Showing 1–11 of 11 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 occultationsAug 15, 2023A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS$_4$ measured from stellar occultationsSep 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 dataNov 29, 2019(704) Interamnia: A transitional object between a dwarf planet and a typical irregular-shaped minor bodyMay 20, 2019A new non-convex model of the binary asteroid (809) Lundia obtained with the SAGE modelling techniqueNov 7, 2017Against the biases in spins and shapes of asteroidsJul 24, 2017Shape and spin determination of Barbarian asteroids