During the search for new variable stars some known binary systems have been observed. For the majority of them the collected data allowed to determine times of the primary or/and secondary minimum. CCD frames were reduced with a software developed for the SAVS sky survey. The minima times were computed with Kwee-van Woerden method. In total 58 times of minima were determined for 31 binary systems. The list of observed stars is given in the table below.
Full results were published in IBVS 5494 (compressed PostScript).