Search for counterpart to IceCube-211125A with ANTARES
ATel #15065; Alexis Coleiro (APC/Universite de Paris) and Damien Dornic (CPPM/CNRS) on behalf of the ANTARES Collaboration.
on 26 Nov 2021; 09:58 UT
Credential Certification: Antoine Kouchner (kouchner@apc.univ-paris-diderot.fr)
Subjects: >GeV, TeV, Neutrinos, Transient
Using data from the ANTARES detector, we have performed a follow-up analysis of the recently reported bronze track event IceCube-211125A (GCN #31126). The reconstructed origin was 6 degrees below the horizon for ANTARES at the time of the alert.
No muon neutrino candidate events were recorded within 90% error box of the IceCube event during a +/- 1h time-window centered on the IceCube event time, and over which the potential source remained visible 82.5% of the time window. This leads to a preliminary 90% confidence level upper limit on the muon-neutrino radiant fluence from a point source of about 12 GeV.cm^-2 over the energy range 5 TeV â 5 PeV (the range corresponding to 5-95% of the detectable flux) for an E^-2 power-law spectrum, and 35 GeV.cm^-2 (1 - 500 TeV) for an E^-2.5 spectrum.
A search over an extended time window of +/- 1 day has also yielded no detection (37% visibility).
ANTARES [http://antares.in2p3.fr/] is the largest undersea neutrino detector (Mediterranean Sea) and it is primarily sensitive to astrophysical neutrinos in the TeV-PeV energy range. At 10 TeV, the median angular resolution for muon neutrinos is about 0.5 degrees. In the range 1-100 TeV ANTARES has a competitive sensitivity to this position in the sky.
