A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 b
ARES IV: Probing the Atmospheres of the Two Warm Small Planets HD 106315c and HD 3167c with the HST/WFC3 Camera
Clouds and Clarity: Revisiting Atmospheric Feature Trends in Neptune-size Exoplanets
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
Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-sized Exoplanet HD 106315c
The Rossiter-McLaughlin effect revolutions: an ultra-short period planet and a warm mini-Neptune on perpendicular orbits
Transmission Spectroscopy for the Warm Sub-Neptune HD 3167c: Evidence for Molecular Absorption and a Possible High-metallicity Atmosphere
Water Absorption in the Transmission Spectrum of the Water World Candidate GJ 9827 d
Instrument
WFC3/IR
Temporal Coverage
2017-11-24T10:45:44Z/2020-12-02T13:46:57Z
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, Crossfield et al., 2020, 'The Atmospheric Diversity of Mini-Neptunes in Multi-planet Systems', 1.0, European Space Agency, https://doi.org/10.5270/esa-7xwtyua