Fig. 6

Fit results for the parameters δ and K0/L of our models with re-acceleration in core-collapse SNRs. Results are shown for Emin = 2, 5, and 10 GeV nucleon-1 (top to bottom), for the SNR models CC # 1, # 2, and # 3 of Table 2 and for the reference model (left to right). The shaded areas represent the 1-, 2-, and 3-σ contour limits. The markers “ × ” indicate the best-fit parameters for each configuration; the χ2/d.f. ratio is reported in each panel.
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