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 |
|---|---|
| Article number | 022005 |
| Number of pages | 15 |
| Journal | Physical Review D |
| Volume | 96 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 15 Jul 2017 |
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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 and Virgo Collaboration.
In: Physical Review D, Vol. 96, No. 2, 022005, 15.07.2017.Research output: Contribution to journal › Article › Research › peer-review
TY - JOUR
T1 - Search for high-energy neutrinos from gravitational wave event GW151226 and candidate LVT151012 with ANTARES and IceCube
AU - Ackley, Kendall Danielle
AU - Lasky, Paul Daniel
AU - Levin, Yuri
AU - Qiu, Shi
AU - Sammut, Letizia Maria
AU - Thrane, Eric
AU - Whittle, Chris
AU - Zhu, Xingjiang
AU - ANTARES Collaboration
AU - IceCube Collaboration
AU - LIGO Scientific Collaboration and Virgo 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.
UR - http://www.scopus.com/inward/record.url?scp=85027050091&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.96.022005
DO - 10.1103/PhysRevD.96.022005
M3 - Article
AN - SCOPUS:85027050091
VL - 96
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 2
M1 - 022005
ER -