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Proceedings Article

Testing of mid-infrared detector arrays for FORCAST

[+] Author Affiliations
Joseph D. Adams, Terry L. Herter, George E. Gull, Bruce Pirger, Justin Schoenwald, Marc Berthoud

Cornell Univ. (USA)

Luke D. Keller

Cornell Univ. (USA) and Ithaca College (USA)

Proc. SPIE 5499, Optical and Infrared Detectors for Astronomy, 442 (September 29, 2004); doi:10.1117/12.551490
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From Conference Volume 5499

  • Optical and Infrared Detectors for Astronomy
  • James D. Garnett; James W. Beletic
  • Glasgow, Scotland | June 21, 2004

abstract

This paper presents results on performance testing of mid-infrared detector arrays for the Faint Object Infrared Camera for the SOFIA Telescope (FORCAST). FORCAST is a two-channel camera that utilizes a Si:As blocked impurity band (BIB) 256 x 256 detector array for imaging through discrete filters at 5 - 25 microns, and a Si:Sb BIB 256 x 256 detector array for imaging at 25 - 40 microns, over a 3.2' x 3.2' field of view, under high thermal background conditions. DRS Technologies has designed and fabricated several Si:As BIB and Si:Sb BIB engineering grade detector arrays which we test as candidate arrays for FORCAST. We present their initial laboratory test performance results.

© (2004) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Joseph D. Adams ; Terry L. Herter ; Luke D. Keller ; George E. Gull ; Bruce Pirger, et al.
"Testing of mid-infrared detector arrays for FORCAST", Proc. SPIE 5499, Optical and Infrared Detectors for Astronomy, 442 (September 29, 2004); doi:10.1117/12.551490; http://dx.doi.org/10.1117/12.551490


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