Physical models of ten asteroids from an observers' collaboration network

@article{urech2007PhysicalMO,
  title={Physical models of ten asteroids from an observers' collaboration network},
  author={Josef Ďurech and Mikko Kaasalainen and Anna Marciniak and William H. Allen and Raoul Behrend and Colin Bembrick and Thomas C Bennett and Laurent Bernasconi and J{\'e}r{\^o}me Berthier and Greg Bolt and Salahi Boroumand and L. Crespo da Silva and Roberto Crippa and Martin Crow and Russell I. Durkee and Roger Dymock and M. Fagas and Michael Helmut Fauerbach and St{\'e}phane Fauvaud and Merideth Frey and Rui Soles Gonçalves and R. Hirsch and D. Jardine and Krzysztof Kamiński and Robert A. Koff and Tomasz Kwiatkowski and Angel F. Lopez and Federico Manzini and Tadeusz Michałowski and Robert Pacheco and Margaret Pan and Frederick Pilcher and R. Poncy and Donald P. Pray and Wojtek Pych and R. Roy and Guido E Santacana and Stephen M. Slivan and Stefano Sposetti and R. David Stephens and Brian D. Warner and Marek Wolf},
  journal={Astronomy and Astrophysics},
  year={2007},
  volume={465},
  pages={331-337}
}
Aims. We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network of observers that will be of extreme importance for future all-sky asteroid photometric surveys. Methods. The lightcurve inversion method was used to derive spin states and shape models of the asteroids. Results. We derived spin states and shape model for ten new asteroids… 
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