[vsnet-outburst 23047] CS Ind superoutburst continues

[Taichi Kato]

CS Ind superoutburst continues

   Time-series photometry is of course still highly
desired.  A superoutburst in an object above the period
gap may last shorter (due to the weak 3:1 resonance),
and intensive observations at this moment is very
much needed before it starts fading rapidly.

  YYYYMMDD(UT)   mag  observer
  20181110.494   169  (Rod Stubbings)
  20181115.624   121  (Rod Stubbings)
  20181116.494   119  (Rod Stubbings)
  20181125.469   151  (Rod Stubbings)
  20181128.478   123  (Rod Stubbings)
  20181129.458   123  (Rod Stubbings)
  20181130.485   124  (Rod Stubbings)
  20181130.501   121  (Rod Stubbings)
  20181130.515   124  (Rod Stubbings)
  20181130.519   121  (Rod Stubbings)
  20181130.521   121  (Rod Stubbings)
  20181130.524   121  (Rod Stubbings)
  20181130.526   121  (Rod Stubbings)
  20181130.528   121  (Rod Stubbings)
  20181130.530   122  (Rod Stubbings)
  20181130.532   124  (Rod Stubbings)
  20181130.533   121  (Rod Stubbings)
  20181130.535   124  (Rod Stubbings)
  20181130.539   124  (Rod Stubbings)
  20181130.540   121  (Rod Stubbings)
  20181130.542   124  (Rod Stubbings)
  20181130.542   121  (Rod Stubbings)
  20181130.544   124  (Rod Stubbings)
  20181130.546   124  (Rod Stubbings)
  20181130.548   121  (Rod Stubbings)
  20181130.549   122  (Rod Stubbings)
  20181130.550   124  (Rod Stubbings)
  20181130.553   123  (Rod Stubbings)
  20181130.556   123  (Rod Stubbings)
  20181202.481   126  (Rod Stubbings)
  20181202.533   124  (Rod Stubbings)
  20181205.483   127  (Rod Stubbings)