Fig. 1
From top to bottom: 7 mm radio light curve obtained in this work together with the 7 mm peak flux density of VLBA images obtained from the VLBI-BU BLAZAR monitoring programme; R-band photometry from SMARTS (Bonning et al. 2012); Fermi-LAT γ-ray light curve for energies >100 MeV, binned in five-day intervals (Abdo et al. 2009a,b, 2010c); R-band polarization degree and position angle obtained in this work.
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