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Significant Dust-Obscured Star Formation in Luminous Lyman-break Galaxies at $z$$\sim$$7$$-$$8$, , , , , , , , , и 6 other автор(ы). (2021)cite arxiv:2105.12133Comment: 21 pages, 12 figures, 2 tables. Submitted to ApJ.Schrodinger's Galaxy Candidate: Puzzlingly Luminous at $z\approx17$, or Dusty/Quenched at $z\approx5$?, , , , , , , , , и 15 other автор(ы). (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 MUSE Hubble Ultra Deep Field Survey: IV. Global properties of C III emitters, , , , , , , , , и 5 other автор(ы). (2017)cite arxiv:1710.06432Comment: 16 pages and 13 figures, accepted for publication in A&A.Measurement of rotation in two galaxies in the Epoch of Reionization from ALMA-detected CII emission, , , , , , , , , и 2 other автор(ы). (2017)cite arxiv:1706.04614Comment: 13 pages, 5 figues, 1 table, submitted.The Lyman-continuum photon production efficiency in the high-redshift Universe, , , , , , и . (2015)cite arxiv:1512.03214Comment: 4 pages, 2 figures, submitted to MNRAS. Comments welcome.MMT Spectroscopy of Lyman-alpha at z$\simeq$7: Evidence for Accelerated Reionization Around Massive Galaxies, , , , , , и . (2020)cite arxiv:2010.03566Comment: 19 pages, 9 figures. Submitted to MNRAS.Inferred H\alpha Flux as a Star-Formation Rate Indicator at z ~ 4-5: Implications for Dust Properties, Burstiness, and the z = 4-8 Star-Formation-Rate Functions, , , , , и . (2015)cite arxiv:1511.08808Comment: 19 pages, 11 figures, 9 tables, submitted to ApJ.The HDUV Survey: A Revised Assessment of the Relationship between UV Slope and Dust Attenuation for High-Redshift Galaxies, , , , , , , , , и 6 other автор(ы). (2017)cite arxiv:1705.09302Comment: 22 pages, 3 tables, 11 figures, submitted to the Astrophysical Journal.The Evolution of Mass-size Relation for Lyman Break Galaxies From z=1 to z=7, , , , , , , , и . (2012)cite arxiv:1207.6634Comment: Accepted for publication in The Astrophysical Journal Letters.