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The most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index

, , , , , , , , , , , , and . (2019)cite arxiv:1909.07888Comment: Accepted for publication in A&A.

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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.The VIMOS Ultra Deep Survey: Ly$\alpha$ Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5, , , , , , , , , and 38 other author(s). (2015)cite arxiv:1503.01753Comment: 17 pages, 10 figures, 1 table, submitted to A&A.The Role of Dust in Models of Population Synthesis, , , , and . (2013)cite arxiv:1309.5938Comment: Accepted for publication in MNRAS.The VIMOS Ultra-Deep Survey: the Ly$\alpha$ emission line morphology at $2 < z < 6$, , , , , , , , , and 13 other author(s). (2020)cite arxiv:2007.01322Comment: 18 pages, 13 figures, submitted to A&A.The Lyman Continuum escape fraction of galaxies at z=3.3 in the VUDS-LBC/COSMOS field, , , , , , , , , and 45 other author(s). (2015)cite arxiv:1509.01101Comment: 21 pages, 9 figures. Accepted for publication in A&A.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.