Paper
21 August 1998 Near-IR arrays for ground-based and space-based astronomy
Alan W. Hoffman, Ken J. Ando, Arnold D. Estrada, James D. Garnett, Nancy A. Lum, Peter J. Love, Joseph P. Rosbeck, K. P. Sparkman, Albert M. Fowler, Judith L. Pipher, William J. Forrest
Author Affiliations +
Abstract
This paper is a review of current astronomy projects at Raytheon/SBRC in the near-IR band. Another paper in this same session (3354-11) covers astronomy projects in longer wavelengths. For ground-based astronomy, InSb arrays with formats of 256 X 256, 512 X 512, and 1024 X 1024 have been developed and tested. For space-based astronomy, four projects are discussed with array formats ranging from 256 X 256 to 2K X 2K. The space projects support instruments on the SIRTF, IRIS, NGST, and Rosetta missions. Representative data are presented from 1024 X 1024 and 256 X 256 arrays obtained by test facilities at NOAO and the University of Rochester.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Alan W. Hoffman, Ken J. Ando, Arnold D. Estrada, James D. Garnett, Nancy A. Lum, Peter J. Love, Joseph P. Rosbeck, K. P. Sparkman, Albert M. Fowler, Judith L. Pipher, and William J. Forrest "Near-IR arrays for ground-based and space-based astronomy", Proc. SPIE 3354, Infrared Astronomical Instrumentation, (21 August 1998); https://doi.org/10.1117/12.317271
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Cited by 8 scholarly publications.
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KEYWORDS
Astronomy

Sensors

Infrared astronomy

Infrared radiation

Quantum efficiency

IRIS Consortium

Detector arrays

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