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1011 -487 998 -479 ct +985 -471 969 -458 950 -440 ct 944 -435 919 -409 873 -363 ct p ef +1589 -525 m 1600 -350 l 1589 -350 l 1573 -403 1551 -440 1522 -463 ct 1493 -486 1458 -498 1417 -498 ct +1383 -498 1352 -489 1325 -472 ct 1297 -455 1275 -427 1260 -389 ct 1244 -351 1236 -304 1236 -248 ct +1236 -201 1243 -161 1258 -127 ct 1273 -93 1296 -67 1326 -48 ct 1355 -30 1390 -21 1428 -21 ct +1461 -21 1491 -28 1516 -43 ct 1542 -57 1570 -85 1600 -128 ct 1612 -120 l 1586 -74 1556 -41 1522 -20 ct +1488 1 1447 11 1400 11 ct 1314 11 1249 -19 1202 -82 ct 1167 -129 1150 -185 1150 -248 ct +1150 -300 1161 -347 1184 -390 ct 1207 -433 1239 -466 1279 -490 ct 1319 -513 1363 -525 1411 -525 ct +1448 -525 1485 -516 1521 -498 ct 1531 -492 1539 -489 1544 -489 ct 1550 -489 1556 -492 1561 -497 ct +1568 -503 1573 -513 1575 -525 ct p ef pom gr @@ -2239,5 +2227,5 @@ gs pum -137 348 t +143 347 t 22 -271 m 22 -294 l 143 -294 l 135 -325 l 213 -282 l 135 -240 l 143 -271 l p ef @@ -2246,5 +2234,5 @@ gs pum -137 424 t +129 435 t 66 -280 m 176 -280 l 205 -280 226 -273 241 -261 ct 255 -248 262 -233 262 -215 ct 262 -201 258 -187 249 -174 ct 240 -161 226 -150 208 -142 ct 190 -133 171 -129 150 -129 ct @@ -2260,5 +2248,5 @@ gs pum -421 537 t +424 524 t 36 -175 m 40 -175 43 -174 45 -172 ct 47 -169 49 -166 49 -163 ct 49 -159 47 -156 45 -154 ct 43 -151 40 -150 36 -150 ct 33 -150 30 -151 27 -154 ct 25 -156 24 -159 24 -163 ct @@ -2290,5 +2278,5 @@ gs pum -193 372 t +195 373 t 126 -181 m 122 -168 l 92 -168 l 69 -78 l 59 -38 49 -7 39 14 ct 24 44 9 66 -7 77 ct -19 86 -32 91 -45 91 ct -53 91 -60 88 -66 83 ct -70 80 -72 75 -72 70 ct -72 66 -70 62 -67 58 ct @@ -2307,5 +2295,5 @@ gs pum -421 467 t +417 477 t 63 -116 m 80 -116 94 -109 104 -96 ct 113 -85 117 -73 117 -58 ct 117 -48 115 -38 110 -27 ct 105 -17 98 -9 90 -4 ct 81 0 72 3 61 3 ct 44 3 31 -3 21 -16 ct 12 -28 8 -41 8 -55 ct @@ -2332,7 +2320,6 @@ gr gr -13905 16898 m 13805 17198 l 14005 17197 l 13905 16898 l p ef -13905 17894 m 14004 17593 l 13804 17594 l 13905 17894 l p ef -1 lw 0 lj 13905 17138 m 13905 17654 l ps +13305 16898 m 13205 17198 l 13405 17197 l 13305 16898 l p ef +1 lw 0 lj 13305 17138 m 13305 17894 l ps 0 lw 1 lj [ 53.09149 53.09149 ] 0 ld 13610 10615 m 13610 13174 l ps @@ -2619,4 +2606,56 @@ 0 lw 1 lj 8517 16675 m 8517 17599 l 10937 17599 l ps 8517 20288 m 8517 21199 l 10937 21199 l ps +gs +12121 17216 m 13266 17216 l 13266 17685 l 12121 17685 l 12121 17216 l eoclip newpath +gs +tm setmatrix +11486 16581 t +1 1 s +0 0 m 1145 0 l 1145 469 l 0 469 l 0 0 l eoclip newpath +gs +pum +136 372 t +136 -265 m 104 -154 l 131 -154 l 149 -154 163 -157 171 -162 ct 180 -168 187 -179 193 -194 ct +201 -194 l 172 -92 l 164 -92 l 166 -101 167 -108 167 -114 ct 167 -120 166 -125 164 -129 ct +161 -132 158 -135 154 -137 ct 150 -138 141 -139 127 -139 ct 101 -139 l 74 -46 l +71 -37 70 -31 70 -26 ct 70 -22 71 -19 75 -16 ct 77 -15 83 -14 92 -14 ct 117 -14 l +144 -14 166 -18 182 -28 ct 198 -37 212 -54 225 -77 ct 233 -77 l 206 0 l -9 0 l +-6 -7 l 3 -7 11 -8 14 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+%%BoundingBox: 10 389 784 496 +%%HiResBoundingBox: 10.233594 389.275781 783.362109 495.067969 +%................................... +%%Creator: ESP Ghostscript 815 (epswrite) +%%CreationDate: 2008/10/25 12:03:08 +%%DocumentData: Clean7Bit %%LanguageLevel: 2 %%EndComments %%BeginProlog -%%BeginResource: procset SDRes-Prolog 1.0 0 -/b4_inc_state save def -/dict_count countdictstack def -/op_count count 1 sub def -userdict begin -0 setgray 0 setlinecap 1 setlinewidth 0 setlinejoin 10 setmiterlimit[] 0 setdash newpath -/languagelevel where {pop languagelevel 1 ne {false setstrokeadjust false setoverprint} if} if -/bdef {bind def} bind def -/c {setgray} bdef -/l {neg lineto} bdef -/rl {neg rlineto} bdef -/lc {setlinecap} bdef -/lj {setlinejoin} bdef -/lw {setlinewidth} bdef -/ml {setmiterlimit} bdef -/ld {setdash} bdef -/m {neg moveto} bdef -/ct {6 2 roll neg 6 2 roll neg 6 2 roll neg curveto} bdef -/r {rotate} bdef -/t {neg translate} bdef -/s {scale} bdef -/sw {show} bdef -/gs {gsave} bdef -/gr {grestore} bdef -/f {findfont dup length dict begin -{1 index /FID ne {def} {pop pop} ifelse} forall /Encoding ISOLatin1Encoding def -currentdict end /NFont exch definefont pop /NFont findfont} bdef -/p {closepath} bdef -/sf {scalefont setfont} bdef -/ef {eofill}bdef -/pc {closepath stroke}bdef -/ps {stroke}bdef -/pum {matrix currentmatrix}bdef -/pom {setmatrix}bdef -/bs {/aString exch def /nXOfs exch def /nWidth exch def currentpoint nXOfs 0 rmoveto pum nWidth aString stringwidth pop div 1 scale aString show pom moveto} bdef +% This copyright applies to everything between here and the %%EndProlog: +% Copyright (C) 2004 artofcode LLC, Benicia, CA. All rights reserved. +%%BeginResource: procset GS_epswrite_2_0_1001 +/GS_epswrite_2_0_1001 80 dict dup begin +/PageSize 2 array def/setpagesize{ PageSize aload pop 3 index eq exch +4 index eq and{ pop pop pop}{ PageSize dup 1 +5 -1 roll put 0 4 -1 roll put dup null eq {false} {dup where} ifelse{ exch get exec} +{ pop/setpagedevice where +{ pop 1 dict dup /PageSize PageSize put setpagedevice} +{ /setpage where{ pop PageSize aload pop pageparams 3 {exch pop} repeat +setpage}if}ifelse}ifelse}ifelse} bind def +/!{bind def}bind def/#{load def}!/N/counttomark # +/rG{3{3 -1 roll 255 div}repeat setrgbcolor}!/G{255 div setgray}!/K{0 G}! +/r6{dup 3 -1 roll rG}!/r5{dup 3 1 roll rG}!/r3{dup rG}! +/w/setlinewidth #/J/setlinecap # +/j/setlinejoin #/M/setmiterlimit #/d/setdash #/i/setflat # +/m/moveto #/l/lineto #/c/rcurveto # +/p{N 2 idiv{N -2 roll rlineto}repeat}! +/P{N 0 gt{N -2 roll moveto p}if}! +/h{p closepath}!/H{P closepath}! +/lx{0 rlineto}!/ly{0 exch rlineto}!/v{0 0 6 2 roll c}!/y{2 copy c}! +/re{4 -2 roll m exch dup lx exch ly neg lx h}! +/^{3 index neg 3 index neg}! +/f{P fill}!/f*{P eofill}!/s{H stroke}!/S{P stroke}! +/q/gsave #/Q/grestore #/rf{re fill}! +/Y{P clip newpath}!/Y*{P eoclip newpath}!/rY{re Y}! +/|={pop exch 4 1 roll 1 array astore cvx 3 array astore cvx exch 1 index def exec}! +/|{exch string readstring |=}! +/+{dup type/nametype eq{2 index 7 add -3 bitshift 2 index mul}if}! +/@/currentfile #/${+ @ |}! +/B{{2 copy string{readstring pop}aload pop 4 array astore cvx +3 1 roll}repeat pop pop true}! +/Ix{[1 0 0 1 11 -2 roll exch neg exch neg]exch}! +/,{true exch Ix imagemask}!/If{false exch Ix imagemask}!/I{exch Ix image}! +/Ic{exch Ix false 3 colorimage}! +/F{/Columns counttomark 3 add -2 roll/Rows exch/K -1/BlackIs1 true>> +/CCITTFaxDecode filter}!/FX{<> +/CCITTFaxDecode filter}!/FX{< +, +289 4027 15 115 /5R +$X +s8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&ts8N&t 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showpage +%%PageTrailer +%%Trailer %%Pages: 1 -%%DocumentNeededResources: -%%DocumentSuppliedResources: procset Adobe_AGM_Image (1.0 0) -%%+ procset Adobe_CoolType_Utility_MAKEOCF (1.13 0) -%%+ procset Adobe_CoolType_Core (2.12 0) -%%+ procset Adobe_AGM_Core (2.0 0) -%%+ procset Adobe_AGM_Utils (1.0 0) -%%DocumentFonts: -%%DocumentNeededFonts: -%%DocumentNeededFeatures: -%%DocumentSuppliedFeatures: -%%DocumentProcessColors: Black -%%DocumentCustomColors: -%%CMYKCustomColor: -%%RGBCustomColor: -%%EndComments -%%BeginDefaults -%%ViewingOrientation: 1 0 0 1 -%%EndDefaults -%%BeginProlog -%ADOBeginClientInjection: DocumentProlog Start "AI10" -%ADOEndClientInjection: DocumentProlog Start "AI10" -%%BeginResource: procset Adobe_AGM_Utils 1.0 0 -%%Version: 1.0 0 -%%Copyright: Copyright (C) 2000-2000 Adobe Systems, Inc. All Rights Reserved. -systemdict /setpacking known -{ - currentpacking - true setpacking -} if -userdict /Adobe_AGM_Utils 60 dict dup begin put -/bdf -{ - bind def -} bind def -/nd{ - null def -}bdf -/xdf -{ - exch def -}bdf -/ldf -{ - load def -}bdf -/ddf -{ - put -}bdf -/xddf -{ - 3 -1 roll put -}bdf -/xpt -{ - exch put -}bdf -/ndf -{ - - exch dup where{ - pop pop pop - }{ - xdf - }ifelse -}def -/cdndf -{ - exch dup currentdict exch known{ - pop pop - }{ - exch def - }ifelse -}def -/bdict -{ - mark -}bdf -/edict -{ - counttomark 2 idiv dup dict begin {def} repeat pop currentdict end -}def - -/ps_level - /languagelevel where{ - pop systemdict /languagelevel get exec - }{ - 1 - }ifelse -def -/level2 - ps_level 2 ge -def -/level3 - ps_level 3 ge -def -/ps_version - {version cvr} stopped { - -1 - }if -def -/makereadonlyarray -{ - /packedarray where{ - pop packedarray - }{ - array astore readonly - }ifelse -}bdf -/map_reserved_ink_name -{ - dup type /stringtype eq{ - dup /Red eq{ - pop (_Red_) - }{ - dup /Green eq{ - pop (_Green_) - }{ - dup /Blue eq{ - pop (_Blue_) - }{ - dup /Cyan eq{ - pop (_Cyan_) - }{ - dup /Magenta eq{ - pop (_Magenta_) - }{ - dup /Yellow eq{ - pop (_Yellow_) - }{ - dup /Black eq{ - pop (_Black_) - }{ - dup () cvn eq{ - pop (Process) - }if - }ifelse - }ifelse - }ifelse - }ifelse - }ifelse - }ifelse - }ifelse - }if -}bdf -/AGMUTIL_GSTATE 22 dict def -/get_gstate -{ - AGMUTIL_GSTATE begin - /AGMUTIL_GSTATE_clr_spc currentcolorspace def - /AGMUTIL_GSTATE_clr_indx 0 def - /AGMUTIL_GSTATE_clr_comps 12 array def - mark currentcolor counttomark - {AGMUTIL_GSTATE_clr_comps AGMUTIL_GSTATE_clr_indx 3 -1 roll put - /AGMUTIL_GSTATE_clr_indx AGMUTIL_GSTATE_clr_indx 1 add def} repeat pop - /AGMUTIL_GSTATE_fnt rootfont def - /AGMUTIL_GSTATE_lw currentlinewidth def - /AGMUTIL_GSTATE_lc currentlinecap def - /AGMUTIL_GSTATE_lj currentlinejoin def - /AGMUTIL_GSTATE_ml currentmiterlimit def - currentdash /AGMUTIL_GSTATE_do xdf /AGMUTIL_GSTATE_da xdf - /AGMUTIL_GSTATE_sa currentstrokeadjust def - - /AGMUTIL_GSTATE_clr_rnd currentcolorrendering def - /AGMUTIL_GSTATE_op currentoverprint def - /AGMUTIL_GSTATE_bg currentblackgeneration cvlit def - /AGMUTIL_GSTATE_ucr currentundercolorremoval cvlit def - currentcolortransfer cvlit /AGMUTIL_GSTATE_gy_xfer xdf cvlit /AGMUTIL_GSTATE_b_xfer xdf - cvlit /AGMUTIL_GSTATE_g_xfer xdf cvlit /AGMUTIL_GSTATE_r_xfer xdf - /AGMUTIL_GSTATE_ht currenthalftone def - /AGMUTIL_GSTATE_flt currentflat def - end -}def -/set_gstate -{ - AGMUTIL_GSTATE begin - AGMUTIL_GSTATE_clr_spc setcolorspace - AGMUTIL_GSTATE_clr_indx {AGMUTIL_GSTATE_clr_comps AGMUTIL_GSTATE_clr_indx 1 sub get - /AGMUTIL_GSTATE_clr_indx AGMUTIL_GSTATE_clr_indx 1 sub def} repeat setcolor - AGMUTIL_GSTATE_fnt setfont - AGMUTIL_GSTATE_lw setlinewidth - AGMUTIL_GSTATE_lc setlinecap - AGMUTIL_GSTATE_lj setlinejoin - AGMUTIL_GSTATE_ml setmiterlimit - AGMUTIL_GSTATE_da AGMUTIL_GSTATE_do setdash - AGMUTIL_GSTATE_sa setstrokeadjust - - AGMUTIL_GSTATE_clr_rnd setcolorrendering - AGMUTIL_GSTATE_op setoverprint - AGMUTIL_GSTATE_bg cvx setblackgeneration - AGMUTIL_GSTATE_ucr cvx setundercolorremoval - AGMUTIL_GSTATE_r_xfer cvx AGMUTIL_GSTATE_g_xfer cvx AGMUTIL_GSTATE_b_xfer cvx - AGMUTIL_GSTATE_gy_xfer cvx setcolortransfer - - AGMUTIL_GSTATE_ht /HalftoneType get dup 9 eq exch 100 eq or - { - currenthalftone /HalftoneType get AGMUTIL_GSTATE_ht /HalftoneType get ne - { - mark AGMUTIL_GSTATE_ht {sethalftone} stopped cleartomark - } if - }{ - AGMUTIL_GSTATE_ht sethalftone - } ifelse - - AGMUTIL_GSTATE_flt setflat - end -}def -/AGMUTIL_str256 256 string def -/AGMUTIL_src256 256 string def -/AGMUTIL_dst64 64 string def -/AGMUTIL_srcLen nd -/AGMUTIL_ndx nd -/rdline -{ - currentfile AGMUTIL_str256 readline pop -} bdf -/rdcmntline -{ - currentfile AGMUTIL_str256 readline pop - (%) anchorsearch {pop} if -} bdf -/filter_cmyk -{ - dup type /filetype ne{ - 0 () /SubFileDecode filter - }if - [ - exch - { - AGMUTIL_src256 readstring pop - dup length /AGMUTIL_srcLen exch def - /AGMUTIL_ndx 0 def - - AGMCORE_plate_ndx 4 AGMUTIL_srcLen 1 sub{ - 1 index exch get - AGMUTIL_dst64 AGMUTIL_ndx 3 -1 roll put - /AGMUTIL_ndx AGMUTIL_ndx 1 add def - }for - pop - AGMUTIL_dst64 0 AGMUTIL_ndx getinterval - } - bind - /exec cvx - ] cvx -} bdf -/AGMUTIL_imagefile nd -/AGMUTIL_imbuf nd -/read_image_file -{ - AGMUTIL_imagefile 0 setfileposition - dup /DataSource {AGMUTIL_imagefile AGMUTIL_imbuf readstring pop} put - exch - load exec -}def -/write_image_file -{ - begin - { (AGMUTIL_imagefile) (w+) file } stopped{ - false - }{ - Adobe_AGM_Utils/AGMUTIL_imagefile xddf - Adobe_AGM_Utils/AGMUTIL_imbuf Width BitsPerComponent mul 7 add 8 idiv string ddf - 1 1 Height { - pop - DataSource dup type /filetype eq{ - AGMUTIL_imbuf readstring pop - }{ - exec - } ifelse - AGMUTIL_imagefile exch writestring - }for - true - }ifelse - end -}def -/close_image_file -{ - AGMUTIL_imagefile closefile (AGMUTIL_imagefile) deletefile -}def -/consumeimagedata -{ - begin - currentdict /MultipleDataSources known not - {/MultipleDataSources false def} if - MultipleDataSources - { - 1 dict begin - /flushbuffer Width cvi string def - 1 1 Height cvi - { - pop - 0 1 DataSource length 1 sub - { - DataSource exch get - dup type dup - /filetype eq - { - exch flushbuffer readstring pop pop - }if - /arraytype eq - { - exec pop - }if - }for - }for - end - } - { - /DataSource load type dup - /filetype eq - { - 1 dict begin - /flushbuffer Width Decode length 2 div mul cvi string def - 1 1 Height { pop DataSource flushbuffer readstring pop pop} for - end - }if - /arraytype eq - { - 1 1 Height { pop DataSource pop } for - }if - }ifelse - end -}bdf -/addprocs -{ - 2{/exec load}repeat - 3 1 roll - [ 5 1 roll ] bind cvx -}def -/modify_halftone_xfer -{ - currenthalftone dup length dict copy begin - currentdict 2 index known{ - 1 index load dup length dict copy begin - currentdict/TransferFunction known{ - /TransferFunction load - }{ - currenttransfer - }ifelse - addprocs /TransferFunction xdf - currentdict end def - currentdict end sethalftone - }{ - currentdict/TransferFunction known{ - /TransferFunction load - }{ - currenttransfer - }ifelse - addprocs /TransferFunction xdf - currentdict end sethalftone - pop - }ifelse -}def -/doc_setup{ - Adobe_AGM_Utils begin -}bdf -/doc_trailer{ - currentdict Adobe_AGM_Utils eq{ - end - }if -}bdf -systemdict /setpacking known -{ - setpacking -} if -%%EndResource -%%BeginResource: procset Adobe_AGM_Core 2.0 0 -%%Version: 2.0 0 -%%Copyright: Copyright (C) 1997-1999 Adobe Systems, Inc. All Rights Reserved. -systemdict /setpacking known -{ - currentpacking - true setpacking -} if -userdict /Adobe_AGM_Core 205 dict dup begin put -/nd{ - null def -}bind def -/Adobe_AGM_Core_Id /Adobe_AGM_Core_2.0_0 def -/AGMCORE_str256 256 string def -/AGMCORE_src256 256 string def -/AGMCORE_save nd -/AGMCORE_graphicsave nd -/AGMCORE_c 0 def -/AGMCORE_m 0 def -/AGMCORE_y 0 def -/AGMCORE_k 0 def -/AGMCORE_cmykbuf 4 array def -/AGMCORE_screen [currentscreen] cvx def -/AGMCORE_tmp 0 def -/AGMCORE_&setgray nd -/AGMCORE_&setcolor nd -/AGMCORE_&setcolorspace nd -/AGMCORE_&setcmykcolor nd -/AGMCORE_cyan_plate nd -/AGMCORE_magenta_plate nd -/AGMCORE_yellow_plate nd -/AGMCORE_black_plate nd -/AGMCORE_plate_ndx nd -/AGMCORE_get_ink_data nd -/AGMCORE_is_cmyk_sep nd -/AGMCORE_host_sep nd -/AGMCORE_will_host_sep nd -/AGMCORE_avoid_L2_sep_space nd -/AGMCORE_distilling nd -/AGMCORE_composite_job nd -/AGMCORE_producing_seps nd -/AGMCORE_ps_level -1 def -/AGMCORE_ps_version -1 def -/AGMCORE_environ_ok nd -/AGMCORE_CSA_cache 0 dict def -/AGMCORE_CSD_cache 0 dict def -/AGMCORE_pattern_cache 0 dict def -/AGMCORE_currentoverprint false def -/AGMCORE_deltaX nd -/AGMCORE_deltaY nd -/AGMCORE_name nd -/AGMCORE_sep_special nd -/AGMCORE_err_strings 4 dict def -/AGMCORE_cur_err nd -/AGMCORE_ovp nd -/AGMCORE_current_spot_alias false def -/AGMCORE_inverting false def -/AGMCORE_feature_dictCount nd -/AGMCORE_feature_opCount nd -/AGMCORE_feature_ctm nd -/AGMCORE_ConvertToProcess false def -/AGMCORE_Default_CTM matrix def -/knockout_unitsq nd -/AGMCORE_CRD_cache where{ - pop -}{ - /AGMCORE_CRD_cache 0 dict def -}ifelse -/AGMCORE_key_known -{ - where{ - /Adobe_AGM_Core_Id known - }{ - false - }ifelse -}ndf -/flushinput -{ - save - /CompareBuffer 3 -1 roll def - /readbuffer 256 string def - mark - { - currentfile readbuffer {readline} stopped - {cleartomark mark} - { - not - {pop exit} - if - CompareBuffer eq - {exit} - if - }ifelse - }loop - cleartomark - restore -}bdf -/getspotfunction -{ - AGMCORE_screen exch pop exch pop - dup type /dicttype eq{ - dup /HalftoneType get 1 eq{ - /SpotFunction get - }{ - dup /HalftoneType get 2 eq{ - /GraySpotFunction get - }{ - pop - { - abs exch abs 2 copy add 1 gt{ - 1 sub dup mul exch 1 sub dup mul add 1 sub - }{ - dup mul exch dup mul add 1 exch sub - }ifelse - }bind - }ifelse - }ifelse - }if -} def -/clp_npth -{ - clip newpath -} def -/eoclp_npth -{ - eoclip newpath -} def -/stkpath_clp_npth -{ - strokepath clip newpath -} def -/stk_n_clp_npth -{ - gsave stroke grestore clip newpath -} def -/npth_clp -{ - newpath clip -} def -/graphic_setup -{ - /AGMCORE_graphicsave save def - concat - 0 setgray - 0 setlinecap - 0 setlinejoin - 1 setlinewidth - [] 0 setdash - 10 setmiterlimit - newpath - false setoverprint - false setstrokeadjust - Adobe_AGM_Core/spot_alias get exec - /Adobe_AGM_Image where { - pop - Adobe_AGM_Image/spot_alias 2 copy known{ - get exec - }{ - pop pop - }ifelse - } if - 100 dict begin - /showpage {} def - mark -} def -/graphic_cleanup -{ - cleartomark - end - AGMCORE_graphicsave restore -} def -/compose_error_msg -{ - grestoreall initgraphics - /Helvetica findfont 10 scalefont setfont - - /AGMCORE_deltaY 100 def - /AGMCORE_deltaX 310 def - - clippath pathbbox newpath pop pop 36 add exch 36 add exch moveto - 0 AGMCORE_deltaY rlineto AGMCORE_deltaX 0 rlineto - 0 AGMCORE_deltaY neg rlineto AGMCORE_deltaX neg 0 rlineto closepath - 0 AGMCORE_&setgray - gsave 1 AGMCORE_&setgray fill grestore - 1 setlinewidth gsave stroke grestore - - currentpoint AGMCORE_deltaY 15 sub add exch 8 add exch moveto - - /AGMCORE_deltaY 12 def - /AGMCORE_tmp 0 def - AGMCORE_err_strings exch get - { - dup 32 eq - { - pop - AGMCORE_str256 0 AGMCORE_tmp getinterval - stringwidth pop currentpoint pop add AGMCORE_deltaX 28 add gt - { - currentpoint AGMCORE_deltaY sub exch pop - clippath pathbbox pop pop pop 44 add exch moveto - } if - AGMCORE_str256 0 AGMCORE_tmp getinterval show ( ) show - - 0 1 AGMCORE_str256 length 1 sub - { - AGMCORE_str256 exch 0 put - }for - /AGMCORE_tmp 0 def - } - { - AGMCORE_str256 exch AGMCORE_tmp exch put - /AGMCORE_tmp AGMCORE_tmp 1 add def - } ifelse - } forall -} bdf -/doc_setup{ - Adobe_AGM_Core begin - - /AGMCORE_will_host_separate xdf - /AGMCORE_ps_version xdf - /AGMCORE_ps_level xdf - - errordict /AGM_handleerror known not{ - errordict /AGM_handleerror errordict /handleerror get put - errordict /handleerror { - Adobe_AGM_Core begin - $error /newerror get AGMCORE_cur_err null ne and{ - $error /newerror false put - AGMCORE_cur_err compose_error_msg - }if - $error /newerror true put - end - errordict /AGM_handleerror get exec - } bind put - }if - - /AGMCORE_environ_ok - ps_level AGMCORE_ps_level ge - ps_version AGMCORE_ps_version ge and - AGMCORE_ps_level -1 eq or - def - - AGMCORE_environ_ok not - {/AGMCORE_cur_err /AGMCORE_bad_environ def} if - - /AGMCORE_&setgray systemdict/setgray get def - level2{ - /AGMCORE_&setcolor systemdict/setcolor get def - /AGMCORE_&setcolorspace systemdict/setcolorspace get def - }if - /AGMCORE_distilling - /product where{ - pop systemdict/setdistillerparams known product (Adobe PostScript Parser) ne and - }{ - false - }ifelse - def - /AGMCORE_in_rip_sep - /AGMCORE_in_rip_sep where{ - pop AGMCORE_in_rip_sep - }{ - AGMCORE_distilling - { - false - }{ - userdict/Adobe_AGM_OnHost_Seps known{ - false - }{ - level2{ - currentpagedevice/Separations 2 copy known{ - get - }{ - pop pop false - }ifelse - }{ - false - }ifelse - }ifelse - }ifelse - }ifelse - def - level2 not{ - /xput{ - dup load dup length exch maxlength eq{ - dup dup load dup - length dup 0 eq {pop 1} if 2 mul dict copy def - }if - load begin - def - end - }def - }{ - /xput{ - load 3 1 roll put - }def - }ifelse - /AGMCORE_GSTATE AGMCORE_key_known not{ - /AGMCORE_GSTATE 21 dict def - /AGMCORE_gstack 32 array def - /AGMCORE_gstackptr 0 def - /AGMCORE_gstacksaveptr 0 def - /AGMCORE_gstackframekeys 8 def - - /AGMCORE_&gsave /gsave ldf - /AGMCORE_&grestore /grestore ldf - /AGMCORE_&grestoreall /grestoreall ldf - /AGMCORE_&save /save ldf - /AGMCORE_gdictcopy { - begin - { def } forall - end - }def - /AGMCORE_gput { - AGMCORE_gstack AGMCORE_gstackptr get - 3 1 roll - put - }def - /AGMCORE_gget { - AGMCORE_gstack AGMCORE_gstackptr get - exch - get - }def - /gsave { - AGMCORE_&gsave - AGMCORE_gstack AGMCORE_gstackptr get - AGMCORE_gstackptr 1 add - dup 32 ge {limitcheck} if - Adobe_AGM_Core exch - /AGMCORE_gstackptr exch put - AGMCORE_gstack AGMCORE_gstackptr get - AGMCORE_gdictcopy - }def - /grestore { - AGMCORE_&grestore - AGMCORE_gstackptr 1 sub - dup AGMCORE_gstacksaveptr lt {1 add} if - Adobe_AGM_Core exch - /AGMCORE_gstackptr exch put - }def - /grestoreall { - AGMCORE_&grestoreall - Adobe_AGM_Core - /AGMCORE_gstackptr AGMCORE_gstacksaveptr put - }def - /save { - AGMCORE_&save - AGMCORE_gstack AGMCORE_gstackptr get - AGMCORE_gstackptr 1 add - dup 32 ge {limitcheck} if - Adobe_AGM_Core begin - /AGMCORE_gstackptr exch def - /AGMCORE_gstacksaveptr AGMCORE_gstackptr def - end - AGMCORE_gstack AGMCORE_gstackptr get - AGMCORE_gdictcopy - }def - 0 1 AGMCORE_gstack length 1 sub { - AGMCORE_gstack exch AGMCORE_gstackframekeys dict put - } for - }if - /currentcmykcolor [0 0 0 0] AGMCORE_gput - /currentstrokeadjust false AGMCORE_gput - /currentcolorspace [/DeviceGray] AGMCORE_gput - /sep_tint 0 AGMCORE_gput - /sep_colorspace_dict null AGMCORE_gput - /indexed_colorspace_dict null AGMCORE_gput - /currentcolor_intent () AGMCORE_gput - /customcolor_tint 1 AGMCORE_gput - end -}def -/page_setup -{ - /setcmykcolor where{ - pop - Adobe_AGM_Core/AGMCORE_&setcmykcolor /setcmykcolor load put - }if - Adobe_AGM_Core begin - /setcmykcolor - { - 4 copy AGMCORE_cmykbuf astore /currentcmykcolor exch AGMCORE_gput - 1 sub 4 1 roll - 3 { - 3 index add neg dup 0 lt { - pop 0 - } if - 3 1 roll - } repeat - setrgbcolor pop - }ndf - /currentcmykcolor - { - /currentcmykcolor AGMCORE_gget aload pop - }ndf - /setoverprint - { - pop - }ndf - /currentoverprint - { - false - }ndf - /AGMCORE_deviceDPI 72 0 matrix defaultmatrix dtransform dup mul exch dup mul add sqrt def - /AGMCORE_cyan_plate 1 0 0 0 test_cmyk_color_plate def - /AGMCORE_magenta_plate 0 1 0 0 test_cmyk_color_plate def - /AGMCORE_yellow_plate 0 0 1 0 test_cmyk_color_plate def - /AGMCORE_black_plate 0 0 0 1 test_cmyk_color_plate def - /AGMCORE_plate_ndx - AGMCORE_cyan_plate{ - 0 - }{ - AGMCORE_magenta_plate{ - 1 - }{ - AGMCORE_yellow_plate{ - 2 - }{ - AGMCORE_black_plate{ - 3 - }{ - 4 - }ifelse - }ifelse - }ifelse - }ifelse - def - /AGMCORE_composite_job - AGMCORE_cyan_plate AGMCORE_magenta_plate and AGMCORE_yellow_plate and AGMCORE_black_plate and def - - /AGMCORE_producing_seps AGMCORE_composite_job not AGMCORE_in_rip_sep or def - - /AGMCORE_host_sep AGMCORE_producing_seps AGMCORE_in_rip_sep not and def - - /AGM_preserve_spots - /AGM_preserve_spots where{ - pop AGM_preserve_spots - }{ - AGMCORE_distilling AGMCORE_producing_seps or - }ifelse - def - /AGM_is_distiller_preserving_spotimages - { - currentdistillerparams/PreserveOverprintSettings known - { - currentdistillerparams/PreserveOverprintSettings get - { - currentdistillerparams/ColorConversionStrategy known - { - currentdistillerparams/ColorConversionStrategy get - /LeaveColorUnchanged eq - }{ - true - }ifelse - }{ - false - }ifelse - }{ - false - }ifelse - }def - /convert_spot_to_process where {pop}{ - /convert_spot_to_process - { - dup dup (None) eq exch (All) eq or - { - pop false - }{ - AGMCORE_host_sep - { - gsave - 1 0 0 0 setcmykcolor currentgray 1 exch sub - 0 1 0 0 setcmykcolor currentgray 1 exch sub - 0 0 1 0 setcmykcolor currentgray 1 exch sub - 0 0 0 1 setcmykcolor currentgray 1 exch sub - add add add 0 eq - { - pop false - }{ - false setoverprint - 1 1 1 1 5 -1 roll findcmykcustomcolor 1 setcustomcolor - currentgray 0 eq - }ifelse - grestore - }{ - AGMCORE_distilling - { - pop AGM_is_distiller_preserving_spotimages not - }{ - Adobe_AGM_Core/AGMCORE_name xddf - false - currentpagedevice/OverrideSeparations known - { - currentpagedevice/OverrideSeparations get - { - /HqnSpots /ProcSet resourcestatus - { - pop pop pop true - }if - }if - }if - { - AGMCORE_name /HqnSpots /ProcSet findresource /TestSpot get exec not - }{ - gsave - [/Separation AGMCORE_name /DeviceGray {}]setcolorspace - false - currentpagedevice/SeparationColorNames 2 copy known - { - get - { AGMCORE_name eq or}forall - not - }{ - pop pop pop true - }ifelse - grestore - }ifelse - }ifelse - }ifelse - }ifelse - }def - }ifelse - /convert_to_process where {pop}{ - /convert_to_process - { - dup length 0 eq - { - pop false - }{ - AGMCORE_host_sep - { - true exch - { - convert_spot_to_process and - } - forall - }{ - false exch - { - convert_spot_to_process or - } - forall - }ifelse - }ifelse - }def - }ifelse - AGMCORE_host_sep AGMCORE_will_host_separate not and { - /AGMCORE_cur_err /AGMCORE_color_space_onhost_seps def - AGMCORE_color_space_onhost_seps - }if - /AGMCORE_avoid_L2_sep_space - version cvr 2012 lt - level2 and - AGMCORE_producing_seps not and - def - /AGMCORE_is_cmyk_sep - AGMCORE_cyan_plate AGMCORE_magenta_plate or AGMCORE_yellow_plate or AGMCORE_black_plate or - def - /AGM_avoid_0_cmyk where{ - pop AGM_avoid_0_cmyk - }{ - AGM_preserve_spots - userdict/Adobe_AGM_OnHost_Seps known - userdict/Adobe_AGM_InRip_Seps known or - not and - }ifelse - { - /setcmykcolor[ - { - 4 copy add add add 0 eq currentoverprint and{ - pop 0.0005 - }if - }/exec cvx - /AGMCORE_&setcmykcolor load dup type/operatortype ne{ - /exec cvx - }if - ]cvx def - }if - AGMCORE_host_sep{ - /AGMCORE_get_ink_data - AGMCORE_cyan_plate{ - {pop pop pop} - }{ - AGMCORE_magenta_plate{ - {4 3 roll pop pop pop} - }{ - AGMCORE_yellow_plate{ - {4 2 roll pop pop pop} - }{ - {4 1 roll pop pop pop} - }ifelse - }ifelse - }ifelse - def - /clip AGMCORE_key_known not{ - Adobe_AGM_Core/AGMCORE_&clip /clip load put - /clip - { - current_spot_alias{ - currentdict/InksUsed known{ - [ - InksUsed{ - dup map_alias{ - /Name get exch pop - }if - }forall - ] - /InksUsed xdf - }if - }if - AGMCORE_&clip - }def - }if - /eoclip AGMCORE_key_known not{ - Adobe_AGM_Core/AGMCORE_&eoclip /eoclip load put - /eoclip - { - current_spot_alias{ - currentdict/InksUsed known{ - [ - InksUsed{ - dup map_alias{ - /Name get exch pop - }if - }forall - ] - /InksUsed xdf - }if - }if - AGMCORE_&eoclip - }def - }if - }if - AGMCORE_in_rip_sep{ - /setcustomcolor - { - exch aload pop - dup 7 1 roll inRip_spot_has_ink not { - 4 {4 index mul 4 1 roll} - repeat - /DeviceCMYK setcolorspace - 6 -2 roll pop pop - }{ - Adobe_AGM_Core begin - /AGMCORE_k xdf /AGMCORE_y xdf /AGMCORE_m xdf /AGMCORE_c xdf - end - [/Separation 4 -1 roll /DeviceCMYK - {dup AGMCORE_c mul exch dup AGMCORE_m mul exch dup AGMCORE_y mul exch AGMCORE_k mul} - ] - setcolorspace - }ifelse - setcolor - }ndf - /setseparationgray - { - [/Separation (All) /DeviceGray {}] setcolorspace_opt - 1 exch sub setcolor - }ndf - }{ - /setseparationgray - { - AGMCORE_&setgray - }ndf - }ifelse - /findcmykcustomcolor - { - 5 makereadonlyarray - }ndf - /setcustomcolor - { - exch aload pop pop - 4 {4 index mul 4 1 roll} repeat - setcmykcolor pop - }ndf - - /has_color - /colorimage where{ - AGMCORE_producing_seps{ - pop true - }{ - systemdict eq - }ifelse - }{ - false - }ifelse - def - - /map_index - { - 1 index mul exch getinterval {255 div} forall - }def - - level2{ - /mo /moveto ldf - /li /lineto ldf - /cv /curveto ldf - /knockout_unitsq - { - 1 setgray - 0 0 1 1 rectfill - }def - /level2ScreenFreq{ - begin - 60 - HalftoneType 1 eq{ - pop Frequency - }if - HalftoneType 2 eq{ - pop GrayFrequency - }if - HalftoneType 5 eq{ - pop Default level2ScreenFreq - }if - end - }def - /currentScreenFreq{ - currenthalftone level2ScreenFreq - }def - level2 /setcolorspace AGMCORE_key_known not and{ - - /AGMCORE_&&&setcolorspace /setcolorspace ldf - /AGMCORE_ReplaceMappedColor - { - dup type dup /arraytype eq exch /packedarraytype eq or - { - dup 0 get dup /Separation eq - { - pop - dup length array copy - dup dup 1 get - current_spot_alias - { - dup map_alias - { - begin - /sep_colorspace_dict currentdict AGMCORE_gput - pop pop pop - - [ - /Separation Name - CSA map_csa - dup /MappedCSA xdf - /sep_colorspace_proc load - ] - dup Name - end - }if - }if - map_reserved_ink_name 1 exch put - }{ - /DeviceN eq - { - dup length array copy - dup dup 1 get [ - exch { - current_spot_alias{ - dup map_alias{ - /Name get exch pop - }if - }if - map_reserved_ink_name - } forall - ] 1 exch put - }if - }ifelse - }if - }def - /setcolorspace - { - dup type dup /arraytype eq exch /packedarraytype eq or - { - dup 0 get /Indexed eq - { - AGMCORE_distilling - { - /PhotoshopDuotoneList where - { - pop false - }{ - true - }ifelse - }{ - true - }ifelse - { - aload pop 3 -1 roll - AGMCORE_ReplaceMappedColor - 3 1 roll 4 array astore - }if - }{ - AGMCORE_ReplaceMappedColor - }ifelse - }if - AGMCORE_&&&setcolorspace - }def - }if - }{ - - /adj - { - currentstrokeadjust{ - transform - 0.25 sub round 0.25 add exch - 0.25 sub round 0.25 add exch - itransform - }if - }def - /mo{ - adj moveto - }def - /li{ - adj lineto - }def - /cv{ - 6 2 roll adj - 6 2 roll adj - 6 2 roll adj curveto - }def - /knockout_unitsq - { - 1 setgray - 8 8 1 [8 0 0 8 0 0] {} image - }def - /currentstrokeadjust{ - /currentstrokeadjust AGMCORE_gget - }def - /setstrokeadjust{ - /currentstrokeadjust exch AGMCORE_gput - }def - /currentScreenFreq{ - currentscreen pop pop - }def - /setcolorspace - { - /currentcolorspace exch AGMCORE_gput - } def - - /currentcolorspace - { - /currentcolorspace AGMCORE_gget - } def - - /n_color_components - { - dup type /arraytype eq{ - 0 get - }if - dup /DeviceGray eq{ - pop 1 - }{ - /DeviceCMYK eq{ - 4 - }{ - 3 - }ifelse - }ifelse - } def - - /setcolor_devicecolor - { - dup type /arraytype eq{ - 0 get - }if - dup /DeviceGray eq{ - pop setgray - }{ - /DeviceCMYK eq{ - setcmykcolor - }{ - setrgbcolor - }ifelse - }ifelse - }def - - /setcolor - { - currentcolorspace 0 get - dup /DeviceGray ne{ - dup /DeviceCMYK ne{ - dup /DeviceRGB ne{ - dup /Separation eq{ - pop - currentcolorspace 3 get exec - currentcolorspace 2 get - }{ - dup /Indexed eq{ - pop - currentcolorspace 3 get dup type /stringtype eq{ - currentcolorspace 1 get n_color_components - 3 -1 roll map_index - }{ - exec - }ifelse - currentcolorspace 1 get - }{ - /AGMCORE_cur_err /AGMCORE_invalid_color_space def - AGMCORE_invalid_color_space - }ifelse - }ifelse - }if - }if - }if - setcolor_devicecolor - } def - }ifelse - - /sop /setoverprint ldf - /lw /setlinewidth ldf - /lc /setlinecap ldf - /lj /setlinejoin ldf - /ml /setmiterlimit ldf - /dsh /setdash ldf - /sadj /setstrokeadjust ldf - /gry /setgray ldf - /rgb /setrgbcolor ldf - /cmyk /setcmykcolor ldf - /sep /setsepcolor ldf - /idx /setindexedcolor ldf - /colr /setcolor ldf - /csacrd /set_csa_crd ldf - /sepcs /setsepcolorspace ldf - /idxcs /setindexedcolorspace ldf - /cp /closepath ldf - /clp /clp_npth ldf - /eclp /eoclp_npth ldf - /spclp /stkpath_clp_npth ldf - /f /fill ldf - /ef /eofill ldf - /s /stroke ldf - /sclp /stk_n_clp_npth ldf - /nclp /npth_clp ldf - /gset /graphic_setup ldf - /gcln /graphic_cleanup ldf - - currentdict{ - dup xcheck 1 index type dup /arraytype eq exch /packedarraytype eq or and { - bind - }if - def - }forall -}def -/page_trailer -{ - end -}def -/doc_trailer{ -}def -systemdict /findcolorrendering known{ - /findcolorrendering systemdict /findcolorrendering get def -}if -systemdict /setcolorrendering known{ - /setcolorrendering systemdict /setcolorrendering get def -}if -/test_cmyk_color_plate -{ - gsave - setcmykcolor currentgray 1 ne - grestore -}def -/inRip_spot_has_ink -{ - dup Adobe_AGM_Core/AGMCORE_name xddf - convert_spot_to_process not -}def -/current_ink -{ - dup length 0 eq{ - pop true - }{ - Adobe_AGM_Core/ink_result false put - { - dup /ProcessCyan eq{ - AGMCORE_cyan_plate ink_result or Adobe_AGM_Core/ink_result xddf - }{ - dup /ProcessMagenta eq{ - AGMCORE_magenta_plate ink_result or Adobe_AGM_Core/ink_result xddf - }{ - dup /ProcessYellow eq{ - AGMCORE_yellow_plate ink_result or Adobe_AGM_Core/ink_result xddf - }{ - dup /ProcessBlack eq{ - AGMCORE_black_plate ink_result or Adobe_AGM_Core/ink_result xddf - }{ - dup /sep_colorspace_dict AGMCORE_gget dup null eq{ - pop false ink_result or Adobe_AGM_Core/ink_result xddf - }{ - /Name get eq{ - 1 setsepcolor - currentgray 1 ne ink_result or Adobe_AGM_Core/ink_result xddf - }{ - false ink_result or Adobe_AGM_Core/ink_result xddf - }ifelse - }ifelse - }ifelse - }ifelse - }ifelse - }ifelse - pop - } forall - ink_result - }ifelse -}def -/map255_to_range -{ - 1 index sub - 3 -1 roll 255 div mul add -}def -/set_csa_crd -{ - /sep_colorspace_dict null AGMCORE_gput - begin - CSA map_csa setcolorspace_opt - set_crd - end -} -def -/setsepcolor -{ - - /sep_colorspace_dict AGMCORE_gget begin - dup /sep_tint exch AGMCORE_gput - TintProc - end -} def -/sep_colorspace_proc -{ - Adobe_AGM_Core/AGMCORE_tmp xddf - /sep_colorspace_dict AGMCORE_gget begin - currentdict/Components known{ - Components aload pop - TintMethod/Lab eq{ - 2 {AGMCORE_tmp mul NComponents 1 roll} repeat - LMax sub AGMCORE_tmp mul LMax add NComponents 1 roll - }{ - TintMethod/Subtractive eq{ - NComponents{ - AGMCORE_tmp mul NComponents 1 roll - }repeat - }{ - NComponents{ - 1 sub AGMCORE_tmp mul 1 add NComponents 1 roll - } repeat - }ifelse - }ifelse - }{ - ColorLookup AGMCORE_tmp ColorLookup length 1 sub mul round cvi get - aload pop - }ifelse - end -} def -/sep_colorspace_gray_proc -{ - Adobe_AGM_Core/AGMCORE_tmp xddf - /sep_colorspace_dict AGMCORE_gget begin - GrayLookup AGMCORE_tmp GrayLookup length 1 sub mul round cvi get - end -} def -/sep_proc_name -{ - dup 0 get - dup /DeviceRGB eq exch /DeviceCMYK eq or level2 not and has_color not and{ - pop [/DeviceGray] - /sep_colorspace_gray_proc - }{ - /sep_colorspace_proc - }ifelse -} def -/setsepcolorspace -{ - - current_spot_alias{ - dup begin - Name map_alias{ - exch pop - }if - end - }if - dup /sep_colorspace_dict exch AGMCORE_gput - begin - /MappedCSA CSA map_csa def - Adobe_AGM_Core/AGMCORE_sep_special Name dup () eq exch (All) eq or ddf - - AGMCORE_avoid_L2_sep_space{ - [/Indexed MappedCSA sep_proc_name 255 exch - { 255 div } /exec cvx 3 -1 roll [ 4 1 roll load /exec cvx ] cvx - ] setcolorspace_opt - /TintProc { - 255 mul round cvi setcolor - }bdf - }{ - MappedCSA 0 get /DeviceCMYK eq - currentdict/Components known and - AGMCORE_sep_special not and{ - /TintProc [ - Components aload pop Name findcmykcustomcolor - /exch cvx /setcustomcolor cvx - ] cvx bdf - }{ - AGMCORE_host_sep Name (All) eq and{ - /TintProc { - 1 exch sub setseparationgray - }bdf - }{ - AGMCORE_in_rip_sep MappedCSA 0 get /DeviceCMYK eq and - AGMCORE_host_sep or - Name () eq and{ - /TintProc [ - MappedCSA sep_proc_name exch 0 get /DeviceCMYK eq{ - cvx /setcmykcolor cvx - }{ - cvx /setgray cvx - }ifelse - ] cvx bdf - }{ - AGMCORE_producing_seps MappedCSA 0 get dup /DeviceCMYK eq exch /DeviceGray eq or and AGMCORE_sep_special not and{ - /TintProc [ - /dup cvx - MappedCSA sep_proc_name cvx exch - 0 get /DeviceGray eq{ - 1 /exch cvx /sub cvx 0 0 0 4 -1 /roll cvx - }if - /Name cvx /findcmykcustomcolor cvx /exch cvx - - AGMCORE_host_sep{ - AGMCORE_is_cmyk_sep - }{ - Name inRip_spot_has_ink not - }ifelse - { - /pop cvx 1 - }if - /setcustomcolor cvx - ] cvx bdf - }{ - /TintProc /setcolor ldf - - [/Separation Name MappedCSA sep_proc_name load ] setcolorspace_opt - }ifelse - }ifelse - }ifelse - }ifelse - }ifelse - set_crd - setsepcolor - end -} def -/setindexedcolorspace -{ - dup /indexed_colorspace_dict exch AGMCORE_gput - begin - /MappedCSA CSA map_csa def - AGMCORE_host_sep level2 not and{ - 0 0 0 0 setcmykcolor - }{ - [/Indexed MappedCSA - level2 not has_color not and{ - dup 0 get dup /DeviceRGB eq exch /DeviceCMYK eq or{ - pop [/DeviceGray] - }if - HiVal GrayLookup - }{ - HiVal - currentdict/RangeArray known{ - { - /indexed_colorspace_dict AGMCORE_gget begin - Lookup exch - dup HiVal gt{ - pop HiVal - }if - NComponents mul NComponents getinterval {} forall - NComponents 1 sub -1 0{ - RangeArray exch 2 mul 2 getinterval aload pop map255_to_range - NComponents 1 roll - }for - end - } bind - }{ - Lookup - }ifelse - }ifelse - ] setcolorspace_opt - - set_crd - }ifelse - end -}def -/setindexedcolor -{ - AGMCORE_host_sep{ - /indexed_colorspace_dict AGMCORE_gget/Lookup get 4 3 -1 roll map_index setcmykcolor - }{ - setcolor - }ifelse -} def -/ignoreimagedata -{ - currentoverprint not{ - gsave - dup begin - 1 setgray - 0 0 ImageMatrix itransform - Width Height ImageMatrix idtransform rectfill - end - grestore - }if - consumeimagedata -}def -/add_csa -{ - Adobe_AGM_Core begin - /AGMCORE_CSA_cache xput - end -}def -/map_csa -{ - dup type /nametype eq{ - Adobe_AGM_Core/AGMCORE_CSA_cache get exch get - }if -}def -/add_csd -{ - Adobe_AGM_Core begin - /AGMCORE_CSD_cache xput - end -}def -/get_csd -{ - dup type /nametype eq{ - Adobe_AGM_Core/AGMCORE_CSD_cache get exch get - }if -}def -/get_csd_by_name -{ - dup type dup /nametype eq exch /stringtype eq or{ - Adobe_AGM_Core begin - /AGMCORE_CSD_Name xdf - AGMCORE_CSD_cache - { - dup /Name get AGMCORE_CSD_Name eq - { - exch pop exit - }{ - pop - }ifelse - pop - }forall - end - }if -}def -/cachepattern_level2 -{ - 4 dict begin - /comparebuffer exch def - /holdbuffer exch def - /readbuffer 1024 string def - /LZWFilter holdbuffer /LZWEncode filter def - { - currentfile readbuffer readline not - {pop exit} - if - dup LZWFilter exch writestring - LZWFilter (\n) writestring - comparebuffer eq - {exit} - if - }loop - LZWFilter closefile - end -}def -/cachepattern_level3 -{ - 3 dict begin - /comparebuffer exch def - /readbuffer 1024 string def - /DoEOL false def - { - DoEOL - { - (\n) - /DoEOL false def - } - { - currentfile readbuffer readline not - {pop ()} - { - dup length 0 eq - { pop(\n)} - { - dup comparebuffer eq - {pop ()} - {/DoEOL true def} - ifelse - } - ifelse - } - ifelse - } - ifelse - } /ReusableStreamDecode filter - end -}def -/add_pattern -{ - Adobe_AGM_Core begin - /AGMCORE_pattern_cache xput - end -}def -/get_pattern -{ - dup type /nametype eq{ - Adobe_AGM_Core/AGMCORE_pattern_cache get exch get - }if -}def -/make_pattern -{ - dup matrix currentmatrix matrix concatmatrix 0 0 3 2 roll itransform - exch 3 index /XStep get 1 index exch 2 copy div cvi mul sub sub - exch 3 index /YStep get 1 index exch 2 copy div cvi mul sub sub - matrix translate exch matrix concatmatrix - makepattern -}def -/set_pattern -{ - dup /PatternType get 1 eq{ - dup /PaintType get 1 eq{ - false sop [/DeviceGray] setcolorspace 0 setgray - }if - }if - setpattern -}def -/setcolorspace_opt -{ - dup currentcolorspace eq{ - pop - }{ - setcolorspace - }ifelse -}def -/updatecolorrendering -{ - - currentcolorrendering/Intent known{ - currentcolorrendering/Intent get - }{ - null - }ifelse - - Intent ne{ - false - Intent - AGMCORE_CRD_cache { - exch pop - begin - dup Intent eq{ - currentdict setcolorrendering_opt - end - exch pop true exch - exit - }if - end - } forall - pop - not{ - systemdict /findcolorrendering known{ - Intent findcolorrendering pop - /ColorRendering findresource - dup length dict copy - setcolorrendering_opt - }if - }if - }if -} def -/add_crd -{ - AGMCORE_CRD_cache 3 1 roll put -}def -/set_crd -{ - AGMCORE_host_sep not level2 and{ - currentdict/CRD known{ - AGMCORE_CRD_cache CRD get dup null ne{ - setcolorrendering_opt - }{ - pop - }ifelse - }{ - currentdict/Intent known{ - updatecolorrendering - }if - }ifelse - }if -}def -/setcolorrendering_opt -{ - dup currentcolorrendering eq{ - pop - }{ - begin - /Intent Intent def - currentdict - end - setcolorrendering - }ifelse -}def -/cdndf -{ - exch dup currentdict exch known{ - pop pop - }{ - exch def - }ifelse -}def -/cpaint_gcomp -{ - convert_to_process Adobe_AGM_Core/AGMCORE_ConvertToProcess xddf - Adobe_AGM_Core/AGMCORE_ConvertToProcess get not - { - (%end_cpaint_gcomp) flushinput - }if -}def -/cpaint_gsep -{ - Adobe_AGM_Core/AGMCORE_ConvertToProcess get - { - (%end_cpaint_gsep) flushinput - }if -}def -/cpaint_gend -{ - newpath -}def -/AGMCORE_ctm_stack bdict - /push_ctm { - stack length size le{ - stack dup length 2 mul array - dup /stack exch def - copy pop - }if - stack size 3 -1 roll put - /size size 1 add def - } - /pop_ctm { - /size size 1 sub def - size 0 lt{ - /size 0 def - }if - stack size get - } - /stack 1 array - /size 0 -edict -def -/save_ctm -{ - matrix currentmatrix AGMCORE_ctm_stack begin - push_ctm - end -}def -/restore_ctm -{ - AGMCORE_ctm_stack begin - pop_ctm - end - setmatrix -}def -/path_rez -{ - dup 0 ne{ - AGMCORE_deviceDPI exch div - dup 1 lt{ - pop 1 - }if - setflat - }{ - pop - }ifelse -}def -/rdcmntline { - currentfile AGMCORE_str256 readline pop - (%) anchorsearch {pop} if -} def -/set_spot_alias_ary -{ - /AGMCORE_SpotAliasAry where{ - pop pop - }{ - Adobe_AGM_Core/AGMCORE_SpotAliasAry xddf - true set_spot_alias - }ifelse -}def -/set_spot_alias -{ - /AGMCORE_SpotAliasAry where{ - /AGMCORE_current_spot_alias 3 -1 roll put - }{ - pop - }ifelse -}def -/current_spot_alias -{ - /AGMCORE_SpotAliasAry where{ - /AGMCORE_current_spot_alias get - }{ - false - }ifelse -}def -/map_alias -{ - /AGMCORE_SpotAliasAry where{ - begin - /AGMCORE_name xdf - false - AGMCORE_SpotAliasAry{ - dup/Name get AGMCORE_name eq{ - save exch - /Adobe_AGM_Core currentdict def - /CSD get get_csd - exch restore - exch pop true - exit - }{ - pop - }ifelse - }forall - end - }{ - pop false - }ifelse -}bdf -/spot_alias -{ - true set_spot_alias - - /AGMCORE_&setcustomcolor AGMCORE_key_known not { - Adobe_AGM_Core/AGMCORE_&setcustomcolor /setcustomcolor load put - } if - /customcolor_tint 1 AGMCORE_gput - - Adobe_AGM_Core begin - /setcustomcolor - { - - dup /customcolor_tint exch AGMCORE_gput - - current_spot_alias{ - 1 index 4 get map_alias{ - mark 3 1 roll - setsepcolorspace - counttomark 0 ne{ - setsepcolor - }if - pop - pop - }{ - AGMCORE_&setcustomcolor - }ifelse - }{ - AGMCORE_&setcustomcolor - }ifelse - }bdf - end -}def -/begin_feature -{ - Adobe_AGM_Core/AGMCORE_feature_dictCount countdictstack put - count Adobe_AGM_Core/AGMCORE_feature_opCount 3 -1 roll put - {Adobe_AGM_Core/AGMCORE_feature_ctm matrix currentmatrix put}if -}def -/end_feature -{ - 2 dict begin - /spd /setpagedevice load def - /setpagedevice { get_gstate spd set_gstate } def - stopped{$error/newerror false put}if - end - count Adobe_AGM_Core/AGMCORE_feature_opCount get sub dup 0 gt{{pop}repeat}{pop}ifelse - countdictstack Adobe_AGM_Core/AGMCORE_feature_dictCount get sub dup 0 gt{{end}repeat}{pop}ifelse - {Adobe_AGM_Core/AGMCORE_feature_ctm get setmatrix}if -}def -/set_negative -{ - Adobe_AGM_Core begin - /AGMCORE_inverting exch def - level2{ - currentpagedevice/NegativePrint known{ - currentpagedevice/NegativePrint get Adobe_AGM_Core/AGMCORE_inverting get ne{ - true begin_feature true{ - bdict /NegativePrint Adobe_AGM_Core/AGMCORE_inverting get edict setpagedevice - }end_feature - }if - /AGMCORE_inverting false def - }if - }if - AGMCORE_inverting{ - [{1 exch sub}/exec load dup currenttransfer exch]cvx bind settransfer - gsave newpath clippath 1 /setseparationgray where{pop setseparationgray}{setgray}ifelse - fill grestore - }if - end -}def -/lw_save_restore_override { - /md where { - pop - md begin - /pmSVsetup{} def - /endp{}def - /pse{}def - /psb{}def - /orig_showpage where - {pop} - {/orig_showpage /showpage load def} - ifelse - /showpage {orig_showpage gR} def - end - }if -}def -/pscript_showpage_override { - /NTPSOct95 where - { - begin - showpage - save - /showpage /restore load def - /restore {exch pop}def - end - }if -}def -/driver_media_override -{ - /md where { - pop - md /initializepage known { - md /initializepage {} put - } if - md /rC known { - md /rC {4{pop}repeat} put - } if - }if - - Adobe_AGM_Core /AGMCORE_Default_CTM matrix currentmatrix put -}def -/driver_check_media_override -{ - Adobe_AGM_Core /AGMCORE_Default_CTM get matrix currentmatrix ne - { - Adobe_AGM_Core /AGMCORE_Default_CTM get setmatrix - }if -}def -AGMCORE_err_strings begin - /AGMCORE_bad_environ (Environment not satisfactory for this job. Ensure that the PPD is correct or that the PostScript level requested is supported by this printer. ) def - /AGMCORE_color_space_onhost_seps (This job contains colors that will not separate with on-host methods. ) def - /AGMCORE_invalid_color_space (This job contains an invalid color space. ) def -end -end -systemdict /setpacking known -{ - setpacking -} if -%%EndResource -%%BeginResource: procset Adobe_CoolType_Core 2.12 0 -%%Copyright: Copyright 1997-2001 Adobe Systems Incorporated. All Rights Reserved. -%%Version: 2.12 0 -userdict/Adobe_CoolType_Core 60 dict dup begin put/Level2? systemdict -/languagelevel known dup{pop systemdict/languagelevel get 2 ge}if def Level2? -not{/currentglobal false def/setglobal/pop load def/gcheck{pop false}bind def -/currentpacking false def/setpacking/pop load def/SharedFontDirectory 0 dict -def}if currentpacking true setpacking/@_SaveStackLevels{Adobe_CoolType_Data -begin @opStackCountByLevel @opStackLevel 2 copy known not{2 copy 3 dict dup -/args 7 index 5 add array put put get}{get dup/args get dup length 3 index lt{ -dup length 5 add array exch 1 index exch 0 exch putinterval 1 index exch/args -exch put}{pop}ifelse}ifelse begin count 2 sub 1 index lt{pop count 1 sub}if -dup/argCount exch def dup 0 gt{exch 1 index 2 add 1 roll args exch 0 exch -getinterval astore pop}{pop}ifelse count 1 sub/restCount exch def end -/@opStackLevel @opStackLevel 1 add def countdictstack 1 sub -@dictStackCountByLevel exch @dictStackLevel exch put/@dictStackLevel -@dictStackLevel 1 add def end}bind def/@_RestoreStackLevels{ -Adobe_CoolType_Data begin/@opStackLevel @opStackLevel 1 sub def -@opStackCountByLevel @opStackLevel get begin count restCount sub dup 0 gt{{pop -}repeat}{pop}ifelse args 0 argCount getinterval{}forall end/@dictStackLevel -@dictStackLevel 1 sub def @dictStackCountByLevel @dictStackLevel get end -countdictstack exch sub dup 0 gt{{end}repeat}{pop}ifelse}bind def -/@_PopStackLevels{Adobe_CoolType_Data begin/@opStackLevel @opStackLevel 1 sub -def/@dictStackLevel @dictStackLevel 1 sub def end}bind def/@Raise{exch cvx -exch errordict exch get exec stop}bind def/@ReRaise{cvx $error/errorname get -errordict exch get exec stop}bind def/@Stopped{0 @#Stopped}bind def/@#Stopped{ -@_SaveStackLevels stopped{@_RestoreStackLevels true}{@_PopStackLevels false} -ifelse}bind def/@Arg{Adobe_CoolType_Data begin @opStackCountByLevel -@opStackLevel 1 sub get/args get exch get end}bind def/doc_setup{ -Adobe_CoolType_Core begin/mov/moveto load def/nfnt/newencodedfont load def -/mfnt/makefont load def/sfnt/setfont load def/ufnt/undefinefont load def/chp -/charpath load def/awsh/awidthshow load def/wsh/widthshow load def/ash/ashow -load def/sh/show load def end userdict/Adobe_CoolType_Data 6 dict dup begin -/AddWidths? false def/CC 0 def/charcode 2 string def/@opStackCountByLevel 32 -dict def/@opStackLevel 0 def/@dictStackCountByLevel 32 dict def -/@dictStackLevel 0 def end put}bind def/doc_trailer{currentdict -Adobe_CoolType_Core eq{end}if}bind def/page_setup{Adobe_CoolType_Core begin} -bind def/page_trailer{end}bind def/unload{systemdict/languagelevel known{ -systemdict/languagelevel get 2 ge{userdict/Adobe_CoolType_Core 2 copy known{ -undef}{pop pop}ifelse}if}if}bind def/ndf{1 index where{pop pop pop}{dup xcheck -{bind}if def}ifelse}def/findfont dup systemdict begin userdict begin -/globaldict where{/globaldict get begin}if dup where pop exch get/globaldict -where{pop end}if end end def/systemfindfont/findfont load def/undefinefont{pop -}ndf/copyfont{currentglobal 3 1 roll 1 index gcheck setglobal dup null eq{0}{ -dup length}ifelse 2 index length add 1 add dict begin exch{1 index/FID eq{pop -pop}{def}ifelse}forall dup null eq{pop}{{def}forall}ifelse currentdict end -exch setglobal}bind def/copyarray{currentglobal exch dup gcheck setglobal dup -length array copy exch setglobal}bind def/newencodedfont{currentglobal{ -SharedFontDirectory 3 index known{SharedFontDirectory 3 index get -/FontReferenced known}{false}ifelse}{FontDirectory 3 index known{FontDirectory -3 index get/FontReferenced known}{SharedFontDirectory 3 index known{ -SharedFontDirectory 3 index get/FontReferenced known}{false}ifelse}ifelse} -ifelse dup{3 index findfont/FontReferenced get 2 index findfont ne{pop false} -if}if{pop 1 index findfont/Encoding get exch 0 1 255{2 copy get 3 index 3 1 -roll put}for pop pop pop}{findfont dup dup maxlength 2 add dict begin exch{1 -index/FID ne{def}{pop pop}ifelse}forall/FontReferenced exch def/Encoding exch -dup length array copy def/FontName 1 index dup type/stringtype eq{cvn}if def -currentdict end definefont pop}ifelse}bind def/SetSubstituteStrategy{ -$SubstituteFont begin dup type/dicttype ne{0 dict}if currentdict/$Strategies -known{exch $Strategies exch 2 copy known{get 2 copy maxlength exch maxlength -add dict begin{def}forall{def}forall currentdict dup/$Init known{dup/$Init get -exec}if end/$Strategy exch def}{pop pop pop}ifelse}{pop pop}ifelse end}bind -def/scff{$SubstituteFont begin dup type/stringtype eq{dup length exch}{null} -ifelse/$sname exch def/$slen exch def end{findfont}@Stopped{dup length dup 21 -add string dup 4 3 roll 0 exch 128 string cvs putinterval exch 1 index exch -(_was-malformed-so-was)putinterval cvn{findfont}@Stopped{pop/Courier findfont} -if}if $SubstituteFont begin/$sname null def/$slen 0 def end}bind def -/isWidthsOnlyFont{dup/WidthsOnly known{pop pop true}{dup/FDepVector known{ -/FDepVector get{isWidthsOnlyFont dup{exit}if}forall}{dup/FDArray known{ -/FDArray get{isWidthsOnlyFont dup{exit}if}forall}{pop}ifelse}ifelse}ifelse} -bind def/?set{$SubstituteFont begin/$substituteFound false def/$fontname 4 -index def/$doSmartSub false def end 3 index findfont $SubstituteFont begin -$substituteFound{false}{dup/FontName known{dup/FontName get $fontname eq 1 -index/DistillerFauxFont known not and/currentdistillerparams where{pop false 2 -index isWidthsOnlyFont not and}if}{false}ifelse}ifelse exch pop/$doSmartSub -true def end{exch pop exch pop exch 2 dict dup/Found 3 index put exch findfont -exch}{exch exec exch findfont 2 dict dup/Downloaded 6 5 roll put}ifelse dup -/FontName 4 index put copyfont definefont pop}bind def/?str1 256 string def -/?str2 256 string def/?add{1 index type/integertype eq{exch true 4 2}{false 3 -1}ifelse roll 1 index findfont dup/Widths known{Adobe_CoolType_Data/AddWidths? -true put gsave dup 1000 scalefont setfont}if/Downloaded known{exec exch{exch -?str2 cvs exch findfont/Downloaded get 1 dict begin/Downloaded 1 index def -?str1 cvs length ?str1 1 index 1 add 3 index putinterval exch length 1 add 1 -index add ?str1 2 index(*)putinterval ?str1 0 2 index getinterval cvn findfont -?str1 3 index(+)putinterval 2 dict dup/FontName ?str1 0 6 index getinterval -cvn put dup/Downloaded Downloaded put end copyfont dup/FontName get exch -definefont pop pop pop}{pop}ifelse}{pop exch{findfont dup/Found get dup length -exch ?str1 cvs pop ?str1 1 index(+)putinterval ?str1 1 index 1 add 4 index -?str2 cvs putinterval ?str1 exch 0 exch 5 4 roll ?str2 cvs length 1 add add -getinterval cvn 1 dict exch 1 index exch/FontName exch put copyfont dup -/FontName get exch definefont pop}{pop}ifelse}ifelse Adobe_CoolType_Data -/AddWidths? get{grestore Adobe_CoolType_Data/AddWidths? false put}if}bind def -/?sh{currentfont/Downloaded known{exch}if pop}bind def/?chp{currentfont -/Downloaded known{pop}{false chp}ifelse}bind def/?mv{currentfont/Downloaded -known{moveto pop pop}{pop pop moveto}ifelse}bind def setpacking userdict -/$SubstituteFont 25 dict put 1 dict begin/SubstituteFont dup $error exch 2 -copy known{get}{pop pop{pop/Courier}bind}ifelse def/currentdistillerparams -where dup{pop pop currentdistillerparams/CannotEmbedFontPolicy 2 copy known{ -get/Error eq}{pop pop false}ifelse}if not{countdictstack array dictstack 0 get -begin userdict begin $SubstituteFont begin/$str 128 string def/$fontpat 128 -string def/$slen 0 def/$sname null def/$match false def/$fontname null def -/$substituteFound false def/$doSmartSub true def/$depth 0 def/$fontname null -def/$italicangle 26.5 def/$dstack null def/$Strategies 10 dict dup begin -/$Type3Underprint{currentglobal exch false setglobal 11 dict begin/UseFont -exch $WMode 0 ne{dup length dict copy dup/WMode $WMode put/UseFont exch -definefont}if def/FontName $fontname dup type/stringtype eq{cvn}if def -/FontType 3 def/FontMatrix[.001 0 0 .001 0 0]def/Encoding 256 array dup 0 1 -255{/.notdef put dup}for pop def/FontBBox[0 0 0 0]def/CCInfo 7 dict dup begin -/cc null def/x 0 def/y 0 def end def/BuildChar{exch begin CCInfo begin 1 -string dup 0 3 index put exch pop/cc exch def UseFont 1000 scalefont setfont -cc stringwidth/y exch def/x exch def x y setcharwidth $SubstituteFont -/$Strategy get/$Underprint get exec 0 0 moveto cc show x y moveto end end}bind -def currentdict end exch setglobal}bind def/$GetaTint 2 dict dup begin -/$BuildFont{dup/WMode known{dup/WMode get}{0}ifelse/$WMode exch def $fontname -exch dup/FontName known{dup/FontName get dup type/stringtype eq{cvn}if}{ -/unnamedfont}ifelse exch $deepcopyfont exch 1 index exch/FontBasedOn exch put -dup/FontName $fontname dup type/stringtype eq{cvn}if put definefont}bind def -/$Underprint{gsave x abs y abs gt{/y 1000 def}{/x -1000 def 500 120 translate} -ifelse Level2?{[/Separation(All)/DeviceCMYK{0 0 0 1 pop}]setcolorspace}{0 -setgray}ifelse 10 setlinewidth x .8 mul[7 3]{y mul 8 div 120 sub x 10 div exch -moveto 0 y 4 div neg rlineto dup 0 rlineto 0 y 4 div rlineto closepath gsave -Level2?{.2 setcolor}{.8 setgray}ifelse fill grestore stroke}forall pop -grestore}bind def end def/$Oblique 1 dict dup begin/$BuildFont{currentglobal -exch dup gcheck setglobal null copyfont begin/FontBasedOn currentdict/FontName -known{FontName dup type/stringtype eq{cvn}if}{/unnamedfont}ifelse def/FontName -$fontname dup type/stringtype eq{cvn}if def/currentdistillerparams where{pop}{ -/FontInfo currentdict/FontInfo known{FontInfo null copyfont}{2 dict}ifelse dup -begin/ItalicAngle $italicangle def/FontMatrix FontMatrix[1 0 ItalicAngle dup -sin exch cos div 1 0 0]matrix concatmatrix readonly end 4 2 roll def def} -ifelse FontName currentdict end definefont exch setglobal}bind def end def -/$None 1 dict dup begin/$BuildFont{}bind def end def end def/$Oblique -SetSubstituteStrategy/$findfontByEnum{dup type/stringtype eq{cvn}if dup -/$fontname exch def $sname null eq{$str cvs dup length $slen sub $slen -getinterval}{pop $sname}ifelse $fontpat dup 0(fonts/*)putinterval exch 7 exch -putinterval/$match false def $SubstituteFont/$dstack countdictstack array -dictstack put mark{$fontpat 0 $slen 7 add getinterval{/$match exch def exit} -$str filenameforall}stopped{cleardictstack currentdict true $SubstituteFont -/$dstack get{exch{1 index eq{pop false}{true}ifelse}{begin false}ifelse}forall -pop}if cleartomark/$slen 0 def $match false ne{$match(fonts/)anchorsearch pop -pop cvn}{/Courier}ifelse}bind def/$ROS 1 dict dup begin/Adobe 4 dict dup begin -/Japan1[/Ryumin-Light/HeiseiMin-W3/GothicBBB-Medium/HeiseiKakuGo-W5 -/HeiseiMaruGo-W4/Jun101-Light]def/Korea1[/HYSMyeongJo-Medium/HYGoThic-Medium] -def/GB1[/STSong-Light/STHeiti-Regular]def/CNS1[/MKai-Medium/MHei-Medium]def -end def end def/$cmapname null def/$deepcopyfont{dup/FontType get 0 eq{1 dict -dup/FontName/copied put copyfont begin/FDepVector FDepVector copyarray 0 1 2 -index length 1 sub{2 copy get $deepcopyfont dup/FontName/copied put/copied -exch definefont 3 copy put pop pop}for def currentdict end}{$Strategies -/$Type3Underprint get exec}ifelse}bind def/$buildfontname{length $str 1 index -(-)putinterval 1 add $str 1 index $cmapname $fontpat cvs putinterval $cmapname -length add $str exch 0 exch getinterval cvn}bind def/$findfontByROS{/$fontname -exch def $ROS Registry 2 copy known{get Ordering 2 copy known{get}{pop pop[]} -ifelse}{pop pop[]}ifelse false exch{dup/CIDFont resourcestatus{pop pop save 1 -index/CIDFont findresource dup/WidthsOnly known{dup/WidthsOnly get}{false} -ifelse exch pop exch restore{pop}{exch pop true exit}ifelse}{pop}ifelse}forall -{$str cvs $buildfontname}{false(*){save exch dup/CIDFont findresource dup -/WidthsOnly known{dup/WidthsOnly get not}{true}ifelse exch/CIDSystemInfo get -dup/Registry get Registry eq exch/Ordering get Ordering eq and and{exch -restore exch pop true exit}{pop restore}ifelse}$str/CIDFont resourceforall{ -$buildfontname}{$fontname $findfontByEnum}ifelse}ifelse}bind def end end -currentdict/$error known currentdict/languagelevel known and dup{pop $error -/SubstituteFont known}if dup{$error}{Adobe_CoolType_Core}ifelse begin{ -/SubstituteFont/CMap/Category resourcestatus{pop pop{$SubstituteFont begin -/$substituteFound true def dup length $slen gt $sname null ne or $slen 0 gt -and{$sname null eq{dup $str cvs dup length $slen sub $slen getinterval cvn}{ -$sname}ifelse dup/CMap resourcestatus{pop pop dup/$cmapname exch def/CMap -findresource/CIDSystemInfo get{def}forall $findfontByROS}{128 string cvs dup -(-)search{3 1 roll search{3 1 roll pop{dup cvi}stopped{pop pop pop pop pop -$findfontByEnum}{4 2 roll pop pop exch length exch 2 index length 2 index sub -exch 1 sub -1 0{$str cvs dup length 4 index 0 4 index 4 3 roll add getinterval -exch 1 index exch 3 index exch putinterval dup/CMap resourcestatus{pop pop 4 1 -roll pop pop pop dup/$cmapname exch def/CMap findresource/CIDSystemInfo get{ -def}forall $findfontByROS true exit}{pop}ifelse}for dup type/booleantype eq{ -pop}{pop pop $findfontByEnum}ifelse}ifelse}{pop pop pop $findfontByEnum}ifelse -}{pop pop $findfontByEnum}ifelse}ifelse}{//SubstituteFont exec}ifelse/$slen 0 -def end}}{{$SubstituteFont begin/$substituteFound true def dup length $slen gt -$sname null ne or $slen 0 gt and{$findfontByEnum}{//SubstituteFont exec}ifelse -end}}ifelse bind readonly def Adobe_CoolType_Core/scfindfont/systemfindfont -load put}{/scfindfont{$SubstituteFont begin dup systemfindfont dup/FontName -known{dup/FontName get dup 3 index ne}{/noname true}ifelse dup{ -/$origfontnamefound 2 index def/$origfontname 4 index def/$substituteFound -true def}if exch pop{$slen 0 gt $sname null ne 3 index length $slen gt or and{ -pop dup $findfontByEnum findfont dup maxlength 1 add dict begin{1 index/FID eq -{pop pop}{def}ifelse}forall currentdict end definefont dup/FontName known{dup -/FontName get}{null}ifelse $origfontnamefound ne{$origfontname $str cvs print -( substitution revised, using )print dup/FontName known{dup/FontName get}{ -(unspecified font)}ifelse $str cvs print(. -)print}if}{exch pop}ifelse}{exch pop}ifelse end}bind def}ifelse end end -Adobe_CoolType_Core/findfont{$SubstituteFont begin $depth 0 eq{/$fontname 1 -index dup type/stringtype ne{$str cvs}if def/$substituteFound false def}if -/$depth $depth 1 add def end scfindfont $SubstituteFont begin/$depth $depth 1 -sub def $substituteFound $depth 0 eq and $doSmartSub and{currentdict/$Strategy -known{$Strategy/$BuildFont get exec}if}if end}bind put}if end end -%%EndResource -%%BeginResource: procset Adobe_CoolType_Utility_MAKEOCF 1.13 0 -%%Copyright: Copyright 1987-2001 Adobe Systems Incorporated. -%%Version: 1.13 0 -systemdict/languagelevel known dup{currentglobal false setglobal}{false}ifelse -exch userdict/Adobe_CoolType_Utility 2 copy known{2 copy get dup maxlength 25 -add dict copy}{25 dict}ifelse put Adobe_CoolType_Utility begin/ct_Level2? exch -def/ct_Clone? 1183615869 internaldict dup/CCRun known not exch/eCCRun known -not ct_Level2? and or def/ct_UseNativeCapability? systemdict/composefont known -def/ct_MakeOCF 35 dict def/ct_Vars 25 dict def/ct_GlyphDirProcs 6 dict def -/ct_BuildCharDict 15 dict dup begin/charcode 2 string def/dst_string 1500 -string def/nullstring()def/usewidths? true def end def ct_Level2?{setglobal}{ -pop}ifelse ct_GlyphDirProcs begin/GetGlyphDirectory{systemdict/languagelevel -known{pop/CIDFont findresource/GlyphDirectory get}{1 index/CIDFont -findresource/GlyphDirectory get dup type/dicttype eq{dup dup maxlength exch -length sub 2 index lt{dup length 2 index add dict copy 2 index/CIDFont -findresource/GlyphDirectory 2 index put}if}if exch pop exch pop}ifelse +}def/+ -{systemdict/languagelevel known{currentglobal false setglobal 3 dict begin/vm -exch def}{1 dict begin}ifelse/$ exch def systemdict/languagelevel known{vm -setglobal/gvm currentglobal def $ gcheck setglobal}if ?{$ begin}if}def/?{$ -type/dicttype eq}def/|{userdict/Adobe_CoolType_Data known{Adobe_CoolType_Data -/AddWidths? known{currentdict Adobe_CoolType_Data begin begin AddWidths?{ -Adobe_CoolType_Data/CC 3 index put ?{def}{$ 3 1 roll put}ifelse CC charcode -exch 1 index 0 2 index 256 idiv put 1 index exch 1 exch 256 mod put -stringwidth 2 array astore currentfont/Widths get exch CC exch put}{?{def}{$ 3 -1 roll put}ifelse}ifelse end end}{?{def}{$ 3 1 roll put}ifelse}ifelse}{?{def}{ -$ 3 1 roll put}ifelse}ifelse}def/!{?{end}if systemdict/languagelevel known{gvm -setglobal}if end}def/:{string currentfile exch readstring pop}executeonly def -end ct_MakeOCF begin/ct_cHexEncoding[/c00/c01/c02/c03/c04/c05/c06/c07/c08/c09 -/c0A/c0B/c0C/c0D/c0E/c0F/c10/c11/c12/c13/c14/c15/c16/c17/c18/c19/c1A/c1B/c1C -/c1D/c1E/c1F/c20/c21/c22/c23/c24/c25/c26/c27/c28/c29/c2A/c2B/c2C/c2D/c2E/c2F -/c30/c31/c32/c33/c34/c35/c36/c37/c38/c39/c3A/c3B/c3C/c3D/c3E/c3F/c40/c41/c42 -/c43/c44/c45/c46/c47/c48/c49/c4A/c4B/c4C/c4D/c4E/c4F/c50/c51/c52/c53/c54/c55 -/c56/c57/c58/c59/c5A/c5B/c5C/c5D/c5E/c5F/c60/c61/c62/c63/c64/c65/c66/c67/c68 -/c69/c6A/c6B/c6C/c6D/c6E/c6F/c70/c71/c72/c73/c74/c75/c76/c77/c78/c79/c7A/c7B -/c7C/c7D/c7E/c7F/c80/c81/c82/c83/c84/c85/c86/c87/c88/c89/c8A/c8B/c8C/c8D/c8E -/c8F/c90/c91/c92/c93/c94/c95/c96/c97/c98/c99/c9A/c9B/c9C/c9D/c9E/c9F/cA0/cA1 -/cA2/cA3/cA4/cA5/cA6/cA7/cA8/cA9/cAA/cAB/cAC/cAD/cAE/cAF/cB0/cB1/cB2/cB3/cB4 -/cB5/cB6/cB7/cB8/cB9/cBA/cBB/cBC/cBD/cBE/cBF/cC0/cC1/cC2/cC3/cC4/cC5/cC6/cC7 -/cC8/cC9/cCA/cCB/cCC/cCD/cCE/cCF/cD0/cD1/cD2/cD3/cD4/cD5/cD6/cD7/cD8/cD9/cDA -/cDB/cDC/cDD/cDE/cDF/cE0/cE1/cE2/cE3/cE4/cE5/cE6/cE7/cE8/cE9/cEA/cEB/cEC/cED -/cEE/cEF/cF0/cF1/cF2/cF3/cF4/cF5/cF6/cF7/cF8/cF9/cFA/cFB/cFC/cFD/cFE/cFF]def -/ct_CID_STR_SIZE 8000 def/ct_mkocfStr100 100 string def/ct_defaultFontMtx[.001 -0 0 .001 0 0]def/ct_1000Mtx[1000 0 0 1000 0 0]def/ct_raise{exch cvx exch -errordict exch get exec stop}bind def/ct_reraise{cvx $error/errorname get -(Error: )print dup( )cvs print errordict exch get exec stop -}bind def/ct_cvnsi{1 index add 1 sub 1 exch 0 4 1 roll{2 index exch get exch 8 -bitshift add}for exch pop}bind def/ct_GetInterval{Adobe_CoolType_Utility -/ct_BuildCharDict get begin/dst_index 0 def dup dst_string length gt{dup -string/dst_string exch def}if 1 index ct_CID_STR_SIZE idiv/arrayIndex exch def -2 index arrayIndex get 2 index arrayIndex ct_CID_STR_SIZE mul sub{dup 3 index -add 2 index length le{2 index getinterval dst_string dst_index 2 index -putinterval length dst_index add/dst_index exch def exit}{1 index length 1 -index sub dup 4 1 roll getinterval dst_string dst_index 2 index putinterval -pop dup dst_index add/dst_index exch def sub/arrayIndex arrayIndex 1 add def 2 -index dup length arrayIndex gt{arrayIndex get}{pop exit}ifelse 0}ifelse}loop -pop pop pop dst_string 0 dst_index getinterval end}bind def ct_Level2?{ -/ct_resourcestatus currentglobal mark true setglobal{/unknowninstancename -/Category resourcestatus}stopped{cleartomark setglobal true}{cleartomark -currentglobal not exch setglobal}ifelse{{mark 3 1 roll/Category findresource -begin ct_Vars/vm currentglobal put({ResourceStatus} stopped)0()/SubFileDecode -filter cvx exec{cleartomark false}{{3 2 roll pop true}{cleartomark false} -ifelse}ifelse ct_Vars/vm get setglobal end}}{{resourcestatus}}ifelse bind def -/CIDFont/Category ct_resourcestatus{pop pop}{currentglobal true setglobal -/Generic/Category findresource dup length dict copy dup/InstanceType/dicttype -put/CIDFont exch/Category defineresource pop setglobal}ifelse -ct_UseNativeCapability?{/CIDInit/ProcSet findresource begin 12 dict begin -begincmap/CIDSystemInfo 3 dict dup begin/Registry(Adobe)def/Ordering(Identity) -def/Supplement 0 def end def/CMapName/Identity-H def/CMapVersion 1 def -/CMapType 1 def 1 begincodespacerange<0000>endcodespacerange 1 -begincidrange<0000>0 endcidrange endcmap CMapName currentdict/CMap -defineresource pop end end}if}{/ct_Category 2 dict begin/CIDFont 10 dict def -/ProcSet 2 dict def currentdict end def/defineresource{ct_Category 1 index 2 -copy known{get dup dup maxlength exch length eq{dup length 10 add dict copy -ct_Category 2 index 2 index put}if 3 index 3 index put pop exch pop}{pop pop -/defineresource/undefined ct_raise}ifelse}bind def/findresource{ct_Category 1 -index 2 copy known{get 2 index 2 copy known{get 3 1 roll pop pop}{pop pop -/findresource/undefinedresource ct_raise}ifelse}{pop pop/findresource -/undefined ct_raise}ifelse}bind def/resourcestatus{ct_Category 1 index 2 copy -known{get 2 index known exch pop exch pop{0 -1 true}{false}ifelse}{pop pop -/findresource/undefined ct_raise}ifelse}bind def/ct_resourcestatus -/resourcestatus load def}ifelse/ct_CIDInit 2 dict begin/ct_cidfont_stream_init -{{dup(Binary)eq{pop null currentfile ct_Level2?{{cid_BYTE_COUNT() -/SubFileDecode filter}stopped{pop pop pop}if}if/readstring load exit}if dup -(Hex)eq{pop currentfile ct_Level2?{{null exch/ASCIIHexDecode filter/readstring -}stopped{pop exch pop(>)exch/readhexstring}if}{(>)exch/readhexstring}ifelse -load exit}if/StartData/typecheck ct_raise}loop cid_BYTE_COUNT ct_CID_STR_SIZE -le{2 copy cid_BYTE_COUNT string exch exec pop 1 array dup 3 -1 roll 0 exch put -}{cid_BYTE_COUNT ct_CID_STR_SIZE div ceiling cvi dup array exch 2 sub 0 exch 1 -exch{2 copy 5 index ct_CID_STR_SIZE string 6 index exec pop put pop}for 2 -index cid_BYTE_COUNT ct_CID_STR_SIZE mod string 3 index exec pop 1 index exch -1 index length 1 sub exch put}ifelse cid_CIDFONT exch/GlyphData exch put 2 -index null eq{pop pop pop}{pop/readstring load 1 string exch{3 copy exec pop -dup length 0 eq{pop pop pop pop pop true exit}if 4 index eq{pop pop pop pop -false exit}if}loop pop}ifelse}bind def/StartData{mark{currentdict dup/FDArray -get 0 get/FontMatrix get 0 get .001 eq{dup/CDevProc known not{/CDevProc -1183615869 internaldict/stdCDevProc 2 copy known{get}{pop pop{pop pop pop pop -pop 0 -1000 7 index 2 div 880}}ifelse def}if}{/CDevProc{pop pop pop pop pop 0 -1 cid_temp/cid_CIDFONT get/FDArray get 0 get/FontMatrix get 0 get div 7 index -2 div 1 index .88 mul}def}ifelse/cid_temp 15 dict def cid_temp begin -/cid_CIDFONT exch def 3 copy pop dup/cid_BYTE_COUNT exch def 0 gt{ -ct_cidfont_stream_init FDArray{/Private get dup/SubrMapOffset known{begin -/Subrs SubrCount array def Subrs SubrMapOffset SubrCount SDBytes ct_Level2?{ -currentdict dup/SubrMapOffset undef dup/SubrCount undef/SDBytes undef}if end -/cid_SD_BYTES exch def/cid_SUBR_COUNT exch def/cid_SUBR_MAP_OFFSET exch def -/cid_SUBRS exch def cid_SUBR_COUNT 0 gt{GlyphData cid_SUBR_MAP_OFFSET -cid_SD_BYTES ct_GetInterval 0 cid_SD_BYTES ct_cvnsi 0 1 cid_SUBR_COUNT 1 sub{ -exch 1 index 1 add cid_SD_BYTES mul cid_SUBR_MAP_OFFSET add GlyphData exch -cid_SD_BYTES ct_GetInterval 0 cid_SD_BYTES ct_cvnsi cid_SUBRS 4 2 roll -GlyphData exch 4 index 1 index sub ct_GetInterval dup length string copy put} -for pop}if}{pop}ifelse}forall}if cleartomark pop pop end CIDFontName -currentdict/CIDFont defineresource pop end end}stopped{cleartomark/StartData -ct_reraise}if}bind def currentdict end def/ct_saveCIDInit{/CIDInit/ProcSet -ct_resourcestatus{true}{/CIDInitC/ProcSet ct_resourcestatus}ifelse{pop pop -/CIDInit/ProcSet findresource ct_UseNativeCapability?{pop null}{/CIDInit -ct_CIDInit/ProcSet defineresource pop}ifelse}{/CIDInit ct_CIDInit/ProcSet -defineresource pop null}ifelse ct_Vars exch/ct_oldCIDInit exch put}bind def -/ct_restoreCIDInit{ct_Vars/ct_oldCIDInit get dup null ne{/CIDInit exch/ProcSet -defineresource pop}{pop}ifelse}bind def/ct_BuildCharSetUp{1 index begin -CIDFont begin Adobe_CoolType_Utility/ct_BuildCharDict get begin/ct_dfCharCode -exch def/ct_dfDict exch def CIDFirstByte ct_dfCharCode add dup CIDCount ge{pop -0}if/cid exch def{GlyphDirectory cid 2 copy known{get}{pop pop nullstring} -ifelse dup length FDBytes sub 0 gt{dup FDBytes 0 ne{0 FDBytes ct_cvnsi}{pop 0} -ifelse/fdIndex exch def dup length FDBytes sub FDBytes exch getinterval -/charstring exch def exit}{pop cid 0 eq{/charstring nullstring def exit}if/cid -0 def}ifelse}loop}def/ct_SetCacheDevice{0 0 moveto dup stringwidth 3 -1 roll -true charpath pathbbox 0 -1000 7 index 2 div 880 setcachedevice2 0 0 moveto} -def/ct_CloneSetCacheProc{1 eq{stringwidth pop -2 div -880 0 -1000 setcharwidth -moveto}{usewidths?{currentfont/Widths get cid 2 copy known{get exch pop aload -pop}{pop pop stringwidth}ifelse}{stringwidth}ifelse setcharwidth 0 0 moveto} -ifelse}def/ct_Type3ShowCharString{ct_FDDict fdIndex 2 copy known{get}{ -currentglobal 3 1 roll 1 index gcheck setglobal ct_Type1FontTemplate dup -maxlength dict copy begin FDArray fdIndex get dup/FontMatrix 2 copy known{get} -{pop pop ct_defaultFontMtx}ifelse/FontMatrix exch dup length array copy def -/Private get/Private exch def/Widths rootfont/Widths get def/CharStrings 1 -dict dup/.notdefdup length string copy put def currentdict -end/ct_Type1Font exch definefont dup 5 1 roll put setglobal}ifelse dup -/CharStrings get 1 index/Encoding get ct_dfCharCode get charstring put -rootfont/WMode 2 copy known{get}{pop pop 0}ifelse exch 1000 scalefont setfont -ct_str1 0 ct_dfCharCode put ct_str1 exch ct_dfSetCacheProc ct_SyntheticBold{ -currentpoint ct_str1 show newpath moveto ct_str1 true charpath ct_StrokeWidth -setlinewidth stroke}{ct_str1 show}ifelse}def/ct_Type4ShowCharString{ct_dfDict -ct_dfCharCode charstring FDArray fdIndex get dup/FontMatrix get dup -ct_defaultFontMtx ct_matrixeq not{ct_1000Mtx matrix concatmatrix concat}{pop} -ifelse/Private get Adobe_CoolType_Utility/ct_Level2? get not{ct_dfDict/Private -3 -1 roll{put}1183615869 internaldict/superexec get exec}if 1183615869 -internaldict Adobe_CoolType_Utility/ct_Level2? get{1 index}{3 index/Private -get mark 6 1 roll}ifelse dup/RunInt known{/RunInt get}{pop/CCRun}ifelse get -exec Adobe_CoolType_Utility/ct_Level2? get not{cleartomark}if}bind def -/ct_BuildCharIncremental{{Adobe_CoolType_Utility/ct_MakeOCF get begin -ct_BuildCharSetUp ct_ShowCharString}stopped{stop}if end end end end}bind def -/BaseFontNameStr(BF00)def/ct_Type1FontTemplate 14 dict begin/FontType 1 def -/FontMatrix[.001 0 0 .001 0 0]def/FontBBox[-250 -250 1250 1250]def/Encoding -ct_cHexEncoding def/PaintType 0 def currentdict end def/BaseFontTemplate 11 -dict begin/FontMatrix[.001 0 0 .001 0 0]def/FontBBox[-250 -250 1250 1250]def -/Encoding ct_cHexEncoding def/BuildChar/ct_BuildCharIncremental load def -ct_Clone?{/FontType 3 def/ct_ShowCharString/ct_Type3ShowCharString load def -/ct_dfSetCacheProc/ct_CloneSetCacheProc load def/ct_SyntheticBold false def -/ct_StrokeWidth 1 def}{/FontType 4 def/Private 1 dict dup/lenIV 4 put def -/CharStrings 1 dict dup/.notdefput def/PaintType 0 def -/ct_ShowCharString/ct_Type4ShowCharString load def}ifelse/ct_str1 1 string def -currentdict end def/BaseFontDictSize BaseFontTemplate length 5 add def -/ct_matrixeq{true 0 1 5{dup 4 index exch get exch 3 index exch get eq and dup -not{exit}if}for exch pop exch pop}bind def/ct_makeocf{15 dict begin exch/WMode -exch def exch/FontName exch def/FontType 0 def/FMapType 2 def/FontMatrix -matrix def/bfCount 1 index/CIDCount get 256 idiv 1 add dup 256 gt{pop 256}if -def/Encoding 256 array 0 1 bfCount 1 sub{2 copy dup put pop}for bfCount 1 255{ -2 copy bfCount put pop}for def/FDepVector bfCount dup 256 lt{1 add}if array -def BaseFontTemplate BaseFontDictSize dict copy begin/CIDFont exch def CIDFont -/FontBBox known{CIDFont/FontBBox get/FontBBox exch def}if CIDFont/CDevProc -known{CIDFont/CDevProc get/CDevProc exch def}if currentdict end -BaseFontNameStr 3(0)putinterval 0 1 bfCount dup 256 eq{1 sub}if{FDepVector -exch 2 index BaseFontDictSize dict copy begin dup/CIDFirstByte exch 256 mul -def FontType 3 eq{/ct_FDDict 2 dict def}if currentdict end 1 index 16 -BaseFontNameStr 2 2 getinterval cvrs pop BaseFontNameStr exch definefont put} -for ct_Clone?{/Widths 1 index/CIDFont get/GlyphDirectory get length dict def} -if FontName currentdict end definefont ct_Clone?{gsave dup 1000 scalefont -setfont ct_BuildCharDict begin/usewidths? false def currentfont/Widths get -begin exch/CIDFont get/GlyphDirectory get{pop dup charcode exch 1 index 0 2 -index 256 idiv put 1 index exch 1 exch 256 mod put stringwidth 2 array astore -def}forall end/usewidths? true def end grestore}{exch pop}ifelse}bind def -/ct_ComposeFont{ct_UseNativeCapability?{2 index/CMap ct_resourcestatus{pop pop -exch pop}{/CIDInit/ProcSet findresource begin 12 dict begin begincmap/CMapName -3 index def/CMapVersion 1 def/CMapType 1 def exch/WMode exch def/CIDSystemInfo -3 dict dup begin/Registry(Adobe)def/Ordering CMapName ct_mkocfStr100 cvs -(Adobe-)search{pop pop(-)search{dup length string copy exch pop exch pop}{pop -(Identity)}ifelse}{pop(Identity)}ifelse def/Supplement 0 def end def 1 -begincodespacerange<0000>endcodespacerange 1 begincidrange<0000>0 -endcidrange endcmap CMapName currentdict/CMap defineresource pop end end} -ifelse composefont}{3 2 roll pop 0 get/CIDFont findresource ct_makeocf}ifelse} -bind def/ct_MakeIdentity{ct_UseNativeCapability?{1 index/CMap -ct_resourcestatus{pop pop}{/CIDInit/ProcSet findresource begin 12 dict begin -begincmap/CMapName 2 index def/CMapVersion 1 def/CMapType 1 def/CIDSystemInfo -3 dict dup begin/Registry(Adobe)def/Ordering CMapName ct_mkocfStr100 cvs -(Adobe-)search{pop pop(-)search{dup length string copy exch pop exch pop}{pop -(Identity)}ifelse}{pop(Identity)}ifelse def/Supplement 0 def end def 1 -begincodespacerange<0000>endcodespacerange 1 begincidrange<0000>0 -endcidrange endcmap CMapName currentdict/CMap defineresource pop end end} -ifelse composefont}{exch pop 0 get/CIDFont findresource ct_makeocf}ifelse}bind -def currentdict readonly pop end end -%%EndResource -Adobe_CoolType_Core begin /$Oblique SetSubstituteStrategy end -%%BeginResource: procset Adobe_AGM_Image 1.0 0 -%%Version: 1.0 0 -%%Copyright: Copyright (C) 2000-2000 Adobe Systems, Inc. All Rights Reserved. -systemdict /setpacking known -{ - currentpacking - true setpacking -} if -userdict /Adobe_AGM_Image 65 dict dup begin put -/Adobe_AGM_Image_Id /Adobe_AGM_Image_1.0_0 def -/nd{ - null def -}bind def -/AGMIMG_&image nd -/AGMIMG_&colorimage nd -%%don't initialize AGMIMG_&customcolorimage, it wrecks havoc in a nested environment -%%AGMIMG_ccimage_exists not {/AGMIMG_&customcolorimage nd} if -/AGMIMG_&imagemask nd -/AGMIMG_mbuf () def -/AGMIMG_ybuf () def -/AGMIMG_kbuf () def -/AGMIMG_c 0 def -/AGMIMG_m 0 def -/AGMIMG_y 0 def -/AGMIMG_k 0 def -/AGMIMG_tmp nd -/AGMIMG_imagestring0 nd -/AGMIMG_imagestring1 nd -/AGMIMG_imagestring2 nd -/AGMIMG_imagestring3 nd -/AGMIMG_imagestring4 nd -/AGMIMG_imagestring5 nd -/AGMIMG_cnt nd -/AGMIMG_fsave nd -/AGMIMG_colorAry nd -/AGMIMG_override nd -/AGMIMG_name nd -/invert_image_samples nd -/knockout_image_samples nd -/img nd -/sepimg nd -/idximg nd -/doc_setup -{ - Adobe_AGM_Core begin - Adobe_AGM_Image begin - /AGMIMG_&image systemdict/image get def - /AGMIMG_&imagemask systemdict/imagemask get def - /colorimage where{ - pop - /AGMIMG_&colorimage /colorimage ldf - }if - end - end -}def -/page_setup -{ - Adobe_AGM_Image begin - /AGMIMG_ccimage_exists {/customcolorimage where - { - pop - /Adobe_AGM_OnHost_Seps where - { - pop false - }{ - /Adobe_AGM_InRip_Seps where - { - pop false - }{ - true - }ifelse - }ifelse - }{ - false - }ifelse - }bdf - level2{ - /invert_image_samples - { - Adobe_AGM_Image/AGMIMG_tmp Decode length ddf - /Decode [ Decode 1 get Decode 0 get] def - }def - /knockout_image_samples - { - Operator/imagemask ne{ - /Decode [1 1] def - }if - }def - }{ - /invert_image_samples - { - {1 exch sub} currenttransfer addprocs settransfer - }def - /knockout_image_samples - { - { pop 1 } currenttransfer addprocs settransfer - }def - }ifelse - /img /imageormask ldf - /sepimg /sep_imageormask ldf - /idximg /indexed_imageormask ldf - currentdict{ - dup xcheck 1 index type dup /arraytype eq exch /packedarraytype eq or and{ - bind - }if - def - }forall -}def -/page_trailer -{ - end -}def -/doc_trailer -{ -}def -/imageormask_sys -{ - begin - save mark - level2{ - currentdict - Operator /imagemask eq{ - AGMIMG_&imagemask - }{ - AGMIMG_&image - }ifelse - }{ - Width Height - Operator /imagemask eq{ - Decode 0 get 1 eq Decode 1 get 0 eq and - ImageMatrix /DataSource load - AGMIMG_&imagemask - }{ - BitsPerComponent ImageMatrix /DataSource load - AGMIMG_&image - }ifelse - }ifelse - cleartomark restore - end -}def -/overprint_plate -{ - currentoverprint{ - 0 get - dup /DeviceGray eq{ - pop AGMCORE_black_plate not - }{ - /DeviceCMYK eq{ - AGMCORE_is_cmyk_sep not - }if - }ifelse - }{ - false - }ifelse -}def -/imageormask -{ - begin - SkipImageProc not{ - save mark - level2 AGMCORE_host_sep not and{ - currentdict - Operator /imagemask eq{ - imagemask - }{ - AGMCORE_in_rip_sep currentoverprint and currentcolorspace 0 get /DeviceGray eq and{ - [/Separation /Black /DeviceGray {}] setcolorspace - /Decode [ Decode 1 get Decode 0 get ] def - }if - image - }ifelse - }{ - Width Height - Operator /imagemask eq{ - Decode 0 get 1 eq Decode 1 get 0 eq and - ImageMatrix /DataSource load - AGMCORE_host_sep{ - currentgray 1 ne{ - currentdict imageormask_sys - }{ - currentoverprint not{ - 1 AGMCORE_&setgray - knockout_image_samples - currentdict imageormask_sys - }{ - currentdict ignoreimagedata - }ifelse - }ifelse - }{ - imagemask - }ifelse - }{ - BitsPerComponent ImageMatrix - MultipleDataSources{ - 0 1 NComponents 1 sub{ - DataSource exch get - }for - }{ - /DataSource load - }ifelse - Operator /colorimage eq{ - AGMCORE_host_sep{ - MultipleDataSources level2 or NComponents 4 eq and{ - MultipleDataSources{ - 4 {pop} repeat - /DataSource [ - DataSource 0 get /exec cvx - DataSource 1 get /exec cvx - DataSource 2 get /exec cvx - DataSource 3 get /exec cvx - /AGMCORE_get_ink_data cvx - ] cvx def - }{ - /DataSource /DataSource load filter_cmyk 0 () /SubFileDecode filter def - }ifelse - - /Decode [ Decode 0 get Decode 1 get ] def - /MultipleDataSources false def - /NComponents 1 def - /Operator /image def - AGMCORE_is_cmyk_sep{ - currentoverprint InksUsed current_ink not and{ - currentdict consumeimagedata - }{ - invert_image_samples - 1 AGMCORE_&setgray - currentdict imageormask_sys - }ifelse - }{ - currentdict ignoreimagedata - }ifelse - }{ - - MultipleDataSources NComponents AGMIMG_&colorimage - }ifelse - }{ - true NComponents colorimage - }ifelse - }{ - Operator /image eq{ - AGMCORE_host_sep{ - /DoImage true def - HostSepColorImage{ - invert_image_samples - }{ - AGMCORE_black_plate not{ - /DoImage false def - currentdict ignoreimagedata - }if - }ifelse - 1 AGMCORE_&setgray - DoImage - {currentdict imageormask_sys} if - }{ - image - }ifelse - }{ - Operator/knockout eq{ - pop pop pop pop pop - currentoverprint InksUsed current_ink not and{ - }{ - currentcolorspace overprint_plate not{ - knockout_unitsq - }if - }ifelse - }if - }ifelse - }ifelse - }ifelse - }ifelse - cleartomark restore - }if - end -}def -/sep_imageormask -{ - /sep_colorspace_dict AGMCORE_gget begin - /MappedCSA CSA map_csa def - begin - SkipImageProc not{ - save mark - - AGMCORE_avoid_L2_sep_space{ - /Decode [ Decode 0 get 255 mul Decode 1 get 255 mul ] def - }if - AGMIMG_ccimage_exists - MappedCSA 0 get /DeviceCMYK eq and - currentdict/Components known and - Name () ne and - Name (All) ne and - Operator /image eq and - AGMCORE_producing_seps not and - level2 not and - { - Width Height BitsPerComponent ImageMatrix - [ - /DataSource load /exec cvx - { - 0 1 2 index length 1 sub{ - 1 index exch - 2 copy get 255 xor put - }for - } /exec cvx - ] cvx bind - MappedCSA 0 get /DeviceCMYK eq{ - Components aload pop - }{ - 0 0 0 Components aload pop 1 exch sub - }ifelse - Name findcmykcustomcolor - customcolorimage - }{ - AGMCORE_producing_seps not{ - level2{ - AGMCORE_avoid_L2_sep_space not currentcolorspace 0 get /Separation ne and{ - [/Separation Name MappedCSA sep_proc_name exch 0 get exch load ] setcolorspace_opt - /sep_tint AGMCORE_gget setcolor - }if - currentdict imageormask - }{ - currentdict - Operator /imagemask eq{ - imageormask - }{ - sep_imageormask_lev1 - }ifelse - }ifelse - }{ - AGMCORE_host_sep{ - Operator/knockout eq{ - currentoverprint InksUsed current_ink not and{ - }{ - currentdict/ImageMatrix get concat - knockout_unitsq - }ifelse - }{ - currentgray 1 ne{ - AGMCORE_is_cmyk_sep Name (All) ne and{ - level2{ - [ /Separation Name [/DeviceGray] - { - sep_colorspace_proc AGMCORE_get_ink_data - 1 exch sub - } bind - ] AGMCORE_&setcolorspace - /sep_tint AGMCORE_gget AGMCORE_&setcolor - currentdict imageormask_sys - }{ - currentdict - Operator /imagemask eq{ - imageormask_sys - }{ - sep_image_lev1_sep - }ifelse - }ifelse - }{ - Operator/imagemask ne{ - invert_image_samples - }if - currentdict imageormask_sys - }ifelse - }{ - currentdict consumeimagedata - currentoverprint not Name (All) eq or{ - gsave - knockout_unitsq - grestore - }if - }ifelse - }ifelse - }{ - currentcolorspace 0 get /Separation ne{ - [/Separation Name MappedCSA sep_proc_name exch 0 get exch load ] setcolorspace_opt - /sep_tint AGMCORE_gget setcolor - }if - currentoverprint - MappedCSA 0 get /DeviceCMYK eq and - Name inRip_spot_has_ink not and - Name (All) ne and { - imageormask_l2_overprint - }{ - currentdict imageormask - }ifelse - }ifelse - }ifelse - }ifelse - cleartomark restore - }if - end - end -}def -/imageormask_l2_overprint -{ - - currentdict - currentcmykcolor add add add 0 eq{ - currentdict consumeimagedata - }{ - level3{ - - currentcmykcolor - /AGMIMG_k xdf - /AGMIMG_y xdf - /AGMIMG_m xdf - /AGMIMG_c xdf - Operator/imagemask eq{ - [/DeviceN [ - AGMIMG_c 0 ne {/Cyan} if - AGMIMG_m 0 ne {/Magenta} if - AGMIMG_y 0 ne {/Yellow} if - AGMIMG_k 0 ne {/Black} if - ] /DeviceCMYK {}] setcolorspace - - AGMIMG_c 0 ne {AGMIMG_c} if - AGMIMG_m 0 ne {AGMIMG_m} if - AGMIMG_y 0 ne {AGMIMG_y} if - AGMIMG_k 0 ne {AGMIMG_k} if - setcolor - }{ - /Decode [ Decode 0 get 255 mul Decode 1 get 255 mul ] def - [/Indexed - [ - /DeviceN [ - AGMIMG_c 0 ne {/Cyan} if - AGMIMG_m 0 ne {/Magenta} if - AGMIMG_y 0 ne {/Yellow} if - AGMIMG_k 0 ne {/Black} if - ] - /DeviceCMYK { - AGMIMG_k 0 eq {0} if - AGMIMG_y 0 eq {0 exch} if - AGMIMG_m 0 eq {0 3 1 roll} if - AGMIMG_c 0 eq {0 4 1 roll} if - } - ] - 255 - { - 255 div - - mark exch - dup dup dup - - - AGMIMG_k 0 ne{ - /sep_tint AGMCORE_gget mul MappedCSA sep_proc_name exch pop load exec 4 1 roll pop pop pop - counttomark 1 roll - }{ - pop - }ifelse - - AGMIMG_y 0 ne{ - /sep_tint AGMCORE_gget mul MappedCSA sep_proc_name exch pop load exec 4 2 roll pop pop pop - counttomark 1 roll - }{ - pop - }ifelse - - AGMIMG_m 0 ne{ - /sep_tint AGMCORE_gget mul MappedCSA sep_proc_name exch pop load exec 4 3 roll pop pop pop - counttomark 1 roll - }{ - pop - }ifelse - - AGMIMG_c 0 ne{ - /sep_tint AGMCORE_gget mul MappedCSA sep_proc_name exch pop load exec pop pop pop - counttomark 1 roll - }{ - pop - }ifelse - counttomark 1 add -1 roll pop - } - ] setcolorspace - }ifelse - - imageormask_sys - }{ - write_image_file{ - currentcmykcolor - 0 ne{ - [/Separation /Black /DeviceGray {}] setcolorspace - gsave - /Black - [{1 exch sub /sep_tint AGMCORE_gget mul} /exec cvx MappedCSA sep_proc_name cvx exch pop {4 1 roll pop pop pop 1 exch sub} /exec cvx] - cvx modify_halftone_xfer - Operator currentdict read_image_file - grestore - }if - 0 ne{ - [/Separation /Yellow /DeviceGray {}] setcolorspace - gsave - /Yellow - [{1 exch sub /sep_tint AGMCORE_gget mul} /exec cvx MappedCSA sep_proc_name cvx exch pop {4 2 roll pop pop pop 1 exch sub} /exec cvx] - cvx modify_halftone_xfer - Operator currentdict read_image_file - grestore - }if - 0 ne{ - [/Separation /Magenta /DeviceGray {}] setcolorspace - gsave - /Magenta - [{1 exch sub /sep_tint AGMCORE_gget mul} /exec cvx MappedCSA sep_proc_name cvx exch pop {4 3 roll pop pop pop 1 exch sub} /exec cvx] - cvx modify_halftone_xfer - Operator currentdict read_image_file - grestore - }if - 0 ne{ - [/Separation /Cyan /DeviceGray {}] setcolorspace - gsave - /Cyan - [{1 exch sub /sep_tint AGMCORE_gget mul} /exec cvx MappedCSA sep_proc_name cvx exch pop {pop pop pop 1 exch sub} /exec cvx] - cvx modify_halftone_xfer - Operator currentdict read_image_file - grestore - } if - close_image_file - }{ - imageormask - }ifelse - }ifelse - }ifelse -} def -/indexed_imageormask -{ - begin - save mark - - currentdict - AGMCORE_host_sep{ - - Operator/knockout eq{ - /indexed_colorspace_dict AGMCORE_gget /CSA get map_csa overprint_plate not{ - knockout_unitsq - }if - }{ - AGMCORE_is_cmyk_sep{ - Operator /imagemask eq{ - imageormask_sys - }{ - level2{ - indexed_image_lev2_sep - }{ - indexed_image_lev1_sep - }ifelse - }ifelse - }{ - currentoverprint not{ - knockout_image_samples - imageormask_sys - }{ - currentdict consumeimagedata - }ifelse - }ifelse - }ifelse - }{ - level2{ - imageormask - }{ - Operator /imagemask eq{ - imageormask - }{ - indexed_imageormask_lev1 - }ifelse - }ifelse - }ifelse - cleartomark restore - end -}def -/indexed_image_lev2_sep -{ - /indexed_colorspace_dict AGMCORE_gget begin - begin - - currentcolorspace - dup 1 /DeviceGray put - dup 3 [ - currentcolorspace 3 get - { - exch 4 mul 4 getinterval {} forall - AGMCORE_get_ink_data 255 div 1 exch sub - } /exec cvx - ] cvx put - setcolorspace - - currentdict - Operator /imagemask eq{ - AGMIMG_&imagemask - }{ - AGMIMG_&image - }ifelse - - end end -}def -/OPIimage -{ - dup type /dicttype ne{ - 10 dict begin - /DataSource xdf - /ImageMatrix xdf - /BitsPerComponent xdf - /Height xdf - /Width xdf - /ImageType 1 def - /Decode [0 1 def] - currentdict - end - }if - dup begin - /NComponents 1 cdndf - /MultipleDataSources false cdndf - /SkipImageProc {false} cdndf - /HostSepColorImage false cdndf - /Decode [ - 0 - currentcolorspace 0 get /Indexed eq{ - 2 BitsPerComponent exp 1 sub - }{ - 1 - }ifelse - ] cdndf - /Operator /image cdndf - end - /sep_colorspace_dict AGMCORE_gget null eq{ - imageormask - }{ - gsave - dup begin invert_image_samples end - sep_imageormask - grestore - }ifelse -}def -/spot_alias -{ - /mapto_sep_imageormask - { - dup type /dicttype ne{ - 12 dict begin - /ImageType 1 def - /DataSource xdf - /ImageMatrix xdf - /BitsPerComponent xdf - /Height xdf - /Width xdf - /MultipleDataSources false def - }{ - begin - }ifelse - /Decode [/customcolor_tint AGMCORE_gget 0] def - /Operator /image def - /HostSepColorImage false def - /InksUsed [] def - /SkipImageProc {false} def - currentdict - end - sep_imageormask - }bdf - /customcolorimage - { - Adobe_AGM_Image/AGMIMG_colorAry xddf - /customcolor_tint AGMCORE_gget - bdict - /Name AGMIMG_colorAry 4 get - /CSA [ /DeviceCMYK ] - /TintMethod /Subtractive - /TintProc null - /MappedCSA null - /NComponents 4 - /Components [ AGMIMG_colorAry aload pop pop ] - edict - setsepcolorspace - mapto_sep_imageormask - }ndf - Adobe_AGM_Image/AGMIMG_&customcolorimage /customcolorimage load put - /customcolorimage - { - Adobe_AGM_Image/AGMIMG_override false put - dup 4 get map_alias{ - /customcolor_tint AGMCORE_gget exch setsepcolorspace - pop - mapto_sep_imageormask - }{ - AGMIMG_&customcolorimage - }ifelse - }bdf -}def -level2 not{ - /colorbuf - { - 0 1 2 index length 1 sub{ - dup 2 index exch get - 255 exch sub - 2 index - 3 1 roll - put - }for - }def - /tint_image_to_color - { - begin - Width Height BitsPerComponent ImageMatrix - /DataSource load - end - Adobe_AGM_Image begin - /AGMIMG_mbuf 0 string def - /AGMIMG_ybuf 0 string def - /AGMIMG_kbuf 0 string def - { - colorbuf dup length AGMIMG_mbuf length ne - { - dup length dup dup - /AGMIMG_mbuf exch string def - /AGMIMG_ybuf exch string def - /AGMIMG_kbuf exch string def - } if - dup AGMIMG_mbuf copy AGMIMG_ybuf copy AGMIMG_kbuf copy pop - } - addprocs - {AGMIMG_mbuf}{AGMIMG_ybuf}{AGMIMG_kbuf} true 4 colorimage - end - } def - /sep_imageormask_lev1 - { - begin - MappedCSA 0 get dup /DeviceRGB eq exch /DeviceCMYK eq or has_color not and{ - - { - 255 mul round cvi GrayLookup exch get - } currenttransfer addprocs settransfer - currentdict imageormask - }{ - /sep_colorspace_dict AGMCORE_gget/Components known{ - MappedCSA 0 get /DeviceCMYK eq{ - Components aload pop - }{ - 0 0 0 Components aload pop 1 exch sub - }ifelse - - Adobe_AGM_Image/AGMIMG_k xddf - Adobe_AGM_Image/AGMIMG_y xddf - Adobe_AGM_Image/AGMIMG_m xddf - Adobe_AGM_Image/AGMIMG_c xddf - - AGMIMG_y 0.0 eq AGMIMG_m 0.0 eq and AGMIMG_c 0.0 eq and{ - {AGMIMG_k mul 1 exch sub} currenttransfer addprocs settransfer - currentdict imageormask - }{ - - currentcolortransfer - {AGMIMG_k mul 1 exch sub} exch addprocs 4 1 roll - {AGMIMG_y mul 1 exch sub} exch addprocs 4 1 roll - {AGMIMG_m mul 1 exch sub} exch addprocs 4 1 roll - {AGMIMG_c mul 1 exch sub} exch addprocs 4 1 roll - setcolortransfer - currentdict tint_image_to_color - }ifelse - }{ - - MappedCSA 0 get /DeviceGray eq { - {255 mul round cvi ColorLookup exch get 0 get} currenttransfer addprocs settransfer - currentdict imageormask - }{ - MappedCSA 0 get /DeviceCMYK eq { - currentcolortransfer - {255 mul round cvi ColorLookup exch get 3 get 1 exch sub} exch addprocs 4 1 roll - {255 mul round cvi ColorLookup exch get 2 get 1 exch sub} exch addprocs 4 1 roll - {255 mul round cvi ColorLookup exch get 1 get 1 exch sub} exch addprocs 4 1 roll - {255 mul round cvi ColorLookup exch get 0 get 1 exch sub} exch addprocs 4 1 roll - setcolortransfer - currentdict tint_image_to_color - }{ - currentcolortransfer - {pop 1} exch addprocs 4 1 roll - {255 mul round cvi ColorLookup exch get 2 get} exch addprocs 4 1 roll - {255 mul round cvi ColorLookup exch get 1 get} exch addprocs 4 1 roll - {255 mul round cvi ColorLookup exch get 0 get} exch addprocs 4 1 roll - setcolortransfer - currentdict tint_image_to_color - }ifelse - }ifelse - }ifelse - }ifelse - end - }def - /sep_image_lev1_sep - { - begin - /sep_colorspace_dict AGMCORE_gget/Components known{ - Components aload pop - - Adobe_AGM_Image/AGMIMG_k xddf - Adobe_AGM_Image/AGMIMG_y xddf - Adobe_AGM_Image/AGMIMG_m xddf - Adobe_AGM_Image/AGMIMG_c xddf - - {AGMIMG_c mul 1 exch sub} - {AGMIMG_m mul 1 exch sub} - {AGMIMG_y mul 1 exch sub} - {AGMIMG_k mul 1 exch sub} - }{ - {255 mul round cvi ColorLookup exch get 0 get 1 exch sub} - {255 mul round cvi ColorLookup exch get 1 get 1 exch sub} - {255 mul round cvi ColorLookup exch get 2 get 1 exch sub} - {255 mul round cvi ColorLookup exch get 3 get 1 exch sub} - }ifelse - - AGMCORE_get_ink_data currenttransfer addprocs settransfer - - currentdict imageormask_sys - - end - }def - /indexed_imageormask_lev1 - { - /indexed_colorspace_dict AGMCORE_gget begin - begin - currentdict - MappedCSA 0 get dup /DeviceRGB eq exch /DeviceCMYK eq or has_color not and{ - - {HiVal mul round cvi GrayLookup exch get HiVal div} currenttransfer addprocs settransfer - imageormask - }{ - - MappedCSA 0 get /DeviceGray eq { - {HiVal mul round cvi Lookup exch get HiVal div} currenttransfer addprocs settransfer - imageormask - }{ - MappedCSA 0 get /DeviceCMYK eq { - currentcolortransfer - {4 mul HiVal mul round cvi 3 add Lookup exch get HiVal div 1 exch sub} exch addprocs 4 1 roll - {4 mul HiVal mul round cvi 2 add Lookup exch get HiVal div 1 exch sub} exch addprocs 4 1 roll - {4 mul HiVal mul round cvi 1 add Lookup exch get HiVal div 1 exch sub} exch addprocs 4 1 roll - {4 mul HiVal mul round cvi Lookup exch get HiVal div 1 exch sub} exch addprocs 4 1 roll - setcolortransfer - tint_image_to_color - }{ - currentcolortransfer - {pop 1} exch addprocs 4 1 roll - {3 mul HiVal mul round cvi 2 add Lookup exch get HiVal div} exch addprocs 4 1 roll - {3 mul HiVal mul round cvi 1 add Lookup exch get HiVal div} exch addprocs 4 1 roll - {3 mul HiVal mul round cvi Lookup exch get HiVal div} exch addprocs 4 1 roll - setcolortransfer - tint_image_to_color - }ifelse - }ifelse - }ifelse - end end - }def - /indexed_image_lev1_sep - { - /indexed_colorspace_dict AGMCORE_gget begin - begin - {4 mul HiVal mul round cvi Lookup exch get HiVal div 1 exch sub} - {4 mul HiVal mul round cvi 1 add Lookup exch get HiVal div 1 exch sub} - {4 mul HiVal mul round cvi 2 add Lookup exch get HiVal div 1 exch sub} - {4 mul HiVal mul round cvi 3 add Lookup exch get HiVal div 1 exch sub} - - AGMCORE_get_ink_data currenttransfer addprocs settransfer - - currentdict imageormask_sys - - end end - }def -}if -end -systemdict /setpacking known -{ - setpacking -} if -%%EndResource -%ADOBeginClientInjection: DocumentProlog End "AI10" -%ADOEndClientInjection: DocumentProlog End "AI10" -currentdict Adobe_AGM_Utils eq {end} if -%%EndProlog -%%BeginSetup -%ADOBeginClientInjection: DocumentSetup Start "AI10" -%ADOEndClientInjection: DocumentSetup Start "AI10" -Adobe_AGM_Utils begin -2 2010 true Adobe_AGM_Core/doc_setup get exec -Adobe_CoolType_Core/doc_setup get exec -Adobe_AGM_Image/doc_setup get exec -%ADOBeginClientInjection: DocumentSetup End "AI10" -%ADOEndClientInjection: DocumentSetup End "AI10" -currentdict Adobe_AGM_Utils eq {end} if -%%EndSetup -%%Page: slalib.eps 1 -%%EndPageComments -%%BeginPageSetup -%ADOBeginClientInjection: PageSetup Start "AI10" -%ADOEndClientInjection: PageSetup Start "AI10" -Adobe_AGM_Utils begin -Adobe_AGM_Core/page_setup get exec -Adobe_CoolType_Core/page_setup get exec -Adobe_AGM_Image/page_setup get exec -%ADOBeginClientInjection: PageSetup End "AI10" -%ADOEndClientInjection: PageSetup End "AI10" -%%EndPageSetup -Adobe_AGM_Core/AGMCORE_save save ddf -1 -1 scale 0 -470.717 translate -[1 0 0 1 0 0 ] concat -mark -/0 -[/DeviceGray] add_csa -/CSA /0 -/1 -[/DeviceCMYK] add_csa -/CSA /1 -/2 -[/DeviceRGB] add_csa -/CSA /2 -cleartomark -800 path_rez -% page clip -gsave -newpath -gsave % PSGState -0 0 mo -0 470.717 li -151.127 470.717 li -151.127 0 li -clp -[1 0 0 1 0 0 ] concat -%ADOBeginClientInjection: BeginPageContent "AI10" -%ADOEndClientInjection: BeginPageContent "AI10" -gsave % PSGState -0 0 mo -151 0 li -151 471 li -0 471 li -0 0 li -clp -70.562 434.872 mo -75.5479 443.507 li 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0 cmyk -f -149.165 349.067 mo -1.96289 349.067 li -1.96289 364.665 li -149.165 364.665 li -149.165 349.067 li -0 0 0 0 cmyk -f -0 0 0 1 cmyk -%ADOBeginSubsetFont: SwitzerlandPlain Initial -11 dict begin -/FontName /SwitzerlandPlain def -/FontMatrix [1 1000 div 0 0 1 1000 div 0 0 ] def -/Encoding 256 array 0 1 255 {1 index exch /.notdef put} for def -/PaintType 0 def -/FontType 1 def -/FontBBox { 0 0 0 0 } def -/FontInfo 1 dict dup begin - /OrigFontType /TrueType def -end readonly def -currentdict -end - -systemdict begin -dup /Private 7 dict dup begin -/BlueValues [-15 0 600 650] def -/MinFeature {16 16} def -/password 5839 def -/ND {def} def -/NP {put} def -/RD {string currentfile exch readhexstring pop} def -2 index /CharStrings 213 dict dup begin -/.notdef -<10bf317005b6d50bd3b903bc9f60e6e804630266f839393d56ae50cbf672 -fad4fea4e66b781c5b13aed0b3> ND -/space -<10bf317079c770d631> ND -/parenleft -<10bf31703d39c8e26f012f215855c39a8b6fb0b9350d012940cca5f23d54 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-5A817A5F10DA33F5CBC8979A7DDA71B3AB -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -0000000000000000000000000000000000000000000000000000000000000000 -cleartomark -/Symbol findfont /Encoding get -dup 97 /alpha put -dup 100 /delta put -pop -%ADOEndSubsetFont -/Symbol*1 -[ -97{/.notdef}repeat /alpha 2{/.notdef}repeat /delta 155{/.notdef}repeat -] /Symbol nfnt -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -96.839 137.521 mov -(a) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -106.935 137.521 mov -(, ) sh -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -115.802 137.521 mov -(d) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -123.706 137.521 mov -(\)) sh -22.7014 199.09 mov -(Apparent \(h, ) sh -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -115.209 199.09 mov -(d) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -123.113 199.09 mov -(\)) sh -14.262 264.509 mov -1.77734 0 111 -1.77734 0 (Top) awsh -40.0823 264.509 mov -(ocentric \(h, ) sh -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -123.649 264.509 mov -(d) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -131.552 264.509 mov -(\)) sh -3.98145 327.724 mov -1.77734 0 111 -1.77734 0 (Top) awsh -29.8018 327.724 mov -(ocentric \(Az, Alt\)) sh -10.2197 394.683 mov -(Observed \(Az, Alt\)) sh -27.5264 167.642 mov -(Earth rotation) sh -11.9326 233.831 mov -(Diurnal aberration) sh -39.0869 362.359 mov -(Refraction) sh -17.8713 296.834 mov -(\(h, ) sh -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -40.9612 296.834 mov -(d) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -48.865 296.834 mov -(\) to \(Az, Alt\)) sh -26.9972 19.436 mov -(Catalog \() sh -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -91.9503 19.436 mov -(a) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -102.046 19.436 mov -(, ) sh -/Symbol*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -110.913 19.436 mov -(d) sh -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -118.817 19.436 mov -(\)) sh -12.3779 38.436 mov -(J2000, geocentric) sh -150.627 443.897 mo -.5 443.897 li -.5 470.217 li -150.627 470.217 li -150.627 443.897 li -0 0 0 0 cmyk -f -150.627 443.897 mo -.5 443.897 li -.5 470.217 li -150.627 470.217 li -150.627 443.897 li -cp -0 0 0 1 cmyk -s -149.165 414.796 mo -1.96289 414.796 li -1.96289 430.394 li -149.165 430.394 li -149.165 414.796 li -0 0 0 0 cmyk -f -0 0 0 1 cmyk -%ADOBeginSubsetFont: SwitzerlandPlain AddGlyphs - -systemdict begin -/SwitzerlandPlain -findfont dup -/Private get begin -/CharStrings get begin -systemdict /gcheck known {currentglobal currentdict gcheck setglobal} if -/period -<10bf317013061ae4b395170a1de13a7b0c431dcde57e5ecebb> ND -/M -<10bf317021c268885041a821075d00f34ad3a76ccf2c2f2877ceb684c158 -004c8ec7f975e2eb982f7b3a9bfd058377b85a151242fc04e73ca4fa9c> ND -/P -<10bf317013087f8385570c540d0515ceb9cfdcd2b5bce1be9e2cf9021ef5 -2bd1ea19d93084f2002fd39f7f05b2e0571dcfc0ae0fbd22777fdf0d82a7 -a36634bec110e58bc4f5bf779d89f2aebb62dcfcaadc5ec86efd31f5ea04 -32499c701a> ND -systemdict /gcheck known {setglobal} if end end -end -/SwitzerlandPlain findfont /Encoding get -dup 46 /period put -dup 77 /M put -dup 80 /P put -pop -%ADOEndSubsetFont -/SwitzerlandPlain*1 -[ -32{/.notdef}repeat /space 7{/.notdef}repeat /parenleft /parenright 2{/.notdef}repeat /comma /.notdef -/period /slash /zero /.notdef /two 14{/.notdef}repeat /A /.notdef -/C /D /E 4{/.notdef}repeat /J 2{/.notdef}repeat /M /.notdef -/O /P /.notdef /R /.notdef /T 12{/.notdef}repeat /a -/b /c /d /e /f /g /h /i -2{/.notdef}repeat /l /.notdef /n /o /p /.notdef /r -/s /t /u /v 3{/.notdef}repeat /z 133{/.notdef}repeat -] /SwitzerlandPlain nfnt -/SwitzerlandPlain*1 findfont [16 0 0 -16 0 0 ]mfnt sfnt -13.2666 462.723 mov -1.77734 0 101 -1.77734 0 (Tel) awsh -33.7432 462.723 mov -(escope Coord.) sh -22.5947 428.088 mov -(Pointing Model) sh -grestore % PSGState -%ADOBeginClientInjection: EndPageContent "AI10" -userdict /annotatepage 2 copy known {get exec}{pop pop} ifelse -%ADOEndClientInjection: EndPageContent "AI10" -% page clip -grestore -grestore % PSGState -Adobe_AGM_Core/AGMCORE_save get restore -%%PageTrailer -%ADOBeginClientInjection: PageTrailer Start "AI10" -%ADOEndClientInjection: PageTrailer Start "AI10" -Adobe_AGM_Image/page_trailer get exec -Adobe_CoolType_Core/page_trailer get exec -Adobe_AGM_Core/page_trailer get exec -currentdict Adobe_AGM_Utils eq {end} if -%ADOBeginClientInjection: PageTrailer End "AI10" -%ADOEndClientInjection: PageTrailer End "AI10" -%%Trailer -%ADOBeginClientInjection: DocumentTrailer Start "AI10" -%ADOEndClientInjection: DocumentTrailer Start "AI10" -Adobe_AGM_Image/doc_trailer get exec -Adobe_CoolType_Core/doc_trailer get exec -Adobe_AGM_Core/doc_trailer get exec -%ADOBeginClientInjection: DocumentTrailer End "AI10" -%ADOEndClientInjection: DocumentTrailer End "AI10" -%%EOF -%AI9_PrintingDataEnd - -userdict /AI9_read_buffer 256 string put -userdict begin -/ai9_skip_data -{ - mark - { - currentfile AI9_read_buffer { readline } stopped - { - } - { - not - { - exit - } if - (%AI9_PrivateDataEnd) eq - { - exit - } if - } ifelse - } loop - cleartomark -} def -end -userdict /ai9_skip_data get exec -%AI9_PrivateDataBegin -%!PS-Adobe-3.0 EPSF-3.0 -%%Creator: Adobe Illustrator(R) 10.0 -%%AI8_CreatorVersion: 10.0 -%%For: (Robert Wagner) (TUM) -%%Title: (slalib-drpaper.eps) -%%CreationDate: 5/26/2008 11:47 PM -%AI9_DataStream -%Gas`+?*>QbFf'H!!WRp2(C"^"W%.QW60_4NXWF0?[U@3?+,raB5r)%;cH<66%pO(Ls8+oSA46cEEim=n`fr?f!Sr5HF!2a2Z)hL>CiqfcOu 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title = {\url{http://www.mpi-hd.mpg.de/hfm/CosmicRay/shower.png}}, year=2006} -@MISC{www:showerartist, key = {{www-06}}, title = {\url{http://abyss.uoregon.edu/~js/glossary/cosmic_rays.html}}, year=2006} -@MISC{www:mars, key = {{www-07}}, title = {\url{http://magic.astro.uni-wuerzburg.de/mars/}}, year=2006} -@MISC{www:google, key = {{www-08}}, title = {\url{http://earth.google.com}}, year=2006} -@MISC{www:slalib, key = {{www-09}}, title = {\url{http://star-www.rl.ac.uk/star/docs/sun67.htx/sun67.html}}, year=2006} -@MISC{www:root, key = {{The ROOT System Home Page}}, title = {\url{http://root.cern.ch}}, year=2008} -@MISC{www:htmldoc, key = {{www-11}}, title = {\url{http://magic.astro.uni-wuerzburg.de/mars/htmldoc/}}, year=2006} -@MISC{www:mysql, key = {{www-12}}, title = {\url{http://www.mysql.com}}, year=2006} -@MISC{www:unified, key = {{www-13}}, title = {\url{http://chandra.harvard.edu/resources/illustrations/quasar.html}}, year=2006, note={Credit: NASA/CXC, Melissa Weiss}} -@MISC{www:asdc, key = {{www-14}}, title = {\url{http://www.asdc.asi.it/blazars/}}, year=2006} -@MISC{www:kva, key = {{www-15}}, title = {\url{http://tur3.tur.iac.es/}}, year=2006} -@MISC{www:integral, key = {{www-16}}, title = {\url{http://altamira.asu.cas.cz/iblwg/show.php?id=131}}, year=2006} -@MISC{www:ned, key = {{www-17}}, title = {\url{http://nedwww.ipac.caltech.edu/cgi-bin/nph-objsearch?objname=1es1218+304}}, year=2006} -@MISC{www:gcn, key = {{GCN}}, title = {\url{http://gcn.gsfc.nasa.gov}}, year=2008} - -%@MISC{www:BH1m, key = {{www-02}}, title = {\url{http://www.gsfc.nasa.gov/gsfc/spacesci/pictures/blackhole/BH1m.jpg}}, year=2006} -%@MISC{www:hillas, key = {{www-10}}, title = {\url{http://lpnhe-auger.in2p3.fr/slides/hillas.ps}}, year=2006} -%@MISC{www:agnartist2, key = {{www-03}}, title = {\url{http://upload.wikimedia.org/wikipedia/en/4/40/Galaxies_AGN_Inner-Structure-of.jpg}}, year=2006} - - -@BOOK{Peebles:1983, - author = {Peebles, Philip~James~Edwin}, - title = {Principles of Physical Cosmology}, - publisher = {Princton Series in Physics}, - year = 1983 -} - -@BOOK{Weekes:2003, - author = {Weekes, T.~C.}, - title = {Very high energy gamma-ray astronomy}, - series = {Astronomy and Astrophysics}, - publisher = {Institute of Physics Publishing}, - year = 2003 -} - -@BOOK{Rybicki:1979, - author = {{Rybicki}, George B. and {Lightman}, Alan P.}, - title = "Radiative Processes in Astrophysics", - publisher = { Wiley-Interscience }, - year = 1979 -} - -@BOOK{Begelman:1995, - author = {Begelman, M. and Rees, M.}, - title = "{Gravity's Fatal Attraction: Black Holes in the Universe}", - year = 1995, -publisher = {Scientific American Library} -} - -@BOOK{Mueller:2005, - author = {{M\"uller}, A.}, - title = "{Lexikon der Astrophysik}", - year = 2005, - month = sep, - url = {http://www.mpe.mpg.de/~amueller} -} - -@BOOK{Zensus:1987, - author = {{Pearson}, T.~J. and {Zensus}, J.~A.}, - year = 1987, - title = {Superluminal radio sources}, - publisher = {Cambridge 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-@MASTERSTHESIS{Bretz:1999, - author = {Bretz, T.}, - title = {Magnetfeldeigenschaften des {S}pektrometers {HADES}}, - school = {Technische Universit{\"a}t M{\"u}nchen}, - year = {1999} -} - -%MASTERSTHESIS{Doro:2005, -% author = {Doro, Michele}, -% year = {2005} -% - -@MISC{Giommi:2006, - author = { Giommi, P. and others}, - year = 2006, - howpublished = {in preparation} -} - -@MISC{Giommi:2005, - author = { Giommi, P.}, - year = 2006, - howpublished = {private communication} -} - -@ARTICLE{Dondi:1995, - author = {{Dondi}, L. and {Ghisellini}, G.}, - title = "{Gamma-ray-loud blazars and beaming}", - journal = {\mnras}, - year = 1995, - month = apr, - volume = 273, - pages = {583-595}, - asdurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995MNRAS.273..583D&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Fermi:1954, - author = {{Fermi}, E.}, - title = "{Galactic Magnetic Fields and the Origin of Cosmic Radiation.}", - journal = {\apj}, - year = 1954, - month = jan, - volume = 119, - pages = {1-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1954ApJ...119....1F&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Fermi:1949, - author = {{Fermi}, E.}, - journal = {Phys.~Rev.}, - volume = 75, - pages = 1169, - year = {1949} -} - -@ARTICLE{Wentzel:1963, - author = {{Wentzel}, D.~G.}, - title = "{Fermi Acceleration of Charged Particles.}", - journal = {\apj}, - year = 1963, - month = jan, - volume = 137, - pages = {135-+}, - adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1963ApJ...137..135W&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@BOOK{Spitzer:1956, - author = {{Spitzer}, L.}, - title = "{Physics of Fully Ionized gases}", -publisher = {Interscience, New York }, - year = 1956, -} - -@ARTICLE{Einstein:1905, - author = {{Einstein}, A.}, - title = "{Zur Elektrodynamik bewegter K{\"o}rper}", - journal = {Annalen der Physik}, - year = 1905, - volume = 17, - pages = {891-921}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1905AnP....17..891E&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Einstein:1916, - author = {{Einstein}, A.}, - title = "{Die Grundlage der allgemeinen Relativit{\"a}tstheorie}", - journal = {Annalen der Physik}, - year = 1916, - volume = 49, - pages = {769-822}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1916AnP....49..769E&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Eddington:1935a, - author = {{Eddington}, A.~S.}, - title = "{On "relativistic degeneracy,"}", - journal = {\mnras}, - year = 1935, - month = jan, - volume = 95, - pages = {194-206}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1935MNRAS..95..194E&db_key=AST}, - adsnote = {Provided by the 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pages = {8-16} -} - -@ARTICLE{LiMa:1983, - author = {{Li}, T.-P. and {Ma}, Y.-Q.}, - title = "{Analysis methods for results in gamma-ray astronomy}", - journal = {\apj}, - year = 1983, - month = sep, - volume = 272, - pages = {317-324}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1983ApJ...272..317L&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Bartko:2005pa, - author = {Bartko, H. and Gaug, M. and Moralejo, A. and Sidro, N.}, - collaboration = {MAGIC}, - title = {{FADC} pulse reconstruction using a digital filter for the {MAGIC} telescope}, - year = {2005}, - note = {astro-ph/0506459}, - eprint = {astro-ph/0506459}, - journal = {astro-ph}, - SLACcitation = {%%CITATION = ASTRO-PH 0506459;%%} -} - -@INPROCEEDINGS{Hillas:1985icrc, - author = {{Hillas}, A.~M.}, - title = {Cerenkov light images of {EAS} produced by primary gamma}, -booktitle = {$19^{th}$ International Cosmic Ray Conference}, - year = 1985, - month = Aug, - pages = {445-448}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ICRC....3..445H&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@INPROCEEDINGS{Blandford:1993, - author = {{Blandford, R.~D.}}, - title = {Gamma ray jets from active galactiv nuclei}, -booktitle = {Compton Gamma Ray Observatory}, - journal = {AIP Conf. Proc.}, - volume = 280, - year = 1993, - pages = {533}, - editor = {Gehrels} -} - -@ARTICLE{Kneiske:2004, - author = {{Kneiske}, T.~M. and {Bretz}, T. and {Mannheim}, K. and {Hartmann}, D.~H.}, - title = {Implications of cosmological gamma-ray absorption. {II}. Modification of gamma-ray spectra}, - journal = {\aap}, - year = 2004, - month = jan, - volume = 413, - pages = {807-815}, - adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004A%26A...413..807K&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Kneiske:2002, - author = {{Kneiske}, T.~M. and {Mannheim}, K. and {Hartmann}, D.~H.}, - title = {Implications of cosmological gamma-ray absorption. {I}. {E}volution of the metagalactic radiation field}, - journal = {\aap}, - year = 2002, - month = apr, - volume = 386, - pages = {1-11}, - adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2002A%26A...386....1K&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Hernandez:2005, - author = {{Hern{\'a}ndez-Rey}, J.~J.}, - title = "{The Neutrino Telescope Antares}", - journal = {\apss}, - year = 2005, - month = jun, - volume = 297, - pages = {257-267}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2005Ap%26SS.297..257H&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@INPROCEEDINGS{Bretz:2003icrc, - author = {{Bretz}, T.}, - title = {The {MAGIC} {A}nalysis and {R}econstruction {S}oftware}, -booktitle = {$28^{th}$ International Cosmic Ray Conference}, - year = 2003, - month = Aug -} - -@INPROCEEDINGS{Bretz:2004gamma, - author = {{Bretz}, T.}, - title = {{MARS} - {R}oadmap to a standard analysis}, -booktitle = {$2^{nd}$ International Symposium on High Energy Gamma-Ray Astronomy}, - year = 2004, - month = Jul -} - -@INPROCEEDINGS{Bretz:2008gamma, - author = {{Bretz}, T. and {Dorner}, D.}, - title = {{MARS} - {T}he {C}herenkov {O}bservatory edition}, -booktitle = {$3^{rd}$ International Symposium on High Energy Gamma-Ray Astronomy}, - year = 2008, - month = Jul -} - -@INPROCEEDINGS{Bretz:2005paris, - author = {{Bretz}, T. and Dorner, D.}, - title = {{MARS} - {A} framework for a standard analysis}, -booktitle = {Towards a network of atmospheric Cherenkov detectors VII}, - year = 2005, - month = Apr -} - -@INPROCEEDINGS{Dorner:2005paris, - author = {{Dorner}, D. and Bretz, T.}, - title = {A concept for data managment and processing}, -booktitle = {Towards a network of atmospheric Cherenkov detectors VII}, - pages = {571-575}, - year = 2005, - month = Apr -} - -@INPROCEEDINGS{Bastieri:2005, - author = {Bastieri, D. and others}, - title = {The mirrors of the {MAGIC} telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Dorner:2005icrc, - author = {Dorner, D. and Berger, K. and Bretz, T. and Gaug, M. and others}, - title = {Data Managment and Processing for the {MAGIC} telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - volume = 5, - pages = 175, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Beixeras:2005, - author = {Beixeras, C. and others}, - title = "{MAGIC II}", -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - volume = 5, - pages = {227}, - year = 2005, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Cortina:2005, - author = {Cortina, J. and others}, - title = {Technical performance of the {MAGIC} telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Bretz:2005mars, - author = {Bretz, T.}, - title = {Standard Analysis for the {MAGIC} Telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - volume = 4, - year = 2005, - pages = 315, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Gaug:2005, - author = {Gaug, M. and Bartko, H. and Cortina, J. and Rico, J. and others}, - title = {Calibration of the {MAGIC} telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Riegel:2005icrc, - author = {{Riegel}, B. and Bretz, T.}, - title = {A systematic study of the interdependance of the {IACT} image parameters}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - volume = 5, - pages = 215, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Riegel:2005icrc2, - author = {{Riegel}, B. and Bretz, T. and Dorner, D. and Wagner, R.~M.}, - title = {A tracking monitor for the {MAGIC} telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - volume = 5, - pages = 219, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Goebel:2005, - author = {{Goebel}, F. and Mase, K. and Meyer, M. and Mirzoyan, R. and Shayduk, M. and Teshima, M. and others}, - title = {Absolute energy scale calibration of the {MAGIC} telescope using muon images}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Majumdar:2005icrc, - author = {{Majumdar}, P. and {Moralejo}, A. and {Bigongiari}, C. and {Blanch}, O. and {Sobczynska}, D.}, - title = {{M}onte {C}arlo simulation for the {MAGIC} telescope}, -booktitle = {$29^{th}$ International Cosmic Ray Conference}, - year = 2005, - month = Aug, - note = {astro-ph/0508274} -} - -@INPROCEEDINGS{Meyer:2005icrc, - author = {{Meyer}, M. and Mannheim, K. and Bretz, T. and Dorner, D. and Riegel, B. and H\"ohne, D. and Berger, K. and others}, - title = {{MAGIC} observations of high-peaked {BL} {L}ac objects}, -booktitle = {$28^{th}$ International Cosmic Ray Conference}, - volume = 4, - pages = 335, - year = 2005, - month = Aug, - note = {astro-ph/0508273} -} - -@ARTICLE{Lessard:2001, - author = {{Lessard}, R.~W. and {Buckley}, J.~H. and {Connaughton}, V. and {Le Bohec}, S.}, - title = "{A new analysis method for reconstructing the arrival direction of TeV gamma rays using a single imaging atmospheric Cherenkov telescope}", - journal = {Astroparticle Physics}, - year = 2001, - month = mar, - volume = 15, - pages = {1-18}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001APh....15....1L&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Urry:1995, - author = {{Urry}, C.~M. and {Padovani}, P.}, - title = "{Unified Schemes for Radio-Loud Active Galactic Nuclei}", - journal = {\pasp}, - year = 1995, - month = sep, - volume = 107, - pages = {803-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995PASP..107..803U&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Urry:2000, - author = {{Urry}, C.~M. and {Scarpa}, R. and {O'Dowd}, M. and {Falomo}, R. and - {Pesce}, J.~E. and {Treves}, A.}, - title = "{The Hubble Space Telescope Survey of BL Lacertae Objects. II. Host Galaxies}", - journal = {\apj}, - year = 2000, - month = apr, - volume = 532, - pages = {816-829}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000ApJ...532..816U&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Porter:1960, - author = {Hill, D.~A. and Porter, N.~A}, - title = "{Photography of \v{C}erenkov Light from Extensive Air Showers in the Atmosphere}", - month = aug, - year = 1960, - journal = {\nat}, - volume = 191, - pages = 690, - note = {Letters to Editor} -} - -@ARTICLE{Jelley:1963, - author = {{Jelley}, J.~V. and {Porter}, N.~A.}, - title = "{{\v C}erenkov Radiation from the Night Sky, and its Application to {$\gamma$}-Ray Astronomy}", - journal = {\qjras}, - year = 1963, - month = sep, - volume = 4, - pages = {275-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1963QJRAS...4..275J&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Padovani:1995, - author = {{Padovani}, P. and {Giommi}, P.}, - title = "{The connection between x-ray- and radio-selected BL Lacertae objects}", - journal = {\apj}, - year = 1995, - month = may, - volume = 444, - pages = {567-581}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1995ApJ...444..567P&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Boella:1997, - author = {{Boella}, G. and {Butler}, R.~C. and {Perola}, G.~C. and {Piro}, L. and - {Scarsi}, L. and {Bleeker}, J.~A.~M.}, - title = "{BeppoSAX, the wide band mission for X-ray astronomy}", - journal = {\aaps}, - year = 1997, - month = apr, - volume = 122, - pages = {299-307}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997A%26AS..122..299B&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Catanese:1999, - author = {{Catanese}, M. and {Weekes}, T.~C.}, - title = "{Very High Energy Gamma-Ray Astronomy}", - journal = {\pasp}, - year = 1999, - month = oct, - volume = 111, - pages = {1193-1222}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999PASP..111.1193C&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Daum:1997, - author = {{Daum}, A. and others}, - title = "{First results on the performance of the HEGRA IACT array}", - journal = {Astroparticle Physics}, - year = 1997, - month = dec, - volume = 8, - pages = {1-2}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997APh.....8....1D&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Aharonian:2004, - author = {{Aharonian}, F. and others}, - title = "{Observations of 54 Active Galactic Nuclei with the HEGRA system of Cherenkov telescopes}", - journal = {\aap}, - year = 2004, - month = jul, - volume = 421, - pages = {529-537}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004A%26A...421..529A&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Pohl:2000, - author = {{Pohl}, M. and {Schlickeiser}, R.}, - title = "{On the conversion of blast wave energy into radiation in active galactic nuclei and gamma-ray bursts}", - journal = {\aap}, - year = 2000, - month = feb, - volume = 354, - pages = {395-410}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000A%26A...354..395P&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Mannheim:1993, - author = {{Mannheim}, K.}, - title = "{The proton blazar}", - journal = {\aap}, - year = 1993, - month = mar, - volume = 269, - pages = {67-76}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1993A%26A...269...67M&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -# CHECK AGAIN! -@INPROCEEDINGS{Sikora:2001, - author = {{Sikora}, M.}, - title = "{Jets in Quasars}", -booktitle = {ASP Conf. Ser. 227: Blazar Demographics and Physics}, - year = 2001, - pages = {95-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001ASPC..227...95S&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Sikora:1987, - author = {{Sikora}, M. and {Kirk}, J.~G. and {Begelman}, M.~C. and {Schneider}, P. - }, - title = "{Electron injection by relativistic protons in active galactic nuclei}", - journal = {\apjl}, - year = 1987, - month = sep, - volume = 320, - pages = {L81-L85}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987ApJ...320L..81S&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -# CHECK AGAIN -@ARTICLE{Burns:1982, - author = {{Burns}, M.~L. and {Lovelace}, R.~V.~E.}, - title = "{Theory of electron-positron showers in double radio sources}", - journal = {\apj}, - year = 1982, - month = nov, - volume = 262, - pages = {87-99}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982ApJ...262...87B&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Svensson:1987, - author = {{Svensson}, R.}, - title = "{Non-thermal pair production in compact X-ray sources - First-order Compton cascades is soft radiation fields}", - journal = {\mnras}, - year = 1987, - month = jul, - volume = 227, - pages = {403-451}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1987MNRAS.227..403S&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@BOOK{Berezinskii:1990, - author = {{Berezinskii}, V.~S. and {Bulanov}, S.~V. and {Dogiel}, V.~A. and - {Ptuskin}, V.~S.}, - title = "{Astrophysics of cosmic rays}", -publisher = {Amsterdam: North-Holland, 1990, edited by Ginzburg, V.L.}, -year = 1990, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1990acr..book.....B&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Mannheim:1991, - author = {{Mannheim}, K. and {Biermann}, P.~L. and {Kruells}, W.~M.}, - title = "{A novel mechanism for nonthermal X-ray emission}", - journal = {\aap}, - year = 1991, - month = nov, - volume = 251, - pages = {723-731}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1991A%26A...251..723M&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@INPROCEEDINGS{Mannheim:1997, - author = {{Mannheim}, K.}, - title = "{AGN Models: High-Energy Emission.}", -booktitle = {Very High Energy Phenomena in the Universe; Moriond Workshop}, - year = 1997, - pages = {17-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1997vhep.conf...17M&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Mannheim:1998, - author = {{Mannheim}, K.}, - title = "{Possible Production of High-Energy Gamma Rays from Proton Acceleration in the Extragalactic Radio Source Markarian 501}", - journal = {Science}, - year = 1998, - month = jan, - volume = 279, - pages = {684-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998Sci...279..684M&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Hauser:2001, - author = {{Hauser}, M.~G. and {Dwek}, E.}, - title = "{The Cosmic Infrared Background: Measurements and Implications}", - journal = {\araa}, - year = 2001, - volume = 39, - pages = {249-307}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2001ARA%26A..39..249H&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -# TO BE CHECKED! -@ARTICLE{Perlman:1998, - author = {{Perlman}, E.~S. and {Padovani}, P. and {Giommi}, P. and {Sambruna}, R. and - {Jones}, L.~R. and {Tzioumis}, A. and {Reynolds}, J.}, - title = "{The Deep X-Ray Radio Blazar Survey. I. Methods and First Results}", - journal = {\aj}, - year = 1998, - month = apr, - volume = 115, - pages = {1253-1294}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998AJ....115.1253P&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@INPROCEEDINGS{Laurent-Muehleisen:1998, - author = {{Laurent-Muehleisen}, S.~A. and {Kollgaard}, R.~I. and {Feigelson}, E.~D. - }, - title = "{The Rosat-Green Bank Sample of Intermediate BL Lac Objects}", -booktitle = {ASP Conf. Ser. 144: IAU Colloq. 164: Radio Emission from Galactic and Extragalactic Compact Sources}, - year = 1998, - pages = {163-+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998ASPC..144..163L&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Caccianiga:1999, - author = {{Caccianiga}, A. and {Maccacaro}, T. and {Wolter}, A. and {della Ceca}, R. and - {Gioia}, I.~M.}, - title = "{The REX Survey: A Search for Radio-emitting X-Ray Sources}", - journal = {\apj}, - year = 1999, - month = mar, - volume = 513, - pages = {51-68}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1999ApJ...513...51C&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Caccianiga:2004, - author = {{Caccianiga}, A. and {March{\~a}}, M.~J.~M.}, - title = "{The CLASS blazar survey: testing the blazar sequence}", - journal = {\mnras}, - year = 2004, - month = mar, - volume = 348, - pages = {937-954}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2004MNRAS.348..937C&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Kellermann:1989, - author = {{Kellermann}, K.~I. and {Sramek}, R. and {Schmidt}, M. and {Shaffer}, D.~B. and - {Green}, R.}, - title = "{VLA observations of objects in the Palomar Bright Quasar Survey}", - journal = {\aj}, - year = 1989, - month = oct, - volume = 98, - pages = {1195-1207}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1989AJ.....98.1195K&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Rowan:1977, - author = {{Rowan-Robinson}, M.}, - title = "{On the unity of activity in galaxies}", - journal = {\apj}, - year = 1977, - month = may, - volume = 213, - pages = {635-647}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1977ApJ...213..635R&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Lawrence:1982, - author = {{Lawrence}, A. and {Elvis}, M.}, - title = "{Obscuration and the various kinds of Seyfert galaxies}", - journal = {\apj}, - year = 1982, - month = may, - volume = 256, - pages = {410-426}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1982ApJ...256..410L&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Giommi:1994, - author = {{Giommi}, P. and {Padovani}, P.}, - title = "{Bl-Lacertae Reunification}", - journal = {\mnras}, - year = 1994, - month = may, - volume = 268, - pages = {L51+}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1994MNRAS.268L..51G&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Antonucci:1985, - author = {{Antonucci}, R.~R.~J. and {Ulvestad}, J.~S.}, - title = "{Extended radio emission and the nature of blazars}", - journal = {\apj}, - year = 1985, - month = jul, - volume = 294, - pages = {158-182}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1985ApJ...294..158A&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Fossati:1998, - author = {{Fossati}, G. and {Maraschi}, L. and {Celotti}, A. and {Comastri}, A. and - {Ghisellini}, G.}, - title = "{A unifying view of the spectral energy distributions of blazars}", - journal = {\mnras}, - year = 1998, - month = sep, - volume = 299, - pages = {433-448}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=1998MNRAS.299..433F&db_key=AST}, - adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System} -} - -@ARTICLE{Aharonian:2000, - author = {{Aharonian}, F.}, - title = "{TeV gamma rays from BL Lac objects due to synchrotron radiation of extremely high energy protons}", - journal = {\na}, - year = 2000, - month = nov, - volume = 5, - pages = {377-395}, - adsurl = {http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?bibcode=2000NewA....5..377A&db_key=AST}, - 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Or switch it on % for the whole article with \linenumbers. -\usepackage{lineno} +%\usepackage{lineno} %\linenumbers -\usepackage[numbers]{natbib} +%\usepackage[numbers]{natbib} \usepackage{textcomp,graphicx,times,wrapfig,xspace,url,amssymb,amsmath,wasysym,stmaryrd} @@ -57,23 +57,12 @@ \title{The drive system of the\\Major Atmospheric Gamma-ray Imaging Cherenkov Telescope} -\newcommand{\corref}{\thanksref} -\newcommand{\cortext}{\thanks} - -%\tnotetext[t1]{This document is collaborative effort} -%\tnotetext[t2]{This document is collaborative effort more} - +%\newcommand{\corref}{\thanksref} +%\newcommand{\cortext}{\thanks} \author[tb]{T.~Bretz\corref{cor1}} -\address[tb]{Universit\"{a}t W\"{urzburg}, Am Hubland, D-97074 W\"{u}rzburg, Germany} -%\ead{tbretz@astro.uni-wuerzburg.de} -%\fntext[fn1]{My name is Thomas Bretz} - -\author[tb]{D.~Dorner},\author[rw]{R.~M.~Wagner} -%\address[dd]{Integral Science Data Center} -%\ead{dorner@astro.uni-wuerzburg.de} - - -%\ead[rw]{robert.wagner@mpp.mpg.de} -\address[rw]{Max-Planck-Institut f\"ur Physik, F\"ohringer Ring 6, D-80805 M\"{u}nchen, Germany} - +\author[tb]{D.~Dorner} +\author[rw]{R.~M.~Wagner} +\author[rw]{P.~Sawallisch} +\address[tb]{Universit\"{a}t W\"{u}rzburg, Am Hubland, 97074 W\"{u}rzburg, Germany} +\address[rw]{Max-Planck-Institut f\"ur Physik, F\"ohringer Ring 6, 80805 M\"{u}nchen, Germany} \cortext[cor1]{Corresponding author: tbretz@astro.uni-wuerzburg.de} @@ -86,29 +75,28 @@ \begin{abstract} The MAGIC telescope is an imaging atmospheric Cherenkov telescope, -designed to observe very high energy gamma-rays achieving a low energy -threshold. One of the key science goals is the fast follow-up of the +designed to observe very high energy gamma-rays while achieving a low +energy threshold. One of the key science goals is fast follow-up of the enigmatic and short lived gamma-ray bursts. The drive system for the telescope has to meet two basic demands: (1)~During normal -observations, the 64-ton telescope has to be repositioned accurately, -and has to track a given sky position with high precision at a typical +observations, the 72-ton telescope has to be positioned accurately, and +has to track a given sky position with high precision at a typical rotational speed in the order of one revolution per day. (2)~For successfully observing GRB prompt emission and afterglows, it has to be -powerful enough to reposition the telescope to an arbitrary point on -the sky within a few ten seconds and commence normal tracking immediately -thereafter. To meet these requirements, the implementation and -realization of the drive system relies strongly on standard industry -components to ensure robustness and reliability. In this paper, we -describe the mechanical setup, the drive control and the calibration of -the pointing, as well as present measurements of the accuracy of the -system. We show that within the limits of the mount the drive system is -mechanically able to operate with an accuracy even better than the -feedback values from the axes. In the context of future projects, -envisaging telescope arrays comprising about 100 individual -instruments, the robustness and scalability of the concept is -emphasized. +powerful enough to position to an arbitrary point on the sky within a +few ten seconds and commence normal tracking immediately thereafter. To +meet these requirements, the implementation and realization of the +drive system relies strongly on standard industry components to ensure +robustness and reliability. In this paper, we describe the mechanical +setup, the drive control and the calibration of the pointing, as well +as present measurements of the accuracy of the system. We show that the +drive system is mechanically able to operate the motors with an +accuracy even better than the feedback values from the axes. In the +context of future projects, envisaging telescope arrays comprising +about 100 individual instruments, the robustness and scalability of the +concept is emphasized. \end{abstract} \begin{keyword} -MAGIC\sep drive system\sep IACT\sep scalability\sep calibration\sep fast repositioning +MAGIC\sep drive system\sep IACT\sep scalability\sep calibration\sep fast positioning \end{keyword} @@ -120,12 +108,12 @@ The MAGIC telescope on the Canary Island of La~Palma, located 2200\,m -above sea level at 28\textdegree{}45'\,N and 17\textdegree{}54'\,W, is an -imaging atmospheric Cherenkov telescope designed to achieve a low -energy threshold, fast repositioning, and high tracking accuracy, -e.g.~\cite{Lorenz:2004, Cortina:2005}. The MAGIC design, and the +above sea level at 28\textdegree{}45$^\prime$\,N and 17\textdegree{}54$^\prime$\,W, is +an imaging atmospheric Cherenkov telescope designed to achieve a low +energy threshold, fast positioning, and high tracking +accuracy~\cite{Lorenz:2004, Cortina:2005}. The MAGIC design, and the currently ongoing construction of a second telescope -(MAGIC\,II;~\cite{Goebel:2007}), pave the way to the ground-based +(MAGIC\,II;~\cite{Goebel:2007}), pave the way for ground-based detection of gamma-ray sources at cosmological distances down to less -than 80\,GeV. After the discovery of the distant blazars 1ES\,1218+304 +than 25\,GeV~\cite{Sci}. After the discovery of the distant blazars 1ES\,1218+304 at a redshift of $z$\,=\,0.182~\citep{2006ApJ...642L.119A} and 1ES\,1011+496 at $z$\,=\,0.212~\citep{2007ApJ...667L..21A}, the most @@ -136,34 +124,38 @@ in the mid-infrared to near-infrared wavelength range was believed to be strong enough to inhibit propagation of gamma-rays across -cosmological distances~\citep{2001MNRAS.320..504S}. However, it could -be shown that the results of deep galaxy surveys with the Hubble and -Spitzer Space telescopes are consistent with these findings, if the -spurious feature at one micron is attributed to a foreground effect -resulting from an inaccurate subtraction of zodiacal -light~\citep{Hauser:2001, 2007arXiv0707.2915K, Kneiske:2004}. The low -level of pair attenuation of gamma-rays greatly improves the prospects -of searching for very high energy gamma-rays from gamma-ray bursts -(GRBs). Their remarkable similarities with blazar flares, albeit at -much shorter timescales, presumably arise from the scaling behavior of -relativistic jets, the common physical cause of these phenomena. Since -most GRBs reside at large redshifts, their detection relies on the low -level of absorption at very high energies~\citep{1996ApJ...467..532M}. -Moreover, the cosmological absorption decreases with photon energy, -favoring MAGIC to discover GRBs due to its low energy threshold. - -Due to the short life time of GRBs and the limited field of view of +cosmological distances~\citep{2001MNRAS.320..504S, 2007arXiv0707.2915K, Hauser:2001}. +%However, it could +%be shown that the results of deep galaxy surveys with the Hubble and +%Spitzer Space telescopes are consistent with these findings, if the +%spurious feature at one micron is attributed to a foreground effect +%resulting from an inaccurate subtraction of zodiacal +%light~\citep{Hauser:2001, 2007arXiv0707.2915K, Kneiske:2004}. +The +apparent low level of pair attenuation of gamma-rays greatly improves +the prospects of searching for very high energy gamma-rays from +gamma-ray bursts (GRBs), cf.~\citep{Kneiske:2004}. Their remarkable similarities with blazar +flares, albeit at much shorter timescales, presumably arise from the +scaling behavior of relativistic jets, the common physical cause of +these phenomena. Since most GRBs reside at large redshifts, their +detection at very high energies relies on the low level of +absorption~\citep{1996ApJ...467..532M}. Moreover, the cosmological +absorption decreases with photon energy, favoring MAGIC to discover +GRBs due to its low energy threshold. + +Due to the short life times of GRBs and the limited field of view of imaging atmospheric Cherenkov telescopes, the drive system of the MAGIC telescope has to meet two basic demands: during normal observations, -the 64-ton telescope has to be repositioned accurately, and has to +the 72-ton telescope has to be positioned accurately, and has to track a given sky position, i.e., counteract the apparent rotation of the celestial sphere, with high precision at a typical rotational speed in the order of one revolution per day. For catching the GRB prompt -emission and afterglows, it has to be powerful enough to reposition the +emission and afterglows, it has to be powerful enough to position the telescope to an arbitrary point on the sky within a very short time -($\apprle$\,60\,s) and commence normal tracking immediately +%($\apprle$\,60\,s) +and commence normal tracking immediately thereafter. To keep the system simple, i.e., robust, both requirements should be achieved without an indexing gear. The telescope's total -weight of 64~tons is a comparatively low measure, reflecting the -construction principle of using low-weight materials whenever possible. +weight of 72~tons is comparatively low, reflecting the +use of low-weight materials whenever possible. For example, the mount consists of a space frame of carbon-fiber reinforced plastic tubes, and the mirrors are made of polished @@ -174,12 +166,12 @@ setup of the drive system are outlined. The control loops and performance goals are described in section~\ref{sec3}, while the -implementation of the repositioning and tracking algorithms and the +implementation of the positioning and tracking algorithms and the calibration of the drive system are explained in section~\ref{sec4}. The system can be scaled to meet the demands of other telescope designs -as shown in section~\ref{sec5}. Finally, in section~\ref{conclusions} -we draw conclusions from our experience of operating the MAGIC -telescope with this drive system for four years. - -\section{General design considerations} +as shown in section~\ref{sec5}. Finally, in section~\ref{outlook} and +section~\ref{conclusions} we draw conclusions from our experience of +operating the MAGIC telescope with this drive system for four years. + +\section{General design considerations}\label{design} The drive system of the MAGIC telescope is quite similar to that of @@ -187,65 +179,79 @@ quite a few aspects that influenced the design of the MAGIC drive system in comparison to optical telescopes and small-diameter Imaging -Atmospheric Cherenkov telescope (IACT). - -The tracking and stability requirements for IACTs are much less -demanding than for optical telescopes. Although IACTs, like optical -telescopes, track celestial objects, they observe quite different -phenomena: Optical telescopes observe visible light, which originates -at infinity and is parallel. The best-possible optical resolution is -required and in turn, equal tracking precision due to comparably long -integration times, i.e., seconds to hours. In ground-based astronomy at -very high gamma-ray energies, IACTs record the Cherenkov light produced -by an electromagnetic air-shower in the atmosphere, induced by a -primary gamma-ray, i.e., from a close by (5\,km\,-\,20\,km) and -extended event with a diffuse transverse extension and a typical -extension of a few km. Due to the stochastic nature of the shower -development, the detected light will have an inherent limitation in -explanatory power, improving normally with the energy, i.e., -shower-particle multiplicity. As, in this case, the Cherenkov light is -emitted with under a small angle off the particle tracks, these photons -do not even point directly to the source like in optical astronomy. -Nevertheless, the shower points towards the direction of the incoming -gamma-ray and thus towards its source on the sky, and for this reason -its origin can be reconstructed analyzing its image. Modern IACTs -achieve an energy-dependent pointing resolution for individual showers -of 0.1\textdegree\,-\,0.01\textdegree. These are the predictions from -Monte Carlo simulations assuming, amongst other things, ideal tracking. -This sets the limits achievable in practical cases. Consequently, the -required tracking precision must be at least of the same order or even -better. Although the short integration times, on the order of a few -nanoseconds, would allow for an offline correction, this should be -avoided since it may give rise to an additional systematic error. - -MAGIC, as other large IACTs, has no protective dome. It is constantly -exposed to daily changing weather conditions and intense sunlight, and -therefore suffers much more material aging than optical telescopes. A -much simpler mechanical mount had to be used, resulting in a design of -considerably less stiffness, long-term irreversible deformations, and -small unpredictable deformations due to varying wind pressure. The -tracking system does not need to be more precise than the mechanical -structure and, consequently, can be much simpler and hence cheaper as -compared to that of large optical telescopes. +Atmospheric Cherenkov telescopes (IACT). + +Although IACTs have optical components, the tracking and stability +requirements for IACTs are much less demanding than for optical +telescopes. Like optical telescopes, IACTs track celestial +objects, but observe quite different phenomena: Optical telescopes +observe visible light, which originates at infinity and is parallel. +Consequently, the best-possible optical resolution is required and in +turn, equal tracking precision due to comparably long integration +times, i.e., seconds to hours. In contrast, IACTs record the Cherenkov +light produced by an electromagnetic air-shower in the atmosphere, +induced by a primary gamma-ray, i.e., from a close by +(5\,km\,-\,20\,km) and extended event with a diffuse transverse +extension and a typical extension of a few hundred meters. Due to the +stochastic nature of the shower development, the detected light will +have an inherent limitation in explanatory power, improving normally +with the energy, i.e., shower-particle multiplicity. As +the Cherenkov light is emitted under a small angle off the particle +tracks, these photons do not even point directly to the source like in +optical astronomy. Nevertheless, the shower points towards the +direction of the incoming gamma-ray and thus towards its source on the +sky. For this reason its origin can be reconstructed analyzing its +image. Modern IACTs achieve an energy-dependent pointing resolution for +individual showers of 6$^\prime$\,-\,0.6$^\prime$. These are the +predictions from Monte Carlo simulations assuming, amongst other +things, ideal tracking. This sets the limits achievable in practical +cases. Consequently, the required tracking precision must be at least +of the same order or even better. Although the short integration times, +on the order of a few nanoseconds, would allow for an offline +correction, this should be avoided since it may give rise to an +additional systematic error. + +%MAGIC, as other large IACTs, has no protective dome. It is constantly +%exposed to daily changing weather conditions and intense sunlight, and +%therefore suffers much more material aging than optical telescopes. A +%much simpler mechanical mount had to be used, resulting in a design of +%considerably less stiffness, long-term irreversible deformations, and +%small unpredictable deformations due to varying wind pressure. The +%tracking system does not need to be more precise than the mechanical +%structure and, consequently, can be much simpler and hence cheaper as +%compared to that of large optical telescopes. To meet one of the main physics goals, the observation of prompt and -afterglow emission of GRBs, repositioning of the telescope to their +afterglow emission of GRBs, positioning of the telescope to their assumed sky position is required in a time as short as possible. Alerts, provided by satellites, arrive at the MAGIC site typically -within 10\,s after the outburst~\citep{2007ApJ...667..358A}. To achieve -a positioning time to any position on the sky within less than a minute -requires a very light-weight but sturdy telescope and a fast-acting and -powerful drive system. -\begin{figure*}[htb] +within 10\,s after the outburst~\citep{2007ApJ...667..358A}. +Since the life times of GRBs show a bimodal distribution~\cite{Paciesas:1999} +with a peak between 10\,s and 100\,s. To achieve +a positioning time to any position on the sky within a reasonable +time inside this window, i.e. less than a minute, +a very light-weight but sturdy telescope and a fast-acting and +powerful drive system is required. +\begin{figure*}[htbp] \begin{center} - \includegraphics*[width=0.48\textwidth,angle=0,clip]{figure1a.eps} - \hfill - \includegraphics*[width=0.48\textwidth,angle=0,clip]{figure1b.eps} -\caption{{\em Left}: One of the bogeys with its two railway rails. The -motor is encapsulated in the grey box on the yellow drive unit. It drives -the tooth double-toothed wheel gearing into the chain through a gear -and a clutch. {\em Right}: The drive unit driving the elevation axis -from the back side. Visible is the actuator of the safety holding brake -and its corresponding brake disc mounted on the motor-driven axis. The -motor is attached on the opposite side. } + \includegraphics*[width=0.91\textwidth,angle=0,clip]{figure1.eps} +\caption{The top picture shows the MAGIC\,I telescope with the major +components of the drive system. The elevation drive unit, from its back +side, is enlarged in the bottom left picture. Visible is the actuator +of the safety holding brake and its corresponding brake disk mounted on +the motor-driven axis. The motor is attached on the opposite side. The +picture on the bottom right shows one of the azimuth bogeys with its +two railway rails. The motor is housed in the grey box on the +yellow drive unit. It drives the tooth double-toothed wheel gearing +into the chain through a gear and a clutch.} +% \includegraphics*[width=0.48\textwidth,angle=0,clip]{figure1a.eps} +% \hfill +% \includegraphics*[width=0.48\textwidth,angle=0,clip]{figure1b.eps} +%\caption{{\em Left}: One of the bogeys with its two railway rails. The +%motor is encapsulated in the grey box on the yellow drive unit. It drives +%%the tooth double-toothed wheel gearing into the chain through a gear +%and a clutch. {\em Right}: The drive unit driving the elevation axis +%from the back side. Visible is the actuator of the safety holding brake +%and its corresponding brake disk mounted on the motor-driven axis. The +%motor is attached on the opposite side. } \label{figure1} \end{center} @@ -256,34 +262,53 @@ The implementation of the drive system relies strongly on standard industry components to ensure robustness, reliability and proper -support. The azimuth drive ring of 21\,m diameter is made from a normal -railway rail, which was delivered in pre-bent sections and welded on -site. The fixing onto the concrete foundation uses standard rail-fixing -elements, and allows for movements caused by temperature changes. The -maximum allowable deviation from the horizontal plane as well as -deviation from flatness is $\pm 2$\,mm, and from the ideal circle it is -1\,cm. Each of the six bogeys holds two standard crane wheels of 60\,cm -diameter with a rather broad wheel tread. This allows for deviations in -the 11.5\,m-distance to the central axis due to extreme temperature -changes, which can even be asymmetric in case of different exposure to -sunlight on either side. The central bearing of the azimuth axis is a -high-quality ball bearing, while for the elevation axis, due to lower -weight, a less expensive sliding bearing with a teflon layer was -installed. These sliding bearings have a slightly spherical surface to -allow for small misalignments during installation and some bending of -the elevation axis stubs under load. +technical support. Its major drive components, described hereafter, are +shown on the pictures in fig.~\ref{figure2}. + +The azimuth drive ring of 20\,m diameter is made from a normal railway +rail, which was delivered in pre-bent sections and welded on site. Its +head is only about 74\,mm broad and has a bent profile. The fixing onto +the concrete foundation uses standard rail-fixing elements, and allows +for movements caused by temperature changes. The maximum allowable +deviation from the horizontal plane as well as deviation from flatness +is $\pm 2$\,mm, and from the ideal circle it is $\Delta$r\,=\,8\,mm. +The rail support was leveled with a theodolite every 60\,cm +with an overall tolerance of $\pm 1.5$\,mm every 60\,cm. In between the +deviation is negligible. Each of the six bogeys holds two standard +crane wheels of 60\,cm diameter with a rather broad wheel tread of +110\,mm. This allows for deviations in the 11.5\,m-distance to the +central axis due to extreme temperature changes, which can even be +asymmetric in case of different exposure to sunlight on either side. +For the central bearing of the azimuth axis, a high-quality ball +bearing was installed fairly assuming that the axis is vertically +stable. For the elevation axis, due to lower weight, a less expensive +sliding bearing with a teflon layer was used. These sliding bearings +have a slightly spherical surface to allow for small misalignments +during installation and some bending of the elevation axis stubs under +load. The drive mechanism is based on duplex roller chains and sprocket wheels in a rack-and-pinion mounting. The chains have a breaking -strength of 17~tons and a chain-link spacing of 2.5\,cm. The initial +strength of 19~tons and a chain-link spacing of 2.5\,cm. The initial play between the chain links and the sprocket-wheel teeth is about 3\,mm\,-\,5\,mm, according to the data sheet, corresponding to much less than an arcsecond on the telescope axes. The azimuth drive chain is fixed on a dedicated ring on the concrete foundation, but has quite -some radial distance variation of up to 3\,cm. The elevation drive +some radial distance variation of up to 5\,mm. The elevation drive chain is mounted on a slightly oval ring below the mirror dish, because the ring forms an integral part of the camera support mast structure. -Commercial synchronous motors (type designation Bosch Rexroth -MHD\,112C-058) are used together with low-play planetary gears linked +% Bosch Rexroth AG, 970816 Lohr am Main, Germany +% www.boschrexroth.de + +% Wittenstein alpha GmbH, Walter-Wittenstein-Stra"se 1, D-97999 Igersheim +% www.wittenstein-alpha.de + +% updated +Commercial synchronous motors (type designation Bosch +Rexroth\footnote{\url{http://www.boschrexroth.de}\\Bosch Rexroth AG, +97816 Lohr am Main, Germany} MHD\,112C-058) are used together with +low-play planetary gears (type designation +alpha\footnote{\url{http://www.wittenstein-alpha.de}\\Wittenstein alpha +GmbH, 97999 Igersheim, Germany} GTS\,210-M02-020\,B09, ratio 20) linked to the sprocket wheels. These motors intrinsically allow for a positional accuracy better than one arcsecond of the motor axis. Having @@ -292,11 +317,17 @@ installation height of more than 2200\,m a.s.l., due to lower air pressure and consequently less efficient cooling, the nominal values -given must be reduced by about 25\%. The azimuth motors are mounted on -small lever arms. In order to follow the small radial irregularities of -the azimuthal drive chain, the motors are pressed against it by -springs. The elevation-drive motor is mounted on a nearly 1\,m long +given must be reduced by about 20\%. Deceleration is done operating the +motors as generator which is as powerful as acceleration. The motors +contain 70\,Nm holding brakes which are not meant to be used as driving +brake. The azimuth motors are mounted on small lever arms. In order to +follow the small irregularities of the azimuthal drive chain, the units +are forced to follow the drive chain, horizontally and vertically, by +guide rolls. The elevation-drive motor is mounted on a nearly 1\,m long lever arm to be able to compensate the oval shape of the chain and the fact that the center of the circle defined by the drive chain is -shifted 50\,cm away from the axis towards the camera. +shifted 356\,mm away from the axis towards the camera. The elevation +drive is also equipped with an additional brake, operated only as +holding brake, for safety reasons in case of extremely strong wind +pressure. No further brake are installed on the telescope. The design of the drive system control, c.f.~\citet{Bretz:2003drive}, @@ -319,6 +350,6 @@ $\theta$\,=\,+100\textdegree{} to $\theta$\,=\,-70\textdegree{} where the change of sign implies a movement {\em across the zenith}. This -so-called {\it reverse mode} is currently not in use, as it might imply -hysteresis effects of the active mirror control system, still under +so-called {\it reverse mode} is currently not in use, as it might result +in hysteresis effects of the active mirror control system, still under investigation, due to shifting of weight at zenith. The accessible range in both directions and on both axes is limited by software to the @@ -334,16 +365,16 @@ \section{Setup of the motion control system}\label{sec3} -Like for the mechanical drive system, also for the motion-control system -standard industry components were used. The drive is controlled by the -feedback of encoders measuring the angular positions of the motors and -the telescope axes. The encoders on the motor axes provide -information to microcontrollers dedicated for motion control, -initiating and monitoring every movement. Professional build-in servo -loops take over the suppression of oscillations. The correct pointing -position of the system is ensured by a computer program evaluating the -feedback from the telescope axes and initiating the motion executed by -the micro controllers. Additionally, the motor-axis encoders are also -evaluated to increase accuracy. The details of this system, as shown in -figure~\ref{figure2}, are discussed below. +The motion control system similarly uses standard industry components. +The drive is controlled by the feedback of encoders measuring the +angular positions of the motors and the telescope axes. The encoders on +the motor axes provide information to micro controllers dedicated for +motion control, initiating and monitoring every movement. Professional +built-in servo loops take over the suppression of oscillations. The +correct pointing position of the system is ensured by a computer +program evaluating the feedback from the telescope axes and initiating +the motion executed by the micro controllers. Additionally, the +motor-axis encoders are also evaluated to increase accuracy. The +details of this system, as shown in figure~\ref{figure2}, are discussed +below. \begin{figure*}[htb] @@ -365,21 +396,22 @@ The angular telescope positions are measured by three shaft-encoders -(Hengstler AC61/1214EQ.72OLZ). These absolute multi-turn encoders have -a resolution of 4\,096 (10\,bit) revolutions and 16\,384 (14\,bit) -steps per revolution, corresponding to an intrinsic angular resolution -of 1.3\,arcmin per step. One shaft encoder is located on the azimuth -axis, while two more encoders are fixed on either side of the elevation -axis, increasing the resolution and allowing for measurements of the -twisting of the dish (fig.~\ref{figure3}). All shaft encoders used are -watertight (IP\,67) to withstand the extreme weather conditions -occasionally encountered at the telescope site. The motor positions are -read out at a frequency of 1\,kHz from 10\,bit relative rotary encoders -fixed on the motor axes. Due to the gear ratio of more than one -thousand between motor and load, the 14\,bit resolution of the shaft -encoder system on the axes can be interpolated further using the -position readout of the motors. For communication with the axis -encoders, a CANbus interface with the CANopen protocol is in use -(operated at 125\,kbps). The motor encoders are directly connected by -an analog interface. +(type designation Hengstler\footnote{\url{http://www.hengstler.de}\\Hengstler GmbH, +78554 Aldingen, Germany} AC61/1214EQ.72OLZ). These absolute multi-turn +encoders have a resolution of 4\,096 (10\,bit) revolutions and 16\,384 +(14\,bit) steps per revolution, corresponding to an intrinsic angular +resolution of 1.3$^\prime$ per step. One shaft encoder is located on +the azimuth axis, while two more encoders are fixed on either side of +the elevation axis, increasing the resolution and allowing for +measurements of the twisting of the dish (fig.~\ref{figure3}). All +shaft encoders used are watertight (IP\,67) to withstand the extreme +weather conditions occasionally encountered at the telescope site. The +motor positions are read out at a frequency of 1\,kHz from 10\,bit +relative rotary encoders fixed on the motor axes. Due to the gear ratio +of more than one thousand between motor and load, the 14\,bit +resolution of the shaft encoder system on the axes can be interpolated +further using the position readout of the motors. For communication +with the axis encoders, a CANbus interface with the CANopen protocol is +in use (operated at 125\,kbps). The motor encoders are directly +connected by an analog interface. \subsection{Motor control} @@ -388,11 +420,11 @@ units ({\em DKC}, type designation Bosch Rexroth, DKC~ECODRIVE\,03.3-200-7-FW), serving as intelligent frequency -converters and power supplies. An input value, given either analog or +converters. An input value, given either analog or digital, is converted to a predefined output, e.g., command position, velocity or torque. All command values are processed through a chain of -build-in controllers, cf. fig.~\ref{figure4}, resulting in a final +built-in controllers, cf. fig.~\ref{figure4}, resulting in a final command current applied to the motor. This internal chain of control -loops, maintaining the movement of the motors, works at a frequency of -1\,kHz fed back by the rotary encoders on the corresponding motor axes. +loops, maintaining the movement of the motors at a frequency of +1\,kHz, fed back by the rotary encoders on the corresponding motor axes. Several safety limits ensure damage-free operation of the system even under unexpected operation conditions. These safety limits are, e.g., @@ -404,5 +436,7 @@ slave is driven by the command torque output of the master. This operation mode ensures that both motors can apply their combined force -to the telescope structure without oscillations. +to the telescope structure without oscillations. In principle it is +possible to use a bias torque to eliminate play. This feature +was not used because the play is negligible anyhow. \begin{figure}[htb] @@ -414,5 +448,6 @@ position to the opposite side. The average offset from zero corresponds to a the twist of the two shaft encoders with respect to -each other. Under normal conditions the torsion between both ends of +each other. The error bars denote the spread of several measurements. +Under normal conditions the torsion between both ends of the axis is less than the shaft-encoder resolution.} \label{figure3} @@ -423,5 +458,5 @@ \begin{figure*}[htb] \begin{center} - \includegraphics*[width=0.6\textwidth,angle=0,clip]{figure4.eps} + \includegraphics*[width=0.78\textwidth,angle=0,clip]{figure4.eps} \caption{The internal flow control between the individual controllers inside the drive control unit. Depending on the type of the command @@ -433,25 +468,28 @@ \end{figure*} -The master DKC for each axis is controlled by presetting a rotational +% zub machine control AG, Kastaniensteif 7, CH-6047 Kastanienbaum +% www.zub.de + +The master for each axis is controlled by presetting a rotational speed defined by $\pm$10\,V on its analog input. The input voltage is -produced by a programmable microcontroller dedicated to analog motion -control, produced by Z\&B ({\em MACS}, type designation MACS). The -feedback is realized through a 500-step emulation of the motor's rotary -encoders by the DKCs for each axis seperately. Elevation and azimuth -movement is regulated by individual MACSs. The MACS controller itself -communicates with the control software (see below) through a CANbus -connection. +produced by a programmable micro controller dedicated to analog motion +control, produced by Z\&B\footnote{\url{http://www.zub.de}\\zub machine control AG, 6074 +Kastanienbaum, Switzerland} ({\em MACS}, type +designation MACS). The feedback is realized through a 500-step +emulation of the motor's rotary encoders by the DKCs. Elevation and azimuth movement is regulated by individual +MACSs. The MACS controller itself communicates with the control +software (see below) through a CANbus connection. It turned out that in particular the azimuth motor system seems to be limited by the large moment of inertia of the telescope -($J_{\mathrm{az}}\approx4400$\,tm$^2$, for comparison -$J_{\mathrm{el}}\approx850$\,tm$^2$; note that the exact numbers depend +($J_{\mathrm{az}}$\,$\approx$\,4400\,tm$^2$, for comparison +$J_{\mathrm{el}}$\,$\approx$\,850\,tm$^2$; note that the exact numbers depend on the current orientation of the telescope). At the same time, the requirements on the elevation drive are much less demanding.\\ -\noindent {\em MAGIC\,II}\quad For the drive system currently under commissioning for -MAGIC\,II, several improvements have been provided:\\ +\noindent {\em MAGIC\,II}\quad For the drive system +several improvements have been provided:\\\vspace{-2ex} \begin{itemize} -\item 13\,bit absolute shaft-encoders (type designation Heidenhain +\item 13\,bit absolute shaft-encoders (type designation Heidenhain\footnote{\url{http://www.heidenhain.de}\\Dr.~Johannes Heidenhain GmbH, 83301 Traunreut, Germany} ROQ\,425) are installed, providing an additional sine-shaped $\pm$1\,Vss output within each step. This allows for a more accurate @@ -465,6 +503,9 @@ better motion control of the system. \item The analog transmission of the master's command torque to the -slave is substituted by a direct digital bi-directional communication -of the DKCs. +slave is replaced by a direct digital communication (EcoX) +of the DKCs. This allows for more robust and precise slave control. +Furthermore the motors could be coupled with relative angular synchronism +allowing to suppress deformations of the structure by keeping the +axis connecting both motors stable. \item A single professional programmable logic controller (PLC), in German: {\em Speicherprogammierbare Steuerung} (SPS, type designation Rexroth @@ -491,7 +532,7 @@ \subsubsection{Positioning} -Whenever the telescope has to be repositioned, the relative distance to +Whenever the telescope has to be positioned, the relative distance to the new position is calculated in telescope coordinates and then -converted to motor revolutions. Then, the micro-controllers are +converted to motor revolutions. Then, the micro controllers are instructed to move the motors accordingly. Since the motion is controlled by the feedback of the encoders on the motor axes, not on @@ -534,5 +575,5 @@ i.e., the movement of the axis is stopped. -\subsection{Fast repositioning} +\subsection{Fast positioning} The observation of GRBs and their afterglows in very-high energy @@ -541,5 +582,5 @@ after their outburst via the {\em Gamma-ray Burst Coordination Network}~\cite{www:gcn}, typical burst durations of 10\,s to -100\,s~\cite{Paciesas:1999} demand a fast repositioning of the +100\,s~\cite{Paciesas:1999} demand a fast positioning of the telescope. The current best value for the acceleration has been set to 11.7\,mrad\,s$^{-2}$. It is constrained by the maximum constant force @@ -556,7 +597,7 @@ ignoring all other control elements. -Currently, automatic repositioning by +Currently, automatic positioning by $\Delta\varphi$\,=\,180\textdegree{} in azimuth to the target position -is achieved within 45\,s. The repositioning time in elevation is not +is achieved within 45\,s. The positioning time in elevation is not critical in the sense that the probability to move a longer path in elevation than in azimuth is negligible. Allowing the telescope drive @@ -570,4 +611,12 @@ the telescope structure. +With the upgraded MAGIC\,II drive system, during commissioning in 2008 August, a +maximum acceleration and deceleration of $a_{az}$\,=\,30\,mrad\,s$^{-2}$ +and $a_{zd}$\,=\,90\,mrad/s$^{-2}$ and a maximum velocity of +$v_{az}$\,=\,290\,mrad\,s$^{-1}$ and $v_{zd}$\,=\,330\,mrad\,s$^{-1}$ +could be reached. With these values the limits of the motor power are +exhausted. This allowed a movement of +$\Delta\varphi$\,=\,180\textdegree/360\textdegree{} in azimuth within 20\,s\,/\,33\,s. + \subsection{Tracking precision} @@ -586,14 +635,8 @@ axes into account. In almost all cases it is well below the resolution of the shaft encoders, and in 80\% of the time it does not exceed 1/8 -of this value ($sim$10\,arcsec). This means that the accuracy of the +of this value ($\sim$10$^{\prime\prime}$). This means that the accuracy of the motion control, based on the encoder feedback, is much better than -1\,arcmin on the sky, which is roughly a fifth of the diameter of a -pixel in the MAGIC photomultiplier (PM) camera (0.1\textdegree{}, -c.f.~\cite{Beixeras:2005}). - -In the case of a real telescope ultimate limits of the tracking -precision are given by the precision with which the correct command -value is known. Its calibration is discussed in the following. - +1$^\prime$ on the sky, which is roughly a fifth of the diameter of a +pixel in the MAGIC camera (6$^\prime$, c.f.~\cite{Beixeras:2005}). \begin{figure}[htb] \begin{center} @@ -604,4 +647,6 @@ deviation is shown as absolute control deviation projected on the sky. The blue lines correspond to fractions of the shaft-encoder resolution. +The peak at half of the shaft-encoder resolution results from cases +in which one of the two averaged elevation encoders is off by one step. } \label{figure5} @@ -609,7 +654,11 @@ \end{figure} +In the case of a real telescope ultimate limits of the tracking +precision are given by the precision with which the correct command +value is known. Its calibration is discussed hereafter. + \section{Calibration}\label{sec4} -To calibrate the position, command value-astrometric corrections, +To calibrate the position command value, astrometric corrections (converting the celestial target position into the target position of an ideal telescope) and misalignment corrections (converting it further @@ -627,4 +676,18 @@ into the position as seen from Earth's center (apparent position) -- take into account precession and nutation of the Earth and annual +\begin{figure}[htb] +\begin{center} % Goldener Schnitt + \includegraphics*[width=0.185\textwidth,angle=0,clip]{figure6.eps} +\caption{The transformation applied to a given set of catalog source +coordinates to real-telescope coordinates. These corrections include +all necessary astrometric corrections, as well as the pointing +correction to transform from an ideal-telescope frame to the frame of a +real telescope. +%A detailed description of all corrections and the +%calibration of the pointing model is given in section~\ref{sec4}. +} +\label{figure6} +\end{center} +\end{figure} aberration, i.e., apparent displacements caused by the finite speed of light combined with the motion of the observer around the Sun during @@ -637,38 +700,39 @@ misalignment correction, all these effects are taken into account. -\begin{figure}[htb] -\begin{center} % Goldener Schnitt - \includegraphics*[width=0.185\textwidth,angle=0,clip]{figure6.eps} -\caption{The transformation applied to a given set of catalog source -coordinates to real-telescope coordinates. These corrections include -all necessary astrometric corrections, as well as the pointing -correction to transform from an ideal-telescope frame to the frame of a -real telescope. A detailed description of all corrections and the -calibration of the pointing model is given in section~\ref{sec4}.} -\label{figure6} -\end{center} -\end{figure} - \subsection{Pointing model} Imperfections and deformations of the mechanical construction lead to -deviations from an ideal telescope. These deviations include the non-exact -alignment of axes, and deformations of the telescope structure. To -assure reliable pointing and tracking accuracy, such effects have to be -taken into account. Therefore the tracking software employs an -analytical pointing model based on the {\rm TPOINT}\texttrademark{} -telescope modeling software~\cite{tpoint}, also used for -optical telescopes. This model, called {\em pointing model}, -parameterizes deviations from the ideal telescope. Calibrating the -pointing model by mispointing measurements of bright stars, which -allows to determine the necessary corrections, is a standard procedure. -Once calibrated, the model is applied online. Since an analytical model -is used, the source of any deviation can be identified and traced back -to components of the telescope mount.\\ +deviations from an ideal telescope, including the non-exact +alignment of axes, and deformations of the telescope structure. + +%new +In the case of the MAGIC telescopes the optical axis of the mirror is +defined by an automatic alignment system. This active mirror control +is programmed not to change the optical axis once defined, but only +controls the optical point spread function of the mirror, i.e., it does +not change the center of gravity of the light distribution. +This procedure is applied whenever the telescope is observing including +any kind of calibration measurement for the drive system. The precision +of the axis alignment of the mirrors is better than 0.2$^\prime$ and can +therefor be neglected. +%new + +%To assure reliable pointing and tracking accuracy, such effects have to +%be taken into account. +Consequently, to assure reliable pointing and tracking accuracy, +mainly the mechanical effects have to be taken into account. +Therefore the tracking software employs an analytical pointing model +based on the {\rm TPOINT}\texttrademark{} telescope modeling +software~\cite{tpoint}, also used for optical telescopes. This model, +called {\em pointing model}, parameterizes deviations from the ideal +telescope. Calibrating the pointing model by mispointing measurements +of bright stars, which allows to determine the necessary corrections, +is a standard procedure. Once calibrated, the model is applied online. +Since an analytical model is used, the source of any deviation can be +identified and traced back to components of the telescope mount.\\ Corrections are parameterized by alt-azimuthal terms~\cite{tpoint}, i.e., derived from vector transformations within the proper coordinate -system. The following possible misalignments are taken into account:\\ - +system. The following possible misalignments are taken into account:\\\vspace{-2ex} \begin{description} \item[Zero point corrections ({\em index errors})] Trivial offsets @@ -700,5 +764,8 @@ the encoders, has such a high static friction that in case of reversing the direction of the movement, the shaft-encoder will not indicate any -movement, even though the telescope is rotating. +movement for a small and stable rotation angle, even though the +telescope is rotating. Since this offset is stable, it can easily +be corrected after it is fully passed. The passage of the hysteresis +is currently corrected offline only. \end{itemize} \vspace{1em} @@ -708,9 +775,7 @@ unnecessary. Another class of deformations of the telescope-support frame and the mirrors are non-deterministic and, consequently, pose an -ultimate limit of the precision of the pointing correction. - -As discussed below, the size of the total correction (excluding the -index error) is on the order of 0.1\textdegree{}. Therefore all individual -correction terms are smaller or of similar size. +ultimate limit of the precision of the pointing. + +% Moved to results \subsection{Determination} @@ -719,10 +784,10 @@ To determine the coefficients of a pointing model, calibration -data is recorded, consisting of mispointing measurements depending +data is recorded. It consists of mispointing measurements depending on altitude and azimuth angle. Bright stars are tracked with the telescope at positions uniformly distributed in local coordinates, -i.e.\, in altitude and azimuth angle. To measure the real pointing -position of the telescope, the reflection of a bright star on a -screen in front of the MAGIC PM camera is determined. The center +i.e., in altitude and azimuth angle. The real pointing +position is derived from the position of the reflection of a bright +star on a screen in front of the MAGIC camera. The center of the camera is defined by LEDs mounted on an ideal ($\pm$1\,mm) circle around the camera center, cf.~\citet{Riegel:2005icrc}. @@ -735,15 +800,16 @@ A 0.0003\,lux, 1/2\(^{\prime\prime}\) high-sensitivity standard PAL CCD -camera (\mbox{Watec}~WAT-902\,H, technical details given in -table~\ref{table}) equipped with a zoom lens (type: Computar) is used +camera (type designation \mbox{Watec}~WAT-902\,H) equipped with a zoom lens (type: Computar) is used for the mispointing measurements. The camera is read out at a rate of -25\,frames per second using a framer-grabber card in a standard PC. The -tradeoff for the high sensitivity of the camera is its high noise level -in each single frame recorded. Since there are no rapidly moving -objects within the field of view, a high picture quality can be +25\,frames per second using a standard frame-grabber card in a standard +PC. The camera has been chosen providing adequate performance and +easy readout, due to the use of standard components, for a very cheap price +($<$\,500\,Euro). The tradeoff for the high sensitivity of the camera is its high +noise level in each single frame recorded. Since there are no rapidly +moving objects within the field of view, a high picture quality can be achieved by averaging typically 125\,frames (corresponding to 5\,s). An -example is shown in figure~\ref{figure7}. This example also -illustrates the high sensitivity of the camera, since both pictures of -the telescope structure have been taken with the residual light of less +example is shown in figure~\ref{figure7}. This example also illustrates +the high sensitivity of the camera, since both pictures of the +telescope structure have been taken with the residual light of less than a half-moon. In the background individual stars can be seen. Depending on the installed optics, stars up to 12$^\mathrm{m}$ are @@ -753,28 +819,27 @@ images of stars on the screen. -\begin{table}[htb] -\begin{center} -\small -\begin{tabular}{|l|l|}\hline -Model&Watec WAT-902H (CCIR)\\\hline\hline -Pick-up Element&1/2" CCD image sensor\\ -&(interline transfer)\\\hline -Number of total pixels&795(H)x596(V)\\\hline -Minimum Illumination&0.0003\,lx. F/1.4 (AGC Hi)\\ -&0.002\,lx. F/1.4 (AGC Lo)\\\hline -Automatic gain&High: 5\,dB\,-\,50\,dB\\ -&Low: 5\,dB\,-\,32\,dB\\\hline -S/N&46\,dB (AGC off)\\\hline -Shutter Speed&On: 1/50\,-\,1/100\,000\,s\\ (electronic iris)&Off: 1/50\,s\\\hline -Backlight compensation&On\\\hline -Power Supply&DC +10.8\,V\,-\,13.2\,V\\\hline -Weight&Approx. 90\,g\\\hline -\end{tabular} -\end{center} -\caption{Technical specifications of the CCD camera used for -measuring of the position of the calibration stars on the PM camera lid.} -\label{table} -\end{table} - +%\begin{table}[htb] +%\begin{center} +%\small +%\begin{tabular}{|l|l|}\hline +%Model&Watec WAT-902H (CCIR)\\\hline\hline +%Pick-up Element&1/2" CCD image sensor\\ +%&(interline transfer)\\\hline +%Number of total pixels&795(H)x596(V)\\\hline +%Minimum Illumination&0.0003\,lx. F/1.4 (AGC Hi)\\ +%&0.002\,lx. F/1.4 (AGC Lo)\\\hline +%Automatic gain&High: 5\,dB\,-\,50\,dB\\ +%&Low: 5\,dB\,-\,32\,dB\\\hline +%S/N&46\,dB (AGC off)\\\hline +%Shutter Speed&On: 1/50\,-\,1/100\,000\,s\\ (electronic iris)&Off: 1/50\,s\\\hline +%Backlight compensation&On\\\hline +%Power Supply&DC +10.8\,V\,-\,13.2\,V\\\hline +%Weight&Approx. 90\,g\\\hline +%\end{tabular} +%\end{center} +%\caption{Technical specifications of the CCD camera used for +%measuring of the position of the calibration stars on the PM camera lid.} +%\label{table} +%\end{table} \begin{figure*}[htb] \begin{center} @@ -795,11 +860,11 @@ figure~\ref{figure8}. Using the seven LEDs mounted on a circle around the camera center, the position of the camera center is determined. -Only the upper half of the area instrumented with PMs is visible, since +Only the upper half of the area instrumented is visible, since the lower half is covered by the lower lid, holding a special reflecting surface in the center of the camera. The LED positions are evaluated by a simple cluster-finding algorithm looking at pixels more than three standard deviations above the noise level. The LED position -is defined as the center of gravity of its light distribution. The -search region is defined by the surrounding black-coloured boxes. For +is defined as the center of gravity of its light distribution, its +search region by the surrounding black-colored boxes. For simplicity the noise level is determined just by calculating the mean and the root-mean-square within the individual search regions below a @@ -813,10 +878,12 @@ gravity, as well as the reconstructed circle on which the LEDs are located. The LEDs on the bottom part are hidden by the lower lid, -holding a screen in front of the PM camera. For calibration, the center -of gravity of the measured star, as visible in the center, is compared -to the center of the circle given by the LEDs, coinciding with the -center of the PM camera. The black regions are the search regions for +holding a screen in front of the camera. +%For calibration, the center +%of gravity of the measured star, as visible in the center, is compared +%to the center of the circle given by the LEDs, coinciding with the +%center of the PM camera. +The black regions are the search regions for the LEDs and the calibration star. A few dead pixels in the CCD camera -can also be recognized. } +can also be recognized.} \label{figure8} \end{center} @@ -831,13 +898,13 @@ determination can be improved further by applying small offsets of the non-ideal LED positions. The radius distribution is Gaussian -and its resolution is $\sigma\,\apprle$\,1\,mm +and its resolution is $\sigma$\,$\apprle$\,1\,mm ($\mathrm{d}r/r\approx0.3$\textperthousand) on the camera plane -corresponding to $\sim$1\,arcsec. - -The center of the LED ring is calculated as the average of all circle -centers after quality cuts. The resolution of the center is -$\sim$2\,arcsec. In this setup, the large number of LEDs guarantees -operation even in case one LED is damaged or could not be detected due -to scattered light. +corresponding to $\sim$1$^{\prime\prime}$. + +The center of the ring is calculated as the average of all circle +centers after quality cuts. Its resolution is +$\sim$2$^{\prime\prime}$. In this setup, the large number of LEDs guarantees +operation even in case one LED could not be detected due to damage or +scattered light. To find the spot of the reflected star itself, the same cluster-finder @@ -866,9 +933,18 @@ be improved to a value below the intrinsic resolution of the system, i.e., below shaft-encoder resolution. In more than 83\% of all cases the -tracking accuracy is better than 0.02\textdegree{} ($\sim$1.3\,arcmin) -and it hardly ever exceeds 0.04\textdegree. The few datasets exceeding -0.04\textdegree{} are very likely due to imperfect measurement of the -real pointing position of the telescope, i.e.\, the center of gravity of +tracking accuracy is better than 1.3$^\prime$ +and it hardly ever exceeds 2.5$^\prime$. The few datasets exceeding +2.5$^\prime$ are very likely due to imperfect measurement of the +real pointing position of the telescope, i.e., the center of gravity of the star light. + +The average absolute correction applied (excluding the index error) is on +the order of 4$^\prime$. Given the size, weight and structure of +the telescope this proves a very good alignment and low sagging of the +structure. The elevation hysteresis, which is intrinsic to the +structure, the non-perpendicularity and non-centricity of the axes are +all in the order of 3$^\prime$, while the azimuth axis +misalignment is $<$\,0.6$^\prime$. These numbers are well in agreement +with the design tolerances of the telescope. \begin{figure}[htb] @@ -890,5 +966,5 @@ \subsubsection{Limitations} -The ultimate limit on the achievable tracking precision are effects, +The ultimate limit on the achievable pointing precision are effects, which are difficult to correlate or measure, and non-deterministic deformations of the structure or mirrors. For example, the azimuth @@ -899,83 +975,65 @@ deformations. Other deformations are caused by temperature changes and wind loads which are difficult to control for telescopes without dome, -and which cannot be modelled. It should be noted that the azimuth structure +and which cannot be modeled. It should be noted that the azimuth structure can change its diameter by up to 3\,cm due to day-night temperature differences, indicating that thermal effects have a non-negligible and non-deterministic influence. +Like every two axis mount, also an alt-azimuth mount has a blind spot +near its upward position resulting from misalignments of the axis which +are impossible to correct by moving one axis or the other. From the +size of the applied correction it can be derived that the blind spot +must be on the order of $\lesssim$\,6$^\prime$ around zenith. +Although the MAGIC drive system is powerful enough to keep on track +pointing about 6$^\prime$ away from zenith, for safety reasons, i.e., +to avoid fast movment under normal observation conditions, the observation +limit has been set to $\theta$\,$<$\,30$^\prime$. Such fast movements +are necessary to change the azimuth position from moving the telescope +upwards in the East to downwards in the South. In the case of an ideal +telescope, pointing at zenith, even an infinitely fast movement would +be required. + \subsubsection{Stability} -With each measurement of a calibration-star also the present tracking -uncertainty is recorded. This allows for monitoring of the tracking +With each measurement of a calibration-star also the present pointing +uncertainty is recorded. This allows for monitoring of the pointing quality and for offline correction. In figure~\ref{figure10} the -evolution of the measured residuals over the years are shown. The -continuous monitoring has been started in March 2005 and is still -ongoing. Quantiles are shown since the distribution can be highly -asymmetric. The points have been grouped, where the grouping reflects -data taken under the same conditions (pointing model, mirror alignment, -etc.) It should be noted, that the measured residuals depend on zenith -and azimuth angle, i.e., the distributions shown are biased due to -inhomogeneous distributions on the sky in case of low statistics. -Therefore the available statistics is given in table~\ref{table2}. -%, for convenience, together with the average measured mispointing. - \begin{figure}[htb] \begin{center} \includegraphics*[width=0.48\textwidth,angle=0,clip]{figure10.eps} - \caption{The distribution of mispointing measurements, which is an -exact measure of accuracy of the command values send to the drive -system. The plot shows its time-evolution. Details on the separation -and the available statistics is given in the caption of -table~\ref{table2}. Since the distribution is highly asymmetric, -quantiles are shown, from bottom to top, at 5\%, 13\%, 32\%, 68\%, 87\% -and 95\%. The dark grey region belong to the region between quantiles -32\% and 68\%. -} +\caption{The distribution of mispointing measurements. The +measurement is a direct measurement of the pointing accuracy. The plot +shows its time-evolution. Details on the bin edges and the available +statistics is given in the caption of table~\ref{table2}. Since the +distribution is asymmetric, quantiles are shown, from bottom to top, at +5\%, 13\%, 32\%, 68\%, 87\% and 95\%. The dark grey region belong to +the region between quantiles 32\% and 68\%. } \label{figure10} -\end{center} +\end{center} \end{figure} - -The mirror focusing can influence the alignment of the optical axis of -the telescope, i.e., it can modify the pointing model. Therefore a mirror -refocusing can worsen the tracking accuracy, later corrected by a new -pointing model. Also the determination of the pointing model relies on -a good statistical basis, because the measured residuals are of a -similar magnitude as the accuracy of a single calibration-star -measurement. The visible improvements and deterioration are mainly a -consequence of new mirror focusing and following implementations of new -pointing models. The improvement over the past year is explained by the -gain in statistics. - -On average the systematic pointing uncertainty was always better than -three shaft-encoder steps (corresponding to 4\,arcmin), most of the -time better than 2.6\,arcmin and well below one shaft-encoder step, -i.e.\ 1.3\,arcmin, in the past year. Except changes to the pointing -model or the optical axis, as indicated by the bin edges, no -degradation or change with time of the pointing model could be found. - -\section{Scalability}\label{sec5} - -With the aim to reach lower energy thresholds the next generation of -Cherenkov telescopes will become larger and heavier. Therefore more -powerful drive systems will be needed. The scalable drive system of the -MAGIC telescope is suited to meet this challenge. With its synchronous -motors and their master-slave setup it can easily be extended to larger -telescopes at moderate costs or even scaled down using less powerful -components. A motion accuracy at least of the order of the -shaft-encoder resolution is guaranteed. Real tracking accuracy -- -already including all possible pointing corrections -- is dominated by -dynamic and unpredictable deformations of the mount, e.g., temperature -expansion. - +evolution of the measured residuals over the years are shown. The +continuous monitoring has been started in March 2005 and is still +ongoing. Quantiles are shown since the distribution can be +asymmetric depending on how the residuals are distributed on the sky. The +points have been grouped, where the grouping reflects data taken under +the same conditions (pointing model, mirror alignment, etc.). It should +be noted, that the measured residuals depend on zenith and azimuth +angle, i.e., the distributions shown are biased due to inhomogeneous +distributions on the sky in case of low statistics. Therefore the +available statistics is given in table~\ref{table2}. \begin{table}[htb] \begin{center} \begin{tabular}{|l|c|}\hline Begin&Counts\\\hline\hline -2005/03/20&29\\ -2005/04/29&43\\ -2005/05/25&30\\ -2005/06/08&26\\ -2005/08/15&160\\ -2005/09/12&22\\ +2005/03/20&29\\%& 2005/11/24&38\\ +2005/04/29&43\\%& 2006/03/19&502\\ +2005/05/25&30\\%& 2006/10/17&827\\ +2005/06/08&26\\%& 2007/07/31&87\\ +2005/08/15&160\\%& 2008/01/14&542\\ +2005/09/12&22\\\hline%& 2008/06/18&128\\\hline +\end{tabular} +\hfill +\begin{tabular}{|l|c|}\hline +Begin&Counts\\\hline\hline 2005/11/24&38\\ 2006/03/19&502\\ @@ -984,5 +1042,5 @@ 2008/01/14&542\\ 2008/06/18&128\\\hline -\end{tabular} +\end{tabular}\hfill \end{center} \caption{Available statistics corresponding to the distributions @@ -995,5 +1053,46 @@ \end{table} -\section{Outlook} +The mirror focusing can influence the alignment of the optical axis of +the telescope, i.e., it can modify the pointing model. Therefore a +calibration of the mirror refocusing can worsen the tracking accuracy, +later corrected by a new pointing model. Although the automatic mirror +control is programmed such that a new calibration should not change the +center of gravity of the light distribution, it happened sometimes in +the past due to software errors. + +The determination of the pointing model also relies on a good +statistical basis, because the measured residuals are of a similar +magnitude as the accuracy of a single calibration-star measurement. The +visible improvements and deterioration are mainly a consequence of new +mirror focusing and following implementations of new pointing models. +The improvement over the past year is explained by the gain in +statistics. + +On average the systematic pointing uncertainty was always better than +three shaft-encoder steps (corresponding to 4$^\prime$), most of the +time better than 2.6$^\prime$ and well below one shaft-encoder step, +i.e.\ 1.3$^\prime$, in the past year. Except changes to the pointing +model or the optical axis, as indicated by the bin edges, no +degradation or change with time of the pointing model or +a worsening of the limit given by the telescope mechanics could be found. + +\section{Scalability}\label{sec5} + +With the aim to reach lower energy thresholds, the next generation of +Cherenkov telescopes will also include larger and heavier ones. +Therefore more powerful drive systems will be needed. The scalable +drive system of the MAGIC telescope is suited to meet this challenge. +With its synchronous motors and their master-slave setup, it can easily +be extended to larger telescopes at moderate costs, or even scaled down +to smaller ones using less powerful components. Consequently, +telescopes in future projects, with presumably different sizes, can be +driven by similar components resulting in a major +simplification of maintenance. With the current setup, a tracking +accuracy at least of the order of the shaft-encoder resolution is +guaranteed. Pointing accuracy -- already including all possible +pointing corrections -- is dominated by dynamic and unpredictable +deformations of the mount, e.g., temperature expansion. + +\section{Outlook}\label{outlook} Currently, efforts are ongoing to implement the astrometric subroutines @@ -1018,4 +1117,7 @@ without influencing the general functionality of the system. +An upgrade of the MAGIC\,I drive system according to the improvements +applied for MAGIC\,II is ongoing. + \section{Conclusions}\label{conclusions} @@ -1023,39 +1125,37 @@ system for the MAGIC telescope. From its hardware installation and software implementation, the installed drive system exceeds its design -specifications. At the same time the system performs reliably and -stably, showing no deterioration after five years of routine operation. -The mechanical precision of the motor movement is almost ten times -better than the readout on the telescope axes. The tracking accuracy is -dominated by random deformations and hysteresis effects of the mount, -but still within limits within which the position of the telescope axes -can be measured. The system features integrated tools, like an -analytical pointing model. Fast repositioning for gamma-ray bursts -followup is achieved on average within less than 45 seconds, or, if -movements {\em across the zenith} are allowed, within less than 30 -seconds. Thus, the drive system makes MAGIC the best suited telescope -for observations of gamma-ray burst at very high energies. +specifications as given in section~\ref{design}. At the same time the +system performs reliably and stably, showing no deterioration after +five years of routine operation. The mechanical precision of the motor +movement is almost ten times better than the readout on the telescope +axes. The tracking accuracy is dominated by random deformations and +hysteresis effects of the mount, but still negligible +compared to the measurement of the position of the telescope axes. The +system features integrated tools, like an analytical pointing model. +Fast positioning for gamma-ray burst followup is achieved on average +within less than 45 seconds, or, if movements {\em across the zenith} +are allowed, 30 seconds. Thus, the drive system makes +MAGIC the best suited telescope for observations of these phenomena at +very high energies. For the second phase of the MAGIC project and particularly for the -second telescope, the system has been further improved by replacing the -partially analog communication with a completely digital one. +second telescope, the drive system has been further improved. By design, the drive system is easily scalable from its current dimensions to larger and heavier telescope installations as required for future projects. The improved stability is also expected to meet the stability requirements, necessary when operating a larger number of -telecopes. +telescopes. \section[]{Acknowledgments} The authors acknowledge the support of the MAGIC collaboration, and -thank the IAC for providing excellent working conditions at the Roque -de los Muchachos Observatory in La Palma. The MAGIC telescope project -is mainly supported by BMBF (Germany), MCI-NN (Spain), INFN and MUR -(Italy). We thank the construction department of the MPI for Physics, -particularly Peter Sawallisch, for their help in the design and -installation of the drive system. We are grateful for Eckart Lorenz's -help with the hardware installations and also for some important -comments concerning this manuscript. R.M.W.\ acknowledges financial -support by the Max Planck Society. His research is also supported in -part by the DFG Cluster of Excellence ``Origin and Structure of the -Universe''. +thank the IAC for providing excellent working conditions at the +Observatorio del Roque de los Muchachos. The MAGIC project is mainly +supported by BMBF (Germany), MCI (Spain), INFN (Italy). We thank the +construction department of the MPI for Physics, for their help in the +design and installation of the drive system as well as Eckart Lorenz, +for some important comments concerning this manuscript. R.M.W.\ +acknowledges financial support by the MPG. His research is also +supported by the DFG Cluster of Excellence ``Origin and Structure of +the Universe''. \begin{thebibliography}{00} @@ -1069,16 +1169,18 @@ \bibitem[Cortina et~al.(2005)]{Cortina:2005} J.~Cortina et~al. (MAGIC Collab.), in: Proc. 29th Int. Cosm. Ray Conf., Pune, India, August 2005, Vol. 5, 359. \bibitem[Goebel(2007)]{Goebel:2007} F.~Goebel (MAGIC Collab.), in: Proc. 30th Int. Cosm. 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