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Published October 12, 2004 | Published
Book Section - Chapter Open

Comparison of laboratory and in-flight performance of infared array camera (IRAC) detector arrays on Spitzer Space Telescope

Abstract

The Infrared Array Camera (IRAC) on Spitzer Space Telescope includes four Raytheon Vision Systems focal plane arrays, two with InSb detectors, and two with Si:As detectors. A brief comparison of pre- flight laboratory results vs. in-flight performance is given, including quantum efficiency and noise, as well as a discussion of irregular effects, such as residual image performance, "first frame effect", "banding", "column pull-down" and multiplexer bleed. Anomalies not encountered in pre-flight testing, as well as post-flight laboratory tests on these anomalies at the University of Rochester and at NASA Ames using sister parts to the flight arrays, are emphasized.

Additional Information

© 2004 Society of Photo-optical Instrumentation Engineers (SPIE). This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of technology under NASA contract 1407, and by experimental support work at NASA Ames under "Infrared Detector Development Support", FY 04 RTOP 188-02-01 and at the University of Rochester under grant SVS 660011 from Smithsonian Astrophysical Observatory (SAO), which in turn is supported by NASA through Contract Number 960541 issued by JPL for IRAC. Support for the writing of this paper is under SAO grant SV4-74011.

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