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dc.contributor.authorAiello, S
dc.contributor.authorAlbert, Arthur
dc.contributor.authorAlves Garre, Sergio
dc.contributor.authorAly, Zineb
dc.contributor.authorAmbrosone, Antonio
dc.contributor.authorAmeli, Fabrizio
dc.contributor.authorAndré, Michel
dc.contributor.authorAnghinolfi, Marco
dc.contributor.authorAnguita, M.
dc.contributor.authorArdid Ramírez, Miguel
dc.contributor.authorArdid Ramírez, Joan Salvador
dc.contributor.authorAublin, J.
dc.contributor.authorBagatelas, Christos
dc.contributor.otherCentre Tecnològic de Vilanova i la Geltrú
dc.date.accessioned2023-03-09T14:34:49Z
dc.date.available2023-03-09T14:34:49Z
dc.date.issued2023-02-01
dc.identifier.citationAiello, S. [et al.]. KM3NeT broadcast optical data transport system. "Journal of instrumentation", 1 Febrer 2023, vol. 18, núm. T02001.
dc.identifier.issn1748-0221
dc.identifier.otherhttps://arxiv.org/abs/2210.13328
dc.identifier.urihttp://hdl.handle.net/2117/384808
dc.description.abstractThe optical data transport system of the KM3NeT neutrino telescope at the bottom of the Mediterranean Sea will provide more than 6000 optical modules in the detector arrays with a point-to-point optical connection to the control stations onshore. The ARCA and ORCA detectors of KM3NeT are being installed at a depth of about 3500 m and 2500 m, respectively and their distance to the control stations is about 100 kilometers and 40 kilometers. In particular, the two detectors are optimised for the detection of cosmic neutrinos with energies above about 1 TeV (ARCA) and for the detection of atmospheric neutrinos with energies in the range 1 GeV–1 TeV (ORCA). The expected maximum data rate is 200 Mbps per optical module. The implemented optical data transport system matches the layouts of the networks of electro-optical cables and junction boxes in the deep sea. For efficient use of the fibres in the system the technology of Dense Wavelength Division Multiplexing is applied. The performance of the optical system in terms of measured bit error rates, optical budget are presented. The next steps in the implementation of the system are also discussed.
dc.language.isoeng
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshTelescopes
dc.subject.lcshAstroparticle physics
dc.subject.lcshOptical detectors
dc.subject.lcshTerms—time calibration
dc.subject.otherCherenkov detectors
dc.subject.otherData Processing
dc.subject.otherLarge detector systems for particle and astroparticle physics
dc.subject.otherOptics
dc.titleKM3NeT broadcast optical data transport system
dc.typeArticle
dc.subject.lemacNeutrins
dc.subject.lemacDetectors òptics
dc.subject.lemacTelescopis
dc.subject.lemacAstrofísica
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.identifier.doi10.1088/1748-0221/18/02/T02001
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://iopscience.iop.org/article/10.1088/1748-0221/18/02/T02001
dc.rights.accessOpen Access
local.identifier.drac35235373
dc.description.versionPostprint (published version)
local.citation.authorAiello, S.; Albert, A.; Alves, S.; Zineb, A.; Ambrosone, A.; Ameli, F.; Andre, M.; Anghinolfi, M.; Anguita, M.; Ardid, M.; Ardid, J.; Aublin, J.; Bagatelas, C.
local.citation.publicationNameJournal of instrumentation
local.citation.volume18
local.citation.numberT02001
dc.description.authorshipArticle signat per 254 autors/es: L. Bailly-Salins, B. Baret, S. Basegmez du Pree, Y. Becherini, M. Bendahman, F. Benfenati, E. Berbee, V. Bertin, S. Biagi, M. Boettcher, M. Bou Cabo, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, H. Brânzaş, R. Bruijn, Brunner, R. Bruno, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, F. Carenini, V. Carretero, P. Castaldi, S. Celli, L. Cerisy, M. Chabab, N. Chau, A. Chen, R. Cherkaoui El Moursli, S. Cherubini, V. Chiarella, T. Chiarusi, M. Circella, R. Cocimano, J.A.B. Coelho, A. Coleiro, R. Coniglione, P. Coyle, A. Creusot, A. Cruz, G. Cuttone, A. D’Amico, R. Dallier, Y. Darras, A. De Benedittis, B. De Martino, R. Del Burgo, I. Di Palma, A.F. Díaz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, M. Dörr, E. Drakopoulou, D. Drouhin, T. Eberl, A. Eddyamoui, T. van Eeden, M. Eff, D. van Eijk,I. El Bojaddaini, S. El Hedri, A. Enzenhöfer, V. Espinosa, G. Ferrara, M.D. Filipović, F. Filippini, L.A. Fusco, J. Gabriel, T. Gal, J. García Méndez, A. Garcia Soto, F. Garufi, 𝑓 C. Gatius Oliver, N. Geißelbrecht, L. Gialanella, E. Giorgio, A. Girardi, I. Goos, S.R. Gozzini, R. Gracia, K. Graf, D. Guderian, C. Guidi, B. Guillon, M. Gutiérrez, L. Haegel, H. van Haren, A. Heijboer, A. Hekalo, L. Hennig, J.J. Hernández-Rey, F. Huang, W. Idrissi Ibnsalih, G. Illuminati, C.W. James, D. Janezashvili, M. de Jong, P. de Jong, B.J. Jung, P. Kalaczyński, O. Kalekin, U.F. Katz, N.R. Khan Chowdhury, G. Kistauri, F. van der Knaap, P. Kooijman, A. Kouchner, V. Kulikovskiy, M. Labalme, R. Lahmann, A. Lakhal, M. Lamoureux, G. Larosa, C. Lastoria, A. Lazo, R. Le Breton, S. Le Stum, G. Lehaut, E. Leonora, N. Lessing, G. Levi, S. Liang, M. Lindsey Clark,𝑙 F. Longhitano, L. Maderer, J. Majumdar, J. Mańczak, A. Margiotta, A. Marinelli, C. Markou, L. Martin, J.A. Martínez-Mora, A. Martini, F. Marzaioli, M. Mastrodicasa, S. Mastroianni, K.W. Melis, S. Miccichè, G. Miele, P. Migliozzi, E. Migneco, P. Mijakowski, C.M. Mollo, L. Morales-Gallegos, C. Morley-Wong, A. Moussa, R. Muller, M.R. Musone, M. Musumeci, L. Nauta, S. Navas, C.A. Nicolau, B. Nkosi, B. Ó Fearraigh, A. Orlando, E. Oukacha, J. Palacios González, G. Papalashvili, R. Papaleo, E.J. Pastor Gomez, A.M. Păun, G.E. Păvălaş, C. Pellegrino, S. Peña Martínez,𝑙 M. Perrin-Terrin,𝑑 J. Perronnel, V. Pestel, P. Piattelli, O. Pisanti, C. Poirè, V. Popa, T. Pradier, S. Pulvirenti, G. Quéméner, U. Rahaman, N. Randazzo, S. Razzaque, I.C. Rea, D. Real, S. Reck, G. Riccobene, J. Robinson, A. Romanov, F. Salesa Greus, D.F.E. Samtleben, A. Sánchez Losa, M. Sanguineti, C. Santonastaso, D. Santonocito, P. Sapienza, A. Sathe, J. Schmelling, J. Schnabel, M.F. Schneider, J. Schumann, H. M. Schutte, J. Seneca, I. Sgura, R. Shanidze, A. Sharma, A. Simonelli, A. Sinopoulou, M.V. Smirnov, B. Spisso, M. Spurio, D. Stavropoulos, S.M. Stellacci, M. Taiuti, K. Tavzarashvili, Y. Tayalati, H. Tedjditi, H. Thiersen, S. Tsagkli, V. Tsourapis, E. Tzamariudaki, V. Van Elewyck, G. Vannoye, G. Vasileiadis, F. Versari, S. Viola, D. Vivolo, H. Warnhofer, J. Wilms, E. de Wolf, H. Yepes-Ramirez, T. Yousfi, S. Zavatarelli, A. Zegarelli, D. Zito, J.D. Zornoza, J. Zúñiga𝑐 and N. Zywucka


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