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Fig. 2


H.E.S.S. radial profile of the uncorrelated excess map centered on the position of the putative pulsar. The solid dark blue line shows the result of the best-fit model (labeled (C) in Table 1) estimated in Sect. 2.1. The dark blue and light blue dashed lines represent the point-like and Gaussian components of this model. The profile from the single Gaussian model (labeled (B) in Table 1) is plotted in orange.

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