학술논문

The prototype detection unit of the KM3NeT detector: KM3NeT Collaboration
Document Type
Original Paper
Author
Adrián-Martínez, S.Ageron, M.Aharonian, F.Aiello, S.Albert, A.Ameli, F.Anassontzis, E. G.Androulakis, G. C.Anghinolfi, M.Anton, G.Anvar, S.Ardid, M.Avgitas, T.Balasi, K.Band, H.Barbarino, G.Barbarito, E.Barbato, F.Baret, B.Baron, S.Barrios, J.Belias, A.Berbee, E.van den Berg, A. M.Berkien, A.Bertin, V.Beurthey, S.van Beveren, V.Beverini, N.Biagi, S.Biagioni, A.Bianucci, S.Billault, M.Birbas, A.Boer Rookhuizen, H.Bormuth, R.Bouché, V.Bouhadef, B.Bourlis, G.Boutonnet, C.Bouwhuis, M.Bozza, C.Bruijn, R.Brunner, J.Cacopardo, G.Caillat, L.Calamai, M.Calvo, D.Capone, A.Caramete, L.Caruso, F.Cecchini, S.Ceres, A.Cereseto, R.Champion, C.Château, F.Chiarusi, T.Christopoulou, B.Circella, M.Classen, L.Cocimano, R.Coleiro, A.Colonges, S.Coniglione, R.Cosquer, A.Costa, M.Coyle, P.Creusot, A.Cuttone, G.D’Amato, C.D’Amico, A.De Bonis, G.De Rosa, G.Deniskina, N.Destelle, J.-J.Distefano, C.Di Capua, F.Donzaud, C.Dornic, D.Dorosti-Hasankiadeh, Q.Drakopoulou, E.Drouhin, D.Drury, L.Durand, D.Eberl, T.Elsaesser, D.Enzenhöfer, A.Fermani, P.Fusco, L. A.Gajanana, D.Gal, T.Galatà, S.Garufi, F.Gebyehu, M.Giordano, V.Gizani, N.Gracia Ruiz, R.Graf, K.Grasso, R.Grella, G.Grmek, A.Habel, R.van Haren, H.Heid, T.Heijboer, A.Heine, E.Henry, S.Hernández-Rey, J. J.Herold, B.Hevinga, M. A.van der Hoek, M.Hofestädt, J.Hogenbirk, J.Hugon, C.Hößl, J.Imbesi, M.James, C. W.Jansweijer, P.Jochum, J.de Jong, M.Jongen, M.Kadler, M.Kalekin, O.Kappes, A.Kappos, E.Katz, U.Kavatsyuk, O.Keller, P.Kieft, G.Koffeman, E.Kok, H.Kooijman, P.Koopstra, J.Korporaal, A.Kouchner, A.Kreykenbohm, I.Kulikovskiy, V.Lahmann, R.Lamare, P.Larosa, G.Lattuada, D.Le Provost, H.Leismüller, K. P.Leisos, A.Lenis, D.Leonora, E.Lindsey Clark, M.Llorens Alvarez, C. D.Löhner, H.Lonardo, A.Loucatos, S.Louis, F.Maccioni, E.Mannheim, K.Manolopoulos, K.Margiotta, A.Mariş, O.Markou, C.Martínez-Mora, J. A.Martini, A.Masullo, R.Melis, K. W.Michael, T.Migliozzi, P.Migneco, E.Miraglia, A.Mollo, C. M.Mongelli, M.Morganti, M.Mos, S.Moudden, Y.Musico, P.Musumeci, M.Nicolaou, C.Nicolau, C. A.Orlando, A.Orzelli, A.Papaikonomou, A.Papaleo, R.Păvălaş, G. E.Peek, H.Pellegrino, C.Pellegriti, M. G.Perrina, C.Piattelli, P.Pikounis, K.Popa, V.Pradier, Th.Priede, M.Pühlhofer, G.Pulvirenti, S.Racca, C.Raffaelli, F.Randazzo, N.Rapidis, P. A.Razis, P.Real, D.Resvanis, L.Reubelt, J.Riccobene, G.Rovelli, A.Saldaña, M.Samtleben, D. F. E.Sanguineti, M.Santangelo, A.Sapienza, P.Schmelling, J.Schnabel, J.Sciacca, V.Sedita, M.Seitz, T.Sgura, I.Simeone, F.Sipala, V.Spitaleri, A.Spurio, M.Stavropoulos, G.Steijger, J.Stolarczyk, T.Stransky, D.Taiuti, M.Terreni, G.Tézier, D.Théraube, S.Thompson, L. F.Timmer, P.Trasatti, L.Trovato, A.Tselengidou, M.Tsirigotis, A.Tzamarias, S.Tzamariudaki, E.Vallage, B.Van Elewyck, V.Vermeulen, J.Vernin, P.Vicini, P.Viola, S.Vivolo, D.Werneke, P.Wiggers, L.Wilms, J.de Wolf, E.van Wooning, R. H. L.Zonca, E.Zornoza, J. D.Zúñiga, J.Zwart, A.
Source
The European Physical Journal C: Particles and Fields. February 2016 76(2):1-12
Subject
Language
English
ISSN
1434-6044
1434-6052
Abstract
A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80 km offshore the Italian coast. KM3NeT in its final configuration will contain several hundreds of detection units. Each detection unit is a mechanical structure anchored to the sea floor, held vertical by a submerged buoy and supporting optical modules for the detection of Cherenkov light emitted by charged secondary particles emerging from neutrino interactions. This prototype string implements three optical modules with 31 photomultiplier tubes each. These optical modules were developed by the KM3NeT Collaboration to enhance the detection capability of neutrino interactions. The prototype detection unit was operated since its deployment in May 2014 until its decommissioning in July 2015. Reconstruction of the particle trajectories from the data requires a nanosecond accuracy in the time calibration. A procedure for relative time calibration of the photomultiplier tubes contained in each optical module is described. This procedure is based on the measured coincidences produced in the sea by the ∘.