Light curve analysis of main belt asteroids 4747, 5255, 11411, 15433, 17866
Eglitis, Ilgmars; Kristers, Nagainis
Latvia
Abstract
The main belt asteroids 4747, 5255, 11411, 15433, and 17866 were studied at the Baldone Astrophysical Observatory in the time span range 2018-2022. The obtained light curve data together with published Minor Planet Center data are analyzed with Fourier series, Lomb-Scargle periodogram, and phase dispersion minimization methods. A plan of analysis is given. The results computed from different observatories' data are compared, and mean-weighted periods are obtained.