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Ga:Ge array developmentWork at the University of Arizona and at Lawrence Berkeley Laboratory on the development of a far infrared array camera for the Multiband Imaging Photometer on the Space Infrared Telescope Facility (SIRTF) is discussed. The camera design uses stacked linear arrays of Ge:Ga photoconductors to make a full two-dimensional array. Initial results from a 1 x 16 array using a thermally isolated J-FET readout are presented. Dark currents below 300 electrons s(exp -1) and readout noises of 60 electrons were attained. Operation of these types of detectors in an ionizing radiation environment are discussed. Results of radiation testing using both low energy gamma rays and protons are given. Work on advanced C-MOS cascode readouts that promise lower temperature operation and higher levels of performance than the current J-FET based devices is described.
Document ID
19900012007
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Young, Erick T.
(Arizona Univ. Tucson., United States)
Rieke, G. H.
(Arizona Univ. Tucson., United States)
Low, Frank J.
(Arizona Univ. Tucson., United States)
Haller, E. E.
(California Univ. Berkeley. Lawrence Berkeley Lab., United States)
Beeman, J. W.
(California Univ. Berkeley. Lawrence Berkeley Lab., 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
Instrumentation And Photography
Accession Number
90N21323
Funding Number(s)
CONTRACT_GRANT: NASW-3703
CONTRACT_GRANT: NAGW-1285
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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