activity
20132022
most citedThe size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

258 citations · 509 across the 10 of their papers we have counts for

collaborators

12 papers

astro-ph.EP20223 cited

Anticipating the DART impact: Orbit estimation of Dimorphos using a simplified model

Shantanu P. Naidu, Steven R. Chesley, Davide Farnocchia +5

We used the times of occultations and eclipses between the components of the 65803 Didymos binary system observed in its lightcurves from 2003-2021 to estimate the orbital paramete…

astro-ph.EP202011 cited

Spin Change of Asteroid 2012 TC4 probably by Radiation Torques

Hee-Jae Lee, Josef Ďurech, David Vokrouhlický +9

Asteroid 2012 TC4 is a small (10 m) near-Earth object that was observed during its Earth close approaches in 2012 and 2017. Earlier analyses of light curves revealed its exci…

astro-ph.EP2020258 cited

The size, shape, density and ring of the dwarf planet Haumea from a stellar occultation

J. L. Ortiz, P. Santos-Sanz, B. Sicardy +90

Among the four known transneptunian dwarf planets, Haumea is an exotic, very elongated, and fast rotating body. In contrast to the other dwarf planets, its size, shape, albedo, and…

astro-ph.EP2019

A satellite orbit drift in binary near-Earth asteroids (66391) 1999 KW4 and (88710) 2001 SL9 -- Indication of the BYORP effect

P. Scheirich, P. Pravec, P. Kušnirák +34

We obtained thorough photometric observations of two binary near-Earth asteroids (66391) Moshup = 1999 KW4 and (88710) 2001 SL9 taken from 2000 to 2019 and derived physical and dyn…

astro-ph.EP201918 cited

Cascade disruptions in asteroid clusters

Petr Fatka, Petr Pravec, David Vokrouhlicky

We studied asteroid clusters suggesting a possibility of at least two disruption events in their recent history (< 5 Myr). We searched for new members of known asteroid pairs and c…

astro-ph.EP201990 cited

Asteroid pairs: a complex picture

P. Pravec, P. Fatka, D. Vokrouhlický +45

We studied 93 asteroid pairs. We estimated times elapsed since separation of pair members that are between 7*10^3 and a few 10^6 yr. We derived the rotation periods for all the pri…