Evidence for Nightside Water Emission Found in Transit of Ultra-hot Jupiter WASP-33 b

To date, the dayside thermal structure of ultra-hot Jupiters (UHJs) is generally considered to be inverted, but their nightside thermal structure has been less explored. Here, we explore the impact of nightside thermal emission on high-resolution infrared transmission spectroscopy, which should not...

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Bibliografski detalji

Glavni autori:	Yuanheng Yang, Guo Chen, Fei Yan, Xianyu Tan, Jianghui Ji
Format:	Artigo
Jezik:	Inglês
Izdano:	IOP Publishing 2024-01-01
Serija:	The Astrophysical Journal Letters
Teme:	Exoplanet atmospheres Exoplanet atmospheric composition Transmission spectroscopy High resolution spectroscopy Hot Jupiters Exoplanets
Online pristup:	https://doi.org/10.3847/2041-8213/ad65cf
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