Tamás Szalai

Eötvös Loránd University — Hungary

Physics and Astronomy · Physical Sciences

26h-index1.8kcitations126works5.02yr avg
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Research Topics

Gamma-ray bursts and supernovae(96), Stellar, planetary, and galactic studies(46), Astro and Planetary Science(27), Astrophysical Phenomena and Observations(27), Astronomy and Astrophysical Research(24)

Publications125 total

JWST Observations of SN 2023ixf. II. The Panchromatic Evolution between 250 and 720 Days after the Explosion
The Astrophysical Journal·2025· 3 citedOpen Access
Two Decades of Dust Evolution in SN 2005af through JWST, Spitzer, and Chemical Modeling
The Astrophysical Journal·2025· 1 citedOpen Access
SN 2023ixf in M101: Physical Parameters from Bolometric Light Curve Modeling
The Astrophysical Journal·2025· 1 citedOpen Access
Very Late-time JWST and Keck Spectra of the Oxygen-rich Supernova 1995N
The Astrophysical Journal·2025· 3 citedOpen Access
SN 2022xlp: The second-known well-observed, intermediate-luminosity Iax supernova
Astronomy and Astrophysics·2025· 1 citedOpen Access
SN 2023ixf in M101: physical parameters from bolometric light curve modeling
arXiv (Cornell University)·2025Open Access
JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip
The Astrophysical Journal·2025· 10 citedOpen Access
Large Cold Dust Reservoir Revealed in Transitional SN Ib 2014C by James Webb Space Telescope Mid-infrared Spectroscopy
The Astrophysical Journal·2025· 7 citedOpen Access
JWST and Ground-based Observations of the Type Iax Supernovae SN 2024pxl and SN 2024vjm: Evidence for Weak Deflagration Explosions
ArXiv.org·2025Open Access
Photometry and Spectroscopy of SN 2024pxl: A Luminosity Link Among Type Iax Supernovae
arXiv (Cornell University)·2025Open Access
Very Late-Time JWST and Keck Spectra of the Oxygen-Rich Supernova 1995N
arXiv (Cornell University)·2025Open Access
Modeling the circumstellar interaction around SN 2004gq
Astronomy and Astrophysics·2025· 1 citedOpen Access
JWST/MIRI detects the dusty SN1993J about 30 years after explosion
Astronomy and Astrophysics·2025· 3 citedOpen Access
NEOWISE-R Caught the Luminous SN 2023ixf in Messier 101
The Astrophysical Journal·2024· 8 citedOpen Access
JWST/MIRI Observations of Newly Formed Dust in the Cold, Dense Shell of the Type IIn SN 2005ip
arXiv (Cornell University)·2024Open Access
Ejecta Masses in Type Ia Supernovae—Implications for the Progenitor and the Explosion Scenario*
Publications of the Astronomical Society of the Pacific·2024· 3 citedOpen Access
Constraining Dust Formation in the Superluminous Supernova 2017gci with JWST Observations
arXiv (Cornell University)·2024Open Access
Ejecta masses in Type Ia Supernovae -- Implications for the Progenitor and the Explosion Scenario
arXiv (Cornell University)·2024Open Access
The story of SN 2021aatd: A peculiar 1987A-like supernova with an early-phase luminosity excess
Astronomy and Astrophysics·2024· 1 citedOpen Access
NEOWISE-R Caught the Luminous SN 2023ixf in Messier 101
arXiv (Cornell University)·2024Open Access
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Frequent Co-authors

J. Vinkó(21), Jennifer E. Andrews(15), A. V. Filippenko(14), András Pál(13), R. J. Foley(12), Schuyler D. Van Dyk(12), Ori D. Fox(12), J. C. Wheeler(11), A. Rest(10), Barnabás Barna(10), K. Vida(10), D. A. Howell(10), C. McCully(10), Melissa Shahbandeh(10), Thomas G. Brink(10), G. H. Marion(9), K. Azalee Bostroem(9), K. Sárneczky(9), WeiKang Zheng(9), J. Johansson(9)