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A dc-coupled, high sensitivity bolometric detector system for the Infrared Telescope in SpaceWe report the performance of an ac bridge readout system that has been developed for use on the Infrared Telescope in Space which is scheduled for launch in 1994. The ac bridge readout provides excellent dc stability enabling observing strategies well-suited to space-borne observations. The ability to modulate the optical signal slowly allows the use of new, highly sensitive, long time-constant bolometers. At 300 mK, the bolometers have an electrical noise equivalent power of 3 x 10 exp -17 W/sq rt Hz. The total noise of the differential signal, including amplifier noise, is less than 8 x 10 exp -17 W/sq rt Hz at frequencies as low as 35 mHz.
Document ID
19930066572
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Devlin, M.
(NASA Headquarters Washington, DC United States)
Lange, A. E.
(NASA Headquarters Washington, DC United States)
Wilbanks, T.
(California Univ. Berkeley, United States)
Sato, S.
(Nagoya Univ. Japan)
Date Acquired
August 16, 2013
Publication Date
April 1, 1993
Publication Information
Publication: IEEE Transactions on Nuclear Science
Volume: 40
Issue: 2
ISSN: 0018-9499
Subject Category
Spacecraft Instrumentation
Accession Number
93A50569
Funding Number(s)
CONTRACT_GRANT: NSF AST-88-57462
CONTRACT_GRANT: NAGW-1597
CONTRACT_GRANT: NAGW-1352
Distribution Limits
Public
Copyright
Other

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