Fig. 14
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Spectral energy distributions of the Crab pulsar and pulsar wind nebula components as determined using GammaLib and ctools (red) and by Kuiper et al. (2001) using COMPASS (blue). Results for the Crab pulsar are shown as dots, and results for the Crab pulsar wind nebula are shown as triangles. The figure also shows the 1σ uncertainty bands of the best fitting spectral models for both components.
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