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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).

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Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , and 15 other author(s). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.First spectroscopic observations of the galaxies that reionized the Universe, , , , , , , , , and 23 other author(s). (2023)cite arxiv:2308.08540Comment: 29 pages, 7 figures, 2 tables.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.Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z=1.522, , , , , , and . (2019)cite arxiv:1902.09564Comment: 8 pages, 5 figures, resubmitted to ApJL following referee report.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).The colors and sizes of recently quenched galaxies: a result of compact starburst before quenching, , , , , , , , , and 4 other author(s). (2019)cite arxiv:1912.03683Comment: 16 pages, 8 figures, 1 table, accepted by ApJ.Two Remarkably Luminous Galaxy Candidates at $z\approx11-13$ Revealed by JWST, , , , , , , , , and 14 other author(s). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.The JWST UNCOVER Treasury survey: Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization, , , , , , , , , and 24 other author(s). (2022)cite arxiv:2212.04026Comment: 17 pages, 8 figures, 4 tables, submitted to ApJ, comments welcome.Discovery of a dark, massive, ALMA-only galaxy at z~5-6 in a tiny 3-millimeter survey, , , , , , , , , and . (2019)cite arxiv:1905.11996Comment: Submitted to ApJ, 2 galaxies, too many pages, 8 figures, 2 tables.Spatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies at z~1 from 3D-HST: evidence for rapid inside-out assembly of disk galaxies, , , , , , , , , and 6 other author(s). (2012)cite arxiv:1202.1822 Comment: ApJ Letters, in press. The public 3D-HST website is http://3dhst.research.yale.edu/Home.html.