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Fig. 2

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The mm and 1FGL light curves for 0235+164, shown by filled circles and triangles, respectively. The total flux density curve at 37 GHz has been decomposed using individual exponential flares following the method described in Valtaoja et al. (1999). The filled triangle represents the most significant peak in the γ-ray flux density during the 1FGL period. The dashed vertical line is drawn to highlight the relation between the peak in the γ-ray light curve and the ongoing millimeter flare.

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