Paper
12 July 2008 Stability of the Infrared Array Camera for the Spitzer Space Telescope
S. Carey, J. Surace, M. Lacy, W. Glaccum, P. Lowrance, J. L. Hora, S. Willner
Author Affiliations +
Abstract
We present an analysis of the stability of the Infrared Array Camera (IRAC) on board the Spitzer Space Telescope over the first 4.5 years of in-flight operations. IRAC consists of two InSb and two Si:As 256x256 imaging arrays with passbands centered on 3.6, 4.5. 5.8 and 8.0 microns. Variations in photometric stability, read noise, dark offsets, pixel responsivity and number of hot and noisy pixels for each detector array are trended with time. To within our measurement uncertainty, the performance of the IRAC arrays has not changed with time. The most significant variation is that number of hot pixels in the 8 micron array has increased linearly with time at a rate of 60 pixels per year. We expect that the 3.6 and 4.5 micron arrays should remain stable during the post-cryogenic phase of the Spitzer mission. We will briefly discuss some science that is enabled by the excellent stability of IRAC.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
S. Carey, J. Surace, M. Lacy, W. Glaccum, P. Lowrance, J. L. Hora, and S. Willner "Stability of the Infrared Array Camera for the Spitzer Space Telescope", Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 70102V (12 July 2008); https://doi.org/10.1117/12.790030
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Cited by 4 scholarly publications.
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KEYWORDS
Calibration

Infrared telescopes

Infrared cameras

Space telescopes

Photometry

Cameras

Infrared radiation

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