Fig. A.1.

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Comparison of the potential contribution of ℓ > 0 resonances in Table A.2 to the 18F(p, α) rates utilized in the astrophysical calculations in the present work (normalized to our Set IX). We demonstrate that the potential influence of the sum of those four resonances is not much more than, e.g., the uncertainty in Γα of the 6.13 MeV state observed by Kahl et al. (2019).
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