Dear colleagues, I have just uploaded the August 21/22 light curve of WZ Sge, that I obtained at CBA Belgium Observatory, to my web site (see address below). It was not a particularly favourable photometric night, hampered also by low clouds. I nevertheless managed to collect a dense time-series, over a period of about 6 hours. The resulting light curve clearly shows a number of interesting features. First, the rebrightening of WZ Sge, which was still very obvious in the hours preceding our observations, seems to have come to an end. The superhumps are much smaller than in any of our previous observing nights, having an amplitude of \'barely\' 0.06 mag. In between superhumps, there are a number of dips. The most pronounced dip (the one immediately preceding the superhump peaks) likely is to be attributed to eclipses. Best regards, Tonny Vanmunster CBA Belgium Observatory http://vsnet.lunarpages.com/cbabelgium ------------------------------------------------------------------ This mail sent through Wanadoo WebMail: http://webmail.wanadoo.be/