High speed BVR(I)C photometry of the short period RS CVn binary SV Cam is presented. Its light curve is asymmetric with a depression of brightness by 0.04-0.05 mag after the primary eclipse. Good fit of the synthetic light curve to the observational data in all colors can be obtained assuming presence of two cool spots with equal angular sizes of 20° and temperatures 4350 K located at middle latitude above and below the stellar equator on opposite hemispheres of the primary star.
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