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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.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.An Overview of the 2014 ALMA Long Baseline Campaign, , , , , , , , , and 240 other author(s). (2015)cite arxiv:1504.04877Comment: 11 pages, 7 figures, 2 tables; accepted for publication in the Astrophysical Journal Letters.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.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.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.Multi-wavelength properties of radio and machine-learning identified counterparts to submillimeter sources in S2COSMOS, , , , , , , , , and 29 other author(s). (2019)cite arxiv:1910.03596Comment: 24 pages, 14 figures, 3 tables, resubmitted to ApJ.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.