[vsnet-grb-info 24748] LIGO/Virgo S200112r: Upper limits from Konus-Wind observations

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Wed Jan 22 16:19:23 JST 2020


TITLE:   GCN CIRCULAR
NUMBER:  26847
SUBJECT: LIGO/Virgo S200112r: Upper limits from Konus-Wind observations
DATE:    20/01/22 07:18:10 GMT
FROM:    Anna Ridnaia at Ioffe Institute  <ridnaia at mail.ioffe.ru>

A. Ridnaia, S. Golenetskii, R.Aptekar, D. Frederiks,
M. Ulanov, D. Svinkin, A. Tsvetkova, A. Lysenko, 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 S200112r (2020-01-12 15:58:38.094 UTC, hereafter T0;
LIGO/Virgo Collaboration GCN Circ. 26715).

No triggered KW GRBs happened ~3 hours before and ~1.5 days
after 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 9.3x10^-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 2.8x10^-7 erg/cm^2/s (20 - 1500 keV, 2.944 s scale).

All the quoted values are preliminary.



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