Selection of Infrared-variable Objects in the IRAC Calibration Field

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Scientific paper

Since the beginning of its mission in 2003, the Spitzer Space Telescope has spent two to three hours of every IRAC instrument campaign observing a particularly dark field located a few degrees from the north galactic pole: the IRAC Dark Calibration Field. The resulting survey is now the deepest integration from 3.5 to 8.0 microns. Its unique temporal depth (109 epochs over a span of 2000 days so far) provides a means of closely monitoring the variability of 15,000 stars and galaxies in the mid-infrared. We have photometered all 109 epochs in all four IRAC bands. Based on these 4x15,000 light-curves, we detected 30 IR-variable galaxies confirming previous observations (Hund et al., 2007) and 20 long-period variability stars (Fouesneau et al., 2009 in prep.). In this contribution, we review the multi-epoch analysis and related issues, especially the light-curve periodicity analysis. We present variable candidates, already confirmed by additional observations at other wavelengths. Finally, we discuss the outcomes and perspectives of such a deep survey.

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