Skip to main content
Testing. You are viewing the public testing version of GCN. For the production version, go to https://gcn.nasa.gov.
End of INTEGRAL Operations. See news and announcements

GCN Circular 28530

Subject
IceCube-200926A: Upper limits from Fermi-GBM Observations
Date
2020-09-29T19:51:21Z (4 years ago)
From
Joshua Wood at MSFC/Fermi-GBM <joshua.r.wood@nasa.gov>
J. Wood (NASA/MSFC) reports on behalf of the Fermi-GBM team:

For the IceCube high-energy neutrino candidate event IceCube-200926A
(GCN 28504), at the event time Fermi-GBM was observing the reported
neutrino location at:

RA: 96.46 (+ 0.73 - 0.55  deg 90% PSF containment) J2000
Dec: -4.33 (+ 0.61  - 0.76  deg 90% PSF containment) J2000

There was no Fermi-GBM onboard trigger around the event time of the
neutrino candidate. An automated, blind search for short gamma-ray
bursts below the onboard triggering threshold in Fermi-GBM also
identified no counterpart candidates. The GBM targeted search,
the most sensitive, coherent search for GRB-like signals,
was run from +/-30 s around the neutrino candidate time.
From this search, no significant signal was found related
to IceCube-200926A.

We set upper limits on impulsive gamma-ray emission. Using the
representative soft, normal, and hard GRB-like templates described in
arXiv:1612.02395, we set the following 3 sigma flux upper limits over
10-1000 keV (in units of 10^-7 erg/s/cm^2):

Timescale   Soft     Normal   Hard
-------------------------------------------
0.128 s:    7.1      9.7      17.
1.024 s:    2.3      3.4      5.9
8.192 s:    1.0      1.5      2.6

These results are preliminary.
Looking for U.S. government information and services? Visit USA.gov