Paper
21 September 2012 A Spitzer IRAC measure of the zodiacal light
Jessica E. Krick, William J. Glaccum, Sean J. Carey, Patrick J. Lowrance, Jason A. Surace, James G. Ingalls, Joseph L. Hora, William T. Reach
Author Affiliations +
Abstract
The dominant non-instrumental background source for space-based infrared observatories is the zodiacal light (ZL). We present Spitzer Infrared Array Camera (IRAC) measurements of the ZL at 3.6, 4.5, 5.8, and 8.0 μm, taken as part of the instrument calibrations. We measure the changing surface brightness levels in approximately weekly IRAC observations near the north ecliptic pole over the period of roughly 8.5 years. This long time baseline is crucial for measuring the annual sinusoidal variation in the signal levels due to the tilt of the dust disk with respect to the ecliptic, which is the true signal of the ZL. This is compared to both Cosmic Background Explorer Diffuse Infrared Background Experiment data and a ZL model based thereon. Our data show a few percent discrepancy from the Kelsall et al.(1998)1 model including a potential warping of the interplanetary dust disk and a previously detected overdensity in the dust cloud directly behind the Earth in its orbit. Accurate knowledge of the ZL is important for both extragalactic and Galactic astronomy including measurements of the cosmic infrared background, absolute measures of extended sources, and comparison to extrasolar interplanetary dust models. IRAC data can be used to further inform and test future ZL models.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jessica E. Krick, William J. Glaccum, Sean J. Carey, Patrick J. Lowrance, Jason A. Surace, James G. Ingalls, Joseph L. Hora, and William T. Reach "A Spitzer IRAC measure of the zodiacal light", Proc. SPIE 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, 84421X (21 September 2012); https://doi.org/10.1117/12.926664
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Cited by 1 scholarly publication.
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KEYWORDS
Data modeling

Cryogenics

Calibration

Clouds

Galactic astronomy

Thermal modeling

Stars

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