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.
Papers
More filters
Journal ArticleDOI
Spectra of High-Redshift Type Ia Supernovae and a Comparison with their Low-Redshift Counterparts
I. M. Hook,D. A. Howell,Greg Aldering,Rahman Amanullah,M. S. Burns,Alex Conley,Alex Conley,S. E. Deustua,Richard S. Ellis,Sebastien Fabbro,Vitaliy Fadeyev,Gastón Folatelli,G. Garavini,G. Garavini,R. Gibbons,G. Goldhaber,G. Goldhaber,Ariel Goobar,Donald E. Groom,A. G. Kim,R. A. Knop,Marek Kowalski,Chris Lidman,S. Nobili,S. Nobili,Peter Nugent,Reynald Pain,C. R. Pennypacker,Saul Perlmutter,Saul Perlmutter,Pilar Ruiz-Lapuente,G. Sainton,Bradley E. Schaefer,Eric P. Smith,A. L. Spadafora,Vallery Stanishev,R. C. Thomas,Nicholas A. Walton,Lifan Wang,W. M. Wood-Vasey,W. M. Wood-Vasey +40 more
TL;DR: In this article, the authors presented spectra for 14 high-redshift (0.17 < z < 0.83) supernovae, which were discovered by the Supernova Cosmology Project as part of a campaign to measure cosmological parameters, and found that the dates of the spectra relative to maximum light determined from this fitting process are consistent with the dates determined from the photometric light curves, and moreover the spectral time-sequence for SNe Type Ia at low and high redshift is indistinguishable.
Journal ArticleDOI
Observational Predictions for Sub-Chandrasekhar Mass Explosions: Further Evidence for Multiple Progenitor Systems for Type Ia Supernovae
TL;DR: In this paper, a numerical parameter survey of sub-Chandrasekhar mass white dwarf (WD) explosions is presented, and the authors identify a relationship between Si II velocity and luminosity which identifies a sub-class of observed supernovae that are consistent with these models.
Journal ArticleDOI
A UV resonance line echo from a shell around a hydrogen-poor superluminous supernova
Ragnhild Lunnan,Ragnhild Lunnan,Claes Fransson,Paul Vreeswijk,S. E. Woosley,Giorgos Leloudas,Daniel A. Perley,Robert M. Quimby,Robert M. Quimby,Lin Yan,N. Blagorodnova,Brian D. Bue,S. B. Cenko,S. B. Cenko,A. De Cia,David O. Cook,Christoffer Fremling,Pradip Gatkine,Avishay Gal-Yam,Mansi M. Kasliwal,Shrinivas R. Kulkarni,Frank J. Masci,Peter Nugent,Peter Nugent,A. Nyholm,Adam Rubin,Nao Suzuki,P. Wozniak +27 more
TL;DR: A class of rare and energetic superluminous supernovae (SLSN-I) have been discovered in untargeted transient surveys in the past decade as discussed by the authors.
Journal ArticleDOI
Constraining the Progenitor Companion of the Nearby Type Ia SN 2011fe with a Kiloday Nebular Spectrum
Melissa L. Graham,Peter Nugent,Mark Sullivan,Alexei V. Filippenko,S. Bradley Cenko,Jeffrey M. Silverman,Kelsey I. Clubb,WeiKang Zheng +7 more
TL;DR: In this paper, the authors present a "kiloday" optical nebular spectrum of the nearby Type Ia supernova (SN) 2011fe, obtained +981 days after explosion.
Journal ArticleDOI
THE DETECTION OF A SN IIn IN OPTICAL FOLLOW-UP OBSERVATIONS OF ICECUBE NEUTRINO EVENTS
M. G. Aartsen,K. Abraham,Markus Ackermann,Jenni Adams,Juanan Aguilar,Markus Ahlers,Maryon Ahrens,D. Altmann,T. Anderson,M. Archinger,Carlos Arguelles,T. C. Arlen,J. Auffenberg,Xinhua Bai,Steven W. Barwick,V. Baum,R. C. Bay,J. J. Beatty,J. Becker Tjus,K. H. Becker,E. Beiser,Segev BenZvi,P. Berghaus,D. Berley,Elisa Bernardini,A. Bernhard,D. Z. Bessonu,G. Binder,G. Binder,D. Bindig,M. Bissok,E. Blaueuss,J. Blumenthal,D. J. Boersma,Christian Bohm,M. Boerner,F. Bos,D. Bose,S. Boeser,Olga Botner,J. Braun,L. Brayeur,H.-P. Bretz,A. M. Brown,N. Buzinsky,J. Casey,M. Casier,E. Cheung,Dmitry Chirkin,A. Christov,B. Christy,K. Clark,L. Classen,S. Coenders,D. F. Cowen,A. H. Cruz Silva,J. Daughhetee,J. C. Davis,M. Day,J. P. A. M. de André,C. De Clercq,H. Dembinski,S. De Ridder,Paolo Desiati,K. D. de Vries,G. de Wasseige,Tyce DeYoung,J. C. Díaz-Vélez,J. P. Dumm,M. Dunkman,R. Eagan,B. Eberhardt,T. Ehrhardt,B. Eichmann,S. Euler,Paul Evenson,O. Fadiran,S. Fahey,A. R. Fazely,Anatoli Fedynitch,J. Feintzeig,J. Felde,Kirill Filimonov,C. Finley,T. Fischer-Wasels,S. Flis,T. Fuchs,M. Glagla,Thomas K. Gaisser,R. Gator,Jay Gallagher,L. Gerhardt,L. Gerhardt,Karim Ghorbani,D. Gier,L. Gladstone,T. Gluesenkamp,A. Goldschmidt,G. Golup,Javier Gonzalez,Dariusz Gora,Darren Grant,P. Gretskov,J. C. Groh,A. Gross,C. Ha,C. Ha,C. Haack,A. Haj Ismail,Allan Hallgren,Francis Halzen,B. Hansmann,Kael Hanson,D. Hebecker,D. Heereman,K. Helbing,R. Hellauer,D. Hellwig,S. Hickford,Joshua Hignight,G. C. Hill,Kara Hoffman,R. Hoffmann,K. Holzapfe,A. Homeier,K. Hoshina,F. Huang,M. E. Huber,W. Huelsnitz,P. O. Hulth,Klas Hultqvist,S. In,Aya Ishihara,E. Jacobi,George Japaridze,K. Jero,M. Jurkovic,B. Kaminsky,Alexander Kappes,T. Karg,Albrecht Karle,M. Kauer,Azadeh Keivani,J. L. Kelley,Julian Kemp,Ali Kheirandish,J. Kiryluk,J. Klaes,Spencer Klein,Spencer Klein,G. Kohnen,R. Koirala,Hermann Kolanoski,R. Konietz,A. Koob,L. Koepke,C. Kopper,S. Kopper,D. J. Koskinen,M. Kowalski,K. Krings,G. Kroll,M. Kroll,J. Kunnen,N. Kurahashi,T. Kuwabara,M. Labare,J. L. Lanfranchi,M. J. Larson,M. Lesiak-Bzdak,M. Leuermann,J. Leuner,J. Luenemann,James Madsen,G. Maggi,Kendall Mahn,Reina H. Maruyama,K. Mase,H. S. Matis,R. Maunu,F. McNally,K. Meagher,M. Medici,A. Meli,T. Menne,G. Merino,Thomas Meures,S. Miarecki,S. Miarecki,E. Middell,E. Middlemas,J. Miller,L. Mohrmann,Teresa Montaruli,R. Morse,R. Nahnhauer,U. Naumann,H. Niederhausen,S. C. Nowicki,D. R. Nygre,A. Obertacke,A. Olivas,A. Omairat,Aongus O'Murchadha,T. Palczewski,H. Pandya,Larissa Paul,Joshua Pepper,Carlos Pérez de los Heros,C. Pfendner,Damian Pieloth,E. Pinat,J. Posselt,P. B. Price,Gerald Przybylski,J. Puetz,M. Quinnan,L. Raedel,M. Rameez,K. Rawlins,P. Redl,R. Reimann,M. Relich,Elisa Resconi,Wolfgang Rhode,Mike Richman,S. Richter,B. Riedel,Sally Robertson,M. Rongen,Carsten Rott,T. Ruhe,D. Ryckbosch,S. M. Saba,L. Sabbatini,H. G Sander,A. Sandrock,J. Sandroos,Subir Sarkar,Subir Sarkar,K. Schatto,F. Scheriau,M. Schimp,T. Schmidt,M. Schmitz,S. Schoenen,S. Schoeneberg,A. Schoenwald,A. Schukraft,L. Schulte,D. Seckel,S. Seunarine,R. Shanidze,M. W. E. Smith,D. Soldin,Glenn Spiczak,C. Ering,M. Stahlberg,M. Stamatikos,Todor Stanev,N. A. Stanisha,A. Stasik,T. Stezelberger,R. G. Stokstad,A. Stoessl,E. A. Strahlers,R. Ström,N. L. Strotjohann,G. W. Suwvan,Michael Sutherland,H. Taavola,Ignacio Taboada,Samvel Ter-Antonyan,A. Terliuk,G. Tešić,S. Tilav,P. A. Toale,M. N. Tobin,D. Tosi,M. Tselengidou,A. Turcati,E. Unger,M. Usner,Sofia Vallecorsa,N. van Eundhoven,Justin Vandenbroucke,J. van Santen,Stijn Vanheule,J. Veenkamp,M. Vehring,M. Voge,M. Vraeghe,C. Walck,M. Wallraff,N. Wandkowsky,Ch. Weaver,Chris Wendt,S. Westerhoff,B. J. Whelan,N. Whitehorn,C. Wichary,K. Wiebe,Christopher Wiebusch,L. Wille,Dawn Williams,H. Wissing,M. Wolf,T. R. Wood,Kurt Woschnagg,Donglian Xu,Xianwu Xu,Y. Xu,J. P. Yanez,G. B. Yodh,S. Yoshida,P. Zarzhitsky,M. Zoll,Eran O. Ofek,Mansi M. Kasliwal,Peter Nugent,Peter Nugent,Iair Arcavi,Iair Arcavi,Joshua S. Bloom,Joshua S. Bloom,Shrinivas R. Kulkarni,Daniel A. Perley,Tom A. Barlow,Assaf Horesh,Avishay Gal-Yam,D. A. Howell,D. A. Howell,B. Dilday,Phil Evans,J. A. Kennea,W. S. Burgett,K. C. Chambers,N. Kaiser,C. Waters,H. Flewelling,J. L. Tonry,Armin Rest,S. J. Smartt +342 more
TL;DR: In this article, a Type IIn supernova (SN IIn) PTF12csy was found 0.2 degrees 2 away from the neutrino alert direction, with an error radius of 0.0684, corresponding to a luminosity distance of about 300 Mpc.