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Properties of the CGM and IGM: constraints on galaxy formation models from the Sunyaev-Zel'dovich effect, , , , , , , and . (2020)cite arxiv:2007.11583Comment: 14 pages, 6 figures, submitted to MNRAS.Zooming in on accretion - I. The structure of halo gas, , , , , and . (2015)cite arxiv:1503.02665Comment: High-res PDF and simulation movies available at http://www.cfa.harvard.edu/~dnelson/#research (MNRAS submitted, comments welcome).The abundance, distribution, and physical nature of highly ionized oxygen OVI, OVII, and OVIII in IllustrisTNG, , , , , , , , , and 1 other author(s). (2017)cite arxiv:1712.00016Comment: Submitted to MNRAS. For an interactive OVI/OVIII visualization, see the 2D explorer at http://www.tng-project.org.Ultra-high energy cosmic rays deflection by the Intergalactic Magnetic Field, , , , , and . (2021)cite arxiv:2101.07207.Hydrogen Reionization in the Illustris Universe, , , , , , , and . (2015)cite arxiv:1503.00734Comment: 19 pages, 17 figures, submitted to MNRAS, comments are welcome.Atomic and molecular gas in IllustrisTNG galaxies at low redshift, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1902.10714Comment: 22 pages, 11 figures. Comments welcome. Additional figures and link to data at http://www.benediktdiemer.com/data/hi-h2-in-illustris/.The fraction of dark matter within galaxies from the IllustrisTNG simulations, , , , , , , , , and 2 other author(s). (2018)cite arxiv:1801.10170Comment: 27 pages, 14 figures, highlights: Figs. 11, 12, 13. Revised version accepted by MNRAS. Please contact lovell@hi.is with any comments.The CAMELS project: Cosmology and Astrophysics with MachinE Learning Simulations, , , , , , , , , and 11 other author(s). (2020)cite arxiv:2010.00619Comment: 33 pages, 18 figures, CAMELS webpage at https://www.camel-simulations.org.High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies, , , , , , , and . (2021)cite arxiv:2104.12788Comment: 15 pages, 12 figures. To be submitted to MNRAS.The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation, , , , , , , , , and 6 other author(s). (2014)cite arxiv:1411.0667Comment: 11 pages, 9 figures. Submitted to MNRAS, comments welcome. The official Illustris website can be found at http://www.illustris-project.org/.