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Early Quenching of Massive Protocluster Galaxies Around z=2.2 Radio Galaxies

, , , and . (2016)cite arxiv:1606.07452Comment: 9 pages; 9 figures; 2 tables; Accepted for publication in MNRAS.

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Cold, clumpy accretion onto an active supermassive black hole, , , , , , , , , and 15 other author(s). (2016)cite arxiv:1606.02304Comment: Published in the June 9th, 2016 issue of Nature.The abundance of ultra-diffuse galaxies from groups to clusters: UDGs are relatively more common in more massive haloes, , , , , , , , , and 10 other author(s). (2017)cite arxiv:1706.02704Comment: 11 pages, 8 figures. Submitted for publication in A&A.Early Quenching of Massive Protocluster Galaxies Around z=2.2 Radio Galaxies, , , and . (2016)cite arxiv:1606.07452Comment: 9 pages; 9 figures; 2 tables; Accepted for publication in MNRAS.