IRS Spectra of a Unique Infrared-Varying Galaxy in the IRAC-CF

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A detailed analysis of the 87 multi-epoch mosaics taken by Spitzer/IRAC of the IRAC Dark Calibration Field at 17:40, +69:00 has uncovered numerous objects exhibiting strong variability at 3.6 um -- to our knowledge, the only variable galaxies discovered by Spitzer to date. Happily, one of these is bright enough at 24 um (0.5 mJy) to be accessible with the IRS/LL1 and LL2 in a modest allocation of only 4.1 h facility time, (S/N ~ 7 on the continuum). This object is extremely unlikely to be a foreground star -- and if it is in fact AGN dominated, then its variability, which takes place on timescales of ~ 1 year, ought toprovide a new window on substructures within AGNs. In combination with the moderate-depth ground-based photometry we have in hand, recently-completed HST/F814W observations, Akari/11, 15, and 18 um imaging observations, and approved Palomar spectroscopy, the observations will allow us to unambiguously constrain the nature of this object.

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