TITLE: GCN CIRCULAR NUMBER: 11723 SUBJECT: Konus-Wind observation of GRB 110213A DATE: 11/02/14 11:36:03 GMT FROM: Dmitry Frederiks at Ioffe Institute S. Golenetskii, R.Aptekar, D. Frederiks, E. Mazets, V. Pal'shin, P. Oleynik, M. Ulanov, D. Svinkin, and T. Cline on behalf of the Konus-Wind team, report: The long GRB 110213A, (Swift/BAT trigger=445414: D'Elia, et al., GCN 11705; Barthelmy et.al, GCN 11714) triggered Konus-Wind at T0=19048.893s UT (05:17:28.893) The burst light curve consists of a single pulse with a total duration of ~50 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/GRB110213_T19048/ As observed by Konus-Wind the burst had a fluence of (1.0 ± 0.15)x10-5 erg/cm2, and a 256-ms peak flux, measured from T0+1.024s, of (1.4 ± 0.2)x10-6 erg/cm2/s (both in the 20 keV - 2 MeV energy range). The time-integrated spectrum of the burst (from T0 to T0+24.832 s) is best fitted in the 20 keV - 2 MeV range by a power law with exponential cutoff model, for which alpha = -1.65 (-0.2, +0.3), and Ep = 91(-26, +31) keV, chi2 = 62.5/61 dof. The spectrum at the maximum count rate (measured from T0 to T0+8.448 s) is well fitted in the 20 keV - 2 MeV range by a power law with exponential cutoff model, for which alpha = -1.53 (-0.21, +0.24), and Ep = 110(-20, +32) keV, chi2 = 52.8/61 dof. This spectrum is nearly well fitted in the 20 keV - 2 MeV range by the GRB (Band) model, for which: the low-energy photon index alpha = -1.28 (-0.32, +0.44), the high energy photon index beta = -2.4 (-0.7, +0.2), the peak energy Ep = 89(-19, +28) keV, chi2 = 49.1/60 dof. Assuming the Bok telescope redshift z = 1.46 (Milne & Cenko, GCN 11708) and a standard cosmology model with H_0 = 71 km/s/Mpc, Omega_M = 0.27, Omega_Lambda = 0.73, the isotropic energy release E_iso is (5.5 ± 0.08)x10^52 erg, the peak luminosity L_iso_max is (1.9 ± 0.3)x10^52 erg/s, and Ep_rest is 224 ± 74 keV. All the quoted results are preliminary. All the quoted errors are at the 90% confidence level.