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Massimi, C. and Altstadt, S. and Andrzejewski, J. and Audouin, L. and Barbagallo, M. and Bécares, V. and Bev cváv r, F. and Belloni, F. and Berthoumieux, E. and Billowes, J. and Bisterzo, S. and Bosnar, D. and Brugger, M. and Calviani, M. and Calviño, F. and Cano-Ott, D. and Carrapic co, C. and Castelluccio, D. M. and Cerutti, F. and Chiaveri, E. and Cosentino, L. and Chin, M. and Clai, G. and Colonna, N. and Cortés, G. and Cortés-Giraldo, M. A. and Cristallo, S. and Diakaki, M. and Domingo-Pardo, C. and Duran, I. and Dressler, R. and Eleftheriadis, C. and Ferrari, A. and Finocchiaro, P. and Fraval, K. and Ganesan, S. and Garc`ia, A. R. and Giubrone, G. and Gonc calves, I. F. and González-Romero, E. and Griesmayer, E. and Guerrero, C. and Gunsing, F. and Hernández-Prieto, A. and Jenkins, D. G. and Jericha, E. and Kadi, Y. and Käppeler, F. and Karadimos, D. and Kivel, N. and Koehler, P. and Kokkoris, M. and Kopecky, S. and Krtiv cka, M. and Kroll, J. and Lampoudis, C. and Langer, C. and Leal-Cidoncha, E. and Lederer, C. and Leeb, H. and Leong, L. S. and Lo Meo, S. and Losito, R. and Mallick, A. and Manousos, A. and Marganiec, J. and Mart`inez, T. and Mastinu, P. F. and Mastromarco, M. and Mendoza, E. and Mengoni, A. and Milazzo, P. M. and Mingrone, F. and Mirea, M. and Mondelaers, W. and Musumarra, A. and Paradela, C. and Pavlik, A. and Perkowski, J. and Pignatari, M. and Piersanti, L. and Plompen, A. and Praena, J. and Quesada, J. M. and Rauscher, T. and Reifarth, R. and Riego, A. and Robles, M. S. and Rubbia, C. and Sabaté-Gilarte, M. and Sarmento, R. and Saxena, A. and Schillebeeckx, P. and Schmidt, S. and Schumann, D. and Tagliente, G. and Tain, J. L. and Tarr`io, D. and Tassan-Got, L. and Tsinganis, A. and Valenta, S. and Vannini, G. and Van Rijs, I. and Variale, V. and Vaz, P. and Ventura, A. and Vermeulen, M. J. and Vlachoudis, V. and Vlastou, R. and Wallner, A. and Ware, T. and Weigand, M. and Weiß, C. and Wynants, R. and Wright, T. and v Zugec, P.. (2017) Neutron spectroscopy of 26Mg states: Constraining the stellar neutron source 22Ne(α,n)25Mg. Physics Letters B, 768. pp. 1-6.