A New Window into Planet Formation and Migration: Refractory-to-Volatile Elemental Ratios in Ultra-hot Jupiters
An Optical Transmission Spectrum for the Ultra-hot Jupiter WASP-121b Measured with the Hubble Space Telescope
A Population Study of Gaseous Exoplanets
Detection of H2O and Evidence for TiO/VO in an Ultra-hot Exoplanet Atmosphere
Detection of TiO and VO in the Atmosphere of WASP-121b and Evidence For its Temporal Variation
Exploring the Ability of Hubble Space Telescope WFC3 G141 to Uncover Trends in Populations of Exoplanet Atmospheres through a Homogeneous Transmission Survey of 70 Gaseous Planets
Gemini/GMOS optical transmission spectroscopy of WASP-121b: signs of variability in an ultra-hot Jupiter?
H2O abundances and cloud properties in ten hot giant exoplanets
Is the Atmosphere of the Ultra-hot Jupiter WASP-121 b Variable?
Retrieval analysis of 38 WFC3 transmission spectra and resolution of the normalization degeneracy
Revisiting KELT-19Ab, WASP-156b, and WASP-121b in the TESS Era
Statistical Analysis of Hubble/WFC3 Transit Spectroscopy of Extrasolar Planets
Strong biases in retrieved atmospheric composition caused by day-night chemical heterogeneities
The Mantis Network II: examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling
Instrument
WFC3, WFC3/IR
Temporal Coverage
2016-02-06T04:51:46Z/2016-02-06T12:00:14Z
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, Evans-Soma comma Thomas, 2016, 'Characterizing an extreme planet on the verge of tidal disruption', 1.0, European Space Agency, https://doi.org/10.5270/esa-vtf5u0n