Showing 1–12 of 12 results
/ Date/ Name
Sep 18, 2025A high geometric albedo and small size of the Haumea cluster member (24835) 1995 SM55 from a stellar occultation and photometric observationsMay 14, 2025Asteroid sizes determined with thermophysical model and stellar occultationsOct 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 occultationsMay 25, 2022The multichord stellar occultation on 2019 October 22 by the trans-Neptunian object (84922) 2003 VS$_2$Jan 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 ModelDec 11, 2020The 2017 May 20$^{\rm th}$ stellar occultation by the elongated centaur (95626) 2002 GZ$_{32}$Jun 4, 2020The size, shape, density and ring of the dwarf planet Haumea from a stellar occultationMay 18, 2020The large Trans-Neptunian Object 2002 TC$_{302}$ from combined stellar occultation, photometry and astrometry dataMar 6, 2019Pluto's lower atmosphere and pressure evolution from ground-based stellar occultations, 1988-2016Dec 17, 2018Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle