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  Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube

ANTARES Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, & Virgo Collaboration (in preparation). Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-002D-0A3B-6 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-002D-0A3C-4
Genre: Paper

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1703.06298.pdf (Preprint), 4MB
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File downloaded from arXiv at 2017-04-19 11:01
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 Creators:
ANTARES Collaboration, Author              
IceCube Collaboration, Author              
LIGO Scientific Collaboration1, Author
Virgo Collaboration, Author              
Affiliations:
1MPI for Gravitational Physics, Max Planck Society, Am Mühlenberg 1, 14476 Golm, DE, escidoc:24007              

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Free keywords: Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE
 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 2 and 4 neutrino candidates detected by IceCube, and 1 and 0 detected by ANTARES, within $\pm500$ 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 non-detection to constrain isotropic-equivalent high-energy neutrino emission from GW151226 adopting the GW event's 3D localization, to less than $2\times 10^{51}-2\times10^{54}$ erg.

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 Dates: 2017-03-18
 Publication Status: Not specified
 Pages: 7 pages (+ author list), 4 figures
 Publishing info: -
 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1703.06298
URI: http://arxiv.org/abs/1703.06298
 Degree: -

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