Fig. 1.
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Best fit with residuals of the multi-wavelength flux density of the 2013 observations of A0620−00 from Dinçer et al. (2017). In the upper panel, we show the result for the case of BHJet, and in the lower panel, we show the case of MLJet. The solid black line shows the total absorbed emission, and the individual components are explained in the legend.
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