Determination of S17„0... from published data

The experimental landscape for the Be+ p radiative capture reaction is rapidly changing as new high precision data become available. We present an evaluation of existing data, detailing the treatment of systematic errors and discrepancies, and show how they constrain the astrophysical S factor sS17d, independent of any nuclear structure model. With theoretical models robustly determining the behavior of the subthreshold pole, the extrapolation error can be reduced and a constraint placed on the slope of S17. Using only radiative capture data, we find S17s0d=20.7±0.6sstatd±1.0ssystd eV b if data sets are completely independent, while if data sets are completely correlated we find S17s0d=21.4±0.5sstatd±1.4ssystd eV b. The truth likely lies somewhere in between these two limits. Although we employ a formalism capable of treating discrepant data, we note that the central value of the S factor is dominated by the recent high precision data of Junghans et al. [Phys. Rev. C 68, 065803 (2003)], which imply a substantially higher value than other radiative capture and indirect measurements. Therefore we conclude that further progress will require new high precision data with a detailed error budget.