Auxiliary information

Discovery of VHE gamma-rays from the high-frequency-peaked\\ BL Lac object RGB J0152+017

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 limits
Energy 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