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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.

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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).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.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.A Predicted Correlation Between Age Gradient and Star Formation History in FIRE Dwarf Galaxies, , , , , , , , , and 2 other author(s). (2019)cite arxiv:1901.05487Comment: 13 pages, 8 figures. Submitted to MNRAS, comments welcome.Evidence for a Vast Prograde Stellar Stream in the Solar Vicinity, , , , , , , , and . (2019)cite arxiv:1907.07190Comment: 7+2 pages, 4+3 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.The Astropy Problem, , , , , , , , , and 144 other author(s). eprint arXiv:astro-ph.IM/1610.03159, (October 2016)How To Model Supernovae in Simulations of Star and Galaxy Formation, , , , , , , , and . (2017)cite arxiv:1707.07010Comment: 16 pages, 9 figures (+8 pages, 5 figures in appendices). Submitted to MNRAS.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.