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Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations

, , , , , , , , , and . (2022)cite arxiv:2203.06201Comment: 18 pages, 9 figures. Submitted to MNRAS, comments welcome.

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Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function, , , , and . (2021)cite arxiv:2109.14647Comment: 11 pages, 6 figures, submitted to MNRAS.Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations, , , , , , , , , and . (2022)cite arxiv:2203.06201Comment: 18 pages, 9 figures. Submitted to MNRAS, comments welcome.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/.Local positive feedback in the overall negative: the impact of quasar winds on star formation in the FIRE cosmological simulations, , , , , , , , , and 3 other author(s). (2023)cite arxiv:2301.01784Comment: 17 pages, 12 figures. Accepted for publication in MNRAS.Why do Black Holes Trace Bulges (& Central Surface Densities), Instead of Galaxies as a Whole?, , , , and . (2021)cite arxiv:2103.10444Comment: 8 pages, 3 figures, submitted to MNRAS. Comments welcome.