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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Journal ArticleDOI
Spectroscopic confirmation of high-redshift supernovae with the ESO VLT
Chris Lidman,D. A. Howell,D. A. Howell,Gastón Folatelli,G. Garavini,G. Garavini,S. Nobili,S. Nobili,Greg Aldering,Rahman Amanullah,P. Antilogus,Pierre Astier,Guillermo A. Blanc,M. S. Burns,Alex Conley,Alex Conley,S. E. Deustua,Mamoru Doi,Richard S. Ellis,Sebastien Fabbro,Vitaliy Fadeyev,R. Gibbons,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,I. M. Hook,Nobunari Kashikawa,A. G. Kim,R. A. Knop,Brian C. Lee,Javier Méndez,Tomoki Morokuma,Kentaro Motohara,Peter Nugent,Reynald Pain,Saul Perlmutter,Saul Perlmutter,V. Prasad,Robert Quimby,J. Raux,Nicolas Regnault,Nicolas Regnault,Pilar Ruiz-Lapuente,G. Sainton,Bradley E. Schaefer,K. Schahmaneche,Eric P. Smith,A. L. Spadafora,Vallery Stanishev,Nicholas A. Walton,Lifan Wang,W. M. Wood-Vasey,W. M. Wood-Vasey,Naoki Yasuda +54 more
TL;DR: In this article, the authors presented VLT FORS1 and FORS2 spectra of 39 candidate high-redshift supernovae that were discovered as part of a cosmological study using type Ia supernova (SNe Ia) over a wide range of redshifts.
Journal ArticleDOI
On the Afterglow and Host Galaxy of GRB021004: A Comprehensive Study with the Hubble Space Telescope
J. P. U. Fynbo,J. Gorosabel,Alain Smette,A. S. Fruchter,Jens Hjorth,K. Pedersen,A. J. Levan,I. Burud,Kailash C. Sahu,P. M. Vreeswijk,E. Bergeron,Chryssa Kouveliotou,Nial Tanvir,Stephen E. Thorsett,R. A. M. J. Wijers,J. M. Castro Cerón,A. J. Castro-Tirado,P. M. Garnavich,S. T. Holland,P. Jakobsson,Palle Møller,Peter Nugent,Elena Pian,James E. Rhoads,B. Thomsen,Dan M. Watson,S. E. Woosley +26 more
TL;DR: In this article, the authors report on HST observations of the late-time afterglow and host galaxy of GRB021004 (z=2.33) and find that the afterglog evolved achromatically within the errors.
Journal ArticleDOI
Type Ia supernova spectral features in the context of their host galaxy properties
Yen-Chen Pan,Yen-Chen Pan,Mark Sullivan,Kate Maguire,Avishay Gal-Yam,Isobel Hook,D. A. Howell,Peter Nugent,Paolo A. Mazzali +8 more
TL;DR: In this article, spectroscopic measurements of 122 Type Ia supernovae (SNe Ia) with z 3 x 10(9) M-circle dot were analyzed, and it was shown that these highest velocity SNE Ia explode in the inner regions of their host galaxies, similar to the study of Wang et al.
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Evidence for Late-stage Eruptive Mass Loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient
Anna Y. Q. Ho,Daniel A. Goldstein,Steve Schulze,David K. Khatami,Daniel A. Perley,Mattias Ergon,Avishay Gal-Yam,Alessandra Corsi,Igor Andreoni,Cristina Barbarino,Eric C. Bellm,N. Blagorodnova,Joe Bright,Eric Burns,S. Bradley Cenko,S. Bradley Cenko,Virginia Cunningham,Kaushik De,Richard Dekany,Alison Dugas,Rob Fender,Claes Fransson,Christoffer Fremling,Adam Goldstein,Matthew J. Graham,David Hale,Assaf Horesh,Tiara Hung,Mansi M. Kasliwal,N. Paul M. Kuin,Shrinivas R. Kulkarni,Thomas Kupfer,Ragnhild Lunnan,Frank J. Masci,Chow-Choong Ngeow,Peter Nugent,Eran O. Ofek,Maria T. Patterson,Glen Petitpas,Ben Rusholme,Hanna Sai,Itai Sfaradi,David L. Shupe,Jesper Sollerman,Maayane T. Soumagnac,Yutaro Tachibana,Francesco Taddia,Richard Walters,Xiaofeng Wang,Yuhan Yao,X. Zhang +50 more
TL;DR: Ho et al. as discussed by the authors presented detailed observations of ZTF18abukavn (SN2018gep), which was discovered in high-cadence data from the Zwicky Transient Facility as a rapidly rising (1.4 ± 0.1 mag hr-1) and luminous (Mg, peak = -20 mag) transient.
Journal ArticleDOI
GROWTH on S190426c: Real-time Search for a Counterpart to the Probable Neutron Star–Black Hole Merger using an Automated Difference Imaging Pipeline for DECam
Daniel A. Goldstein,Igor Andreoni,Peter Nugent,Peter Nugent,Mansi M. Kasliwal,Michael W. Coughlin,Shreya Anand,Joshua S. Bloom,Joshua S. Bloom,Jorge Martínez-Palomera,Keming Zhang,Tomas Ahumada,Ashot Bagdasaryan,Jeff Cooke,Kaushik De,Dmitry A. Duev,U. Christoffer Fremling,Pradip Gatkine,Matthew J. Graham,Eran O. Ofek,Leo Singer,Lin Yan +21 more
TL;DR: Goldstein et al. as discussed by the authors used the DECam observations of S190426c, the first possible NS-black hole merger detected in GWs, as part of the multi-facility follow-up by the Global Relay of Observatories Watching Transients Happen collaboration.