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Cited article:
A. Amblard, A. Cooray, P. Serra, P. Temi, E. Barton, M. Negrello, R. Auld, M. Baes, I. K. Baldry, S. Bamford
A&A, 518 (2010) L9
Published online: 2010-07-16
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HerMES: deep number counts at 250 μm, 350 μm and 500 μm in the COSMOS and GOODS-N fields and the build-up of the cosmic infrared background
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Submillimetre galaxies reside in dark matter haloes with masses greater than 3 × 1011 solar masses
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Dusty extreme starbursts in the early universe
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Measurement of CIB power spectra over large sky areas fromPlanckHFI maps
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STAR FORMATION BIMODALITY IN EARLY-TYPE GALAXIES
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CROSS-CORRELATION OF NEAR- AND FAR-INFRARED BACKGROUND ANISOTROPIES AS TRACED BYSPITZERANDHERSCHEL
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The Astrophysical Journal 811 (2) 125 (2015)
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CORRELATIONS IN THE (SUB)MILLIMETER BACKGROUND FROM ACT × BLAST
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The Astrophysical Journal 744 (1) 40 (2012)
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Herschel-ATLAS/GAMA: spatial clustering of low-redshift submm galaxies
E. van Kampen, D. J. B. Smith, S. Maddox, et al.
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Revealing the cold dust in low-metallicity environments
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Which haloes host Herschel-ATLAS galaxies in the local Universe?
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Far-infrared Herschel SPIRE spectroscopy of lensed starbursts reveals physical conditions of ionized gas
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Evolution of the far-infrared-radio correlation and infrared spectral energy distributions of massive galaxies over z= 0-2
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THE INFRARED PROPERTIES OF SOURCES MATCHED IN THE
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An ALMA survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS field: halo masses for submillimetre galaxies
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Cross-correlation of Far-infrared Background Anisotropies and CMB Lensing from Herschel and Planck Satellites
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Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
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