ACCESS and LRG-BEASTS: A Precise New Optical Transmission Spectrum of the Ultrahot Jupiter WASP-103b
Assessing spectra and thermal inversions due to TiO in hot Jupiter atmospheres
Five Key Exoplanet Questions Answered via the Analysis of 25 Hot-Jupiter Atmospheres in Eclipse
Global Climate and Atmospheric Composition of the Ultra-hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations
Near-infrared Emission Spectrum of WASP-103b Using Hubble Space Telescope/Wide Field Camera 3
On Spectroscopic Phase-curve Retrievals: H2 Dissociation and Thermal Inversion in the Atmosphere of the Ultrahot Jupiter WASP-103 b
The Atmospheric Circulation of Ultra-hot Jupiters
Thermal emission from the hot Jupiter WASP-103 b in J and Ks bands
Instrument
WFC3, WFC3/IR
Temporal Coverage
2015-06-15T16:55:26Z/2015-06-17T20:34:18Z
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, Zhao comma Ming, 2016, 'Near-IR spectroscopy of the newly discovered benchmark hot Jupiter WASP-103b', 1.0, European Space Agency, https://doi.org/10.5270/esa-85b9lap