Image Details
Caption: Figure 4.
Spectral Energy Distribution of RCW 86 from 100 MeV to 50 TeV with the Fermi-LAT and H.E.S.S. (H. E. S. S. Collaboration et al. 2016) data points shown as black circles and triangles, respectively. The black solid line passing through the H.E.S.S. points corresponds to the best-fit spectrum from H. E. S. S. Collaboration et al. (2016). The smaller and larger errors on the Fermi fluxes are statistical and total errors (quadratic sum of statistical and systematic errors), respectively. The range of upper limit values (black and red lines) correspond to the uncertainty in the diffuse modeling. The dark gray shaded area (delimited by black dashed lines) represents the 68% confidence band of the fitted Fermi-LAT spectrum.
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