Résumé : Photoneutron cross sections were measured for 80Se near the neutron separation energy with laser Compton-backscattered γ-ray beams at AIST. Neutron capture rates are evaluated for 79Se with the photoreaction data as experimental constraints on the El γ-strength function, a key parameter in the Hauser-Feshbach statistical model calculation. Solving the set of differential equations under a single neutron exposure, we analyzed the solar abundance ratio of the weak components of 80Kr and 82Kr in terms of the s-process branching at 79Se. We discuss the region of temperature and neutron density allowed for the weak s-process nucleosynthesis.