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[vsnet-j 1266] SBS 1017+533

SBS 1017+533

　多分スーパーです。非常によい観測条件です（天候を除けば・・）

   As reported by Gary Poyner, the SU UMa-type dwarf nova SBS 1017+533
is undergoing a likely superoutburst.  The last superoutburst was reported
in 2000 September-October, which was not well observed because of the
poor location in the sky.  The current outburst seems to provide an
excellent opportunity to study this dwarf nova in detail.  Follow-up
time-resolved photometry is strongly recommended.

  YYYYMMDD(UT)   mag  observer
  20010410.849  <146  (T. Kinnunen)
  20010416.969   158: (G. Poyner)
  20010418.960   159  (G. Poyner)
  20010420.910   159  (G. Poyner)
  20010423.908  <156  (G. Poyner)
  20010424.921   161  (G. Poyner)
  20010425.913   162: (G. Poyner)
  20010428.869  <143  (T. Kinnunen)
  20010428.914  <156  (G. Poyner)
  20010429.913  <151  (G. Poyner)
  20010430.913  <147  (G. Poyner)
  20010506.917  <146  (G. Poyner)
  20010507.906  <151  (G. Poyner)
  20010512.928  <156  (G. Poyner)
  20010516.953   159  (G. Poyner)
  20010519.996   160  (G. Poyner)
  20010521.987  <151  (G. Poyner)
  20010523.008  <156  (G. Poyner)
  20010523.926  <156  (G. Poyner)
  20010528.935   130  (G. Poyner)

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