Fig. A.8.
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SED model for epoch MJD 57293 in the EC-dominated scenario (Table 8). Unlike the models for the older flaring epoch 54761 (Figs. A.1, A.2), this model does not include a bulk-Compton component and can be explained with only the usual SSC+EC components. The source exhibits an important softening in the X-ray spectrum that could also be explained by bulk-Compton emission.
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