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Table 2:

Spectral parameters values with their respective statistical errors for a power law shape with an exponential cut-off, with $\beta = 1$. The fits are performed in the [160 GeV-70 TeV] energy range.
Year $\Phi_0{}^a$ $\Gamma^b$ $E_{\rm {cut}}{}^c$ $E_{\rm {cut,true}}{}^d$ 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 2.40 $\pm$ 0.10 2.20 $\pm$ 0.07 20.70 $\pm$ 11.80 22.20 $\pm$ 11.80 1.81 $\pm$ 0.14 25/26
2005 2.56 $\pm$ 0.09 1.94 $\pm$ 0.07 9.09 $\pm$ 2.13 9.61 $\pm$ 2.13 2.09 $\pm$ 0.16 33/25
2006 2.35 $\pm$ 0.16 2.16 $\pm$ 0.11 32.90 $\pm$ 39.50 35.50 $\pm$ 39.50 1.88 $\pm$ 0.22 17/23
All 2.55 $\pm$ 0.06 2.10 $\pm$ 0.04 14.70 $\pm$ 3.41 15.70 $\pm$ 3.41 1.99 $\pm$ 0.09 23/26
a Flux normalisation. b Reconstructed spectral index. c Reconstructed cut-off energy without corrections for the systematic bias. d Reconstructed cut-off 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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