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The Origin and Evolution of Lyman-alpha Blobs in Cosmological Galaxy Formation Simulations

, , , , , , , , , and . (2020)cite arxiv:2004.08397Comment: Submitted to ApJ; comments welcome. 23 pages, 21 figures.

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The Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations, , , , , and . (2016)cite arxiv:1610.08523Comment: 22 pages, 17 figures, Submitted to MNRAS.Star(bursts) of FIRE: observational signatures of bursty star formation in galaxies, , , , , , and . (2015)cite arxiv:1510.03869Comment: 21 pages, 15 figures, submitted to MNRAS.When Feedback Fails: The Scaling and Saturation of Star Formation Efficiency, , , , , and . (2016)cite arxiv:1612.05635Comment: Submitted to MNRAS; 16 pages, 6 figures.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.On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium, , , , , , , and . (2017)cite arxiv:1704.08254Comment: Submitted to MNRAS. Comments welcome.What FIREs Up Star Formation: the Emergence of the Kennicutt-Schmidt Law from Feedback, , , , , , , , and . (2017)cite arxiv:1701.01788Comment: 15 pages, 10 figures, submitted to MNRAS.Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes, , , , , , , , , and . (2017)cite arxiv:1710.00008Comment: 11 pages, 9 figures, submitted to MNRAS, comments welcome.The MOSDEF Survey: Broad Emission Lines at z=1.4-3.8, , , , , , , , , and 5 other author(s). (2017)cite arxiv:1710.03230.Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies, , , , , , , , and . (2017)cite arxiv:1712.02795Comment: 9 pages, 4 figures.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.