Data Set Information
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| DATA_SET_NAME |
IRAS FOCAL PLANE ARRAY V1.0
|
| DATA_SET_ID |
IRAS-FPA-6-RDR-INSTRUMENT-INFO-V1.0
|
| NSSDC_DATA_SET_ID |
|
| DATA_SET_TERSE_DESCRIPTION |
|
| DATA_SET_DESCRIPTION |
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).
|
| DATA_SET_RELEASE_DATE |
1997-03-24T00:00:00.000Z
|
| START_TIME |
1965-01-01T12:00:00.000Z
|
| STOP_TIME |
N/A (ongoing)
|
| MISSION_NAME |
INFRARED ASTRONOMICAL SATELLITE
|
| MISSION_START_DATE |
1983-01-26T12:00:00.000Z
|
| MISSION_STOP_DATE |
1983-11-23T12:00:00.000Z
|
| TARGET_NAME |
|
| TARGET_TYPE |
|
| INSTRUMENT_HOST_ID |
IRAS
|
| INSTRUMENT_NAME |
FOCAL PLANE ARRAY
|
| INSTRUMENT_ID |
FPA
|
| INSTRUMENT_TYPE |
CAMERA
|
| NODE_NAME |
Small Bodies
|
| ARCHIVE_STATUS |
SUPERSEDED
|
| 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.
|
| CITATION_DESCRIPTION |
Sykes M.V., T.L. Brown, and A.C. Raugh, IRAS FOCAL PLANE ARRAY V1.0, IRAS-FPA-6-RDR-INSTRUMENT-INFO-V1.0, NASA Planetary Data System, 1997.
|
| ABSTRACT_TEXT |
This data presented with this data set includes: (a) 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; (b) 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); (c) 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); (d) 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); (e) 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).
|
| PRODUCER_FULL_NAME |
MARK SYKES
|
| SEARCH/ACCESS DATA |
SBN PSI WEBSITE
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