paper

Hyper-luminous Dust Obscured Galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE

arXiv:1506.00320 · doi:10.1093/pasj/psv057

Abstract

We present the photometric properties of a sample of infrared (IR) bright dust obscured galaxies (DOGs). Combining wide and deep optical images obtained with the Hyper Suprime-Cam (HSC) on the Subaru Telescope and all-sky mid-IR (MIR) images taken with Wide-Field Infrared Survey Explorer (WISE), we discovered 48 DOGs with and , where , , and [22] represent AB magnitude in the -band, -band, and 22 m, respectively, in the GAMA 14hr field ( 9 deg). Among these objects, 31 ( 65 %) show power-law spectral energy distributions (SEDs) in the near-IR (NIR) and MIR regime, while the remainder show a NIR bump in their SEDs. Assuming that the redshift distribution for our DOGs sample is Gaussian, with mean and sigma = 1.99 0.45, we calculated their total IR luminosity using an empirical relation between 22 m luminosity and total IR luminosity. The average value of the total IR luminosity is (3.5 1.1) L, which classifies them as hyper-luminous infrared galaxies (HyLIRGs). We also derived the total IR luminosity function (LF) and IR luminosity density (LD) for a flux-limited subsample of 18 DOGs with 22 m flux greater than 3.0 mJy and with -band magnitude brighter than 24 AB magnitude. The derived space density for this subsample is log = -6.59 0.11 [Mpc]. The IR LF for DOGs including data obtained from the literature is well fitted by a double-power law. The derived lower limit for the IR LD for our sample is 3.8 10 [L Mpc] and its contributions to the total IR LD, IR LD of all ultra-luminous infrared galaxies (ULIRGs), and that of all DOGs are 3 %, 9 %, and 15 %, respectively.

15 pages, 15 figures, and 3 tables, accepted for publication in PASJ (Subaru special issue)