Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

A. Albert; M. André; M. Anghinolfi; G. Anton; M. Ardid; J. J. Aubert; T. Avgitas; B. Baret; J. Barrios-Martí; S. Basa; V. Bertin; S. Biagi; R. Bormuth; S. Bourret; M. C. Bouwhuis; R. Bruijn; J. Brunner; J. Busto; A. Capone; L. Caramete; J. Carr; S. Celli; T. Chiarusi; M. Circella; J. A.B. Coelho; A. Coleiro; R. Coniglione; H. Costantini; P. Coyle; A. Creusot; A. Deschamps; G. De Bonis; C. Distefano; I. Di Palma; C. Donzaud; D. Dornic; D. Drouhin; T. Eberl; I. El Bojaddaini; D. Elsässer; A. Enzenhöfer; I. Felis; L. A. Fusco; S. Galatà; P. Gay; V. Giordano; H. Glotin; T. Grégoire; R. Gracia Ruiz; V. Mandic; (LIGO Scientific Collaboration, and Virgo Collaboration); (ANTARES Collaboration); (IceCube Collaboration)

doi:10.1103/PhysRevD.96.022005

Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

A. Albert, M. André, M. Anghinolfi, G. Anton, M. Ardid, J. J. Aubert, T. Avgitas, B. Baret, J. Barrios-Martí, S. Basa, V. Bertin, S. Biagi, R. Bormuth, S. Bourret, M. C. Bouwhuis, R. Bruijn, J. Brunner, J. Busto, A. Capone, L. CarameteJ. Carr, S. Celli, T. Chiarusi, M. Circella, J. A.B. Coelho, A. Coleiro, R. Coniglione, H. Costantini, P. Coyle, A. Creusot, A. Deschamps, G. De Bonis, C. Distefano, I. Di Palma, C. Donzaud, D. Dornic, D. Drouhin, T. Eberl, I. El Bojaddaini, D. Elsässer, A. Enzenhöfer, I. Felis, L. A. Fusco, S. Galatà, P. Gay, V. Giordano, H. Glotin, T. Grégoire, R. Gracia Ruiz, V. Mandic, (LIGO Scientific Collaboration, and Virgo Collaboration), (ANTARES Collaboration), (IceCube Collaboration)

Physics and Astronomy (Twin Cities)

Research output: Contribution to journal › Article › peer-review

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Abstract

The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection 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.

Original language	English (US)
Article number	022005
Journal	Physical Review D
Volume	96
Issue number	2
DOIs	https://doi.org/10.1103/PhysRevD.96.022005
State	Published - Jul 15 2017

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© 2017 American Physical Society.

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Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J. J., Avgitas, T., Baret, B., Barrios-Martí, J., Basa, S., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Bouwhuis, M. C., Bruijn, R., Brunner, J., Busto, J., Capone, A., ... (IceCube Collaboration) (2017). Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube. Physical Review D, 96(2), Article 022005. https://doi.org/10.1103/PhysRevD.96.022005

Albert, A, André, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, JJ, Avgitas, T, Baret, B, Barrios-Martí, J, Basa, S, Bertin, V, Biagi, S, Bormuth, R, Bourret, S, Bouwhuis, MC, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coelho, JAB, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Elsässer, D, Enzenhöfer, A, Felis, I, Fusco, LA, Galatà, S, Gay, P, Giordano, V, Glotin, H, Grégoire, T, Gracia Ruiz, R, Mandic, V, (LIGO Scientific Collaboration, and Virgo Collaboration), (ANTARES Collaboration) & (IceCube Collaboration) 2017, 'Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube', Physical Review D, vol. 96, no. 2, 022005. https://doi.org/10.1103/PhysRevD.96.022005

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title = "Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube",

abstract = "The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection 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.",

author = "A. Albert and M. Andr{\'e} and M. Anghinolfi and G. Anton and M. Ardid and Aubert, {J. J.} and T. Avgitas and B. Baret and J. Barrios-Mart{\'i} and S. Basa and V. Bertin and S. Biagi and R. Bormuth and S. Bourret and Bouwhuis, {M. C.} and R. Bruijn and J. Brunner and J. Busto and A. Capone and L. Caramete and J. Carr and S. Celli and T. Chiarusi and M. Circella and Coelho, {J. A.B.} and A. Coleiro and R. Coniglione and H. Costantini and P. Coyle and A. Creusot and A. Deschamps and {De Bonis}, G. and C. Distefano and {Di Palma}, I. and C. Donzaud and D. Dornic and D. Drouhin and T. Eberl and {El Bojaddaini}, I. and D. Els{\"a}sser and A. Enzenh{\"o}fer and I. Felis and Fusco, {L. A.} and S. Galat{\`a} and P. Gay and V. Giordano and H. Glotin and T. Gr{\'e}goire and {Gracia Ruiz}, R. and V. Mandic and {(LIGO Scientific Collaboration, and Virgo Collaboration)} and {(ANTARES Collaboration)} and {(IceCube Collaboration)}",

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AU - Albert, A.

AU - André, M.

AU - Anghinolfi, M.

AU - Anton, G.

AU - Ardid, M.

AU - Aubert, J. J.

AU - Avgitas, T.

AU - Baret, B.

AU - Barrios-Martí, J.

AU - Basa, S.

AU - Bertin, V.

AU - Biagi, S.

AU - Bormuth, R.

AU - Bourret, S.

AU - Bouwhuis, M. C.

AU - Bruijn, R.

AU - Brunner, J.

AU - Busto, J.

AU - Capone, A.

AU - Caramete, L.

AU - Carr, J.

AU - Celli, S.

AU - Chiarusi, T.

AU - Circella, M.

AU - Coelho, J. A.B.

AU - Coleiro, A.

AU - Coniglione, R.

AU - Costantini, H.

AU - Coyle, P.

AU - Creusot, A.

AU - Deschamps, A.

AU - De Bonis, G.

AU - Distefano, C.

AU - Di Palma, I.

AU - Donzaud, C.

AU - Dornic, D.

AU - Drouhin, D.

AU - Eberl, T.

AU - El Bojaddaini, I.

AU - Elsässer, D.

AU - Enzenhöfer, A.

AU - Felis, I.

AU - Fusco, L. A.

AU - Galatà, S.

AU - Gay, P.

AU - Giordano, V.

AU - Glotin, H.

AU - Grégoire, T.

AU - Gracia Ruiz, R.

AU - Mandic, V.

AU - (LIGO Scientific Collaboration, and Virgo Collaboration)

AU - (ANTARES Collaboration)

AU - (IceCube Collaboration)

PY - 2017/7/15

Y1 - 2017/7/15

N2 - The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection 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.

AB - The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by Antares, within ±500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection 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.

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U2 - 10.1103/PhysRevD.96.022005

DO - 10.1103/PhysRevD.96.022005

M3 - Article

AN - SCOPUS:85027050091

SN - 2470-0010

VL - 96

JO - Physical Review D

JF - Physical Review D

IS - 2

M1 - 022005

ER -

Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

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