1D atmospheric study of the temperate sub-Neptune K2-18b
An Exploration of Model Degeneracies with a Unified Phase Curve Retrieval Analysis: The Light and Dark Sides of WASP-43 b
Aurora: A Generalized Retrieval Framework for Exoplanetary Transmission Spectra
Carbon-bearing Molecules in a Possible Hycean Atmosphere
Consistently Simulating a Wide Range of Atmospheric Scenarios for K2-18b with a Flexible Radiative Transfer Module
Formation and dynamics of water clouds on temperate sub-Neptunes: the example of K2-18b
Haze evolution in temperate exoplanet atmospheres through surface energy measurements
Methane as a dominant absorber in the habitable-zone sub-Neptune K2-18 b
Photochemistry and Spectral Characterization of Temperate and Gas-rich Exoplanets
Stellar Surface Inhomogeneities as a Potential Source of the Atmospheric Signal Detected in the K2-18b Transmission Spectrum
Water Vapor and Clouds on the Habitable-zone Sub-Neptune Exoplanet K2-18b
Water vapour in the atmosphere of the habitable-zone eight-Earth-mass planet K2-18 b
Instrument
WFC3, WFC3/IR
Temporal Coverage
2017-01-04T19:47:08Z/2017-02-21T18:40:57Z
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, BENNEKE BJOERN, 2017, 'A Search for Methane, Ammonia, and Water on Two Habitable Zone Super-Earths', 1.0, European Space Agency, https://doi.org/10.5270/esa-sh5riis
