J2329 recent light curve We have analyzed the light curve of J2329 on November 19, 20, and 21 (data from Kyoto team and Tom Krajci; 2276 points). The object keeps its very gradual decline. The period analysis yielded a shorter periodicity of 0.044590(16) d. The folded light curve show a sinusoidal and double-peak profile with an amplitude of about 0.2mag. After subtracting this periodic profiles, we found another period in the residual light curve. It is a period of 0.045935(67) d, significantly longer than that mentioned above. The averaged light curve show a fast-rise and slow-decline profile with a smaller amplitude of 0.05mag. If we consider the former and latter are originated from the orbital and superhump period, respectively, it indicates a superhump excess of 3.9% (!). Time-series observations are thus still valuable for this object. We are now having a run on this object at Kyoto under very clear sky. Regards, Makoto Uemura