17O(p,g)18F
Di Leva et al. 2014
The reaction cross section was measured using both the prompt detection of the emitted γ rays and an activation technique. Measurements were carried out at the Laboratory for Underground Nuclear Astrophysics (Gran Sasso, Italy) where the strongly reduced cosmic-ray-induced background allows for improved sensitivity compared to previous studies.
Link to the paper.
Nuclear reaction rate in the MESA format:
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