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High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube
Journal article   Open access   Peer reviewed

High-energy Neutrino follow-up search of Gravitational Wave Event GW150914 with ANTARES and IceCube

Antares Collaboration, IceCube Collaboration, LIGO Scientific Collaboration, Virgo Collaboration, Gwenhaël de Wasseige and Mark Louis Andre
Physical review D
2016
url
https://doi.org/10.1103/physrevd.93.122010View
Accepted (AM)Open Access (Publisher-Specific) Open
url
https://doi.org/10.1103/PhysRevD.93.122010View
Published, Version of Record (VoR) Open

Abstract

angular resolution ANTARES atmosphere: background electromagnetic gravitational radiation gravitational radiation: emission IceCube LIGO neutrino: detector
We present the high-energy-neutrino follow-up observations of the first gravitational wave transient GW150914 observed by the Advanced LIGO detectors on September 14, 2015. We search for coincident neutrino candidates within the data marc:recorded by the IceCube and Antares neutrino detectors. A possible joint detection could be used in targeted electromagnetic follow-up observations, given the significantly better angular resolution of neutrino events compared to gravitational waves. We find no neutrino candidates in both temporal and spatial coincidence with the gravitational wave event. Within ±500  s of the gravitational wave event, the number of neutrino candidates detected by IceCube and Antares were three and zero, respectively. This is consistent with the expected atmospheric background, and none of the neutrino candidates were directionally coincident with GW150914. We use this nondetection to constrain neutrino emission from the gravitational-wave event.

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Collaboration types
Domestic collaboration
International collaboration
Web of Science research areas
Astronomy & Astrophysics
Physics, Particles & Fields
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