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    Bertin, V.; Bruijn, R.; Celli, S.; Coleiro, A.; Di Palma, I.; Kreykenbohm, I.; Kulikovskiy, V.; Sánchez-Losa, A.; Spurio, M.; Taiuti, M.; Zornoza, J. D.; Al Samarai, I.; Carver, T.; Chirkin, D.; DeYoung, T.; Ehrhardt, T.; Fuchs, T.; Krückl, G.; Mahn, K. B. M.; Nahnhauer, R.; Robertson, S.; Ruhe, T.; Seunarine, S.; Stachurska, J.; Stanev, T.; Tosi, D.; Abbott, T. D.; Agathos, M.; Baune, C.; Bersanetti, D.; Bisht, A.; Brady, P. R.; Brown, D. D.; Brown, N. M.; Callister, T. A.; Charlton, P.; Corbitt, T. R.; Coyne, R.; D’Antonio, S.; Da Silva Costa, C. F.; Dattilo, V.; Daw, E. J.; Deléglise, S.; Dent, T.; De Rosa, R.; DeRosa, R. T.; DeSalvo, R.; Di Fiore, L.; Di Virgilio, A.; Donovan, F.; Dovale Álvarez, M.; Ducrot, M.; Eggenstein, H. -B.; Etienne, Z.; Factourovich, M.; Fehrmann, H.; Fries, E. M.; Gayathri, V.; Giaime, J. A.; Gill, K.; Guidi, G. M.; Hild, S.; Huerta, E. A.; Junker, J.; Karki, S.; Koch, P.; Kuo, L.; Lord, J. E.; McGuire, S. C.; McIntyre, G.; McRae, T.; Mendell, G.; Mirshekari, S.; Mohapatra, S. R. P.; Mukherjee, Arunava; Munch, J.; Muniz, E. A. M.; Noack, A.; Oberling, J.; Oh, S. H.; Page, J.; Pan, H.; Pitkin, M.; Qiu, S.; Rolland, L.; Schale, P.; Schwalbe, S. G.; Sorrentino, F.; Vedovato, G.; Voss, D. V.; Wang, M.; Ward, R. L.; Whiting, B. F.; Williams, R. D.; Wimmer, M. H.; Wu, D. S.; Yamamoto, H.; Yap, M. J.; Zevin, M.; Zhang, Y.

    Physical review. D, 07/2017, Letnik: 96, Številka: 2
    Journal Article

    The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). Here, we introduce a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find 2 and 4 neutrino candidates detected by IceCube, and 1 and 0 detected by ANTARES, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are discovered to be directionally coincident with GW151226 or LVT151012. We use non-detection to constrain isotropic-equivalent high-energy neutrino emission from GW151226 adopting the GW event's 3D localization, to less than 2×1051₋2×1054 erg.