Astrophysical S 17 (0) factor from a measurement of d( A beam stopper at 0 • allowed the use of a higher 7 Be beam intensity. Measurement of the elastic scattering in the entrance channel using kinematic coincidence, facilitated the determination of the optical model parameters needed for the analysis of the transfer data. The present measurement significantly reduces errors in the extracted 7 Be(p,γ) cross section using the ANC method. We get S 17 (0) = 20.7 ± 2.4 eV b.PACS numbers: 25.60. Je, 25.60.Bx, 26.20.+F, 26.65.+t
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