PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = " 2017-09-20 SOC: TF Added note about SOCC as separate from primary Alice. " /* FILE CHARACTERISTICS DATA ELEMENTS */ RECORD_TYPE = FIXED_LENGTH RECORD_BYTES = 28 FILE_RECORDS = 1024 /* DATA OBJECT POINTERS */ ^TABLE = ("PA_AEFF_SOCC_002.TAB", 1) /* GENERAL DATA DESCRIPTION PARAMETERS */ MISSION_NAME = "NEW HORIZONS KUIPER BELT EXTENDED MISSION" DATA_SET_ID = "NH-A-ALICE-3-KEM1-V2.0" PRODUCT_ID = "PA_AEFF_SOCC_002" PRODUCER_INSTITUTION_NAME = "SOUTHWEST RESEARCH INSTITUTE" PRODUCT_CREATION_TIME = 2017-04-30T00:00:00 /* 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 = 1024 COLUMNS = 2 ROW_BYTES = 28 NAME = "EFFECTIVE AREA TABLE" DESCRIPTION = " Note this table is for the 2x2 deg SOCC, not the primary Alice aperture. 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_007.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 = 13 COLUMN_NUMBER = 1 DATA_TYPE = ASCII_REAL UNIT = "ANGSTROM" FORMAT = "F13.3" END_OBJECT = COLUMN OBJECT = COLUMN NAME = "EFFECTIVE AREA" START_BYTE = 15 BYTES = 12 COLUMN_NUMBER = 2 DATA_TYPE = ASCII_REAL UNIT = "CM**2" FORMAT = "E12.6" END_OBJECT = COLUMN END_OBJECT = TABLE END