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The VIMOS Ultra Deep Survey: Emerging from the Dark, a Massive Proto-Cluster at z~4.57, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1703.10170Comment: 26 pages, 14 figures, 1 table, submitted to A&A.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.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 VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6, , , , , , , , , and 35 other author(s). (2014)cite arxiv:1403.3938Comment: 43 pages, 30 figures, submitted to A&A.Discovery of a rich proto-cluster at z=2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS), , , , , , , , , and 35 other author(s). (2014)cite arxiv:1403.3691Comment: 14 pages, 9 figures, submitted to 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 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.Size evolution of star-forming galaxies with $2<z<4.5$ in the VIMOS Ultra-Deep Survey, , , , , , , , , and 8 other author(s). (2016)cite arxiv:1602.01840Comment: 22 pages, 20 figures (+3 in appendix), submitted to A&A.The VIMOS Ultra Deep Survey: The role of HI kinematics and HI column density on the escape of Lyalpha photons in star-forming galaxies at 2<z<4, , , , , , , , , and 15 other author(s). (2017)cite arxiv:1707.01443Comment: Accepted on May 2017.Very low-luminosity galaxies in the early universe have observed sizes similar to single star cluster complexes, , , , , , and . (2017)cite arxiv:1711.02090Comment: 23 pages, 14 figures, 4 tables, submitted to the Astrophysical Journal, Figures 9 and 10 show comparisons with the sizes and luminosities of local star cluster complexes and evolved objects, respectively, Figure 11 presents our constraints on the z~6 proto-globular cluster LF.