Details
Original language | English |
---|---|
Article number | 122010 |
Journal | Physical Review D |
Volume | 93 |
Issue number | 12 |
Publication status | Published - 23 Jun 2016 |
Abstract
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 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.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- Physics and Astronomy (miscellaneous)
Cite this
- Standard
- Harvard
- Apa
- Vancouver
- BibTeX
- RIS
In: Physical Review D, Vol. 93, No. 12, 122010, 23.06.2016.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube
AU - ANTARES Collaboration
AU - Icecube Collaboration
AU - The LIGO Scientific Collaboration
AU - The Virgo Collaboration
AU - Adrián-Martínez, S.
AU - Albert, A.
AU - André, M.
AU - Anghinolfi, M.
AU - Anton, G.
AU - Ardid, M.
AU - Aubert, J. J.
AU - Avgitas, T.
AU - Ahlers, M.
AU - Ahrens, M.
AU - Kelley, J. L.
AU - Klein, S. R.
AU - Schmidt, T.
AU - Wendt, C.
AU - Wolf, M.
AU - Xu, X. W.
AU - Xu, Y.
AU - Adya, V. B.
AU - Bose, S.
AU - Brown, D. D.
AU - Chen, Y.
AU - Danilishin, S. L.
AU - Danzmann, Karsten
AU - Fricke, T. T.
AU - Hanke, M. M.
AU - Hennig, J.
AU - Heurs, Michele
AU - Kawazoe, Fumiko
AU - Lee, H. M.
AU - Lück, Harald
AU - Luo, J.
AU - Nguyen, T. T.
AU - Schmidt, J.
AU - Schmidt, P.
AU - Shaltev, M.
AU - Steinmeyer, Daniel
AU - Sun, L.
AU - Vahlbruch, Henning Fedor Cornelius
AU - Wang, M.
AU - Wang, X.
AU - Wang, Y.
AU - Wei, L. W.
AU - Willke, Benno
AU - Wittel, Holger
AU - Zhang, L.
AU - Zhang, Y.
AU - Zhou, M.
AU - Wagner, S.
AU - Allen, Bruce
AU - Bisht, A.
AU - Denker, Timo
AU - Kaufer, Stefan
AU - Krüger, Christian
AU - Lough, J. D.
AU - Sawadsky, A.
PY - 2016/6/23
Y1 - 2016/6/23
N2 - 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 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.
AB - 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 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.
UR - http://www.scopus.com/inward/record.url?scp=84976408194&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.93.122010
DO - 10.1103/PhysRevD.93.122010
M3 - Article
AN - SCOPUS:84976408194
VL - 93
JO - Physical Review D
JF - Physical Review D
SN - 2470-0010
IS - 12
M1 - 122010
ER -