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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.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.Non-linearity and environmental dependence of the star forming galaxies Main Sequence, , , , , , , , , and 23 other author(s). (2015)cite arxiv:1511.01899Comment: 14 pages, 14 figures, accepted for publication in MNRAS.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.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.Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6?, , , , , , , , , and 20 other author(s). (2013)cite arxiv:1310.1398Comment: 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 Mean Star-Forming Properties of QSO Host Galaxies, , , , , , , , , and 15 other author(s). (2013)cite arxiv:1310.1922Comment: 10 figures, 1 table; accepted for publication in Astronomy & Astrophysics.Dust temperature and CO-to-H2 conversion factor variations in the SFR-M* plane, , , , , , , , , and 8 other author(s). (2012)cite arxiv:1210.2760Comment: Accepted for publication in Astronomy and Astrophysics (A&A); 15 pages, 6 figures.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.