SIMPLE = T / Fits standard BITPIX = -32 / Bits per pixel NAXIS = 1 / Number of axes NAXIS1 = 1502 / Axis length EXTEND = F / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator DATE = '2005-02-17T14:36:07' / Date FITS file was generated IRAF-TLM= '14:36:07 (17/02/2005)' / Time of last modification NEXTEND = 3 / Number of standard extensions FILENAME= 'o6m5030b0_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= 'o6m5030b0 ' / rootname of the observation setPRIMESI = 'STIS ' / instrument designated as prime / TARGET INFORMATION TARGNAME= '3C382.0 ' / proposer's target name RA_TARG = 2.787643333333E+02 / right ascension of the target (deg) (J2000) DEC_TARG= 3.269613888889E+01 / declination of the target (deg) (J2000) / PROPOSAL INFORMATION PROPOSID= 9495 / PEP proposal identifier LINENUM = '03.037 ' / 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= '2003-07-23' / UT date of start of first exposure in file TTIMEOBS= '15:29:02' / UT start time of first exposure in file TEXPSTRT= 5.284364516493E+04 / start time (MJD) of 1st exposure in file TEXPEND = 5.284365275743E+04 / end time (MJD) of last exposure in the file TEXPTIME= 6.3000000E+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 15.3a ' / OPUS software system version number CAL_VER = '2.15c (29-January-2004)' / CALSTIS code version PROCTIME= 5.322690118056E+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 CTECORR = 'PERFORM ' / correction for CCD charge transfer inefficiencyX2DCORR = 'COMPLETE' / rectify 2-D spectral image / CALIBRATION REFERENCE FILES BPIXTAB = 'oref$h1v11475o_bpx.fits' / bad pixel table DARKFILE= 'oref$n841149to_drk.fits' / dark image file name PFLTFILE= 'oref$n491401ho_pfl.fits' / pixel to pixel flat field file name DFLTFILE= 'N/A ' / delta flat field file name LFLTFILE= ' ' / low order flat PHOTTAB = 'oref$ncc1900lo_pht.fits' / Photometric throughput table APERTAB = 'oref$n7p1032ao_apt.fits' / relative aperture throughput table CCDTAB = 'oref$n951041ko_ccd.fits' / CCD calibration parameters ATODTAB = 'N/A ' / analog to digital correction file BIASFILE= 'oref$n841149qo_bia.fits' / bias image file name SHADFILE= 'N/A ' / shutter shading correction file CRREJTAB= 'oref$j3m1403io_crr.fits' / cosmic ray rejection parameters WAVECAL = 'o6m5030b0_wav.fits ' / wavecal image file name APDESTAB= 'oref$o2o1431lo_apd.fits' / aperture description table SPTRCTAB= 'oref$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$n841149qo_bia.fits' / associated wavecal bias image file name WCPTAB = 'oref$lag1815lo_wcp.fits' / wavecal parameters table TDSTAB = 'oref$o4817264o_tds.fits' / time-dependent sensitivity algorithm used / COSMIC RAY REJECTION ALGORITHM PARAMETERS MEANEXP = 3.1500000E+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= 2.4996826E+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 = 4.8000002E+00 / calibrated CCD read noise value / TARGET ACQUISITION DATASET IDENTIFIERS ACQNAME = 'o6m503RAT ' / rootname of acquisition exposure ACQTYPE = ' ' / type of acquisition PEAKNAM1= 'o6m503RBT ' / 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= 0.228 / 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= 'Do the Most Powerful Radio Galaxies Host the Most Massive Black Hole'PROPTTL2= 's ? 'OBSET_ID= '03' / 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 = 'O6M5030B0 ' / unique identifier assigned to association ASN_TAB = 'o6m5030b0_asn.fits ' / name of the association table SKYSUM = 0.0000000E+00 / Total sky level (DN) EXPNAME = 'o6m503t7q ' / 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 = 2898.1669921875 / first axis value at reference pixel CTYPE1 = 'LINEAR ' / the coordinate type for the first axis CD1_1 = 4.8820831685127 / partial of first axis coordinate w.r.t. x LTM1_1 = 1. / reciprocal of sampling rate in X RA_APER = 2.787643333333E+02 / RA of aperture reference position DEC_APER= 3.269613888889E+01 / Declination of aperture reference position PA_APER = 1.083595290894E+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 = 2.973401756997E+00 / Spectrum shift in AXIS1 calculated from WAVECALSHIFTA2 = -1.661462919885E+00 / Spectrum shift in AXIS2 calculated from WAVECAL / EXPOSURE INFORMATION ORIENTAT= 108.765 / position angle of image y axis (deg. e of n) SUNANGLE= 122.482002 / angle between sun and V1 axis MOONANGL= 112.510208 / angle between moon and V1 axis SUN_ALT = 58.722775 / altitude of the sun above Earth's limb FGSLOCK = 'FINE ' / commanded FGS lock (FINE,COARSE,GYROS,UNKNOWN) DATE-OBS= '2003-07-23' / UT date of start of observation (yyyy-mm-dd) TIME-OBS= '15:29:02' / UT time of start of observation (hh:mm:ss) EXPSTART= 5.284364516493E+04 / exposure start time (Modified Julian Date) EXPEND = 5.284365275743E+04 / exposure end time (Modified Julian Date) EXPTIME = 6.3000000E+02 / exposure duration (seconds)--calculated EXPFLAG = 'NORMAL ' / Exposure interruption indicator V_HELIO = 4.952594108541E+00 / 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 /2 /2 / number of image sets combined during CR r / 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 = 880480 / 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 = 26.6827 / (V) CEB A&B Amp Bias OCBCDAV = 26.7221 / (V) CEB C&D amp bias OCBLGCDV= -3.38383 / (V) CEB last gate C&D OCBSWALV= -6.00587 / (V) CB summing well A Lo OCBRCDLV= 0.0438864 / (V) CB reset gate CD Lo OCCDHTAV= 19.447100 / average CCD housing temperature (degC) / IMAGE STATISTICS AND DATA QUALITY FLAGS NGOODPIX= 121174 / number of good pixels SDQFLAGS= 31743 / serious data quality flags GOODMIN = -7.4632812E-14 / minimum value of good pixels GOODMAX = 6.9881519E-13 / maximum value of good pixels GOODMEAN= 1.1221265E-15 / mean value of good pixels SNRMIN = -6.4135246E+00 / minimum signal to noise of good pixels SNRMAX = 1.9745895E+02 / maximum signal to noise of good pixels SNRMEAN = 1.2302160E+00 / mean value of signal to noise of good pixels SOFTERRS= 0 / number of soft error pixels (DQF=1) MEANDARK= 1.6849106E+01 / average of the dark values subtracted MEANBLEV= 1.1657677E+03 / average of all bias levels subtracted / PHOTOMETRY KEYWORDS SPORDER = 1 / Spectral order DIFF2PT = 2.4662750E-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 1 299.70 301.70' WCSDIM = 1 CDELT1 = 4.8820831685127 WAT0_001= 'system=equispec' WAT1_001= 'wtype=linear label=Wavelength units=Angstroms' END (W@(l((((n('(3(I(m9(-)(h((H(((( ((p(*:(Z(:(((((}I(v(t(p!(h (f3(g^(a,(^d(_h(`I(^+(_H(]((\(]"(Y2t(X&(Y<(X3(V(W(Wtb(T~(Qn6(T(W(RK(Svz(I*Y(E5(M](OG(O2X(Q`(N-h(P(L`(I(O_(QD(P(M(Jy(Lۺ(J(L(M0(K(N(N (L"(Od"(R(Q(P%(Nn(T\(Ur(X/([o(W(WL([5v(U(UP(V'(S3b(O(NG(P(R(R(S1(P(Pr(M(LV(NLN(M9(MY(Kq(Kq(LB(Gq(EW(G(Gq(F!(C(C (Fk(FU(Bz(=m (<(>(?(A(D}(BH(A(A(DuV(Eː(C(B(Cb(A(?p(>(? (=(<(=O(<(;(= (}(>9(;`(9e(: (<[,(:Z(7B (8 8(6&(4(5;?(6(5(2W(1(1Fi(4x(5:(3u(3|(2(2"T(4?(3~(3AB(2C(2a(2U(1(0 (/(-J(.<7(. k(+(-{(-()/()F(,%(*m(*x(*]()(((&(%b(&aS(&y<($3(#O(#(#(!w( ˵( N(\(B((L(v(f((u?(m(X((L((( (O(N((( ( ( (\(Y(B(~(#(i(F((Y(( I ( ( (6Y((Q((r(3(['`b'^'t' '8'0'M6'ZV'r''S'Fk'')''Z'<'i'F' '〇'm'va'5r' ''$D'_' '/'ڠ'݊'ݰ'd'ڼ''۬y'װ'''ىk' G'܇'ږx'@''F'w'y''<'ϓy'є'-'^'țs'G'Ȑ'į'FG'-':'x'''D'=A'D''''G'p'§'6Q'ë;''ĞI'x'o'(X'BC'7u'o,'X['*A'δ'''Ϻ 'ш'?'o''ٖq':'''ھ~'o'1'2'҇ ''Z'<1'':'R'x'C''y';''4J''j'7?'''''j]''sM'fM''&'<''m''w'K'Z.'M''_'b'.'A'KB''+' g'3'['Bq''X'''\'''|''nm''o''_''e'V'9'h''E')j''~'/('u'D'''~'o''_;'O''4'T''*''f'ɳ'VZ'q'ɟ?'i''̰''o''j'֜'ݺJ'f''I'rS''''.'㕇'ܤn'':'`G'.''''$''7'ÚI''E''{='''ޯ'E'' ''`'ɗ''E3'2'#'Q'Gd'`E''')'''P'\'j'=>''.'''j'Z' ''P' n'['l9''''r'Q'''2''2m'^''@'O#','' 'l'A'>'}t'i'G'|'z'{'~'}$q'|''~h' .'Ni'~'~}'+G'~'}v)'}'z3'x&'w4'{'z'x}3'wՑ'u4'rp'q's 'sm'~)'=' 9'x['6'}%'{~'~e'~lk'3'~/'}'|,@'z('z'zc'v'w'x 'v@'t 'uZ.'w'v'uX'v,'vd'su'rd3'p'o'o'o5'ok 'p+ 'rj'p'lv'l'n'mX'i'et{'ar'c'g_O'g{,'gm'ge'fh 'e='g 'f%'fE'g'g'fpR'eg'fN 'f;'ag'`w'a'b'c'c4'c7'bE'b7'a'aC'd_|'e''fO8'g'jb'kG'jb'l'n^'m\'k'lx'jJ'j'jz'kZ'nD'kw'j'kr'he'i'm'k'l7W'm6='m 'm'k:'k'o2'nk'l'l'l'm'q'sG'r!v'q'p'o 'p 'qf'q7'q'p'l'i'j$'k2.'iC'h'ij'k('iR'f'e*'d6'dD'aUL'^'_Dj'\'Y@'Y'd"s'c'\r'Y 'X'Zz'Y 'Uw'U<'VR`'Uc'P'L'KNP'Pj'T'T'Tq'Q'O'P'QQ'M'L{+'Lj'LY'KZ'I'H'F('JN8'K|'Hձ'I'Glc'G'I`'Gq\'EDŽ'G{'H1'F'H&'H'Gu'GI'I''KՎ'J'G'Hr'I3'GȒ'F'F='J 'K'J'Hơ'I7'LV'Li'M'Qɱ'U'WL'T"&'Q̧'O'P"'S'TO'XL'\ '_'eq'g'm've'}'='`2'%p''eT'c'm' 5'R'n''I''''Ͱ'Ѧ'֋'܀''p'P'o'i'E/'' 'Y2''a'Ka'(_+(x(B(;C(ܴ((@("y(%~s((k(*(,}a(.i(-$(,Ro('M(%(/( A(y(A('(n( j(k@(o(L'Z'D'''ӽF'd''\']'N'a''7''' 'Բ'q''$ '%'}!'p'h%'a'XP'SJ'O@'L'JW'GS'C'?`'=^3'8'5='4J'4wM'4\'2'/'.K1'/d'.'+0'-'-l',('-'',Q''['$u'%H''ԣ'''&'&7'&'%,'$g'#|^'#'!aZ' (' Q'"'$1'!2'g'Q'='*''"'''L' Y' !'''K*'E'c''dm'!' Y1'''L''1'ܕ''A@'(' z' ''V'[''.'' s'''X'''')5''@'M'G''za''' &' 3'IX'z'ZO''A''1-' ' ' ' ' ' /':'t''' 'k' K''+'E$' D';W'wB'' H'A'P' ''V?' w' K' ^' -' ' u'^&&3&JA'vq'b''f' <' <' B4''́'.j'+&'&{&+E&-&&N'U'e'''L'N ''#'&An&k&?&f&<&''''vA&&&cD&e&m&&2''ݠ&1&Yj&&|&,&O&-&]&& &3&C &N&y&x& &a&&\n&۬=& "&&&⾐&&> & &n&v&I&۴a&/&ٳ &ą&%&&&鉞&dE&&g&k&b&d&d& & &8&̛R&l&&̦&x&ܶ&ހ&A&ߟ&& <&ް&֐q&j&~&ǡ&ȃ~&>&P&|&7&U& V& &&佋&&&ћ&`&Ϲ-&J&ƾ&&&4&FM&r&$&T&t&r&+&&)&&—&9&c0&+c&{&Ȣ&ͽ&>&:&^&ӯ&1@&Ƭ&&u$&fz&ƿ&+&E&:m& &̝&&/&P&\&;& (&&x &/l&n&ē&ԁe&ܚ(&&&&&T&[&c&;5&j&&%&Â+&]O&ε&͈l& U&̼&bG&Q&0&<&X&t&&/&+&A&c&D&(&ͬu&Ȇ&E&ȓ}&&%~&̤&Ͳ&ν&&&L&k&c&/(&A&M1&vB&l&¢H&N!&ű &&&_R&-&JD&&&&)&& &3K&F&Ȁ&&;F&ԇ&+&&Y&&~&]&&&H&ţ& R& &&)'&?&mH& &]G&&L&&fA&&e=&#&8^&&#&&&n&=&9&.&U&&l&T&9&&.&ke&&&fu&1&!&&|&&d&&&o&&8c&<&r&vx@&s &m0&p&y&I&F&&&c && &S&M&H&yE&p3&hA&n&oB&n&s&&*L&9&?&v&s&h&K&&Z&&x{h&l&fA&ddC&j&&&Ĵ&&{&&c&t&}I&l]&^&bh&q&s&{&&&.&&v&&ٻ&sf&f&]k&U &\>&]:_&\&cL&cv&^n&e0&n~&t}&y&a&9&&'A&&&&og &\&S&Pɢ&Ma&W:&`=&g\&w&O&ۣ&&&*&r"&p&`&Um &R/[&ON4&L:&>ty&=&:߼&5&KQE&Vb&M&V&c&fx&pS&x&ysx&z6&& &&&w&x˪&u: &_BD&PT&H\&>*&7͛&6&9"&4`8&4h&=&EQP&A&?2[&Pš&iM&q9&r\&J<&>&yQ\&vŘ&z&r&]m&@&6V&>&;X&0_&3&/&)[&'#q&+&'9&&M(&.g&=y&?*V&D@&Mz&R1&Yv#&`k%&Y5U