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What is the Maximum Mass of a Population III Galaxy?

, , and . (2017)cite arxiv:1701.00814Comment: 9 pages, 7 figures, submitted to MNRAS.

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Self-consistent Semi-analytic Modeling of Feedback During Primordial Star Formation and Reionization, , and . (2020)cite arxiv:2001.11118Comment: 16 pages, 7 figures, to be submitted to ApJ.Does disk fragmentation prevent the formation of supermassive stars in protogalaxies?, and . (Jun 19, 2014)Rapid Formation of Massive Black Holes in close proximity to Embryonic Proto-Galaxies, , , , , and . (2017)cite arxiv:1703.03805Comment: Published in Nature Astronomy, March 13th 2017.MassiveNuS: Cosmological Massive Neutrino Simulations, , , , , , , and . (2017)cite arxiv:1711.10524Comment: 25 pages, 9 figures, submitted to JCAP. Data available at http://columbialensing.org.Evolution in the Escape Fraction of Ionizing Photons and the Decline in Strong Lya Emission from z>6 Galaxies, , , , and . (2014)cite arxiv:1401.7676Comment: 9 pages, 3 figures. Resubmitted to MNRAS following revision based on referee report.Low density, radiatively inefficient rotating-accretion flow onto a black hole, , , and . (Sep 21, 2017)Non-Gaussian information from weak lensing data via deep learning., , , and . CoRR, (2018)The Migration of Gap-Opening Planets is not Locked to Viscous Disk Evolution, , , , and . (2014)cite arxiv:1405.3711Comment: ApJ Accepted.Hyper-Eddington accretion flows onto massive black holes, , and . (2015)cite arxiv:1511.02116Comment: 21 pages, 14 figures, submitted to MNRAS.Ly\alpha\ emission line reconstruction for high-$z$ QSOs, , , , and . (2016)cite arxiv:1605.09388Comment: 24 pages, 16 figures, 1 table. Submitted to MNRAS.