Showing 41–60 of 172 results
/ Date/ Name
Mar 16, 2004Atmospheric Escape from Hot JupitersJul 8, 2013An HST Optical to Near-IR Transmission Spectrum of the Hot Jupiter WASP-19b: Detection of Atmospheric Water and Likely Absence of TiOAug 9, 2013Hubble Space Telescope hot Jupiter Transmission Spectral Survey: detection of water in HAT-P-1b from Wide Field Camera 3 near-infrared spatial scan observationsDec 7, 2001Deuterium abundance toward G191-B2B: Results from the Far Ultraviolet Spectroscopic Explorer (FUSE) MissionApr 30, 2008Molecular hydrogen in the circumstellar environments of Herbig Ae/Be stars probed by FUSEMay 5, 2008Rayleigh scattering by H2 in the extrasolar planet HD209458bJun 22, 2017MOVES I. The evolving magnetic field of the planet-hosting star HD189733Nov 11, 2025HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426Sep 4, 2024The K2-24 planetary system revisited by CHEOPSSep 5, 2024TOI-3568 b: a super-Neptune in the sub-Jovian desertMay 2, 2025Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emissionJul 8, 2024Characterisation of the Warm-Jupiter TOI-1130 system with CHEOPS and photo-dynamical approachJan 23, 2012Evaporation of extrasolar planetsJul 12, 2023Investigating the visible phase-curve variability of 55 Cnc eSep 7, 2022The EBLM project -- IX. Five fully convective M-dwarfs, precisely measured with CHEOPS and TESS light curvesDec 29, 2010The upper atmosphere of the exoplanet HD209458b revealed by the sodium D lines: Temperature-pressure profile, ionization layer, and thermosphereFeb 28, 2011Hubble Space Telescope Transmission Spectroscopy of the Exoplanet HD 189733b: High-altitude atmospheric haze in the optical and near-UV with STISNov 21, 2023Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valleyJan 18, 2023The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPSMar 10, 2010Evaporation of the planet HD189733b observed in HI Lyman-alpha