%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 Belhorma, B.
%A Bertin, V.
%A Biagi, S.
%A Bormuth, R.
%A Bourret, S.
%A Bouwhuis, M. C.
%A Branza, H.
%A Bruijn, R.
%A Brunner, J.
%A Busto, J.
%A Capone, A.
%A Caramete, L.
%A Carr, J.
%A Celli, S.
%A El Moursli, R. C.
%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 Diaz, 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 Elsasser, D.
%A Enzenhofer, A.
%A Ettahiri, A.
%A Fassi, F.
%A Felis, I.
%A Fusco, L. A.
%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 All-sky search for high-energy neutrinos from gravitational wave event GW170104 with the ANTARES neutrino telescope
%D 2017
%L fdi:010071951
%G ENG
%J European Physical Journal C
%@ 1434-6044
%M ISI:000419035700002
%N 12
%P art. 911 [7 ]
%R 10.1140/epjc/s10052-017-5451-z
%U https://www.documentation.ird.fr/hor/fdi:010071951
%> https://horizon.documentation.ird.fr/exl-doc/pleins_textes/divers18-01/010071951.pdf
%V 77
%W Horizon (IRD)
%X Advanced LIGO detected a significant gravitational wave signal (GW170104) originating from the coalescence of two black holes during the second observation run on January 4th, 2017. Anall-sky high-energy neutrino follow-up search has been made using data from the Antares neutrino telescope, including both upgoing and downgoing events in two separate analyses. No neutrino candidates were found within +/- 500 s around the GW event time nor any time clustering of events over an extended time window of +/- 3 months. The non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from GW170104 to less than similar to 1.2 x 10(55) erg for a E-2 spectrum. This constraint is valid in the energy range corresponding to the 5-95% quantiles of the neutrino flux [3.2 TeV; 3.6 PeV], if the GW emitter was below the Antares horizon at the alert time.
%$ 060 ; 020 ; 032