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V632 Cyg outburst photometry Dear Colleagues, We have finished analyzing the Kyoto Dec. 12 observation. The data seem to show slow modulations (amplitude ~0.1 mag) with a time-scale of ~2 hr. The periodicity has not been confirmed because of the temporary intereference by clouds. This modulation could be a hint of emerging superhumps; since the present outburst is a long, bright one rarely seen in recent years, further intensive observations are strongly encouraged. Astrometric identification of the quiescent counterpart is in progress by Yamaoka-san. Regards, Taichi Kato VSNET Collaboration team
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