%0 Journal Article
%T All-sky search for high-energy neutrinos from gravitational wave event GW170104 with the ANTARES neutrino telescope
%A ANTARES Collaboration (Albert, A. et al
%A Barrios-Marti, J.
%A Coleiro, A.
%A Hernandez-Rey, J. J.
%A Illuminati, G.
%A Lotze, M.
%A Tönnis, C.
%A Zornoza, J. D.
%A Zuñiga, J.
%J European Physical Journal C
%D 2017
%V 77
%N 12
%I Springer
%@ 1434-6044
%G English
%F ANTARESCollaborationAlbert_etal2017
%O WOS:000419035700002
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3441), last updated on Mon, 19 Aug 2019 06:55:53 +0000
%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.
%R 10.1140/epjc/s10052-017-5451-z
%U http://arxiv.org/abs/1710.03020
%U https://doi.org/10.1140/epjc/s10052-017-5451-z
%P 911 - 7pp