A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
A large range of haziness conditions in hot-Jupiter atmospheres
A Model of the Ha and Na Transmission Spectrum of HD 189733b
Combining low- to high-resolution transit spectroscopy of HD 189733b. Linking the troposphere and the thermosphere of a hot gas giant
Constraining the Atmospheric Composition of the Day-Night Terminators of HD 189733b: Atmospheric Retrieval with Aerosols
H2O abundances and cloud properties in ten hot giant exoplanets
Hubble Space Telescope transmission spectroscopy of the exoplanet HD 189733b: high-altitude atmospheric haze in the optical and near-ultraviolet with STIS
PLATON II: New Capabilities and a Comprehensive Retrieval on HD 189733b Transit and Eclipse Data
Probing the atmosphere of HD189733b with the Na I and K I lines
Spatially resolved spectroscopy across stellar surfaces. III. Photospheric Fe I lines across HD 189733A (K1 V)
Temperature-pressure profile of the hot Jupiter HD 189733b from HST sodium observations: detection of upper atmospheric heating
The Importance of Optical Wavelength Data on Atmospheric Retrievals of Exoplanet Transmission Spectra
The prevalence of dust on the exoplanet HD 189733b from Hubble and Spitzer observations
The widest broadband transmission spectrum (0.38-1.71 mm) of HD 189733b from ground-based chromatic Rossiter-McLaughlin observations
Instrument
STIS/CCD
Temporal Coverage
2009-10-31T03:50:46Z/2010-11-30T07:17:14Z
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, Sing et al., 2011, 'Charaterizing Atmospheric Sodium in the Transiting hot-Jupiter HD189733b', 1.0, European Space Agency, https://doi.org/10.5270/esa-xl0d9va