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Fig. C.1.

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Cosmic-ray model contributions from the heavier nuclei carbon, oxygen, magnesium, silicon, and iron together with the corresponding data from AMS-02 (Aguilar et al. 2017 for C and O and Aguilar et al. 2020 for Mg and Si), CREAM-II (Ahn et al. 2009), ATIC-2 (Panov et al. 2009), NUCLEON (Grebenyuk et al. 2019), KASCADE-Grande (The KASCADE-Grande Collaboration 2013), and IceCube/IceTop (Aartsen et al. 2019, for C-O and Fe). The contributions are the same in Model A and Model B. The first components are shown with the black dashed lines and the second components with the dashed-dotted lines, summing up to the total contributions (solid black lines).

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