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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 10.

Figure 10.

1D posterior distributions (with 68% and 95% credible intervals) for the different CR propagation parameters in a low-resolution, {p, p¯, and He} propagation scenario using MultiNest as a sampler (no neural network speed up, magenta) and from BAMBI runs with two different values for the neural network input parameter σ. Light blue: σ = 0.5; Orange: σ = 0.8. All BAMBI chains have been post-processed in the same way as in our main paper runs.