The January 2010 flare of Mrk 421: Insights from a stochastic acceleration model

Open Access

Fig. D.1.

Combined model: Synchrotron peak position ( $ν_{sync}^{*}$ $Mathematical equation: $ \nu^{*}_{\mathrm{sync}} $$ ) of the SED is directly correlated with the peak of the γ³n(γ) distribution (γ_3p)

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