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1 June 1994 Status report on 1024x1024 HgCdTe detector arrays for low-background operation in the 1.0- to 2.5-um range
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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.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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, and William E. Kleinhans "Status report on 1024x1024 HgCdTe detector arrays for low-background operation in the 1.0- to 2.5-um range", Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); https://doi.org/10.1117/12.176774
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