A giant comet-like cloud of hydrogen escaping the warm Neptune-mass exoplanet GJ 436b
Evaporation of hot jupiters and hot neptunes
HST/STIS Lyman-a observations of the quiet M dwarf GJ 436. Predictions for the exospheric transit signature of the hot Neptune GJ 436b
The long egress of GJ 436bs giant exosphere
The Ultraviolet Radiation Environment around M dwarf Exoplanet Host Stars
The ultraviolet radiation environment in the habitable zones around low-mass exoplanet host stars
Using Ly a transits to constrain models of atmospheric escape
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2010-01-05T13:54:17Z/2010-01-05T14:42:14Z
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, Ehrenreich comma David, 2010, 'Detecting the upper atmosphere of a transiting hot Neptune: A feasibility study', 1.0, European Space Agency, https://doi.org/10.5270/esa-gcnrys0