F. Manzini

TL;DR: In this article, the authors used a large-scale dataset of optical data from more than 100 observers who submittheir optical data to publicly available databases and derived 3D shape models of asteroids together with their rotation periods and orientations of rotation axes.

TL;DR: In this paper, the authors used disk-integrated optical data (i.e., classical dense-intime photometry obtained from public databases and through a large collaboration network as well as sparse-in-time individual measurements from a few sky surveys) as an input for the convex inversion method, and derived 3D shape models of asteroids, together with their rotation periods and orientations of rotation axes.

TL;DR: In this paper, the authors studied a sample of 93 asteroid pairs, i.e., pairs of genetically related asteroids that are on highly similar heliocentric orbits, and derived the absolute magnitude differences of the studied asteroid pairs that provided their mass ratios q.

TL;DR: In this article, a photometric study of the main-belt binary C-type asteroid 121 Hermione, performed during its 2007 opposition, was performed using the rare observational opportunity of one of the annual equinoxes of Hermione occurring close to its opposition in June 2007.

TL;DR: In this paper, the authors present evidence that four minor planets of the main belt are binary systems based on CCD photometric measurements made by many observers coordinated in a network of observatories.