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

Open Access

Fig. A.2.

SED fits: expanding blob model. Similar to Fig. 6 for the expanding blob model. The best-fit value and MCMC range for the SED (top subplot) and the EED (bottom subplot) for each observation date in January 2010 are shown. The residuals of the model and the χ², reduced χ² ( $χ_{red}^{2}$ $Mathematical equation: $ \chi^{2}_{\mathrm{red}} $$ ) and degrees of freedom (N_DoF) of the fit are mentioned in the subplot underneath the SED.

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