Showing 1–20 of 23 results
/ Date/ Name
Sep 15, 2009Misaligned spin and orbital axes cause the anomalous precession of DI HerculisApr 15, 2013Detection of carbon monoxide in the high-resolution day-side spectrum of the exoplanet HD 189733bSep 23, 2021The 12CO/13CO isotopologue ratio of a young, isolated brown dwarf. Possibly distinct formation pathways of super-Jupiters and brown dwarfsMay 23, 2013Search for Rayleigh scattering in the atmosphere of GJ1214bJun 30, 2016The slow spin of the young sub-stellar companion GQ Lupi b and its orbital configurationSep 25, 2024The ESO SupJup Survey III: Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+Oct 8, 2021Characterizing the protolunar disk of the accreting companion GQ Lupi BOct 5, 2021Measuring titanium isotope ratios in exoplanet atmospheresMar 19, 2019Spectroscopic Transit Search: a self-calibrating method for detecting planets around bright starsJan 12, 2023Observability of silicates in volatile atmospheres of super-Earths and sub-NeptunesJun 22, 2010The orbital motion, absolute mass, and high-altitude winds of exoplanet HD209458bJul 6, 2000The GHz-Peaked Spectrum radio galaxy 2021+614: Detection of slow motion in a compact symmetric objectApr 8, 2009The changing phases of extrasolar planet CoRoT-1bMar 11, 2020A weak spectral signature of water vapour in the atmosphere of HD 179949 b at high spectral resolution in the L-bandSep 8, 2020Diffraction-limited integral-field spectroscopy for extreme adaptive optics systems with the Multi-Core fiber-fed Integral-Field UnitAug 24, 2022Transmission spectroscopy of the ultra-hot Jupiter MASCARA-4 b: Disentangling the hydrostatic and exospheric regimes of ultra-hot JupitersFeb 18, 2020No Massive Companion to the Coherent Radio-Emitting M Dwarf GJ 1151Jan 8, 2019Testing the Detectability of Extraterrestrial $\mathrm{O}_2$ with the ELTs using Real Data with Real NoiseDec 7, 2018Ground-based detection of an extended helium atmosphere in the Saturn-mass exoplanet WASP-69bNov 20, 2020Is TiO emission present in the ultra-hot Jupiter WASP-33b? A reassessment using the improved ExoMol Toto line list