A
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
More filters
Journal ArticleDOI
Shock Breakout in Dense Circumstellar Material with Application to PS1-13arp
TL;DR: In this paper, the authors explore the impact of dense CSM interaction on the SBO width and luminosity using both analytic and numerical modeling, where they parameterize the CSM as a steady-state wind.
Journal ArticleDOI
Nebular Halpha emission in SN Ia 2016jae
N. Elias-Rosa,Ping Chen,S. Benetti,Subo Dong,J. L. Prieto,Enrico Cappellaro,J. A. Kollmeier,N. I. Morrell,Anthony L. Piro,M. M. Phillips +9 more
TL;DR: In this article, the authors presented SN 2016jae, which was classified as a Type Ia supernova from a spectrum obtained soon after the discovery and reached a B-band peak of -17.93 +-0.34 mag, followed by a fast luminosity decline with sBV 0.56 +- 0.06 and inferred Dm15(B) of 1.10 mag.
Journal ArticleDOI
Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
Héctor Martínez-Rodríguez,Carles Badenes,Hiroya Yamaguchi,Hiroya Yamaguchi,Eduardo Bravo,Francis Timmes,Francis Timmes,Broxton J. Miles,Dean M. Townsley,Anthony L. Piro,Hideyuki Mori,Hideyuki Mori,Brett H. Andrews,Sangwook Park +13 more
TL;DR: In this paper, a new method was proposed to determine ejecta neutronization using Ca and S lines in the X-ray spectra of Type Ia supernova remnants (SNRs).
Posted Content
The Dynamic X-ray Sky of the Local Universe
Alicia M. Soderberg,Jonathan E. Grindlay,Joshua S. Bloom,Suvi Gezari,Anthony L. Piro,Tomaso Belloni,Jifeng Liu,Ada Paizis,Edo Berger,Paolo De Coppi,Nobu Kawai,Neil Gehrels,Brian D. Metzger,Branden Allen,Didier Barret,Angela Bazzano,Giovanni F. Bignami,P. A. Caraveo,Stephane Corbel,Andrea De Luca,Jeremy J. Drake,Pepi Fabbiano,Mark H. Finger,Marco Feroci,Dieter H. Hartmann,Jaesub Hong,G. Jernigan,Philip Kaaret,Chryssa Kouveliotou,Alexander Kutyrev,Avi Loeb,Giovanni Pareschi,G. K. Skinner,Rosanne Di Stefano,Gianpiero Tagliaferri,Pietro Ubertini,Michiel van der Klis,Colleen A. Wilson-Hodge +37 more
TL;DR: In this article, the authors focus on the transient phase space that is not yet sampled due to the lack of a sensitive, wide-field and triggering facility dedicated exclusively to catching high energy transients and enabling rapid coordinated multi-wavelength follow-up.
Posted Content
Inflation and Dark Energy from spectroscopy at $z > 2$
Simone Ferraro,Michael J. Wilson,Muntazir Abidi,David Alonso,Behzad Ansarinejad,Robert Armstrong,Jacobo Asorey,Arturo Avelino,Carlo Baccigalupi,Kevin Bandura,Nicholas Battaglia,Chetan Bavdhankar,José Luis Bernal,Florian Beutler,Matteo Biagetti,Guillermo A. Blanc,Jonathan Blazek,Adam S. Bolton,Julian Borrill,Brenda Frye,E. Buckley-Geer,Philip Bull,Cliff Burgess,Christian T. Byrnes,Zheng Cai,Francisco J. Castander,Emanuele Castorina,Tzu-Ching Chang,Jonás Chaves-Montero,Shi-Fan Chen,Xingang Chen,Christophe Balland,Christophe Yèche,Joanne Cohn,William R. Coulton,Hélène M. Courtois,Rupert A. C. Croft,Francis-Yan Cyr-Racine,Guido D'Amico,Kyle S. Dawson,Jacques Delabrouille,Arjun Dey,Olivier Doré,Kelly A. Douglass,Duan Yutong,Cora Dvorkin,Alexander Eggemeier,Daniel J. Eisenstein,Xiaohui Fan,Pedro G. Ferreira,Andreu Font-Ribera,Simon Foreman,Juan Garcia-Bellido,Martina Gerbino,Vera Gluscevic,Satya Gontcho A Gontcho,Dan Green,Julien Guy,ChangHoon Hahn,Shaul Hanany,Will Handley,Nimish P. Hathi,Adam J. Hawken,César Hernández-Aguayo,Renée Hložek,Dragan Huterer,Mustapha Ishak,Marc Kamionkowski,Dionysios Karagiannis,Ryan E. Keeley,Robert Kehoe,Rishi Khatri,Alex G. Kim,Jean-Paul Kneib,Juna A. Kollmeier,Ely D. Kovetz,Elisabeth Krause,Alex Krolewski,Benjamin L'Huillier,Martin Landriau,Michael Levi,Michele Liguori,Eric V. Linder,Zarija Lukić,Axel de la Macorra,A. A. Plazas,Jennifer L. Marshall,Paul Martini,Kiyoshi Masui,Patrick McDonald,P. Daniel Meerburg,Joel Meyers,Mehrdad Mirbabayi,John Moustakas,Adam D. Myers,Nathalie Palanque-Delabrouille,Laura Newburgh,Jeffrey A. Newman,Gustavo Niz,Hamsa Padmanabhan,Povilas Palunas,Will J. Percival,F. Piacentini,Matthew M. Pieri,Anthony L. Piro,Abhishek Prakash,Jason Rhodes,Ashley J. Ross,Graziano Rossi,Gwen C. Rudie,Lado Samushia,Misao Sasaki,Emmanuel Schaan,David J. Schlegel,Marcel Schmittfull,Michael Schubnell,Neelima Sehgal,Leonardo Senatore,Hee-Jong Seo,Arman Shafieloo,Huanyuan Shan,Joshua D. Simon,Sara M. Simon,Zachary Slepian,Anže Slosar,Srivatsan Sridhar,Albert Stebbins,Stephanie Escoffier,Eric R. Switzer,Gregory Tarle,Mark Trodden,Cora Uhlemann,L. Arturo Urenña-López,Eleonora Di Valentino,Mariana Vargas-Magaña,Yi Wang,Scott Watson,Martin White,Weishuang Xu,Byeonghee Yu,Gong-Bo Zhao,Yi Zheng,Hong-Ming Zhu +142 more
TL;DR: In this paper, it was shown that a future spectroscopic survey can test the Gaussianity of the initial conditions up to a factor of ~50 better than our current bounds, crossing the crucial theoretical threshold of $sigma(f{NL}^{\rm local})$ of order unity that separates single field and multi-field models.