TY - JOUR
T1 - KM3NeT Time calibration with Nanobeacons
AU - KM3NeT Collaboration
AU - Losa, Agustín Sánchez
AU - González, Juan Palacios
AU - Greus, Francisco Salesa
AU - Román, Juan Zúñiga
AU - Máñez, Diego Real
AU - Díaz-Aldagalán, David Calvo
AU - Aiello, S.
AU - Albert, A.
AU - Alves Garre, S.
AU - Aly, Z.
AU - Ambrosone, A.
AU - Ameli, F.
AU - Andre, M.
AU - Androutsou, E.
AU - Anguita, M.
AU - Aphecetche, L.
AU - Ardid, M.
AU - Ardid, S.
AU - Atmani, H.
AU - Aublin, J.
AU - Bailly-Salins, L.
AU - Bardačová, Z.
AU - Baret, B.
AU - Bariego-Quintana, A.
AU - Basegmez du Pree, S.
AU - Becherini, Y.
AU - Bendahman, M.
AU - Benfenati, F.
AU - Benhassi, M.
AU - Benoit, D. M.
AU - Berbee, E.
AU - Bertin, V.
AU - Biagi, S.
AU - Boettcher, M.
AU - Bonanno, D.
AU - Boumaaza, J.
AU - Bouta, M.
AU - Bouwhuis, M.
AU - Bozza, C.
AU - Bozza, R. M.
AU - Brânzaş, H.
AU - Bretaudeau, F.
AU - Bruijn, R.
AU - Brunner, J.
AU - Bruno, R.
AU - Buis, E.
AU - Buompane, R.
AU - Busto, J.
AU - Caiffi, B.
AU - Razzaque, S.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.
PY - 2024/9/27
Y1 - 2024/9/27
N2 - The KM3NeT Collaboration is building a neutrino telescope in the Mediterranean Sea. The detector is expected to achieve an angular resolution better than 0.1 degrees for energies above 10 TeV. This is critical for attaining one of the key goals of the experiment, i.e. the identification of cosmic neutrino sources. In order to achieve a good angular resolution, the detector requires a relative time calibration of the order of 1 ns. The Nanobeacon is a cost-effective time calibration device developed by the KM3NeT Collaboration to synchronise in situ the detector photomultipliers with a nanosecond relative accuracy. In this contribution we will describe the design and operation of the Nanobeacon. Moreover, we will present the results of data taken in real sea-conditions and we will show how they are used to validate the time calibration parameters measured onshore.
AB - The KM3NeT Collaboration is building a neutrino telescope in the Mediterranean Sea. The detector is expected to achieve an angular resolution better than 0.1 degrees for energies above 10 TeV. This is critical for attaining one of the key goals of the experiment, i.e. the identification of cosmic neutrino sources. In order to achieve a good angular resolution, the detector requires a relative time calibration of the order of 1 ns. The Nanobeacon is a cost-effective time calibration device developed by the KM3NeT Collaboration to synchronise in situ the detector photomultipliers with a nanosecond relative accuracy. In this contribution we will describe the design and operation of the Nanobeacon. Moreover, we will present the results of data taken in real sea-conditions and we will show how they are used to validate the time calibration parameters measured onshore.
UR - http://www.scopus.com/inward/record.url?scp=85212305516&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85212305516
SN - 1824-8039
VL - 444
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1062
T2 - 38th International Cosmic Ray Conference, ICRC 2023
Y2 - 26 July 2023 through 3 August 2023
ER -