An optical transmission spectrum for the ultra-hot Jupiter WASP-121b measured with the Hubble Space Telescope

We present an atmospheric transmission spectrum for the ultra-hot Jupiter WASP-121b, measured using the Space Telescope Imaging Spectrograph (STIS) onboard the Hubble Space Telescope (HST). Across the 0.47-1 micron wavelength range, the data imply an atmospheric opacity comparable to - and in some s...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2018-10
Hauptverfasser:	Evans, Thomas M, Sing, David K, Goyal, Jayesh, Nikolov, Nikolay, Marley, Mark S, Zahnle, Kevin, Henry, Gregory W, Barstow, Joanna K, Alam, Munazza K, Sanz-Forcada, Jorge, Kataria, Tiffany, Lewis, Nikole K, Lavvas, Panayotis, Ballester, Gilda E, Ben-Jaffel, Lotfi, Blumenthal, Sarah D, Bourrier, Vincent, Drummond, Benjamin, Antonio Garcia Munoz, Lopez-Morales, Mercedes, Tremblin, Pascal, Ehrenreich, David, Wakeford, Hannah R, Buchhave, Lars A, Alain Lecavelier des Etangs, Hebrard, Eric, Williamson, Michael H
Format:	Artikel
Sprache:	eng
Schlagworte:	Abundance Atmospheric circulation Confidence intervals Energy budget Extrasolar planets Gas giant planets High temperature Hubble Space Telescope Jupiter atmosphere Opacity Organic chemistry Rayleigh scattering Space telescopes Spectral bands Stellar radiation Vapor phases Wavelengths
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Schreiben Sie den ersten Kommentar!