AMON IC_HAWC NuEm-201124A: No Neutrino Counterpart detected with ANTARES
ATel #14223; Alexis Coleiro (APC/Universite de Paris) and Damien Dornic (CPPM/CNRS) on behalf of the ANTARES Collaboration
on 26 Nov 2020; 09:18 UT
Credential Certification: Antoine Kouchner (kouchner@apc.univ-paris-diderot.fr)
Subjects: Gamma Ray, >GeV, TeV, Neutrinos, Transient
Using data from the ANTARES detector, we have performed a follow-up analysis of the recently reported AMON IC-HAWC coincidence alert NuEm-201124A (GCN#28950 https://gcn.gsfc.nasa.gov/gcn3/28950.gcn3).
No up-going muon neutrino candidate events were detected within 3 degrees from the coincidence coordinates over a time period [10h48 - 14h13 UTC] corresponding to 57% of the HAWC transit time mentioned in the AMON notice, during which the potential source remained visible in the up-going field of view of ANTARES.
This leads to a preliminary 90% confidence level upper limit on the muon neutrino radiant fluence from a point source located at the coordinates of the coincidence as reported by AMON, of about 19 GeV.cm^-2 over the energy range 4TeV â 4PeV (the range corresponding to 5-95% of the detectable flux) for an E^-2 power-law spectrum, and about 31 GeV.cm^-2 (720 GeV - 380TeV) for an E^-2.5 spectrum.
A search over an extended time window of +/-1 day has also yielded no detection (46% visibility).
ANTARES [https://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.
