Astrophysical S-factors for H-burning stars

This dataset contains the latest recommendations of astrophysical S-factors for nuclear fusion reactions occurring in hydrogen-burning stars, included in the Solar Fusion III decadal review article (submitted for publication, e-print available at arXiv:2405.06470). The data includes S-factors and their derivatives at zero energy (where available). That is, S(0), S´(0), S´´(0), in units of MeV·b, b, and b/MeV, respectively. Fractional uncertainties are also provided (marked as fr_err). Unavailable data are marked as NA. This data was used to compute the Standard Solar Models B23 / SF-III. For further information and references consult the Solar Fusion III article linked above.