activity
20102026
most citedPuzzling asteroid 21 Lutetia: our knowledge prior to the Rosetta fly-by

57 citations · 193 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.EP2026

Rotation, spectral type, and albedo of the potentially hazardous asteroid (153814) 2001 WN Prior to the 2028 June close approach

Jin Beniyama, Alexey V. Sergeyev, Konstantinos Odysseas Xenos +6

The potentially hazardous asteroid (153814) 2001 WN will pass inside the lunar distance on June 26, 2028, offering a rare opportunity to characterize a kilometer-scale near-Ear…

astro-ph.EP2025

Contact binary asteroid (153201) 2000 WO107: rotation, shape model, and density

Yurij Krugly, Oleksiy Golubov, Ihor Kyrylenko +10

We combine different methods to investigate the rotation, determine the shape and estimate the density of near-Earth asteroid (153201) 2000 WO. We carried out photometric o…

astro-ph.EP2022★ 12 cited

Asteroid phase curves using sparse Gaia DR2 data and differential dense light curves

E. Wilawer, D. Oszkiewicz, A. Kryszczyńska +10

The amount of sparse asteroid photometry being gathered by both space- and ground-based surveys is growing exponentially. This large volume of data poses a computational challenge…

astro-ph.EP2022

Observations of asteroid magnitude-phase relations at the Kharadze Abastumani Astrophysical Observatory

V. G. Shevchenko1, R. Ya. Inasaridze, Yu. N. Krugly +6

In frame of an implementation of the cooperative program studying of asteroids between the Kharadze Abastumani Astrophysical Observatory and the Astronomical Institute of V.N. Kara…

astro-ph.EP2021★ 9 cited

Photometry of selected outer main belt asteroids

V. Shevchenko, O. Mikhalchenko, I. Belskaya +17

We present new photometric observations for twelve asteroids ((122) Gerda, (152) Atala, (260) Huberta, (665) Sabine, (692) Hippodamia, (723) Hammonia, (745) Mauritia, (768) Struvea…

astro-ph.EP2019★ 17 cited

Phase integral of asteroids

Vasilij G. Shevchenko, Irina N. Belskaya, Olga I. Mikhalchenko +6

The values of the phase integral q were determined for asteroids using (i) a numerical integration of the brightness phase functions over a wide phase-angle range and (ii) the rela…