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The integrated stellar content of dark matter halos

, , , , , , , , and . (2011)cite arxiv:1109.0010Comment: Submitted to ApJ. 16 Pages, 11 Figures. Comments Welcome.

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A filament of dark matter between two clusters of galaxies, , , , , , and . (2012)cite arxiv:1207.0809Comment: Nature, in press.Discovery of a galaxy cluster with a violently starbursting core at z=2.506, , , , , , , , , and 9 other author(s). (2016)cite arxiv:1604.07404Comment: submitted.Chemical Enrichment RGS cluster sample (CHEERS): Constraints on turbulence, , , , , , , , and . (Jan 6, 2015)Building robust AGN mock catalogs to unveil black hole evolution and for survey planning, , , , , , , and . (2021)cite arxiv:2105.02883Comment: Accepted for publication in the Astrophysical Journal.Clustering, host halos and environment of z$\sim$2 galaxies as a function of their physical properties, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1405.0492Comment: 18 pages, 16 figures, Accepted by A&A.The integrated stellar content of dark matter halos, , , , , , , , and . (2011)cite arxiv:1109.0010Comment: Submitted to ApJ. 16 Pages, 11 Figures. Comments Welcome.LoCuSS: Pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2, , , , , and . (2017)cite arxiv:1710.04230Comment: 5 pages, 2 figures. Accepted for publication in MNRAS Letters.CANDELS: Constraining the AGN-Merger Connection with Host Morphologies at z~2, , , , , , , , , and 28 other author(s). (2011)cite arxiv:1109.2588 Comment: 10 Pages, 5 Figures, Revised draft submitted to ApJ.Do group dynamics play a role in the evolution of member galaxies?, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1308.1406Comment: 14 pages, 6 figures, MNRAS accepted.BUDHIES III: The fate of HI and the quenching of galaxies in evolving environments, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1604.07832Comment: 21 pages (including appendix). Accepted for publication in MNRAS.