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[vsnet-campaign-dn 243] DM Dra analysis of Oct. 27 data



DM Dra analysis of Oct. 27 data

Dear Colleagues,

    We have finally analyzed the time-series data on DM Dra on Oct. 27,
observed by K. Matsumoto, the Kyoto team.  The observation covered 0.091 d.
There is a hint of a maximum during the early part of the observing run.
However, the amplitude of superhumps (if exists) did not much exceed 0.1
mag.  It may have been we observed the presumed superoutburst at the epoch
of decreased superhump amplitude (as was observed in V1028 Cyg).
    We would be very grateful to hear about other succesful observations,
if exists.

    The outburst was poorly covered due to the unfavorable hour angle
and altitude condition.  We hope we could more thoroughly follow the
outburst on the next (hopefully more favorable, and earlier noticed and
informed) outburst.

Regards,
Taichi Kato and Katsura Matsumoto,
VSNET Collaboration team

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