--- 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 = 4570594214.81 / 1st row - Number of seconds since Nov 17 1858
RA = 351.21461 / 1st row - Right ascension of telescope boresigh
DEC = 53.034883 / 1st row - Declination of telescope boresight (d
SPA = 160.657 / 1st row - Camera col position angle wrt north (
IPA = 53.623 / 1st row - Instrument rotator position angle (de
IPARATE = 0.0090 / 1st row - Instrument rotator angular velocity (
AZ = 222.97807 / 1st row - Azimuth (encoder) of tele (0=N?) (de
ALT = 53.851674 / 1st row - Altitude (encoder) of tele (de
FOCUS = -251.00000 / 1st row - Focus piston (microns?)
DATE-OBS = '2003-09-18' / 1st row - TAI date
TAIHMS = '09:30:14.80' / 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 = 4100 / Run number
FRAME = 84 / Frame sequence number within the run
STRIPE = 1220 / Stripe index number (23 <--> eta=0)
STRIP = 'N' / Strip in the stripe being tracked.
FLAVOR = 'engineering' / Flavor of this run
OBSERVER = 'long' / 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 = 186.88230 / RA of the great circle's ascending node (deg)
INCL = 78.51139 / 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 = '1220 N' / e.g., 'stripe 50.6 degrees, north strip'
EXPTIME = '53.907456' / 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 = 2048 / Number of lines in a frame
DAVERS = 'v14_47' / Version of DA software
SCDMETHD = 'sqrtDynamic' / scdMethod
SCDWIDTH = 1280 / scdDisplayWidth
SCDDECMF = 1 / scdDecimateFactor
SCDOFSET = 410 / scdDisplayOffset
SCDDYNTH = -20 / scdDynamicThresh
SCDSTTHL = 416 / scdStaticThreshL
SCDSTTHR = 416 / scdStaticThreshR
SCDREDSZ = 512 / scdReduceSize
SCDSKYL = 411 / scdSkyLeft
SCDSKYR = 412 / 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 60'
CAMCOL = 0 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 100 / 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 = 484 / Star threshold - lo column numbers
STHRESHR = 485 / Star threshold - hi column numbers
SABSKYL = 50 / Value to add to sky level = threshold - lo colu
SABSKYR = 50 / 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 = 26277 / Left Frame bias x TSHIFT
FRBIASR = 26188 / Right Frame bias x TSHIFT
FRSKYL = 27812 / Left Mean Sky Value x TSHIFT
FRSKYR = 27836 / Right Mean Sky Value x TSHIFT
FROSCNL = 26190 / Left Mean Oscn Value x TSHIFT
FROSCNR = 26190 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 147853 / 10*Average time per row (usec)
TIMEFRAM = 155701 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 61'
CAMCOL = 1 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 100 / 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 = 1264 / Star threshold - lo column numbers
STHRESHR = 1264 / 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 = 79811 / Left Frame bias x TSHIFT
FRBIASR = 79814 / Right Frame bias x TSHIFT
FRSKYL = 79977 / Left Mean Sky Value x TSHIFT
FRSKYR = 79962 / Right Mean Sky Value x TSHIFT
FROSCNL = 79808 / Left Mean Oscn Value x TSHIFT
FROSCNR = 79816 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 147853 / 10*Average time per row (usec)
TIMEFRAM = 155701 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -1 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 62'
CAMCOL = 2 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 100 / 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 = 74048 / Left Frame bias x TSHIFT
FRBIASR = 73385 / Right Frame bias x TSHIFT
FRSKYL = 73529 / Left Mean Sky Value x TSHIFT
FRSKYR = 73538 / Right Mean Sky Value x TSHIFT
FROSCNL = 73356 / Left Mean Oscn Value x TSHIFT
FROSCNR = 73361 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 147853 / 10*Average time per row (usec)
TIMEFRAM = 155701 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = -3 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 63'
CAMCOL = 3 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 100 / 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 = 1225 / Star threshold - lo column numbers
STHRESHR = 1225 / 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 = 77088 / Left Frame bias x TSHIFT
FRBIASR = 77077 / Right Frame bias x TSHIFT
FRSKYL = 77471 / Left Mean Sky Value x TSHIFT
FRSKYR = 77487 / Right Mean Sky Value x TSHIFT
FROSCNL = 77076 / Left Mean Oscn Value x TSHIFT
FROSCNR = 77079 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 147853 / 10*Average time per row (usec)
TIMEFRAM = 155701 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 64'
CAMCOL = 4 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 100 / 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 = 253 / Star threshold - lo column numbers
STHRESHR = 254 / 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 = 15088 / Left Frame bias x TSHIFT
FRBIASR = 14902 / Right Frame bias x TSHIFT
FRSKYL = 15277 / Left Mean Sky Value x TSHIFT
FRSKYR = 15294 / Right Mean Sky Value x TSHIFT
FROSCNL = 14921 / Left Mean Oscn Value x TSHIFT
FROSCNR = 14960 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 147853 / 10*Average time per row (usec)
TIMEFRAM = 155701 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 65'
CAMCOL = 5 / Column in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 100 / 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 = 913 / Star threshold - lo column numbers
STHRESHR = 914 / 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 = 55990 / Left Frame bias x TSHIFT
FRBIASR = 57231 / Right Frame bias x TSHIFT
FRSKYL = 57491 / Left Mean Sky Value x TSHIFT
FRSKYR = 57535 / Right Mean Sky Value x TSHIFT
FROSCNL = 57228 / Left Mean Oscn Value x TSHIFT
FROSCNR = 57222 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 147853 / 10*Average time per row (usec)
TIMEFRAM = 155701 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 13 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 60'
CAMCOL = 0 / Column in imaging camera
BSCOUNT = 4 / Number of Bright Stars
FOCFLAG = 1 / 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 = 0 / Number used in stokes medians
RMEDIAN = -11.547781 / Median of rmajor for Stars
QMEDIAN = -9999.000000 / Median of Q for Stars
UMEDIAN = -9999.000000 / Median of U for Stars
AUTHOR = 'Node=sdssad1 Type=astro Cr=3 Bd=0 #=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 61'
CAMCOL = 1 / Column in imaging camera
BSCOUNT = 100 / 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 = 91 / 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=sdssad1 Type=astro Cr=3 Bd=0 #=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 62'
CAMCOL = 2 / Column in imaging camera
BSCOUNT = 100 / 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 = 96 / 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=sdssad1 Type=astro Cr=3 Bd=0 #=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 63'
CAMCOL = 3 / Column in imaging camera
BSCOUNT = 100 / 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 = 93 / 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=sdssad1 Type=astro Cr=3 Bd=0 #=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 64'
CAMCOL = 4 / Column in imaging camera
BSCOUNT = 100 / 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 = 88 / 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=sdssad1 Type=astro Cr=3 Bd=0 #=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 65'
CAMCOL = 5 / Column in imaging camera
BSCOUNT = 100 / 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 = 86 / 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=sdssad1 Type=astro Cr=3 Bd=0 #=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.