IceCube-220524A

The IceCube Collaboration (http://icecube.wisc.edu/) reports:


On 2022-05-24 at 07:41:32.185 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 2.8556 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/136662_35405932.amon), 
more��sophisticated reconstruction algorithms have been applied offline, 
with the direction refined to:


Date: 2022-05-24

Time: 07:41:32.185 UT

RA: +47.20 (+4.21/-2.51 deg 90% PSF containment) J2000

Dec: -3.28 (+0.77/-0.89 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 
J0307.8-0419 at RA: +46.95 deg, Dec: -4.33 deg (2.06 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

The IceCube Collaboration (http://icecube.wisc.edu/) reports:

IceCube has performed a search [1] for additional track-like muon neutrino events arriving from the direction of IceCube-220524A (https://gcn.gsfc.nasa.gov/gcn3/32102.gcn3
Loading...
 
 ) in a time range of 1000 seconds centered on the alert event time (2022-05-24 07:33:12.185 UTC to 2022-05-24 07:49:52.185 UTC) during which IceCube was collecting good quality data. Excluding the event that prompted the alert, zero track-like events are found within the 90% containment region of IceCube-220524A. The IceCube sensitivity to neutrino point sources with an E^-2.5 spectrum (E^2 dN/dE at 1 TeV) within the locations spanned by the 90% spatial containment region of IceCube-220524A ranges from 1.5e-01 to 2.9e-01 GeV cm^-2 in a 1000 second time window. 90% of events IceCube would detect from a source at this declination with an E^-2.5 spectrum have energies in the approximate energy range between 3e+02 GeV and 2e+05 GeV.

A subsequent search was performed including 2 days of data centered on the alert event time (2022-05-23 07:41:32.185 UTC to 2022-05-25 07:41:32.185 UTC).  In this case, we report a p-value of 1.00, consistent with no significant excess of track events. The IceCube sensitivity to neutrino point sources with an E^-2.5 spectrum (E^2 dN/dE at 1 TeV) within the locations spanned by the 90% spatial containment region of IceCube-220524A ranges from 1.6e-01 to 3.0e-01 GeV cm^-2 in a 2 day time window.

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<mailto:roc@icecube.wisc.edu>.

[1] IceCube Collaboration, R. Abbasi  et al., ApJ 910 4 (2021)

S. Garrappa (DESY-Zeuthen) and S. Buson (Univ. of Wuerzburg) on behalf 
of the Fermi-LAT collaboration:

We report an analysis of observations of the vicinity of the high-energy 
IC220524A neutrino event (GCN 32102
Loading...
 
 ) with all-sky survey data from the 
Large Area Telescope (LAT), on board the Fermi Gamma-ray Space 
Telescope. The IceCube event was detected on 2022-05-24 at 07:41:32.185 
UT (T0) with J2000 position RA = +47.20 (+4.21, -2.51) deg, Decl. = 
-3.28 (+0.77, -0.89) deg (90% PSF containment). No cataloged gamma-ray 
(>100 MeV) sources are located within the 90% IC220524A localization 
region (4FGL-DR3; arXiv:2201.11184
Loading...
 
 ; The Fermi-LAT collaboration 2020, 
ApJS, 247, 33).

We searched for intermediate (days to years) timescale emission from a 
new gamma-ray transient source. Preliminary analysis indicates no 
significant (> 5 sigma) new excess emission (> 100 MeV) at the IC220524A 
best-fit position. Assuming a power-law spectrum (photon index = 2.0 
fixed) for a point source at the IC220524A best-fit position, the >100 
MeV flux upper limit (95% confidence) is < 5.9e-10 ph cm^-2 s^-1 for 
~13-years (2008-08-04 to 2022-05-24 UTC), and < 8.5e-9 (< 5.4e-8) ph 
cm^-2 s^-1 for a 1-month (1-day) integration time before T0.

Since Fermi normally operates in an all-sky scanning mode, regular 
monitoring of this source will continue. For these observations the 
Fermi-LAT contact persons are S. Garrappa (simone.garrappa at desy.de) 
and S. Buson (sara.buson at uni-wuerzburg.de).

The Fermi-LAT is a pair conversion telescope designed to cover the 
energy band from 20 MeV to greater than 300 GeV. It is the product of an 
international collaboration between NASA and DOE in the U.S. and many 
scientific institutions across France, Italy, Japan and Sweden.