Aguilar, JA; Al Samarai, I; Albert, A; Andre, M; Anghinolfi, M; Anton, G; Anvar, S; Ardid Ramírez, Miguel; Assis Jesus, A.C.; Astraatmadja, T.; Aubert, J.-J.; Bou Cabo, Manuel; Camarena Femenia, Francisco; Larosa, Giuseppina; Martínez Mora, Juan Antonio(Elsevier, 2011-04)
An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ...
Aguilar, J. A.; Al Samarai, I.; Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Anvar, S.; Ardid Ramírez, Miguel; Jesus, A. C. Assis; Astraatmadja, T.; Bou Cabo, Manuel; Camarena Femenia, Francisco; Ferri García, Marcelino; Larosa, Giuseppina; Martínez Mora, Juan Antonio(Elsevier, 2012-05-21)
The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. ...
Aguilar, J. A.; Al Samarai, I.; Albert, A.; Anghinolfi, M.; Anton, G.; Anvar, S.; Ardid Ramírez, Miguel; Jesus, A. C. Assis; Astraatmadja, T.; Aubert, J. -J.; Auer, R.; Bou Cabo, Manuel; Camarena Femenia, Francisco; Larosa, Giuseppina; Martínez Mora, Juan Antonio(Elsevier, 2011-01-11)
The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated ...
Poirè, Chiara(Universitat Politècnica de València, 2022-10-24)
[ES] Los neutrinos de alta energía son partículas esquivas: no tienen carga, tienen una sección transversal de interacción muy pequeña con la materia ordinaria y su masa es extremadamente pequeña. Los neutrinos son una ...
Aslan Suárez, Antonio Alejandro(Universitat Politècnica de València, 2021-09-02)
[ES] Las radiaciones electromagnéticas no son la única forma que el ser humano tiene para estudiar los astros, de hecho, el estudio de la trayectoria de los neutrinos que llegan a la Tierra puede permitir el estudio de ...
[EN] Silicon Photomultipliers find applications across various fields. One potential Silicon Photomultiplier application domain is neutrino telescopes, where they may enhance the angular resolution. However, the elevated ...
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; 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) ...
Adrián Martínez, Silvia; Al Samarai, I; Albert, A.; André, A; Anghinolfi, M.; Anton, G; Anvar, S.; Ardid Ramírez, Miguel; Bou Cabo, Manuel; Camarena Femenia, Francisco; Ferri García, Marcelino; Larosa, Giuseppina; Martínez Mora, Juan Antonio(Elsevier, 2012-04)
The group velocity of light has been measured at eight different wavelengths between 385 nm and 532 nm in the Mediterranean Sea at a depth of about 2.2 km with the ANTARES optical beacon systems. A parametrisation of the ...
[EN] Calibration of acoustic neutrino telescopes with neutrino-like signals is essential to evaluate the feasibility of the technique and to know the efficiency of the detectors. However, it is not straightforward to have ...
Ardid Ramírez, Miguel; Bou Cabo, Manuel; Camarena Femenia, Francisco; Espinosa Roselló, Víctor; Larosa, Giuseppina; Llorens Alvarez, Carlos David; Martínez Mora, Juan Antonio(Elsevier, 2011-01-11)
[EN] In this paper we present a possible solution for the acoustic positioning system of KM3NeT, a future very large undersea neutrino telescope. The system consists of an array of budget-priced acoustic transducers that ...
Rocabado Rocha, José Luís(Universitat Politècnica de València, 2020-10-28)
[ES] Se utilizarán técnicas de machine learning para determinar la dirección de llegada de los neutrinos detectados por los sensores del telescopio submarino ANTARES (http://antares.in2p3.fr). Para ello se analizará un ...
Hernández-Rey, Juan José; Ardid Ramírez, Miguel; Bou Cabo, Manuel; Calvo, David; Díaz, Antonio F.; Gozzini, Sara Rebecca; Martínez Mora, Juan Antonio; Navas, Sergio; Real, Diego; Salesa Greus, Francisco; Sánchez Losa, Agustín; Zornoza, Juan de Dios; Zúniga, Juan(MDPI AG, 2022-02)
[EN] The primary scientific goal of neutrino telescopes is the detection and study of cosmic neutrino signals. However, the range of physics topics that these instruments can tackle is exceedingly wide and diverse. Neutrinos ...
Adrián Martínez, Silvia; Aguilar, JA; Al Samarai, I; Albert, A; Andre, M; Anghinolfi, M; Anton, G; Anvar, S; Ardid Ramírez, Miguel; Bou Cabo, Manuel; Camarena Femenia, Francisco; Ferri García, Marcelino; Larosa, Giuseppina; Martínez Mora, Juan Antonio(Elsevier, 2012-05)
Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to ...
Aguilar, J.A; Al Samarai, I; Albert, A.; André, M.; Anghinolfi, M.; Anton, G; Anvar, S.; Ardid Ramírez, Miguel; Bou Cabo, Manuel; Camarena Femenia, Francisco; Larosa, Giuseppina; Martínez Mora, Juan Antonio(Elsevier, 2011-02)
The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the ...