TY - INPR A1 - Domingo-Pardo, César A1 - Babiano Suarez, Victor A1 - Balibrea Correa, Javier A1 - Caballero Ontanaya, Luis A1 - Ladarescu, Ion A1 - Lerendegui-Marco, Jorge A1 - Taı́n Enríquez, José Luis A1 - Calviño Tavares, Francisco A1 - Casanovas Hoste, Adrià A1 - Segarra, Alejandro A1 - Tarifeño-Saldivia, Ariel A1 - Guerrero Sánchez, Carlos A1 - Millán Callado, María de los Ángeles A1 - Quesada Molina, José Manuel A1 - Rodríguez González, María Teresa A1 - Aberle, Oliver A1 - Alcayne, Victor A1 - Amaducci, Simone A1 - Andrzejewski, Józef A1 - Audouin, Laurent A1 - Bacak, Michael A1 - Barbagallo, Massimo A1 - Bennett, Samuel A1 - Berthoumieux, Eric A1 - Bosnar, Damir A1 - Brown, Adam S. A1 - Busso, Maurizio A1 - Caamaño, Manuel A1 - Calviani, Marco A1 - Cano-Ott, Daniel A1 - Cerutti, Francesco A1 - Chiaveri, Enrico A1 - Colonna, Nicola A1 - Cortés Rossell, Guillem Pere A1 - Cortés-Giraldo, Miguel Antonio A1 - Cosentino, Luigi A1 - Cristallo, Sergio A1 - Damone, Lucia Anna A1 - Davies, Paul John A1 - Diakaki, Maria A1 - Dietz, Mirco A1 - Dressler, Rugard A1 - Ducasse, Quentin A1 - Dupont, Emmeric A1 - Durán, Ignacio A1 - Eleme, Zinovia A1 - Fernández Domínguez, Beatriz A1 - Ferrari, Alfredo A1 - Gonçalves, Isabel Maria Ferro A1 - Finocchiaro, Paolo A1 - Furman, Valter A1 - Garg, Ruchi A1 - Gawlik, Aleksandra A1 - Gilardoni, Simone A1 - Göbel, Kathrin A1 - González Romero, Enrique Miguel A1 - Gunsing, Frank A1 - Heyse, Jan A1 - Jenkins, David A1 - Jericha, Erwin A1 - Jiri, U. A1 - Junghans, Arnd Rudolf A1 - Kadi, Yacine A1 - Käppeler, Franz A1 - Kimura, Atsushi A1 - Knapová, Ingrid A1 - Kokkoris, Michael A1 - Kopatch, Yuri N. A1 - Krtička, Milan A1 - Kurtulgil, Cem Deniz A1 - Lederer-Woods, Claudia A1 - Lonsdale, Sarah-Jane A1 - Macina, Daniela A1 - Manna, Alice A1 - Martı́nez, Trinitario A1 - Masi, Alessandro A1 - Massimi, Cristian A1 - Mastinu, Pierfrancesco A1 - Mastromarco, Mario A1 - Maugeri, Emilio Andrea A1 - Mazzone, Annamaria A1 - Mendoza Cembranos, Emilio A1 - Mengoni, Alberto A1 - Michalopoulou, Veatriki A1 - Milazzo, Paolo Maria A1 - Mingrone, Federica A1 - Moreno-Soto, Javier A1 - Musumarra, Agatino A1 - Negret, Alexandru A1 - Ogállar Ruiz, Francisco A1 - Oprea, Andreea A1 - Patronis, Nikolas A1 - Pavlik, Andreas A1 - Perkowski, Jarosław A1 - Petrone, Cristina A1 - Piersanti, Luciano A1 - Pirovano, Elisa A1 - Porras Sánchez, José Ignacio A1 - Praena, Javier A1 - Ramos Doval, Diego A1 - Reifarth, René A1 - Rochman, Dimitri A1 - Rubbia, Carlo A1 - Sabaté-Gilarte, Marta A1 - Saxena, Alok A1 - Schillebeeckx, Peter A1 - Schumann, Dorothea A1 - Sekhar, Adhitya A1 - Smith, Alastair Gavin A1 - Sosnin, Nikolay V. A1 - Sprung, Peter A1 - Stamatopoulos, Athanasios A1 - Tagliente, Giuseppe A1 - Tassan-Got, Laurent A1 - Thomas, Benedikt A1 - Torres-Sánchez, Pablo A1 - Tsinganis, Andrea A1 - Urlaß, Sebastian A1 - Valenta, Stanislav A1 - Vannini, Gianni A1 - Variale, Vincenzo A1 - Vaz, Pedro A1 - Ventura, Alberto A1 - Vescovi, Diego A1 - Vlachoudis, Vasilis A1 - Vlastou, Rosa A1 - Wallner, Anton A1 - Woods, Philip John A1 - Wright, Tobias J. A1 - Žugec, Petar T1 - Review and new concepts for neutron-capture measurements of astrophysical interest N2 - The idea of slow-neutron capture nucleosynthesis formulated in 1957 triggered a tremendous experimental effort in different laboratories worldwide to measure the relevant nuclear physics input quantities, namely (n,γ) cross sections over the stellar temperature range (from few eV up to several hundred keV) for most of the isotopes involved from Fe up to Bi. A brief historical review focused on total energy detectors will be presented to illustrate how, advances in instrumentation have led, over the years, to the assessment and discovery of many new aspects of s-process nucleosynthesis and to the progressive refinement of theoretical models of stellar evolution. A summary will be presented on current efforts to develop new detection concepts, such as the Total-Energy Detector with γ-ray imaging capability (i-TED). The latter is based on the simultaneous combination of Compton imaging with neutron time-of-flight (TOF) techniques, in order to achieve a superior level of sensitivity and selectivity in the measurement of stellar neutron capture rates. Y1 - 2019 UR - http://publikationen.ub.uni-frankfurt.de/frontdoor/index/index/docId/71679 UR - https://nbn-resolving.org/urn:nbn:de:hebis:30:3-716790 ER -