Showing 1–20 of 24 results
/ Date/ Name
Aug 19, 2025Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267May 14, 2025Asteroid sizes determined with thermophysical model and stellar occultationsApr 25, 2025A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771Jun 3, 2024CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operationsApr 4, 2024Multi-purpose InSTRument for Astronomy at Low-resolution: MISTRAL@OHPOct 27, 2023Physical properties of Centaur (60558) 174P/Echeclus from stellar occultationsAug 15, 2023A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS$_4$ measured from stellar occultationsSep 6, 2022Two temperate super-Earths transiting a nearby late-type M dwarfJan 25, 2022Constraints on the structure and seasonal variations of Triton's atmosphere from the 5 October 2017 stellar occultation and previous observationsSep 1, 2021Properties of slowly rotating asteroids from the Convex Inversion Thermophysical ModelSep 9, 2020A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266Jun 24, 2020TRAPPIST-1: Global Results of the Spitzer Exploration Science Program {\it Red Worlds}Mar 12, 2020Three Short Period Jupiters from TESSNov 29, 2019(704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor bodyJun 2, 2019Two new HATNet hot Jupiters around A stars, and the first glimpse at the occurrence rate of hot Jupiters from TESSMar 6, 2019Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016Dec 21, 2018The discovery of WASP-134b, WASP-134c, WASP-137b, WASP-143b and WASP-146b: three hot Jupiters and a pair of warm Jupiters orbiting Solar-type starsSep 11, 2017The Castalia Mission to Main Belt Comet 133P/Elst-PizarroMay 30, 2017The 67P/Churyumov-Gerasimenko observation campaign in support of the Rosetta missionFeb 5, 2016The dust environment of comet 67P/Churyumov-Gerasimenko from Rosetta OSIRIS and VLT observations in the 4.5 to 2.9 au heliocentric distance range inbound