@article{PAR00016654,
  title = {{F}irst all-flavor neutrino pointlike source search 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}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 {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}alata, {S}. 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} search for cosmic neutrino sources using the data collected with the {ANTARES} neutrino telescope between early 2007 and the end of 2015 is performed. {F}or the first time, all neutrino interactions-charged and neutral-current interactions of all flavors-are considered in a search for point-like sources with the {ANTARES} detector. {I}n previous analyses, only muon neutrino charged-current interactions were used. {T}his is achieved by using a novel reconstruction algorithm for shower-like events in addition to the standard muon track reconstruction. {T}he shower channel contributes about 23% of all signal events for an {E}-2 energy spectrum. {N}o significant excess over background is found. {T}he most signal-like cluster of events is located at (alpha, delta) = (343.8 degrees, 23.5 degrees) with a significance of 1.9 sigma. {T}he neutrino flux sensitivity of the search is about {E}(2)d {P}hi/d{E} = 6 x 10(-9) {G}e{V} cm(-2) s(-1) for declinations from -90 degrees up to -42 degrees, and below 10(-8) {G}e{V} cm(-2) s(-1) for declinations up to 5 degrees. {T}he directions of 106 source candidates and 13 muon track events from the {I}ce{C}ube high-energy sample events are investigated for a possible neutrino signal and upper limits on the signal flux are determined.},
  keywords = {},
  booktitle = {},
  journal = {{P}hysical {R}eview {D}},
  volume = {96},
  numero = {8},
  pages = {art. 082001 [15 ]},
  ISSN = {2470-0010},
  year = {2017},
  DOI = {10.1103/{P}hys{R}ev{D}.96.082001},
  URL = {https://www.documentation.ird.fr/hor/{PAR}00016654},
}