TITLE: GCN CIRCULAR NUMBER: 15870 SUBJECT: Konus-Wind observation of exceptionally bright GRB 140219A DATE: 14/02/21 11:42:29 GMT FROM: Valentin Pal'shin at Ioffe Inst S. Golenetskii, R.Aptekar, D. Frederiks, V. Pal'shin, P. Oleynik, M. Ulanov, D. Svinkin, and T. Cline on behalf of the Konus-Wind team, report: The long-duration, exceptionally bright and hard GRB 140219A (localized by IPN: Hurley et al., GCN 15864; GBM detection: Zhang, GCN 15866; LAT detection: Guiriec et al., GCN 15867) triggered Konus-Wind at T0=71162.611 s UT (19:46:02.611). The burst light curve shows an extremely bright multi-peaked pulse with a duration of ~2.5 s followed by a less intense multi-peaked emission episodes until ~T0+26 s and a very weak tail until ~T0+35 s. The emission is seen up to ~18 MeV. As observed by Konus-Wind, the burst had a fluence of (1.14 ± 0.02)x10^-3 erg/cm2, and a 16-ms peak flux, measured from T0+0.240 s, of (1.44 ± 0.12)x10^-3 erg/cm2/s (both in the 20 keV - 10 MeV energy range). The time-integrated spectrum (measured from T0 to T0+38.912 s) is best fit (in the 26 keV - 18 MeV range) by a GRB (Band) model with the following model parameters: the low-energy photon index alpha = -1.07 ± 0.01, the high energy photon index beta = -3.26(-0.88,+0.38), the peak energy Ep = 2777 ± 70 keV, chi2 = 112.7/96 dof. The spectrum of the main pulse (measured from T0 to T0+2.304 s) is best fit (in the 26 keV - 18 MeV range) by a GRB (Band) model with the following model parameters: the low-energy photon index alpha = -0.65 ± 0.04, the high energy photon index beta = -3.28(-0.89,+0.39), the peak energy Ep = 3363 ± 141 keV, chi2 = 47.9/77 dof. The Konus-Wind light curve of this GRB is available at http://www.ioffe.ru/LEA/GRBs/GRB140219_T71162/ All the quoted errors are at the 90% confidence level. All the quoted results are preliminary. The derived peak flux and Epeak are the highest ever measured for GRBs with Konus-Wind during almost 20 years of its continuous observations: the peak flux is ~50% higher than the previous record holder, GRB 110918A, with the measured peak flux of ~0.9x10^-3 erg/cm2/s (Frederiks et al. ApJ, 779, 151 (2013)). Follow-up observations are strongly encouraged.