We performed a time-series observation of this new SU UMa-type
dwarf nova on October 30, in the post-superoutburst phase. The light
curve shows a possible humps whose phase seems to be further shifted
compared with that on October 29. The object was 0.35mag fainter than
that observed on October 29. Our last night run is now under reduction.
Regards,
Makoto Uemura

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