F.A. Aharonian et al. (H.E.S.S. Collaboration), Astron. Astrophys. 481 (2008) L103-L107
H.E.S.S. data points for Figure 2, differential energy spectrum (soft cuts)
Points with a flux error of 0 are 99% upper limitsEnergy interval Flux Flux Error [TeV] [/TeV cm^2 s] 0.240000 0.37696 2.03399e-11 6.67404e-12 0.376955 0.59206 5.64448e-12 1.63425e-12 0.592063 0.92992 1.20326e-12 5.01844e-13 0.929922 1.46058 3.12378e-13 2.16144e-13 1.460580 2.29405 1.18592e-13 8.50016e-14 2.294050 3.60315 4.09740e-14 3.51122e-14 3.603150 5.65927 5.39081e-14 0 5.659270 8.88871 1.30559e-14 0 8.888710 13.9610 7.84155e-15 0 13.96100 21.9278 5.90947e-15 0
H.E.S.S. data points for Figure 2, differential energy spectrum (std cuts)
Energy interval Flux Flux Error [TeV] [/TeV cm^2 s] 0.300000 0.414922 1.85729e-11 5.19143e-12 0.414922 0.573867 5.22912e-12 1.65301e-12 0.573867 0.793700 1.80028e-12 6.80499e-13 0.793700 1.097750 6.32447e-13 3.46693e-13