WZ Sge: eclipse and superhump structure Dear Colleagues, The analysis of the Aug. 10-11 data (B. Martin, Kyoto, G. Masi) using the same technique as in [vsnet-alert 6251] shows the persistence of a shallow dip (0.04 mag) at the predicted phase of eclipses. The hump features reported in [vsnet-alert 6251] have moved with respect to the orbital phase -- they are not therefore associated with the early superhumps, but are moving superhumps with complex multiple peaks. More detailed analysis is in progress. Regards, Taichi Kato VSNET Collaboration team