New Asteroid Models Based on Combined Dense and Sparse Photometry

Details New Asteroid Models Based on Combined Dense and Sparse Photometry New Asteroid Models Based on Combined Dense and Sparse Photometry

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010dps....42.3915h&link_type=abstract

American Astronomical Society, DPS meeting #42, #39.15; Bulletin of the American Astronomical Society, Vol. 42, p.1035

Astronomy and Astrophysics

Astronomy

1

Scientific paper

For thousands of asteroids we investigated several ten thousands of sparse photometric data from astrometric projects. These data are available on AstDyS server (Asteroids -- Dynamic Site, http://hamilton.dm.unipi.it). We picked 7 astrometric surveys and used their calibrated photometry in lightcurve inversion method for determination of asteroid's convex shapes and rotational states. We present nearly 100 new asteroid models derived from combined dense and sparse data sets, where sparse photometry is taken from AstDyS server and dense lightcurves are from the Uppsala Asteroid Photometric Catalogue (UAPC) and from several individual observers.

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