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Chemical Abundance Patterns and the Early Environment of Dwarf Galaxies, , , and . (2013)cite arxiv:1306.5239Comment: 9 pages, 6 figures, accepted by ApJ.Warm Gas in the Virgo Cluster: I. Distribution of Lya Absorbers, , , , and . (2012)cite arxiv:1204.6316Comment: ApJ resubmitted, 15 pages, 6 figures, 8 tables.Alleviating the scaling problem of cosmological hydrodynamic simulations with HECA., , , , , and . XSEDE, page 9:1-9:4. ACM, (2013)Achieving extreme resolution in numerical cosmology using adaptive mesh refinement: resolving primordial star formation., , and . SC, page 13. ACM, (2001)Warm Gas in and Around Simulated Galaxy Clusters as Probed by Absorption Lines, , and . (2015)cite arxiv:1507.07983Comment: 21 pages, 14 figures.Implications of galaxy buildup for putative IMF variations in massive galaxies, , and . (2016)cite arxiv:1612.05658Comment: 21 pages, 9 figures, 2 tables. Key figures are 3, 6, and 7. Submitted to ApJ.A Survey of High Level Frameworks in Block-Structured Adaptive Mesh Refinement Packages., , , , , , , , , and 4 other author(s). CoRR, (2016)ENZO: An Adaptive Mesh Refinement Code for Astrophysics (Version 2.6)., , , , , , , , , and 45 other author(s). J. Open Source Softw., 4 (42): 1636 (2019)Ram Pressure Stripping of the Large Magellanic Cloud's Disk as a Probe of the Milky Way's Circumgalactic Medium, , , , , and . (2015)cite arxiv:1507.07935Comment: 34 Pages, submitted to ApJ, comments welcomed and appreciated.Exploring cosmology applications on distributed environments., , and . Future Gener. Comput. Syst., 19 (6): 839-847 (2003)