PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = "2003-05-05, PDS-SBN, Created." OBJECT = DATA_SET DATA_SET_ID = "IRAS-C-FPA-6-RDR-TEMPEL1-DI-V1.0" OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = " IRAS SPECTRAL RESPONSE FOR TEMPEL 1 DI PROCESSING V1.0" DATA_SET_TERSE_DESC = " IRAS spectral response tables used to reprocess Additional Observations and Survey Scans containing comet 9P/Tempel 1 to support the NASA Deep Impact Mission." DATA_SET_COLLECTION_MEMBER_FLG = "N" START_TIME = "N/A" STOP_TIME = "N/A" NATIVE_START_TIME = "N/A" NATIVE_STOP_TIME = "N/A" DATA_OBJECT_TYPE = TABLE DATA_SET_RELEASE_DATE = 2003-05-29 /* Preliminary Review Date */ PRODUCER_FULL_NAME = "STEPHANIE A. MCLAUGHLIN" SOFTWARE_FLAG = "N" DETAILED_CATALOG_FLAG = "N" PROCESSING_START_TIME = "N/A" PROCESSING_STOP_TIME = "N/A" DATA_SET_DESC = " The Infrared Astronomical Satellite provides radiometry for the celestial sphere in four filter passbands. This dataset was provided by Russell Walker and was used to reprocess Additional Observations and Survey Scans containing comet 9P/Tempel 1. The 12-micron spectral response table in this data includes an entry for 7.636 microns. This entry is not included in the equivalent spectral response table for the IRAS Zodiacal Dust History Archive held by PDS. The 100-micron spectral response table in this data includes an entry at the end for 145.000 microns with a relative spectral response of 0.000. The equivalent spectral response table for the IRAS Zodiacal Archive does not include this entry. Its last entry is for 140.0 microns with a relative spectral response of 0.010. Finally, the filter tables for the IRAS Tempel 1 Archive include only wavelength and equivalent spectral response. The IRAS Zodiacal Dust Archive includes the wavelength, optics transmittance, relative detector response, and equivalent spectral response." CONFIDENCE_LEVEL_NOTE = " The detector spectral response of the Ge:Ga detectors used at 100 microns was assumed to be the same as that of the 60 micron detectors even though the material came from a different source. Limits on out-of-band leaks, at short and long wavelengths, are tabulated in BEICHMANETAL1988. At 12 and 25 microns, these leaks effect the calibration by less than 0.02 percent. At 60 and 100 microns, the effect is less than 10 percent." END_OBJECT = DATA_SET_INFORMATION OBJECT = DATA_SET_TARGET TARGET_NAME = "N/A" END_OBJECT = DATA_SET_TARGET OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = "IRAS" INSTRUMENT_ID = "FPA" END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_PARAMETER_INFORMATION SAMPLING_PARAMETER_NAME = WAVE_12 MINIMUM_SAMPLING_PARAMETER = 7.0 MAXIMUM_SAMPLING_PARAMETER = 15.5 SAMPLING_PARAMETER_INTERVAL = (0.14, 0.36, 0.5) SAMPLING_PARAMETER_UNIT = "MICRON" END_OBJECT = DATA_SET_PARAMETER_INFORMATION OBJECT = DATA_SET_PARAMETER_INFORMATION SAMPLING_PARAMETER_NAME = WAVE_25 MINIMUM_SAMPLING_PARAMETER = 15.5 MAXIMUM_SAMPLING_PARAMETER = 31.5 SAMPLING_PARAMETER_INTERVAL = 0.5 SAMPLING_PARAMETER_UNIT = "MICRON" END_OBJECT = DATA_SET_PARAMETER_INFORMATION OBJECT = DATA_SET_PARAMETER_INFORMATION SAMPLING_PARAMETER_NAME = WAVE_60 MINIMUM_SAMPLING_PARAMETER = 27.0 MAXIMUM_SAMPLING_PARAMETER = 87.0 SAMPLING_PARAMETER_INTERVAL = 3.0 SAMPLING_PARAMETER_UNIT = "MICRON" END_OBJECT = DATA_SET_PARAMETER_INFORMATION OBJECT = DATA_SET_PARAMETER_INFORMATION SAMPLING_PARAMETER_NAME = WAVE_100 MINIMUM_SAMPLING_PARAMETER = 65.0 MAXIMUM_SAMPLING_PARAMETER = 145.0 SAMPLING_PARAMETER_INTERVAL = 5.0 SAMPLING_PARAMETER_UNIT = "MICRON" END_OBJECT = DATA_SET_PARAMETER_INFORMATION OBJECT = DATA_SET_HOST INSTRUMENT_HOST_ID = "IRAS" INSTRUMENT_ID = "FPA" END_OBJECT = DATA_SET_HOST OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "BEICHMANETAL1988" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END