Dataset referencing 2025MA13
E.Masha, F.Casaburo, R.S.Sidhu, M.Aliotta, C.Ananna, L.Barbieri, F.Barile, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Cavanna, G.F.Ciani, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, D.Dell'Aquila, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, R.M.Gesue, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, J.Marsh, R.Menegazzo, D.Mercogliano, V.Paticchio, D.Piatti, P.Prati, D.Rapagnani, V.Rigato, D.Robb, L.Schiavulli, J.Skowronski, O.Straniero, T.Szucs, S.Zavatarelli
A high energy resolution gas target setup to study selected NeNa cycle reactions
NUCLEAR REACTIONS 20,21Ne(p, γ), E<400 keV; measured reaction products, Eγ, Iγ; deduced resonance energies, strengths, decay branching ratios for resonances. The 400 kV accelerator at the Laboratory for Underground Nuclear Astrophysics (LUNA), the Gran Sasso National Laboratory (INFN-LNGS) in Italy.
doi: 10.1140/epja/s10050-025-01512-w