%0 Journal Article
%9 ACL : Articles dans des revues avec comité de lecture répertoriées par l'AERES
%A Albert, A.
%A Andre, M.
%A Anghinolfi, M.
%A Anton, G.
%A Ardid, M.
%A Aubert, J. J.
%A Avgitas, T.
%A Baret, B.
%A Barrios-Marti, J.
%A Basa, S.
%A Bertin, V.
%A Biagi, S.
%A Bormuth, R.
%A Bourret, S.
%A Bouwhuis, M. C.
%A Bruijn, R.
%A Brunner, J.
%A Busto, J.
%A Capone, A.
%A Caramete, L.
%A Carr, J.
%A Celli, S.
%A Chiarusi, T.
%A Circella, M.
%A Coelho, J. A. B.
%A Coleiro, A.
%A Coniglione, R.
%A Costantini, H.
%A Coyle, P.
%A Creusot, A.
%A Deschamps, A.
%A De Bonis, G.
%A Distefano, C.
%A Di Palma, I.
%A Domi, A.
%A Donzaud, C.
%A Dornic, D.
%A Drouhin, D.
%A Eberl, T.
%A El Bojaddaini, I.
%A Elsasser, D.
%A Enzenhofer, A.
%A Felis, I.
%A Folger, F.
%A Fusco, L. A.
%A Galata, S.
%A Gay, P.
%A Giordano, V.
%A Glotin, H.
%A Gregoire, T.
%A Ruiz, R. G.
%A Graf, K.
%A Hallmann, S.
%A van Haren, H.
%A Heijboer, A. J.
%A Hello, Yann
%A et al.
%T An algorithm for the reconstruction of high-energy neutrino-induced particle showers and its application to the ANTARES neutrino telescope
%D 2017
%L fdi:010070236
%G ENG
%J European Physical Journal C
%@ 1434-6044
%M ISI:000403843200003
%N 6
%P art. 419 [11 ]
%R 10.1140/epjc/s10052-017-4979-2
%U https://www.documentation.ird.fr/hor/fdi:010070236
%> https://www.documentation.ird.fr/intranet/publi/2017/07/010070236.pdf
%V 77
%W Horizon (IRD)
%X 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 100TeV. Applying this algorithm to 6 years of data taken with theANTARES detector, 8 events with reconstructed shower energies above 10TeV 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 E-2.Phi(90%) = 4.9 . 10(-8) GeV.cm(-2).s(-1).sr(-1) is set, applicable to the energy range from 23TeV to 7.8PeV, assuming an unbroken E-2 spectrum and neutrino flavour equipartition at Earth.
%$ 020