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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.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.FIR colours of nearby late-type galaxies in the Herschel Reference Survey, , , , , , , , , and 14 other author(s). (2012)cite arxiv:1201.2305Comment: Accepted for publication on A&amp;A.The quenching of the star formation activity in cluster galaxies, , , , , , , , , and . (2016)cite arxiv:1609.00545Comment: Accepted fro publication on Astronomy & Astrophysics.The suppression of star formation by powerful active galactic nuclei, , , , , , , , , and 68 other author(s). (2013)cite arxiv:1310.4147Comment: Published in Nature, May 2012. Includes supplementary information.GOODS-HERSCHEL: evidence for a UV extinction bump in galaxies at z &gt; 1, , , , , , , , , and 9 other author(s). (2011)cite arxiv:1107.1049Comment: 17 pages,12 figures, accepted for publication in A&amp;A.The evolution of the dust and gas content in galaxies, , , , , , , , , and 29 other author(s). (2013)cite arxiv:1311.3670Comment: Accepted for publication in A&A.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.Measuring star formation with resolved observations: the test case of M33, , , , , , , , , and 8 other author(s). (2015)cite arxiv:1502.01347Comment: 15 pages, 9 figures, 1 table. Accepted for publication in A&A.