A solar C/O and sub-solar metallicity in a hot Jupiter atmosphere
Assessing the C/O Ratio Formation Diagnostic: A Potential Trend with Companion Mass
Confirmation of Subsolar Metallicity for WASP-77Ab from JWST Thermal Emission Spectroscopy
Confirmation of Water Absorption in the Thermal Emission Spectrum of the Hot Jupiter WASP-77Ab with HST/WFC3
Enhancing Exoplanet Ephemerides by Leveraging Professional and Citizen Science Data: A Test Case with WASP-77 A b
Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse
Lessons from Hubble and Spitzer: 1D Self-consistent Model Grids for 19 Hot Jupiter Emission Spectra
Instrument
WFC3/IR
Temporal Coverage
2020-11-07T08:04:11Z/2020-12-19T19:04:55Z
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, Weiner Mansfield comma Megan, 2021, 'Stuck in the Middle with WASP-77Ab: Defining Transitions in Hot Jupiter Atmospheres', 1.0, European Space Agency, https://doi.org/10.5270/esa-p9ksrxb