Name of the Speaker(s): Jose Nicolas Gonzalez Perez
Institution: Instituto de Astrofisica de Canarias
Title of the communication: Is microvariability in OJ287
seen more frequently during flares?
Preliminary abstract (12 lines max.):
In the last 3 years the light curve of
OJ287 has shown a large degree of
activity. We present a comparison between
the rapid variability observed in the low
and high states in order to determine if
this BL object exhibits more and faster
variablity during flares. If this is
the case, al least a part of
microvariability is related to the
mechanism that produces the flares, despite the two order
of magnitude difference in
typical time scales between microvariability and flares.