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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.
Papers
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Journal ArticleDOI
Implications from ASKAP Fast Radio Burst Statistics
Wenbin Lu,Anthony L. Piro +1 more
TL;DR: In this article, a simplified model of a power-law volumetric rate per unit isotropic energy dN/dE ∝ E^(−γ) with a maximum energy E_(max) in a uniform Euclidean universe was proposed to study the fluence and dispersion measure (DM) distributions of the ASKAP sample.
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Connecting the progenitors, pre-explosion variability and giant outbursts of luminous blue variables with Gaia16cfr
Charles D. Kilpatrick,Ryan J. Foley,Maria R. Drout,Yen-Chen Pan,Fiona H. Panther,David A. Coulter,Alexei V. Filippenko,G. Howard Marion,Anthony L. Piro,Armin Rest,Ivo R. Seitenzahl,Ivo R. Seitenzahl,G. Strampelli,Xi E. Wang +13 more
TL;DR: The work of AVF was conducted in part at the Aspen Center for Physics, which was supported by NSF grant PHY-1607611; the author thanks the======Center for its hospitality during the neutron stars workshop in 2017======June and July as discussed by the authors.
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Transient X-Ray Binaries in Elliptical Galaxies
Anthony L. Piro,Lars Bildsten +1 more
TL;DR: In this article, Chandra observations of elliptical galaxies have revealed large numbers of low-mass X-ray binaries (LMXBs) accreting at rates greater than 10-9 M☉ yr-1.
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Neutronization during carbon simmering in type ia supernova progenitors
TL;DR: In this article, the authors used the MESA stellar evolution code to examine the production of neutron-rich isotopes in a Type Ia supernova (SN Ia) progenitor.
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Updated parameter estimates for GW190425 using astrophysical arguments and implications for the electromagnetic counterpart
Ryan J. Foley,David A. Coulter,Charles D. Kilpatrick,Anthony L. Piro,Enrico Ramirez-Ruiz,Enrico Ramirez-Ruiz,Josiah Schwab +6 more
TL;DR: In this paper, the authors explore the expected electromagnetic signatures of the progenitor system of the compact binary merger GW190425 and make several astrophysically motivated assumptions to further constrain the parameters of the system.