Fitting B/C cosmic-ray data in the AMS-02 era: a cookbook - Model numerical precision, data covariance matrix of errors, cross-section nuisance parameters, and mock data

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Fig. 6.

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Median, 1-σ, and 2-σ for the distribution of σ^NSS/σ_ref(E_k/n) values, from 1000 Gaussian distributed normalisation values (9), energy scale (10), and slopes (11) with respective mean and variance (μ, σ)^Norm = (1, 0.05), (μ, σ)^Scale = (1, 0.2), and (μ, σ)^Slope = (0, 0.02).

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