Compagnucci, A.Formicola, A.Campostrini, M.Cruz, J.Aliotta, M.Ananna, C.Barbieri, L.Barile, F.Bemmerer, D.Best, A.Boeltzig, A.Broggini, C.Bruno, C. G.Caciolli, A.Casaburo, F.Cavanna, F.Ciani, G. F.Colombetti, P.Corvisiero, P.Csedreki, L.Davinson, T.Depalo, R.Leva, A. DiElekes, Z.Ferraro, F.Fülöp, ZsGuglielmetti, A.Gustavino, C.Gyürky, GyImbriani, G.Junker, M.Lugaro, M.Marigo, P.Marsh, J.Masha, E.Menegazzo, R.Paticchio, V.Piatti, D.Prati, P.Rapagnani, D.Rigato, V.Robb, D.Schiavulli, L.Sidhu, R. S.Skowronski, J.Straniero, O.Szücs, T.Turkat, S.Zavatarelli, S.2025-09-052025-09-052025-08-151434-6001PURE: 127907158PURE UUID: 9707d6ca-6c56-4c83-a6f3-68078ab9c62bScopus: 105013222317WOS: 001550338400001ORCID: /0000-0003-3242-0328/work/191286749http://hdl.handle.net/10362/187594Funding Information: This work was supported by HUN-REN Researcher Mobility Program 2023; by NKFIH grant K134197; by Fundação para a Ciência e Tecnologia (FCT, Portugal) through national funds to the Associated Laboratory in Translation and Innovation Towards Global Health REAL (LA/P/0117/2020); by the EU (ChETEC-INFRA, 101008324). E.M. acknowledges a fellowship by the Alexander von Humboldt Foundation. The work of the CAD service (M. Mongelli) and the mechanical workshop (C. Pastore, S. Martiradonna, N. Lacalamita and M. Franco) of INFN Bari is acknowledged. Open access funding provided by HUN-REN Institute for Nuclear Research. Publisher Copyright: © The Author(s) 2025.While the 14N(p,γ)15O reaction plays a key role in the hydrogen-burning processes in various stellar conditions, its reaction rate is not known with sufficient precision. Therefore, the first scientific project at the recently launched Bellotti Ion Beam Facility of the Laboratori Nazionali del Gran Sasso was the measurement of the 14N(p,γ)15O reaction cross section in the proton energy range between 250 and 1500 keV. In this paper, the experimental techniques are summarized with special emphasis on the description of solid state nitrogen target production and characterization. The first results of the reaction yield measured at 55∘ detection angle are also presented.112726084engNuclear and High Energy PhysicsTowards a comprehensive study of the 14N(p,γ)15O astrophysical key reactionjournal article10.1140/epja/s10050-025-01658-7Description of the experimental technique including novel target preparationhttps://www.scopus.com/pages/publications/105013222317https://www.webofscience.com/wos/woscc/full-record/WOS:001550338400001