A search for chaos in the blazar: W2R 1926+42 and its possible consequence

We search for low-dimensional chaotic signatures in the optical lightcurve of the Kepler field blazar W2R 1926+42. The frequently used correlation integral method is employed in our analysis. We find no apparent evidence for the presence of low-dimensional chaos in the lightcurve. If further confirmed, these results could be of importance for modeling the blazar emission mechanisms.