activity
20042018
most citedThe Great Observatories Origins Deep Survey - VLT/FORS2 Spectroscopy in the GOODS-South Field

194 citations · 598 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2018★ 14 cited

Measurements of the Cross Spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz

M. P. Viero, C. L. Reichardt, B. A. Benson +40

We present measurements of the power spectra of cosmic infrared background (CIB) and cosmic microwave background (CMB) fluctuations in six frequency bands. Maps at the lower three…

astro-ph.GA2016★ 103 cited

The quenching of the star formation activity in cluster galaxies

A. Boselli, Y. Roehlly, M. Fossati +7

We study the star formation quenching mechanism in cluster galaxies by fitting the SED of the Herschel Reference Survey, a complete volume-limited K-band-selected sample of nearby…

astro-ph.CO2011★ 33 cited

Modeling of the HERMES J105751.1+573027 submillimeter source lensed by a dark matter dominated foreground group of galaxies

R. Gavazzi, A. Cooray, A. Conley +85

We present the results of a gravitational lensing analysis of the bright $\zs=2.957$ sub-millimeter galaxy (SMG), HERMES J105751.1+573027 found in {\it Herschel}/SPIRE Science Demo…

astro-ph.CO2011★ 105 cited

Discovery of a Multiply-Lensed Submillimeter Galaxy in Early HerMES Herschel/SPIRE Data

A. Conley, A. Cooray, J. D. Vieira +88

We report the discovery of a bright ($f(250\mum) > 400$ mJy), multiply-lensed submillimeter galaxy \obj\ in {\it Herschel}/SPIRE Science Demonstration Phase data from the HerMES pr…

astro-ph.CO2010★ 59 cited

HerMES: SPIRE Science Demonstration Phase Maps

L. Levenson, G. Marsden, M. Zemcov +30

We describe the production and verification of sky maps of the five SPIRE fields observed as part of the Herschel Multi-tiered Extragalactic Survey (HerMES) during the Science Demo…

astro-ph.CO2010★ 69 cited

HerMES: Halo Occupation Number and Bias Properties of Dusty Galaxies from Angular Clustering Measurements

Asantha Cooray, A. Amblard, L. Wang +77

We measure the angular correlation function, w(theta), from 0.5 to 30 arcminutes of detected sources in two wide fields of the Herschel Multi-tiered Extragalactic Survey (HerMES).…