V632 Cyg time-series photometry Dear Colleagues, The Kyoto team obtained time-series photometry of V632 Cyg last night (observers: M. Uemura and R. Ishioka). We have reduced initial 0.05-d part. The resultant light curve is relatively flat, without a clear indication of superhump-type modulations. We will proceed to reduce the remaining images, in order to check any variability was detected. Regards, Taichi Kato VSNET Collaboration team
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