We have performed preliminary analysis of observations last night at Ouda. We have obtained over 6000 images with integration time of 1-2s. The object is rapidly fading with 1.1mag/d. There are humps with amplitudes of about 0.1mag and a period near the superhump period. The QPOs of 3-5 minutes have again become strong, which is very similar to the previously reported one during the rapid fading phase from the rebrightening. Regards, Makoto Uemura