GCN Circular 25523

P. Veres (UAH) reports on behalf of the Fermi-GBM Team and the
GBM-LIGO/Virgo group:

For S190828l and using the initial bayestar skymap, Fermi-GBM was observing
29% of the localization probability at event time.

There was no Fermi-GBM onboard trigger around the event time of the
LIGO/Virgo detection of GW trigger S190828l (GCN 25503
Not found
 
 
). 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 merger time, and also identified no counterpart
candidates.

We therefore set upper limits on impulsive gamma-ray emission. Using the
representative soft, normal, and hard GRB-like templates described in
arXiv:1612.02395
Not found
 
 
, we set the following 3 sigma flux upper limits over
10-1000 keV (in units of erg/s/cm^2):

Timescale  Soft     Normal   Hard
------------------------------------
0.128 s:   1.8e-07  2.3e-07  5.0e-07
1.024 s:   6.4e-08  1.0e-07  2.1e-07
8.192 s:   2.7e-08  3.5e-08  7.7e-08

Assuming the median luminosity distance of 1609 Mpc (z=0.31) from the GW
detection, we estimate the following intrinsic luminosity upper limits over
the 1 keV-10 MeV energy range (in units of 10^49 erg/s):

Timescale  Soft     Normal   Hard
------------------------------------
0.128 s:     8.9          10         37
1.024 s:     3.2          4.4        16
8.192 s:     1.3          1.5        5.7