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The dust mass function from z~0 to z~2, , , , , and . (2019)cite arxiv:1909.11333Comment: MNRAS in press, 12 pages, 6 pages.Herschel Far-IR counterparts of SDSS galaxies: Analysis of commonly used Star Formation Rate estimates, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1403.3615Comment: 24 pages, 23 figures, accepted for publication in MNRAS.Three Lyman-alpha emitting filaments converging to a massive galaxy group at z=2.91: a case for cold gas infall, , , , , , , , , and 14 other author(s). (2020)cite arxiv:2006.11089Comment: 17 pages, 11 figures, 2 tables. Submitted to A&A. Comments welcome.The VLA-COSMOS 3 GHz Large Project: The cosmic star formation history since z~5, , , , , , , , , and 12 other author(s). (2017)cite arxiv:1703.09724Comment: 18 pages, 8 figures.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.