WZ Sge: slowly re-brightening The Kyoto observation last night (Ishioka et al.) shows the object becomes 0.05mag brighter than August 19, which indicates that the the rate of re-brightening is quite gradual. In the last night light curve, we can see a hump with an amplitude of about 0.35mag. Follow-up observations are encouraged! Regards, Makoto Uemura VSNET Collaboration team