@article{PAR00017887,
  title = {{T}he {S}earch for {N}eutrinos from {TXS} 0506+056 with the {ANTARES} {T}elescope},
  author = {{A}lbert, {A}. and {A}ndr{\'e}, {M}. and {A}nghinolfi, {M}. and {A}nton, {G}. 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}enin, {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, {T}. {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},
  editor = {},
  language = {{ENG}},
  abstract = {{T}he results of three different searches for neutrino candidates, associated with the {I}ce{C}ube-170922{A} event or from the direction of {TXS} 0506+056, by the {ANTARES} neutrino telescope, are presented. {T}he first search refers to the online follow-up of the {I}ce{C}ube alert; the second is based on the standard time-integrated method employed by the {C}ollaboration to search for point-like neutrino sources; the third uses information from the {I}ce{C}ube time-dependent analysis that reported bursting activity centered on 2014 {D}ecember 13, as input for an {ANTARES} time-dependent analysis. {T}he online follow-up and the time-dependent analysis yield no events related to the source. {T}he time-integrated study performed over a period from 2007 to 2017 fits 1.03 signal events, which corresponds to a p-value of 3.4% (not considering trial factors). {O}nly for two other astrophysical objects in our candidate list has a smaller p-value been found. {W}hen considering that 107 sources have been investigated, the post-trial p-value for {TXS} 0506+056 corresponds to 87%.},
  keywords = {astroparticle physics ; elementary particles ; galaxies: active},
  booktitle = {},
  journal = {{A}strophysical {J}ournal {L}etters},
  volume = {863},
  numero = {2},
  pages = {{L}30},
  ISSN = {2041-8205},
  year = {2018},
  DOI = {10.3847/2041-8213/aad8c0},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00017887},
}