0.94-2.42 mm Ground-based Transmission Spectra of the Hot Jupiter HD-189733b
A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion
A large range of haziness conditions in hot-Jupiter atmospheres
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
Limb darkening laws for two exoplanet host stars derived from 3D stellar model atmospheres. Comparison with 1D models and HST light curve observations
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
Probing the extreme planetary atmosphere of WASP-12b
Probing the haze in the atmosphere of HD 189733b with Hubble Space Telescope/WFC3 transmission spectroscopy
Spatially resolved spectroscopy across stellar surfaces. III. Photospheric Fe I lines across HD 189733A (K1 V)
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
Unveiling cloudy exoplanets: the influence of cloud model choices on retrieval solutions
Instrument
STIS/CCD, WFC3, WFC3/IR
Temporal Coverage
2009-11-20T03:08:06Z/2010-11-10T08:00:47Z
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, Pont et al., 2011, 'A Complete Optical and NIR Atmospheric Transmission Spectrum of the Exoplanet HD189733b', 1.0, European Space Agency, https://doi.org/10.5270/esa-3v5he4o