Table 3: Summary of the parameters of power law fits ( ${\rm d}N/{\rm d}E = N_0 (E/{\rm TeV})^{-\Gamma }$ ). For comparison with the 3D Model analysis (1) used here, the results from the standard analysis (2) are also given. Both analyses yield consistent results. In addition to the parameter values, the $\chi ^2$ probabilities of the fits are given.
$\Gamma$ N₀ $P(~\chi^2)$

[10^-13 cm^-2 s^-1 TeV^-1]

(1) $3.09~\pm~0.24_{\rm stat}~\pm~0.10_{\rm sys}$ $3.00~\pm~0.80_{\rm stat}~\pm~0.31_{\rm sys}$ 0.47

(2) $3.06~\pm~0.21_{\rm stat}~\pm~0.10_{\rm sys}$ $3.07~\pm~0.75_{\rm stat}~\pm~0.31_{\rm sys}$ 0.60

**Table 3:** Summary of the parameters of power law fits ( ${\rm d}N/{\rm d}E = N_0 (E/{\rm TeV})^{-\Gamma }$ ). For comparison with the 3D Model analysis (1) used here, the results from the standard analysis (2) are also given. Both analyses yield consistent results. In addition to the parameter values, the $\chi ^2$ probabilities of the fits are given.
	$\Gamma$	N₀	$P(~\chi^2)$
		[10^-13 cm^-2 s^-1 TeV^-1]
(1)	$3.09~\pm~0.24_{\rm stat}~\pm~0.10_{\rm sys}$	$3.00~\pm~0.80_{\rm stat}~\pm~0.31_{\rm sys}$	0.47
(2)	$3.06~\pm~0.21_{\rm stat}~\pm~0.10_{\rm sys}$	$3.07~\pm~0.75_{\rm stat}~\pm~0.31_{\rm sys}$	0.60

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