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The Al25(p,γ)Si26 reaction is part of a reaction network with impact on the observed galactic Al26 abundance. A new determination of the proton strength of the lowest ℓ=0 proton resonance in Si26 is required to more precisely calculate the thermal reaction rate. To this end, the Al25(d,n)Si26 proton-transfer reaction is measured in inverse kinematics using an in-flight radioactive beam at the RESOLUT facility.
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