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Fig. 8


95% CL envelopes for the proton and helium fluxes for the four propagation configurations of models of Table 2. The three panels correspond respectively to the result of the MCMC analysis on AMS-01 data (left panel), BESS98 data (middle panel), and BESS-TeV (right panel). For the sake of comparison, the IS (demodulated) AMS-01 (black circles), BESS98 (red squares), BESS-TeV (blue triangles), along with the Voyager data (stars).

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