SIMPLE = T /Written by IDL: 10-Dec-1996 15:56:39.00 BITPIX = 8 / NAXIS = 0 / EXTEND = T /File contains extensions DATE = '10/12/96' / ORIGIN = 'CASB - ST ScI' / END XTENSION= 'BINTABLE' /Written by IDL: 10-Dec-1996 15:56:45.00 BITPIX = 8 / NAXIS = 2 /Binary table NAXIS1 = 28 /Number of bytes per row NAXIS2 = 17 /Number of rows PCOUNT = 0 /Random parameter count GCOUNT = 1 /Group count TFIELDS = 4 /Number of columns EXTNAME = 'Photometric CALTABLE' /Extension name TFORM1 = '1D ' /Real*8 (double precision) TTYPE1 = 'INTEGRATED_SIGNAL' /Measured Calibration Parameter TUNIT1 = 'log10Counts' /Units of column 1 TFORM2 = '1D ' /Real*8 (double precision) TTYPE2 = 'MAGNITUDE' /Physical Calibration Parameter TUNIT2 = 'E_Magnitude' /Units of column 2 TFORM3 = '1D ' /Real*8 (double precision) TTYPE3 = 'UNCERTAINTY' /1 sigma physical parameter deviation TUNIT3 = 'E_Magnitude' /Units of column 3 TFORM4 = '1J ' /Integer*4 (long integer) TTYPE4 = 'NUMBER_OF_OBJECTS' /Used to derive physical calibration TUNIT4 = 'Objects ' /Units of column 4 CALCNTXT= 'POSS_E ' /Context in which calibration is valid CALVERSN= '10/07/1996' /Calibration version THRESHLD= 500 /Threshold above sky which signal is measured The lookup table in this extension may be used to infer the magnitude of stars on plates within the context of CALCNTXT. The log(Integrated Signal) is obtained for a star by summing the total counts above THRESHLD above the background. For example, if the background for a star is measured to be 4000 and THRESHLD is 500, then the integrated signal is the sum of counts above 4500. "Number of Objects" is the number of objects used to derive the calibrated magnitude in each row of the table. END