Galaxy Clusters in the IRAC Dark Field. II. Mid-Infrared Sources

July 2009 • 2009ApJ...700..123K

Authors • Krick, J. E. • Surace, J. A. • Thompson, D. • Ashby, M. L. N. • Hora, J. L. • Gorjian, V. • Yan, L.

Abstract • We present infrared (IR) luminosities, star formation rates (SFR), colors, morphologies, locations, and active galactic nuclei (AGNs) properties of 24 μm detected sources in photometrically detected high-redshift clusters in order to understand the impact of environment on star formation (SF) and AGN evolution in cluster galaxies. We use three newly identified z = 1 clusters selected from the IRAC dark field; the deepest ever mid-IR survey with accompanying, 14 band multiwavelength data including deep Hubble Space Telescope imaging and deep wide-area Spitzer MIPS 24 μm imaging. We find 90 cluster members with MIPS detections within two virial radii of the cluster centers, of which 17 appear to have spectral energy distributions dominated by AGNs and the rest dominated by SF. We find that 43% of the star-forming sample have IR luminosities L _IR > 10¹¹ L _sun (luminous IR galaxies). The majority of sources (81%) are spirals or irregulars. A large fraction (at least 25%) show obvious signs of interactions. The MIPS-detected member galaxies have varied spatial distributions as compared to the MIPS-undetected members with one of the three clusters showing SF galaxies being preferentially located on the cluster outskirts, while the other two clusters show no such trend. Both the AGN fraction and the summed SFR of cluster galaxies increase from redshift zero to one, at a rate that is a few times faster in clusters than over the same redshift range in the field. Cluster environment does have an effect on the evolution of both AGN fraction and SFR from redshift one to the present, but does not affect the IR luminosities or morphologies of the MIPS sample. SF happens in the same way regardless of environment making MIPS sources look the same in the cluster and field, however the cluster environment does encourage a more rapid evolution with time as compared to the field.

Links

• PREPRINT http://arxiv.org/abs/0905.1973
• NED https://ned.ipac.caltech.edu/uri/NED::InRefcode/2009ApJ...700..123K
• ELECTR https://doi.org/10.1088%2F0004-637X%2F700%2F1%2F123
• SIMBAD http://simbad.u-strasbg.fr/simbo.pl?bibcode=2009ApJ...700..123K
• PDF https://iopscience.iop.org/article/10.1088/0004-637X/700/1/123/pdf
• PDF https://stacks.iop.org/0004-637X/700/123/pdf
• DATA https://archive.stsci.edu/mastbibref.php?bibcode=2009ApJ...700..123K
• DATA https://hst.esac.esa.int/ehst/#/pages/search;bibcode=2009ApJ...700..123K
• DATA https://irsa.ipac.caltech.edu/bibdata/2009/K/2009ApJ...700..123K.html
• SPIRES http://inspirehep.net/search?p=find+eprint+arXiv:0905.1973