[vsnet-grb-info 24300] LIGO/Virgo S191213g: Upper limits from IceCube neutrino searches
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Fri Dec 13 14:07:45 JST 2019
TITLE: GCN CIRCULAR
NUMBER: 26399
SUBJECT: LIGO/Virgo S191213g: Upper limits from IceCube neutrino searches
DATE: 19/12/13 05:04:48 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
S191213g
in a time range of 1000 seconds [3] centered on the alert event time
(2019-12-13 04:25:48.142 UTC to 2019-12-13 04:42:28.142 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
S191213g calculated from the map circulated in the 1-Preliminary 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 S191213g ranges from 0.029 to 0.382 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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