Swift observations of the very intense flaring activity of Mrk 421 during 2006. I. Phenomenological picture of electron acceleration and predictions for MeV/GeV emission

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Table 4:

SSC best-fit model results for the 2006 *Swift* observations and using as electron distribution a log-parabola with a power-law low-energy branch (Eq. (13)).
Date	B	R	$\delta$	N(*)	r	s	$\gamma_{c}(**)$	$\gamma_{p}^{\rm LP}(***)$	$\gamma_{\rm max}$	$\gamma_{\rm min}$	u_e/u_b
	G	cm		$\mbox{cm}^{-3}$
22-04-2006	0.1	$2.1\times10^{15}$	25	13.5	0.75	2.30	$1.75\times10^{5}$	$2.0\times10^3$	$2.5\times10^{6}$	$1.1\times10^{3}$	119
23-06-2006	0.1	$2.1\times10^{15}$	25	15.0	0.65	2.30	$2.85\times10^{5}$	$4.8\times10^3$	$4.0\times10^{6}$	$1.1\times10^{3}$	135
15-07-2006	0.1	$2.1\times10^{15}$	25	21.0	0.85	2.32	$2.50\times10^{5}$	$1.0\times10^4$	$3.0\times10^{6}$	$1.1\times10^{3}$	185

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