Počet záznamů: 1
Search for High-energy neutrinos from binary neutron star merger GW170817 with ANTARES, iceCube, and the Pierre Auger observatory
- 1.0484926 - FZÚ 2021 RIV US eng J - Článek v odborném periodiku
Albert, A. - André, M. - Anghinolfi, M. - Blažek, Jiří - Boháčová, Martina - Chudoba, Jiří - Ebr, Jan - Juryšek, Jakub - Mandát, Dušan - Palatka, Miroslav - Pech, Miroslav - Prouza, Michael - Řídký, Jan - dos Santos, Eva M. Martins - Schovánek, Petr - Trávníček, Petr - Vícha, Jakub - Yushkov, Alexey … celkem 1938 autorů
Search for High-energy neutrinos from binary neutron star merger GW170817 with ANTARES, iceCube, and the Pierre Auger observatory.
Astrophysical Journal Letters. Roč. 850, č. 2 (2017), s. 1-18, č. článku L35. ISSN 2041-8205. E-ISSN 2041-8213
Grant CEP: GA MŠMT LG15014; GA MŠMT EF16_013/0001402
Grant ostatní: OP VVV - AUGER-CZ(XE) CZ.02.1.01/0.0/0.0/16_013/0001402
Výzkumná infrastruktura: AUGER-CZ - 90038
Institucionální podpora: RVO:68378271
Klíčová slova: gamma-ray burst * general * gravitational waves * neutrinos
Obor OECD: Particles and field physics
Impakt faktor: 6.634, rok: 2017
Způsob publikování: Open access
The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merger of this binary was also recorded by the Fermi Gamma-ray Burst Monitor (Fermi-GBM), and the Anti-Coincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory (INTEGRAL), indicating particle acceleration by the source. The precise location of the event was determined by optical detections of emission following the merger. We searched for high-energy neutrinos from the merger in the GeV-EeV energy range using the ANTARES, IceCube, and Pierre Auger Observatories. No neutrinos directionally coincident with the source were detected within +/- 500 s around the merger time. Additionally, no MeV neutrino burst signal was detected coincident with the merger.
Trvalý link: http://hdl.handle.net/11104/0280049
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