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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.

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A Spitzer Survey for Dust in Type IIn Supernovae

TL;DR: In this paper, the authors present results from a warm Spitzer/IRAC survey of the positions of all 68 known SNe IIn within a distance of 250 Mpc between 1999 and 2008 that have remained unobserved by Spitzer more than 100 days post-discovery.
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Sn 2008s: a cool super-eddington wind in a supernova impostor

TL;DR: Based on the low peak luminosity for a SN of MR = −13.9 mag, photometric and spectral evolution unlike that of low-luminosity SNe, a late-time decline rate slower than 56Co decay, and slow outflow speeds of 600-1000 km s−1, the authors conclude that SN 2008S is not a true core-collapse SN and is probably not an electron-capture SN.
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SN 2009ip and SN 2010mc: core-collapse Type IIn supernovae arising from blue supergiants

TL;DR: In this article, the authors show that the late-time spectrum of SN 2009ip closely resembles spectra of SN 1987A, and that the changing Hα equivalent width after explosion matches behavior typically seen in core-collapse SNe IIn.
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A Pan-Carina YSO Catalog: Intermediate-Mass Young Stellar Objects in the Carina Nebula Identified Via Mid-Infrared Excess Emission

TL;DR: A catalog of 1439 young stellar objects (YSOs) spanning the 1.42 deg^2 field surveyed by the Chandra Carina Complex Project (CCCP), which includes the major ionizing clusters and the most active sites of ongoing star formation within the Great Nebula in Carina is presented in this article.
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A MASSIVE PROGENITOR OF THE LUMINOUS TYPE IIn SUPERNOVA 2010jl

TL;DR: In this paper, the authors report archival Hubble Space Telescope (HST) observations of its host galaxy UGC 5189A taken roughly 10 yr prior to explosion, as well as early-time optical spectra of the SN.