Author of the publication

The AGORA High-Resolution Galaxy Simulations Comparison Project. II: Isolated Disk Test

, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2016)cite arxiv:1610.03066Comment: 28 pages, 35 figures, Submitted for publication in the Astrophysical Journal, Image resolution greatly reduced, High-resolution version of this article is available at http://www.slac.stanford.edu/~mornkr/agora/AGORA_Paper4_draft.pdf, The first paper of the AGORA Initiative is at http://adsabs.harvard.edu/abs/2014ApJS..210...14K, More information on AGORA is at http://www.AGORAsimulations.org/.

Please choose a person to relate this publication to

To differ between persons with the same name, the academic degree and the title of an important publication will be displayed. You can also use the button next to the name to display some publications already assigned to the person.

 

Other publications of authors with the same name

The AGORA High-Resolution Galaxy Simulations Comparison Project. II: Isolated Disk Test, , , , , , , , , and 34 other author(s). (2016)cite arxiv:1610.03066Comment: 28 pages, 35 figures, Submitted for publication in the Astrophysical Journal, Image resolution greatly reduced, High-resolution version of this article is available at http://www.slac.stanford.edu/~mornkr/agora/AGORA_Paper4_draft.pdf, The first paper of the AGORA Initiative is at http://adsabs.harvard.edu/abs/2014ApJS..210...14K, More information on AGORA is at http://www.AGORAsimulations.org/.3D Distribution Map of HI Gas and Galaxies Around an Enormous Ly$\alpha$ Nebula and Three QSOs at $z=2.3$ Revealed by the HI Tomographic Mapping Technique, , , , , , , , , and 15 other author(s). (2019)cite arxiv:1910.02962Comment: 14 pages, 7 figures, submitted to ApJ.Alleviating the scaling problem of cosmological hydrodynamic simulations with HECA., , , , , and . XSEDE, page 9:1-9:4. ACM, (2013)Steep Faint-end Slopes of Galaxy Mass and Luminosity Functions at z >=6 in Cosmological SPH Simulations, , and . (2011)cite arxiv:1104.2345 Comment: 14 pages, 5 tables, 12 figures. Submitted.Direct Collapse to Supermassive Black Hole Seeds: Comparing the AMR and SPH Approaches, , and . (2015)cite arxiv:1512.03822Comment: 18 pages, 14 figures, Submitted to MNRAS.Reconstructing HI power spectrum with minimal parameters using the dark matter distribution beyond halos, , , and . (2020)cite arxiv:2011.13165Comment: 11 pages, 9 figures, Submitted to MNRAS.Supermassive Black Hole Seed Formation at High Redshifts: Long-Term Evolution of the Direct Collapse, , , and . (2015)cite arxiv:1508.05098Comment: 13 pages, 11 figures, submitted to MNRAS.Gas clump formation via thermal instability in high-redshift dwarf galaxy mergers, , and . (2017)cite arxiv:1710.11503Comment: 11 pages, 11 figures.The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields, , , , , , and . (2020)cite arxiv:2012.06795Comment: Submitted to ApJ. Comments welcome.Effect of radiative transfer on damped Lyman-alpha and Lyman limit systems in cosmological SPH simulations, , and . (2011)cite arxiv:1112.5691Comment: 18 pages, 16 figures, submitted to MNRAS.