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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 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.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 VIMOS Public Extragalactic Survey (VIPERS): First Data Release of 57 204 spectroscopic measurements, , , , , , , , , and 39 other author(s). (2013)cite arxiv:1310.1008Comment: 17 pages, 17 figures, submitted to Astronomy & Astrophysics.The dependence of Galactic outflows on the properties and orientation of zCOSMOS galaxies at z ~ 1, , , , , , , , , and 37 other author(s). (2013)cite arxiv:1307.6553Comment: 12 pages, 14 figures, ApJ submitted.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&amp;A; 19 pages, 17 figures.The cosmic evolution of oxygen and nitrogen abundances in star-forming galaxies over the last 10 Gyrs, , , , , , , , , and 28 other author(s). (2012)cite arxiv:1210.0334Comment: 15 pages, 13 figures. Accepted for publication in Astronomy & Astrophysics.Peering through the holes: the far UV color of star-forming galaxies at z~3-4 and the escaping fraction of ionizing radiation, , , , , , , , , and 4 other author(s). (2015)cite arxiv:1502.04708Comment: Accepted for publication in Astronomy & Astrophysics. 13 pages, 7 figures.Analogs of primeval galaxies two billion years after the Big Bang, , , , , , , , , and 23 other author(s). (2017)cite arxiv:1701.04416Comment: 25 pages, 8 figs, 2 tables. Accepted for publication.Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys, , , , , , , , , and 2 other author(s). (2017)cite arxiv:1709.01936Comment: Accepted for publication in MNRAS. 21 pages (+9 pages of appendix), 18 Figures. Machine readable tables will be available online.