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Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?

, , , , , , , , , , , , , , , , , , , , , , , , and . (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.

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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.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.A Machine Learning Approach to Predict Missing Flux Densities in Multi-band Galaxy Surveys, , , , , , , , , and 14 other author(s). (2022)cite arxiv:2208.14781Comment: 15 pages, 14 figures, accepted for publication in ApJ.