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The COSMOS2015 Catalog: Exploring the 1<z<6 Universe with half a million galaxies, , , , , , , , , and 27 other author(s). (2016)cite arxiv:1604.02350Comment: Accepted for publication in ApJ.A Coherent Study of Emission Lines from Broad-Band Photometry: Specific Star-Formation Rates and OIII/H\beta Ratio at 3 < z < 6, , , , , , , , , and 7 other author(s). (2016)cite arxiv:1601.07173Comment: 18 pages, 11 figures, 3 tables.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.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.The Hyper Suprime-Cam SSP Survey: Overview and Survey Design, , , , , , , , , and 133 other author(s). (2017)cite arxiv:1704.05858Comment: 14 pages, 6 figures, 4 tables. Submitted to Publications of the Astronomical Society of Japan.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.Rest-UV Absorption Lines as Metallicity Estimator: the Metal Content of Star-Forming Galaxies at z~5, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1512.00018Comment: 20 pages, 13 figures, 4 tables; Submitted to ApJ.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.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.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.