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Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations

, , , , and . (2016)cite arxiv:1604.07842Comment: 17 pages, 19 figures, 2 tables, submitted to ApJ.

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Late Pop III Star Formation During the Epoch of Reionization: Results from the Renaissance Simulations, , , and . (2016)cite arxiv:1604.03586Comment: 8 pages, 4 figures, 3 tables. Accepted by ApJ.First Light: Exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations, , , , and . (2017)cite arxiv:1701.02749Comment: 17 pages, 13 figures.Cosmology on the Blue Waters Early Science System., , , , , , , , , and . SC Companion, page 1578. IEEE Computer Society, (2012)Tracing the Evolution of High Redshift Galaxies Using Stellar Abundances, , , , and . (2013)cite arxiv:1312.0606Comment: 15 pages, 4 figures, submitted to ApJ.Massive Star Formation in Metal-Enriched Haloes at High Redshift, , , , and . (2020)cite arxiv:2006.14625Comment: 10 pages. Submitted to the Open Journal of Astrophysics. Comments welcome.Visualizing likelihood density functions via optimal region projection., , , , , , and . Comput. Graph., (2014)Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations, , , , and . (2016)cite arxiv:1604.07842Comment: 17 pages, 19 figures, 2 tables, submitted to ApJ.K-Athena: a performance portable structured grid finite volume magnetohydrodynamics code., , and . CoRR, (2019)Towards performance portability in the Spark astrophysical magnetohydrodynamics solver in the Flash-X simulation framework., , , , , and . Parallel Comput., (2021)As A Matter of State: The role of thermodynamics in magnetohydrodynamic turbulence, , and . (2019)cite arxiv:1908.03989Comment: 15 pages, 7 figures, submitted to ApJ, comments are welcome.