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A massive, quiescent galaxy at redshift of z=3.717

, , , , , , , , , , and . (2017)cite arxiv:1702.01751Comment: Accepted for publication in Nature. (Note press embargoed until publication date which is TBD).
DOI: 10.1038/nature21680

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ZFIRE: Similar Stellar Growth in H$\alpha$-emitting Cluster and Field Galaxies at z~2, , , , , , , , , and 6 other author(s). (2016)cite arxiv:1612.01534Comment: ApJ in press; full version of Table 1 available from ApJ and upon request. Survey websites are http://zfire.swinburne.edu.au and http://zfourge.tamu.edu.A substantial population of massive quiescent galaxies at z~4 from ZFOURGE, , , , , , , , , and 14 other author(s). (2013)cite arxiv:1312.4952Comment: 8 pages, 4 figures, 1 table, re-submitted to ApjL after second referee report.The Size Evolution of Star-forming Galaxies Since z~7 Using ZFOURGE, , , , , , , , , and 3 other author(s). (2016)cite arxiv:1612.05262Comment: 7 pages, 4 figures, accepted to Apj letters.Discovery of Extreme OIII+H$\beta$ Emitting Galaxies Tracing an Overdensity at z~3.5 in CDF-South, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1703.03814Comment: Accepted for publication in ApJL. 8 pages, 4 figures.The distribution of satellites around massive galaxies at 1<z<3 in ZFOURGE/CANDELS: dependence on star formation activity, , , , , , , , , and 16 other author(s). (2014)cite arxiv:1406.6056Comment: 19 pages, 17 figures, Resubmitted to ApJ after responding to referee report. Information on ZFOURGE can be found at http://zfourge.tamu.edu.A massive, quiescent galaxy at redshift of z=3.717, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1702.01751Comment: Accepted for publication in Nature. (Note press embargoed until publication date which is TBD).Satellite Quenching and Galactic Conformity at 0.3 < z < 2.5, , , , , , , , , and 14 other author(s). (2015)cite arxiv:1511.02862Comment: Submitted to ApJ after first round of referee comments, 22 pages, 12 figures.ZFIRE: Galaxy Cluster Kinematics, H$\alpha$ Star Formation Rates, and Gas-Phase Metallicities of XMM-LSS J02182-05102 at z=1.6233, , , , , , , , , and 4 other author(s). (2015)cite arxiv:1508.03057Comment: Accepted for publication by ApJ. Survey website is zfire.swinburne.edu.au.Effect of local environment and stellar mass on galaxy quenching and morphology at $0.5<z<2.0$, , , , , , , , , and 13 other author(s). (2017)cite arxiv:1706.03780Comment: 29 pages, 15 figure, submitted to ApJ.The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package, , , , , , , , , and 126 other author(s). (2022)cite arxiv:2206.14220Comment: 43 pages, 5 figures. To appear in ApJ. The author list has two parts: the authors that made significant contributions to the writing and/or coordination of the paper, followed by maintainers of and contributors to the Astropy Project. The position in the author list does not correspond to contributions to the Astropy Project as a whole.