WZ Sge: fading from the 8-th rebrightening Dear Colleagues, We have received new data from D. Starkey, and added new data from Ouda observation (observer M. Uemura) and Kyoto observatin (observer R. Ishioka). Starkey's data between Sep. 5.05 and 5.21 clearly show the fading trend, as was observed during the 7-th rebrighetening. The overall behavior of the 8-th rebeightening is similar to the 7-th rebrightening, except for remarkable changes in the hump and eclipse profiles. The flat maximum (or the outburst duty cycle) seems to have become longer in recent rebrightenings. The star may be around maximum of the 9-th rebrightening now (?) Time-series analysis will be presented later. Regards, Taichi Kato VSNET Collaboration team