The hot Neptune WASP-166 b with ESPRESSO II: confirmation of atmospheric sodium

The hot Neptune WASP-166 b with ESPRESSO II: confirmation of atmospheric sodium

The hot Neptune desert, a distinct lack of highly irradiated planets in the size range of Neptune, remains one of the most intriguing results of exoplanet population studies. A deeper understanding of the atmosphere of exoplanets sitting at the edge or even within the Neptune desert will allow us to...

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Bibliographic Details
Main Authors: Allart, R. (Author), Anderson, D.R (Author), Brogi, M. (Author), Buchschacher, N. (Author), Cegla, H.M (Author), Doyle, L. (Author), Gandhi, S. (Author), Lafarga, M. (Author), Lovis, C. (Author), Seidel, J.V (Author), Sosnowska, D. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Instrumentation: spectrographs
Methods: observational
Planetary Systems
Planets and satellites: atmospheres
Techniques: spectroscopic
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