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[vsnet-campaign 399] SY Vol still bright

SY Vol still bright

   The likely large-amplitude dwarf nova SY Vol is still bright according
to observations by Rod Stubbings.  If this star is an SU UMa-type dwarf nova,
the present outburst should be a superoutburst.  Time-resolved photometry
is very strongly encouraged.  Follow-up information will be provided
in vsnet-campaign and vsnet-campaign-dn.

  YYYYMMDD(UT)   mag  observer
  20000723.492   142  (R. Stubbings)
  20000723.533   142  (R. Stubbings)
  20000724.514   140  (R. Stubbings)
  20000724.551   140  (R. Stubbings)
  20000724.585   140  (R. Stubbings)
  20000727.480   144  (R. Stubbings)

Regards,
Taichi Kato

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