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Dust properties of Lyman break galaxies at $z\sim3$, , , , , , , , , and 11 other author(s). (2015)cite arxiv:1512.04120Comment: Accepted to A&A, 17 Pages, 14 Figures, 2 Tables.A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34, , , , , , , , , and 54 other author(s). (2013)cite arxiv:1304.4256Comment: 35 pages, 19 figures, 5 tables, including Supplementary Information (version formatted by the authors). To appear in Nature. Under press embargo until 18:00 London time/13:00 US Eastern Time on 17 April 2013.GOODS-Herschel Measurements of the Dust Attenuation of Typical Star-Forming Galaxies at High Redshift: Observations of UV-Selected Galaxies at z~2, , , , , , , , , and 13 other author(s). (2011)cite arxiv:1107.2653Comment: 19 pages, 10 figures, 5 tables, submitted to the Astrophysical Journal.The quenching of the star formation activity in cluster galaxies, , , , , , , , , and . (2016)cite arxiv:1609.00545Comment: Accepted fro publication on Astronomy & Astrophysics.On the redshift evolution (0 < z < 4) of dust attenuation and of the total (UV+IR) star formation rate density, , , , , , , , , and 12 other author(s). (2013)cite arxiv:1304.7000Comment: Submitted to A&A.