[vsnet-grb-info 20017] IceCube-171106A - IceCube observation of a high-energy neutrino candidate
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Nov 7 07:37:35 JST 2017
TITLE: GCN CIRCULAR
NUMBER: 22105
SUBJECT: IceCube-171106A - IceCube observation of a high-energy neutrino candidate
DATE: 17/11/06 22:37:07 GMT
FROM: Ignacio Taboada at Georgia Inst of Tech <itaboada at gatech.edu>
The IceCube Collaboration (http://icecube.wisc.edu/) reports:
On November 6, 2017 IceCube detected a track-like, very-high-energy
event with a high probability of being of astrophysical origin. The
event was identified by the Extremely High Energy (EHE) track event
selection. The IceCube detector was in a normal operating state. EHE
events typically have a neutrino interaction vertex that is outside the
detector and produce a muon that traverses the detector volume, and have
a high light level (a proxy for energy).
After the initial automated alert
(https://gcn.gsfc.nasa.gov/notices_amon/17569642_130214.amon), more
sophisticated reconstruction algorithms have been applied offline, with
the direction refined to:
Date: 17/11/06 (yy/mm/dd)
Time: 18:39:39.21 UT
RA: 340.00 (-0.50/+0.70 deg 90% PSF containment) J2000
Dec: +7.40 (-0.25/+0.35 deg 90% PSF containment) J2000
Initial offline analysis of this event indicates that the event is
consistent with being produced by a neutrino with energy in excess of 1
PeV. The initially reported signalness and energy values are likely
underestimated.
As indicated in the initial notice, the neutrino candidate is temporally
close to Fermi GBM trigger 531686417. However, recently, Fermi GBM has
been triggering frequently on a galactic source that is not spatially
coincident with the event reported here.
We 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 at icecube.wisc.edu
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