Figure 4.
MW light curves of AO 0235$+$164 for $\gamma$-rays, optical R-band, and radio emission (230, 37, 22, 11, 8, and 5 GHz) with the most prominent flares modelled by exponential laws. The dotted lines indicate events that are poorly described by this method due to incomplete data.

MW light curves of AO 0235|$+$|164 for |$\gamma$|-rays, optical R-band, and radio emission (230, 37, 22, 11, 8, and 5 GHz) with the most prominent flares modelled by exponential laws. The dotted lines indicate events that are poorly described by this method due to incomplete data.

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