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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.

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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.Cosmology of the Early Universe Viewed Through the New Infrastructure., and . Commun. ACM, 40 (11): 84-94 (1997)SeedMe: A scientific data sharing and collaboration platform., , , , and . XSEDE, page 48:1-48:6. ACM, (2016)Self-consistent solution of cosmological radiation-hydrodynamics and chemical ionization., , , and . J. Comput. Phys., 228 (18): 6833-6854 (2009)Achieving extreme resolution in numerical cosmology using adaptive mesh refinement: resolving primordial star formation., , and . Sci. Program., 10 (4): 291-302 (2002)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.Accelerating data-intensive science with Gordon and Dash., and . TG, page 14:1-14:7. ACM, (2010)Gateways to Discovery: Cyberinfrastructure for the Long Tail of Science., , , , , , , , , and 3 other author(s). XSEDE, page 39:1-39:8. ACM, (2014)Using Gordon to accelerate LHC science., , , , , , , , , and 2 other author(s). XSEDE, page 59:1-59:4. ACM, (2013)Galaxies Collide On the I-Way: an Example of Heterogeneous Wide-Area Collaborative Supercomputing., , , , , , , , , and 1 other author(s). Int. J. High Perform. Comput. Appl., 10 (2-3): 132-144 (1996)