TITLE: GCN CIRCULAR NUMBER: 39549 SUBJECT: IceCube-250302A - IceCube observation of a high-energy neutrino candidate track-like event DATE: 25/03/02 16:04:00 GMT FROM: A. Zegarelli at Ruhr University Bochum azegarelli@icecube.wisc.edu
The IceCube Collaboration (http://icecube.wisc.edu/) reports:
On 2025-03-02 at 03:20:52.90 UT IceCube detected a track-like event with a high probability of being of astrophysical origin. The event was selected by the ICECUBE_Astrotrack_GOLD alert stream. The average astrophysical neutrino purity for Gold alerts is 50%. This alert has an estimated false alarm rate of 0.1579 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/140601_60511904.amon), more sophisticated reconstruction algorithms have been applied offline, with the direction refined to:
Date: 2025-03-02 Time: 03:20:52.90 UT RA: 348.05 (+0.38 -0.43 deg 90% PSF containment) J2000 Dec: 3.77 (+0.42 -0.41 deg 90% PSF containment) J2000
No known gamma-ray sources listed in the Fermi 4FGL-DR4 or 3FHL catalogs are located within the 90% uncertainty region of the event.
However, given the particularly high signalness (~97%) and energy (~1.5 PeV) of this event, we strongly encourage follow-up by ground and space-based instruments to help identify a possible astrophysical source for the candidate neutrino.
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
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