@article{fdi:010074929,
  title = {{S}earch for multimessenger sources of gravitational waves and high-energy neutrinos with advanced {LIGO} during {I}ts first observing run, {ANTARES}, and {I}ce{C}ube},
  author = {{A}lbert, {A}. and {A}ndre, {M}. and {A}nghinolfi, {M}. and {A}rdid, {M}. and {A}ubert, {J}. {J}. and {A}ublin, {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}oumaaza, {J}. and {B}ourret, {S}. and {B}ouwhuis, {M}. {C}. and {B}ranzas, {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 {C}habab, {M}. 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}olomer, {M}. 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}istefano, {C}. and {D}i {P}alma, {I}. and {D}omi, {A}. and {D}ona, {R}. 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}ermani, {P}. and {F}errara, {G}. and {F}usco, {L}. and {G}ay, {P}. 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. and {ANTARES} {C}ollaboration and {I}ce{C}ube {C}ollaboration and {LIGO} {S}cientific {C}ollaboration and {V}irgo {C}ollaboration},
  editor = {},
  language = {{ENG}},
  abstract = {{A}strophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. {H}igh-energy neutrinos are signatures of such outflows. {T}he detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the outflow. {W}e searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from {A}dvanced {LIGO} from its first observing run {O}1, and data from the {ANTARES} and {I}ce{C}ube neutrino observatories from the same time period. {W}e focused on candidate events whose astrophysical origins could not be determined from a single messenger. {W}e found no significant coincident candidate, which we used to constrain the rate density of astrophysical sources dependent on their gravitational-wave and neutrino emission processes.},
  keywords = {gravitational waves ; neutrinos},
  booktitle = {},
  journal = {{A}strophysical {J}ournal},
  volume = {870},
  numero = {2},
  pages = {art. 134 [16 p.]},
  ISSN = {0004-637{X}},
  year = {2019},
  DOI = {10.3847/1538-4357/aaf21d},
  URL = {https://www.documentation.ird.fr/hor/fdi:010074929},
}