We started tonight run on VW CrB at 12:50 (UT) at Kyoto.
We can clearly see the object on our monitor. The magnitude
looks remains at that of the last night.
In the light curve obtained last night, we see two possible
humps with an amplitude of 0.2-0.3mag. Their detailed profile
is not clear due to the bad sky condition. The nightly averaged
magnitude is declining with a rate of 0.05mag/d during July 4--8,
still keeps the very gradual decay.
Regards,
Makoto Uemura, Ryoko Ishioka, and Taichi Kato

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