40 citations · 93 across the 4 of their papers we have counts for
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Distribution of shape elongations of main belt asteroids derived from Pan-STARRS1 photometry
H. Cibulková, H. Nortunen, J. Ďurech +10
Context. A lot of photometric data is produced by surveys such as Pan-STARRS, LONEOS, WISE or Catalina. These data are a rich source of information about the physical properties of…
Spin states of asteroids in the Eos collisional family
J. Hanuš, M. Delbo', V. Alí-Lagoa +33
Eos family was created during a catastrophic impact about 1.3 Gyr ago. Rotation states of individual family members contain information about the history of the whole population. W…
Shape and spin distributions of asteroid populations from brightness variation estimates and large databases
H. Nortunen, M. Kaasalainen, J. Ďurech +3
Context. Many databases on asteroid brightnesses (e.g. ALCDEF, WISE) are potential sources for extensive asteroid shape and spin modelling. Individual lightcurve inversion models r…
A six-part collisional model of the main asteroid belt
Helena Cibulková, Miroslav Brož, Paula G. Benavidez
In this work, we construct a new model for the collisional evolution of the main asteroid belt. Our goals are to test the scaling law of Benz and Asphaug (1999) and ascertain if it…