WZ Sge: fading from the 12-th rebrighteng, Ouda and Kyoto observation Dear Colleagues, The rapid fading from the 12-th rebrightening has been confirmed both in Ouda (observer M. Uemura) and Kyoto (observer R. Ishioka) observations. The preliminary magnitude on Sep. 13.5 UT is comparable to that on Sep. 11.5 UT, the minimum after the 11-th rebrightening. The speed of decline is also comparable to that of the fading from the 11-th rebrightening. We have also confirmed that the hump structure was also present during the maximum of the 12-th rebrightening. There also seems to be a hint of QPO signals. Further analysis is in progress, and we encourage intensive observations of this very important stage of the outburst. Regards, Taichi Kato VSNET Collaboration team