Distribution of spin-axes longitudes and shape elongations of main-belt asteroids

@article{Cibulkova2016DistributionOS,
  title={Distribution of spin-axes longitudes and shape elongations of main-belt asteroids},
  author={H. Cibulkov'a and J. vDurech and D. Vokrouhlick'y and M. Kaasalainen and D. Oszkiewicz},
  journal={Astronomy and Astrophysics},
  year={2016},
  volume={596}
}
Context. Large all-sky surveys provide us with a lot of photometric data that are sparse in time (typically a few measurements per night) and can be potentially used for the determination of shapes and rotational states of asteroids. The method generally used to derive these parameters is the light curve inversion. However, for most asteroids their sparse data are not accurate enough to derive a unique model and the light curve inversion method is thus not very efficient. Aims. To fully utilize… Expand
Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry
Spin states of asteroids in the Eos collisional family
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