[vsnet-grb-info 24122] LIGO/Virgo S191110af: Upper limits from IceCube neutrino searches

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Mon Nov 11 09:07:58 JST 2019


TITLE:   GCN CIRCULAR
NUMBER:  26221
SUBJECT: LIGO/Virgo S191110af: Upper limits from IceCube neutrino searches
DATE:    19/11/11 00:05:52 GMT
FROM:    Raamis Hussain at IceCube  <raamis.hussain at icecube.wisc.edu>

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

Searches [1,2] for track-like muon neutrino events detected by IceCube
consistent with the sky localization of gravitational-wave candidate
S191110af
 in a time range of 1000 seconds [3] centered on the alert event time
(2019-11-10 22:58:24.183 UTC to 2019-11-10 23:15:04.183 UTC) have been
performed.

During this time period IceCube was collecting good quality data.
No significant track-like events are found in spatial coincidence of
S191110af calculated from the map circulated in the 2-Initial notice.

IceCube's sensitivity assuming an E^-2 spectrum (E^2 dN/dE) to neutrino
point sources within the locations spanned by the 90% spatial containment
of S191110af ranges from 0.029 to 1.067 GeV cm^-2 in a 1000 second
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 at icecube.wisc.edu


[1] Bartos et al. arXiv:1810.11467 (2018) and Countryman et
al.arXiv:1901.05486 (2019)
[2] PoS(ICRC2019)918 and Braun et al., Astroparticle Physics 29, 299 (2008)
[3] Baret et al., Astroparticle Physics 35, 1 (2011)



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