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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.

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Variations in the slope of the resolved star-forming main sequence: a tool for constraining the mass of star-forming regions, , , , , , , and . (2019)cite arxiv:1912.04290Comment: submitted to MNRAS-Letters.Predictions of the LCII -- SFR and CII Luminosity Function at the Epoch of Reionization, , , , , , , and . (2020)cite arxiv:2004.11912Comment: 17 pages, 13 figures, submitted to the ApJ.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.Galaxy mergers on a moving mesh: a comparison with smoothed-particle hydrodynamics, , , , and . (2013)cite arxiv:1309.2942Comment: Submitted to MNRAS. Animations for all simulations available at http://www.cfa.harvard.edu/itc/research/arepomerger/ . 25 pages, 14 figures. Comments encouraged.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.How stellar feedback simultaneously regulates star formation and drives outflows, and . (2015)cite arxiv:1510.05650Comment: Fig. 5 illustrates the key conclusion. Submitted to MNRAS. Comments welcome.Is a top-heavy initial mass function needed to reproduce the submillimeter galaxy number counts?, , and . (2017)cite arxiv:1705.05377Comment: 6 pages, 3 figures, submitted to ApJL.The stellar masses and specific star-formation rates of submillimetre galaxies, , , , , and . (2011)cite arxiv:1108.6058Comment: Resubmitted to A&A after responding to referee's comments. 12 pages, 4 figures, 2 tables. Comments welcome.The total infrared luminosity may significantly overestimate the star formation rate of recently quenched galaxies, , , , , , , , , and . (2014)cite arxiv:1402.0006Comment: 6 pages, 3 figures. Submitted to MNRAS Letters. Comments encouraged.FIRE-2 Simulations: Physics versus Numerics in Galaxy Formation, , , , , , , , , and 18 other author(s). (2017)cite arxiv:1702.06148Comment: 66 pages, 39 figures. Simulation animations and visualizations available at http://www.tapir.caltech.edu/~phopkins/Site/animations and http://fire.northwestern.edu Paper includes complete FIRE algorithms and public ICs (http://www.tapir.caltech.edu/~phopkins/publicICs).