@article{fdi:010070389, title = {{S}earch for high-energy neutrinos from gravitational wave event {GW}151226 and candidate {LVT}151012 with {ANTARES} and {I}ce{C}ube}, 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}ertin, {V}. and {B}iagi, {S}. and {B}ormuth, {R}. and {B}ourret, {S}. 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}elli, {S}. 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}eschamps, {A}. and {D}e {B}onis, {G}. and {D}istefano, {C}. and {D}i {P}alma, {I}. 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}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. and {ANTARES} and {I}ce{C}ube and {LIGO} {S}ci and {V}irgo}, editor = {}, language = {{ENG}}, abstract = {{T}he {A}dvanced {LIGO} observatories detected gravitational waves from two binary black hole mergers during their first observation run ({O}1). {W}e present a high-energy neutrino follow-up search for the second gravitational wave event, {GW}151226, as well as for gravitational wave candidate {LVT}151012. {W}e find two and four neutrino candidates detected by {I}ce{C}ube, and one and zero detected by {ANTARES}, within +/- 500 s around the respective gravitational wave signals, consistent with the expected background rate. {N}one of these neutrino candidates are found to be directionally coincident with {GW}151226 or {LVT}151012. {W}e use nondetection to constrain isotropic-equivalent high-energy neutrino emission from {GW}151226, adopting the {GW} event's 3{D} localization, to less than 2 x 10(51)-2 x 10(54) erg.}, keywords = {}, booktitle = {}, journal = {{P}hysical {R}eview {D}}, volume = {96}, numero = {2}, pages = {art. 022005 [15 p.]}, ISSN = {2470-0010}, year = {2017}, DOI = {10.1103/{P}hys{R}ev{D}.96.022005}, URL = {https://www.documentation.ird.fr/hor/fdi:010070389}, }