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<dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:invenio="http://invenio-software.org/elements/1.0" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"><dc:identifier>doi:10.1016/j.astropartphys.2025.103135</dc:identifier><dc:language>eng</dc:language><dc:creator>Soleti, S.R.</dc:creator><dc:creator>Gómez-Cadenas, J.J.</dc:creator><dc:creator>Apilluelo, J.</dc:creator><dc:creator>Asquith, L.</dc:creator><dc:creator>Bannister, E.F.</dc:creator><dc:creator>Barradas, N.P.</dc:creator><dc:creator>Baylis, C.L.</dc:creator><dc:creator>Beney, J.L.</dc:creator><dc:creator>e Santos, M. Berberan</dc:creator><dc:creator>de la Bernardie, X.</dc:creator><dc:creator>Bezerra, T.J.C.</dc:creator><dc:creator>Bongrand, M.</dc:creator><dc:creator>Bourgeois, C.</dc:creator><dc:creator>Breton, D.</dc:creator><dc:creator>Busto, J.</dc:creator><dc:creator>Burns, K.</dc:creator><dc:creator>Cabrera, A.</dc:creator><dc:creator>Cadiou, A.</dc:creator><dc:creator>Calvo, E.</dc:creator><dc:creator>de Carlos Generowicz, M.</dc:creator><dc:creator>Chauveau, E.</dc:creator><dc:creator>Cattermole, B.J.</dc:creator><dc:creator>Chen, M.</dc:creator><dc:creator>Chimenti, P.</dc:creator><dc:creator>Cowen, D.F.</dc:creator><dc:creator>Das, S.Kr.</dc:creator><dc:creator>Dusini, S.</dc:creator><dc:creator>Earle, A.</dc:creator><dc:creator>Felizardo, M.</dc:creator><dc:creator>Martins, C. Frigerio</dc:creator><dc:creator>Galán, J.</dc:creator><dc:creator>García, J.A.</dc:creator><dc:creator>Gazzini, R.</dc:creator><dc:creator>Gibson-Foster, A.</dc:creator><dc:creator>Girard-Carillo, C.</dc:creator><dc:creator>Griffith, W.C.</dc:creator><dc:creator>Guitière, M.</dc:creator><dc:creator>Haddad, F.</dc:creator><dc:creator>Hartnell, J.</dc:creator><dc:creator>Holin, A.</dc:creator><dc:creator>Irastorza, I.G.</dc:creator><dc:creator>Jovanovic, I.</dc:creator><dc:creator>Kling, A.</dc:creator><dc:creator>Koch, L.</dc:creator><dc:creator>Lasorak, P.</dc:creator><dc:creator>Le Du, J.F.</dc:creator><dc:creator>Lefevre, F.</dc:creator><dc:creator>Loaiza, P.</dc:creator><dc:creator>Lock, J.A.</dc:creator><dc:creator>Luzón, G.</dc:creator><dc:creator>Maalmi, J.</dc:creator><dc:creator>Malhado, J.P.</dc:creator><dc:creator>Mantovani, F.</dc:creator><dc:creator>Marques, J.G.</dc:creator><dc:creator>Marquet, C.</dc:creator><dc:creator>Martínez, M.</dc:creator><dc:creator>Navas-Nicolás, D.</dc:creator><dc:creator>Nunokawa, H.</dc:creator><dc:creator>Ochoa-Ricoux, J.P.</dc:creator><dc:creator>Palmeira, T.</dc:creator><dc:creator>Palomares, C.</dc:creator><dc:creator>Petyt, D.</dc:creator><dc:creator>Pillot, P.</dc:creator><dc:creator>Pin, A.</dc:creator><dc:creator>Porter, J.C.C.</dc:creator><dc:creator>Pravikoff, M.S.</dc:creator><dc:creator>Richards, S.</dc:creator><dc:creator>Rodrigues, N.</dc:creator><dc:creator>Roche, M.</dc:creator><dc:creator>Rosero, R.</dc:creator><dc:creator>Roskovec, B.</dc:creator><dc:creator>Roy, N.</dc:creator><dc:creator>Sarsa, M.L.</dc:creator><dc:creator>Serafini, A.</dc:creator><dc:creator>Shepherd-Themistocleous, C.</dc:creator><dc:creator>Shorrock, W.</dc:creator><dc:creator>Silva, M.</dc:creator><dc:creator>Simard, L.</dc:creator><dc:creator>Stocco, D.</dc:creator><dc:creator>Strati, V.</dc:creator><dc:creator>Stutzmann, J.S.</dc:creator><dc:creator>Suekane, F.</dc:creator><dc:creator>Tuccori, N.</dc:creator><dc:creator>Verdugo, A.</dc:creator><dc:creator>Viaud, B.</dc:creator><dc:creator>Wakely, S.M.</dc:creator><dc:creator>Wendel, G.</dc:creator><dc:creator>Wilhelm, A.S.</dc:creator><dc:creator>Wong, A.W.R.</dc:creator><dc:creator>Yeh, M.</dc:creator><dc:creator>Yermia, F.</dc:creator><dc:title>COCOA: A compact Compton camera for astrophysical observation of MeV-scale gamma rays</dc:title><dc:identifier>ART-2025-144326</dc:identifier><dc:description>COCOA (COmpact COmpton cAmera) is a next-generation gamma-ray telescope designed for astrophysical observations in the MeV energy range. The detector comprises a scatterer volume employing the LiquidO detection technology and an array of scintillating crystals acting as absorber. Surrounding plastic scintillator panels serve as a veto system for charged particles. The detector’s compact, scalable design enables flexible deployment on microsatellites or high-altitude balloons. Gamma rays at MeV energies have not been well explored historically (the so-called “MeV gap”) and COCOA has the potential to improve the sensitivity in this energy band.</dc:description><dc:date>2025</dc:date><dc:source>http://zaguan.unizar.es/record/161675</dc:source><dc:doi>10.1016/j.astropartphys.2025.103135</dc:doi><dc:identifier>http://zaguan.unizar.es/record/161675</dc:identifier><dc:identifier>oai:zaguan.unizar.es:161675</dc:identifier><dc:identifier.citation>Astroparticle Physics 172 (2025), 103135 [12 pp.]</dc:identifier.citation><dc:rights>by</dc:rights><dc:rights>https://creativecommons.org/licenses/by/4.0/deed.es</dc:rights><dc:rights>info:eu-repo/semantics/openAccess</dc:rights></dc:dc>

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