A Hubble PanCET Study of HAT-P-11b: A Cloudy Neptune with a Low Atmospheric Metallicity
A Population Study of Gaseous Exoplanets
Haze evolution in temperate exoplanet atmospheres through surface energy measurements
H2O abundances and cloud properties in ten hot giant exoplanets
Retrieval analysis of 38 WFC3 transmission spectra and resolution of the normalization degeneracy
Statistical Analysis of Hubble/WFC3 Transit Spectroscopy of Extrasolar Planets
The Influence of Nonuniform Cloud Cover on Transit Transmission Spectra
Trends in Atmospheric Properties of Neptune-size Exoplanets
Water vapour absorption in the clear atmosphere of a Neptune-sized exoplanet
Instrument
WFC3, WFC3/IR
Temporal Coverage
2012-10-18T05:06:51Z/2012-12-16T00:46:23Z
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, Deming comma Drake, 2013, 'Atmospheric Composition of the ExoNeptune HAT-P-11', 1.0, European Space Agency, https://doi.org/10.5270/esa-25r0kpy