PDS_VERSION_ID = PDS3 RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 28 FILE_RECORDS = 1245 ^TABLE = ( "PHOLUS_SPECTRUM.TAB", 1) MISSION_NAME = "NEW HORIZONS" DATA_SET_ID = "NH-P-MVIC-3-PLUTO-V3.0" PRODUCT_ID = " PHOLUS_SPECTRUM " PRODUCER_INSTITUTION_NAME = "SOUTHWEST RESEARCH INSTITUTE" PRODUCT_CREATION_TIME = 2017-04-30 INSTRUMENT_NAME = " CCD IMAGER " INSTRUMENT_ID = " CCD " INSTRUMENT_HOST_NAME = "NEW HORIZONS" OBJECT = TABLE NAME = " PHOLUS_SPECTRUM " INTERCHANGE_FORMAT = ASCII ROWS = 1245 COLUMNS = 2 ROW_BYTES = 28 DESCRIPTION = " Spectrum of specific intensity of target PHOLUS This is the result of combining an albedo model spectrum for the target and the solar range to the target with the solar flux spectrum (i.e. STIS_SOLAR). The pedigree of the albedo model spectrum: This is the Cruikshank et al. 1998 model, except using Will Grundy's Hapke code instead of Ted Roush's, so it looks slightly different. It should be noted that Pholus may actually be a bit brighter than this spectrum(the absolute albedo is still somewhat uncertain, and this is on the low side of the plausible range). There are no data on the albedo of Pholus below 0.44 microns, so the part from 0.3 to 0.44 is very poorly constrained. " OBJECT = COLUMN NAME = " WAVELENGTH " START_BYTE = 1 BYTES = 13 COLUMN_NUMBER = 1 DATA_TYPE = ASCII_REAL FORMAT = "F13.7" UNIT = "micron" END_OBJECT = COLUMN OBJECT = COLUMN NAME = " PHOLUS SPECIFIC INTENSITY " START_BYTE = 15 BYTES = 12 COLUMN_NUMBER = 2 DATA_TYPE = ASCII_REAL FORMAT = "F12.7" UNIT = "W m**-2 micron**-1 sr**-1" END_OBJECT = COLUMN END_OBJECT = TABLE END