2021
DOI: 10.48550/arxiv.2107.14472
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Multi-messenger and real-time astrophysics with the Baikal-GVD telescope

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Cited by 2 publications
(2 citation statements)
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“…Their probability being of background origin was estimated as 0.32, 0.29, 0.36, respectively [12]. The calculated limits on the neutrino fluence for energies 1 TeV -10 PeV with spectrum E −2 assuming equal fluence in all flavors for each considered alert were in the range of 1 -2.5 GeV/cm 2 [12], [15].…”
Section: Pos(ecrs)096mentioning
confidence: 95%
“…Their probability being of background origin was estimated as 0.32, 0.29, 0.36, respectively [12]. The calculated limits on the neutrino fluence for energies 1 TeV -10 PeV with spectrum E −2 assuming equal fluence in all flavors for each considered alert were in the range of 1 -2.5 GeV/cm 2 [12], [15].…”
Section: Pos(ecrs)096mentioning
confidence: 95%
“…Those multi-messenger programs will exploit the legacy of current real-time frameworks designed for IceCube and ANTARES (Ageron et al, 2012;. A similar procedure is being developed for Baikal-GVD [283]. Most of the triggers will be sent publicly to the astrophysical community as IceCube already does using GCN notices distributed through AMON (Astrophysical multi-messenger Observatory Network, Smith et al, 2013).…”
Section: Transient Sources and Alertsmentioning
confidence: 99%