HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES

@article{Calanog2013HerMESTF,
  title={HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES},
  author={J. A. Calanog and Julie Wardlow and Hai Fu and Asantha Cooray and Roberto J. Assef and James J. Bock and Caitlin M. Casey and Alex Conley and Duncan Farrah and Edo Ibar and Jeyhan S. Kartaltepe and Georgios E. Magdis and Lucia Marchetti and S. J. Oliver and Ismael P{\'e}rez-Fournon and Dominik A. Riechers and Dimitra Rigopoulou and Isaac Roseboom and Bernhard Schulz and Douglas Scott and Myrto Symeonidis and Mattia Vaccari and Marco P. Viero and Michael Zemcov},
  journal={The Astrophysical Journal},
  year={2013},
  volume={775}
}
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… 

Figures and Tables from this paper

Far-infrared Properties of Infrared-bright Dust-obscured Galaxies Selected with IRAS and AKARI Far-infrared All-sky Survey

We investigate the star-forming activity of a sample of infrared (IR)-bright dust-obscured galaxies (DOGs) that show an extreme red color in the optical and IR regime, . Combining an IR-bright DOG

The composite nature of Dust-Obscured Galaxies (DOGs) at z ∼ 2–3 in the COSMOS field – I. A far-infrared view

Dust-Obscured Galaxies (DOGs) are bright 24 μm-selected sources with extreme obscuration at optical wavelengths. They are typically characterized by a rising power-law continuum of hot dust (T_D ∼

Hyper-luminous dust-obscured galaxies discovered by the Hyper Suprime-Cam on Subaru and WISE

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

A SUBMILLIMETER CONTINUUM SURVEY OF LOCAL DUST-OBSCURED GALAXIES

We conduct a 350 μm dust continuum emission survey of 17 dust-obscured galaxies (DOGs) at z = 0.05–0.08 with the Caltech Submillimeter Observatory (CSO). We detect 14 DOGs with S350 μm = 114–650 mJy

DUST PROPERTIES OF LOCAL DUST-OBSCURED GALAXIES WITH THE SUBMILLIMETER ARRAY

We report Submillimeter Array observations of the 880 μm dust continuum emission for four dust-obscured galaxies (DOGs) in the local universe. Two DOGs are clearly detected with Sν(880 μm) =10–13 mJy

Far-Infrared Surveys of Galaxy Evolution

Roughly half of the radiation from evolving galaxies in the early Universe reaches us in the far-infrared and submillimeter wavelength ranges. Recent major advances in observing capabilities, in

X-ray observations of dust obscured galaxies in the Chandra Deep Field South

We present the properties of X-ray detected dust obscured galaxies (DOGs) in the Chandra Deep Field South. In recent years, it has been proposed that a significant percentage of the elusive

AGN and star formation across cosmic time

We investigate the balance of power between stars and AGN across cosmic history, based on the comparison between the infrared (IR) galaxy luminosity function (LF) and the IR AGN LF. The former

Comparison of cosmological simulations and deep submillimetre galaxy surveys

Recent progress in submillimetre surveys by single-dish telescopes allows us to further challenge the consistency between cosmological simulations and observations. In particular, we compare our

CONSTRAINING THE Lyα ESCAPE FRACTION WITH FAR-INFRARED OBSERVATIONS OF Lyα EMITTERS

We study the far-infrared properties of 498 Lyα emitters (LAEs) at z = 2.8, 3.1, and 4.5 in the Extended Chandra Deep Field-South, using 250, 350, and 500 μm data from the Herschel Multi-tiered

References

SHOWING 1-10 OF 82 REFERENCES

The Nature of Faint Spitzer-selected Dust-obscured Galaxies

We use deep far-IR, submillimeter, radio, and X-ray imaging and mid-IR spectroscopy to explore the nature of a sample of Spitzer-selected dust-obscured galaxies (DOGs) in GOODS-N. A sample of 79

THE STAR FORMATION HISTORIES OF z ∼ 2 DUST-OBSCURED GALAXIES AND SUBMILLIMETER-SELECTED GALAXIES

The Spitzer Space Telescope has identified a population of ultraluminous infrared galaxies (ULIRGs) at z ∼ 2 that may play an important role in the evolution of massive galaxies. We measure the

EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION IN z ∼ 2 DUSTY GALAXIES FROM THE GOODS-HERSCHEL SURVEY

Dusty galaxies at z ∼ 2 span a wide range of relative brightness between rest-frame mid-infrared (8 μm) and ultraviolet wavelengths. We attempt to determine the physical mechanism responsible for

Dusty Star Forming Galaxies at High Redshift

HUBBLE SPACE TELESCOPE MORPHOLOGIES OF z ∼ 2 DUST OBSCURED GALAXIES. I. POWER-LAW SOURCES

We present high-spatial resolution optical and near-infrared imaging obtained using the ACS, WFPC2, and NICMOS cameras aboard the Hubble Space Telescope of 31 24 μm bright z ≈ 2 Dust Obscured

A Significant Population of Very Luminous Dust-Obscured Galaxies at Redshift z ~ 2

The Spitzer Space Telescope has revealed a significant population of high-redshift (z ∼ 2) dust-obscured galaxies with large mid-infrared to ultraviolet luminosity ratios. Due to their optical

GOODS-HERSCHEL: IMPACT OF ACTIVE GALACTIC NUCLEI AND STAR FORMATION ACTIVITY ON INFRARED SPECTRAL ENERGY DISTRIBUTIONS AT HIGH REDSHIFT

We explore the effects of active galactic nuclei (AGNs) and star formation activity on the infrared (0.3–1000 μm) spectral energy distributions (SEDs) of luminous infrared galaxies from z = 0.5 to

Herschel unveils a puzzling uniformity of distant dusty galaxies

The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR)

A POPULATION OF DUST-RICH QUASARS AT z ∼ 1.5

We report Herschel SPIRE (250, 350, and 500 μm) detections of 32 quasars with redshifts 0.5 ⩽z < 3.6 from the Herschel Multi-tiered Extragalactic Survey (HerMES). These sources are from a MIPS 24 μm

GOODS–Herschel: an infrared main sequence for star-forming galaxies

We present the deepest 100 to 500 μm far-infrared observations obtained with the Herschel Space Observatory as part of the GOODS-Herschel key program, and examine the infrared (IR) 3–500 μm spectral
...