GCN Circular 27612
Subject
IceCube-200421A - IceCube observation of a high-energy neutrino candidate event
Date
2020-04-21T03:10:12Z (4 years ago)
From
Erik Blaufuss at U. Maryland/IceCube <blaufuss@umd.edu>
The IceCube Collaboration (http://icecube.wisc.edu/) reports:
On 21 April, 2020 at 00:35:24.24 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 threshold astrophysical neutrino purity for Bronze alerts is 30% . This alert has an estimated false alarm rate of 2.8 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/133985_60770138.amon), more sophisticated reconstruction algorithms have been applied offline, with the direction refined to:
Date: 21 April 2020
Time: 00:35:24.24 UT
RA: 87.93 (+3.44/- 2.83 (+1.88/-1.64) deg 90% (50%) PSF containment) J2000
Dec: 8.23 (+2.09/-1.84 (+1.25/-1.19) deg 90% (50%) 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 50% uncertainty region. The nearest gamma-ray source in either catalog is 4FGL J0545.0+0613 at RA: 86.27 deg, Dec: 6.23 deg (2.59 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