{
  "bibcode": "2014GCN.16897....1G",
  "body": "S. Golenetskii, R.Aptekar, D. Frederiks, V. Pal'shin, P. Oleynik,\nM. Ulanov, D. Svinkin, A. Tsvetkova, A. Lysenko, and T. Cline\non behalf of the Konus-Wind team, report:\n\nThe long-duration GRB 141005A (Swift-BAT trigger 614415:\nD'Elia, GCN 16882; Krimm et al., GCN 16893;\nFermi-GBM detection: Roberts, GCN 16889)\ntriggered Konus-Wind at T0=18787.727 s UT (05:13:07.727).\n\nThe burst light curve shows a single pulse with a duration of ~3 s.\nThe emission is seen up to ~1 MeV.\n\nAs observed by Konus-Wind, the burst\nhad a fluence of 2.3(-0.2,+0.3)x10^-6 erg/cm2,\nand a 64-ms peak energy flux, measured from T0+0.390 s,\nof 1.6(-0.5,+0.5)x10^-6 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+8.448 s)\nis best fit in the 20 keV - 1 MeV range\nby a power law with exponential cutoff model:\ndN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep)\nwith  alpha = -0.34(-0.49,+0.58),\nand Ep = 104(-14,+18) keV (chi2 = 33/55 dof).\nFitting by a GRB (Band) model yields the same alpha and Ep,\nand an upper limit on the high energy photon index:\nbeta < -2.37 (chi2 = 31/54 dof).\n\nThe Konus-Wind light curve of this GRB is available at\nhttp://www.ioffe.ru/LEA/GRBs/GRB141005_T18787/\n\nAll the quoted errors are at the 90% confidence level.\nAll the quoted values are preliminary.",
  "circularId": 16897,
  "createdOn": 1412620202000,
  "email": "tsvetkova@mail.ioffe.ru",
  "subject": "Konus-Wind observation of GRB 141005A",
  "submitter": "Anastasia Tsvetkova at Ioffe Institute  <tsvetkova@mail.ioffe.ru>",
  "eventId": "GRB 141005A"
}