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...
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: | |
Online Access: | View Fulltext in Publisher |
Similar Items
-
An HST/STIS Optical Transmission Spectrum of Warm Neptune GJ 436b
by: Lothringer, Joshua D., et al.
Published: (2018) -
HST HOT-JUPITER TRANSMISSION SPECTRAL SURVEY: CLEAR SKIES FOR COOL SATURN WASP-39b
by: Fischer, Patrick D., et al.
Published: (2016) -
Program of telluric lines monitoring
by: Vince I., et al.
Published: (2006-01-01) -
Instrumental profile of the Debrecen solar spectrograph
by: Murakezi J., et al.
Published: (2003-01-01) -
Astronomical instrumentation in the mid-infrared and an observational study of Saturn's stratosphere
by: Greathouse, Thomas Kirk
Published: (2008)