[vsnet-outburst 7337] OT_J102146.4+234926 post-dip outburst continues

[Taichi Kato]

   The WZ Sge-type plateau after rebrightening continues without
noticeable outburst structure (unlike WZ Sge).  The reported
time-resolved photometry has shown the presence of superhumps
(the phase analysis suggests the interpretation of late
superhumps).

   More analysis will be presented by Uemura-san.

  YYYYMMDD(UT)   mag  observer
  20061028.512  139V  (Catalina Sky Survey)
  20061117.535  144V  (Catalina Sky Survey)
  20061121.490  145C  (Tom Krajci)
  20061121.704  14.48V  (Hiroyuki Maehara)
  20061121.834  14.420C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061127.813  16.036C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061128.834  14.840C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061129.810  14.884C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061130.873  14.546C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061201.768  14.597C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061203.814  14.79C  (Kazuhiro Nakajima)
  20061204.717  14.616C  (Higashi-Hiroshima Observatory (Hiroshima Univ.))
  20061204.819  14.78C  (Kazuhiro Nakajima)
  20061205.017  14.77V  (Javor Kac)