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19942013
most citedMid-Infrared Spectral Diagnosis of Submillimeter Galaxies

379 citations · 2.3k across the 37 of their papers we have counts for

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Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO201187 cited

Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS

Ivan Valtchanov, J. Virdee, R. J. Ivison +51

We present Herschel-SPIRE Fourier Transform Spectrometer (FTS) and radio follow-up observations of two Herschel-ATLAS (H-ATLAS) detected strongly lensed distant galaxies. In one of…

astro-ph.CO201016 cited

HerMES : SPIRE detection of high redshift massive compact galaxies in GOODS-N field

A. Cava, G. Rodighiero, I. Perez-Fournon +47

We have analysed the rest-frame far infrared (FIR) properties of a sample of massive (Mstar > 10^11Msun) galaxies at 2<z<3 in the GOODS (Great Observatories Origins Deep Survey) No…

astro-ph.CO2009184 cited

Over half of the far-infrared background light comes from galaxies at z >= 1.2

Mark J. Devlin, Peter A. R. Ade, Itziar Aretxaga +26

Submillimetre surveys during the past decade have discovered a population of luminous, high-redshift, dusty starburst galaxies. In the redshift range 1 <= z <= 4, these massive sub…

astro-ph.CO200945 cited

Radio and mid-infrared identification of BLAST source counterparts in the Chandra Deep Field South

Simon Dye, Peter A. R. Ade, James J. Bock +28

We have identified radio and/or mid-infrared counterparts to 198 out of 350 sources detected at >=5 sigma over ~ 9 square degrees centered on the Chandra Deep Field South (CDFS) by…

astro-ph.CO200915 cited

A Bright Submillimeter Source in the Bullet Cluster (1E0657--56) Field Detected with BLAST

Marie Rex, Peter A. R. Ade, Itziar Aretxaga +26

We present the 250, 350, and 500 micron detection of bright submillimeter emission in the direction of the Bullet Cluster measured by the Balloon-borne Large Aperture Submillimeter…

astro-ph.CO20094 cited

Observing the Evolution of the Universe

James Aguirre, Alexandre Amblard, Amjad Ashoorioon +172

How did the universe evolve? The fine angular scale (l>1000) temperature and polarization anisotropies in the CMB are a Rosetta stone for understanding the evolution of the univers…