N
Nathan Smith
Researcher at University of Arizona
Publications - 543
Citations - 30830
Nathan Smith is an academic researcher from University of Arizona. The author has contributed to research in topics: Supernova & Nebula. The author has an hindex of 86, co-authored 503 publications receiving 28124 citations. Previous affiliations of Nathan Smith include University of Hawaii at Manoa & University of California.
Papers
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Journal ArticleDOI
The shocking near-infrared spectrum of the Homunculus Nebula surrounding η Carinae
TL;DR: In this article, near-infrared long-slit spectra of the Homunculus Nebula surrounding η Carinae reveal emission from molecular hydrogen for the first time in this object and strong intrinsic [Fe II] emission.
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Discovery of an Intermediate-luminosity Red Transient in M51 and Its Likely Dust-obscured, Infrared-variable Progenitor
Jacob E. Jencson,Scott M. Adams,Howard E. Bond,Howard E. Bond,Schuyler D. Van Dyk,Mansi M. Kasliwal,John Bally,Nadejda Blagorodnova,Kaushik De,Christoffer Fremling,Yuhan Yao,Andrew S. Fruchter,David Rubin,Cristina Barbarino,Jesper Sollerman,Adam A. Miller,E. K. S. Hicks,Matthew A. Malkan,Igor Andreoni,Eric C. Bellm,Robert Buchheim,Richard Dekany,Michael Feeney,Sara Frederick,Avishay Gal-Yam,Robert D. Gehrz,Matteo Giomi,Matthew J. Graham,Wayne Green,David Hale,M. Hankins,Mark Hanson,George Helou,Anna Y. Q. Ho,Tiara Hung,Mario Juric,M. Kendurkar,Shrinivas R. Kulkarni,Ryan M. Lau,Frank J. Masci,James D. Neill,Kevin Quin,Reed Riddle,Ben Rusholme,Forrest Sims,Nathan Smith,Roger M. H. Smith,Maayane T. Soumagnac,Yutaro Tachibana,Yutaro Tachibana,Samaporn Tinyanont,Richard Walters,Stanley Watson,Robert E. Williams,Robert E. Williams +54 more
TL;DR: Jencson et al. as discussed by the authors presented the discovery of an optical transient (OT) in Messier 51, designated M51 OT2019-1 (also ZTF 19aadyppr, AT 2019abn, ATLAS19bzl), by the Zwicky Transient Facility.
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Infrared [Fe II] emission in the circumstellar nebulae of luminous blue variables
TL;DR: In this paper, infrared spectra of other luminous blue variables (LBV) and LBV candidates were obtained for the H-band (1.5 to 1.75 µm) for the central stars and nebulae of η Car, AG Car, P Cygni, Wra 751, HR Car, HD 168625, HD160529, R 127 and S Doradus.
Journal ArticleDOI
SN 2017gmr: An energetic Type II-P supernova with asymmetries
Jennifer E. Andrews,D. J. Sand,S. Valenti,Nathan Smith,Raya Dastidar,Debapriya Sahu,Kuntal Misra,Avinash Singh,Daichi Hiramatsu,Peter Brown,Griffin Hosseinzadeh,S. Wyatt,J. Vinko,G. C. Anupama,Iair Arcavi,Chris Ashall,S. Benetti,Marco Berton,K. A. Bostroem,Mattia Bulla,Jamison Burke,S. Chen,Laura Chomiuk,Aleksandar Cikota,Enrico Congiu,B. Cseh,Scott C. Davis,N. Elias-Rosa,Tamar Faran,Morgan Fraser,Lluís Galbany,C. Gall,Avishay Gal-Yam,Anjasha Gangopadhyay,M. Gromadzki,J. B. Haislip,D. A. Howell,Eric Hsiao,Cosimo Inserra,Erkki Kankare,Hanindyo Kuncarayakti,Vladimir Kouprianov,Brajesh Kumar,Xue Li,Han Lin,Kate Maguire,Paolo A. Mazzali,C. McCully,Peter Milne,Jun Mo,N. I. Morrell,Matt Nicholl,P. Ochner,F. Olivares,A. Pastorello,Ferdinando Patat,M. M. Phillips,G. Pignata,S. J. Prentice,A. Reguitti,D. E. Reichart,Ósmar Rodríguez,Liming Rui,Pankaj Sanwal,Krisztián Sárneczky,Melissa Shahbandeh,Mridweeka Singh,Stephen J. Smartt,Jay Strader,Maximilian Stritzinger,R. Szakats,L. Tartaglia,Huijuan Wang,Lingzhi Wang,Xiaofeng Wang,John C Wheeler,Danfeng Xang,O. Yaron,D. R. Young,Junbo Zhang +79 more
TL;DR: In this paper, high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days was presented.
Journal ArticleDOI
SN 2017gmr : An Energetic Type II-P Supernova with Asymmetries
Jennifer E. Andrews,David J. Sand,S. Valenti,Nathan Smith,Raya Dastidar,Raya Dastidar,D. K. Sahu,Kuntal Misra,Kuntal Misra,Avinash Singh,Avinash Singh,Daichi Hiramatsu,Daichi Hiramatsu,Peter J. Brown,Griffin Hosseinzadeh,S. Wyatt,Jozsef Vinko,Jozsef Vinko,G. C. Anupama,Iair Arcavi,Chris Ashall,S. Benetti,Marco Berton,Marco Berton,K. A. Bostroem,Mattia Bulla,Jamison Burke,Jamison Burke,S. Chen,S. Chen,Laura Chomiuk,Aleksandar Cikota,Enrico Congiu,Enrico Congiu,B. Cseh,Scott C. Davis,Nancy Elias-Rosa,Tamar Faran,Morgan Fraser,Lluís Galbany,Christa Gall,Avishay Gal-Yam,Anjasha Gangopadhyay,Anjasha Gangopadhyay,Mariusz Gromadzki,J. B. Haislip,D. A. Howell,D. A. Howell,Eric Hsiao,Cosimo Inserra,Erkki Kankare,Hanindyo Kuncarayakti,Vladimir Kouprianov,Vladimir Kouprianov,Brajesh Kumar,Xue Li,Han Lin,Kate Maguire,Paolo A. Mazzali,Paolo A. Mazzali,Curtis McCully,Curtis McCully,Peter Milne,Jun Mo,Nidia Morrell,Matt Nicholl,P. Ochner,F. Olivares,F. Olivares,A. Pastorello,Ferdinando Patat,Mark M. Phillips,G. Pignata,G. Pignata,S. J. Prentice,A. Reguitti,A. Reguitti,D. E. Reichart,Ósmar Rodríguez,Ósmar Rodríguez,Liming Rui,Pankaj Sanwal,Pankaj Sanwal,Krisztián Sárneczky,Melissa Shahbandeh,M. J. Singh,M. J. Singh,Stephen J. Smartt,Jay Strader,Maximilian Stritzinger,Róbert Szakáts,Leonardo Tartaglia,Huijuan Wang,Lingzhi Wang,Xiaofeng Wang,John C Wheeler,Danfeng Xiang,O. Yaron,D. R. Young,Junbo Zhang +99 more
TL;DR: In this paper, high-cadence UV, optical, and near-infrared data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days was presented.