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°UккккUU`УкUUHH╘И{┌z|uUHH╘И∙U`ФбUHH╘И|┌{uHH╘И·UU`ХбUH$╘ }┌~vUH$╘ √UккккUU`ЦкUUHьнz╘ ~┌}vUHьнz╘ №UккккUU`ЧкUHH╘И┌~5vHH╘И¤┘`ШбdА┘┌БМHУ╙3K║^иБ┌ВАH RH RйЫFootnoteHq∙v?№^иВ┌БГАHz╖╕Hz╖╕йSingle LineUH'┤Г┌ВЕАДДFootnote РД▐Г ЩUHз∙vDгf^иЕ▄ГЖАUH░╖╕H░╖╕йDouble LineH║╘Ж┌ЕЙАUЗИDouble LineU╘З▌ИЖ╘╘И▌ЗЖ╘HЖ╘ Й┌ЖЛАUККSingle LineU╘К▌Й╘UHZ┤Л┌ЙМАU TableFootnoteE╕╛GX-RЯb^иМ┌ЛАUE╕╛PoE╕╛Poй┌ TableFootnotedН┘ООHH╘ИО┌Н┘HH╘ИС■н,K║`Щб #UT UTкк`ЬгHIGH SPEED PHOTOMETER ?№=UR UTккhЭгSCIENCE DATA HEADER L №`Юл ┤Z №`Ял h №hамFoFSIMPLE л = F image conforms to the fits standard v №hбм∙vFBITPIX л!= 32 bits per data value Д №hвмЙGDATATYPEл"= REAL*4 datatype of the array ЖТ №hгмENAXIS л#= 1 number of data axes а №hдмFNAXIS1 л$= length of 1st data axis о №hемFGROUPS л%= T image is in group format ╝ №hжмМFGCOUNT л&= 1 number of groups ╩ №hзмoFPCOUNT л'= 10 number of group parameters ╪ № илO PSIZE = 448 bits in the group parameter block ф №@илЩI Є №`йлJ №`кл ┤ №`ллJ / GROUP PARAMETERS: OSS №`мл v №* №hнлBIIPTYPE1 = мCRVAL1 л( time at reference pixel-first packet tim 8 № олTY/ PDTYPE1 = REAL*8 (Modified Julian D №@ол №#Date) C R №`плa R PSIZE1 = 64 I ` №h░л IPTYPE2 = мCRPIX1 л) pixel number of reference pixel in №`▒л R PDTYPE2 = REAL*4 C | №`▓л R PSIZE2 = 32 I К №h│лHPTYPE3 = мCD1_1 л* time increment between pixels (seconds) Ш №`┤л №R PDTYPE3 = REAL*4 C ж №`╡л R PSIZE3 = 32 I ┤ №h╢лRSJPTYPE4 = мDATAMIN л+ minimum data value in the group ┬ №`╖л= R PDTYPE4 = REAL*4 C ╨ №`╕л8 R PSIZE4 = 32 I ▐ №h╣лJPTYPE5 = мDATAMAX л, maximum data value in the group ь №`║л №R PDTYPE5 = REAL*4 C · №`╗лR PSIZE5 = 32 I №h╝лJPTYPE6 = мFILLCNT л- number of segments containing fill №`╜л №R PDTYPE6 = INTEGER*4 C $ №`╛лнR PSIZE6 = 32 I 2 №h┐лIPTYPE7 = мERRCNT л. number of segments containing errors @ №`└л №R PDTYPE7 = INTEGER*4 C N №`┴лR PSIZE7 = 32 I \ №h┬лJPTYPE8 = мFPKTTIMEл/ the time of the first packet j № ├л №/ PDTYPE8 = REAL*8 (Modified Julian mav №@├лn #Date) C л №dП┘ ЦЦ dР┘СС2 HH╘ИС┌Р HH╘ИОУ■.`─лLLR PSIZE8 = 64 I h┼л JPTYPE9 = мLPKTTIMEл0 the time of the last packet $ ╞л / PDTYPE9 = REAL*8 (Modified Julian 0@╞л#Date) C л>`╟лmeR PSIZE9 = 64 I Lh╚л IPTYPE10 = мCTYPE1 л1 the first coordinate type Z ╔л O PDTYPE10= CHARACTER*8 лf@╔лthC st t`╩л R PSIZE10 = 64 I В`╦л J Р`╠л Ю`═лJ / HSP DATA DESCRIPTOR KEYWORDS м`╬л ║h╧мGINSTRUMEл2= HSP instrument in use ╚h╨мGROOTNAMEл3= rootname of the observation set cke╓h╤мGFILETYPEл4= shp, udl, dst, dsk, ast, ask, asd, asa фh╥м) EBUNIT л5= COUNTS brightness units: COUNTS or DN (analog Є`╙л J `╘л fir`╒л J / CALIBRATION FLAGS AND INDICATORS `╓л *h╫мDMODE л6= instrument mode SCP, SSP, ARS 8h╪м GDETECTOBл7= detector in use (0-5) - object data Fh┘м GDETECTSKл8= detector in use (0-5) - sky data Th┌м GPTSRCFLGл9= point source flag (P=point, E=extended) bh█мGAPERTOBJл:= aperture in use - object data ph▄мGAPERTSKYл;= aperture in use - sky data n s~`▌лJ М`▐л Ъ`▀ллJ / CALIBRATION SWITCHES: perform,omit,complete и`рл ╢hсм GDET_CHR л<= retrieve detector characteristics `╒─hтм GDEADTIMEл== deadtime correction `╓╥hумGTRUE_CNTл>= compute the true count rates рhфмGTRUE_PHCл?= compute the true photocurrents a ю`хлJ №`цл м `чл= J / CALIBRATION KEYWORDS `шл= &hщм -GDATA_TYPл@= data type: digital, analog 4hъм -GDATA_SRCлA= data source: star, sky, area scan Bhым GDATA_FMTлB= data format: byte, word, lwrd, alog, all ллPhьм EWORDS лC= number of HSP samples in a line р^hэмELINES лD= number of lines in a group slhюмGINT_TIMEлE= time of integration (in 1/1.024 microsec zhямGTIMEBIASлF= instrument time bias (in 1/1.024 microse es dТ┘УУ HH╘ИУ┌ТntHH╘ИСХ■ . hЁм GSAMPTIMEлG= time of integration (in seconds) hём EDELAY лH= delay between integrations (seconds) $hЄм GDETECTORлI= detector used for this file , a2hєм GAPERTUREлJ= name of the aperture used for this file sk@hЇм GPA_APER лK= position ang of aperture used with targe woNhїмl GAPERAREAлL= aperature area s i\hЎм рGBDEXPFLGлM= bus director expander flag up jhўмGPT_EFFICлN= scaled point source cathode efficiency 1.0xh°мGEX_EFFICлO= scaled extended source cathode efficienc /1.Жh∙мGDARKRATEлP= scaled cathode dark rate У┌Фh·мGPRE_AMP лQ= scaled tube pre-amp contribution PTIвh√м GHIGHVOLTлR= scaled high voltage factor AY ░h№м GTUBEGAINлS= scaled tube gain factor R╛h¤м dFDEADTM лT= deadtime ╠h■м GCVCOFSETлU= scaled CVC offset APE┌h м FVGAIND лV= gain setting ш`л J Ў`л b`лerJ / CALIBRATION TABLE NAMES `л c e e hмDCCP0 лW= aperture area table name ca.hм1.DCCP1 лX= high voltage factor table name r<hм DCCP2 лY= gain factor table name -aJhм DCCP3 лZ= pre-amplifier noise table name vXhм DCCP4 л[= relative sensitivity table name tufh м DCCP5 л\= dark signal table name tith м DCCP7 л]= CVC offset table name leВhмнDCCP8 л^= dead time table name gaРhм DCCP9 л_= dark aperture translation table name Ю` л J м`л/ RAT║`л J / PHOTOMETRY KEYWORDS ╚`л per╓hмmeGGRAPHTABл`= the HST graph table volфhмnaGCOMPTAB лa= the HST components table or Єhм GPHOTMODEлb= Photometric Mode nohм GPHOTFLAMлc= 0.0 Inverse Sensitivity ityhм GPHOTZPT лd= 0.0 Zero Point e hмtiGPHOTPLAMлe= 0.0 Pivot Wavelength *hмFPHOTBW лf= 0.0 RMS Bandwidth of the Filter 8`лJ F`л ` T`л J / STATISTICAL KEYWORDS b`л `phм DDATE лg= date this file was written (dd/mm/yy) ~hмGPODPSFF лh= 0=(no podps fill); 1=(podps fill presen dФ┘naХХ HH╘ИХ┌Ф HH╘ИУЦ■MO.hмtoGSTDCFFF лi= 0=(no st dcf fill); 1=(st dcf fill prese hмerGSTDCFFP лj= st dcf fill pattern (hex) $` лo J 2`!лot len@`"л J / APERTURE POSITION N`#л \h$мGRA_APER лk= right ascension of the aperture (deg) jh%мGDEC_APERлl= declination of the aperture (deg) x`&л J Ж`'лfi s wФ`(л J / EXPOSURE INFORMATION в`)лn ░h*мGEQUINOX лm= J2000 equinox of the celestial coordinate syst H╛h+мGSUNANGLEлn= angle between sun and V1 axis (deg) ╠h,мllGMOONANGLлo= angle between moon and V1 axis (deg) ┌h-мteGSUN_ALT лp= altitude of the sun above Earth╒s limb ( шh.м GFGSLOCK лq= commanded FGS lock (FINE,COARSE,GYROS,UN л Ў`/л J `0л мh1м= GDATE-OBSлr= UT date of start of observation (dd/mm/y м h2м= GTIME-OBSлs= UT time of start of observation (hh:mm:s л .h3м GEXPSTARTлt= exposure start time (Modified Julian Dat лfi<h4мFEXPEND лu= exposure end time (Modified Julian Date) Jh5мGEXPTIME лv= exposure duration (seconds)--calculated uinXh6мl GEXPFLAG лw= Exposure interruption indicator glef`7л1 J t`8лV1 (dВ`9лJ / TARGET & PROPOSAL ID Р`:л h.Юh;мGTARGNAMEлx= proposer╒s target name `/мh<мGRA_TARG лy= right ascension of the target (deg) (J20 `0║h=мGDEC_TARGлz= declination of the target (deg) (J2000) n (╚h>мGPEQUINOXл{= proposed equinox of celestial coordinate n (╓`?лJ ф`@л h4ЄhAмuGPROPOSIDл|= PEP proposal identifier мhBм= GPEP_EXPOл}= PEP exposure identifier including sequen мl hCм= GLINENUM л~= PEP proposal line number л1 hDм GSEQLINE л= PEP line number of defined sequence лV1*hEмGSEQNAME лА= PEP define/use sequence name 8`FлJ F`Gл ThHмEND лБ b`Ъб rp`Iбth a~`Jб0 HH╘ИЦ┌П= HH╘ИХЩ■ (, `Kб> #UT UTкк`Nг= HIGH SPEED PHOTOMETER ox =UR UTккhOгinAREA SCAN HEADER В лL №`Pл Z №`Qл h №hRм FSIMPLE лГ= F image conforms to the fits standard v №hSмl FBITPIX лД= 32 bits per data value Д №hTмosGDATATYPEлЕ= REAL*4 datatype of the array = Т №hUмpoENAXIS лЖ= 2 number of data axes а №hVм lFNAXIS1 лЗ= length of 1st data axis о №hWм PFNAXIS2 лИ= length of 2nd data axis ╝ №hXм FGROUPS лЙ= T image is in group format ╩ №hYмHFGCOUNT лК= 1 number of groups ╪ №hZм FPCOUNT лЛ= 18 number of group parameters ц № [лO PSIZE = 768 bits in the group parameter block hOЄ №@[лADI В №`\лPJ №`]лe rms №`^лarJ / GROUP PARAMETERS: OSS * №`_л Д №8 №h`лDAIPTYPE1 = мCRVAL1 лМ right ascension of reference pixel (deg) №F №`aлNAR PDTYPE1 = REAL*8 C T №`bлЗR PSIZE1 = 64 I b №hcл IPTYPE2 = мCRVAL2 лН declination of reference pixel (deg) лp №`dлimR PDTYPE2 = REAL*8 C ~ №`eлouR PSIZE2 = 64 I М №hfлrsIPTYPE3 = мCRPIX1 лО x-coordinate of reference pixel Ъ №`gлr R PDTYPE3 = REAL*4 C и №`hл R PSIZE3 = 32 I ╢ №hiл IPTYPE4 = мCRPIX2 лП y-coordinate of reference pixel ─ №`jл №R PDTYPE4 = REAL*4 C ╥ №`kлR PSIZE4 = 32 I р №hlлHPTYPE5 = мCD1_1 лР partial of the right ascension w.r.t. x ю №`mл №R PDTYPE5 = REAL*4 C № №`nлR PSIZE5 = 32 I №hoлHPTYPE6 = мCD1_2 лС partial of the right ascension w.r.t. y №`pл №R PDTYPE6 = REAL*4 C & №`qлR PSIZE6 = 32 I 4 №hrлHPTYPE7 = мCD2_1 лТ partial of the declination w.r.t. x B №`sл №R PDTYPE7 = REAL*4 C P №`tлR PSIZE7 = 32 I ^ №huлHPTYPE8 = мCD2_2 лУ partial of the declination w.r.t. y l №`vл №R PDTYPE8 = REAL*4 C z №`wлR PSIZE8 = 32 I dЧ┘ZEЮЮ dШ┘ ЩЩHH╘ИЩ┌ШHH╘ИЦЫ■.t/ hxл №JPTYPE9 = мDATAMIN лФ the minimum value of the data `yлR PDTYPE9 = REAL*4 C $`zлR PSIZE9 = 32 I 2h{л №JPTYPE10 = мDATAMAX лХ the maximum value of the data @`|лR PDTYPE10= REAL*4 C N`}лR PSIZE10 = 32 I \h~л №JPTYPE11 = мMIR_REVRлЦ is the image mirror reversed j`лR PDTYPE11= LOGICAL*4 C x`АлR PSIZE11 = 32 I ЖhБлJPTYPE12 = мORIENTATлЧ the orientation of the image (deg) Ф`ВлR PDTYPE12= REAL*4 C в`ГлR PSIZE12 = 32 I ░hДлJPTYPE13 = мFILLCNT лШ number of segments containing fill ╛`ЕлR PDTYPE13= INTEGER*4 C ╠`ЖлR PSIZE13 = 32 I ┌hЗлIPTYPE14 = мERRCNT лЩ number of segments containing errors ш`ИлR PDTYPE14= INTEGER*4 C Ў`ЙлR PSIZE14 = 32 I hКлJPTYPE15 = мFPKTTIMEлЪ the time of the first packet Лл/ PDTYPE15= REAL*8 (Modified Julian th@Ллhe#Date) C л,`Мл4 R PSIZE15 = 64 I :hНл JPTYPE16 = мLPKTTIMEлЫ the time of the last packet H Ол= / PDTYPE16= REAL*8 (Modified Julian ng T@Ол#Date) C b`Пл R PSIZE16 = 64 I phРл IPTYPE17 = мCTYPE1 лЬ the first coordinate type C~ Слr O PDTYPE17= CHARACTER*8 К@Сл C Ш`Тл R PSIZE17 = 64 I жhУл IPTYPE18 = мCTYPE2 лЭ the second coordinate type h┤ Фл O PDTYPE18= CHARACTER*8 └@ФлDaC ╬`Хл R PSIZE18 = 64 I ▄`Цл J ъ`Чл °`Шл= J / HSP DATA DESCRIPTOR KEYWORDS `Щл hЪмGINSTRUMEлЮ= HSP instrument in use "hЫмGROOTNAMEлЯ= rootname of the observation set e 0hЬмGFILETYPEла= shp, udl, dst, dsk, ast, ask, asd, asa >hЭм EBUNIT лб= COUNTS brightness units: COUNTS or DN (analog L`Юл J Z`Ял sech`алe J / CALIBRATION FLAGS AND INDICATORS v`бл ДhвмDMODE лв= instrument mode SCP, SSP, ARS dЪ┘ ЫЫHH╘ИЫ┌Ъ HH╘ИЩЭ■ . hгмЧGDETECTOBлг= detector in use (0-5) - object data OR hдм GAPERTOBJлд= aperture in use - object data $`елtrJ 2`жлtn f t@`зл J / GENERIC CONVERSION KEYWORDS N`илsd \hймЭGDATA_TYPле= data type: digital, analog jhкм GDATA_SRCлж= AREA SCAN data source: star, sky, area scan xhлм GDATA_FMTлз= data format: byte, word, lwrd, alog, all INЖ`млJ Ф`нл m CP,в`ол J / CALIBRATION KEYWORDS ░`пл H╛h░мEWORDS ли= number of HSP words samples in a line ╠h▒м uELINES лй= number of lines in a group ┌h▓мe GINT_TIMEлк= time of integration (in 1/1.024 microsec шh│м GTIMEBIASлл= instrument time bias (in 1/1.024 microse Ўh┤м GSAMPTIMEлм= time of integration (in seconds) h╡мEDELAY лн= delay between integrations (seconds) oh╢м GBDEXPFLGло= bus director expander flag , a `╖л J .`╕лIN <`╣лБJ / STATISTICAL KEYWORDS J`║лP, Xh╗м DDATE лп= date this file was written (dd/mm/yy) fh╝м GPODPSFF л░= 0=(no podps fill); 1=(podps fill presen samth╜м GSTDCFFF л▒= 0=(no st dcf fill); 1=(st dcf fill prese up Вh╛мGSTDCFFP л▓= st dcf fill pattern (hex) 1.0Р`┐лJ Ю`└л м`┴лJ / APERTURE POSITION ║`┬лл ╚h├мweGRA_APER л│= right ascension of the aperture (deg) ╓h─мr GDEC_APERл┤= declination of the aperture (deg) ф`┼л J Є`╞л / `╟лDSJ / EXPOSURE INFORMATION `╚л= h╔м wGEQUINOX л╡= J2000 equinox of the celestial coordinate syst *h╩мllGSUNANGLEл╢= angle between sun and V1 axis (deg) 8h╦мllGMOONANGLл╖= angle between moon and V1 axis (deg) Fh╠мteGSUN_ALT л╕= altitude of the sun above Earth╒s limb ( Th═м GFGSLOCK л╣= commanded FGS lock (FINE,COARSE,GYROS,UN лb`╬л J p`╧л мwe~h╨м= GDATE-OBSл║= UT date of start of observation (dd/mm/y мr dЬ┘liЭЭ (HH╘ИЭ┌Ь HH╘ИЫЮ■ . h╤мGTIME-OBSл╗= UT time of start of observation (hh:mm:s / h╥мONGEXPSTARTл╝= exposure start time (Modified Julian Dat h╔$h╙мFEXPEND л╜= exposure end time (Modified Julian Date) 2h╘мGEXPTIME л╛= exposure duration (seconds)--calculated @h╒мGEXPFLAG л┐= Exposure interruption indicator N`╓лJ \`╫л = j`╪лedJ / TARGET & PROPOSAL ID x`┘л Жh┌м GTARGNAMEл└= proposer╒s target name = Фh█м oGRA_TARG л┴= right ascension of the target (deg) (J20 вh▄м (GDEC_TARGл┬= declination of the target (deg) (J2000) ░h▌мGPEQUINOXл├= proposed equinox of celestial coordinate n (╛`▐лJ ╠`▀л h╙┌hрм╜GPROPOSIDл─= PEP proposal identifier мшhсм= GPEP_EXPOл┼= PEP exposure identifier including sequen мЎhтм= GLINENUM л╞= PEP proposal line number лhум GSEQLINE л╟= PEP line number of defined sequence лhфмGSEQNAME л╚= PEP define/use sequence name `хлJ .`цл <hчмEND л╔ J`Mб rX`Lбth af`шб t`щбDE AВ`ъб dР`ыбta tЮ`ьб м`эбPE N║`юбн p╚`яб c s╓`Ёб ( ф`ёб Є`Єб `єб `Їб `їб ╙*`Ўб╜ R8`ўб F`°бen iT`∙б b`·б= Ep`√б ~`№бen iHH╘ИЮ┌ЧHH╘ИЭб■ p,l `¤б #UT UTкк` гHIGH SPEED PHOTOMETER = =UR UTккhгe UNIQUE DATA LOG ╩ L №`л hфZ №`л h №hмusFSIMPLE л╦= F image conforms to the fits standard v №hм FBITPIX л╠= 16 bits per data value Д №hмGDATATYPEл═= UNSIGNED*2 datatype of the array бТ №hмщENAXIS л╬= 1 number of data axes ьа №hмFNAXIS1 л╧= 965 length of 1st data axis о №hмFGROUPS л╨= T image is in group format ╝ №h мFGCOUNT л╤= 1 number of groups ╩ №h м iFPCOUNT л╥= 3 number of group parameters ╪ № лenO PSIZE = 128 bits in the group parameter block pф №@лI б Є №`л J №` л hф №`лJ / GROUP PARAMETERS: OSS №`л v №* №hлBIJPTYPE1 = мFILLCNT л╙ number of segments containing fill 8 №`лTYR PDTYPE1 = INTEGER*4 C F №`л╬R PSIZE1 = 32 I T №hлюIPTYPE2 = мERRCNT л╘ number of segments containing errors лb №`лimR PDTYPE2 = INTEGER*4 C p №`лouR PSIZE2 = 32 I ~ №hлrsJPTYPE3 = мPKTTIME л╒ time from the packet ancillary data М № лr / PDTYPE3 = REAL*8 (Modified Julian б Ш №@л #Date) C ж №`л R PSIZE3 = 64 I ┤ №`лRSJ ┬ №`л= ILL╨ №`лerJ / HSP DATA DESCRIPTOR KEYWORDS ▐ №`л ь №hм GINSTRUMEл╓= HSP instrument in use · №hм GROOTNAMEл╫= rootname of the observation set ╘ №hмs GFILETYPEл╪= UDL shp, udl, dst, dsk, ast, ask, asd, asa №h м FCTYPE1 л┘= UNITLESS unitless, line, pixel, channel, sample, $ №`!л J 2 №`"л╒ e f@ №`#лilJ / SCIENCE FILE SETS: T=present,F=absent N №`$л @\ №h%м GDST_FILEл┌= digital star science is present j №h&м GDSK_FILEл█= digital sky science is present x №h'м GAST_FILEл▄= analog star science is present `dЯ┘TAдд dа┘ббHH╘Иб┌а HH╘ИЮг■ . №h(мROGASK_FILEл▌= analog sky science is present №h)мFIGASD_FILEл▐= area scan digital is present №$h*мCTGASA_FILEл▀= area scan analog is present 2`+л J @`,л f N`-л J / STATISTICAL KEYWORDS \`.л jh/мFIDDATE лр= date this file was written (dd/mm/yy) №x`0лDSJ Ж`1лAS EФ`2л aJ / CDBS KEYWORDS в`3л ░h4м┘GVDATAFMTлс= Format of current observation ╛h5мGVFAPVECXлт= x cmp apt vct f/ tav ╠h6мнGVFAPVECYлу= y cmp apt vct f/ tav ┌h7мigGVFCENVEXлф= x cmp trg ct vct tav шh8мnaGVFCENVEYлх= y cmp trg ct vct tav Ўh9м GVFCTVECXлц= x cmp crs trg vt tav `-h:м GVFCTVECYлч= y cmp crs trg vt tav `.h;мGVFFTVECXлш= x cmp fn trg vct tav /yy h<мGVFFTVECYлщ= y cmp fn trg vct tav .h=мGVFOBJCNTлъ= count of trg obj <h>м GVFPFACTXлы= tav vct cnv fctr - x TJh?м FGVFPFACTYль= tav vct vnv fctr - y XXh@м xGVFSLWVEXлэ= x cmp slew vct tav YfhAм yGVFSLWVEYлю= y cmp slew vct tav XthBм xGVGAIND1 ля= gain setting of detector 1 YВhCм yGVGAIND2 лЁ= gain setting of detector 2 XРhDм xGVGAIND3 лё= gain setting of detector 3 YЮhEм yGVGAIND4 лЄ= gain setting of detector 4 XмhFм xGVGAIND5 лє= gain setting of detector 5 Y║hGм yGVGAINDS лЇ= gain setting of detector "sky" T╚hHм cGVHIVOLT1лї= high voltage setting for detector 1 X╓hIм tGVHIVOLT2лЎ= high voltage setting for detector 2 YфhJм tGVHIVOLT3лў= high voltage setting for detector 3 XЄhKм xGVHIVOLT4л°= high voltage setting for detector 4 YhLм yGVHIVOLT5л∙= high voltage setting for detector 5 hMм gGVHIVOLTSл·= high voltage setting for detector "sky" hNм gGVHORSTPTл√= no. of horiz steps/spatial point in area *hOм gGVHPOINTSл№= no. of horiz points (columns) in area sc 8hPм gGVNOINTPTл¤= no. of integrations/pt in area scans FhQм gGVPADTHR1л■= PAD threshold setting for detector 1 ThRм gGVPADTHR2л = PAD threshold setting for detector 2 1bhSм hGVPADTHR3л = PAD threshold setting for detector 3 2phTм hGVPADTHR4л = PAD threshold setting for detector 4 3~hUм hGVPADTHR5л = PAD threshold setting for detector 5 4dв┘гг HH╘Иг┌вHH╘Ибд■r .orhVмGVPADTHRSл = PAD threshold setting for detector "sky" torhWмGVHORIZ1 л = Horizontal deflection for detector 1 nt $hXмGVHORIZ2 л = Horizontal deflection for detector 2 in 2hYмGVHORIZ3 л = Horizontal deflection for detector 3 sc@hZмGVHORIZ4 л = Horizontal deflection for detector 4 ctoNh[мFVVERT1 л = Vertical deflection for detector 1 \h\мFVVERT2 л = Vertical deflection for detector 2 jh]мFVVERT3 л = Vertical deflection for detector 3 xh^м FVVERT4 л = Vertical deflection for detector 4 Жh_м5 GVREQDET л = requested detector for the object observ HФh`мGVSKYDET л = currently selected sky detector hVвhaм GVVERSTPTл = no. of vert. steps/spatial pt. in area s hW░hbм GVVPOINTSл = no. of vertical points (rows) in area sc hX╛hcм GVOLTAGE л = commanded high voltage setting of obj de hY╠hdм FTHRESH л = PAD threshold setting for the object det ┌heмFVHORIZ л = commanded horizontal deflection of obj d шhfмT1EVVERT л = commanded vertical deflection of obj det ЎhgмT2GVFOCUSD1л = focus command value for detector 1 hhмлGVFOCUSD2л = focus command value for detector 2 h^hiм GVFOCUSD3л = focus command value for detector 3 м5 hjмGVFOCUSD4л = focus command value for detector 4 м.hkм= GVFOCUSD л = focus command value for object detector м <`lл= J / TARGET & PROPOSAL ID J`mл= Xhnм pGTARGNAMEл = proposer╒s target name fhoмvoGRA_TARG л = right ascension of the target (deg) (J20 thpмttGDEC_TARGл = declination of the target (deg) (J2000) coВhqм dGPEQUINOXл = proposed equinox of celestial coordinate andР`rлtiJ Ю`sлec мhtмGPROPOSIDл = PEP proposal identifier ║huмGPEP_EXPOл = PEP exposure identifier including sequen ╚hvмGLINENUM л = PEP proposal line number ╓hwмGSEQLINE л = PEP line number of defined sequence ectфhxмGSEQNAME л != PEP define/use sequence name Є`yлJ `zл h{мEND л " `■б r*`|бth a8`}б F`~бDE AT`б db`Абta tp`Ббco ~`ВбPE NHH╘Ид┌ЯuiHH╘Игз■,ti`Гб #UT UTкк`Ег HIGH SPEED PHOTOMETER =UR UTккhЖгsSTANDARD HEADER PACKET # L №`Зл= Z №`Илen r h №hЙм FSIMPLE л $= F image conforms to the fits standard v №hКмn FBITPIX л %= 16 bits per data value Д №hЛм GDATATYPEл &= UNSIGNED*2 datatype of the array r oТ №hМм ENAXIS л '= 1 number of data axes sа №hНм FNAXIS1 л (= 965 length of 1st data axis о №hОм FGROUPS л )= T image is in group format ╝ №hПмFGCOUNT л *= 1 number of groups ╩ №hРмFPCOUNT л += 3 number of group parameters ╪ № СлO PSIZE = 128 bits in the group parameter block ,tiф №@Сл I #UTЄ №`ТлHIJ №`Ул= №`ФлenJ / GROUP PARAMETERS: OSS №`Хл v №* №hЦлBIJPTYPE1 = мFILLCNT л , number of segments containing fill 8 №`ЧлTYR PDTYPE1 = INTEGER*4 C F №`Шл'R PSIZE1 = 32 I T №hЩл IPTYPE2 = мERRCNT л - number of segments containing errors лb №`ЪлimR PDTYPE2 = INTEGER*4 C p №`ЫлouR PSIZE2 = 32 I ~ №hЬлrsJPTYPE3 = мPKTTIME л . time from the packet ancillary data М № Элr / PDTYPE3 = REAL*8 (Modified Julian #UTШ №@ЭлHI#Date) C ж №`Юл R PSIZE3 = 64 I ┤ №`ЯлRSJ ┬ №`ал= ILL╨ №`блerJ / HSP DATA DESCRIPTOR KEYWORDS ▐ №`вл ь №hгм GINSTRUMEл /= HSP instrument in use · №hдм GROOTNAMEл 0= rootname of the observation set - №hемs GFILETYPEл 1= SHP shp, udl, dst, dsk, ast, ask, asd, asa №hжм FCTYPE1 л 2= UNITLESS unitless, line, pixel, channel, sample, $ №hзм GDEFAULTSл 3= F default values used in reformatting thes = 2 №`ил.J @ №`йл fieN №`клJ / STATISTICAL KEYWORDS \ №`лл j №hмм DDATE л 4= date this file was written (dd/mm/yy) x №hнм GDCFOBSN л 5= DCF observation number in SHP dж┘P зз DSHH╘Из┌жHH╘Идй■RU. hомtrGPROC_TYPл 6= NORMAL level of reprocessing (NORMAL, MINOR, MA `плtnJ $`░л, dst2`▒лsdJ / TIME CONVERSION KEYWORDS @`▓лsa Nh│м GCLKDRFTRл 7= spacecraft clock drift rate = \h┤м.GCLKRATE л 8= spacecraft clock rate jh╡м GSPCLINCNл 9= spacecraft clock at UTC0 ICAxh╢м EUTCO1 л := bytes 5-8 of UTC0 =Жh╖мhiEUTCO2 л ;= bytes 1-4 of UTC0 Фh╕м oDUTC0 л <= Coordinated Universal Time (Mod Julian D в`╣лJ ░`║л ╛`╗л_TJ / CDBS KEYWORDS ╠`╝л ┌h╜м GVCVAMP1 л == current-voltage amplifier 1 шh╛м GVCVAMP2 л >= current-voltage amplifier 2 Ўh┐м GVCVAMP3 л ?= current-voltage amplifier 3 rah└м= GVCVAMP4 л @= current-voltage amplifier 4 h┴м GVCVAMP5 л A= current-voltage amplifier 5 C0 h┬мCAGVDT1M15 л B= detector supply 1 M15 .h├мGVDT1P05 л C= detector supply 1 P05 <h─мGVDT1P15 л D= detector supply 1 P15 uliJh┼мGVDT2M15 л E= detector supply 2 M15 Xh╞мGVDT2P05 л F= detector supply 2 P05 fh╟м GVDT2P15 л G= detector supply 2 P15 th╚м cGVDT3M15 л H= detector supply 3 M15 Вh╔м cGVDT3P05 л I= detector supply 3 P05 Рh╩м cGVDT3P15 л J= detector supply 3 P15 Юh╦м cGVDT4M15 л K= detector supply 4 M15 мh╠м cGVDT4P05 л L= detector supply 4 P05 ║h═м dGVDT4P15 л M= detector supply 4 P15 ╚h╬м dGVDT5M15 л N= detector supply 5 M15 ╓h╧м dGVDT5P05 л O= detector supply 5 P05 фh╨м dGVDT5P15 л P= detector supply 5 P15 Єh╤м dGVFOCUS1 л Q= focus 1 h╥м dGVFOCUS2 л R= focus 2 h╙м dGVFOCUS3 л S= focus 3 h╘м dGVFOCUS4 л T= focus 4 *h╒м dGVFTAVERRл U= TAV error status 8h╓м dGVHDEFL1 л V= horizontal deflection 1 Fh╫м dGVHDEFL2 л W= horizontal deflection 2 Th╪м dGVHDEFL3 л X= horizontal deflection 3 bh┘м dGVHDEFL4 л Y= horizontal deflection 4 ph┌м dGVHVPSM1 л Z= HVPS 1 output monitor ~h█м dGVHVPSM2 л [= HVPS 2 output monitor dи┘ йй! HH╘Ий┌иHH╘Изл■ . h▄мGVHVPSM3 л \= HVPS 3 output monitor h▌мGVHVPSM4 л ]= HVPS 4 monitor output $h▐мGVHVPSM5 л ^= HVPS 5 output monitor 2h▀мGVTHRES1 л _= threshold 1 @hрмGVTHRES2 л `= threshold 2 NhсмGVTHRES3 л a= threshold 3 \hтмGVTHRES4 л b= threshold 4 jhумGVTHRES5 л c= threshold 5 xhфмGVTPAFB1 л d= temperature aft bulkhead 1 ЖhхмGVTPAFB2 л e= temperature aft bulkhead 2 ФhцмGVTPDEA1 л f= temperature DEA 1 вhчм HGVTPDEA2 л g= temperature DEA 2 ░hшм HGVTPDEA3 л h= temperature DEA 3 ╛hщм HGVTPDEA4 л i= temperature DEA 4 ╠hъм tGVTPDEA5 л j= temperature DEA 5 ┌hым tGVTPDET1 л k= temperature detector 1 шhьм tGVTPDET2 л l= temperature detector 2 Ўhэм tGVTPDET3 л m= temperature detector 3 hюм tGVTPDET4 л n= temperature detector 4 hям tGVTPDET5 л o= temperature detector 5 hЁм tGVTPFILT л p= temperature filter .hём tGVTPFWB1 л q= temperature forward bulkhead 1 <hЄм tGVTPFWB2 л r= temperature forward bulkhead 2 Jhєм tGVTPMTPA л s= temperature mount point A XhЇм tGVTPMTPB л t= temperature mount point B fhїм tGVTPMTPC л u= temperature mount point C thЎм tGVTPNP2C л v= temperature inboard P2 skin center Вhўм tGVTPNP3C л w= temperature inboard P3 skin center Рh°м tGVTPODP2 л x= temperature P2 ODS radiator forward Юh∙м tGVTPODP3 л y= temperature P3 ODS radiator forward мh·м tGVTPODSA л z= temperature ODS aft ║h√м tGVTPPCDS л {= temperature PCDS ╚h№м tGVTPPSP2 л |= temperature PCDS/SCN bay P2 skin ╓h¤м tGVTPPSP3 л }= temperature PCDS/SCN bay P3 skin фh■м tGVTPRIUA л ~= temperature RIU A Єh м tGVTPRIUB л = temperature RIU B hм tGVTPSYCN л А= temperature system controller hм tGVVDEFL1 л Б= vertical deflection 1 hм tGVVDEFL2 л В= vertical deflection 2 *hмGVVDEFL3 л Г= vertical deflection 3 8hм tGVVDEFL4 л Д= vertical deflection 4 Fhм tEHVPSM л Е= high voltage power supply outpt of obj d DThм GDEA_TEMPл Ж= DEA temperature of the object detector PSPbhм GDET_TEMPл З= detector temperature of the object detec PSPphм FVFOCUS л И= focus of the object detector ~` л J dк┘tuлл" HH╘Ил┌кVTHH╘Ийн■te.ro` л `лFLJ / SUPPORT SCHEDULE: PROGRAMMATIC DATA $`лFL 2h мtiGPROGRMIDл Й= program id (base 36) @hмtiGPR_INV_Lл К= last name of principal investigator NhмtiGPR_INV_Fл Л= first name of principal investigator Е\hмvoGPR_INV_Mл М= middle initial of principal investigator = jhмpeGAFFILIATл Н= proposal class (eg: GO, IDT, OS) = xhмr GACCPDATEл О= proposal acceptance date (yyyyddd) = Жhм tGOBSET_IDл П= observation set id Фhм GCALIBRATл Р= Y calibrate data flag вhмGOBSERVTNл С= observation number (base 36) te░hмGEXPACKETл Т= expected number of source packets ULE╛hмA GPRODTYPEл У= output product medium type D╠hм pGOPFORMATл Ф= output product format specification L┌hм lGCALIBTYPл Х= calibration type : E, I or Blank Fшhм fGCDBSDATAл Ц= cdbs notification flag: ╒CAL╒ or ╒FALSE╒ MЎ`л mJ `л p al `л, J / SUPPORT SCHEDULE: FLAGS AND INDICATORS `лyy .hмGSS_MODE л Ч= instrument mode SCP, SSP, ARS <h мGSS_DETOBл Ш= detector in use (0-5) - object data Jh!мGSS_DETSKл Щ= detector in use (0-5) - sky data Xh"мGSS_PTSRCл Ъ= point source flag (P=point, E=extended) fh#мGRTAMATCHл Ы= above f&i match RTA (TRUE,FALSE,NO RTA F t`$лJ В`%л м lР`&л= J / SUPPORT SCHEDULE: DATA GROUP II DATA Ю`'л= мh(мonGWRD11_14л Ь= word 11/14 (0-255) ║h)м GPSTRTIMEл Э= predicted obs. start time (yyyy.ddd:hh:m л, ╚h*м GPSTPTIMEл Ю= predicted obs. stop time (yyyy.ddd:hh:mm лyy╓h+мGAPEROBJ л Я= si object aperture id фh,мGAPERSKY л а= si sky aperture id a Єh-мGTARG_ID л б= SPSS target ID from proposal+target no. h.мGAPERTYPEл в= aperture type (SICS, SIAS, SIDS) ndeh/мERA_V1 л г= 0.0 right ascension of v1 axis of st (deg) Nh0мFDEC_V1 л д= 0.0 declination of v1 axis of st (deg) *h1мEPA_V3 л е= 0.0 position angle of v3 axis of st (deg) P8h2м GGAPEROFFXл ж= 0.0 x comp of object offset in aperture (arc мonFh3м= GAPEROFFYл з= 0.0 y comp of object offset in aperture (arc м Th4м= GANGLESEPл и= 0.0 ang separation of target from ref obj (a м bh5м= GDGESTAR л й= FGS ID(F1,F2,F3) concat. w/ dom. gd. sta мph6м= GSGESTAR л к= FGS ID(F1,F2,F3) concat. w/ subdom. gd. м~h7м= GPA_APER л л= 0.0 position ang of aperture used with targe мdм┘S нн#l+HH╘Ин┌мHH╘Илп■pe., h8м FPA_REF л м= 0.0 position ang of target from ref. object h9м) GSAAAVOIDл н= SAA model for SAA Avoidance (range 02-99 xis$h:м GTARAQMODл о= target acquisition mode (values 00, 01, s o2h;мGPOSTNSTXл п= 0.0 position of space telescope x axis (km) ap@h<мGPOSTNSTYл ░= 0.0 position of space telescope y axis (km) apNh=мGPOSTNSTZл ▒= 0.0 position of space telescope z axis (km) rom\h>мGVELOCSTXл ▓= 0.0 vel of space telescope along x axis (km/ / djh?мGVELOCSTYл │= 0.0 vel of space telescope along y axis (km/ / sxh@мGVELOCSTZл ┤= 0.0 vel of space telescope along z axis (km/ sedЖhAмFRA_SUN л ╡= 0.0 right ascension of the sun (deg) ФhBмGDEC_SUN л ╢= 0.0 declination of the sun (deg) FPAвhCм GRA_MOON л ╖= 0.0 right ascension of the moon (deg) AVO░hDм GDEC_MOONл ╕= 0.0 declination of the moon (deg) AQM╛hEм GVELABBRAл ╣= 0.0 aberration in position of the target TNS╠hFм GANNPARRAл ║= 0.0 par. shift in position, non-solar sys ta TNS┌hGм GV2APERCEл ╗= 0.0 V2 offset of target from aper. center (a TNSшhHм GV3APERCEл ╝= 0.0 V3 offset of target from aper. center (a OCSЎhIм GEQRADTRGл ╜= 0.0 equatorial radius of target (km) OCShJм GFLATNTRGл ╛= 0.0 flattening of target OCShKм GNPDECTRGл ┐= 0.0 north pole declination of target (deg) SUN hLм GNPRATRG л └= 0.0 north pole right ascension of target (de .hMм dGROTRTTRGл ┴= 0.0 rotation rate of target <hNм rGLONGPMERл ┬= 0.0 longitude of prime meridian (deg) NJhOмGEPLONGPMл ├= 0.0 epoch of longitude of prime meridian (se AXhPм aGSURFLATDл ─= 0.0 surface feature latitude (deg) AfhQм pGSURFLONGл ┼= 0.0 surface feature longitude (deg) EthRм VGSURFALTDл ╞= 0.0 surface feature altitude (km) EВhSм VFMTFLAG л ╟= moving target flag; T if it is a moving РhTм GS0INVMAGл ╚= 0.0 S0 inverse magnitude TNTЮhUм FS0XDIR л ╔= 0.0 S0 X direction мhVм0 FS0YDIR л ╩= 0.0 S0 Y direction ║hWм= FS0ZDIR л ╦= 0.0 S0 Z direction ╚hXм GTRK_TYPEл ╠= track 48 or track 51 commanding used (T4 hN╓hYм GT51_RATEл ═= 0.0 rate of motion commanded (arcsecs/sec) hOфhZм┘GT51_ANGLл ╬= 0.0 position angle of motion of aperture (de hPЄh[м GTARGDISTл ╧= distance to target from Earth╒s center ( hQh\м GPAR_CORRл ╨= parallax correction used (T or F) hRh]м FRA_REF л ╤= 0.0 right ascension of reference object (deg h^млGDEC_REF л ╥= 0.0 declination of reference object (deg) hT*`_л J 8``л ╔ 0 F`aлonJ / ONBOARD EPHEMERIS MODEL PARAMETERS T`bл bhcмGEPCHTIMEл ╙= 0.0 epoch time of parameters (secs since 1/1 phdмGSDMEANANл ╘= 0.0 2nd deriv coef for mean anomaly (revs/se g u~heмGSDMA3SQ л ╒= 0.0 3 * (SDMEANAN**2) radians/second**2. ecsdо┘пп$ HH╘Ип┌оrtHH╘Ин▒■.= hfмe GHSTHORB л ╓= 0.0 half the duration of the ST orbit (secon = hgмx GCIRVELOCл ╫= 0.0 circular orbit linear velocity (meters/s = 0$hhмceGCOSINCLIл ╪= 0.0 cosine of inclination .0 2hiм oGECCENTRYл ┘= 0.0 eccentricity @hjм GECCENTX2л ┌= 0.0 eccentricity times 2 `aNhkм GECBDX4D3л █= 0.0 eccentricity cubed times 4/3 `b\hlмGESQDX5D2л ▄= 0.0 eccentricity squared times 5/2 sijhmмFECBDX3 л ▌= 0.0 eccentricity cubed times 3 xhnмGFDMEANANл ▐= 0.0 1st derivative coef for mean anomly (rev secЖhoмGRCASCNRDл ▀= 0.0 rt chge right ascension ascend node (rad п┌ФhpмGRCASCNRVл р= 0.0 rt chge right ascension ascend node (rev HORвhqм GARGPERIGл с= 0.0 argument of perigee (revolutions/second) VEL░hrм GMEANANOMл т= 0.0 mean anomaly (radians) INC╛hsм GRCARGPERл у= 0.0 rate change of argument of perigee (revs ENT╠htм GRASCASCNл ф= 0.0 right ascension of ascending node (revol ENT┌huм GSINEINCLл х= 0.0 sine of inclination DX4шhvм GSEMILRECл ц= 0.0 semi-latus rectum (meters) DX5Ўhwм GTIMEFFECл ч= 0.0 time parameters took effect (secs since DX3hxм GOBSSTRTTл ш= 0.0 predicted obs. start time (secs since 1/ N`yл 1J `zл r e r.`{лenJ / PROPOSAL INFO: Instrument Configuration <`|лen e (Jh}мFCONFIG л щ= proposed instrument configuration Xh~мFOPMODE л ъ= proposed operation mode fhмFSPEC_1 л ы= spectral element thАмNTFSPEC_2 л ь= spectral element ВhБмl FSPEC_3 л э= spectral element РhВм FSPEC_4 л ю= spectral element ЮhГм FAPER_1 л я= instrument aperture мhДм (FAPER_2 л Ё= instrument aperture ║hЕмmeFAPER_3 л ё= instrument aperture ╚hЖм FAPER_4 л Є= instrument aperture ╓`Зл J ф`Ил мЄ`Йл J / PROPOSAL INFO: Target Description `Кл prhЛмodGTAR_TYPEл є= target type ctrhМм GTARDESCRл Ї= target description l e*hНм GTARDESC2л ї= target description (cont.) eme8hОм GTARGCAT л Ў= first target category t FhПм GTARKEY1 л ў= target key description for targcat ThРм GTARKEY2 л °= target key description for targcat bhСмGTARKEY3 л ∙= target key description for targcat phТмGTARKEY4 л ·= target key description for targcat ~hУмGTARKEY5 л √= target key description for targcat d░┘▒▒% HH╘И▒┌░ THH╘Ип│■.КhФмGTARGCAT2л №= second target category hХмGTARKEY6 л ¤= target key description for targcat2 $hЦмGTARKEY7 л ■= target key description for targcat2 2hЧмGTARKEY8 л = target key description for targcat2 @hШмGTARKEY9 л= target key description for targcat2 gcaNhЩмGTARKEY10л= target key description for targcat2 gca\hЪмFALIAS1 л= synonym for target name jhЫмFALIAS2 л= synonym for target name x`Ьл J Ж`Эл Ф`ЮлJ / PROPOSAL INFO: Flux Information в`Ял ■░hамEMAG_V л= expected V Magnitude ╛hбм FSURF_V л= expected V surface brightness ╠hвм EMAG_B л= expected B Magnitude i┌hгм FSURF_B л= expected B surface brightness шhдмcaEMAG_U л= expected U Magnitude eЎhемtaFSURF_U л = expected U surface brightness hжмfoEMAG_R л = expected R Magnitude yhзмamFSURF_R л= expected R surface brightness hимGCOL_B_V л= expected B-V color .hйм GCOL_U_B л = expected U-B color <hкмOPGCOL_V_R л= expected V-R color ■JhлмEE_B_V л= E(B-V) Xhмм GEXTNCT_Vл= extinction in V ╠f`нлMAJ t`ол_B В`плctJ / PROPOSAL INFO: Exposure Information Р`░лU tudЮh▒м GCMD_EXP л= commanded time per exposure (from TRANS) briм`▓л J ║`│л ╚`┤ллJ / PROPOSAL INFO: Moving Target Information ╓`╡л фh╢мV GMT_LV1_1л= moving target information Єh╖мB GMT_LV1_2л= moving target information h╕мR GMT_LV1_3л= moving target information h╣м GMT_LV1_4л= moving target information h║м GMT_LV1_5л= moving target information *h╗м GMT_LV2_1л= moving target information лct8h╝м GMT_LV2_2л= moving target information лU Fh╜мGMT_LV2_3л= moving target information TRATh╛мGMT_LV2_4л= moving target information bh┐мGMT_LV2_5л= moving target information : Mph└мmaGMT_LV3_1л= moving target information 1~h┴м mGMT_LV3_2л= moving target information 2d▓┘nf││& HH╘И│┌▓HH╘И▒╡■on. h┬мGMT_LV3_3л= moving target information h├мGMT_LV3_4л= moving target information $h─мGMT_LV3_5л = moving target information 2`┼лJ @`╞л h╜N`╟лJ / PROPOSAL INFO: Target Properties \`╚л jh╔мetGREDSHIFTл!= expected redshift of target xh╩мetGPARALLAXл"= expected parallax of target Жh╦мetEMU_RA л#= expected RA proper motion Фh╠мtaFMU_DEC л$= expected DEC proper motion вh═мGMU_EPOCHл%= epoch of the proper motion ■░h╬мGSP_TYPE л&= spectral type ╛h╧мGRAD_VEL л'= radial velocity (km/sec) ╠`╨лJ ┌`╤л ш`╥л J / PROPOSAL INFO: Spatial Scan Info Ў`╙л h╘м GSCAN_TYPл(= C:bostrophidon; D:╒C╒with dwell; N:unkno h╒мGSCAN_WIDл)= scan width (arcsec) t h╓мGANG_SIDEл*= angle between sides of parallelogram (de t .h╫мGDWELL_LNл+= dwell points per line for scan pointing <h╪мGDWELL_TMл,= wait time (duration) at each dwell point Jh┘мGSCAN_ANGл-= position angle of scan line (deg) Xh┌мGSCAN_RATл.= commanded rate of the line scan (arcsec/ fh█мGNO_LINESл/= number of lines per scan (1-99) th▄мGSCAN_LENл0= scan length (arcsec) Вh▌мGSCAN_CORл1= scan coordinate frame of ref: celestial, : SР`▐л J Ю`▀л C ropм`рлweJ / TARGET & PROPOSAL ID ║`сл ╚hтмGTARGNAMEл2= proposer╒s target name am ╓hумGRA_TARG л3= right ascension of the target (deg) (J20 ntiфhфмGDEC_TARGл4= declination of the target (deg) (J2000) poЄhхмGPEQUINOXл5= proposed equinox of celestial coordinate `цлJ `чл мhшм= GPROPOSIDл6= PEP proposal identifier м*hщм= GPEP_EXPOл7= PEP exposure identifier including sequen м8hъм= GLINENUM л8= PEP proposal line number л Fhым GSEQLINE л9= PEP line number of defined sequence л CThьмGSEQNAME л:= PEP define/use sequence name b`элJ p`юл ~hямEND л; d┤┘si╡╡' (HH╘И╡┌┤TAHH╘И│■tade`Дб%╟?H5▀v %╟?HDD in hнл м ▌Ї╙UDFH┤D┌v FK5 &·КCю╛qFрGDIJ =√ЫКC?&Ч╔7Ю1Х╣/╩2╓╟&·4H┤,ф 4"/Щ/A{3╝╙'├A2╨""/2°жКC+$nКC╪жgl ЕCiуGсFHDHK PМ┌iуgliуь7 +ьпiу#m▓iу■░м ╗FиhъЖУКC╨╛qHсGIDGJK P pМ┌КCЖУ&Ч╔щў1Х╣&╛^2╓╟/Оc4H┤)вJ4"&яi/A{"╦г'├A#╕S"/#П╨КCЛwКC╪жne 2°жКCїIсHJDFJ C2°жКC=√ЫКC■░м ╗Fи= &·КCю╛qJтIKDHK nFIgl .ШФ+H┤K┘JDGJq(du Leftdv Right dА ReferenceяdН╡dРdТ (dФdПdШdЪdЬdЧdа dв d Я┌d !жKd! 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