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Proceedings Paper

Status report on 1024x1024 HgCdTe detector arrays for low-background operation in the 1.0- to 2.5-um range
Author(s): Klaus-Werner Hodapp; Donald N. B. Hall; Kadri Vural; Lester J. Kozlowski; Gary L. Bostrup; Annie Chi-yi Chen; Donald E. Cooper; Robert B. Bailey; Scott A. Cabelli; William E. Kleinhans
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Paper Abstract

The University of Hawaii and the Rockwell International Science Center are developing a large format SWIR detector array optimized for low background astronomical imaging and spectroscopic observations. This so called HgCdTe astronomical wide area IR imager (HAWAII) device will be based on the technology developed for the NICMOS project, but will incorporate several modifications of this design to improve the performance.

Paper Details

Date Published: 1 June 1994
PDF: 6 pages
Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); doi: 10.1117/12.176774
Show Author Affiliations
Klaus-Werner Hodapp, Univ. of Hawaii Institute for Astronomy (United States)
Donald N. B. Hall, Univ. of Hawaii Institute for Astronomy (United States)
Kadri Vural, Rockwell International Science Ctr. (United States)
Lester J. Kozlowski, Rockwell International Science Ctr. (United States)
Gary L. Bostrup, Rockwell International Science Ctr. (United States)
Annie Chi-yi Chen, Rockwell International Science Ctr. (United States)
Donald E. Cooper, Rockwell International Science Ctr. (United States)
Robert B. Bailey, Rockwell International Science Ctr. (United States)
Scott A. Cabelli, Rockwell International Science Ctr. (United States)
William E. Kleinhans, Valley Oaks Semiconductor, Inc. (United States)


Published in SPIE Proceedings Vol. 2198:
Instrumentation in Astronomy VIII
David L. Crawford; Eric R. Craine, Editor(s)

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