Abstract
Abstract Visual (BV) light curves of the RS CVn type binary system SZ Psc are presented. The light curves show a period change towards decreasing phases. New parameters for the system are found based on an analysis of the observed light curves using a Djuraŝevic's inverseproblem method. The observed light curves of SZ Psc, in both observational bands, can be successfully interpreted within the Roche model with three spotted areas on the surface of the more massive component. Characteristics of the spots and a genera discussion of the observed light curves and the results are given.
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