PDS_VERSION_ID = PDS3 LABEL_REVISION_NOTE = " 30 Apr 1998, a.c.raugh: Begin label revision history. 4 Sep 1998, t.l.brown: pulled out reference descriptions, added refkeyids in text. Changed DATA_PROVIDER_FULL_NAME to OBSERVER_FULL_NAME." OBJECT = DATA_SET DATA_SET_ID = "IRAS-FPA-6-RDR-INSTRUMENT-INFO-V1.0" DATA_SET_LOCAL_ID = FPA OBJECT = DATA_SET_INFORMATION DATA_SET_NAME = "IRAS FOCAL PLANE ARRAY V1.0" DATA_SET_COLLECTION_MEMBER_FLG = "N" DATA_OBJECT_TYPE = TABLE START_TIME = "N/A" STOP_TIME = "N/A" DATA_SET_RELEASE_DATE = 1997-03-24 /* Peer Review Date */ PRODUCER_FULL_NAME = "Mark Sykes" OBSERVER_FULL_NAME = "Mehrdad Moshir" /* Generated the Data */ DETAILED_CATALOG_FLAG = "N" DATA_SET_DESC = " Data Set Overview ================= This data presented with this data set include FPA.TAB - The IRAS Detector File which provides for each detector of the focal plane array its operational status, associated filter, location, dimension, sterradiance, and readout time offset. FILTER1.TAB - The transmission and response values given in this table are to energy/wavelength and represent averages over all of the IRAS detectors of Band 1 (12 microns). FILTER2.TAB - The transmission and response values given in this table are to energy/wavelength and represent averages over all of the IRAS detectors of Band 2 (25 microns). FILTER3.TAB - The transmission and response values given in this table are to energy/wavelength and represent averages over all of the IRAS detectors of Band 3 (60 microns). FILTER4.TAB - The transmission and response values given in this table are to energy/wavelength and represent averages over all of the IRAS detectors of Band 4 (100 microns)." CONFIDENCE_LEVEL_NOTE = " Review ====== FPA.TAB underwent peer review on March 24, 1997. FILTER1.TAB, FILTER2.TAB, FILTER3.TAB, and FILTER4.TAB were peer reviewed on April 26, 1993, and updated on March 24, 1997. Focal Plane Model ----------------- An explication of the focal plane model adopted here is given in McCallon (1992) [MCCALLON1992]. Detector Spectral Response -------------------------- 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 Beichman et. al (1988) [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_REFERENCE_INFORMATION REFERENCE_KEY_ID = "BEICHMANETAL1988" END_OBJECT = DATA_SET_REFERENCE_INFORMATION OBJECT = DATA_SET_REFERENCE_INFORMATION REFERENCE_KEY_ID = "MCCALLON1992" END_OBJECT = DATA_SET_REFERENCE_INFORMATION END_OBJECT = DATA_SET END