Auxiliary information

Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with H.E.S.S.

F.A. Aharonian et al. (H.E.S.S. Collaboration), A&A 435 (L17) 2005, astro-ph/0504120


H.E.S.S. data points for Figure 3

Energy interval 	Mean energy 	Flux Flux Error


[TeV] [TeV] [/TeV cm^2 s]

0.28 0.34 0.31 1.3e-10 3.2e-11
0.34 0.49 0.41 3.6e-11 3.8e-12
0.49 0.73 0.60 1.9e-11 1.6e-12
0.73 1.1 0.89 7.2e-12 6.5e-12
1.1 1.6 1.31 3.2e-12 6.5e-13
1.6 2.3 1.90 1.6e-12 1.5e-13
2.3 3.6 2.87 5.5e-13 7.0e-14
3.6 4.8 4.15 2.2e-13 3.4e-14
4.8 7.6 6.09 9.5e-14 1.7e-14
7.6 10.4 8.90 4.7e-14 9.5e-15
10.4 15.7 12.8 1.2e-14 4.1e-15
15.7 23.2 19.1 6.2e-15 2.0e-15
23.2 34.8 28.4 2.4e-15 1.2e-15
34.8 46.2 40.1 7.8e-16 5.5e-16

Remarks: Statistical errors only. Systematic error on energy scale estimated to 25%. See paper for details


H.E.S.S. sky plot of Figure 2

FITS file

Remarks: The plot is smoothed with a Gaussian (0.04°) according to the instrument's point spread function. See paper for details