Santos-Sanz, P; Ortiz, JL; Sicardy, B; Popescu, M; Benedetti-Rossi, G; Morales, N; Vara-Lubiano, M; Camargo, JIB; Pereira, CL; Rommel, FL; Assafin, M; Desmars, J; Braga-Ribas, F; Duffard, R; Oliveira, JM; Vieira-Martins, R; Fernandez-Valenzuela, E; Morgado, BE; Acar, M; Anghel, S; Atalay, E; Ates, A; Bakis, H; Bakis, V; Eker, Z; Erece, O; Kaspi, S; Kayhan, C; Kilic, SE; Kilic, Y; Manulis, I; Nedelcu, DA; Niaei, MS; Nir, G; Ofek, E; Ozisik, T; Petrescu, E; Satir, O; Solmaz, A; Sonka, A; Tekes, M; Unsalan, O; Yesilyaprak, C; Anghel, R; Curelaru, L; Danescu, C; Dumitrescu, V; Gherase, R; Hudin, L; Stoian, AM; Tercu, JO; Truta, R; Turcu, V; Vantdevara, C; Belskaya, I; Dementiev, TO; Gazeas, K; Karampotsiou, S; Kashuba, V; Kiss, C; Koshkin, N; Kozhukhov, OM; Krugly, Y; Lecacheux, J; Pal, A; Szakats, R; Zhukov, V; Bamberger, D; Mondon, B; Pratt, A; Schnabel, C; Selva, A; Teng, JP; Tigani, K; Tsamis, V; Weber, C; Wells, G; Kalkan, S; Kudak, V; Marciniak, A; Ogloza, W; Ozdemir, T; Pakstiene, E; Perig, V; Zejmo, M; Puskullu, C
(2022)
Context. As part of our international program aimed at obtaining accurate physical properties of trans-Neptunian objects (TNOs), we predicted a stellar occultation by the TNO (38628) Huya of the star Gaia DR2 4352760586390566400 ...