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We have obtained CCD photometry in 2010-11 of V963 Per (=GSC3355 0394), whichis a recently identified close binary star with unequal eclipse depths. Theseven new eclipse timings yield an improved ephemeris, but we caution thatsecondary eclipse can be affected by variation of the light curve. Thisvariation seems to be on a monthly timescale at the few percent level.

New light curves and ephemeris for the close eclipsing binary V963 PER