ...

      double spxprm::dvoptwave

      (Returned) ... vice versa [/s] (wavetype && velotype).

      double spxprm::dwavezopt

      (Returned) Derivative of vacuum wavelength with respect to redshift [m], and ...

      double spxprm::dzoptwave

      (Returned) ... vice versa [/m] (wavetype && velotype).

      double spxprm::dwaveawav

      (Returned) Derivative of vacuum wavelength with respect to air wavelength [dimensionless], and ...

      double spxprm::dawavwave

      (Returned) ... vice versa [dimensionless] (wavetype).

      double spxprm::dwavevelo

      (Returned) Derivative of vacuum wavelength with respect to relativistic velocity [s], and ...

      double spxprm::dvelowave

      (Returned) ... vice versa [/s] (wavetype && velotype).

      double spxprm::dawavvelo

      (Returned) Derivative of air wavelength with respect to relativistic velocity [s], and ...

      double spxprm::dveloawav

      (Returned) ... vice versa [/s] (wavetype && velotype).

      double spxprm::dvelobeta

      (Returned) Derivative of relativistic velocity with respect to relativistic beta [m/s] (constant, $= c$, the speed of light in vacuu0), and ...

      double spxprm::dbetavelo

      (Returned) ... vice versa [s/m] (constant, $= 1/c$, always available).

      struct wcserr * spxprm::err [read]

      (Returned) If enabled, when an error status is returned this struct contains detailed information about the error, see wcserr_enable().

      void *padding (An unused variable inserted for alignment purposes only.)

      Global variable: const char *spx_errmsg[] - Status return messages Error messages to match the status value returned from each function.

      void* spxprm::padding

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structtabprm.html0000644001153600020070000006444112310355626022526 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: tabprm Struct Reference

      tabprm Struct Reference

      Tabular transformation parameters. More...

      #include <tab.h>


      Data Fields

      int flag
      int M
      int * K
      int * map
      double * crval
      double ** index
      double * coord
      int nc
      int padding
      int * sense
      int * p0
      double * delta
      double * extrema
      struct wcserr * err
      int m_flag
      int m_M
      int m_N
      int set_M
      int * m_K
      int * m_map
      double * m_crval
      double ** m_index
      double ** m_indxs
      double * m_coord

      Detailed Description

      The tabprm struct contains information required to transform tabular coordinates. It consists of certain members that must be set by the user (given) and others that are set by the WCSLIB routines (returned). Some of the latter are supplied for informational purposes while others are for internal use only.

      Field Documentation

      int tabprm::flag

      (Given and returned) This flag must be set to zero whenever any of the following tabprm structure members are set or changed:

      This signals the initialization routine, tabset(), to recompute the returned members of the tabprm struct. tabset() will reset flag to indicate that this has been done.

      PLEASE NOTE: flag should be set to -1 when tabini() is called for the first time for a particular tabprm struct in order to initialize memory management. It must ONLY be used on the first initialization otherwise memory leaks may result.

      int tabprm::M

      (Given or returned) Number of tabular coordinate axes.

      If tabini() is used to initialize the linprm struct (as would normally be the case) then it will set M from the value passed to it as a function argument. The user should not subsequently modify it.

      int * tabprm::K

      (Given or returned) Pointer to the first element of a vector of length tabprm::M whose elements $(K_1, K_2,... K_M)$ record the lengths of the axes of the coordinate array and of each indexing vector.

      If tabini() is used to initialize the linprm struct (as would normally be the case) then it will set K from the array passed to it as a function argument. The user should not subsequently modify it.

      int * tabprm::map

      (Given) Pointer to the first element of a vector of length tabprm::M that defines the association between axis m in the M-dimensional coordinate array (1 $\leq$ m $\leq$ M) and the indices of the intermediate world coordinate and world coordinate arrays, x[] and world[], in the argument lists for tabx2s() and tabs2x().

      When x[] and world[] contain the full complement of coordinate elements in image-order, as will usually be the case, then map[m-1] == i-1 for axis i in the N-dimensional image (1 $\leq$ i $\leq$ N). In terms of the FITS keywords

      map[PVi_3a - 1] == i - 1.

      However, a different association may result if x[], for example, only contains a (relevant) subset of intermediate world coordinate elements. For example, if M == 1 for an image with N > 1, it is possible to fill x[] with the relevant coordinate element with nelem set to 1. In this case map[0] = 0 regardless of the value of i.

      double * tabprm::crval

      (Given) Pointer to the first element of a vector of length tabprm::M whose elements contain the index value for the reference pixel for each of the tabular coordinate axes.

      double ** tabprm::index

      (Given) Pointer to the first element of a vector of length tabprm::M of pointers to vectors of lengths $(K_1, K_2,... K_M)$ of 0-relative indexes (see tabprm::K).

      The address of any or all of these index vectors may be set to zero, i.e. 

              index[m] == 0;

      this is interpreted as default indexing, i.e. 

              index[m][k] = k;

      double * tabprm::coord

      (Given) Pointer to the first element of the tabular coordinate array, treated as though it were defined as 

              double coord[K_M]...[K_2][K_1][M];

      (see tabprm::K) i.e. with the M dimension varying fastest so that the M elements of a coordinate vector are stored contiguously in memory.

      int tabprm::nc

      (Returned) Total number of coordinate vectors in the coordinate array being the product$K_1 K_2 \ldots K_M$(see tabprm::K).

      int tabprm::padding

      (An unused variable inserted for alignment purposes only.)

      int * tabprm::sense

      (Returned) Pointer to the first element of a vector of length tabprm::M whose elements indicate whether the corresponding indexing vector is monotonic increasing (+1), or decreasing (-1).

      int * tabprm::p0

      (Returned) Pointer to the first element of a vector of length tabprm::M of interpolated indices into the coordinate array such that $\Upsilon_m$, as defined in Paper III, is equal to (p0[m] + 1) + tabprm::delta[m].

      double * tabprm::delta

      (Returned) Pointer to the first element of a vector of length tabprm::M of interpolated indices into the coordinate array such that $\Upsilon_m$, as defined in Paper III, is equal to (tabprm::p0[m] + 1) + delta[m].

      double * tabprm::extrema

      (Returned) Pointer to the first element of an array that records the minimum and maximum value of each element of the coordinate vector in each row of the coordinate array, treated as though it were defined as 

              double extrema[K_M]...[K_2][2][M]

      (see tabprm::K). The minimum is recorded in the first element of the compressed $K_1$ dimension, then the maximum. This array is used by the inverse table lookup function, tabs2x(), to speed up table searches.

      struct wcserr * tabprm::err [read]

      (Returned) If enabled, when an error status is returned this struct contains detailed information about the error, see wcserr_enable().

      int tabprm::m_flag

      (For internal use only.)

      int tabprm::m_M

      (For internal use only.)

      int tabprm::m_N

      (For internal use only.)

      int tabprm::set_M

      (For internal use only.)

      int tabprm::m_K

      (For internal use only.)

      int tabprm::m_map

      (For internal use only.)

      int tabprm::m_crval

      (For internal use only.)

      int tabprm::m_index

      (For internal use only.)

      int tabprm::m_indxs

      (For internal use only.)

      int tabprm::m_coord

      (For internal use only.)

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structwcsprm.html0000644001153600020070000024511012310355626022546 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsprm Struct Reference

      wcsprm Struct Reference

      Coordinate transformation parameters. More...

      #include <wcs.h>


      Data Fields

      int flag
      int naxis
      double * crpix
      double * pc
      double * cdelt
      double * crval
      char(* cunit )[72]
      char(* ctype )[72]
      double lonpole
      double latpole
      double restfrq
      double restwav
      int npv
      int npvmax
      struct pvcard * pv
      int nps
      int npsmax
      struct pscard * ps
      double * cd
      double * crota
      int altlin
      int velref
      char alt [4]
      int colnum
      int * colax
      char(* cname )[72]
      double * crder
      double * csyer
      char dateavg [72]
      char dateobs [72]
      double equinox
      double mjdavg
      double mjdobs
      double obsgeo [3]
      char radesys [72]
      char specsys [72]
      char ssysobs [72]
      double velosys
      double zsource
      char ssyssrc [72]
      double velangl
      char wcsname [72]
      int ntab
      int nwtb
      struct tabprm * tab
      struct wtbarr * wtb
      char lngtyp [8]
      char lattyp [8]
      int lng
      int lat
      int spec
      int cubeface
      int * types
      void * padding
      struct linprm lin
      struct celprm cel
      struct spcprm spc
      struct wcserr * err
      void * m_padding
      int m_flag
      int m_naxis
      double * m_crpix
      double * m_pc
      double * m_cdelt
      double * m_crval
      char(* m_cunit )[72]
      char((* m_ctype )[72]
      struct pvcard * m_pv
      struct pscard * m_ps
      double * m_cd
      double * m_crota
      int * m_colax
      char(* m_cname )[72]
      double * m_crder
      double * m_csyer
      struct tabprm * m_tab
      struct wtbarr * m_wtb

      Detailed Description

      The wcsprm struct contains information required to transform world coordinates. It consists of certain members that must be set by the user (given) and others that are set by the WCSLIB routines (returned). Some of the former are not actually required for transforming coordinates. These are described as "auxiliary"; the struct simply provides a place to store them, though they may be used by wcshdo() in constructing a FITS header from a wcsprm struct. Some of the returned values are supplied for informational purposes and others are for internal use only as indicated.

      In practice, it is expected that a WCS parser would scan the FITS header to determine the number of coordinate axes. It would then use wcsini() to allocate memory for arrays in the wcsprm struct and set default values. Then as it reread the header and identified each WCS keyrecord it would load the value into the relevant wcsprm array element. This is essentially what wcspih() does - refer to the prologue of wcshdr.h. As the final step, wcsset() is invoked, either directly or indirectly, to set the derived members of the wcsprm struct. wcsset() strips off trailing blanks in all string members and null-fills the character array.

      Field Documentation

      int wcsprm::flag

      (Given and returned) This flag must be set to zero whenever any of the following wcsprm struct members are set or changed:

      This signals the initialization routine, wcsset(), to recompute the returned members of the celprm struct. celset() will reset flag to indicate that this has been done.

      PLEASE NOTE: flag should be set to -1 when wcsini() is called for the first time for a particular wcsprm struct in order to initialize memory management. It must ONLY be used on the first initialization otherwise memory leaks may result.

      int wcsprm::naxis

      (Given or returned) Number of pixel and world coordinate elements.

      If wcsini() is used to initialize the linprm struct (as would normally be the case) then it will set naxis from the value passed to it as a function argument. The user should not subsequently modify it.

      double * wcsprm::crpix

      (Given) Address of the first element of an array of double containing the coordinate reference pixel, CRPIXja.

      double * wcsprm::pc

      (Given) Address of the first element of the PCi_ja (pixel coordinate) transformation matrix. The expected order is 

              struct wcsprm wcs;
        wcs.pc = {PC1_1, PC1_2, PC2_1, PC2_2};

      This may be constructed conveniently from a 2-D array via 

              double m[2][2] = {{PC1_1, PC1_2},
                          {PC2_1, PC2_2}};

      which is equivalent to 

              double m[2][2];
        m[0][0] = PC1_1;
        m[0][1] = PC1_2;
        m[1][0] = PC2_1;
        m[1][1] = PC2_2;

      The storage order for this 2-D array is the same as for the 1-D array, whence 

              wcs.pc = *m;

      would be legitimate.

      double * wcsprm::cdelt

      (Given) Address of the first element of an array of double containing the coordinate increments, CDELTia.

      double * wcsprm::crval

      (Given) Address of the first element of an array of double containing the coordinate reference values, CRVALia.

      wcsprm::cunit

      (Given) Address of the first element of an array of char[72] containing the CUNITia keyvalues which define the units of measurement of the CRVALia, CDELTia, and CDi_ja keywords.

      As CUNITia is an optional header keyword, cunit[][72] may be left blank but otherwise is expected to contain a standard units specification as defined by WCS Paper I. Utility function wcsutrn(), described in wcsunits.h, is available to translate commonly used non-standard units specifications but this must be done as a separate step before invoking wcsset().

      For celestial axes, if cunit[][72] is not blank, wcsset() uses wcsunits() to parse it and scale cdelt[], crval[], and cd[][*] to degrees. It then resets cunit[][72] to "deg".

      For spectral axes, if cunit[][72] is not blank, wcsset() uses wcsunits() to parse it and scale cdelt[], crval[], and cd[][*] to SI units. It then resets cunit[][72] accordingly.

      wcsset() ignores cunit[][72] for other coordinate types; cunit[][72] may be used to label coordinate values.

      These variables accomodate the longest allowed string-valued FITS keyword, being limited to 68 characters, plus the null-terminating character.

      wcsprm::ctype

      (Given) Address of the first element of an array of char[72] containing the coordinate axis types, CTYPEia.

      The ctype[][72] keyword values must be in upper case and there must be zero or one pair of matched celestial axis types, and zero or one spectral axis. The ctype[][72] strings should be padded with blanks on the right and null-terminated so that they are at least eight characters in length.

      These variables accomodate the longest allowed string-valued FITS keyword, being limited to 68 characters, plus the null-terminating character.

      double wcsprm::lonpole

      (Given and returned) The native longitude of the celestial pole, $\phi_{\mathrm p}$, given by LONPOLEa [deg] or by PVi_2a [deg] attached to the longitude axis which takes precedence if defined, and ...

      double wcsprm::latpole

      (Given and returned) ... the native latitude of the celestial pole, $\theta_{\mathrm p}$, given by LATPOLEa [deg] or by PVi_3a [deg] attached to the longitude axis which takes precedence if defined.

      lonpole and latpole may be left to default to values set by wcsini() (see celprm::ref), but in any case they will be reset by wcsset() to the values actually used. Note therefore that if the wcsprm struct is reused without resetting them, whether directly or via wcsini(), they will no longer have their default values.

      double wcsprm::restfrq

      (Given) The rest frequency [Hz], and/or ...

      double wcsprm::restwav

      (Given) ... the rest wavelength in vacuuo [m], only one of which need be given, the other should be set to zero.

      int wcsprm::npv

      (Given) The number of entries in the wcsprm::pv[] array.

      int wcsprm::npvmax

      (Given or returned) The length of the wcsprm::pv[] array.

      npvmax will be set by wcsini() if it allocates memory for wcsprm::pv[], otherwise it must be set by the user. See also wcsnpv().

      struct pvcard * wcsprm::pv [read]

      (Given or returned) Address of the first element of an array of length npvmax of pvcard structs. Set by wcsini() if it allocates memory for pv[], otherwise it must be set by the user. See also wcsnpv().

      As a FITS header parser encounters each PVi_ma keyword it should load it into a pvcard struct in the array and increment npv. wcsset() interprets these as required.

      Note that, if they were not given, wcsset() resets the entries for PVi_1a, PVi_2a, PVi_3a, and PVi_4a for longitude axis i to match phi_0 and theta_0 (the native longitude and latitude of the reference point), LONPOLEa and LATPOLEa respectively.

      int wcsprm::nps

      (Given) The number of entries in the wcsprm::ps[] array.

      int wcsprm::npsmax

      (Given or returned) The length of the wcsprm::ps[] array.

      npsmax will be set by wcsini() if it allocates memory for wcsprm::ps[], otherwise it must be set by the user. See also wcsnps().

      struct pscard * wcsprm::ps [read]

      (Given or returned) Address of the first element of an array of length npsmax of pscard structs. Set by wcsini() if it allocates memory for ps[], otherwise it must be set by the user. See also wcsnps().

      As a FITS header parser encounters each PSi_ma keyword it should load it into a pscard struct in the array and increment nps. wcsset() interprets these as required (currently no PSi_ma keyvalues are recognized).

      double * wcsprm::cd

      (Given) For historical compatibility, the wcsprm struct supports two alternate specifications of the linear transformation matrix, those associated with the CDi_ja keywords, and ...

      double * wcsprm::crota

      (Given) ... those associated with the CROTAia keywords. Although these may not formally co-exist with PCi_ja, the approach taken here is simply to ignore them if given in conjunction with PCi_ja.

      int wcsprm::altlin

      (Given) altlin is a bit flag that denotes which of the PCi_ja, CDi_ja and CROTAia keywords are present in the header:

      • Bit 0: PCi_ja is present.

      • Bit 1: CDi_ja is present.

        Matrix elements in the IRAF convention are equivalent to the product CDi_ja = CDELTia * PCi_ja, but the defaults differ from that of the PCi_ja matrix. If one or more CDi_ja keywords are present then all unspecified CDi_ja default to zero. If no CDi_ja (or CROTAia) keywords are present, then the header is assumed to be in PCi_ja form whether or not any PCi_ja keywords are present since this results in an interpretation of CDELTia consistent with the original FITS specification.

        While CDi_ja may not formally co-exist with PCi_ja, it may co-exist with CDELTia and CROTAia which are to be ignored.

      • Bit 2: CROTAia is present.

        In the AIPS convention, CROTAia may only be associated with the latitude axis of a celestial axis pair. It specifies a rotation in the image plane that is applied AFTER the CDELTia; any other CROTAia keywords are ignored.

        CROTAia may not formally co-exist with PCi_ja.

        CROTAia and CDELTia may formally co-exist with CDi_ja but if so are to be ignored.

      CDi_ja and CROTAia keywords, if found, are to be stored in the wcsprm::cd and wcsprm::crota arrays which are dimensioned similarly to wcsprm::pc and wcsprm::cdelt. FITS header parsers should use the following procedure:

      • Whenever a PCi_ja keyword is encountered: 
         altlin |= 1;

      • Whenever a CDi_ja keyword is encountered: 
         altlin |= 2;

      • Whenever a CROTAia keyword is encountered: 
         altlin |= 4;

      If none of these bits are set the PCi_ja representation results, i.e. wcsprm::pc and wcsprm::cdelt will be used as given.

      These alternate specifications of the linear transformation matrix are translated immediately to PCi_ja by wcsset() and are invisible to the lower-level WCSLIB routines. In particular, wcsset() resets wcsprm::cdelt to unity if CDi_ja is present (and no PCi_ja).

      If CROTAia are present but none is associated with the latitude axis (and no PCi_ja or CDi_ja), then wcsset() reverts to a unity PCi_ja matrix.

      int wcsprm::velref

      (Given) AIPS velocity code VELREF, refer to spcaips().

      char wcsprm::alt

      (Given, auxiliary) Character code for alternate coordinate descriptions (i.e. the 'a' in keyword names such as CTYPEia). This is blank for the primary coordinate description, or one of the 26 upper-case letters, A-Z.

      An array of four characters is provided for alignment purposes, only the first is used.

      int wcsprm::colnum

      (Given, auxiliary) Where the coordinate representation is associated with an image-array column in a FITS binary table, this variable may be used to record the relevant column number.

      It should be set to zero for an image header or pixel list.

      int * wcsprm::colax

      (Given, auxiliary) Address of the first element of an array of int recording the column numbers for each axis in a pixel list.

      The array elements should be set to zero for an image header or image array in a binary table.

      wcsprm::cname

      (Given, auxiliary) The address of the first element of an array of char[72] containing the coordinate axis names, CNAMEia.

      These variables accomodate the longest allowed string-valued FITS keyword, being limited to 68 characters, plus the null-terminating character.

      double * wcsprm::crder

      (Given, auxiliary) Address of the first element of an array of double recording the random error in the coordinate value, CRDERia.

      double * wcsprm::csyer

      (Given, auxiliary) Address of the first element of an array of double recording the systematic error in the coordinate value, CSYERia.

      char wcsprm::dateavg

      (Given, auxiliary) The date of a representative mid-point of the observation in ISO format, yyyy-mm-ddThh:mm:ss.

      char wcsprm::dateobs

      (Given, auxiliary) The date of the start of the observation unless otherwise explained in the comment field of the DATE-OBS keyword, in ISO format, yyyy-mm-ddThh:mm:ss.

      double wcsprm::equinox

      (Given, auxiliary) The equinox associated with dynamical equatorial or ecliptic coordinate systems, EQUINOXa (or EPOCH in older headers). Not applicable to ICRS equatorial or ecliptic coordinates.

      double wcsprm::mjdavg

      (Given, auxiliary) Modified Julian Date (MJD = JD - 2400000.5), MJD-AVG, corresponding to DATE-AVG.

      double wcsprm::mjdobs

      (Given, auxiliary) Modified Julian Date (MJD = JD - 2400000.5), MJD-OBS, corresponding to DATE-OBS.

      double wcsprm::obsgeo

      (Given, auxiliary) Location of the observer in a standard terrestrial reference frame, OBSGEO-X, OBSGEO-Y, OBSGEO-Z [m].

      char wcsprm::radesys

      (Given, auxiliary) The equatorial or ecliptic coordinate system type, RADESYSa.

      char wcsprm::specsys

      (Given, auxiliary) Spectral reference frame (standard of rest), SPECSYSa, and ...

      char wcsprm::ssysobs

      (Given, auxiliary) ... the actual frame in which there is no differential variation in the spectral coordinate across the field-of-view, SSYSOBSa.

      double wcsprm::velosys

      (Given, auxiliary) The relative radial velocity [m/s] between the observer and the selected standard of rest in the direction of the celestial reference coordinate, VELOSYSa.

      double wcsprm::zsource

      (Given, auxiliary) The redshift, ZSOURCEa, of the source, and ...

      char wcsprm::ssyssrc

      (Given, auxiliary) ... the spectral reference frame (standard of rest) in which this was measured, SSYSSRCa.

      double wcsprm::velangl

      (Given, auxiliary) The angle [deg] that should be used to decompose an observed velocity into radial and transverse components.

      char wcsprm::wcsname

      (Given, auxiliary) The name given to the coordinate representation, WCSNAMEa. This variable accomodates the longest allowed string-valued FITS keyword, being limited to 68 characters, plus the null-terminating character.

      int wcsprm::ntab

      (Given) See wcsprm::tab.

      int wcsprm::nwtb

      (Given) See wcsprm::wtb.

      struct tabprm * wcsprm::tab [read]

      (Given) Address of the first element of an array of ntab tabprm structs for which memory has been allocated. These are used to store tabular transformation parameters.

      Although technically wcsprm::ntab and tab are "given", they will normally be set by invoking wcstab(), whether directly or indirectly.

      The tabprm structs contain some members that must be supplied and others that are derived. The information to be supplied comes primarily from arrays stored in one or more FITS binary table extensions. These arrays, referred to here as "wcstab arrays", are themselves located by parameters stored in the FITS image header.

      struct wtbarr * wcsprm::wtb [read]

      (Given) Address of the first element of an array of nwtb wtbarr structs for which memory has been allocated. These are used in extracting wcstab arrays from a FITS binary table.

      Although technically wcsprm::nwtb and wtb are "given", they will normally be set by invoking wcstab(), whether directly or indirectly.

      char wcsprm::lngtyp

      (Returned) Four-character WCS celestial longitude and ...

      char wcsprm::lattyp

      (Returned) ... latitude axis types. e.g. "RA", "DEC", "GLON", "GLAT", etc. extracted from 'RA--', 'DEC-', 'GLON', 'GLAT', etc. in the first four characters of CTYPEia but with trailing dashes removed. (Declared as char[8] for alignment reasons.)

      int wcsprm::lng

      (Returned) Index for the longitude coordinate, and ...

      int wcsprm::lat

      (Returned) ... index for the latitude coordinate, and ...

      int wcsprm::spec

      (Returned) ... index for the spectral coordinate in the imgcrd[][] and world[][] arrays in the API of wcsp2s(), wcss2p() and wcsmix().

      These may also serve as indices into the pixcrd[][] array provided that the PCi_ja matrix does not transpose axes.

      int wcsprm::cubeface

      (Returned) Index into the pixcrd[][] array for the CUBEFACE axis. This is used for quadcube projections where the cube faces are stored on a separate axis (see wcs.h).

      int * wcsprm::types

      (Returned) Address of the first element of an array of int containing a four-digit type code for each axis.

      • First digit (i.e. 1000s):
        • 0: Non-specific coordinate type.
        • 1: Stokes coordinate.
        • 2: Celestial coordinate (including CUBEFACE).
        • 3: Spectral coordinate.

      • Second digit (i.e. 100s):
        • 0: Linear axis.
        • 1: Quantized axis (STOKES, CUBEFACE).
        • 2: Non-linear celestial axis.
        • 3: Non-linear spectral axis.
        • 4: Logarithmic axis.
        • 5: Tabular axis.

      • Third digit (i.e. 10s):
        • 0: Group number, e.g. lookup table number, being an index into the tabprm array (see above).

      • The fourth digit is used as a qualifier depending on the axis type.

        • For celestial axes:
          • 0: Longitude coordinate.
          • 1: Latitude coordinate.
          • 2: CUBEFACE number.

        • For lookup tables: the axis number in a multidimensional table.

      CTYPEia in "4-3" form with unrecognized algorithm code will have its type set to -1 and generate an error.

      void *padding (An unused variable inserted for alignment purposes only.)

      void* wcsprm::padding

      struct linprm wcsprm::lin [read]

      (Returned) Linear transformation parameters (usage is described in the prologue to lin.h).

      struct celprm wcsprm::cel [read]

      (Returned) Celestial transformation parameters (usage is described in the prologue to cel.h).

      struct spcprm wcsprm::spc [read]

      (Returned) Spectral transformation parameters (usage is described in the prologue to spc.h).

      struct wcserr * wcsprm::err [read]

      (Returned) If enabled, when an error status is returned this struct contains detailed information about the error, see wcserr_enable().

      void *m_padding (For internal use only.)

      void* wcsprm::m_padding

      int wcsprm::m_flag

      (For internal use only.)

      int wcsprm::m_naxis

      (For internal use only.)

      double * wcsprm::m_crpix

      (For internal use only.)

      double * wcsprm::m_pc

      (For internal use only.)

      double * wcsprm::m_cdelt

      (For internal use only.)

      double * wcsprm::m_crval

      (For internal use only.)

      wcsprm::m_cunit

      (For internal use only.)

      wcsprm::m_ctype

      (For internal use only.)

      struct pvcard * wcsprm::m_pv [read]

      (For internal use only.)

      struct pscard * wcsprm::m_ps [read]

      (For internal use only.)

      double * wcsprm::m_cd

      (For internal use only.)

      double * wcsprm::m_crota

      (For internal use only.)

      int * wcsprm::m_colax

      (For internal use only.)

      wcsprm::m_cname

      (For internal use only.)

      double * wcsprm::m_crder

      (For internal use only.)

      double * wcsprm::m_csyer

      (For internal use only.)

      struct tabprm * wcsprm::m_tab [read]

      (For internal use only.)

      struct wtbarr * wcsprm::m_wtb [read]

      (For internal use only.)

      Generated on Mon Feb 6 10:41:58 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/structwtbarr.html0000644001153600020070000002621412310355626022536 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wtbarr Struct Reference

      wtbarr Struct Reference

      Extraction of coordinate lookup tables from BINTABLE. More...

      #include <getwcstab.h>


      Data Fields

      int i
      int m
      int kind
      char extnam [72]
      int extver
      int extlev
      char ttype [72]
      long row
      int ndim
      int * dimlen
      double ** arrayp

      Detailed Description

      Function wcstab(), which is invoked automatically by wcspih(), sets up an array of wtbarr structs to assist in extracting coordinate lookup tables from a binary table extension (BINTABLE) and copying them into the tabprm structs stored in wcsprm. Refer to the usage notes for wcspih() and wcstab() in wcshdr.h, and also the prologue to tab.h.

      For C++ usage, because of a name space conflict with the wtbarr typedef defined in CFITSIO header fitsio.h, the wtbarr struct is renamed to wtbarr_s by preprocessor macro substitution with scope limited to wcs.h itself.

      Field Documentation

      int wtbarr::i

      (Given) Image axis number.

      int wtbarr::m

      (Given) wcstab array axis number for index vectors.

      int wtbarr::kind

      (Given) Character identifying the wcstab array type:

      • c: coordinate array,
      • i: index vector.

      char wtbarr::extnam

      (Given) EXTNAME identifying the binary table extension.

      int wtbarr::extver

      (Given) EXTVER identifying the binary table extension.

      int wtbarr::extlev

      (Given) EXTLEV identifying the binary table extension.

      char wtbarr::ttype

      (Given) TTYPEn identifying the column of the binary table that contains the wcstab array.

      long wtbarr::row

      (Given) Table row number.

      int wtbarr::ndim

      (Given) Expected dimensionality of the wcstab array.

      int * wtbarr::dimlen

      (Given) Address of the first element of an array of int of length ndim into which the wcstab array axis lengths are to be written.

      double ** wtbarr::arrayp

      (Given) Pointer to an array of double which is to be allocated by the user and into which the wcstab array is to be written.

      Generated on Mon Feb 6 10:41:58 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/tab_8h-source.html0000644001153600020070000020236712310355626022440 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: tab.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/tab_8h.html0000644001153600020070000013063312310355626021136 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: tab.h File Reference

      tab.h File Reference

      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  tabprm
       Tabular transformation parameters. More...

      Defines

      #define TABLEN   (sizeof(struct tabprm)/sizeof(int))
       Size of the tabprm struct in int units.
      #define tabini_errmsg   tab_errmsg
       Deprecated.
      #define tabcpy_errmsg   tab_errmsg
       Deprecated.
      #define tabfree_errmsg   tab_errmsg
       Deprecated.
      #define tabprt_errmsg   tab_errmsg
       Deprecated.
      #define tabset_errmsg   tab_errmsg
       Deprecated.
      #define tabx2s_errmsg   tab_errmsg
       Deprecated.
      #define tabs2x_errmsg   tab_errmsg
       Deprecated.

      Enumerations

      enum  tab_errmsg_enum {
        TABERR_SUCCESS = 0, TABERR_NULL_POINTER = 1, TABERR_MEMORY = 2, TABERR_BAD_PARAMS = 3,
        TABERR_BAD_X = 4, TABERR_BAD_WORLD = 5
      }

      Functions

      int tabini (int alloc, int M, const int K[], struct tabprm *tab)
       Default constructor for the tabprm struct.
      int tabmem (struct tabprm *tab)
       Acquire tabular memory.
      int tabcpy (int alloc, const struct tabprm *tabsrc, struct tabprm *tabdst)
       Copy routine for the tabprm struct.
      int tabfree (struct tabprm *tab)
       Destructor for the tabprm struct.
      int tabprt (const struct tabprm *tab)
       Print routine for the tabprm struct.
      int tabset (struct tabprm *tab)
       Setup routine for the tabprm struct.
      int tabx2s (struct tabprm *tab, int ncoord, int nelem, const double x[], double world[], int stat[])
       Pixel-to-world transformation.
      int tabs2x (struct tabprm *tab, int ncoord, int nelem, const double world[], double x[], int stat[])
       World-to-pixel transformation.

      Variables

      const char * tab_errmsg []
       Status return messages.

      Detailed Description

      These routines implement the part of the FITS WCS standard that deals with tabular coordinates, i.e. coordinates that are defined via a lookup table. They define methods to be used for computing tabular world coordinates from intermediate world coordinates (a linear transformation of image pixel coordinates), and vice versa. They are based on the tabprm struct which contains all information needed for the computations. The struct contains some members that must be set by the user, and others that are maintained by these routines, somewhat like a C++ class but with no encapsulation.

      tabini(), tabmem(), tabcpy(), and tabfree() are provided to manage the tabprm struct, and another, tabprt(), to print its contents.

      A setup routine, tabset(), computes intermediate values in the tabprm struct from parameters in it that were supplied by the user. The struct always needs to be set up by tabset() but it need not be called explicitly - refer to the explanation of tabprm::flag.

      tabx2s() and tabs2x() implement the WCS tabular coordinate transformations.

      Accuracy:
      No warranty is given for the accuracy of these routines (refer to the copyright notice); intending users must satisfy for themselves their adequacy for the intended purpose. However, closure effectively to within double precision rounding error was demonstrated by test routine ttab.c which accompanies this software.

      Define Documentation

      #define TABLEN   (sizeof(struct tabprm)/sizeof(int))

      Size of the tabprm struct in int units, used by the Fortran wrappers.

      #define tabini_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      #define tabcpy_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      #define tabfree_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      #define tabprt_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      #define tabset_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      #define tabx2s_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      #define tabs2x_errmsg   tab_errmsg

      Deprecated:
      Added for backwards compatibility, use tab_errmsg directly now instead.

      Enumeration Type Documentation

      enum tab_errmsg_enum

      Enumerator:
      TABERR_SUCCESS 
      TABERR_NULL_POINTER 
      TABERR_MEMORY 
      TABERR_BAD_PARAMS 
      TABERR_BAD_X 
      TABERR_BAD_WORLD 

      Function Documentation

      int tabini ( int  alloc,
      int  M,
      const int  K[],
      struct tabprm *  tab 
      )

      tabini() allocates memory for arrays in a tabprm struct and sets all members of the struct to default values.

      PLEASE NOTE: every tabprm struct should be initialized by tabini(), possibly repeatedly. On the first invokation, and only the first invokation, the flag member of the tabprm struct must be set to -1 to initialize memory management, regardless of whether tabini() will actually be used to allocate memory.

      Parameters:
      [in] alloc If true, allocate memory unconditionally for arrays in the tabprm struct.
      If false, it is assumed that pointers to these arrays have been set by the user except if they are null pointers in which case memory will be allocated for them regardless. (In other words, setting alloc true saves having to initalize these pointers to zero.)
      [in] M The number of tabular coordinate axes.
      [in] K Vector of length M whose elements $(K_1, K_2,... K_M)$ record the lengths of the axes of the coordinate array and of each indexing vector. M and K[] are used to determine the length of the various tabprm arrays and therefore the amount of memory to allocate for them. Their values are copied into the tabprm struct.
      It is permissible to set K (i.e. the address of the array) to zero which has the same effect as setting each element of K[] to zero. In this case no memory will be allocated for the index vectors or coordinate array in the tabprm struct. These together with the K vector must be set separately before calling tabset().
      [in,out] tab Tabular transformation parameters. Note that, in order to initialize memory management tabprm::flag should be set to -1 when tab is initialized for the first time (memory leaks may result if it had already been initialized).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Invalid tabular parameters.
      For returns > 1, a detailed error message is set in tabprm::err if enabled, see wcserr_enable().

      int tabmem ( struct tabprm *  tab  ) 

      tabmem() takes control of memory allocated by the user for arrays in the tabprm struct.

      Parameters:
      [in,out] tab Tabular transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.
      • 2: Memory allocation failed.
      For returns > 1, a detailed error message is set in tabprm::err if enabled, see wcserr_enable().

      int tabcpy ( int  alloc,
      const struct tabprm *  tabsrc,
      struct tabprm *  tabdst 
      )

      tabcpy() does a deep copy of one tabprm struct to another, using tabini() to allocate memory for its arrays if required. Only the "information to be provided" part of the struct is copied; a call to tabset() is required to set up the remainder.

      Parameters:
      [in] alloc If true, allocate memory unconditionally for arrays in the tabprm struct.
      If false, it is assumed that pointers to these arrays have been set by the user except if they are null pointers in which case memory will be allocated for them regardless. (In other words, setting alloc true saves having to initalize these pointers to zero.)
      [in] tabsrc Struct to copy from.
      [in,out] tabdst Struct to copy to. tabprm::flag should be set to -1 if tabdst was not previously initialized (memory leaks may result if it was previously initialized).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.
      • 2: Memory allocation failed.
      For returns > 1, a detailed error message is set in tabprm::err (associated with tabdst) if enabled, see wcserr_enable().

      int tabfree ( struct tabprm *  tab  ) 

      tabfree() frees memory allocated for the tabprm arrays by tabini(). tabini() records the memory it allocates and tabfree() will only attempt to free this.

      PLEASE NOTE: tabfree() must not be invoked on a tabprm struct that was not initialized by tabini().

      Parameters:
      [out] tab Coordinate transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.

      int tabprt ( const struct tabprm *  tab  ) 

      tabprt() prints the contents of a tabprm struct using wcsprintf(). Mainly intended for diagnostic purposes.

      Parameters:
      [in] tab Tabular transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.

      int tabset ( struct tabprm *  tab  ) 

      tabset() allocates memory for work arrays in the tabprm struct and sets up the struct according to information supplied within it.

      Note that this routine need not be called directly; it will be invoked by tabx2s() and tabs2x() if tabprm::flag is anything other than a predefined magic value.

      Parameters:
      [in,out] tab Tabular transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.
      • 3: Invalid tabular parameters.
      For returns > 1, a detailed error message is set in tabprm::err if enabled, see wcserr_enable().

      int tabx2s ( struct tabprm *  tab,
      int  ncoord,
      int  nelem,
      const double  x[],
      double  world[],
      int  stat[] 
      )

      tabx2s() transforms intermediate world coordinates to world coordinates using coordinate lookup.

      Parameters:
      [in,out] tab Tabular transformation parameters.
      [in] ncoord,nelem The number of coordinates, each of vector length nelem.
      [in] x Array of intermediate world coordinates, SI units.
      [out] world Array of world coordinates, in SI units.
      [out] stat Status return value status for each coordinate:
      • 0: Success.
      • 1: Invalid intermediate world coordinate.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.
      • 3: Invalid tabular parameters.
      • 4: One or more of the x coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in tabprm::err if enabled, see wcserr_enable().

      int tabs2x ( struct tabprm *  tab,
      int  ncoord,
      int  nelem,
      const double  world[],
      double  x[],
      int  stat[] 
      )

      tabs2x() transforms world coordinates to intermediate world coordinates.

      Parameters:
      [in,out] tab Tabular transformation parameters.
      [in] ncoord,nelem The number of coordinates, each of vector length nelem.
      [in] world Array of world coordinates, in SI units.
      [out] x Array of intermediate world coordinates, SI units.
      [out] stat Status return value status for each vector element:
      • 0: Success.
      • 1: Invalid world coordinate.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null tabprm pointer passed.
      • 3: Invalid tabular parameters.
      • 5: One or more of the world coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in tabprm::err if enabled, see wcserr_enable().

      Variable Documentation

      const char * tab_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/tab_b.gif0000644001153600020070000000004312310355626020630 0ustar cslocumSTSCI\science00000000000000GIF89a€„°Ç,D;pywcs-1.12/wcslib/html/tab_l.gif0000644001153600020070000000130212310355626020641 0ustar cslocumSTSCI\science00000000000000GIF89a ,Õö÷ùñô÷öøúüýþúûüùúûøùúêïóïóöÆÕßÒÞæØâéÞçíÝæìåìñèîòô÷ùóöø³ÈÕÁÒÝËÙâÏÜäÖá薴ŹɯÂÍ»ÎÙÃÔÞÂÓÝÈ×àÌÚâÕáèÙäê×âèåìðëðó„°ÇÑÞåÜæëãëïëñôîóõ÷úûûüüÿÿÿþþþ, ,ÿ@–P±É`H$!%CqVe2X­ŠÌJ(“Ä +€˜3 2$ÀÆ ¼kvŠä-Ëçõu*…"}ã|}|~q(" $f„ 'Žl(Œ&&$r‘™ › & ! )¢¤›{¨£¥r­ª°©¯„±¯¬´¦·»º³®«§¾¶ÃÂÀ¿²¹ÇÄËƲÌÉεҽͼ„ÔÈÓ×иÙÝÕÏÙÊâÜßãçæê¾äÛÅëÇíáîÖìéïøñ÷õüÑðåùü¤Pß?‚ƒœÇÛBm åAœÎáÀ†%V܈î!Çk÷Ø/áÄ;^¤¨²$Æ–#Mf)f͇(WÎL‰“æKçÒ„° ’I)L:eD ¡Cµ´x*4 U¨h  %A«£^ÁNKb¬Ùe§X±‚´k»x!ÁÖí—2tÝÖ !¯š5tÛæé—À]$¬´%ƒXíâ.i[¬]Y­•ÊfžEëõkg`µ††:zëçÒž;£}ºµj×aa‹–Mš¶é׸cçž½»vïÛºƒóî›8ðáÈ‹'?®¼9óç©G_>Ýyuè¬_ßž]zwêß­‡Ç¾º¼mîæµG~½ûôÞთ/ž>ùööÙ«Ïÿ¿ÿýÿÅà|ÖWà}v;pywcs-1.12/wcslib/html/tab_r.gif0000644001153600020070000000503112310355626020652 0ustar cslocumSTSCI\science00000000000000GIF89a,Õö÷ùñô÷öøúüýþúûüùúûøùúêïóïóöÆÕßÒÞæØâéÞçíÝæìåìñèîòô÷ùóöø³ÈÕÁÒÝËÙâÏÜäÖá薴ŹɯÂÍ»ÎÙÃÔÞÂÓÝÈ×àÌÚâÕáèÙäê×âèåìðëðó„°ÇÑÞåÜæëãëïëñôîóõ÷úûûüüÿÿÿþþþ,,ÿ@’pH,ȤrÉl:ŸÐ¨tJ­Z¯Ø¬v •h<¬pkL.›Ïè´zÍn»ßð¸|N¯Ûïø¼~ÏwVa+‡ˆ‰Š‹ŒŽ‘’“”•–—˜™š›œžŸ “*)^,*ª«¬­®¯°±²³´µ¶·¸¹º»¼½¾¿ÀÁÂö)'ÆÎÏÐÑÒÓÔÕÖ×ØÙÚÛÜÝÞßàáâãäåæÚ¥(" ðñòóôõö÷øùúûüýþÿ H° ÁƒòK"ƒRHœH±¢Å‹3jÜȱ£Ç CŠI²¤É“(Sª\éÅu&@€ Á²¦Í›8sêÜɳ§Oÿ–(±€DУH“*]Ê´©Ó§P£JJµªÕ«X³jÝʵ«×¯S84± ‰hÓª]˶­Û·pãÊK·®Ý»xóêÝË·¯ß¿€Ó} âDÌf(^̸±ãÇ#KžL¹²å˘3kÞ̹³çÏ C‹m¹ðCÄHœXͺµë×°cËžM»¶íÛ¸sëÞÍ»·ïßÀƒ N÷ÃJ” Á®¹óçУKŸN½ºõëسkßν»÷ïàËO¾úñ€ dÇ@€‚‚L¤"ÉÈF:ò‘Œ¤$9† (8…&ÉÉNzò“  ¥(G©FB^²!˨)WÉÊVºò•°l¤)1™ wÄò–¸Ì¥.wÊYºäƒà¥0‡IÌbó¾|ÉHpÌf:ó™Ðìe pJ±ˆ€}Ȧ6·ÉÍnzó›à §8û0Â%"¸æ8×ÉÎvºóðŒ§<ÉPÎQ`ò%×$€>÷ÉÏ~úóŸ ¨@JЂô M¨BÊІ:ô¡¨D'ZPKF Ö¼&16ÊÑŽzô£ ©HGJRb ÷Lç5ÏÁÒ–ºô¥ÿ0©LgJÓšš#(e>¯‰Óžúô§@ ªP‡JÔ¢õ¨HMªR—ÊÔ¦:õ©PªT§JÕª&5;%U·ÊÕ®zõ«` «XÇJV«ÂC§‹ÑjY×ÊÖ¶ºõ­p«\ŠU´À¦xÍ«^÷Ê×¾úõ¯ÐÀi)$‚”ô°ˆM¬bËØÆ:vˆ, ಘͬf7ËÙÎzö³  ­hGKÚÒšö´¨M­jWËÚÖºöµ°­*$ÛSPô¶¸Í­nwËÛÞúö·ÀÅm +„â¸ÈM®r—ËÜæ:÷¹ÐE®?±9ÏêZ÷ºØÍ®v¿9€î"‚ºÛ ¯xÇKÞòb—™ÑLÿ¯z×Ë^A¢·½ð¯|ç†÷Ò÷¾øͯ0í«ßþú÷¿¡ä/€Là»×ÀN°‚ï(à;øÁ n0„'LaýJ¸ÂÎ0{/¬á{ؘþ°ˆG|Ë“øÄ(¥‰SÌâCrÅ.Ž±Œ ãÛøÆv¬1ŽwÌc6ê¸Ç@ÞñƒLd¹ÈHNñ‘“Ìd/¹ÉPÎð“£LeO¹ÊXŽp–·|â+sùËýõ2˜ÇL_1“ùÌí53š×M5³ùÍÇt3œç¼_:ÛÙÂwÎs™õÌgøʹπp ýÌ?úÐ/F´¢ë¼èFãÒÐŽŽt!-éJã‘Ò–Îô1­éN»‘ÓžuÿA-êP“ºÔ>5ª3­êUWºÕ®Ž4¬cÝèYÓZѶ¾õ¡s­ëAóº×€þ5°ù,ìaç¹Øƶ3²“=çe3ûÍÎ~öš£-í3S»Úc¾6¶¿¬ímo¹ÛÞÆ2¸ÃMåq“Êæ>7“Ó­n$³»ÝD~7¼,ïyó¸ÞöÆ1¾ómã}óÛÈÿvµ¿Þâ\É/µÁNâ…3ÜÉ÷´Ã#Þá‰S\ÊguÆ-mñO¸ã0ÈC¾à‘“\Ë'_´ÉS^à•³|À.ùc.ó0לÐ4¿9~s®ó=÷¼Ï<ÿy|ƒ.ô4]ÏD?ºz“®ô67]ÙO§3Ó£ÞÌ©SÄW‡vÖÙl>õ­3Úëdî:Øu)ö±?ÚìÙF;˜Ë®öW²½í­|;ÜW)÷¹²îvtÞ˽w¾÷Ý|à×=xÂÞÝA;pywcs-1.12/wcslib/html/tabs.css0000644001153600020070000000334212310355626020542 0ustar cslocumSTSCI\science00000000000000/* tabs styles, based on http://www.alistapart.com/articles/slidingdoors */ DIV.tabs { float : left; width : 100%; background : url("tab_b.gif") repeat-x bottom; margin-bottom : 4px; } DIV.tabs UL { margin : 0px; padding-left : 10px; list-style : none; } DIV.tabs LI, DIV.tabs FORM { display : inline; margin : 0px; padding : 0px; } DIV.tabs FORM { float : right; } DIV.tabs A { float : left; background : url("tab_r.gif") no-repeat right top; border-bottom : 1px solid #84B0C7; font-size : x-small; font-weight : bold; text-decoration : none; } DIV.tabs A:hover { background-position: 100% -150px; } DIV.tabs A:link, DIV.tabs A:visited, DIV.tabs A:active, DIV.tabs A:hover { color: #1A419D; } DIV.tabs SPAN { float : left; display : block; background : url("tab_l.gif") no-repeat left top; padding : 5px 9px; white-space : nowrap; } DIV.tabs INPUT { float : right; display : inline; font-size : 1em; } DIV.tabs TD { font-size : x-small; font-weight : bold; text-decoration : none; } /* Commented Backslash Hack hides rule from IE5-Mac \*/ DIV.tabs SPAN {float : none;} /* End IE5-Mac hack */ DIV.tabs A:hover SPAN { background-position: 0% -150px; } DIV.tabs LI.current A { background-position: 100% -150px; border-width : 0px; } DIV.tabs LI.current SPAN { background-position: 0% -150px; padding-bottom : 6px; } DIV.navpath { background : none; border : none; border-bottom : 1px solid #84B0C7; } pywcs-1.12/wcslib/html/testing.html0000644001153600020070000001776412310355626021457 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Example code, testing and verification

      Example code, testing and verification

      WCSLIB has an extensive test suite that also provides programming templates as well as demonstrations. Test programs, with names that indicate the main WCSLIB routine under test, reside in ./{C,Fortran}/test and each contains a brief description of its purpose.

      The high- and middle-level test programs are more instructive for applications programming, while the low-level tests are vital for verifying the integrity of the mathematical routines.

      • High level:
        twcstab provides an example of high-level applications programming using WCSLIB and CFITSIO. It constructs an input FITS test file, specifically for testing TAB coordinates, partly using wcstab.keyrec, and then extracts the coordinate description from it following the steps outlined in wcshdr.h.

        tpih1 and tpih2 verify wcspih(). The first prints the contents of the structs returned by wcspih() using wcsprt() and the second uses cpgsbox() to draw coordinate graticules. Input for these comes from a FITS WCS test header implemented as a list of keyrecords, wcs.keyrec, one keyrecord per line, together with a program, tofits, that compiles these into a valid FITS file.

        tfitshdr also uses wcs.keyrec to test the generic FITS header parsing routine.

        twcsfix sets up a wcsprm struct containing various non-standard constructs and then invokes wcsfix() to translate them all to standard usage.

      • Middle level:
        twcs tests closure of wcss2p() and wcsp2s() for a number of selected projections. twcsmix verifies wcsmix() on the $1^\circ$ grid of celestial longitude and latitude for a number of selected projections. It plots a test grid for each projection and indicates the location of successful and failed solutions. twcssub tests the extraction of a coordinate description for a subimage from a wcsprm struct by wcssub().

        tunits tests wcsutrne(), wcsunitse() and wcsulexe(), the units specification translator, converter and parser, either interactively or using a list of units specifications contained in units_test.

      • Low level:
        tlin, tlog, tprj1, tsph, tspc, tspc, and ttab1 test "closure" of the respective routines. Closure tests apply the forward and reverse transformations in sequence and compare the result with the original value. Ideally, the result should agree exactly, but because of floating point rounding errors there is usually a small discrepancy so it is only required to agree within a "closure tolerance".

        tprj1 tests for closure separately for longitude and latitude except at the poles where it only tests for closure in latitude. Note that closure in longitude does not deal with angular displacements on the sky. This is appropriate for many projections such as the cylindricals where circumpolar parallels are projected at the same length as the equator. On the other hand, tsph does test for closure in angular displacement.

        The tolerance for reporting closure discrepancies is set at $10^{-10}$ degree for most projections; this is slightly less than 3 microarcsec. The worst case closure figure is reported for each projection and this is usually better than the reporting tolerance by several orders of magnitude. tprj1 and tsph test closure at all points on the $1^\circ$ grid of native longitude and latitude and to within $5^\circ$ of any latitude of divergence for those projections that cannot represent the full sphere. Closure is also tested at a sequence of points close to the reference point (tprj1) or pole (tsph).

        Closure has been verified at all test points for SUN workstations. However, non-closure may be observed for other machines near native latitude $-90^\circ$ for the zenithal, cylindrical and conic equal area projections (ZEA, CEA and COE), and near divergent latitudes of projections such as the azimuthal perspective and stereographic projections (AZP and STG). Rounding errors may also carry points between faces of the quad-cube projections (CSC, QSC, and TSC). Although such excursions may produce long lists of non-closure points, this is not necessarily indicative of a fundamental problem.

        Note that the inverse of the COBE quad-qube projection (CSC) is a polynomial approximation and its closure tolerance is intrinsically poor.

        Although tests for closure help to verify the internal consistency of the routines they do not verify them in an absolute sense. This is partly addressed by tcel1, tcel2, tprj2, ttab2 and ttab3 which plot graticules for visual inspection of scaling, orientation, and other macroscopic characteristics of the projections.
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/threads.html0000644001153600020070000000750712310355626021426 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Thread-safety

      Thread-safety

      With the following exceptions WCSLIB 4.10 is thread-safe:

      • The C code generated by Flex is not re-entrant. Flex does have the capacity for producing re-entrant scanners but they have a different API. This may be handled by a compile-time option in future but in the meantime calls to the header parsers should be serialized via a mutex.

      • The low-level functions wcsnpv() and wcsnps() are not thread-safe but within the library itself they are only used by the Flex scanners wcspih() and wcsbth(). They would rarely need to be used by application programmers.

      • Diagnostic functions that print the contents of the various structs, namely celprt(), linprt(), prjprt(), spcprt(), tabprt(), wcsprt(), and wcsperr() use printf() which is thread-safe by the POSIX requirement on stdio. However, this is only at the function level. Where multiple threads invoke these functions simultaneously their output is likely to be interleaved.

      • wcserr_enable() sets a static variable and so is not thread-safe. However, this facility is not intended to be used dynamically. If detailed error messages are required, enable wcserr when execution starts and don't change it.
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/vector.html0000644001153600020070000003175512310355626021300 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: Vector API

      Vector API

      WCSLIB's API is vector-oriented. At the least, this allows the function call overhead to be amortised by spreading it over multiple coordinate transformations. However, vector computations may provide an opportunity for caching intermediate calculations and this can produce much more significant efficiencies. For example, many of the spherical projection equations are partially or fully separable in the mathematical sense, i.e. $ (x,y) = f(\phi) g(\theta) $, so if $ \theta $ was invariant for a set of coordinate transformations then $ g(\theta) $ would only need to be computed once. Depending on the circumstances, this may well lead to speedups of a factor of two or more.

      WCSLIB has two different categories of vector API:

      • Certain steps in the WCS algorithm chain operate on coordinate vectors as a whole rather than particular elements of it. For example, the linear transformation takes one or more pixel coordinate vectors, multiples by the transformation matrix, and returns whole intermediate world coordinate vectors.
        The routines that implement these steps, wcsp2s(), wcss2p(), linp2x(), linx2p(), tabx2s(), and tabs2x(), accept and return two-dimensional arrays, i.e. a number of coordinate vectors. Because WCSLIB permits these arrays to contain unused elements, three parameters are needed to describe them:
        • naxis: the number of coordinate elements, as per the FITS NAXIS or WCSAXES keyvalues,
        • ncoord: the number of coordinate vectors,
        • nelem: the total number of elements in each vector, unused as well as used. Clearly, nelem must equal or exceed naxis. (Note that when ncoord is unity, nelem is irrelevant and so is ignored. It may be set to 0.)
        ncoord and nelem are specified as function arguments while naxis is provided as a member of the wcsprm (or linprm) struct.
        For example, wcss2p() accepts an array of world coordinate vectors, world[ncoord][nelem]. In the following example, naxis = 4, ncoord = 5, and nelem = 7: 
            s1  x1  y1  t1  u   u   u
    s2  x2  y2  t2  u   u   u
    s3  x3  y3  t3  u   u   u
    s4  x4  y4  t4  u   u   u
    s5  x5  y5  t5  u   u   u
        where u indicates unused array elements, and the array is laid out in memory as 
            s1  x1  y1  t1  u   u   u   s2  x2  y2  ...
        Note that the stat[] vector returned by routines in this category is of length ncoord, as are the intermediate phi[] and theta[] vectors returned by wcsp2s() and wcss2p().
        Note also that the function prototypes for routines in this category have to declare these two-dimensional arrays as one-dimensional vectors in order to avoid warnings from the C compiler about declaration of "incomplete types". This was considered preferable to declaring them as simple pointers-to-double which gives no indication that storage is associated with them.

      • Other steps in the WCS algorithm chain typically operate only on a part of the coordinate vector. For example, a spectral transformation operates on only one element of an intermediate world coordinate that may also contain celestial coordinate elements. In the above example, spcx2s() might operate only on the s (spectral) coordinate elements.
        Routines like spcx2s() and celx2s() that implement these steps accept and return one-dimensional vectors in which the coordinate element of interest is specified via a starting address, a length, and a stride. To continue the previous example, the starting address for the spectral elements is s1, the length is 5, and the stride is 7.

      Vector lengths

      Routines such as spcx2s() and celx2s() accept and return either one coordinate vector, or a pair of coordinate vectors (one-dimensional C arrays). As explained above, the coordinate elements of interest are usually embedded in a two-dimensional array and must be selected by specifying a starting point, length and stride through the array. For routines such as spcx2s() that operate on a single element of each coordinate vector these parameters have a straightforward interpretation.

      However, for routines such as celx2s() that operate on a pair of elements in each coordinate vector, WCSLIB allows these parameters to be specified independently for each input vector, thereby providing a much more general interpretation than strictly needed to traverse an array.

      This is best described by illustration. The following diagram describes the situation for cels2x(), as a specific example, with nlng = 5, and nlat = 3:

                   lng[0]   lng[1]   lng[2]  lng[3]   lng[4]
             ------   ------   ------  ------   ------
  lat[0]  |  x,y[0]   x,y[1]   x,y[2]  x,y[3]   x,y[4]
  lat[1]  |  x,y[5]   x,y[6]   x,y[7]  x,y[8]   x,y[9]
  lat[2]  |  x,y[10]  x,y[11]  x,y[12] x,y[13]  x,y[14]

      In this case, while only 5 longitude elements and 3 latitude elements are specified, the world-to-pixel routine would calculate nlng * nlat = 15 (x,y) coordinate pairs. It is the responsibility of the caller to ensure that sufficient space has been allocated in all of the output arrays, in this case phi[], theta[], x[], y[] and stat[].

      Vector computation will often be required where neither lng nor lat is constant. This is accomplished by setting nlat = 0 which is interpreted to mean nlat = nlng but only the matrix diagonal is to be computed. Thus, for nlng = 3 and nlat = 0 only three (x,y) coordinate pairs are computed:

                   lng[0]   lng[1]   lng[2]
             ------   ------   ------
  lat[0]  |  x,y[0]
  lat[1]  |           x,y[1]
  lat[2]  |                    x,y[2]

      Note how this differs from nlng = 3, nlat = 1:

                   lng[0]   lng[1]   lng[2]
             ------   ------   ------
  lat[0]  |  x,y[0]   x,y[1]   x,y[2]

      The situation for celx2s() is similar; the x-coordinate (like lng) varies fastest.

      Similar comments can be made for all routines that accept arguments specifying vector length(s) and stride(s). (tabx2s() and tabs2x() do not fall into this category because the -TAB algorithm is fully N-dimensional so there is no way to know in advance how many coordinate elements may be involved.)

      The reason that WCSLIB allows this generality is related to the aforementioned opportunities that vector computations may provide for caching intermediate calculations and the significant efficiencies that can result. The high-level routines, wcsp2s() and wcss2p(), look for opportunities to collapse a set of coordinate transformations where one of the coordinate elements is invariant, and the low-level routines take advantage of such to cache intermediate calculations.

      Vector strides

      As explained above, the vector stride arguments allow the caller to specify that successive elements of a vector are not contiguous in memory. This applies equally to vectors given to, or returned from a function.

      As a further example consider the following two arrangements in memory of the elements of four (x,y) coordinate pairs together with an s coordinate element (e.g. spectral):

      • x1 x2 x3 x4 y1 y2 y3 y4 s1 s2 s3 s4
        the address of x[] is x1, its stride is 1, and length 4,
        the address of y[] is y1, its stride is 1, and length 4,
        the address of s[] is s1, its stride is 1, and length 4.

      • x1 y1 s1 x2 y2 s2 x3 y3 s3 x4 y4 s4
        the address of x[] is x1, its stride is 3, and length 4,
        the address of y[] is y1, its stride is 3, and length 4,
        the address of s[] is s1, its stride is 3, and length 4.

      For routines such as cels2x(), each of the pair of input vectors is assumed to have the same stride. Each of the output vectors also has the same stride, though it may differ from the input stride. For example, for cels2x() the input lng[] and lat[] vectors each have vector stride sll, while the x[] and y[] output vectors have stride sxy. However, the intermediate phi[] and theta[] arrays each have unit stride, as does the stat[] vector.

      If the vector length is 1 then the stride is irrelevant and so ignored. It may be set to 0.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcs_8h-source.html0000644001153600020070000053226012310355626022464 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcs.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcs_8h.html0000644001153600020070000026640112310355626021167 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcs.h File Reference

      wcs.h File Reference

      #include "lin.h"
      #include "cel.h"
      #include "spc.h"
      #include "tab.h"
      #include "wcserr.h"

      Go to the source code of this file.

      Data Structures

      struct  pvcard
       Store for PVi_ma keyrecords. More...
      struct  pscard
       Store for PSi_ma keyrecords. More...
      struct  wtbarr
       Extraction of coordinate lookup tables from BINTABLE. More...
      struct  wcsprm
       Coordinate transformation parameters. More...

      Defines

      #define WCSSUB_LONGITUDE   0x1001
       Mask for extraction of longitude axis by wcssub().
      #define WCSSUB_LATITUDE   0x1002
       Mask for extraction of latitude axis by wcssub().
      #define WCSSUB_CUBEFACE   0x1004
       Mask for extraction of CUBEFACE axis by wcssub().
      #define WCSSUB_CELESTIAL   0x1007
       Mask for extraction of celestial axes by wcssub().
      #define WCSSUB_SPECTRAL   0x1008
       Mask for extraction of spectral axis by wcssub().
      #define WCSSUB_STOKES   0x1010
       Mask for extraction of STOKES axis by wcssub().
      #define WCSLEN   (sizeof(struct wcsprm)/sizeof(int))
       Size of the wcsprm struct in int units.
      #define wcscopy(alloc, wcssrc, wcsdst)   wcssub(alloc, wcssrc, 0x0, 0x0, wcsdst)
       Copy routine for the wcsprm struct.
      #define wcsini_errmsg   wcs_errmsg
       Deprecated.
      #define wcssub_errmsg   wcs_errmsg
       Deprecated.
      #define wcscopy_errmsg   wcs_errmsg
       Deprecated.
      #define wcsfree_errmsg   wcs_errmsg
       Deprecated.
      #define wcsprt_errmsg   wcs_errmsg
       Deprecated.
      #define wcsset_errmsg   wcs_errmsg
       Deprecated.
      #define wcsp2s_errmsg   wcs_errmsg
       Deprecated.
      #define wcss2p_errmsg   wcs_errmsg
       Deprecated.
      #define wcsmix_errmsg   wcs_errmsg
       Deprecated.

      Enumerations

      enum  wcs_errmsg_enum {
        WCSERR_SUCCESS = 0, WCSERR_NULL_POINTER = 1, WCSERR_MEMORY = 2, WCSERR_SINGULAR_MTX = 3,
        WCSERR_BAD_CTYPE = 4, WCSERR_BAD_PARAM = 5, WCSERR_BAD_COORD_TRANS = 6, WCSERR_ILL_COORD_TRANS = 7,
        WCSERR_BAD_PIX = 8, WCSERR_BAD_WORLD = 9, WCSERR_BAD_WORLD_COORD = 10, WCSERR_NO_SOLUTION = 11,
        WCSERR_BAD_SUBIMAGE = 12, WCSERR_NON_SEPARABLE = 13
      }

      Functions

      int wcsnpv (int n)
       Memory allocation for PVi_ma.
      int wcsnps (int n)
       Memory allocation for PSi_ma.
      int wcsini (int alloc, int naxis, struct wcsprm *wcs)
       Default constructor for the wcsprm struct.
      int wcssub (int alloc, const struct wcsprm *wcssrc, int *nsub, int axes[], struct wcsprm *wcsdst)
       Subimage extraction routine for the wcsprm struct.
      int wcsfree (struct wcsprm *wcs)
       Destructor for the wcsprm struct.
      int wcsprt (const struct wcsprm *wcs)
       Print routine for the wcsprm struct.
      int wcsperr (const struct wcsprm *wcs, const char *prefix)
       Print error messages from a wcsprm struct.
      int wcsset (struct wcsprm *wcs)
       Setup routine for the wcsprm struct.
      int wcsp2s (struct wcsprm *wcs, int ncoord, int nelem, const double pixcrd[], double imgcrd[], double phi[], double theta[], double world[], int stat[])
       Pixel-to-world transformation.
      int wcss2p (struct wcsprm *wcs, int ncoord, int nelem, const double world[], double phi[], double theta[], double imgcrd[], double pixcrd[], int stat[])
       World-to-pixel transformation.
      int wcsmix (struct wcsprm *wcs, int mixpix, int mixcel, const double vspan[], double vstep, int viter, double world[], double phi[], double theta[], double imgcrd[], double pixcrd[])
       Hybrid coordinate transformation.
      int wcssptr (struct wcsprm *wcs, int *i, char ctype[9])
       Spectral axis translation.

      Variables

      const char * wcs_errmsg []
       Status return messages.

      Detailed Description

      These routines implement the FITS World Coordinate System (WCS) standard which defines methods to be used for computing world coordinates from image pixel coordinates, and vice versa. They are based on the wcsprm struct which contains all information needed for the computations. The struct contains some members that must be set by the user, and others that are maintained by these routines, somewhat like a C++ class but with no encapsulation.

      Three routines, wcsini(), wcssub(), and wcsfree() are provided to manage the wcsprm struct and another, wcsprt(), to prints its contents. Refer to the description of the wcsprm struct for an explanation of the anticipated usage of these routines. wcscopy(), which does a deep copy of one wcsprm struct to another, is defined as a preprocessor macro function that invokes wcssub().

      wcsperr() prints the error message(s) (if any) stored in a wcsprm struct, and the linprm, celprm, prjprm, spcprm, and tabprm structs that it contains.

      A setup routine, wcsset(), computes intermediate values in the wcsprm struct from parameters in it that were supplied by the user. The struct always needs to be set up by wcsset() but this need not be called explicitly - refer to the explanation of wcsprm::flag.

      wcsp2s() and wcss2p() implement the WCS world coordinate transformations. In fact, they are high level driver routines for the WCS linear, logarithmic, celestial, spectral and tabular transformation routines described in lin.h, log.h, cel.h, spc.h and tab.h.

      Given either the celestial longitude or latitude plus an element of the pixel coordinate a hybrid routine, wcsmix(), iteratively solves for the unknown elements.

      wcssptr() translates the spectral axis in a wcsprm struct. For example, a 'FREQ' axis may be translated into 'ZOPT-F2W' and vice versa.

      Quadcube projections:
      The quadcube projections (TSC, CSC, QSC) may be represented in FITS in either of two ways:

      a: The six faces may be laid out in one plane and numbered as follows: 

                                        0
 
                         4  3  2  1  4  3  2
 
                                  5

      Faces 2, 3 and 4 may appear on one side or the other (or both). The world-to-pixel routines map faces 2, 3 and 4 to the left but the pixel-to-world routines accept them on either side.

      b: The "COBE" convention in which the six faces are stored in a three-dimensional structure using a CUBEFACE axis indexed from 0 to 5 as above.

      These routines support both methods; wcsset() determines which is being used by the presence or absence of a CUBEFACE axis in ctype[]. wcsp2s() and wcss2p() translate the CUBEFACE axis representation to the single plane representation understood by the lower-level WCSLIB projection routines.

      Define Documentation

      #define WCSSUB_LONGITUDE   0x1001

      Mask to use for extracting the longitude axis when sub-imaging, refer to the axes argument of wcssub().

      #define WCSSUB_LATITUDE   0x1002

      Mask to use for extracting the latitude axis when sub-imaging, refer to the axes argument of wcssub().

      #define WCSSUB_CUBEFACE   0x1004

      Mask to use for extracting the CUBEFACE axis when sub-imaging, refer to the axes argument of wcssub().

      #define WCSSUB_CELESTIAL   0x1007

      Mask to use for extracting the celestial axes (longitude, latitude and cubeface) when sub-imaging, refer to the axes argument of wcssub().

      #define WCSSUB_SPECTRAL   0x1008

      Mask to use for extracting the spectral axis when sub-imaging, refer to the axes argument of wcssub().

      #define WCSSUB_STOKES   0x1010

      Mask to use for extracting the STOKES axis when sub-imaging, refer to the axes argument of wcssub().

      #define WCSLEN   (sizeof(struct wcsprm)/sizeof(int))

      Size of the wcsprm struct in int units, used by the Fortran wrappers.

      #define wcscopy ( alloc,
      wcssrc,
      wcsdst   )     wcssub(alloc, wcssrc, 0x0, 0x0, wcsdst)

      wcscopy() does a deep copy of one wcsprm struct to another. As of WCSLIB 3.6, it is implemented as a preprocessor macro that invokes wcssub() with the nsub and axes pointers both set to zero.

      #define wcsini_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcssub_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcscopy_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcsfree_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcsprt_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcsset_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcsp2s_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcss2p_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      #define wcsmix_errmsg   wcs_errmsg

      Deprecated:
      Added for backwards compatibility, use wcs_errmsg directly now instead.

      Enumeration Type Documentation

      enum wcs_errmsg_enum

      Enumerator:
      WCSERR_SUCCESS 
      WCSERR_NULL_POINTER 
      WCSERR_MEMORY 
      WCSERR_SINGULAR_MTX 
      WCSERR_BAD_CTYPE 
      WCSERR_BAD_PARAM 
      WCSERR_BAD_COORD_TRANS 
      WCSERR_ILL_COORD_TRANS 
      WCSERR_BAD_PIX 
      WCSERR_BAD_WORLD 
      WCSERR_BAD_WORLD_COORD 
      WCSERR_NO_SOLUTION 
      WCSERR_BAD_SUBIMAGE 
      WCSERR_NON_SEPARABLE 

      Function Documentation

      int wcsnpv ( int  n  ) 

      wcsnpv() changes the value of NPVMAX (default 64). This global variable controls the number of PVi_ma keywords that wcsini() should allocate space for.

      PLEASE NOTE: This function is not thread-safe.

      Parameters:
      [in] n Value of NPVMAX; ignored if < 0.
      Returns:
      Current value of NPVMAX.

      int wcsnps ( int  n  ) 

      wcsnps() changes the values of NPSMAX (default 8). This global variable controls the number of PSi_ma keywords that wcsini() should allocate space for.

      PLEASE NOTE: This function is not thread-safe.

      Parameters:
      [in] n Value of NPSMAX; ignored if < 0.
      Returns:
      Current value of NPSMAX.

      int wcsini ( int  alloc,
      int  naxis,
      struct wcsprm *  wcs 
      )

      wcsini() optionally allocates memory for arrays in a wcsprm struct and sets all members of the struct to default values. Memory is allocated for up to NPVMAX PVi_ma keywords or NPSMAX PSi_ma keywords per WCS representation. These may be changed via wcsnpv() and wcsnps() before wcsini() is called.

      PLEASE NOTE: every wcsprm struct should be initialized by wcsini(), possibly repeatedly. On the first invokation, and only the first invokation, wcsprm::flag must be set to -1 to initialize memory management, regardless of whether wcsini() will actually be used to allocate memory.

      Parameters:
      [in] alloc If true, allocate memory unconditionally for the crpix, etc. arrays.
      If false, it is assumed that pointers to these arrays have been set by the user except if they are null pointers in which case memory will be allocated for them regardless. (In other words, setting alloc true saves having to initalize these pointers to zero.)
      [in] naxis The number of world coordinate axes. This is used to determine the length of the various wcsprm vectors and matrices and therefore the amount of memory to allocate for them.
      [in,out] wcs Coordinate transformation parameters.
      Note that, in order to initialize memory management, wcsprm::flag should be set to -1 when wcs is initialized for the first time (memory leaks may result if it had already been initialized).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int wcssub ( int  alloc,
      const struct wcsprm *  wcssrc,
      int *  nsub,
      int  axes[],
      struct wcsprm *  wcsdst 
      )

      wcssub() extracts the coordinate description for a subimage from a wcsprm struct. It does a deep copy, using wcsini() to allocate memory for its arrays if required. Only the "information to be provided" part of the struct is extracted; a call to wcsset() is required to set up the remainder.

      The world coordinate system of the subimage must be separable in the sense that the world coordinates at any point in the subimage must depend only on the pixel coordinates of the axes extracted. In practice, this means that the PCi_ja matrix of the original image must not contain non-zero off-diagonal terms that associate any of the subimage axes with any of the non-subimage axes.

      Note that while the required elements of the tabprm array are extracted, the wtbarr array is not. (Thus it is not appropriate to call wcssub() after wcstab() but before filling the tabprm structs - refer to wcshdr.h.)

      wcssub() can also add axes to a wcsprm struct. The new axes will be created using the defaults set by wcsini() which produce a simple, unnamed, linear axis with world coordinate equal to the pixel coordinate. These default values can be changed in before invoking wcsset().

      Parameters:
      [in] alloc If true, allocate memory for the crpix, etc. arrays in the destination. Otherwise, it is assumed that pointers to these arrays have been set by the user except if they are null pointers in which case memory will be allocated for them regardless.
      [in] wcssrc Struct to extract from.
      [in,out] nsub 
      [in,out] axes Vector of length *nsub containing the image axis numbers (1-relative) to extract. Order is significant; axes[0] is the axis number of the input image that corresponds to the first axis in the subimage, etc.
      Use an axis number of 0 to create a new axis using the defaults set by wcsini().
      nsub (the pointer) may be set to zero, and so also may nsub, to indicate the number of axes in the input image; the number of axes will be returned if nsub != 0x0. axes itself (the pointer) may be set to zero to indicate the first *nsub axes in their original order.
      Set both nsub and axes to zero to do a deep copy of one wcsprm struct to another.
      Subimage extraction by coordinate axis type may be done by setting the elements of axes[] to the following special preprocessor macro values:
      • WCSSUB_LONGITUDE: Celestial longitude.
      • WCSSUB_LATITUDE: Celestial latitude.
      • WCSSUB_CUBEFACE: Quadcube CUBEFACE axis.
      • WCSSUB_SPECTRAL: Spectral axis.
      • WCSSUB_STOKES: Stokes axis.
      Refer to the notes (below) for further usage examples.
      On return, *nsub will contain the number of axes in the subimage; this may be zero if there were no axes of the required type(s) (in which case no memory will be allocated). axes[] will contain the axis numbers that were extracted, or 0 for newly created axes. The vector length must be sufficient to contain all axis numbers. No checks are performed to verify that the coordinate axes are consistent, this is done by wcsset().
      [in,out] wcsdst Struct describing the subimage. wcsprm::flag should be set to -1 if wcsdst was not previously initialized (memory leaks may result if it was previously initialized).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 12: Invalid subimage specification.
      • 13: Non-separable subimage coordinate system.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().
      Notes:
      Combinations of subimage axes of particular types may be extracted in the same order as they occur in the input image by combining preprocessor codes, for example 
            *nsub = 1;
      axes[0] = WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_SPECTRAL;

      would extract the longitude, latitude, and spectral axes in the same order as the input image. If one of each were present, *nsub = 3 would be returned.

      For convenience, WCSSUB_CELESTIAL is defined as the combination WCSSUB_LONGITUDE | WCSSUB_LATITUDE | WCSSUB_CUBEFACE.

      The codes may also be negated to extract all but the types specified, for example 

            *nsub = 4;
      axes[0] = WCSSUB_LONGITUDE;
      axes[1] = WCSSUB_LATITUDE;
      axes[2] = WCSSUB_CUBEFACE;
      axes[3] = -(WCSSUB_SPECTRAL | WCSSUB_STOKES);

      The last of these specifies all axis types other than spectral or Stokes. Extraction is done in the order specified by axes[] a longitude axis (if present) would be extracted first (via axes[0]) and not subsequently (via axes[3]). Likewise for the latitude and cubeface axes in this example.

      From the foregoing, it is apparent that the value of *nsub returned may be less than or greater than that given. However, it will never exceed the number of axes in the input image (plus the number of newly-created axes if any were specified on input).

      int wcsfree ( struct wcsprm *  wcs  ) 

      wcsfree() frees memory allocated for the wcsprm arrays by wcsini() and/or wcsset(). wcsini() records the memory it allocates and wcsfree() will only attempt to free this.

      PLEASE NOTE: wcsfree() must not be invoked on a wcsprm struct that was not initialized by wcsini().

      Parameters:
      [out] wcs Coordinate transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int wcsprt ( const struct wcsprm *  wcs  ) 

      wcsprt() prints the contents of a wcsprm struct using wcsprintf(). Mainly intended for diagnostic purposes.

      Parameters:
      [in] wcs Coordinate transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int wcsperr ( const struct wcsprm *  wcs,
      const char *  prefix 
      )

      wcsperr() prints the error message(s), if any, stored in a wcsprm struct, and the linprm, celprm, prjprm, spcprm, and tabprm structs that it contains. If there are no errors then nothing is printed. It uses wcserr_prt(), q.v.

      Parameters:
      [in] wcs Coordinate transformation parameters.
      [in] prefix If non-NULL, each output line will be prefixed with this string.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int wcsset ( struct wcsprm *  wcs  ) 

      wcsset() sets up a wcsprm struct according to information supplied within it (refer to the description of the wcsprm struct).

      wcsset() recognizes the NCP projection and converts it to the equivalent SIN projection and likewise translates GLS into SFL. It also translates the AIPS spectral types ('FREQ-LSR', 'FELO-HEL', etc.), possibly changing the input header keywords wcsprm::ctype and/or wcsprm::specsys if necessary.

      Note that this routine need not be called directly; it will be invoked by wcsp2s() and wcss2p() if the wcsprm::flag is anything other than a predefined magic value.

      Parameters:
      [in,out] wcs Coordinate transformation parameters.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int wcsp2s ( struct wcsprm *  wcs,
      int  ncoord,
      int  nelem,
      const double  pixcrd[],
      double  imgcrd[],
      double  phi[],
      double  theta[],
      double  world[],
      int  stat[] 
      )

      wcsp2s() transforms pixel coordinates to world coordinates.

      Parameters:
      [in,out] wcs Coordinate transformation parameters.
      [in] ncoord,nelem The number of coordinates, each of vector length nelem but containing wcs.naxis coordinate elements. Thus nelem must equal or exceed the value of the NAXIS keyword unless ncoord == 1, in which case nelem is not used.
      [in] pixcrd Array of pixel coordinates.
      [out] imgcrd Array of intermediate world coordinates. For celestial axes, imgcrd[][wcs.lng] and imgcrd[][wcs.lat] are the projected $x$-, and $y$-coordinates in pseudo "degrees". For spectral axes, imgcrd[][wcs.spec] is the intermediate spectral coordinate, in SI units.
      [out] phi,theta Longitude and latitude in the native coordinate system of the projection [deg].
      [out] world Array of world coordinates. For celestial axes, world[][wcs.lng] and world[][wcs.lat] are the celestial longitude and latitude [deg]. For spectral axes, imgcrd[][wcs.spec] is the intermediate spectral coordinate, in SI units.
      [out] stat Status return value for each coordinate:
      • 0: Success.
      • 1+: A bit mask indicating invalid pixel coordinate element(s).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      • 8: One or more of the pixel coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int wcss2p ( struct wcsprm *  wcs,
      int  ncoord,
      int  nelem,
      const double  world[],
      double  phi[],
      double  theta[],
      double  imgcrd[],
      double  pixcrd[],
      int  stat[] 
      )

      wcss2p() transforms world coordinates to pixel coordinates.

      Parameters:
      [in,out] wcs Coordinate transformation parameters.
      [in] ncoord,nelem The number of coordinates, each of vector length nelem but containing wcs.naxis coordinate elements. Thus nelem must equal or exceed the value of the NAXIS keyword unless ncoord == 1, in which case nelem is not used.
      [in] world Array of world coordinates. For celestial axes, world[][wcs.lng] and world[][wcs.lat] are the celestial longitude and latitude [deg]. For spectral axes, world[][wcs.spec] is the spectral coordinate, in SI units.
      [out] phi,theta Longitude and latitude in the native coordinate system of the projection [deg].
      [out] imgcrd Array of intermediate world coordinates. For celestial axes, imgcrd[][wcs.lng] and imgcrd[][wcs.lat] are the projected $x$-, and $y$-coordinates in pseudo "degrees". For quadcube projections with a CUBEFACE axis the face number is also returned in imgcrd[][wcs.cubeface]. For spectral axes, imgcrd[][wcs.spec] is the intermediate spectral coordinate, in SI units.
      [out] pixcrd Array of pixel coordinates.
      [out] stat Status return value for each coordinate:
      • 0: Success.
      • 1+: A bit mask indicating invalid world coordinate element(s).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      • 9: One or more of the world coordinates were invalid, as indicated by the stat vector.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int wcsmix ( struct wcsprm *  wcs,
      int  mixpix,
      int  mixcel,
      const double  vspan[],
      double  vstep,
      int  viter,
      double  world[],
      double  phi[],
      double  theta[],
      double  imgcrd[],
      double  pixcrd[] 
      )

      wcsmix(), given either the celestial longitude or latitude plus an element of the pixel coordinate, solves for the remaining elements by iterating on the unknown celestial coordinate element using wcss2p(). Refer also to the notes below.

      Parameters:
      [in,out] wcs Indices for the celestial coordinates obtained by parsing the wcsprm::ctype[].
      [in] mixpix Which element of the pixel coordinate is given.
      [in] mixcel Which element of the celestial coordinate is given:
      • 1: Celestial longitude is given in world[wcs.lng], latitude returned in world[wcs.lat].
      • 2: Celestial latitude is given in world[wcs.lat], longitude returned in world[wcs.lng].
      [in] vspan Solution interval for the celestial coordinate [deg]. The ordering of the two limits is irrelevant. Longitude ranges may be specified with any convenient normalization, for example [-120,+120] is the same as [240,480], except that the solution will be returned with the same normalization, i.e. lie within the interval specified.
      [in] vstep Step size for solution search [deg]. If zero, a sensible, although perhaps non-optimal default will be used.
      [in] viter If a solution is not found then the step size will be halved and the search recommenced. viter controls how many times the step size is halved. The allowed range is 5 - 10.
      [in,out] world World coordinate elements. world[wcs.lng] and world[wcs.lat] are the celestial longitude and latitude [deg]. Which is given and which returned depends on the value of mixcel. All other elements are given.
      [out] phi,theta Longitude and latitude in the native coordinate system of the projection [deg].
      [out] imgcrd Image coordinate elements. imgcrd[wcs.lng] and imgcrd[wcs.lat] are the projected $x$-, and $y$-coordinates in pseudo "degrees".
      [in,out] pixcrd Pixel coordinate. The element indicated by mixpix is given and the remaining elements are returned.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      • 10: Invalid world coordinate.
      • 11: No solution found in the specified interval.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().
      Notes:
      Initially the specified solution interval is checked to see if it's a "crossing" interval. If it isn't, a search is made for a crossing solution by iterating on the unknown celestial coordinate starting at the upper limit of the solution interval and decrementing by the specified step size. A crossing is indicated if the trial value of the pixel coordinate steps through the value specified. If a crossing interval is found then the solution is determined by a modified form of "regula falsi" division of the crossing interval. If no crossing interval was found within the specified solution interval then a search is made for a "non-crossing" solution as may arise from a point of tangency. The process is complicated by having to make allowance for the discontinuities that occur in all map projections.

      Once one solution has been determined others may be found by subsequent invokations of wcsmix() with suitably restricted solution intervals.

      Note the circumstance that arises when the solution point lies at a native pole of a projection in which the pole is represented as a finite curve, for example the zenithals and conics. In such cases two or more valid solutions may exist but wcsmix() only ever returns one.

      Because of its generality wcsmix() is very compute-intensive. For compute-limited applications more efficient special-case solvers could be written for simple projections, for example non-oblique cylindrical projections.

      int wcssptr ( struct wcsprm *  wcs,
      int *  i,
      char  ctype[9] 
      )

      wcssptr() translates the spectral axis in a wcsprm struct. For example, a 'FREQ' axis may be translated into 'ZOPT-F2W' and vice versa.

      Parameters:
      [in,out] wcs Coordinate transformation parameters.
      [in,out] i Index of the spectral axis (0-relative). If given < 0 it will be set to the first spectral axis identified from the ctype[] keyvalues in the wcsprm struct.
      [in,out] ctype Desired spectral CTYPEia. Wildcarding may be used as for the ctypeS2 argument to spctrn() as described in the prologue of spc.h, i.e. if the final three characters are specified as "???", or if just the eighth character is specified as '?', the correct algorithm code will be substituted and returned.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      • 12: Invalid subimage specification (no spectral axis).
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      Variable Documentation

      const char * wcs_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcsfix_8h-source.html0000644001153600020070000013506612310355626023176 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsfix.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcsfix_8h.html0000644001153600020070000014255412310355626021700 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsfix.h File Reference

      wcsfix.h File Reference

      #include "wcs.h"
      #include "wcserr.h"

      Go to the source code of this file.

      Defines

      #define CDFIX   0
       Index of cdfix() status value in vector returned by wcsfix().
      #define DATFIX   1
       Index of datfix() status value in vector returned by wcsfix().
      #define UNITFIX   2
       Index of unitfix() status value in vector returned by wcsfix().
      #define SPCFIX   3
       Index of spcfix() status value in vector returned by wcsfix().
      #define CELFIX   4
       Index of celfix() status value in vector returned by wcsfix().
      #define CYLFIX   5
       Index of cylfix() status value in vector returned by wcsfix().
      #define NWCSFIX   6
       Number of elements in the status vector returned by wcsfix().
      #define cylfix_errmsg   wcsfix_errmsg
       Deprecated.

      Enumerations

      enum  wcsfix_errmsg_enum {
        FIXERR_DATE_FIX = -4, FIXERR_SPC_UPDATE = -3, FIXERR_UNITS_ALIAS = -2, FIXERR_NO_CHANGE = -1,
        FIXERR_SUCCESS = 0, FIXERR_NULL_POINTER = 1, FIXERR_MEMORY = 2, FIXERR_SINGULAR_MTX = 3,
        FIXERR_BAD_CTYPE = 4, FIXERR_BAD_PARAM = 5, FIXERR_BAD_COORD_TRANS = 6, FIXERR_ILL_COORD_TRANS = 7,
        FIXERR_BAD_CORNER_PIX = 8, FIXERR_NO_REF_PIX_COORD = 9, FIXERR_NO_REF_PIX_VAL = 10
      }

      Functions

      int wcsfix (int ctrl, const int naxis[], struct wcsprm *wcs, int stat[])
       Translate a non-standard WCS struct.
      int wcsfixi (int ctrl, const int naxis[], struct wcsprm *wcs, int stat[], struct wcserr info[])
       Translate a non-standard WCS struct.
      int cdfix (struct wcsprm *wcs)
       Fix erroneously omitted CDi_ja keywords.
      int datfix (struct wcsprm *wcs)
       Translate DATE-OBS and derive MJD-OBS or vice versa.
      int unitfix (int ctrl, struct wcsprm *wcs)
       Correct aberrant CUNITia keyvalues.
      int spcfix (struct wcsprm *wcs)
       Translate AIPS-convention spectral types.
      int celfix (struct wcsprm *wcs)
       Translate AIPS-convention celestial projection types.
      int cylfix (const int naxis[], struct wcsprm *wcs)
       Fix malformed cylindrical projections.

      Variables

      const char * wcsfix_errmsg []
       Status return messages.

      Detailed Description

      Routines in this suite identify and translate various forms of non-standard construct that are known to occur in FITS WCS headers. These range from the translation of non-standard values for standard WCS keywords, to the repair of malformed coordinate representations.

      Non-standard keyvalues:
      AIPS-convention celestial projection types, NCP and GLS, and spectral types, 'FREQ-LSR', 'FELO-HEL', etc., set in CTYPEia are translated on-the-fly by wcsset() but without modifying the relevant ctype[], pv[] or specsys members of the wcsprm struct. That is, only the information extracted from ctype[] is translated when wcsset() fills in wcsprm::cel (celprm struct) or wcsprm::spc (spcprm struct).

      On the other hand, these routines do change the values of wcsprm::ctype[], wcsprm::pv[], wcsprm::specsys and other wcsprm struct members as appropriate to produce the same result as if the FITS header itself had been translated.

      Auxiliary WCS header information not used directly by WCSLIB may also be translated. For example, the older DATE-OBS date format (wcsprm::dateobs) is recast to year-2000 standard form, and MJD-OBS (wcsprm::mjdobs) will be deduced from it if not already set.

      Certain combinations of keyvalues that result in malformed coordinate systems, as described in Sect. 7.3.4 of Paper I, may also be repaired. These are handled by cylfix().

      Non-standard keywords:
      The AIPS-convention CROTAn keywords are recognized as quasi-standard and as such are accomodated by the wcsprm::crota[] and translated to wcsprm::pc[][] by wcsset(). These are not dealt with here, nor are any other non-standard keywords since these routines work only on the contents of a wcsprm struct and do not deal with FITS headers per se. In particular, they do not identify or translate CD00i00j, PC00i00j, PROJPn, EPOCH, VELREF or VSOURCEa keywords; this may be done by the FITS WCS header parser supplied with WCSLIB, refer to wcshdr.h.

      wcsfix() and wcsfixi() apply all of the corrections handled by the following specific functions which may also be invoked separately:

      • cdfix(): Sets the diagonal element of the CDi_ja matrix to 1.0 if all CDi_ja keywords associated with a particular axis are omitted.

      • datfix(): recast an older DATE-OBS date format in dateobs to year-2000 standard form and derive mjdobs from it if not already set. Alternatively, if mjdobs is set and dateobs isn't, then derive dateobs from it.

      • unitfix(): translate some commonly used but non-standard unit strings in the CUNITia keyvalues, e.g. 'DEG' -> 'deg'.

      • spcfix(): translate AIPS-convention spectral types, 'FREQ-LSR', 'FELO-HEL', etc., in ctype[] as set from CTYPEia.

      • celfix(): translate AIPS-convention celestial projection types, NCP and GLS, in ctype[] as set from CTYPEia.

      • cylfix(): fixes WCS keyvalues for malformed cylindrical projections that suffer from the problem described in Sect. 7.3.4 of Paper I.

      Define Documentation

      #define CDFIX   0

      Index of the status value returned by cdfix() in the status vector returned by wcsfix().

      #define DATFIX   1

      Index of the status value returned by datfix() in the status vector returned by wcsfix().

      #define UNITFIX   2

      Index of the status value returned by unitfix() in the status vector returned by wcsfix().

      #define SPCFIX   3

      Index of the status value returned by spcfix() in the status vector returned by wcsfix().

      #define CELFIX   4

      Index of the status value returned by celfix() in the status vector returned by wcsfix().

      #define CYLFIX   5

      Index of the status value returned by cylfix() in the status vector returned by wcsfix().

      #define NWCSFIX   6

      Number of elements in the status vector returned by wcsfix().

      #define cylfix_errmsg   wcsfix_errmsg

      Deprecated:
      Added for backwards compatibility, use wcsfix_errmsg directly now instead.

      Enumeration Type Documentation

      enum wcsfix_errmsg_enum

      Enumerator:
      FIXERR_DATE_FIX 
      FIXERR_SPC_UPDATE 
      FIXERR_UNITS_ALIAS 
      FIXERR_NO_CHANGE 
      FIXERR_SUCCESS 
      FIXERR_NULL_POINTER 
      FIXERR_MEMORY 
      FIXERR_SINGULAR_MTX 
      FIXERR_BAD_CTYPE 
      FIXERR_BAD_PARAM 
      FIXERR_BAD_COORD_TRANS 
      FIXERR_ILL_COORD_TRANS 
      FIXERR_BAD_CORNER_PIX 
      FIXERR_NO_REF_PIX_COORD 
      FIXERR_NO_REF_PIX_VAL 

      Function Documentation

      int wcsfix ( int  ctrl,
      const int  naxis[],
      struct wcsprm *  wcs,
      int  stat[] 
      )

      wcsfix() is identical to wcsfixi(), but lacks the info argument.

      int wcsfixi ( int  ctrl,
      const int  naxis[],
      struct wcsprm *  wcs,
      int  stat[],
      struct wcserr  info[] 
      )

      wcsfix() applies all of the corrections handled separately by cdfix(), datfix(), unitfix(), spcfix(), celfix(), and cylfix().

      Parameters:
      [in] ctrl Do potentially unsafe translations of non-standard unit strings as described in the usage notes to wcsutrn().
      [in] naxis Image axis lengths. If this array pointer is set to zero then cylfix() will not be invoked.
      [in,out] wcs Coordinate transformation parameters.
      [out] stat Status returns from each of the functions. Use the preprocessor macros NWCSFIX to dimension this vector and CDFIX, DATFIX, UNITFIX, SPCFIX, CELFIX, and CYLFIX to access its elements. A status value of -2 is set for functions that were not invoked.
      [out] info Status messages from each of the functions. Use the preprocessor macros NWCSFIX to dimension this vector and CDFIX, DATFIX, UNITFIX, SPCFIX, CELFIX, and CYLFIX to access its elements.
      Returns:
      Status return value:
      • 0: Success.
      • 1: One or more of the translation functions returned an error.

      int cdfix ( struct wcsprm *  wcs  ) 

      cdfix() sets the diagonal element of the CDi_ja matrix to unity if all CDi_ja keywords associated with a given axis were omitted. According to Paper I, if any CDi_ja keywords at all are given in a FITS header then those not given default to zero. This results in a singular matrix with an intersecting row and column of zeros.

      Parameters:
      [in,out] wcs Coordinate transformation parameters.
      Returns:
      Status return value:
      • -1: No change required (not an error).
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int datfix ( struct wcsprm *  wcs  ) 

      datfix() translates the old DATE-OBS date format set in wcsprm::dateobs to year-2000 standard form (yyyy-mm-ddThh:mm:ss) and derives MJD-OBS from it if not already set. Alternatively, if wcsprm::mjdobs is set and wcsprm::dateobs isn't, then datfix() derives wcsprm::dateobs from it. If both are set but disagree by more than half a day then status 5 is returned.

      Parameters:
      [in,out] wcs Coordinate transformation parameters. wcsprm::dateobs and/or wcsprm::mjdobs may be changed.
      Returns:
      Status return value:
      • -1: No change required (not an error).
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 5: Invalid parameter value.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().
      Notes:
      The MJD algorithms used by datfix() are from D.A. Hatcher, 1984, QJRAS, 25, 53-55, as modified by P.T. Wallace for use in SLALIB subroutines CLDJ and DJCL.

      int unitfix ( int  ctrl,
      struct wcsprm *  wcs 
      )

      unitfix() applies wcsutrn() to translate non-standard CUNITia keyvalues, e.g. 'DEG' -> 'deg', also stripping off unnecessary whitespace.

      Parameters:
      [in] ctrl Do potentially unsafe translations described in the usage notes to wcsutrn().
      [in,out] wcs Coordinate transformation parameters.
      Returns:
      Status return value:
      • -1: No change required (not an error).
      • 0: Success (an alias was applied).
      • 1: Null wcsprm pointer passed.
      When units are translated (i.e. status 0), status -2 is set in the wcserr struct to allow an informative message to be returned.

      int spcfix ( struct wcsprm *  wcs  ) 

      spcfix() translates AIPS-convention spectral coordinate types, '{FREQ,FELO,VELO}-{LSR,HEL,OBS}' (e.g. 'FREQ-OBS', 'FELO-HEL', 'VELO-LSR') set in wcsprm::ctype[], subject to VELREF set in wcsprm::velref.

      Note that if wcs::specsys is already set then it will not be overridden.

      Parameters:
      [in,out] wcs Coordinate transformation parameters. wcsprm::ctype[] and/or wcsprm::specsys may be changed.
      Returns:
      Status return value:
      • -1: No change required (not an error).
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int celfix ( struct wcsprm *  wcs  ) 

      celfix() translates AIPS-convention celestial projection types, NCP and GLS, set in the ctype[] member of the wcsprm struct.

      Two additional pv[] keyvalues are created when translating NCP. If the pv[] array was initially allocated by wcsini() then the array will be expanded if necessary. Otherwise, error 2 will be returned if two empty slots are not already available for use.

      Parameters:
      [in,out] wcs Coordinate transformation parameters. wcsprm::ctype[] and/or wcsprm::pv[] may be changed.
      Returns:
      Status return value:
      • -1: No change required (not an error).
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int cylfix ( const int  naxis[],
      struct wcsprm *  wcs 
      )

      cylfix() fixes WCS keyvalues for malformed cylindrical projections that suffer from the problem described in Sect. 7.3.4 of Paper I.

      Parameters:
      [in] naxis Image axis lengths.
      [in,out] wcs Coordinate transformation parameters.
      Returns:
      Status return value:
      • -1: No change required (not an error).
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      • 8: All of the corner pixel coordinates are invalid.
      • 9: Could not determine reference pixel coordinate.
      • 10: Could not determine reference pixel value.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      Variable Documentation

      const char * wcsfix_errmsg[]

      Error messages to match the status value returned from each function.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcshdr_8h-source.html0000644001153600020070000036417212310355626023167 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcshdr.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcshdr_8h.html0000644001153600020070000042505112310355626021663 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcshdr.h File Reference

      wcshdr.h File Reference

      #include "wcs.h"

      Go to the source code of this file.

      Defines

      #define WCSHDR_none   0x00000000
       Bit mask for wcspih() and wcsbth() - reject all extensions.
      #define WCSHDR_all   0x000FFFFF
       Bit mask for wcspih() and wcsbth() - accept all extensions.
      #define WCSHDR_reject   0x10000000
       Bit mask for wcspih() and wcsbth() - reject non-standard keywords.
      #define WCSHDR_CROTAia   0x00000001
       Bit mask for wcspih() and wcsbth() - accept CROTAia, iCROTna, TCROTna.
      #define WCSHDR_EPOCHa   0x00000002
       Bit mask for wcspih() and wcsbth() - accept EPOCHa.
      #define WCSHDR_VELREFa   0x00000004
       Bit mask for wcspih() and wcsbth() - accept VELREFa.
      #define WCSHDR_CD00i00j   0x00000008
       Bit mask for wcspih() and wcsbth() - accept CD00i00j.
      #define WCSHDR_PC00i00j   0x00000010
       Bit mask for wcspih() and wcsbth() - accept PC00i00j.
      #define WCSHDR_PROJPn   0x00000020
       Bit mask for wcspih() and wcsbth() - accept PROJPn.
      #define WCSHDR_RADECSYS   0x00000040
       Bit mask for wcspih() and wcsbth() - accept RADECSYS.
      #define WCSHDR_VSOURCE   0x00000080
       Bit mask for wcspih() and wcsbth() - accept VSOURCEa.
      #define WCSHDR_DOBSn   0x00000100
       Bit mask for wcspih() and wcsbth() - accept DOBSn.
      #define WCSHDR_LONGKEY   0x00000200
       Bit mask for wcspih() and wcsbth() - accept long forms of the alternate binary table and pixel list WCS keywords.
      #define WCSHDR_CNAMn   0x00000400
       Bit mask for wcspih() and wcsbth() - accept iCNAMn, TCNAMn, iCRDEn, TCRDEn, iCSYEn, TCSYEn.
      #define WCSHDR_AUXIMG   0x00000800
       Bit mask for wcspih() and wcsbth() - allow the image-header form of an auxiliary WCS keyword to provide a default value for all images.
      #define WCSHDR_ALLIMG   0x00001000
       Bit mask for wcspih() and wcsbth() - allow the image-header form of all image header WCS keywords to provide a default value for all images.
      #define WCSHDR_IMGHEAD   0x00010000
       Bit mask for wcsbth() - restrict to image header keywords only.
      #define WCSHDR_BIMGARR   0x00020000
       Bit mask for wcsbth() - restrict to binary table image array keywords only.
      #define WCSHDR_PIXLIST   0x00040000
       Bit mask for wcsbth() - restrict to pixel list keywords only.
      #define WCSHDO_none   0x00
       Bit mask for wcshdo() - don't write any extensions.
      #define WCSHDO_all   0xFF
       Bit mask for wcshdo() - write all extensions.
      #define WCSHDO_safe   0x0F
       Bit mask for wcshdo() - write safe extensions only.
      #define WCSHDO_DOBSn   0x01
       Bit mask for wcshdo() - write DOBSn.
      #define WCSHDO_TPCn_ka   0x02
       Bit mask for wcshdo() - write TPCn_ka.
      #define WCSHDO_PVn_ma   0x04
       Bit mask for wcshdo() - write iPVn_ma, TPVn_ma, iPSn_ma, TPSn_ma.
      #define WCSHDO_CRPXna   0x08
       Bit mask for wcshdo() - write jCRPXna, TCRPXna, iCDLTna, TCDLTna, iCUNIna, TCUNIna, iCTYPna, TCTYPna, iCRVLna, TCRVLna.
      #define WCSHDO_CNAMna   0x10
       Bit mask for wcshdo() - write iCNAMna, TCNAMna, iCRDEna, TCRDEna, iCSYEna, TCSYEna.
      #define WCSHDO_WCSNna   0x20
       Bit mask for wcshdo() - write WCSNna instead of TWCSna.

      Enumerations

      enum  wcshdr_errmsg_enum {
        WCSHDRERR_SUCCESS = 0, WCSHDRERR_NULL_POINTER = 1, WCSHDRERR_MEMORY = 2, WCSHDRERR_BAD_COLUMN = 3,
        WCSHDRERR_PARSER = 4, WCSHDRERR_BAD_TABULAR_PARAMS = 5
      }

      Functions

      int wcspih (char *header, int nkeyrec, int relax, int ctrl, int *nreject, int *nwcs, struct wcsprm **wcs)
       FITS WCS parser routine for image headers.
      int wcsbth (char *header, int nkeyrec, int relax, int ctrl, int keysel, int *colsel, int *nreject, int *nwcs, struct wcsprm **wcs)
       FITS WCS parser routine for binary table and image headers.
      int wcstab (struct wcsprm *wcs)
       Tabular construction routine.
      int wcsidx (int nwcs, struct wcsprm **wcs, int alts[27])
       Index alternate coordinate representations.
      int wcsbdx (int nwcs, struct wcsprm **wcs, int type, short alts[1000][28])
       Index alternate coordinate representions.
      int wcsvfree (int *nwcs, struct wcsprm **wcs)
       Free the array of wcsprm structs.
      int wcshdo (int relax, struct wcsprm *wcs, int *nkeyrec, char **header)
       Write out a wcsprm struct as a FITS header.

      Variables

      const char * wcshdr_errmsg []
       Status return messages.

      Detailed Description

      Routines in this suite are aimed at extracting WCS information from a FITS file. They provide the high-level interface between the FITS file and the WCS coordinate transformation routines.

      Additionally, function wcshdo() is provided to write out the contents of a wcsprm struct as a FITS header.

      Briefly, the anticipated sequence of operations is as follows:

      • 1: Open the FITS file and read the image or binary table header, e.g. using CFITSIO routine fits_hdr2str().

      • 2: Parse the header using wcspih() or wcsbth(); they will automatically interpret 'TAB' header keywords using wcstab().

      • 3: Allocate memory for, and read 'TAB' arrays from the binary table extension, e.g. using CFITSIO routine fits_read_wcstab() - refer to the prologue of getwcstab.h. wcsset() will automatically take control of this allocated memory, in particular causing it to be free'd by wcsfree().

      • 4: Translate non-standard WCS usage using wcsfix(), see wcsfix.h.

      • 5: Initialize wcsprm struct(s) using wcsset() and calculate coordinates using wcsp2s() and/or wcss2p(). Refer to the prologue of wcs.h for a description of these and other high-level WCS coordinate transformation routines.

      • 6: Clean up by freeing memory with wcsvfree().

      In detail:

      • wcspih() is a high-level FITS WCS routine that parses an image header. It returns an array of up to 27 wcsprm structs on each of which it invokes wcstab().

      • wcsbth() is the analogue of wcspih() for use with binary tables; it handles image array and pixel list keywords. As an extension of the FITS WCS standard, it also recognizes image header keywords which may be used to provide default values via an inheritance mechanism.

      • wcstab() assists in filling in members of the wcsprm struct associated with coordinate lookup tables ('TAB'). These are based on arrays stored in a FITS binary table extension (BINTABLE) that are located by PVi_ma keywords in the image header.

      Define Documentation

      #define WCSHDR_none   0x00000000

      Bit mask for the relax argument of wcspih() and wcsbth() - reject all extensions.

      Refer to wcsbth() note 5.

      #define WCSHDR_all   0x000FFFFF

      Bit mask for the relax argument of wcspih() and wcsbth() - accept all extensions.

      Refer to wcsbth() note 5.

      #define WCSHDR_reject   0x10000000

      Bit mask for the relax argument of wcspih() and wcsbth() - reject non-standard keywords.

      Refer to wcsbth() note 5.

      #define WCSHDR_CROTAia   0x00000001

      Bit mask for the relax argument of wcspih() and wcsbth() - accept CROTAia, iCROTna, TCROTna.

      Refer to wcsbth() note 5.

      #define WCSHDR_EPOCHa   0x00000002

      Bit mask for the relax argument of wcspih() and wcsbth() - accept EPOCHa.

      Refer to wcsbth() note 5.

      #define WCSHDR_VELREFa   0x00000004

      Bit mask for the relax argument of wcspih() and wcsbth() - accept VELREFa.

      Refer to wcsbth() note 5.

      #define WCSHDR_CD00i00j   0x00000008

      Bit mask for the relax argument of wcspih() and wcsbth() - accept CD00i00j.

      Refer to wcsbth() note 5.

      #define WCSHDR_PC00i00j   0x00000010

      Bit mask for the relax argument of wcspih() and wcsbth() - accept PC00i00j.

      Refer to wcsbth() note 5.

      #define WCSHDR_PROJPn   0x00000020

      Bit mask for the relax argument of wcspih() and wcsbth() - accept PROJPn.

      Refer to wcsbth() note 5.

      #define WCSHDR_RADECSYS   0x00000040

      Bit mask for the relax argument of wcspih() and wcsbth() - accept RADECSYS.

      Refer to wcsbth() note 5.

      #define WCSHDR_VSOURCE   0x00000080

      Bit mask for the relax argument of wcspih() and wcsbth() - accept VSOURCEa.

      Refer to wcsbth() note 5.

      #define WCSHDR_DOBSn   0x00000100

      Bit mask for the relax argument of wcspih() and wcsbth() - accept DOBSn.

      Refer to wcsbth() note 5.

      #define WCSHDR_LONGKEY   0x00000200

      Bit mask for the relax argument of wcspih() and wcsbth() - accept long forms of the alternate binary table and pixel list WCS keywords.

      Refer to wcsbth() note 5.

      #define WCSHDR_CNAMn   0x00000400

      Bit mask for the relax argument of wcspih() and wcsbth() - accept iCNAMn, TCNAMn, iCRDEn, TCRDEn, iCSYEn, TCSYEn.

      Refer to wcsbth() note 5.

      #define WCSHDR_AUXIMG   0x00000800

      Bit mask for the relax argument of wcspih() and wcsbth() - allow the image-header form of an auxiliary WCS keyword with representation-wide scope to provide a default value for all images.

      Refer to wcsbth() note 5.

      #define WCSHDR_ALLIMG   0x00001000

      Bit mask for the relax argument of wcspih() and wcsbth() - allow the image-header form of all image header WCS keywords to provide a default value for all image arrays in a binary table (n.b. not pixel list).

      Refer to wcsbth() note 5.

      #define WCSHDR_IMGHEAD   0x00010000

      Bit mask for the keysel argument of wcsbth() - restrict keyword types considered to image header keywords only.

      #define WCSHDR_BIMGARR   0x00020000

      Bit mask for the keysel argument of wcsbth() - restrict keyword types considered to binary table image array keywords only.

      #define WCSHDR_PIXLIST   0x00040000

      Bit mask for the keysel argument of wcsbth() - restrict keyword types considered to pixel list keywords only.

      #define WCSHDO_none   0x00

      Bit mask for the relax argument of wcshdo() - don't write any extensions.

      Refer to the notes for wcshdo().

      #define WCSHDO_all   0xFF

      Bit mask for the relax argument of wcshdo() - write all extensions.

      Refer to the notes for wcshdo().

      #define WCSHDO_safe   0x0F

      Bit mask for the relax argument of wcshdo() - write only extensions that are considered safe.

      Refer to the notes for wcshdo().

      #define WCSHDO_DOBSn   0x01

      Bit mask for the relax argument of wcshdo() - write DOBSn, the column-specific analogue of DATE-OBS for use in binary tables and pixel lists.

      Refer to the notes for wcshdo().

      #define WCSHDO_TPCn_ka   0x02

      Bit mask for the relax argument of wcshdo() - write TPCn_ka if less than eight characters instead of TPn_ka.

      Refer to the notes for wcshdo().

      #define WCSHDO_PVn_ma   0x04

      Bit mask for the relax argument of wcshdo() - write iPVn_ma, TPVn_ma, iPSn_ma, TPSn_ma, if less than eight characters instead of iVn_ma, TVn_ma, iSn_ma, TSn_ma.

      Refer to the notes for wcshdo().

      #define WCSHDO_CRPXna   0x08

      Bit mask for the relax argument of wcshdo() - write jCRPXna, TCRPXna, iCDLTna, TCDLTna, iCUNIna, TCUNIna, iCTYPna, TCTYPna, iCRVLna, TCRVLna, if less than eight characters instead of jCRPna, TCRPna, iCDEna, TCDEna, iCUNna, TCUNna, iCTYna, TCTYna, iCRVna, TCRVna.

      Refer to the notes for wcshdo().

      #define WCSHDO_CNAMna   0x10

      Bit mask for the relax argument of wcshdo() - write iCNAMna, TCNAMna, iCRDEna, TCRDEna, iCSYEna, TCSYEna, if less than eight characters instead of iCNAna, TCNAna, iCRDna, TCRDna, iCSYna, TCSYna.

      Refer to the notes for wcshdo().

      #define WCSHDO_WCSNna   0x20

      Bit mask for the relax argument of wcshdo() - write WCSNna instead of TWCSna.

      Refer to the notes for wcshdo().

      Enumeration Type Documentation

      enum wcshdr_errmsg_enum

      Enumerator:
      WCSHDRERR_SUCCESS 
      WCSHDRERR_NULL_POINTER 
      WCSHDRERR_MEMORY 
      WCSHDRERR_BAD_COLUMN 
      WCSHDRERR_PARSER 
      WCSHDRERR_BAD_TABULAR_PARAMS 

      Function Documentation

      int wcspih ( char *  header,
      int  nkeyrec,
      int  relax,
      int  ctrl,
      int *  nreject,
      int *  nwcs,
      struct wcsprm **  wcs 
      )

      wcspih() is a high-level FITS WCS routine that parses an image header, either that of a primary HDU or of an image extension. All WCS keywords defined in Papers I, II, and III are recognized, and also those used by the AIPS convention and certain other keywords that existed in early drafts of the WCS papers as explained in wcsbth() note 5.

      Given a character array containing a FITS image header, wcspih() identifies and reads all WCS keywords for the primary coordinate representation and up to 26 alternate representations. It returns this information as an array of wcsprm structs.

      wcspih() invokes wcstab() on each of the wcsprm structs that it returns.

      Use wcsbth() in preference to wcspih() for FITS headers of unknown type; wcsbth() can parse image headers as well as binary table and pixel list headers.

      Parameters:
      [in,out] header Character array containing the (entire) FITS image header from which to identify and construct the coordinate representations, for example, as might be obtained conveniently via the CFITSIO routine fits_hdr2str().
      Each header "keyrecord" (formerly "card image") consists of exactly 80 7-bit ASCII printing characters in the range 0x20 to 0x7e (which excludes NUL, BS, TAB, LF, FF and CR) especially noting that the keyrecords are NOT null-terminated.
      For negative values of ctrl (see below), header[] is modified so that WCS keyrecords processed by wcspih() are removed from it.
      [in] nkeyrec Number of keyrecords in header[].
      [in] relax Degree of permissiveness:
      • 0: Recognize only FITS keywords defined by the published WCS standard.
      • WCSHDR_all: Admit all recognized informal extensions of the WCS standard.
      Fine-grained control of the degree of permissiveness is also possible as explained in wcsbth() note 5.
      [in] ctrl Error reporting and other control options for invalid WCS and other header keyrecords:
      • 0: Do not report any rejected header keyrecords.
      • 1: Produce a one-line message stating the number of WCS keyrecords rejected (nreject).
      • 2: Report each rejected keyrecord and the reason why it was rejected.
      • 3: As above, but also report all non-WCS keyrecords that were discarded, and the number of coordinate representations (nwcs) found.
      The report is written to stderr.
      For ctrl < 0, WCS keyrecords processed by wcspih() are removed from header[]:
      • -1: Remove only valid WCS keyrecords whose values were successfully extracted, nothing is reported.
      • -2: Also remove WCS keyrecords that were rejected, reporting each one and the reason that it was rejected.
      • -3: As above, and also report the number of coordinate representations (nwcs) found.
      • -11: Same as -1 but preserving the basic keywords '{DATE,MJD}-{OBS,AVG}' and 'OBSGEO-{X,Y,Z}'.
      If any keyrecords are removed from header[] it will be null-terminated (NUL not being a legal FITS header character), otherwise it will contain its original complement of nkeyrec keyrecords and possibly not be null-terminated.
      [out] nreject Number of WCS keywords rejected for syntax errors, illegal values, etc. Keywords not recognized as WCS keywords are simply ignored. Refer also to wcsbth() note 5.
      [out] nwcs Number of coordinate representations found.
      [out] wcs Pointer to an array of wcsprm structs containing up to 27 coordinate representations.
      Memory for the array is allocated by wcspih() which also invokes wcsini() for each struct to allocate memory for internal arrays and initialize their members to default values. Refer also to wcsbth() note 8. Note that wcsset() is not invoked on these structs.
      This allocated memory must be freed by the user, first by invoking wcsfree() for each struct, and then by freeing the array itself. A routine, wcsvfree(), is provided to do this (see below).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 4: Fatal error returned by Flex parser.
      Notes:
      Refer to wcsbth() notes 1, 2, 3, 5, 7, and 8.

      int wcsbth ( char *  header,
      int  nkeyrec,
      int  relax,
      int  ctrl,
      int  keysel,
      int *  colsel,
      int *  nreject,
      int *  nwcs,
      struct wcsprm **  wcs 
      )

      wcsbth() is a high-level FITS WCS routine that parses a binary table header. It handles image array and pixel list WCS keywords which may be present together in one header.

      As an extension of the FITS WCS standard, wcsbth() also recognizes image header keywords in a binary table header. These may be used to provide default values via an inheritance mechanism discussed in note 5 (c.f. WCSHDR_AUXIMG and WCSHDR_ALLIMG), or may instead result in wcsprm structs that are not associated with any particular column. Thus wcsbth() can handle primary image and image extension headers in addition to binary table headers (it ignores NAXIS and does not rely on the presence of the TFIELDS keyword).

      All WCS keywords defined in Papers I, II, and III are recognized, and also those used by the AIPS convention and certain other keywords that existed in early drafts of the WCS papers as explained in note 5 below.

      wcsbth() sets the colnum or colax[] members of the wcsprm structs that it returns with the column number of an image array or the column numbers associated with each pixel coordinate element in a pixel list. wcsprm structs that are not associated with any particular column, as may be derived from image header keywords, have colnum == 0.

      Note 6 below discusses the number of wcsprm structs returned by wcsbth(), and the circumstances in which image header keywords cause a struct to be created. See also note 9 concerning the number of separate images that may be stored in a pixel list.

      The API to wcsbth() is similar to that of wcspih() except for the addition of extra arguments that may be used to restrict its operation. Like wcspih(), wcsbth() invokes wcstab() on each of the wcsprm structs that it returns.

      Parameters:
      [in,out] header Character array containing the (entire) FITS binary table, primary image, or image extension header from which to identify and construct the coordinate representations, for example, as might be obtained conveniently via the CFITSIO routine fits_hdr2str().
      Each header "keyrecord" (formerly "card image") consists of exactly 80 7-bit ASCII printing characters in the range 0x20 to 0x7e (which excludes NUL, BS, TAB, LF, FF and CR) especially noting that the keyrecords are NOT null-terminated.
      For negative values of ctrl (see below), header[] is modified so that WCS keyrecords processed by wcsbth() are removed from it.
      [in] nkeyrec Number of keyrecords in header[].
      [in] relax Degree of permissiveness:
      • 0: Recognize only FITS keywords defined by the published WCS standard.
      • WCSHDR_all: Admit all recognized informal extensions of the WCS standard.
      Fine-grained control of the degree of permissiveness is also possible, as explained in note 5 below.
      [in] ctrl Error reporting and other control options for invalid WCS and other header keyrecords:
      • 0: Do not report any rejected header keyrecords.
      • 1: Produce a one-line message stating the number of WCS keyrecords rejected (nreject).
      • 2: Report each rejected keyrecord and the reason why it was rejected.
      • 3: As above, but also report all non-WCS keyrecords that were discarded, and the number of coordinate representations (nwcs) found.
      The report is written to stderr.
      For ctrl < 0, WCS keyrecords processed by wcsbth() are removed from header[]:
      • -1: Remove only valid WCS keyrecords whose values were successfully extracted, nothing is reported.
      • -2: Also remove WCS keyrecords that were rejected, reporting each one and the reason that it was rejected.
      • -3: As above, and also report the number of coordinate representations (nwcs) found.
      • -11: Same as -1 but preserving the basic keywords '{DATE,MJD}-{OBS,AVG}' and 'OBSGEO-{X,Y,Z}'.
      If any keyrecords are removed from header[] it will be null-terminated (NUL not being a legal FITS header character), otherwise it will contain its original complement of nkeyrec keyrecords and possibly not be null-terminated.
      [in] keysel Vector of flag bits that may be used to restrict the keyword types considered: If zero, there is no restriction.
      Keywords such as EQUIna or RFRQna that are common to binary table image arrays and pixel lists (including WCSNna and TWCSna, as explained in note 4 below) are selected by both WCSHDR_BIMGARR and WCSHDR_PIXLIST. Thus if inheritance via WCSHDR_ALLIMG is enabled as discussed in note 5 and one of these shared keywords is present, then WCSHDR_IMGHEAD and WCSHDR_PIXLIST alone may be sufficient to cause the construction of coordinate descriptions for binary table image arrays.
      [in] colsel Pointer to an array of table column numbers used to restrict the keywords considered by wcsbth().
      A null pointer may be specified to indicate that there is no restriction. Otherwise, the magnitude of cols[0] specifies the length of the array:
      • cols[0] > 0: the columns are included,
      • cols[0] < 0: the columns are excluded.
      For the pixel list keywords TPn_ka and TCn_ka (and TPCn_ka and TCDn_ka if WCSHDR_LONGKEY is enabled), it is an error for one column to be selected but not the other. This is unlike the situation with invalid keyrecords, which are simply rejected, because the error is not intrinsic to the header itself but arises in the way that it is processed.
      [out] nreject Number of WCS keywords rejected for syntax errors, illegal values, etc. Keywords not recognized as WCS keywords are simply ignored, refer also to note 5 below.
      [out] nwcs Number of coordinate representations found.
      [out] wcs Pointer to an array of wcsprm structs containing up to 27027 coordinate representations, refer to note 6 below.
      Memory for the array is allocated by wcsbth() which also invokes wcsini() for each struct to allocate memory for internal arrays and initialize their members to default values. Refer also to note 8 below. Note that wcsset() is not invoked on these structs.
      This allocated memory must be freed by the user, first by invoking wcsfree() for each struct, and then by freeing the array itself. A routine, wcsvfree(), is provided to do this (see below).
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Invalid column selection.
      • 4: Fatal error returned by Flex parser.
      Notes:
      1. wcspih() determines the number of coordinate axes independently for each alternate coordinate representation (denoted by the "a" value in keywords like CTYPEia) from the higher of

        1. NAXIS,
        2. WCSAXESa,
        3. The highest axis number in any parameterized WCS keyword. The keyvalue, as well as the keyword, must be syntactically valid otherwise it will not be considered.

        If none of these keyword types is present, i.e. if the header only contains auxiliary WCS keywords for a particular coordinate representation, then no coordinate description is constructed for it.

        wcsbth() is similar except that it ignores the NAXIS keyword if given an image header to process.

        The number of axes, which is returned as a member of the wcsprm struct, may differ for different coordinate representations of the same image.

      2. wcspih() and wcsbth() enforce correct FITS "keyword = value" syntax with regard to "= " occurring in columns 9 and 10.

        However, they do recognize free-format character (NOST 100-2.0, Sect. 5.2.1), integer (Sect. 5.2.3), and floating-point values (Sect. 5.2.4) for all keywords.

      3. Where CROTAn, CDi_ja, and PCi_ja occur together in one header wcspih() and wcsbth() treat them as described in the prologue to wcs.h.

      4. WCS Paper I mistakenly defined the pixel list form of WCSNAMEa as TWCSna instead of WCSNna; the 'T' is meant to substitute for the axis number in the binary table form of the keyword - note that keywords defined in WCS Papers II and III that are not parameterised by axis number have identical forms for binary tables and pixel lists. Consequently wcsbth() always treats WCSNna and TWCSna as equivalent.

      5. wcspih() and wcsbth() interpret the relax argument as a vector of flag bits to provide fine-grained control over what non-standard WCS keywords to accept. The flag bits are subject to change in future and should be set by using the preprocessor macros (see below) for the purpose.

        • WCSHDR_none: Don't accept any extensions (not even those in the errata). Treat non-conformant keywords in the same way as non-WCS keywords in the header, i.e. simply ignore them.

        • WCSHDR_all: Accept all extensions recognized by the parser.

        • WCSHDR_reject: Reject non-standard keywords (that are not otherwise accepted). A message will optionally be printed on stderr, as determined by the ctrl argument, and nreject will be incremented.

          This flag may be used to signal the presence of non-standard keywords, otherwise they are simply passed over as though they did not exist in the header.

          Useful for testing conformance of a FITS header to the WCS standard.

        • WCSHDR_CROTAia: Accept CROTAia (wcspih()), iCROTna (wcsbth()), TCROTna (wcsbth()).
        • WCSHDR_EPOCHa: Accept EPOCHa.
        • WCSHDR_VELREFa: Accept VELREFa. wcspih() always recognizes the AIPS-convention keywords, CROTAn, EPOCH, and VELREF for the primary representation (a = ' ') but alternates are non-standard.

          wcsbth() accepts EPOCHa and VELREFa only if WCSHDR_AUXIMG is also enabled.

        • WCSHDR_CD00i00j: Accept CD00i00j (wcspih()).
        • WCSHDR_PC00i00j: Accept PC00i00j (wcspih()).
        • WCSHDR_PROJPn: Accept PROJPn (wcspih()). These appeared in early drafts of WCS Paper I+II (before they were split) and are equivalent to CDi_ja, PCi_ja, and PVi_ma for the primary representation (a = ' '). PROJPn is equivalent to PVi_ma with m = n $\le$ 9, and is associated exclusively with the latitude axis.

        • WCSHDR_RADECSYS: Accept RADECSYS. This appeared in early drafts of WCS Paper I+II and was subsequently replaced by RADESYSa.

          wcsbth() accepts RADECSYS only if WCSHDR_AUXIMG is also enabled.

        • WCSHDR_VSOURCE: Accept VSOURCEa or VSOUna (wcsbth()). This appeared in early drafts of WCS Paper III and was subsequently dropped in favour of ZSOURCEa and ZSOUna.

          wcsbth() accepts VSOURCEa only if WCSHDR_AUXIMG is also enabled.

        • WCSHDR_DOBSn (wcsbth() only): Allow DOBSn, the column-specific analogue of DATE-OBS. By an oversight this was never formally defined in the standard.

        • WCSHDR_LONGKEY (wcsbth() only): Accept long forms of the alternate binary table and pixel list WCS keywords, i.e. with "a" non- blank. Specifically
          jCRPXna TCRPXna : jCRPXn jCRPna TCRPXn TCRPna CRPIXja
          TPCn_ka : ijPCna TPn_ka PCi_ja
          TCDn_ka : ijCDna TCn_ka CDi_ja
          iCDLTna TCDLTna : iCDLTn iCDEna TCDLTn TCDEna CDELTia
          iCUNIna TCUNIna : iCUNIn iCUNna TCUNIn TCUNna CUNITia
          iCTYPna TCTYPna : iCTYPn iCTYna TCTYPn TCTYna CTYPEia
          iCRVLna TCRVLna : iCRVLn iCRVna TCRVLn TCRVna CRVALia
          iPVn_ma TPVn_ma : iVn_ma TVn_ma PVi_ma
          iPSn_ma TPSn_ma : iSn_ma TSn_ma PSi_ma

          where the primary and standard alternate forms together with the image-header equivalent are shown rightwards of the colon.

          The long form of these keywords could be described as quasi- standard. TPCn_ka, iPVn_ma, and TPVn_ma appeared by mistake in the examples in WCS Paper II and subsequently these and also TCDn_ka, iPSn_ma and TPSn_ma were legitimized by the errata to the WCS papers.

          Strictly speaking, the other long forms are non-standard and in fact have never appeared in any draft of the WCS papers nor in the errata. However, as natural extensions of the primary form they are unlikely to be written with any other intention. Thus it should be safe to accept them provided, of course, that the resulting keyword does not exceed the 8-character limit.

          If WCSHDR_CNAMn is enabled then also accept

          iCNAMna TCNAMna : --- iCNAna --- TCNAna CNAMEia
          iCRDEna TCRDEna : --- iCRDna --- TCRDna CRDERia
          iCSYEna TCSYEna : --- iCSYna --- TCSYna CSYERia

          Note that CNAMEia, CRDERia, CSYERia, and their variants are not used by WCSLIB but are stored in the wcsprm struct as auxiliary information.

        • WCSHDR_CNAMn (wcsbth() only): Accept iCNAMn, iCRDEn, iCSYEn, TCNAMn, TCRDEn, and TCSYEn, i.e. with "a" blank. While non-standard, these are the obvious analogues of iCTYPn, TCTYPn, etc.

        • WCSHDR_AUXIMG (wcsbth() only): Allow the image-header form of an auxiliary WCS keyword with representation-wide scope to provide a default value for all images. This default may be overridden by the column-specific form of the keyword.

          For example, a keyword like EQUINOXa would apply to all image arrays in a binary table, or all pixel list columns with alternate representation "a" unless overridden by EQUIna.

          Specifically the keywords are:

          LATPOLEa for LATPna
          LONPOLEa for LONPna
          RESTFREQ for RFRQna
          RESTFRQa for RFRQna
          RESTWAVa for RWAVna

          whose keyvalues are actually used by WCSLIB, and also keywords that provide auxiliary information that is simply stored in the wcsprm struct:

          EPOCH ... (No column-specific form.)
          EPOCHa ... Only if WCSHDR_EPOCHa is set.
          EQUINOXa for EQUIna
          RADESYSa for RADEna
          RADECSYS for RADEna ... Only if WCSHDR_RADECSYS is set.
          SPECSYSa for SPECna
          SSYSOBSa for SOBSna
          SSYSSRCa for SSRCna
          VELOSYSa for VSYSna
          VELANGLa for VANGna
          VELREF ... (No column-specific form.)
          VELREFa ... Only if WCSHDR_VELREFa is set.
          VSOURCEa for VSOUna ... Only if WCSHDR_VSOURCE is set.
          WCSNAMEa for WCSNna ... Or TWCSna (see below).
          ZSOURCEa for ZSOUna
          DATE-AVG for DAVGn
          DATE-OBS for DOBSn
          MJD-AVG for MJDAn
          MJD-OBS for MJDOBn
          OBSGEO-X for OBSGXn
          OBSGEO-Y for OBSGYn
          OBSGEO-Z for OBSGZn

          where the image-header keywords on the left provide default values for the column specific keywords on the right.

          Keywords in the last group, such as MJD-OBS, apply to all alternate representations, so MJD-OBS would provide a default value for all images in the header.

          This auxiliary inheritance mechanism applies to binary table image arrays and pixel lists alike. Most of these keywords have no default value, the exceptions being LONPOLEa and LATPOLEa, and also RADESYSa and EQUINOXa which provide defaults for each other. Thus the only potential difficulty in using WCSHDR_AUXIMG is that of erroneously inheriting one of these four keywords.

          Unlike WCSHDR_ALLIMG, the existence of one (or all) of these auxiliary WCS image header keywords will not by itself cause a wcsprm struct to be created for alternate representation "a". This is because they do not provide sufficient information to create a non-trivial coordinate representation when used in conjunction with the default values of those keywords, such as CTYPEia, that are parameterized by axis number.

        • WCSHDR_ALLIMG (wcsbth() only): Allow the image-header form of *all* image header WCS keywords to provide a default value for all image arrays in a binary table (n.b. not pixel list). This default may be overridden by the column-specific form of the keyword.

          For example, a keyword like CRPIXja would apply to all image arrays in a binary table with alternate representation "a" unless overridden by jCRPna.

          Specifically the keywords are those listed above for WCSHDR_AUXIMG plus

          WCSAXESa for WCAXna

          which defines the coordinate dimensionality, and the following keywords which are parameterized by axis number:

          CRPIXja for jCRPna
          PCi_ja for ijPCna
          CDi_ja for ijCDna
          CDELTia for iCDEna
          CROTAi for iCROTn
          CROTAia ... Only if WCSHDR_CROTAia is set.
          CUNITia for iCUNna
          CTYPEia for iCTYna
          CRVALia for iCRVna
          PVi_ma for iVn_ma
          PSi_ma for iSn_ma
          CNAMEia for iCNAna
          CRDERia for iCRDna
          CSYERia for iCSYna

          where the image-header keywords on the left provide default values for the column specific keywords on the right.

          This full inheritance mechanism only applies to binary table image arrays, not pixel lists, because in the latter case there is no well-defined association between coordinate axis number and column number.

          Note that CNAMEia, CRDERia, CSYERia, and their variants are not used by WCSLIB but are stored in the wcsprm struct as auxiliary information.

          Note especially that at least one wcsprm struct will be returned for each "a" found in one of the image header keywords listed above:

          • If the image header keywords for "a" are not inherited by a binary table, then the struct will not be associated with any particular table column number and it is up to the user to provide an association.

          • If the image header keywords for "a" are inherited by a binary table image array, then those keywords are considered to be "exhausted" and do not result in a separate wcsprm struct.

        For example, to accept CD00i00j and PC00i00j and reject all other extensions, use 

                 relax = WCSHDR_reject | WCSHDR_CD00i00j | WCSHDR_PC00i00j;

        The parser always treats EPOCH as subordinate to EQUINOXa if both are present, and VSOURCEa is always subordinate to ZSOURCEa.

        Likewise, VELREF is subordinate to the formalism of WCS Paper III, see spcaips().

        Neither wcspih() nor wcsbth() currently recognize the AIPS-convention keywords ALTRPIX or ALTRVAL which effectively define an alternative representation for a spectral axis.

      6. Depending on what flags have been set in its relax argument, wcsbth() could return as many as 27027 wcsprm structs:

        • Up to 27 unattached representations derived from image header keywords.

        • Up to 27 structs for each of up to 999 columns containing an image arrays.

        • Up to 27 structs for a pixel list.

        Note that it is considered legitimate for a column to contain an image array and also form part of a pixel list, and in particular that wcsbth() does not check the TFORM keyword for a pixel list column to check that it is scalar.

        In practice, of course, a realistic binary table header is unlikely to contain more than a handful of images.

        In order for wcsbth() to create a wcsprm struct for a particular coordinate representation, at least one WCS keyword that defines an axis number must be present, either directly or by inheritance if WCSHDR_ALLIMG is set.

        When the image header keywords for an alternate representation are inherited by a binary table image array via WCSHDR_ALLIMG, those keywords are considered to be "exhausted" and do not result in a separate wcsprm struct. Otherwise they do.

      7. Neither wcspih() nor wcsbth() check for duplicated keywords, in most cases they accept the last encountered.

      8. wcspih() and wcsbth() use wcsnpv() and wcsnps() (refer to the prologue of wcs.h) to match the size of the pv[] and ps[] arrays in the wcsprm structs to the number in the header. Consequently there are no unused elements in the pv[] and ps[] arrays, indeed they will often be of zero length.

      9. The FITS WCS standard for pixel lists assumes that a pixel list defines one and only one image, i.e. that each row of the binary table refers to just one event, e.g. the detection of a single photon or neutrino.

        In the absence of a formal mechanism for identifying the columns containing pixel coordinates (as opposed to pixel values or ancillary data recorded at the time the photon or neutrino was detected), Paper I discusses how the WCS keywords themselves may be used to identify them.

        In practice, however, pixel lists have been used to store multiple images. Besides not specifying how to identify columns, the pixel list convention is also silent on the method to be used to associate table columns with image axes.

        wcsbth() simply collects all WCS keywords for a particular coordinate representation (i.e. the "a" value in TCTYna) into one wcsprm struct. However, these alternates need not be associated with the same table columns and this allows a pixel list to contain up to 27 separate images. As usual, if one of these representations happened to contain more than two celestial axes, for example, then an error would result when wcsset() is invoked on it. In this case the "colsel" argument could be used to restrict the columns used to construct the representation so that it only contained one pair of celestial axes.

      int wcstab ( struct wcsprm *  wcs  ) 

      wcstab() assists in filling in the information in the wcsprm struct relating to coordinate lookup tables.

      Tabular coordinates ('TAB') present certain difficulties in that the main components of the lookup table - the multidimensional coordinate array plus an index vector for each dimension - are stored in a FITS binary table extension (BINTABLE). Information required to locate these arrays is stored in PVi_ma and PSi_ma keywords in the image header.

      wcstab() parses the PVi_ma and PSi_ma keywords associated with each 'TAB' axis and allocates memory in the wcsprm struct for the required number of tabprm structs. It sets as much of the tabprm struct as can be gleaned from the image header, and also sets up an array of wtbarr structs (described in the prologue of wcs.h) to assist in extracting the required arrays from the BINTABLE extension(s).

      It is then up to the user to allocate memory for, and copy arrays from the BINTABLE extension(s) into the tabprm structs. A CFITSIO routine, fits_read_wcstab(), has been provided for this purpose, see getwcstab.h. wcsset() will automatically take control of this allocated memory, in particular causing it to be free'd by wcsfree(); the user must not attempt to free it after wcsset() has been called.

      Note that wcspih() and wcsbth() automatically invoke wcstab() on each of the wcsprm structs that they return.

      Parameters:
      [in,out] wcs Coordinate transformation parameters (see below).
      wcstab() sets ntab, tab, nwtb and wtb, allocating memory for the tab and wtb arrays. This allocated memory will be free'd automatically by wcsfree().
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Invalid tabular parameters.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().

      int wcsidx ( int  nwcs,
      struct wcsprm **  wcs,
      int  alts[27] 
      )

      wcsidx() returns an array of 27 indices for the alternate coordinate representations in the array of wcsprm structs returned by wcspih(). For the array returned by wcsbth() it returns indices for the unattached (colnum == 0) representations derived from image header keywords - use wcsbdx() for those derived from binary table image arrays or pixel lists keywords.

      Parameters:
      [in] nwcs Number of coordinate representations in the array.
      [in] wcs Pointer to an array of wcsprm structs returned by wcspih() or wcsbth().
      [out] alts Index of each alternate coordinate representation in the array: alts[0] for the primary, alts[1] for 'A', etc., set to -1 if not present.
      For example, if there was no 'P' representation then 
                                alts['P'-'A'+1] == -1;

      Otherwise, the address of its wcsprm struct would be 
                                wcs + alts['P'-'A'+1];
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int wcsbdx ( int  nwcs,
      struct wcsprm **  wcs,
      int  type,
      short  alts[1000][28] 
      )

      wcsbdx() returns an array of 999 x 27 indices for the alternate coordinate representions for binary table image arrays xor pixel lists in the array of wcsprm structs returned by wcsbth(). Use wcsidx() for the unattached representations derived from image header keywords.

      Parameters:
      [in] nwcs Number of coordinate representations in the array.
      [in] wcs Pointer to an array of wcsprm structs returned by wcsbth().
      [in] type Select the type of coordinate representation:
      • 0: binary table image arrays,
      • 1: pixel lists.
      [out] alts Index of each alternate coordinate represention in the array: alts[col][0] for the primary, alts[col][1] for 'A', to alts[col][26] for 'Z', where col is the 1-relative column number, and col == 0 is used for unattached image headers. Set to -1 if not present.
      alts[col][27] counts the number of coordinate representations of the chosen type for each column.
      For example, if there was no 'P' represention for column 13 then 
                                alts[13]['P'-'A'+1] == -1;

      Otherwise, the address of its wcsprm struct would be 
                                wcs + alts[13]['P'-'A'+1];
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int wcsvfree ( int *  nwcs,
      struct wcsprm **  wcs 
      )

      wcsvfree() frees the memory allocated by wcspih() or wcsbth() for the array of wcsprm structs, first invoking wcsfree() on each of the array members.

      Parameters:
      [in,out] nwcs Number of coordinate representations found; set to 0 on return.
      [in,out] wcs Pointer to the array of wcsprm structs; set to 0 on return.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Null wcsprm pointer passed.

      int wcshdo ( int  relax,
      struct wcsprm *  wcs,
      int *  nkeyrec,
      char **  header 
      )

      wcshdo() translates a wcsprm struct into a FITS header. If the colnum member of the struct is non-zero then a binary table image array header will be produced. Otherwise, if the colax[] member of the struct is set non-zero then a pixel list header will be produced. Otherwise, a primary image or image extension header will be produced.

      If the struct was originally constructed from a header, e.g. by wcspih(), the output header will almost certainly differ in a number of respects:

      • The output header only contains WCS-related keywords. In particular, it does not contain syntactically-required keywords such as SIMPLE, NAXIS, BITPIX, or END.

      • Deprecated (e.g. CROTAn) or non-standard usage will be translated to standard (this is partially dependent on whether wcsfix() was applied).

      • Quantities will be converted to the units used internally, basically SI with the addition of degrees.

      • Floating-point quantities may be given to a different decimal precision.

      • Elements of the PCi_ja matrix will be written if and only if they differ from the unit matrix. Thus, if the matrix is unity then no elements will be written.

      • Additional keywords such as WCSAXESa, CUNITia, LONPOLEa and LATPOLEa may appear.

      • The original keycomments will be lost, although wcshdo() tries hard to write meaningful comments.

      • Keyword order may be changed.

      Keywords can be translated between the image array, binary table, and pixel lists forms by manipulating the colnum or colax[] members of the wcsprm struct.

      Parameters:
      [in] relax Degree of permissiveness:
      • 0: Recognize only FITS keywords defined by the published WCS standard.
      • -1: Admit all informal extensions of the WCS standard.
      Fine-grained control of the degree of permissiveness is also possible as explained in the notes below.
      [in,out] wcs Pointer to a wcsprm struct containing coordinate transformation parameters. Will be initialized if necessary.
      [out] nkeyrec Number of FITS header keyrecords returned in the "header" array.
      [out] header Pointer to an array of char holding the header. Storage for the array is allocated by wcshdo() in blocks of 2880 bytes (32 x 80-character keyrecords) and must be free'd by the user to avoid memory leaks.
      Each keyrecord is 80 characters long and is *NOT* null-terminated, so the first keyrecord starts at (*header)[0], the second at (*header)[80], etc.
      Returns:
      Status return value (associated with wcs_errmsg[]):
      • 0: Success.
      • 1: Null wcsprm pointer passed.
      • 2: Memory allocation failed.
      • 3: Linear transformation matrix is singular.
      • 4: Inconsistent or unrecognized coordinate axis types.
      • 5: Invalid parameter value.
      • 6: Invalid coordinate transformation parameters.
      • 7: Ill-conditioned coordinate transformation parameters.
      For returns > 1, a detailed error message is set in wcsprm::err if enabled, see wcserr_enable().
      Notes:
      wcshdo() interprets the relax argument as a vector of flag bits to provide fine-grained control over what non-standard WCS keywords to write. The flag bits are subject to change in future and should be set by using the preprocessor macros (see below) for the purpose.

      • WCSHDO_none: Don't use any extensions.

      • WCSHDO_all: Write all recognized extensions, equivalent to setting each flag bit.

      • WCSHDO_safe: Write all extensions that are considered to be safe and recommended.

      • WCSHDO_DOBSn: Write DOBSn, the column-specific analogue of DATE-OBS for use in binary tables and pixel lists. WCS Paper III introduced DATE-AVG and DAVGn but by an oversight DOBSn (the obvious analogy) was never formally defined by the standard. The alternative to using DOBSn is to write DATE-OBS which applies to the whole table. This usage is considered to be safe and is recommended.

      • WCSHDO_TPCn_ka: WCS Paper I defined

        • TPn_ka and TCn_ka for pixel lists

        but WCS Paper II uses TPCn_ka in one example and subsequently the errata for the WCS papers legitimized the use of

        • TPCn_ka and TCDn_ka for pixel lists

        provided that the keyword does not exceed eight characters. This usage is considered to be safe and is recommended because of the non-mnemonic terseness of the shorter forms.

      • WCSHDO_PVn_ma: WCS Paper I defined

        • iVn_ma and iSn_ma for bintables and
        • TVn_ma and TSn_ma for pixel lists

        but WCS Paper II uses iPVn_ma and TPVn_ma in the examples and subsequently the errata for the WCS papers legitimized the use of

        • iPVn_ma and iPSn_ma for bintables and
        • TPVn_ma and TPSn_ma for pixel lists

        provided that the keyword does not exceed eight characters. This usage is considered to be safe and is recommended because of the non-mnemonic terseness of the shorter forms.

      • WCSHDO_CRPXna: For historical reasons WCS Paper I defined

        • jCRPXn, iCDLTn, iCUNIn, iCTYPn, and iCRVLn for bintables and
        • TCRPXn, TCDLTn, TCUNIn, TCTYPn, and TCRVLn for pixel lists

        for use without an alternate version specifier. However, because of the eight-character keyword constraint, in order to accommodate column numbers greater than 99 WCS Paper I also defined

        • jCRPna, iCDEna, iCUNna, iCTYna and iCRVna for bintables and
        • TCRPna, TCDEna, TCUNna, TCTYna and TCRVna for pixel lists

        for use with an alternate version specifier (the "a"). Like the PC, CD, PV, and PS keywords there is an obvious tendency to confuse these two forms for column numbers up to 99. It is very unlikely that any parser would reject keywords in the first set with a non-blank alternate version specifier so this usage is considered to be safe and is recommended.

      • WCSHDO_CNAMna: WCS Papers I and III defined

        • iCNAna, iCRDna, and iCSYna for bintables and
        • TCNAna, TCRDna, and TCSYna for pixel lists

        By analogy with the above, the long forms would be

        • iCNAMna, iCRDEna, and iCSYEna for bintables and
        • TCNAMna, TCRDEna, and TCSYEna for pixel lists

        Note that these keywords provide auxiliary information only, none of them are needed to compute world coordinates. This usage is potentially unsafe and is not recommended at this time.

      • WCSHDO_WCSNna: In light of wcsbth() note 4, write WCSNna instead of TWCSna for pixel lists. While wcsbth() treats WCSNna and TWCSna as equivalent, other parsers may not. Consequently, this usage is potentially unsafe and is not recommended at this time.

      Variable Documentation

      const char * wcshdr_errmsg[]

      Error messages to match the status value returned from each function. Use wcs_errmsg[] for status returns from wcshdo().

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcslib_8h-source.html0000644001153600020070000003235712310355626023155 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcslib.h Source File
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      pywcs-1.12/wcslib/html/wcslib_8h.html0000644001153600020070000000575412310355626021660 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcslib.h File Reference

      wcslib.h File Reference

      #include "cel.h"
      #include "fitshdr.h"
      #include "lin.h"
      #include "log.h"
      #include "prj.h"
      #include "spc.h"
      #include "sph.h"
      #include "spx.h"
      #include "tab.h"
      #include "wcs.h"
      #include "wcserr.h"
      #include "wcsfix.h"
      #include "wcshdr.h"
      #include "wcsmath.h"
      #include "wcsprintf.h"
      #include "wcstrig.h"
      #include "wcsunits.h"
      #include "wcsutil.h"

      Go to the source code of this file.

      Detailed Description

      This header file is provided purely for convenience. Use it to include all of the separate WCSLIB headers.
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcsmath_8h-source.html0000644001153600020070000002120212310355626023323 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsmath.h Source File
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      wcsmath.h File Reference

      Go to the source code of this file.

      Defines

      #define PI   3.141592653589793238462643
      #define D2R   PI/180.0
       Degrees to radians conversion factor.
      #define R2D   180.0/PI
       Radians to degrees conversion factor.
      #define SQRT2   1.4142135623730950488
      #define SQRT2INV   1.0/SQRT2
      #define UNDEFINED   987654321.0e99
       Value used to indicate an undefined quantity.
      #define undefined(value)   (value == UNDEFINED)
       Macro used to test for an undefined quantity.

      Detailed Description

      Definition of mathematical constants used by WCSLIB.

      Define Documentation

      #define PI   3.141592653589793238462643

      #define D2R   PI/180.0

      Factor $\pi/180^\circ$ to convert from degrees to radians.

      #define R2D   180.0/PI

      Factor $180^\circ/\pi$ to convert from radians to degrees.

      #define SQRT2   1.4142135623730950488

      $\sqrt{2}$, used only by molset() (MOL projection).

      #define SQRT2INV   1.0/SQRT2

      $1/\sqrt{2}$, used only by qscx2s() (QSC projection).

      #define UNDEFINED   987654321.0e99

      Value used to indicate an undefined quantity (noting that NaNs cannot be used portably).

      #define undefined ( value   )     (value == UNDEFINED)

      Macro used to test for an undefined value.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcstrig_8h-source.html0000644001153600020070000005240312310355626023346 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcstrig.h Source File
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      wcstrig.h File Reference

      #include <math.h>
      #include "wcsconfig.h"

      Go to the source code of this file.

      Defines

      #define WCSTRIG_TOL   1e-10
       Domain tolerance for asin() and acos() functions.

      Functions

      double cosd (double angle)
       Cosine of an angle in degrees.
      double sind (double angle)
       Sine of an angle in degrees.
      void sincosd (double angle, double *sin, double *cos)
       Sine and cosine of an angle in degrees.
      double tand (double angle)
       Tangent of an angle in degrees.
      double acosd (double x)
       Inverse cosine, returning angle in degrees.
      double asind (double y)
       Inverse sine, returning angle in degrees.
      double atand (double s)
       Inverse tangent, returning angle in degrees.
      double atan2d (double y, double x)
       Polar angle of $(x,y)$, in degrees.

      Detailed Description

      When dealing with celestial coordinate systems and spherical projections (some moreso than others) it is often desirable to use an angular measure that provides an exact representation of the latitude of the north or south pole. The WCSLIB routines use the following trigonometric functions that take or return angles in degrees:

      These "trigd" routines are expected to handle angles that are a multiple of $90^\circ$ returning an exact result. Some C implementations provide these as part of a system library and in such cases it may (or may not!) be preferable to use them. WCSLIB provides wrappers on the standard trig functions based on radian measure, adding tests for multiples of $90^\circ$.

      However, wcstrig.h also provides the choice of using preprocessor macro implementations of the trigd functions that don't test for multiples of $90^\circ$ (compile with -DWCSTRIG_MACRO). These are typically 20% faster but may lead to problems near the poles.

      Define Documentation

      #define WCSTRIG_TOL   1e-10

      Domain tolerance for the asin() and acos() functions to allow for floating point rounding errors.

      If $v$ lies in the range $1 < |v| < 1 + WCSTRIG\_TOL$ then it will be treated as $|v| == 1$.

      Function Documentation

      double cosd ( double  angle  ) 

      cosd() returns the cosine of an angle given in degrees.

      Parameters:
      [in] angle [deg].
      Returns:
      Cosine of the angle.

      double sind ( double  angle  ) 

      sind() returns the sine of an angle given in degrees.

      Parameters:
      [in] angle [deg].
      Returns:
      Sine of the angle.

      void sincosd ( double  angle,
      double *  sin,
      double *  cos 
      )

      sincosd() returns the sine and cosine of an angle given in degrees.

      Parameters:
      [in] angle [deg].
      [out] sin Sine of the angle.
      [out] cos Cosine of the angle.
      Returns:

      double tand ( double  angle  ) 

      tand() returns the tangent of an angle given in degrees.

      Parameters:
      [in] angle [deg].
      Returns:
      Tangent of the angle.

      double acosd ( double  x  ) 

      acosd() returns the inverse cosine in degrees.

      Parameters:
      [in] x in the range [-1,1].
      Returns:
      Inverse cosine of x [deg].

      double asind ( double  y  ) 

      asind() returns the inverse sine in degrees.

      Parameters:
      [in] y in the range [-1,1].
      Returns:
      Inverse sine of y [deg].

      double atand ( double  s  ) 

      atand() returns the inverse tangent in degrees.

      Parameters:
      [in] s 
      Returns:
      Inverse tangent of s [deg].

      double atan2d ( double  y,
      double  x 
      )

      atan2d() returns the polar angle, $\beta$, in degrees, of polar coordinates $(\rho,\beta)$ corresponding Cartesian coordinates $(x,y)$. It is equivalent to the $\arg(x,y)$ function of WCS Paper II, though with transposed arguments.

      Parameters:
      [in] y Cartesian $y$-coordinate.
      [in] x Cartesian $x$-coordinate.
      Returns:
      Polar angle of $(x,y)$ [deg].

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcsunits_8h-source.html0000644001153600020070000013665012310355626023552 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsunits.h Source File
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      pywcs-1.12/wcslib/html/wcsunits_8h.html0000644001153600020070000015634512310355626022257 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsunits.h File Reference

      wcsunits.h File Reference

      #include "wcserr.h"

      Go to the source code of this file.

      Defines

      #define WCSUNITS_PLANE_ANGLE   0
       Array index for plane angle units type.
      #define WCSUNITS_SOLID_ANGLE   1
       Array index for solid angle units type.
      #define WCSUNITS_CHARGE   2
       Array index for charge units type.
      #define WCSUNITS_MOLE   3
       Array index for mole units type.
      #define WCSUNITS_TEMPERATURE   4
       Array index for temperature units type.
      #define WCSUNITS_LUMINTEN   5
       Array index for luminous intensity units type.
      #define WCSUNITS_MASS   6
       Array index for mass units type.
      #define WCSUNITS_LENGTH   7
       Array index for length units type.
      #define WCSUNITS_TIME   8
       Array index for time units type.
      #define WCSUNITS_BEAM   9
       Array index for beam units type.
      #define WCSUNITS_BIN   10
       Array index for bin units type.
      #define WCSUNITS_BIT   11
       Array index for bit units type.
      #define WCSUNITS_COUNT   12
       Array index for count units type.
      #define WCSUNITS_MAGNITUDE   13
       Array index for stellar magnitude units type.
      #define WCSUNITS_PIXEL   14
       Array index for pixel units type.
      #define WCSUNITS_SOLRATIO   15
       Array index for solar mass ratio units type.
      #define WCSUNITS_VOXEL   16
       Array index for voxel units type.
      #define WCSUNITS_NTYPE   17
       Number of entries in the units array.

      Enumerations

      enum  wcsunits_errmsg_enum {
        UNITSERR_SUCCESS = 0, UNITSERR_BAD_NUM_MULTIPLIER = 1, UNITSERR_DANGLING_BINOP = 2, UNITSERR_BAD_INITIAL_SYMBOL = 3,
        UNITSERR_FUNCTION_CONTEXT = 4, UNITSERR_BAD_EXPON_SYMBOL = 5, UNITSERR_UNBAL_BRACKET = 6, UNITSERR_UNBAL_PAREN = 7,
        UNITSERR_CONSEC_BINOPS = 8, UNITSERR_PARSER_ERROR = 9, UNITSERR_BAD_UNIT_SPEC = 10, UNITSERR_BAD_FUNCS = 11,
        UNITSERR_UNSAFE_TRANS = 12
      }

      Functions

      int wcsunitse (const char have[], const char want[], double *scale, double *offset, double *power, struct wcserr **err)
       FITS units specification conversion.
      int wcsutrne (int ctrl, char unitstr[], struct wcserr **err)
       Translation of non-standard unit specifications.
      int wcsulexe (const char unitstr[], int *func, double *scale, double units[], struct wcserr **err)
       FITS units specification parser.
      int wcsunits (const char have[], const char want[], double *scale, double *offset, double *power)
      int wcsutrn (int ctrl, char unitstr[])
      int wcsulex (const char unitstr[], int *func, double *scale, double units[])

      Variables

      const char * wcsunits_errmsg []
       Status return messages.
      const char * wcsunits_types []
       Names of physical quantities.
      const char * wcsunits_units []
       Names of units.

      Detailed Description

      Routines in this suite deal with units specifications and conversions:

      • wcsunitse(): given two unit specifications, derive the conversion from one to the other.

      • wcsutrne(): translates certain commonly used but non-standard unit strings. It is intended to be called before wcsulexe() which only handles standard FITS units specifications.

      • wcsulexe(): parses a standard FITS units specification of arbitrary complexity, deriving the conversion to canonical units.

      Define Documentation

      #define WCSUNITS_PLANE_ANGLE   0

      Array index for plane angle units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_SOLID_ANGLE   1

      Array index for solid angle units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_CHARGE   2

      Array index for charge units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_MOLE   3

      Array index for mole ("gram molecular weight") units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_TEMPERATURE   4

      Array index for temperature units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_LUMINTEN   5

      Array index for luminous intensity units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_MASS   6

      Array index for mass units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_LENGTH   7

      Array index for length units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_TIME   8

      Array index for time units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_BEAM   9

      Array index for beam units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_BIN   10

      Array index for bin units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_BIT   11

      Array index for bit units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_COUNT   12

      Array index for count units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_MAGNITUDE   13

      Array index for stellar magnitude units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_PIXEL   14

      Array index for pixel units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_SOLRATIO   15

      Array index for solar mass ratio units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_VOXEL   16

      Array index for voxel units in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      #define WCSUNITS_NTYPE   17

      Number of entries in the units array returned by wcsulex(), and the wcsunits_types[] and wcsunits_units[] global variables.

      Enumeration Type Documentation

      enum wcsunits_errmsg_enum

      Enumerator:
      UNITSERR_SUCCESS 
      UNITSERR_BAD_NUM_MULTIPLIER 
      UNITSERR_DANGLING_BINOP 
      UNITSERR_BAD_INITIAL_SYMBOL 
      UNITSERR_FUNCTION_CONTEXT 
      UNITSERR_BAD_EXPON_SYMBOL 
      UNITSERR_UNBAL_BRACKET 
      UNITSERR_UNBAL_PAREN 
      UNITSERR_CONSEC_BINOPS 
      UNITSERR_PARSER_ERROR 
      UNITSERR_BAD_UNIT_SPEC 
      UNITSERR_BAD_FUNCS 
      UNITSERR_UNSAFE_TRANS 

      Function Documentation

      int wcsunitse ( const char  have[],
      const char  want[],
      double *  scale,
      double *  offset,
      double *  power,
      struct wcserr **  err 
      )

      wcsunitse() derives the conversion from one system of units to another.

      A deprecated form of this function, wcsunits(), lacks the wcserr** parameter.

      Parameters:
      [in] have FITS units specification to convert from (null- terminated), with or without surrounding square brackets (for inline specifications); text following the closing bracket is ignored.
      [in] want FITS units specification to convert to (null- terminated), with or without surrounding square brackets (for inline specifications); text following the closing bracket is ignored.
      [out] scale,offset,power Convert units using 
                                pow(scale*value + offset, power);

      Normally offset is zero except for log() or ln() conversions, e.g. "log(MHz)" to "ln(Hz)". Likewise, power is normally unity except for exp() conversions, e.g. "exp(ms)" to "exp(/Hz)". Thus conversions ordinarily consist of 
                                value *= scale;
      [out] err If enabled, for function return values > 1, this struct will contain a detailed error message, see wcserr_enable(). May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • 0: Success.
      • 1-9: Status return from wcsulexe().
      • 10: Non-conformant unit specifications.
      • 11: Non-conformant functions.
      scale is zeroed on return if an error occurs.

      int wcsutrne ( int  ctrl,
      char  unitstr[],
      struct wcserr **  err 
      )

      wcsutrne() translates certain commonly used but non-standard unit strings, e.g. "DEG", "MHZ", "KELVIN", that are not recognized by wcsulexe(), refer to the notes below for a full list. Compounds are also recognized, e.g. "JY/BEAM" and "KM/SEC/SEC". Extraneous embedded blanks are removed.

      A deprecated form of this function, wcsutrn(), lacks the wcserr** parameter.

      Parameters:
      [in] ctrl Although "S" is commonly used to represent seconds, its translation to "s" is potentially unsafe since the standard recognizes "S" formally as Siemens, however rarely that may be used. The same applies to "H" for hours (Henry), and "D" for days (Debye). This bit-flag controls what to do in such cases:
      • 1: Translate "S" to "s".
      • 2: Translate "H" to "h".
      • 4: Translate "D" to "d".
      Thus ctrl == 0 doesn't do any unsafe translations, whereas ctrl == 7 does all of them.
      [in,out] unitstr Null-terminated character array containing the units specification to be translated.
      Inline units specifications in the a FITS header keycomment are also handled. If the first non-blank character in unitstr is '[' then the unit string is delimited by its matching ']'. Blanks preceding '[' will be stripped off, but text following the closing bracket will be preserved without modification.
      [in,out] err If enabled, for function return values > 1, this struct will contain a detailed error message, see wcserr_enable(). May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • -1: No change was made, other than stripping blanks (not an error).
      • 0: Success.
      • 9: Internal parser error.
      • 12: Potentially unsafe translation, whether applied or not (see notes).
      Notes:
      Translation of non-standard unit specifications: apart from leading and trailing blanks, a case-sensitive match is required for the aliases listed below, in particular the only recognized aliases with metric prefixes are "KM", "KHZ", "MHZ", and "GHZ". Potentially unsafe translations of "D", "H", and "S", shown in parentheses, are optional. 
            Unit       Recognized aliases
      ----       -------------------------------------------------------------
      Angstrom   angstrom
      arcmin     arcmins, ARCMIN, ARCMINS
      arcsec     arcsecs, ARCSEC, ARCSECS
      beam       BEAM
      byte       Byte
      d          day, days, (D), DAY, DAYS
      deg        degree, degrees, DEG, DEGREE, DEGREES
      GHz        GHZ
      h          hr, (H), HR
      Hz         hz, HZ
      kHz        KHZ
      Jy         JY
      K          kelvin, kelvins, Kelvin, Kelvins, KELVIN, KELVINS
      km         KM
      m          metre, meter, metres, meters, M, METRE, METER, METRES, METERS
      min        MIN
      MHz        MHZ
      Ohm        ohm
      Pa         pascal, pascals, Pascal, Pascals, PASCAL, PASCALS
      pixel      pixels, PIXEL, PIXELS
      rad        radian, radians, RAD, RADIAN, RADIANS
      s          sec, second, seconds, (S), SEC, SECOND, SECONDS
      V          volt, volts, Volt, Volts, VOLT, VOLTS
      yr         year, years, YR, YEAR, YEARS

      The aliases "angstrom", "ohm", and "Byte" for (Angstrom, Ohm, and byte) are recognized by wcsulexe() itself as an unofficial extension of the standard, but they are converted to the standard form here.

      int wcsulexe ( const char  unitstr[],
      int *  func,
      double *  scale,
      double  units[],
      struct wcserr **  err 
      )

      wcsulexe() parses a standard FITS units specification of arbitrary complexity, deriving the scale factor required to convert to canonical units - basically SI with degrees and "dimensionless" additions such as byte, pixel and count.

      A deprecated form of this function, wcsulex(), lacks the wcserr** parameter.

      Parameters:
      [in] unitstr Null-terminated character array containing the units specification, with or without surrounding square brackets (for inline specifications); text following the closing bracket is ignored.
      [out] func Special function type, see note 4:
      • 0: None
      • 1: log() ...base 10
      • 2: ln() ...base e
      • 3: exp()
      [out] scale Scale factor for the unit specification; multiply a value expressed in the given units by this factor to convert it to canonical units.
      [out] units A units specification is decomposed into powers of 16 fundamental unit types: angle, mass, length, time, count, pixel, etc. Preprocessor macro WCSUNITS_NTYPE is defined to dimension this vector, and others such WCSUNITS_PLANE_ANGLE, WCSUNITS_LENGTH, etc. to access its elements.
      Corresponding character strings, wcsunits_types[] and wcsunits_units[], are predefined to describe each quantity and its canonical units.
      [out] err If enabled, for function return values > 1, this struct will contain a detailed error message, see wcserr_enable(). May be NULL if an error message is not desired.
      Returns:
      Status return value:
      • 0: Success.
      • 1: Invalid numeric multiplier.
      • 2: Dangling binary operator.
      • 3: Invalid symbol in INITIAL context.
      • 4: Function in invalid context.
      • 5: Invalid symbol in EXPON context.
      • 6: Unbalanced bracket.
      • 7: Unbalanced parenthesis.
      • 8: Consecutive binary operators.
      • 9: Internal parser error.
      scale and units[] are zeroed on return if an error occurs.
      Notes:
      1. wcsulexe() is permissive in accepting whitespace in all contexts in a units specification where it does not create ambiguity (e.g. not between a metric prefix and a basic unit string), including in strings like "log (m ** 2)" which is formally disallowed.

      2. Supported extensions:
        • "angstrom" (OGIP usage) is allowed in addition to "Angstrom".
        • "ohm" (OGIP usage) is allowed in addition to "Ohm".
        • "Byte" (common usage) is allowed in addition to "byte".

      3. Table 6 of WCS Paper I lists eleven units for which metric prefixes are allowed. However, in this implementation only prefixes greater than unity are allowed for "a" (annum), "yr" (year), "pc" (parsec), "bit", and "byte", and only prefixes less than unity are allowed for "mag" (stellar magnitude).

        Metric prefix "P" (peta) is specifically forbidden for "a" (annum) to avoid confusion with "Pa" (Pascal, not peta-annum). Note that metric prefixes are specifically disallowed for "h" (hour) and "d" (day) so that "ph" (photons) cannot be interpreted as pico-hours, nor "cd" (candela) as centi-days.

      4. Function types log(), ln() and exp() may only occur at the start of the units specification. The scale and units[] returned for these refers to the string inside the function "argument", e.g. to "MHz" in log(MHz) for which a scale of $10^6$ will be returned.

      int wcsunits ( const char  have[],
      const char  want[],
      double *  scale,
      double *  offset,
      double *  power 
      )

      int wcsutrn ( int  ctrl,
      char  unitstr[] 
      )

      int wcsulex ( const char  unitstr[],
      int *  func,
      double *  scale,
      double  units[] 
      )

      Variable Documentation

      const char * wcsunits_errmsg[]

      Error messages to match the status value returned from each function.

      const char * wcsunits_types[]

      Names for physical quantities to match the units vector returned by wcsulexe():

      • 0: plane angle
      • 1: solid angle
      • 2: charge
      • 3: mole
      • 4: temperature
      • 5: luminous intensity
      • 6: mass
      • 7: length
      • 8: time
      • 9: beam
      • 10: bin
      • 11: bit
      • 12: count
      • 13: stellar magnitude
      • 14: pixel
      • 15: solar ratio
      • 16: voxel

      const char * wcsunits_units[]

      Names for the units (SI) to match the units vector returned by wcsulexe():

      • 0: degree
      • 1: steradian
      • 2: Coulomb
      • 3: mole
      • 4: Kelvin
      • 5: candela
      • 6: kilogram
      • 7: metre
      • 8: second

      The remainder are dimensionless.

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcsutil_8h-source.html0000644001153600020070000005524612310355626023366 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsutil.h Source File
      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/html/wcsutil_8h.html0000644001153600020070000004171712310355626022066 0ustar cslocumSTSCI\science00000000000000 WCSLIB 4.10: wcsutil.h File Reference

      wcsutil.h File Reference

      Go to the source code of this file.

      Functions

      void wcsutil_blank_fill (int n, char c[])
       Fill a character string with blanks.
      void wcsutil_null_fill (int n, char c[])
       Fill a character string with NULLs.
      int wcsutil_allEq (int nvec, int nelem, const double *first)
       Test for equality of a particular vector element.
      void wcsutil_setAll (int nvec, int nelem, double *first)
       Set a particular vector element.
      void wcsutil_setAli (int nvec, int nelem, int *first)
       Set a particular vector element.
      void wcsutil_setBit (int nelem, const int *sel, int bits, int *array)
       Set bits in selected elements of an array.
      char * wcsutil_fptr2str (int(*func)(), char hext[])

      Detailed Description

      Simple utility functions for internal use only by WCSLIB. They are documented here solely as an aid to understanding the code. They are not intended for external use - the API may change without notice!

      Function Documentation

      void wcsutil_blank_fill ( int  n,
      char  c[] 
      )

      INTERNAL USE ONLY.

      wcsutil_blank_fill() pads a character string with blanks starting with the terminating NULL character.

      Used by the Fortran wrapper functions in translating C character strings into Fortran CHARACTER variables.

      Parameters:
      [in] n Length of the character array, c[].
      [in,out] c The character string. It will not be null-terminated on return.
      Returns:

      void wcsutil_null_fill ( int  n,
      char  c[] 
      )

      INTERNAL USE ONLY.

      wcsutil_null_fill() strips off trailing blanks and pads the character array holding the string with NULL characters.

      Used mainly to make character strings intelligible in the GNU debugger which prints the rubbish following the terminating NULL, obscuring the valid part of the string.

      Parameters:
      [in] n Number of characters.
      [in,out] c The character string.
      Returns:

      int wcsutil_allEq ( int  nvec,
      int  nelem,
      const double *  first 
      )

      INTERNAL USE ONLY.

      wcsutil_allEq() tests for equality of a particular element in a set of vectors.

      Parameters:
      [in] nvec The number of vectors.
      [in] nelem The length of each vector.
      [in] first Pointer to the first element to test in the array. The elements tested for equality are 
                                *first == *(first + nelem)
                                 == *(first + nelem*2)
                                            :
                                 == *(first + nelem*(nvec-1));

      The array might be dimensioned as 
                                double v[nvec][nelem];
      Returns:
      Status return value:
      • 0: Not all equal.
      • 1: All equal.

      void wcsutil_setAll ( int  nvec,
      int  nelem,
      double *  first 
      )

      INTERNAL USE ONLY.

      wcsutil_setAll() sets the value of a particular element in a set of vectors.

      Parameters:
      [in] nvec The number of vectors.
      [in] nelem The length of each vector.
      [in,out] first Pointer to the first element in the array, the value of which is used to set the others 
                                *(first + nelem) = *first;
                          *(first + nelem*2) = *first;
                                  :
                          *(first + nelem*(nvec-1)) = *first;

      The array might be dimensioned as 
                                double v[nvec][nelem];
      Returns:

      void wcsutil_setAli ( int  nvec,
      int  nelem,
      int *  first 
      )

      INTERNAL USE ONLY.

      wcsutil_setAli() sets the value of a particular element in a set of vectors.

      Parameters:
      [in] nvec The number of vectors.
      [in] nelem The length of each vector.
      [in,out] first Pointer to the first element in the array, the value of which is used to set the others 
                                *(first + nelem) = *first;
                          *(first + nelem*2) = *first;
                                  :
                          *(first + nelem*(nvec-1)) = *first;

      The array might be dimensioned as 
                                int v[nvec][nelem];
      Returns:

      void wcsutil_setBit ( int  nelem,
      const int *  sel,
      int  bits,
      int *  array 
      )

      INTERNAL USE ONLY.

      wcsutil_setBit() sets bits in selected elements of an array.

      Parameters:
      [in] nelem Number of elements in the array.
      [in] sel Address of a selection array of length nelem. May be specified as the null pointer in which case all elements are selected.
      [in] bits Bit mask.
      [in,out] array Address of the array of length nelem.
      Returns:

      char* wcsutil_fptr2str ( int(*)()  func,
      char  hext[] 
      )

      Generated on Mon Feb 6 10:41:57 2012 for WCSLIB 4.10 by  doxygen 1.5.6
      pywcs-1.12/wcslib/INSTALL0000644001153600020070000003104412310355626017164 0ustar cslocumSTSCI\science00000000000000------------------------------------------------------------------------------ WCSLIB 4.10 and PGSBOX 4.10 INSTALLATION -------------------------------------- WCSLIB requires an ANSI C compiler with standard ANSI C environment, that is, a standard C library and header files as defined in Appendix B of Kernigan & Ritchie, 2nd ed. Installation of WCSLIB is handled by GNU autoconf; GNU make (referred to here as 'gmake') must be used. The WCSLIB distribution also includes PGSBOX (refer to the README file), to unpack it type zcat wcslib-4.10.tar.gz | tar pvxf - cd wcslib-4.10 then if you do not need to specify any configuration options, simply run gmake This will run 'configure' to generate "makedefs" which is included by the top- level GNUmakefile and those in each subdirectory, and then build 'libwcs.a', which includes both the C library and Fortran wrappers, and also libpgsbox.a. (WARNING: The build may fail with gmake 3.79, upgrade to 3.79.1 or later.) configure tries to determine the location of the PGPLOT and CFITSIO libraries required by some programs in the test suite. If it fails to find them you can, if you wish, tailor the few variables found at the start of "makedefs". Of course you do not need to exercise the test suite in order to build and install the library - if configure fails to find anything required for that it will issue an explicit error message. To build and exercise the test suite use gmake check To install the object libraries and header files, do gmake install TWEAKING THE INSTALLATION DEFAULTS ---------------------------------- By default the library and header files are installed in the lib and include subdirectories of /usr/local/. To change this, or any other options, run configure separately before gmake: ./configure --prefix=/some/other/dir gmake Use ./configure --help to list configure's options. Useful options are --with-pgplotinc --with-pgplotlib --with-cfitsioinc --with-cfitsiolib Which allow additional directories to be added to the library and include file search path. Installation of WCSLIB differs a little from most packages in that all configurable makefile variables are defined in a single file, "makedefs", which configure generates from "makedefs.in". If you need to redefine any of the makefile variables you can modify makedefs, or preferably makedefs.in. The makefile will automatically detect this and re-run config.status to re-generate a new makedefs. configure also creates four header files: wcsconfig.h: Contains general purpose preprocessor definitions. It is included by the other wcsconfig header files. wcsconfig_f77.h: By common convention the WCSLIB Fortran wrappers have been written (in C) using function names in lower case with an underscore ("_") suffix. wcsconfig_f77.h defines a preprocessor macro, F77_FUNC(name,NAME), that may redefine these to suit different name mangling schemes used by some Fortran compilers. wcsconfig_tests.h: Contains C preprocessor definitions for compiling the test/demo programs. wcsconfig_utils.h: Contains C preprocessor macro definitions for compiling the utility programs provided with WCSLIB. If you do have trouble building the library please send me config.log. The INSTALL file provided with GNU autoconf 2.53 is appended without change. Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: INSTALL,v 4.10 2012/02/05 23:41:45 cal103 Exp $ ============================================================================== Copyright 1994, 1995, 1996, 1999, 2000, 2001, 2002 Free Software Foundation, Inc. This file is free documentation; the Free Software Foundation gives unlimited permission to copy, distribute and modify it. Basic Installation ================== These are generic installation instructions. The `configure' shell script attempts to guess correct values for various system-dependent variables used during compilation. It uses those values to create a `Makefile' in each directory of the package. It may also create one or more `.h' files containing system-dependent definitions. Finally, it creates a shell script `config.status' that you can run in the future to recreate the current configuration, and a file `config.log' containing compiler output (useful mainly for debugging `configure'). It can also use an optional file (typically called `config.cache' and enabled with `--cache-file=config.cache' or simply `-C') that saves the results of its tests to speed up reconfiguring. (Caching is disabled by default to prevent problems with accidental use of stale cache files.) If you need to do unusual things to compile the package, please try to figure out how `configure' could check whether to do them, and mail diffs or instructions to the address given in the `README' so they can be considered for the next release. If you are using the cache, and at some point `config.cache' contains results you don't want to keep, you may remove or edit it. The file `configure.ac' (or `configure.in') is used to create `configure' by a program called `autoconf'. You only need `configure.ac' if you want to change it or regenerate `configure' using a newer version of `autoconf'. The simplest way to compile this package is: 1. `cd' to the directory containing the package's source code and type `./configure' to configure the package for your system. If you're using `csh' on an old version of System V, you might need to type `sh ./configure' instead to prevent `csh' from trying to execute `configure' itself. Running `configure' takes awhile. While running, it prints some messages telling which features it is checking for. 2. Type `make' to compile the package. 3. Optionally, type `make check' to run any self-tests that come with the package. 4. Type `make install' to install the programs and any data files and documentation. 5. You can remove the program binaries and object files from the source code directory by typing `make clean'. To also remove the files that `configure' created (so you can compile the package for a different kind of computer), type `make distclean'. There is also a `make maintainer-clean' target, but that is intended mainly for the package's developers. If you use it, you may have to get all sorts of other programs in order to regenerate files that came with the distribution. Compilers and Options ===================== Some systems require unusual options for compilation or linking that the `configure' script does not know about. Run `./configure --help' for details on some of the pertinent environment variables. You can give `configure' initial values for variables by setting them in the environment. You can do that on the command line like this: ./configure CC=c89 CFLAGS=-O2 LIBS=-lposix *Note Defining Variables::, for more details. Compiling For Multiple Architectures ==================================== You can compile the package for more than one kind of computer at the same time, by placing the object files for each architecture in their own directory. To do this, you must use a version of `make' that supports the `VPATH' variable, such as GNU `make'. `cd' to the directory where you want the object files and executables to go and run the `configure' script. `configure' automatically checks for the source code in the directory that `configure' is in and in `..'. If you have to use a `make' that does not support the `VPATH' variable, you have to compile the package for one architecture at a time in the source code directory. After you have installed the package for one architecture, use `make distclean' before reconfiguring for another architecture. Installation Names ================== By default, `make install' will install the package's files in `/usr/local/bin', `/usr/local/man', etc. You can specify an installation prefix other than `/usr/local' by giving `configure' the option `--prefix=PATH'. You can specify separate installation prefixes for architecture-specific files and architecture-independent files. If you give `configure' the option `--exec-prefix=PATH', the package will use PATH as the prefix for installing programs and libraries. Documentation and other data files will still use the regular prefix. In addition, if you use an unusual directory layout you can give options like `--bindir=PATH' to specify different values for particular kinds of files. Run `configure --help' for a list of the directories you can set and what kinds of files go in them. If the package supports it, you can cause programs to be installed with an extra prefix or suffix on their names by giving `configure' the option `--program-prefix=PREFIX' or `--program-suffix=SUFFIX'. Optional Features ================= Some packages pay attention to `--enable-FEATURE' options to `configure', where FEATURE indicates an optional part of the package. They may also pay attention to `--with-PACKAGE' options, where PACKAGE is something like `gnu-as' or `x' (for the X Window System). The `README' should mention any `--enable-' and `--with-' options that the package recognizes. For packages that use the X Window System, `configure' can usually find the X include and library files automatically, but if it doesn't, you can use the `configure' options `--x-includes=DIR' and `--x-libraries=DIR' to specify their locations. Specifying the System Type ========================== There may be some features `configure' cannot figure out automatically, but needs to determine by the type of machine the package will run on. Usually, assuming the package is built to be run on the _same_ architectures, `configure' can figure that out, but if it prints a message saying it cannot guess the machine type, give it the `--build=TYPE' option. TYPE can either be a short name for the system type, such as `sun4', or a canonical name which has the form: CPU-COMPANY-SYSTEM where SYSTEM can have one of these forms: OS KERNEL-OS See the file `config.sub' for the possible values of each field. If `config.sub' isn't included in this package, then this package doesn't need to know the machine type. If you are _building_ compiler tools for cross-compiling, you should use the `--target=TYPE' option to select the type of system they will produce code for. If you want to _use_ a cross compiler, that generates code for a platform different from the build platform, you should specify the "host" platform (i.e., that on which the generated programs will eventually be run) with `--host=TYPE'. Sharing Defaults ================ If you want to set default values for `configure' scripts to share, you can create a site shell script called `config.site' that gives default values for variables like `CC', `cache_file', and `prefix'. `configure' looks for `PREFIX/share/config.site' if it exists, then `PREFIX/etc/config.site' if it exists. Or, you can set the `CONFIG_SITE' environment variable to the location of the site script. A warning: not all `configure' scripts look for a site script. Defining Variables ================== Variables not defined in a site shell script can be set in the environment passed to `configure'. However, some packages may run configure again during the build, and the customized values of these variables may be lost. In order to avoid this problem, you should set them in the `configure' command line, using `VAR=value'. For example: ./configure CC=/usr/local2/bin/gcc will cause the specified gcc to be used as the C compiler (unless it is overridden in the site shell script). `configure' Invocation ====================== `configure' recognizes the following options to control how it operates. `--help' `-h' Print a summary of the options to `configure', and exit. `--version' `-V' Print the version of Autoconf used to generate the `configure' script, and exit. `--cache-file=FILE' Enable the cache: use and save the results of the tests in FILE, traditionally `config.cache'. FILE defaults to `/dev/null' to disable caching. `--config-cache' `-C' Alias for `--cache-file=config.cache'. `--quiet' `--silent' `-q' Do not print messages saying which checks are being made. To suppress all normal output, redirect it to `/dev/null' (any error messages will still be shown). `--srcdir=DIR' Look for the package's source code in directory DIR. Usually `configure' can determine that directory automatically. `configure' also accepts some other, not widely useful, options. Run `configure --help' for more details. pywcs-1.12/wcslib/makedefs.in0000644001153600020070000002020312310355626020235 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile definitions for building WCSLIB 4.10 # # makedefs is generated from makedefs.in by configure. It contains variable # definitions and some general-purpose rules for building WCSLIB. # # Targets defined here # -------------------- # printenv: Print the environment as seen within makefile rules. # show: Print the values of all makefile variables used. # # Notes: # 1) If you need to make changes then it may be preferable to modify # makedefs.in (not makedefs). The makefile will detect this and # automatically re-run config.status to regenerate makedefs. # # 2) There are three choices for trigd functions - cosd(), sind(), tand(), # acosd(), asind(), atand(), and atan2d(), made by setting WCSTRIG: # # 1: Use the wrapper functions supplied with WCSLIB (default): # WCSTRIG := WRAPPER # # 2: Use native trigd functions supplied in a mathematics library such # as libsunmath (you will also need to add the library to the LIBS # variable below): # WCSTRIG := NATIVE # # 3: Use C preprocessor macro implementations of the trigd functions # (this method is typically 20% faster but may lead to rounding # errors near the poles): # WCSTRIG := MACRO # # 3) Variables for creating the shared (dynamic) library are currently # only set by 'configure' if the GNU C compiler is used. However, # you can set these variables by hand, preferably in makedefs.in. # # Shared libraries require position-independent code (PIC) which imposes # a performance overhead. Consequently the static libraries are # compiled separately without this option. # # The shared library will be installed with version number, e.g. as # libwcs.so.4.10 or libwcs.4.10.dylib with or without the symlink # required to make it visible to the linker (controlled by the SHRLN # variable). On Macs it is deliberately not created because its very # existence precludes static linking with the cctools linker. You can # still link dynamically by using -lwcs.4.10. # # 4) PGPLOT is Tim Pearson's Fortran graphics library with separate C # interface available from astro.caltech.edu. It is only required by # one utility, wcsgrid, and the test programs that plot test grids # (tprj2, tcel1, tcel2, tspc, ttab2, ttab3, twcsmix, and tpih2). You can # skip these by setting PGPLOTLIB to blank. # # It is difficult for configure to deduce what auxiliary graphics # libraries may be needed for PGPLOT since it depends on which of many # possible graphics drivers were selected when PGPLOT was installed. # Therefore it is quite likely that you will need to add additional # libraries to PGPLOTLIB. # # 5) CFITSIO is Bill Pence's FITS I/O library written in C with Fortran # wrappers, available from http://heasarc.gsfc.nasa.gov/fitsio. # # CFITSIO is required by three utilities, HPXcvt, wcsgrid, and wcsware, # and also by the test programs twcstab and twcshdr. wcsware and the # test programs use fits_read_wcstab() which is implemented by # getwcstab.c. However, this implementation is included in CFITSIO post # 3.004beta, so getwcstab.c is required here only for older releases # (controlled by variable GETWCSTAB). getwcstab.o itself is not inserted # into the WCSLIB object library. # # If available, CFITSIO is also optionally used for test programs # tfitshdr, tbth1, tpih1 and tpih2 by setting preprocessor macro # -DDO_CFITSIO. # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: makedefs.in,v 4.10 2012/02/05 23:41:45 cal103 Exp $ #----------------------------------------------------------------------------- # Version. LIBVER := @LIBVER@ WCSLIBPKG := wcslib-@PACKAGE_VERSION@ # System architecture. ARCH := @ARCH@ # Flex and options. FLEX := @FLEX@ FLFLAGS := # C preprocessor and options. CPP := @CPP@ CPPFLAGS := @DEFS@ WCSTRIG := WRAPPER # C compiler and options. CC := @CC@ CFLAGS := @CFLAGS@ # Fortran compiler and options. FC := @F77@ FFLAGS := @FFLAGS@ # Static object library. WCSLIB := libwcs-$(LIBVER).a RANLIB := @RANLIB@ # Shared (dynamic) library (see note 3 above). SHRLIB := @SHRLIB@ SONAME := @SONAME@ SHRFLAGS := @SHRFLAGS@ SHRLD := @SHRLD@ SHRLN := @SHRLN@ # What subdirectories to build. SUBDIRS := @SUBDIRS@ TSTDIRS := @TSTDIRS@ # Top of the 'make install' hierarchy: pgsbox -> Fortran -> C. INSTDIR := @INSTDIR@ # Installation utilities and locations. LN_S := @LN_S@ INSTALL := @INSTALL@ # Needed for the definitions provided by autoconf. prefix := @prefix@ exec_prefix := @exec_prefix@ datarootdir := @datarootdir@ PACKAGE_TARNAME := @PACKAGE_TARNAME@ docdir := @docdir@ LIBDIR := $(DESTDIR)@libdir@ BINDIR := $(DESTDIR)@bindir@ INCDIR := $(DESTDIR)@includedir@/wcslib-$(LIBVER) INCLINK := $(DESTDIR)@includedir@/wcslib DOCDIR := $(DESTDIR)@docdir@ HTMLDIR := $(DESTDIR)@htmldir@ PDFDIR := $(DESTDIR)@pdfdir@ MANDIR := $(DESTDIR)@mandir@ # For putting timestamps in the build log. TIMER := date +"%a %Y/%m/%d %X %z, executing on $$HOST" # The remaining options are for building utilities and test programs. # ------------------------------------------------------------------- # Linker options (use CC for linking). LD = $(CC) LDFLAGS := @LDFLAGS@ # PGPLOT (see note 4 above). PGPLOTINC := @PGPLOTINC@ PGPLOTLIB := @PGPLOTLIB@ # CFITSIO (see note 5 above). CFITSIOINC := @CFITSIOINC@ CFITSIOLIB := @CFITSIOLIB@ GETWCSTAB := @GETWCSTAB@ # Libraries required by the above Fortran compiler. FLIBS := @FLIBS@ # Libraries required by WCSLIB itself. LIBS := @LIBS@ #----------------------------------------------------------------------------- # You shouldn't need to change anything below here. #----------------------------------------------------------------------------- SHELL := /bin/sh VPATH := .. # Common targets. .PHONY : all build printenv show all : show build # Print the environment as seen by makefile rules. printenv : -@ printenv | sort # Print variable definitions. show :: wcsconfig.h -@ echo '' -@ uname -a -@ echo '' -@ $(MAKE) --version | head -1 -@ echo ' MAKEFLAGS := $(MAKEFLAGS)' -@ echo '' -@ echo 'For building and installing $(WCSLIBPKG)...' -@ echo ' ARCH := $(ARCH)' -@ echo ' FLEX := $(FLEX)' -@ echo ' FLFLAGS := $(FLFLAGS)' -@ echo ' CPP := $(CPP)' -@ echo ' CPPFLAGS := $(CPPFLAGS)' -@ echo ' WCSTRIG := $(WCSTRIG)' -@ echo ' CC := $(CC)' -@ echo ' CFLAGS := $(CFLAGS)' -@ echo ' FC := $(FC)' -@ echo ' FFLAGS := $(FFLAGS)' -@ echo ' WCSLIB := $(WCSLIB)' -@ echo ' RANLIB := $(RANLIB)' -@ echo ' SHRLIB := $(SHRLIB)' -@ echo ' SONAME := $(SONAME)' -@ echo ' SHRFLAGS := $(SHRFLAGS)' -@ echo ' SHRLD := $(SHRLD)' -@ echo ' SHRLN := $(SHRLN)' -@ echo ' LN_S := $(LN_S)' -@ echo ' INSTALL := $(INSTALL)' -@ echo ' LIBDIR := $(LIBDIR)' -@ echo ' BINDIR := $(BINDIR)' -@ echo ' INCDIR := $(INCDIR)' -@ echo ' INCLINK := $(INCLINK)' -@ echo ' DOCDIR := $(DOCDIR)' -@ echo ' HTMLDIR := $(HTMLDIR)' -@ echo ' PDFDIR := $(PDFDIR)' -@ echo ' MANDIR := $(MANDIR)' -@ echo ' TIMER := $(TIMER)' -@ echo '' -@ echo 'Important wcsconfig.h defines...' -@ echo " `grep HAVE_SINCOS $<`" -@ echo " `grep WCSLIB_INT64 $<`" -@ echo '' -@ echo 'To build utilities and test programs...' -@ echo ' LD := $(LD)' -@ echo ' LDFLAGS := $(LDFLAGS)' -@ echo ' PGPLOTINC := $(PGPLOTINC)' -@ echo ' PGPLOTLIB := $(PGPLOTLIB)' -@ echo ' CFITSIOINC := $(CFITSIOINC)' -@ echo ' CFITSIOLIB := $(CFITSIOLIB)' -@ echo ' GETWCSTAB := $(GETWCSTAB)' -@ echo ' FLIBS := $(FLIBS)' -@ echo ' LIBS := $(LIBS)' -@ echo '' # Code development overrides, for use in the code subdirectories. -include ../flavours pywcs-1.12/wcslib/pgsbox/0000755001153600020070000000000012310355732017431 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/pgsbox/cpgsbox.c0000644001153600020070000001031212310355626021241 0ustar cslocumSTSCI\science00000000000000/*============================================================================ PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. Copyright (C) 1997-2012, Mark Calabretta This file is part of PGSBOX. PGSBOX is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. PGSBOX is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with PGSBOX. If not, see . Correspondence concerning PGSBOX may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: cpgsbox.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *===========================================================================*/ #include #include "cpgsbox.h" /* Fortran name mangling. */ #include #define pgsbok_ F77_FUNC(pgsbok, PGSBOK) #define pglbok_ F77_FUNC(pglbok, PGLBOK) void pgsbok_(const float blc[2], const float trc[2], char idents[3][80], const char opt[2], const int *labctl, const int *labden, const int ci[7], const int gcode[2], const double *tiklen, const int *ng1, const double *grid1, const int *ng2, const double *grid2, const int *doeq, nlfunc_t nlfunc, const int *nlc, const int *nli, const int *nld, char *nlcprm, int *nliprm, double *nldprm, const int *nc, int *ic, double cache[][4], int *ierr); void pglbok_(char idents[3][80], const char opt[2], const int *labctl, const int *labden, const int ci[7], const int gcode[2], const double *tiklen, const int *ng1, const double *grid1, const int *ng2, const double *grid2, const int *doeq, const int *nc, int *ic, double cache[][4], int *ierr); void cpgsbox( const float blc[2], const float trc[2], char (*idents)[80], const char opt[2], int labctl, int labden, const int ci[7], const int gcode[2], double tiklen, int ng1, const double *grid1, int ng2, const double *grid2, int doeq, nlfunc_t nlfunc, int nlc, int nli, int nld, char nlcprm[], int nliprm[], double nldprm[], int nc, int *ic, double cache[][4], int *ierr) { char ids[3][80]; int j, k; /* Convert variable length strings to fixed-length char arrays. */ k = 0; for (j = 0; j < 3; j++) { if (strlen(idents[j]) > 80) { strncpy(ids[j], idents[j], 80); } else { strcpy(ids[j], idents[j]); for (k = strlen(idents[j]); k < 80; k++) { ids[j][k] = ' '; } } } pgsbok_(blc, trc, ids, opt, &labctl, &labden, ci, gcode, &tiklen, &ng1, grid1, &ng2, grid2, &doeq, nlfunc, &nlc, &nli, &nld, nlcprm, nliprm, nldprm, &nc, ic, cache, ierr); return; } /*==========================================================================*/ void cpglbox( char (*idents)[80], const char opt[2], int labctl, int labden, const int ci[7], const int gcode[2], double tiklen, int ng1, const double *grid1, int ng2, const double *grid2, int doeq, int nc, int *ic, double cache[][4], int *ierr) { char ids[3][80]; int j, k; /* Convert variable length strings to fixed-length char arrays. */ k = 0; for (j = 0; j < 3; j++) { if (strlen(idents[j]) > 80) { strncpy(ids[j], idents[j], 80); } else { strcpy(ids[j], idents[j]); for (k = strlen(idents[j]); k < 80; k++) { ids[j][k] = ' '; } } } pglbok_(ids, opt, &labctl, &labden, ci, gcode, &tiklen, &ng1, grid1, &ng2, grid2, &doeq, &nc, ic, cache, ierr); return; } pywcs-1.12/wcslib/pgsbox/cpgsbox.h0000644001153600020070000000675312310355626021264 0ustar cslocumSTSCI\science00000000000000/*============================================================================ PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. Copyright (C) 1997-2012, Mark Calabretta This file is part of PGSBOX. PGSBOX is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. PGSBOX is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with PGSBOX. If not, see . Correspondence concerning PGSBOX may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: cpgsbox.h,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * * cpgsbox() and cpglbox() are C wrappers for PGSBOX and PGLBOX. Refer to the * prologue of pgsbox.f for an explanation of the argument list and usage * notes. * * The argument lists for cpgsbox()/cpglbox() differ from PGSBOX/PGLBOX in * the following respects: * * idents char[3][80] * Fixed length character array. * opt char[2] Fixed length character array. * nlfunc nlfunc_t typedef for external function defined in cpgsbox.h. * cache double[][4] * Array indices reversed. * * Note also that the array arguments to cpgsbox()/cpglbox() are all * 0-relative, while several of those of PGSBOX/PGLBOX are 0-relative (GRID1, * GRID2, and CACHE) with the remainder 1-relative. In particular, the two- * dimensional CACHE array has a mixture of 0-, and 1-relative indices, and * the indices are reversed in C because of the differing C and FORTRAN array * indexing policy. Moreover, as in PGSBOX/PGLBOX, nc is the upper array * index, not the array length, so the array should be dimensioned as * cache[nc+1][4]. * *===========================================================================*/ #ifndef PGSBOX_CPGSBOX #define PGSBOX_CPGSBOX #ifdef __cplusplus extern "C" { #endif typedef void nlfunc_t(int *, int *, int *, int *, char *, int *, double *, double *, double *, int *, double *, int *); void cpgsbox( const float blc[2], const float trc[2], char (*idents)[80], const char opt[2], int labctl, int labden, const int ci[7], const int gcode[2], double tiklen, int ng1, const double *grid1, int ng2, const double *grid2, int doeq, nlfunc_t nlfunc, int nlc, int nli, int nld, char nlcprm[], int nliprm[], double nldprm[], int nc, int *ic, double cache[][4], int *ierr); void cpglbox( char (*idents)[80], const char opt[2], int labctl, int labden, const int ci[7], const int gcode[2], double tiklen, int ng1, const double *grid1, int ng2, const double *grid2, int doeq, int nc, int *ic, double cache[][4], int *ierr); #ifdef __cplusplus } #endif #endif /* PGSBOX_CPGSBOX */ pywcs-1.12/wcslib/pgsbox/cpgtest.c0000644001153600020070000011416212310355626021255 0ustar cslocumSTSCI\science00000000000000/*============================================================================ PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. Copyright (C) 1997-2012, Mark Calabretta This file is part of PGSBOX. PGSBOX is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. PGSBOX is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with PGSBOX. If not, see . Correspondence concerning PGSBOX may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: cpgtest.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * * cpgtest * *---------------------------------------------------------------------------*/ #include #include #include #include #include #include #include /* Fortran name mangling. */ #include #define lngvel_ F77_FUNC(lngvel, LNGVEL) #define fscan_ F77_FUNC(fscan, FSCAN) #define pgcrfn_ F77_FUNC(pgcrfn, PGCRFN) #define pgwcsl_ F77_FUNC(pgwcsl, PGWCSL) int main() { const double pi = 3.141592653589793238462643; const double d2r = pi/180.0; char devtyp[16], fcode[2][4], idents[3][80], nlcprm[1], opt[2]; int c0[7], ci[7], gcode[2], ic, ierr, j, large, naxis[2], nliprm[2], status; float blc[2], scl, trc[2]; double cache[257][4], dec0, grid1[9], grid2[9], nldprm[8], rotn, tiklen; struct wcsprm wcs; nlfunc_t lngvel_, fscan_, pgcrfn_, pgwcsl_; /* Setup. */ naxis[0] = 512; naxis[1] = 512; blc[0] = 0.5f; blc[1] = 0.5f; trc[0] = naxis[0] + 0.5f; trc[1] = naxis[1] + 0.5f; strcpy(devtyp, "/XWINDOW"); cpgbeg(0, devtyp, 1, 1); j = 16; cpgqinf("TYPE", devtyp, &j); if (strcmp(devtyp, "PS") == 0 || strcmp(devtyp, "VPS") == 0 || strcmp(devtyp, "CPS") == 0 || strcmp(devtyp, "VCPS") == 0) { /* Switch black and white. */ cpgscr(0, 1.0f, 1.0f, 1.0f); cpgscr(1, 0.0f, 0.0f, 0.0f); } large = strcmp(devtyp, "XWINDOW") == 0; if (large) { scl = 1.0f; cpgvstd(); } else { scl = 0.7f; cpgvsiz(1.0f, 3.0f, 1.0f, 3.0f); } /* Yellow. */ cpgscr(2, 1.0f, 1.0f, 0.0f); /* White. */ cpgscr(3, 1.0f, 1.0f, 1.0f); /* Pale blue. */ cpgscr(4, 0.5f, 0.5f, 0.8f); /* Pale red. */ cpgscr(5, 0.8f, 0.5f, 0.5f); /* Grey. */ cpgscr(6, 0.7f, 0.7f, 0.7f); /* Dark green. */ cpgscr(7, 0.3f, 0.5f, 0.3f); c0[0] = -1; c0[1] = -1; c0[2] = -1; c0[3] = -1; c0[4] = -1; c0[5] = -1; c0[6] = -1; cpgwnad(0.0f, 1.0f, 0.0f, 1.0f); cpgask(1); cpgpage(); wcs.flag = -1; /*-------------------------------------------------------------------------- * Longitude-velocity map; the y-axis is regularly spaced in frequency but is * to be labelled as a true relativistic velocity. * - PGSBOX uses subroutine LNGVEL. * - Separable (i.e. orthogonal), non-linear coordinate system. * - Automatic choice of coordinate increments. * - Extraction of a common scaling factor. * - Automatic choice of what edges to label. * - Request for tickmarks (internal) for one coordinate and grid lines * for the other. * - Simple two-colour grid using two calls with deferred labelling on * the first call. * - Degree labelling. * - Suppression of zero arcmin and arcsec fields in sexagesimal degree * format. *------------------------------------------------------------------------*/ printf("\nLongitude-velocity map\n"); /* Reference pixel coordinates. */ nldprm[0] = 1.0; nldprm[1] = 256.0; /* Reference pixel values. */ nldprm[2] = 0.0; nldprm[3] = 1.420e9; /* Coordinate increments. */ nldprm[4] = 360.0/(naxis[0]-1); nldprm[5] = 4e6; /* Rest frequency. */ nldprm[6] = 1.420e9; /* Annotation. */ strcpy(idents[0], "galactic longitude"); strcpy(idents[1], "velocity (m/s)"); strcpy(idents[2], "HI line"); opt[0] = 'F'; opt[1] = ' '; /* Normal size lettering. */ cpgsch(1.0f*scl); /* Yellow tick marks for longitude and grid lines for velocity. */ cpgsci(2); gcode[0] = 1; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; /* Defer labelling. */ ic = -1; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, lngvel_, 1, 1, 7, nlcprm, nliprm, nldprm, 256, &ic, cache, &ierr); /* Draw fiducial grid lines in white and do labelling. */ cpgsci(1); gcode[0] = 2; gcode[1] = 2; grid1[1] = 180.0; grid2[1] = 0.0; cpgsbox(blc, trc, idents, opt, 0, 0, c0, gcode, 0.0, 1, grid1, 1, grid2, 0, lngvel_, 1, 1, 7, nlcprm, nliprm, nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Azimuth-frequency scan; this sort of output might be obtained from an * antenna that scans in azimuth with a receiver that scans simultaneously * in frequency. * - PGSBOX uses subroutine FSCAN. * - Non-separable (i.e. non-orthogonal) non-linear coordinate system. * - Automatic choice of what edges to label; results in labelling the * bottom, left and right sides of the plot. * - Cyclic labelling. FSCAN returns the azimuth in the range * 0 - 720 degrees but PGSBOX is set to normalize this to two cycles of * 0 - 360 degrees. * - Logarithmic labelling. * - Automatic choice of coordinate increments but with request for all * grid lines for the logarithmic coordinate. * - Degree labelling. * - Suppression of common zero arcmin and arcsec fields in sexagesimal * degree format. *------------------------------------------------------------------------*/ printf("\nAzimuth-frequency scan\n"); /* Reference pixel coordinates. */ nldprm[0] = 0.5; nldprm[1] = 0.5; /* Reference pixel values. */ nldprm[2] = 0.0; nldprm[3] = 8.5; /* Coordinate increments. */ nldprm[4] = 720.0/(naxis[0]+1); nldprm[5] = 0.002; /* Rate of change of NLDPRM[3] with x-pixel. */ nldprm[6] = -0.002; /* Annotation. */ strcpy(idents[0], "azimuth"); strcpy(idents[1], "\\gn/Hz"); strcpy(idents[2], "Frequency/azimuth scan"); opt[0] = 'D'; opt[1] = 'L'; /* Normal size lettering. */ cpgsch(1.0f*scl); /* Draw full grid lines. */ cpgsci(1); gcode[0] = 2; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; /* Setting labden = 9900 forces all logarithmic grid lines to be drawn. */ ic = -1; cpgsbox(blc, trc, idents, opt, 0, 9900, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, fscan_, 1, 1, 7, nlcprm, nliprm, nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Z versus time plot. * - PGSBOX uses subroutine PGCRFN. * - Separable (i.e. orthogonal), non-linear coordinate system. * - Use of function PGCRFN for separable axis types. * - Automatic choice of what edges to label; results in labelling the * bottom and left sides of the plot. * - Automatic choice of coordinate increments. * - Logarithmic labelling over many orders of magnitude. * - Single-character annotation on a vertical axis is upright. *------------------------------------------------------------------------*/ printf("\nZ versus time plot\n"); /* Function types. */ strncpy(fcode[0], "Lin ", 4); strncpy(fcode[1], "Log ", 4); /* Reference pixel coordinates. */ nldprm[0] = 0.5; nldprm[1] = -50.0; /* Coordinate increments. */ nldprm[2] = 0.04; nldprm[3] = 0.02; /* Reference pixel values. */ nldprm[4] = -3.0; nldprm[5] = 1.0; /* Annotation. */ strcpy(idents[0], "Age of universe (sec)"); strcpy(idents[1], "Y"); strcpy(idents[2], ""); opt[0] = 'L'; opt[1] = ' '; /* Normal size lettering. */ cpgsch(1.0f*scl); /* Draw ticks for the first coordinate, grid lines for the second. */ cpgsci(1); gcode[0] = 1; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; ic = -1; cpgsbox(blc, trc, idents, opt, 0, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, pgcrfn_, 8, 2, 4, fcode[0], nliprm, nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Simple SIN projection near the south celestial pole. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate system. * - Demonstrate parameter definition for PGWCSL. * - Discovery of grid lines that do not cross any axis. * - Automatic choice of what edges to label; results in labelling all * sides of the plot. * - Automatic choice of coordinate increments but with request for * increased grid density for each coordinate. * - Double precision accuracy. * - Cyclic coordinates. PGWCSL returns the right ascension in the range * -180 to +180 degrees, i.e. with a discontinuity at +/- 180 degrees. * - Labelling of degrees as time in the range 0 - 24h. * - Suppression of labels that would overlap one another. * - Sexagesimal degree labelling with automatically determined * precision. * - Suppression of common zero minute and second fields in sexagesimal * time format. *------------------------------------------------------------------------*/ printf("\nSimple SIN projection\n"); wcs.flag = -1; status = wcsini(1, 2, &wcs); /* Set projection type to SIN. */ strcpy(wcs.ctype[0], "RA---SIN"); strcpy(wcs.ctype[1], "DEC--SIN"); /* Reference pixel coordinates. */ wcs.crpix[0] = 384.0; wcs.crpix[1] = 256.0; /* Coordinate increments. */ wcs.cdelt[0] = -1.0/3600000.0; wcs.cdelt[1] = 1.0/3600000.0; /* Spherical coordinate references. */ dec0 = -89.99995; wcs.crval[0] = 25.0; wcs.crval[1] = dec0; /* Set parameters for an NCP projection. */ dec0 *= d2r; wcs.pv[0].i = 2; wcs.pv[0].m = 1; wcs.pv[0].value = 0.0; wcs.pv[0].i = 2; wcs.pv[1].m = 2; wcs.pv[1].value = cos(dec0)/sin(dec0); /* Annotation. */ strcpy(idents[0], "Right ascension"); strcpy(idents[1], "Declination"); strcpy(idents[2], "WCS SIN projection"); opt[0] = 'G'; opt[1] = 'E'; /* Compact lettering. */ cpgsch(0.8f*scl); /* Draw full grid lines. */ cpgsci(1); gcode[0] = 2; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; /* Draw the celestial grid. The grid density is set for each world */ /* coordinate by specifying LABDEN = 1224. */ ic = -1; cpgsbox(blc, trc, idents, opt, 0, 1224, c0, gcode, 0.0, 0, grid1, 0, grid2, 0, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*------------------------------------------------------------------------- * Conic equal area projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate system. * - Coordinate system undefined in areas of the plot. * - Demonstrate parameter definition for PGWCSL. * - Discontinuous grid lines handled by PGWCSL. * - Discovery of grid lines that do not cross any axis. * - Colour control for grid and labelling. * - Reduced size lettering. * - Automatic choice of what edges to label; results in labelling all * sides of the plot. * - Automatic choice of coordinate increments. * - Cyclic coordinates. PGWCSL returns the longitude in the range -180 * to +180 degrees, i.e. with a discontinuity at +/- 180 degrees. * - Suppression of labels that would overlap one another. * - Suppression of common zero arcmin and arcsec fields in sexagesimal * degree format. *------------------------------------------------------------------------*/ printf("\nConic equal area projection\n"); status = wcsini(1, 2, &wcs); /* Set projection type to conic equal-area. */ strcpy(wcs.ctype[0], "RA---COE"); strcpy(wcs.ctype[1], "DEC--COE"); /* Reference pixel coordinates. */ wcs.crpix[0] = 256.0; wcs.crpix[1] = 256.0; /* Coordinate increments. */ wcs.cdelt[0] = -1.0/3.0; wcs.cdelt[1] = 1.0/3.0; /* Spherical coordinate references. */ wcs.crval[0] = 90.0; wcs.crval[1] = 30.0; wcs.lonpole = 150.0; /* Middle latitude and offset from standard parallels. */ wcs.npv = 2; wcs.pv[0].i = 2; wcs.pv[0].m = 1; wcs.pv[0].value = 60.0; wcs.pv[1].i = 2; wcs.pv[1].m = 2; wcs.pv[1].value = 15.0; /* Annotation. */ strcpy(idents[0], "longitude"); strcpy(idents[1], "latitude"); strcpy(idents[2], "WCS conic equal area projection"); opt[0] = 'E'; opt[1] = 'E'; /* Reduced size lettering. */ cpgsch(0.8f*scl); /* Draw full grid lines. */ gcode[0] = 2; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; /* Use colour to associate grid lines and labels. */ /* Meridians in red. */ cpgscr(10, 0.5f, 0.0f, 0.0f); /* Parallels in blue. */ cpgscr(11, 0.0f, 0.2f, 0.5f); /* Longitudes in red. */ cpgscr(12, 0.8f, 0.3f, 0.0f); /* Latitudes in blue. */ cpgscr(13, 0.0f, 0.4f, 0.7f); /* Longitude labels in red. */ cpgscr(14, 0.8f, 0.3f, 0.0f); /* Latitude labels in blue. */ cpgscr(15, 0.0f, 0.4f, 0.7f); /* Title in cyan. */ cpgscr(16, 0.3f, 1.0f, 1.0f); ci[0] = 10; ci[1] = 11; ci[2] = 12; ci[3] = 13; ci[4] = 14; ci[5] = 15; ci[6] = 16; /* Draw the celestial grid letting PGSBOX choose the increments. */ ic = -1; cpgsbox(blc, trc, idents, opt, 0, 0, ci, gcode, 0.0, 0, grid1, 0, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Set parameters to draw the native grid. */ wcs.crval[0] = 0.0; wcs.crval[1] = 60.0; wcs.lonpole = 999.0; wcs.latpole = 999.0; status = wcsset(&wcs); /* We just want to delineate the boundary, in green. */ cpgsci(7); grid1[1] = -180.0; grid1[2] = 180.0; grid2[1] = -90.0; grid2[2] = 90.0; ic = -1; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 2, grid1, 2, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgsci(1); cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Polyconic projection with colour-coded grid. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate system. * - Coordinate system undefined in areas of the plot. * - Demonstrate parameter definition for PGWCSL. * - Discontinuous grid lines handled by PGWCSL. * - Colour coded labelling. * - Colour coded grid implemented by the caller. * - Basic management of the axis-crossing table (see code). * - Reduced size lettering. * - Tick marks external to the frame. * - User selection of what edges to label with request for both * coordinates to be labelled on bottom, left and top edges. * - User selection of grid lines to plot. * - Concatenation of annotation at bottom and left; automatically * suppressed at the top since only one coordinate is labelled there. * - Suppression of labels that would overlap one another. * - Degree labelling. * - Labelling of degrees as time in the range -12 - +12h. * - Suppression of common zero minute and second fields in sexagesimal * time format. *------------------------------------------------------------------------*/ printf("\nPolyconic projection with colour-coded grid\n"); status = wcsini(1, 2, &wcs); /* Set projection type to polyconic. */ strcpy(wcs.ctype[0], "RA---PCO"); strcpy(wcs.ctype[1], "DEC--PCO"); /* Reference pixel coordinates. */ wcs.crpix[0] = 192.0; wcs.crpix[1] = 640.0; /* Rotate 30 degrees. */ rotn = 30.0*d2r; *(wcs.pc) = cos(rotn); *(wcs.pc+1) = sin(rotn); *(wcs.pc+2) = -sin(rotn); *(wcs.pc+3) = cos(rotn); /* Coordinate increments. */ wcs.cdelt[0] = -1.0/5.0; wcs.cdelt[1] = 1.0/5.0; /* Spherical coordinate references. */ wcs.crval[0] = 332.0; wcs.crval[1] = 40.0; wcs.lonpole = -30.0; /* Annotation. */ strcpy(idents[0], "Hour angle"); strcpy(idents[1], "Declination"); strcpy(idents[2], "WCS polyconic projection"); opt[0] = 'H'; opt[1] = 'B'; /* Reduced size lettering. */ cpgsch(0.9f*scl); /* Draw external (TIKLEN < 0) tick marks every 5 degrees. */ gcode[0] = 1; gcode[1] = 1; tiklen = -2.0; cpgsci(6); grid1[0] = 5.0; grid2[0] = 5.0; ic = -1; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, tiklen, 0, grid1, 0, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Resetting the table index to zero causes information about the */ /* tick marks to be discarded. */ ic = 0; /* Draw full grid lines in yellow rather than tick marks. */ cpgsci(2); gcode[0] = 2; gcode[1] = 2; /* Draw the primary meridian and equator. */ grid1[1] = 0.0; grid2[1] = 0.0; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 1, grid1, 1, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* At this point the axis-crossing table will have entries for the */ /* primary meridian and equator. Labelling was deferred in the */ /* previous call, and the table is passed intact on the second call */ /* to accumulate further axis-crossings. */ /* Draw 90 degree meridians and poles in white. */ cpgsci(3); grid1[1] = 90.0; grid1[2] = 180.0; grid1[3] = 270.0; grid2[1] = -90.0; grid2[2] = 90.0; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 3, grid1, 2, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the first set of 15 degree meridians and parallels in blue. */ cpgsci(4); grid1[1] = 15.0; grid1[2] = 60.0; grid1[3] = 105.0; grid1[4] = 150.0; grid1[5] = 195.0; grid1[6] = 240.0; grid1[7] = 285.0; grid1[8] = 330.0; grid2[1] = -75.0; grid2[2] = -30.0; grid2[3] = 15.0; grid2[4] = 60.0; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 8, grid1, 4, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the second set of 15 degree meridians and parallels in red. */ cpgsci(5); grid1[1] = 30.0; grid1[2] = 75.0; grid1[3] = 120.0; grid1[4] = 165.0; grid1[5] = 210.0; grid1[6] = 255.0; grid1[7] = 300.0; grid1[8] = 345.0; grid2[1] = -60.0; grid2[2] = -15.0; grid2[3] = 30.0; grid2[4] = 75.0; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 8, grid1, 4, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* The axis-crossing table has now accumulated information for all of */ /* the preceding meridians and parallels but no labels have been */ /* produced. It will acquire information for the the next set of */ /* meridians and parallels before being processed by this call to */ /* PGSBOX which finally produces the labels. */ /* Draw the 45 degree meridians and parallels in grey and use colour */ /* to differentiate grid labels. */ /* Meridians and parallels in grey. */ cpgscr(10, 0.7f, 0.7f, 0.7f); cpgscr(11, 0.7f, 0.7f, 0.7f); /* Longitudes tinged red. */ cpgscr(12, 1.0f, 0.9f, 0.6f); /* Latitudes tinged green. */ cpgscr(13, 0.8f, 1.0f, 0.9f); /* Longitude labels tinged red. */ cpgscr(14, 1.0f, 0.9f, 0.6f); /* Latitude labels tinged green. */ cpgscr(15, 0.8f, 1.0f, 0.9f); /* Title in white. */ cpgscr(16, 1.0f, 1.0f, 1.0f); ci[0] = 10; ci[1] = 11; ci[2] = 12; ci[3] = 13; ci[4] = 14; ci[5] = 15; ci[6] = 16; cpgsci(6); /* Tell PGSBOX what edges to label. */ grid1[1] = 45.0; grid1[2] = 135.0; grid1[3] = 225.0; grid1[4] = 315.0; grid2[1] = -45.0; grid2[2] = 45.0; cpgsbox(blc, trc, idents, opt, 2333, 0, ci, gcode, 0.0, 4, grid1, 2, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Native grid in green (delineates boundary). */ cpgsci(7); grid1[1] = -180.0; grid1[2] = 180.0; grid2[1] = -999.0; wcs.crval[0] = 0.0; wcs.crval[1] = 0.0; wcs.lonpole = 999.0; status = wcsset(&wcs); ic = -1; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 2, grid1, 1, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgsci(1); cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Plate Carree projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Rectangular image. * - Dual coordinate grids. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate system. * - Demonstrate parameter definition for PGWCSL. * - Discontinuous grid lines handled by PGWCSL. * - Colour coding of grid and labelling. * - Reduced size lettering. * - Manual labelling control. * - Manual and automatic choice of coordinate increments. * - Cyclic coordinates. PGWCSL returns the longitude in the range -180 * to +180 degrees, i.e. with a discontinuity at +/- 180 degrees. * - Suppression of labels that would overlap one another. *------------------------------------------------------------------------*/ printf("\nPlate Carree projection\n"); naxis[0] = 181; naxis[1] = 91; blc[0] = 0.5; blc[1] = 0.5; trc[0] = naxis[0] + 0.5; trc[1] = naxis[1] + 0.5; /* Reset viewport for rectangular image. */ if (large) { cpgvstd(); } else { cpgvsiz(1.0f, 3.0f, 1.0f, 3.0f); } cpgwnad(0.0f, 1.0f, 0.0f, ((float)naxis[1])/((float)naxis[0])); status = wcsini(1, 2, &wcs); /* Set projection type to plate carree. */ strcpy(wcs.ctype[0], "GLON-CAR"); strcpy(wcs.ctype[1], "GLAT-CAR"); /* Reference pixel coordinates. */ wcs.crpix[0] = 226.0; wcs.crpix[1] = 46.0; /* Linear transformation matrix. */ rotn = 15.0*d2r; *(wcs.pc) = cos(rotn); *(wcs.pc+1) = sin(rotn); *(wcs.pc+2) = -sin(rotn); *(wcs.pc+3) = cos(rotn); /* Coordinate increments. */ wcs.cdelt[0] = -1.0; wcs.cdelt[1] = 1.0; /* Set parameters to draw the native grid. */ wcs.crval[0] = 0.0; wcs.crval[1] = 0.0; /* The reference pixel was defined so that the native longitude runs */ /* from 225 deg to 45 deg and this will cause the grid to be truncated */ /* at the 180 deg boundary. However, being a cylindrical projection */ /* it is possible to recentre it in longitude. cylfix() will modify */ /* modify CRPIX, CRVAL, and LONPOLE to suit. */ status = cylfix(naxis, &wcs); /* Annotation. */ strcpy(idents[0], ""); strcpy(idents[1], ""); strcpy(idents[2], "WCS plate caree projection"); opt[0] = 'C'; opt[1] = 'C'; /* Reduced size lettering. */ cpgsch(0.8f*scl); /* Draw full grid lines. */ gcode[0] = 2; gcode[1] = 2; /* Draw native grid in green. */ cpgscr(16, 0.0f, 0.2f, 0.0f); /* Title in cyan. */ cpgscr(17, 0.3f, 1.0f, 1.0f); ci[0] = 16; ci[1] = 16; ci[2] = 7; ci[3] = 7; ci[4] = -1; ci[5] = -1; ci[6] = 17; grid1[0] = 15.0; grid2[0] = 15.0; ic = -1; cpgsbox(blc, trc, idents, opt, 2100, 0, ci, gcode, 0.0, 0, grid1, 0, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Reset CRPIX previously modified by cylfix(). */ wcs.crpix[0] = 226.0; wcs.crpix[1] = 46.0; /* Galactic reference coordinates. */ wcs.crval[0] = 30.0; wcs.crval[1] = 35.0; wcs.lonpole = 999.0; status = wcsset(&wcs); status = cylfix(naxis, &wcs); /* Annotation. */ strcpy(idents[0], "longitude"); strcpy(idents[1], "latitude"); strcpy(idents[2], ""); opt[0] = 'E'; opt[1] = 'E'; /* Use colour to associate grid lines and labels. */ /* Meridians in red. */ cpgscr(10, 0.5f, 0.0f, 0.0f); /* Parallels in blue. */ cpgscr(11, 0.0f, 0.2f, 0.5f); /* Longitudes in red. */ cpgscr(12, 0.8f, 0.3f, 0.0f); /* Latitudes in blue. */ cpgscr(13, 0.0f, 0.4f, 0.7f); /* Longitude labels in red. */ cpgscr(14, 0.8f, 0.3f, 0.0f); /* Latitude labels in blue. */ cpgscr(15, 0.0f, 0.4f, 0.7f); ci[0] = 10; ci[1] = 11; ci[2] = 12; ci[3] = 13; ci[4] = 14; ci[5] = 15; ci[6] = -1; grid1[0] = 0.0; grid2[0] = 0.0; /* Draw the celestial grid letting PGSBOX choose the increments. */ ic = -1; cpgsbox(blc, trc, idents, opt, 21, 0, ci, gcode, 0.0, 0, grid1, 0, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgsci(1); cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Plate Carree projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - BLC, TRC unrelated to pixel coordinates. * - Demonstrate parameter definition for PGWCSL. * - Poles and 180 meridian projected along edges of the frame. * - Reduced size lettering. * - Manual and automatic choice of coordinate increments. * - Suppression of common zero minute and second fields in sexagesimal * time format. *------------------------------------------------------------------------*/ printf("\nPlate Carree projection\n"); blc[0] = -180.0; blc[1] = -90.0; trc[0] = 180.0; trc[1] = +90.0; /* Reset viewport for rectangular image. */ if (large) { cpgvstd(); } else { cpgvsiz(1.0f, 3.0f, 1.0f, 3.0f); } cpgwnad (blc[0], trc[0], blc[1], trc[1]); status = wcsini(1, 2, &wcs); /* Set projection type to plate carree. */ strcpy(wcs.ctype[0], "RA---CAR"); strcpy(wcs.ctype[1], "DEC--CAR"); /* Reference pixel coordinates. */ wcs.crpix[0] = 0.0; wcs.crpix[1] = 0.0; /* Coordinate increments. */ wcs.cdelt[0] = -1.0; wcs.cdelt[1] = 1.0; /* Set parameters to draw the native grid. */ wcs.crval[0] = 0.0; wcs.crval[1] = 0.0; /* Annotation. */ strcpy(idents[0], "Right ascension"); strcpy(idents[1], "Declination"); strcpy(idents[2], "WCS plate caree projection"); opt[0] = 'G'; opt[1] = 'E'; /* Reduced size lettering. */ cpgsch(0.7f*scl); /* Draw full grid lines. */ gcode[0] = 2; gcode[1] = 2; cpgsci(1); grid1[0] = 0.0; grid2[0] = 0.0; ic = -1; cpgsbox(blc, trc, idents, opt, 2121, 1212, c0, gcode, 0.0, 0, grid1, 0, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Cylindrical perspective projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - BLC, TRC unrelated to pixel coordinates. * - Demonstrate parameter definition for PGWCSL. * - Reduced size lettering. * - Manual and automatic choice of coordinate increments. * - Suppression of common zero minute and second fields in sexagesimal * time format. *------------------------------------------------------------------------*/ printf("\nCylindrical perspective projection\n"); blc[0] = -180.0; blc[1] = -90.0; trc[0] = 180.0; trc[1] = +90.0; /* Reset viewport for rectangular image. */ if (large) { cpgvstd(); } else { cpgvsiz(1.0f, 3.0f, 1.0f, 3.0f); } cpgwnad (blc[0], trc[0], blc[1], trc[1]); status = wcsini(1, 2, &wcs); /* Set projection type to cylindrical perspective. */ strcpy(wcs.ctype[0], "RA---CYP"); strcpy(wcs.ctype[1], "DEC--CYP"); /* Reference pixel coordinates. */ wcs.crpix[0] = 0.0; wcs.crpix[1] = 0.0; /* Coordinate increments. */ wcs.cdelt[0] = -1.0; wcs.cdelt[1] = 1.0; /* Set parameters to draw the native grid. */ wcs.crval[0] = 45.0; wcs.crval[1] = -90.0; wcs.lonpole = 999.0; /* mu and lambda projection parameters. */ wcs.npv = 2; wcs.pv[0].i = 2; wcs.pv[0].m = 1; wcs.pv[0].value = 0.0; wcs.pv[1].i = 2; wcs.pv[1].m = 2; wcs.pv[1].value = 1.0; /* Annotation. */ strcpy(idents[0], "Right ascension"); strcpy(idents[1], "Declination"); strcpy(idents[2], "WCS cylindrical perspective projection"); opt[0] = 'G'; opt[1] = 'E'; /* Reduced size lettering. */ cpgsch(0.7f*scl); /* Draw full grid lines. */ gcode[0] = 2; gcode[1] = 2; cpgsci(1); grid1[0] = 0.0; grid2[0] = 0.0; ic = -1; cpgsbox(blc, trc, idents, opt, 2121, 1212, c0, gcode, 0.0, 0, grid1, 0, grid2, 1, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Gnomonic projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Demonstrate parameter definition for PGWCSL. * - Reduced size lettering. * - Manual and automatic choice of coordinate increments. * - Suppression of common zero minute and second fields in sexagesimal * time format. *------------------------------------------------------------------------*/ printf("\nTAN projection\n"); naxis[0] = 100; naxis[1] = 100; blc[0] = 0.5; blc[1] = 0.5; trc[0] = naxis[0] + 0.5; trc[1] = naxis[1] + 0.5; /* Reset viewport for rectangular image. */ if (large) { cpgvstd(); } else { cpgvsiz(1.0f, 3.0f, 1.0f, 3.0f); } cpgwnad(0.0f, 1.0f, 0.0f, ((float)naxis[1])/((float)naxis[0])); status = wcsini(1, 2, &wcs); /* Set projection type to gnomonic. */ strcpy(wcs.ctype[0], "RA---TAN"); strcpy(wcs.ctype[1], "DEC--TAN"); /* Reference pixel coordinates. */ wcs.crpix[0] = 50.5; wcs.crpix[1] = 1.0; /* Coordinate increments. */ wcs.cdelt[0] = 1e-3; wcs.cdelt[1] = 1e-3; /* Set parameters to draw the native grid. */ wcs.crval[0] = 45.0; wcs.crval[1] = -89.7; wcs.lonpole = 999.0; /* Annotation. */ strcpy(idents[0], "Right ascension"); strcpy(idents[1], "Declination"); strcpy(idents[2], "WCS TAN projection"); opt[0] = 'E'; opt[1] = 'E'; /* Reduced size lettering. */ cpgsch(0.7f*scl); /* Draw full grid lines. */ gcode[0] = 2; gcode[1] = 2; cpgsci(1); grid1[0] = 0.0; grid2[0] = 0.0; ic = -1; cpgsbox(blc, trc, idents, opt, 0, 1212, c0, gcode, 0.0, 0, grid1, 0, grid2, 0, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Linear-linear plot with two types of alternative labelling. * - PGSBOX uses subroutine PGCRFN. * - Separable (i.e. orthogonal), linear coordinate system. * - Use of function PGCRFN for separable axis types. * - Alternative labelling and axis annotation. * - Direct manipulation of the axis-crossing table. * - Tick mark and grid line control. * - User selection of what edges to label. * - Automatic choice of coordinate increments. *------------------------------------------------------------------------*/ printf("\nLinear plot with alternative labelling\n"); if (large) { cpgvstd(); } else { cpgvsiz(1.0f, 3.0f, 1.0f, 3.0f); } cpgwnad(0.0f, 1.0f, 0.0f, 1.0f); naxis[0] = 512; naxis[1] = 512; blc[0] = 0.5; blc[1] = 0.5; trc[0] = naxis[0] + 0.5; trc[1] = naxis[1] + 0.5; /* Function types. */ strncpy(fcode[0], "Lin ", 4); strncpy(fcode[1], "Lin ", 4); /* Reference pixel coordinates. */ nldprm[0] = 0.5; nldprm[1] = 0.5; /* Coordinate increments. */ nldprm[2] = 0.03; nldprm[3] = 0.03; /* Reference pixel values. */ nldprm[4] = 20.0; nldprm[5] = 0.0; /* Annotation. */ strcpy(idents[0], "temperature of frog (\\uo\\dC)"); strcpy(idents[1], "distance hopped (m)"); strcpy(idents[2], ""); opt[0] = ' '; opt[1] = ' '; /* Reduced size lettering. */ cpgsch(0.8f*scl); /* Draw tick marks at the bottom for the first coordinate, grid lines */ /* for the second. Setting GCODE[0] = -1 inhibits information being */ /* stored for labels on the top edge while GCODE[1] = 2 causes */ /* information to be stored for labels on the right edge even if those */ /* labels are not actually produced. */ cpgsci(1); gcode[0] = -1; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; /* Set LABCTL = 21 to label the bottom and left edges only. */ ic = -1; cpgsbox(blc, trc, idents, opt, 21, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, pgcrfn_, 8, 2, 4, fcode[0], nliprm, nldprm, 256, &ic, cache, &ierr); /* Information for labels on the right edge was stored in the crossing */ /* table on the first call to PGSBOX. We now want to manipulate it to */ /* convert metres to feet. Note that while it's a simple matter to draw */ /* alternative sets of tick marks on opposite edges of the frame, as */ /* with the two temperature scales, we have the slightly more difficult */ /* requirement of labelling grid lines with different values at each */ /* end. */ for (j = 0; j <= ic; j++) { /* Look for entries associated with the right edge of the frame. */ if (cache[j][0] == 4.0) { /* Convert to feet, rounding to the nearest 0.1. */ cache[j][3] *= 1e3/(25.4*12.0); cache[j][3] = floor(cache[j][3]*10.0 + 0.5)/10.0; } } /* Annotation for the right edge. */ strcpy(idents[0], ""); strcpy(idents[1], "(feet)"); /* Set LABCTL = 12000 to label the right edge with the second coordinate */ /* without redrawing the grid lines. */ cpgsbox(blc, trc, idents, opt, 12000, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, pgcrfn_, 8, 2, 4, fcode[0], nliprm, nldprm, 256, &ic, cache, &ierr); /* The alternative temperature scale in Fahrenheit is to be constructed */ /* with a new set of tick marks. */ nldprm[2] = nldprm[2]*1.8; nldprm[4] = nldprm[4]*1.8 + 32.0; /* Draw tick marks at the top for the first coordinate, don't redo grid */ /* lines for the second. */ gcode[0] = -100; gcode[1] = 0; /* Annotation for the top edge. */ strcpy(idents[0], "(\\uo\\dF)"); strcpy(idents[1], ""); /* Set LABCTL = 100 to label the top edge; Set IC = -1 to redetermine */ /* the coordinate extrema. */ ic = -1; cpgsbox(blc, trc, idents, opt, 100, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, pgcrfn_, 8, 2, 4, fcode[0], nliprm, nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("bc", 0.0f, 0, "bc", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Calendar axes using subroutine PGLBOX. * - Separable (i.e. orthogonal), linear coordinate system. * - Use of PGLBOX for simple linear axis types. * - Automatic choice of what edges to label; results in labelling the * bottom and left sides of the plot. * - Automatic choice of coordinate increments. * - Calendar date axis labelling. * - Single-character annotation on a vertical axis is upright. *------------------------------------------------------------------------*/ printf("\nCalendar axes using subroutine PGLBOX\n"); cpgswin(51900.0f, 52412.0f, 51900.0f, 57020.0f); /* Annotation. */ strcpy(idents[0], "Date started"); strcpy(idents[1], "Date finished"); strcpy(idents[2], "Calendar axes using subroutine PGLBOX"); opt[0] = 'Y'; opt[1] = 'Y'; /* Reduced size lettering. */ cpgsch(0.7f*scl); /* Draw tick marks on each axis. */ cpgsci(1); gcode[0] = 1; gcode[1] = 1; grid1[0] = 0.0; grid2[0] = 0.0; ic = -1; cpglbox(idents, opt, 0, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*-------------------------------------------------------------------------- * Simple linear axes handled by PGWCSL. * - Separable (i.e. orthogonal), linear coordinate system. * - Automatic choice of what edges to label; results in labelling the * bottom and left sides of the plot. * - Automatic choice of coordinate increments. * - Tick marks and labels at the edges of the frame. * - Single-character annotation on a vertical axis is upright. *------------------------------------------------------------------------*/ printf("\nSimple linear axes handled by pgwcsl()\n"); naxis[0] = 3; naxis[1] = 3; blc[0] = 0.5; blc[1] = 0.5; trc[0] = naxis[0] + 0.5; trc[1] = naxis[1] + 0.5; status = wcsini(1, 2, &wcs); strcpy(wcs.ctype[0], "x"); strcpy(wcs.ctype[1], "y"); /* Reference pixel coordinates. */ wcs.crpix[0] = 2.0; wcs.crpix[1] = 2.0; /* Coordinate increments. */ wcs.cdelt[0] = 1.0; wcs.cdelt[1] = 1.0; /* Spherical coordinate references. */ wcs.crval[0] = 2.0; wcs.crval[1] = 2.0; /* Annotation. */ strcpy(idents[0], "X"); strcpy(idents[1], "Y"); strcpy(idents[2], "Simple linear axes handled by pgwcsl()"); opt[0] = ' '; opt[1] = ' '; /* Reduced size lettering. */ cpgsch(0.8f*scl); /* Draw full grid lines. */ cpgsci(1); gcode[0] = 1; gcode[1] = 1; grid1[0] = 0.0; grid2[0] = 0.0; ic = -1; cpgsbox(blc, trc, idents, opt, 0, 0, c0, gcode, 2.0, 0, grid1, 0, grid2, 0, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(&wcs), nldprm, 256, &ic, cache, &ierr); /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); cpgpage(); /*------------------------------------------------------------------------*/ wcsfree(&wcs); cpgask(0); cpgend(); return 0; } pywcs-1.12/wcslib/pgsbox/fscan.f0000644001153600020070000001155312310355626020701 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. * Copyright (C) 1997-2012, Mark Calabretta * * This file is part of PGSBOX. * * PGSBOX is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * PGSBOX is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with PGSBOX. If not, see http://www.gnu.org/licenses. * * Correspondence concerning PGSBOX may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: fscan.f,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *======================================================================= * * FSCAN defines an azimuth/frequency coordinate system for PGSBOX. * * Given: * OPCODE I Transformation code: * +2: Compute a set of pixel coordinates that * describe a path between this and the * previous pair of world coordinates * remembered from the last call with * OPCODE = +1 or +2. * +1: Compute pixel coordinates from world * coordinates. * 0: Initialize. * -1: Compute world coordinates from pixel * coordinates. * * NLC I Number of elements in NLCPRM (=1). * * NLI I Number of elements in NLIPRM (=1). * * NLD I Number of elements in NLDPRM (=7). * * NLCPRM C(NLC)*1 Character array (ignored). * * NLIPRM I(NLI) Integer array (ignored). * * Given and/or returned: * NLDPRM D(NLD) Double precision coefficients (see below). * * WORLD D(2) World coordinates. WORLD(1) and WORLD(2) * are the longitude in degrees, and * log10(frequency/1Hz). * Given if OPCODE > 0, returned if OPCODE < 0. * * PIXEL D(2) Pixel coordinates. * Given if OPCODE < 0, returned if OPCODE > 0. * * CONTRL I Control flag for OPCODE = +2 (ignored, always * set to 0 on return). * * CONTXT D(20) Context elements (ignored). * * Returned: * IERR I Status return value: * 0: Success. * 1: Invalid coordinate transformation * parameters. * * Notes: * The NLDPRM array is constructed as follows: * - (1) Axis 1 reference pixel coordinate * - (2) Axis 2 reference pixel coordinate * - (3) Axis 1 reference pixel value (degree) * - (4) Axis 2 reference pixel value * - (5) Axis 1 coordinate increment (degree/pixel) * - (6) Axis 2 coordinate increment * - (7) Rate of change of NLDPRM(4) with x-pixel * *======================================================================= SUBROUTINE FSCAN (OPCODE, NLC, NLI, NLD, NLCPRM, NLIPRM, NLDPRM, : WORLD, PIXEL, CONTRL, CONTXT, IERR) *----------------------------------------------------------------------- INTEGER CONTRL, IERR, NLC, NLD, NLI, NLIPRM(NLI), OPCODE DOUBLE PRECISION CONTXT(20), NLDPRM(NLD), PIXEL(2), S, WORLD(2) CHARACTER NLCPRM(NLC)*1 *----------------------------------------------------------------------- IERR = 0 IF (OPCODE.GT.0) THEN * Compute pixel coordinates from world coordinates. PIXEL(1) = NLDPRM(1) + (WORLD(1) - NLDPRM(3))/NLDPRM(5) S = NLDPRM(4) + PIXEL(1)*NLDPRM(7) PIXEL(2) = NLDPRM(2) + (WORLD(2) - S)/NLDPRM(6) CONTRL = 0 ELSE IF (OPCODE.EQ.0) THEN * Initialize. IF (NLC.LT.1 .OR. NLI.LT.1 .OR. NLD.LT.7) IERR = 1 IF (NLDPRM(5).EQ.0D0) IERR = 1 IF (NLDPRM(6).EQ.0D0) IERR = 1 IF (NLDPRM(7).EQ.0D0) IERR = 1 CONTRL = 0 ELSE IF (OPCODE.EQ.-1) THEN * Compute world coordinates from pixel coordinates. WORLD(1) = NLDPRM(3) + NLDPRM(5)*(PIXEL(1) - NLDPRM(1)) WORLD(2) = NLDPRM(4) + NLDPRM(6)*(PIXEL(2) - NLDPRM(2)) + : PIXEL(1)*NLDPRM(7) ELSE IERR = 1 END IF RETURN END pywcs-1.12/wcslib/pgsbox/GNUmakefile0000644001153600020070000001343012310355626021506 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile for building PGSBOX 4.10 # # Summary of the main targets # --------------------------- # build: Build the library. # # clean: Delete intermediate object files. # # cleaner: clean, and also delete the test executables. # # cleanest (distclean, or realclean): cleaner, and also delete the pgsbox # and WCSLIB object libraries. # # check (or test): Compile and run the test programs. By default they are # executed in batch mode; use # # make MODE=interactive check # # to run them interactively. # # tests: Compile the test programs (but don't run them). # # Notes: # 1) If you need to make changes then preferably modify ../makedefs.in # instead and re-run configure. # # 2) In compiling the test programs, this makefile assumes that the # WCSLIB 4.10 sources reside in ../C and ../Fortran (as in the # distribution kit). # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: GNUmakefile,v 4.10 2012/02/05 23:41:45 cal103 Exp $ #----------------------------------------------------------------------------- # Get configure settings. include ../makedefs PGSBOXLIB := libpgsbox-$(LIBVER).a MODULES := pgsbox.o \ cpgsbox.o \ pgwcsl.o \ pgcrfn.o WCSLIB := ../C/$(WCSLIB) # For building the sharable library. PICLIB := libpgsbox-PIC.a WCSSHR := ../C/$(SHRLIB) SHRLIB := $(subst libwcs,libpgsbox,$(SHRLIB)) SONAME := $(subst libwcs,libpgsbox,$(SONAME)) SHRLD := $(subst libwcs,libpgsbox,$(SHRLD)) SHRLN := $(subst libwcs,libpgsbox,$(SHRLN)) CPPFLAGS += -I. -I.. -I../C vpath %.h ..:../C vpath %.in .. vpath %.inc ../Fortran # Pattern rules #-------------- $(PGSBOXLIB)(%.o) : %.f -@ echo '' $(FC) -I../Fortran $(FFLAGS) -c $< $(AR) r $(PGSBOXLIB) $% -@ $(RM) $% $(PGSBOXLIB)(%.o) : %.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) -c $< $(AR) r $(PGSBOXLIB) $% -@ $(RM) $% $(PICLIB)(%.o) : %.f -@ echo '' $(FC) -I../Fortran $(FFLAGS) $(SHRFLAGS) -c $< $(AR) r $(PICLIB) $% -@ $(RM) $% $(PICLIB)(%.o) : %.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) $(SHRFLAGS) -c $< $(AR) r $(PICLIB) $% -@ $(RM) $% %.i : %.c -@ echo '' -@ $(RM) $@ $(CPP) $(CPPFLAGS) $(CFLAGS) $< > $@ %.d : %.c -@ echo '' -@ $(CPP) $(CPPFLAGS) $(CFLAGS) $< | \ sed -n -e 's|^# 1 "\([^/].*\.h\)".*|\1|p' | \ sort -u # Static and static pattern rules #-------------------------------- .PHONY : build check clean cleaner cleanest distclean install realclean test \ tests wcslib build : lib lib : $(PGSBOXLIB) $(SHRLIB) $(PGSBOXLIB) : $(MODULES:%=$(PGSBOXLIB)(%)) -@ echo '' $(RANLIB) $@ $(SHRLIB) : $(PICLIB) -@ echo '' -@ $(RM) -r tmp - mkdir tmp && \ cd tmp && \ trap 'cd .. ; $(RM) -r tmp' 0 1 2 3 15 ; \ $(AR) x ../$(PICLIB) && \ $(SHRLD) -o $@ *.o ../$(WCSSHR) $(LDFLAGS) $(PGPLOTLIB) $(FLIBS) && \ mv $@ .. $(PICLIB) : $(MODULES:%.o=$(PICLIB)(%.o)) ; install : build $(MAKE) -C ../Fortran install $(INSTALL) -m 644 $(PGSBOXLIB) $(LIBDIR) $(RANLIB) $(LIBDIR)/$(PGSBOXLIB) $(RM) $(LIBDIR)/libpgsbox.a $(LN_S) $(PGSBOXLIB) $(LIBDIR)/libpgsbox.a - if [ "$(SHRLIB)" != "" ] ; then \ $(INSTALL) -m 644 $(SHRLIB) $(LIBDIR) ; \ if [ -h "$(LIBDIR)/$(SONAME)" ] ; then \ $(RM) $(LIBDIR)/$(SONAME) ; \ fi ; \ $(LN_S) $(SHRLIB) $(LIBDIR)/$(SONAME) ; \ if [ "$(SHRLN)" != "" ] ; then \ if [ -h "$(LIBDIR)/$(SHRLN)" ] ; then \ $(RM) $(LIBDIR)/$(SHRLN) ; \ fi ; \ $(LN_S) $(SONAME) $(LIBDIR)/$(SHRLN) ; \ fi ; \ fi $(INSTALL) -m 444 *.h $(INCDIR) clean : - $(RM) -r *.o *.i a.out core *.dSYM $(EXTRA_CLEAN) cleaner : clean - $(RM) pgtest cpgtest cleanest distclean realclean : cleaner - $(RM) $(PICLIB) libpgsbox-*.a libpgsbox.so.* libpgsbox.*.dylib check test : tests -@ echo '' -@ $(TIMER) -@ echo 'Running the PGSBOX test program, PGTEST:' -@ if [ '$(MODE)' = interactive ] ; then \ ./pgtest ; \ else \ ./pgtest < /dev/null ; \ fi -@ echo '' -@ echo '' -@ $(TIMER) -@ echo 'Running the cpgsbox() test program, cpgtest:' -@ if [ '$(MODE)' = interactive ] ; then \ ./cpgtest ; \ else \ ./cpgtest < /dev/null ; \ fi tests : wcslib pgtest cpgtest wcslib : $(WCSLIB) $(WCSLIB) : -@ echo '' $(MAKE) -C ../Fortran lib pgtest : pgtest.f fscan.f lngvel.f $(PGSBOXLIB) $(WCSLIB) -@ $(RM) $@ -@ echo '' $(FC) -I../Fortran $(FFLAGS) $(LDFLAGS) -o $@ $^ \ $(PGPLOTLIB) $(LIBS) cpgtest : cpgtest.c fscan.f lngvel.f $(PGSBOXLIB) $(WCSLIB) -@ $(RM) $@ -@ echo '' $(FC) -I../Fortran $(FFLAGS) -c fscan.f lngvel.f $(CC) $(CPPFLAGS) $(PGPLOTINC) $(CFLAGS) $(LDFLAGS) -o $@ \ $(^:.f=.o) $(PGPLOTLIB) $(FLIBS) $(LIBS) -@ $(RM) fscan.o lngvel.o GNUmakefile : ../makedefs ; ../makedefs ../wcsconfig_f77.h : makedefs.in wcsconfig_f77.h.in \ ../config.status -@ $(RM) ../wcsconfig_f77.h cd .. && ./config.status show :: -@ echo 'For building libpgsbox...' -@ echo ' PGSBOXLIB := $(PGSBOXLIB)' -@ echo ' PICLIB := $(PICLIB)' -@ echo ' WCSSHR := $(WCSSHR)' -@ echo ' SHRLIB := $(SHRLIB)' -@ echo ' SONAME := $(SONAME)' -@ echo ' SHRFLAGS := $(SHRFLAGS)' -@ echo ' SHRLD := $(SHRLD)' -@ echo ' SHRLN := $(SHRLN)' -@ echo '' -@ echo ' MODULES := $(MODULES)' # Dependencies #------------- $(PGSBOXLIB)(cpgsbox.o) : cpgsbox.h wcsconfig_f77.h $(PGSBOXLIB)(pgwcsl.o) : cel.h lin.h prj.h spc.h sph.h spx.h tab.h wcs.h \ wcsconfig_f77.h pgtest.o : wcs.inc cpgtest.o : cel.h cpgsbox.h lin.h prj.h spc.h spx.h tab.h wcs.h wcsfix.h \ wcsconfig_f77.h pywcs-1.12/wcslib/pgsbox/lngvel.f0000644001153600020070000001224512310355626021075 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. * Copyright (C) 1997-2012, Mark Calabretta * * This file is part of PGSBOX. * * PGSBOX is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * PGSBOX is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with PGSBOX. If not, see http://www.gnu.org/licenses. * * Correspondence concerning PGSBOX may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: lngvel.f,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *======================================================================= * * LNGVEL defines a longitude/velocity coordinate system for PGSBOX. * The second (Y) axis is assumed to be equispaced in frequency but * required to be labelled with the relativistic Doppler velocity. * * Given: * OPCODE I Transformation code: * +2: Compute a set of pixel coordinates that * describe a path between this and the * previous pair of world coordinates * remembered from the last call with * OPCODE = +1 or +2. * +1: Compute pixel coordinates from world * coordinates. * 0: Initialize. * -1: Compute world coordinates from pixel * coordinates. * * NLC I Number of elements in NLCPRM (=1). * * NLI I Number of elements in NLIPRM (=1). * * NLD I Number of elements in NLDPRM (=7). * * NLCPRM C(NLC)*1 Character array (ignored). * * NLIPRM I(NLI) Integer array (ignored). * * Given and/or returned: * NLDPRM D(NLD) Double precision coefficients (see below). * * WORLD D(2) World coordinates. WORLD(1) and WORLD(2) are * the longitude and velocity, in degrees and m/s. * Given if OPCODE > 0, returned if OPCODE < 0. * * PIXEL D(2) Pixel coordinates. * Given if OPCODE < 0, returned if OPCODE > 0. * * CONTRL I Control flag for OPCODE = +2 (ignored, always * set to 0 on return). * * CONTXT D(20) Context elements (ignored). * * Returned: * IERR I Status return value: * 0: Success. * 1: Invalid coordinate transformation * parameters. * * Notes: * The NLDPRM array is constructed as follows: * - (1) Axis 1 reference pixel coordinate * - (2) Axis 2 reference pixel coordinate * - (3) Axis 1 reference pixel value (degree) * - (4) Axis 2 reference pixel value (Hz) * - (5) Axis 1 coordinate increment (degree/pixel) * - (6) Axis 2 coordinate increment (Hz/pixel) * - (7) Rest frequency (Hz) * *======================================================================= SUBROUTINE LNGVEL (OPCODE, NLC, NLI, NLD, NLCPRM, NLIPRM, NLDPRM, : WORLD, PIXEL, CONTRL, CONTXT, IERR) *----------------------------------------------------------------------- INTEGER CONTRL, IERR, NLC, NLD, NLI, NLIPRM(NLI), OPCODE DOUBLE PRECISION CONTXT(20), CVEL, FREQ, NLDPRM(NLD), PIXEL(2), S, : WORLD(2) CHARACTER NLCPRM(NLC)*1 PARAMETER (CVEL = 2.9979D8) *----------------------------------------------------------------------- IERR = 0 IF (OPCODE.GT.0) THEN * Compute pixel coordinates from world coordinates. PIXEL(1) = NLDPRM(1) + (WORLD(1) - NLDPRM(3))/NLDPRM(5) S = (CVEL-WORLD(2))/(CVEL+WORLD(2)) IF (S.LT.0D0) THEN IERR = 2 RETURN END IF FREQ = NLDPRM(7)*SQRT(S) PIXEL(2) = NLDPRM(2) + (FREQ - NLDPRM(4))/NLDPRM(6) CONTRL = 0 ELSE IF (OPCODE.EQ.0) THEN * Initialize. IF (NLC.LT.1 .OR. NLI.LT.1 .OR. NLD.LT.7) IERR = 1 IF (NLDPRM(5).EQ.0D0) IERR = 1 IF (NLDPRM(6).EQ.0D0) IERR = 1 IF (NLDPRM(7).EQ.0D0) IERR = 1 CONTRL = 0 ELSE IF (OPCODE.EQ.-1) THEN * Compute world coordinates from pixel coordinates. WORLD(1) = NLDPRM(3) + NLDPRM(5)*(PIXEL(1) - NLDPRM(1)) FREQ = NLDPRM(4) + NLDPRM(6)*(PIXEL(2) - NLDPRM(2)) S = (FREQ/NLDPRM(7))**2 WORLD(2) = CVEL*(1D0 - S)/(1D0 + S) ELSE IERR = 1 END IF RETURN END pywcs-1.12/wcslib/pgsbox/pgcrfn.f0000644001153600020070000001402312310355626021061 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. * Copyright (C) 1997-2012, Mark Calabretta * * This file is part of PGSBOX. * * PGSBOX is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * PGSBOX is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with PGSBOX. If not, see http://www.gnu.org/licenses. * * Correspondence concerning PGSBOX may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: pgcrfn.f,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *======================================================================= * * PGCRFN defines separable pairs of non-linear coordinate systems for * PGSBOX. * * Given: * OPCODE I Transformation code: * +2: Compute a set of pixel coordinates that * describe a path between this and the * previous pair of world coordinates * remembered from the last call with * OPCODE = +1 or +2. * +1: Compute pixel coordinates from world * coordinates. * 0: Initialize. * -1: Compute world coordinates from pixel * coordinates. * * NLC I Number of elements in FCODE (=8). * * NLI I Number of elements in NLIPRM (=2). * * NLD I Number of elements in NLDPRM. * * FCODE C(NLC)*1 Character array (contains the CTYPE array, * see below). * * Given and/or returned: * NLIPRM I(NLI) Integer coefficients (see below). * * NLDPRM D(2,NLD) Double precision coefficients (see below). * * WORLD D(2) World coordinates. * Given if OPCODE > 0, returned if OPCODE < 0. * * PIXEL D(2) Pixel coordinates. * Given if OPCODE < 0, returned if OPCODE > 0. * * CONTRL I Control flag for OPCODE = +2 (ignored, always * set to 0 on return). * * CONTXT D(20) Context elements (ignored). * * Returned: * IERR I Status return value: * 0: Success. * 1: Invalid parameters. * 2: Invalid world coordinate. * 3: Invalid pixel coordinate. * * Notes: * PGCRFN assumes a simple 2-D image. The FCODE array contains * two four-character mnemonics that select function types: * * "Lin " Linear * "Log " Logarithmic * "Pow " Power law * * The first two elements of NLIPRM are set on initialization to * offsets used by computed GO TOs for each function type. * * Note that PGCRFN treats NLDPRM as an array of dimension two. * The NLDPRM are used as follows: * * Type WORLD(J) = * Lin NLDPRM(J,3) + S * Log NLDPRM(J,3) * LOG10(S) * Pow (NLDPRM(J,3) + S)**NLDPRM(J,4) * * Where in each case S = NLDPRM(J,2)*(PIXEL(J) - NLDPRM(J,1)) * *======================================================================= SUBROUTINE PGCRFN (OPCODE, NLC, NLI, NLD, FCODE, NLIPRM, NLDPRM, : WORLD, PIXEL, CONTRL, CONTXT, IERR) *----------------------------------------------------------------------- INTEGER CONTRL, IERR, J, NLC, NLD, NLI, OPCODE, NLIPRM(NLI) DOUBLE PRECISION CONTXT(20), NLDPRM(2,NLD), PIXEL(2), S, WORLD(2) CHARACTER FCODE(2)*4, FCODES*20 DATA FCODES(1:20) /'Lin Log Pow '/ *----------------------------------------------------------------------- IERR = 0 IF (OPCODE.GT.0) THEN * Compute pixel coordinates from world coordinates. DO 200 J = 1, 2 GO TO (110, 120, 130) NLIPRM(J) IERR = 1 RETURN * Linear. 110 S = WORLD(J) - NLDPRM(J,3) GO TO 190 * Logarithmic to base 10. 120 S = 10D0**(WORLD(J)/NLDPRM(J,3)) GO TO 190 * Power. 130 S = WORLD(J)**(1D0/NLDPRM(J,4)) - NLDPRM(J,3) 190 PIXEL(J) = NLDPRM(J,1) + S/NLDPRM(J,2) 200 CONTINUE CONTRL = 0 ELSE IF (OPCODE.EQ.0) THEN * Initialize. IF (NLC.LT.8 .OR. NLI.LT.2 .OR. NLD.LT.3) THEN IERR = 1 RETURN END IF * Compute pointers. NLIPRM(1) = (INDEX(FCODES,FCODE(1)) + 3)/4 NLIPRM(2) = (INDEX(FCODES,FCODE(2)) + 3)/4 IF (NLIPRM(1).EQ.0 .OR. NLIPRM(2).EQ.0) THEN IERR = 1 RETURN END IF CONTRL = 0 ELSE IF (OPCODE.EQ.-1) THEN * Compute world coordinates from pixel coordinates. DO 300 J = 1, 2 S = NLDPRM(J,2)*(PIXEL(J) - NLDPRM(J,1)) GO TO (210, 220, 230) NLIPRM(J) IERR = 1 RETURN * Linear. 210 WORLD(J) = NLDPRM(J,3) + S GO TO 300 * Logarithmic to base 10. 220 IF (S.LE.0D0) THEN IERR = 1 RETURN END IF WORLD(J) = NLDPRM(J,3)*LOG10(S) GO TO 300 * Power. 230 S = S + NLDPRM(J,3) IF (S.LE.0D0 .AND. MOD(NLDPRM(J,4),1D0).NE.0D0) THEN IERR = 1 RETURN END IF WORLD(J) = S**NLDPRM(J,4) 300 CONTINUE ELSE IERR = 1 END IF RETURN END pywcs-1.12/wcslib/pgsbox/pgcrvl.f0000644001153600020070000000360712310355626021105 0ustar cslocumSTSCI\science00000000000000*======================================================================= * PGSBOX 4.10 *----------------------------------------------------------------------- * * ATTENTION! * ---------- * * PGCRVL is defunct. * * Do not use this routine - use PGSBOX instead. * --------------------------------------------- * * What remains here is a driver for the more general PGSBOX routine * which is not based on pixel coordinates. * * This residue of PGCRVL exists mainly for backwards compatibility. * PGCRVL's old AXEN argument is here translated into the BLC and TRC * arguments required by PGSBOX. * * New applications should use PGSBOX directly. * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: pgcrvl.f,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *======================================================================= SUBROUTINE PGCRVL (AXEN, IDENTS, OPT, LABCTL, LABDEN, CI, GCODE, : TIKLEN, NG1, GRID1, NG2, GRID2, DOEQ, NLFUNC, NLC, NLI, NLD, : NLCPRM, NLIPRM, NLDPRM, NC, IC, CACHE, IERR) *----------------------------------------------------------------------- LOGICAL DOEQ INTEGER AXEN(2), CI(7), GCODE(2), IC, IERR, LABCTL, LABDEN, NC, : NG1, NG2, NLC, NLD, NLI, NLIPRM(NLI) REAL BLC(2), TRC(2) DOUBLE PRECISION CACHE(4,0:NC), GRID1(0:NG1), GRID2(0:NG2), : NLDPRM(NLD), TIKLEN CHARACTER IDENTS(3)*(*), NLCPRM(NLC)*1, OPT(2)*(*) EXTERNAL NLFUNC *----------------------------------------------------------------------- BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = AXEN(1) + 0.5 TRC(2) = AXEN(2) + 0.5 CALL PGSBOX (BLC, TRC, IDENTS, OPT, LABCTL, LABDEN, CI, GCODE, : TIKLEN, NG1, GRID1, NG2, GRID2, DOEQ, NLFUNC, NLC, NLI, NLD, : NLCPRM, NLIPRM, NLDPRM, NC, IC, CACHE, IERR) RETURN END pywcs-1.12/wcslib/pgsbox/pgsbox.f0000644001153600020070000025560212310355626021116 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. * Copyright (C) 1997-2012, Mark Calabretta * * This file is part of PGSBOX. * * PGSBOX is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * PGSBOX is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with PGSBOX. If not, see http://www.gnu.org/licenses. * * Correspondence concerning PGSBOX may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: pgsbox.f,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *======================================================================= * * PGSBOX draws and labels a curvilinear coordinate grid. The caller * must provide a separate external function, NLFUNC, to define the * non-linear coordinate transformation. * * PGLBOX, a simplified ENTRY point to PGSBOX, has been provided for * drawing simple linear axes without the need to specify NLFUNC. * PGLBOX allows simplified access to formatting control for labelling * world coordinate axes that is not provided by the standard PGPLOT * routines, PGBOX or PGTBOX. PGLBOX uses the world coordinate range * set by a prior call to PGSWIN and omits the following arguments: * * BLC, TRC, NLFUNC, NLC, NLI, NLD, NLCPRM, NLIPRM, NLDPRM * * The remaining arguments are specified in the same order as PGSBOX. * * Given: * BLC R(2) Cartesian coordinates of the bottom left-hand * TRC R(2) corner and top right-hand corner of the frame. * Any convenient Cartesian system may be used in * conjunction with the non-linear transformation * function, NLFUNC, described below. * * For example, FITS images have pixel coordinate * (1,1) at the centre of the pixel in the bottom * left-hand corner. Thus it would be * appropriate to set BLC to (0.5,0.5) and TRC to * (NAXIS1+0.5, NAXIS2+0.5). * * IDENTS C(3)*(*) Identification strings: * 1: Name of the first world coordinate * element used for axis labelling. * 2: Name of the second world coordinate. * 3: Title, written at top. * * OPT C(2)*(*) Formatting control for the world coordinates, * used for axis labelling (see notes 1 and 2): * ' ': plain numeric * 'A': angle in degrees expressed in decimal * notation normalized in the range [0,360). * 'B': as 'A' but normalized in the range * (-180,180]. * 'C': as 'A' but unnormalized. * 'D': angle in degrees expressed in sexagesimal * notation, DD^MM'SS".S, normalized in the * range [0,360). * 'E': as 'D' but normalized in the range * (-180,180]. * 'F': as 'D' but unnormalized. * 'G': angle in degrees expressed in hms * notation, HHhMMmSSs.S, normalized in the * range [0,24) hours. * 'H': as 'G' but normalized in the range * (-12,12] hours. * 'I': as 'G' but unnormalized. * 'L': logarithmic (see note 2) * 'T': time in hours expressed as HH:MM:SS.S * 'Y': Modified Julian Date to be expressed as * a Gregorian calendar date, YYYY/MM/DD. * (MJD = JD - 2400000.5.) * * For the angular types, NLFUNC is assumed to * return the angle in degrees whereupon it will * be formatted for display in the specified way. * For example, an angle of -417.2958 degrees * (returned by NLFUNC): * * 'A': 302^.7042 * 'B': -57^.2958 * 'C': -417^.2958 * 'D': 302^42'15" * 'E': -57^17'45" * 'F': -417^17'45" * 'H': 20h10m49s * 'I': -3h49m11s * 'J': -27h49m11s * * These are properly superscripted. * * LABCTL I Decimal encoded grid labelling control: * -1: Accumulate information on grid labels * (see note 3) but do not write them. * 0: Let PGSBOX decide what edges to label. * 1: Label bottom of frame with the first * world coordinate. * 2: Label bottom of frame with the second * world coordinate. * 10: ... left side of frame. * 20: ... left side of frame. * 100: ... top of frame. * 200: ... top of frame. * 1000: ... right side of frame. * 2000: ... right side of frame. * 10000: Write labels from information * accumulated in previous calls without * drawing grid lines or tick marks. * * LABCTL = 0 usually gets what you want. * LABCTL = 3333 labels all sides with both world * coordinates. * * LABDEN I Decimal encoded labelling density control for * use where PGSBOX is called upon to determine a * suitable grid spacing (e.g. via NG1 = 0, * GRID1(0) = 0). LABDEN = 100*D2 + D1 where * D1, and D2 are the approximate number of grid * lines for the first and second world * coordinate. LABDEN = 0 is effectively the same * as LABDEN = 808. * * CI I(7) Table of predefined colours established by * calls to PGSCR. This is used to control the * colour used for different parts of the plot. * CI table entries are used as follows: * * world * coordinate * Index usage element * ----- -------------- ---------- * 1 grid lines 1 * 2 grid lines 2 * 3 numeric labels 1 * 4 numeric labels 2 * 5 axis annotation 1 * 6 axis annotation 2 * 7 title - * * For example, CI(3) is used for numeric labels * for the first world coordinate. * * Colour selection is disabled for component J * if CI(J) < 0. * * GCODE(2) I Code for the type of grid to draw for each * world coordinate: * 0: No grid or tick marks. * 1: Tick marks (on all edges). * 2: Full coordinate grid. * * Tick marks can be restricted to particular * edges of the frame; a negative GCODE is * interpreted as a decimal encoded control * variable: * -1: bottom * -10: left * -100: top * -1000: right * * The digit scales the basic tick length. For * example, GCODE(1) = -102 restricts tick marks * for the first world coordinate to the bottom * and top edges of the frame. Those on the * bottom will be twice the length specified by * TIKLEN. * * TIKLEN D Tick length, in mm. Negative values produce * outside tick marks. * * NG1 I Upper array index for GRID1. * * GRID1 D(0:NG1) Grid values in WORLD(1) in the same units as * returned by NLFUNC. * * If NG1 is zero, then * a: if GRID1(0) is greater than zero it * defines a uniform grid spacing. * b: if GRID1(0) is zero a suitable spacing * will be determined (see LABDEN). * c: if GRID1(0) is less than zero then no * grid lines will be drawn. * * If NG1 is greater than zero, then GRID1(0) is * ignored. * * NG2 I Upper array index for GRID2. * * GRID2 D(0:NG2) Grid values in WORLD(2) in the same units as * returned by NLFUNC, interpreted the same way * as GRID1. * * DOEQ L If NG1 = NG2 = 0, and GRID1(0) = 0D0 and/or * GRID2(0) = 0D0, then choose the same grid * spacing for each world coordinate. * * NLFUNC Ext Non-linear coordinate function, see below. * * NLC I Number of elements in NLCPRM (must be >0). * * NLI I Number of elements in NLIPRM (must be >0). * * NLD I Number of elements in NLDPRM (must be >0). * * Given and/or returned: * NLCPRM C(NLC)*1 Character coefficients for NLFUNC. * * NLIPRM I(NLI) Integer coefficients for NLFUNC. * * NLDPRM D(NLD) Double precision coefficients for NLFUNC. * * NC I Upper array index for CACHE (see note 3). * * IC I Current number of entries in the CACHE table. * Should be set to -1 on the first call to * PGSBOX (see note 3). * * CACHE D(4,0:NC) Table of points where the tick marks or grid * lines cross the frame (see note 3). * 1: Frame segment * 1: bottom * 2: left * 3: top * 4: right * 2: X or Y-Cartesian coordinate. * 3: World coordinate element (1 or 2). * 4: Value. * * CACHE(,0) is used to cache the extrema of the * coordinate values between calls. CACHE(1,NC-1) * is also used to store related information. * * CACHE(,NC) will contain the margin widths in * Cartesian coordinates when the labels are * produced (i.e. the same Cartesian system used * for BLC and TRC). * * Returned: * IERR I Status return value: * 0: Success * 1: Initialization error * 2: Invalid coordinate system * 3: Cache overflow (see note 3). * * Notes: * 1: Where a logarithmic world coordinate type is indicated PGSBOX * chooses grid lines and labels on the basis that the value * returned by NLFUNC is a base 10 logarithm. PGSBOX does not * itself take logarithms or antilogarithms. For example, if the * range of values returned by NLFUNC were 0.9 - 2.5, then PGSBOX * would draw a subset of the following set of grid lines and * labels: * * value label * ------------------ ----- * 0.9031 = log10(8) 8 * 0.9542 = log10(9) 9 * 1.0000 = log10(10) 10**1 * 1.3010 = log10(20) 2 * 1.4771 = log10(30) 3 * 1.6021 = log10(40) 4 * 1.6990 = log10(50) 5 * 1.7782 = log10(60) 6 * 1.8451 = log10(70) 7 * 1.9031 = log10(80) 8 * 1.9542 = log10(90) 9 * 2.0000 = log10(100) 10**2 * 2.3010 = log10(200) 2 * 2.4771 = log10(300) 3 * * The subset chosen depends on the coordinate increment as * specified by the caller (e.g. via NG1 = 0, GRID1(0) > 0) or as * deduced by PGSBOX from the required density of grid lines * specified in the LABDEN argument. The selection is made * according to the following table: * * increment grid lines * (0.00,0.12] 1, 2, 3, 4, 5, 6, 7, 8, 9 * (0.12,0.18] 1, 2, 3, 4, 5, 7 * (0.18,0.23] 1, 2, 3, 5, 7 * (0.23,0.28] 1, 2, 3, 5 * (0.28,0.40] 1, 2, 5 * (0.40,0.70] 1, 3 * (0.70,1.00] 1 * * For increments greater than 1 the nearest integer is used. * * 2: PGSBOX will attempt to handle discontinuities in angle, such as * may occur when cycling through 360 degrees, wherever the * discontinuity may occur, for example * * 359 -> 0 -> 1 * * or * * 179 -> 180 -> -179 * * Only single cycles are detected, so the sequence * * -360 -> 0 -> ... -> 359 -> 0 -> ... -> 359 * * would not be handled properly. In such cases NLFUNC should be * changed to return a normalized angle, or else a continuous * sequence. * * 3: PGSBOX maintains a table of axis crossings, CACHE, in which it * stores information used for axis labelling. The caller need not * normally be concerned about the use of this table other than to * provide sufficient space. Typically, NC = 256 should be enough; * if not, IERR = 3 will be returned. * * However, a coordinate grid may be produced via multiple calls to * PGSBOX with deferment of axis labelling. This might be done to * change the pen colour and/or thickness for different sets of * grid lines. The table accumulates information from each * successive call until the labels are produced. The table index, * IC, may be reset to zero by the caller to discard the * information collected. * * The extrema of the world coordinate elements are stored in * CACHE(,0). When a coordinate grid is plotted with multiple * calls to PGSBOX the initial call should always have IC set to -1 * to signal that PGSBOX needs to determine the extrema. On * subsequent calls with IC non-negative PGSBOX uses the extrema * cached from the first call. This can speed up execution * considerably. * *- - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - * * The curvilinear coordinate grid is defined by external function * NLFUNC whose interface is defined as follows: * * Given: * OPCODE I Transformation code: * +2: Compute a set of Cartesian coordinates * that describe a path between this and * the previous pair of world coordinates * remembered from the last call with * OPCODE = +1 or +2. Usually only takes * a single step unless traversing a * discontinuity or some other * irregularity (see explanation below). * +1: Compute Cartesian coordinates from world * coordinates. * 0: Initialize. * -1: Compute world coordinates from Cartesian * coordinates. * * N.B. NLFUNC must not change the input * coordinates; that is the world coordinates for * OPCODEs = +2 and +1, or the Cartesian * coordinates for OPCODE = -1. * * NLC I Number of elements in NLCPRM (must be >0). * * NLI I Number of elements in NLIPRM (must be >0). * * NLD I Number of elements in NLDPRM (must be >0). * * Given and/or returned: * NLCPRM C(NLC)*1 Character array. * * NLIPRM I(NLI) Integer coefficients. * * NLDPRM D(NLD) Double precision coefficients. * * WORLD D(2) World coordinates. Given if OPCODE > 0, * returned if OPCODE < 0. * * XY D(2) Cartesian coordinates. Given if OPCODE < 0, * returned if OPCODE > 0. * * CONTRL I Control flag for OPCODE = +2: * 0: Normal state. * 1: Force PGSBOX to flush its plotting buffer * and call NLFUNC again with the same world * coordinates. * 2: Force PGSBOX to call NLFUNC again with * the same world coordinates (without * flushing its plotting buffer). * * CONTXT D(20) Context elements for OPCODE = +2. * * Returned: * IERR I Status return value: * 0: Success. * 1: Invalid parameters. * 2: Invalid world coordinate. * 3: Invalid Cartesian coordinate. * * The following status returns are recognized for * opcodes +2 and +1 * -1: Accept the returned (x,y) coordinates but * do not consider this as one end of a * crossing segment for labelling world * coordinate 1. * -2: Ditto for world coordinate 2. * -3: Ditto for world coordinates 1 and 2. * * PGSBOX passes its NLCPRM, NLIPRM, and NLDPRM adjustable size array * arguments of length NLC, NLI, and NLD to NLFUNC without * modification. Comments within NLFUNC should specify the parameters * it wants passed to it via these arrays. * * PGSBOX first calls NLFUNC with OPCODE = 0 to cause it to initialize * its work arrays (if necessary). It then uses OPCODE = -1 to * determine the range of world coordinate values. It anchors the * start of each coordinate grid line with a call with OPCODE = +1, and * then tracks it with OPCODE = +2. * * The CONTXT array is also passed to NLFUNC without modification to * allow it to preserve state information between calls for OPCODE = 2. * In particular, NLFUNC can use this to detect discontinuities in the * grid lines. * * The CONTRL argument is provided so that NLFUNC can force PGSBOX to * call it again with or without flushing its plotting buffer. This * may be needed when plotting a grid line through a discontinuity. * PGSBOX does not modify CONTRL. * * Notes: * 1: NLFUNC must not change the input coordinates; that is the world * coordinates for OPCODEs = +1 and +2, or the Cartesian coordinates * for OPCODE = -1. * * 2: NLFUNC must define a single-valued function, that is, each * Cartesian coordinate (x,y) must map to a unique world coordinate * pair (xi,eta). * * 3: Notwithstanding the fact that PGSBOX declares NLCPRM, NLIPRM, * and NLDPRM as single dimension arrays of length NLC, NLI, and * NLD, NLFUNC may treat these as higher-dimensional arrays, for * example, NLDPRM(2,NLD). (The FORTRAN standard requires that * only the last dimension is adjustable.) * *======================================================================= SUBROUTINE PGSBOX (BLC_, TRC_, IDENTS, OPT, LABCTL, LABDEN, CI, : GCODE, TIKLEN, NG1, GRID1, NG2, GRID2, DOEQ, NLFUNC, NLC, NLI, : NLD, NLCPRM, NLIPRM, NLDPRM, NC, IC, CACHE, IERR) *----------------------------------------------------------------------- INTEGER BUFSIZ PARAMETER (BUFSIZ = 2048) LOGICAL DOEDGE, DOEQ, DOLBOX, FULLSM, GETEND, INSIDE, ISANGL(2), : LABLOK, MAJOR, OVERFL, PREVIN INTEGER CI(7), CI0, CJ(7), CONTRL, DENS(2), FSEG, GCODE(2), IC, : ID, IERR, IM, ISTEP, IW0, IWJ, IWK, IX, IY, IYPREV, J, : K, KX, L, LABCTL, LABDEN, LDIV(2), LTABL(6,2:6), NC, : NG(2), NG1, NG2, NLC, NLD, NLI, NLIPRM(NLI), NP, : NSTEP(2), NWJ, NX, NY, TCODE(2,4) REAL BLC(2), BLC_(2), S, TRC(2), TRC_(2), WXY(4), X1, X2, : XPOINT, XR(BUFSIZ), XSCL, XSPAN, XTOL, XVP1, XVP2, : Y1, Y2, YR(BUFSIZ), YSCL, YSPAN, YTOL, YVP1, YVP2 DOUBLE PRECISION CONTXT(20), CACHE(4,0:NC), DW(2), DX, DY, FACT, : G0(2), GSTEP(2), GRID1(0:NG1), GRID2(0:NG2), : NLDPRM(NLD), STEP, SW(2), TIKLEN, TMP, VMAX(2,2), : VMIN(2,2), W1PREV, W1X0, W2PREV, W2X0, WJUMP, WMAX(2), : WMIN(2), WORLD(9), XY(9) CHARACTER FTYPE(2), IDENTS(3)*(*), NLCPRM(NLC)*1, OPT(2)*(*) EXTERNAL NLFUNC * Approximate number of grid lines for each coordinate. INTEGER DENS0 PARAMETER (DENS0 = 8) * Double precision round-off tolerance. DOUBLE PRECISION TOL PARAMETER (TOL = 1D-8) * Number of steps per grid line. DATA NSTEP /80, 80/ * Table of logarithmic grid values. DATA LTABL /3, 10, 0, 0, 0, 0, : 2, 5, 10, 0, 0, 0, : 2, 3, 5, 10, 0, 0, : 2, 3, 5, 7, 10, 0, : 2, 3, 4, 5, 7, 10/ * These are to stop compiler messages about uninitialized variables. DATA IW0 /0/ DATA LABLOK, PREVIN /2 * .FALSE./ DATA G0 /2 * 0D0/ DATA W1X0, W1PREV, W2X0, W2PREV /4 * 0D0/ DATA WORLD, XY /9 * 0D0, 9 * 0D0/ *----------------------------------------------------------------------- * Initialize. DOLBOX = .FALSE. CALL NLFUNC (0, NLC, NLI, NLD, NLCPRM, NLIPRM, NLDPRM, WORLD, : XY, CONTRL, CONTXT, IERR) * Quick return for now. IF (IERR.NE.0) THEN IERR = 1 RETURN END IF BLC(1) = BLC_(1) BLC(2) = BLC_(2) TRC(1) = TRC_(1) TRC(2) = TRC_(2) DOEDGE = GCODE(1).NE.2 .AND. GCODE(2).NE.2 *----------------------------------------------------------------------- GO TO 10 ENTRY PGLBOX (IDENTS, OPT, LABCTL, LABDEN, CI, GCODE, TIKLEN, NG1, : GRID1, NG2, GRID2, DOEQ, NC, IC, CACHE, IERR) DOLBOX = .TRUE. BLC(1) = 0.0 BLC(2) = 0.0 TRC(1) = 1.0 TRC(2) = 1.0 DOEDGE = .TRUE. CONTRL = 0 IERR = 0 10 CONTINUE *----------------------------------------------------------------------- IF (NC.LT.1) THEN IERR = 3 RETURN END IF NG(1) = NG1 NG(2) = NG2 FTYPE(1) = OPT(1)(1:1) FTYPE(2) = OPT(2)(1:1) * Extend the PGPLOT window and rescale it. CALL PGQVP (0, XVP1, XVP2, YVP1, YVP2) CALL PGQWIN (WXY(1), WXY(2), WXY(3), WXY(4)) CALL PGSVP (0.0, 1.0, 0.0, 1.0) XSCL = (TRC(1)-BLC(1))/(XVP2-XVP1) YSCL = (TRC(2)-BLC(2))/(YVP2-YVP1) CALL PGSWIN (BLC(1)-XSCL*XVP1, TRC(1)+XSCL*(1.0-XVP2), : BLC(2)-YSCL*YVP1, TRC(2)+YSCL*(1.0-YVP2)) * Determine initial colour and set colour indices. CALL PGQCI (CI0) DO 20 J = 1, 7 IF (CI(J).GE.0) THEN CJ(J) = CI(J) ELSE CJ(J) = CI0 END IF 20 CONTINUE * Labels only? IF (LABCTL.GE.10000) GO TO 130 XSPAN = WXY(2) - WXY(1) YSPAN = WXY(4) - WXY(3) XTOL = XSPAN*TOL YTOL = YSPAN*TOL * Find world coordinate ranges: * WMIN(1:2) ...lower limit of each world coordinate element. * WMAX(1:2) ...upper limit of each world coordinate element. * GSTEP(1:2) ...spacing between grid lines for each element. * DW(1:2) ...span from WMIN to WMAX. * SW(1:2) ...increment in world coordinate between plotting steps. * NSTEP(1:2) ...number of plotting steps between WMIN and WMAX. FULLSM = .FALSE. IF (IC.GE.0 .AND. IC.LT.NC-1) FULLSM = CACHE(1,NC-1).EQ.1D0 IF (IC.GE.0 .AND. (FULLSM .OR. DOEDGE)) THEN * Use extrema cached from a previous call. WMIN(1) = CACHE(1,0) WMAX(1) = CACHE(2,0) WMIN(2) = CACHE(3,0) WMAX(2) = CACHE(4,0) ELSE * Do a coarse search to find approximate ranges. WMIN(1) = 1D99 WMAX(1) = -1D99 WMIN(2) = 1D99 WMAX(2) = -1D99 * Need to consider cycles in angle through 360 degrees. ISANGL(1) = INDEX('ABCDEFGHI',FTYPE(1)).NE.0 ISANGL(2) = INDEX('ABCDEFGHI',FTYPE(2)).NE.0 VMIN(1,1) = 1D99 VMIN(1,2) = 1D99 VMAX(1,1) = -1D99 VMAX(1,2) = -1D99 VMIN(2,1) = 1D99 VMIN(2,2) = 1D99 VMAX(2,1) = -1D99 VMAX(2,2) = -1D99 * Sample coordinates on a 50 x 50 grid. NX = 50 NY = 50 DX = DBLE(TRC(1)-BLC(1))/NX DY = DBLE(TRC(2)-BLC(2))/NY K = 0 IYPREV = -1 DO 40 IY = 0, NY XY(2) = BLC(2) + IY*DY * Sample the edges only? KX = 1 IF (DOEDGE) THEN IF (IY.NE.0 .AND. IY.NE.NY) KX = NX END IF DO 30 IX = 0, NX, KX XY(1) = BLC(1) + IX*DX IF (DOLBOX) THEN WORLD(1) = WXY(1) + XY(1)*XSPAN WORLD(2) = WXY(3) + XY(2)*YSPAN ELSE CALL NLFUNC (-1, NLC, NLI, NLD, NLCPRM, NLIPRM, : NLDPRM, WORLD, XY, CONTRL, CONTXT, IERR) END IF IF (IERR.EQ.0) THEN K = K + 1 IF (ISANGL(1)) THEN IF (K.EQ.1) W1X0 = WORLD(1) IF (IY.NE.IYPREV) THEN W1PREV = W1X0 W1X0 = WORLD(1) END IF * Iron out jumps. WJUMP = WORLD(1) - W1PREV IF (ABS(WJUMP).GT.180D0) THEN WJUMP = WJUMP + SIGN(180D0,WJUMP) WJUMP = 360D0*INT(WJUMP/360D0) WORLD(1) = WORLD(1) - WJUMP END IF W1PREV = WORLD(1) IYPREV = IY END IF IF (ISANGL(2)) THEN IF (K.EQ.1) W2X0 = WORLD(2) IF (IY.NE.IYPREV) THEN W2PREV = W2X0 W2X0 = WORLD(2) END IF * Iron out jumps. WJUMP = WORLD(2) - W2PREV IF (ABS(WJUMP).GT.180D0) THEN WJUMP = WJUMP + SIGN(180D0,WJUMP) WJUMP = 360D0*INT(WJUMP/360D0) WORLD(2) = WORLD(2) - WJUMP END IF W2PREV = WORLD(2) IYPREV = IY END IF IF (WORLD(1).LT.WMIN(1)) WMIN(1) = WORLD(1) IF (WORLD(1).GT.WMAX(1)) WMAX(1) = WORLD(1) IF (WORLD(2).LT.WMIN(2)) WMIN(2) = WORLD(2) IF (WORLD(2).GT.WMAX(2)) WMAX(2) = WORLD(2) IF (ISANGL(1)) THEN * Normalize to the range [0,360). WORLD(1) = MOD(WORLD(1), 360D0) IF (WORLD(1).LT.0D0) WORLD(1) = WORLD(1) + 360D0 IF (WORLD(1).LT.VMIN(1,1)) VMIN(1,1) = WORLD(1) IF (WORLD(1).GT.VMAX(1,1)) VMAX(1,1) = WORLD(1) * Normalize to the range (-180,180]. IF (WORLD(1).GT.180D0) WORLD(1) = WORLD(1) - 360D0 IF (WORLD(1).LT.VMIN(1,2)) VMIN(1,2) = WORLD(1) IF (WORLD(1).GT.VMAX(1,2)) VMAX(1,2) = WORLD(1) END IF IF (ISANGL(2)) THEN * Normalize to the range [0,360). WORLD(2) = MOD(WORLD(2), 360D0) IF (WORLD(2).LT.0D0) WORLD(2) = WORLD(2) + 360D0 IF (WORLD(2).LT.VMIN(2,1)) VMIN(2,1) = WORLD(2) IF (WORLD(2).GT.VMAX(2,1)) VMAX(2,1) = WORLD(2) * Normalize to the range (-180,180]. IF (WORLD(2).GT.180D0) WORLD(2) = WORLD(2) - 360D0 IF (WORLD(2).LT.VMIN(2,2)) VMIN(2,2) = WORLD(2) IF (WORLD(2).GT.VMAX(2,2)) VMAX(2,2) = WORLD(2) END IF END IF 30 CONTINUE 40 CONTINUE IF (K.EQ.0) THEN * No valid coordinates found within the frame. IERR = 2 GO TO 999 END IF * Check for cycles in angle. DO 50 J = 1, 2 IF (ISANGL(J)) THEN IF (WMAX(J)-WMIN(J).LT.360D0 .AND. : WMAX(J)-WMIN(J).GT.VMAX(J,1)-VMIN(J,1)+TOL) THEN * Must have a cycle, preserve the sign. IF (WMAX(J).GE.0D0) THEN WMIN(J) = VMIN(J,1) WMAX(J) = VMAX(J,1) ELSE WMIN(J) = VMIN(J,1) - 360D0 WMAX(J) = VMAX(J,1) - 360D0 END IF END IF IF (WMAX(J)-WMIN(J).LT.360D0 .AND. : WMAX(J)-WMIN(J).GT.VMAX(J,2)-VMIN(J,2)+TOL) THEN * Must have a cycle, preserve the sign. IF (WMAX(J).GE.0D0) THEN IF (VMAX(J,2).GE.0D0) THEN WMIN(J) = VMIN(J,2) WMAX(J) = VMAX(J,2) ELSE WMIN(J) = VMIN(J,2) + 360D0 WMAX(J) = VMAX(J,2) + 360D0 END IF ELSE IF (VMAX(J,2).LT.0D0) THEN WMIN(J) = VMIN(J,2) WMAX(J) = VMAX(J,2) ELSE WMIN(J) = VMIN(J,2) - 360D0 WMAX(J) = VMAX(J,2) - 360D0 END IF END IF END IF END IF 50 CONTINUE * Cache extrema for subsequent calls. CACHE(1,0) = WMIN(1) CACHE(2,0) = WMAX(1) CACHE(3,0) = WMIN(2) CACHE(4,0) = WMAX(2) * Was full sampling done? IF (DOEDGE) THEN CACHE(1,NC-1) = 0D0 ELSE CACHE(1,NC-1) = 1D0 END IF IC = 0 END IF * Choose an appropriate grid spacing. IF (LABDEN.GT.0) THEN * User specified grid density. DENS(1) = MOD(LABDEN,100) DENS(2) = LABDEN/100 IF (DENS(1).EQ.0) DENS(1) = DENS0 IF (DENS(2).EQ.0) DENS(2) = DENS0 ELSE * Default grid density. DENS(1) = DENS0 DENS(2) = DENS0 END IF IF (NG(1).EQ.0) G0(1) = GRID1(0) IF (NG(2).EQ.0) G0(2) = GRID2(0) DO 60 J = 1, 2 IF (J.EQ.1) THEN K = 2 ELSE K = 1 END IF IF (NG(J).EQ.0 .AND. G0(J).LT.0D0) THEN * Defeat grid lines and tick marks. GCODE(J) = 0 END IF IF (NG(J).EQ.0 .AND. G0(J).GT.0D0) THEN * User-specified, directly. GSTEP(J) = G0(J) ELSE IF (DOEQ .AND. NG(K).EQ.0 .AND. G0(K).GT.0D0) THEN * User-specified, indirectly. GSTEP(J) = G0(K) ELSE * Left to us to choose. Even if grid lines are not drawn for * coordinate J, i.e. NG(J) = 0 and G0(J) < 0, GSTEP(J) is still * needed because it is used to deduce SW(J) which is used for * drawing grid lines for the other coordinate. DW(J) = WMAX(J) - WMIN(J) STEP = DW(J)/DENS(J) FACT = 1D0 IF (INDEX('GHI',FTYPE(J)).NE.0) THEN * Rescale degrees to hours. FACT = 1D0/15D0 STEP = STEP*FACT ELSE IF (FTYPE(J).EQ.'Y' .AND. STEP.LT.0.5D0) THEN * Calendar increment of less than 12h; use time format. FTYPE(J) = 'y' * Rescale days to hours. FACT = 24D0 STEP = STEP*FACT END IF IF (INDEX('ABCDEF',FTYPE(J)).NE.0 .AND. STEP.GE.1D0) THEN * Angle with multi-degree increment. IF (STEP.LT.1.5D0) THEN STEP = 1D0 ELSE IF (STEP.LT.3D0) THEN STEP = 2D0 ELSE IF (STEP.LT.7D0) THEN STEP = 5D0 ELSE IF (STEP.LT.12D0) THEN STEP = 10D0 ELSE IF (STEP.LT.20D0) THEN STEP = 15D0 ELSE IF (STEP.LT.40D0) THEN STEP = 30D0 ELSE IF (STEP.LT.70D0) THEN STEP = 45D0 ELSE IF (STEP.LT.120D0) THEN STEP = 90D0 ELSE IF (STEP.LT.270D0) THEN STEP = 180D0 ELSE IF (STEP.LT.520D0) THEN STEP = 360D0 ELSE STEP = 360D0*INT(STEP/360D0 + 0.5) END IF ELSE IF (INDEX('GHITy',FTYPE(J)).NE.0 .AND. : STEP.GE.1D0) THEN * Angle or time in hms format with multi-hour increment. IF (STEP.LT.1.5D0) THEN STEP = 1D0 ELSE IF (STEP.LT.2.5D0) THEN STEP = 2D0 ELSE IF (STEP.LT.3.5D0) THEN STEP = 3D0 ELSE IF (STEP.LT.5D0) THEN STEP = 4D0 ELSE IF (STEP.LT.7D0) THEN STEP = 6D0 ELSE IF (STEP.LT.10D0) THEN STEP = 8D0 ELSE IF (STEP.LT.15D0) THEN STEP = 12D0 ELSE IF (STEP.LT.21D0) THEN STEP = 18D0 ELSE IF (STEP.LT.36D0) THEN STEP = 24D0 ELSE STEP = 24D0*INT(STEP/24D0 + 0.5) END IF STEP = STEP/FACT ELSE IF (INDEX('DEFGHITy',FTYPE(J)).NE.0 .AND. : STEP.LT.1D0) THEN * Angle or time in sexagesimal format with sub-degree/hour * increment. FACT = FACT*60D0 STEP = STEP*60D0 IF (STEP.LT.1D0) THEN * Sub-minute increment. FACT = FACT*60D0 STEP = STEP*60D0 END IF IF (STEP.LT.1D0) THEN * Sub-second increment. TMP = 10D0**(INT(LOG10(STEP))-1) IF (1.5*TMP.GE.STEP) THEN STEP = TMP ELSE IF (3D0*TMP.GE.STEP) THEN STEP = 2D0*TMP ELSE IF (7D0*TMP.GE.STEP) THEN STEP = 5D0*TMP ELSE STEP = 10D0*TMP END IF END IF END IF ELSE IF (STEP.LT.1.5D0) THEN STEP = 1D0 ELSE IF (STEP.LT.2.5D0) THEN STEP = 2D0 ELSE IF (STEP.LT.3.5D0) THEN STEP = 3D0 ELSE IF (STEP.LT.4.5D0) THEN STEP = 4D0 ELSE IF (STEP.LT.5.5D0) THEN STEP = 5D0 ELSE IF (STEP.LT.8D0) THEN STEP = 6D0 ELSE IF (STEP.LT.11D0) THEN STEP = 10D0 ELSE IF (STEP.LT.14D0) THEN STEP = 12D0 ELSE IF (STEP.LT.18D0) THEN STEP = 15D0 ELSE IF (STEP.LT.25D0) THEN STEP = 20D0 ELSE IF (STEP.LT.45D0) THEN STEP = 30D0 ELSE STEP = 60D0 END IF END IF STEP = STEP/FACT ELSE IF (FTYPE(J).EQ.'Y') THEN * Calendar axis: use coded steps. IF (STEP.LT.15D0) THEN * Timespan of a few months; use multi-day increments. STEP = ANINT(STEP) IF (STEP.LT.1D0) THEN STEP = 1D0 ELSE IF (STEP.GT.9D0) THEN * Fortnightly. STEP = 14D0 ELSE IF (STEP.GT.4D0) THEN * Weekly. STEP = 7D0 END IF ELSE IF (STEP.LT.270D0) THEN * Timespan of a few years; use multi-month increments. STEP = ANINT(STEP/30.44D0) IF (STEP.LT.1.5D0) THEN STEP = 1D0 ELSE IF (STEP.LT.2.5D0) THEN STEP = 2D0 ELSE IF (STEP.LT.3.5D0) THEN STEP = 3D0 ELSE IF (STEP.LT.4.5D0) THEN STEP = 4D0 ELSE STEP = 6D0 END IF * Coding for multi-month increments. STEP = 100D0*STEP ELSE * Multi-year increments. STEP = ANINT(DW(J)/DENS(J)/365.25D0) IF (STEP.LT.1D0) THEN STEP = 1D0 ELSE TMP = 10D0**INT(LOG10(STEP)) IF (1.5D0*TMP.GE.STEP) THEN STEP = TMP ELSE IF (3D0*TMP.GE.STEP) THEN STEP = 2D0*TMP ELSE IF (7D0*TMP.GE.STEP) THEN STEP = 5D0*TMP ELSE STEP = 10D0*TMP END IF END IF END IF END IF * Coding for multi-year increments. STEP = 10000D0*STEP END IF ELSE * Just numbers. TMP = 10D0**INT(LOG10(STEP)) IF (STEP.LT.1D0) TMP = TMP/10D0 IF (1.5D0*TMP.GE.STEP) THEN STEP = TMP ELSE IF (3D0*TMP.GE.STEP) THEN STEP = 2D0*TMP ELSE IF (7D0*TMP.GE.STEP) THEN STEP = 5D0*TMP ELSE STEP = 10D0*TMP END IF END IF END IF * Adjust the step size for logarithmic values. IF (FTYPE(J).EQ.'L') THEN IF (STEP.GT.0.7D0) THEN LDIV(J) = 1 STEP = NINT(STEP) ELSE IF (STEP.GT.0.4D0) THEN LDIV(J) = 2 ELSE IF (STEP.GT.0.28D0) THEN LDIV(J) = 3 ELSE IF (STEP.GT.0.23D0) THEN LDIV(J) = 4 ELSE IF (STEP.GT.0.18D0) THEN LDIV(J) = 5 ELSE IF (STEP.GT.0.12D0) THEN LDIV(J) = 6 ELSE LDIV(J) = 9 END IF STEP = 1D0/LDIV(J) END IF END IF END IF GSTEP(J) = STEP END IF 60 CONTINUE * Equal grid spacing? IF (DOEQ .AND. NG(1).EQ.0 .AND. NG(2).EQ.0) THEN IF (GRID1(0).EQ.0D0 .AND. GRID2(0).EQ.0D0) THEN GSTEP(1) = MIN(GSTEP(1), GSTEP(2)) GSTEP(2) = GSTEP(1) ELSE IF (GRID1(0).EQ.0D0) THEN GSTEP(1) = GSTEP(2) ELSE IF (GRID2(0).EQ.0D0) THEN GSTEP(2) = GSTEP(1) END IF END IF * Fine tune the end points. DO 70 J = 1, 2 IF (FTYPE(J).EQ.'L') THEN WMIN(J) = AINT(WMIN(J)-1D0) WMAX(J) = AINT(WMAX(J)+1D0) ELSE IF (FTYPE(J).EQ.'Y') THEN * Calendar axis. IF (GSTEP(J).LT.100D0) THEN * Daily increments. WMIN(J) = AINT(WMIN(J)) WMAX(J) = AINT(WMAX(J)+1D0) ELSE * Start on Jan/01. CALL PGMJD (0, WMIN(J), IY, IM, ID) CALL PGMJD (1, WMIN(J), IY, 1, 1) CALL PGMJD (0, WMAX(J), IY, IM, ID) IF (GSTEP(J).LT.10000D0) THEN * Monthly increments. CALL PGMJD (1, WMAX(J), IY, 12, 1) ELSE * Yearly increments. CALL PGMJD (1, WMAX(J), IY+1, 1, 1) END IF END IF ELSE TMP = AINT(WMIN(J)/GSTEP(J))*GSTEP(J) IF (TMP.GE.WMIN(J)) TMP = TMP - GSTEP(J) WMIN(J) = TMP TMP = AINT(WMAX(J)/GSTEP(J))*GSTEP(J) IF (TMP.LE.WMAX(J)) TMP = TMP + GSTEP(J) WMAX(J) = TMP END IF DW(J) = WMAX(J) - WMIN(J) SW(J) = DW(J)/NSTEP(J) * Adjust NSTEP so that SW divides GSTEP. IF (SW(J).LT.GSTEP(J)) THEN SW(J) = GSTEP(J)/ANINT(GSTEP(J)/SW(J)) ELSE SW(J) = GSTEP(J) END IF NSTEP(J) = ANINT(DW(J)/SW(J)) 70 CONTINUE * Draw the grid. * Get absolute scale for tick marks. CALL PGQVP (2, X1, X2, Y1, Y2) XSCL = (X2-X1)/(TRC(1)-BLC(1)) YSCL = (Y2-Y1)/(TRC(2)-BLC(2)) * Decode tick mark control. DO 80 J = 1, 2 IF (GCODE(J).EQ.2) THEN TCODE(J,1) = -1 TCODE(J,2) = -1 TCODE(J,3) = -1 TCODE(J,4) = -1 ELSE IF (GCODE(J).EQ.1) THEN TCODE(J,1) = 1 TCODE(J,2) = 1 TCODE(J,3) = 1 TCODE(J,4) = 1 ELSE IF (GCODE(J).LT.0) THEN K = ABS(GCODE(J)) TCODE(J,1) = MOD(K,10) TCODE(J,2) = MOD(K/10,10) TCODE(J,3) = MOD(K/100,10) TCODE(J,4) = MOD(K/1000,10) ELSE TCODE(J,1) = 0 TCODE(J,2) = 0 TCODE(J,3) = 0 TCODE(J,4) = 0 END IF 80 CONTINUE * Draw each set of grid lines. OVERFL = .FALSE. DO 120 J = 1, 2 IF (GCODE(J).EQ.0) GO TO 120 IF (J.EQ.1) THEN CALL PGSCI (CJ(1)) K = 2 ELSE CALL PGSCI (CJ(2)) K = 1 END IF IF (NG(J).GT.0) THEN NWJ = NG(J) ELSE IF (FTYPE(J).EQ.'Y' .AND. GSTEP(J).GE.100D0) THEN * Calendar axis. CALL PGMJD (0, WMAX(J), IY, IM, ID) IF (GSTEP(J).LT.10000D0) THEN NWJ = 12*IY + IM CALL PGMJD (0, WMIN(J), IY, IM, ID) NWJ = (NWJ - (12*IY + IM))/INT(GSTEP(J)/100D0) ELSE NWJ = IY CALL PGMJD (0, WMIN(J), IY, IM, ID) NWJ = (NWJ - IY)/INT(GSTEP(J)/10000D0) END IF ELSE NWJ = NINT(DW(J)/GSTEP(J)) IW0 = NINT(WMIN(J)/GSTEP(J)) END IF DO 110 IWJ = 0, NWJ MAJOR = .FALSE. * Determine the world coordinate of the grid line. IF (NG(J).GT.0) THEN * User-specified. IF (IWJ.EQ.0) GO TO 110 IF (J.EQ.1) THEN WORLD(1) = GRID1(IWJ) ELSE WORLD(2) = GRID2(IWJ) END IF ELSE * Internally computed. IF (FTYPE(J).EQ.'Y' .AND. GSTEP(J).GE.100D0) THEN * Calendar axis. CALL PGMJD (0, WMIN(J), IY, IM, ID) IF (GSTEP(J).LT.10000D0) THEN IM = IM + IWJ*INT(GSTEP(J)/100D0) CALL PGMJD (1, WORLD(J), IY, IM, ID) ELSE IY = IY + IWJ*INT(GSTEP(J)/10000D0) CALL PGMJD (1, WORLD(J), IY, IM, ID) END IF ELSE WORLD(J) = (IW0 + IWJ)*GSTEP(J) * Logarithmic? IF (FTYPE(J).EQ.'L') THEN TMP = MOD(WORLD(J),1D0) IF (TMP.LT.0D0) TMP = TMP + 1D0 L = NINT(TMP*LDIV(J)) IF (L.EQ.0) THEN * Major tick mark. MAJOR = .TRUE. ELSE * Adjust logarithmic scales. IF (LDIV(J).LE.6) THEN L = LTABL(L,LDIV(J)) ELSE L = L + 1 END IF WORLD(J) = WORLD(J) - TMP + LOG10(DBLE(L)) END IF END IF END IF END IF NP = 0 GETEND = .TRUE. DO 100 IWK = 0, NSTEP(K) WORLD(K) = WMIN(K) + IWK*SW(K) IF (GETEND) THEN * Get end-point context. IF (DOLBOX) THEN XY(1) = (WORLD(1) - WXY(1))/XSPAN XY(2) = (WORLD(2) - WXY(3))/YSPAN ELSE CALL NLFUNC (1, NLC, NLI, NLD, NLCPRM, NLIPRM, : NLDPRM, WORLD, XY, CONTRL, CONTXT, IERR) END IF IF (IERR.LE.0) THEN X1 = REAL(XY(1)) Y1 = REAL(XY(2)) INSIDE = X1.GT.BLC(1) .AND. X1.LT.TRC(1) .AND. : Y1.GT.BLC(2) .AND. Y1.LT.TRC(2) NP = 1 XR(1) = X1 YR(1) = Y1 PREVIN = INSIDE GETEND = .FALSE. LABLOK = IERR.NE.-J .AND. IERR.NE.-3 END IF GO TO 100 END IF DO 90 ISTEP = 1, 1000 IF (DOLBOX) THEN XY(1) = (WORLD(1) - WXY(1))/XSPAN XY(2) = (WORLD(2) - WXY(3))/YSPAN ELSE CALL NLFUNC (2, NLC, NLI, NLD, NLCPRM, NLIPRM, : NLDPRM, WORLD, XY, CONTRL, CONTXT, IERR) END IF IF (IERR.GT.0) THEN * Flush buffer. IF (NP.GT.1) CALL PGLINE(NP, XR, YR) NP = 0 GETEND = .TRUE. GO TO 100 END IF IF (NP.EQ.BUFSIZ) THEN * Recycle buffer. CALL PGLINE(NP, XR, YR) XR(1) = XR(NP) YR(1) = YR(NP) NP = 1 END IF X2 = REAL(XY(1)) Y2 = REAL(XY(2)) INSIDE = X2.GT.BLC(1) .AND. X2.LT.TRC(1) .AND. : Y2.GT.BLC(2) .AND. Y2.LT.TRC(2) IF (.NOT.INSIDE) THEN * For tick marks at the left or right edge. IF ((X2.EQ.BLC(1) .OR. X2.EQ.TRC(1)) .AND. : Y2.GT.BLC(2) .AND. Y2.LT.TRC(2)) THEN INSIDE = X2.EQ.XR(NP) END IF END IF IF (.NOT.INSIDE) THEN * For tick marks at the bottom or top edge. IF ((Y2.EQ.BLC(2) .OR. Y2.EQ.TRC(2)) .AND. : X2.GT.BLC(1) .AND. X2.LT.TRC(1)) THEN INSIDE = Y2.EQ.YR(NP) END IF END IF IF (NP.EQ.0) THEN NP = 1 XR(1) = X2 YR(1) = Y2 ELSE IF (INSIDE) THEN * This point is inside the frame... IF (.NOT.PREVIN) THEN * ...but the previous one was outside. X1 = XR(NP) Y1 = YR(NP) FSEG = 0 XPOINT = 0.0 IF (ABS(X2-X1).GT.XTOL) THEN S = (Y2-Y1)/(X2-X1) IF (XR(NP).LE.BLC(1)) THEN FSEG = 2 XR(NP) = BLC(1) XPOINT = Y1 + (XR(NP) - X1)*S YR(NP) = XPOINT ELSE IF (XR(NP).GE.TRC(1)) THEN FSEG = 4 XR(NP) = TRC(1) XPOINT = Y1 + (XR(NP) - X1)*S YR(NP) = XPOINT END IF END IF IF (ABS(Y2-Y1).GT.YTOL) THEN S = (X2-X1)/(Y2-Y1) IF (YR(NP).LE.BLC(2)) THEN FSEG = 1 YR(NP) = BLC(2) XPOINT = X1 + (YR(NP) - Y1)*S XR(NP) = XPOINT ELSE IF (YR(NP).GE.TRC(2)) THEN FSEG = 3 YR(NP) = TRC(2) XPOINT = X1 + (YR(NP) - Y1)*S XR(NP) = XPOINT END IF END IF IF (FSEG.EQ.0) THEN * The crossing is too oblique. INSIDE = .FALSE. ELSE * Record this crossing point. IF (TCODE(J,FSEG).NE.0 .AND. LABLOK) THEN IF (IC.LT.NC-1) THEN IC = IC + 1 CACHE(1,IC) = FSEG CACHE(2,IC) = XPOINT CACHE(3,IC) = J CACHE(4,IC) = WORLD(J) ELSE * Cache overflow. OVERFL = .TRUE. END IF END IF IF (TCODE(J,FSEG).GT.0) THEN * Just want tick marks. S = (XSCL*(X2-X1))**2 + (YSCL*(Y2-Y1))**2 S = SQRT(S)/TCODE(J,FSEG) IF (MAJOR) S = S/1.5 NP = NP + 1 XR(NP) = XR(NP-1) + (X2-X1)*TIKLEN/S YR(NP) = YR(NP-1) + (Y2-Y1)*TIKLEN/S CALL PGLINE(NP, XR, YR) NP = 1 END IF END IF END IF IF (INSIDE .AND. GCODE(J).EQ.2) THEN * Full grid. NP = NP + 1 END IF XR(NP) = X2 YR(NP) = Y2 ELSE * This point is outside the frame... IF (PREVIN) THEN * ...but the previous one was inside. X1 = XR(NP) Y1 = YR(NP) NP = NP + 1 XR(NP) = X2 YR(NP) = Y2 FSEG = 0 XPOINT = 0.0 IF (ABS(X2-X1).GT.XTOL) THEN S = (Y2-Y1)/(X2-X1) IF (XR(NP).LE.BLC(1)) THEN FSEG = 2 XR(NP) = BLC(1) XPOINT = Y1 + (XR(NP) - X1)*S YR(NP) = XPOINT ELSE IF (XR(NP).GE.TRC(1)) THEN FSEG = 4 XR(NP) = TRC(1) XPOINT = Y1 + (XR(NP) - X1)*S YR(NP) = XPOINT END IF END IF IF (ABS(Y2-Y1).GT.YTOL) THEN S = (X2-X1)/(Y2-Y1) IF (YR(NP).LE.BLC(2)) THEN FSEG = 1 YR(NP) = BLC(2) XPOINT = X1 + (YR(NP) - Y1)*S XR(NP) = XPOINT ELSE IF (YR(NP).GE.TRC(2)) THEN FSEG = 3 YR(NP) = TRC(2) XPOINT = X1 + (YR(NP) - Y1)*S XR(NP) = XPOINT END IF END IF IF (FSEG.EQ.0) THEN * The crossing is too oblique. INSIDE = .TRUE. IF (GCODE(J).EQ.2) THEN * Full grid. NP = NP + 1 END IF XR(NP) = X2 YR(NP) = Y2 ELSE * Record this crossing point. IF (TCODE(J,FSEG).NE.0 .AND. LABLOK) THEN IF (IC.LT.NC-1) THEN IC = IC + 1 CACHE(1,IC) = FSEG CACHE(2,IC) = XPOINT CACHE(3,IC) = J CACHE(4,IC) = WORLD(J) ELSE * Cache overflow. OVERFL = .TRUE. END IF END IF IF (TCODE(J,FSEG).GT.0) THEN * Just want tick marks. X1 = XR(NP) Y1 = YR(NP) X2 = XR(NP-1) Y2 = YR(NP-1) S = (XSCL*(X2-X1))**2 + (YSCL*(Y2-Y1))**2 S = SQRT(S)/TCODE(J,FSEG) IF (MAJOR) S = S/1.5 XR(NP-1) = X1 + (X2-X1)*TIKLEN/S YR(NP-1) = Y1 + (Y2-Y1)*TIKLEN/S END IF * Flush buffer. IF (TCODE(J,FSEG).NE.0) THEN CALL PGLINE(NP, XR, YR) END IF NP = 0 END IF ELSE * The previous point was also outside. XR(NP) = X2 YR(NP) = Y2 END IF END IF END IF PREVIN = INSIDE LABLOK = IERR.NE.-J .AND. IERR.NE.-3 IF (CONTRL.EQ.0) THEN GO TO 100 ELSE IF (CONTRL.EQ.1) THEN * Flush buffer. IF (NP.GT.1) CALL PGLINE(NP, XR, YR) NP = 0 END IF 90 CONTINUE 100 CONTINUE IF (NP.GT.1) CALL PGLINE(NP, XR, YR) 110 CONTINUE 120 CONTINUE IERR = 0 IF (OVERFL) IERR = 3 * Produce axis labels. 130 IF (LABCTL.NE.-1) CALL PGCRLB (BLC, TRC, IDENTS, FTYPE, LABCTL, : CJ, NC, IC, CACHE) * Restore the original viewport, window and pen colour. 999 CALL PGSVP (XVP1, XVP2, YVP1, YVP2) CALL PGSWIN (WXY(1), WXY(2), WXY(3), WXY(4)) CALL PGSCI (CI0) RETURN END *======================================================================= * * PGCRLB is a helper routine for PGSBOX, not meant to be called directly * since it expects the viewport and window to be scaled to the full * extent; it labels a curvilinear coordinate grid. * * Given: * BLC R(2) Cartesian coordinates of the bottom left-hand * corner. * TRC R(2) Cartesian coordinates of the top right-hand * corner. * * IDENTS C(3)*(*) Identification strings (see PGSBOX). * * FTYPE C(2)*1 Axis types, used for axis labelling (see * PGSBOX). * * LABCTL I Decimal encoded grid labelling control (see * PGSBOX). * * CI I(7) Colour table (see PGSBOX). * * Given and/or returned: * NC I Upper array index for CACHE. * * IC I Current number of entries in the CACHE table. * * CACHE D(4,0:NC) Table of points where the tick marks or grid * lines cross the frame (see PGSBOX). * * Author: Mark Calabretta, Australia Telescope National Facility *======================================================================= SUBROUTINE PGCRLB (BLC, TRC, IDENTS, FTYPE, LABCTL, CI, NC, IC, : CACHE) *----------------------------------------------------------------------- LOGICAL ANGLE, DODEG, DOMIN, DOYEAR, LFORCE, SEXA(2), TICKIT INTEGER CI(7), DOLAB(4), EDGE, EDJE, IC, ID, ID2, IM, IM2, : IMAG(2), ITER, IWRLD, IY, IY2, J, JC, K, K1, K2, KWRLD, : L, LABCTL, LD, LM, LMAG(2), LS, LV, M, M1, M2, MM, NC, : NCH, NI(2,0:4), NLAB, NLABS(2,-2:6), NSWAP, PP, : PRVDEG(2), PRVMIN(2), PRVEDG, PRVYR(2), SEXSUP(2), : SKOP(4) REAL ANGL, BLC(2), FJUST, BNDRY(4), OMAG(2), SI(2), TRC(2), : X, XBOX(4), XCH, XL, XW1, XW2, Y, YCH, YBOX(4), YL, YW1, : YW2, Z DOUBLE PRECISION CACHE(4,0:NC), MJD1(2), MJD2(2), TMP, VS CHARACTER ESCAPE*1, EXPONT*20, FMT*8, IDENTS(3)*(*), TEXT*80, : FTYPE(2)*1, TXT(2)*80 DATA ESCAPE /'\\'/ * These are to stop compiler messages about uninitialized variables. DATA DODEG, DOMIN, DOYEAR /3 * .FALSE./ DATA XL, YL /2 * -999.0/ *----------------------------------------------------------------------- * Normalize angular table entries. IF (INDEX('ABDEGH',FTYPE(1)).NE.0 .OR. : INDEX('ABDEGH',FTYPE(2)).NE.0) THEN DO 10 J = 1, IC IWRLD = NINT(CACHE(3,J)) IF (INDEX('ADG', FTYPE(IWRLD)).NE.0) THEN CACHE(4,J) = MOD(CACHE(4,J), 360D0) IF (CACHE(4,J).LT.0D0) CACHE(4,J) = CACHE(4,J) + 360D0 ELSE IF (INDEX('BEH', FTYPE(IWRLD)).NE.0) THEN CACHE(4,J) = MOD(CACHE(4,J), 360D0) IF (CACHE(4,J).LE.-180D0) THEN CACHE(4,J) = CACHE(4,J) + 360D0 ELSE IF (CACHE(4,J).GT.180D0) THEN CACHE(4,J) = CACHE(4,J) - 360D0 END IF END IF IF (INDEX('GHI', FTYPE(IWRLD)).NE.0) THEN * Angle expressed as time. CACHE(4,J) = CACHE(4,J)/15D0 END IF 10 CONTINUE END IF * Reorganize the table entries. * Sort crossings for each of the four frame segments. DO 40 ITER = 1, IC NSWAP = 0 DO 30 J = 1, IC-1 IF (CACHE(1,J).LT.CACHE(1,J+1)) GO TO 30 IF (CACHE(1,J).EQ.CACHE(1,J+1) .AND. : CACHE(2,J).LE.CACHE(2,J+1)) GO TO 30 NSWAP = NSWAP + 1 DO 20 M = 1, 4 TMP = CACHE(M,J) CACHE(M,J) = CACHE(M,J+1) CACHE(M,J+1) = TMP 20 CONTINUE 30 CONTINUE IF (NSWAP.EQ.0) GO TO 50 40 CONTINUE * Squeeze out duplicates. 50 JC = IC DO 90 J = 2, IC IF (J.GT.JC) GO TO 100 DO 60 M = 1, 4 IF (CACHE(M,J).NE.CACHE(M,J-1)) GO TO 90 60 CONTINUE * This entry is the same as the previous one. JC = JC - 1 DO 80 K = J, JC DO 70 M = 1, 4 CACHE(M,K) = CACHE(M,K+1) 70 CONTINUE 80 CONTINUE 90 CONTINUE 100 IC = JC * How do we label the edges of the frame? * Determine separability indices. NI(1,0) = 0 NI(1,1) = 0 NI(1,2) = 0 NI(1,3) = 0 NI(1,4) = 0 NI(2,0) = 0 NI(2,1) = 0 NI(2,2) = 0 NI(2,3) = 0 NI(2,4) = 0 DO 110 J = 1, IC IWRLD = NINT(CACHE(3,J)) EDGE = NINT(CACHE(1,J)) NI(IWRLD,0) = NI(IWRLD,0) + 1 NI(IWRLD,EDGE) = NI(IWRLD,EDGE) + 1 110 CONTINUE SI(1) = 0.0 SI(2) = 0.0 IF (NI(1,0).GT.0) SI(1) = 2.0*REAL(NI(1,1)+NI(1,3))/NI(1,0) - 1.0 IF (NI(2,0).GT.0) SI(2) = 2.0*REAL(NI(2,1)+NI(2,3))/NI(2,0) - 1.0 * Which coordinates go on which edges? IF (LABCTL.GT.0) THEN * User-defined. L = LABCTL ELSE * Work it out ourselves. L = 0 IF (ABS(SI(1)-SI(2)).GT.1.0) THEN * Approximately horizontal/vertical grid lines. IF (SI(1).GT.SI(2)) THEN * First world coordinate with vertical grid lines. IF (NI(1,1).GT.3 .OR. NI(1,1).GE.NI(1,3)) THEN * Label bottom of frame. L = L + 1 ELSE * Label top of frame. L = L + 100 END IF * Second world coordinate with horizontal grid lines. IF (NI(2,2).GT.3 .OR. NI(2,2).GE.NI(2,4)) THEN * Label left side of frame. L = L + 20 ELSE * Label right side of frame. L = L + 2000 END IF ELSE * First world coordinate with horizontal grid lines. IF (NI(1,2).GT.3 .OR. NI(1,2).GE.NI(1,4)) THEN * Label left side of frame. L = L + 10 ELSE * Label right side of frame. L = L + 1000 END IF * Second world coordinate with vertical grid lines. IF (NI(2,1).GT.3 .OR. NI(2,1).GE.NI(2,3)) THEN * Label bottom of frame. L = L + 2 ELSE * Label top of frame. L = L + 200 END IF END IF ELSE * Skew grid lines or worse. IF (SI(1).GT.0.5D0) THEN * First world coordinate with vertical grid lines. IF (NI(1,1).GT.3 .OR. NI(1,1).GT.NI(1,3)) THEN L = 1 ELSE L = 100 END IF IF (SI(2).GT.0.5D0) THEN * Second world coordinate also with vertical grid lines. IF (L.EQ.1) THEN L = 201 ELSE IF (NI(2,1).GT.1 .OR. NI(2,1).GT.NI(2,3)) THEN L = 102 ELSE L = 300 END IF END IF ELSE * Second world coordinate with diagonal grid lines. L = L + 2020 END IF ELSE IF (SI(1).LT.-0.5D0) THEN * First world coordinate with horizontal grid lines. IF (NI(1,2).GT.3 .OR. NI(1,2).GT.NI(1,4)) THEN L = 10 ELSE L = 1000 END IF IF (SI(2).LT.-0.5D0) THEN * Second world coordinate also with horizontal grid. IF (L.EQ.10) THEN L = 2010 ELSE IF (NI(2,2).GT.1 .OR. NI(2,2).GT.NI(2,4)) THEN L = 1020 ELSE L = 3000 END IF END IF ELSE * Second world coordinate with diagonal grid lines. L = L + 202 END IF ELSE IF (SI(2).GT.0.5D0) THEN * Second world coordinate with vertical grid lines. IF (NI(2,1).GT.3 .OR. NI(2,1).GT.NI(2,3)) THEN L = 1012 ELSE L = 1210 END IF ELSE IF (SI(2).LT.-0.5D0) THEN * Second world coordinate with horizontal grid lines. IF (NI(2,2).GT.3 .OR. NI(2,2).GT.NI(2,4)) THEN L = 121 ELSE L = 2101 END IF ELSE * Desperation stakes! Label all four axes. K1 = NI(1,3) + NI(1,1) K2 = NI(2,4) + NI(2,2) L = 2121 M1 = NI(1,4) + NI(1,1) M2 = NI(2,3) + NI(2,2) IF (M1.GE.K1 .AND. M2.GE.K2) THEN L = 1221 K1 = M1 K2 = M2 END IF M1 = NI(1,2) + NI(1,1) M2 = NI(2,4) + NI(2,3) IF (M1.GE.K1 .AND. M2.GE.K2) THEN L = 2211 K1 = M1 K2 = M2 END IF M1 = NI(1,4) + NI(1,2) M2 = NI(2,3) + NI(2,1) IF (M1.GE.K1 .AND. M2.GE.K2) THEN L = 1212 K1 = M1 K2 = M2 END IF M1 = NI(1,3) + NI(1,2) M2 = NI(2,4) + NI(2,1) IF (M1.GE.K1 .AND. M2.GE.K2) THEN L = 2112 K1 = M1 K2 = M2 END IF M1 = NI(1,4) + NI(1,3) M2 = NI(2,2) + NI(2,1) IF (M1.GE.K1 .AND. M2.GE.K2) THEN L = 1122 K1 = M1 K2 = M2 END IF END IF END IF END IF * Mark labels as unwanted by setting their edges negative. DOLAB(1) = MOD(L,10) DOLAB(2) = MOD(L/10,10) DOLAB(3) = MOD(L/100,10) DOLAB(4) = MOD(L/1000,10) DO 120 J = 1, IC EDGE = NINT(CACHE(1,J)) IWRLD = NINT(CACHE(3,J)) IF (IWRLD.EQ.1) THEN IF (MOD(DOLAB(EDGE),2).NE.1) CACHE(1,J) = -EDGE ELSE IF (MOD(DOLAB(EDGE)/2,2).NE.1) CACHE(1,J) = -EDGE END IF 120 CONTINUE * Determine labelling precision. * Order of magnitude for plain numeric world coordinates. IMAG(1) = 0 IMAG(2) = 0 IF (FTYPE(1).EQ.' ' .OR. FTYPE(2).EQ.' ') THEN OMAG(1) = 0.0 OMAG(2) = 0.0 DO 130 J = 1, IC IWRLD = NINT(CACHE(3,J)) IF (FTYPE(IWRLD).EQ.' ') THEN * Plain numeric. IF (CACHE(4,J).EQ.0D0) GO TO 130 OMAG(IWRLD) = OMAG(IWRLD) + LOG10(ABS(CACHE(4,J))) IMAG(IWRLD) = IMAG(IWRLD) + 1 END IF 130 CONTINUE IF (IMAG(1).GT.0) IMAG(1) = INT(OMAG(1)/IMAG(1)) IF (IMAG(1).GE.-2 .AND. IMAG(1).LE.4) IMAG(1) = 0 IF (IMAG(2).GT.0) IMAG(2) = INT(OMAG(2)/IMAG(2)) IF (IMAG(2).GE.-2 .AND. IMAG(2).LE.4) IMAG(2) = 0 * Renormalize grid values. IF (IMAG(1).NE.0 .OR. IMAG(2).NE.0) THEN DO 140 J = 1, IC IWRLD = NINT(CACHE(3,J)) CACHE(4,J) = CACHE(4,J)/10D0**IMAG(IWRLD) 140 CONTINUE END IF END IF * Sexagesimal labelling. SEXA(1) = INDEX('DEFGHITy', FTYPE(1)).NE.0 SEXA(2) = INDEX('DEFGHITy', FTYPE(2)).NE.0 IF (SEXA(1) .OR. SEXA(2)) THEN DO 150 K = -2, 6 NLABS(1,K) = 0 NLABS(2,K) = 0 150 CONTINUE DO 180 J = 1, IC * Use this label? EDGE = NINT(CACHE(1,J)) IF (EDGE.LT.0) GO TO 180 * Skip non-sexagesimal coordinates. IWRLD = NINT(CACHE(3,J)) IF (.NOT.SEXA(IWRLD)) GO TO 180 * Defeat rounding errors. IF (FTYPE(IWRLD).EQ.'y') THEN TMP = ABS(MOD(CACHE(4,J),1D0)*86400D0) + 5D-7 ELSE TMP = ABS(CACHE(4,J)*3600D0) + 5D-7 END IF LV = INT(MOD(TMP, 1D0)*1D6) IF (LV.NE.0) THEN * Sub-arcsec/second resolution. M = 1 DO 160 K = 1, 6 M = M*10 IF (MOD(LV,M).NE.0) THEN L = 7 - K GO TO 170 END IF 160 CONTINUE ELSE LS = INT(TMP) IF (MOD(LS,60).NE.0) THEN L = 0 ELSE IF (MOD(LS,3600).NE.0) THEN L = -1 ELSE L = -2 END IF END IF * Use CACHE(1,J) temporarily to hold L. 170 NLABS(IWRLD,L) = NLABS(IWRLD,L) + 1 CACHE(1,J) = CACHE(1,J) + 0.1 + L/100.0 180 CONTINUE * How many fields are needed to get enough labels? DO 200 IWRLD = 1, 2 NLAB = 0 DO 190 K = -2, 6 NLAB = NLAB + NLABS(IWRLD,K) IF (NLAB.GT.3 .OR. K.EQ.6) THEN LMAG(IWRLD) = K GO TO 200 END IF NLABS(IWRLD,K+1) = NLABS(IWRLD,K) + NLABS(IWRLD,K+1) 190 CONTINUE 200 CONTINUE * Disable unwanted labels. DO 210 J = 1, IC * Use this label? EDGE = NINT(CACHE(1,J)) IF (EDGE.LT.0) GO TO 210 * Skip non-sexagesimal coordinates. IWRLD = NINT(CACHE(3,J)) IF (.NOT.SEXA(IWRLD)) GO TO 210 L = NINT(100*MOD(CACHE(1,J),1.0)) - 10 IF (L.LE.LMAG(IWRLD)) THEN * Wanted. CACHE(1,J) = EDGE ELSE * Not wanted. CACHE(1,J) = -EDGE END IF 210 CONTINUE END IF * Produce labels. XW1 = BLC(1) XW2 = TRC(1) YW1 = BLC(2) YW2 = TRC(2) * These will define a box that just contains the labels. BNDRY(1) = YW1 BNDRY(2) = XW1 BNDRY(3) = YW2 BNDRY(4) = XW2 * These will record the edges on which labels were actually written. SKOP(1) = 0 SKOP(2) = 0 SKOP(3) = 0 SKOP(4) = 0 * Calendar date range. MJD1(1) = 1D99 MJD1(2) = 1D99 MJD2(1) = -1D99 MJD2(2) = -1D99 * Character height. CALL PGQCS (4, XCH, YCH) PRVEDG = 0 * Loop through the axis crossing table. DO 340 J = 1, IC * Determine the position. IWRLD = NINT(CACHE(3,J)) CALL PGSCI (CI(IWRLD+2)) EDGE = ABS(NINT(CACHE(1,J))) IF (EDGE.NE.PRVEDG) THEN * Start of new edge. IF (SEXA(1) .OR. SEXA(2)) THEN * Sexagesimal field suppression policy. PRVDEG(1) = -1 PRVMIN(1) = -1 PRVDEG(2) = -1 PRVMIN(2) = -1 SEXSUP(1) = 0 SEXSUP(2) = 0 * Vertical sides. IF (MOD(EDGE,2).EQ.0) THEN DO 220 K = J, IC EDJE = ABS(NINT(CACHE(1,K))) IF (EDJE.NE.EDGE) GO TO 230 KWRLD = NINT(CACHE(3,K)) IF (SEXSUP(KWRLD).EQ.1) GO TO 220 IF (FTYPE(KWRLD).EQ.'y') THEN TMP = ABS(MOD(CACHE(4,K),1D0)*24D0) ELSE TMP = ABS(CACHE(4,K)) END IF LV = INT(TMP*3600D0 + 5D-7) LD = LV/3600 LM = (LV - LD*3600)/60 LS = LV - LD*3600 - LM*60 TMP = TMP - LD IF (TMP.LT.5D-7) THEN * Write deg/hr field only when min/sec are zero. SEXSUP(KWRLD) = 1 ELSE IF (TMP*60-LM.LT.3D-5) THEN * Write min field only when sec is zero; only * write the deg/hr field when min is written. SEXSUP(KWRLD) = 2 END IF 220 CONTINUE END IF END IF 230 CONTINUE PRVYR(1) = -1 PRVYR(2) = -1 XL = -999.0 YL = -999.0 END IF PRVEDG = EDGE LFORCE = .FALSE. * Fix up edge encoding. EDGE = NINT(CACHE(1,J)) CACHE(1,J) = ABS(EDGE) * Use this label? IF (EDGE.LT.0) GO TO 340 IF (EDGE.EQ.1) THEN * Bottom. FJUST = 0.5 X = CACHE(2,J) Y = YW1 - 1.5*YCH ELSE IF (EDGE.EQ.2) THEN * Left. FJUST = 1.0 X = XW1 - 0.5*XCH Y = CACHE(2,J) - YCH/2.0 ELSE IF (EDGE.EQ.3) THEN * Top. FJUST = 0.5 X = CACHE(2,J) Y = YW2 + 0.5*YCH ELSE IF (EDGE.EQ.4) THEN * Right. FJUST = 0.0 X = XW2 + 0.5*XCH Y = CACHE(2,J) - YCH/2.0 END IF * Format the numeric label. IF (INDEX('ABC', FTYPE(IWRLD)).NE.0) THEN * Decimal angle; allow up to 6 decimal digits. TMP = ABS(CACHE(4,J)) + 5D-7 LD = INT(TMP) K = 1 IF (CACHE(4,J).LT.0D0) THEN * Insert a minus sign. TEXT(1:1) = '-' K = 2 END IF CALL PGNUMB (LD, 0, 1, TEXT(K:), NCH) K = K + NCH TEXT(K:) = ESCAPE // 'uo' // ESCAPE // 'd' K = K + 4 LV = INT(MOD(TMP,1D0)*1D6) IF (LV.NE.0) CALL PGNUMB (LV, -6, 1, TEXT(K:), NCH) TEXT(K:K) = 'd' ELSE IF (SEXA(IWRLD)) THEN * Sexagesimal format; angle or time? ANGLE = INDEX('DEF', FTYPE(IWRLD)).NE.0 L = LMAG(IWRLD) * Use integer arithmetic to avoid rounding problems. IF (FTYPE(IWRLD).EQ.'y') THEN TMP = ABS(MOD(CACHE(4,J),1D0)*24D0) * Determine date range. IF (CACHE(4,J).LT.MJD1(IWRLD)) MJD1(IWRLD) = CACHE(4,J) IF (CACHE(4,J).GT.MJD2(IWRLD)) MJD2(IWRLD) = CACHE(4,J) ELSE TMP = ABS(CACHE(4,J)) END IF VS = TMP*3600D0 + 5D-7 LV = INT(VS) * Sexagesimal fields. LD = LV/3600 LM = (LV - LD*3600)/60 LS = LV - LD*3600 - LM*60 * Field suppression policy. IF (SEXSUP(IWRLD).GT.0) THEN TMP = TMP - LD IF (TMP.LT.5D-7) THEN DODEG = .TRUE. DOMIN = .TRUE. ELSE IF (SEXSUP(IWRLD).EQ.2) THEN DOMIN = TMP*60-LM.LT.3D-5 DODEG = DOMIN .AND. LD.NE.PRVDEG(IWRLD) ELSE DODEG = .FALSE. DOMIN = .FALSE. END IF ELSE DODEG = LD.NE.PRVDEG(IWRLD) DOMIN = LM.NE.PRVMIN(IWRLD) END IF K = 1 IF (L.EQ.-2 .OR. DODEG) THEN * Write the degree/hour field. DODEG = .TRUE. IF (CACHE(4,J).LT.0D0) THEN * Insert a minus sign. TEXT(1:1) = '-' K = 2 END IF IF (ANGLE) THEN * Angle. CALL PGNUMB (LD, 0, 1, TEXT(K:), NCH) K = K + NCH TEXT(K:) = ESCAPE // 'uo' // ESCAPE // 'd' K = K + 5 ELSE * Time. IF (LD.LE.9 .AND. INDEX('Ty',FTYPE(IWRLD)).EQ.0) THEN * Write leading zeroes in the hour field. WRITE (TEXT(K:), '(I2.2)') LD K = K + 2 ELSE CALL PGNUMB (LD, 0, 1, TEXT(K:), NCH) K = K + NCH END IF TEXT(K:) = ESCAPE // 'uh' // ESCAPE // 'd' K = K + 5 END IF END IF IF (L.GE.-1 .AND. : .NOT.(L.LE.0 .AND. K.GT.1 .AND. LM.EQ.0 .AND. LS.EQ.0)) THEN * Write arcminute/minute field. IF (L.EQ.-1 .OR. K.GT.1 .OR. DOMIN) THEN DOMIN = .TRUE. IF (ANGLE) THEN WRITE (TEXT(K:), '(I2.2,A)') LM, '''' K = K + 3 ELSE WRITE (TEXT(K:), '(I2.2,A)') LM, : ESCAPE // 'um' // ESCAPE // 'd' K = K + 7 END IF END IF IF (L.GE.0) THEN * Arcsec/second field. IF (ANGLE) THEN WRITE (TEXT(K:), '(I2.2,A)') LS, '"' K = K + 3 ELSE WRITE (TEXT(K:), '(I2.2,A)') LS, : ESCAPE // 'us' // ESCAPE // 'd' K = K + 7 END IF IF (L.GT.0) THEN * Sub-arcsec/second field. WRITE (FMT, '(A,I1,A,I1,A)') '(A,I', L, '.', L, ')' LV = INT(MOD(VS,1D0)*10**L) WRITE (TEXT(K:), FMT) '.', LV END IF END IF END IF ELSE IF (FTYPE(IWRLD).EQ.'L') THEN * Logarithmic. TMP = MOD(CACHE(4,J),1D0) IF (TMP.LT.0D0) TMP = TMP + 1D0 MM = NINT(10D0**TMP) IF (MM.EQ.10) THEN TMP = TMP - 1D0 MM = 1 END IF PP = NINT(CACHE(4,J) - TMP) IF (MM.NE.1) THEN WRITE (TEXT, '(I1)') MM ELSE * FORTRAN is really abysmal sometimes. WRITE (TEXT, '(I8)') PP DO 240 K = 1, 8 IF (TEXT(K:K).NE.' ') GO TO 250 240 CONTINUE 250 TEXT = '10' // ESCAPE // 'u' // TEXT(K:8) LFORCE = .TRUE. END IF ELSE IF (FTYPE(IWRLD).EQ.'Y') THEN * Convert MJD to Gregorian calendar date, YYYY/MM/DD. CALL PGMJD(0, CACHE(4,J), IY, IM, ID) DOYEAR = IY.NE.PRVYR(IWRLD) IF (DOYEAR) THEN WRITE (TEXT, 260) IY, IM, ID 260 FORMAT (I12,'/',I2.2,'/',I2.2) DO 270 K = 1, 12 IF (TEXT(K:K).NE.' ') GO TO 280 270 CONTINUE 280 TEXT = TEXT(K:18) ELSE WRITE (TEXT, 290) IM, ID 290 FORMAT (I2.2,'/',I2.2) END IF ELSE * Plain number; allow up to six significant digits. IF (CACHE(4,J).NE.0D0) THEN PP = INT(LOG10(ABS(CACHE(4,J)))) - 6 MM = NINT(CACHE(4,J)/10D0**PP) ELSE PP = 0 MM = 0 END IF CALL PGNUMB (MM, PP, 0, TEXT, NCH) END IF * Write the label if it doesn't overlap the previous one. CALL PGQTXT (X, Y, 0.0, FJUST, TEXT, XBOX, YBOX) IF (LFORCE .OR. XBOX(1).GT.XL .OR. YBOX(1).GT.YL) THEN IF (IWRLD.EQ.1) THEN CALL PGSCI (CI(3)) ELSE CALL PGSCI (CI(4)) END IF CALL PGPTXT (X, Y, 0.0, FJUST, TEXT) XL = XBOX(4) + 0.5*XCH YL = YBOX(2) + 0.5*YCH * Sexagesimal formatting. IF (SEXA(IWRLD)) THEN IF (DODEG) PRVDEG(IWRLD) = LD IF (DOMIN) PRVMIN(IWRLD) = LM END IF * Calendar formatting. IF (FTYPE(IWRLD).EQ.'Y') THEN IF (DOYEAR) PRVYR(IWRLD) = IY END IF * Record the fact. IF (IWRLD.EQ.1) THEN SKOP(EDGE) = 2*(SKOP(EDGE)/2) + 1 ELSE SKOP(EDGE) = 2 + MOD(SKOP(EDGE),2) END IF * Boundary within which the numeric labels lie. IF (YBOX(1).LT.BNDRY(1)) BNDRY(1) = YBOX(1) IF (XBOX(1).LT.BNDRY(2)) BNDRY(2) = XBOX(1) IF (YBOX(3).GT.BNDRY(3)) BNDRY(3) = YBOX(3) IF (XBOX(3).GT.BNDRY(4)) BNDRY(4) = XBOX(3) * Check the distance to the previous grid line. TICKIT = .FALSE. K = J - 1 IF (DOLAB(EDGE).NE.3) THEN * Only one coordinate element labelled on this edge, no need * to worry about grid lines belonging to the other. DO 300 K = J-1, 1, -1 IF (IWRLD.EQ.NINT(CACHE(3,K))) GO TO 310 300 CONTINUE END IF 310 IF (K.GE.1) THEN EDJE = ABS(NINT(CACHE(1,K))) IF (EDJE.EQ.EDGE) THEN IF (EDGE.EQ.1 .OR. EDGE.EQ.3) THEN IF (XBOX(1).LT.CACHE(2,K)) TICKIT = .TRUE. ELSE IF (YBOX(1).LT.CACHE(2,K)) TICKIT = .TRUE. END IF END IF END IF * Check the distance to the next grid line. K = J + 1 IF (DOLAB(EDGE).NE.3) THEN * Only one coordinate element labelled on this edge, no need * to worry about grid lines belonging to the other. DO 320 K = J+1, IC IF (IWRLD.EQ.NINT(CACHE(3,K))) GO TO 330 320 CONTINUE END IF 330 IF (K.LE.IC) THEN EDJE = ABS(NINT(CACHE(1,K))) IF (EDJE.EQ.EDGE) THEN IF (EDGE.EQ.1 .OR. EDGE.EQ.3) THEN IF (XBOX(3).GT.CACHE(2,K)) TICKIT = .TRUE. ELSE IF (YBOX(3).GT.CACHE(2,K)) TICKIT = .TRUE. END IF END IF END IF * Density of grid lines is high. IF (TICKIT) THEN * Draw outside pip mark to disambiguate grid lines. Z = REAL(CACHE(2,J)) IF (EDGE.EQ.1) THEN CALL PGMOVE (Z, YW1-0.3*YCH) CALL PGDRAW (Z, YW1) ELSE IF (EDGE.EQ.2) THEN CALL PGMOVE (XW1-0.3*XCH, Z) CALL PGDRAW (XW1, Z) ELSE IF (EDGE.EQ.3) THEN CALL PGMOVE (Z, YW2+0.3*YCH) CALL PGDRAW (Z, YW2) ELSE IF (EDGE.EQ.4) THEN CALL PGMOVE (XW2+0.3*XCH, Z) CALL PGDRAW (XW2, Z) END IF END IF END IF 340 CONTINUE * Write the identification strings. * World coordinates. DO 470 EDGE = 1, 4 TEXT = ' ' DO 440 IWRLD = 1, 2 TXT(IWRLD) = ' ' IF (MOD(SKOP(EDGE)/IWRLD,2).EQ.0) GO TO 440 * Strip off leading blanks. L = LEN(IDENTS(IWRLD)) DO 350 K = 1, L IF (IDENTS(IWRLD)(K:K).NE.' ') THEN TXT(IWRLD) = IDENTS(IWRLD)(K:L) GO TO 360 END IF 350 CONTINUE 360 IF (IMAG(IWRLD).NE.0 .OR. FTYPE(IWRLD).EQ.'y') THEN * Find the last non-blank. DO 370 K = 40, 1, -1 IF (TXT(IWRLD)(K:K).NE.' ') GO TO 380 370 CONTINUE 380 K = K + 1 IF (IMAG(IWRLD).NE.0) THEN * Add scaling information. CALL PGNUMB (IMAG(IWRLD), 0, 1, EXPONT, NCH) TXT(IWRLD)(K:) = ' x10' // ESCAPE // 'u' // EXPONT ELSE * Add calendar date range. CALL PGMJD(0, MJD1(IWRLD), IY, IM, ID) WRITE (TEXT, 390) IY, IM, ID 390 FORMAT (I12,'/',I2.2,'/',I2.2) DO 400 L = 1, 12 IF (TEXT(L:L).NE.' ') GO TO 410 400 CONTINUE 410 TXT(IWRLD)(K:) = ' (' // TEXT(L:18) K = K + 21 - L CALL PGMJD(0, MJD2(IWRLD), IY2, IM2, ID2) WRITE (TEXT, 390) IY2, IM2, ID2 IF (IY2.EQ.IY) THEN IF (IM2.EQ.IM) THEN IF (ID2.EQ.ID) THEN TXT(IWRLD)(K:) = ')' ELSE TXT(IWRLD)(K:) = ' - ' // TEXT(17:18) // ')' END IF ELSE TXT(IWRLD)(K:) = ' - ' // TEXT(14:18) // ')' END IF ELSE DO 420 L = 1, 12 IF (TEXT(L:L).NE.' ') GO TO 430 420 CONTINUE 430 TXT(IWRLD)(K:) = ' - ' // TEXT(L:18) // ')' END IF END IF END IF 440 CONTINUE K = 0 IF (TXT(1).NE.' ') THEN * Identify first world coordinate... TEXT = TXT(1) CALL PGSCI (CI(5)) IF (TXT(2).NE.' ') THEN * ...and also second world coordinate. DO 450 K = 40, 1, -1 IF (TEXT(K:K).NE.' ') GO TO 460 450 CONTINUE 460 K = K + 1 TEXT(K:) = ', ' // TXT(2) END IF ELSE IF (TXT(2).NE.' ') THEN * Identify second world coordinate only. TEXT = TXT(2) CALL PGSCI (CI(6)) ELSE * No text to write. GO TO 470 END IF IF (EDGE.EQ.1) THEN X = (XW1 + XW2)/2.0 Y = BNDRY(1) - 1.5*YCH ANGL = 0.0 ELSE IF (EDGE.EQ.2) THEN IF (TEXT(2:).EQ.' ') THEN * One character, write upright. X = BNDRY(2) - 1.0*XCH Y = (YW1 + YW2)/2.0 ANGL = 0.0 ELSE X = BNDRY(2) - 0.5*XCH Y = (YW1 + YW2)/2.0 ANGL = 90.0 END IF ELSE IF (EDGE.EQ.3) THEN X = (XW1 + XW2)/2.0 Y = BNDRY(3) + 0.5*YCH ANGL = 0.0 ELSE IF (EDGE.EQ.4) THEN IF (TEXT(2:).EQ.' ') THEN * One character, write upright. X = BNDRY(4) + 1.0*XCH Y = (YW1 + YW2)/2.0 ANGL = 0.0 ELSE X = BNDRY(4) + 0.5*XCH Y = (YW1 + YW2)/2.0 ANGL = -90.0 END IF END IF CALL PGQTXT (X, Y, ANGL, 0.5, TEXT, XBOX, YBOX) IF (K.EQ.0) THEN CALL PGPTXT (X, Y, ANGL, 0.5, TEXT) ELSE * Two-colour annotation. CALL PGPTXT (XBOX(1), YBOX(1), ANGL, 0.0, TEXT(:K)) CALL PGSCI (CI(6)) CALL PGPTXT (XBOX(4), YBOX(4), ANGL, 1.0, TEXT(K+1:)) END IF * Update the boundary. IF (YBOX(1).LT.BNDRY(1)) BNDRY(1) = YBOX(1) IF (YBOX(3).LT.BNDRY(1)) BNDRY(1) = YBOX(3) IF (XBOX(1).LT.BNDRY(2)) BNDRY(2) = XBOX(1) IF (XBOX(3).LT.BNDRY(2)) BNDRY(2) = XBOX(3) IF (YBOX(1).GT.BNDRY(3)) BNDRY(3) = YBOX(1) IF (YBOX(3).GT.BNDRY(3)) BNDRY(3) = YBOX(3) IF (XBOX(1).GT.BNDRY(4)) BNDRY(4) = XBOX(1) IF (XBOX(3).GT.BNDRY(4)) BNDRY(4) = XBOX(3) 470 CONTINUE * Title. IF (IDENTS(3).NE.' ') THEN CALL PGSCI (CI(7)) X = (XW1 + XW2)/2.0 Y = BNDRY(3) + 0.5*YCH CALL PGQTXT (X, Y, 0.0, 0.5, IDENTS(3), XBOX, YBOX) CALL PGPTXT (X, Y, 0.0, 0.5, IDENTS(3)) * Update the boundary. IF (XBOX(1).LT.BNDRY(2)) BNDRY(2) = XBOX(1) IF (YBOX(3).GT.BNDRY(3)) BNDRY(3) = YBOX(3) IF (XBOX(3).GT.BNDRY(4)) BNDRY(4) = XBOX(3) END IF * Return margin widths in Cartesian coordinates. CACHE(1,NC) = YW1 - BNDRY(1) CACHE(2,NC) = XW1 - BNDRY(2) CACHE(3,NC) = BNDRY(3) - YW2 CACHE(4,NC) = BNDRY(4) - XW2 RETURN END *======================================================================= * MJD to/from Gregorian calendar date. * * Given: * CODE I If 1, compute MJD from IY,IM,ID, else vice * versa. * * Given and/or returned: * MJD D Modified Julian date, (MJD = JD - 2400000.5). * IY I Year. * IM I Month (for CODE.EQ.1 may exceed 12, or be zero, * or negative). * ID I Day of month (for CODE.EQ.1, may exceed the * legitimate number of days in the month, or be * zero, or negative). * * Notes: * These algorithms are from D.A. Hatcher, QJRAS 25, 53-55, as modified * by P.T. Wallace for use in SLALIB (subroutines CLDJ and DJCL). * * Author: Mark Calabretta, Australia Telescope National Facility *----------------------------------------------------------------------- SUBROUTINE PGMJD (CODE, MJD, IY, IM, ID) *----------------------------------------------------------------------- INTEGER CODE, DD, ID, IM, IY, JD, JM, JY, N4 DOUBLE PRECISION MJD *----------------------------------------------------------------------- IF (CODE.EQ.1) THEN * Calendar date to MJD. IF (IM.LT.1) THEN JY = IY - 1 + IM/12 JM = 12 + MOD(IM,12) ELSE JY = IY + (IM-1)/12 JM = MOD(IM-1,12) + 1 END IF MJD =DBLE((1461*(JY - (12-JM)/10 + 4712))/4 : +(306*MOD(JM+9, 12) + 5)/10 : -(3*((JY - (12-JM)/10 + 4900)/100))/4 : + ID - 2399904) ELSE * MJD to calendar date. JD = 2400001 + INT(MJD) N4 = 4*(JD + ((2*((4*JD - 17918)/146097)*3)/4 + 1)/2 - 37) DD = 10*(MOD(N4-237, 1461)/4) + 5 IY = N4/1461 - 4712 IM = MOD(2 + DD/306, 12) + 1 ID = MOD(DD, 306)/10 + 1 END IF RETURN END *======================================================================= * This FORTRAN wrapper on PGSBOX exists solely to define fixed-length * CHARACTER arguments for cpgsbox(). * * Author: Mark Calabretta, Australia Telescope National Facility *----------------------------------------------------------------------- SUBROUTINE PGSBOK (BLC, TRC, IDENTS, OPT, LABCTL, LABDEN, CI, : GCODE, TIKLEN, NG1, GRID1, NG2, GRID2, DOEQ, NLFUNC, NLC, NLI, : NLD, NLCPRM, NLIPRM, NLDPRM, NC, IC, CACHE, IERR) *----------------------------------------------------------------------- LOGICAL DOEQ INTEGER CI(7), GCODE(2), IC, IERR, LABCTL, LABDEN, NC, NG1, NG2, : NLC, NLD, NLI, NLIPRM(NLI) REAL BLC(2), TRC(2) DOUBLE PRECISION CACHE(4,0:NC), GRID1(0:NG1), GRID2(0:NG2), : NLDPRM(NLD), TIKLEN CHARACTER IDENTS(3)*80, NLCPRM(NLC)*1, OPT(2)*1 EXTERNAL NLFUNC *----------------------------------------------------------------------- CALL PGSBOX (BLC, TRC, IDENTS, OPT, LABCTL, LABDEN, CI, GCODE, : TIKLEN, NG1, GRID1, NG2, GRID2, DOEQ, NLFUNC, NLC, NLI, NLD, : NLCPRM, NLIPRM, NLDPRM, NC, IC, CACHE, IERR) RETURN END *======================================================================= * This FORTRAN wrapper on PGLBOX exists solely to define fixed-length * CHARACTER arguments for cpglbox(). * * Author: Mark Calabretta, Australia Telescope National Facility *----------------------------------------------------------------------- SUBROUTINE PGLBOK (IDENTS, OPT, LABCTL, LABDEN, CI, GCODE, TIKLEN, : NG1, GRID1, NG2, GRID2, DOEQ, NC, IC, CACHE, IERR) *----------------------------------------------------------------------- LOGICAL DOEQ INTEGER CI(7), GCODE(2), IC, IERR, LABCTL, LABDEN, NC, NG1, NG2 DOUBLE PRECISION CACHE(4,0:NC), GRID1(0:NG1), GRID2(0:NG2), TIKLEN CHARACTER IDENTS(3)*80, OPT(2)*1 *----------------------------------------------------------------------- CALL PGLBOX (IDENTS, OPT, LABCTL, LABDEN, CI, GCODE, TIKLEN, NG1, : GRID1, NG2, GRID2, DOEQ, NC, IC, CACHE, IERR) RETURN END pywcs-1.12/wcslib/pgsbox/pgtest.f0000644001153600020070000012115612310355626021116 0ustar cslocumSTSCI\science00000000000000*======================================================================= * * PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. * Copyright (C) 1997-2012, Mark Calabretta * * This file is part of PGSBOX. * * PGSBOX is free software: you can redistribute it and/or modify it * under the terms of the GNU Lesser General Public License as published * by the Free Software Foundation, either version 3 of the License, or * (at your option) any later version. * * PGSBOX is distributed in the hope that it will be useful, but WITHOUT * ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or * FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public * License for more details. * * You should have received a copy of the GNU Lesser General Public * License along with PGSBOX. If not, see http://www.gnu.org/licenses. * * Correspondence concerning PGSBOX may be directed to: * Internet email: mcalabre@atnf.csiro.au * Postal address: Dr. Mark Calabretta * Australia Telescope National Facility, CSIRO * PO Box 76 * Epping NSW 1710 * AUSTRALIA * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: pgtest.f,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *======================================================================= PROGRAM PGTEST *======================================================================= LOGICAL LARGE INTEGER C0(7), CI(7), GCODE(2), IC, IERR, J, NAXIS(2), : NLIPRM(2), STATUS REAL BLC(2), SCL, TRC(2) DOUBLE PRECISION CACHE(4,0:256), DEC0, GRID1(0:8), GRID2(0:8), : NLDPRM(8), ROTN, TIKLEN CHARACTER CTYPE(2)*72, DEVTYP*16, ESCAPE*1, FCODE(2)*4, : IDENTS(3)*80, NLCPRM(1)*1, OPT(2)*1 DOUBLE PRECISION D2R, PI PARAMETER (PI = 3.141592653589793238462643D0) PARAMETER (D2R = PI/180D0) INCLUDE 'wcs.inc' INTEGER WCS(WCSLEN) EXTERNAL LNGVEL EXTERNAL FSCAN EXTERNAL PGCRFN EXTERNAL PGWCSL * A portability fix - does '\' itself need to be escaped? DATA ESCAPE /'\\'/ *----------------------------------------------------------------------- * Setup. NAXIS(1) = 512 NAXIS(2) = 512 BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = NAXIS(1) + 0.5 TRC(2) = NAXIS(2) + 0.5 * CALL PGBEG (0, '?', 1, 1) call pgbeg (0, '/xw', 1, 1) CALL PGQINF ('TYPE', DEVTYP, J) IF (DEVTYP.EQ.'PS' .OR. : DEVTYP.EQ.'VPS' .OR. : DEVTYP.EQ.'CPS' .OR. : DEVTYP.EQ.'VCPS') THEN * Switch black and white. CALL PGSCR (0, 1.0, 1.0, 1.0) CALL PGSCR (1, 0.0, 0.0, 0.0) END IF LARGE = DEVTYP.EQ.'XWINDOW' IF (LARGE) THEN SCL = 1.0 CALL PGVSTD () ELSE SCL = 0.7 CALL PGVSIZ (1.0, 3.0, 1.0, 3.0) END IF * Yellow. CALL PGSCR (2, 1.0, 1.0, 0.0) * White. CALL PGSCR (3, 1.0, 1.0, 1.0) * Pale blue. CALL PGSCR (4, 0.5, 0.5, 0.8) * Pale red. CALL PGSCR (5, 0.8, 0.5, 0.5) * Grey. CALL PGSCR (6, 0.7, 0.7, 0.7) * Dark green. CALL PGSCR (7, 0.3, 0.5, 0.3) C0(1) = -1 C0(2) = -1 C0(3) = -1 C0(4) = -1 C0(5) = -1 C0(6) = -1 C0(7) = -1 CALL PGWNAD (0.0, 1.0, 0.0, 1.0) CALL PGASK (.TRUE.) CALL PGPAGE () STATUS = WCSPUT (WCS, WCS_FLAG, -1, 0, 0) *----------------------------------------------------------------------- * Longitude-velocity map; the y-axis is regularly spaced in * frequency but is to be labelled as a true relativistic velocity. * - PGSBOX uses subroutine LNGVEL. * - Separable (i.e. orthogonal), non-linear coordinate system. * - Automatic choice of coordinate increments. * - Extraction of a common scaling factor. * - Automatic choice of what edges to label. * - Request for tickmarks (internal) for one coordinate and grid * lines for the other. * - Simple two-colour grid using two calls with deferred * labelling on the first call. * - Degree labelling. * - Suppression of zero arcmin and arcsec fields in sexagesimal * degree format. WRITE (*, '(/,A)') 'Longitude-velocity map' * Reference pixel coordinates. NLDPRM(1) = 1D0 NLDPRM(2) = 256D0 * Reference pixel values. NLDPRM(3) = 0D0 NLDPRM(4) = 1.420D9 * Coordinate increments. NLDPRM(5) = 360D0/(NAXIS(1)-1) NLDPRM(6) = 4D6 * Rest frequency. NLDPRM(7) = 1.420D9 * Annotation. IDENTS(1) = 'galactic longitude' IDENTS(2) = 'velocity (m/s)' IDENTS(3) = 'HI line' OPT(1) = 'F' OPT(2) = ' ' * Normal size lettering. CALL PGSCH (1.0*SCL) * Yellow tick marks for longitude and grid lines for velocity. CALL PGSCI (2) GCODE(1) = 1 GCODE(2) = 2 * Defer labelling. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 2D0, 0, 0D0, : 0, 0D0, .FALSE., LNGVEL, 1, 1, 7, ' ', 0, NLDPRM, 256, IC, : CACHE, IERR) * Draw fiducial grid lines in white and do labelling. CALL PGSCI (1) GCODE(1) = 2 GCODE(2) = 2 GRID1(1) = 180D0 GRID2(1) = 0D0 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 0, C0, GCODE, 0D0, 1, : GRID1, 1, GRID2, .FALSE., LNGVEL, 1, 1, 7, ' ', 0, NLDPRM, 256, : IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Azimuth-frequency scan; this sort of output might be obtained from * an antenna that scans in azimuth with a receiver that scans * simultaneously in frequency. * - PGSBOX uses subroutine FSCAN. * - Non-separable (i.e. non-orthogonal) non-linear coordinate * system. * - Automatic choice of what edges to label; results in labelling * the bottom, left and right sides of the plot. * - Cyclic labelling. FSCAN returns the azimuth in the range * 0 - 720 degrees but PGSBOX is set to normalize this to two * cycles of 0 - 360 degrees. * - Logarithmic labelling. * - Automatic choice of coordinate increments but with request * for all grid lines for the logarithmic coordinate. * - Degree labelling. * - Suppression of common zero arcmin and arcsec fields in * sexagesimal degree format. WRITE (*, '(/,A)') 'Azimuth-frequency scan' * Reference pixel coordinates. NLDPRM(1) = 0.5D0 NLDPRM(2) = 0.5D0 * Reference pixel values. NLDPRM(3) = 0D0 NLDPRM(4) = 8.5D0 * Coordinate increments. NLDPRM(5) = 720D0/(NAXIS(1)+1) NLDPRM(6) = 0.002D0 * Rate of change of NLDPRM(4) with x-pixel. NLDPRM(7) = -0.002D0 * Annotation. IDENTS(1) = 'azimuth' IDENTS(2) = ESCAPE // 'gn/Hz' IDENTS(3) = 'Frequency/azimuth scan' OPT(1) = 'D' OPT(2) = 'L' * Normal size lettering. CALL PGSCH (1.0*SCL) * Draw full grid lines. CALL PGSCI (1) GCODE(1) = 2 GCODE(2) = 2 * Setting LABDEN = 9900 forces all logarithmic grid lines to be * drawn. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 9900, C0, GCODE, 2D0, 0, : 0D0, 0, 0D0, .FALSE., FSCAN, 1, 1, 7, ' ', 0, NLDPRM, 256, IC, : CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Z versus time plot. * - PGSBOX uses subroutine PGCRFN. * - Separable (i.e. orthogonal), non-linear coordinate system. * - Use of function PGCRFN for separable axis types. * - Automatic choice of what edges to label; results in labelling * the bottom and left sides of the plot. * - Automatic choice of coordinate increments. * - Logarithmic labelling over many orders of magnitude. * - Single-character annotation on a vertical axis is upright. WRITE (*, '(/,A)') 'Z versus time plot' * Function types. FCODE(1) = 'Lin ' FCODE(2) = 'Log ' * Reference pixel coordinates. NLDPRM(1) = 0.5D0 NLDPRM(2) = -50D0 * Coordinate increments. NLDPRM(3) = 0.04D0 NLDPRM(4) = 0.02D0 * Reference pixel values. NLDPRM(5) = -3.0D0 NLDPRM(6) = 1.0D0 * Annotation. IDENTS(1) = 'Age of universe (sec)' IDENTS(2) = 'Y' IDENTS(3) = ' ' OPT(1) = 'L' OPT(2) = ' ' * Normal size lettering. CALL PGSCH (1.0*SCL) * Draw ticks for the first coordinate, grid lines for the second. CALL PGSCI (1) GCODE(1) = 1 GCODE(2) = 2 IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 0, C0, GCODE, 2D0, 0, 0D0, : 0, 0D0, .FALSE., PGCRFN, 8, 2, 4, FCODE, NLIPRM, NLDPRM, 256, : IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Simple SIN projection near the south celestial pole. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate * system. * - Demonstrate parameter definition for PGWCSL. * - Discovery of grid lines that do not cross any axis. * - Automatic choice of what edges to label; results in labelling * all sides of the plot. * - Automatic choice of coordinate increments but with request * for increased grid density for each coordinate. * - Double precision accuracy. * - Cyclic coordinates. PGWCSL returns the right ascension in * the range -180 to +180 degrees, i.e. with a discontinuity * at +/- 180 degrees. * - Labelling of degrees as time in the range 0 - 24h. * - Suppression of labels that would overlap one another. * - Sexagesimal degree labelling with automatically determined * precision. * - Suppression of common zero minute and second fields in * sexagesimal time format. WRITE (*, '(/,A)') 'Simple SIN projection' STATUS = WCSINI (2, WCS) * Set projection type to SIN. CTYPE(1) = 'RA---SIN' CTYPE(2) = 'DEC--SIN' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 384D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 256D0, 2, 0) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, -1D0/3600000D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0/3600000D0, 2, 0) * Spherical coordinate references. DEC0 = -89.99995D0 STATUS = WCSPUT (WCS, WCS_CRVAL, 25D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, DEC0, 2, 0) * Set parameters for an NCP projection. DEC0 = DEC0*D2R STATUS = WCSPUT (WCS, WCS_PV, 0D0, 2, 1) STATUS = WCSPUT (WCS, WCS_PV, COS(DEC0)/SIN(DEC0), 2, 2) * Annotation. IDENTS(1) = 'Right ascension' IDENTS(2) = 'Declination' IDENTS(3) = 'WCS SIN projection' OPT(1) = 'G' OPT(2) = 'E' * Reduced size lettering. CALL PGSCH (0.8*SCL) * Draw full grid lines. CALL PGSCI (1) GCODE(1) = 2 GCODE(2) = 2 * Draw the celestial grid. The grid density is set for each world * coordinate by specifying LABDEN = 1224. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 1224, C0, GCODE, 0D0, 0, : 0D0, 0, 0D0, .FALSE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Conic equal area projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate * system. * - Coordinate system undefined in areas of the plot. * - Demonstrate parameter definition for PGWCSL. * - Discontinuous grid lines handled by PGWCSL. * - Discovery of grid lines that do not cross any axis. * - Colour control for grid and labelling. * - Reduced size lettering. * - Automatic choice of what edges to label; results in labelling * all sides of the plot. * - Automatic choice of coordinate increments. * - Cyclic coordinates. PGWCSL returns the longitude in the * range -180 to +180 degrees, i.e. with a discontinuity at * +/- 180 degrees. * - Suppression of labels that would overlap one another. * - Suppression of common zero arcmin and arcsec fields in * sexagesimal degree format. WRITE (*, '(/,A)') 'Conic equal area projection' STATUS = WCSINI (2, WCS) * Set projection type to conic equal-area. CTYPE(1) = 'RA---COE' CTYPE(2) = 'DEC--COE' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 256D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 256D0, 2, 0) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, -1D0/3D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0/3D0, 2, 0) * Spherical coordinate references. STATUS = WCSPUT (WCS, WCS_CRVAL, 90D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 30D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, 150D0, 0, 0) * Middle latitude and offset from standard parallels. STATUS = WCSPUT (WCS, WCS_PV, 60D0, 2, 1) STATUS = WCSPUT (WCS, WCS_PV, 15D0, 2, 2) * Annotation. IDENTS(1) = 'longitude' IDENTS(2) = 'latitude' IDENTS(3) = 'WCS conic equal area projection' OPT(1) = 'E' OPT(2) = 'E' * Reduced size lettering. CALL PGSCH (0.8*SCL) * Draw full grid lines. GCODE(1) = 2 GCODE(2) = 2 * Use colour to associate grid lines and labels. * Meridians in red. CALL PGSCR (10, 0.5, 0.0, 0.0) * Parallels in blue. CALL PGSCR (11, 0.0, 0.2, 0.5) * Longitudes in red. CALL PGSCR (12, 0.8, 0.3, 0.0) * Latitudes in blue. CALL PGSCR (13, 0.0, 0.4, 0.7) * Longitude labels in red. CALL PGSCR (14, 0.8, 0.3, 0.0) * Latitude labels in blue. CALL PGSCR (15, 0.0, 0.4, 0.7) * Title in cyan. CALL PGSCR (16, 0.3, 1.0, 1.0) CI(1) = 10 CI(2) = 11 CI(3) = 12 CI(4) = 13 CI(5) = 14 CI(6) = 15 CI(7) = 16 * Draw the celestial grid letting PGSBOX choose the increments. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 0, CI, GCODE, 0D0, 0, 0D0, : 0, 0D0, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, NLDPRM, 256, : IC, CACHE, IERR) * Set parameters to draw the native grid. STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 60D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, 999D0, 0, 0) STATUS = WCSPUT (WCS, WCS_LATPOLE, 999D0, 0, 0) * We just want to delineate the boundary, in green. CALL PGSCI (7) GRID1(1) = -180D0 GRID1(2) = 180D0 GRID2(1) = -90D0 GRID2(2) = 90D0 IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 0D0, 2, : GRID1, 2, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the frame. CALL PGSCI (1) CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Polyconic projection with colour-coded grid. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate * system. * - Coordinate system undefined in areas of the plot. * - Demonstrate parameter definition for PGWCSL. * - Discontinuous grid lines handled by PGWCSL. * - Colour coded labelling. * - Colour coded grid implemented by the caller. * - Basic management of the axis-crossing table (see code). * - Reduced size lettering. * - Tick marks external to the frame. * - User selection of what edges to label with request for both * coordinates to be labelled on bottom, left and top edges. * - User selection of grid lines to plot. * - Concatenation of annotation at bottom and left; automatically * suppressed at the top since only one coordinate is labelled * there. * - Suppression of labels that would overlap one another. * - Degree labelling. * - Labelling of degrees as time in the range -12 - +12h. * - Suppression of common zero minute and second fields in * sexagesimal time format. WRITE (*, '(/,A)') 'Polyconic projection with colour-coded grid' STATUS = WCSINI (2, WCS) * Set projection type to polyconic. CTYPE(1) = 'RA---PCO' CTYPE(2) = 'DEC--PCO' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 192D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 640D0, 2, 0) * Rotate 30 degrees. ROTN = 30D0*D2R STATUS = WCSPUT (WCS, WCS_PC, COS(ROTN), 1, 1) STATUS = WCSPUT (WCS, WCS_PC, SIN(ROTN), 1, 2) STATUS = WCSPUT (WCS, WCS_PC, -SIN(ROTN), 2, 1) STATUS = WCSPUT (WCS, WCS_PC, COS(ROTN), 2, 2) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, -1D0/5D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0/5D0, 2, 0) * Spherical coordinate references. STATUS = WCSPUT (WCS, WCS_CRVAL, 332D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 40D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, -30D0, 0, 0) * Annotation. IDENTS(1) = 'Hour angle' IDENTS(2) = 'Declination' IDENTS(3) = 'WCS polyconic projection' OPT(1) = 'H' OPT(2) = 'B' * Reduced size lettering. CALL PGSCH (0.9*SCL) * Draw external (TIKLEN < 0) tick marks every 5 degrees. CALL PGSCI (6) GCODE(1) = 1 GCODE(2) = 1 TIKLEN = -2D0 IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, TIKLEN, 0, : 5D0, 0, 5D0, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, NLDPRM, : 256, IC, CACHE, IERR) * Resetting the table index to zero causes information about the * tick marks to be discarded. IC = 0 * Draw full grid lines in yellow rather than tick marks. CALL PGSCI (2) GCODE(1) = 2 GCODE(2) = 2 * Draw the primary meridian and equator. GRID1(1) = 0D0 GRID2(1) = 0D0 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 0D0, 1, : GRID1, 1, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * At this point the axis-crossing table will have entries for the * primary meridian and equator. Labelling was deferred in the * previous call, and the table is passed intact on the second call * to accumulate further axis-crossings. * Draw 90 degree meridians and poles in white. CALL PGSCI (3) GRID1(1) = 90D0 GRID1(2) = 180D0 GRID1(3) = 270D0 GRID2(1) = -90D0 GRID2(2) = 90D0 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 0D0, 3, : GRID1, 2, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the first set of 15 degree meridians and parallels in blue. CALL PGSCI (4) GRID1(1) = 15D0 GRID1(2) = 60D0 GRID1(3) = 105D0 GRID1(4) = 150D0 GRID1(5) = 195D0 GRID1(6) = 240D0 GRID1(7) = 285D0 GRID1(8) = 330D0 GRID2(1) = -75D0 GRID2(2) = -30D0 GRID2(3) = 15D0 GRID2(4) = 60D0 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 0D0, 8, : GRID1, 4, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the second set of 15 degree meridians and parallels in red. CALL PGSCI (5) GRID1(1) = 30D0 GRID1(2) = 75D0 GRID1(3) = 120D0 GRID1(4) = 165D0 GRID1(5) = 210D0 GRID1(6) = 255D0 GRID1(7) = 300D0 GRID1(8) = 345D0 GRID2(1) = -60D0 GRID2(2) = -15D0 GRID2(3) = 30D0 GRID2(4) = 75D0 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 0D0, 8, : GRID1, 4, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * The axis-crossing table has now accumulated information for all of * the preceding meridians and parallels but no labels have been * produced. It will acquire information for the the next set of * meridians and parallels before being processed by this call to * PGSBOX which finally produces the labels. * Draw the 45 degree meridians and parallels in grey and use colour * to differentiate grid labels. * Meridians and parallels in grey. CALL PGSCR (10, 0.7, 0.7, 0.7) CALL PGSCR (11, 0.7, 0.7, 0.7) * Longitudes tinged red. CALL PGSCR (12, 1.0, 0.9, 0.6) * Latitudes tinged green. CALL PGSCR (13, 0.8, 1.0, 0.9) * Longitude labels tinged red. CALL PGSCR (14, 1.0, 0.9, 0.6) * Latitude labels tinged green. CALL PGSCR (15, 0.8, 1.0, 0.9) * Title in white. CALL PGSCR (16, 1.0, 1.0, 1.0) CI(1) = 10 CI(2) = 11 CI(3) = 12 CI(4) = 13 CI(5) = 14 CI(6) = 15 CI(7) = 16 CALL PGSCI (6) * Tell PGSBOX what edges to label. GRID1(1) = 45D0 GRID1(2) = 135D0 GRID1(3) = 225D0 GRID1(4) = 315D0 GRID2(1) = -45D0 GRID2(2) = 45D0 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 2333, 0, CI, GCODE, 0D0, 4, : GRID1, 2, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Native grid in green (delineates boundary). CALL PGSCI (7) GRID1(1) = -180D0 GRID1(2) = 180D0 GRID2(1) = -999D0 STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, 999D0, 0, 0) IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, -1, 0, C0, GCODE, 0D0, 2, : GRID1, 1, GRID2, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the frame. CALL PGSCI (1) CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Plate Carree projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Rectangular image. * - Dual coordinate grids. * - Non-separable (i.e. non-orthogonal) curvilinear coordinate * system. * - Demonstrate parameter definition for PGWCSL. * - Discontinuous grid lines handled by PGWCSL. * - Colour coding of grid and labelling. * - Reduced size lettering. * - Manual labelling control. * - Manual and automatic choice of coordinate increments. * - Cyclic coordinates. PGWCSL returns the longitude in the * range -180 to +180 degrees, i.e. with a discontinuity at * +/- 180 degrees. * - Suppression of labels that would overlap one another. WRITE (*, '(/,A)') 'Plate Carree projection' NAXIS(1) = 181 NAXIS(2) = 91 BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = NAXIS(1) + 0.5 TRC(2) = NAXIS(2) + 0.5 * Reset viewport for rectangular image. IF (LARGE) THEN CALL PGVSTD () ELSE CALL PGVSIZ (1.0, 3.0, 1.0, 3.0) END IF CALL PGWNAD (0.0, 1.0, 0.0, REAL(NAXIS(2))/REAL(NAXIS(1))) STATUS = WCSINI (2, WCS) * Set projection type to plate carree. CTYPE(1) = 'GLON-CAR' CTYPE(2) = 'GLAT-CAR' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 226D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 46D0, 2, 0) * Linear transformation matrix. ROTN = 15D0*D2R STATUS = WCSPUT (WCS, WCS_PC, COS(ROTN), 1, 1) STATUS = WCSPUT (WCS, WCS_PC, SIN(ROTN), 1, 2) STATUS = WCSPUT (WCS, WCS_PC, -SIN(ROTN), 2, 1) STATUS = WCSPUT (WCS, WCS_PC, COS(ROTN), 2, 2) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, -1D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0, 2, 0) * Set parameters to draw the native grid. STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 2, 0) * The reference pixel was defined so that the native longitude runs * from 225 deg to 45 deg and this will cause the grid to be * truncated at the 180 deg boundary. However, being a cylindrical * projection it is possible to recentre it in longitude. CYLFIX * will modify CRPIX, CRVAL, and LONPOLE to suit. CALL CYLFIX (NAXIS, WCS) * Annotation. IDENTS(1) = ' ' IDENTS(2) = ' ' IDENTS(3) = 'WCS plate caree projection' OPT(1) = 'C' OPT(2) = 'C' * Reduced size lettering. CALL PGSCH (0.8*SCL) * Draw full grid lines. GCODE(1) = 2 GCODE(2) = 2 * Draw native grid in green. CALL PGSCR (16, 0.0, 0.2, 0.0) * Title in cyan. CALL PGSCR (17, 0.3, 1.0, 1.0) CI(1) = 16 CI(2) = 16 CI(3) = 7 CI(4) = 7 CI(5) = -1 CI(6) = -1 CI(7) = 17 IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 2100, 0, CI, GCODE, 0D0, 0, : 15D0, 0, 15D0, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Reset CRPIX previously modified by CYLFIX. STATUS = WCSPUT (WCS, WCS_CRPIX, 226D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 46D0, 2, 0) * Galactic reference coordinates. STATUS = WCSPUT (WCS, WCS_CRVAL, 30D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 35D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, 999D0, 0, 0) CALL CYLFIX (NAXIS, WCS) * Annotation. IDENTS(1) = 'longitude' IDENTS(2) = 'latitude' IDENTS(3) = ' ' OPT(1) = 'E' OPT(2) = 'E' * Use colour to associate grid lines and labels. * Meridians in red. CALL PGSCR (10, 0.5, 0.0, 0.0) * Parallels in blue. CALL PGSCR (11, 0.0, 0.2, 0.5) * Longitudes in red. CALL PGSCR (12, 0.8, 0.3, 0.0) * Latitudes in blue. CALL PGSCR (13, 0.0, 0.4, 0.7) * Longitude labels in red. CALL PGSCR (14, 0.8, 0.3, 0.0) * Latitude labels in blue. CALL PGSCR (15, 0.0, 0.4, 0.7) CI(1) = 10 CI(2) = 11 CI(3) = 12 CI(4) = 13 CI(5) = 14 CI(6) = 15 CI(7) = -1 * Draw the celestial grid letting PGSBOX choose the increments. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 21, 0, CI, GCODE, 0D0, 0, 0D0, : 0, 0D0, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, NLDPRM, 256, : IC, CACHE, IERR) * Draw the frame. CALL PGSCI (1) CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Plate Carree projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - BLC, TRC unrelated to pixel coordinates. * - Demonstrate parameter definition for PGWCSL. * - Poles and 180 meridian projected along edges of the frame. * - Reduced size lettering. * - Manual and automatic choice of coordinate increments. * - Suppression of common zero minute and second fields in * sexagesimal time format. WRITE (*, '(/,A)') 'Plate Carree projection' BLC(1) = -180.0 BLC(2) = -90.0 TRC(1) = 180.0 TRC(2) = +90.0 * Reset viewport for rectangular image. IF (LARGE) THEN CALL PGVSTD () ELSE CALL PGVSIZ (1.0, 3.0, 1.0, 3.0) END IF CALL PGWNAD (BLC(1), TRC(1), BLC(2), TRC(2)) STATUS = WCSINI (2, WCS) * Set projection type to plate carree. CTYPE(1) = 'RA---CAR' CTYPE(2) = 'DEC--CAR' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 0D0, 2, 0) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, -1D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0, 2, 0) * Set parameters to draw the native grid. STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 0D0, 2, 0) * Annotation. IDENTS(1) = 'Right ascension' IDENTS(2) = 'Declination' IDENTS(3) = 'WCS plate caree projection' OPT(1) = 'G' OPT(2) = 'E' * Reduced size lettering. CALL PGSCH (0.7*SCL) * Draw full grid lines. GCODE(1) = 2 GCODE(2) = 2 CALL PGSCI (1) IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 2121, 1212, C0, GCODE, 0D0, 0, : 0D0, 0, 0D0, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, NLDPRM, : 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Cylindrical perspective projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - BLC, TRC unrelated to pixel coordinates. * - Demonstrate parameter definition for PGWCSL. * - Reduced size lettering. * - Manual and automatic choice of coordinate increments. * - Suppression of common zero minute and second fields in * sexagesimal time format. WRITE (*, '(/,A)') 'Cylindrical perspective projection' BLC(1) = -180.0 BLC(2) = -90.0 TRC(1) = 180.0 TRC(2) = +90.0 * Reset viewport for rectangular image. IF (LARGE) THEN CALL PGVSTD () ELSE CALL PGVSIZ (1.0, 3.0, 1.0, 3.0) END IF CALL PGWNAD (BLC(1), TRC(1), BLC(2), TRC(2)) STATUS = WCSINI (2, WCS) * Set projection type to cylindrical perspective. CTYPE(1) = 'RA---CYP' CTYPE(2) = 'DEC--CYP' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 0D0, 2, 0) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, -1D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0, 2, 0) * Set parameters to draw the native grid. STATUS = WCSPUT (WCS, WCS_CRVAL, 45D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, -90D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, 999D0, 0, 0) * mu and lambda projection parameters. STATUS = WCSPUT (WCS, WCS_PV, 0D0, 2, 1) STATUS = WCSPUT (WCS, WCS_PV, 1D0, 2, 2) * Annotation. IDENTS(1) = 'Right ascension' IDENTS(2) = 'Declination' IDENTS(3) = 'WCS cylindrical perspective projection' OPT(1) = 'G' OPT(2) = 'E' * Reduced size lettering. CALL PGSCH (0.7*SCL) * Draw full grid lines. GCODE(1) = 2 GCODE(2) = 2 CALL PGSCI (1) IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 2121, 1212, C0, GCODE, 0D0, 0, : 0D0, 0, 0D0, .TRUE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, NLDPRM, : 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Gnomonic projection. * - PGSBOX uses subroutine PGWCSL to interface to WCSLIB. * - Demonstrate parameter definition for PGWCSL. * - Reduced size lettering. * - Manual and automatic choice of coordinate increments. * - Suppression of common zero minute and second fields in * sexagesimal time format. WRITE (*, '(/,A)') 'TAN projection' NAXIS(1) = 100 NAXIS(2) = 100 BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = NAXIS(1) + 0.5 TRC(2) = NAXIS(2) + 0.5 * Reset viewport for rectangular image. IF (LARGE) THEN CALL PGVSTD () ELSE CALL PGVSIZ (1.0, 3.0, 1.0, 3.0) END IF CALL PGWNAD (0.0, 1.0, 0.0, REAL(NAXIS(2))/REAL(NAXIS(1))) STATUS = WCSINI (2, WCS) * Set projection type to gnomonic. CTYPE(1) = 'RA---TAN' CTYPE(2) = 'DEC--TAN' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 50.5D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 1.0D0, 2, 0) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, 1D-3, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D-3, 2, 0) * Set parameters to draw the native grid. STATUS = WCSPUT (WCS, WCS_CRVAL, -45.0D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, -89.7D0, 2, 0) STATUS = WCSPUT (WCS, WCS_LONPOLE, 999D0, 0, 0) * Annotation. IDENTS(1) = 'Right ascension' IDENTS(2) = 'Declination' IDENTS(3) = 'WCS TAN projection' OPT(1) = 'E' OPT(2) = 'E' * Reduced size lettering. CALL PGSCH (0.7*SCL) * Draw full grid lines. GCODE(1) = 2 GCODE(2) = 2 CALL PGSCI (1) IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 1212, C0, GCODE, 0D0, 0, : 0D0, 0, 0D0, .FALSE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Linear-linear plot with two types of alternative labelling. * - PGSBOX uses subroutine PGCRFN. * - Separable (i.e. orthogonal), linear coordinate system. * - Use of function PGCRFN for separable axis types. * - Alternative labelling and axis annotation. * - Direct manipulation of the axis-crossing table. * - Tick mark and grid line control. * - User selection of what edges to label. * - Automatic choice of coordinate increments. WRITE (*, '(/,A)') 'Linear plot with alternative labelling' IF (LARGE) THEN CALL PGVSTD () ELSE CALL PGVSIZ (1.0, 3.0, 1.0, 3.0) END IF CALL PGWNAD (0.0, 1.0, 0.0, 1.0) NAXIS(1) = 512 NAXIS(2) = 512 BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = NAXIS(1) + 0.5 TRC(2) = NAXIS(2) + 0.5 * Function types. FCODE(1) = 'Lin ' FCODE(2) = 'Lin ' * Reference pixel coordinates. NLDPRM(1) = 0.5D0 NLDPRM(2) = 0.5D0 * Coordinate increments. NLDPRM(3) = 0.03D0 NLDPRM(4) = 0.03D0 * Reference pixel values. NLDPRM(5) = 20D0 NLDPRM(6) = 0D0 * Annotation. IDENTS(1) = 'temperature of frog (' // ESCAPE // 'uo' // : ESCAPE // 'dC)' IDENTS(2) = 'distance hopped (m)' IDENTS(3) = ' ' OPT(1) = ' ' OPT(2) = ' ' * Reduced size lettering. CALL PGSCH (0.8*SCL) * Draw tick marks at the bottom for the first coordinate, grid lines * for the second. Setting GCODE(1) = -1 inhibits information being * stored for labels on the top edge while GCODE(2) = 2 causes * information to be stored for labels on the right edge even if * those labels are not actually produced. CALL PGSCI (1) GCODE(1) = -1 GCODE(2) = 2 * Set LABCTL = 21 to label the bottom and left edges only. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 21, 0, C0, GCODE, 2D0, 0, 0D0, : 0, 0D0, .FALSE., PGCRFN, 8, 2, 4, FCODE, NLIPRM, NLDPRM, 256, : IC, CACHE, IERR) * Information for labels on the right edge was stored in the * crossing table on the first call to PGSBOX. We now want to * manipulate it to convert metres to feet. Note that while it's * a simple matter to draw alternative sets of tick marks on opposite * edges of the frame, as with the two temperature scales, we have * the slightly more difficult requirement of labelling grid lines * with different values at each end. DO 10 J = 1, IC * Look for entries associated with the right edge of the frame. IF (CACHE(1,J).EQ.4D0) THEN * Convert to feet, rounding to the nearest 0.1. CACHE(4,J) = CACHE(4,J) * 1D3/(25.4*12D0) CACHE(4,J) = AINT(CACHE(4,J)*10D0 + 0.5D0)/10D0 END IF 10 CONTINUE * Annotation for the right edge. IDENTS(1) = ' ' IDENTS(2) = '(feet)' * Set LABCTL = 12000 to label the right edge with the second * coordinate without redrawing the grid lines. CALL PGSBOX (BLC, TRC, IDENTS, OPT, 12000, 0, C0, GCODE, 2D0, 0, : 0D0, 0, 0D0, .FALSE., PGCRFN, 8, 2, 4, FCODE, NLIPRM, NLDPRM, : 256, IC, CACHE, IERR) * The alternative temperature scale in Fahrenheit is to be * constructed with a new set of tick marks. NLDPRM(3) = NLDPRM(3)*1.8D0 NLDPRM(5) = NLDPRM(5)*1.8D0 + 32D0 * Draw tick marks at the top for the first coordinate, don't redo * grid lines for the second. GCODE(1) = -100 GCODE(2) = 0 * Annotation for the top edge. IDENTS(1) = '(' // ESCAPE // 'uo' // ESCAPE // 'dF)' IDENTS(2) = ' ' * Set LABCTL = 100 to label the top edge; Set IC = -1 to redetermine * the coordinate extrema. IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 100, 0, C0, GCODE, 2D0, 0, : 0D0, 0, 0D0, .FALSE., PGCRFN, 8, 2, 4, FCODE, NLIPRM, NLDPRM, : 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Calendar axes using subroutine PGLBOX. * - Separable (i.e. orthogonal), linear coordinate system. * - Use of PGLBOX for simple linear axis types. * - Automatic choice of what edges to label; results in labelling * the bottom and left sides of the plot. * - Automatic choice of coordinate increments. * - Calendar date axis labelling. * - Single-character annotation on a vertical axis is upright. WRITE (*, '(/,A)') 'Calendar axes using subroutine PGLBOX' CALL PGSWIN (51900.0, 52412.0, 51900.0, 57020.0) * Annotation. IDENTS(1) = 'Date started' IDENTS(2) = 'Date finished' IDENTS(3) = 'Calendar axes using subroutine PGLBOX' OPT(1) = 'Y' OPT(2) = 'Y' * Reduced size lettering. CALL PGSCH (0.7*SCL) * Draw tick marks on each axis. CALL PGSCI (1) GCODE(1) = 1 GCODE(2) = 1 IC = -1 CALL PGLBOX (IDENTS, OPT, 0, 0, C0, GCODE, 2D0, 0, 0D0, 0, 0D0, : .FALSE., 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- * Simple linear axes handled by PGWCSL. * - Separable (i.e. orthogonal), linear coordinate system. * - Automatic choice of what edges to label; results in labelling * the bottom and left sides of the plot. * - Automatic choice of coordinate increments. * - Tick marks and labels at the edges of the frame. * - Single-character annotation on a vertical axis is upright. WRITE (*, '(/,A)') 'Simple linear axes handled by pgwcsl()' NAXIS(1) = 3 NAXIS(2) = 3 BLC(1) = 0.5 BLC(2) = 0.5 TRC(1) = NAXIS(1) + 0.5 TRC(2) = NAXIS(2) + 0.5 STATUS = WCSINI (2, WCS) CTYPE(1) = 'X' CTYPE(2) = 'Y' STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(1), 1, 0) STATUS = WCSPUT (WCS, WCS_CTYPE, CTYPE(2), 2, 0) * Reference pixel coordinates. STATUS = WCSPUT (WCS, WCS_CRPIX, 2D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRPIX, 2D0, 2, 0) * Coordinate increments. STATUS = WCSPUT (WCS, WCS_CDELT, 1D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CDELT, 1D0, 2, 0) * Spherical coordinate references. STATUS = WCSPUT (WCS, WCS_CRVAL, 2D0, 1, 0) STATUS = WCSPUT (WCS, WCS_CRVAL, 2D0, 2, 0) * Annotation. IDENTS(1) = 'X' IDENTS(2) = 'Y' IDENTS(3) = 'Simple linear axes handled by pgwcsl()' OPT(1) = ' ' OPT(2) = ' ' * Reduced size lettering. CALL PGSCH (0.8*SCL) * Draw tick marks only. CALL PGSCI (1) GCODE(1) = 1 GCODE(2) = 1 IC = -1 CALL PGSBOX (BLC, TRC, IDENTS, OPT, 0, 0, C0, GCODE, 2D0, 0, : 0D0, 0, 0D0, .FALSE., PGWCSL, 1, WCSLEN, 1, NLCPRM, WCS, : NLDPRM, 256, IC, CACHE, IERR) * Draw the frame. CALL PGBOX ('BC', 0.0, 0, 'BC', 0.0, 0) CALL PGPAGE () *----------------------------------------------------------------------- STATUS = WCSFREE (WCS) CALL PGASK (0) CALL PGEND () END pywcs-1.12/wcslib/pgsbox/pgwcsl.c0000644001153600020070000001543312310355626021104 0ustar cslocumSTSCI\science00000000000000/*============================================================================ PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. Copyright (C) 1997-2012, Mark Calabretta This file is part of PGSBOX. PGSBOX is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. PGSBOX is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with PGSBOX. If not, see . Correspondence concerning PGSBOX may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: pgwcsl.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *===========================================================================*/ #include #include #include /* Fortran name mangling. */ #include #define pgwcsl_ F77_FUNC(pgwcsl, PGWCSL) void pgwcsl_(opcode, nlc, nli, nld, nlcprm, wcs, nldprm, world, pixel, contrl, contxt, ierr) const int *opcode, *nlc, *nli, *nld; const char *nlcprm; int *wcs; double *nldprm; double *world; double *pixel; int *contrl; double contxt[20]; int *ierr; { int i, outside, stat; double dp, imgcrd[9], lat, lng, ph, phi, sdummy, th, theta; static double wrld[9]; struct wcsprm *wcsp; struct celprm *wcscel; *ierr = 0; wcsp = (struct wcsprm *)wcs; wcscel = &(wcsp->cel); if (*opcode == 2) { /* Compute pixel coordinates from world coordinates. */ if (wcsp->lng < 0) { /* Simple linear coordinates. */ if (wcss2p(wcsp, 1, 0, world, &phi, &theta, imgcrd, pixel, &stat)) { *ierr = 1; } return; } wrld[wcsp->lng] = world[0]; if (world[1] > 90.0) { wrld[wcsp->lat] = 90.0; outside = -2; } else if (world[1] < -90.0) { wrld[wcsp->lat] = -90.0; outside = -2; } else { wrld[wcsp->lat] = world[1]; outside = 0; } if (*contrl == 0) { if (wcss2p(wcsp, 1, 0, wrld, &phi, &theta, imgcrd, pixel, &stat)) { /* Translate status return values. */ *ierr = stat ? 2 : 1; return; } if (fabs(phi-contxt[2]) > 180.0) { /* Hit a discontinuity at phi = +/- 180. */ contxt[4] = pixel[0]; contxt[5] = pixel[1]; if (contxt[2] > phi) { ph = 179.9999; dp = (phi - contxt[2]) + 360.0; } else { ph = -179.9999; dp = (phi - contxt[2]) - 360.0; } /* First approximation for theta. */ if (dp == 0.0) { th = contxt[3]; } else { th = contxt[3] + (ph-contxt[2])*(theta-contxt[3])/dp; } /* Iterate once to refine the value of theta. */ sphx2s(wcscel->euler, 1, 1, 1, 1, &ph, &th, &lng, &lat); if (wrld[wcsp->lng] == contxt[0]) { /* We are following a meridian of longitude. */ lng = wrld[wcsp->lng]; } else { /* We are following a parallel of latitude. */ lat = wrld[wcsp->lat]; } sphs2x(wcscel->euler, 1, 1, 1, 1, &lng, &lat, &sdummy, &th); contxt[0] = wrld[wcsp->lng]; contxt[1] = wrld[wcsp->lat]; contxt[2] = phi; contxt[3] = theta; /* Pixel coordinates crossing into the discontinuity. */ sphx2s(wcscel->euler, 1, 1, 1, 1, &ph, &th, wrld+wcsp->lng, wrld+wcsp->lat); if (wcss2p(wcsp, 1, 0, wrld, &phi, &theta, imgcrd, pixel, &stat)) { /* Translate status return values. */ *ierr = stat ? 2 : 1; return; } /* Pixel coordinates crossing out of the discontinuity. */ ph *= -1.0; sphx2s(wcscel->euler, 1, 1, 1, 1, &ph, &th, wrld+wcsp->lng, wrld+wcsp->lat); if (wcss2p(wcsp, 1, 0, wrld, &phi, &theta, imgcrd, contxt+6, &stat)) { /* Translate status return values. */ *ierr = stat ? 2 : 1; return; } *contrl = 1; } else { /* Normal mode, no discontinuity. */ contxt[0] = wrld[wcsp->lng]; contxt[1] = wrld[wcsp->lat]; contxt[2] = phi; contxt[3] = theta; } } else { if (*contrl == 1) { /* Move to the other side of the discontinuity. */ pixel[0] = contxt[6]; pixel[1] = contxt[7]; *contrl = 2; } else { /* Complete the traversal. */ pixel[0] = contxt[4]; pixel[1] = contxt[5]; *contrl = 0; } } *ierr = outside; } else if (*opcode == 1) { /* Compute pixel coordinates from world coordinates. */ if (wcsp->lng < 0) { /* Simple linear coordinates. */ if (wcss2p(wcsp, 1, 0, world, &phi, &theta, imgcrd, pixel, &stat)) { *ierr = 1; } return; } wrld[wcsp->lng] = world[0]; if (world[1] > 90.0) { wrld[wcsp->lat] = 90.0; outside = -2; } else if (world[1] < -90.0) { wrld[wcsp->lat] = -90.0; outside = -2; } else { wrld[wcsp->lat] = world[1]; outside = 0; } if (wcss2p(wcsp, 1, 0, wrld, &phi, &theta, imgcrd, pixel, &stat)) { /* Translate status return values. */ *ierr = stat ? 2 : 1; return; } contxt[0] = wrld[wcsp->lng]; contxt[1] = wrld[wcsp->lat]; contxt[2] = phi; contxt[3] = theta; *ierr = outside; } else if (*opcode == 0) { /* Initialize. */ if (*nli < WCSLEN) { *ierr = 1; return; } if ((*ierr = wcsset(wcsp))) { *ierr = *ierr <= 2 ? 1 : 2; } for (i = 2; i < 9; i++) { wrld[i] = 0.0; } *contrl = 0; } else if (*opcode == -1) { /* Compute world coordinates from pixel coordinates. */ if (wcsp2s(wcsp, 1, 0, pixel, imgcrd, &phi, &theta, wrld, &stat)) { /* Translate status return values. */ *ierr = stat ? 3 : 1; return; } if (wcsp->lng < 0) { /* Simple linear coordinates. */ world[0] = wrld[0]; world[1] = wrld[1]; } else { world[0] = wrld[wcsp->lng]; world[1] = wrld[wcsp->lat]; if (phi < -180.0 || phi > 180.0) { /* Pixel is outside the principle range of native longitude. */ *ierr = 3; return; } } } else { *ierr = 1; } return; } pywcs-1.12/wcslib/pgsbox/pgwcsl.h0000644001153600020070000001244412310355626021110 0ustar cslocumSTSCI\science00000000000000/*============================================================================ PGSBOX 4.10 - draw curvilinear coordinate axes for PGPLOT. Copyright (C) 1997-2012, Mark Calabretta This file is part of PGSBOX. PGSBOX is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. PGSBOX is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with PGSBOX. If not, see . Correspondence concerning PGSBOX may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: pgwcsl.h,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * * pgwcsl_() is an NLFUNC for PGSBOX that defines curvilinear celestial * coordinate systems by interfacing to WCSLIB 4.x. * * Since WCSLIB 4.x is a C library, pgwcsl_() is written in C. However, as * PGSBOX expects NLFUNC to be a FORTRAN subroutine, its interfaces * necessarily emulate those of a FORTRAN subroutine. Hence the trailing * underscore in the name of the function and the pointer (reference) * argument list. * * The wcsprm struct on which WCSLIB 4.x is based is passed as an integer * array of size WCSLEN at least (WCSLEN is defined in wcs.h). While the * contents of this array are not interpretable in FORTRAN, it may be * constructed and interrogated by service routines (WCSPUT and WCSGET) * provided with the FORTRAN wrappers for WCSLIB 4.x. The array is cast to * (struct wcsprm *) for use here and in WCSLIB. * * Given: * opcode int* Transformation code: * 2: Compute a set of pixel coordinates that * describe a path between this and the previous * pair of world coordinates remembered from the * last call with opcode == 1 || 2. * 1: Compute pixel coordinates from world * coordinates. * 0: Initialize. * -1: Compute world coordinates from pixel * coordinates. * * nlc int* Number of elements in nlcprm[] (not used). * * nli int* Number of elements in wcs (at least WCSLEN). * * nld int* Number of elements in nldprm (not used). * * nlcprm char[nlc] * Character array (not used). * * Given and/or returned: * wcs int[nli] Integer array that contains the wcsprm struct (see * below). * * nldprm double[nld] * Double precision array (not used). * * world double[2] * World coordinates. world[0] and world[1] are the * longitude and latitude, in degrees. Given if * opcode > 0, returned if opcode < 0. * * pixel double[2] * Pixel coordinates. Given if opcode < 0, returned if * opcode > 0. * * contrl int* Control flag for opcode == 2: * 0: Normal state * 1: A discontinuity has been encountered; force * PGSBOX to flush its plotting buffer and call * pgwcsl_() again with the same world * coordinates. * 2: Call pgwcsl_() again with the same world * coordinates. * * contxt double[20] * Context elements for opcode == 2. * * Returned: * ierr int* Status return value: * 0: Success. * 1: Invalid parameters. * 2: Invalid world coordinate. * 3: Invalid pixel coordinate. * * Notes * ----- * 1) pgwcsl_() assumes a simple 2-D image. * * 2) The wcsprm struct (contained in the wcs[] array) is maintained by * pgwcsl_() and WCSLIB and must not be disturbed by the caller after * initialization with opcode == 0. * * 3) pgwcsl_() doesn't properly handle discontinuities between the faces * of the quadcube projections nor in the polar region of the HPX * projection. * * *===========================================================================*/ #ifndef PGSBOX_PGWCSL #define PGSBOX_PGWCSL #include "cpgsbox.h" /* Fortran name mangling. */ #include #define pgwcsl_ F77_FUNC(pgwcsl, PGWCSL) #ifdef __cplusplus extern "C" { #endif nlfunc_t pgwcsl_; #ifdef __cplusplus } #endif #endif /* PGSBOX_PGWCSL */ pywcs-1.12/wcslib/README0000644001153600020070000000407712310355626017021 0ustar cslocumSTSCI\science00000000000000------------------------------------------------------------------------------ WCSLIB 4.10 and PGSBOX 4.10 ------------------------------------------------------------------------------ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA ------------------------------------------------------------------------------ Please refer to ./INSTALL ...Installation instructions. ./html/index.html ...The WCSLIB programmer's manual in HTML format. ./wcslib.pdf ...The WCSLIB programmer's manual in PDF format. ./CHANGES ...Log of changes made to WCSLIB. ./THANKS ...List of contributors to WCSLIB. ./VALIDATION ...List of platforms on which the installation procedures and test suite were exercised. ./COPYING ...A copy of the GNU General Public License, v3.0. ./COPYING.LESSER ...A copy of the Lesser GNU General Public License. Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: README,v 4.10 2012/02/05 23:41:45 cal103 Exp $ pywcs-1.12/wcslib/THANKS0000644001153600020070000000414312310355626017046 0ustar cslocumSTSCI\science00000000000000I would like to acknowledge the following people who have contributed to WCSLIB and/or PGSBOX in some way since 1995 - via bug reports, patches, suggestions for improvements, positive feedback, etc. James M. Anderson (MPIfR) Robbie Auld (Cardiff U.) Klaus Banse (ESO) David Barnes (ATNF/CSIRO) David Berry (STARLINK & JAC) Emmanuel Bertin (IAP) Jeremy Brewer (U. Pittsburgh) Wim Brouw (ATNF/CSIRO) Peter Bunclark (IoA, U. Cambridge) Pan Chai (GSFC/NASA) Charles Copley Neil Crighton Cesar Enrique Garcia Dabo (ESO) Lindsey Davis (NOAO) Ger van Diepen (ASTRON) Patrick Dowler (CADC/NRC) Michael Droettboom (STScI) Rick Ebert (IPAC/NASA) Ken Ebisawa (GSFC/NASA) Sébastien Fabbro (Gentoo linux maintainer) Bob Garwood (NRAO) Brian Glendenning (NRAO) Eric Greisen (NRAO) Michael Halle (AM/Harvard) Booth Hartley (IPAC/NASA) Phil Hodge (STScI) Bryan Irby (GSFC/NASA) Justin Jonas (Rhodes U.) Yves Jung (ESO) David Kaplan (KITP/UCSB) Daniel S. Katz (JPL/NASA) Neil Killeen (ATNF/CSIRO) David King (NRAO) Paul F. Kunz (SLAC/Stanford U.) Jonas Møller Larsen (ESO) Jim Lewis (IoA, U. Cambridge) Marco Lombardi (ESO) Lars Kristian Lundin (ESO) Robert Lupton (Princeton U.) Craig Markwardt (GSFC/NASA) Malte Marquarding (ATNF/CSIRO) Tom Marsh (U. Warwick) Sean Mattingly (IPAC/NASA) Dave McConnell (ATNF/CSIRO) Thomas A. McGlynn (GSFC/NASA) Michelle Miller (NOAO) Doug Mink (CfA) August Muench (CfA) Fergal Mullally (Princeton U.) Clive Page (U. Leicester) Sergio Pascual (U. Complutense de Madrid) Bill Pence (NASA/GSFC) Olivier Perdereau (LAL/IN2P3) Dirk Petry (ESO) Ray Plante (NCSA/UIUC) Niruj Mohan Ramanujam (Leiden Obs) Harold Ravlin (U. Illinois) Boud Roukema (TCfA) Keith A. Scollick (GSFC/NASA) Arno Schoenmakers (ASTRON) Hanno Spreeuw (ASTRON) Ole Streicher (Debian maintainer) Hans Terlouw (Kapteyn, Groningen) Peter Teuben (U. Maryland) Harro Verkouter (JIVE) John C. Vernaleo (GSFC/NASA) Martin Vogelaar (Kapteyn, Groningen) Stephen Walton (CSUN) Boyd Waters NRAO) Randall Wayth (Curtin U.) Matthew Whiting (ATNF/CSIRO) Peter Williams (UCB) Daren Scot Wilson (NRAO) Tony Wong (ATNF/CSIRO) $Id: THANKS,v 4.10 2012/02/05 23:41:45 cal103 Exp $ pywcs-1.12/wcslib/utils/0000755001153600020070000000000012310355732017267 5ustar cslocumSTSCI\science00000000000000pywcs-1.12/wcslib/utils/fitshdr.c0000644001153600020070000002213312310355626021101 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: fitshdr.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * Usage: fitshdr [infile] *----------------------------------------------------------------------------- * List headers from a FITS file specified on the command line, or else on * stdin, printing them as 80-character keyrecords without trailing blanks. * * If invoked as 'rpfhdr' rather than 'fitshdr' it also handles RPFITS format * which has a block size of 2560 (rather than 2880) but otherwise looks like * FITS. * * Handles large files (>2GiB) via macros in wcsconfig_utils.h. *---------------------------------------------------------------------------*/ char usage[] = "List headers from a FITS file specified on the command line, or else on\n" "stdin, printing them as 80-character keyrecords without trailing blanks.\n" "\n" "Options:\n" " -q N Quit after reading the Nth header, where N is an integer\n" " (optional space between -q and N).\n"; /* Get LFS definitions for stdio.h. */ #include #include #include #include #include #include #include #include int main(int argc, char **argv) { char cbuff[2880], *cptr; char dashes[84] = "----------------------------------------" "----------------------------------------"; char equals[84] = "========================================" "========================================"; char spaces[84] = " " " "; char *format, rpfits[8] = "RPFITS"; int i, len; unsigned int blksiz = 2880, ihdr = 0, inhdr = 0, nhdr = 0, seekable = 1; unsigned long long int iblock = 0, nblock = 0, nbyte; struct stat instat; /* Parse options. */ for (i = 1; i < argc && argv[i][0] == '-'; i++) { switch (argv[i][1]) { case 'q': if (strlen(argv[i]) == 2) { nhdr = atoi(&argv[++i][0]); } else { nhdr = atoi(&argv[i][2]); } break; default: fprintf(stderr, "\nUsage: fitshdr [-q N] []\n\n%s\n", usage); return 1; } } /* If an input file name was specified then reopen it as stdin */ /* (doesn't affect seekability). */ if (i < argc) { if (access(argv[i], R_OK) == -1) { perror(argv[i]); return 2; } if (freopen(argv[i], "r", stdin) == NULL) { perror(argv[i]); return 2; } } /* Check for standard FITS or RPFITS. */ if (!fread(cbuff, (size_t)80, (size_t)1, stdin)) { perror(argv[i]); return 2; } if (strncmp(cbuff, "SIMPLE = ", 10) == 0) { if (!fread(cbuff+80, (size_t)80, (size_t)1, stdin)) { perror(argv[i]); return 2; } /* Assume FITS by default. */ format = rpfits + 2; blksiz = 2880; /* Check for RPFITS. */ if (strncmp(cbuff+80, "FORMAT = RPFITS", 30) == 0 || strncmp(cbuff+80, "FORMAT = 'RPFITS'", 30) == 0) { if (strcmp(*argv, "rpfhdr") == 0) { /* If invoked as 'rpfhdr' then allow RPFITS. */ format = rpfits; blksiz = 2560; } else { /* Otherwise disallow RPFITS but issue a warning. */ printf("WARNING: Input appears to be RPFITS, continuing anyway using " "2880-byte blocks.\n" ); } } /* Read the rest of the first block. */ if (!fread(cbuff+160, (size_t)(blksiz-160), (size_t)1, stdin)) { perror(argv[i]); return 2; } inhdr = 1; } else { /* If we have not been invoked as 'rpfhdr' then bail out now. */ if (strcmp(*argv, "rpfhdr") != 0) { fprintf(stderr, "Input file does not appear to be standard FITS.\n" ); return 1; } /* RPFITS may have a block or two of rubbish before the first header. */ format = rpfits; blksiz = 2560; if (!fread(cbuff+80, (size_t)(blksiz-80), (size_t)1, stdin)) { perror(argv[i]); return 2; } while (iblock < 4) { if (!fread(cbuff, (size_t)blksiz, (size_t)1, stdin)) { perror(argv[i]); return 2; } iblock++; if (strncmp(cbuff, "SIMPLE = ", 10) == 0) { inhdr = 1; break; } } if (!inhdr) { fprintf(stderr, "Input does not appear to be FITS or RPFITS.\n" ); return 1; } if (iblock) { nbyte = blksiz * iblock; printf("Skipped %lld block%s of rubbish of size %d bytes (%lld " "bytes).\n", iblock, (iblock > 1)?"s":"", blksiz, nbyte); } } printf("%s\n%s header number %d at block number %lld.\n%s\n", equals, format, ++ihdr, ++iblock, dashes); /* Scan through the file. */ while (1) { if (!inhdr) { /* Searching for a header. */ if (!fread(cbuff, (size_t)10, (size_t)1, stdin)) break; if (strncmp(cbuff, "SIMPLE = ", 10) == 0 || strncmp(cbuff, "XTENSION= ", 10) == 0) { /* Found a header. */ if (iblock) { nbyte = blksiz * nblock; printf("Skipped %lld block%s of data of size %d bytes (%lld " "bytes).\n", nblock, (nblock == 1)?"":"s", blksiz, nbyte); } if (!fread(cbuff+10, (size_t)(blksiz-10), (size_t)1, stdin)) break; printf("%s\n%s header number %d at block number %lld.\n%s\n", equals, format, ++ihdr, ++iblock, dashes); inhdr = 1; nblock = 0; } else { /* Seek past it if possible. */ if (seekable) { #ifdef HAVE_FSEEKO if (fseeko(stdin, (off_t)(blksiz-10), SEEK_CUR)) { #else if (fseek(stdin, (long)(blksiz-10), SEEK_CUR)) { #endif if (errno == ESPIPE || errno == EBADF) { seekable = 0; } else { break; } } } if (!seekable) { if (!fread(cbuff+10, (size_t)(blksiz-10), (size_t)1, stdin)) break; } iblock++; } } if (inhdr) { for (cptr = cbuff; cptr < cbuff + blksiz; cptr += 80) { /* Write out a keyrecord without trailing blanks. */ for (len = 80; len > 0; len--) { if (cptr[len-1] != ' ') break; } printf("%.*s\n", len, cptr); /* Check for end-of-header. */ if (strncmp(cptr, "END ", 8) == 0) { inhdr = 0; printf("%s\n", dashes); fflush(stdout); break; } } /* Get the next header block. */ if (inhdr) { if (!fread(cbuff, (size_t)blksiz, (size_t)1, stdin)) break; iblock++; } } else { if (!nblock) { if (nhdr && ihdr == nhdr) { printf("Stopping at data section number %d which begins at block " "number %lld.\n", ihdr, iblock); return 0; } printf("Data section number %d beginning at block number %lld.\n", ihdr, iblock); } nblock++; if (nblock%1000 == 0) { /* Report progress on stderr in case it's saved to file. */ nbyte = blksiz * nblock; fprintf(stderr, "Skipping %lld blocks of data of size %d bytes " "(%lld bytes). \r", nblock, blksiz, nbyte); fflush(stderr); } } } if (feof(stdin)) { nbyte = blksiz * nblock; printf("Skipped %lld block%s of data of size %d bytes (%lld bytes). \n", nblock, (nblock == 1)?"":"s", blksiz, nbyte); nbyte = blksiz * iblock; printf("%s\nEnd-of-file after %d HDU%s in %lld x %d-byte blocks (%lld " "bytes).\n", equals, ihdr, (ihdr == 1)?"":"s", iblock, blksiz, nbyte); if (argc > 1 && !stat(argv[i], &instat)) { if (nbyte != instat.st_size) { printf("WARNING: File is too short by %lld bytes.\n", nbyte - instat.st_size); } } printf("%s\n", dashes); fprintf(stderr, "%s\r", spaces); } else { perror(argv[i]); return 2; } return 0; } pywcs-1.12/wcslib/utils/GNUmakefile0000644001153600020070000000767212310355626021357 0ustar cslocumSTSCI\science00000000000000#----------------------------------------------------------------------------- # GNU makefile for WCSLIB 4.10 utilities: fitshdr, HPXcvt, wcsgrid and wcsware. # # Summary of the main targets # --------------------------- # build: Build all utilities. # clean (or cleaner): Delete intermediate object files. # distclean (or realclean): cleaner, and also delete the executables. # cleanest: distclean, and also delete the man pages. # # Notes: # 1: If you need to make changes then preferably modify ../makedefs.in # instead and re-run configure. # # 2: In compiling these utilities, this makefile assumes that the WCSLIB 4.10 # sources reside in ../{pgsbox,C} (as in the distribution kit). # # Author: Mark Calabretta, Australia Telescope National Facility # http://www.atnf.csiro.au/~mcalabre/index.html # $Id: GNUmakefile,v 4.10 2012/02/05 23:41:45 cal103 Exp $ #----------------------------------------------------------------------------- # Get configure settings. include ../makedefs UTILS := fitshdr ifneq "$(CFITSIOINC)" "" ifneq "$(CFITSIOLIB)" "" UTILS += HPXcvt wcsware ifneq "$(PGPLOTINC)" "" ifneq "$(PGPLOTLIB)" "" UTILS += wcsgrid endif endif endif endif MAN := $(addsuffix .1,$(UTILS)) WCSLIB := ../C/$(WCSLIB) PGSBOXLIB := ../pgsbox/libpgsbox-$(LIBVER).a ifneq "$(GETWCSTAB)" "" GETWCSTAB := ../C/$(GETWCSTAB) endif CPPFLAGS += -I.. -I../C vpath %.h ..:../C:../pgsbox vpath %.in .. # Static and static pattern rules #-------------------------------- .PHONY : build clean cleaner cleanest distclean install man realclean build : $(UTILS) fitshdr : fitshdr.c -@ echo '' $(CC) $(CPPFLAGS) $(CFLAGS) -c -o $@.o $< $(LD) -o $@ $@.o $(LDFLAGS) $(LIBS) -@ $(RM) $@.o HPXcvt : HPXcvt.c -@ echo '' $(CC) $(CPPFLAGS) $(CFITSIOINC) $(CFLAGS) -c -o $@.o $< $(LD) -o $@ $@.o $(LDFLAGS) $(CFITSIOLIB) $(LIBS) -@ $(RM) $@.o wcsware : wcsware.c $(GETWCSTAB) $(WCSLIB) -@ echo '' $(CC) -DDO_CFITSIO $(CPPFLAGS) -I../pgsbox -I../C $(CFITSIOINC) \ $(CFLAGS) -c -o $@.o $< $(LD) $(LDFLAGS) -o $@ $@.o $(GETWCSTAB) $(CFITSIOLIB) $(WCSLIB) \ $(FLIBS) $(LIBS) -@ $(RM) $@.o wcsgrid : wcsgrid.c $(PGSBOXLIB) $(GETWCSTAB) $(WCSLIB) -@ echo '' $(CC) -DDO_CFITSIO $(CPPFLAGS) -I../pgsbox -I../C $(PGPLOTINC) \ $(CFITSIOINC) $(CFLAGS) -c -o $@.o $< $(LD) $(LDFLAGS) -o $@ $@.o $(PGSBOXLIB) $(PGPLOTLIB) \ $(GETWCSTAB) $(CFITSIOLIB) $(WCSLIB) $(FLIBS) $(LIBS) -@ $(RM) $@.o ../C/getwcstab.o : $(MAKE) -C ../C $(@F) clean cleaner : - $(RM) -r *.o *.i a.out core *.dSYM $(EXTRA_CLEAN) distclean realclean : cleaner - $(RM) $(UTILS) cleanest : distclean - $(RM) $(MAN) $(PGSBOXLIB) : -@ echo '' $(MAKE) -C ../pgsbox lib $(WCSLIB) : -@ echo '' $(MAKE) -C ../C lib install : build - if [ ! -d "$(BINDIR)" ] ; then \ $(INSTALL) -d -m 2775 $(BINDIR) ; \ fi $(INSTALL) -m 755 $(UTILS) $(BINDIR) - if [ ! -d "$(MANDIR)" ] ; then \ $(INSTALL) -d -m 2775 $(MANDIR)/man1 ; \ fi $(INSTALL) -m 755 $(MAN) $(MANDIR)/man1 GNUmakefile : ../makedefs ; ../makedefs ../wcsconfig.h ../wcsconfig_utils.h : makedefs.in wcsconfig.h.in \ wcsconfig_utils.h.in ../config.status -@ $(RM) ../wcsconfig.h ../wcsconfig_utils.h cd .. && ./config.status man : $(MAN) fitshdr.1 : fitshdr help2man --no-discard-stderr --version-string=$(LIBVER) \ -n "List headers from a FITS file" -N ./$< > $@ wcsware.1 : wcsware help2man --no-discard-stderr --version-string=$(LIBVER) \ -n "Extract WCS keywords for an image" -N ./$< > $@ wcsgrid.1 : wcsgrid help2man --no-discard-stderr --version-string=$(LIBVER) \ -n "Extract WCS keywords for an image" -N ./$< > $@ HPXcvt.1 : HPXcvt help2man --no-discard-stderr --version-string=$(LIBVER) \ -n "Reorganise HEALPix data into a 2-D FITS image" -N ./$< > $@ # Dependency lists. fitshdr : wcsconfig.h wcsconfig_utils.h wcsware : getwcstab.h wcs.h wcsfix.h wcshdr.h wcsgrid : cpgsbox.h getwcstab.h wcs.h wcsfix.h wcshdr.h pywcs-1.12/wcslib/utils/HPXcvt.c0000644001153600020070000006621712310355626020625 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: HPXcvt.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * * HPXcvt reorganises HEALPix data into a 2-D FITS image. Refer to the usage * notes below. * *---------------------------------------------------------------------------*/ char usage[] = "Usage: HPXcvt [-C] [-c] [-n|-r] [-q] [-x]\n" " [ []]\n" "\n" "HPXcvt reorganises HEALPix data into a 2-D FITS image with HPX coordinate\n" "system. The input data may be stored in a FITS file as a primary image\n" "or image extension, or as a binary table extension. Both NESTED and RING\n" "pixel indices are supported. The input and output files may be omitted or\n" "specified as \"-\" to indicate stdin and stdout respectively.\n" "\n" "Options:\n" " -C Binary table column number from which to read data,\n" " default 1 (n.b. WMAP exclusion masks are in column 2).\n" "\n" " -c Specify the coordinate system to be used to label the\n" " output map if the COORDSYS keyword is absent from the input\n" " FITS header. Recognised values are g (galactic),\n" " e (ecliptic) or q (equatorial).\n" "\n" " -n|-r Assume n(ested) or r(ing) organization if the ORDERING\n" " keyword is absent from the input FITS header.\n" "\n" " -q Recentre longitude at quad(mod 4) x 90 degrees, where\n" " quad(rant) is an integer.\n" "\n" " -x Use a north-polar or south-polar layout.\n"; #include #include #include #include #include #include #include #include #define HEALPIX_NULLVAL (-1.6375e30) struct healpix { char *infile; /* Input file. */ char *outfile; /* Output file. */ int col; /* Input binary table column number. */ char crdsys; /* G(alactic), E(cliptic), or (e)Q(uatorial). */ char ordering; /* R(ing) or N(ested). */ char layout; /* Required output layout, */ /* 0: equatorial (default), */ /* 1: north, or */ /* 2: south. */ char quad; /* Recentre longitude on quadrant (modulo 4). */ int nside; /* Dimension of a base-resolution pixel. */ long npix; /* Total number of pixels in the data array. */ float *data; /* Pointer to memory allocated to hold data. */ }; int HEALPixIn(struct healpix *hpxdat); int HPXout(struct healpix *hpxdat); int NESTidx(int nside, int facet, int rotn, int row, long *healidx); int RINGidx(int nside, int facet, int rotn, int row, long *healidx); int HPXhdr(fitsfile *fptr, struct healpix *hpxdat); int main(int argc, char **argv) { int crdsys, i, layout, quad, status; struct healpix hpxdat; hpxdat.col = 1; hpxdat.crdsys = '?'; hpxdat.ordering = '?'; hpxdat.layout = 0; hpxdat.quad = 0; /* Parse options. */ for (i = 1; i < argc && argv[i][0] == '-'; i++) { if (!argv[i][1]) break; switch (argv[i][1]) { case 'C': hpxdat.col = atoi(argv[i]+2); if (hpxdat.col < 1) hpxdat.col = 1; break; case 'c': crdsys = toupper(argv[i][2]); switch (crdsys) { case 'G': case 'E': case 'Q': hpxdat.crdsys = (char)crdsys; }; break; case 'n': hpxdat.ordering = 'N'; break; case 'q': quad = atoi(argv[i]+2)%4; if (quad < 0) quad += 4; hpxdat.quad = (char)quad; break; case 'r': hpxdat.ordering = 'R'; break; case 'x': layout = toupper(argv[i][2]); switch (layout) { case 'N': hpxdat.layout = 1; break; case 'S': hpxdat.layout = 2; break; }; break; default: fprintf(stderr, "%s", usage); return 1; } } if (i < argc) { hpxdat.infile = argv[i++]; if (i < argc) { hpxdat.outfile = argv[i++]; if (i < argc) { fprintf(stderr, "%s", usage); return 1; } } else { hpxdat.outfile = "-"; } } else { hpxdat.infile = "-"; } /* Check accessibility of the input file. */ if (strcmp(hpxdat.infile, "-") && access(hpxdat.infile, R_OK) == -1) { printf("HPXcvt: Cannot access %s.\n", hpxdat.infile); return 1; } /* Get the HEALPix data as a vector. */ if ((status = HEALPixIn(&hpxdat))) { return 2; } if (hpxdat.ordering == '?') { fprintf(stderr, "WARNING: ORDERING keyword absent, assuming RING.\n"); hpxdat.ordering = 'r'; } printf("HPXcvt: Read 12 * %d^2 = %ld pixels with %s indexing.\n", hpxdat.nside, hpxdat.npix, (hpxdat.ordering == 'N') ? "nested" : "ring"); /* Map and write it out as a FITS image. */ if ((status = HPXout(&hpxdat))) return 3; if (hpxdat.data) free(hpxdat.data); return 0; } /*--------------------------------------------------------------------------*/ int HEALPixIn(struct healpix *hpxdat) { char crdsys[32], ordering[32]; int anynul, hdutype, iaxis, nfound, status; long firstpix, ipix, lastpix, naxis, *naxes = 0x0, nside = 0, repeat; float *datap, nulval; LONGLONG firstelem, irow, nelem, npix = 0, nrow = 0; fitsfile *fptr; status = 0; hpxdat->data = 0x0; /* Open the FITS file and move to the first HDU with NAXIS != 0. */ if (fits_open_data(&fptr, hpxdat->infile, READONLY, &status)) goto fitserr; /* Is this the primary HDU or an extension? */ if (fits_get_hdu_type(fptr, &hdutype, &status)) goto fitserr; if (!(hdutype == IMAGE_HDU || hdutype == BINARY_TBL)) { fprintf(stderr, "ERROR: %s does not contain HEALPix data.\n", hpxdat->infile); return 1; } /* Get the image size. */ if (fits_read_key_lng(fptr, "NAXIS", &naxis, 0x0, &status)) goto fitserr; naxes = malloc(naxis*sizeof(long)); if (fits_read_keys_lng(fptr, "NAXIS", 1, (int)naxis, naxes, &nfound, &status)) goto fitserr; if (hdutype == IMAGE_HDU) { /* Look for the first non-degenerate image axis. */ for (iaxis = 0; iaxis < nfound; iaxis++) { if (naxes[iaxis] > 1) { /* Assume for now that it is the total number of pixels. */ npix = naxes[iaxis]; break; } } } else if (hdutype == BINARY_TBL) { /* Binary tables are simpler. */ if (nfound > 1) nrow = naxes[1]; /* (Note that fits_get_coltypell() is not available in cfitsio 2.x.) */ if (fits_get_coltype(fptr, hpxdat->col, 0x0, &repeat, 0x0, &status)) { goto fitserr; } nelem = (LONGLONG)repeat; } if (!npix && !nrow) { fprintf(stderr, "ERROR: Could not determine image size.\n"); goto cleanup; } /* Number of pixels per side of each base-resolution pixel. */ if (fits_read_key_lng(fptr, "NSIDE", &nside, 0x0, &status)) { /* Some HEALPix files, e.g. SFD dust maps, don't record NSIDE. */ if (status != KEY_NO_EXIST) goto fitserr; status = 0; } /* FIRSTPIX and LASTPIX, if present, record the 0-relative pixel numbers of * the first and last pixels stored in the data. */ firstpix = -1; if (fits_read_key_lng(fptr, "FIRSTPIX", &firstpix, 0x0, &status)) { if (status != KEY_NO_EXIST) goto fitserr; status = 0; } lastpix = -1; if (fits_read_key_lng(fptr, "LASTPIX", &lastpix, 0x0, &status)) { if (status != KEY_NO_EXIST) goto fitserr; status = 0; } if (!nside) { /* Deduce NSIDE. */ if (lastpix >= 0) { /* If LASTPIX is present without NSIDE we can only assume it's npix. */ nside = (int)(sqrt((double)((lastpix+1) / 12)) + 0.5); } else if (npix) { nside = (int)(sqrt((double)(npix / 12)) + 0.5); } else if (nrow) { nside = (int)(sqrt((double)((nrow * nelem) / 12)) + 0.5); } } hpxdat->nside = (int)nside; hpxdat->npix = 12*nside*nside; /* Ensure that FIRSTPIX and LASTPIX are set. */ if (firstpix < 0) firstpix = 0; if (lastpix < 0) lastpix = hpxdat->npix - 1; /* Any sign of a coordinate system identifier? */ if (fits_read_key_str(fptr, "COORDSYS", crdsys, 0x0, &status)) { if (status != KEY_NO_EXIST) goto fitserr; status = 0; } else if (crdsys[0] == 'G') { hpxdat->crdsys = 'G'; } else if (crdsys[0] == 'E') { hpxdat->crdsys = 'E'; } else if (crdsys[0] == 'C') { /* ("celestial") */ hpxdat->crdsys = 'Q'; } /* Nested or ring ordering? */ if (fits_read_key_str(fptr, "ORDERING", ordering, 0x0, &status)) { /* Some HEALPix files, e.g. SFD dust maps, don't record ORDERING. */ if (status != KEY_NO_EXIST) goto fitserr; status = 0; } else if (strcmp(ordering, "NESTED") == 0) { hpxdat->ordering = 'N'; } else if (strcmp(ordering, "RING") == 0) { hpxdat->ordering = 'R'; } else { fprintf(stderr, "WARNING: Invalid ORDERING keyword: %s.\n", ordering); } /* Allocate memory and read the data. */ if ((hpxdat->data = malloc((hpxdat->npix)*sizeof(float))) == NULL) { perror("HPXcvt"); goto cleanup; } nulval = HEALPIX_NULLVAL; datap = hpxdat->data; for (ipix = 0; ipix < firstpix; ipix++) { *(datap++) = nulval; } firstelem = (LONGLONG)1; if (hdutype == IMAGE_HDU) { if (fits_read_img_flt(fptr, 0l, firstelem, npix, nulval, datap, &anynul, &status)) goto fitserr; } else if (hdutype == BINARY_TBL) { for (irow = 0; irow < nrow; irow++) { if (fits_read_col_flt(fptr, hpxdat->col, irow+1, firstelem, nelem, nulval, datap, &anynul, &status)) goto fitserr; datap += nelem; } } datap = hpxdat->data + (lastpix + 1); for (ipix = (lastpix+1); ipix < hpxdat->npix; ipix++) { *(datap++) = nulval; } /* Clean up. */ fits_close_file(fptr, &status); status = 0; return 0; fitserr: fits_report_error(stderr, status); cleanup: if (naxes) free(naxes); if (hpxdat->data) free(hpxdat->data); hpxdat->data = 0x0; return 1; } /*--------------------------------------------------------------------------*/ int HPXout(struct healpix *hpxdat) { /* Number of facets on a side of each layout. */ const int NFACET[] = {5, 4, 4}; /* Arrays that define the facet location and rotation for each recognised * layout. Bear in mind that these appear to be upside-down, i.e. the top * line contains facet numbers for the bottom row of the output image. * Facets numbered -1 are blank. */ /* Equatorial (diagonal) facet layout. */ const int FACETS[][5][5] = {{{ 6, 9, -1, -1, -1}, { 1, 5, 8, -1, -1}, {-1, 0, 4, 11, -1}, {-1, -1, 3, 7, 10}, {-1, -1, -1, 2, 6}}, /* North polar (X) facet layout. */ {{ 8, 4, 4, 11, -1}, { 5, 0, 3, 7, -1}, { 5, 1, 2, 7, -1}, { 9, 6, 6, 10, -1}, {-1, -1, -1, -1, -1}}, /* South polar (X) facet layout. */ {{ 1, 6, 6, 2, -1}, { 5, 9, 10, 7, -1}, { 5, 8, 11, 7, -1}, { 0, 4, 4, 3, -1}, {-1, -1, -1, -1, -1}}}; /* All facets of the equatorial layout are rotated by +45 degrees with * respect to the normal orientation, i.e. that with the equator running * horizontally. The rotation recorded for the polar facets is the number * of additional positive (anti-clockwise) 90 degree turns with respect to * the equatorial layout. */ /* Equatorial (diagonal), no facet rotation. */ const int FROTAT[][5][5] = {{{ 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}}, /* North polar (X) facet rotation. */ {{ 3, 3, 0, 0, 0}, { 3, 3, 0, 0, 0}, { 2, 2, 1, 1, 0}, { 2, 2, 1, 1, 0}, { 0, 0, 0, 0, 0}}, /* South polar (X) facet rotation. */ {{ 1, 1, 2, 2, 0}, { 1, 1, 2, 2, 0}, { 0, 0, 3, 3, 0}, { 0, 0, 3, 3, 0}, { 0, 0, 0, 0, 0}}}; /* Facet halving codes. 0: the facet is whole (or wholly blank), * 1: blanked bottom-right, 2: top-right, 3: top-left, 4: bottom-left. * Positive values mean that the diagonal is included, otherwise not. */ /* Equatorial (diagonal), no facet halving. */ const int FHALVE[][5][5] = {{{ 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}, { 0, 0, 0, 0, 0}}, /* North polar (X) facet halving. */ {{ 0, 1, -4, 0, 0}, {-3, 0, 0, 2, 0}, { 4, 0, 0, -1, 0}, { 0, -2, 3, 0, 0}, { 0, 0, 0, 0, 0}}, /* South polar (X) facet halving. */ {{ 0, 1, -4, 0, 0}, {-3, 0, 0, 2, 0}, { 4, 0, 0, -1, 0}, { 0, -2, 3, 0, 0}, { 0, 0, 0, 0, 0}}}; char history[72]; int facet, halve, i1, i2, ifacet, j, jfacet, layout, nfacet, nside, rotn, status; long *healidx = 0x0, *healp, naxes[2]; float nulval = HEALPIX_NULLVAL, *row = 0x0, *rowp; LONGLONG fpixel, group, nelem; fitsfile *fptr; nside = hpxdat->nside; layout = hpxdat->layout; nfacet = NFACET[layout]; /* Create the output FITS file. */ status = 0; naxes[0] = nfacet * nside; naxes[1] = naxes[0]; if (fits_create_file(&fptr, hpxdat->outfile, &status)) goto fitserr; if (fits_create_img(fptr, FLOAT_IMG, 2, naxes, &status)) goto fitserr; /* Write WCS keyrecords. */ if ((status = HPXhdr(fptr, hpxdat))) goto fitserr; /* Allocate arrays. */ if ((healidx = malloc(nside * sizeof(long))) == NULL || (row = malloc(nside * sizeof(float))) == NULL) { perror("HPXcvt"); goto cleanup; } /* Loop vertically facet-by-facet. */ fpixel = 1; group = 0; nelem = nside; for (jfacet = 0; jfacet < nfacet; jfacet++) { /* Loop row-by-row. */ for (j = 0; j < nside; j++) { /* Loop horizontally facet-by-facet. */ for (ifacet = 0; ifacet < nfacet; ifacet++) { facet = FACETS[layout][jfacet][ifacet]; rotn = FROTAT[layout][jfacet][ifacet]; halve = FHALVE[layout][jfacet][ifacet]; /* Recentre longitude? */ if (hpxdat->quad && facet >= 0) { if (facet <= 3) { facet += hpxdat->quad; if (facet > 3) facet -= 4; } else if (facet <= 7) { facet += hpxdat->quad; if (facet > 7) facet -= 4; } else { facet += hpxdat->quad; if (facet > 11) facet -= 4; } } /* Write out the data. */ if (facet < 0) { /* A blank facet. */ if (fits_write_img_null(fptr, group, fpixel, nelem, &status)) { goto fitserr; } } else { if (hpxdat->ordering == 'N') { /* Get nested indices. */ status = NESTidx(nside, facet, rotn, j, healidx); } else { /* Get ring indices. */ status = RINGidx(nside, facet, rotn, j, healidx); } /* Gather data into the output vector. */ healp = healidx; for (rowp = row; rowp < row + nside; rowp++) { *rowp = hpxdat->data[*(healp++)]; } /* Apply blanking to halved facets. */ if (halve) { if (abs(halve) == 1) { /* Blank bottom-right. */ i1 = j; i2 = nside; if (halve > 0) i1++; } else if (abs(halve) == 2) { /* Blank top-right. */ i1 = nside - j; i2 = nside; if (halve < 0) i1--; } else if (abs(halve) == 3) { /* Blank top-left. */ i1 = 0; i2 = j; if (halve < 0) i2++; } else { /* Blank bottom-left. */ i1 = 0; i2 = nside - j; if (halve > 0) i2--; } for (rowp = row + i1; rowp < row + i2; rowp++) { *rowp = nulval; } } /* Write out this facet's contribution to this row of the map. */ if (fits_write_imgnull_flt(fptr, group, fpixel, nelem, row, nulval, &status)) { goto fitserr; } } fpixel += nelem; } } } /* Write history. */ sprintf(history, "Original input file: %s", hpxdat->infile); fits_write_history(fptr, history, &status); sprintf(history, " Original NSIDE: %d", hpxdat->nside); fits_write_history(fptr, history, &status); sprintf(history, " Original ordering: %s", (hpxdat->ordering == 'N') ? "NESTED" : "RING"); if (hpxdat->ordering == 'r') strcat(history, " (assumed)"); fits_write_history(fptr, history, &status); /* Clean up. */ fits_close_file(fptr, &status); status = 0; return 0; fitserr: fits_report_error(stderr, status); cleanup: if (healidx) free(healidx); if (row) free(row); return 1; } /*--------------------------------------------------------------------------*/ /* (imap,jmap) are 0-relative pixel coordinates in the output map with origin * at the bottom-left corner of the specified facet which is rotated by * (45 + rotn * 90) degrees from its natural orientation; imap increases to * the right and jmap upwards. */ int NESTidx(int nside, int facet, int rotn, int jmap, long *healidx) { int h, i, imap, j, nside1, bit; long *hp; /* Nested index (0-relative) of the first pixel in this facet. */ h = facet * nside * nside; nside1 = nside - 1; hp = healidx; for (imap = 0; imap < nside; imap++, hp++) { /* (i,j) are 0-relative pixel coordinates with origin in the southern * corner of the facet; i increases to the north-east and j to the * north-west. */ if (rotn == 0) { i = nside1 - imap; j = jmap; } else if (rotn == 1) { i = nside1 - jmap; j = nside1 - imap; } else if (rotn == 2) { i = imap; j = nside1 - jmap; } else if (rotn == 3) { i = jmap; j = imap; } *hp = 0; bit = 1; while (i || j) { if (i & 1) *hp |= bit; bit <<= 1; if (j & 1) *hp |= bit; bit <<= 1; i >>= 1; j >>= 1; } *hp += h; } return 0; } /*--------------------------------------------------------------------------*/ /* (imap,jmap) pixel coordinates are as described above for NESTidx(). This * function computes the double-pixelisation index then converts it to the * regular ring index. */ int RINGidx(int nside, int facet, int rotn, int jmap, long *healidx) { const int I0[] = { 1, 3, -3, -1, 0, 2, 4, -2, 1, 3, -3, -1}; const int J0[] = { 1, 1, 1, 1, 0, 0, 0, 0, -1, -1, -1, -1}; int i, i0, imap, j, j0, n2side, n8side, npj, npole, nside1; long *hp; n2side = 2 * nside; n8side = 8 * nside; /* Double-pixelisation index of the last pixel in the north polar cap. */ npole = (n2side - 1) * (n2side - 1) - 1; /* Double-pixelisation pixel coordinates of the centre of the facet. */ i0 = nside * I0[facet]; j0 = nside * J0[facet]; nside1 = nside - 1; hp = healidx; for (imap = 0; imap < nside; imap++, hp++) { /* (i,j) are 0-relative, double-pixelisation pixel coordinates. The * origin is at the intersection of the equator and prime meridian, * i increases to the east (N.B.) and j to the north. */ if (rotn == 0) { i = i0 + nside1 - (jmap + imap); j = j0 + jmap - imap; } else if (rotn == 1) { i = i0 + imap - jmap; j = j0 + nside1 - (imap + jmap); } else if (rotn == 2) { i = i0 + (imap + jmap) - nside1; j = j0 + imap - jmap; } else if (rotn == 3) { i = i0 + jmap - imap; j = j0 + jmap + imap - nside1; } /* Convert i for counting pixels. */ if (i < 0) i += n8side; i++; if (j > nside) { /* North polar regime. */ if (j == n2side) { *hp = 0; } else { /* Number of pixels in a polar facet with this value of j. */ npj = 2 * (n2side - j); /* Index of the last pixel in the row above this. */ *hp = (npj - 1) * (npj - 1) - 1; /* Number of pixels in this row in the polar facets before this. */ *hp += npj * (i/n2side); /* Pixel number in this polar facet. */ *hp += i%n2side - (j - nside) - 1; } } else if (j >= -nside) { /* Equatorial regime. */ *hp = npole + n8side * (nside - j) + i; } else { /* South polar regime. */ *hp = 24 * nside * nside + 1; if (j > -n2side) { /* Number of pixels in a polar facet with this value of j. */ npj = 2 * (j + n2side); /* Total number of pixels in this row or below it. */ *hp -= (npj + 1) * (npj + 1); /* Number of pixels in this row in the polar facets before this. */ *hp += npj * (i/n2side); /* Pixel number in this polar facet. */ *hp += i%n2side + (nside + j) - 1; } } /* Convert double-pixelisation index to regular. */ *hp -= 1; *hp /= 2; } return 0; } /*--------------------------------------------------------------------------*/ int HPXhdr(fitsfile *fptr, struct healpix *hpxdat) { char comment[64], cval[16], *ctype1, *ctype2, *descr1, *descr2, *pcode; int status; float crpix1, crpix2, crval1, crval2; double cdelt1, cdelt2; status = 0; fits_update_key_log(fptr, "EXTEND", 0, "No FITS extensions are present", &status); fits_write_date(fptr, &status); /* Set pixel transformation parameters. */ if (hpxdat->layout == 0) { crpix1 = (5 * hpxdat->nside + 1) / 2.0f; } else { crpix1 = (4 * hpxdat->nside + 1) / 2.0f; } crpix2 = crpix1; fits_write_key(fptr, TFLOAT, "CRPIX1", &crpix1, "Coordinate reference pixel", &status); fits_write_key(fptr, TFLOAT, "CRPIX2", &crpix2, "Coordinate reference pixel", &status); if (hpxdat->layout == 0) { fits_write_key_flt(fptr, "PC1_1", 0.5f, -1, "Transformation matrix element", &status); fits_write_key_flt(fptr, "PC1_2", 0.5f, -1, "Transformation matrix element", &status); fits_write_key_flt(fptr, "PC2_1", -0.5f, -1, "Transformation matrix element", &status); fits_write_key_flt(fptr, "PC2_2", 0.5f, -1, "Transformation matrix element", &status); } cdelt1 = -90.0 / hpxdat->nside; cdelt2 = -cdelt1; fits_write_key_dbl(fptr, "CDELT1", cdelt1, -8, "[deg] Coordinate increment", &status); fits_write_key_dbl(fptr, "CDELT2", cdelt2, -8, "[deg] Coordinate increment", &status); /* Celestial transformation parameters. */ if (hpxdat->layout == 0) { pcode = "HPX"; } else { pcode = "XPH"; } if (hpxdat->crdsys == 'G') { /* Galactic. */ ctype1 = "GLON"; ctype2 = "GLAT"; descr1 = "Galactic longitude"; descr2 = "Galactic latitude"; } else if (hpxdat->crdsys == 'E') { /* Ecliptic, who-knows-what. */ ctype1 = "ELON"; ctype2 = "ELAT"; descr1 = "Ecliptic longitude"; descr2 = "Ecliptic latitude"; } else if (hpxdat->crdsys == 'Q') { /* Equatorial, who-knows-what. */ ctype1 = "RA--"; ctype2 = "DEC-"; descr1 = "Right ascension"; descr2 = "Declination"; } else { /* Unknown. */ ctype1 = "XLON"; ctype2 = "XLAT"; descr1 = "Longitude"; descr2 = " Latitude"; } sprintf(cval, "%s-%s", ctype1, pcode); sprintf(comment, "%s in an %s projection", descr1, pcode); fits_write_key_str(fptr, "CTYPE1", cval, comment, &status); sprintf(cval, "%s-%s", ctype2, pcode); sprintf(comment, "%s in an %s projection", descr2, pcode); fits_write_key_str(fptr, "CTYPE2", cval, comment, &status); crval1 = 0.0f + 90.0f * hpxdat->quad; if (hpxdat->layout == 0) { crval2 = 0.0f; } else if (hpxdat->layout == 1) { crval2 = 90.0f; } else { crval2 = -90.0f; } sprintf(comment, "[deg] %s at the reference point", descr1); fits_write_key(fptr, TFLOAT, "CRVAL1", &crval1, comment, &status); sprintf(comment, "[deg] %s at the reference point", descr2); fits_write_key(fptr, TFLOAT, "CRVAL2", &crval2, comment, &status); if (hpxdat->layout == 0) { fits_write_key_lng(fptr, "PV2_1", (LONGLONG)4, "HPX H parameter (longitude)", &status); fits_write_key_lng(fptr, "PV2_2", (LONGLONG)3, "HPX K parameter (latitude)", &status); } /* Commentary. */ fits_write_record(fptr, " ", &status); if (hpxdat->layout == 0) { fits_write_comment(fptr, "Celestial map with FITS-standard HPX coordinate system generated by", &status); } else { fits_write_comment(fptr, "Celestial map with experimental XPH coordinate system generated by", &status); } fits_write_comment(fptr, "'HPXcvt' which reorganises HEALPix data without interpolation as", &status); fits_write_comment(fptr, "described in \"Mapping on the HEALPix grid\" by Mark Calabretta and", &status); fits_write_comment(fptr, "Boud Roukema. See http://www.atnf.csiro.au/people/mcalabre", &status); return status; } pywcs-1.12/wcslib/utils/wcsgrid.c0000644001153600020070000002311612310355626021102 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsgrid.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * * wcsgrid extracts the WCS keywords for an image from the specified FITS file * and uses pgsbox() to plot a 2-D coordinate graticule for each representation * found. Refer to the usage notes below. * * TODO * Subimaging option. *---------------------------------------------------------------------------*/ char usage[] = "Usage: wcsgrid [-a] [-d] [-h] []\n" "\n" "wcsgrid extracts the WCS keywords for an image from the specified FITS\n" "file and uses pgsbox() to plot a 2-D coordinate graticule for each\n" "alternate representation found.\n\n" "The FITS file may be specified according to the syntax understood by\n" "cfitsio, for example \"file.fits.gz+1\" refers to the first extension of\n" "a gzip'd FITS file. Use \"-\" or omit the file name for input from stdin.\n" "\n" "Options:\n" " -a Plot a graticule only for the alternate representation\n" " specified (ignored if there is only one).\n" " -d PGPLOT device type (default XWINDOW, use \"?\" for list).\n" " -h Move to HDU number (1-relative) which is expected to\n" " contain an image array. (Useful for input from stdin.)\n"; #include #include #include #include #include #include #include #include #include #include #include #include int main(int argc, char **argv) { char alt = '\0', *header, idents[3][80], *infile, keyword[16], nlcprm[1], opt[2], pgdev[16]; int c0[] = {-1, -1, -1, -1, -1, -1, -1}; int alts[27], gcode[2], hdunum = 1, hdutype, i, ic, naxes, naxis[2], nkeyrec, nreject, nwcs, stat[NWCSFIX], status; float blc[2], trc[2]; double cache[257][4], grid1[3], grid2[3], nldprm[1]; struct wcsprm *wcs; nlfunc_t pgwcsl_; fitsfile *fptr; /* Parse options. */ strcpy(pgdev, "/XWINDOW"); for (i = 1; i < argc && argv[i][0] == '-'; i++) { if (!argv[i][1]) break; switch (argv[i][1]) { case 'a': alt = toupper(argv[i][2]); break; case 'd': if (argv[i][2] == '?') { cpgldev(); return 0; } if (argv[i][2] == '/') { strncpy(pgdev+1, argv[i]+3, 15); } else { strncpy(pgdev+1, argv[i]+2, 15); } break; case 'h': hdunum = atoi(argv[i]+2); break; default: fprintf(stderr, "%s", usage); return 1; } } if (i < argc) { infile = argv[i++]; if (i < argc) { fprintf(stderr, "%s", usage); return 1; } } else { infile = "-"; } /* Check accessibility of the input file. */ if (strcmp(infile, "-") && access(infile, R_OK) == -1) { printf("wcsgrid: Cannot access %s.\n", infile); return 1; } /* Open the FITS file and move to the required HDU. */ status = 0; if (fits_open_file(&fptr, infile, READONLY, &status)) goto fitserr; if (fits_movabs_hdu(fptr, hdunum, &hdutype, &status)) goto fitserr; if (hdutype != IMAGE_HDU) { fprintf(stderr, "ERROR, HDU number %d does not contain an image array.\n", hdunum); return 1; } /* Check that we have at least two image axes. */ if (fits_read_key(fptr, TINT, "NAXIS", &naxes, NULL, &status)) { goto fitserr; } if (naxes < 2) { fprintf(stderr, "ERROR, HDU number %d does not contain a 2-D image.\n", hdunum); return 1; } else if (naxes > 2) { printf("HDU number %d contains a %d-D image array.\n", hdunum, naxes); } /* Read in the FITS header, excluding COMMENT and HISTORY keyrecords. */ if (fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status)) { goto fitserr; } /* Interpret the WCS keywords. */ if ((status = wcspih(header, nkeyrec, WCSHDR_all, -3, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status, wcshdr_errmsg[status]); return 1; } free(header); /* Read -TAB arrays from the binary table extension (if necessary). */ if (fits_read_wcstab(fptr, wcs->nwtb, (wtbarr *)wcs->wtb, &status)) { goto fitserr; } /* Translate non-standard WCS keyvalues. */ if ((status = wcsfix(7, 0, wcs, stat))) { status = 0; for (i = 0; i < NWCSFIX; i++) { if (stat[i] > 0) { fprintf(stderr, "wcsfix ERROR %d: %s.\n", stat[i], wcsfix_errmsg[stat[i]]); /* Ignore problems with CDi_ja and DATE-OBS. */ if (!(i == CDFIX || i == DATFIX)) status = 1; } } if (status) return 1; } /* Sort out alternates. */ if (alt) { wcsidx(nwcs, &wcs, alts); if (alt == ' ') { if (alts[0] == -1) { fprintf(stderr, "WARNING, no primary coordinate representation, " "doing all.\n"); alt = '\0'; } } else if (alt < 'A' || alt > 'Z') { fprintf(stderr, "WARNING, alternate specifier \"%c\" is invalid, " "doing all.\n", alt); alt = '\0'; } else { if (alts[alt - 'A' + 1] == -1) { fprintf(stderr, "WARNING, no alternate coordinate representation " "\"%c\", doing all.\n", alt); alt = '\0'; } } } /* Get image dimensions from the header. */ sprintf(keyword, "NAXIS%d", wcs->lng + 1); fits_read_key(fptr, TINT, "NAXIS1", naxis, NULL, &status); sprintf(keyword, "NAXIS%d", wcs->lat + 1); fits_read_key(fptr, TINT, "NAXIS2", naxis+1, NULL, &status); if ((naxis[0] < 2) || (naxis[1] < 2)) { fprintf(stderr, "ERROR, HDU number %d contains degenerate image axes.\n", hdunum); return 1; } fits_close_file(fptr, &status); /* Plot setup. */ blc[0] = 0.5f; blc[1] = 0.5f; trc[0] = naxis[0] + 0.5f; trc[1] = naxis[1] + 0.5f; if (cpgbeg(0, pgdev, 1, 1) != 1) { fprintf(stderr, "ERROR, failed to open PGPLOT device %s.\n", pgdev); return 1; } cpgvstd(); cpgwnad(blc[0], trc[0], blc[0], trc[1]); cpgask(1); cpgpage(); /* Compact lettering. */ cpgsch(0.8f); /* Draw full grid lines. */ gcode[0] = 2; gcode[1] = 2; grid1[0] = 0.0; grid2[0] = 0.0; /* These are for the projection boundary. */ grid1[1] = -180.0; grid1[2] = 180.0; grid2[1] = -90.0; grid2[2] = 90.0; cpgsci(1); for (i = 0; i < nwcs; i++) { if (alt && (wcs+i)->alt[0] != alt) { continue; } if ((status = wcsset(wcs+i))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); continue; } /* Draw the frame. */ cpgbox("BC", 0.0f, 0, "BC", 0.0f, 0); /* Axis labels; use CNAMEia in preference to CTYPEia. */ if ((wcs+i)->cname[0][0]) { strcpy(idents[0], (wcs+i)->cname[0]); } else { strcpy(idents[0], (wcs+i)->ctype[0]); } if ((wcs+i)->cname[1][0]) { strcpy(idents[1], (wcs+i)->cname[1]); } else { strcpy(idents[1], (wcs+i)->ctype[1]); } /* Title; use WCSNAME. */ strcpy(idents[2], (wcs+i)->wcsname); if (strlen(idents[2])) { printf("\n%s\n", idents[2]); } /* Formatting control for celestial coordinates. */ if (strncmp((wcs+i)->ctype[0], "RA", 2) == 0) { /* Right ascension in HMS, declination in DMS. */ opt[0] = 'G'; opt[1] = 'E'; } else { /* Other angles in decimal degrees. */ opt[0] = 'A'; opt[1] = 'B'; } /* Draw the celestial grid. The grid density is set for each world */ /* coordinate by specifying LABDEN = 1224. */ ic = -1; cpgsbox(blc, trc, idents, opt, 0, 1224, c0, gcode, 0.0, 0, grid1, 0, grid2, 0, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(wcs+i), nldprm, 256, &ic, cache, &status); /* Delimit the projection boundary. */ if ((wcs+i)->cel.prj.category != ZENITHAL) { /* Reset to the native coordinate graticule. */ (wcs+i)->crval[0] = (wcs+i)->cel.prj.phi0; (wcs+i)->crval[1] = (wcs+i)->cel.prj.theta0; (wcs+i)->lonpole = 999.0; (wcs+i)->latpole = 999.0; status = wcsset(wcs+i); ic = -1; cpgsbox(blc, trc, idents, opt, -1, 0, c0, gcode, 0.0, 2, grid1, 2, grid2, 0, pgwcsl_, 1, WCSLEN, 1, nlcprm, (int *)(wcs+i), nldprm, 256, &ic, cache, &status); } cpgpage(); } status = wcsvfree(&nwcs, &wcs); return 0; fitserr: fits_report_error(stderr, status); fits_close_file(fptr, &status); return 1; } pywcs-1.12/wcslib/utils/wcsware.c0000644001153600020070000002471512310355626021121 0ustar cslocumSTSCI\science00000000000000/*============================================================================ WCSLIB 4.10 - an implementation of the FITS WCS standard. Copyright (C) 1995-2012, Mark Calabretta This file is part of WCSLIB. WCSLIB is free software: you can redistribute it and/or modify it under the terms of the GNU Lesser General Public License as published by the Free Software Foundation, either version 3 of the License, or (at your option) any later version. WCSLIB is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU Lesser General Public License for more details. You should have received a copy of the GNU Lesser General Public License along with WCSLIB. If not, see . Correspondence concerning WCSLIB may be directed to: Internet email: mcalabre@atnf.csiro.au Postal address: Dr. Mark Calabretta Australia Telescope National Facility, CSIRO PO Box 76 Epping NSW 1710 AUSTRALIA Author: Mark Calabretta, Australia Telescope National Facility http://www.atnf.csiro.au/~mcalabre/index.html $Id: wcsware.c,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *============================================================================= * wcsware extracts the WCS keywords for an image from the specified FITS file, * constructs wcsprm structs for each coordinate representation found and * performs a variety of operations using them. *---------------------------------------------------------------------------*/ char usage[] = "Usage: wcsware [-a] [-f] [-h] [-p] [-x] []\n" "\n" "wcsware extracts the WCS keywords for an image from the specified FITS\n" "file, constructs wcsprm structs for each coordinate representation found\n" "and performs a variety of operations using them.\n\n" "The FITS file may be specified according to the syntax understood by\n" "cfitsio, for example \"file.fits.gz+1\" refers to the first extension of\n" "a gzip'd FITS file. Use \"-\" or omit the file name for input from stdin.\n" "\n" "Options:\n" " -a Specify an alternate coordinate representation to be used\n" " (ignored if there is only one).\n" " -f Apply wcsfix() to the header.\n" " -h Move to HDU number (1-relative) which is expected to\n" " contain an image array. (Useful for input from stdin.)\n" " -p Print the struct(s) using wcsprt() (default operation).\n" " -x Convert pixel coordinates, obtained from stdin, to world\n" " coordinates using wcsp2s().\n" " -w Convert world coordinates, obtained from stdin, to pixel\n" " coordinates using wcss2p().\n"; #include #include #include #include #include #include #include #include #include #include int main(int argc, char **argv) { char alt = ' ', *header, idents[3][80], *infile; int alts[27], c, dofix = 0, doprt = 0, dopix = 0, doworld = 0, hdunum = 1, hdutype, i, j, nelem, nkeyrec, nreject, nwcs, *stat = 0x0, status; double *imgcrd = 0x0, phi, *pixcrd = 0x0, theta, *world = 0x0; struct wcsprm *wcs; fitsfile *fptr; /* Parse options. */ for (i = 1; i < argc && argv[i][0] == '-'; i++) { if (!argv[i][1]) break; switch (argv[i][1]) { case 'a': alt = toupper(argv[i][2]); break; case 'f': dofix = 1; break; case 'h': hdunum = atoi(argv[i]+2); break; case 'p': doprt = 1; break; case 'x': dopix = 1; break; case 'w': doworld = 1; break; default: fprintf(stderr, "%s", usage); return 1; } } if (i < argc) { infile = argv[i++]; if (i < argc) { fprintf(stderr, "%s", usage); return 1; } } else { infile = "-"; } /* Check accessibility of the input file. */ if (strcmp(infile, "-") && access(infile, R_OK) == -1) { printf("wcsware: Cannot access %s.\n", infile); return 1; } if (!dopix && !doworld) doprt = 1; /* Open the FITS file and move to the required HDU. */ status = 0; if (fits_open_file(&fptr, infile, READONLY, &status)) goto fitserr; if (fits_movabs_hdu(fptr, hdunum, &hdutype, &status)) goto fitserr; if (hdutype != IMAGE_HDU) { fprintf(stderr, "ERROR, HDU number %d does not contain an image array.\n", hdunum); return 1; } /* Read in the FITS header, excluding COMMENT and HISTORY keyrecords. */ if (fits_hdr2str(fptr, 1, NULL, 0, &header, &nkeyrec, &status)) { goto fitserr; } /* Interpret the WCS keywords. */ if ((status = wcspih(header, nkeyrec, WCSHDR_all, -3, &nreject, &nwcs, &wcs))) { fprintf(stderr, "wcspih ERROR %d: %s.\n", status, wcshdr_errmsg[status]); return 1; } free(header); if (wcs == 0x0) { fprintf(stderr, "No world coordinate systems found.\n"); return 1; } /* Read -TAB arrays from the binary table extension (if necessary). */ if (fits_read_wcstab(fptr, wcs->nwtb, (wtbarr *)wcs->wtb, &status)) { goto fitserr; } fits_close_file(fptr, &status); /* Translate non-standard WCS keyvalues? */ if (dofix) { stat = malloc(NWCSFIX * sizeof(int)); if ((status = wcsfix(7, 0, wcs, stat))) { for (i = 0; i < NWCSFIX; i++) { if (stat[i] > 0) { fprintf(stderr, "wcsfix ERROR %d: %s.\n", status, wcsfix_errmsg[stat[i]]); } } return 1; } } /* Sort out alternates. */ if (alt) { wcsidx(nwcs, &wcs, alts); if (alt == ' ') { if (alts[0] == -1) { fprintf(stderr, "WARNING, no primary coordinate representation.\n"); alt = '\0'; } } else if (alt < 'A' || alt > 'Z') { fprintf(stderr, "WARNING, alternate specifier \"%c\" is invalid.\n", alt); alt = '\0'; } else { if (alts[alt - 'A' + 1] == -1) { fprintf(stderr, "WARNING, no alternate coordinate representation " "\"%c\".\n", alt); alt = '\0'; } } } /* Initialize and possibly print the structs. */ for (i = 0; i < nwcs; i++) { if (alt && (wcs+i)->alt[0] != alt) { continue; } else if (i) { printf("\nType for next: "); fgetc(stdin); } if ((status = wcsset(wcs+i))) { fprintf(stderr, "wcsset ERROR %d: %s.\n", status, wcs_errmsg[status]); continue; } /* Get WCSNAME out of the wcsprm struct. */ strcpy(idents[2], (wcs+i)->wcsname); if (strlen(idents[2])) { printf("\n%s\n", idents[2]); } /* Print the struct. */ if (doprt) { wcsprt(wcs+i); } /* Transform coordinates? */ if (dopix || doworld) { nelem = (wcs+i)->naxis; world = realloc(world, nelem * sizeof(double)); imgcrd = realloc(imgcrd, nelem * sizeof(double)); pixcrd = realloc(pixcrd, nelem * sizeof(double)); stat = realloc(stat, nelem * sizeof(int)); if (dopix) { /* Transform pixel coordinates. */ while (1) { printf("\nEnter %d pixel coordinate element%s: ", nelem, (nelem==1)?"":"s"); c = fgetc(stdin); if (c == EOF || c == '\n') { if (c == EOF) printf("\n"); break; } ungetc(c, stdin); scanf("%lf", pixcrd); for (j = 1; j < nelem; j++) { scanf("%*[ ,]%lf", pixcrd+j); } while (fgetc(stdin) != '\n'); printf("Pixel: "); for (j = 0; j < nelem; j++) { printf("%s%14.9g", j?", ":"", pixcrd[j]); } if ((status = wcsp2s(wcs+i, 1, nelem, pixcrd, imgcrd, &phi, &theta, world, stat))) { fprintf(stderr, "wcsp2s ERROR %d: %s.\n", status, wcs_errmsg[status]); } else { printf("\nImage: "); for (j = 0; j < nelem; j++) { if (j == (wcs+i)->lng || j == (wcs+i)->lat) { /* Print angles in fixed format. */ printf("%s%14.6f", j?", ":"", imgcrd[j]); } else { printf("%s%14.9g", j?", ":"", imgcrd[j]); } } printf("\nWorld: "); for (j = 0; j < nelem; j++) { if (j == (wcs+i)->lng || j == (wcs+i)->lat) { /* Print angles in fixed format. */ printf("%s%14.6f", j?", ":"", world[j]); } else { printf("%s%14.9g", j?", ":"", world[j]); } } printf("\n"); } } } if (doworld) { /* Transform world coordinates. */ while (1) { printf("\nEnter %d world coordinate element%s: ", nelem, (nelem==1)?"":"s"); c = fgetc(stdin); if (c == EOF || c == '\n') { if (c == EOF) printf("\n"); break; } ungetc(c, stdin); scanf("%lf", world); for (j = 1; j < nelem; j++) { scanf("%*[ ,]%lf", world+j); } while (fgetc(stdin) != '\n'); printf("World: "); for (j = 0; j < nelem; j++) { if (j == (wcs+i)->lng || j == (wcs+i)->lat) { /* Print angles in fixed format. */ printf("%s%14.6f", j?", ":"", world[j]); } else { printf("%s%14.9g", j?", ":"", world[j]); } } if ((status = wcss2p(wcs+i, 1, nelem, world, &phi, &theta, imgcrd, pixcrd, stat))) { fprintf(stderr, "wcss2p ERROR %d: %s.\n", status, wcs_errmsg[status]); } else { printf("\nImage: "); for (j = 0; j < nelem; j++) { if (j == (wcs+i)->lng || j == (wcs+i)->lat) { /* Print angles in fixed format. */ printf("%s%14.6f", j?", ":"", imgcrd[j]); } else { printf("%s%14.9g", j?", ":"", imgcrd[j]); } } printf("\nPixel: "); for (j = 0; j < nelem; j++) { printf("%s%14.9g", j?", ":"", pixcrd[j]); } printf("\n"); } } } } } status = wcsvfree(&nwcs, &wcs); return 0; fitserr: fits_report_error(stderr, status); fits_close_file(fptr, &status); return 1; } pywcs-1.12/wcslib/VALIDATION0000644001153600020070000001521612310355626017513 0ustar cslocumSTSCI\science00000000000000Platforms on which the installation procedures and test suite were exercised WCSLIB version 4.10 (2012/02/06) -------------------------------- * Dell Latitude D630 (Intel Centrino, i686) running Debian linux 5.0.9 (lenny) uname -r (kernel version): 2.6.32-bpo.5-686 gcc --version: gcc --version: g gfortran --version: GNU Fortran (Debian 4.3.2-1.1) 4.3.2 WCSLIB version 4.8 (2011/08/15) ------------------------------- * Dell Latitude D620 (Intel Centrino Duo, i686), Debian linux 4.0 (etch) uname -r (kernel version): 2.6.24-1-686 (32-bit) gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) * Dell PowerEdge 2950 (Intel Xeon, 8 x X5460), Debian linux 5.0.8 (lenny) uname -r (kernel version): 2.6.26-2-amd64 (64-bit) gcc --version: gcc (Debian 4.3.2-1.1) 4.3.2 gfortran --version: GNU Fortran (Debian 4.3.2-1.1) 4.3.2 * Marvell SheevaPlug (Feroceon 88FR131 rev 1 ARM v5L), Debian linux 6.0 (squeeze) uname -r (kernel version): 2.6.32-5-kirkwood gcc --version: gcc (Debian 4.4.5-8) 4.4.5 gfortran --version: GNU Fortran (Debian 4.4.5-8) 4.4.5 * Mac mini (Intel Core 2 Duo) running Mac OS X 10.6.2 (10C540) uname -r (Darwin kernel version): 10.2.0 gcc --version: i686-apple-darwin10-gcc-4.2.1 (GCC) 4.2.1 (Apple Inc. build 5646) gfortran --version: GNU Fortran (GCC) 4.5.0 20100107 (experimental) * Enterprise 450 Model 2250 (Sparc, sun4u 64-bit), SunOS 5.9 (Solaris 9) uname -r (SunOS version): 5.9 gcc --version: gcc (GCC) 4.5.1 gfortran --version: GNU Fortran (GCC) 4.5.1 WCSLIB version 4.7 (2011/02/07) ------------------------------- * Dell Latitude D630 (Intel Centrino, i686) running Debian linux 4.0 (etch) uname -r (kernel version): 2.6.24-1-686 gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) * Sun SunFire V20z (AMD Opteron, x86_64) running Debian linux 4.0 (etch) uname -r (kernel version): 2.6.18-6-amd64 gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) * Enterprise 450 Model 2250 (Sparc, sun4u 64-bit), SunOS 5.9 (Solaris 9) uname -r (SunOS version): 5.9 gcc --version: gcc (GCC) 4.5.1 gfortran --version: GNU Fortran (GCC) 4.5.1 and cc -V: cc: Sun WorkShop 6 update 2 C 5.3 Patch 111679-14 2004/02/20 f77 -V: f77: Sun WorkShop 6 update 2 FORTRAN 77 5.3 Patch 111691-07 2004/04/23 * Mac Xserve (Quad-Core Intel Xeon) running Mac OS X 10.6.5 (10H575) uname -r (Darwin kernel version): 10.5.0 gcc --version: 4.2.1 (Apple Inc. build 5664) gfortran --version: GNU Fortran (GCC) 4.5.0 20100107 (experimental) * Mac mini (Intel Core 2 Duo) running Mac OS X 10.6.2 (10C540) uname -r (Darwin kernel version): 10.2.0 gcc --version: i686-apple-darwin10-gcc-4.2.1 (GCC) 4.2.1 (Apple Inc. build 5646) gfortran --version: GNU Fortran (GCC) 4.5.0 20100107 (experimental) * Mac mini (Intel Core Duo) running Mac OS X 10.4.9 (8P2137) uname -r (Darwin kernel version): 8.9.1 gcc --version: gcc (GCC) 4.3.0 20070316 (experimental) g77 --version: GNU Fortran (GCC) 3.4.0 WCSLIB version 4.5 (2010/07/16) ------------------------------- * Dell Latitude D630 (Intel Centrino, i686) running Debian linux 4.0 (etch) uname -r (kernel version): 2.6.24-1-686 gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) and gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) ifort -V: Intel(R) Fortran Compiler for 32-bit applications, Version 8.1 Build 20041118Z Package ID: l_fc_pc_8.1.023 * Mac mini (Intel Core 2 Duo, i386) running Mac OS X 10.6.2 (10C540) uname -r (Darwin kernel version): 10.2.0 gcc --version: i686-apple-darwin10-gcc-4.2.1 (GCC) 4.2.1 (Apple Inc. build 5646) gfortran --version: GNU Fortran (GCC) 4.5.0 20100107 (experimental) * Mac mini (Intel Core Duo, i386) running Mac OS X 10.4.9 (8P2137) uname -r (Darwin kernel version): 8.9.1 gcc --version: gcc (GCC) 4.3.0 20070316 (experimental) g77 --version: GNU Fortran (GCC) 3.4.0 and gcc --version: gcc (GCC) 4.3.0 20070316 (experimental) gfortran --version: GNU Fortran (GCC) 4.3.0 20070316 (experimental) * Sun SunFire V20z (AMD Opteron, x86_64) running Debian linux 4.0 (etch) uname -r (kernel version): 2.6.18-6-amd64 gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) and gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) gfortran --version: GNU Fortran 95 (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) * Sun Ultra-60 (Sparc, sun4u) running SunOS 5.6 (Solaris 2.6) uname -r (SunOS version): 5.6 gcc --version: 2.95.3 g77 --version: GNU Fortran 0.5.25 20010315 (release) and cc -V: cc: Sun WorkShop 6 update 2 C 5.3 Patch 111679-14 2004/02/20 f77 -V: f77: Sun WorkShop 6 update 2 FORTRAN 77 5.3 Patch 111691-07 2004/04/23 WCSLIB version 4.4 (2009/08/06) ------------------------------- * Dell Latitude D630 (Intel Centrino, i686) running Debian linux 4.0 (etch) uname -r (kernel version): 2.6.24-1-686 gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) * Mac mini (Intel Core Duo, i386) running Mac OS X 10.4.9 (8P2137) uname -r (Darwin kernel version): 8.9.1 gcc --version: gcc (GCC) 4.3.0 20070316 (experimental) g77 --version: GNU Fortran (GCC) 3.4.0 and gcc --version: gcc (GCC) 4.3.0 20070316 (experimental) gfortran --version: GNU Fortran (GCC) 4.3.0 20070316 (experimental) * Sun SunFire V20z (AMD Opteron, x86_64) running Debian linux 4.0 (etch) uname -r (kernel version): 2.6.18-6-amd64 gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) g77 --version: GNU Fortran (GCC) 3.4.6 (Debian 3.4.6-5) and gcc --version: gcc (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) gfortran --version: GNU Fortran 95 (GCC) 4.1.2 20061115 (prerelease) (Debian 4.1.1-21) * Sun SunBlade 1000 (Sparc, sun4u) running SunOS 5.8 (Solaris 2.8) uname -r (SunOS version): 5.8 gcc --version: 2.95.3 g77 --version: GNU Fortran 0.5.25 20010315 (release) and cc -V: cc: Sun WorkShop 6 update 2 C 5.3 Patch 111679-14 2004/02/20 f77 -V: f77: Sun WorkShop 6 update 2 FORTRAN 77 5.3 Patch 111691-07 2004/04/23 ------------------------------------------------------------------------------ $Id: VALIDATION,v 4.10 2012/02/05 23:41:45 cal103 Exp $ pywcs-1.12/wcslib/wcsconfig.h.in0000644001153600020070000000122512310355626020671 0ustar cslocumSTSCI\science00000000000000/*============================================================================ * * wcsconfig.h is generated from wcsconfig.h.in by 'configure'. It contains * C preprocessor macro definitions for compiling WCSLIB 4.10 * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcsconfig.h.in,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *===========================================================================*/ /* WCSLIB library version number. */ #undef WCSLIB_VERSION /* Define to 1 if sincos() is available. */ #undef HAVE_SINCOS /* 64-bit integer data type. */ #undef WCSLIB_INT64 pywcs-1.12/wcslib/wcsconfig_f77.h.in0000644001153600020070000000207412310355626021357 0ustar cslocumSTSCI\science00000000000000/*============================================================================ * * wcsconfig_f77.h is generated from wcsconfig_f77.h.in by 'configure'. It * contains C preprocessor definitions for building the WCSLIB 4.10 Fortran * wrappers. * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcsconfig_f77.h.in,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *===========================================================================*/ /* Integer array type large enough to hold an address. Set here to int[2] for * 64-bit addresses, but could be defined as int* on 32-bit machines. */ typedef int iptr[2]; /* Macro for mangling Fortran subroutine names that do not contain * underscores. Typically a name like "WCSINI" (case-insensitive) will become * something like "wcsini_" (case-sensitive). The Fortran wrappers, which are * written in C, are preprocessed into names that match the latter. The macro * takes two arguments which specify the name in lower and upper case. */ #undef F77_FUNC pywcs-1.12/wcslib/wcsconfig_tests.h.in0000644001153600020070000000126712310355626022121 0ustar cslocumSTSCI\science00000000000000/*============================================================================ * * wcsconfig_test.h is generated from wcsconfig_test.h.in by 'configure'. It * contains C preprocessor definitions for compiling the WCSLIB 4.10 test/demo * programs. * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcsconfig_tests.h.in,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *===========================================================================*/ #include /* Define to 1 if the CFITSIO library is available. */ #undef HAVE_CFITSIO /* Define to the printf format modifier for size_t type. */ #undef MODZ pywcs-1.12/wcslib/wcsconfig_utils.h.in0000644001153600020070000000250012310355626022106 0ustar cslocumSTSCI\science00000000000000/*============================================================================ * * wcsconfig_utils.h is generated from wcsconfig_utils.h.in by 'configure'. * It contains C preprocessor macro definitions for compiling the WCSLIB 4.10 * utilities. * * Author: Mark Calabretta, Australia Telescope National Facility * http://www.atnf.csiro.au/~mcalabre/index.html * $Id: wcsconfig_utils.h.in,v 4.10 2012/02/05 23:41:45 cal103 Exp $ *===========================================================================*/ #include /* Definitions for Large File Support (LFS), i.e. files larger than 2GiB, for * the fitshdr utility. */ /* Define to 1 if fseeko() is available (for small or large files). */ #undef HAVE_FSEEKO /* Define _LARGEFILE_SOURCE to get prototypes from stdio.h for the LFS * functions fseeko() and ftello() which use an off_t argument in place of a * long. */ #undef _LARGEFILE_SOURCE /* There seems to be a bug in autoconf that causes _LARGEFILE_SOURCE not to be * set in Linux. This dreadful kludge gets around it for now. */ #if (defined HAVE_FSEEKO && !defined _LARGEFILE_SOURCE) #define _LARGEFILE_SOURCE #endif /* Number of bits in a file offset (off_t) on systems where it can be set. */ #undef _FILE_OFFSET_BITS /* Define for large files needed on AIX-type systems. */ #undef _LARGE_FILES pywcs-1.12/wcslib/wcslib.pc.in0000644001153600020070000000041412310355626020344 0ustar cslocumSTSCI\science00000000000000prefix=@prefix@ exec_prefix=@exec_prefix@ libdir=@libdir@ includedir=@includedir@/wcslib Name: WCSLIB Description: An implementation of the FITS World Coordinate System standard Version: @PACKAGE_VERSION@ Requires: Libs: -L${libdir} -lwcs -lm Cflags: -I${includedir} pywcs-1.12/wcslib/wcslib.pdf0000644001153600020070000645654512310355626020140 0ustar cslocumSTSCI\science00000000000000%PDF-1.4 %ÐÔÅØ 5 0 obj << /S /GoTo /D (section.1) >> endobj 8 0 obj 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(\376\377\000F\000i\000l\000e\000\040\000I\000n\000d\000e\000x) endobj 33 0 obj << /S /GoTo /D (subsection.4.1) >> endobj 36 0 obj (\376\377\000F\000i\000l\000e\000\040\000L\000i\000s\000t) endobj 37 0 obj << /S /GoTo /D (section.5) >> endobj 40 0 obj (\376\377\000D\000a\000t\000a\000\040\000S\000t\000r\000u\000c\000t\000u\000r\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 41 0 obj << /S /GoTo /D (subsection.5.1) >> endobj 44 0 obj (\376\377\000c\000e\000l\000p\000r\000m\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 45 0 obj << /S /GoTo /D (subsubsection.5.1.1) >> endobj 48 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 49 0 obj << /S /GoTo /D (subsubsection.5.1.2) >> endobj 52 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 53 0 obj << /S /GoTo /D (subsection.5.2) >> endobj 56 0 obj (\376\377\000f\000i\000t\000s\000k\000e\000y\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 57 0 obj << /S /GoTo /D (subsubsection.5.2.1) >> endobj 60 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 61 0 obj << /S /GoTo /D (subsubsection.5.2.2) >> endobj 64 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 65 0 obj << /S /GoTo /D (subsection.5.3) >> endobj 68 0 obj (\376\377\000f\000i\000t\000s\000k\000e\000y\000i\000d\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 69 0 obj << /S /GoTo /D (subsubsection.5.3.1) >> endobj 72 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 73 0 obj << /S /GoTo /D (subsubsection.5.3.2) >> endobj 76 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 77 0 obj << /S /GoTo /D (subsection.5.4) >> endobj 80 0 obj (\376\377\000l\000i\000n\000p\000r\000m\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 81 0 obj << /S /GoTo /D (subsubsection.5.4.1) >> endobj 84 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 85 0 obj << /S /GoTo /D (subsubsection.5.4.2) >> endobj 88 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 89 0 obj << /S /GoTo /D (subsection.5.5) >> endobj 92 0 obj (\376\377\000p\000r\000j\000p\000r\000m\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 93 0 obj << /S /GoTo /D (subsubsection.5.5.1) >> endobj 96 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 97 0 obj << /S /GoTo /D (subsubsection.5.5.2) >> endobj 100 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 101 0 obj << /S /GoTo /D (subsection.5.6) >> endobj 104 0 obj (\376\377\000p\000s\000c\000a\000r\000d\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 105 0 obj << /S /GoTo /D (subsubsection.5.6.1) >> endobj 108 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 109 0 obj << /S /GoTo /D (subsubsection.5.6.2) >> endobj 112 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 113 0 obj << /S /GoTo /D (subsection.5.7) >> endobj 116 0 obj 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(\376\377\000w\000c\000s\000p\000r\000m\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 177 0 obj << /S /GoTo /D (subsubsection.5.12.1) >> endobj 180 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 181 0 obj << /S /GoTo /D (subsubsection.5.12.2) >> endobj 184 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 185 0 obj << /S /GoTo /D (subsection.5.13) >> endobj 188 0 obj (\376\377\000w\000t\000b\000a\000r\000r\000\040\000S\000t\000r\000u\000c\000t\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 189 0 obj << /S /GoTo /D (subsubsection.5.13.1) >> endobj 192 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 193 0 obj << /S /GoTo /D (subsubsection.5.13.2) >> endobj 196 0 obj (\376\377\000F\000i\000e\000l\000d\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 197 0 obj << /S /GoTo /D (section.6) >> endobj 200 0 obj (\376\377\000F\000i\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 201 0 obj << /S /GoTo /D (subsection.6.1) >> endobj 204 0 obj (\376\377\000c\000e\000l\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 205 0 obj << /S /GoTo /D (subsubsection.6.1.1) >> endobj 208 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 209 0 obj << /S /GoTo /D (subsubsection.6.1.2) >> endobj 212 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 213 0 obj << /S /GoTo /D (subsubsection.6.1.3) >> endobj 216 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 217 0 obj << /S /GoTo /D (subsubsection.6.1.4) >> endobj 220 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 221 0 obj << /S /GoTo /D (subsubsection.6.1.5) >> endobj 224 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 225 0 obj << /S /GoTo /D (subsection.6.2) >> endobj 228 0 obj (\376\377\000f\000i\000t\000s\000h\000d\000r\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 229 0 obj << /S /GoTo /D (subsubsection.6.2.1) >> endobj 232 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 233 0 obj << /S /GoTo /D (subsubsection.6.2.2) >> endobj 236 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 237 0 obj << /S /GoTo /D (subsubsection.6.2.3) >> endobj 240 0 obj (\376\377\000T\000y\000p\000e\000d\000e\000f\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 241 0 obj << /S /GoTo /D (subsubsection.6.2.4) >> endobj 244 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 245 0 obj << /S /GoTo /D (subsubsection.6.2.5) >> endobj 248 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 249 0 obj << /S /GoTo /D (subsection.6.3) >> endobj 252 0 obj (\376\377\000g\000e\000t\000w\000c\000s\000t\000a\000b\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 253 0 obj << /S /GoTo /D (subsubsection.6.3.1) >> endobj 256 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 257 0 obj << /S /GoTo /D (subsubsection.6.3.2) >> endobj 260 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 261 0 obj << /S /GoTo /D (subsection.6.4) >> endobj 264 0 obj (\376\377\000l\000i\000n\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 265 0 obj << /S /GoTo /D (subsubsection.6.4.1) >> endobj 268 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 269 0 obj << /S /GoTo /D (subsubsection.6.4.2) >> endobj 272 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 273 0 obj << /S /GoTo /D (subsubsection.6.4.3) >> endobj 276 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 277 0 obj << /S /GoTo /D (subsubsection.6.4.4) >> endobj 280 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 281 0 obj << /S /GoTo /D (subsubsection.6.4.5) >> endobj 284 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 285 0 obj << /S /GoTo /D (subsection.6.5) >> endobj 288 0 obj (\376\377\000l\000o\000g\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 289 0 obj << /S /GoTo /D (subsubsection.6.5.1) >> endobj 292 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 293 0 obj << /S /GoTo /D (subsubsection.6.5.2) >> endobj 296 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 297 0 obj << /S /GoTo /D (subsubsection.6.5.3) >> endobj 300 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 301 0 obj << /S /GoTo /D (subsubsection.6.5.4) >> endobj 304 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 305 0 obj << /S /GoTo /D (subsection.6.6) >> endobj 308 0 obj (\376\377\000p\000r\000j\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 309 0 obj << /S /GoTo /D (subsubsection.6.6.1) >> endobj 312 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 313 0 obj << /S /GoTo /D (subsubsection.6.6.2) >> endobj 316 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 317 0 obj << /S /GoTo /D (subsubsection.6.6.3) >> endobj 320 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 321 0 obj << /S /GoTo /D (subsubsection.6.6.4) >> endobj 324 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 325 0 obj << /S /GoTo /D (subsubsection.6.6.5) >> endobj 328 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 329 0 obj << /S /GoTo /D (subsection.6.7) >> endobj 332 0 obj (\376\377\000s\000p\000c\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 333 0 obj << /S /GoTo /D (subsubsection.6.7.1) >> endobj 336 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 337 0 obj << /S /GoTo /D (subsubsection.6.7.2) >> endobj 340 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 341 0 obj << /S /GoTo /D (subsubsection.6.7.3) >> endobj 344 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 345 0 obj << /S /GoTo /D (subsubsection.6.7.4) >> endobj 348 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 349 0 obj << /S /GoTo /D (subsubsection.6.7.5) >> endobj 352 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 353 0 obj << /S /GoTo /D (subsection.6.8) >> endobj 356 0 obj (\376\377\000s\000p\000h\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 357 0 obj << /S /GoTo /D (subsubsection.6.8.1) >> endobj 360 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 361 0 obj << /S /GoTo /D (subsubsection.6.8.2) >> endobj 364 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 365 0 obj << /S /GoTo /D (subsection.6.9) >> endobj 368 0 obj (\376\377\000s\000p\000x\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 369 0 obj << /S /GoTo /D (subsubsection.6.9.1) >> endobj 372 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 373 0 obj << /S /GoTo /D (subsubsection.6.9.2) >> endobj 376 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 377 0 obj << /S /GoTo /D (subsubsection.6.9.3) >> endobj 380 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 381 0 obj << /S /GoTo /D (subsubsection.6.9.4) >> endobj 384 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 385 0 obj << /S /GoTo /D (subsubsection.6.9.5) >> endobj 388 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 389 0 obj << /S /GoTo /D (subsection.6.10) >> endobj 392 0 obj (\376\377\000t\000a\000b\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 393 0 obj << /S /GoTo /D (subsubsection.6.10.1) >> endobj 396 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 397 0 obj << /S /GoTo /D (subsubsection.6.10.2) >> endobj 400 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 401 0 obj << /S /GoTo /D (subsubsection.6.10.3) >> endobj 404 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 405 0 obj << /S /GoTo /D (subsubsection.6.10.4) >> endobj 408 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 409 0 obj << /S /GoTo /D (subsubsection.6.10.5) >> endobj 412 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 413 0 obj << /S /GoTo /D (subsection.6.11) >> endobj 416 0 obj (\376\377\000w\000c\000s\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 417 0 obj << /S /GoTo /D (subsubsection.6.11.1) >> endobj 420 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 421 0 obj << /S /GoTo /D (subsubsection.6.11.2) >> endobj 424 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 425 0 obj << /S /GoTo /D (subsubsection.6.11.3) >> endobj 428 0 obj (\376\377\000E\000n\000u\000m\000e\000r\000a\000t\000i\000o\000n\000\040\000T\000y\000p\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 429 0 obj << /S /GoTo /D (subsubsection.6.11.4) >> endobj 432 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 433 0 obj << /S /GoTo /D (subsubsection.6.11.5) >> endobj 436 0 obj (\376\377\000V\000a\000r\000i\000a\000b\000l\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 437 0 obj << /S /GoTo /D (subsection.6.12) >> endobj 440 0 obj (\376\377\000w\000c\000s\000e\000r\000r\000.\000h\000\040\000F\000i\000l\000e\000\040\000R\000e\000f\000e\000r\000e\000n\000c\000e) endobj 441 0 obj << /S /GoTo /D (subsubsection.6.12.1) >> endobj 444 0 obj (\376\377\000D\000e\000t\000a\000i\000l\000e\000d\000\040\000D\000e\000s\000c\000r\000i\000p\000t\000i\000o\000n) endobj 445 0 obj << /S /GoTo /D (subsubsection.6.12.2) >> endobj 448 0 obj (\376\377\000D\000e\000f\000i\000n\000e\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 449 0 obj << /S /GoTo /D (subsubsection.6.12.3) >> endobj 452 0 obj (\376\377\000F\000u\000n\000c\000t\000i\000o\000n\000\040\000D\000o\000c\000u\000m\000e\000n\000t\000a\000t\000i\000o\000n) endobj 453 0 obj << /S /GoTo /D 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(structtabprm_e19ca756ab2190f5d5ced59ad0a1a4bc) 1753 0 R (structtabprm_f00d4a4e089737a799fb91e1a68040dc) 1740 0 R (structtabprm_fa6969fd752bb4e3823e8facf86bbd60) 1743 0 R (structwcserr) 1027 0 R] /Limits [(structtabprm_cee8b63d1691f1f531a1bb4854c6bf4c) (structwcserr)] >> endobj 7596 0 obj << /Names [(structwcserr_210814c32ace19b9d09e4774e94a3c3c) 1829 0 R (structwcserr_278b3daecfc93a28c31750e6a6dc3718) 1831 0 R (structwcserr_311c9994c1d3793b2c98d706987bcd09) 1830 0 R (structwcserr_417d725c2e5615c3fb73cc210e0ccff2) 1828 0 R (structwcserr_cf8ea013ae1dc84ed25d5ace5a0a7000) 1832 0 R (structwcsprm) 1028 0 R] /Limits [(structwcserr_210814c32ace19b9d09e4774e94a3c3c) (structwcsprm)] >> endobj 7597 0 obj << /Names [(structwcsprm_042875def8cab8354c5b2c40ab9fa374) 2027 0 R (structwcsprm_04fbd6ed1b338e225f2291523e64be2c) 1941 0 R (structwcsprm_0730c37f09502eb364f4e7d7addb8ab8) 1958 0 R (structwcsprm_08098820949433d1336841d32d0b62b5) 1975 0 R (structwcsprm_092c11d209ecdd16bb79858c68e4d582) 2031 0 R (structwcsprm_0936d10c2ac93d13d096b1711ac639a1) 1965 0 R] /Limits [(structwcsprm_042875def8cab8354c5b2c40ab9fa374) (structwcsprm_0936d10c2ac93d13d096b1711ac639a1)] >> endobj 7598 0 obj << /Names [(structwcsprm_0d15534535c7f9308c9daa2cceff29e7) 2032 0 R (structwcsprm_0e31f1eef036258c2957da9b985945dd) 1873 0 R (structwcsprm_13fab263ca03f35844fdaca289b7dfac) 2033 0 R (structwcsprm_15485177ea8bbacefc29a5a5cba98c8f) 1954 0 R (structwcsprm_164e3852bcd2dea8b5f73e1dff79ddf5) 1988 0 R (structwcsprm_2166fb650f937d8870711d8be5986b66) 1968 0 R] /Limits [(structwcsprm_0d15534535c7f9308c9daa2cceff29e7) (structwcsprm_2166fb650f937d8870711d8be5986b66)] >> endobj 7599 0 obj << /Names [(structwcsprm_292133b2b7143b969a3af6a3f2cf3709) 1971 0 R (structwcsprm_3224bd06f8f4d2d7d398533eb44a49e8) 1981 0 R (structwcsprm_3495a5b0ef529706ec9a0af5c3163d63) 1864 0 R (structwcsprm_35bff8de85e5a8892e1b68db69ca7a68) 1861 0 R (structwcsprm_42052d557bdef2c5640a6d19b6d9ed8b) 1943 0 R (structwcsprm_42e0ff2da3b0c1ca0a9509f787ed1951) 1990 0 R] /Limits [(structwcsprm_292133b2b7143b969a3af6a3f2cf3709) (structwcsprm_42e0ff2da3b0c1ca0a9509f787ed1951)] >> endobj 7600 0 obj << /Names [(structwcsprm_49eee6450b1a646d3fe01b8965a63af4) 1953 0 R (structwcsprm_4c89dafecd036e169f96cb84d53ace65) 1942 0 R (structwcsprm_4ed527b90d49e8365c1b727f7bec29c7) 2030 0 R (structwcsprm_5072893bd9beddb33967697d501acdce) 2023 0 R (structwcsprm_5444415c94c7ab0226788f5efe93221d) 2029 0 R (structwcsprm_5780880281f2f9d085d2e06919b7647a) 1986 0 R] /Limits [(structwcsprm_49eee6450b1a646d3fe01b8965a63af4) (structwcsprm_5780880281f2f9d085d2e06919b7647a)] >> endobj 7601 0 obj << /Names [(structwcsprm_5b56e1b378a6ae9f8dfff5c364f0653c) 1973 0 R (structwcsprm_5d0b60efc55a61525b9beb26ead4859e) 1872 0 R (structwcsprm_5e04127eb71da6e1350467a7a6d236f5) 1870 0 R (structwcsprm_5ed753e401cda620a04adfb4ebfb8e0d) 1987 0 R (structwcsprm_603ef3ab7f3bc42cf8d8bf99b79b63ac) 1985 0 R (structwcsprm_65801f93622504672ee3faf8f2110e48) 1961 0 R] /Limits [(structwcsprm_5b56e1b378a6ae9f8dfff5c364f0653c) (structwcsprm_65801f93622504672ee3faf8f2110e48)] >> endobj 7602 0 obj << /Names [(structwcsprm_6778d31ec5a2ee643dc5f0a8af630b03) 1989 0 R (structwcsprm_6a3fa7adc304567271c5cc0eda3ac986) 2026 0 R (structwcsprm_6a88e64207df5007151c2c25028ce3eb) 1960 0 R (structwcsprm_70cac2976524a5f0a6aeb2b3fcb95834) 1862 0 R (structwcsprm_7320fc64e7705cc7495eba07482b5c55) 1951 0 R (structwcsprm_7a0a1ce2432cef9377f70367ea1fd18c) 1866 0 R] /Limits [(structwcsprm_6778d31ec5a2ee643dc5f0a8af630b03) (structwcsprm_7a0a1ce2432cef9377f70367ea1fd18c)] >> endobj 7603 0 obj << /Names [(structwcsprm_7a88af56c4c978c6d4213ae1f4bec87a) 2028 0 R (structwcsprm_8625c0a6ff99c754566c46c2372df801) 1970 0 R (structwcsprm_8715975565c8bbd0c562a32eee40fd20) 1966 0 R (structwcsprm_88b55f6c8d122f3ff63532de85698864) 1957 0 R (structwcsprm_8b3a65921acc0dabfa4efd19a003ea6e) 1947 0 R (structwcsprm_9063e8d0c956e9eae7f7d6f3608b9ed2) 1972 0 R] /Limits [(structwcsprm_7a88af56c4c978c6d4213ae1f4bec87a) (structwcsprm_9063e8d0c956e9eae7f7d6f3608b9ed2)] >> endobj 7604 0 obj << /Names [(structwcsprm_912eed291f15134e8cfb8750acc6c4bc) 1874 0 R (structwcsprm_922f0f57b8c35cad3d01ceedeba01d4b) 1952 0 R (structwcsprm_94c26ce331cc876d63baeeada9820241) 1969 0 R (structwcsprm_9eac54f497e1244c8106dd3ebba12223) 1963 0 R (structwcsprm_9eca2fcc30058310d020181ae16bf256) 1944 0 R (structwcsprm_9ee8fb568ca75874bab00825b768f8ca) 1950 0 R] /Limits [(structwcsprm_912eed291f15134e8cfb8750acc6c4bc) (structwcsprm_9ee8fb568ca75874bab00825b768f8ca)] >> endobj 7605 0 obj << /Names [(structwcsprm_9fd60ce9e6bc31df07ed02ce64b48be4) 1967 0 R (structwcsprm_a0ae3f3605566be2e85e51e5b52c3b52) 1867 0 R (structwcsprm_ad387ccbd7847672b5dc2223d9124120) 1956 0 R (structwcsprm_adad828f07e3affd1511e533b00da19f) 1863 0 R (structwcsprm_b253d36f0dc1716952285c6078622e66) 1980 0 R (structwcsprm_b63cdcf6ff8febd1b40d0e044ca7d7ef) 1979 0 R] /Limits [(structwcsprm_9fd60ce9e6bc31df07ed02ce64b48be4) (structwcsprm_b63cdcf6ff8febd1b40d0e044ca7d7ef)] >> endobj 7606 0 obj << /Names [(structwcsprm_b7f7173e6d2b1b8028a3275bdd751e79) 1976 0 R (structwcsprm_b9729795155b8f37afd80784fb70068b) 1977 0 R (structwcsprm_c089e5d0e3191255ceaea7f8591b27ea) 1962 0 R (structwcsprm_c0cb013b1505fb7abd4167ac0db0e0aa) 1959 0 R (structwcsprm_c3c9c869bef4e4850dfd9762b33ce908) 1948 0 R (structwcsprm_c8391dd770637dbb841067996b7777ba) 1982 0 R] /Limits [(structwcsprm_b7f7173e6d2b1b8028a3275bdd751e79) (structwcsprm_c8391dd770637dbb841067996b7777ba)] >> endobj 7607 0 obj << /Names [(structwcsprm_ce7e0986c79d73bd3a0613034b71974f) 2035 0 R (structwcsprm_da1b98589c0127d34766b4c6b5d6cb41) 1871 0 R (structwcsprm_de355cdce054938cfa36e06ef9c51446) 1865 0 R (structwcsprm_de8495d3ca5047eeadba5934d0bb2708) 1978 0 R (structwcsprm_e09d5bf005e3bd7ee880353e8816ceb8) 2034 0 R (structwcsprm_e1f462606974e1324cd38f143eda691e) 1868 0 R] /Limits [(structwcsprm_ce7e0986c79d73bd3a0613034b71974f) (structwcsprm_e1f462606974e1324cd38f143eda691e)] >> endobj 7608 0 obj << /Names [(structwcsprm_e352318ce3202dab1b5db8b9ceec7703) 1974 0 R (structwcsprm_e6b40e2adeb31414871c7cae68619d63) 1955 0 R (structwcsprm_e7609283351ea46484690f873f8ea9c3) 1949 0 R (structwcsprm_e83952aec7c1ac76c090bc89bf4eeea7) 1983 0 R (structwcsprm_ee7f71c872491b25e1d1440e5dfa8153) 2025 0 R (structwcsprm_f124a4259475ea355ced38e73a05363a) 1946 0 R] /Limits [(structwcsprm_e352318ce3202dab1b5db8b9ceec7703) (structwcsprm_f124a4259475ea355ced38e73a05363a)] >> endobj 7609 0 obj << /Names [(structwcsprm_f1cb3e68560d1ac42c620cfe3900af95) 2024 0 R (structwcsprm_f300da5a94594a9769ab312bb56dde83) 1964 0 R (structwcsprm_f54ce939604be183231f0ee006e2f8ed) 1984 0 R (structwcsprm_f8f679749574250cb9ba09e1f05fab5d) 1869 0 R (structwcsprm_fd2f31d782b3becce4ca2f9b495ec0b1) 1945 0 R (structwtbarr) 1029 0 R] /Limits [(structwcsprm_f1cb3e68560d1ac42c620cfe3900af95) (structwtbarr)] >> endobj 7610 0 obj << /Names [(structwtbarr_10c8dba85b62e2794071dd50a41c4bb1) 2276 0 R (structwtbarr_1e88ad32570534a006e96cba721489b5) 2268 0 R (structwtbarr_24487eda7b17800f41bd4a452c6306d5) 2274 0 R (structwtbarr_2ff7c235353320c6dd98951484012ee7) 2278 0 R (structwtbarr_41c30234dbdf18ac094872cf39562172) 2281 0 R (structwtbarr_750832793167bbeebd1074e29844415d) 2277 0 R] /Limits [(structwtbarr_10c8dba85b62e2794071dd50a41c4bb1) (structwtbarr_750832793167bbeebd1074e29844415d)] >> endobj 7611 0 obj << /Names [(structwtbarr_8743b84c99b4b5e7ab7bf0653507a180) 2266 0 R (structwtbarr_901403d05f985d4a1fbd2fdc9585bd50) 2280 0 R (structwtbarr_9f1fcad814aa3da08dfa75ede2a07deb) 2272 0 R (structwtbarr_f862b4f90b0406ed8dd0c240768d4bd3) 2279 0 R (structwtbarr_f8ea7b15992ab7a86be63ff83318be41) 2270 0 R (subsection.1.1) 10 0 R] /Limits [(structwtbarr_8743b84c99b4b5e7ab7bf0653507a180) (subsection.1.1)] >> endobj 7612 0 obj << /Names [(subsection.1.2) 14 0 R (subsection.3.1) 26 0 R (subsection.4.1) 34 0 R (subsection.5.1) 42 0 R (subsection.5.10) 150 0 R (subsection.5.11) 162 0 R] /Limits [(subsection.1.2) (subsection.5.11)] >> endobj 7613 0 obj << /Names [(subsection.5.12) 174 0 R (subsection.5.13) 186 0 R (subsection.5.2) 54 0 R (subsection.5.3) 66 0 R (subsection.5.4) 78 0 R (subsection.5.5) 90 0 R] /Limits [(subsection.5.12) (subsection.5.5)] >> endobj 7614 0 obj << /Names [(subsection.5.6) 102 0 R (subsection.5.7) 114 0 R (subsection.5.8) 126 0 R (subsection.5.9) 138 0 R (subsection.6.1) 202 0 R (subsection.6.10) 390 0 R] /Limits [(subsection.5.6) (subsection.6.10)] >> endobj 7615 0 obj << /Names [(subsection.6.11) 414 0 R (subsection.6.12) 438 0 R (subsection.6.13) 454 0 R (subsection.6.14) 478 0 R (subsection.6.15) 502 0 R (subsection.6.16) 510 0 R] /Limits [(subsection.6.11) (subsection.6.16)] >> endobj 7616 0 obj << /Names [(subsection.6.17) 522 0 R (subsection.6.18) 538 0 R (subsection.6.19) 554 0 R (subsection.6.2) 226 0 R (subsection.6.20) 578 0 R (subsection.6.3) 250 0 R] /Limits [(subsection.6.17) (subsection.6.3)] >> endobj 7617 0 obj << /Names [(subsection.6.4) 262 0 R (subsection.6.5) 286 0 R (subsection.6.6) 306 0 R (subsection.6.7) 330 0 R (subsection.6.8) 354 0 R (subsection.6.9) 366 0 R] /Limits [(subsection.6.4) (subsection.6.9)] >> endobj 7618 0 obj << /Names [(subsubsection.5.1.1) 46 0 R (subsubsection.5.1.2) 50 0 R (subsubsection.5.10.1) 154 0 R (subsubsection.5.10.2) 158 0 R (subsubsection.5.11.1) 166 0 R (subsubsection.5.11.2) 170 0 R] /Limits [(subsubsection.5.1.1) (subsubsection.5.11.2)] >> endobj 7619 0 obj << /Names [(subsubsection.5.12.1) 178 0 R (subsubsection.5.12.2) 182 0 R (subsubsection.5.13.1) 190 0 R (subsubsection.5.13.2) 194 0 R (subsubsection.5.2.1) 58 0 R (subsubsection.5.2.2) 62 0 R] /Limits [(subsubsection.5.12.1) (subsubsection.5.2.2)] >> endobj 7620 0 obj << /Names [(subsubsection.5.3.1) 70 0 R (subsubsection.5.3.2) 74 0 R (subsubsection.5.4.1) 82 0 R (subsubsection.5.4.2) 86 0 R (subsubsection.5.5.1) 94 0 R (subsubsection.5.5.2) 98 0 R] /Limits [(subsubsection.5.3.1) (subsubsection.5.5.2)] >> endobj 7621 0 obj << /Names [(subsubsection.5.6.1) 106 0 R (subsubsection.5.6.2) 110 0 R (subsubsection.5.7.1) 118 0 R (subsubsection.5.7.2) 122 0 R (subsubsection.5.8.1) 130 0 R (subsubsection.5.8.2) 134 0 R] /Limits [(subsubsection.5.6.1) (subsubsection.5.8.2)] >> endobj 7622 0 obj << /Names [(subsubsection.5.9.1) 142 0 R (subsubsection.5.9.2) 146 0 R (subsubsection.6.1.1) 206 0 R (subsubsection.6.1.2) 210 0 R (subsubsection.6.1.3) 214 0 R (subsubsection.6.1.4) 218 0 R] /Limits [(subsubsection.5.9.1) (subsubsection.6.1.4)] >> endobj 7623 0 obj << /Names [(subsubsection.6.1.5) 222 0 R (subsubsection.6.10.1) 394 0 R (subsubsection.6.10.2) 398 0 R (subsubsection.6.10.3) 402 0 R (subsubsection.6.10.4) 406 0 R (subsubsection.6.10.5) 410 0 R] /Limits [(subsubsection.6.1.5) (subsubsection.6.10.5)] >> endobj 7624 0 obj << /Names [(subsubsection.6.11.1) 418 0 R (subsubsection.6.11.2) 422 0 R (subsubsection.6.11.3) 426 0 R (subsubsection.6.11.4) 430 0 R (subsubsection.6.11.5) 434 0 R (subsubsection.6.12.1) 442 0 R] /Limits [(subsubsection.6.11.1) (subsubsection.6.12.1)] >> endobj 7625 0 obj << /Names [(subsubsection.6.12.2) 446 0 R (subsubsection.6.12.3) 450 0 R (subsubsection.6.13.1) 458 0 R (subsubsection.6.13.2) 462 0 R (subsubsection.6.13.3) 466 0 R (subsubsection.6.13.4) 470 0 R] /Limits [(subsubsection.6.12.2) (subsubsection.6.13.4)] >> endobj 7626 0 obj << /Names [(subsubsection.6.13.5) 474 0 R (subsubsection.6.14.1) 482 0 R (subsubsection.6.14.2) 486 0 R (subsubsection.6.14.3) 490 0 R (subsubsection.6.14.4) 494 0 R (subsubsection.6.14.5) 498 0 R] /Limits [(subsubsection.6.13.5) (subsubsection.6.14.5)] >> endobj 7627 0 obj << /Names [(subsubsection.6.15.1) 506 0 R (subsubsection.6.16.1) 514 0 R (subsubsection.6.16.2) 518 0 R (subsubsection.6.17.1) 526 0 R (subsubsection.6.17.2) 530 0 R 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