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The high A_V Quasar Survey: A z=2.027 metal-rich damped Lyman-alpha absorber towards a red quasar at z=3.21

, , , , , , , , and . (2017)cite arxiv:1706.07016Comment: 7 pages, 4 figures. Accepted for publication in A&A.

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Chronicling the Host Galaxy Properties of the Remarkable Repeating FRB 20201124A, , , , , , , , , and 10 other author(s). (2021)cite arxiv:2106.11993Comment: 18 pages, 5 figures, 3 tables; Submitted.The high A_V Quasar Survey: A z=2.027 metal-rich damped Lyman-alpha absorber towards a red quasar at z=3.21, , , , , , , , and . (2017)cite arxiv:1706.07016Comment: 7 pages, 4 figures. Accepted for publication in A&A.Measuring the HI content of individual galaxies out to the epoch of reionization with CII, , , , and . (2021)cite arxiv:2108.13442Comment: Accepted for publication in ApJ.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.