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

A. Albert; A. Margiotta; K. A. Olive; K. Agashe; C. Amsler; Marta C. Antonelli; D. M. Asner; H. Baer; T. Basaglia; C. W. Bauer; M.G. Aartsen; K. Abraham; M. Ackermann; Morten Ankersen Medici; D. Jason Koskinen; Subir Sarkar; Michael James Larson; M Rameez; E. Hansen; Markus Tobias Ahlers

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, A. Margiotta, K. A. Olive, K. Agashe, C. Amsler, Marta C. Antonelli, D. M. Asner, H. Baer, T. Basaglia, C. W. Bauer, M.G. Aartsen, K. Abraham, M. Ackermann, Morten Ankersen Medici, D. Jason Koskinen, Subir Sarkar, Michael James Larson, M Rameez, E. Hansen, Markus Tobias Ahlers

38 Citationer (Scopus)

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.

Originalsprog	Engelsk
Artikelnummer	022005
Tidsskrift	Physical Review D
Vol/bind	96
ISSN	2470-0010
DOI	https://doi.org/10.1103/physrevd.96.022005
Status	Udgivet - 15 jul. 2017

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10.1103/physrevd.96.022005

PhysRevD.96.022005Forlagets udgivne version, 2,4 MB
PhysRevD.96.022005.pdfForlagets udgivne version, 2,54 MBLicens: CC BY-NC

http://arxiv.org/pdf/1703.06298Licens: Andet

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Albert, A., Margiotta, A., Olive, K. A., Agashe, K., Amsler, C., Antonelli, M. C., Asner, D. M., Baer, H., Basaglia, T., Bauer, C. W., Aartsen, M. G., Abraham, K., Ackermann, M., Medici, M. A., Koskinen, D. J., Sarkar, S., Larson, M. J., Rameez, M., Hansen, E., & Ahlers, M. T. (2017). Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube. Physical Review D, 96, Artikel 022005. https://doi.org/10.1103/physrevd.96.022005

Albert, A, Margiotta, A, Olive, KA, Agashe, K, Amsler, C, Antonelli, MC, Asner, DM, Baer, H, Basaglia, T, Bauer, CW, Aartsen, MG, Abraham, K, Ackermann, M, Medici, MA, Koskinen, DJ, Sarkar, S, Larson, MJ, Rameez, M, Hansen, E & Ahlers, MT 2017, 'Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube', Physical Review D, bind 96, 022005. https://doi.org/10.1103/physrevd.96.022005

@article{8c24e2bce6b84399a798f8e8abbab921,

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 A. Margiotta and Olive, {K. A.} and K. Agashe and C. Amsler and Antonelli, {Marta C.} and Asner, {D. M.} and H. Baer and T. Basaglia and Bauer, {C. W.} and M.G. Aartsen and K. Abraham and M. Ackermann and Medici, {Morten Ankersen} and Koskinen, {D. Jason} and Subir Sarkar and Larson, {Michael James} and M Rameez and E. Hansen and Ahlers, {Markus Tobias}",

year = "2017",

month = jul,

day = "15",

doi = "10.1103/physrevd.96.022005",

language = "English",

volume = "96",

journal = "Physical Review D",

issn = "2470-0010",

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TY - JOUR

T1 - Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube

AU - Albert, A.

AU - Margiotta, A.

AU - Olive, K. A.

AU - Agashe, K.

AU - Amsler, C.

AU - Antonelli, Marta C.

AU - Asner, D. M.

AU - Baer, H.

AU - Basaglia, T.

AU - Bauer, C. W.

AU - Aartsen, M.G.

AU - Abraham, K.

AU - Ackermann, M.

AU - Medici, Morten Ankersen

AU - Koskinen, D. Jason

AU - Sarkar, Subir

AU - Larson, Michael James

AU - Rameez, M

AU - Hansen, E.

AU - Ahlers, Markus Tobias

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.

U2 - 10.1103/physrevd.96.022005

DO - 10.1103/physrevd.96.022005

M3 - Journal article

SN - 2470-0010

VL - 96

JO - Physical Review D

JF - Physical Review D

M1 - 022005

ER -

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

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