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The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4

, , , , and . (2016)cite arxiv:1606.05352Comment: 16 pages, 12 Figures.

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A Moving Mesh Hydrodynamic Solver for ChaNGa, , and . (2017)cite arxiv:1707.05333Comment: 15 pages, 7 figures, accepted to MNRAS.The origin of metals in the circum-galactic medium of massive galaxies at z=3, , , , , and . (2011)cite arxiv:1109.3713 Comment: 13 pages, 16 figures. Submitted to ApJ.Low shear diffusion central schemes for particle methods., , and . J. Comput. Phys., (2020)A lower fragmentation mass scale for clumps in high redshift galaxies: a systematic numerical study, , , and . (2014)cite arxiv:1412.3319Comment: 22 pages, 21 figures and two tables. Submitted to MNRAS. Comments welcome.The Little Galaxies that Could (Reionize the Universe): Predicting Faint End Slopes & Escape Fractions at z > 4, , , , and . (2016)cite arxiv:1606.05352Comment: 16 pages, 12 Figures.What is a GMC? Are Observers and Simulators Discussing the Same Star-forming Clouds?, , , , , , and . (Aug 7, 2015)Implementing Molecular Hydrogen in Hydrodynamic Simulations of Galaxy Formation, , , , , and . (2012)cite arxiv:1205.5567Comment: 20 pages, 15 figures, resubmitted to MNRAS following referee report.Giant Molecular Cloud Formation in Disk Galaxies: Characterizing Simulated versus Observed Cloud Catalogues, , , and . (2013)cite arxiv:1308.0339Comment: 13 pages, 11 figures, 1 table; Accepted for publication in ApJ.MaGICC-WDM: The effects of Warm Dark Matter in hydrodynamical simulations of disc galaxy formation, , , , , , and . (2013)cite arxiv:1308.1088Comment: 14 pages, 9 figures, 2 tables; submitted to MNRAS.Dark MaGICC: the effect of Dark Energy on galaxy formation. Cosmology does matter, , , , and . (2014)cite arxiv:1401.3338Comment: 11 pages, 13 figures.