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Lyman-alpha and CIII Emission in z=7-9 Galaxies: Accelerated Reionization Around Luminous Star Forming Systems?, , , , , , , , , and 2 other author(s). (2016)cite arxiv:1606.01304Comment: Submitted to MNRAS, 13 pages, 8 figures.Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-alpha emitters, , , , , , , , , and 9 other author(s). (2020)cite arxiv:2002.11117Comment: 12 Pages, 6 Figures; Accepted for publication in MNRAS.A highly magnified candidate for a young galaxy seen when the Universe was 500 Myrs old, , , , , , , , , and 26 other author(s). (2012)cite arxiv:1204.2305Comment: Submitted to the Nature Journal. 39 Pages, 13 figures.The MUSE-Wide survey: A measurement of the Ly$\alpha$ emitting fraction among $z>3$ galaxies, , , , , , , , , and 8 other author(s). (2017)cite arxiv:1709.00991Comment: 10 pages, 5 figures.The MUSE Hubble Ultra Deep Field Survey: I. Survey description, data reduction and source detection, , , , , , , , , and 17 other author(s). (2017)cite arxiv:1710.03002Comment: 21 pages.ALMA Spectroscopic Survey in the Hubble Ultra Deep Field: The Infrared Excess of UV-selected z=2-10 galaxies as a function of UV-continuum Slope and Stellar Mass, , , , , , , , , and 18 other author(s). (2016)cite arxiv:1606.05280Comment: 31 pages, 16 figures, 13 tables, incorporating the first feedback from the referee on our submitted ApJ manuscript, paper VI of the ASPECS (ALMA Spectroscopic Survey in the Hubble Ultra Deep Field) series.ALMA spectroscopic survey in the Hubble Ultra Deep Field: CO luminosity functions and the evolution of the cosmic density of molecular gas, , , , , , , , , and 30 other author(s). (2016)cite arxiv:1607.06770Comment: Submitted to the Astrophysical Journal, incorporating the first round of referee comments.Lyman-alpha Emission from a Luminous z=8.68 Galaxy: Implications for Galaxies as Tracers of Cosmic Reionization, , , , , , , , and . (2015)cite arxiv:1507.02679Comment: ApJL Submitted; 6 pages, 4 figures, 1 table.Not In Our Backyard: Spectroscopic Support for the CLASH z=11 Candidate MACS0647-JD, , , , , , , , , and 5 other author(s). (2015)cite arxiv:1502.05681Comment: 14 Pages. 6 Figures. 2nd revised version. To appear in ApJ. Please contact npirzkal@stsci.edu for comments on this paper.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.