GCN Circular 17918

S. Golenetskii, R.Aptekar, D. Frederiks, V. Pal'shin, P. Oleynik,
M. Ulanov, D. Svinkin, A. Tsvetkova, A.Lysenko, and T. Cline
on behalf of the Konus-Wind team, report:

A long-duration GRB triggered Konus-Wind on June 8, 2015
at T0=42325.791 s UT (11:45:25.791), ~80 s before
the MAXI trigger (GRB 150608A; Arimoto, et al., GCN Circ. 17912
Not found
 
 
).

The KW light curve shows a multi-peaked complex which
started at ~T0-75 s and lasted until ~T0+5 s.
This phase of the emission was followed, in ~75 s,
by a weaker pulse, which triggered MAXI.
Taking into account the proximity of this burst
to the MAXI/GSC trigger and consistency of the
KW ecliptic latitude response with the position
of GRB 150608A we suggest that KW observed
the main part of GRB 150608A.

The K-W light curve of this burst is available at
http://www.ioffe.rssi.ru/LEA/GRBs/GRB150608_T42325/

As observed by Konus-Wind, the burst had a fluence of 
2.4(-0.3,+0.3)x10^-5 erg/cm2, and a 2.944-s peak flux,
measured from T0-0.302 s, of 8.8(-1.2,+1.2)x10^-7 erg/cm2/s
(both in the 20 keV - 10 MeV energy range).

Since the bulk of the burst emission lies before the triggered
mode record, the spectral analysis was performed using
KW 3-channel waiting mode data.

Modeling the 3-channel time-integrated spectrum
(from T0-73.209 s to T0+5.586 s) by a power law
with exponential cutoff (CPL) model:
dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep)
yields alpha = -1.56 �� 0.14, and Ep = 209 �� 46 keV.

Modelling the 3-channel spectrum near the peak count rate
(from T0-3.246 s to T0+2.642 s) by the CPL model
yields alpha = -0.94 �� 0.26, and Ep = 199 �� 37 keV.

All the quoted errors are estimated at the 1 sigma confidence level.
All the presented results are preliminary.