P
Peter Nugent
Researcher at Lawrence Berkeley National Laboratory
Publications - 774
Citations - 102726
Peter Nugent is an academic researcher from Lawrence Berkeley National Laboratory. The author has contributed to research in topics: Supernova & Galaxy. The author has an hindex of 127, co-authored 754 publications receiving 92988 citations. Previous affiliations of Peter Nugent include Liverpool John Moores University & National Autonomous University of Mexico.
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On the afterglow and host galaxy of GRB 021004: A comprehensive study with the Hubble Space Telescope
Johan P. U. Fynbo,Javier Gorosabel,Javier Gorosabel,Alain Smette,Alain Smette,A. S. Fruchter,Jens Hjorth,Kristian Pedersen,Andrew J. Levan,I. Burud,Kailash C. Sahu,Paul Vreeswijk,E. Bergeron,Chryssa Kouveliotou,Nial R. Tanvir,Stephen E. Thorsett,Ralph A. M. J. Wijers,J. M. Castro Cerón,J. M. Castro Cerón,A. J. Castro-Tirado,Peter M. Garnavich,S. T. Holland,S. T. Holland,S. T. Holland,Pall Jakobsson,Palle Møller,Peter Nugent,Elena Pian,James E. Rhoads,B. Thomsen,Darach Watson,S. E. Woosley +31 more
TL;DR: In this paper, the authors used the Hubble Space Telescope (HST) observations of the late-time afterglow and host galaxy of GRB 021004 (z = 2.33).
Metallicity Effects in NLTE Model Atmospheres of Type IA Supernovae
TL;DR: In this article, a grid of photospheric phase atmospheres of Type Ia supernovae (SNe Ia) with metallicities from ten times to one thirtieth the solar metallicity in the C+O layer of the deflagration model, W7, was calculated.
Journal ArticleDOI
Detailed Spectroscopic Analysis of SN 1987A: The Distance to the LMC using the SEAM method
Robert C. Mitchell,E. Baron,David Branch,Peter H. Hauschildt,Peter Nugent,Peter Lundqvist,Sergei Blinnikov,Chun S. J. Pun +7 more
TL;DR: In this article, the authors used a hydrodynamical model to model the observed spectra from day 1 to day 81 using a broad baseline of detailed spectroscopic models and found a distance modulus mu = 18.5 +/- 0.2 using the SEAM method of determining distances to supernovae.
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On the early-time excess emission in hydrogen-poor superluminous supernovae
Paul Vreeswijk,Giorgos Leloudas,Giorgos Leloudas,Avishay Gal-Yam,Annalisa De Cia,Annalisa De Cia,Daniel A. Perley,Daniel A. Perley,Robert M. Quimby,Robert M. Quimby,Roni Waldman,Roni Waldman,Mark Sullivan,Lin Yan,Eran O. Ofek,Christoffer Fremling,Francesco Taddia,Jesper Sollerman,Stefano Valenti,Iair Arcavi,Iair Arcavi,D. Andrew Howell,D. Andrew Howell,Alexei V. Filippenko,S. Bradley Cenko,S. Bradley Cenko,O. Yaron,Mansi M. Kasliwal,Yi Cao,Sagi Ben-Ami,Sagi Ben-Ami,Assaf Horesh,Adam Rubin,Ragnhild Lunnan,Peter Nugent,Peter Nugent,Russ R. Laher,Umaa Rebbapragada,Przemysław Woźniak,Shrinivas R. Kulkarni +39 more
TL;DR: In this article, the authors presented the light curves of the hydrogen-poor superluminous supernovae (SLSNe-I) PTF12dam and iPTF13dcc, discovered by the (intermediate) Palomar Transient Factory.
Journal ArticleDOI
Restframe I-band Hubble diagram for type Ia supernovae up to redshift z~0.5
S. Nobili,S. Nobili,Rahman Amanullah,G. Garavini,G. Garavini,Ariel Goobar,Chris Lidman,Vallery Stanishev,Greg Aldering,P. Antilogus,Pierre Astier,M. S. Burns,A. Conley,A. Conley,S. E. Deustua,Richard S. Ellis,Sebastien Fabbro,V. Fadeyev,Gastón Folatelli,R. Gibbons,G. Goldhaber,G. Goldhaber,Donald E. Groom,I. M. Hook,Dale Andrew Howell,A. G. Kim,R. A. Knop,Peter Nugent,Reynald Pain,Saul Perlmutter,Saul Perlmutter,Robert Quimby,J. Raux,N. Regnault,N. Regnault,Pilar Ruiz-Lapuente,G. Sainton,K. Schahmaneche,E. Smith,A. L. Spadafora,R. C. Thomas,Lifan Wang +41 more
TL;DR: In this article, the authors presented a technique for fitting restframe I-band light curves on a data set of 42 type la supernovae (SNe Ia) and constructed a Hubble diagram with 26 SNe from the subset at 0.01 < z < 0.1.