GCN Circular 32523
Subject
IceCube-220907A - IceCube observation of a high-energy neutrino candidate track-like event
Date
2022-09-07T12:26:59Z (2 years ago)
From
Dr. Massimiliano Lincetto at Ruhr-Universitaet Bochum <lincetto@astro.rub.de>
The IceCube Collaboration (http://icecube.wisc.edu/) reports:
On 2022-09-07 at 06:46:47.52 UT IceCube detected a track-like event with
a moderate probability of being of astrophysical origin. The event was
selected by the ICECUBE_Astrotrack_Bronze alert stream. The average
astrophysical neutrino purity��for Bronze alerts is 30%. This alert has
an estimated false alarm rate of 0.46 events per year due to atmospheric
backgrounds. The IceCube detector was in a normal operating state at the
time of detection.
After the initial automated alert
(https://gcn.gsfc.nasa.gov/notices_amon_g_b/137019_70165712.amon),
more��sophisticated reconstruction algorithms have been applied offline,
with the direction refined to:
Date: 2022-09-07
Time: 06:46:47.52 UT
RA: 224.81 (+2.07 / -1.95 deg 90% PSF containment) J2000
Dec: +44.70 (+0.94 / -1.06 deg 90% PSF containment) J2000
We encourage follow-up by ground and space-based instruments to help
identify a possible astrophysical source for the candidate neutrino.
There are no Fermi 4FGL or 3FHL catalog sources in the 90% uncertainty
region. The nearest gamma-ray source in either catalog is 4FGL
J1504.6+4343 at RA: 226.16, Dec: 43.72 deg (1.38 deg away from the
best-fit event position).
The IceCube Neutrino Observatory is a cubic-kilometer neutrino detector
operating at the geographic South Pole, Antarctica. The IceCube realtime
alert point of contact can be reached at roc@icecube.wisc.edu