Fig. 10
Top: PA variability combining the results obtained in this work with those of Marscher et al. (2010), Sasada et al. (2011), and Jermak et al. (2016). Bottom: SMARTS R band and Fermi-LAT light curves. Vertical marks in the time axis represent the epochs in which rotations of more than 50° were detected in intervals of one day.
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