WZ Sge: time-resolved spectra H. Baba provided an image of spectra taken by Dr. K. Sadakane at Okayama Astrophysical Observatory on July 24. The spectra can now be seen in VSNET WZ Sge web page: http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/DNe/wzsge01.html In these figure, double peak emission lines of He II 4686 and C III/N III blend are clearly seen. We can see the variations of their profiles. More detailed information will be presented by H. Baba. Regards, VSNET collaboration team