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.
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New Silhouette Disks with Reflection Nebulae and Outflows in the Orion Nebula and M43
TL;DR: In this article, the authors reported the detection of several new circumstellar disks seen in silhouette in the outskirts of the Orion nebula and M43, detected as part of our Halpha survey of Orion with the HST/ACS.
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Massive stars dying alone: The extremely remote environment of SN 2009ip
TL;DR: In this article, the authors used the HST from the Space Telescope Science Institute (STS-13787) as a data collection platform for the first HST mission to the International Journal of Astronautics (IJOA).
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A disrupted circumstellar torus inside eta Carinae's Homunculus Nebula
Nathan Smith,Robert D. Gehrz,P. M. Hinz,William F. Hoffmann,Eric E. Mamajek,Michael Meyer,Joseph L. Hora +6 more
TL;DR: In this paper, thermal infrared images of the bipolar nebula surrounding eta Carinae at six wavelengths from 4.8 to 24.5 microns were obtained with the MIRAC3 camera system at the Magellan Observatory.
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Searching for Highly Magnified Stars at Cosmological Distances: Discovery of a Redshift 0.94 Blue Supergiant in Archival Images of the Galaxy Cluster MACS J0416.1-2403
Wenlei Chen,Patrick L. Kelly,Jose M. Diego,Masamune Oguri,Masamune Oguri,Liliya L. R. Williams,Adi Zitrin,Tommaso Treu,Nathan Smith,Tom Broadhurst,Tom Broadhurst,Tom Broadhurst,Nick Kaiser,Ryan J. Foley,Alexei V. Filippenko,Laura Salo,Jens Hjorth,Jonatan Selsing,Jonatan Selsing +18 more
TL;DR: In this article, the analysis of highly magnified stars at the University of Minnesota by P.L.K, A.V.F., and T.T.H. was supported by NSF grant AST-1908823.
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Keck LWS Images of the Compact Nebula around RY Scuti in the Thermal Infrared
TL;DR: In this paper, the 3 to 20 μm Keck Telescope images of the massive eclipsing binary RY Scuti with ~025 spatial resolution were reported, showing complex structure near the diffraction limit of the 10 m telescope in a nebula less than 2'' across.