The NEO Physical Observations and Properties Simulation (NEOPOPS) project
Simone Ieva(Astronomical Observatory of Rome), the NEOPOPs team, Petr Pravec(Czech Academy of Sciences, Astronomical Institute), Juan Luis Cano(Planetary Science Institute), E. Dotto(Astronomical Observatory of Rome), Maxime Devogèle, Elena Mazzotta Epifani(National Institute for Astrophysics), Jules Bourdelle de Micas(National Institute for Astrophysics), S. Bagnulo(Armagh Observatory & Planetarium), Monica Lazzarin(Osservatorio Astronomico di Padova), M. A. Barucci(Centre National de la Recherche Scientifique)
Cited by 0
Related Papers
The operational environment and rotational acceleration of asteroid (101955) Bennu from OSIRIS-REx observations
|Nature Communications|2019|903
The impact and recovery of asteroid 2008 TC3
|Nature|2009|376
Dust measurements in the coma of comet 67P/Churyumov-Gerasimenko inbound to the Sun
|Science|2015|362
OSIRIS – The Scientific Camera System Onboard Rosetta
|Space Science Reviews|2007|334
Evidence for widespread hydrated minerals on asteroid (101955) Bennu
|Nature Astronomy|2019|333