Journal article
HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES
The Astrophysical journal, Vol.775(1), 61
09/05/2013
DOI: 10.1088/0004-637X/775/1/61
Abstract
Dust-obscured galaxies (DOGs) are an ultraviolet-faint, infrared-bright galaxy population that reside at z ∼ 2 and are believed to be in a phase of dusty star-forming and active galactic nucleus (AGN) activity. We present far-infrared (far-IR) observations of a complete sample of DOGs in the 2 deg2 of the Cosmic Evolution Survey. The 3077 DOGs have 〈z〉 = 1.9 ± 0.3 and are selected from 24 μm and r+ observations using a color cut of r+ − [24] ⩾ 7.5 (AB mag) and S24 ⩾ 100 μJy. Based on the near-IR spectral energy distributions, 47% are bump DOGs (star formation dominated) and 10% are power-law DOGs (AGN-dominated). We use SPIRE far-IR photometry from the Herschel Multi-tiered Extragalactic Survey to calculate the IR luminosity and characteristic dust temperature for the 1572 (51%) DOGs that are detected at 250 μm (⩾3σ). For the remaining 1505 (49%) that are undetected, we perform a median stacking analysis to probe fainter luminosities. Herschel-detected and undetected DOGs have average luminosities of (2.8 ± 0.4) × 1012 L☉ and (0.77 ± 0.08) × 1012 L☉, and dust temperatures of (33 ± 7) K and (37 ± 5) K, respectively. The IR luminosity function for DOGs with S24 ⩾ 100 μJy is calculated, using far-IR observations and stacking. DOGs contribute 10%–30% to the total star formation rate (SFR) density of the universe at z = 1.5–2.5, dominated by 250 μm detected and bump DOGs. For comparison, DOGs contribute 30% to the SFR density for all z = 1.5–2.5 galaxies with S24 ⩾ 100 μJy. DOGs have a large scatter about the star formation main sequence and their specific SFRs show that the observed phase of star formation could be responsible for their total observed stellar mass at z ∼ 2.
Details
- Title: Subtitle
- HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES
- Creators
- J. A CalanogJ WardlowHai FuA CoorayR. J AssefJ BockC. M CaseyA ConleyD FarrahE IbarJ KartaltepeG MagdisL MarchettiS. J OliverI Pérez-FournonD RiechersD RigopoulouI. G RoseboomB SchulzDouglas ScottM SymeonidisM VaccariM VieroM Zemcov
- Resource Type
- Journal article
- Publication Details
- The Astrophysical journal, Vol.775(1), 61
- DOI
- 10.1088/0004-637X/775/1/61
- ISSN
- 0004-637X
- eISSN
- 1538-4357
- Publisher
- Institute of Physics (IOP)
- Language
- English
- Date published
- 09/05/2013
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984199695902771
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