@article{fdi:010071951,
  title = {{A}ll-sky search for high-energy neutrinos from gravitational wave event {GW}170104 with the {ANTARES} neutrino telescope},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}nton, {G}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}vgitas, {T}. and {B}aret, {B}. and {B}arrios-{M}arti, {J}. and {B}asa, {S}. and {B}elhorma, {B}. and {B}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. and {B}ourret, {S}. and {B}ouwhuis, {M}. {C}. and {B}ranza, {H}. and {B}ruijn, {R}. and {B}runner, {J}. and {B}usto, {J}. and {C}apone, {A}. and {C}aramete, {L}. and {C}arr, {J}. and {C}elli, {S}. and {E}l {M}oursli, {R}. {C}. and {C}hiarusi, {T}. and {C}ircella, {M}. and {C}oelho, {J}. {A}. {B}. and {C}oleiro, {A}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}iaz, {A}. {F}. and {D}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}i {P}alma, {I}. and {D}omi, {A}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {B}ojaddaini, {I}. and {E}l {K}hayati, {N}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {E}ttahiri, {A}. and {F}assi, {F}. and {F}elis, {I}. and {F}usco, {L}. {A}. and {G}ay, {P}. and {G}iordano, {V}. and {G}lotin, {H}. and {G}regoire, {T}. and {R}uiz, {R}. {G}. and {G}raf, {K}. and {H}allmann, {S}. and van {H}aren, {H}. and {H}eijboer, {A}. {J}. and {H}ello, {Y}ann and et al.},
  editor = {},
  language = {{ENG}},
  abstract = {{A}dvanced {LIGO} detected a significant gravitational wave signal ({GW}170104) originating from the coalescence of two black holes during the second observation run on {J}anuary 4th, 2017. {A}nall-sky high-energy neutrino follow-up search has been made using data from the {A}ntares neutrino telescope, including both upgoing and downgoing events in two separate analyses. {N}o 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. {T}he non-detection is used to constrain isotropic-equivalent high-energy neutrino emission from {GW}170104 to less than similar to 1.2 x 10(55) erg for a {E}-2 spectrum. {T}his constraint is valid in the energy range corresponding to the 5-95% quantiles of the neutrino flux [3.2 {T}e{V}; 3.6 {P}e{V}], if the {GW} emitter was below the {A}ntares horizon at the alert time.},
  keywords = {},
  booktitle = {},
  journal = {{E}uropean {P}hysical {J}ournal {C}},
  volume = {77},
  numero = {12},
  pages = {art. 911 [7 p.]},
  ISSN = {1434-6044},
  year = {2017},
  DOI = {10.1140/epjc/s10052-017-5451-z},
  URL = {https://www.documentation.ird.fr/hor/fdi:010071951},
}