Yen-Chen Pan

Affiliations: 
NAOJ 
Area:
Astronomy
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"Yen-Chen Pan"
Cross-listing: Physics Tree

Parents

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Mark 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
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