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LoCuSS: The infall of X-ray groups onto massive clusters, , , , , , , , , and 3 other author(s). (2017)cite arxiv:1709.04945Comment: 20 pages, 17 figures. Submitted to MNRAS. Comments welcome.Ripping Apart at the Seams: The Network of Stripped Gas Surrounding M86, , , , , , and . (2012)cite arxiv:1212.3612Comment: 10 pages, 5 figures. Please contact Steven Ehlert (sehlert@stanford.edu) for higher resolution figures.The surprisingly large dust and gas content of quiescent galaxies at z>1.4, , , , , , , , , and 6 other author(s). (2017)cite arxiv:1703.02207Comment: 6 pages, 4 figures (main); 9 pages, 6 figures (supplementary); submitted to Nature Astronomy, comments welcome.Galaxy evolution in overdense environments at high redshift: passive early-type galaxies in a cluster at redshift 2, , , , , , , , , and 1 other author(s). (2013)cite arxiv:1305.3577Comment: 17 pages, 13 figures, ApJ in press.Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6?, , , , , , , , , and 20 other author(s). (2013)cite arxiv:1310.1398Comment: Accepted for publication in MNRAS.Non-linearity and environmental dependence of the star forming galaxies Main Sequence, , , , , , , , , and 23 other author(s). (2015)cite arxiv:1511.01899Comment: 14 pages, 14 figures, accepted for publication in MNRAS.The evolution of the star formation activity per halo mass up to redshift ~ 1.6 as seen by Herschel, , , , , , , , , and 33 other author(s). (2011)cite arxiv:1110.2946 Comment: 8 pages, 3 figures, accepted for publication on A&A.LoCuSS: The slow quenching of star formation in cluster galaxies and the need for pre-processing, , , , , , , , , and 1 other author(s). (2015)cite arxiv:1504.05604Comment: 22 pages, 23 figures. Accepted for publication in ApJ.A giant Ly$\alpha$ nebula in the core of an X-ray cluster at $z=1.99$: implications for early energy injection, , , , , , , , , and 10 other author(s). (2016)cite arxiv:1605.03194Comment: 15 pages, 10 figures, 1 appendix. Resubmitted to ApJ after referee reports.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.