Skip to main content
New Announcement Feature, Code of Conduct, Circular Revisions. See news and announcements

GCN Circular 34877

Subject
LIGO/Virgo/KAGRA S231025a: two counterpart neutrino candidates from IceCube neutrino searches
Date
2023-10-25T03:45:25Z (7 months ago)
From
acz2122@columbia.edu
Via
Web form
The IceCube Collaboration (http://icecube.wisc.edu/) reports:

A search for track-like muon neutrino events detected by IceCube consistent with the sky
localization of the low-significance gravitational wave candidate S231025a in a time range of 1000 seconds
centered on the alert event time (2023-10-25 03:03:04 UTC to 2023-10-25 03:19:44 UTC)
has been performed [1,2]. During this time period IceCube was collecting good quality data.
One hypothesis test was conducted for this low-significance gravitational wave event. The
search uses a Bayesian approach to quantify the joint GW + neutrino event significance, which
assumes a binary merger scenario and accounts for known astrophysical priors, such as GW source
distance, in the significance estimate [3].

Two track-like events are found in spatial and temporal coincidence with the gravitational-wave
candidate S231025a calculated from the map circulated by LVK as S231025a-2-Preliminary. This
represents an overall pre-trial p-value of 0.0010 for the Bayesian search.

The reported p-value here does not account for any trials correction (multiple hypotheses testing). The false alarm rate of these coincidences can be obtained by multiplying the p-values with their corresponding GW trigger rates. Further details are available at https://gcn.nasa.gov/missions/icecube and at https://roc.icecube.wisc.edu/public/LvkNuTrackSearch.


Properties of the coincident event(s) are shown below.

dt(s)	RA(deg)		Dec(deg)	Angular uncertainty(deg)  p-value(generic transient) p-value(Bayesian)
-----------------------------------------------------------------------------------------------------
-331.09   226.87     -4.88          1.81                        not applicable		0.0253
+284.41   240.49     -3.37          2.06                        not applicable		0.0011



where:
dt = Time of track event minus time of GW trigger (sec)
Angular uncertainty = Angular uncertainty of track event: the radius of a circle
 	representing 90% CL containment by area.
p-value = the p-value for this specific track event from each search.

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


[1] M. G. Aartsen et al 2020 ApJL 898 L10
[2] Abbasi et al. Astrophys.J. 944 (2023) 1, 80
[3] I. Bartos et al. 2019 Phys. Rev. D 100, 083017
Looking for U.S. government information and services? Visit USA.gov