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When Feedback Fails: The Scaling and Saturation of Star Formation Efficiency

, , , , , and . (2016)cite arxiv:1612.05635Comment: Submitted to MNRAS; 16 pages, 6 figures.

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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.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.The Cosmic Ultraviolet Baryon Survey (CUBS) -- III. Physical properties and elemental abundances of Lyman limit systems at $z<1$, , , , , , , , , and 11 other author(s). (2021)cite arxiv:2106.04608Comment: Accepted for publication in MNRAS after a minor revision. 18 pages, 11 figures, and a nine-page Appendix with four additional figures.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 contribution of globular clusters to cosmic reionization, , , , and . (2020)cite arxiv:2006.10065Comment: 10 pages, 7 figures, comments welcome, key results in Table 3 and Figure 3.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.When the Jeans don't fit: How stellar feedback drives stellar kinematics and complicates dynamical modeling in low-mass galaxies, , , , , , , and . (2016)cite arxiv:1610.04232Comment: Submitted to ApJ. Main results in Figures 3, 7, and 8.When Feedback Fails: The Scaling and Saturation of Star Formation Efficiency, , , , , and . (2016)cite arxiv:1612.05635Comment: Submitted to MNRAS; 16 pages, 6 figures.