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Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo

, , , , , , , , , , , , , , , , , , , , , , and . (2022)cite arxiv:2203.14972Comment: Accepted for publication in ApJ Letters, 9 pages, 5 figures. Interactive versions of Fig. 2 and data products are available at https://github.com/spt-smg/publicdata.

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The Role of Active Galactic Nuclei in the Quenching of Massive Galaxies in the SQuiGGLE Survey, , , , , , , and . (2020)cite arxiv:2007.02967Comment: 10 pages, 4 figures, posted after review by ApJL.Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo, , , , , , , , , and 13 other author(s). (2022)cite arxiv:2203.14972Comment: Accepted for publication in ApJ Letters, 9 pages, 5 figures. Interactive versions of Fig. 2 and data products are available at https://github.com/spt-smg/publicdata.Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z $\sim$ 3, , , , , , , , , and 10 other author(s). (2019)cite arxiv:1906.05469.Massive quenched galaxies at z~0.7 retain large molecular gas reservoirs, , , , , , , and . (2017)cite arxiv:1708.03337Comment: Accepted for publication in ApJ Letters (6 pages, 5 figures).