{
  "eventId": "GRB 240119A",
  "submitter": "Dmitry Frederiks at Ioffe Institute <fred@mail.ioffe.ru>",
  "createdOn": 1705938027089,
  "submittedHow": "email-legacy",
  "bibcode": "2024GCN.35594....1F",
  "circularId": 35594,
  "body": "D. Frederiks, A.Lysenko, A. Ridnaia, D. Svinkin,\nA. Tsvetkova,  M. Ulanov, and T. Cline,\non behalf of the Konus-Wind team, report:\n\nThe short GRB 240119A (Fermi-GBM detection: The Fermi GBM team, GCN 35583;\nAstroSat-CZTI detection: Joshi et al.: GCN 35589;\nGECAM-B detection: Zhang et al.: GCN 355921;\nIPN triangulation: Svinkin et al., GCN 35592)\ntriggered Konus-Wind (KW) at T0=62945.465 s UT (17:29:05.465).\n\nThe burst light curve shows a single emission pulse\nwhich starts at ~T0-0.032 s and has a duration of ~0.13 s.\nThe emission is seen up to ~2 MeV.\n\nThe Konus-Wind light curve of this GRB is available at\nhttp://www.ioffe.ru/LEA/GRBs/GRB240119_T62945/\n\nAs observed by Konus-Wind, the burst had\na total fluence of (8.1 ± 1.7)x10^-7 erg/cm^2 and\na 16-ms peak energy flux, measured from T0-0.016 s,\nof (1.9 ± 0.4)x10^-5 erg/cm^2/s (both in the 20 keV - 10 MeV energy range).\n\nThe spectrum of the burst (measured from T0-0.048 s to T0+0.080 s)\ncan be described, in the 20 keV - 1.5 MeV range, by a power law with\nexponential cutoff (CPL) model: dN/dE ~ (E^alpha)*exp(-E*(2+alpha)/Ep)\nwith  alpha = -0.23(-0.32,+0.40) and Ep = 678(-141,+254) keV.\n\n\nAll the quoted errors are estimated at the 68% confidence level.\nAll the presented results are preliminary.\n\n",
  "subject": "Konus-Wind detection of GRB 240119A (short/hard)"
}