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
SN 2010jp (PTF10aaxi): a jet in a Type II supernova
Nathan Smith,S. Bradley Cenko,Nat Butler,Joshua S. Bloom,Mansi M. Kasliwal,Assaf Horesh,Shrinivas R. Kulkarni,Nicholas M. Law,Peter Nugent,Peter Nugent,Eran O. Ofek,Dovi Poznanski,Dovi Poznanski,Robert M. Quimby,Branimir Sesar,Sagi Ben-Ami,Iair Arcavi,Avishay Gal-Yam,David Polishook,Dong Xu,O. Yaron,Dale A. Frail,Mark Sullivan +22 more
TL;DR: In this paper, the authors present photometry and spectroscopy of the peculiar Type II supernova (SN) SN 2010jp, also named PTF10aaxi, and propose that this line profile indicates a bipolar jet-driven explosion, with the central component produced by normal SN ejecta and CSM interaction at mid and low latitudes, while the high-velocity bumps and broad-line wings arise in a nonrelativistic bipolar jet.
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Discovery and early multi-wavelength measurements of the energetic type Ic supernova PTF12gzk: a massive-star explosion in a dwarf host galaxy
Sagi Ben-Ami,Avishay Gal-Yam,Alexei V. Filippenko,Paolo A. Mazzali,Maryam Modjaz,O. Yaron,Iair Arcavi,S. Bradley Cenko,Assaf Horesh,D. Andrew Howell,D. Andrew Howell,Melissa L. Graham,Melissa L. Graham,J. Chuck Horst,M. Im,Yiseul Jeon,Shrinivas R. Kulkarni,Douglas C. Leonard,Daniel A. Perley,Elena Pian,Elena Pian,David J. Sand,David J. Sand,Mark Sullivan,Juliette C. Becker,D. Bersier,Joshua S. Bloom,Joshua S. Bloom,Michael Bottom,Peter de Nully Brown,Kelsey I. Clubb,Ben Dilday,Richard C. Dixon,Aryeh L. Fortinsky,D. B. Fox,Luis A. Gonzalez,Avet Harutyunyan,Mansi M. Kasliwal,Weidong Li,Matthew A. Malkan,Ilan Manulis,Thomas Matheson,Nicholas Moskovitz,Philip S. Muirhead,Peter Nugent,Peter Nugent,Eran O. Ofek,Robert M. Quimby,Joseph W. Richards,Nathaniel R. Ross,Kinchen J. Searcy,Jeffrey M. Silverman,Nathan Smith,Andrew Vanderburg,Emma S. Walker +54 more
TL;DR: In this paper, the discovery and extensive early-time observations of the Type Ic supernova PTF12gzk have been presented, and a dense spectral sequence is used to estimate the physical parameters of the exploding star and of the explosion.
Journal ArticleDOI
Carnegie supernova project-II: Extending the near-infrared hubble diagram for type ia supernovae to z∼0.1 ∗
Mark M. Phillips,Carlos Contreras,Eric Hsiao,Eric Hsiao,Eric Hsiao,Nidia Morrell,Christopher R. Burns,Maximilian Stritzinger,Chris Ashall,Wendy L. Freedman,Wendy L. Freedman,P. Hoeflich,S. E. Persson,Anthony L. Piro,Nicholas B. Suntzeff,S. A. Uddin,J. Anais,E. Baron,Luis Busta,A. Campillay,A. Campillay,S. Castellon,C. Corco,T. Diamond,T. Diamond,Christa Gall,Christa Gall,C. Gonzalez,S. Holmbo,Kevin Krisciunas,Miguel Roth,J. Seron,Francesco Taddia,Simón Torres,Joseph P. Anderson,C. Baltay,G. Folatelli,Lluís Galbany,Ariel Goobar,E. Hadjiyska,Mario Hamuy,Mansi M. Kasliwal,C. Lidman,Peter Nugent,Peter Nugent,Saul Perlmutter,David Rabinowitz,Stuart D. Ryder,Brian P. Schmidt,Benjamin J. Shappee,Emma S. Walker +50 more
TL;DR: The Carnegie Supernova Project-II (CSP-II) was an NSF-funded, four-year program to obtain optical and near-infrared observations of a “Cosmology” sample of ∼100 TypeIa supernovae located in the smooth Hubble flow as mentioned in this paper.
Journal ArticleDOI
K2 Observations of SN 2018oh Reveal a Two-Component Rising Light Curve for a Type Ia Supernova
Georgios Dimitriadis,Ryan J. Foley,A. Rest,D. Kasen,Anthony L. Piro,Abigail Polin,David O. Jones,A. Villar,Gautham Narayan,D. A. Coulter,Charles D. Kilpatrick,Yen-Chen Pan,César Rojas-Bravo,O. D. Fox,Saurabh Jha,Peter Nugent,Adam G. Riess,Daniel Scolnic,Maria R. Drout,Geert Barentsen,J. Dotson,Michael Gully-Santiago,Christina Hedges,Ann Marie Cody,Thomas Barclay,Steve B. Howell,P. M. Garnavich,Brad E. Tucker,Edward J. Shaya,Richard F. Mushotzky,Rob P. Olling,S. Margheim,Alfredo Zenteno,Jeffrey L. Coughlin,J. van Cleve,J. Vinicius de Miranda Cardoso,K. A. Larson,K. M. McCalmont-Everton,C. A. Peterson,S. E. Ross,L. H. Reedy,D. Osborne,C. McGinn,L. Kohnert,L. Migliorini,A. Wheaton,B. Spencer,C. Labonde,G. Castillo,G. Beerman,K. Steward,M. Hanley,R. M. Larsen,R. Gangopadhyay,R. Kloetzel,T. Weschler,V. Nystrom,J. Moffatt,M. Redick,K. Griest,M. Packard,M. Muszynski,J. Kampmeier,R. Bjella,S. Flynn,B. Elsaesser,K. C. Chambers,H. Flewelling,M. E. Huber,E. A. Magnier,C. Z. Waters,A. S. B. Schultz,Joanna Bulger,T. B. Lowe,M. Willman,Stephen J. Smartt,K. W. Smith,Sean D. Points,G. Strampelli,J. Brimacombe,Ping Chen,J. A. Muñoz,Robert L. Mutel,J. C. Shields,Patrick J. Vallely,Steven Villanueva,Wenxiong Li,X. F. Wang,Jia Zhang,Han Lin,Jun Mo,Xulin Zhao,Han-Na Sai,Xiaojia Zhang,Kaicheng Zhang,Tianmeng Zhang,Lifan Wang,E. Baron,J. M. Derkacy,Linyi Li,Zhen-Peng Chen,Danfeng Xiang,Liming Rui,Fang Huang,Xiang Li,Griffin Hosseinzadeh,D. A. Howell,Iair Arcavi,Daichi Hiramatsu,Jamison Burke,S. Valenti,John L. Tonry,L. Denneau,A. N. Heinze,H. Weiland,B. Stalder,J. Vinko,Krisztián Sárneczky,A. Pa,A. Bódi,Zs. Bognár,B. Csák,B. Cseh,G. Csörnyei,O. Hanyecz,Bernadett Ignácz,Cs. Kalup,R. Konyves-Toth,L. Kriskovics,A. Ordasi,I. Rajmon,Ádám Sódor,R. Szabó,R. Szakats,G. Zsidi,Steven Williams,J. Nordin,Régis Cartier,C. Frohmaier,Lluís Galbany,Claudia P. Gutiérrez,Isobel Hook,Cosimo Inserra,M. N. K. Smith,D. J. Sand,Jennifer E. Andrews,Nathan Smith,Christopher Bilinski +147 more
TL;DR: In this article, a 30-min cadence Kepler (K2) light curve of the Type Ia supernova (SN Ia) 2018oh (ASASSN-18bt) is presented, starting weeks before explosion and covering the moment of explosion and subsequent rise, and continuing past peak brightness.
Journal ArticleDOI
A mildly relativistic outflow from the energetic, fast-rising blue optical transient CSS161010 in a dwarf galaxy
Deanne L. Coppejans,Raffaella Margutti,Raffaella Margutti,Giacomo Terreran,A. J. Nayana,A. J. Nayana,Eric R. Coughlin,Tanmoy Laskar,Kate D. Alexander,Michael Bietenholz,Damiano Caprioli,Poonam Chandra,Maria R. Drout,Maria R. Drout,D. Frederiks,C. Frohmaier,K. H. Hurley,Christopher S. Kochanek,Morgan MacLeod,Aaron M. Meisner,Peter Nugent,A. Ridnaia,D. J. Sand,Dmitry S. Svinkin,Charlotte Ward,Charlotte Ward,Sheng Yang,Sheng Yang,Sheng Yang,A. Baldeschi,Igor Chilingarian,Igor Chilingarian,Y. Dong,C. Esquivia,C. Esquivia,W. Fong,C. Guidorzi,Peter Lundqvist,Dan Milisavljevic,Kerry Paterson,Daniel E. Reichart,B. J. Shappee,M. C. Stroh,S. Valenti,B. A. Zauderer,B. A. Zauderer,Bing Zhang +46 more
TL;DR: Coppejans et al. as discussed by the authors presented X-ray and radio observations of the Fast Blue Optical Transient CRTS-CSS161010 J045834-081803 at t = 69-531 days.