Lederer, CMassimi, CAltstadt, SAndrzejewski, J.Audouin, LBarbagallo, MBecares, VBecvar, FBillowes, J.Schumann, D.Wallner, AntonBoccone, VBrugger, MCalviani, MChiaveri, EChin, MDuran, IEleftheriadis, CGuerrero, CKorschinek, GuntherMilazzo, P MTsinganis, A.Vlachoudis, V2015-12-130031-9007http://hdl.handle.net/1885/77437The Ni63(n,γ) cross section has been measured for the first time at the neutron time-of-flight facility n-TOF at CERN from thermal neutron energies up to 200 keV. In total, capture kernels of 12 (new) resonances were determined. Maxwellian averaged crossAuthor/s retain copyrightKeywords: Massive stars; Neutron capture cross section; S-process; Stellar models; Stellar nucleosynthesis; Thermal neutron energy; Time of flight; Chemical elements; Nucleosynthesis; Stars201310.1103/PhysRevLett.110.0225012016-02-24