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Disambiguation of "Hayward, Christopher C."

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Chaotic and Clumpy Galaxy Formation in an Extremely Massive Reionization-Era Halo

, , , , , , , , , , , , , , , , , , , , , , and . (2022)cite arxiv:2203.14972Comment: Accepted for publication in ApJ Letters, 9 pages, 5 figures. Interactive versions of Fig. 2 and data products are available at https://github.com/spt-smg/publicdata.

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Christopher C Strelioff

Peter Hayward

Sandra Scott-Hayward

Christopher Christopher

Guido C C Clinckspoor

 

Other publications of authors with the same name

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.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.An ALMA survey of submillimeter galaxies in the COSMOS field: Multiwavelength counterparts and redshift, , , , , , , , , and 22 other author(s). (2017)cite arxiv:1708.05748Comment: Submitted to Astronomy & Astrophysics for review 17 pages in body + 26 in appendices.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.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.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.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).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.