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
about
Celebrating 30 years of science from the James Clerk Maxwell TelescopeHerschel reveals the obscured star formation in HiZELS H emitters at z = 1.47The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450-μm-selected galaxies and their contribution to the cosmic infrared backgroundThe SCUBA-2 Cosmology Legacy Survey: demographics of the 450-μm populationAzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts and evidence for large-scale structurePlanck 2013 results. XVIII. The gravitational lensing-infrared background correlationPlanck 2013 results. XXX. Cosmic infrared background measurements and implications for star formationThe Herschel Virgo Cluster Survey XVII. SPIRE point-source catalogs and number countsPlanck intermediate results XXVII. High-redshift infrared galaxy overdensity candidates and lensed sources discovered by Planck and confirmed by Herschel-SPIREPlanck intermediate results XXXIX. The Planck list of high-redshift source candidatesCharacterization of Scuba-2 450 μm and 850 μm selected galaxies in the COSMOS fieldFMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1GOODS-Herschel: identification of the individual galaxies responsible for the 80–290μm cosmic infrared backgroundThe Herschel Virgo Cluster Survey XX. Dust and gas in the foreground Galactic cirrusMeasurement of CIB power spectra over large sky areas fromPlanckHFI mapsProbing star formation in the dense environments of z ∼ 1 lensing haloes aligned with dusty star-forming galaxies detected with the South Pole TelescopeMulti-wavelength characterisation ofz~ 2 clustered, dusty star-forming galaxies discovered byPlanckThe redshift evolution of the distribution of star formation among dark matter halos as seen in the infraredMicrowave and radio emission of dusty star-forming galaxies: implication for the cosmic radio backgroundDust properties of Lyman-break galaxies at z ~ 3The clustering evolution of dusty star-forming galaxiesSimulated observations of sub-millimetre galaxies: the impact of single-dish resolution and field varianceHidden starbursts and active galactic nuclei at 0 < z < 4 from theHerschel-VVDS-CFHTLS-D1 field: Inferences on coevolution and feedbackEvidence for feedback in action from the molecular gas content in thez~ 1.6 outflowing QSO XID2028The influence of wavelength, flux, and lensing selection effects on the redshift distribution of dusty, star-forming galaxiesThe evolution of the dust and gas content in galaxiesStar formation rates in luminous quasars at 2 <z< 3HerMES: unveiling obscured star formation – the far-infrared luminosity function of ultraviolet-selected galaxies at z ∼ 1.5TheHerschel -ATLAS data release 1 – I. Maps, catalogues and number counts
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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
description
article publié dans la revue scientifique Astronomy and Astrophysics
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im Juni 2012 veröffentlichter wissenschaftlicher Artikel
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scientific article published in Astronomy and Astrophysics
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wetenschappelijk artikel
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наукова стаття, опублікована в червні 2012
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HerMES: deep number counts at ...... the cosmic infrared background
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HerMES: deep number counts at ...... the cosmic infrared background
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HerMES: deep number counts at ...... the cosmic infrared background
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HerMES: deep number counts at ...... the cosmic infrared background
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HerMES: deep number counts at ...... the cosmic infrared background
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HerMES: deep number counts at ...... the cosmic infrared background
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HerMES: deep number counts at ...... the cosmic infrared background
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A. Amblard
A. J. Smith
A. Papageorgiou
B. O’Halloran
C. D. Dowell
C. P. Pearson
D. L. Clements
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10.1051/0004-6361/201118698
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2012-06-01T00:00:00Z
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2012A&A...542A..58B