WZ Sge: Nyrola observation on July 26-27 Dear Colleagues, The Nyrola Observatory team (Moilanen) has kindly sent high-quality high-speed CCD photometry of WZ Sge last night. The light curve shows that the amplitude of early superhumps has slightly decayed, as have been seen in other WZ Sge-type superoutbursts. The profile of the early superhumps has become more structured, and there may be emerging evidence of QPOs (quasi-periodic oscillations). We are intensively analyzing all the reported data and the Kyoto data. The result will be duly reflected on the WWW light curve. Regards, Taichi Kato VSNET Collaboration team