--- 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 = 4405738812.20 / 1st row - Number of seconds since Nov 17 1858
RA = 265.25208 / 1st row - Right ascension of telescope boresigh
DEC = -0.003218 / 1st row - Declination of telescope boresight (d
SPA = 89.991 / 1st row - Camera col position angle wrt north (
IPA = 52.098 / 1st row - Instrument rotator position angle (de
IPARATE = 0.0000 / 1st row - Instrument rotator angular velocity (
AZ = 312.94618 / 1st row - Azimuth (encoder) of tele (0=N?) (de
ALT = 46.738784 / 1st row - Altitude (encoder) of tele (de
FOCUS = -999999999999.999999 / 1st row - Focus piston (microns?)
DATE-OBS = '28/06/98' / 1st row - TAI date
TAIHMS = '08:20:12.19' / 1st row - TAI time (HH:MM:SS.SS) (TAI-UT = appr
DAVERS = 'v12_2' / Version of DA software
FRAME = 404 / Frame sequence number within the run
RUN = '85' / Run number
--- header unit 1: binary table ---
XTENSION = 'BINTABLE'
BITPIX = 8
NAXIS = 2
NAXIS1 = 12
NAXIS2 = 2128
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'QUART 15'
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 = 75400 / Left Frame bias x TSHIFT
FRBIASR = 76880 / Right Frame bias x TSHIFT
FRSKYL = 87729 / Left Mean Sky Value x TSHIFT
FRSKYR = 88578 / Right Mean Sky Value x TSHIFT
FROSCNL = 75587 / Left Mean Oscn Value x TSHIFT
FROSCNR = 76725 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 25'
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 = 1064 / Number of quartiles calculated - lo col numbers
NQCALCR = 1064 / Number of quartiles calculated - hi col numbers
FRBIASL = 122690 / Left Frame bias x TSHIFT
FRBIASR = 122306 / Right Frame bias x TSHIFT
FRSKYL = 134607 / Left Mean Sky Value x TSHIFT
FRSKYR = 134765 / Right Mean Sky Value x TSHIFT
FROSCNL = 122320 / Left Mean Oscn Value x TSHIFT
FROSCNR = 122316 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 35'
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 = 1063 / Number of quartiles calculated - lo col numbers
NQCALCR = 1064 / Number of quartiles calculated - hi col numbers
FRBIASL = 97140 / Left Frame bias x TSHIFT
FRBIASR = 83102 / Right Frame bias x TSHIFT
FRSKYL = 93648 / Left Mean Sky Value x TSHIFT
FRSKYR = 84686 / Right Mean Sky Value x TSHIFT
FROSCNL = 90119 / Left Mean Oscn Value x TSHIFT
FROSCNR = 82003 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 45'
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 = 1064 / Number of quartiles calculated - lo col numbers
NQCALCR = 1064 / Number of quartiles calculated - hi col numbers
FRBIASL = 62406 / Left Frame bias x TSHIFT
FRBIASR = 58997 / Right Frame bias x TSHIFT
FRSKYL = 73015 / Left Mean Sky Value x TSHIFT
FRSKYR = 69037 / Right Mean Sky Value x TSHIFT
FROSCNL = 62414 / Left Mean Oscn Value x TSHIFT
FROSCNR = 59087 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 55'
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 = 1064 / Number of quartiles calculated - hi col numbers
FRBIASL = 72182 / Left Frame bias x TSHIFT
FRBIASR = 70180 / Right Frame bias x TSHIFT
FRSKYL = 77900 / Left Mean Sky Value x TSHIFT
FRSKYR = 75350 / Right Mean Sky Value x TSHIFT
FROSCNL = 72090 / Left Mean Oscn Value x TSHIFT
FROSCNR = 70146 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
QTNCUT = 570 / SigCut = qtNcut * 0.00527 * sigma
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 15'
CAMROW = 1 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 40 / 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 = 1417 / Star threshold - lo column numbers
STHRESHR = 1431 / 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 = 75400 / Left Frame bias x TSHIFT
FRBIASR = 76880 / Right Frame bias x TSHIFT
FRSKYL = 87729 / Left Mean Sky Value x TSHIFT
FRSKYR = 88578 / Right Mean Sky Value x TSHIFT
FROSCNL = 75587 / Left Mean Oscn Value x TSHIFT
FROSCNR = 76725 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 131048 / 10*Average time per row (usec)
TIMEFRAM = 155592 / 10*T to analyze PREVframe (usec),scaled to 1 li
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 25'
CAMROW = 2 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 40 / 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 = 2148 / Star threshold - lo column numbers
STHRESHR = 2151 / 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 = 122690 / Left Frame bias x TSHIFT
FRBIASR = 122306 / Right Frame bias x TSHIFT
FRSKYL = 134607 / Left Mean Sky Value x TSHIFT
FRSKYR = 134765 / Right Mean Sky Value x TSHIFT
FROSCNL = 122320 / Left Mean Oscn Value x TSHIFT
FROSCNR = 122316 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 131048 / 10*Average time per row (usec)
TIMEFRAM = 155592 / 10*T to analyze PREVframe (usec),scaled to 1 li
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 35'
CAMROW = 3 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 18 / 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 = 1499 / Star threshold - lo column numbers
STHRESHR = 1372 / 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 = 97140 / Left Frame bias x TSHIFT
FRBIASR = 83102 / Right Frame bias x TSHIFT
FRSKYL = 93648 / Left Mean Sky Value x TSHIFT
FRSKYR = 84686 / Right Mean Sky Value x TSHIFT
FROSCNL = 90119 / Left Mean Oscn Value x TSHIFT
FROSCNR = 82003 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 131048 / 10*Average time per row (usec)
TIMEFRAM = 155592 / 10*T to analyze PREVframe (usec),scaled to 1 li
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 45'
CAMROW = 4 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 40 / 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 = 1187 / Star threshold - lo column numbers
STHRESHR = 1126 / 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 = 62406 / Left Frame bias x TSHIFT
FRBIASR = 58997 / Right Frame bias x TSHIFT
FRSKYL = 73015 / Left Mean Sky Value x TSHIFT
FRSKYR = 69037 / Right Mean Sky Value x TSHIFT
FROSCNL = 62414 / Left Mean Oscn Value x TSHIFT
FROSCNR = 59087 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 131048 / 10*Average time per row (usec)
TIMEFRAM = 155592 / 10*T to analyze PREVframe (usec),scaled to 1 li
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 3
EXTNAME = 'STAMP 55'
CAMROW = 5 / Row in imaging camera
PSSIZE = 29 / Postage Stamp Size
BSCOUNT = 40 / 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 = 1266 / Star threshold - lo column numbers
STHRESHR = 1226 / 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 = 72182 / Left Frame bias x TSHIFT
FRBIASR = 70180 / Right Frame bias x TSHIFT
FRSKYL = 77900 / Left Mean Sky Value x TSHIFT
FRSKYR = 75350 / Right Mean Sky Value x TSHIFT
FROSCNL = 72090 / Left Mean Oscn Value x TSHIFT
FROSCNR = 70146 / Right Mean Oscn Value x TSHIFT
SKIPPED = 0 / Number of rows ignored
TIMEROW = 131048 / 10*Average time per row (usec)
TIMEFRAM = 155592 / 10*T to analyze PREVframe (usec),scaled to 1 li
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 15'
CAMROW = 1 / Row in imaging camera
BSCOUNT = 40 / 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
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 25'
CAMROW = 2 / Row in imaging camera
BSCOUNT = 40 / 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
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 35'
CAMROW = 3 / Row in imaging camera
BSCOUNT = 18 / 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
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 45'
CAMROW = 4 / Row in imaging camera
BSCOUNT = 40 / 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
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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 = 40
PCOUNT = 0
GCOUNT = 1
TFIELDS = 12
EXTNAME = 'STAR 55'
CAMROW = 5 / Row in imaging camera
BSCOUNT = 40 / 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
AUTHOR = 'Node=sdssid5 Type=photo Cr=2 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.