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Table 2.

The γ-ray spectral data as displayed in Figs. 1 and 2.

Min. – Mean – Max. Energy Flux
Energy (TeV) (erg s−1 cm−2)
(6.00 – 8.45 – 12.0) × 10−5 <1.52 × 10−12
(1.20 – 1.70 – 2.39) × 10−4 (1.06 ± 0.62) × 10−12
(2.39 – 3.39 – 4.76) × 10−4 (1.86 ± 0.33) × 10−12
(4.76 – 6.79 – 9.50) × 10−4 (1.48 ± 0.21) × 10−12
(0.95 – 1.36 – 1.89) × 10−3 (1.64 ± 0.20) × 10−12
(1.89 – 2.72 – 3.78) × 10−3 (1.30 ± 0.21) × 10−12
(3.78 – 5.43 – 7.54) × 10−3 (1.06 ± 0.25) × 10−12
(0.75 – 1.09 – 1.50) × 10−2 (3.79 ± 2.42) × 10−13
(1.50 – 2.17 – 3.00) × 10−2 (1.10 ± 0.51) × 10−12
0.03 – 0.08 – 0.23 (2.65 ± 1.71) × 10−13
0.26 – 0.35 – 0.43 (2.97 ± 1.25) × 10−13
0.43 – 0.55 – 0.71 (2.26 ± 0.77) × 10−13
0.71 – 0.88 – 1.17 (2.05 ± 0.64) × 10−13
1.17 – 1.43 – 1.93 (2.88 ± 0.70) × 10−13
1.93 – 2.33 – 3.17 (2.67 ± 0.78) × 10−13
3.17 – 3.93 – 5.75 <1.34 × 10−13
5.75 – 7.07 – 10.4 <1.99 × 10−13

Notes. The Fermi and H.E.S.S. spectral points are separated by the horizontal line. The energy flux uncertainties correspond to the statistical uncertainties only. The flux limits are calculated for a confidence interval of 95%.

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