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An algorithm for the reconstruction of high-energy neutrino-induced particle showers and its application to the ANTARES neutrino telescope
Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.-J.; Avgitas, T.; Baret, B.; Barrios-Martí, J.; Basa, S.; Bertin, V.; Biagi, S.; Bormuth, R.; Bourret, S.; Bouwhuis, M.C.; Bruijn, R.; Brunner, J.; Busto, J.; Capone, A.; Caramete, L.; Carr, J.; Celli, S.; Chiarusi, T.; Circella, M.; Coelho, C.O.A.; Coleiro, A.; Coniglione, R.; Costantini, H.; Coyle, P.; Creusot, A.; Deschamps, A.; De Bonis, G.; Distefano, C.; Di Palma, I.; Domi, A.; Donzaud, C.; Dornic, D.; Drouhin, D.; Eberl, T.; El Bojaddaini, I.; Elsässer, D.; Enzenhofer, A.; Felis, I.; Folger, F.; Fusco, L.A.; Galata, S.; Gay, P.; Giordano, V.; Glotin, H.; Grégoire, T.; Gracia-Ruiz, R.; Graf, K.; Hallmann, S.; van Haren, H.; Heijboer, A.J.; Hello, Y.; Hernandez-Rey, J.J.; Hößl, J.; Hofestädt, J.; Hugon, C.; Illuminati, G.; James, C.W.; de Jong, M.; Jongen, M.; Kadler, M.; Kalekin, O.; Katz, U.; Kießling, D.; Kouchner, A.; Kreter, M.; Kreykenbohm, I.; Kulikovskiy, V.; Lachaud, C.; Lahmann, R.; Lefevre, D.; Leonora, E.; Lotze, M.; Loucatos, S.; Marcelin, M.; Margiotta, A.; Marinelli, A.; Martinez-Mora, J.A.; Mele, R.; Melis, K.; Michael, T.; Migliozzi, P.; Moussa, A.; Nezri, E.; Organokov, M.; Pavalas, G.E.; Pellegrino, C.; Perrina, C.; Piattelli, P.; Popa, V.; Pradier, T.; Quinn, L.; Racca, C.; Riccobene, G.; Sanchez-Losa, A.; Saldaña, M.; Salvadori, I.; Samtleben, D.F.E.; Sanguineti, M.; Sapienza, P.; Schussler, F.; Sieger, C.; Spurio, M.; Stolarczyk, T.; Taiuti, M.; Tayalati, Y.; Trovato, A.; Turpin, D.; Tönnis, C.; Vallage, B.; Van Elewyck, V.; Versari, F.; Vivolo, D.; Vizzoca, A.; Wilms, J.; Zornoza, J.D.; Zuniga, J. (2017). An algorithm for the reconstruction of high-energy neutrino-induced particle showers and its application to the ANTARES neutrino telescope. Eur. Phys. J. C 77(6): 419. https://dx.doi.org/10.1140/epjc/s10052-017-4979-2
In: The European Physical Journal C. Springer: Berlin. ISSN 1434-6044, meer
Peer reviewed article  

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  • Albert, A.
  • André, M.
  • Anghinolfi, M.
  • Anton, G.
  • Ardid, M.
  • Aubert, J.-J.
  • Avgitas, T.
  • Baret, B.
  • Barrios-Martí, J.
  • Basa, S.
  • Bertin, V.
  • Biagi, S.
  • Bormuth, R.
  • Bourret, S.
  • Bouwhuis, M.C.
  • Bruijn, R.
  • Brunner, J.
  • Busto, J.
  • Capone, A.
  • Caramete, L.
  • Carr, J.
  • Celli, S.
  • Chiarusi, T.
  • Circella, M.
  • Coelho, C.O.A.
  • Coleiro, A.
  • Coniglione, R.
  • Costantini, H.
  • Coyle, P.
  • Creusot, A.
  • Deschamps, A.
  • De Bonis, G.
  • Distefano, C.
  • Di Palma, I.
  • Domi, A.
  • Donzaud, C.
  • Dornic, D.
  • Drouhin, D.
  • Eberl, T.
  • El Bojaddaini, I.
  • Elsässer, D.
  • Enzenhofer, A.
  • Felis, I.
  • Folger, F.
  • Fusco, L.A.
  • Galata, S.
  • Gay, P.
  • Giordano, V.
  • Glotin, H.
  • Grégoire, T.
  • Gracia-Ruiz, R.
  • Graf, K.
  • Hallmann, S.
  • van Haren, H., meer
  • Heijboer, A.J.
  • Hello, Y.
  • Hernandez-Rey, J.J.
  • Hößl, J.
  • Hofestädt, J.
  • Hugon, C.
  • Illuminati, G.
  • James, C.W.
  • de Jong, M.
  • Jongen, M.
  • Kadler, M.
  • Kalekin, O.
  • Katz, U.
  • Kießling, D.
  • Kouchner, A.
  • Kreter, M.
  • Kreykenbohm, I.
  • Kulikovskiy, V.
  • Lachaud, C.
  • Lahmann, R.
  • Lefevre, D.
  • Leonora, E.
  • Lotze, M.
  • Loucatos, S.
  • Marcelin, M.
  • Margiotta, A.
  • Marinelli, A.
  • Martinez-Mora, J.A.
  • Mele, R.
  • Melis, K.
  • Michael, T.
  • Migliozzi, P.
  • Moussa, A.
  • Nezri, E.
  • Organokov, M.
  • Pavalas, G.E.
  • Pellegrino, C.
  • Perrina, C.
  • Piattelli, P.
  • Popa, V.
  • Pradier, T.
  • Quinn, L.
  • Racca, C.
  • Riccobene, G.
  • Sanchez-Losa, A.
  • Saldaña, M.
  • Salvadori, I.
  • Samtleben, D.F.E.
  • Sanguineti, M.
  • Sapienza, P.
  • Schussler, F.
  • Sieger, C.
  • Spurio, M.
  • Stolarczyk, T.
  • Taiuti, M.
  • Tayalati, Y.
  • Trovato, A.
  • Turpin, D.
  • Tönnis, C.
  • Vallage, B.
  • Van Elewyck, V.
  • Versari, F.
  • Vivolo, D.
  • Vizzoca, A.
  • Wilms, J.
  • Zornoza, J.D.
  • Zuniga, J.

Abstract
    A novel algorithm to reconstruct neutrino-induced particle showers within the ANTARES neutrino telescope is presented. The method achieves a median angular resolution of 6∘ for shower energies below 100 TeV. Applying this algorithm to 6 years of data taken with the ANTARES detector, 8 events with reconstructed shower energies above 10 TeV are observed. This is consistent with the expectation of about 5 events from atmospheric backgrounds, but also compatible with diffuse astrophysical flux measurements by the IceCube collaboration, from which 2–4 additional events are expected. A 90% C.L. upper limit on the diffuse astrophysical neutrino flux with a value per neutrino flavour of E2⋅Φ90%=4.9⋅10−8GeV⋅cm−2⋅s−1⋅sr−1 is set, applicable to the energy range from 23 TeV to 7.8 PeV, assuming an unbroken E−2 spectrum and neutrino flavour equipartition at Earth.

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