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Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z=3.35: A Detailed Look at an Early Progenitor of Local Most Massive Ellipticals

, , , , , , , , , and . (2014)cite arxiv:1406.0002Comment: 15 pages, 7 figures. Submitted to ApJ. Comments welcome.

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Evidence for Widespread AGN Activity among Massive Quiescent Galaxies at z ~ 2, , , and . (2012)cite arxiv:1212.1158Comment: 9 pages, 3 figures, 3 tables; Accepted for publication in ApJ.Discovery of Massive, Mostly Star-formation Quenched Galaxies with Extremely Large Lyman-alpha Equivalent Widths at z ~ 3, , , , , , , , , and 14 other author(s). (2015)cite arxiv:1507.04439Comment: Accepted for publication in ApJ Letters on 15th July, 2015. 6 pages including 3 figures and 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.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.SImulator of GAlaxy Millimeter/submillimeter Emission (SIGAME): CO emission from massive z=2 main sequence galaxies, , , , , , and . (2015)cite arxiv:1507.00012Comment: 29 pages, 19 figures; submitted to MNRAS; Comments welcome.SILVERRUSH. VIII. Spectroscopic Identifications of Early Large Scale Structures with Protoclusters Over 200 Mpc at z~6-7: Strong Associations of Dusty Star-Forming Galaxies, , , , , , , , , and 25 other author(s). (2019)cite arxiv:1902.09555Comment: 17 pages, 11 figures, Accepted for Publication in ApJ.X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at $z\gtrsim2$, , , , , , , , , and 16 other author(s). (2019)cite arxiv:1912.01619Comment: 30 pages, 10 figures, accepted in ApJ.Spectroscopic Confirmation of an Ultra Massive and Compact Galaxy at z=3.35: A Detailed Look at an Early Progenitor of Local Most Massive Ellipticals, , , , , , , , , and . (2014)cite arxiv:1406.0002Comment: 15 pages, 7 figures. Submitted to ApJ. Comments welcome.Rubin-Euclid Derived Data Products: Initial Recommendations, , , , , , , , , and 110 other author(s). (2022)cite arxiv:2201.03862Comment: Report of the Rubin-Euclid Derived Data Products Working Group, 78 pages, 11 figures.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.