[en] The angular distributions of the ¹⁵N(³He,d)¹⁶O reaction were measured with the aim to determine the direct capture rate of the astrophysical reaction ¹⁵N(p, γ)¹⁶O by deducing asymptotic normalization coefficients (ANC). The ¹⁵N(p,γ)¹⁶O reaction is a part of the CNO cycle having importance in the nucleosynthesis of the N and O isotopes. The measurement was carried out on the cyclotron U120M of NPI CAS at the energy 25.74 MeV of ³He ions in a gas chamber containing the high purity ¹⁵N isotope. The preliminary results of corresponding spectroscopic factors and ANC's were used for the estimation of the S-factor for the direct capture ¹⁵N(p,γ)¹⁶O. Using the widths of the resonances E_R = 312 and 962 keV, the total S-factor was determined within the framework of the R-matrix approach