Differential Photometry of Asteroids 314, 2271, 2544, 3028, 3687, 23481 and 2002 NY40

Details Differential Photometry of Asteroids 314, 2271, 2544, 3028, 3687, 23481 and 2002 NY40 Differential Photometry of Asteroids 314, 2271, 2544, 3028, 3687, 23481 and 2002 NY40

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...20114105d&link_type=abstract

American Astronomical Society Meeting 201, #141.05; Bulletin of the American Astronomical Society, Vol. 35, p.567

Astronomy and Astrophysics

Astronomy

Scientific paper

Using the Stull Observatory .82m Austin-Fellows telescope, from May 2002 to August 2002, we observed several asteroids to measure their rotation periods or put a limit on the amplitude of thier change in magnitude. We used ensemble photometry to extract the asteroids' intrinsic variations from the irregular variations in sky transparency. We will present results for (2271) Kiso, (3028) Zhangguoxi, (314) Rosalia, (3687) Dzus,(23481) 1991 GT4, (2544) Gubarev and the Near Earth Asteroid 2002 NY40. Most of these targets are members of dynamical families.

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