[vsnet-alert 22750] KIS J192651.94+503301.7: superhump period

[Taichi Kato]

KIS J192651.94+503301.7: superhump period

   The superhump period during the main superoutburst
was 0.06227(1) d (stage B).  There was a relatively
long phase of stage A (nearly 50 cycles).
The superhump period is typical for a WZ Sge-type
dwarf nova with multiple rebrightenings.

Observers: Tonny Vanmunster, Tamas Tordai, Ian Miller,
Crimean Astrophys. Obs., Geoff Stone, Itoh-san
and Stephen Brincat,