[vsnet-alert 9681] NSV01485: superhump period from Dubovsky's observations

[Taichi Kato]

  Pavol A. Dubovsky have provided time-resolved photometry
(a total of five nights) of NSV01485 during its September
superoutburst.  The mean superhump period is 0.07392(1) d,
which is slightly shorter than the previously reported period
by Tonny Vanmunster.  The data also show a hint of shortening
of the superhump period during the superoutburst.  This behavior
is typical for an SU UMa-type dwarf nova with this superhump
period.  Further more detailed analysis will be undertaken with
other data sets.