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All Rights Reserved) readonly def /FullName (CMR10) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /BGAAAA+CMR10 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 50 /two put dup 51 /three put readonly def /FontBBox{-251 -250 1009 969}readonly def /UniqueID 5000793 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou\c3R*R?쨤ȯ@ gSr RIzE_EMv,X!%6]ަ_3+_hJإ0o'z 9K$|tV\)Z! j#ZŚz1UA~ "p?{u@]A}s ijB)~Ob {z;O9mT[Ğ^dUl$Wh: ?Ƃ(r6;Bt6cFCr$/;!,KqLeWuG h7IQ[u20uZ8*#qP|̖I̓pe}#YۇW{ Hs(}CE c;[e/SmV& i2ǡmc\0kC'sp)X0@$2jOGG9%fLJD@m2b5\cdy!iz+lxa+2S@uIY5F>qgROEowK*;/sDGǡx=>J ujLDfdžk4ؐ. vî|1wm% QiwXDN}}x|E.gK{ T >k&mxo.<n&lQ>I, 7 LU/GGSL@PEdԑϟ5: :""l5ȸM-/5p7Z՘B8]4t/ī+Ic/xe\% SqP=]I C!#ԽE~!|kZ `f<槷$TtPxCknKAAYsrƨF0,tu|bk"]fL`*ðydN)Ql1$?XN E>cfV=[miGU>LfqcD t.2'-;p[MR+S"#bp`1i0zCD] ~+KX>`o9N(V%U0H?Ӫ~'XPl +Mkгp(I-hq.=fKr涍.y<,=l20FndہQ6_@sPNц&-&Dr!ۀOp]!&|h]DD_GJIK'.zH*$Q]"A et`[vv3&g}`5 dz+u YcvpoDr:fWukOH<9]<Śªh : 1W5ϕ!3чc=HUP]; 9-bdq~%YO336"w@Ŝr[q3l?E h!'d'$.JL=9'}lm+Ұؙpߜ aЦ fMJvoyp&o+ FӚE}c g)C (),A$5%d*#)LYDkwv:?TJFTG4 .o(gUwr0Tc{s"\ӖJtZo?e 4 +Syd*BDG: 46,JLp^wm7Gyb]/Li)HXy7[]%̐7 Kؗ0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 38 0 obj 4070 endobj 39 0 obj 783 endobj 40 0 obj 2755 endobj 41 0 obj 532 endobj 42 0 obj /BGAAAA+CMR10 endobj 43 0 obj << /Ascent 694 /CapHeight 683 /Descent -194 /FontName 42 0 R /ItalicAngle 0 /StemV 69 /XHeight 431 /FontBBox [ -251 -250 1009 969 ] /Flags 4 /CharSet (/two/three) /FontFile 37 0 R >> endobj 21 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 44 0 R /BaseFont 50 0 R /FontDescriptor 51 0 R >> endobj 44 0 obj [ 628 857 782 714 761 850 799 600 685 631 792 659 579 531 456 416 451 513 481 364 592 600 619 507 451 588 529 588 452 556 612 641 671 639 477 610 853 529 374 671 1028 1028 1028 1028 286 286 514 514 514 514 514 514 514 514 514 514 514 514 286 286 799 514 799 514 544 771 778 734 848 756 656 805 850 449 566 870 699 993 822 782 656 811 778 628 600 699 599 971 849 597 699 400 400 400 1028 1028 424 544 440 445 533 478 499 490 592 352 420 535 307 906 620 498 516 459 464 479 371 591 499 737 583 506 478 335 392 653 514 286 ] endobj 45 0 obj << /Length 46 0 R /Length1 47 0 R /Length2 48 0 R /Length3 49 0 R >> stream %!PS-AdobeFont-1.1: CMMI9 1.100 %%CreationDate: 1996 Jul 23 07:53:55 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.100) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMMI9) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle -14.04 def /isFixedPitch false def end readonly def /FontName /NCAAAA+CMMI9 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 63 /star put readonly def /FontBBox{-29 -250 1075 750}readonly def /UniqueID 5087384 def currentdict end currentfile eexec oc;j~EЪ)s̾;.;rTejiK/df5A|{S/ )Sc\^ȟmp+#vL17~k d# ]LeVߐGoo٥\k 9Mՙ= 0)xf 1kX9JS:6_OɭRXZ5Ws E:d"BA.ޕ#z;h*ihUB9gӲ LGb ("K#`O/nms ]ԙn$z7MmGoT٢Ewpｄ BMZ "XIDUQ q~{s R~"eEύ|[9BuODcЭ/3=w߇,ĺT+(!dǗ½Pnf.zuM,.Y]D花YXO>R[*?#SVZ6qoPZM'U,5v Z5Y>u\afa63ڦN?%9+ qfj |bƕp\Kolzz`OɊK׿++B';> ґ$E b&?J'HvwM|!2h*t~ğK֊҈VX"~E1M]~swk-HћyhSߟu YBZ9캲WY ՅY3B#h7Off\*Kp#\[*]]HW HҾ`QI@6`+}}z\oѬXIV)X.]d_͓r"8?(]^iU,+aBo&2pfCPu]ǷwN);'hb V'/I;em|@ ?>aM@h72P5>ػs_r/ɚJ [֡7+= pTuhC%k\.;/0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 46 0 obj 2452 endobj 47 0 obj 770 endobj 48 0 obj 1150 endobj 49 0 obj 532 endobj 50 0 obj /NCAAAA+CMMI9 endobj 51 0 obj << /Ascent 694 /CapHeight 683 /Descent -194 /FontName 50 0 R /ItalicAngle -14 /StemV 74 /XHeight 431 /FontBBox [ -29 -250 1075 750 ] /Flags 4 /CharSet (/star) /FontFile 45 0 R >> endobj 15 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 52 0 R /BaseFont 58 0 R /FontDescriptor 59 0 R >> endobj 52 0 obj [ 826 295 826 531 826 531 826 826 826 826 826 826 826 1063 531 531 826 826 826 826 826 826 826 826 826 826 826 826 1063 1063 826 826 1063 1063 531 531 1063 1063 1063 826 1063 1063 649 649 1063 1063 1063 826 288 1063 708 708 944 944 0 0 590 590 708 531 767 767 826 826 649 849 695 563 822 561 758 631 904 585 720 807 731 1265 869 842 743 868 907 643 586 663 656 1055 756 706 764 708 708 708 708 708 649 649 472 472 472 472 531 531 413 413 295 531 531 649 531 295 885 796 885 444 708 708 826 826 472 472 472 649 826 826 826 826 ] endobj 53 0 obj << /Length 54 0 R /Length1 55 0 R /Length2 56 0 R /Length3 57 0 R >> stream %!PS-AdobeFont-1.1: CMSY8 1.0 %%CreationDate: 1991 Aug 15 07:22:10 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMSY8) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle -14.035 def /isFixedPitch false def end readonly def /FontName /NAAAAA+CMSY8 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 13 /circlecopyrt put readonly def /FontBBox{-30 -955 1185 779}readonly def /UniqueID 5000818 def currentdict end currentfile eexec oc;j~EЪ/ ȭX~id}S5Q!gtⵎkJc;rN^X5.Sy +'IqV:r㚉#,# dBZ *R*"7٨y! [R߻*|]~[C֨a[#ԙ jY!4J"3&ejc\J$2626wIaUIrnFB/Г(Hp%#O.,snݸt%\b9?_\ <+n6f Sf/@ 6M+E^o!FB&yJkpBs泧(B - v@X*]FZp!׳G L &FIR)5VÕޏ)(0q 6uhXx8RJߜӯ6*_FrF"ύ u~oU ݥ17]jmr<]::[{e ,RTިUY1p]]9( M\UYIyWuW /vl_eXë:sbm0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 54 0 obj 1975 endobj 55 0 obj 775 endobj 56 0 obj 668 endobj 57 0 obj 532 endobj 58 0 obj /NAAAAA+CMSY8 endobj 59 0 obj << /Ascent 750 /CapHeight 683 /Descent 0 /FontName 58 0 R /ItalicAngle -14 /StemV 89 /XHeight 431 /FontBBox [ -30 -955 1185 779 ] /Flags 4 /CharSet (/circlecopyrt) /FontFile 53 0 R >> endobj 14 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 60 0 R /BaseFont 66 0 R /FontDescriptor 67 0 R >> endobj 60 0 obj [ 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 531 ] endobj 61 0 obj << /Length 62 0 R /Length1 63 0 R /Length2 64 0 R /Length3 65 0 R >> stream %!PS-AdobeFont-1.1: CMTT8 1.0 %%CreationDate: 1991 Aug 20 16:46:05 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMTT8) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch true def end readonly def /FontName /XWQBQO+CMTT8 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 45 /hyphen put dup 46 /period put dup 47 /slash put dup 58 /colon put dup 60 /less put dup 62 /greater put dup 64 /at put dup 97 /a put dup 100 /d put dup 101 /e put dup 102 /f put dup 103 /g put dup 104 /h put dup 105 /i put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 118 /v put dup 119 /w put dup 121 /y put dup 126 /asciitilde put readonly def /FontBBox{-5 -232 545 699}readonly def /UniqueID 5000830 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou_1oO3095϶܄xC)nZAPEEs'}8iHkTwitߎ&}=VP!hQGAG%1/mC+*NQ,-)p1a=MY <5;QםBAx /aC?V"{x"+,wF-"lE|ش+)ip`<ۑ$1sVM);RuMܘF=I`1k9`He+q`#%`˸Z gk;H:~ųrw/pb*\v#$;@/Rf/94jŠz}LQH}gg$O Ÿ`f#[R0A5YF/0'};$MJ;m;%,(/OCNR ۏos֎3϶_H2=Aq翚PGc#`Lkj\¥![:)yQ @r3&Vu+k+cT&pIa6|y lY(GfR ݇ecÊh 29=kr`Z"N"7PՓPbQL7.{7nM)hp9jS?˞aRB.c"t44NuJYa{N'# A -5U zxY)QE'Vc_cU5nOz5KæژK+&oq1?ܯ2wc YD(BE<%>߱R:HϭckwRWBaIa50y%堲Rnuh2G&^@*8AuoA[zJg\&/7R](g>6Mݙ߇rN%Y?rjպ&1Li +MVF.S!+.;+ /cy_z(}Jsk%+?մs-#z6IΓ~-piu1|&=?- \o\M@ڥ5ڐ$Ɇ\MIs}GrId~oLO/ u'fI7zj>^ u3ksY ~V(nҬX#|j!*$_f`L(Oڠ떺5#)=EhM9})LK+f\oMgW9o?&&K">Ħ\Uprt$%{OXJѐS#!$cUUљ_ y>`~݅2IWĂ RY(lG4FJFU_ۣ諧qطSnlI,ސ ${6}%V0pNaYrHv9 hQ},Ežmg犣AKN/po ?8901Bsˆrc4Dv]K~uAϏ& `<Ctzծ&G`lC5yM07#.$8M$*hR$'ynĹ\Cv`)/zlĬ!t{M Al_iZ_Jfe4mщ7Ϊ]en!՛$E΍")%`%r@Gௐұ^ ÓcX {]7qR\%r>duu<|xىn^ wj4BZ sڃK"C+9ֳ;WXGiZk/k )Ź O{JlVXTK=Lݒ.CX̬16I7/,PwU +DimqMt),A/McJ&yV+:k@'_Z zB?6'0j BH"v   6r*NoF !s?*<]RoW^!5^5+CIvp?y \_*-(1+_ YkkJt,d9 2C}F_0#$Ykr qnnϣ ǀި$wݒƯ; C6!VFxV_^x;6|/,%W"f)+qȑ/[(6|na%Kz7&/_i)K!i6|)S:>2t-"mIꮇާfrr˔2pBwCF5#bo3՚WZ YAAi@%.D{ױ&dSVQX$|n*-\ɝ*>h !akPT7tF\+!Z}n9+D3 kbe/soEmF},(:2 DL\(GlTmz{Jn=|%;m(Im~-1.d?uX7ѮD@i_kX:`j_nxW;θd %>=ZU®!GsB=K2)uFXhc*;j5iOVkQlIy'itj]߲(PYYg~UEնŨe5~%ک˥}Vޯkv$ؘa=$jb͡{EkBg- 2V&* > nd~J{S4k<Й ޏQA'XDmowƌَԦ6RQȥ"]c_qƧz?}+L9@vp*˓ Ba%n1鰻W{Pgw~uUچpW(dϴ $ X@T]NtpJ'K6$8l5%&tCTw1l#bciQc%li5JDFRMg°< LZ3FL6֩VI$.VX7z>4±&[d+UNۯr+TtxjJn;ǼFXdC^0"S82k6//\?3zǙ)^7 1aΖOxێ9"X9ʯV߿VaU*䍷@Z3՞U#.D4\M[}Ȇf=9Sg٬WSGx1?B PG"լ!7bs2vA4' zωӭ7&n\Dgx;懌A'RƝq91 =1G;_=A#|/Q{ϷPwUN^N?ɉLxn͗%d*pN5@kD; h38Şl45:lQ{ﰤ ʖ%iZV0Pֵt6;q0JJC\"ٝqT&=c٤< }}&ݿTُ^y2FEncƎz+*.4"ɓJʗ c]6R(g}ЪKmY&r;T`qN ϥ"mAN W爓=B9!K x$5K!ۭi9#>@Q/i_%6>ZDrq&_<'jB|t)8iX]Ҥ> endobj 13 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 68 0 R /BaseFont 74 0 R /FontDescriptor 75 0 R >> endobj 68 0 obj [ 664 885 826 737 708 796 767 826 767 826 767 620 590 590 885 885 295 325 531 531 531 531 531 796 472 531 767 826 531 959 1077 826 295 295 531 885 531 885 826 295 413 413 531 826 295 354 295 531 531 531 531 531 531 531 531 531 531 531 295 295 295 826 502 502 826 796 752 767 811 723 693 834 796 383 545 825 664 973 796 826 723 826 782 590 767 796 796 1091 796 796 649 295 531 295 531 295 295 531 590 472 590 472 325 531 590 295 325 561 295 885 590 531 590 561 414 419 413 590 561 767 561 561 472 531 1063 531 531 531 ] endobj 69 0 obj << /Length 70 0 R /Length1 71 0 R /Length2 72 0 R /Length3 73 0 R >> stream %!PS-AdobeFont-1.1: CMR8 1.0 %%CreationDate: 1991 Aug 20 16:39:40 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMR8) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /GWTXIJ+CMR8 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 44 /comma put dup 45 /hyphen put dup 46 /period put dup 48 /zero put dup 49 /one put dup 50 /two put dup 54 /six put dup 55 /seven put dup 56 /eight put dup 57 /nine put dup 66 /B put dup 71 /G put dup 77 /M put dup 80 /P put dup 82 /R put dup 84 /T put dup 86 /V put dup 97 /a put dup 98 /b put dup 99 /c put dup 100 /d put dup 101 /e put dup 102 /f put dup 103 /g put dup 104 /h put dup 105 /i put dup 107 /k put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 113 /q put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 118 /v put dup 119 /w put dup 121 /y put readonly def /FontBBox{-36 -250 1070 750}readonly def /UniqueID 5000791 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou\@[6]nhmlhaH+4/?3&n=a6E#|~.ԅˡw,"rg[eHi>u Wת>~ӖѿJmdvA [4|ܾ.Vz_1. Ff |X9^Rw] ۊ31S\DKZW` P^3 eێ 8`2?l;Ȋ!eXxh Df@=$*IBXԏ!Wx-b1 C; p}hQi=HXbgbmǣR,>_Q! Z؞Ar]< Qjt8?B,mN3v լǵ+K6 t{AJcQ%r?v60RmXsŤ+pǸi:Us)kPW\~; 7T.N }.&:D~4LDV5bgANӪ&׏+“Ļɂ? \Sek鬁dVPzjmSȬߤj;-0@3q!,ay ,`y۪ik9kmosrA~}wڇ$Ĥtt&px: J,Me'EA"NL?dFG۩SC;XnTM"``B^V\)ޞ ϼ^"M \3{ƒ {+."X8&2ǾM۱!vj4XS" Z*{.Mœ$ܹDN} hpt5#od7gmz-!r^x]/%vAIZ08W3ӰwcBJ!5⬘ 6a![0g&ۢVE"yU_A4d5*#K?7n$ o I366Fyž DivIj0U=/ ٩ħϗlq8uweQ«'I{Kg^fuyI z HUI[m<<D=da .˪aŐ5zX0S(|f"d担ivuke{J4g2u?"Ri 9k<.F3O4K;x vhX6b[[d4+"J4 ]{eum"vUrj'QȵMBQ:wzG :IϚܰzqE0' F&ｾdNUS/[Eꒋ5i rq0!C 89.`'̧`֝RsTΫ~O\)f²w=DhFr="yu1;µshq#rk}28%rA e̮P7V~HX c~wʠْ닧\# EUS%GfXGf%<4D4[_Aw9#MRbWMڶ0Y? ^u:'E~,czIIhVfv}{U;Wu$5xل? u-{Jy]PA laNOPݡ魦[ 9z@z470F`91J-32V|HEm,hFb\'S!UO~LI"[`}x{߀EvUޫt:CW|Fa{ BH}X#8ħPA::9pxZ8 ; )g ,4 wg %qW3^ZQ6~O%Q6Q)ODcj)ȖSFznp(] H˷ r'jCL u5ԁCa4.c 9W 74xK^G#B[G@86ѽ v#šη }q^KLM<9!Iomluu)gqErEJ/;=&$Un;9]VFSUF|:]+ '/qR#KMPsRw=ƑCY"hl V,H3,>c]{"CU˂ZfizV')+lؘ)]h|կq a~Bd}W5;tk)5V&XK{ `[FSb[ M1/2<틮D\OI.7bC^9q=eHcH1$W}=ڙ.)ɏ(:=wʶB,Dެ [[) 墂S-`<l$:AYX?*A)*IceN4%˺RY4Lf>=*+;2L|ϢuvW+_E&Tt.(ZOOé5uM4O_b%Y`A}XXlio+WNZWK(p/&j"uA(jEU<nӛsФנh7- =riS74䈆Hz^M|d ڛXş [ 0Mj ]Lq`:ik^e73xH9@C]y~eR4 R==C ßl`Ԃ{@Rɳa8T7ؗ@ )7^D]PPQmNTbz m0- 'FJ[~^ küۘ"%`91X Px돎ų&0dW z9ܹ#@%> :zI*!ì2 C㖭c1~zIO+ Q8[[L ߴZ@$MN ׊gb An&' m5?K)rdĵanU||>,rV S_m6OSAhzj|u78`ehUKLKˤ9.//yT-Eҭ$5lPm,>P_$JUuql36Al)`%LCMB*OL$Imk܅]),0C~3:.}Ey >P^>zHip+)rGOxbʣ' !n9,^ϵ|K }؀?=)™((+c@H͊X]Wz ޹^LB#>g_|"Dia=XdR9үfmQ9<1h"j?w*05 WMs=&x/MB<Sju1g<;oRNE6Dp_JZԱXFjC`AcSW m![%κBݢLx ޿6~#V鰼ј 3'Pd  qIʩm#V'qI\[ CF:i|ZJnɲrf;F:R+Wb䋳Om c7}?y NÜ=Gd?8ک_&'kBk:+RwV븦/r?"63M)U!ր `ڢ_oÐ6)Qe$9 e|>P-hYX[.!%t I|讈"FՅH" m'l哴^]t B `Wz\&Qzb!YTGH+WgeΧI HlT|XwmVF|;0M K0}o)`dx >ʱ^fX '=#=G `JۭKks鋵O\PlBGoǬݰ[#X2ž棭"Q"@y39`Lu#jZ9w}.췔렣DY+Mѷ`ms?4H)eǣ7wobp$&Vdǐ˽mWbPjg2ܱ6?]_|mC[h둇LF[M@_^.)5'CLuA@qC\ޭHr]3vo. DgvćA\ x=m+ǦYz7yH}Ŋ.53+= Љ> endobj 12 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 76 0 R /BaseFont 82 0 R /FontDescriptor 83 0 R >> endobj 76 0 obj [ 799 286 799 514 799 514 799 799 799 799 799 799 799 1028 514 514 799 799 799 799 799 799 799 799 799 799 799 799 1028 1028 799 799 1028 1028 514 514 1028 1028 1028 799 1028 1028 628 628 1028 1028 1028 799 279 1028 685 685 914 914 0 0 571 571 685 514 742 742 799 799 628 821 674 543 794 542 736 611 871 563 697 782 708 1229 842 816 717 839 874 622 563 642 632 1018 732 685 742 685 685 685 685 685 628 628 457 457 457 457 514 514 400 400 286 514 514 628 514 286 857 771 857 428 685 685 799 799 457 457 457 628 799 799 799 799 ] endobj 77 0 obj << /Length 78 0 R /Length1 79 0 R /Length2 80 0 R /Length3 81 0 R >> stream %!PS-AdobeFont-1.1: CMSY9 1.0 %%CreationDate: 1991 Aug 15 07:22:27 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMSY9) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle -14.035 def /isFixedPitch false def end readonly def /FontName /NMAAAA+CMSY9 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 104 /angbracketleft put dup 105 /angbracketright put readonly def /FontBBox{-30 -958 1146 777}readonly def /UniqueID 5000819 def currentdict end currentfile eexec oc;j~EЪ/ ȭX~id}S5Q!gtⵎkJc;rN^X5.Sy +'IqV:r㚉#,# dBZ *R*"7٨y=cLIPsF'f> ba ]fv}3N/+ 9AK}ʶ|HLc2 `bMbX: lAEXeh"ɧgC[VlVW!EkN+Si}ɸ?sjI5lUw#ady0v#N̏F]3ۛ5B^0{xMcN0^c%QPX%aLF;'!iߎK +|W~؎"|$OsqbwDほ/#4UQT[k4ľZeO*]A)o𰮂US" :890000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 78 0 obj 2123 endobj 79 0 obj 807 endobj 80 0 obj 784 endobj 81 0 obj 532 endobj 82 0 obj /NMAAAA+CMSY9 endobj 83 0 obj << /Ascent 750 /CapHeight 683 /Descent 0 /FontName 82 0 R /ItalicAngle -14 /StemV 87 /XHeight 431 /FontBBox [ -30 -958 1146 777 ] /Flags 4 /CharSet (/angbracketleft/angbracketright) /FontFile 77 0 R >> endobj 11 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 84 0 R /BaseFont 90 0 R /FontDescriptor 91 0 R >> endobj 84 0 obj [ 711 986 920 827 789 924 855 920 855 920 855 690 657 657 986 986 329 362 592 592 592 592 592 893 526 617 855 920 592 1071 1203 920 329 360 618 986 592 986 920 329 460 460 592 920 329 394 329 592 592 592 592 592 592 592 592 592 592 592 329 329 360 920 559 559 920 893 841 855 907 777 744 930 924 446 611 926 711 1122 924 889 808 889 887 657 823 909 893 1222 893 893 723 329 618 329 592 329 329 575 657 526 657 543 362 592 657 329 362 625 329 986 657 592 657 625 488 467 460 657 625 855 625 625 526 592 1183 592 592 592 ] endobj 85 0 obj << /Length 86 0 R /Length1 87 0 R /Length2 88 0 R /Length3 89 0 R >> stream %!PS-AdobeFont-1.1: CMBX9 1.0 %%CreationDate: 1991 Aug 20 16:36:25 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMBX9) readonly def /FamilyName (Computer Modern) readonly def /Weight (Bold) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /FDWFJS+CMBX9 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 11 /ff put dup 12 /fi put dup 13 /fl put dup 45 /hyphen put dup 50 /two put dup 51 /three put dup 67 /C put dup 71 /G put dup 73 /I put dup 77 /M put dup 79 /O put dup 83 /S put dup 85 /U put dup 91 /bracketleft put dup 93 /bracketright put dup 97 /a put dup 98 /b put dup 99 /c put dup 100 /d put dup 101 /e put dup 102 /f put dup 103 /g put dup 104 /h put dup 105 /i put dup 107 /k put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 113 /q put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 118 /v put dup 119 /w put dup 120 /x put dup 121 /y put dup 122 /z put readonly def /FontBBox{-58 -250 1195 750}readonly def /UniqueID 5000767 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou_dV`Ky Z]uMYb[1[l',t\pڮԞZO4GJ7 c]>^1j̙|JtquJcw\ ᓮl+͉uҿ Tw[kj6ꑸ&Py K,Q+ wҳ%lTkİO rO]H*jQۅjy;Q沋Tf g'-\#"waf`] 7A|qmY DQn9l˃b%!-1k WV $qg^fF(S.'Nm~}2 ;Z[fIXNuV& u*06E upB3]}/5(#IN 2f9{SDW`#Cɂ8̋̔3|FYÁa7*VÐ6L|WU :clh" k-V^ M::z}uґvat47T|YXrzBu(R~Aq,ϙ'Jz,vo<bjH*6O[ǎUЊksdE|L.hbf%=MhNkdͭW []% !EZOfoNf |CM@b4LSG `%哼$S{RjNͼeI!Iᨹn~\2\"e9w,`>4D/xc[ `s'|J"%9Sؤ:ď~_9uiB/߷G~h]fpFw+Բ].NjئlHfc:CTh10=Z+Uf3uSU*xh^XN, ycʽ&=gY=I@+:ZT8L#T]_RQ%{(ëi$8U[X|AץA_e23 ,Վ;Y*ā8imS|cKExjRRDSu3^(H8"TBL< K^$^㟤MeZ}p{8f]?DuHHč `ŵKwx5(;0DxqBwҲӧjwMb!^Aq&| kkRv!:b# m+:y*n7pqU`ɕC#5tG\tܺ șcn Jv0N.[-6D wȏ(%5_q2TjPUs0֊$mD!!#U=.q>MǔACSZ;izM`w|v[ۣ#cݱM [6xK0:Prn2 r)b_:i{Mz\+/6X90rj-67`.N?L+s4J0vG` D$TQ+p*)È?;}w8,J>(٘:W= 'y'O!5I8s#$!A1.췔\@pGrE_!g(H_̡{AsO忸aUR\m*)6 KKv[[ʣpEaPw #uFuwS=rD2^HxcYao6v{+. nlO| f/!DN4t'sT#z8>Qa*5nq>q qUpju /&ԗX8?)W>.0ेIjU ͇[bù)GOibO?$6u;EFO[#!JB1ٽ O1_t46A tLvʮb+梭/b{ʩ^;'yV$ 8&x.#Et/iK3oC N4بMQP-5H,yOD+DHX ˩ eTw)]dZ^)|T!凸s=a[`}j&e=v } mqSR]O->r͉}繹,C50QvY]PtS0Z&\N*G2Hٚ/wu{ԵL~_E~ݥpa? (֘T p !T4ޅ;G6rնۊt5"tPRDw2RsioW2Mxtgʞ^u ؂bDO~\[t0R6j28ۚn" L*Ͷ$Ba72g=3D?[<SV2¥Q*1193hvA4wP,SAA/Yًr,4 +͈1<ׇV32͠AM6(_+ʩpiKFQsM^K$c_2_uԑ+QAm߹\n O h=boA]YtF_p,c~ EkY0`Qɬ~\K>]FB; \2SЌLyRYp|3 I gn 'l[IFQZvPH#֔ /&ҏ2*4679\{zU3`B!Hiz۰ 'L!hBj`O/p͚  "l|mu4F,8j1mVpnr9s{.wCAOxީ$}FG(t]5&k"36^O@1/^6FOsE=;fb6=Ucbl-U{\Wk'$ɱ6NgœuH(pF6o 0-ǥ7.g|K[ׁx* }RB+u.Bknd-0 TmGlewv1бէ;{qt@W@Qh] p~F 9`wg!¦%YPN"Uc9'"s+f;EꞢceQ9)@=VLJ*쭭M'0e@6r5u}.mh"A!:?VIU'MhjI^fncɱa (ǀ^\D>Ezt|㋣ 4hM|u.n{aa׭9<-3 V,ao3*b,khbDq'҆Px"3unƳM,pT]E[%9yw4 E&px H31ڙg@P"&R !2K-1f`KC0D.<֯o1)ҩd& /`}s}'gTv9^\;H.Wqt64T%I=5lІOs~Jc?/l%)YH>DPމ*`޳omogW.N̓dM!*cR<`|MŁZ5 57ƙ=|ǦHom8_b[JD=@3rͦo9L~,K9XJôX/D(~:p]m:n&|„Q#޶)oaB4聤lbgN 2 #V֭{G*=kYuM{Z4f3(?>c=ࡕ UqlXxV5N NC<(Tr 9i|MrSo& eܗ(5!VcK,MkIZ.W7Y[O$8 ^1VtObӯ DRckYI]߾r$R&mbxhI 8@gj0*`Hb0Y52A1z<[^4¸sYN 1]_ksJs z}\9aߩHH 7O~^TERU$XӾ+u HrnG\qdN|.vٻlu) #tQ$6?g*S>\xIA&PFw >XQP_̉9dc=:R[ Ѕ>K8ⶁ^Ip=.w=?i]eNd/ j QN¹bϸ̶jqS (Js@[c>]s =kH7B)@(gdBL;N%c,+HE~<2>;# ǜi$T^T}}IO8ÒTڤҏ(_BNf_ҰkflT6(VSߛZdD+T)T;N딭ڙ50000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 86 0 obj 9096 endobj 87 0 obj 1359 endobj 88 0 obj 7205 endobj 89 0 obj 532 endobj 90 0 obj /FDWFJS+CMBX9 endobj 91 0 obj << /Ascent 694 /CapHeight 686 /Descent -194 /FontName 90 0 R /ItalicAngle 0 /StemV 117 /XHeight 444 /FontBBox [ -58 -250 1195 750 ] /Flags 4 /CharSet (/ff/fi/fl/hyphen/two/three/C/G/I/M/O/S/U/bracketleft/bracketright/a/b/c/d/e/f/g/h/i/k/l/m/n/o/p/q/r/s/t/u/v/w/x/y/z) /FontFile 85 0 R >> endobj 10 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 92 0 R /BaseFont 98 0 R /FontDescriptor 99 0 R >> endobj 92 0 obj [ 676 938 875 787 750 880 813 875 813 875 813 656 625 625 938 938 313 344 563 563 563 563 563 850 500 574 813 875 563 1019 1144 875 313 343 581 938 563 938 875 313 438 438 563 875 313 375 313 563 563 563 563 563 563 563 563 563 563 563 313 313 343 875 531 531 875 850 800 813 862 738 707 884 880 419 581 881 676 1067 880 845 769 845 839 625 782 865 850 1162 850 850 688 313 581 313 563 313 313 547 625 500 625 513 344 563 625 313 344 594 313 938 625 563 625 594 459 444 438 625 594 813 594 594 500 563 1125 563 563 563 ] endobj 93 0 obj << /Length 94 0 R /Length1 95 0 R /Length2 96 0 R /Length3 97 0 R >> stream %!PS-AdobeFont-1.1: CMBX12 1.0 %%CreationDate: 1991 Aug 20 16:34:54 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMBX12) readonly def /FamilyName (Computer Modern) readonly def /Weight (Bold) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /BBVGHH+CMBX12 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 45 /hyphen put dup 83 /S put dup 97 /a put dup 99 /c put dup 100 /d put dup 101 /e put dup 103 /g put dup 105 /i put dup 107 /k put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 113 /q put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 121 /y put readonly def /FontBBox{-53 -251 1139 750}readonly def /UniqueID 5000769 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou_dV`Ky Z]uMYb[1[l',t\pڮԞZO4GJ7 i!U&Ϸݢh`ZṆhKGz; #1&()$J3KُօEsjFf"P$-I޵˕B 6=hqDV<` EkENrraƌJG ~L{6IE6U'y 0gK>&)o>2\U]$XW-1f@'B 1mW=L%5t.O-]N CT4>&wvNXŅCf עr1fׁVCȖ~q0 Xf^^$ӷ%G7dȱ\lFc0]g<銷_&W{>}N|ӷ 054H4ܞlG>T_cќ6Y1 nUr-u$yfOσ4nAyغINz+:΃΃Џ}=|z`v+D{.;FWLEc6o, e&ۺH%&e+ o='a9ܮ;-sg}l3K?SEhAr;}5٠땷7_KߔZn+ Kw$ZdvԬ|d- 1̝s t/ $bۂ^`DѾrO~˲`a-@k̉ဣԮPl SXx05ا)jn,{oXHir䅼$YH6Z.;p A:KfrivˣK8Uy?PeWkJ\6~C=k8yJRQYkc$q4a cC4ݧp۞cnXΩèc%r.VϚy6}5WY]zZwt-]Nx:&իiQ(7˩$둝_p%39@cw@ɪƅqCr]8îg̖D*FXAvj؄։AyWV93^Ldy/xkeQ q}9"¼ib |S(D :bGUP|ƈj)Ϗ\p? QyNoq6KyTQj*0 у_8}Q 0`6T?H̨c!ɋ♳F"ŎDihv[ƨ?j>Z(㻅!DSp(I!  k+( f @ѲKP0;[8mst LsI.}Mu<.|ePC)įi_QHJվcw񳛋U]@k AO\†KrLuwz&NA%dqAg[!1^\H5_w8CkTM-ևδM>M_ AZ6ؗӫl5]^F`${3)K5 p$~Hj}@, taed(f&Nۘ,$(nL`m\ɑ.*E}@5n,ݠ7bWwޘܯ"QpȎ&qU!8V#O w*RDzuan3ޔKL/6,6H,spx1qO{cWNU)` )|x19ɿ_%/(Z|LlRg 5ze:~z*hւoqm_~Ew%?X(!]\Kf~E:q&w>s/S$0D*K\O*bQWz]dEy u]$hXhջ\&atGrXM0b"m=yC)ȫvF@8+wCya߮ajb/N ZӏK:X؈*]E=e?L=}=K/$E8^(gg HkOXMmNJ+Rkg?Z`yL$-$ͺKJ eNKs5| R]U r ԰ͱ"rap%u%8rZp%`\z5˱N)i_7[- J&2Uh:9 :-01G}-K4khoquR33Am3aQDTyHT*;-WE̍N M0e!##LɃ~]̢9rYuJ4dYUdW:%s!&FONklJDs e,K9aD% 7ŀ%hv@]AZFͿ0aPimsL;n(?O id! v 1EYTC:/9ULpq*ez*#Ub~pFK|z90}557WnI%> T}*h`<>'ձu}RWchCǎbr}|ج9iJvHD gճ=&> %znl"ɛwˢº X\jj^V(s 6d`B>C\,(˿Tˀ 7ն >VLr&QTE:,z煮{[tuᑎbzKHF8v)%j_ 75^zyb>_ 4@SQ`X"3ij;׫5pI/d>lDg,!CIS՗xj0v'꘭/9oǭ#!?ս]B7>Y e?ˎf8.Q@mb~5F.W2ɯSB6Fz^*hmuM7:H-U*[DƯ­~#sӚ~^  姷:p12cј^lș/gkraznCp\p =>8zyKz}ɁyǐxnwD7Әۇ_5ȘXFx6QY,%Ic`3[KIٜ%\C]-8  MV m#*XޜE\ K+ܗ'ވU{E4-4!lXE!{ hq; -0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 94 0 obj 5539 endobj 95 0 obj 1046 endobj 96 0 obj 3961 endobj 97 0 obj 532 endobj 98 0 obj /BBVGHH+CMBX12 endobj 99 0 obj << /Ascent 694 /CapHeight 686 /Descent -194 /FontName 98 0 R /ItalicAngle 0 /StemV 109 /XHeight 444 /FontBBox [ -53 -251 1139 750 ] /Flags 4 /CharSet (/hyphen/S/a/c/d/e/g/i/k/l/m/n/o/p/q/r/s/t/u/y) /FontFile 93 0 R >> endobj 9 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 100 0 R /BaseFont 106 0 R /FontDescriptor 107 0 R >> endobj 100 0 obj [ 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 525 ] endobj 101 0 obj << /Length 102 0 R /Length1 103 0 R /Length2 104 0 R /Length3 105 0 R >> stream %!PS-AdobeFont-1.1: CMTT9 1.0 %%CreationDate: 1991 Aug 20 16:46:24 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMTT9) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch true def end readonly def /FontName /GLIYKM+CMTT9 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 34 /quotedbl put dup 36 /dollar put dup 39 /quoteright put dup 40 /parenleft put dup 41 /parenright put dup 42 /asterisk put dup 45 /hyphen put dup 46 /period put dup 48 /zero put dup 49 /one put dup 50 /two put dup 57 /nine put dup 67 /C put dup 73 /I put dup 77 /M put dup 83 /S put dup 91 /bracketleft put dup 92 /backslash put dup 93 /bracketright put dup 96 /quoteleft put dup 97 /a put dup 98 /b put dup 99 /c put dup 100 /d put dup 101 /e put dup 102 /f put dup 103 /g put dup 104 /h put dup 105 /i put dup 106 /j put dup 107 /k put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 113 /q put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 118 /v put dup 119 /w put dup 120 /x put dup 121 /y put dup 122 /z put readonly def /FontBBox{-6 -233 542 698}readonly def /UniqueID 5000831 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou_c2Bطj=-)1_]X` Y{nn9׫/uye );9*fHHK-\rБkg\5&(G<`J7dhn)Zl득52 Z$نa#q13@H;+G"1L(seER ;ԱJo"BFKkv/ ֈpZCޯ*@;db s*Mm~4]꽺\Qߍ):۞3#˂3u?O+|mMۉfH21C2/AHw;u&~#V=@Ņ*Ft@*(s9)UdƁF!;ŭ$r)_e_LRXJ*'*|o+ _|flWU6yM`MFPzXktw_K1Bov7}E(>[)Abц>Uu s,H6Wa7]_ΑAXφNp콕Tĩ>2oשW,1e~O 6Y̮X~Ր)Lf3CM f@^Nr2 @_cl[Л[ǩŤ4oW4]y$r"-L:&/@vq*C0bOjN]GEϻ6)V*0=A= ?xQz2B>I.xC O^|'E!Z9}^S~*ңdyqLϐiR:=\MlK%-v+_p?TVC99Bebqʯpr{\ZSAw.Zw$6LÄ|E1ƼNJGC&am OAUJ$kiD 7l q;6@ Yd ~Vi jViq#{,$oZ70Pcj? tïjě1X+NÎ|>G O*JtHglJEiu$[g/59Bao:E(}t~V5,}2zw~jZ{Pex$E;I[>c_q YCZ,R&Y +I/DKT5,IX6f?0 JMƒ)h\Zv3@xs)N0g}?d+s+|ڭ$GE 6R~q!z3.of42f~[\T_EQezDַ~0^q8  ,`enatvK:*`:O 3~Wf2cҘ$ONtIŊ.6ϩ_(* d Ϩ ImߧeZdIJ.чfϼ<,WMg˩ժ[Ck@[re2~GháY +M7>8"xmz:qgHFHo: Owh3R Xvo@ݓ}~rVgruK94&(F=`:ft佺s]j3KW@X!I{nzκFUи|`;DȷX,:étz%U HȒ@~Dq6X @R^L] '+ia*f2ɥDT~,&*Gwt<5#%B?!`mMcF%Bw0RͭsaH+O|79ܞI"vywPɑtEM3pʘ\A.EY[ 8h`N$E0x+d)W@媬~P,D0xf8DYϘWWFKSSb1ƻ;; B;67fJ-,۱Y%P c_M|$$"~DHF"VvoXE m?)X< x'YXd६"!E$˯S0U-`>z-&# *jK\RHCyj>މR3 }XZ|p ɚ]kV#~E,|[]v/j3-p 5%\~mY0BC=33_6HIih1 T­:rŽ%qH~Lb,ֹ1Ȼ ^HANtk3aWTo?/2p4bNX3JYA9)(- 8 ,{qcLr^%Y r=C![k<>ak Q׍lKX_OWĚ/8! J4Tf .6T|[Ы)lD\,W$o )*忯s5Whmڴ6ab! @wm,TƖFO E /k7Jו13D x>6!=Iz+-~KBIp})π솤C:kVm@(Y8C1uszy{u3I(ܛo=U BdQ .w%+ >5Rx}?`X-|:Gvpݠu؊$ұ]{V r'Tg"Ai)S¬@6[,W9pC5C%r?Eo>bj"2VOq$էQr8 Jee @ w2eYZ -n@G9/5*8 %_,Au |gIж4XEH@(I}GXM6S5w=즃ޥ.=t8?eYu=q8Que^e+pB4 \MAF׬ЍR2[-jT/^Nwp-= ogB/k|.϶}WۃkdS&*Kx"O3z+k_k |Yf]%Gsi6α obumoXzczl"[,@3؜Zy*{"!iN{9.$)|OaڼSRDOmx)gCIN\<<&֮}c{K6XrYnFJW4x=5p3D5Ni- nF;;HZD_d-4C>{P}T)D>Mx8Ù`7}4RO/nDsYPg=EVZ55:X3XLf>ՍZsEѪ^-6l2מԪt㖩'%:(a"Xb>#'u ހé/DJk"/.u%4i3%D*B$iMAS v(DLE9{1QM!\)aBheɊuP5Y{JܛΥ ߟ~TX0ZJwRRnĖo7˅`h]HTډRe5v!~>a*xݓ:J֔~j sdz17tr{=lz Ƌ>)POOr=ZJx_o,A̼\hɎ.6DB2ꠝ?ڸH Rxm.O߻{0ѡǒ&Q{$ Sf9 ģlß&[)ogO e|A(6;E!3c!m/oW,ޖ:W'0@ӥ'I⇋S}:UνF_2U2ڭ7xHh{J,;YQbka.5,~8 )*EѓީRЦ.;jv?@P/X 20~Uߡ]2CTh|EYIY}w?g75|]a&1kȼ]z_uE_,XYmR:U4w/{uӌ`|FDdv_yPoMT2iA_Ɛw"0(1߄O$aO ]с%w1fcv ?zyYr FTyumF#?\'gyD3ٌ1A `=\{}N١ޒ ;J53 mgܪR^CtO%CMȠ7&+KD sϱKu-8hNʞFj-Q(l>a0%9#b^n`f2m\f牚;"csb.c-D DQSH@VUxX>^_rN\HOfwD9M-%U,ږ*4&> `qw0. U⣒e0MeZ$='C"ѥ>\Dc$=0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 102 0 obj 9449 endobj 103 0 obj 1510 endobj 104 0 obj 7407 endobj 105 0 obj 532 endobj 106 0 obj /GLIYKM+CMTT9 endobj 107 0 obj << /Ascent 611 /CapHeight 611 /Descent -222 /FontName 106 0 R /ItalicAngle 0 /StemV 74 /XHeight 431 /FontBBox [ -6 -233 542 698 ] /Flags 4 /CharSet (/quotedbl/dollar/quoteright/parenleft/parenright/asterisk/hyphen/period/zero/one/two/nine/C/I/M/S/bracketleft/backslash/bracketright/quoteleft/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) /FontFile 101 0 R >> endobj 8 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 108 0 R /BaseFont 114 0 R /FontDescriptor 115 0 R >> endobj 108 0 obj [ 683 903 844 756 728 814 786 844 786 844 786 553 553 319 319 524 302 424 553 553 553 553 553 814 494 916 736 824 636 975 1092 844 319 319 553 903 553 903 844 319 436 436 553 844 319 378 319 553 553 553 553 553 553 553 553 553 553 553 319 319 844 844 844 524 844 814 771 786 829 742 713 851 814 406 567 843 683 989 814 844 742 844 800 611 786 814 814 1106 814 814 669 319 553 319 553 319 319 613 580 591 624 558 536 641 613 302 424 636 513 747 613 636 558 636 602 458 591 613 613 836 613 613 502 553 1106 553 553 553 ] endobj 109 0 obj << /Length 110 0 R /Length1 111 0 R /Length2 112 0 R /Length3 113 0 R >> stream %!PS-AdobeFont-1.1: CMCSC10 1.0 %%CreationDate: 1991 Aug 18 17:46:49 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMCSC10) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /SOVAAA+CMCSC10 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 103 /g put dup 108 /l put dup 110 /n put dup 111 /o put dup 112 /p put dup 116 /t put dup 117 /u put readonly def /FontBBox{14 -250 1077 750}readonly def /UniqueID 5000772 def currentdict end currentfile eexec oc;j~EЪ)s̾;.;rTejiK/df5A|{S/ )Sc\^ȟmp+#vL17~k d# ]LeVߐGoo٥\k 9Mՙ= 0)xf 0v7ϱ9 àE(O&k{ǛHFſꇼw R^q&AԛhF8N&{oi(^[ol W%'5,.V!0&u%ˎKxZ4pX:;[4+ @c ߌ }s$)PͶ'/CզxBCxSƫE\ 'MXpͰԁ C q6 2T1e|jԲH*} t.-"k5,h:J.X 4Z@0v)FEʫ@"jKNJrYDdcm!G~,f\HAӮhcc>SK}pkkRX>LfU8dWNb䊌b ?g~8o|R<)C쩔j#LJsh@]RWȐLbi1mDqnZu󥵮2B8U' G㊎Х32-r78!p|Jm?ʲ7V*6v/r<"G3G3h<c|cOhs(uYkb%bKdPGzPEDu\vreX4kM(ӦX@[dZ I܅;4y (^+0g昄 {@f/e' cW<(n! Ӳ`\E7t))pچL h Q+EH! ݚt\ŽAT?`S)"!oM96rj5]5.&;RTxCxo9 ACn{l^nZSMR0{ uV~yױ5^^-Zc*Uىc[5Qm. UL;!T5b%?߱b 6Lq$/ey 0fK@M_ ]L%2HXmӴe,hVMp!Ư.MyR iH8)lEQZ|%'p/NҴcTb6bW*QiMuOg=O?[UVb6Ҧm@L/ uaZ+sљ'l簦Iѯ2"6C,O U6UZ8j7qX|f[<4 -~xyM̅C7xJqO1Ls` J6y, D?bxwYj/f֥'u$R]t5?HUC4B&͟jL*Ͱe;*orO5fo'+;p< 2T{D9vOï- |3Ǟ*Dvqp)AK+ Q&& nD;zv;pXlH6? ƏÉe" B8rŝLo@&H[Э*c(J&> endobj 7 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 116 0 R /BaseFont 122 0 R /FontDescriptor 123 0 R >> endobj 116 0 obj [ 642 857 799 714 685 771 742 799 742 799 742 600 571 571 857 857 286 314 514 514 514 514 514 771 457 514 742 799 514 928 1042 799 286 286 514 857 514 857 799 286 400 400 514 799 286 343 286 514 514 514 514 514 514 514 514 514 514 514 286 286 286 799 485 485 799 771 728 742 785 699 671 807 771 371 528 799 642 942 771 799 699 799 757 571 742 771 771 1056 771 771 628 286 514 286 514 286 286 514 571 457 571 457 314 514 571 286 314 542 286 857 571 514 571 542 402 405 400 571 542 742 542 542 457 514 1028 514 514 514 ] endobj 117 0 obj << /Length 118 0 R /Length1 119 0 R /Length2 120 0 R /Length3 121 0 R >> stream %!PS-AdobeFont-1.1: CMR9 1.0 %%CreationDate: 1991 Aug 20 16:39:59 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMR9) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /XRLTXJ+CMR9 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 11 /ff put dup 12 /fi put dup 34 /quotedblright put dup 39 /quoteright put dup 40 /parenleft put dup 41 /parenright put dup 44 /comma put dup 45 /hyphen put dup 46 /period put dup 48 /zero put dup 49 /one put dup 50 /two put dup 51 /three put dup 53 /five put dup 56 /eight put dup 57 /nine put dup 65 /A put dup 66 /B put dup 67 /C put dup 68 /D put dup 69 /E put dup 70 /F put dup 71 /G put dup 72 /H put dup 73 /I put dup 75 /K put dup 76 /L put dup 77 /M put dup 78 /N put dup 79 /O put dup 80 /P put dup 81 /Q put dup 83 /S put dup 84 /T put dup 85 /U put dup 86 /V put dup 87 /W put dup 88 /X put dup 89 /Y put dup 91 /bracketleft put dup 92 /quotedblleft put dup 93 /bracketright put dup 96 /quoteleft put dup 97 /a put dup 98 /b put dup 99 /c put dup 100 /d put dup 101 /e put dup 102 /f put dup 103 /g put dup 104 /h put dup 105 /i put dup 106 /j put dup 107 /k put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 113 /q put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 118 /v put dup 119 /w put dup 120 /x put dup 121 /y put dup 122 /z put dup 123 /endash put dup 124 /emdash put readonly def /FontBBox{-39 -250 1036 750}readonly def /UniqueID 5000792 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou\c3R*R?쨤ȯ@ gSr RIzE_EMv,X!%6]ަ_3+_hJإ0oyX`U) %N5<6[mR"-%Qg !2og,Ydhhu_1A͐ .Um;3YZ`7z *%͟AJ2UhcCp2,숛§#@J s8, ed?Ms."A# p9Ɂv*\X K QF7q {N{G0o?8I*!D]!ض8iȂa>VGkV4;Wy;3Oo8KߝpY,!7T˒jHC9[I?;J_1,>W7'pRlfa{ x[:3;9ԫV4z^EЩ!6A_xcL8iNH~Ȗ&lRF-@3[8Tvޒٳ)yv<Ȍ𓁕c^e:]>l e8UHug+ndkJ Ɋ4!ӸfJRyDnrfO|gvlc5T[+Y{q1i_8׉ecEzZ;׈|]Z(0M]#-+hPFu(5!Do*bBzlEH+axqDibyK#&f%sF#zVP9s`,vqM m,v`9$d4)9gU8fɿTCIn7F=Q^u̫q~sه}4|AH-6 DދK$$N(,.+) >FJB2p =9/;XTdǫb^sGV'6ϩdَ3ՊMkJiZ*oc}qCZz:G_{8t]]"D *j B& !?`0 R-dh,}]B: apjD9z %ZG6䠎X!f8z**6b$.U Yws缳2.^&f=h}>Pt,t\I=gOl&A&c'II ~Al/~R*n4dԷqě@ EqO$QsOplD.TPl6ң D7튺;l G`nIVHS7H3U/b! br.6&Upq,@iyixOliNeD_AAu6 5oDz&縴RH P.Kt^ NTk52.'2~Fq;YdL<=z٨\Pѥh`$5譴[=z T}6Rwr{s.N0#qV/Ӓ z+sA/cCDqH˷b{?iUa0˞`M[ѳBʧ/4X\V>Jmg7ќfi^l0 zF _WE]x4X 4q!)X̘oM/ >tHyaʓ?"o0Ǫރi !^IiYW0/9iXSEQbNK>e]+6Fi̯4&{zP>V.)ōb -O _AwiJҹ]3BMtdejTc,S)k17rR`VG9EYP/×ڇRۂ=M ,4k|zzggjxąsowj`R q=xfv9- 2/$jL fQ]H,d,e(7G\  *2_+R(駝p6]qYSׯcê3Rσƫ$_gq7)FA,٠8I֥8hO^VuVQjKhGtSJ&Ѝm H7-L1lk^4d.rTKE[MS $׆YR*I*p QV6WFiwA:#e@OyVɉ%wO>$;_W54KQێv9,Es]0DȏtRtm5?YMz&R3Y oPZlZ٘7~Dʊ7jVN`G#[t{ʲICu!2m9'%~F[#`:l$rs]Dz)jogQtqCִQ-tt`GT2jˢ\&X7BX=ח-?S%(w0vPvFT" FSg詋x 9^|يQi+SM$cP@&: DҽyC+:J=e@{GZ@Ĝ͋u^o=IU376.&9뵦az"/l00$GVn:@`-1ӽIt#9&0tojW|$ۍ+F qq~YdB O=4͢`@@-Sd("(r+a2'(`^T&&[B9YlsБ'mHȜPi{mDICa'0i ֡t%@wL]iCrHJGԁU0;+`e1LJ $>_>~ΘSӚ'{ʹ:#uFIfzH*q[ 5" `$=>G0$ 붯J{EԒG(\f[wkK.=G)F=lb- $?CnRґ-gӖ<ڻ~Dߚ`ڸC>˵Į~u7^C4!ifm5*s8gTlc2و!\ {(6(bG3_O'fJP 'Ür6D$>ڵa8pTW./nDŽ$w DѼ"ְ n iTspg.l4Nx>qW s<D:\ c:MV}U >Иꀂ'S{|.Pj'a_lȫz'Sx!k$x,wF23i+Q/1wUa`$/5AO#k3p[UTQsÆ08 K~8i ־{o"F[/r<砇!nE Xϝ[c9ua1BmhP|Rdv+]Q&RTF_wZD}cт˒8->D8d'heuRX!Rj:&3a^c 5Wۻ@Oe vg7'O`'%jNE9"})rEY}}R>PN)I,hV7;]w \gЎϯ <*@YMڭ>Aa׈B71κ a`ey~JÐUw*J 4R}=*Yn"$j'WZ<&T%Mue՝%+fhVyXˉnlO@籜Q::|Ve;~%ʲJIp{EAC8iӀ s#:Y?uZfPO ]k&`j{*fPn^83^ò7R2Tꗃx3+bjϦw_2vuQv!gPHx#p/V}MIƋewuOr9zs(Kr|m|?1nUDB&M2C>pn1"BPFf͝&2>ED횅O"+EWGkbh潁,q KƑi G)%?361 SG%0j ^?zBغ~3+(*8V y{J<>+ ߳1ɨS&.I+X˜eu;-^%̣E#H7!`#+x*fNg&?{%vg?ep|S|;֟Ӭ 9qe*zM 9%fr`b\/ieiv">y5YK~_C0&f!8};"p˲`AWSDad +{晔_c_\ÄYݦ$~M:>~py'ˇ^N( &2! "O ~#N\9|X5"%mq¤wV=O:($U<{.6 E4RVO 9>Q蜫]^'<dkqpʿ??.i[XWsRK.Db^w+}xbth!5ge3%{5z dgלd£Y19u9E?ꭇA?hEf<0̌\u,Dا16Wq5ٖ}ٱDB^t5RGd_ b@B Wc6;J>XPXNoذ6g(_o-Ab>7m C+r{RmO>5:BڝYQ荓dxcVtA x1io٘}oÃwuMpddܳy=GCͭБЬ&.?l|…2 ]"Jb.;*\NVb:bo`]jGITg-6oEڭ8~񑺖|_^SPf_pcr !]wh;֏.p !8 rWR9fRu_&7Rs*Ү05oh3'N"k'pE|g)CLAϩTG`Ŵ6=hA7t6HJAca2d˭P^ާMAHΆz~򦊲^2 3_A8HQ뉟HD 7 rdk.?ax`?@FJx4bV^v>GL@.$GF 3?^v>BYÍЬt5F5:0'9R8=HV 4"hiS\C`]4FS>c Evy_˃"< +j؈b eqrw= bRB/!аwKwRDnx:ۗȹd,HkU-f Ђפ=VIAopfazSfdyXTd 7-h$F/$ 08Yc-|4<7t`0}WJaQKɧdEk~X; G #a[!{2Amm!E5 zg Kv6anˌ65)M\{Kjt(a2uMk,萫EZq' noʛ#?Y^z'x.Kq{YKUM,ÕN,lТz*r_ۚ\i! Dr&ɖS䮷?7\׍2!tpw:AQ}#xV™y 䟞~W(T{{MA*ÇDG^݉AVC>ԣv(3S2Pf,хmQ|=:}B'|9p;__95y֟Pz?8[j '܌[6 <ۏL^_) آTA ;{ }e+ 6e .d C~~1nCa,2^wDZz:ogN1/[$<0̞J?}pCu:."ݽyfĿhwQiV]C+Oa)S*hk/2Pa%EW^ pۦ "&<{C;]iͳA!ǰnrt$DFtR"4w.qtX¥GIpZ!̵Fq7 {rh,*#UpttI"P!1"Uu'H*:|<:tYD Q뙂Z4e#g)b6.\8%Wl`ݰZq GfKFVm[m_-ɹPOQ2Ug@Cimo"WRx5[ڍ5;dj-K1 ,@5"4-P!vWqRYAp_cpE|:(x-\/=J0, ~v8p~]ԝkwp6l5|<#w{e2^c J2Z$̝OH5C0@ ǎc URyK eޚe/,en Gu76fj ky| gQ^H,Wh[;y-`X"C?oID}xA;`h|xOp@d-0kq+l MDP+,DsyC.$lxܰ75k?i(2\`B<蟼OG m-%N:F/!حʿ{@̓ گE~r$nSvp1^TIɖ\y_,BaÓMbeVv«7,z@Ԝwʍ݉m72,sj4+=L J-(6ZcjgLg|jJ =E!rgwy:)Mq8[7mͧQp.#c/mG e 54i#M0;*a$Ի)'s Ou`1\u V /[zw_d5VEyC^CW1 PMFeJ2foUr @YC{?4u#&7h%BHtdU5Eo%m@*c|^ g'/Bj㥸()(iB0۰7Ig*m}];u7ua((^{v1^N&_0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 118 0 obj 14522 endobj 119 0 obj 1885 endobj 120 0 obj 12105 endobj 121 0 obj 532 endobj 122 0 obj /XRLTXJ+CMR9 endobj 123 0 obj << /Ascent 694 /CapHeight 683 /Descent -194 /FontName 122 0 R /ItalicAngle 0 /StemV 74 /XHeight 431 /FontBBox [ -39 -250 1036 750 ] /Flags 4 /CharSet (/ff/fi/quotedblright/quoteright/parenleft/parenright/comma/hyphen/period/zero/one/two/three/five/eight/nine/A/B/C/D/E/F/G/H/I/K/L/M/N/O/P/Q/S/T/U/V/W/X/Y/bracketleft/quotedblleft/bracketright/quoteleft/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/endash/emdash) /FontFile 117 0 R >> endobj 6 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 127 /Widths 124 0 R /BaseFont 130 0 R /FontDescriptor 131 0 R >> endobj 124 0 obj [ 612 816 762 680 653 734 707 762 707 762 707 571 544 544 816 816 272 299 490 490 490 490 490 734 435 490 707 762 490 884 993 762 272 272 490 816 490 816 762 272 381 381 490 762 272 326 272 490 490 490 490 490 490 490 490 490 490 490 272 272 272 762 462 462 762 734 693 707 748 666 639 768 734 353 503 761 612 897 734 762 666 762 721 544 707 734 734 1006 734 734 598 272 490 272 490 272 272 490 544 435 544 435 299 490 544 272 299 517 272 816 544 490 544 517 381 386 381 544 517 707 517 517 435 490 979 490 490 490 ] endobj 125 0 obj << /Length 126 0 R /Length1 127 0 R /Length2 128 0 R /Length3 129 0 R >> stream %!PS-AdobeFont-1.1: CMR12 1.0 %%CreationDate: 1991 Aug 20 16:38:05 % Copyright (C) 1997 American Mathematical Society. All Rights Reserved. 11 dict begin /FontInfo 7 dict dup begin /version (1.0) readonly def /Notice (Copyright (C) 1997 American Mathematical Society. All Rights Reserved) readonly def /FullName (CMR12) readonly def /FamilyName (Computer Modern) readonly def /Weight (Medium) readonly def /ItalicAngle 0 def /isFixedPitch false def end readonly def /FontName /QXKDXW+CMR12 def /PaintType 0 def /FontType 1 def /FontMatrix [0.001 0 0 0.001 0 0] readonly def /Encoding 256 array 0 1 255 {1 index exch /.notdef put} for dup 12 /fi put dup 45 /hyphen put dup 65 /A put dup 70 /F put dup 72 /H put dup 73 /I put dup 81 /Q put dup 82 /R put dup 83 /S put dup 84 /T put dup 85 /U put dup 97 /a put dup 98 /b put dup 99 /c put dup 100 /d put dup 101 /e put dup 102 /f put dup 103 /g put dup 105 /i put dup 107 /k put dup 108 /l put dup 109 /m put dup 110 /n put dup 111 /o put dup 112 /p put dup 114 /r put dup 115 /s put dup 116 /t put dup 117 /u put dup 118 /v put readonly def /FontBBox{-34 -251 988 750}readonly def /UniqueID 5000794 def currentdict end currentfile eexec oc;j~EЪ*BgNӽ ؑlKq*޲Xws|QFqv`zXMyp"5O˩YŝP(DT![v67XFlU&3!Rq4wσ~j+ou\@[6]nhmlhaH+4/?3&n=a6E#|~.ԅˠLw2.槝sNY ڻ.,VnNX3|裠k(QIOs m;fߖC1}_a Io#0wݙ\P,f *bG3Z2کP8L3r[vnc_Eh~g9|M) }YaѕH|1m![AzXpPNCU7Uֲ7ΖTgx_hyW^]W}s_Zfs@dYr ȟsy&vJx)ݱ~Kq 45hL#q:4pP?g |GJSn^i26M Ęz0. v31껰xCj 7}0a `~iEfÎB wS:;9l[ vqo (>DlqY?kڑo^8KLG7qZC`D"VEy":`A.P w6b0؁1OFLےӰl}`˼L=="9LUBLyxnZHR?['Xzw:O6ᇆv+UqQnl7 h L0觐v8 _?\CBOd9oaEu¸ B:gj=Z"EqPIB5*eI k@2D۰ $O'c7%=|2y!;pDQѝ-;o)ԝJ"GQtbaK"8o{zN0@A} Hx2`gׂbH@x&'W.'4Oj~<ڏh$韄H$8b RT ȣXVAT`pspc5LSIA9Ah2.P/<(ǎ{8\e;\I3kjO;4.Kk@V1FA\㿂 EHm2WhJMFizsfKK~ r(?!=arl[џQ:q>b!n49\58[^gj Jl#+`f7 }|n !o:' WGA68u%=sR+Rh.-1\j7/޺bϷoi Kq Z?݆ϋB9(n+PtSp: Ex ls^fZ#꒱H `QmizBpUKr/_p9CZ6 0|.=l#{O,FzcTX{U.F-;)V)j!>& jk5 gT{(h :(gֱ`\v=J# 3:b yvPbTpwI4D50BMj)(a"v ͨ=~B/ҍx*xģt*k.O-cDPeneFb,]5A ^0()4>yxc6(YGu (W3p d^Uco0ٷx.?R ?áD /o#kjp4 AsF#\Ny*&RH[; VUo Y'1j#^HZsȔKlNdJصywDZg{iL-z_;NMv-P${ʄ^W8YcUŊ~M2ln=yIG=ۭ`b૗}b=6;bR;hLu*!x)'<O8 kTN0"%;q(aJH#^%,k黌&0LL <# R_L@÷Nkخ"OU1ԈL ҍU/LџNJļxFǼ?+Jn >~7Jg 6BՑdcY\.ȯcuվV 𵳢IG2fHp⇪ovч1B1c`߰F|Si>|έһjKhoHP1 ~(UEe ڢbĠ04i[P8D{k-(4E=7g!̴8sn2HB%g:ikBWtB  CPA"{L[.F뉠Ox|OqPcްS/CKש(ͻK**˫ ؠ5ᐄ5h+RLvZWDZV\-䰘7|ڌKD+hiLc p @06RwaL|'w`朷lkE$A&k - 1!5$ƀ-N[;{JntԤ5 x? sbO5Fg"D3tXIkB%eDJ]{) Mx\)Aš/28FLI&`cBGHĨo-A)3oY"C0 W/Ğyc23Rj(/7*]A uN*-n.&Ơ"|8LSD!K5rdE %ܮd"/2Ci*FoScpϛmT/c~9p.nu]\)M ѲHY<~ԜL!Dž|`@9ޚJ0$Eۺ~39>l-D4`)Pۺ }_zs|b:݋'4^m"9g+aU!CEɐZlZuPZ2dBA8ڳ l xl"tXf-#._] 9?b'6N3:#OWI8UKњ#Jޡ]mb#q\ܵr&)^͒;6bGK:C]+YZTHWr]LrTΤHE28fsgGn16rEmI)CL CVt9IW^58SϷ.zX|DHG< Nmaxԭ$)| 'bNOrR{KTs=V^!4p~&i Q`-ib9sͶR5N7{8Ɠ6CCl>$a't ;yK%Xj~k c袹ΕSj'Vds95#⠖"E`#4D}>ŏ!P#\Ԁ$7c;7 FnXT^Ӗ?eG;0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 0000000000000000000000000000000000000000000000000000000000000000 cleartomark endstream endobj 126 0 obj 7628 endobj 127 0 obj 1185 endobj 128 0 obj 5911 endobj 129 0 obj 532 endobj 130 0 obj /QXKDXW+CMR12 endobj 131 0 obj << /Ascent 694 /CapHeight 683 /Descent -194 /FontName 130 0 R /ItalicAngle 0 /StemV 65 /XHeight 431 /FontBBox [ -34 -251 988 750 ] /Flags 4 /CharSet (/fi/hyphen/A/F/H/I/Q/R/S/T/U/a/b/c/d/e/f/g/i/k/l/m/n/o/p/r/s/t/u/v) /FontFile 125 0 R >> endobj 5 0 obj << /Type /Font /Subtype /Type1 /FirstChar 0 /LastChar 126 /Widths 132 0 R /BaseFont 138 0 R /FontDescriptor 139 0 R >> endobj 132 0 obj [ 400 400 400 400 800 800 800 800 1200 1200 1200 1200 1600 1600 1600 1600 2000 2000 2000 2000 2400 2400 2400 2400 2800 2800 2800 2800 3200 3200 3200 3200 3600 3600 3600 3600 4000 4000 4000 4000 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 100 200 300 400 500 600 700 800 900 1000 1100 1200 1300 1400 1500 0 100 200 300 400 500 600 700 800 900 1000 1100 1200 1300 1400 1500 ] endobj 133 0 obj << /Length 134 0 R /Length1 135 0 R /Length2 136 0 R /Length3 137 0 R >> stream %!PS-AdobeFont-1.1: LCIRCLEW10 1.00 %%CreationDate: 1992 Oct 23 20:22:00 % Copyright (C) 1997 American Mathematical Society. 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without even the implied warranty of %% properly describing the software it documents. %% Permission is granted to make and distribute copies of this %% document in electronic form provided the copyright notice and this %% permission are preserved on all copies. \documentclass[twocolumn]{article} \usepackage{fancybox} \setlength{\parindent}{0truecm} \setlength{\parskip}{1ex} \setlength{\hoffset}{-0.5truecm} \setlength{\voffset}{0truecm} \setlength{\topmargin}{-2.5truecm} \setlength{\marginparsep}{0truecm} \setlength{\marginparwidth}{0truecm} \setlength{\textheight}{25.5truecm} \setlength{\textwidth}{17truecm} \setlength{\oddsidemargin}{0truecm} \setlength{\evensidemargin}{1.2truecm} \setlength{\columnsep}{1.4truecm} \newenvironment{Boxedminipage}% {\begin{Sbox}\begin{minipage}}% {\end{minipage}\end{Sbox}\Ovalbox{\TheSbox}} \newenvironment{SqBoxedminipage}% {\begin{Sbox}\begin{minipage}}% {\end{minipage}\end{Sbox}\fbox{\TheSbox}} \def\version{{0.6.0}} \def\revised{{17 May, 2002}} \def\file#1{{\texttt{`#1'}}} \def\key#1{{\textrm \leavevmode\hbox{% \raise0.4pt\hbox{$\langle$}\kern-.08em\vtop{% \vbox{\hrule\kern-0.4pt \hbox{\raise0.4pt\hbox{\vphantom{$\langle$}}#1}}% \kern-0.4pt\hrule}% \kern-.06em\raise0.4pt\hbox{$\rangle$}}}} \def\variable#1#2#3{{ \vspace{-0.2truecm} \begin{flushright} \begin{minipage}[h]{0.97\linewidth} \vspace{-0.2truecm} \textbf{#1}\hfill[\texttt{#2}] \begin{flushright} \begin{minipage}[h]{0.93\linewidth} \vspace{-0.2truecm} #3 \end{minipage} \end{flushright} \end{minipage} \end{flushright} }} \def\command#1#2{{ \vspace{-0.2truecm} \begin{flushright} \begin{minipage}[h]{0.97\linewidth} \vspace{-0.2truecm} \textbf{#1}\hfill \begin{flushright} \begin{minipage}[h]{0.93\linewidth} \vspace{-0.4truecm} #2 \end{minipage} \end{flushright} \end{minipage} \end{flushright} }} \def\Star{{$\star$}} \begin{document} \small \thispagestyle{empty} \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} \vspace{0.01\textheight} {\Large Quick Reference for}\\ \vspace{0.007\textheight} {\Large gnuplot-mode} \vspace{0.01\textheight} \end{center} \end{Boxedminipage} \end{center} \vspace{3ex} This card describes the features of gnuplot-mode for Emacs. Gnuplot-mode is intended for composing scripts for the \textsc{gnuplot} plotting program. It offers functions for sending commands or entire scripts to the \textsc{gnuplot} program as well as various functions to aid in composing scripts. It works with any version of \textsc{gnuplot} from 3.5 to 3.8. See the comments in the file \file{gnuplot.el} for instructions on installing gnuplot-mode. \vspace{2ex} \begin{minipage}[h]{\linewidth} \begin{center} \centerline{{\large\textbf{gnuplot-mode key sequences}}} \vspace{0.2ex} \begin{tabular}[h]{cl} \hline \hline \\[-1ex] \multicolumn{2}{l}{~\quad\textbf{Gnuplot-mode buffer}}\\[0.5ex] \textrm{key} & \quad description \\ \hline \texttt{C-c C-l} & send a line to gnuplot \\ \texttt{C-c C-v} & send a line and move forward 1 line\\ \texttt{C-c C-r} & send the region to gnuplot \\ \texttt{C-c C-b} & send the buffer to gnuplot \\ \texttt{C-c C-f} & send a file to gnuplot \\ & \\[-1.5ex] \texttt{M-\key{tab}} & complete keyword at point \\ \texttt{C-c C-i} & insert filename at point \\ \texttt{C-c C-j} & jump to next statement \\ \texttt{C-c C-n} & negate set option at point \\ \texttt{C-c C-c} & comment region \\ \texttt{C-c C-o} & set arguments of command at point \\ \texttt{S-mouse-2} & set arguments of command under mouse \\ \texttt{C-c C-h} & get help from the gnuplot info file \\ \texttt{C-c C-e} & look at the gnuplot process buffer \\ & \\[-1.5ex] \texttt{C-c C-k} & kill the gnuplot process \\ \texttt{C-c C-u} & submit a bug report about gnuplot-mode \\ \texttt{C-c C-z} & customize gnuplot-mode \\ \hline \\[-1ex] \multicolumn{2}{l}{~\quad\textbf{Gnuplot process buffer}}\\[0.5ex] \textrm{key} & \quad description \\ \hline \texttt{M-C-p} & plot script \\ \texttt{M-C-f} & load file containing script \\ \hline \hline \end{tabular} \end{center} \end{minipage} \vspace{4ex} \centerline{{\large\textbf{Starting gnuplot-mode}}} \vspace{2ex} \command{M-x gnuplot-mode}{Start gnuplot-mode in the current buffer.} % \command{M-x gnuplot-make-buffer}{Open a new buffer in gnuplot-mode} \vfill \begin{Boxedminipage}{1.05\linewidth} \begin{center} \footnotesize{Gnuplot-mode homepage} \\ \scriptsize{%% \texttt{http://feff.phys.washington.edu/\char126ravel/software/gnuplot-mode/}} \end{center} \end{Boxedminipage} \begin{flushleft} {\footnotesize This page {\copyright} 1998-2002 Bruce Ravel \hfill revised \revised \\ \texttt{} \\ %% \hfill printed \today \\ This page covers version {\version} of gnuplot-mode. Permission is granted to make and distribute copies of this quick reference provided the copyright notice and this permission are preserved on all copies.} \end{flushleft} %%\vfil \pagebreak \centerline{{\large\textbf{Setting up gnuplot-mode}}} \vspace{2ex} Put the lines in the box below in your \file{.emacs} file or in the system wide start-up file to enable gnuplot-mode. The first two lines make Emacs recognize the functions described in the ``Starting gnuplot-mode'' section on this page. The third line causes Emacs to put all files ending in \file{.gp} into gnuplot-mode. The final line defines a hotkey -- in this case \key{F9} -- for starting gnuplot-mode. \begin{SqBoxedminipage}{\linewidth} \begin{Verbatim} (autoload 'gnuplot-mode "gnuplot" "gnuplot major mode" t) (autoload 'gnuplot-make-buffer "gnuplot" "open a buffer in gnuplot mode" t) (setq auto-mode-alist (append '(("\\.gp$" . gnuplot-mode)) auto-mode-alist)) (global-set-key [(f9)] 'gnuplot-make-buffer) \end{Verbatim}%%$ \end{SqBoxedminipage} \vspace{4ex} \begin{description} \item[Using the gnuplot-process buffer] \hfill \\ The process buffer contains an active \textsc{gnuplot} command line for interacting with \textsc{gnuplot} directly. The \texttt{M-C-p} and \texttt{M-C-f} key sequences will plot using the contents of the gnuplot script buffer. \item[Using the GUI to set command arguments] \hfill \\ \texttt{C-c C-c} and \texttt{S-mouse-2} are used to invoke the graphical tool for setting command arguments. Use text fields and option menus to choose appropriate values. Menus and buttons are activated with the middle mouse button. A few plot options may not be fully supported. \item[Customizing variables] \hfill \\ The graphical customization tool for variables can be invoked using \texttt{C-c C-z}. Descriptions of the variables relevant to gnuplot-mode can be obtained by using \texttt{gnuplot} as the regular expression for \texttt{M-x apropos}. \item[On-line help] \hfill \\ Keyword completion and on-line help require that the \textsc{gnuplot} info file be available and that the info-look package be installed. The info file can be made from the documentation supplied with the \textsc{gnuplot} distribution and the info-look package is a standard part of Emacs 20. Users of XEmacs or Emacs 19 should download \file{info-look.el} from the gnuplot-mode homepage. \item[Using pm3d] \hfill \\ All features of the pm3d patch to \textsc{gnuplot} should be available when using gnuplot-mode. One particularly useful feature of pm3d is the ability to push a cursor position into the clipboard. This is done by double-clicking \texttt{mouse-1} in the plot window, then doing \texttt{M-x yank-clipboard-selection} (usually bound to \texttt{mouse-2}) in the gnuplot script buffer. \end{description} \vfill \pagebreak %%% end of first column \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} {\large User configurable variables} \end{center} \end{Boxedminipage} \end{center} \variable{gnuplot-program}{gnuplot}{The name of the gnuplot executable.} % \variable{gnuplot-process-name}{*gnuplot*}{The name of the gnuplot process and process buffer.} % \variable{gnuplot-gnuplot-buffer}{plot.gp}{The name of the gnuplot scratch buffer opened by \texttt{gnuplot-make-buffer}.} % % \variable{gnuplot-display-process}{'window}{Determines how to display the gnuplot process buffer, either 'frame, 'window, or nil} % \variable{gnuplot-info-display}{'window}{Determines how `gnuplot-get-help' displays the info file, either 'frame, 'window, or nil} % \variable{gnuplot-echo-command-line-flag}{t}{If lines that you send to gnuplot from the gnuplot-mode buffer are not appearing at the gnuplot prompt in the process buffer, set this to nil and restart emacs.} % \variable{gnuplot-delay}{0.01}{Time in seconds to allow the gnuplot display to update. Increase this number if the prompts and lines are displayed out of order.} % \variable{gnuplot-quote-character}{'}{Quotation character used when inserting a filename into the script (single, double, or no quote).} \variable{gnuplot-buffer-max-size}{1000}{The maximum size in lines of the gnuplot buffer. Excess lines are trimmed. 0 means to never trim.} %%\vspace{1ex} \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} {\large Hook variables} \end{center} \end{Boxedminipage} \end{center} \variable{gnuplot-mode-hook}{nil}{Functions run when gnuplot minor mode is entered.} % \variable{gnuplot-load-hook}{nil}{Functions run when gnuplot.el is first loaded.} % \variable{gnuplot-after-plot-hook}{nil}{Functions run after gnuplot plots an entire buffer. See the doc string for \texttt{gnuplot-recently-sent}.} % \variable{gnuplot-comint-setup-hook}{nil}{Functions run after setting up the gnuplot process buffer in comint mode.} % \variable{gnuplot-info-hook}{nil}{Functions run before setting up info-look in the gnuplot-mode buffer.} % \vfill\eject \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} {\large Insertion variables} \end{center} \end{Boxedminipage} \end{center} \noindent These variables control the \texttt{Insertions} pull-down menu, which can be used to insert \textsc{gnuplot} commands into the script. The various sub-menu variables can be used to customize which commands appear in the \texttt{Insertions} menu. \vspace{2ex} % \variable{gnuplot-insertions-menu-flag}{t}{Non-nil means to display the \texttt{Insertions} menu in the menubar.} % \variable{gnuplot-insertions-show-help-flag}{nil}{Non-nil means to display help from info file when using the \texttt{Insertions} menu.} % \variable{gnuplot-insertions-adornments}{\Star}{Contents of the \texttt{adornments} sub-menu.} % \variable{gnuplot-insertions-plot-options}{\Star}{Contents of the \texttt{plot-options} sub-menu.} % \variable{gnuplot-insertions-terminal}{\Star}{Contents of the \texttt{terminal} sub-menu.} % \variable{gnuplot-insertions-x-axis}{\Star}{Contents of the \texttt{x axis} sub-menu.} % \variable{gnuplot-insertions-x2-axis}{\Star}{Contents of the \texttt{x2 axis} sub-menu.} % \variable{gnuplot-insertions-y-axis}{\Star}{Contents of the \texttt{y axis} sub-menu.} % \variable{gnuplot-insertions-y2-axis}{\Star}{Contents of the \texttt{y2 axis} sub-menu.} % \variable{gnuplot-insertions-z-axis}{\Star}{Contents of the \texttt{z axis} sub-menu.} % \variable{gnuplot-insertions-parametric-plots}{\Star}{Contents of the \texttt{parametric plots} sub-menu.} % \variable{gnuplot-insertions-polar-plots}{\Star}{Contents of the \texttt{polar plots} sub-menu.} % \variable{gnuplot-insertions-surface-plots}{\Star}{Contents of the \texttt{surface plots} sub-menu.} \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} {\large Toolbar variables} \end{center} \end{Boxedminipage} \end{center} \noindent These variables control the use and location of the toolbar in XEmacs. The toolbar has buttons equivalent to the key sequences \texttt{C-c C-l}, \texttt{C-c C-r}, \texttt{C-c C-b}, \texttt{C-c C-e}, and \texttt{C-c C-h}. \vspace{2ex} % \variable{gnuplot-display-toolbar-flag}{nil}{Non-nil means to display a toolbar if using XEmacs.} % \variable{gnuplot-use-toolbar}{left-toolbar}{Location of XEmacs toolbar. Valid values are \texttt{left-toolbar}, \texttt{right-toolbar}, \texttt{top-toolbar}, \texttt{bottom-toolbar}, \texttt{default-toolbar} and nil.} % \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} {\large Set Arguments} \end{center} \end{Boxedminipage} \end{center} \noindent These variables control the behavior of the graphical interface to setting command arguments. \texttt{C-c C-c} with point over a command or \texttt{S-mouse-2} with the mouse cursor over a command will cause a small frame to pop open with which you can set command arguments. Green button with bold text are bound to pup-up menus --- use the mouse-2 to select an item from the menu. Grey fields are for filling in strings or numbers. Hit the \textbf{[Set Options]} button with \texttt{mouse-2} to insert command arguments into the script. You can also use the \key{tab} key to move among the widgets and \key{ret} to push the buttons. \vspace{2ex} % \variable{gnuplot-gui-popup-flag}{nil}{When non-nil an argument setting frame will pop open whenever the \texttt{Insertions} menu is used.} % \variable{gnuplot-gui-plot-splot-fit-style}{'simple}{\texttt{'simple} or \texttt{'complete} -- describes the extent of the list of properties of for plot, splot, and fit in the GUI.} % \variable{gnuplot-gui-frame-plist}{\Star}{Property list of parameters controlling the argument setting frame. Used by XEmacs.} % \variable{gnuplot-gui-frame-parameters}{\Star}{List of parameters controlling the argument setting frame. Used by Emacs.} % \variable{gnuplot-gui-fontname-list}{\Star}{List of font available on your computer to the terminal drivers.} % \begin{center} \begin{Boxedminipage}{0.75\linewidth} \begin{center} {\large Faces} \end{center} \end{Boxedminipage} \end{center} \noindent These are various faces defined for use with gnuplot-mode. \vspace{2ex} % \variable{gnuplot-prompt-face}{firebrick}{Color of gnuplot prompt (on a light background) in process buffer. Bold and underlined on a monochrome display.} % \variable{gnuplot-gui-menu-face}{dark olive green}{Color of menu buttons (on a light background) in the argument setting frame. Italic on a monochrome display.} % \variable{gnuplot-gui-button-face}{sienna}{Color of push buttons (on a light background) in the argument setting frame. Italic on a monochrome display.} % \variable{gnuplot-gui-label-face}{dark slate blue}{Color of buttons (on a light background) used to set label lists in the argument setting frame. Italic on a monochrome display.} % \vfill \hrule \vspace{0.5ex} \begin{flushleft} \footnotesize{Variables marked with {\Star} have default values that are too long to print here.} \end{flushleft} \end{document} %%% Local Variables: %%% mode: latex %%% TeX-master: t %%% End: gnuplot-mode-0.6.0.orig/Win9x/0040755000175000017500000000000007305170747015746 5ustar arafunearafunegnuplot-mode-0.6.0.orig/Win9x/INSTALL.Win9x0100644000175000017500000001210106717311323017775 0ustar arafunearafune Time-stamp: <1999-05-15 11:29:23 bruce> This file describes how to install gnuplot-mode on a Windows 95 or 98 system so that you may use Gnuplot from within Emacs. Gnuplot-mode was written by Bruce Ravel . Contact him with any questions or comments regarding gnuplot-mode. For questions or comments regarding Emacs or Gnuplot, contact the authors of those programs. ------O------ Gnuplot-mode and Gnuplot can be used with Emacs on a Windows 95 or 98 system, although a small amount of additional effort will be required to get everything working. The best solution is to install a sufficiently recent version of Gnuplot which includes the ability to run as a child process (as of May 15 1999 there is no such version). A more complete description of this is attached to the end of this document. Recent versions of Gnuplot can be found at ftp://ftp.gnuplot.vt.edu/pub/gnuplot/ If you install a very recent version of gnuplot which includes the ability to run as a child process, then the installation instructions for gnuplot-mode are much simpler. After following the normal installation instructions, just add the following line to your Emacs initialization file: (add-hook 'gnuplot-load-hook '(lambda () (setq gnuplot-program "c:/path/to/pgnuplot/pgnuplot.exe"))) Replace "c:/path/to/pgnuplot/pgnuplot.exe" with the full path to pgnuplot on your computer. You can make gnuplot work even with an older version of Gnuplot for Windows by following these steps: 1. Edit the file pgnuplot.c so that the variable FULLPATH at line 5 is pointing at the actual location of the Gnuplot executable on your computer. 2. Using any C compiler, compile pgnuplot.c to pgnuplot.exe 3. Byte-compile gnuplot.el and gnuplot-gui.el as described in the INSTALL file in the main gnuplot-mode directory. Make sure the .elc files a placed in a location where Emacs knows to look, i.e. in its load-path. You can add new directories to the load-path by placing the following line near the top of your Emacs initialization file (.emacs or _emacs): (setq load-path (append (list "c:/path/to/lisp/files") load-path)) 4. Add these lines to your Emacs initialization file (.emacs or _emacs): (autoload 'gnuplot-mode "gnuplot" "gnuplot major mode" t) (autoload 'gnuplot-make-buffer "gnuplot" "open a buffer in gnuplot-mode" t) (setq auto-mode-alist (append '(("\\.gp$" . gnuplot-mode)) auto-mode-alist)) (global-set-key [(f9)] 'gnuplot-make-buffer) (add-hook 'gnuplot-load-hook '(lambda () (setq gnuplot-program "c:/path/to/pgnuplot/pgnuplot.exe"))) The last line is very important. It tells Emacs to launch pgnuplot.exe as its subprocess rather than Gnuplot itself. The first four lines are explained in the comments near the beginning of gnuplot.el. Replace "c:/path/to/pgnuplot/pgnuplot.exe" with the full path to pgnuplot on your computer. ------O------ Resources: Emacs for Windows NT/9x: http://www.cs.washington.edu/homes/voelker/ntemacs.html The Gnuplot distribution site (includes Windows executables): ftp://ftp.gnuplot.vt.edu/pub/gnuplot/ The gnuplot-mode homepage: http://feff.phys.washington.edu/~ravel/gnuplot/ Cygwin, Unix tools for Windows NT/9x: http://sourceware.cygnus.com/cygwin/ ------O------ What follows are the comments of the author of pgnuplot.c, Hans-Bernhard Broeker, describing the function and need for this program. Thu, 11 Feb 1999 Here's the tiny program I came up with to fix the single most annoying problem specific to the Windows version of gnuplot: lack of support for piping commands into it via STDIN. For those who don't know the context: Windows GUI programs like wgnuplot do not have any access to the usual I/O channels stdin and stdout. So the usual method to allow gnuplot to run as a child application, being controlled via a command stream by another one (i.e. the classical 'popen("gnuplot", "w");' method), can not work on Windoze. It's implemented as a separate Win32 console application (that's a different kind of program, which cannot display GUI windows, but does have STDIN/STDOUT channels). This program will get hold of a running wgnuplot (or start one itself, passing on any command line arguments), and deliver each character it sees on its own standard input stream as a keypress message to the command window of wgnuplot. Effectively, this makes 'pgnuplot.exe' an almost 100% complete replacement of wgnuplot.exe, as far as starting the program is concerned, but adding the stdin capabilities. A different way of seeing it is as a prototype of a general application that wants to run wgnuplot as a child process. gnuplot-mode-0.6.0.orig/Win9x/pgnuplot.c0100644000175000017500000000562706716035256017771 0ustar arafunearafune#include /* You MUST change the value of FULLPATH to the actual location of the * gnuplot executable on your computer. */ #define FULLPATH "e:/prg/gp36/gp37hbb/wgnuplot.exe" #define WINDOWNAME "gnuplot" #define PARENTCLASS "wgnuplot_parent" #define TEXTCLASS "wgnuplot_text" #define GRAPHWINDOW "gnuplot graph" #define GRAPHCLASS "wgnuplot_graph" int main (int argc, char *argv[]) { /* Customize this path if needed */ char *d, buf[80]; HWND hwnd_parent; HWND hwnd_text; BOOL startedWgnuplotMyself = FALSE; /* First, try to find if there is an instance of gnuplot * running, already. If so, use that. */ hwnd_parent = FindWindow(PARENTCLASS, WINDOWNAME); if ( ! hwnd_parent) { /* None there, so start one: load gnuplot (minimized in order to * show only the graphic window). Pass all command line arguments * on to wgnuplot, by concatting the wgnuplot full path name and * the given arguments, building up a new, usable command line: */ char *cmdline = strdup (FULLPATH); while (*(++argv)) { /* Puzzle together a working from the given arguments. To account * for possible spaces in arguments, we'll have to put double quotes * around each of them: */ /* FIXME: doesn't check for out of memory */ cmdline = realloc(cmdline, strlen(cmdline)+3+strlen(argv[0])); strcat(cmdline, " \""); strcat(cmdline, *argv); strcat(cmdline, "\""); } if (WinExec(cmdline, SW_SHOWMINNOACTIVE) < 32) { printf("Can't load gnuplot\n"); exit(EXIT_FAILURE); } startedWgnuplotMyself = TRUE; /* wait for the gnuplot window */ /* FIXME: is this necessary? As documented, WinExec shouldn't return * until wgnuplot first calls GetMessage(). By then, the window should * be there, shouldn't it? */ Sleep(1000); hwnd_parent = FindWindow(PARENTCLASS, WINDOWNAME); } if ( ! hwnd_parent) { /* Still no gnuplot window? Problem! */ printf("Can't find the gnuplot window"); exit(EXIT_FAILURE); } /* find the child text window */ hwnd_text = FindWindowEx(hwnd_parent, NULL, "wgnuplot_text", NULL ); if (isatty(fileno(stdin))) { /* Do not try to read from stdin if it hasn't been redirected * (i.e., it should read from a pipe or a file) */ exit(EXIT_SUCCESS); } /* wait for commands on stdin, and pass them on to the wgnuplot text * window */ do { d = fgets(buf, sizeof(buf), stdin); if (NULL == d) { if (startedWgnuplotMyself) { /* close gnuplot cleanly: */ strcpy (buf, "exit"); d = buf; startedWgnuplotMyself = FALSE; } else { break; } } while(*d) { PostMessage(hwnd_text, WM_CHAR, *d, 1L); d++; } } while (NULL != d); /* Just in case stdin didn't have a terminating newline, add one: */ PostMessage(hwnd_text, WM_CHAR, '\n', 1L); return EXIT_SUCCESS; } gnuplot-mode-0.6.0.orig/aclocal.m40100644000175000017500000000310506675575365016602 0ustar arafunearafunednl aclocal.m4 generated automatically by aclocal 1.4 dnl Copyright (C) 1994, 1995-8, 1999 Free Software Foundation, Inc. dnl This file is free software; the Free Software Foundation dnl gives unlimited permission to copy and/or distribute it, dnl with or without modifications, as long as this notice is preserved. dnl This program is distributed in the hope that it will be useful, dnl but WITHOUT ANY WARRANTY, to the extent permitted by law; without dnl even the implied warranty of MERCHANTABILITY or FITNESS FOR A dnl PARTICULAR PURPOSE. # serial 1 AC_DEFUN(AM_PATH_LISPDIR, [# If set to t, that means we are running in a shell under Emacs. # If you have an Emacs named "t", then use the full path. test "$EMACS" = t && EMACS= AC_PATH_PROGS(EMACS, emacs xemacs, no) if test $EMACS != "no"; then AC_MSG_CHECKING([where .elc files should go]) dnl Set default value lispdir="\$(datadir)/emacs/site-lisp" emacs_flavor=`echo "$EMACS" | sed -e 's,^.*/,,'` if test "x$prefix" = "xNONE"; then if test -d $ac_default_prefix/share/$emacs_flavor/site-lisp; then lispdir="\$(prefix)/share/$emacs_flavor/site-lisp" else if test -d $ac_default_prefix/lib/$emacs_flavor/site-lisp; then lispdir="\$(prefix)/lib/$emacs_flavor/site-lisp" fi fi else if test -d $prefix/share/$emacs_flavor/site-lisp; then lispdir="\$(prefix)/share/$emacs_flavor/site-lisp" else if test -d $prefix/lib/$emacs_flavor/site-lisp; then lispdir="\$(prefix)/lib/$emacs_flavor/site-lisp" fi fi fi AC_MSG_RESULT($lispdir) fi AC_SUBST(lispdir)]) gnuplot-mode-0.6.0.orig/dotemacs0100644000175000017500000000153406643011716016444 0ustar arafunearafune;;-------------------------------------------------------------------- ;; Lines enabling gnuplot-mode ;; move the files gnuplot.el to someplace in your lisp load-path or ;; use a line like ;; (setq load-path (append (list "/path/to/gnuplot") load-path)) ;; these lines enable the use of gnuplot mode (autoload 'gnuplot-mode "gnuplot" "gnuplot major mode" t) (autoload 'gnuplot-make-buffer "gnuplot" "open a buffer in gnuplot mode" t) ;; this line automatically causes all files with the .gp extension to ;; be loaded into gnuplot mode (setq auto-mode-alist (append '(("\\.gp$" . gnuplot-mode)) auto-mode-alist)) ;; This line binds the function-9 key so that it opens a buffer into ;; gnuplot mode (global-set-key [(f9)] 'gnuplot-make-buffer) ;; end of line for gnuplot-mode ;;-------------------------------------------------------------------- gnuplot-mode-0.6.0.orig/README0100644000175000017500000001255206717313002015577 0ustar arafunearafune This directory contains files for running Gnuplot from within emacs. This package was assembled by Bruce Ravel . See http://feff.phys.washington.edu/~ravel/gnuplot/ for the latest. Contents ======== README this file INSTALL thorough installation instructions ChangeLog a log of changes by version number gnuplot.el gnuplot mode for emacs gnuplot-gui.el a GUI for setting command arguments interactively info-look.20.2.el programmer's interface to info files, old version info-look.20.3.el programmer's interface to info files, new version dot.el a short lisp file used by the Makefile gnuplot.info info version of gnuplot 3.6 help gpelcard.tex quick reference card for gnuplot mode (latex) gpelcard.ps dotemacs example .emacs lines for enabling gnuplot mode Makefile.in \ Makefile.dst \ aclocal.m4 \ files inherited from the gnuplot distribution configure } for making gnuplot-mode configure.in / install-sh / mkinstalldirs / Win9x/INSTALL.Win9x Extra installation instructions for Windows 95/98 Win9x/pgnuplot.c Program required to run gnuplot from Emacs Soon gnuplot-mode will be included with the gnuplot 3.7 distribution. The installation instructions for the free-standing distribution have been modified to be consistent with that. Installation ============ 1. Unpack the gnuplot.tar.gz and cd to the gnuplot directory. 2. Type "configure". If configure doesn't work for you, see note 7 below. 3. Run "make". If you use XEmacs, run "make EMACS=xemacs" (or change the EMACS variable to "xemacs" in the Makefile, the run "make"). 4. Move the lisp files to the system site_lisp directory if you are installing as root. If you are installing as a normal user move the .elc files to a place where emacs, i.e. your personal emacs directory. 5. Insert the contents of the `dotemacs' file into your .emacs file or into the system's emacs start-up file to enable gnuplot mode. 6. The function `gnuplot-info-lookup-symbol' looks at the Gnuplot info file that comes with this package or that can be made from the Gnuplot distribution. For that function to work, the file gnuplot.info must be placed somewhere where info can find it, for example /usr/info. A line like this in your .emacs allows you to put gnuplot.info any place convenient: (add-to-list 'Info-default-directory-list "/path/to/file") Wouldn't it be //great// if Emacs had some kind of systematized package installing facility? I think so, too! Oh well.... NOTES ===== 1. gnuplot-mode is designed for use with version 3.7 of gnuplot. It should work very well with any of the 3.6 beta versions. Only some of the specialized features will not work with version 3.5 -- the GUI interface to setting command arguments is an example. 2. To use gnuplot-mode with Emacs on Windows 95 or 98 see the instructions in the directory Win9x. 3. The installation materials used by gnuplot-mode come from the gnuplot distribution. 4. If "configure" doesn't work for you, the file "Makefile.dst" can be used. In that case do, "make -f Makefile.dst" and carry on from there. 5. If you do not have the custom library installed, you will get several harmless warnings when compiling gnuplot.el. Most of gnuplot-mode will work even without the custom library installed. 6. The file info-look.el provides the on-line help functionality. Without it, things like on-line help and keyword completion will not work. Using a tool that is a standard part of Emacs is a good idea, but this one gets complicated. This file became part of Emacs with version 20. It changed between 20.2 and 20.3. And it does not come with XEmacs. What's more, the version from 20.2 has a bug and the newer version does not work with Emacs 19. So, this distribution comes with two versions of info-look.el, the version from Emacs 20.2 patched to work correctly and the version from Emacs 20.3. Here's what happens when you run make: a. If you use Emacs 19 or XEmacs 19, then the Makefile will compile the 20.2 version. b. If you use Emacs 20.2 or lower, the Makefile will compile the 20.2 version. c. If you use XEmacs 20 or higher, the Makefile will compile the 20.3 version. d. If you use Emacs 20.3 or higher, the Makefile won't compile any version. 7. The gnuplot-mode distribution comes with the version of the gnuplot info file that gets made by gnuplot 3.7. Use it rather than the old one. If you really must use the older info file, see the document string for the variable `gnuplot-info-hook'. If you already have the info file installed on your computer, you will not need the one that comes with gnuplot-mode. 8. The interactive graphical graphical interface to setting command arguments contained in gnuplot-gui.el is experimental. It is incomplete and may make mistakes. Hopefully, you will find it useful. It *requires* that you are using a version of emacs with the widget library installed or that you have installed it yourself. Version numbers in the 20's of Emacs and XEmacs ship with the widget library. For version numbers in the 19's, it can be obtained at http://www.dina.kvl.dk/~abraham/custom/ gnuplot-mode-0.6.0.orig/configure0100755000175000017500000010235006675576774016660 0ustar arafunearafune#! /bin/sh # Guess values for system-dependent variables and create Makefiles. # Generated automatically using autoconf version 2.13 # Copyright (C) 1992, 93, 94, 95, 96 Free Software Foundation, Inc. # # This configure script is free software; the Free Software Foundation # gives unlimited permission to copy, distribute and modify it. # Defaults: ac_help= ac_default_prefix=/usr/local # Any additions from configure.in: # Initialize some variables set by options. # The variables have the same names as the options, with # dashes changed to underlines. build=NONE cache_file=./config.cache exec_prefix=NONE host=NONE no_create= nonopt=NONE no_recursion= prefix=NONE program_prefix=NONE program_suffix=NONE program_transform_name=s,x,x, silent= site= srcdir= target=NONE verbose= x_includes=NONE x_libraries=NONE bindir='${exec_prefix}/bin' sbindir='${exec_prefix}/sbin' libexecdir='${exec_prefix}/libexec' datadir='${prefix}/share' sysconfdir='${prefix}/etc' sharedstatedir='${prefix}/com' localstatedir='${prefix}/var' libdir='${exec_prefix}/lib' includedir='${prefix}/include' oldincludedir='/usr/include' infodir='${prefix}/info' mandir='${prefix}/man' # Initialize some other variables. subdirs= MFLAGS= MAKEFLAGS= SHELL=${CONFIG_SHELL-/bin/sh} # Maximum number of lines to put in a shell here document. ac_max_here_lines=12 ac_prev= for ac_option do # If the previous option needs an argument, assign it. if test -n "$ac_prev"; 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Fl(y2)40 b(axis)26 b Fn(sub-men)n(u.)2110 3533 y Fj(gn)n(uplot-insertions-z-axis)770 b Fn([)p Fc(?)p Fn(])2236 3674 y(Con)n(ten)n(ts)25 b(of)i(the)e Fl(z)39 b(axis)27 b Fn(sub-men)n(u.)2110 3857 y Fj(gn)n (uplot-insertions-parametric-pl)q(ot)q(s)351 b Fn([)p Fc(?)p Fn(])2236 3990 y(Con)n(ten)n(ts)25 b(of)i(the)e Fl(parametric)41 b(plots)27 b Fn(sub-men)n(u.)2110 4181 y Fj(gn)n(uplot-insertions-p)r(olar-)q(plo)q(ts)572 b Fn([)p Fc(?)p Fn(])2236 4314 y(Con)n(ten)n(ts)25 b(of)i(the)e Fl(polar)40 b(plots)27 b Fn(sub-men)n(u.)2110 4505 y Fj(gn)n(uplot-insertions-surface-plots)502 b Fn([)p Fc(?)p Fn(])2236 4638 y(Con)n(ten)n(ts)25 b(of)i(the)e Fl(surface)41 b(plots)27 b Fn(sub-men)n(u.)2254 4794 y Fp(\007)p 2254 4883 7 60 v 2254 4920 a(\006)3692 4794 y(\004)p 3692 4883 V 3692 4920 a(\005)p 2290 4920 1372 7 v 2290 4794 V 2609 4888 a Fd(T)-8 b(o)s(olbar)31 b(v)-5 b(ariables)2055 5096 y Fn(These)22 b(v)l(ariables)g(con)n(trol)g(the)f(use)h(and)f(lo)r (cation)i(of)f(the)f(to)r(ol-)2055 5187 y(bar)27 b(in)f(XEmacs.)36 b(The)27 b(to)r(olbar)g(has)g(buttons)f(equiv)l(alen)n(t)f(to)2055 5278 y(the)18 b(k)n(ey)g(sequences)h Fl(C-c)40 b(C-l)p Fn(,)21 b Fl(C-c)40 b(C-r)p Fn(,)21 b Fl(C-c)40 b(C-b)p Fn(,)21 b Fl(C-c)40 b(C-e)p Fn(,)2055 5370 y(and)25 b Fl(C-c)40 b(C-h)p Fn(.)2110 5520 y Fj(gn)n(uplot-displa)n(y-to)r (olbar-\015ag)568 b Fn([)p Fl(nil)p Fn(])2236 5616 y(Non-nil)56 b(means)h(to)g(displa)n(y)g(a)h(to)r(olbar)g(if)g(using)2236 5707 y(XEmacs.)1869 5989 y Fb(2)p eop %%Page: 3 3 3 2 bop -63 -275 a Fj(gn)n(uplot-use-to)r(olbar)524 b Fn([)p Fl(left-toolbar)p Fn(])62 -177 y(Lo)r(cation)63 b(of)g(XEmacs)e(to)r(olbar.)145 b(V)-6 b(alid)61 b(v)l(alues)62 -85 y(are)28 b Fl(left-toolbar)p Fn(,)j Fl(right-toolbar)p Fn(,)h Fl(top-toolbar)p Fn(,)62 6 y Fl(bottom-toolbar)p Fn(,)d Fl(default-toolbar)g Fn(and)d(nil.)81 132 y Fp(\007)p 81 240 7 78 v 81 276 a(\006)1519 132 y(\004)p 1519 240 V 1519 276 a(\005)p 117 276 1372 7 v 117 132 V 486 225 a Fd(Set)33 b(Argumen)m(ts)-118 433 y 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1346 a Fn(tab)p 43 1361 V 149 1343 a Fi(i)210 1346 y Fn(k)n(ey)g(to)i(mo)n(v)n(e)f(among)g(the) g(widgets)i(and)1483 1343 y Fi(h)p 1506 1290 95 4 v 1506 1346 a Fn(ret)p 1506 1361 V 1596 1343 a Fi(i)1656 1346 y Fn(to)-118 1437 y(push)25 b(the)g(buttons.)-63 1583 y Fj(gn)n(uplot-gui-p)r(opup-\015ag)754 b Fn([)p Fl(nil)p Fn(])62 1681 y(When)24 b(non-nil)f(an)h(argumen)n(t)f(setting)i(frame)f (will)i(p)r(op)62 1772 y(op)r(en)g(whenev)n(er)f(the)g Fl(Insertions)j Fn(men)n(u)c(is)j(used.)-63 1914 y Fj(gn)n (uplot-gui-plot-splot-)q(\014t-)q(st)n(yle)316 b Fn([)p Fl('simple)p Fn(])62 2012 y Fl('simple)37 b Fn(or)f Fl('complete)i Fn({)e(describ)r(es)g(the)f(exten)n(t)g(of)62 2103 y(the)30 b(list)h(of)g(prop)r(erties)g(of)g(for)g(plot,)h(splot,)g(and)e(\014t)f (in)62 2194 y(the)d(GUI.)-63 2322 y Fj(gn)n(uplot-gui-frame-plist)824 b Fn([)p Fc(?)p Fn(])62 2420 y(Prop)r(ert)n(y)32 b(list)g(of)h (parameters)e(con)n(trolling)i(the)e(argu-)62 2511 y(men)n(t)24 b(setting)j(frame.)34 b(Used)25 b(b)n(y)g(XEmacs.)-63 2653 y Fj(gn)n(uplot-gui-frame-parameters)558 b Fn([)p Fc(?)p Fn(])62 2751 y(List)34 b(of)g(parameters)e(con)n(trolling)j(the) d(argumen)n(t)g(set-)62 2842 y(ting)26 b(frame.)35 b(Used)25 b(b)n(y)g(Emacs.)-63 2984 y Fj(gn)n(uplot-gui-fon)n(tname-list)735 b Fn([)p Fc(?)p Fn(])62 3080 y(List)24 b(of)g(fon)n(t)f(a)n(v)l (ailable)h(on)f(y)n(our)g(computer)f(to)h(the)g(ter-)62 3171 y(minal)j(driv)n(ers.)81 3282 y Fp(\007)p 81 3370 7 59 v 81 3407 a(\006)1519 3282 y(\004)p 1519 3370 V 1519 3407 a(\005)p 117 3407 1372 7 v 117 3282 V 688 3375 a Fd(F)-8 b(aces)-118 3564 y Fn(These)35 b(are)h(v)l(arious)f(faces)h (de\014ned)e(for)i(use)f(with)g(gn)n(uplot-)-118 3655 y(mo)r(de.)-63 3786 y Fj(gn)n(uplot-prompt-face)607 b Fn([)p Fl(firebrick)p Fn(])62 3888 y(Color)30 b(of)f(gn)n(uplot)f (prompt)e(\(on)i(a)h(ligh)n(t)f(bac)n(kground\))62 3979 y(in)48 b(pro)r(cess)h(bu\013er.)100 b(Bold)48 b(and)f(underlined)g(on) h(a)62 4071 y(mono)r(c)n(hrome)25 b(displa)n(y)-6 b(.)-63 4212 y Fj(gn)n(uplot-gui-men)n(u-face)261 b Fn([)p Fl(dark)41 b(olive)f(green)p Fn(])62 4314 y(Color)f(of)f(men)n(u)d(buttons)i(\(on) g(a)h(ligh)n(t)f(bac)n(kground\))62 4406 y(in)54 b(the)g(argumen)n(t)f (setting)i(frame.)119 b(Italic)55 b(on)f(a)62 4497 y(mono)r(c)n(hrome) 25 b(displa)n(y)-6 b(.)-63 4639 y Fj(gn)n(uplot-gui-button-face)605 b Fn([)p Fl(sienna)p Fn(])62 4741 y(Color)42 b(of)g(push)d(buttons)h (\(on)g(a)h(ligh)n(t)g(bac)n(kground\))62 4832 y(in)54 b(the)g(argumen)n(t)f(setting)i(frame.)119 b(Italic)55 b(on)f(a)62 4924 y(mono)r(c)n(hrome)25 b(displa)n(y)-6 b(.)-63 5065 y Fj(gn)n(uplot-gui-lab)r(el-face)328 b Fn([)p Fl(dark)41 b(slate)f(blue)p Fn(])62 5168 y(Color)30 b(of)f(buttons)e(\(on)h(a)g(ligh)n(t)g(bac)n(kground\))f(used)h(to)62 5259 y(set)21 b(lab)r(el)g(lists)h(in)e(the)g(argumen)n(t)g(setting)h (frame.)33 b(Italic)62 5350 y(on)26 b(a)g(mono)r(c)n(hrome)e(displa)n (y)-6 b(.)p -118 5429 1843 4 v -118 5588 a Fh(V)g(ariables)23 b(mark)n(ed)g(with)h Fa(?)g Fh(ha)n(v)n(e)g(default)g(v)l(alues)h(that) g(are)e(to)r(o)-118 5667 y(long)h(to)g(prin)n(t)g(here.)1869 5989 y Fb(3)p eop %%Trailer end userdict /end-hook known{end-hook}if %%EOF gnuplot-mode-0.6.0.orig/mkinstalldirs0100755000175000017500000000132206675575677017555 0ustar arafunearafune#! /bin/sh # mkinstalldirs --- make directory hierarchy # Author: Noah Friedman # Created: 1993-05-16 # Public domain # $Id: mkinstalldirs,v 1.13 1999/01/05 03:18:55 bje Exp $ errstatus=0 for file do set fnord `echo ":$file" | sed -ne 's/^:\//#/;s/^://;s/\// /g;s/^#/\//;p'` shift pathcomp= for d do pathcomp="$pathcomp$d" case "$pathcomp" in -* ) pathcomp=./$pathcomp ;; esac if test ! -d "$pathcomp"; then echo "mkdir $pathcomp" mkdir "$pathcomp" || lasterr=$? if test ! -d "$pathcomp"; then errstatus=$lasterr fi fi pathcomp="$pathcomp/" done done exit $errstatus # mkinstalldirs ends here gnuplot-mode-0.6.0.orig/dot.el0100644000175000017500000000042706635100074016027 0ustar arafunearafune;; These are some lines to help compilation of gnuplot-mode proceed ;; with fewer warning messages (setq load-path (append (list ".") load-path) byte-compile-verbose nil byte-compile-warnings nil) (require 'font-lock) (defun hilit-repaint-command (foo)) gnuplot-mode-0.6.0.orig/gnuplot.info0100644000175000017500000115253006654227003017273 0ustar arafunearafuneThis file is gnuplot.info created by doc2info from ./gnuplot.doc.  File: gnuplot.info, Node: Top, Prev: (dir), Next: gnuplot, Up: (dir) gnuplot ******* * Menu: * gnuplot:: * Commands:: * Graphical User Interfaces:: * Bugs::  File: gnuplot.info, Node: gnuplot, Prev: Top, Up: Top, Next: Copyright * Menu: * Copyright:: * Introduction:: * Seeking-assistance:: * What's New in version 3.7:: * Batch/Interactive Operation:: * Command-line-editing:: * Comments:: * Coordinates:: * Environment:: * Expressions:: * Glossary:: * Plotting:: * Start-up:: * Substitution:: * Syntax:: * Time/Date data::  File: gnuplot.info, Node: Copyright, Prev: gnuplot, Up: gnuplot, Next: Introduction Copyright (C) 1986 - 1993, 1998 Thomas Williams, Colin Kelley Permission to use, copy, and distribute this software and its documentation for any purpose with or without fee is hereby granted, provided that the above copyright notice appear in all copies and that both that copyright notice and this permission notice appear in supporting documentation. Permission to modify the software is granted, but not the right to distribute the complete modified source code. Modifications are to be distributed as patches to the released version. Permission to distribute binaries produced by compiling modified sources is granted, provided you 1. distribute the corresponding source modifications from the released version in the form of a patch file along with the binaries, 2. add special version identification to distinguish your version in addition to the base release version number, 3. provide your name and address as the primary contact for the support of your modified version, and 4. retain our contact information in regard to use of the base software. Permission to distribute the released version of the source code along with corresponding source modifications in the form of a patch file is granted with same provisions 2 through 4 for binary distributions. This software is provided "as is" without express or implied warranty to the extent permitted by applicable law. AUTHORS Original Software: Thomas Williams, Colin Kelley. Gnuplot 2.0 additions: Russell Lang, Dave Kotz, John Campbell. Gnuplot 3.0 additions: Gershon Elber and many others.  File: gnuplot.info, Node: Introduction, Prev: Copyright, Up: gnuplot, Next: Seeking-assistance `gnuplot` (*note gnuplot:: ) is a command-driven interactive function and data plotting program. It is case sensitive (commands and function names written in lowercase are not the same as those written in CAPS). All command names may be abbreviated as long as the abbreviation is not ambiguous. Any number of commands may appear on a line (with the exception that `load` (*note load:: ) or `call` (*note call:: ) must be the final command), separated by semicolons (;). Strings are indicated with quotes. They may be either single or double quotation marks, e.g., load "filename" cd 'dir' although there are some subtle differences (see `syntax` (*note Syntax:: ) for more details). Any command-line arguments are assumed to be names of files containing `gnuplot` commands, with the exception of standard X11 arguments, which are processed first. Each file is loaded with the `load` command, in the order specified. `gnuplot` exits after the last file is processed. When no load files are named, `gnuplot` enters into an interactive mode. The special filename "-" is used to denote standard input. See "help batch/interactive" for more details. Many `gnuplot` commands have multiple options. These options must appear in the proper order, although unwanted ones may be omitted in most cases. Thus if the entire command is "command a b c", then "command a c" will probably work, but "command c a" will fail. Commands may extend over several input lines by ending each line but the last with a backslash (\). The backslash must be the _last_ character on each line. The effect is as if the backslash and newline were not there. That is, no white space is implied, nor is a comment terminated. Therefore, commenting out a continued line comments out the entire command (see `comment`). But note that if an error occurs somewhere on a multi-line command, the parser may not be able to locate precisely where the error is and in that case will not necessarily point to the correct line. In this document, curly braces ({}) denote optional arguments and a vertical bar (|) separates mutually exclusive choices. `gnuplot` keywords or `help` (*note help:: ) topics are indicated by backquotes or `boldface` (where available). Angle brackets (<>) are used to mark replaceable tokens. In many cases, a default value of the token will be taken for optional arguments if the token is omitted, but these cases are not always denoted with braces around the angle brackets. For on-line help on any topic, type `help` followed by the name of the topic or just `help` or `?` to get a menu of available topics. The new `gnuplot` user should begin by reading about `plotting` (*note Plotting:: ) (if on-line, type `help plotting`).  File: gnuplot.info, Node: Seeking-assistance, Prev: Introduction, Up: gnuplot, Next: What's New in version 3.7 There is a mailing list for `gnuplot` (*note gnuplot:: ) users. Note, however, that the newsgroup comp.graphics.apps.gnuplot is identical to the mailing list (they both carry the same set of messages). We prefer that you read the messages through the newsgroup rather than subscribing to the mailing list. Administrative requests should be sent to majordomo@dartmouth.edu Send a message with the body (not the subject) consisting of the single word "help" (without the quotes) for more details. The address for mailing to list members is: info-gnuplot@dartmouth.edu Bug reports and code contributions should be mailed to: bug-gnuplot@dartmouth.edu The list of those interested in beta-test versions is: info-gnuplot-beta@dartmouth.edu There is also a World Wide Web page with up-to-date information, including known bugs: http://www.cs.dartmouth.edu/gnuplot_info.html Before seeking help, please check the FAQ (Frequently Asked Questions) list. If you do not have a copy of the FAQ, you may request a copy by email from the Majordomo address above, ftp a copy from ftp://ftp.dartmouth.edu/pub/gnuplot or see the WWW `gnuplot` page. When posting a question, please include full details of the version of `gnuplot`, the machine, and operating system you are using. A _small_ script demonstrating the problem may be useful. Function plots are preferable to datafile plots. If email-ing to info-gnuplot, please state whether or not you are subscribed to the list, so that users who use news will know to email a reply to you. There is a form for such postings on the WWW site.  File: gnuplot.info, Node: What's New in version 3.7, Prev: Seeking-assistance, Up: gnuplot, Next: Batch/Interactive Operation Gnuplot version 3.7 contains many new features. This section gives a partial list and links to the new items in no particular order. 1. `fit f(x) 'file' via` uses the Marquardt-Levenberg method to fit data. (This is only slightly different from the `gnufit` patch available for 3.5.) 2. Greatly expanded `using` (*note using:: ) command. See plot using. 3. `set timefmt` (*note timefmt:: ) allows for the use of dates as input and output for time series plots. See `Time/Date data` and timedat.dem. 4. Multiline labels and font selection in some drivers. 5. Minor (unlabeled) tics. See `set mxtics` (*note mxtics:: ). 6. `key` (*note key:: ) options for moving the key box in the page (and even outside of the plot), putting a title on it and a box around it, and more. See `set key`. 7. Multiplots on a single logical page with `set multiplot` (*note multiplot:: ). 8. Enhanced `postscript` (*note postscript:: ) driver with super/subscripts and font changes. (This was a separate driver (`enhpost`) that was available as a patch for 3.5.) 9. Second axes: use the top and right axes independently of the bottom and left, both for plotting and labels. See `plot` (*note plot:: ). 10. Special datafile names `'-'` and `""`. See `plot special-filenames` (*note special-filenames:: ). 11. Additional coordinate systems for labels and arrows. See `coordinates` (*note Coordinates:: ). 12. `set size` (*note size:: ) can try to plot with a specified aspect ratio. 13. `set missing` (*note missing:: ) now treats missing data correctly. 14. The `call` (*note call:: ) command: `load` (*note load:: ) with arguments. 15. More flexible `range` commands with `reverse` and `writeback` keywords. 16. `set encoding` (*note encoding:: ) for multi-lingual encoding. 17. New `x11` (*note x11:: ) driver with persistent and multiple windows. 18. New plotting styles: `xerrorbars` (*note xerrorbars:: ), `histeps` (*note histeps:: ), `financebars` (*note financebars:: ) and more. See `set style` (*note style:: ). 19. New tic label formats, including `"%l %L"` which uses the mantissa and exponents to a given base for labels. See `set format` (*note format:: ). 20. New drivers, including `cgm` (*note cgm:: ) for inclusion into MS-Office applications and `gif` for serving plots to the WEB. 21. Smoothing and spline-fitting options for `plot`. See `plot smooth` (*note smooth:: ). 22. `set margin` (*note margin:: ) and `set origin` (*note origin:: ) give much better control over where a graph appears on the page. 23. `set border` (*note border:: ) now controls each border individually. 24. The new commands `if` (*note if:: ) and `reread` (*note reread:: ) allow command loops. 25. Point styles and sizes, line types and widths can be specified on the `plot` command. Line types and widths can also be specified for grids, borders, tics and arrows. See `plot with` (*note with:: ). Furthermore these types may be combined and stored for further use. See `set linestyle` (*note linestyle:: ). 26. Text (labels, tic labels, and the time stamp) can be written vertically by those terminals capable of doing so.  File: gnuplot.info, Node: Batch/Interactive Operation, Prev: What's New in version 3.7, Up: gnuplot, Next: Command-line-editing `gnuplot` (*note gnuplot:: ) may be executed in either batch or interactive modes, and the two may even be mixed together on many systems. Any command-line arguments are assumed to be names of files containing `gnuplot` commands (with the exception of standard X11 arguments, which are processed first). Each file is loaded with the `load` (*note load:: ) command, in the order specified. `gnuplot` exits after the last file is processed. When no load files are named, `gnuplot` enters into an interactive mode. The special filename "-" is used to denote standard input. Both the `exit` (*note exit:: ) and `quit` (*note quit:: ) commands terminate the current command file and `load` the next one, until all have been processed. Examples: To launch an interactive session: gnuplot To launch a batch session using two command files "input1" and "input2": gnuplot input1 input2 To launch an interactive session after an initialization file "header" and followed by another command file "trailer": gnuplot header - trailer  File: gnuplot.info, Node: Command-line-editing, Prev: Batch/Interactive Operation, Up: gnuplot, Next: Comments Command-line editing is supported by the Unix, Atari, VMS, MS-DOS and OS/2 versions of `gnuplot` (*note gnuplot:: ). Also, a history mechanism allows previous commands to be edited and re-executed. After the command line has been edited, a newline or carriage return will enter the entire line without regard to where the cursor is positioned. (The readline function in `gnuplot` is not the same as the readline used in GNU Bash and GNU Emacs. If the GNU version is desired, it may be selected instead of the `gnuplot` version at compile time.) The editing commands are as follows: `Line-editing`: ^B moves back a single character. ^F moves forward a single character. ^A moves to the beginning of the line. ^E moves to the end of the line. ^H and DEL delete the previous character. ^D deletes the current character. ^K deletes from current position to the end of line. ^L,^R redraws line in case it gets trashed. ^U deletes the entire line. ^W deletes the last word. `History`: ^P moves back through history. ^N moves forward through history. On the IBM PC, the use of a TSR program such as DOSEDIT or CED may be desired for line editing. The default makefile assumes that this is the case; by default `gnuplot` will be compiled with no line-editing capability. If you want to use `gnuplot`'s line editing, set READLINE in the makefile and add readline.obj to the link file. The following arrow keys may be used on the IBM PC and Atari versions if readline is used: Left Arrow - same as ^B. Right Arrow - same as ^F. Ctrl Left Arrow - same as ^A. Ctrl Right Arrow - same as ^E. Up Arrow - same as ^P. Down Arrow - same as ^N. The Atari version of readline defines some additional key aliases: Undo - same as ^L. Home - same as ^A. Ctrl Home - same as ^E. Esc - same as ^U. Help - `help` (*note help:: ) plus return. Ctrl Help - `help `.  File: gnuplot.info, Node: Comments, Prev: Command-line-editing, Up: gnuplot, Next: Coordinates Comments are supported as follows: a `#` may appear in most places in a line and `gnuplot` (*note gnuplot:: ) will ignore the rest of the line. It will not have this effect inside quotes, inside numbers (including complex numbers), inside command substitutions, etc. In short, it works anywhere it makes sense to work.  File: gnuplot.info, Node: Coordinates, Prev: Comments, Up: gnuplot, Next: Environment The commands `set arrow` (*note arrow:: ), `set key` (*note key:: ), and `set label` (*note label:: ) allow you to draw something at an arbitrary position on the graph. This position is specified by the syntax: {} , {} {,{} } Each can either be `first`, `second`, `graph` or `screen`. `first` places the x, y, or z coordinate in the system defined by the left and bottom axes; `second` places it in the system defined by the second axes (top and right); `graph` specifies the area within the axes---0,0 is bottom left and 1,1 is top right (for splot, 0,0,0 is bottom left of plotting area; use negative z to get to the base---see `set ticslevel` (*note ticslevel:: )); and screen specifies the screen area (the entire area---not just the portion selected by `set size` (*note size:: )), with 0,0 at bottom left and 1,1 at top right. If the coordinate system for x is not specified, `first` is used. If the system for y is not specified, the one used for x is adopted. If one (or more) axis is timeseries, the appropriate coordinate should be given as a quoted time string according to the `timefmt` (*note timefmt:: ) format string. See `set xdata` (*note xdata:: ) and set timefmt. . `gnuplot` (*note gnuplot:: ) will also accept an integer expression, which will be interpreted as seconds from 1 January 2000.  File: gnuplot.info, Node: Environment, Prev: Coordinates, Up: gnuplot, Next: Expressions A number of shell environment variables are understood by `gnuplot` (*note gnuplot:: ). None of these are required, but may be useful. If GNUTERM is defined, it is used as the name of the terminal type to be used. This overrides any terminal type sensed by `gnuplot` on start-up, but is itself overridden by the .gnuplot (or equivalent) start-up file (see `start-up`) and, of course, by later explicit changes. On Unix, AmigaOS, AtariTOS, MS-DOS and OS/2, GNUHELP may be defined to be the pathname of the HELP file (gnuplot.gih). On VMS, the logical name GNUPLOT$HELP should be defined as the name of the help library for `gnuplot`. The `gnuplot` help can be put inside any system help library, allowing access to help from both within and outside `gnuplot` if desired. On Unix, HOME is used as the name of a directory to search for a .gnuplot file if none is found in the current directory. On AmigaOS, AtariTOS, MS-DOS and OS/2, gnuplot is used. On VMS, SYS$LOGIN: is used. See `help (*note help:: ) start-up`. On Unix, PAGER is used as an output filter for help messages. On Unix, AtariTOS and AmigaOS, SHELL is used for the `shell` (*note shell:: ) command. On MS-DOS and OS/2, COMSPEC is used for the `shell` command. On MS-DOS, if the BGI or Watcom interface is used, PCTRM is used to tell the maximum resolution supported by your monitor by setting it to S. E.g. if your monitor's maximum resolution is 800x600, then use: set PCTRM=S800 If PCTRM is not set, standard VGA is used. FIT_SCRIPT may be used to specify a `gnuplot` command to be executed when a fit is interrupted---see `fit` (*note fit:: ). FIT_LOG specifies the filename of the logfile maintained by fit.  File: gnuplot.info, Node: Expressions, Prev: Environment, Up: gnuplot, Next: Functions In general, any mathematical expression accepted by C, FORTRAN, Pascal, or BASIC is valid. The precedence of these operators is determined by the specifications of the C programming language. White space (spaces and tabs) is ignored inside expressions. Complex constants are expressed as {,}, where and must be numerical constants. For example, {3,2} represents 3 + 2i; {0,1} represents 'i' itself. The curly braces are explicitly required here. Note that gnuplot uses both "real" and "integer" arithmetic, like FORTRAN and C. Integers are entered as "1", "-10", etc; reals as "1.0", "-10.0", "1e1", 3.5e-1, etc. The most important difference between the two forms is in division: division of integers truncates: 5/2 = 2; division of reals does not: 5.0/2.0 = 2.5. In mixed expressions, integers are "promoted" to reals before evaluation: 5/2e0 = 2.5. The result of division of a negative integer by a positive one may vary among compilers. Try a test like "print -5/2" to determine if your system chooses -2 or -3 as the answer. The integer expression "1/0" may be used to generate an "undefined" flag, which causes a point to ignored; the `ternary` (*note Ternary:: ) operator gives an example. The real and imaginary parts of complex expressions are always real, whatever the form in which they are entered: in {3,2} the "3" and "2" are reals, not integers. * Menu: * Functions:: * Operators:: * User-defined::  File: gnuplot.info, Node: Functions, Prev: Expressions, Up: Expressions, Next: abs The functions in `gnuplot` (*note gnuplot:: ) are the same as the corresponding functions in the Unix math library, except that all functions accept integer, real, and complex arguments, unless otherwise noted. For those functions that accept or return angles that may be given in either degrees or radians (sin(x), cos(x), tan(x), asin(x), acos(x), atan(x), atan2(x) and arg(z)), the unit may be selected by `set angles` (*note angles:: ), which defaults to radians. * Menu: * abs:: * acos:: * acosh:: * arg:: * asin:: * asinh:: * atan:: * atan2:: * atanh:: * besj0:: * besj1:: * besy0:: * besy1:: * ceil:: * cos:: * cosh:: * erf:: * erfc:: * exp:: * floor:: * gamma:: * ibeta:: * inverf:: * igamma:: * imag:: * invnorm:: * int:: * lgamma:: * log:: * log10:: * norm:: * rand:: * real:: * sgn:: * sin:: * sinh:: * sqrt:: * tan:: * tanh:: * column:: * tm_hour:: * tm_mday:: * tm_min:: * tm_mon:: * tm_sec:: * tm_wday:: * tm_yday:: * tm_year:: * valid::  File: gnuplot.info, Node: abs, Prev: Functions, Up: Functions, Next: acos The `abs` function returns the absolute value of its argument. The returned value is of the same type as the argument. For complex arguments, abs(x) is defined as the length of x in the complex plane [i.e., sqrt(real(x)**2 + imag(x)**2) ].  File: gnuplot.info, Node: acos, Prev: abs, Up: Functions, Next: acosh The `acos` function returns the arc cosine (inverse cosine) of its argument. `acos` returns its argument in radians or degrees, as selected by `set angles`.  File: gnuplot.info, Node: acosh, Prev: acos, Up: Functions, Next: arg The `acosh` function returns the inverse hyperbolic cosine of its argument in radians.  File: gnuplot.info, Node: arg, Prev: acosh, Up: Functions, Next: asin The `arg` function returns the phase of a complex number in radians or degrees, as selected by `set angles` (*note angles:: ).  File: gnuplot.info, Node: asin, Prev: arg, Up: Functions, Next: asinh The `asin` function returns the arc sin (inverse sin) of its argument. `asin` returns its argument in radians or degrees, as selected by `set angles`.  File: gnuplot.info, Node: asinh, Prev: asin, Up: Functions, Next: atan The `asinh` function returns the inverse hyperbolic sin of its argument in radians.  File: gnuplot.info, Node: atan, Prev: asinh, Up: Functions, Next: atan2 The `atan` function returns the arc tangent (inverse tangent) of its argument. `atan` returns its argument in radians or degrees, as selected by `set angles` (*note angles:: ).  File: gnuplot.info, Node: atan2, Prev: atan, Up: Functions, Next: atanh The `atan2` function returns the arc tangent (inverse tangent) of the ratio of the real parts of its arguments. `atan2` returns its argument in radians or degrees, as selected by `set angles` (*note angles:: ), in the correct quadrant.  File: gnuplot.info, Node: atanh, Prev: atan2, Up: Functions, Next: besj0 The `atanh` function returns the inverse hyperbolic tangent of its argument in radians.  File: gnuplot.info, Node: besj0, Prev: atanh, Up: Functions, Next: besj1 The `besj0` function returns the j0th Bessel function of its argument. `besj0` expects its argument to be in radians.  File: gnuplot.info, Node: besj1, Prev: besj0, Up: Functions, Next: besy0 The `besj1` function returns the j1st Bessel function of its argument. `besj1` expects its argument to be in radians.  File: gnuplot.info, Node: besy0, Prev: besj1, Up: Functions, Next: besy1 The `besy0` function returns the y0th Bessel function of its argument. `besy0` expects its argument to be in radians.  File: gnuplot.info, Node: besy1, Prev: besy0, Up: Functions, Next: ceil The `besy1` function returns the y1st Bessel function of its argument. `besy1` expects its argument to be in radians.  File: gnuplot.info, Node: ceil, Prev: besy1, Up: Functions, Next: cos The `ceil` function returns the smallest integer that is not less than its argument. For complex numbers, `ceil` returns the smallest integer not less than the real part of its argument.  File: gnuplot.info, Node: cos, Prev: ceil, Up: Functions, Next: cosh The `cos` function returns the cosine of its argument. `cos` accepts its argument in radians or degrees, as selected by `set angles` (*note angles:: ).  File: gnuplot.info, Node: cosh, Prev: cos, Up: Functions, Next: erf The `cosh` function returns the hyperbolic cosine of its argument. `cosh` expects its argument to be in radians.  File: gnuplot.info, Node: erf, Prev: cosh, Up: Functions, Next: erfc The `erf` function returns the error function of the real part of its argument. If the argument is a complex value, the imaginary component is ignored.  File: gnuplot.info, Node: erfc, Prev: erf, Up: Functions, Next: exp The `erfc` function returns 1.0 - the error function of the real part of its argument. If the argument is a complex value, the imaginary component is ignored.  File: gnuplot.info, Node: exp, Prev: erfc, Up: Functions, Next: floor The `exp` function returns the exponential function of its argument (`e` raised to the power of its argument). On some implementations (notably suns), exp(-x) returns undefined for very large x. A user-defined function like safe(x) = x<-100 ? 0 : exp(x) might prove useful in these cases.  File: gnuplot.info, Node: floor, Prev: exp, Up: Functions, Next: gamma The `floor` function returns the largest integer not greater than its argument. For complex numbers, `floor` returns the largest integer not greater than the real part of its argument.  File: gnuplot.info, Node: gamma, Prev: floor, Up: Functions, Next: ibeta The `gamma` function returns the gamma function of the real part of its argument. For integer n, gamma(n+1) = n!. If the argument is a complex value, the imaginary component is ignored.  File: gnuplot.info, Node: ibeta, Prev: gamma, Up: Functions, Next: inverf The `ibeta` function returns the incomplete beta function of the real parts of its arguments. p, q > 0 and x in [0:1]. If the arguments are complex, the imaginary components are ignored.  File: gnuplot.info, Node: inverf, Prev: ibeta, Up: Functions, Next: igamma The `inverf` function returns the inverse error function of the real part of its argument.  File: gnuplot.info, Node: igamma, Prev: inverf, Up: Functions, Next: imag The `igamma` function returns the incomplete gamma function of the real parts of its arguments. a > 0 and x >= 0. If the arguments are complex, the imaginary components are ignored.  File: gnuplot.info, Node: imag, Prev: igamma, Up: Functions, Next: invnorm The `imag` function returns the imaginary part of its argument as a real number.  File: gnuplot.info, Node: invnorm, Prev: imag, Up: Functions, Next: int The `invnorm` function returns the inverse normal distribution function of the real part of its argument.  File: gnuplot.info, Node: int, Prev: invnorm, Up: Functions, Next: lgamma The `int` function returns the integer part of its argument, truncated toward zero.  File: gnuplot.info, Node: lgamma, Prev: int, Up: Functions, Next: log The `lgamma` function returns the natural logarithm of the gamma function of the real part of its argument. If the argument is a complex value, the imaginary component is ignored.  File: gnuplot.info, Node: log, Prev: lgamma, Up: Functions, Next: log10 The `log` function returns the natural logarithm (base `e`) of its argument.  File: gnuplot.info, Node: log10, Prev: log, Up: Functions, Next: norm The `log10` function returns the logarithm (base 10) of its argument.  File: gnuplot.info, Node: norm, Prev: log10, Up: Functions, Next: rand The `norm` function returns the normal distribution function (or Gaussian) of the real part of its argument.  File: gnuplot.info, Node: rand, Prev: norm, Up: Functions, Next: real The `rand` function returns a pseudo random number in the interval [0:1] using the real part of its argument as a seed. If seed < 0, the sequence is (re)initialized. If the argument is a complex value, the imaginary component is ignored.  File: gnuplot.info, Node: real, Prev: rand, Up: Functions, Next: sgn The `real` function returns the real part of its argument.  File: gnuplot.info, Node: sgn, Prev: real, Up: Functions, Next: sin The `sgn` function returns 1 if its argument is positive, -1 if its argument is negative, and 0 if its argument is 0. If the argument is a complex value, the imaginary component is ignored.  File: gnuplot.info, Node: sin, Prev: sgn, Up: Functions, Next: sinh The `sin` function returns the sine of its argument. `sin` expects its argument to be in radians or degrees, as selected by `set angles` (*note angles:: ).  File: gnuplot.info, Node: sinh, Prev: sin, Up: Functions, Next: sqrt The `sinh` function returns the hyperbolic sine of its argument. `sinh` expects its argument to be in radians.  File: gnuplot.info, Node: sqrt, Prev: sinh, Up: Functions, Next: tan The `sqrt` function returns the square root of its argument.  File: gnuplot.info, Node: tan, Prev: sqrt, Up: Functions, Next: tanh The `tan` function returns the tangent of its argument. `tan` expects its argument to be in radians or degrees, as selected by `set angles` (*note angles:: ).  File: gnuplot.info, Node: tanh, Prev: tan, Up: Functions, Next: column The `tanh` function returns the hyperbolic tangent of its argument. `tanh` expects its argument to be in radians. A few additional functions are also available.  File: gnuplot.info, Node: column, Prev: tanh, Up: Functions, Next: tm_hour `column(x)` may be used only in expressions as part of `using` (*note using:: ) manipulations to fits or datafile plots. See `plot datafile using`.  File: gnuplot.info, Node: tm_hour, Prev: column, Up: Functions, Next: tm_mday The `tm_hour` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the hour (an integer in the range 0--23) as a real.  File: gnuplot.info, Node: tm_mday, Prev: tm_hour, Up: Functions, Next: tm_min The `tm_mday` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the day of the month (an integer in the range 1--31) as a real.  File: gnuplot.info, Node: tm_min, Prev: tm_mday, Up: Functions, Next: tm_mon The `tm_min` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the minute (an integer in the range 0--59) as a real.  File: gnuplot.info, Node: tm_mon, Prev: tm_min, Up: Functions, Next: tm_sec The `tm_mon` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the month (an integer in the range 1--12) as a real.  File: gnuplot.info, Node: tm_sec, Prev: tm_mon, Up: Functions, Next: tm_wday The `tm_sec` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the second (an integer in the range 0--59) as a real.  File: gnuplot.info, Node: tm_wday, Prev: tm_sec, Up: Functions, Next: tm_yday The `tm_wday` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the day of the week (an integer in the range 1--7) as a real.  File: gnuplot.info, Node: tm_yday, Prev: tm_wday, Up: Functions, Next: tm_year The `tm_yday` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the day of the year (an integer in the range 1--366) as a real.  File: gnuplot.info, Node: tm_year, Prev: tm_yday, Up: Functions, Next: valid The `tm_year` function interprets its argument as a time, in seconds from 1 Jan 2000. It returns the year (an integer) as a real.  File: gnuplot.info, Node: valid, Prev: tm_year, Up: Functions `valid(x)` may be used only in expressions as part of `using` (*note using:: ) manipulations to fits or datafile plots. See `plot datafile using`.  File: gnuplot.info, Node: Operators, Prev: Functions, Up: Expressions, Next: Unary The operators in `gnuplot` (*note gnuplot:: ) are the same as the corresponding operators in the C programming language, except that all operators accept integer, real, and complex arguments, unless otherwise noted. The ** operator (exponentiation) is supported, as in FORTRAN. Parentheses may be used to change order of evaluation. * Menu: * Unary:: * Binary:: * Ternary::  File: gnuplot.info, Node: Unary, Prev: Operators, Up: Operators, Next: Binary The following is a list of all the unary operators and their usages: Symbol Example Explanation - -a unary minus + +a unary plus (no-operation) ~ ~a * one's complement ! !a * logical negation ! a! * factorial $ $3 * call arg/column during `using` (*note using:: ) manipulation (*) Starred explanations indicate that the operator requires an integer argument. Operator precedence is the same as in Fortran and C. As in those languages, parentheses may be used to change the order of operation. Thus -2**2 = -4, but (-2)**2 = 4. The factorial operator returns a real number to allow a greater range.  File: gnuplot.info, Node: Binary, Prev: Unary, Up: Operators, Next: Ternary The following is a list of all the binary operators and their usages: Symbol Example Explanation ** a**b exponentiation * a*b multiplication / a/b division % a%b * modulo + a+b addition - a-b subtraction == a==b equality != a!=b inequality < a a>b greater than >= a>=b greater than or equal to & a&b * bitwise AND ^ a^b * bitwise exclusive OR | a|b * bitwise inclusive OR && a&&b * logical AND || a||b * logical OR (*) Starred explanations indicate that the operator requires integer arguments. Logical AND (&&) and OR (||) short-circuit the way they do in C. That is, the second `&&` operand is not evaluated if the first is false; the second `||` operand is not evaluated if the first is true.  File: gnuplot.info, Node: Ternary, Prev: Binary, Up: Operators There is a single ternary operator: Symbol Example Explanation ?: a?b:c ternary operation The ternary operator behaves as it does in C. The first argument (a), which must be an integer, is evaluated. If it is true (non-zero), the second argument (b) is evaluated and returned; otherwise the third argument (c) is evaluated and returned. The ternary operator is very useful both in constructing piecewise functions and in plotting points only when certain conditions are met. Examples: Plot a function that is to equal sin(x) for 0 <= x < 1, 1/x for 1 <= x < 2, and undefined elsewhere: f(x) = 0<=x && x<1 ? sin(x) : 1<=x && x<2 ? 1/x : 1/0 plot f(x) Note that `gnuplot` (*note gnuplot:: ) quietly ignores undefined values, so the final branch of the function (1/0) will produce no plottable points. Note also that f(x) will be plotted as a continuous function across the discontinuity if a line style is used. To plot it discontinuously, create separate functions for the two pieces. (Parametric functions are also useful for this purpose.) For data in a file, plot the average of the data in columns 2 and 3 against the datum in column 1, but only if the datum in column 4 is non-negative: plot 'file' using 1:( $4<0 ? 1/0 : ($2+$3)/2 ) Please see `plot data-file using` (*note using:: ) for an explanation of the using syntax.  File: gnuplot.info, Node: User-defined, Prev: Operators, Up: Expressions New user-defined variables and functions of one through five variables may be declared and used anywhere, including on the `plot` (*note plot:: ) command itself. User-defined function syntax: ( {,} ... {,} ) = where is defined in terms of through . User-defined variable syntax: = Examples: w = 2 q = floor(tan(pi/2 - 0.1)) f(x) = sin(w*x) sinc(x) = sin(pi*x)/(pi*x) delta(t) = (t == 0) ramp(t) = (t > 0) ? t : 0 min(a,b) = (a < b) ? a : b comb(n,k) = n!/(k!*(n-k)!) len3d(x,y,z) = sqrt(x*x+y*y+z*z) plot f(x) = sin(x*a), a = 0.2, f(x), a = 0.4, f(x) Note that the variable `pi` is already defined. But it is in no way magic; you may redefine it to be whatever you like. Valid names are the same as in most programming languages: they must begin with a letter, but subsequent characters may be letters, digits, "$", or "_". Note, however, that the `fit` (*note fit:: ) mechanism uses several variables with names that begin "FIT_". It is safest to avoid using such names. "FIT_LIMIT", however, is one that you may wish to redefine. See the documentation on `fit` for details. See `show functions` (*note functions:: ), `show variables` (*note variables:: ), and fit.  File: gnuplot.info, Node: Glossary, Prev: Expressions, Up: gnuplot, Next: Plotting Throughout this document an attempt has been made to maintain consistency of nomenclature. This cannot be wholly successful because as `gnuplot` (*note gnuplot:: ) has evolved over time, certain command and keyword names have been adopted that preclude such perfection. This section contains explanations of the way some of these terms are used. A "page" or "screen" is the entire area addressable by `gnuplot`. On a monitor, it is the full screen; on a plotter, it is a single sheet of paper. A screen may contain one or more "plots". A plot is defined by an abscissa and an ordinate, although these need not actually appear on it, as well as the margins and any text written therein. A plot contains one "graph". A graph is defined by an abscissa and an ordinate, although these need not actually appear on it. A graph may contain one or more "lines". A line is a single function or data set. "Line" is also a plotting style. The word will also be used in sense "a line of text". Presumably the context will remove any ambiguity. The lines on a graph may have individual names. These may be listed together with a sample of the plotting style used to represent them in the "key", sometimes also called the "legend". The word "title" occurs with multiple meanings in `gnuplot`. In this document, it will always be preceded by the adjective "plot", "line", or "key" to differentiate among them. A graph may have up to four labelled axes. Various commands have the name of an axis built into their names, such as `set xlabel` (*note xlabel:: ). Other commands have one or more axis names as options, such as `set logscale xy`. The names of the four axes for these usages are "x" for the axis along the bottom border of the plot, "y" for the left border, "x2" for the top border, and "y2" for the right border. "z" also occurs in commands used with 3-d plotting. When discussing data files, the term "record" will be resurrected and used to denote a single line of text in the file, that is, the characters between newline or end-of-record characters. A "point" is the datum extracted from a single record. A "datablock" is a set of points from consecutive records, delimited by blank records. A line, when referred to in the context of a data file, is a subset of a datablock.  File: gnuplot.info, Node: Plotting, Prev: Glossary, Up: gnuplot, Next: Start-up There are three `gnuplot` (*note gnuplot:: ) commands which actually create a plot: `plot` (*note plot:: ), `splot` (*note splot:: ) and `replot` (*note replot:: ). plot generates 2-d plots, splot generates 3-d plots (actually 2-d projections, of course), and `replot` appends its arguments to the previous `plot` or `splot` and executes the modified command. Much of the general information about plotting can be found in the discussion of `plot`; information specific to 3-d can be found in the `splot` section. `plot` operates in either rectangular or polar coordinates -- see `set polar` (*note polar:: ) for details of the latter. `splot` operates only in rectangular coordinates, but the `set mapping` (*note mapping:: ) command allows for a few other coordinate systems to be treated. In addition, the `using` (*note using:: ) option allows both plot and splot to treat almost any coordinate system you'd care to define. `splot` can plot surfaces and contours in addition to points and/or lines. In addition to `splot`, see `set isosamples` (*note isosamples:: ) for information about defining the grid for a 3-d function; `splot datafile` (*note data-file:: ) for information about the requisite file structure for 3-d data values; and `set contour` (*note contour:: ) and set cntrparam` for information about contours.  File: gnuplot.info, Node: Start-up, Prev: Plotting, Up: gnuplot, Next: Substitution When `gnuplot` (*note gnuplot:: ) is run, it looks for an initialization file to load. This file is called `.gnuplot` on Unix and AmigaOS systems, and `GNUPLOT.INI` on other systems. If this file is not found in the current directory, the program will look for it in the home directory (under AmigaOS, Atari(single)TOS, MS-DOS and OS/2, the environment variable `gnuplot` should contain the name of this directory). Note: if NOCWDRC is defined during the installation, `gnuplot` will not read from the current directory. If the initialization file is found, `gnuplot` executes the commands in it. These may be any legal `gnuplot` commands, but typically they are limited to setting the terminal and defining frequently-used functions or variables.  File: gnuplot.info, Node: Substitution, Prev: Start-up, Up: gnuplot, Next: Syntax Command-line substitution is specified by a system command enclosed in backquotes. This command is spawned and the output it produces replaces the name of the command (and backquotes) on the command line. Some implementations also support pipes; see `plot data-file special-filenames` (*note special-filenames:: ). Newlines in the output produced by the spawned command are replaced with blanks. Command-line substitution can be used anywhere on the `gnuplot` (*note gnuplot:: ) command line. Example: This will run the program `leastsq` and replace `leastsq` (including backquotes) on the command line with its output: f(x) = `leastsq` or, in VMS f(x) = `run leastsq`  File: gnuplot.info, Node: Syntax, Prev: Substitution, Up: gnuplot, Next: Time/Date data The general rules of syntax and punctuation in `gnuplot` (*note gnuplot:: ) are that keywords and options are order-dependent. Options and any accompanying parameters are separated by spaces whereas lists and coordinates are separated by commas. Ranges are separated by colons and enclosed in brackets [], text and file names are enclosed in quotes, and a few miscellaneous things are enclosed in parentheses. Braces {} are used for a few special purposes. Commas are used to separate coordinates on the `set` (*note set-show:: ) commands `arrow` (*note arrow:: ), `key` (*note key:: ), and `label` (*note label:: ); the list of variables being fitted (the list after the `via` keyword on the `fit` (*note fit:: ) command); lists of discrete contours or the loop parameters which specify them on the `set cntrparam` (*note cntrparam:: ) command; the arguments of the `set` commands `dgrid3d` (*note dgrid3d:: ), `dummy` (*note dummy:: ), `isosamples` (*note isosamples:: ), `offsets` (*note offsets:: ), `origin` (*note origin:: ), `samples` (*note samples:: ), `size` (*note size:: ), time, and nd `view` (*note view:: ); lists of tics or the loop parameters which specify them; the offsets for titles and axis labels; parametric functions to be used to calculate the x, y, and z coordinates on the `plot` (*note plot:: ), `replot` (*note replot:: ) and `splot` (*note splot:: ) commands; and the complete sets of keywords specifying individual plots (data sets or functions) on the `plot`, `replot` and `splot` commands. Parentheses are used to delimit sets of explicit tics (as opposed to loop parameters) and to indicate computations in the `using` (*note using:: ) filter of the fit, `plot`, `replot` and `splot` commands. (Parentheses and commas are also used as usual in function notation.) Brackets are used to delimit ranges, whether they are given on `set`, `plot` or `splot` commands. Colons are used to separate extrema in `range` specifications (whether they are given on `set`, `plot` or `splot` commands) and to separate entries in the `using` filter of the `plot`, `replot`, `splot` and `fit` commands. Semicolons are used to separate commands given on a single command line. Braces are used in text to be specially processed by some terminals, like `postscript` (*note postscript:: ). They are also used to denote complex numbers: {3,2} = 3 + 2i. Text may be enclosed in single- or double-quotes. Backslash processing of sequences like \n (newline) and \345 (octal character code) is performed for double-quoted strings, but not for single-quoted strings. The justification is the same for each line of a multi-line string. Thus the center-justified string "This is the first line of text.\nThis is the second line." will produce This is the first line of text. This is the second line. but 'This is the first line of text.\nThis is the second line.' will produce This is the first line of text.\nThis is the second line. Filenames may be entered with either single- or double-quotes. In this manual the command examples generally single-quote filenames and double-quote other string tokens for clarity. At present you should not embed \n inside {} when using the enhanced option of the postscript terminal. The EEPIC, Imagen, Uniplex, LaTeX, and TPIC drivers allow a newline to be specified by \\ in a single-quoted string or \\\\ in a double-quoted string. Back-quotes are used to enclose system commands for substitution.  File: gnuplot.info, Node: Time/Date data, Prev: Syntax, Up: gnuplot `gnuplot` (*note gnuplot:: ) supports the use of time and/or date information as input data. This feature is activated by the commands `set xdata time`, `set ydata time`, etc. Internally all times and dates are converted to the number of seconds from the year 2000. The command `set timefmt` (*note timefmt:: ) defines the format for all inputs: data files, ranges, tics, label positions---in short, anything that accepts a data value must receive it in this format. Since only one input format can be in force at a given time, all time/date quantities being input at the same time must be presented in the same format. Thus if both x and y data in a file are time/date, they must be in the same format. The conversion to and from seconds assumes Universal Time (which is the same as Greenwich Standard Time). There is no provision for changing the time zone or for daylight savings. If all your data refer to the same time zone (and are all either daylight or standard) you don't need to worry about these things. But if the absolute time is crucial for your application, you'll need to convert to UT yourself. Commands like `show xrange` (*note xrange:: ) will re-interpret the integer according to `timefmt`. If you change `timefmt`, and then `show` (*note set-show:: ) the quantity again, it will be displayed in the new `timefmt`. For that matter, if you give the deactivation command (like `set xdata` (*note xdata:: )), the quantity will be shown in its numerical form. The command `set format` (*note format:: ) defines the format that will be used for tic labels, whether or not the specified axis is time/date. If time/date information is to be plotted from a file, the `using` (*note using:: ) option _must_ be used on the `plot` (*note plot:: ) or `splot` (*note splot:: ) command. These commands simply use white space to separate columns, but white space may be embedded within the time/date string. If you use tabs as a separator, some trial-and-error may be necessary to discover how your system treats them. The following example demonstrates time/date plotting. Suppose the file "data" contains records like 03/21/95 10:00 6.02e23 This file can be plotted by set xdata time set timefmt "%m/%d/%y" set xrange ["03/21/95":"03/22/95"] set format x "%m/%d" set timefmt "%m/%d/%y %H:%M" plot "data" using 1:3 which will produce xtic labels that look like "03/21". See the descriptions of each command for more details.  File: gnuplot.info, Node: Commands, Prev: gnuplot, Up: Top, Next: cd This section lists the commands acceptable to `gnuplot` (*note gnuplot:: ) in alphabetical order. Printed versions of this document contain all commands; on-line versions may not be complete. Indeed, on some systems there may be no commands at all listed under this heading. Note that in most cases unambiguous abbreviations for command names and their options are permissible, i.e., "`p f(x) w l`" instead of "`plot f(x) with lines`". In the syntax descriptions, braces ({}) denote optional arguments and a vertical bar (|) separates mutually exclusive choices. * Menu: * cd:: * call:: * clear:: * exit:: * fit:: * help:: * if:: * load:: * pause:: * plot:: * print:: * pwd:: * quit:: * replot:: * reread:: * reset:: * save:: * set-show:: * shell:: * splot:: * test:: * update::  File: gnuplot.info, Node: cd, Prev: Commands, Up: Commands, Next: call The `cd` command changes the working directory. Syntax: cd '' The directory name must be enclosed in quotes. Examples: cd 'subdir' cd ".." DOS users _must_ use single-quotes---backslash [\] has special significance inside double-quotes. For example, cd "c:\newdata" fails, but cd 'c:\newdata' works as expected.  File: gnuplot.info, Node: call, Prev: cd, Up: Commands, Next: clear The `call` command is identical to the load command with one exception: you can have up to ten additional parameters to the command (delimited according to the standard parser rules) which can be substituted into the lines read from the file. As each line is read from the `call`ed input file, it is scanned for the sequence `$` (dollar-sign) followed by a digit (0--9). If found, the sequence is replaced by the corresponding parameter from the `call` command line. If the parameter was specified as a string in the `call` line, it is substituted without its enclosing quotes. `$` followed by any character other than a digit will be that character. E.g. use `$$` to get a single `$`. Providing more than ten parameters on the `call` command line will cause an error. A parameter that was not provided substitutes as nothing. Files being `call`ed may themselves contain `call` or `load` (*note load:: ) commands. The `call` command _must_ be the last command on a multi-command line. Syntax: call "" ... The name of the input file must be enclosed in quotes, and it is recommended that parameters are similarly enclosed in quotes (future versions of gnuplot may treat quoted and unquoted arguments differently). Example: If the file 'calltest.gp' contains the line: print "p0=$0 p1=$1 p2=$2 p3=$3 p4=$4 p5=$5 p6=$6 p7=x$7x" entering the command: call 'calltest.gp' "abcd" 1.2 + "'quoted'" -- "$2" will display: p0=abcd p1=1.2 p2=+ p3='quoted' p4=- p5=- p6=$2 p7=xx NOTE: there is a clash in syntax with the datafile `using` (*note using:: ) callback operator. Use `$$n` or `column(n)` to access column n from a datafile inside a `call`ed datafile plot.  File: gnuplot.info, Node: clear, Prev: call, Up: Commands, Next: exit The `clear` command erases the current screen or output device as specified by `set output` (*note output:: ). This usually generates a formfeed on hardcopy devices. Use `set terminal` (*note terminal:: ) to set the device type. For some terminals `clear` erases only the portion of the plotting surface defined by `set size` (*note size:: ), so for these it can be used in conjunction with set multiplot` to create an inset. Example: set multiplot plot sin(x) set origin 0.5,0.5 set size 0.4,0.4 clear plot cos(x) set nomultiplot Please see `set multiplot` (*note multiplot:: ), set size, and nd `set origin` (*note origin:: ) for details of these commands.  File: gnuplot.info, Node: exit, Prev: clear, Up: Commands, Next: fit The commands `exit` and `quit` (*note quit:: ) and the END-OF-FILE character will exit the current `gnuplot` (*note gnuplot:: ) command file and `load` (*note load:: ) the next one. See "help batch/interactive" for more details. Each of these commands will clear the output device (as does the `clear` (*note clear:: ) command) before exiting.  File: gnuplot.info, Node: fit, Prev: exit, Up: Commands, Next: adjustable parameters The `fit` command can fit a user-defined function to a set of data points (x,y) or (x,y,z), using an implementation of the nonlinear least-squares (NLLS) Marquardt-Levenberg algorithm. Any user-defined variable occurring in the function body may serve as a fit parameter, but the return type of the function must be real. Syntax: fit {[xrange] {[yrange]}} '' {datafile-modifiers} via '' | {,,...} Ranges may be specified to temporarily limit the data which is to be fitted; any out-of-range data points are ignored. The syntax is [{dummy_variable=}{}{:}], analogous to `plot` (*note plot:: ); see `plot ranges` (*note ranges:: ). is any valid `gnuplot` (*note gnuplot:: ) expression, although it is usual to use a previously user-defined function of the form f(x) or f(x,y). is treated as in the `plot` command. All the `plot datafile` (*note data-file:: ) modifiers (`using` (*note using:: ), `every` (*note every:: ),...) except `smooth` (*note smooth:: ) are applicable to fit. See `plot datafile`. The default data formats for fitting functions with a single independent variable, y=f(x), are {x:}y or x:y:s; those formats can be changed with the datafile `using` qualifier. The third item, (a column number or an expression), if present, is interpreted as the standard deviation of the corresponding y value and is used to compute a weight for the datum, 1/s**2. Otherwise, all data points are weighted equally, with a weight of one. To fit a function with two independent variables, z=f(x,y), the required format is `using` with four items, x:y:z:s. The complete format must be given---no default columns are assumed for a missing token. Weights for each data point are evaluated from 's' as above. If error estimates are not available, a constant value can be specified as a constant expression (see `plot datafile using`), e.g., `using 1:2:3:(1)`. Multiple datasets may be simultaneously fit with functions of one independent variable by making y a 'pseudo-variable', e.g., the dataline number, and fitting as two independent variables. See `fit multibranch`. The `via` qualifier specifies which parameters are to be adjusted, either directly, or by referencing a parameter file. Examples: f(x) = a*x**2 + b*x + c g(x,y) = a*x**2 + b*y**2 + c*x*y FIT_LIMIT = 1e-6 fit f(x) 'measured.dat' via 'start.par' fit f(x) 'measured.dat' using 3:($7-5) via 'start.par' fit f(x) './data/trash.dat' using 1:2:3 via a, b, c fit g(x,y) 'surface.dat' using 1:2:3:(1) via a, b, c After each iteration step, detailed information about the current state of the fit is written to the display. The same information about the initial and final states is written to a log file, "fit.log". This file is always appended to, so as to not lose any previous fit history; it should be deleted or renamed as desired. The fit may be interrupted by pressing Ctrl-C (any key but Ctrl-C under MSDOS and Atari Multitasking Systems). After the current iteration completes, you have the option to (1) stop the fit and accept the current parameter values, (2) continue the fit, (3) execute a `gnuplot` command as specified by the environment variable FIT_SCRIPT. The default for FIT_SCRIPT is `replot` (*note replot:: ), so if you had previously plotted both the data and the fitting function in one graph, you can display the current state of the fit. Once `fit` has finished, the `update` (*note update:: ) command may be used to store final values in a file for subsequent use as a parameter file. See `update` for details. * Menu: * adjustable parameters:: * beginner's guide:: * error estimates:: * fit controlling:: * multi-branch:: * starting values:: * tips::  File: gnuplot.info, Node: adjustable parameters, Prev: fit, Up: fit, Next: beginner's guide There are two ways that `via` can specify the parameters to be adjusted, either directly on the command line or indirectly, by referencing a parameter file. The two use different means to set initial values. Adjustable parameters can be specified by a comma-separated list of variable names after the `via` keyword. Any variable that is not already defined is is created with an initial value of 1.0. However, the fit is more likely to converge rapidly if the variables have been previously declared with more appropriate starting values. In a parameter file, each parameter to be varied and a corresponding initial value are specified, one per line, in the form varname = value Comments, marked by '#', and blank lines are permissible. The special form varname = value # FIXED means that the variable is treated as a 'fixed parameter', initialized by the parameter file, but not adjusted by `fit` (*note fit:: ). For clarity, it may be useful to designate variables as fixed parameters so that their values are reported by `fit`. The keyword `# FIXED` has to appear in exactly this form.  File: gnuplot.info, Node: beginner's guide, Prev: adjustable parameters, Up: fit, Next: error estimates `fit` (*note fit:: ) is used to find a set of parameters that 'best' fits your data to your user-defined function. The fit is judged on the basis of the the sum of the squared differences or 'residuals' (SSR) between the input data points and the function values, evaluated at the same places. This quantity is often called 'chisquare' (i.e., the Greek letter chi, to the power of 2). The algorithm attempts to minimize SSR, or more precisely, WSSR, as the residuals are 'weighted' by the input data errors (or 1.0) before being squared; see `fit error_estimates` for details. That's why it is called 'least-squares fitting'. Let's look at an example to see what is meant by 'non-linear', but first we had better go over some terms. Here it is convenient to use z as the dependent variable for user-defined functions of either one independent variable, z=f(x), or two independent variables, z=f(x,y). A parameter is a user-defined variable that `fit` will adjust, i.e., an unknown quantity in the function declaration. Linearity/non-linearity refers to the relationship of the dependent variable, z, to the parameters which `fit` is adjusting, not of z to the independent variables, x and/or y. (To be technical, the second {and higher} derivatives of the fitting function with respect to the parameters are zero for a linear least-squares problem). For linear least-squares (LLS), the user-defined function will be a sum of simple functions, not involving any parameters, each multiplied by one parameter. NLLS handles more complicated functions in which parameters can be used in a large number of ways. An example that illustrates the difference between linear and nonlinear least-squares is the Fourier series. One member may be written as z=a*sin(c*x) + b*cos(c*x). If a and b are the unknown parameters and c is constant, then estimating values of the parameters is a linear least-squares problem. However, if c is an unknown parameter, the problem is nonlinear. In the linear case, parameter values can be determined by comparatively simple linear algebra, in one direct step. However LLS is a special case which is also solved along with more general NLLS problems by the iterative procedure that `gnuplot` (*note gnuplot:: ) uses. fit attempts to find the minimum by doing a search. Each step (iteration) calculates WSSR with a new set of parameter values. The Marquardt-Levenberg algorithm selects the parameter values for the next iteration. The process continues until a preset criterium is met, either (1) the fit has "converged" (the relative change in WSSR is less than FIT_LIMIT), or (2) it reaches a preset iteration count limit, FIT_MAXITER (see `fit control variables` (*note control variables:: )). The fit may also be interrupted and subsequently halted from the keyboard (see `fit`). Often the function to be fitted will be based on a model (or theory) that attempts to describe or predict the behaviour of the data. Then `fit` can be used to find values for the free parameters of the model, to determine how well the data fits the model, and to estimate an error range for each parameter. See `fit error_estimates`. Alternatively, in curve-fitting, functions are selected independent of a model (on the basis of experience as to which are likely to describe the trend of the data with the desired resolution and a minimum number of parameters*functions.) The `fit` solution then provides an analytic representation of the curve. However, if all you really want is a smooth curve through your data points, the `smooth` (*note smooth:: ) option to `plot` (*note plot:: ) may be what you've been looking for rather than `fit`.  File: gnuplot.info, Node: error estimates, Prev: beginner's guide, Up: fit, Next: statistical overview In `fit` (*note fit:: ), the term "error" is used in two different contexts, data error estimates and parameter error estimates. Data error estimates are used to calculate the relative weight of each data point when determining the weighted sum of squared residuals, WSSR or chisquare. They can affect the parameter estimates, since they determine how much influence the deviation of each data point from the fitted function has on the final values. Some of the `fit` output information, including the parameter error estimates, is more meaningful if accurate data error estimates have been provided. The 'statistical overview' describes some of the `fit` output and gives some background for the 'practical guidelines'. * Menu: * statistical overview:: * practical guidelines::  File: gnuplot.info, Node: statistical overview, Prev: error estimates, Up: error estimates, Next: practical guidelines The theory of non-linear least-squares (NLLS) is generally described in terms of a normal distribution of errors, that is, the input data is assumed to be a sample from a population having a given mean and a Gaussian (normal) distribution about the mean with a given standard deviation. For a sample of sufficiently large size, and knowing the population standard deviation, one can use the statistics of the chisquare distribution to describe a "goodness of fit" by looking at the variable often called "chisquare". Here, it is sufficient to say that a reduced chisquare (chisquare/degrees of freedom, where degrees of freedom is the number of datapoints less the number of parameters being fitted) of 1.0 is an indication that the weighted sum of squared deviations between the fitted function and the data points is the same as that expected for a random sample from a population characterized by the function with the current value of the parameters and the given standard deviations. If the standard deviation for the population is not constant, as in counting statistics where variance = counts, then each point should be individually weighted when comparing the observed sum of deviations and the expected sum of deviations. At the conclusion `fit` (*note fit:: ) reports 'stdfit', the standard deviation of the fit, which is the rms of the residuals, and the variance of the residuals, also called 'reduced chisquare' when the data points are weighted. The number of degrees of freedom (the number of data points minus the number of fitted parameters) is used in these estimates because the parameters used in calculating the residuals of the datapoints were obtained from the same data. To estimate confidence levels for the parameters, one can use the minimum chisquare obtained from the fit and chisquare statistics to determine the value of chisquare corresponding to the desired confidence level, but considerably more calculation is required to determine the combinations of parameters which produce such values. Rather than determine confidence intervals, `fit` reports parameter error estimates which are readily obtained from the variance-covariance matrix after the final iteration. By convention, these estimates are called "standard errors" or "asymptotic standard errors", since they are calculated in the same way as the standard errors (standard deviation of each parameter) of a linear least-squares problem, even though the statistical conditions for designating the quantity calculated to be a standard deviation are not generally valid for the NLLS problem. The asymptotic standard errors are generally over-optimistic and should not be used for determining confidence levels, but are useful for qualitative purposes. The final solution also produces a correlation matrix, which gives an indication of the correlation of parameters in the region of the solution; if one parameter is changed, increasing chisquare, does changing another compensate? The main diagonal elements, autocorrelation, are all 1; if all parameters were independent, all other elements would be nearly 0. Two variables which completely compensate each other would have an off-diagonal element of unit magnitude, with a sign depending on whether the relation is proportional or inversely proportional. The smaller the magnitudes of the off-diagonal elements, the closer the estimates of the standard deviation of each parameter would be to the asymptotic standard error.  File: gnuplot.info, Node: practical guidelines, Prev: statistical overview, Up: error estimates If you have a basis for assigning weights to each data point, doing so lets you make use of additional knowledge about your measurements, e.g., take into account that some points may be more reliable than others. That may affect the final values of the parameters. Weighting the data provides a basis for interpreting the additional `fit` (*note fit:: ) output after the last iteration. Even if you weight each point equally, estimating an average standard deviation rather than using a weight of 1 makes WSSR a dimensionless variable, as chisquare is by definition. Each fit iteration will display information which can be used to evaluate the progress of the fit. (An '*' indicates that it did not find a smaller WSSR and is trying again.) The 'sum of squares of residuals', also called 'chisquare', is the WSSR between the data and your fitted function; `fit` has minimized that. At this stage, with weighted data, chisquare is expected to approach the number of degrees of freedom (data points minus parameters). The WSSR can be used to calculate the reduced chisquare (WSSR/ndf) or stdfit, the standard deviation of the fit, sqrt(WSSR/ndf). Both of these are reported for the final WSSR. If the data are unweighted, stdfit is the rms value of the deviation of the data from the fitted function, in user units. If you supplied valid data errors, the number of data points is large enough, and the model is correct, the reduced chisquare should be about unity. (For details, look up the 'chi-squared distribution' in your favourite statistics reference.) If so, there are additional tests, beyond the scope of this overview, for determining how well the model fits the data. A reduced chisquare much larger than 1.0 may be due to incorrect data error estimates, data errors not normally distributed, systematic measurement errors, 'outliers', or an incorrect model function. A plot of the residuals, e.g., `plot 'datafile' using 1:($2-f($1))`, may help to show any systematic trends. Plotting both the data points and the function may help to suggest another model. Similarly, a reduced chisquare less than 1.0 indicates WSSR is less than that expected for a random sample from the function with normally distributed errors. The data error estimates may be too large, the statistical assumptions may not be justified, or the model function may be too general, fitting fluctuations in a particular sample in addition to the underlying trends. In the latter case, a simpler function may be more appropriate. You'll have to get used to both `fit` and the kind of problems you apply it to before you can relate the standard errors to some more practical estimates of parameter uncertainties or evaluate the significance of the correlation matrix. Note that `fit`, in common with most NLLS implementations, minimizes the weighted sum of squared distances (y-f(x))**2. It does not provide any means to account for "errors" in the values of x, only in y. Also, any "outliers" (data points outside the normal distribution of the model) will have an exaggerated effect on the solution.  File: gnuplot.info, Node: fit controlling, Prev: error estimates, Up: fit, Next: control variables There are a number of `gnuplot` (*note gnuplot:: ) variables that can be defined to affect `fit` (*note fit:: ). Those which can be defined once gnuplot is running are listed under 'control_variables' while those defined before starting `gnuplot` are listed under 'environment_variables'. * Menu: * control variables:: * environment variables::  File: gnuplot.info, Node: control variables, Prev: fit controlling, Up: fit controlling, Next: environment variables The default epsilon limit (1e-5) may be changed by declaring a value for FIT_LIMIT When the sum of squared residuals changes between two iteration steps by a factor less than this number (epsilon), the fit is considered to have 'converged'. The maximum number of iterations may be limited by declaring a value for FIT_MAXITER A value of 0 (or not defining it at all) means that there is no limit. If you need even more control about the algorithm, and know the Marquardt-Levenberg algorithm well, there are some more variables to influence it. The startup value of `lambda` is normally calculated automatically from the ML-matrix, but if you want to, you may provide your own one with FIT_START_LAMBDA Specifying FIT_START_LAMBDA as zero or less will re-enable the automatic selection. The variable FIT_LAMBDA_FACTOR gives the factor by which `lambda` is increased or decreased whenever the chi-squared target function increased or decreased significantly. Setting FIT_LAMBDA_FACTOR to zero re-enables the default factor of 10.0. Oher variables with the FIT_ prefix may be added to `fit` (*note fit:: ), so it is safer not to use that prefix for user-defined variables. The variables FIT_SKIP and FIT_INDEX were used by earlier releases of `gnuplot` (*note gnuplot:: ) with a 'fit' patch called gnufit and are no longer available. The datafile `every` (*note every:: ) modifier provides the functionality of FIT_SKIP. FIT_INDEX was used for multi-branch fitting, but multi-branch fitting of one independent variable is now done as a pseudo-3D fit in which the second independent variable and `using` (*note using:: ) are used to specify the branch. See `fit multi-branch` (*note multi-branch:: ).  File: gnuplot.info, Node: environment variables, Prev: control variables, Up: fit controlling The environment variables must be defined before `gnuplot` (*note gnuplot:: ) is executed; how to do so depends on your operating system. FIT_LOG changes the name (and/or path) of the file to which the fit log will be written from the default of "fit.log" in the working directory. FIT_SCRIPT specifies a command that may be executed after an user interrupt. The default is `replot` (*note replot:: ), but a `plot` (*note plot:: ) or `load` (*note load:: ) command may be useful to display a plot customized to highlight the progress of the fit.  File: gnuplot.info, Node: multi-branch, Prev: fit controlling, Up: fit, Next: starting values In multi-branch fitting, multiple data sets can be simultaneously fit with functions of one independent variable having common parameters by minimizing the total WSSR. The function and parameters (branch) for each data set are selected by using a 'pseudo-variable', e.g., either the dataline number (a 'column' index of -1) or the datafile index (-2), as the second independent variable. Example: Given two exponential decays of the form, z=f(x), each describing a different data set but having a common decay time, estimate the values of the parameters. If the datafile has the format x:z:s, then f(x,y) = (y==0) ? a*exp(-x/tau) : b*exp(-x/tau) fit f(x,y) 'datafile' using 1:-1:2:3 via a, b, tau For a more complicated example, see the file "hexa.fnc" used by the "fit.dem" demo. Appropriate weighting may be required since unit weights may cause one branch to predominate if there is a difference in the scale of the dependent variable. Fitting each branch separately, using the multi-branch solution as initial values, may give an indication as to the relative effect of each branch on the joint solution.  File: gnuplot.info, Node: starting values, Prev: multi-branch, Up: fit, Next: tips Nonlinear fitting is not guaranteed to converge to the global optimum (the solution with the smallest sum of squared residuals, SSR), and can get stuck at a local minimum. The routine has no way to determine that; it is up to you to judge whether this has happened. `fit` (*note fit:: ) may, and often will get "lost" if started far from a solution, where SSR is large and changing slowly as the parameters are varied, or it may reach a numerically unstable region (e.g., too large a number causing a floating point overflow) which results in an "undefined value" message or `gnuplot` (*note gnuplot:: ) halting. To improve the chances of finding the global optimum, you should set the starting values at least roughly in the vicinity of the solution, e.g., within an order of magnitude, if possible. The closer your starting values are to the solution, the less chance of stopping at another minimum. One way to find starting values is to plot data and the fitting function on the same graph and change parameter values and `replot` (*note replot:: ) until reasonable similarity is reached. The same plot is also useful to check whether the fit stopped at a minimum with a poor fit. Of course, a reasonably good fit is not proof there is not a "better" fit (in either a statistical sense, characterized by an improved goodness-of-fit criterion, or a physical sense, with a solution more consistent with the model.) Depending on the problem, it may be desirable to `fit` with various sets of starting values, covering a reasonable range for each parameter.  File: gnuplot.info, Node: tips, Prev: starting values, Up: fit Here are some tips to keep in mind to get the most out of `fit` (*note fit:: ). They're not very organized, so you'll have to read them several times until their essence has sunk in. The two forms of the `via` argument to `fit` serve two largely distinct purposes. The `via "file"` form is best used for (possibly unattended) batch operation, where you just supply the startup values in a file and can later use `update` (*note update:: ) to copy the results back into another (or the same) parameter file. The `via var1, var2, ...` form is best used interactively, where the command history mechanism may be used to edit the list of parameters to be fitted or to supply new startup values for the next try. This is particularly useful for hard problems, where a direct fit to all parameters at once won't work without good starting values. To find such, you can iterate several times, fitting only some of the parameters, until the values are close enough to the goal that the final fit to all parameters at once will work. Make sure that there is no mutual dependency among parameters of the function you are fitting. For example, don't try to fit a*exp(x+b), because a*exp(x+b)=a*exp(b)*exp(x). Instead, fit either a*exp(x) or exp(x+b). A technical issue: the parameters must not be too different in magnitude. The larger the ratio of the largest and the smallest absolute parameter values, the slower the fit will converge. If the ratio is close to or above the inverse of the machine floating point precision, it may take next to forever to converge, or refuse to converge at all. You will have to adapt your function to avoid this, e.g., replace 'parameter' by '1e9*parameter' in the function definition, and divide the starting value by 1e9. If you can write your function as a linear combination of simple functions weighted by the parameters to be fitted, by all means do so. That helps a lot, because the problem is no longer nonlinear and should converge with only a small number of iterations, perhaps just one. Some prescriptions for analysing data, given in practical experimentation courses, may have you first fit some functions to your data, perhaps in a multi-step process of accounting for several aspects of the underlying theory one by one, and then extract the information you really wanted from the fitting parameters of those functions. With `fit`, this may often be done in one step by writing the model function directly in terms of the desired parameters. Transforming data can also quite often be avoided, though sometimes at the cost of a more difficult fit problem. If you think this contradicts the previous paragraph about simplifying the fit function, you are correct. A "singular matrix" message indicates that this implementation of the Marquardt-Levenberg algorithm can't calculate parameter values for the next iteration. Try different starting values, writing the function in another form, or a simpler function. Finally, a nice quote from the manual of another fitting package (fudgit), that kind of summarizes all these issues: "Nonlinear fitting is an art!"  File: gnuplot.info, Node: help, Prev: fit, Up: Commands, Next: if The `help` command displays on-line help. To specify information on a particular topic use the syntax: help {} If is not specified, a short message is printed about `gnuplot` (*note gnuplot:: ). After help for the requested topic is given, a menu of subtopics is given; help for a subtopic may be requested by typing its name, extending the help request. After that subtopic has been printed, the request may be extended again or you may go back one level to the previous topic. Eventually, the `gnuplot` command line will return. If a question mark (?) is given as the topic, the list of topics currently available is printed on the screen.  File: gnuplot.info, Node: if, Prev: help, Up: Commands, Next: load The `if` command allows commands to be executed conditionally. Syntax: if () will be evaluated. If it is true (non-zero), then the command(s) of the will be executed. If is false (zero), then the entire is ignored. Note that use of `;` to allow multiple commands on the same line will _not_ end the conditionalized commands. Examples: pi=3 if (pi!=acos(-1)) print "?Fixing pi!"; pi=acos(-1); print pi will display: ?Fixing pi! 3.14159265358979 but if (1==2) print "Never see this"; print "Or this either" will not display anything. See `reread` (*note reread:: ) for an example of how if and reread can be used together to perform a loop.  File: gnuplot.info, Node: load, Prev: if, Up: Commands, Next: pause The `load` command executes each line of the specified input file as if it had been typed in interactively. Files created by the `save` (*note save:: ) command can later be `load`ed. Any text file containing valid commands can be created and then executed by the `load` command. Files being `load`ed may themselves contain `load` or `call` (*note call:: ) commands. See comment for information about comments in commands. To `load` with arguments, see `call`. The `load` command _must_ be the last command on a multi-command line. Syntax: load "" The name of the input file must be enclosed in quotes. The special filename "-" may be used to `load` commands from standard input. This allows a `gnuplot` (*note gnuplot:: ) command file to accept some commands from standard input. Please see "help batch/interactive" for more details. Examples: load 'work.gnu' load "func.dat" The `load` command is performed implicitly on any file names given as arguments to `gnuplot`. These are loaded in the order specified, and then `gnuplot` exits.  File: gnuplot.info, Node: pause, Prev: load, Up: Commands, Next: plot The `pause` command displays any text associated with the command and then waits a specified amount of time or until the carriage return is pressed. `pause` is especially useful in conjunction with `load` (*note load:: ) files. Syntax: pause