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Anthony L. Piro
Researcher at Carnegie Institution for Science
Publications - 298
Citations - 14937
Anthony L. Piro is an academic researcher from Carnegie Institution for Science. The author has contributed to research in topics: Supernova & White dwarf. The author has an hindex of 62, co-authored 268 publications receiving 12532 citations. Previous affiliations of Anthony L. Piro include California Institute of Technology & Carnegie Learning.
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Journal ArticleDOI
Magnetorotational Core-Collapse Supernovae in Three Dimensions
Philipp Mösta,Sherwood Richers,Christian D. Ott,Christian D. Ott,Roland Haas,Anthony L. Piro,Kristen Boydstun,Ernazar Abdikamalov,Christian Reisswig,Erik Schnetter,Erik Schnetter,Erik Schnetter +11 more
TL;DR: The 3D dynamics of magnetorotational core-collapse supernovae are fundamentally different from what was anticipated on the basis of previous simulations in axisymmetry (2D).
Journal ArticleDOI
A significantly off-centre 56Ni distribution for the low-luminosity type Ia supernova SN 2016brx from the 100IAS survey
Subo Dong,Boaz Katz,Juna A. Kollmeier,Doron Kushnir,Nancy Elias-Rosa,Subhash Bose,Nidia Morrell,J. L. Prieto,J. L. Prieto,Ping Chen,Christopher S. Kochanek,G M Brandt,T W-S Holoien,Avishay Gal-Yam,A. Morales-Garoffolo,Stuart Parker,Mark M. Phillips,Anthony L. Piro,B. J. Shappee,Joshua D. Simon,K. Z. Stanek +20 more
TL;DR: In this paper, the authors present nebular-phase spectra of the Type Ia supernova 2016brx, a member of the 1991bg-like subclass that lies at the faint end of the SN Ia luminosity function.
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Nebular Spectroscopy of Kepler’s Brightest Supernova
Georgios Dimitriadis,César Rojas-Bravo,Charles D. Kilpatrick,Ryan J. Foley,Anthony L. Piro,J. S. Brown,Puragra Guhathakurta,Amanda C. N. Quirk,Armin Rest,Armin Rest,G. Strampelli,G. Strampelli,Brad E. Tucker,A. Villar +13 more
TL;DR: In this paper, the authors present late-time optical photometry and nebular (+236 and +264 days) spectroscopy of SN 2018oh, the brightest Type Ia supernova (SN Ia) observed by the Kepler telescope.
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The Rise and Fall of ASASSN-18pg: Following a TDE from Early To Late Times.
Thomas W.-S. Holoien,Katie Auchettl,Michael A. Tucker,Benjamin J. Shappee,Shannon G. Patel,James Miller-Jones,Brenna Mockler,Danièl N. Groenewald,J. S. Brown,Christopher S. Kochanek,K. Z. Stanek,Ping Chen,Subo Dong,J. L. Prieto,Todd A. Thompson,Rachael L. Beaton,Thomas Connor,Philip S. Cowperthwaite,Linnea Dahmen,K. Decker French,Nidia Morrell,David A. H. Buckley,Mariusz Gromadzki,Rupak Roy,David A. Coulter,Georgios Dimitriadis,Ryan J. Foley,Charles D. Kilpatrick,Anthony L. Piro,César Rojas-Bravo,Matthew R. Siebert,Sjoert van Velzen +31 more
TL;DR: In this article, the authors present nearly 500 days of observations of the tidal disruption event ASASSN-18pg, spanning from 54 days before peak light to 441 days after peak light, including X-ray, UV and optical photometry, optical spectroscopy, radio observations, and the first published spectropolarimetric observations of a TDE.
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What if the Fast Radio Bursts 110220 and 140514 Are from the Same Source
TL;DR: In this article, the authors consider the hypothesis that two fast radio bursts are from the same neutron star embedded within a supernova remnant (SNR) that provides an evolving dispersion measure as the ejecta expands and becomes more diffuse.