QW Ser superhump evolution Dear Colleagues, We have received new data from Tanabe-san (Okayama U. Sci.) and Kiyota-san (Tsukuba). The Kyoto team (observers: R. Ishioka and M. Uemura) has been also following this superoutburst on every night. Most recent observations show the decrease of amplitude of superhumps to 0.15 mag. There is also a hint of secondary superhump (phase ~0.4). Thanks to the favorable conditions, the present coverage is excellent. Please continue the present coverage (for northern observers) before the run of V4641 Sgr. Regards, Taichi Kato VSNET Collaboration team