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The radial and azimuthal profiles of Mg II absorption around 0.5 &lt; z &lt; 0.9 zCOSMOS galaxies of different colors masses and environments, , , , , , , , , and 43 other author(s). (2011)cite arxiv:1106.0616Comment: 12 pages, 9 figures, submitted to ApJ.The SINS/zC-SINF Survey of $z\sim2$ Galaxy Kinematics: Rest-frame Morphology, Structure, and Colors from Near-infrared Hubble Space Telescope Imaging, , , , , , , , , and 7 other author(s). (2014)cite arxiv:1411.7034Comment: 25 pages (+11 pages appendix), 20 figures; re-submitted to ApJ after responding to the first referee report.zCOSMOS 20k: Satellite galaxies are the main drivers of environmental effects in the galaxy population at least to z~0.7, , , , , , , , , and 34 other author(s). (2013)cite arxiv:1307.4402Comment: 22 pages, 19 figures, submitted to MNRAS.Euclid preparation: V. Predicted yield of redshift 7<z<9 quasars from the wide survey, , , , , , , , , and 119 other author(s). (2019)cite arxiv:1908.04310Comment: Submitted to A&A. This paper has been internally reviewed by the Euclid Consortium.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.$Euclid$ preparation: XV. Forecasting cosmological constraints for the $Euclid$ and CMB joint analysis, , , , , , , , , and 199 other author(s). (2021)cite arxiv:2106.08346Comment: 19 pages, 8 figures, 4 tables, 1 appendix.HeII emitters in the VIMOS VLT Deep Survey: PopIII star formation or peculiar stellar populations in galaxies at 2<z<4.6?, , , , , , , , , and 8 other author(s). (2012)cite arxiv:1212.5270Comment: submitted to A&A; comments are welcome.The Colors of Central and Satellite Galaxies in zCOSMOS out to z ~ 0.8 and Implications for Quenching, , , , , , , , , and 40 other author(s). (2012)cite arxiv:1211.5607Comment: 9 pages, 5 figures, submitted to ApJ.Modelling the number density of Halpha emitters for future spectroscopic near-IR space missions, , , , , , , , and . (2016)cite arxiv:1603.01453Comment: 16 pages, 7 figures, A&A (in press, preprint version available online). Models can be downloaded at http://www.bo.astro.it/~pozzetti/Halpha/Halpha.html.