Published March 5, 2003 | Version Published
Book Section - Chapter Open

Performance of the infrared array camera (IRAC) for SIRTF during instrument integration and test

Abstract

The Infrared Array Camera (IRAC) is one of three focal plane instruments in the Space Infrared Telescope Facility (SIRTF). IRAC is a four-channel camera that obtains simultaneous images at 3.6, 4.5, 5.8, and 8 microns. Two adjacent 5.12x5.12 arcmin fields of view in the SIRTF focal plane are viewed by the four channels in pairs (3.6 and 5.8 microns; 4.5 and 8 microns). All four detector arrays in the camera are 256x256 pixels in size, with the two shorter wavelength channels using InSb and the two longer wavelength channels using Si:As IBC detectors. We describe here the results of the instrument functional and calibration tests completed at Ball Aerospace during the integration with the cryogenic telescope assembly, and provide updated estimates of the in-flight sensitivity and performance of IRAC in SIRTF.

Additional Information

© 2003 Society of Photo-Optical Instrumentation Engineers. We acknowledge funding from NASA Office of Space Science for the work performed at the CfA and GSFC. We thank the Integration and Test group at GSFC for their excellent support of the IRAC testing program, including Ray Jungo, Ed Lander, Marty Brown, Ayman Mekhail, Maureen Armbruster, Peter Gorog, Jim MacLeod, and GSFC QA including Shirley Paul and Norm Lee. We also thank John Polizotti, Leslie Frazier, John Boczenowski, Warren Martell, and Paul Okun from SAO Central Engineering for system engineering and QA support.

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Identifiers

Eprint ID
91876
Resolver ID
CaltechAUTHORS:20181217-161033323

Funding

NASA

Dates

Created
2018-12-18
Created from EPrint's datestamp field
Updated
2021-11-16
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Caltech Custom Metadata

Caltech groups
Infrared Processing and Analysis Center (IPAC)
Series Name
Proceedings of SPIE
Series Volume or Issue Number
4850