@article{fdi:010066724,
  title = {{M}urchison widefield array limits on radio emission from antares neutrino events},
  author = {{C}roft, {S}. and {K}aplan, {D}. {L}. and {T}ingay, {S}. {J}. and {M}urphy, {T}. and {B}ell, {M}. {E}. and {R}owlinson, {A}. and {A}drian-{M}artinez, {S}. and {A}geron, {M}. and {A}lbert, {A}. and {A}ndre, {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}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. and {B}ouwhuis, {M}. {C}. 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}hiarusi, {T}. and {C}ircella, {M}. and {C}oleiro, {A}. and {C}oniglione, {R}. and {C}ostantini, {H}. and {C}oyle, {P}. and {C}reusot, {A}. and {D}ekeyser, {I}. and {D}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}onzaud, {C}. and {D}ornic, {D}. and {D}rouhin, {D}. and {E}berl, {T}. and {E}l {B}ojaddaini, {I}. and {E}lsasser, {D}. and {E}nzenhofer, {A}. and {F}ehn, {K}. and {F}elis, {I}. and {F}ermani, {P}. and {F}usco, {L}. {A}. and {G}alata, {S}. and {G}ay, {P}. and {G}eisselsoder, {S}. and {G}eyer, {K}. and {G}iordano, {V}. and {G}leixner, {A}. and {G}lotin, {H}. and {G}racia-{R}uiz, {R}. 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 = {{W}e present a search, using the {M}urchison {W}idefield {A}rray ({MWA}), for electromagnetic ({EM}) counterparts to two candidate high-energy neutrino events detected by the {ANTARES} neutrino telescope in 2013 {N}ovember and 2014 {M}arch. {T}hese events were selected by {ANTARES} because they are consistent, within 0 degrees.4, with the locations of galaxies within 20 {M}pc of {E}arth. {U}sing {MWA} archival data at frequencies between 118 and 182 {MH}z, taken similar to 20. days prior to, at the same time as, and up to a year after the neutrino triggers, we look for transient or strongly variable radio sources that are consistent with the neutrino positions. {N}o such counterparts are detected, and we set a 5 sigma upper limit for low-frequency radio emission of similar to 10(37) erg s(-1) for progenitors at 20 {M}pc. {I}f the neutrino sources are instead not in nearby galaxies, but originate in binary neutron star coalescences, our limits place the progenitors at z greater than or similar to 0.2. {W}hile it is possible, due to the high background from atmospheric neutrinos, that neither event is astrophysical, the {MWA} observations are nevertheless among the first to follow up neutrino candidates in the radio, and illustrate the promise of wide-field instruments like {MWA} for detecting {EM} counterparts to such events.},
  keywords = {neutrinos ; radio continuum: general},
  booktitle = {},
  journal = {{A}strophysical {J}ournal {L}etters},
  volume = {820},
  numero = {2},
  pages = {{L}24 [7 p.]},
  ISSN = {2041-8205},
  year = {2016},
  DOI = {10.3847/2041-8205/820/2/l24},
  URL = {https://www.documentation.ird.fr/hor/fdi:010066724},
}