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.