WZ Sge spectrum at Bisei Observatory K. Ayani (Bisei Astronomical Observatory) has kindly provided the following spectrum of WZ Sge taken on July 23, between 17h 39m 40s and 17h 49m 37s UT. Balmer lines are in generally absorption (likely filled with emission). More detailed analysis is under way. http://ftp.kusastro.kyoto-u.ac.jp/pub/vsnet/DNe/WZ_Sge/bisei0723.jpg The image will be later linked from the VSNET WZ Sge top page. Regards, VSNET Collaboration team