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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.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.Star-forming dwarf galaxies in the Virgo cluster: the link between molecular gas, atomic gas, and dust, , , , , , , , , and 4 other author(s). (2016)cite arxiv:1602.09077Comment: 19 pages, 11 figures, accepted for publication in Astronomy & Astrophysics.The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel, , , , , , , , , and 33 other author(s). (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&amp;A.Cosmological model dependence of the galaxy luminosity function: far-infrared results in the Lemaitre-Tolman-Bondi model, , , , , , , , , and 2 other author(s). (2013)cite arxiv:1308.2199Comment: 23 pages, 11 figures. Accepted for publication in A&A.Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1403.3615Comment: 24 pages, 23 figures, accepted for publication in MNRAS.Building the cosmic infrared background brick by brick with Herschel/PEP, , , , , , , , , and 17 other author(s). (2011)cite arxiv:1106.3070Comment: Proposed for acceptance on A&A.The lesser role of starbursts for star formation at z=2, , , , , , , , , and 24 other author(s). (2011)cite arxiv:1108.0933Comment: Accepted for publication in ApJ Letters.Dust-obscured star formation and the contribution of galaxies escaping UV/optical color selections at z~2, , , , , , , , , and . (2011)cite arxiv:1106.0498Comment: Accepted for publication in A&amp;A. 16 pages, 13 figures.