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[vsnet-campaign-dn 2525] QW Ser superhump evolution



QW Ser superhump evolution

Dear Colleagues,

    We have received new data from Tanabe-san (Okayama U. Sci.) and
Kiyota-san (Tsukuba).  The Kyoto team (observers: R. Ishioka and M. Uemura)
has been also following this superoutburst on every night.  Most recent
observations show the decrease of amplitude of superhumps to 0.15 mag.
There is also a hint of secondary superhump (phase ~0.4).  Thanks to the
favorable conditions, the present coverage is excellent.  Please continue
the present coverage (for northern observers) before the run of V4641 Sgr.

Regards,
Taichi Kato
VSNET Collaboration team

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