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Table 3:

Spectral parameters values with their respective statistical errors for a smoothed broken power law shape. The fits are performed in the [160 GeV-70 TeV] energy range.
Year $\Phi_0{}^a$ $\Gamma_1{}^b$ $\Gamma_2^{b}$ $E_{\rm {break}}{}^c$ $E_{\rm {break,true}}{}^d$ I($\geq$1 TeV)e $\chi ^{2}$/d.o.f.
  $\rm (10^{-12} TeV^{-1} cm^{-2} s^{-1})$     (TeV) (TeV) $\rm (10^{-12} cm^{-2} s^{-1})$  
2004 2.39 $\pm$ 0.12 2.18 $\pm$ 0.13 2.51 $\pm$ 0.23 2.40 $\pm$ 0.28 2.33 $\pm$ 0.28 1.79 $\pm$ 0.58 25/19
2005 2.64 $\pm$ 0.10 1.73 $\pm$ 0.10 3.07 $\pm$ 0.26 3.35 $\pm$ 0.37 3.37 $\pm$ 0.37 2.11 $\pm$ 0.60 28/18
2006 2.28 $\pm$ 0.18 2.27 $\pm$ 0.24 2.19 $\pm$ 0.28 2.04 $\pm$ 0.38 1.94 $\pm$ 0.38 1.85 $\pm$ 0.87 14/18
All 2.57 $\pm$ 0.07 2.02 $\pm$ 0.08 2.63 $\pm$ 0.14 2.61 $\pm$ 0.19 2.57 $\pm$ 0.19 1.98 $\pm$ 0.38 21/19
a Flux normalisation. b Reconstructed spectral index. c Reconstructed break energy without corrections for the systematic bias. d Reconstructed break energy corrected for the systematic bias. e Integrated $\gamma $-ray flux above 1 TeV.

Source LaTeX | All tables | In the text

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