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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 3.

Figure 3.

2D posterior distributions, showing 1- and 2-sigma credible intervals for the p, p¯, and He scan (blue), and for the light element (Be–Si, magenta). The posterior mean in each case is shown as a dot and the best fit as a cross.