M. Lehký

TL;DR: In this article, the authors used sparse photometry from selected observatories from the AstDyS database (Asteroids- Dynamic Site), either alone or in combination with dense lightcurves, to determine new asteroid models by the lightcurve inversion method.

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 article, the authors present a shape model and bulk density of an interloper in the Eos family, based on the disk-resolved data obtained by the Near InfraRed Camera (Nirc2) mounted on the W.M. Keck II telescope.