%0 Journal Article
%T First all-flavor neutrino pointlike source search with the ANTARES neutrino telescope
%+ Groupe de Recherche en Physique des Hautes Energies (GRPHE)
%+ Centre de Physique des Particules de Marseille (CPPM)
%+ AstroParticule et Cosmologie (APC (UMR_7164))
%+ Laboratoire d'Astrophysique de Marseille (LAM)
%+ Géoazur (GEOAZUR 7329)
%+ Université Paris-Sud - Paris 11 (UP11)
%+ Laboratoire de Physique de Clermont (LPC)
%+ Laboratoire des Sciences de l'Information et des Systèmes (LSIS)
%+ Institut universitaire de France (IUF)
%+ Institut méditerranéen d'océanologie (MIO)
%+ Département de Physique des Particules (ex SPP) (DPhP)
%+ Institut Pluridisciplinaire Hubert Curien (IPHC)
%A Albert, A.
%A André, M.
%A Anghinolfi, M.
%A Anton, G.
%A Ardid, M.
%A Aubert, J.-J.
%A Avgitas, T.
%A Baret, B.
%A Barrios-Mart́i, J.
%A Basa, S.
%A Belhorma, B.
%A Bertin, V.
%A Biagi, S.
%A Bormuth, R.
%A Bourret, S.
%A Bouwhuis, M.C.
%A Brânzaş, H.
%A Bruijn, R.
%A Brunner, J.
%A Busto, J.
%A Capone, A.
%A Caramete, L.
%A Carr, J.
%A Celli, S.
%A Cherkaoui El Moursli, R.
%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 Díaz, A.F.
%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 El Khayati, N.
%A Elsässer, D.
%A Enzenhöfer, A.
%A Ettahiri, A.
%A Fassi, F.
%A Felis, I.
%A Fusco, L.A.
%A Galatà, S.
%A Gay, P.
%A Giordano, V.
%A Glotin, H.
%A Grégoire, T.
%A Gracia Ruiz, R.
%A Graf, K.
%A Hallmann, S.
%A van Haren, H.
%A Heijboer, A.J.
%A Hello, Y.
%A Hernández-Rey, J.J.
%A Hössl, J.
%A Hofestädt, J.
%A Hugon, C.
%A Illuminati, G.
%A James, C.W.
%A de Jong, M.
%A Jongen, M.
%A Kadler, M.
%A Kalekin, O.
%A Katz, U.
%A Kiessling, D.
%A Kouchner, A.
%A Kreter, M.
%A Kreykenbohm, I.
%A Kulikovskiy, V.
%A Lachaud, C.
%A Lahmann, R.
%A Lefèvre, D.
%A Leonora, E.
%A Lotze, M.
%A Loucatos, S.
%A Marcelin, M.
%A Margiotta, A.
%A Marinelli, A.
%A Martínez-Mora, J.A.
%A Mele, R.
%A Melis, K.
%A Michael, T.
%A Migliozzi, P.
%A Moussa, A.
%A Navas, S.
%A Nezri, E.
%A Organokov, M.
%A Păvălaş, G.E.
%A Pellegrino, C.
%A Perrina, C.
%A Piattelli, P.
%A Popa, V.
%A Pradier, T.
%A Quinn, L.
%A Racca, C.
%A Riccobene, G.
%A Sánchez-Losa, A.
%A Saldaña, M.
%A Salvadori, I.
%A Samtleben, D.F.E.
%A Sanguineti, M.
%A Sapienza, P.
%A Schüssler, F.
%A Sieger, C.
%A Spurio, M.
%A Stolarczyk, Th.
%A Taiuti, M.
%A Tayalati, Y.
%A Trovato, A.
%A Turpin, D.
%A Tönnis, C.
%A Vallage, B.
%A van Elewyck, V.
%A Versari, F.
%A Vivolo, D.
%A Vizzoca, A.
%A Wilms, J.
%A Zornoza, J.D.
%A Zúñiga, J.
%< avec comité de lecture
%@ 1550-7998
%J Physical Review D
%I American Physical Society
%V 96
%N 8
%P 082001
%8 2017
%D 2017
%Z 1706.01857
%R 10.1103/PhysRevD.96.082001
%K neutrino: detector
%K neutrino: interaction
%K neutrino: flux
%K muon: track data analysis
%K muon: tracks
%K ANTARES
%K charged current
%K neutral current
%K energy spectrum
%K sensitivity
%K background
%K cluster
%K showers
%K IceCube
%K neutrino muon: interaction
%K upper limit
%Z Physics [physics]/Astrophysics [astro-ph]
%Z Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]
%Z Physics [physics]/High Energy Physics - Experiment [hep-ex]Journal articles
%X A search for cosmic neutrino sources using the data collected with the ANTARES neutrino telescope between early 2007 and the end of 2015 is performed. For the first time, all neutrino interactions—charged- and neutral-current interactions of all flavors—are considered in a search for point-like sources with the ANTARES detector. In previous analyses, only muon neutrino charged-current interactions were used. This is achieved by using a novel reconstruction algorithm for shower-like events in addition to the standard muon track reconstruction. The shower channel contributes about 23% of all signal events for an E-2 energy spectrum. No significant excess over background is found. The most signal-like cluster of events is located at (α,δ)=(343.8°,23.5°) with a significance of 1.9σ. The neutrino flux sensitivity of the search is about E2dΦ/dE=6×10-9  GeV cm-2 s-1 for declinations from -90° up to -42°, and below 10-8  GeV cm-2 s-1 for declinations up to 5°. The directions of 106 source candidates and 13 muon track events from the IceCube high-energy sample events are investigated for a possible neutrino signal and upper limits on the signal flux are determined.
%G English
%Z ANTARES
%2 https://hal.science/hal-01645803/document
%2 https://hal.science/hal-01645803/file/1706.01857.pdf
%L hal-01645803
%U https://hal.science/hal-01645803
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