Aiello,S.; Akrame, S. E.; Ameli, F.; Anassontzis, E. G.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Avgitas, T.; Baars, M.; Bagatelas, C.; Barbarino, G.; Baret, B.; Martínez Mora, Juan Antonio(IOP Publishing, 2018-05)
[EN] The Hamamatsu R12199-02 3-inch photomultiplier tube is the photodetector chosen for the first phase of the KM3NeT neutrino telescope. About 7000 photomultipliers have been characterised for dark count rate, timing ...
Aiello, S.; Albert, A.; Alves Garre, S.; Aly, Z.; Ameli, F.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Bagatelas, C.; Barbarino, G.; Baret, B.; Diego-Tortosa, D.; Espinosa Roselló, Víctor; Martínez Mora, Juan Antonio; Poirè, Chiara(Elsevier, 2020-11)
[EN] The gSeaGen code is a GENIE-based application developed to efficiently generate high statistics samples of events, induced by neutrino interactions, detectable in a neutrino telescope. The gSeaGen code is able to ...
Adrián Martínez, Silvia; Ageron, M.; Aiello, S.; Albert, A.; Ameli, F.; Anassontzis, E. G.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Avgitas, T.; Barbarino, G.; Barbarito, E.; Baret, B.; Llorens Alvarez, Carlos David; Martínez Mora, Juan Antonio; Saldaña-Coscollar, María(Springer-Verlag, 2017-05-02)
[EN] Studying atmospheric neutrino oscillations in the few-GeV range with a multimegaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future ...
Aiello, S.; Ameli, F.; Andre, M.; Androulakis, Giorgos; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Bagatelas, C.; Barbarino, G.; Baret, B.; Basegmez du Pree, Suzan; Belias, Anastasios; Bendahman, Meriem; Berbee, Edward; van den Berg, Ad M.; Bertin, Vincent; Diego-Tortosa, D.; Martínez Mora, Juan Antonio; Poirè, Chiara(Society of Photo-optical Instrumentation Engineers (SPIE), 2019-10)
[EN] The KM3NeT research infrastructure being built at the bottom of the Mediterranean Sea will host
water-Cherenkov telescopes for the detection of cosmic neutrinos. The neutrino telescopes will consist of large
volume ...
Adrián Martínez, Silvia; Aiello, S.; Ameli, F; Anghinolfi, M.; Ardid Ramírez, Miguel; Barbarino, G.; Barbarito, E.; Barbato, F. C. T.; Beverini, N.; Biagi, S.; Biagioni, A.; Bouhadef, B.; Bozza, C.; Llorens Alvarez, Carlos David; Saldaña Coscollar, María(Springer, 2016-02)
The NEMO Phase-2 tower is the first detector which was operated underwater for more than 1 year at the "record" depth of 3500 m. It was designed and built within the framework of the NEMO (NEutrino Mediterranean Observatory) ...
Aiello, S.; Akrame, S. E.; Ameli, F.; Anassontzis, E. G.; Andre, M.; Androulakis, G.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, Miguel; Aublin, J.; Avgitas, T.; Bagatelas, C.; Barbarino, G.; Baret, B.; Barrios-Marti, J.; Diego-Tortosa, D.; Martínez Mora, Juan Antonio; Poirè, Chiara(Elsevier, 2019-09)
[EN] KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the detection of highenergy neutrinos of ...