TITLE:   GCN CIRCULAR
NUMBER:  24417
SUBJECT: LIGO/Virgo S190425z: Konus-Wind observations
DATE:    19/05/07 11:24:07 GMT
FROM:    Dmitry Svinkin at Ioffe Institute  <svinkin@mail.ioffe.ru>

D. Svinkin, S. Golenetskii, R.Aptekar, D. Frederiks,
M. Ulanov, A. Tsvetkova, A. Lysenko, A. Kozlova, and T. Cline,
on behalf of the Konus-Wind team, report:

Konus-Wind (KW) was observing the whole sky at the time of the
LIGO/Virgo event S190425z (2019-04-25 08:18:05.017 UTC, hereafter T0;
LIGO/Virgo Collaboration GCN Circ. 24168).

No triggered KW event happened from ~6 days before and ~2 days
after T0. The closest waiting-mode event was ~0.5 days before T0.
Using waiting-mode data within the interval T0 +/- 100 s,
we found no significant (> 5 sigma) excess over the background
in both KW detectors on temporal scales from 2.944 s to 100 s.

We estimate an upper limit (90% conf.) on the 20 – 1500 keV fluence
to 9.0x10^-7 erg/cm^2 for a burst lasting less than 2.944 s and having a
typical KW short GRB spectrum (an exponentially cut off power law with
alpha =-0.5 and Ep=500 keV). For a typical long GRB spectrum (the Band
function with alpha=-1, beta=-2.5, and Ep=300 keV), the corresponding
limiting peak flux is 2.7x10^-7 erg/cm^2/s (20 – 1500 keV, 2.944 s scale).

All the quoted values are preliminary.