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Here we report on the direct measurement of the resonance strengths of the and 1842 keV resonances in the reaction. At novae temperatures, , the reaction is governed by the low energy resonance at , whereas the resonance serves as a normalization standard for nuclear reaction experiments within the astrophysically relevant energy range. For the resonance, we obtain a resonance strength , with an uncertainty a factor of 2.5 smaller than the previous direct measurement value. For the resonance, we obtain a resonance strength , which is consistent with previous studies but deviates by from the most recent measurement. Our results suggest to be a strong waiting point in the nucleosynthesis path of oxygen-neon (ONe) novae. Published by the American Physical Society2025more » « lessFree, publicly-accessible full text available February 1, 2026
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Kuchera, A N; Shahid, R; Zhao, J; Edmondson, A; DeYoung, P A; Frank, N; McDonaugh, J; Peterson-Veatch, O; Rogers, W F; Redpath, T; et al (, Physical Review C)
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Paneru, S_N; Lee, H_Y; Prokop, C.; Kuvin, S_A; Fichtl, C.; Gastis, P.; Hale, G_M; Leal-Cidoncha, E.; Mosby, M.; Paris, M.; et al (, Physical Review C)
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deBoer, R. J.; Febbraro, M.; Bardayan, D. W.; Boomershine, C.; Brandenburg, K.; Brune, C.; Coil, S.; Couder, M.; Derkin, J.; Dede, S.; et al (, Physical Review Letters)
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Chrisman, D.; Kuchera, A. N.; Baumann, T.; Blake, A.; Brown, B. A.; Brown, J.; Cochran, C.; DeYoung, P. A.; Finck, J. E.; Frank, N.; et al (, Physical Review C)
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