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Fig. 3

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Left: HESS J1303−631 fitted Gaussian mean, c(E), measured from the pulsar position, as a function of energy. Right: the PSF corrected intrinsic Gaussian extension (wint(E), blue) is overlaid with the fitted uncorrected excess Gaussian extension (wimg(E), black dashed) as a function of energy. The points are placed at the average energy of the photons falling in the corresponding energy bin (indicated by the horizontal error bars, not used in fit).

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