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The evolving SFR-M_star relation and sSFR since z~5 from the VUDS spectroscopic survey, , , , , , , , , and 37 other author(s). (2014)cite arxiv:1411.5687Comment: 10 pages, 4 figures, submitted to A&A.Limits on the LyC signal from z~3 sources with secure redshift and HST coverage in the E-CDFS field, , , , , , , , , and 16 other author(s). (2016)cite arxiv:1601.03057Comment: Accepted for publication in A&A on Jan 5th, 2016.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.New constraints on the average escape fraction of Lyman continuum radiation in z~4 galaxies from the VIMOS Ultra Deep Survey (VUDS), , , , , , , , , and 13 other author(s). (2016)cite arxiv:1611.05882Comment: submitted to A&A.Ly\alpha-Lyman Continuum connection in 3.5 < z < 4.3 star-forming galaxies from the VUDS survey, , , , , , , , , and 9 other author(s). (2017)cite arxiv:1710.10184Comment: submitted to A&A.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 most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index, , , , , , , , , and 3 other author(s). (2019)cite arxiv:1909.07888Comment: Accepted for publication in A&A.A major merger origin for the high fraction of galaxies at 2<z<6 with 2 bright clumps in the VIMOS Ultra-Deep Survey, , , , , , , , , and 5 other author(s). (2016)cite arxiv:1611.05869Comment: 17 pages, 11 figures, submitted to A&A.The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5<z<5.5 and the colour selection of high redshift galaxies, , , , , , , , , and 36 other author(s). (2014)cite arxiv:1411.5692Comment: 15 pages, 11 figures, submitted to A&A.The ALPINE-ALMA C II Survey: C II158micron Emission Line Luminosity Functions at $z 4-6$, , , , , , , , , and 21 other author(s). (2020)cite arxiv:2006.04835Comment: 17 pages, 9 Figures, submitted to ApJ. This paper is related to the two other ALPINE papers submitted today by Loiacono and Gruppioni.