Publisher's Note: Astrophysical S factor of the 3 He(α, γ ) 7 Be reaction measured at low energy via detection of prompt and delayed γ rays [Phys. Rev. C 75, 065803 (2007)]
Erratum: The 11 B( p, α 0 ) 8 Be reaction at sub-Coulomb energies via the Trojan-horse method [Phys. Rev. C 69, 055806 (2004)] PACS number(s): 26.20.+f, 25.70.Hi, 99.10.CdIn the above article the energy range where our indirect data were normalized to the directly measured ones was mistakenly reported to be 800-900 keV. The energy range actually used in the normalization procedure was instead 400-900 keV. Moreover, the parametrization used for S(E) is not that shown in formula (11). With the correct parameters, this formula reads S b (E) = 0.30 + 1.97E − 0.67E 2 + 4.91 exp −0.5 E − 0.164 0.052 2 .
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