--- header unit 0: primary ---
SIMPLE = F / FIT STANDARD
BITPIX = 8 / FITS BITS/PIXEL
NAXIS = 0 / No axes
EXTEND = T / Fits extensions are used
SDSS / THIS HEADER CONTAINS SPECIAL SDSS KEYWORDS
UNSIGNED / UNSIGNED DATA - NO BSCALE OR BZERO KEYWORDS
TAI = 4588546499.17 / 1st row - Number of seconds since Nov 17 1858
RA = 125.44831 / 1st row - Right ascension of telescope boresigh
DEC = 19.536609 / 1st row - Declination of telescope boresight (d
SPA = 60.365 / 1st row - Camera col position angle wrt north (
IPA = 0.938 / 1st row - Instrument rotator position angle (de
IPARATE = -0.0016 / 1st row - Instrument rotator angular velocity (
AZ = 285.06141 / 1st row - Azimuth (encoder) of tele (0=N?) (de
ALT = 56.917493 / 1st row - Altitude (encoder) of tele (de
FOCUS = 69.600000 / 1st row - Focus piston (microns?)
DATE-OBS = '2004-04-13' / 1st row - TAI date
TAIHMS = '04:14:59.17' / 1st row - TAI time (HH:MM:SS.SS) (TAI-UT = appr
COMMENT TAI,RA,DEC,SPA,IPA,IPARATE,AZ,ALT,FOCUS at reading of col 0, row 0
BUNITS = 'ADUs'
ORIGIN = 'SDSS'
TELESCOP = '2.5m'
TIMESYS = 'TAI'
RUN = 4549 / Run number
FRAME = 88 / Frame sequence number within the run
STRIPE = 24 / Stripe index number (23 <--> eta=0)
STRIP = 'N' / Strip in the stripe being tracked.
FLAVOR = 'science' / Flavor of this run
OBSERVER = 'jcb' / Observer
SYS_SCN = 'mean' / System of the scan great circle (e.g., mean)
EQNX_SCN = 2000.00 / Equinox of the scan great circle. (years)
NODE = 95.00000 / RA of the great circle's ascending node (deg)
INCL = 35.00000 / Great circle's inclination wrt cel. eq. (deg)
XBORE = -22.74 / Boresight x offset from the array center (mm)
YBORE = 0.00 / Boresight x offset from the array center (mm)
OBJECT = '24 N' / e.g., 'stripe 50.6 degrees, north strip'
EXPTIME = '10.5288' / Exposure time (seconds)
EQUINOX = '2000.0' / Equinox of the TCC coordinates (years)
SYSTEM = 'FK5' / System of the TCC coordinates (e.g., mean)
CCDMODE = 'DRIFT' / 'STARING' or 'DRIFT'
C_OBS = 26322 / CCD row clock rate (usec/row)
COLBIN = 1 / Binning factor perpendicular to the columns
ROWBIN = 1 / Binning factor perpendicular to the rows
NLINES = 400 / Number of lines in a frame
DAVERS = 'v14_47' / Version of DA software
SCDMETHD = 'sqrtDynamic' / scdMethod
SCDWIDTH = 1280 / scdDisplayWidth
SCDDECMF = 1 / scdDecimateFactor
SCDOFSET = 40 / scdDisplayOffset
SCDDYNTH = -20 / scdDynamicThresh
SCDSTTHL = 30 / scdStaticThreshL
SCDSTTHR = 30 / scdStaticThreshR
SCDREDSZ = 512 / scdReduceSize
SCDSKYL = 0 / scdSkyLeft
SCDSKYR = 0 / scdSkyRight
COMMENT CCD-specific parameters
CCDSECL = '[21:1064,1:1361]' / Physical ccd section for low pixels
OVERSECL = '[1:20,1:1361]' / Image section for overscan for low pix
BIASSECL = '[21:40,1:1361]' / Image section for prescan for low pix
DATASECL = '[41:1064,1:1361]' / Image section for data for low pixels
CCDSECR = '[1065:2108,1:1361]' / Physical ccd section for high pixels
DATASECR = '[1065:2088,1:1361]' / Image section for data for high pixels
BIASSECL = '[2089:2108,1:1361]' / Image section for prescan for high pixels
OVERSECR = '[2109:2128,1:1361]' / Image section for overscan for high pixels
--- header unit 1: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 81'
CAMCOL = 1 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 51 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 1 / True means use 5x5 for star finding
STARDIST = 20 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 533 / Star threshold - lo column numbers
STHRESHR = 533 / Star threshold - hi column numbers
SABSKYL = 15 / Value to add to sky level = threshold - lo colu
SABSKYR = 15 / Value to add to sky level = threshold - hi colu
SSATL = 65035 / Star saturation - lo column numbers
SSATR = 65035 / Star saturation - hi column numbers
SLOCOLL = 15 / Number of lo cols to skip for lo column numbers
SLOCOLR = 0 / Number of lo cols to skip for hi column numbers
SHICOLL = 0 / Number of hi cols to skip for lo column numbers
SHICOLR = 15 / Number of hi cols to skip for hi column numbers
TSHIFT = 64 / Bias scaling factor
FRBIASL = 32940 / Left Frame bias x TSHIFT
FRBIASR = 32945 / Right Frame bias x TSHIFT
FRSKYL = 33206 / Left Mean Sky Value x TSHIFT
FRSKYR = 33192 / Right Mean Sky Value x TSHIFT
FROSCNL = 32939 / Left Mean Oscn Value x TSHIFT
FROSCNR = 32943 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 142966 / 10*Average time per row (usec)
TIMEFRAM = 83557 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '841U' / PostStamp ushorts
TTYPE1 = 'PIXELMAP' / Postage Stamp subimage
TUNIT1 = 'ADUs'
TFORM2 = '1I'
TTYPE2 = 'MIDROW' / Frame row (data section) of middle pixel
TFORM3 = '1I'
TTYPE3 = 'MIDCOL' / Frame column (data section) of middle pixel
--- header unit 2: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 82'
CAMCOL = 2 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 53 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 1 / True means use 5x5 for star finding
STARDIST = 20 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 786 / Star threshold - lo column numbers
STHRESHR = 786 / Star threshold - hi column numbers
SABSKYL = 15 / Value to add to sky level = threshold - lo colu
SABSKYR = 15 / Value to add to sky level = threshold - hi colu
SSATL = 65035 / Star saturation - lo column numbers
SSATR = 65035 / Star saturation - hi column numbers
SLOCOLL = 15 / Number of lo cols to skip for lo column numbers
SLOCOLR = 0 / Number of lo cols to skip for hi column numbers
SHICOLL = 0 / Number of hi cols to skip for lo column numbers
SHICOLR = 15 / Number of hi cols to skip for hi column numbers
TSHIFT = 64 / Bias scaling factor
FRBIASL = 49494 / Left Frame bias x TSHIFT
FRBIASR = 49086 / Right Frame bias x TSHIFT
FRSKYL = 49377 / Left Mean Sky Value x TSHIFT
FRSKYR = 49381 / Right Mean Sky Value x TSHIFT
FROSCNL = 49068 / Left Mean Oscn Value x TSHIFT
FROSCNR = 49075 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 142966 / 10*Average time per row (usec)
TIMEFRAM = 83557 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -2 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '841U' / PostStamp ushorts
TTYPE1 = 'PIXELMAP' / Postage Stamp subimage
TUNIT1 = 'ADUs'
TFORM2 = '1I'
TTYPE2 = 'MIDROW' / Frame row (data section) of middle pixel
TFORM3 = '1I'
TTYPE3 = 'MIDCOL' / Frame column (data section) of middle pixel
--- header unit 3: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 83'
CAMCOL = 3 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 44 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 1 / True means use 5x5 for star finding
STARDIST = 20 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 501 / Star threshold - lo column numbers
STHRESHR = 501 / Star threshold - hi column numbers
SABSKYL = 15 / Value to add to sky level = threshold - lo colu
SABSKYR = 15 / Value to add to sky level = threshold - hi colu
SSATL = 65035 / Star saturation - lo column numbers
SSATR = 65035 / Star saturation - hi column numbers
SLOCOLL = 15 / Number of lo cols to skip for lo column numbers
SLOCOLR = 0 / Number of lo cols to skip for hi column numbers
SHICOLL = 0 / Number of hi cols to skip for lo column numbers
SHICOLR = 15 / Number of hi cols to skip for hi column numbers
TSHIFT = 64 / Bias scaling factor
FRBIASL = 31027 / Left Frame bias x TSHIFT
FRBIASR = 30865 / Right Frame bias x TSHIFT
FRSKYL = 31129 / Left Mean Sky Value x TSHIFT
FRSKYR = 31147 / Right Mean Sky Value x TSHIFT
FROSCNL = 30855 / Left Mean Oscn Value x TSHIFT
FROSCNR = 30857 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 142966 / 10*Average time per row (usec)
TIMEFRAM = 83557 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -1 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '841U' / PostStamp ushorts
TTYPE1 = 'PIXELMAP' / Postage Stamp subimage
TUNIT1 = 'ADUs'
TFORM2 = '1I'
TTYPE2 = 'MIDROW' / Frame row (data section) of middle pixel
TFORM3 = '1I'
TTYPE3 = 'MIDCOL' / Frame column (data section) of middle pixel
--- header unit 4: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 84'
CAMCOL = 4 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 45 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 1 / True means use 5x5 for star finding
STARDIST = 20 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1164 / Star threshold - lo column numbers
STHRESHR = 1164 / Star threshold - hi column numbers
SABSKYL = 15 / Value to add to sky level = threshold - lo colu
SABSKYR = 15 / Value to add to sky level = threshold - hi colu
SSATL = 65035 / Star saturation - lo column numbers
SSATR = 65035 / Star saturation - hi column numbers
SLOCOLL = 15 / Number of lo cols to skip for lo column numbers
SLOCOLR = 0 / Number of lo cols to skip for hi column numbers
SHICOLL = 0 / Number of hi cols to skip for lo column numbers
SHICOLR = 15 / Number of hi cols to skip for hi column numbers
TSHIFT = 64 / Bias scaling factor
FRBIASL = 73264 / Left Frame bias x TSHIFT
FRBIASR = 73226 / Right Frame bias x TSHIFT
FRSKYL = 73581 / Left Mean Sky Value x TSHIFT
FRSKYR = 73607 / Right Mean Sky Value x TSHIFT
FROSCNL = 73238 / Left Mean Oscn Value x TSHIFT
FROSCNR = 73248 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 142966 / 10*Average time per row (usec)
TIMEFRAM = 83557 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -1 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '841U' / PostStamp ushorts
TTYPE1 = 'PIXELMAP' / Postage Stamp subimage
TUNIT1 = 'ADUs'
TFORM2 = '1I'
TTYPE2 = 'MIDROW' / Frame row (data section) of middle pixel
TFORM3 = '1I'
TTYPE3 = 'MIDCOL' / Frame column (data section) of middle pixel
--- header unit 5: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 85'
CAMCOL = 5 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 55 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 1 / True means use 5x5 for star finding
STARDIST = 20 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1283 / Star threshold - lo column numbers
STHRESHR = 1283 / Star threshold - hi column numbers
SABSKYL = 15 / Value to add to sky level = threshold - lo colu
SABSKYR = 15 / Value to add to sky level = threshold - hi colu
SSATL = 65035 / Star saturation - lo column numbers
SSATR = 65035 / Star saturation - hi column numbers
SLOCOLL = 15 / Number of lo cols to skip for lo column numbers
SLOCOLR = 0 / Number of lo cols to skip for hi column numbers
SHICOLL = 0 / Number of hi cols to skip for lo column numbers
SHICOLR = 15 / Number of hi cols to skip for hi column numbers
TSHIFT = 64 / Bias scaling factor
FRBIASL = 81011 / Left Frame bias x TSHIFT
FRBIASR = 80964 / Right Frame bias x TSHIFT
FRSKYL = 81192 / Left Mean Sky Value x TSHIFT
FRSKYR = 81180 / Right Mean Sky Value x TSHIFT
FROSCNL = 81003 / Left Mean Oscn Value x TSHIFT
FROSCNR = 81014 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 142966 / 10*Average time per row (usec)
TIMEFRAM = 83557 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -1 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '841U' / PostStamp ushorts
TTYPE1 = 'PIXELMAP' / Postage Stamp subimage
TUNIT1 = 'ADUs'
TFORM2 = '1I'
TTYPE2 = 'MIDROW' / Frame row (data section) of middle pixel
TFORM3 = '1I'
TTYPE3 = 'MIDCOL' / Frame column (data section) of middle pixel
--- header unit 6: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 86'
CAMCOL = 6 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 56 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 1 / True means use 5x5 for star finding
STARDIST = 20 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 733 / Star threshold - lo column numbers
STHRESHR = 733 / Star threshold - hi column numbers
SABSKYL = 15 / Value to add to sky level = threshold - lo colu
SABSKYR = 15 / Value to add to sky level = threshold - hi colu
SSATL = 65035 / Star saturation - lo column numbers
SSATR = 65035 / Star saturation - hi column numbers
SLOCOLL = 15 / Number of lo cols to skip for lo column numbers
SLOCOLR = 0 / Number of lo cols to skip for hi column numbers
SHICOLL = 0 / Number of hi cols to skip for lo column numbers
SHICOLR = 15 / Number of hi cols to skip for hi column numbers
TSHIFT = 64 / Bias scaling factor
FRBIASL = 46058 / Left Frame bias x TSHIFT
FRBIASR = 45733 / Right Frame bias x TSHIFT
FRSKYL = 45962 / Left Mean Sky Value x TSHIFT
FRSKYR = 45968 / Right Mean Sky Value x TSHIFT
FROSCNL = 45721 / Left Mean Oscn Value x TSHIFT
FROSCNR = 45722 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 142966 / 10*Average time per row (usec)
TIMEFRAM = 83557 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -1 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '841U' / PostStamp ushorts
TTYPE1 = 'PIXELMAP' / Postage Stamp subimage
TUNIT1 = 'ADUs'
TFORM2 = '1I'
TTYPE2 = 'MIDROW' / Frame row (data section) of middle pixel
TFORM3 = '1I'
TTYPE3 = 'MIDCOL' / Frame column (data section) of middle pixel
--- header unit 7: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 81'
CAMCOL = 1 / Column in imaging camera
BSCOUNT = 51 / Number of Bright Stars
FOCFLAG = 0 / Focus code run flag
SIGFILT = 1.200000 / Sigma used for gunn filter
VARFILTL = 0.000000 / Variance (left) used for gunn filter
VARFILTR = 0.000000 / Variance (right) used for gunn filter
GAINFILL = 1.000000 / Amp Gain (left) used for gunn filter
GAINFILR = 1.000000 / Amp Gain (right) used for gunn filter
NMEDIAN = 42 / Number used in stokes medians
RMEDIAN = -9999.000000 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'MIDROW' / Frame row of the stamp's middle pixel.
TFORM2 = '1J'
TTYPE2 = 'MIDCOL' / Frame column of the stamp's middle pixel.
TFORM3 = '1E'
TTYPE3 = 'ROWCENTROID' / Row position of star center.
TUNIT3 = 'pixels'
TFORM4 = '1E'
TTYPE4 = 'ROWCENTROIDERR' / Row position of star center. (error)
TUNIT4 = 'pixels'
TFORM5 = '1E'
TTYPE5 = 'COLCENTROID' / Column position of star center.
TUNIT5 = 'pixels'
TFORM6 = '1E'
TTYPE6 = 'COLCENTROIDERR' / Column position of star center. (error)
TUNIT6 = 'pixels'
TFORM7 = '1E'
TTYPE7 = 'RMAJOR' / Major axis radius.
TUNIT7 = 'pixels'
TFORM8 = '1E'
TTYPE8 = 'RMINOR' / Minor axis radius.
TUNIT8 = 'pixels'
TFORM9 = '1E'
TTYPE9 = 'ANGMAJORAXIS' / Major axis position angle.
TUNIT9 = 'degrees'
TFORM10 = '1E'
TTYPE10 = 'PEAK' / Peak of the gaussian fit.
TUNIT10 = 'DNs'
TFORM11 = '1E'
TTYPE11 = 'COUNTS' / Sum of counts over sky.
TUNIT11 = 'DNs'
TFORM12 = '1J'
TTYPE12 = 'STATUSFIT' / 0=ok, less than 0 implies error.
--- header unit 8: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 82'
CAMCOL = 2 / Column in imaging camera
BSCOUNT = 53 / Number of Bright Stars
FOCFLAG = 0 / Focus code run flag
SIGFILT = 1.200000 / Sigma used for gunn filter
VARFILTL = 0.000000 / Variance (left) used for gunn filter
VARFILTR = 0.000000 / Variance (right) used for gunn filter
GAINFILL = 1.000000 / Amp Gain (left) used for gunn filter
GAINFILR = 1.000000 / Amp Gain (right) used for gunn filter
NMEDIAN = 38 / Number used in stokes medians
RMEDIAN = -9999.000000 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'MIDROW' / Frame row of the stamp's middle pixel.
TFORM2 = '1J'
TTYPE2 = 'MIDCOL' / Frame column of the stamp's middle pixel.
TFORM3 = '1E'
TTYPE3 = 'ROWCENTROID' / Row position of star center.
TUNIT3 = 'pixels'
TFORM4 = '1E'
TTYPE4 = 'ROWCENTROIDERR' / Row position of star center. (error)
TUNIT4 = 'pixels'
TFORM5 = '1E'
TTYPE5 = 'COLCENTROID' / Column position of star center.
TUNIT5 = 'pixels'
TFORM6 = '1E'
TTYPE6 = 'COLCENTROIDERR' / Column position of star center. (error)
TUNIT6 = 'pixels'
TFORM7 = '1E'
TTYPE7 = 'RMAJOR' / Major axis radius.
TUNIT7 = 'pixels'
TFORM8 = '1E'
TTYPE8 = 'RMINOR' / Minor axis radius.
TUNIT8 = 'pixels'
TFORM9 = '1E'
TTYPE9 = 'ANGMAJORAXIS' / Major axis position angle.
TUNIT9 = 'degrees'
TFORM10 = '1E'
TTYPE10 = 'PEAK' / Peak of the gaussian fit.
TUNIT10 = 'DNs'
TFORM11 = '1E'
TTYPE11 = 'COUNTS' / Sum of counts over sky.
TUNIT11 = 'DNs'
TFORM12 = '1J'
TTYPE12 = 'STATUSFIT' / 0=ok, less than 0 implies error.
--- header unit 9: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 83'
CAMCOL = 3 / Column in imaging camera
BSCOUNT = 44 / Number of Bright Stars
FOCFLAG = 0 / Focus code run flag
SIGFILT = 1.200000 / Sigma used for gunn filter
VARFILTL = 0.000000 / Variance (left) used for gunn filter
VARFILTR = 0.000000 / Variance (right) used for gunn filter
GAINFILL = 1.000000 / Amp Gain (left) used for gunn filter
GAINFILR = 1.000000 / Amp Gain (right) used for gunn filter
NMEDIAN = 30 / Number used in stokes medians
RMEDIAN = -9999.000000 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'MIDROW' / Frame row of the stamp's middle pixel.
TFORM2 = '1J'
TTYPE2 = 'MIDCOL' / Frame column of the stamp's middle pixel.
TFORM3 = '1E'
TTYPE3 = 'ROWCENTROID' / Row position of star center.
TUNIT3 = 'pixels'
TFORM4 = '1E'
TTYPE4 = 'ROWCENTROIDERR' / Row position of star center. (error)
TUNIT4 = 'pixels'
TFORM5 = '1E'
TTYPE5 = 'COLCENTROID' / Column position of star center.
TUNIT5 = 'pixels'
TFORM6 = '1E'
TTYPE6 = 'COLCENTROIDERR' / Column position of star center. (error)
TUNIT6 = 'pixels'
TFORM7 = '1E'
TTYPE7 = 'RMAJOR' / Major axis radius.
TUNIT7 = 'pixels'
TFORM8 = '1E'
TTYPE8 = 'RMINOR' / Minor axis radius.
TUNIT8 = 'pixels'
TFORM9 = '1E'
TTYPE9 = 'ANGMAJORAXIS' / Major axis position angle.
TUNIT9 = 'degrees'
TFORM10 = '1E'
TTYPE10 = 'PEAK' / Peak of the gaussian fit.
TUNIT10 = 'DNs'
TFORM11 = '1E'
TTYPE11 = 'COUNTS' / Sum of counts over sky.
TUNIT11 = 'DNs'
TFORM12 = '1J'
TTYPE12 = 'STATUSFIT' / 0=ok, less than 0 implies error.
--- header unit 10: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 84'
CAMCOL = 4 / Column in imaging camera
BSCOUNT = 45 / Number of Bright Stars
FOCFLAG = 0 / Focus code run flag
SIGFILT = 1.200000 / Sigma used for gunn filter
VARFILTL = 0.000000 / Variance (left) used for gunn filter
VARFILTR = 0.000000 / Variance (right) used for gunn filter
GAINFILL = 1.000000 / Amp Gain (left) used for gunn filter
GAINFILR = 1.000000 / Amp Gain (right) used for gunn filter
NMEDIAN = 38 / Number used in stokes medians
RMEDIAN = -9999.000000 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'MIDROW' / Frame row of the stamp's middle pixel.
TFORM2 = '1J'
TTYPE2 = 'MIDCOL' / Frame column of the stamp's middle pixel.
TFORM3 = '1E'
TTYPE3 = 'ROWCENTROID' / Row position of star center.
TUNIT3 = 'pixels'
TFORM4 = '1E'
TTYPE4 = 'ROWCENTROIDERR' / Row position of star center. (error)
TUNIT4 = 'pixels'
TFORM5 = '1E'
TTYPE5 = 'COLCENTROID' / Column position of star center.
TUNIT5 = 'pixels'
TFORM6 = '1E'
TTYPE6 = 'COLCENTROIDERR' / Column position of star center. (error)
TUNIT6 = 'pixels'
TFORM7 = '1E'
TTYPE7 = 'RMAJOR' / Major axis radius.
TUNIT7 = 'pixels'
TFORM8 = '1E'
TTYPE8 = 'RMINOR' / Minor axis radius.
TUNIT8 = 'pixels'
TFORM9 = '1E'
TTYPE9 = 'ANGMAJORAXIS' / Major axis position angle.
TUNIT9 = 'degrees'
TFORM10 = '1E'
TTYPE10 = 'PEAK' / Peak of the gaussian fit.
TUNIT10 = 'DNs'
TFORM11 = '1E'
TTYPE11 = 'COUNTS' / Sum of counts over sky.
TUNIT11 = 'DNs'
TFORM12 = '1J'
TTYPE12 = 'STATUSFIT' / 0=ok, less than 0 implies error.
--- header unit 11: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 85'
CAMCOL = 5 / Column in imaging camera
BSCOUNT = 55 / Number of Bright Stars
FOCFLAG = 0 / Focus code run flag
SIGFILT = 1.200000 / Sigma used for gunn filter
VARFILTL = 0.000000 / Variance (left) used for gunn filter
VARFILTR = 0.000000 / Variance (right) used for gunn filter
GAINFILL = 1.000000 / Amp Gain (left) used for gunn filter
GAINFILR = 1.000000 / Amp Gain (right) used for gunn filter
NMEDIAN = 45 / Number used in stokes medians
RMEDIAN = -9999.000000 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'MIDROW' / Frame row of the stamp's middle pixel.
TFORM2 = '1J'
TTYPE2 = 'MIDCOL' / Frame column of the stamp's middle pixel.
TFORM3 = '1E'
TTYPE3 = 'ROWCENTROID' / Row position of star center.
TUNIT3 = 'pixels'
TFORM4 = '1E'
TTYPE4 = 'ROWCENTROIDERR' / Row position of star center. (error)
TUNIT4 = 'pixels'
TFORM5 = '1E'
TTYPE5 = 'COLCENTROID' / Column position of star center.
TUNIT5 = 'pixels'
TFORM6 = '1E'
TTYPE6 = 'COLCENTROIDERR' / Column position of star center. (error)
TUNIT6 = 'pixels'
TFORM7 = '1E'
TTYPE7 = 'RMAJOR' / Major axis radius.
TUNIT7 = 'pixels'
TFORM8 = '1E'
TTYPE8 = 'RMINOR' / Minor axis radius.
TUNIT8 = 'pixels'
TFORM9 = '1E'
TTYPE9 = 'ANGMAJORAXIS' / Major axis position angle.
TUNIT9 = 'degrees'
TFORM10 = '1E'
TTYPE10 = 'PEAK' / Peak of the gaussian fit.
TUNIT10 = 'DNs'
TFORM11 = '1E'
TTYPE11 = 'COUNTS' / Sum of counts over sky.
TUNIT11 = 'DNs'
TFORM12 = '1J'
TTYPE12 = 'STATUSFIT' / 0=ok, less than 0 implies error.
--- header unit 12: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 100
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 86'
CAMCOL = 6 / Column in imaging camera
BSCOUNT = 56 / Number of Bright Stars
FOCFLAG = 0 / Focus code run flag
SIGFILT = 1.200000 / Sigma used for gunn filter
VARFILTL = 0.000000 / Variance (left) used for gunn filter
VARFILTR = 0.000000 / Variance (right) used for gunn filter
GAINFILL = 1.000000 / Amp Gain (left) used for gunn filter
GAINFILR = 1.000000 / Amp Gain (right) used for gunn filter
NMEDIAN = 44 / Number used in stokes medians
RMEDIAN = -9999.000000 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad3 Type=astro Cr=3 Bd=2 #=6 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'MIDROW' / Frame row of the stamp's middle pixel.
TFORM2 = '1J'
TTYPE2 = 'MIDCOL' / Frame column of the stamp's middle pixel.
TFORM3 = '1E'
TTYPE3 = 'ROWCENTROID' / Row position of star center.
TUNIT3 = 'pixels'
TFORM4 = '1E'
TTYPE4 = 'ROWCENTROIDERR' / Row position of star center. (error)
TUNIT4 = 'pixels'
TFORM5 = '1E'
TTYPE5 = 'COLCENTROID' / Column position of star center.
TUNIT5 = 'pixels'
TFORM6 = '1E'
TTYPE6 = 'COLCENTROIDERR' / Column position of star center. (error)
TUNIT6 = 'pixels'
TFORM7 = '1E'
TTYPE7 = 'RMAJOR' / Major axis radius.
TUNIT7 = 'pixels'
TFORM8 = '1E'
TTYPE8 = 'RMINOR' / Minor axis radius.
TUNIT8 = 'pixels'
TFORM9 = '1E'
TTYPE9 = 'ANGMAJORAXIS' / Major axis position angle.
TUNIT9 = 'degrees'
TFORM10 = '1E'
TTYPE10 = 'PEAK' / Peak of the gaussian fit.
TUNIT10 = 'DNs'
TFORM11 = '1E'
TTYPE11 = 'COUNTS' / Sum of counts over sky.
TUNIT11 = 'DNs'
TFORM12 = '1J'
TTYPE12 = 'STATUSFIT' / 0=ok, less than 0 implies error.