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[vsnet-alert 1459] Fading of SBS 1017+533

Fading of SBS 1017+533

    The report from the Ouda team (D. Nogami) indicates that the newly
identifed SU UMa-type dwarf nova SBS 1017+533 is fading rapidly.
Observations are highly recommended during the terminal stage of the current
superoutburst.

  YYMMDD(UT)   mag  observer
  980128.812   127  (T. Kinnunen)
  980128.867   129  (T. Kinnunen)
  980129.208   129  (T. Kinnunen)
  980131.855   134  (T. Kinnunen)
  980131.903   133  (T. Kinnunen)
  980131.932   133  (T. Kinnunen)
  980201.190   133  (T. Kinnunen)
  980201.785   136  (T. Kinnunen)
  980201.887   136  (T. Kinnunen)
  980202.701  13.45V  (Ouda team)
  980202.833   133  (G. Poyner)
  980203.642   130  (T. Watanabe)
  980203.685  13.60V  (Ouda team)
  980203.866   136  (G. Poyner)
  980205.703  14.38V  (Ouda team)
  980206.657  15.97V  (Ouda team)

Regards,
Taichi Kato

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