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Atomic and molecular gas in IllustrisTNG galaxies at low redshift

, , , , , , , , , , , and . (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/.

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HI intensity mapping correlation function from UNIT simulations: BAO and observationally induced anisotropy, , , , , , and . (2021)cite arxiv:2105.10454Comment: Comments welcome; 14 pages, 9 figures.Where do galaxies end? A study of hydrodynamic-simulation galaxies and their integrated properties, , , and . (2014)cite arxiv:1404.4053Comment: Submitted to MNRAS, 18 pages, 16 figures.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/.