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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 4.

Figure 4.

Spectral fluxes with 68% and 95% posterior regions from the posteriors of our light element (Be–Si) scan, shown in magenta in Figure 1, and using the HEAO modulation posteriors. Data shown are HEAO (blue), CREAM (green), and TRACER (cyan). The best fit is shown as a black line, and the dashed lines correspond to the LIS (unmodulated) spectra.