PDS_VERSION_ID = PDS3 /* FILE CHARACTERISTICS DATA ELEMENTS */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 24 FILE_RECORDS = 362 /* DATA OBJECT POINTERS */ ^TABLE = ("pa_aeff_socc_001.tab", 1) /* GENERAL DATA DESCRIPTION PARAMETERS */ MISSION_NAME = "NEW HORIZONS" DATA_SET_ID = "NH-X-ALICE-2-PLUTOCRUISE-V1.0" PRODUCT_ID = "pa_aeff_socc_001" PRODUCER_INSTITUTION_NAME = "SOUTHWEST RESEARCH INSTITUTE" PRODUCT_CREATION_TIME = 2008-02-22T13:50:00 /* INSTRUMENT-RELATED PARAMETERS */ INSTRUMENT_NAME = "ALICE ULTRAVIOLET IMAGING SPECTROGRAPH" INSTRUMENT_ID = "ALICE" INSTRUMENT_HOST_NAME = "NEW HORIZONS" /* DATA OBJECT DEFINITIONS */ OBJECT = TABLE INTERCHANGE_FORMAT = ASCII ROWS = 362 COLUMNS = 2 ROW_BYTES = 24 NAME = "EFFECTIVE AREA TABLE" DESCRIPTION = "The effective area in this table is derived from multiple sources, measured both in the lab and in-flight. Longward of 1181A, the effective area is derived by comparing in-flight observations of the stars Spica, Zeta Puppis and Bellatrix to spectra from IUE. IUE spectra have been corrected according to Massa & Fitzpatrick (2000), with an additional subsequent increase of 4% to correct from the HST/FOS flux scale to HST/STIS, as reported by Bohlin & Gilliland (2004, sec. 5.7). Shortward of 1181 A, the curve is that of the airglow channel (pa_aeff_005.tab) scaled by 3.6x10^-4, to match the SOCC effective area at long wavelengths. The ratio of Airglow effective area to the SOCC effective area appears to be independent of wavelength." OBJECT = COLUMN NAME = "WAVELENGTH" START_BYTE = 1 BYTES = 8 COLUMN_NUMBER = 1 DATA_TYPE = ASCII_REAL UNIT = "ANGSTROMS" FORMAT = "F8.2" END_OBJECT = COLUMN OBJECT = COLUMN NAME = "EFFECTIVE AREA" START_BYTE = 9 BYTES = 14 COLUMN_NUMBER = 2 DATA_TYPE = ASCII_REAL UNIT = "CM**2" FORMAT = "E14.5" END_OBJECT = COLUMN END_OBJECT = TABLE END