UV continuum slope and dust obscuration from z ~ 6 to z ~ 2: the star formation rate density at high redshift
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On the nature of Hα emitters atz∼ 2 from the HiZELS survey: physical properties, Lyα escape fraction and main sequenceThe ultraviolet colours and dust attenuation of Lyman-break galaxiesPlanck 2013 results. XXX. Cosmic infrared background measurements and implications for star formationFMOS near-IR spectroscopy of Herschel-selected galaxies: star formation rates, metallicity and dust attenuation at z ∼ 1Seeking Completeness for high-z ULIRGs: from SCUBA to HerschelTracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICAGOODS-Herschel: dust attenuation properties of UV selected high redshift galaxiesThe VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 < z ≃ 6The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-α emitters from z = 2 to z = 6Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTAThe star formation rate density and dust attenuation evolution over 12 Gyr with the VVDS surveysThe VIMOS VLT Deep Survey: star formation rate density of Lyαemitters from a sample of 217 galaxies with spectroscopic redshifts 2 ≤ z ≤ 6.6The rate of supernovae at redshift 0.1–1.0Large-scale clustering of Lyman α emission intensity from SDSS/BOSSThe Hubble Space Telescope GOODS NICMOS Survey: overview and the evolution of massive galaxies at 1.5 < z < 3Influence of physical galaxy properties on Lyαescape in star-forming galaxiesGAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxiesGalactic winds in cosmological simulations of the circumgalactic mediumThe blue UV slopes ofz ~ 4 Lyman break galaxies: implications for the corrected star formation rate densityThe VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5Dust properties of Lyman-break galaxies at z ~ 3The mass evolution of the first galaxies: stellar mass functions and star formation rates at 4 < z < 7 in the CANDELS GOODS-South fieldConstraints on the star-formation rate ofz~ 3 LBGs with measured metallicity in the CANDELS GOODS-South fieldThe UV continua and inferred stellar populations of galaxies at z ≃ 7–9 revealed by the Hubble Ultra-Deep Field 2012 campaignThe ages, masses and star formation rates of spectroscopically confirmed z ∼ 6 galaxies in CANDELSThe tumultuous formation of the Hubble sequence at z > 1 examined with HST/Wide-Field Camera-3 observations of the Hubble Ultra Deep FieldA high definition view of the COSMOS Wall atz ~ 0.73GMASS ultradeep spectroscopy of galaxies atz ~ 2The star formation rate cookbook at 1 < z < 3: Extinction-corrected relations for UV and [OII]λ3727 luminositiesHerMES: unveiling obscured star formation – the far-infrared luminosity function of ultraviolet-selected galaxies at z ∼ 1.5The evolution of Lyman-break galaxies in the cold dark matter model
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UV continuum slope and dust obscuration from z ~ 6 to z ~ 2: the star formation rate density at high redshift
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Oktober 2009 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
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wetenschappelijk artikel
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наукова стаття, опублікована в жовтні 2009
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name
UV CONTINUUM SLOPE AND DUST OB ...... RATE DENSITY AT HIGH REDSHIFT
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UV continuum slope and dust ob ...... rate density at high redshift
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type
label
UV CONTINUUM SLOPE AND DUST OB ...... RATE DENSITY AT HIGH REDSHIFT
@nl
UV continuum slope and dust ob ...... rate density at high redshift
@en
prefLabel
UV CONTINUUM SLOPE AND DUST OB ...... RATE DENSITY AT HIGH REDSHIFT
@nl
UV continuum slope and dust ob ...... rate density at high redshift
@en
P2093
P50
P356
P1476
UV continuum slope and dust ob ...... rate density at high redshift
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G. D. Illingworth
G. R. Meurer
R. J. Bouwens
R.-R. Chary
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P356
10.1088/0004-637X/705/1/936
P407
P577
2009-10-16T00:00:00Z
P818
P819
2009ApJ...705..936B