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Fig. 9


Broadband fit to radio (filled triangles) and γ-ray observations obtained with HESS (filled circles). Upper limits to the flux densities from Fermi-LAT (arrows pointing downwards) and the best fit to the X-ray data (green hatching) are also included. The radio data correspond to the internal region of SNR G15.4+0.1. The curves labelled S and IC show the model of the synchrotron radiation and inverse Compton mechanism on the CMB by accelerated electron, respectively.

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