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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.

preprint2016arXivOpen access
Banibrata MukhopadhyayRumen BachevAnton Strigachev
astro-ph.GAastro-ph.HE
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Banibrata MukhopadhyayRumen BachevAnton Strigachev

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