We performed time-series photometry on VW CrB in the long outburst
last night at Kyoto. The light curve clearly shows a superhump with an
amplitude of about 0.3mag. This confirms the current outburst is a
genuine superoutburst and it is still ongoing. The light curve sometimes
breaks by clouds, but the hump seems to have a single peak, a typical
profile.
Regards,
Makoto Uemura, Ryoko Ishioka, and Taichi Kato
vsnet-adm@kusastro.kyoto-u.ac.jp