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Greetings, Well, at Aug 20.3 to 20.5 the star seemed to be varying between 13.1 and 13.6 based on Arne's values for the close companion star. The mean value might have faded a few percent over that interval. But the eclipses and superhumps looked good. Regards, Stan ----- Original Message ----- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp> To: <vsnet-alert@kusastro.kyoto-u.ac.jp>; <vsnet-campaign-dn@kusastro.kyoto-u.ac.jp>; <vsnet-superoutburst@kusastro.kyoto-u.ac.jp> Sent: Tuesday, August 21, 2001 2:22 PM Subject: [vsnet-superoutburst 723] WZ Sge: rebrightening, more analysis > WZ Sge: rebrightening, more analysis > > Dear Colleagues, > > We have received additional high-quaility data from B. Martin. > Combined with the previous data, and the new analysis of Kyoto data, > there seems to have been a minimum of brightness in early Aug. 20 (UT). > The object has a more rapid brightening trend during the latter half > of Aug. 20. This may be an indication of an immediate full rebrightening. > Please keep the closest watch!! > > The profiles of eclipses vary, but the sharp, deep eclipses are > present throughout this brightening phase. > > More detailed analysis, and Web update, will be presented later > by Uemura-san. > > Regards, > Taichi Kato > VSNET Collaboration team > >
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