A reanalysis of the LHS 1140 b atmosphere observed with the Hubble Space Telescope
Detectability of biosignatures on LHS 1140 b
Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
Hubble WFC3 Spectroscopy of the Habitable-zone Super-Earth LHS 1140 b
Impact of M-dwarf stellar wind and photoevaporation on the atmospheric evolution of small planets
New Mass and Radius Constraints on the LHS 1140 Planets: LHS 1140 b Is either a Temperate Mini-Neptune or a Water World
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA, WFC3, WFC3/IR
Temporal Coverage
2017-01-27T20:18:48Z/2017-12-15T16:13:46Z
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, Dittmann comma Jason A., 2017, 'Initial Reconaissance of a Transiting Rocky Planet in a Nearby M-Dwarf's Habitable Zone', 1.0, European Space Agency, https://doi.org/10.5270/esa-9d171m4