SIMPLE = T / Fits standard BITPIX = -32 / Bits per pixel NAXIS = 1 / Number of axes NAXIS1 = 3457 / Axis length EXTEND = F / File may contain extensions ORIGIN = 'NOAO-IRAF FITS Image Kernel July 2003' / FITS file originator DATE = '2005-03-09T19:14:47' / Date FITS file was generated IRAF-TLM= '19:14:47 (09/03/2005)' / Time of last modification NEXTEND = 3 / Number of standard extensions FILENAME= 'o56j01010_x2d.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= 'o56j01010 ' / rootname of the observation setPRIMESI = 'STIS ' / instrument designated as prime / TARGET INFORMATION TARGNAME= 'IRAS13224-3809 ' / proposer's target name RA_TARG = 2.013303333333E+02 / right ascension of the target (deg) (J2000) DEC_TARG= -3.841486111111E+01 / declination of the target (deg) (J2000) / PROPOSAL INFORMATION PROPOSID= 7360 / PEP proposal identifier LINENUM = '1.002 ' / proposal logsheet line number PR_INV_L= 'Leighly ' / last name of principal investigatorPR_INV_F= 'Karen ' / first name of principal investigator PR_INV_M= 'M. ' / middle name / initial of principal investigat / SUMMARY EXPOSURE INFORMATION TDATEOBS= '1999-06-05' / UT date of start of first exposure in file TTIMEOBS= '21:57:05' / UT start time of first exposure in file TEXPSTRT= 5.133491464395E+04 / start time (MJD) of 1st exposure in file TEXPEND = 51334.928012 / end time (MJD) of last exposure in the file TEXPTIME= 1155. / 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= 5.322690635417E+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 52X0.5 G230L NUVMAMA 2376' / 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= 'NUV-MAMA ' / detector in use: NUV-MAMA, FUV-MAMA, or CCD OPT_ELEM= 'G230L ' / optical element in use APERTURE= '52X0.5 ' / aperture name PROPAPER= '52X0.5 ' / proposed aperture name FILTER = 'Clear ' / filter in use APER_FOV= '52x0.5 ' / aperture field of view CENWAVE = 2376 / central wavelength of spectrum REPELLER= 'ON ' / repeller voltage: applies only to fuv-mama / MAMA OFFSETS MOFFSET1= 5 / axis 1 MAMA offset (low-res pixels) MOFFSET2= 14 / axis 2 MAMA offset (low-res pixels) / LOCAL RATE CHECK IMAGE LRC_XSTS= F / Local Rate check image exists (T/F) LRC_FAIL= F / Local Rate Check Failed (T/F) / READOUT DEFINITION PARAMETERS CENTERA1= 513 / subarray axis1 center pt in unbinned dect. pix CENTERA2= 513 / subarray axis2 center pt in unbinned dect. pix SIZAXIS1= 1024 / subarray axis1 size in unbinned detector pixelsSIZAXIS2= 1024 / subarray axis2 size in unbinned detector pixelsBINAXIS1= 1 / axis1 data bin size in unbinned detector pixelsBINAXIS2= 1 / axis2 data bin size in unbinned detector pixels / CALIBRATION SWITCHES: PERFORM, OMIT, COMPLETE DQICORR = 'COMPLETE' / data quality initialization RPTCORR = 'OMIT ' / add individual repeat observations DOPPCORR= 'OMIT ' / convolve ref. files with orbital Doppler shift LORSCORR= 'COMPLETE' / Convert MAMA data to Lo-Res before processing GLINCORR= 'COMPLETE' / correct for global detector non-linearities LFLGCORR= 'COMPLETE' / flag pixels for local and global nonlinearitiesDARKCORR= 'COMPLETE' / Subtract dark image FLATCORR= 'COMPLETE' / flat field data 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) SGEOCORR= 'OMIT ' / correct for small scale geometric distortions 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 SC2DCORR= 'OMIT ' / 2-D scattered light correction algorithm / CALIBRATION REFERENCE FILES BPIXTAB = 'oref$hcm14407o_bpx.fits' / bad pixel table DARKFILE= 'oref$lcl11073o_drk.fits' / dark image file name PFLTFILE= 'oref$mbj1658do_pfl.fits' / pixel to pixel flat field file name DFLTFILE= 'N/A ' / delta flat field file name LFLTFILE= 'oref$h5s1140ko_lfl.fits' / low order flat PHOTTAB = 'oref$m5f1245qo_pht.fits' / Photometric throughput table APERTAB = 'oref$n7p1032ao_apt.fits' / relative aperture throughput table MLINTAB = 'oref$j9r16559o_lin.fits' / MAMA linearity correction table SDSTFILE= 'N/A ' / small scale distortion image WAVECAL = 'o56j01010_wav.fits ' / wavecal image file name APDESTAB= 'oref$o2o1431lo_apd.fits' / aperture description table SPTRCTAB= 'oref$l3m14384o_1dt.fits' / spectrum trace table DISPTAB = 'oref$m7p16111o_dsp.fits' / dispersion coefficient table INANGTAB= 'oref$l3m1437ro_iac.fits' / incidence angle correction table LAMPTAB = 'oref$l421050oo_lmp.fits' / template calibration lamp spectra table SDCTAB = 'oref$l3m14383o_sdc.fits' / 2-D spatial distortion correction table XTRACTAB= 'oref$l3m1437to_1dx.fits' / parameters for 1-D spectral extraction tabPCTAB = 'oref$n2o1817do_pct.fits' / Photometry correction table MOFFTAB = 'oref$h4s1350ko_moc.fits' / MAMA offsets table WCPTAB = 'oref$lag1815lo_wcp.fits' / wavecal parameters table CDSTAB = 'oref$k8m0958bo_cds.fits' / Cross-Disperser Scattering table ECHSCTAB= 'oref$k8m0958co_ech.fits' / Echelle Scattering table EXSTAB = 'oref$k8m0958do_exs.fits' / Echelle Cross-Dispersion Scattering table RIPTAB = 'oref$k8m0958fo_rip.fits' / Echelle Ripple table HALOTAB = 'oref$k8m0958eo_hal.fits' / Detector Halo table TELTAB = 'oref$k8m0958ho_tel.fits' / Telescope Point Spread Function table SRWTAB = 'oref$k8m0958go_srw.fits' / Scattering Reference Wavelengths table TDSTAB = 'oref$o4817266o_tds.fits' / time-dependent sensitivity algorithm used TDCTAB = 'oref$m8m10302o_tdc.fits' / Coefficient table for NUV MAMA dark scalin / TARGET ACQUISITION DATASET IDENTIFIERS ACQNAME = 'o56j01QKT ' / 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 = 4 / number of points in primary pattern P1_PSPAC= 1.0 / 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) PATTERN = 'ALONG-SLIT ' / pattern type NUMPOS = 4 / number of positions in pattern STEPSIZE= 1.0 / size of step between positions in pattern PATTDRC = 'PLUS ' / pattern direction / ARCHIVE SEARCH KEYWORDS BANDWID = 1616.0 / bandwidth of the data SPECRES = 740.0 / approx. resolving power at central wavelength CENTRWV = 2376.0 / central wavelength of the data MINWAVE = 1568.0 / minimum wavelength in spectrum MAXWAVE = 3184.0 / maximum wavelength in spectrum PLATESC = 2.4400009E-02 / plate scale (arcsec/pixel) / PAPER PRODUCT SUPPORT KEYWORDS PROPTTL1= 'A Search for Broad Absorption Lines in Narrow-Line Seyfert 1 Galaxie'PROPTTL2= 's 'OBSET_ID= '01' / observation set id TARDESCR= 'GALAXY;SEYFERT '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 = 'O56J01010 ' / unique identifier assigned to association ASN_TAB = 'o56j01010_asn.fits ' / name of the association table EXPNAME = 'o56j01qmq ' / exposure identifier BUNIT = 'erg /s /cm**2 /angstrom /arcsec**2' / brightness units ASN_MTYP= 'SCIENCE ' / 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 = 1127.1600341797 / first axis value at reference pixel CTYPE1 = 'LINEAR ' / the coordinate type for the first axis CD1_1 = 0.58396872767696 / partial of first axis coordinate w.r.t. x LTM1_1 = 1.000000000000E+00 / reciprocal of sampling rate in X RA_APER = 2.013303333333E+02 / RA of aperture reference position DEC_APER= -3.841486111111E+01 / Declination of aperture reference position PA_APER = 4.066271287842E+01 / 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 = 8.043742318165E+00 / Spectrum shift in AXIS1 calculated from WAVECALSHIFTA2 = 0.000000000000E+00 / Spectrum shift in AXIS2 calculated from WAVECAL / EXPOSURE INFORMATION ORIENTAT= 41.046 / position angle of image y axis (deg. e of n) SUNANGLE= 132.952438 / angle between sun and V1 axis MOONANGL= 111.136665 / angle between moon and V1 axis SUN_ALT = 31.894060 / altitude of the sun above Earth's limb FGSLOCK = 'FINE ' / commanded FGS lock (FINE,COARSE,GYROS,UNKNOWN) DATE-OBS= '1999-06-05' / UT date of start of observation (yyyy-mm-dd) TIME-OBS= '21:57:05' / UT time of start of observation (hh:mm:ss) EXPSTART= 5.133491464395E+04 / exposure start time (Modified Julian Date) EXPEND = 5.133492801200E+04 / exposure end time (Modified Julian Date) EXPTIME = 1155.000000 / exposure duration (seconds)--calculated EXPFLAG = 'NORMAL ' / Exposure interruption indicator V_HELIO = 1.660223967097E+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 /1 / 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 = 3406069 / Slit Wheel Absolute position OMSCYL1P= 4698 / Mode select cylinder 1 position OMSCYL3P= 1148 / Mode select cylinder 3 position OMSCYL4P= 2258 / Mode select cylinder 4 position GLOBRATE= 1.772972294372E+03 / global count rate GLOBLIM = 'NOT-EXCEEDED' / was global linearity level exceeded? OM1CAT = 35.2749 / (dgC) M1 charge amplifier temp OM2CAT = 36.2517 / (dgC) M2 charge amplifier temp DOPPON = F / on-board doppler correction enabled DOPPZERO= 0.000000000000E+00 / Doppler shift zero phase time (MJD) DOPPMAG = 0 / Doppler shift magnitude (hi-res pixels) DOPPER = 0.0 / Doppler shift period (seconds) ORBITPER= 0.0 / Orbital Period used on board for Doppler corr. / IMAGE STATISTICS AND DATA QUALITY FLAGS NGOODPIX= 965293 / number of good pixels SDQFLAGS= 31743 / serious data quality flags GOODMIN = -2.0532131E-13 / minimum value of good pixels GOODMAX = 5.5036488E-13 / maximum value of good pixels GOODMEAN= 4.1887145E-16 / mean value of good pixels SNRMIN = -3.2048649E+01 / minimum signal to noise of good pixels SNRMAX = 2.3080059E+01 / maximum signal to noise of good pixels SNRMEAN = -6.4823848E-01 / mean value of signal to noise of good pixels SOFTERRS= 0 / number of soft error pixels (DQF=1) MEANDARK= 1.5170496E+00 / average of the dark values subtracted / PHOTOMETRY KEYWORDS SPORDER = 1 / Spectral order DIFF2PT = 1.5768731E-02 / Diffuse to point source conversion factor CONT2EML= 3.1721312E+01 / Intensity conversion: continuum -> emission SCALE_A1= 2.4400000E-02 / Size of one pixel (arcsec) along dispersion axiOMEGAPIX= 5.953600000000E-04 / Solid angle (arcsec**2) subtended by one pixel BANDID1 = 'spectrum: background none, weights none, clean no' APNUM1 = '1 1 616.10 624.10' WCSDIM = 1 CDELT1 = 0.58396872767696 WAT0_001= 'system=equispec' WAT1_001= 'wtype=linear label=Wavelength units=Angstroms' END $_}$k%&OyR%5&$JŤ L&bm"զt¥*R$S%#%~&3&M%JG#ܣ'l&g&a&i&%&C'='&wC&' 4'P '5D''9S'F'`'Z'omU'bp'd$'g4k'p\i''{'}I'p'N''{'v''v'y"'h'M%'V2'Y'Lo9'_'l{;'f9'I('1g'H']"K'Zx'q'j'h|'GM'E<'iyH'h"'f'g'k'u'jH'r's'xT'3E'~'oF'zV'{u&'t']'Y'b'2,'P'A'K2'X'yq'1'j''p' ''<''''y~z'l/'gn'p'v*U'pu''F'2'u'm'7'"'''vu '}[3'}'{ۄ'vz'''q)'d'j~'m!']q'% ''' F''ΰ'0}&&y&]&%Nc%G%\9O%(b%@%x %I&"'&s&U&`&v''&c'b'.'>/'I2'O'W'IM'D'\;'a'`w'lCX'Zr7'ح'{Sa'}zQ'E'''lb'nc''u&'|0''m'!'v'uS'}'"''+'c&'/l''w'C'g'''F'a''!''*' 3'M'''''Q's' 'AZ'1'('' ''|'xS'lW'Qa'N'sZ'̔'E1'$' ''6''^''1'QW'Su'T''''A'Ie'kl''o'''!G'`''m'r''h'' i'ͬ'9%'S'w,'؞'̍7'Ŧ'̵'A'E' '2'%{'='w'''''o'.1( (($(-a#(0%(3^#(/G(( |1(!%'ի''܊q'Ѫx''''' 'F2''l'W''{'k'y_'<'j('Q',I''(1' 'G''/l'''di'F')'~''c'jx'5''!S'"'#''\''%W' ''('n''&'K'~' 'd'e?'d''N' ''g(''hk''W'''T8'E'tz'&'''ur'!'o'/'''֣''V''A7'/'A'AZ'ʌ'B'J'n'#'''(''}0;'/'Ÿ'~'u*''<''9'('C'b''w'j'C''#;'n'''p';P'>?''j:k'^m'e@'\'fr's'yg'<''''|9'd''b'|7'''&'''-'Z'z%'~'N''=:'z''l'''Ť'X'39''g6_'Lr'T'Xl'mD'tW'^ʮ'^'ẅ'z '>''n.''q']'ce'j)-''l)'lFd'q'do+'o$';'~'q'''^'a'j'}'D6''į'('xD'0y'-n'Tx'{V'zSP' '|L'{S ''K''k''/'8'T''''wt''t !'U'X'v''\'zű'ol.'p/''i''''b'Z'' 'F'uf'v'7'Z'3'': '"'7'aC'?Q'W[']'y'm' 'Z''yN '': 'x'}ڒ''K''?'] 'wJ'?''Q'l'k'i'kN.'t9}'''J''M'ǐ't'te'T8'۪'|''xo'A'Z'5''m'~F'(4'''hE'0'3'VP''WH''X'N'~'J4'xl''('C'x5''t7''ÿ'Ӷ'H+''Lj'3' $'΁''k''~''$'t''''''9'lv'R'X#'''W:'''`'eh'i'Z'*~''E'''3''x'%''M/'޼'D''_''ݯ'|A'j'zA'S'j'M'6D'B'n'pj'c#'-'''}'Oy'z'{ߊ''5''Z5'''{''8'<''D''O'_|'q0'R''0'''5!'{i'ж'@'2'' 9'u>';'a'[N'qn'Mt'@'L'M'u'BN''m'E7'U' l'\''n''Q'''''2J'u''U'G'_'''W'M''l'''}0'$'ug''''l''C ''Թ'2]'''Ɲ'J''%_''Y'at''DR'З''w0''oS'y''q'p'3'4f'{'w'Q's''''O'H''' ''0''3''' '+Y'''@'&@'z'K''5'M'~''q''~Ύ' ''f'm'''+'-6' 8''##'z '''-']'C'~'~j'|'|I'9'7'K''1''''<'~*)'v#'r'v'}C''n'k3''~Y''8'u'Yl' '''{ <'xE'x?'y'z='{K9'{'z'x't's9'wNh'}'~'xR'qY'pU'wc'|'xgF'o f'ff'd'h#A'r'~'^'Z''D'''''K&'UU'v''4'o'a''}'y'vgs'tr't)'u*W'w 'yd'{'}''''cE''a'?'i$'v''''b('k'E''6'j'',''4'D'-'6/'h2'4'c''6~'<'z'i'B'~'i''o''1'''X'@'(c'}`'w'wq'z '}k'R''''J''~@'y'vs'v'}9'?'*G'u'zǔ'u's#'sJ't/'v ;'xf'z '{b'{it'z'{'(h']''''P'}'xhs'v'v'x'}6'''H''E'}H'xg'tʗ'qX'nC'l'n'u*/'{6'|'z.'vS't?'s('r=F'q2'po'r't'u~;'sR'oq'k`{'h 'e&'a۞'`f'cy4'm 3'w'~Ũ'u'}'y'w'q]'r'X's't't9s'q'n'l'lE'o{'t''y'|'{7'xX't 'p'o*'s7I'yEE'~'U'~ʊ'|l'y'u)'q'o*i'nc'p#'sPH'vM'x'x'w'u('t:'tƣ's'nY'hi'd;i'b/'dx'iIY'or'r-W'n'h7 'aG'^']+'^)'a'd'e8'e$'d'cO'cl'd['hA'l['n'o!'n'lq'ki7'n't`'yK'z'y '| ''C'_ '_Z'WD'('3'f'T+'1'+''n'o'''Չ'"~'x'E'tF',')''''~' p'q]'gj'|-'yL'v1'wV'~x'''Ng'A' 'pq'D'.' n''Y'f'â'B'8 ' '"'{0V'v'ra'o'mo'lpa'l?'l'nIC'o2'o'm-'hx 'c'`8'^?']M'^s'_('^']G'\('\g'\q'^em'a:'c T'bd@'_@4'ZM'TZ\'O45'L'MH'N'N,'Mq'KES'G]G'D'E)'Iw'M'NNb'M'K8'I'I7'Itb'J'Lv''N 'PkL'Oܛ'L'HT'FO 'E'G['J<'L'Nl3'Nv'L:'I~'I'OSB'V3'[u'['X'Rղ'L0V'HLP'I'MH'OO'O>'NG'M'L2'J'GY'D5'D'F'I8'K2'Lsz'Jr'E'Al'A'E'I'Io'F'A-';d+'6d'5+'8D';!G';F': '9D'9':';p@';2':'7='4^'4*'8'=W'?I'>K';ݗ'9#F'7s1'8'<4'?K'?$'='='A'F'I'IF'Hb'G%'E'E?#'E7O'F'G'JoS'L'M7'Lƅ'K'J'J 'J['L]'Lv'J'G\'DH'C'C'A'?'>@E'>F'?N'@'Bb'B('@'s'<'8'8x':N';'<y';"'8EU'4t'3'6P'9':'7?'4'5'7 ':dA':['9y'9a':';ߋ'*'@A'B*.'Bw'Az8'@S'@R'A1^'A'@v'?'?+'A/'BP'B['@'?ͮ'A&'C5'D@'Cv'A'@m'?['>6'?t'?C'<'7V'2: '/'/ߧ'1'5 D'7'7'53Y'3ٯ'7p'<'AD'A~'@m'@A'A'@Q';'64'2c'2'5Li'8'<&@'=̆''"'!'$_'). 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