Status report on 1024x1024 HgCdTe detector arrays for low-background operation in the 1.0- to 2.5-um range

Details Status report on 1024x1024 HgCdTe detector arrays for low-background operation in the 1.0- to 2.5-um range Status report on 1024x1024 HgCdTe detector arrays for low-background operation in the 1.0- to 2.5-um range

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2198..668h&link_type=abstract

Proc. SPIE Vol. 2198, p. 668-673, Instrumentation in Astronomy VIII, David L. Crawford; Eric R. Craine; Eds.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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.

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