{
  "bibcode": "2010GCN.11408....1G",
  "body": "S. Golenetskii, R.Aptekar, E. Mazets, V. Pal'shin, D. Frederiks, P.\nOleynik, M. Ulanov, D. Svinkin, and T. Cline on behalf of the Konus-Wind\nteam report:\n\nThe long GRB 101114A discovered in BAT ground analysis (Sakamoto et al., \nGCN 11405) was detected by Konus-Wind in the waiting mode.\n\nThe burst light curve shows a rather bright pulse at ~T0(BAT) preceded \nby two weak pulses at ~T0(BAT)-100 s and ~T0(BAT)-50 s. The total burst \nduration is ~110 s.\n\nAs observed by Konus-Wind, the burst had a fluence of (4.7 +/- \n2.4)x10^-6 erg/cm2 (in the 20 - 1200 keV energy range).\n\nModeling the K-W 3-channel spectrum of the main pulse (accumulated from \nT0-2.2 s to T0+6.6 s) by a power law with exponential cutoff model:\ndN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep)\nyields alpha = -1.15 +/- 0.29, Ep = 296 +/- 129 keV.\n\nAll the quoted errors are estimated at the 1 sigma confidence level.\n\nThe K-W light curve of this burst is available at\nhttp://www.ioffe.rssi.ru/LEA/GRBs/GRB101114A/",
  "circularId": 11408,
  "createdOn": 1289904556000,
  "email": "val@mail.ioffe.ru",
  "subject": "Konus-Wind observation of GRB 101114A",
  "submitter": "Valentin Pal'shin at Ioffe Inst  <val@mail.ioffe.ru>",
  "eventId": "GRB 101114A"
}