S
Shang-Min Tsai
Researcher at University of Oxford
Publications - 59
Citations - 1789
Shang-Min Tsai is an academic researcher from University of Oxford. The author has contributed to research in topics: Exoplanet & Planet. The author has an hindex of 19, co-authored 42 publications receiving 1188 citations. Previous affiliations of Shang-Min Tsai include Academia Sinica & University of Bern.
Papers
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Journal ArticleDOI
The Peculiar Atmospheric Chemistry of KELT-9b
Daniel Kitzmann,Kevin Heng,Paul B. Rimmer,Paul B. Rimmer,Jens Hoeijmakers,Shang-Min Tsai,Matej Malik,Monika Lendl,R. Deitrick,Brice-Olivier Demory +9 more
TL;DR: In this paper, it was shown that the observable atmosphere of KELT-9b is predicted to be close to chemical equilibrium, which greatly simplifies any theoretical interpretation of its spectra.
Journal ArticleDOI
HELIOS: an open-source, GPU-accelerated radiative transfer code for self-consistent exoplanetary atmospheres
Matej Malik,Luc Grosheintz,João M. Mendonça,Simon L. Grimm,Simon L. Grimm,Baptiste Lavie,Daniel Kitzmann,Shang-Min Tsai,Adam Burrows,Laura Kreidberg,Laura Kreidberg,Megan Bedell,Jacob L. Bean,Kevin B. Stevenson,Kevin Heng +14 more
TL;DR: In this article, the authors present HELIOS, an open-source radiative transfer code for studying exoplanetary atmospheres with one-dimensional and planeparallel models.
Journal ArticleDOI
VULCAN: An Open-source, Validated Chemical Kinetics Python Code for Exoplanetary Atmospheres
TL;DR: In this paper, an open-source and validated chemical kinetics code for studying hot exoplanetary atmospheres, which is called VULCAN, is presented for gaseous chemistry from 500 to 2500 K using a reduced C-H-O chemical network with about 300 reactions.
Journal ArticleDOI
The Peculiar Atmospheric Chemistry of KELT-9b
Daniel Kitzmann,Kevin Heng,Paul B. Rimmer,H. J. Hoeijmakers,Shang-Min Tsai,Matej Malik,Monika Lendl,Russell Deitrick,Brice-Olivier Demory +8 more
TL;DR: In this paper, the photochemical kinetics of KELT-9b were used to show that the observable atmosphere is close to chemical equilibrium, which greatly simplifies any theoretical interpretation of its spectra.
Journal ArticleDOI
Three-dimensional Structures of Equatorial Waves and the Resulting Super-rotation in the Atmosphere of a Tidally Locked Hot Jupiter
TL;DR: In this paper, the authors analytically solve linear equations subject to stationary stellar heating with a uniform zonal-mean flow included, and extract wave information in the final equilibrium state of the atmosphere from radiative hydrodynamical simulation for HD 189733b.