WZ Sge: rapid fading and hump structure Dear Colleagues, The analysis of the combined data on Aug. 17 (B. Martin, partially analyzed Kyoto, J. Pietz) has shown the following new features: 1) During the early decline stage, the humps have became smaller in amplitude and complex 2) Later on, early half of the Kyoto data shows little evidence of eclipses! Humps have become even less apparent, and the light curve looks rather flat, except for small-scale fluctuations. 3) Later in Pietz's observations, a new sharp hump structure emerged. The humps have an orbital phase of 0.35-0.4, which is ~0.5 different from the giant humps seen on Aug. 16. This feature may be "late superhumps" finally! Eclipses are not very evident We will further analyze the data. Please continue your observations as long as possible, and keep everyone continuously informed! Regards, Taichi Kato VSNET Collaboration team