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Fig. 10

image

Best-fit values of the spectral index γ (left panel) and the total energy carried by positrons fW0 (right panel) for each point of the plane (age, distance) with the benchmark propagation model MED. The grey lines display the iso-contours for given values of γ (left) and fW0 (right). The black dashed lines represent the iso-contours of the critical p-values. The five selected pulsars with their associated uncertainty on their distance are indicated by the black stars.

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