Optically thick, nonlocal, inhomogeneous, stationary jet model for high-energy radiation from blazars: Application to Mrk 421

Open Access

Fig. 2.

Spectral energy distribution of Mrk 421 during the observations at 56302 MJD; data are from Baloković et al. (2016, see circles). The solid black line is the fit to the differential spectrum obtained in terms of the nonlocal, inhomogeneous jet model. The parameters of the model are listed in Table 1.

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