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Fig. 8
Radio lightcurve at 15 GHz obtained with the OVRO 40 m telescope (points) supplemented with two 14.6 GHz measurements obtained with the Effelsberg 100 m telescope (square). VLBA measurements of the core (component C0, Table 6) are indicated as diamonds. The two arrows mark the peaks of the γ-ray flares observed by Fermi.
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