Fig. 1.
Variability in 3C279 between 2009 and 2014. (a): 7 mm single-dish light curve obtained in this work together with flux per beam of the peak obtained using VLBA data from the VLBA-BU BLAZAR monitoring project; (b): R-band photometry from SMARTS; (c): Fermi/LAT γ-ray light curve from Hayashida et al. (2015); (d): R-band polarization degree (PD) and position angle (PA) obtained in this work.
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