TITLE: GCN CIRCULAR NUMBER: 18360 SUBJECT: Konus-Wind observation of GRB 150922A DATE: 15/09/23 13:09:30 GMT FROM: Dmitry Svinkin at Ioffe Institute S. Golenetskii, R. Aptekar, D. Frederiks, V. Pal'shin, P. Oleynik, M. Ulanov, D. Svinkin, A. Tsvetkova, A. Lysenko, A. Kozlova, and T. Cline on behalf of the Konus-Wind team, report: The short-duration, hard-spectrum GRB 150922A (IPN triangulation: Golenetskii et al., GCN 18357; Fermi GBM detection: Roberts et al., GCN 18358) triggered Konus-Wind at T0=20250.916 s UT (05:37:30.916). The burst light curve shows a multipeak structure with a total duration of ~0.16 s. The emission is seen up to ~2 MeV. The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB150922_T20250/ As observed by Konus-Wind, the burst had a fluence of 7.94(-1.93,+2.25)x10^-7 erg/cm2, and a 16-ms peak flux, measured from T0-0.008 s, of 1.34(-0.52,+0.59)x10^-5 erg/cm2/s (both in the 20 keV - 10 MeV energy range). The time-averaged spectrum of the burst (measured from T0 to T0+0.064 s) is best fit in the 20 keV - 2 MeV range by a power law with exponential cutoff model: dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep) with alpha = -0.17(-0.66,+1.10) and Ep = 393(-132,+222) keV (chi2 = 11/13 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 (chi2 = 11/12 dof) All the quoted errors are at the 90% confidence level. All the quoted values are preliminary.