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
Nebular Hα Limits for Fast Declining SNe Ia
D. J. Sand,Renata Cecília Amaro,Maxwell Moe,Melissa L. Graham,Jennifer E. Andrews,Jamison Burke,Jamison Burke,R. Cartier,Y. Eweis,Lluís Galbany,Daichi Hiramatsu,Daichi Hiramatsu,D. A. Howell,D. A. Howell,Saurabh Jha,Saurabh Jha,M. Lundquist,Thomas Matheson,Curtis McCully,Curtis McCully,Peter Milne,Nathan Smith,S. Valenti,S. Wyatt +23 more
TL;DR: In this paper, the authors used the DIRAC Institute in the Department of Astronomy at the University of Washington (U.W.Seattle) to conduct a study on the performance of the Dijkstra-Lau et al. this paper.
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ALMA-resolved salt emission traces the chemical footprint and inner wind morphology of VY Canis Majoris
Leen Decin,Anita M. S. Richards,Tom J. Millar,Alain Baudry,E. De Beck,Ward Homan,Nathan Smith,M. Van de Sande,Conor J. Walsh +8 more
TL;DR: In this article, high spatial resolution (∼0.24 × 0.13) ALMA science verification (SV) data in band 7, in which four thermal emission lines of gaseous sodium chloride (NaCl) are present at high signal-to-noise ratio.
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A Survey of Irradiated Pillars, Globules, and Jets in the Carina Nebul
TL;DR: In this paper, a wide-field, deep narrowband H$_2$, Br$\gamma, H$\alpha, [S II], [O III], and broadband I and K-band images of the Carina star formation region are presented.
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The reverse shock of SNR1987A at 18 years after outburst
TL;DR: In this article, low-dispersion spectra obtained at the Magellan Observatory were used to study the broad H-alpha emission from the reverse shock of the infant supernova remnant SNR1987A.
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Silicate Emission Profiles from Low-Mass Protostellar Disks in the Orion Nebula: Evidence for Growth and Thermal Processing of Grains
TL;DR: In this paper, the authors present 8-13 μm low-resolution spectra (R ≈ 100) of eight low-mass protostellar objects ("proplyds") in the Orion Nebula using the Long Wavelength Spectrometer at the W. M. Keck Observatory.