SIMPLE = T / Fits standard BITPIX = -32 / Bits per pixel NAXIS = 1 / Number of axes NAXIS1 = 1493 / Axis length EXTEND = F / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator DATE = '2005-02-11T11:05:10' / Date FITS file was generated IRAF-TLM= '11:05:10 (11/02/2005)' / Time of last modification NEXTEND = 3 / Number of standard extensions FILENAME= 'o62o10010_sx2.fits' / name of file FILETYPE= 'SCI ' / type of data found in data file TELESCOP= 'HST' / telescope used to acquire data INSTRUME= 'STIS ' / identifier for instrument used to acquire data EQUINOX = 2000.0 / equinox of celestial coord. system / DATA DESCRIPTION KEYWORDS ROOTNAME= 'o62o10010 ' / rootname of the observation setPRIMESI = 'STIS ' / instrument designated as prime / TARGET INFORMATION TARGNAME= '3C120.0-R ' / proposer's target name RA_TARG = 6.829591666667E+01 / right ascension of the target (deg) (J2000) DEC_TARG= 5.354294444444E+00 / declination of the target (deg) (J2000) / PROPOSAL INFORMATION PROPOSID= 8700 / PEP proposal identifier LINENUM = '10.002 ' / proposal logsheet line number PR_INV_L= 'Martel ' / last name of principal investigatorPR_INV_F= 'Andre ' / first name of principal investigator PR_INV_M= ' ' / middle name / initial of principal investigat / SUMMARY EXPOSURE INFORMATION TDATEOBS= '2000-09-25' / UT date of start of first exposure in file TTIMEOBS= '21:00:56' / UT start time of first exposure in file TEXPSTRT= 5.181287565794E+04 / start time (MJD) of 1st exposure in file TEXPEND = 5.181288012535E+04 / end time (MJD) of last exposure in the file TEXPTIME= 3.6000000E+02 / total exposure time (seconds) / TARGET OFFSETS (POSTARGS) POSTARG1= 0.000000 / POSTARG in axis 1 direction POSTARG2= 0.000000 / POSTARG in axis 2 direction / DIAGNOSTIC KEYWORDS OVERFLOW= 0 / Number of science data overflows OPUS_VER= 'OPUS 14.5a ' / OPUS software system version number CAL_VER = '2.15b (26-August-2003)' / CALSTIS code version PROCTIME= 5.304894473380E+04 / Pipeline processing time (MJD) / SCIENCE INSTRUMENT CONFIGURATION CFSTATUS= 'SUPPORTED ' / configuration status (support., avail., eng.) OBSTYPE = 'SPECTROSCOPIC ' / observation type - imaging or spectroscopic OBSMODE = 'ACCUM ' / operating mode PHOTMODE= 'STIS 52X0.2 A2D1 G430L CCD 4300' / observation con SCLAMP = 'NONE ' / lamp status, NONE or name of lamp which is on LAMPSET = '0.0 ' / spectral cal lamp current value (milliamps) NRPTEXP = 1 / number of repeat exposures in set: default 1 SUBARRAY= F / data from a subarray (T) or full frame (F) DETECTOR= 'CCD ' / detector in use: NUV-MAMA, FUV-MAMA, or CCD OPT_ELEM= 'G430L ' / optical element in use APERTURE= '52X0.2 ' / aperture name PROPAPER= '52X0.2 ' / proposed aperture name FILTER = 'Clear ' / filter in use APER_FOV= '52x0.2 ' / aperture field of view CENWAVE = 4300 / central wavelength of spectrum CRSPLIT = 2 / number of cosmic ray split exposures / ENGINEERING PARAMETERS CCDAMP = 'D ' / CCD amplifier read out (A,B,C,D) CCDGAIN = 1 / commanded gain of CCD CCDOFFST= 3 / commanded CCD bias offset / READOUT DEFINITION PARAMETERS CENTERA1= 532 / subarray axis1 center pt in unbinned dect. pix CENTERA2= 523 / subarray axis2 center pt in unbinned dect. pix SIZAXIS1= 1062 / subarray axis1 size in unbinned detector pixelsSIZAXIS2= 1044 / subarray axis2 size in unbinned detector pixelsBINAXIS1= 2 / axis1 data bin size in unbinned detector pixelsBINAXIS2= 2 / axis2 data bin size in unbinned detector pixels / CALIBRATION SWITCHES: PERFORM, OMIT, COMPLETE DQICORR = 'COMPLETE' / data quality initialization ATODCORR= 'OMIT ' / correct for A to D conversion errors BLEVCORR= 'COMPLETE' / subtract bias level computed from overscan img BIASCORR= 'COMPLETE' / Subtract bias image CRCORR = 'COMPLETE' / combine observations to reject cosmic rays RPTCORR = 'OMIT ' / add individual repeat observations EXPSCORR= 'PERFORM ' / process individual observations after cr-rejectDARKCORR= 'COMPLETE' / Subtract dark image FLATCORR= 'COMPLETE' / flat field data SHADCORR= 'OMIT ' / apply shutter shading correction STATFLAG= T / Calculate statistics? WAVECORR= 'COMPLETE' / use wavecal to adjust wavelength zeropoint X1DCORR = 'PERFORM ' / Perform 1-D spectral extraction BACKCORR= 'PERFORM ' / subtract background (sky and interorder) HELCORR = 'COMPLETE' / convert to heliocenttric wavelengths DISPCORR= 'COMPLETE' / apply 2-dimensional dispersion solutions FLUXCORR= 'COMPLETE' / convert to absolute flux units X2DCORR = 'COMPLETE' / rectify 2-D spectral image / CALIBRATION REFERENCE FILES BPIXTAB = 'oref$h1v11475o_bpx.fits' / bad pixel table DARKFILE= 'oref$kap1603go_drk.fits' / dark image file name PFLTFILE= 'oref$n491401go_pfl.fits' / pixel to pixel flat field file name DFLTFILE= 'N/A ' / delta flat field file name LFLTFILE= ' ' / low order flat PHOTTAB = 'oref$ncc1900lo_pht.fits' / Photometric throughput table APERTAB = 'oref$n7p1032ao_apt.fits' / relative aperture throughput table CCDTAB = 'oref$n951041jo_ccd.fits' / CCD calibration parameters ATODTAB = 'N/A ' / analog to digital correction file BIASFILE= 'oref$kap16118o_bia.fits' / bias image file name SHADFILE= 'N/A ' / shutter shading correction file CRREJTAB= 'oref$j3m1403io_crr.fits' / cosmic ray rejection parameters WAVECAL = 'o62o10010_wav.fits ' / wavecal image file name APDESTAB= 'oref$n7p10329o_apd.fits' / aperture description table SPTRCTAB= 'oref$l2j0137so_1dt.fits' / spectrum trace table DISPTAB = 'oref$l2j0137to_dsp.fits' / dispersion coefficient table INANGTAB= 'oref$h5s11397o_iac.fits' / incidence angle correction table LAMPTAB = 'oref$l421050oo_lmp.fits' / template calibration lamp spectra table SDCTAB = 'oref$n7p1031ro_sdc.fits' / 2-D spatial distortion correction table XTRACTAB= 'oref$n7p1031qo_1dx.fits' / parameters for 1-D spectral extraction tabPCTAB = 'oref$n2o1817ho_pct.fits' / Photometry correction table WBIAFILE= 'oref$kap16118o_bia.fits' / associated wavecal bias image file name WCPTAB = 'oref$lag1815lo_wcp.fits' / wavecal parameters table TDSTAB = 'oref$nas13577o_tds.fits' / time-dependent sensitivity algorithm used / COSMIC RAY REJECTION ALGORITHM PARAMETERS MEANEXP = 1.8000000E+02 / reference exposure time for parameters SCALENSE= 0.0000000E+00 / multiplicative scale factor applied to noise INITGUES= 'minimum ' / initial guess method (MIN or MED) SKYSUB = 'none ' / sky value subtracted (MODE or NONE) CRSIGMAS= '4.0 ' / statistical rejection criteria CRRADIUS= 1.5000000E+00 / rejection propagation radius (pixels) CRTHRESH= 7.5000000E-01 / rejection propagation threshold BADINPDQ= 0 / data quality flag bits to reject REJ_RATE= 2.8186111E+01 / rate at which pixels are affected by cosmic rayCRMASK = T / flag CR-rejected pixels in input files (T/F) / CALIBRATED ENGINEERING PARAMETERS ATODGAIN= 1.0000000E+00 / calibrated CCD amplifier gain value READNSE = 4.1199999E+00 / calibrated CCD read noise value / TARGET ACQUISITION DATASET IDENTIFIERS ACQNAME = 'o62o10D4T ' / rootname of acquisition exposure ACQTYPE = ' ' / type of acquisition PEAKNAM1= ' ' / rootname of 1st peakup exposure PEAKNAM2= ' ' / rootname of 2nd peakup exposure / PATTERN KEYWORDS PATTERN1= 'STIS-ALONG-SLIT ' / primary pattern type P1_SHAPE= 'LINE ' / primary pattern shape P1_PURPS= 'DITHER ' / primary pattern purpose P1_NPTS = 2 / number of points in primary pattern P1_PSPAC= 0.15 / point spacing for primary pattern (arc-sec) P1_LSPAC= 0.000000 / line spacing for primary pattern (arc-sec) P1_ANGLE= 0.000000 / angle between sides of parallelogram patt (deg)P1_FRAME= 'POS-TARG ' / coordinate frame of primary pattern P1_ORINT= 90.0 / orientation of pattern to coordinate frame (degP1_CENTR= 'NO ' / center pattern relative to pointing (yes/no) / ARCHIVE SEARCH KEYWORDS BANDWID = 2800.0 / bandwidth of the data SPECRES = 800.0 / approx. resolving power at central wavelength CENTRWV = 4300.0 / central wavelength of the data MINWAVE = 2900.0 / minimum wavelength in spectrum MAXWAVE = 5700.0 / maximum wavelength in spectrum PLATESC = 0.1 / plate scale (arcsec/pixel) / PAPER PRODUCT SUPPORT KEYWORDS PROPTTL1= 'A STIS Spectroscopic Snapshot Survey of 3CR Radio Galaxies : The Nat'PROPTTL2= 'ure of the Unresolved Nuclei 'OBSET_ID= '10' / observation set id TARDESCR= 'GALAXY;RADIO GALAXY 'MTFLAG = ' ' / moving target flag; T if it is a moving target PARALLAX= 0.000000000000E+00 / target parallax from proposal MU_RA = 0.000000000000E+00 / target proper motion from proposal (degrees RA)MU_DEC = 0.000000000000E+00 / target proper motion from proposal (deg. DEC) MU_EPOCH= 'J2000.0' / epoch of proper motion from proposal / ASSOCIATION KEYWORDS ASN_ID = 'O62O10010 ' / unique identifier assigned to association ASN_TAB = 'o62o10010_asn.fits ' / name of the association table SKYSUM = 0.0000000E+00 / Total sky level (DN) EXPNAME = 'o62o10d6q ' / exposure identifier BUNIT = 'erg /s /cm**2 /angstrom /arcsec**2' / brightness units ASN_MTYP= 'CRSPLIT ' / Role of the Member in the Association / World Coordinate System and Related Parameters WCSAXES = 2 / number of World Coordinate System axes CRPIX1 = 1. / x-coordinate of reference pixel CRVAL1 = 2936.6110839844 / first axis value at reference pixel CTYPE1 = 'LINEAR ' / the coordinate type for the first axis CD1_1 = 4.8824939063024 / partial of first axis coordinate w.r.t. x LTM1_1 = 1. / reciprocal of sampling rate in X RA_APER = 6.829591666667E+01 / RA of aperture reference position DEC_APER= 5.354294444444E+00 / Declination of aperture reference position PA_APER = -1.364251007324E+02 / Position Angle of reference aperture center (deCUNIT1 = 'angstrom' / units of first coordinate value CUNIT2 = 'deg ' / units of second coordinate value / OFFSETS FROM ASSOCIATED WAVECAL SHIFTA1 = 3.017583333007E-01 / Spectrum shift in AXIS1 calculated from WAVECALSHIFTA2 = -2.118239142503E+00 / Spectrum shift in AXIS2 calculated from WAVECAL / EXPOSURE INFORMATION ORIENTAT= -136.02 / position angle of image y axis (deg. e of n) SUNANGLE= 114.471451 / angle between sun and V1 axis MOONANGL= 90.716515 / angle between moon and V1 axis SUN_ALT = -34.720493 / altitude of the sun above Earth's limb FGSLOCK = 'FINE ' / commanded FGS lock (FINE,COARSE,GYROS,UNKNOWN) DATE-OBS= '2000-09-25' / UT date of start of observation (yyyy-mm-dd) TIME-OBS= '21:00:56' / UT time of start of observation (hh:mm:ss) EXPSTART= 5.181287565794E+04 / exposure start time (Modified Julian Date) EXPEND = 5.181288012535E+04 / exposure end time (Modified Julian Date) EXPTIME = 3.6000000E+02 / exposure duration (seconds)--calculated EXPFLAG = 'NORMAL ' / Exposure interruption indicator V_HELIO = -2.548296463090E+01 / heliocentric radial velocity (km/sec) / PATTERN KEYWORDS PATTSTEP= 1 / position number of this point in the pattern PATT_POS= 1 / position number in pattern sequence / REPEATED EXPOSURES INFO NCOMBINE= 2 /4 / number of image sets combined during CR reje / DATA PACKET INFORMATION FILLCNT = 0 / number of segments containing fill ERRCNT = 0 / number of segments containing errors PODPSFF = F / podps fill present (T/F) STDCFFF = F / ST DDF fill present (T/F) STDCFFP = '0x5569' / ST DDF fill pattern (hex) / ENGINEERING PARAMETERS OSWABSP = 878392 / Slit Wheel Absolute position OMSCYL1P= 325 / Mode select cylinder 1 position OMSCYL3P= 5461 / Mode select cylinder 3 position OMSCYL4P= 3042 / Mode select cylinder 4 position OCBABAV = 26.7024 / (V) CEB A&B Amp Bias OCBCDAV = 26.6827 / (V) CEB C&D amp bias OCBLGCDV= -3.37895 / (V) CEB last gate C&D OCBSWALV= -6.00101 / (V) CB summing well A Lo OCBRCDLV= 0.029238 / (V) CB reset gate CD Lo OCCDHTAV= -1.000000 / average CCD housing temperature (degC) / IMAGE STATISTICS AND DATA QUALITY FLAGS NGOODPIX= 137151 / number of good pixels SDQFLAGS= 31743 / serious data quality flags GOODMIN = -1.3678532E-13 / minimum value of good pixels GOODMAX = 1.7684607E-13 / maximum value of good pixels GOODMEAN= 3.8885644E-16 / mean value of good pixels SNRMIN = -4.7056870E+00 / minimum signal to noise of good pixels SNRMAX = 1.5316234E+02 / maximum signal to noise of good pixels SNRMEAN = 7.5147432E-01 / mean value of signal to noise of good pixels SOFTERRS= 0 / number of soft error pixels (DQF=1) MEANDARK= 7.3949556E+00 / average of the dark values subtracted MEANBLEV= 1.1297627E+03 / average of all bias levels subtracted / PHOTOMETRY KEYWORDS SPORDER = 1 / Spectral order DIFF2PT = 2.4662878E-02 / Diffuse to point source conversion factor CONT2EML= 1.0819240E+01 / Intensity conversion: continuum -> emission SCALE_A1= 1.0000000E-01 / Size of one pixel (arcsec) along dispersion axiOMEGAPIX= 1.000000000000E-02 / Solid angle (arcsec**2) subtended by one pixel BANDID1 = 'spectrum: background none, weights none, clean no' APNUM1 = '1 1 299.62 301.62' WCSDIM = 1 CDELT1 = 4.8824939063024 WAT0_001= 'system=equispec' WAT1_001= 'wtype=linear label=Wavelength units=Angstroms' END 'ru'4'v'fI'Y߇'L@'H9'V'hy'b'S>'Ok'H1'>'9,'8)'@'Ox'W 'W;p'Y)K'['[U'X'T'Sm'\['d '_'W'U÷'S='M+'Eۻ'>'7K'1)H'2='1S'.ݍ'0'1'5'?'@'7'7|'='EG'Bp'9k2'7''9'8'=^'EJ'JL'LF\'P_i'Z~'jO'v'qN'b('YU'V'W0'Xj7'Zw$'['[t'\'c~{'j}'j18'dc'b4'fCy'g~'c&e'bk'b'^u'ZY'YF'X,'Y'['[W'Qf'G'Ly?'P'N;'J'KG'LDr'I^'C'C8'BՋ'A^'EA'O'Wp9'[<'^g'_M']Z'W 'O2'I('J~o'L'G'A'G`'Iy'G'U'` 'b'om'~'x 'e'YL'X-'XB'TR'QX'PE'PdO'Np'LD'N'Q'O/>'HѮ'ES'G'I'I'Gt'D'B0'?y'?me'?r'='=W'@:K'A'@'Cc'ID'Lr'HP'G3'I'Ftd'@ώ'=M='='C'E'E]'F;'E'FE'HW'I'I'F'C'G'Fp'=Pm'9'?L'<('67'3': '@'B*('A'Ci'BH':'5GC'6J';~'=y/':'4&'0u'-u'')'%'/')''L'$'!Y'.'e'''G'$mB'(Q'$?'#]')'*'-W@'=.'Jy'E >'1,',eV'5.'7!a'- '!R'P' k/' O'b'u' gd' ' *' ' ' 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