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20082024
most citedDusty Star-Forming Galaxies at High Redshift

803 citations · 10.9k across the 152 of their papers we have counts for

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Showing 2012Show all

9 papers · 1 filter

astro-ph.CO2012★ 170 cited

A Redshift Survey of Herschel Far-Infrared Selected Starbursts and Implications for Obscured Star Formation

C. M. Casey, S. Berta, M. Béthermin +30

We present Keck spectroscopic observations and redshifts for a sample of 767 Herschel-SPIRE selected galaxies (HSGs) at 250, 350, and 500um, taken with the Keck I Low Resolution Im…

astro-ph.CO2012★ 160 cited

Spectral Energy Distributions of Local Luminous And Ultraluminous Infrared Galaxies

Vivian U, David B. Sanders, Joseph M. Mazzarella +19

Luminous and ultraluminous infrared galaxies ((U)LIRGs) are the most extreme star forming galaxies in the universe. The local (U)LIRGs provide a unique opportunity to study their m…

astro-ph.CO2012★ 55 cited

Faint Submillimter Galaxy Counts at 450 micron

Chian-Chou Chen, Lennox L. Cowie, Amy J. Barger +5

We present the results of SCUBA2 observations at 450 micron and 850 micron of the field lensed by the massive cluster A370. With a total survey area > 100 arcmin2 and 1 sigma sensi…

astro-ph.CO2012★ 168 cited

HerMES: Cosmic Infrared Background Anisotropies and the Clustering of Dusty Star-Forming Galaxies

M. P. Viero, L. Wang, M. Zemcov +51

We present measurements of the auto- and cross-frequency power spectra of the cosmic infrared background (CIB) at 250, 350, and 500um (1200, 860, and 600 GHz) from observations tot…

astro-ph.CO2012★ 40 cited

FMOS near-IR spectroscopy of Herschel selected galaxies: star formation rates, metallicity and dust attenuation at z~1

I. G. Roseboom, A. Bunker, M. Sumiyoshi +36

We investigate the properties (e.g. star formation rate, dust attentuation, stellar mass and metallicity) of a sample of infrared luminous galaxies at z \sim 1 via near-IR spectros…

astro-ph.CO2012★ 387 cited

Far-infrared Spectral Energy Distribution Fitting for Galaxies Near and Far

Caitlin M. Casey

Spectral Energy Distribution (SED) fitting in the far-infrared (FIR) is greatly limited by a dearth of data and an excess of free parameters - from galaxies' dust composition, temp…