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20012017
most citedClouds, filaments and protostars: the Herschel Hi-GAL Milky Way

806 citations · 4.5k across the 38 of their papers we have counts for

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25 papers · 1 filter

astro-ph.CO2013★ 28 cited

Constraining the Lyman Alpha Escape Fraction with Far-Infrared Observations of Lyman Alpha Emitters

Julie L. Wardlow, S. Malhotra, Z. Zheng +22

We study the far-infrared properties of 498 Lyman Alpha Emitters (LAEs) at z=2.8, 3.1 and 4.5 in the Extended Chandra Deep Field-South, using 250, 350 and 500 micron data from the…

astro-ph.CO2013★ 139 cited

The Herschel Stripe 82 Survey (HerS): Maps and Early Catalog

M. P. Viero, V. Asboth, I. G. Roseboom +36

We present the first set of maps and band-merged catalog from the Herschel Stripe 82 Survey (HerS). Observations at 250, 350, and 500 micron were taken with the Spectral and Photom…

astro-ph.CO2013★ 54 cited

Herschel reveals the obscured star formation in HiZELS Hα emitters at z=1.47

E. Ibar, D. Sobral, P. N. Best +27

We describe the far-infrared (FIR; rest-frame 8--1000μm) properties of a sample of 443 Hα-selected star-forming galaxies in the COSMOS and UDS fields detected by the HiZELS imaging…

astro-ph.CO2013★ 266 cited

Explaining the [CII]158um Deficit in Luminous Infrared Galaxies - First Results from a Herschel/PACS Study of the GOALS Sample

T. Diaz-Santos, L. Armus, V. Charmandaris +26

We present the first results of a survey of the [CII]158um emission line in 241 luminous infrared galaxies (LIRGs) comprising the Great Observatories All-sky Survey (GOALS) sample,…

astro-ph.CO2013★ 19 cited

Far-IR Emission From Dust-Obscured Galaxies

J. A. Calanog, J. Wardlow, Hai Fu +21

Dust-obscured galaxies (DOGs) are a UV-faint, IR-bright galaxy population that reside at z~2 and are believed to be in a phase of dusty star-forming and AGN activity. We present fa…

astro-ph.CO2013★ 136 cited

HerMES: The Contribution to the Cosmic Infrared Background from Galaxies Selected by Mass and Redshift

M. P. Viero, L. Moncelsi, R. F. Quadri +26

We quantify the fraction of the cosmic infrared background (CIB) that originates from galaxies identified in the UV/optical/near-infrared by stacking 81,250 (~35.7 arcmin^2) K-sele…