Identifying Silicate-absorbed ULIRGs at z ~ 1-2 in the Bootes Field Using the Spitzer IRS
Résumé
Using the 16 mum peak-up imager on the Infrared Spectrograph (IRS) on Spitzer, we present a serendipitous survey of 0.0392 deg2 within the area of the NOAO Deep Wide-Field Survey in Bootes. Combining our results with the available Multiband Imaging Photometer for Spitzer (MIPS) 24 mum survey of this area, we produce a catalog of 150 16 mum sources brighter than 0.18 mJy (3 sigma) for which we derive measures or limits on the 16 mum/24 mum colors. Such colors are especially useful in determining redshifts for sources whose mid-infrared spectra contain strong emission or absorption features that characterize these colors as a function of redshift. We find that the 9.7 mum silicate absorption feature in ultraluminous infrared galaxies (ULIRGs) results in sources brighter at 16 mum than at 24 mum at z~1-1.8 by at least 20%. With a threshold flux ratio of 1.2, restricting our analysis to >5 sigma detections at 16 mum, and using a 3 sigma limit on 24 mum nondetections, the number of silicate-absorbed ULIRG candidates is 36. This defines a strong upper limit of ~920 sources deg-2 on the population of silicate-absorbed ULIRGs at z~1-1.8. This source count is about half of the total number of sources predicted at z~1-2 by various phenomenological models. We note that the high 16 mum/24 mum colors measured cannot be reproduced by any of the mid-IR spectral energy distributions assumed by these models, which points to the strong limitations currently affecting our phenomenological and theoretical understanding of infrared galaxy evolution.