As reported in [vsnet-campaign-dn 542], we performed time-series photometry on February 26 at Kyoto, and detected two superhumps in our four-hour run. The amplitude keeps at 0.3mag. Using the data taken by the Kyoto team and J. Pietz since February 24, the best candidate of the superhump period can be calculated to be 0.08535 +/- 0.00014 day. The average magnitudes has not significantly been changed since February 24. Just now we have finished tonight run on CP Dra at Kyoto. Three hours data will be available. Regards, Makoto Uemura