| Circular_text |
TITLE: GCN CIRCULAR
NUMBER: 23675
SUBJECT: Konus-Wind observation of GRB 190110A
DATE: 19/01/12 21:29:13 GMT
FROM: Anna Kozlova at Ioffe Institute
A. Kozlova, 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:
The long-duration GRB 190110A
(Swift-BAT detection and analysis: Sbarufatti et al., GCN Circ. 23670;
Ukwatta et al., GCN Circ. 23674;
Fermi-GBM detection: Poolakkil & Meegan, GCN Circ. 23671)
triggered Konus-Wind at T0=62689.767 s UT (17:24:49.767).
The burst light curve shows a single pulse
started at ~T0-3.5 s with a total duration of ~5 s.
The emission is seen up to ~8 MeV.
As observed by Konus-Wind, the burst
had a fluence of 3.39(-0.51,+0.88)x10^-6 erg/cm2,
and a 64-ms peak flux, measured from T0+0.158 s,
of 2.21(-0.93,+1.71)x10^-6 erg/cm2/s
(both in the 20 keV - 10 MeV energy range).
The time-averaged spectrum of the burst
(measured from T0 to T0+8.448 s)
is best fit in the 20 keV - 8 MeV range
by a power law with exponential cutoff model:
dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep)
with alpha = -1.44(-0.46,+0.58)
and Ep = 132(-60,+111) keV (chi2 = 62/81 dof).
Fitting by a GRB (Band) model yields the same alpha and Ep,
and an upper limit on the high energy photon index: beta < -2.4
(chi2 = 62/80 dof).
The spectrum near the maximum count rate
(measured from T0+0.128 to T0+0.256 s)
is best fit in the 20 keV - 8 MeV range
by a power law with exponential cutoff model
with alpha = -0.87(-0.82,+1.27)
and Ep = 165(-53,+382) keV (chi2 = 12/18 dof).
Fitting by a GRB (Band) model yields the same alpha and Ep,
and an upper limit on the high energy photon index: beta < -2.0
(chi2 = 12/17 dof).
The Konus-Wind light curve of this GRB is available at
http://www.ioffe.ru/LEA/GRBs/GRB190110_T62689/
All the quoted errors are at the 90% confidence level.
All the quoted values are preliminary.
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