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Stressed detector arrays for airborne astronomyThe development of stressed Ge:Ga detector arrays for far-infrared astronomy from the Kuiper Airborne Observatory (KAO) is discussed. Researchers successfully constructed and used a three channel detector array on five flights from the KAO, and have conducted laboratory tests of a two-dimensional, 25 elements (5x5) detector array. Each element of the three element array performs as well as the researchers' best single channel detector, as do the tested elements of the 25 channel system. Some of the exciting new science possible with far-infrared detector arrays is also discussed.
Document ID
19900012016
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Stacey, G. J.
(California Univ. Berkeley., United States)
Beeman, J. W.
(California Univ. Berkeley., United States)
Haller, E. E.
(California Univ. Berkeley., United States)
Geis, N.
(California Univ. Berkeley, CA, United States)
Poglitsch, A.
(California Univ. Berkeley, CA, United States)
Rumitz, M.
(Max-Planck-Inst. fuer Physik und Astrophysik, Garching, Germany F.R. , United States)
Date Acquired
September 6, 2013
Publication Date
October 1, 1989
Publication Information
Publication: NASA, Ames Research Center, Proceedings of the Third Infrared Detector Technology Workshop
Subject Category
Astronomy
Accession Number
90N21332
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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