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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.Where stars form: inside-out growth and coherent star formation from HST Halpha maps of 2676 galaxies across the main sequence at z~1, , , , , , , , , and 10 other author(s). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST Survey, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1301.0320Comment: Accepted for publication in ApJ Letters.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.Observations of environmental quenching in groups in the 11 Gyr since z=2.5: different quenching for central and satellite galaxies, , , , , , , , , and 9 other author(s). (2014)cite arxiv:1401.2984Comment: Submitted to ApJ.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.The Assembly of Milky Way-like Galaxies Since z~2.5, , , , , , , , , and 9 other author(s). (2013)cite arxiv:1304.2391Comment: Submitted to ApJ Letters. 7 pages, 5 figures.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.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.