An HST/WFC3 Thermal Emission Spectrum of the Hot Jupiter HAT-P-7b
Extremely Irradiated Hot Jupiters: Non-oxide Inversions, H- Opacity, and Thermal Dissociation of Molecules
From thermal dissociation to condensation in the atmospheres of ultra hot Jupiters: WASP-121b in context
Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds
Secondary eclipse of the hot Jupiter WASP-121b at 2 mm
The cloudy shape of hot Jupiter thermal phase curves
Instrument
WFC3/IR
Temporal Coverage
2016-12-23T23:33:17Z/2017-01-04T06:49:47Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Bean et al., 2018, 'Remastering the classics: A thermal inversion for the hot Jupiter archetype HAT-P-7b?', 1.0, European Space Agency, https://doi.org/10.5270/esa-iic251l