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Disambiguation of "Bezanson, Rachel"

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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.

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Jeff Bezanson

Elisabeth Rachel

Ziele und Compliance bei Patienten mit Diabetes mellitus Typ 2. TU Dresden, (2009)

Rachel Thomas

Reinhard Rachel

Rachel Marschang

 

Other publications of authors with the same name

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.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.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.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.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.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).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.Galaxy Structure as a Driver of the Star Formation Sequence Slope and Scatter, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1508.04771Comment: Accepted for publication in the Astrophysical Journal Letters.