[vsnet-alert 16162] UZ Boo rebrightening up to now

[Taichi Kato]

UZ Boo rebrightening up to now

  This object underwent multiple rebrightenings in the past
superoutbursts.  Observations in this phase is very important.
Superhumps appear both in outbursts and in quiescence between
them, and the amplitude is larger in quiescence.  We encourage
time-series photometry when the object fades, rather than
solely paying attention to the outburst state.  Period variations
of superhumps in this phase is a very important subject,
and would become a clue to understanding why rebrightenings occur.

  YYYYMMDD(UT)   mag  observer
  20130805.856   132  (Wolfgang Kriebel)
  20130805.903   134  (Gary Poyner)
  20130805.953  13.47V  (Eddy Muyllaert)
  20130805.953  13.59V  (Gary Poyner)
  20130806.910   147  (Gary Poyner)
  20130806.953  14.83V  (Gary Poyner)
  20130806.960  14.71V  (Eddy Muyllaert)
  20130807.190  14.950V  (Jim Roe)
  20130807.900   163  (Adolfo Darriba Martinez)
  20130807.906  <143  (Jose Ripero)
  20130807.938  16.48V  (Gary Poyner)
  20130808.873  17.18V  (Miguel Rodriguez)
  20130808.900  <162  (Adolfo Darriba Martinez)
  20130808.909  <143  (Jose Ripero)
  20130808.933  16.56V  (Gary Poyner)
  20130808.944  16.66C  (Eddy Muyllaert)
  20130809.865  <143  (Jose Ripero)
  20130809.900  <162  (Adolfo Darriba Martinez)
  20130810.936  16.04V  (Robert J. Modic)
  20130810.942  15.98C  (Eddy Muyllaert)
  20130811.110  14.083V  (Jim Roe)