3D model of hydrogen atmospheric escape from HD 209458b and HD 189733b: radiative blow-out and stellar wind interactions
A Chandra/LETGS Survey of Main-sequence Stars
An extended upper atmosphere around the extrasolar planet HD209458b
Constraints on the Structure of the Heliospheric Interface Based on Ly a Absorption Spectra
CoolCAT
Disentangling Stellar and Airglow Emission Lines from Hubble Space Telescope (HST) Cosmic Origins Spectrograph (COS) Spectra
Exoplanet HD 209458b: Inflated Hydrogen Atmosphere but No Sign of Evaporation
Exoplanet HD 209458b (Osiris): Evaporation Strengthened
Fluctuations and Flares in the Ultraviolet Line Emission of Cool Stars: Implications for Exoplanet Transit Observations
Hydrogen ENA-cloud observation and modeling as a tool to study star-exoplanet interaction
Inhomogeneity within Local Interstellar Clouds
Re-visit of HST FUV Observations of the Hot-Jupiter System HD 209458: No Si III Detection and the Need for COS Transit Observations
Spectral, Spatial, and Time Properties of the Hydrogen Nebula around Exoplanet HD 209458b
Stellar Lya Emission Lines in the Hubble Space Telescope Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and Astrospheres
Ultraviolet Studies of Extra-Solar Planets
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2001-08-11T12:36:33Z/2001-10-30T19:55:46Z
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, Vidal-Madjar comma Alfred, 2002, 'HI Detection of an Extra-Solar Planetary Atmosphere', 1.0, European Space Agency, https://doi.org/10.5270/esa-bawadji
