ИСТИНА

Time series analysis of multicolour CCD photometry of a new WZ Sge‐type dwarf nova V466 And, discovered during its superoutburst in September 2008, revealed the early superhumps, with the period 0.056383 d in the first 11 days, the ordinary superhumps with the period 0.05713 d in the days 13–23 and late superhumps, with unstable period of about 0.056 d in the days 24–33 of the superoutburst. Thereafter, the dwarf nova returned to its pre‐outburst state.