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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.An instability of feedback regulated star formation in galactic nuclei, , , , , , and . (2016)cite arxiv:1601.07186Comment: 14 pages; 11 figures; submitted to MNRAS; comments welcome. Animations of the isolated disks presented in this paper can be found at http://www.mit.edu/~ptorrey/media.html#iso_disks.High Angular Momentum Halo Gas: a Feedback and Code-Independent Prediction of LCDM, , , , , , , , , and . (2016)cite arxiv:1606.08542Comment: 13 pages, 8 figures, 1 table; submitted to ApJ.No missing photons for reionization: moderate ionizing photon escape fractions from the FIRE-2 simulations, , , , , and . (2020)cite arxiv:2003.05945Comment: 16 pages, 11 figures, submitted to MNRAS, comments welcome. Core results are shown in Fig 5 and Fig 7.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.Discrete Effects in Stellar Feedback: Individual Supernovae, Hypernovae, and IMF Sampling in Dwarf Galaxies, , , , , , , , and . (2017)cite arxiv:1712.02795Comment: 9 pages, 4 figures.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.