{
  "bibcode": "2010GCN.11342....1G",
  "body": "S. Golenetskii, R.Aptekar, D. Frederiks, E. Mazets, V. Pal'shin,\nP. Oleynik, M. Ulanov, D. Svinkin, and T. Cline on behalf\nof the Konus-Wind team, report:\n\nThe very long bright GRB 101014A (Fermi/GBM\ntrigger 308722314 / 101014175: Tierney & Goldstein, GCN 11341)\ntriggered Konus-Wind at T0=15115.250s UT (04:11:55.250)\n\nThe burst light curve shows a complex multi-peaked\nstructure with a total duration of ~480 s.\nThe emission is seen up to ~10 MeV.\nThe Konus-Wind light curve of this GRB is available at\nhttp://www.ioffe.ru/LEA/GRBs/GRB101014_T15115/\n\nAs observed by Konus-Wind the burst\nhad a fluence of (2.5 � 0.7)x10-4 erg/cm2,\nand a 256-ms peak flux, measured from T0+208.896s,\nof (2.6 � 0.2)x10-5 erg/cm2/s\n(both in the 20 keV - 10 MeV energy range).\n\nThe time-integrated spectrum of the burst\n(measured from T0 to T0+445.184 s) is best fit\nin the 20 keV - 10 MeV range by the GRB (Band) model,\nfor which:\nthe low-energy photon index alpha = -1.26 (-0.13, +0.15),\nthe high energy photon index beta = -2.2 (-1.4, +0.2),\nthe peak energy Ep = 220(-47, +76)keV (chi2 = 64/84 dof).\n\nThe spectrum at the maximum count rate\n(measured from T0+208.128 to T0+210.176 s) is best fit\nin the 20 keV - 10 MeV range by the GRB (Band) model,\nfor which:\nthe low-energy photon index alpha = -1.12 (-0.05, +0.06),\nthe high energy photon index beta = -2.45 (-0.65, +0.30),\nthe peak energy Ep = 920(-170, +180)keV (chi2 = 79/69 dof).\n\nAll the quoted results are preliminary.\nAll the quoted errors are at the 90% confidence level.",
  "circularId": 11342,
  "createdOn": 1287143111000,
  "email": "fred@mail.ioffe.ru",
  "subject": "Konus-Wind observation of GRB 101014A",
  "submitter": "Dmitry Frederiks at Ioffe Institute  <fred@mail.ioffe.ru>",
  "eventId": "GRB 101014A"
}