--- 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 = 4517708353.09 / 1st row - Number of seconds since Nov 17 1858
RA = 146.43057 / 1st row - Right ascension of telescope boresigh
DEC = 42.977360 / 1st row - Declination of telescope boresight (d
SPA = 61.471 / 1st row - Camera col position angle wrt north (
IPA = 160.773 / 1st row - Instrument rotator position angle (de
IPARATE = 0.0063 / 1st row - Instrument rotator angular velocity (
AZ = 120.53297 / 1st row - Azimuth (encoder) of tele (0=N?) (de
ALT = 61.421576 / 1st row - Altitude (encoder) of tele (de
FOCUS = -312.20000 / 1st row - Focus piston (microns?)
DATE-OBS = '2002-01-14' / 1st row - TAI date
TAIHMS = '06:59:13.09' / 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 = 2887 / Run number
FRAME = 254 / Frame sequence number within the run
STRIPE = 30 / Stripe index number (23 <--> eta=0)
STRIP = 'S' / Strip in the stripe being tracked.
FLAVOR = 'science' / Flavor of this run
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 = 50.00000 / 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 = '30 S' / 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_40' / Version of DA software
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 = 12
NAXIS2 = 2128
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'QUART 12'
CAMROW = 1 / Row in imaging camera
TSHIFT = 64 / Quartile scaling factor
HISTBINS = 260 / Num bins in quartile hists
DBASE = 130 / Maximum delta for hist bases
NQCALCL = 1064 / Number of quartiles calculated - lo col numbers
NQCALCR = 1064 / Number of quartiles calculated - hi col numbers
FRBIASL = 67211 / Left Frame bias x TSHIFT
FRBIASR = 66678 / Right Frame bias x TSHIFT
FRSKYL = 75118 / Left Mean Sky Value x TSHIFT
FRSKYR = 75209 / Right Mean Sky Value x TSHIFT
FROSCNL = 67019 / Left Mean Oscn Value x TSHIFT
FROSCNR = 66766 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'Q1' / 25th percentile
TUNIT1 = 'ADUs x TSHIFT'
TFORM2 = '1J'
TTYPE2 = 'Q2' / 50th percentile
TUNIT2 = 'ADUs x TSHIFT'
TFORM3 = '1J'
TTYPE3 = 'Q3' / 75th percentile
TUNIT3 = 'ADUs x TSHIFT'
--- header unit 2: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 12
NAXIS2 = 2128
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'QUART 22'
CAMROW = 2 / Row in imaging camera
TSHIFT = 64 / Quartile scaling factor
HISTBINS = 260 / Num bins in quartile hists
DBASE = 130 / Maximum delta for hist bases
NQCALCL = 1061 / Number of quartiles calculated - lo col numbers
NQCALCR = 1063 / Number of quartiles calculated - hi col numbers
FRBIASL = 74039 / Left Frame bias x TSHIFT
FRBIASR = 75374 / Right Frame bias x TSHIFT
FRSKYL = 88536 / Left Mean Sky Value x TSHIFT
FRSKYR = 84970 / Right Mean Sky Value x TSHIFT
FROSCNL = 75423 / Left Mean Oscn Value x TSHIFT
FROSCNR = 75371 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'Q1' / 25th percentile
TUNIT1 = 'ADUs x TSHIFT'
TFORM2 = '1J'
TTYPE2 = 'Q2' / 50th percentile
TUNIT2 = 'ADUs x TSHIFT'
TFORM3 = '1J'
TTYPE3 = 'Q3' / 75th percentile
TUNIT3 = 'ADUs x TSHIFT'
--- header unit 3: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 12
NAXIS2 = 2128
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'QUART 32'
CAMROW = 3 / Row in imaging camera
TSHIFT = 64 / Quartile scaling factor
HISTBINS = 260 / Num bins in quartile hists
DBASE = 130 / Maximum delta for hist bases
NQCALCL = 1064 / Number of quartiles calculated - lo col numbers
NQCALCR = 1064 / Number of quartiles calculated - hi col numbers
FRBIASL = 107839 / Left Frame bias x TSHIFT
FRBIASR = 78787 / Right Frame bias x TSHIFT
FRSKYL = 109867 / Left Mean Sky Value x TSHIFT
FRSKYR = 79889 / Right Mean Sky Value x TSHIFT
FROSCNL = 108581 / Left Mean Oscn Value x TSHIFT
FROSCNR = 78526 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'Q1' / 25th percentile
TUNIT1 = 'ADUs x TSHIFT'
TFORM2 = '1J'
TTYPE2 = 'Q2' / 50th percentile
TUNIT2 = 'ADUs x TSHIFT'
TFORM3 = '1J'
TTYPE3 = 'Q3' / 75th percentile
TUNIT3 = 'ADUs x TSHIFT'
--- header unit 4: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 12
NAXIS2 = 2128
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'QUART 42'
CAMROW = 4 / Row in imaging camera
TSHIFT = 64 / Quartile scaling factor
HISTBINS = 260 / Num bins in quartile hists
DBASE = 130 / Maximum delta for hist bases
NQCALCL = 1063 / Number of quartiles calculated - lo col numbers
NQCALCR = 1063 / Number of quartiles calculated - hi col numbers
FRBIASL = 68027 / Left Frame bias x TSHIFT
FRBIASR = 68040 / Right Frame bias x TSHIFT
FRSKYL = 75689 / Left Mean Sky Value x TSHIFT
FRSKYR = 75603 / Right Mean Sky Value x TSHIFT
FROSCNL = 68131 / Left Mean Oscn Value x TSHIFT
FROSCNR = 67911 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'Q1' / 25th percentile
TUNIT1 = 'ADUs x TSHIFT'
TFORM2 = '1J'
TTYPE2 = 'Q2' / 50th percentile
TUNIT2 = 'ADUs x TSHIFT'
TFORM3 = '1J'
TTYPE3 = 'Q3' / 75th percentile
TUNIT3 = 'ADUs x TSHIFT'
--- header unit 5: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 12
NAXIS2 = 2128
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'QUART 52'
CAMROW = 5 / Row in imaging camera
TSHIFT = 64 / Quartile scaling factor
HISTBINS = 260 / Num bins in quartile hists
DBASE = 130 / Maximum delta for hist bases
NQCALCL = 1064 / Number of quartiles calculated - lo col numbers
NQCALCR = 1059 / Number of quartiles calculated - hi col numbers
FRBIASL = 71161 / Left Frame bias x TSHIFT
FRBIASR = 70502 / Right Frame bias x TSHIFT
FRSKYL = 75587 / Left Mean Sky Value x TSHIFT
FRSKYR = 75503 / Right Mean Sky Value x TSHIFT
FROSCNL = 71190 / Left Mean Oscn Value x TSHIFT
FROSCNR = 70448 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 Src=camera'
TFORM1 = '1J'
TTYPE1 = 'Q1' / 25th percentile
TUNIT1 = 'ADUs x TSHIFT'
TFORM2 = '1J'
TTYPE2 = 'Q2' / 50th percentile
TUNIT2 = 'ADUs x TSHIFT'
TFORM3 = '1J'
TTYPE3 = 'Q3' / 75th percentile
TUNIT3 = 'ADUs x TSHIFT'
--- header unit 6: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 12'
CAMROW = 1 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 20 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 0 / True means use 5x5 for star finding
STARDIST = 58 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1223 / Star threshold - lo column numbers
STHRESHR = 1224 / 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 = 15 / Number of lo cols to skip for hi column numbers
SHICOLL = 15 / 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 = 67211 / Left Frame bias x TSHIFT
FRBIASR = 66678 / Right Frame bias x TSHIFT
FRSKYL = 75118 / Left Mean Sky Value x TSHIFT
FRSKYR = 75209 / Right Mean Sky Value x TSHIFT
FROSCNL = 67019 / Left Mean Oscn Value x TSHIFT
FROSCNR = 66766 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 128919 / 10*Average time per row (usec)
TIMEFRAM = 110857 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 = 1686
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 22'
CAMROW = 2 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 20 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 0 / True means use 5x5 for star finding
STARDIST = 58 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1432 / Star threshold - lo column numbers
STHRESHR = 1377 / 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 = 15 / Number of lo cols to skip for hi column numbers
SHICOLL = 15 / 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 = 74039 / Left Frame bias x TSHIFT
FRBIASR = 75374 / Right Frame bias x TSHIFT
FRSKYL = 88536 / Left Mean Sky Value x TSHIFT
FRSKYR = 84970 / Right Mean Sky Value x TSHIFT
FROSCNL = 75423 / Left Mean Oscn Value x TSHIFT
FROSCNR = 75371 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 128919 / 10*Average time per row (usec)
TIMEFRAM = 110857 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 8: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 32'
CAMROW = 3 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 17 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 0 / True means use 5x5 for star finding
STARDIST = 58 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1766 / Star threshold - lo column numbers
STHRESHR = 1298 / 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 = 15 / Number of lo cols to skip for hi column numbers
SHICOLL = 15 / 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 = 107839 / Left Frame bias x TSHIFT
FRBIASR = 78787 / Right Frame bias x TSHIFT
FRSKYL = 109867 / Left Mean Sky Value x TSHIFT
FRSKYR = 79889 / Right Mean Sky Value x TSHIFT
FROSCNL = 108581 / Left Mean Oscn Value x TSHIFT
FROSCNR = 78526 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 128919 / 10*Average time per row (usec)
TIMEFRAM = 110857 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 9: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 42'
CAMROW = 4 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 20 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 0 / True means use 5x5 for star finding
STARDIST = 58 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1233 / Star threshold - lo column numbers
STHRESHR = 1232 / 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 = 15 / Number of lo cols to skip for hi column numbers
SHICOLL = 15 / 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 = 68027 / Left Frame bias x TSHIFT
FRBIASR = 68040 / Right Frame bias x TSHIFT
FRSKYL = 75689 / Left Mean Sky Value x TSHIFT
FRSKYR = 75603 / Right Mean Sky Value x TSHIFT
FROSCNL = 68131 / Left Mean Oscn Value x TSHIFT
FROSCNR = 67911 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 128919 / 10*Average time per row (usec)
TIMEFRAM = 110857 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 10: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 1686
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 52'
CAMROW = 5 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 20 / Number of Bright Stars
PIX4STAR = 5 / Number of pixels in 3x3 needed for star
STAR5X5 = 0 / True means use 5x5 for star finding
STARDIST = 58 / Minimum distance between adjacent stars
SDISTRIB = 1 / True means distribute stamps over frame
STHRESHL = 1231 / Star threshold - lo column numbers
STHRESHR = 1227 / 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 = 15 / Number of lo cols to skip for hi column numbers
SHICOLL = 15 / 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 = 71161 / Left Frame bias x TSHIFT
FRBIASR = 70502 / Right Frame bias x TSHIFT
FRSKYL = 75587 / Left Mean Sky Value x TSHIFT
FRSKYR = 75503 / Right Mean Sky Value x TSHIFT
FROSCNL = 71190 / Left Mean Oscn Value x TSHIFT
FROSCNR = 70448 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 128919 / 10*Average time per row (usec)
TIMEFRAM = 110857 / 10*T to analyze PREVframe (usec),scaled to 1 li
ASTODDOF = 0 / Astrometric odd column adjustment offset
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 11: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 12'
CAMROW = 1 / Row in imaging camera
BSCOUNT = 20 / 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 = 19 / Number used in stokes medians
RMEDIAN = 1.733601 / Median of rmajor for Stars
QMEDIAN = 0.005822 / Median of Q for Stars
UMEDIAN = -0.021870 / Median of U for Stars
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 22'
CAMROW = 2 / Row in imaging camera
BSCOUNT = 20 / 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 = 19 / Number used in stokes medians
RMEDIAN = 1.498924 / Median of rmajor for Stars
QMEDIAN = -0.001320 / Median of Q for Stars
UMEDIAN = 0.005382 / Median of U for Stars
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 13: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 32'
CAMROW = 3 / Row in imaging camera
BSCOUNT = 17 / 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 = 8 / Number used in stokes medians
RMEDIAN = 2.002327 / Median of rmajor for Stars
QMEDIAN = 0.054677 / Median of Q for Stars
UMEDIAN = -0.021110 / Median of U for Stars
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 14: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 42'
CAMROW = 4 / Row in imaging camera
BSCOUNT = 20 / 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 = 18 / Number used in stokes medians
RMEDIAN = 1.433976 / Median of rmajor for Stars
QMEDIAN = -0.004805 / Median of Q for Stars
UMEDIAN = -0.009426 / Median of U for Stars
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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 15: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 48
NAXIS2 = 20
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 52'
CAMROW = 5 / Row in imaging camera
BSCOUNT = 20 / 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 = 12 / Number used in stokes medians
RMEDIAN = 1.693987 / Median of rmajor for Stars
QMEDIAN = 0.029930 / Median of Q for Stars
UMEDIAN = -0.000005 / Median of U for Stars
AUTHOR = 'Node=sdssid2 Type=photo Cr=1 Bd=1 #=5 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.