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We show that the radio, X-ray and gamma-ray spectrum of the supernova remnantRX J1713.7-3946 can be accounted for with the simplest emission model, whereall of these emissions are attributed to a population of relativistic electronsinteracting with the cosmic microwave background radiation, IR interstellarphotons, and a background magnetic field. With a spectral inversion method(Johns & Lin 1992), the parent electron distribution and its uncertainties arederived from the observed photon spectrum. These results are independent on themodel of particle acceleration and strongly support the leptonic scenario forthe TeV emission.

Derivation of the Electron Distribution in SNR RX J1713.7-3946 via a Spectral Inversion Method