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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.A higher efficiency of converting gas to stars push galaxies at z ~ 1.6 well above the star-forming main sequence, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1505.04977Comment: Submitted to ApJ Letters; 6 pages, 4 figures.The ALPINE-ALMA CII Survey: nature, luminosity function and star formation history of continuum non-target galaxies up to z~6, , , , , , , , , and 23 other author(s). (2020)cite arxiv:2006.04974Comment: 23 pages, 14 figures. Submitted to A&A. This paper is related to the two other ALPINE papers submitted today by Loiacono and Yan.The FMOS-COSMOS survey of star-forming galaxies at z~1.6. IV: Excitation state and chemical enrichment of HII regions, , , , , , , , , and 14 other author(s). (2016)cite arxiv:1604.06802Comment: 22 pages, 17 Figures, submitted to ApJ.GMASS ultradeep spectroscopy of galaxies at z ~ 2 - VII. Star formation, extinction, and gas outflows from UV spectra, , , , , , , , , and 6 other author(s). (2011)cite arxiv:1111.4402 Comment: Accepted for publication in A&A; 19 pages, 17 figures.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.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.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.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.