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. Author manuscript; available in PMC: 2021 Nov 12.
Published in final edited form as: Astrophys J. 2016 Jun 3;824(1):16. doi: 10.3847/0004-637x/824/1/16

Figure 6.

Figure 6.

Spectra and p¯p ratio 68% and 95% posterior bands of our p¯, p, He scan, shown in blue in Figure 2. The best fit is plotted in black, and the dashed lines correspond to the LIS (umodulated) spectra. PAMELA data are shown in red. We also show recent AMS-02 (Aguilar et al. 2015, blue) for the available proton and helium flux data, which were not available at the time of our analysis (and hence are not included in the likelihood).