Parents
Sign in to add mentorMark Sullivan | grad student | Oxford (Physics Tree) | |
Ryan J. Foley | post-doc | 2014-2018 | UC Santa Cruz (Physics Tree) |
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Publications
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Ho AYQ, Perley DA, Chen P, et al. (2023) Minutes-duration optical flares with supernova luminosities. Nature |
Pan Y. (2020) High-Velocity Type Ia Supernova Has a Unique Host Environment The Astrophysical Journal. 895 |
Moriya TJ, Suzuki A, Takiwaki T, et al. (2020) Systematic investigation of the effect of 56Ni mixing in the early photospheric velocity evolution of stripped-envelope supernovae Monthly Notices of the Royal Astronomical Society. 497: 1619-1626 |
Moriya TJ, Tanaka M, Morokuma T, et al. (2019) HSC16aayt: A Slowly Evolving Interacting Transient Rising for More than 100 Days The Astrophysical Journal. 882: 70 |
Kilpatrick CD, Foley RJ, Drout MR, et al. (2018) Connecting the progenitors, pre-explosion variability and giant outbursts of luminous blue variables with Gaia16cfr Monthly Notices of the Royal Astronomical Society. 473: 4805-4823 |
Drout MR, Piro AL, Shappee BJ, et al. (2017) Light curves of the neutron star merger GW170817/SSS17a: Implications for r-process nucleosynthesis. Science (New York, N.Y.) |
Shappee BJ, Simon JD, Drout MR, et al. (2017) Early spectra of the gravitational wave source GW170817: Evolution of a neutron star merger. Science (New York, N.Y.) |
Kilpatrick CD, Foley RJ, Kasen D, et al. (2017) Electromagnetic evidence that SSS17a is the result of a binary neutron star merger. Science (New York, N.Y.) |
Coulter DA, Foley RJ, Kilpatrick CD, et al. (2017) Swope Supernova Survey 2017a (SSS17a), the optical counterpart to a gravitational wave source. Science (New York, N.Y.) |
Arcavi I, Gal-Yam A, Sullivan M, et al. (2014) A continuum of H- to He-rich tidal disruption candidates with a preference for E+A galaxies Astrophysical Journal. 793 |