T
Tamás Szalai
Researcher at California Institute of Technology
Publications - 3
Citations - 30
Tamás Szalai is an academic researcher from California Institute of Technology. The author has contributed to research in topics: Spitzer Space Telescope & Supernova. The author has an hindex of 2, co-authored 3 publications receiving 11 citations. Previous affiliations of Tamás Szalai include Ames Research Center.
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Journal ArticleDOI
The slow demise of the long-lived SN 2005ip
O. D. Fox,Claes Fransson,Nathan Smith,J. E. Andrews,K. Azalee Bostroem,T. G. Brink,S. Bradley Cenko,Geoffrey C. Clayton,Alexei V. Filippenko,Wen-fai Fong,Joseph S. Gallagher,Patrick L. Kelly,Charles D. Kilpatrick,Jon C. Mauerhan,Adam Miller,E. Montiel,Maximilian Stritzinger,Tamás Szalai,Tamás Szalai,Schuyler D. Van Dyk,Schuyler D. Van Dyk +20 more
TL;DR: In this article, the authors studied the Type IIn supernova (SN) 2005ip from 1000-5000 days post-explosion at all wavelengths, including X-ray, ultraviolet, nearinfrared, and mid-infrared.
Journal ArticleDOI
Spitzer's last look at extragalactic explosions: Long-term evolution of interacting supernovae
Tamás Szalai,Ori D. Fox,Richard G. Arendt,Eli Dwek,Jennifer E. Andrews,Geoffrey C. Clayton,Alexei V. Filippenko,Joel Johansson,Patrick L. Kelly,Kelsie Krafton,A. P. Marston,Jon C. Mauerhan,Schuyler D. Van Dyk +12 more
TL;DR: In this article, the authors presented new mid-infrared (mid-IR) data for supernovae (SNe) based on measurements with the Spitzer Space Telescope, comparing their recent 3.6 and 4.5 µm photometry with previously published mid-IR and further multiwavelength datasets, they were able to draw some conclusions about the origin and heating mechanism of the dust in these SNe or in their environments.
Posted Content
Spitzer's Last Look at Extragalactic Explosions: Long-Term Evolution of Interacting Supernovae
Tamás Szalai,Ori D. Fox,Richard G. Arendt,Eli Dwek,Jennifer E. Andrews,Geoffrey C. Clayton,Alexei V. Filippenko,Joel Johansson,Patrick L. Kelly,Kelsie Krafton,A. P. Marston,Jon C. Mauerhan,Schuyler D. Van Dyk +12 more
TL;DR: In this paper, the authors presented new mid-infrared (mid-IR) data for supernovae (SNe) based on measurements with the Spitzer Space Telescope, comparing their recent 3.6 and 4.5 µm photometry with previously published mid-IR and further multiwavelength datasets, they were able to draw some conclusions about the origin and heating mechanism of the dust in these SNe or in their environments.