{
  "bibcode": "2014GCN.16945....1S",
  "body": "M. Stanbro (UAH) reports on behalf of the Fermi GBM Team:\n\n\"At 02:04:40.21 UT on 22 October 2014, the Fermi Gamma-Ray Burst Monitor\ntriggered and located GRB 141022B (trigger 435636283 / 141022087).\n\nThe trigger resulted in an Autonomous Repoint Request (ARR)\nthat was accepted and the spacecraft slewed to the GBM in-flight location.\n\nThe on-ground calculated location, using the GBM trigger\ndata, is RA = 119.4, DEC = -75.2 (J2000 degrees,\nequivalent to 7h 58m, -75d 12'), with an uncertainty\nof 1.0 degrees (radius, 1-sigma containment,\nstatistical only; there is additionally a systematic\nerror which is currently estimated to be 2 to 3 degrees).\n\nThe angle from the Fermi LAT boresight is 110 degrees.\n\nThe GBM light curve consists of a single episode consisting of\nseveral pulses with a duration (T90) of about 9.2 s (50-300 keV).\nThe time-averaged spectrum from T0+1.9 s to T0+12.2 s is well\nfit by a Band function with Epeak = 368.1 (+/-11.2) keV,\nalpha = -0.64 +/- 0.02 , and beta = -2.41 (+/-0.05).\n\nThe event fluence (10-1000 keV) in this time interval is\n(7.87 +/- 0.07)E-05 erg/cm^2. The 1-sec peak photon flux measured\nstarting from T0+3.328 s in the 10-1000 keV band\nis 62.9 +/- 1.2 ph/s/cm^2.\n\nThe spectral analysis results presented above are preliminary;\nfinal results will be published in the GBM GRB Catalog.\"",
  "circularId": 16945,
  "createdOn": 1414090868000,
  "email": "mcs0001@uah.edu",
  "subject": "GRB141022B: Fermi GBM Detection",
  "submitter": "Matthew Stanbro at UAH/Fermi  <mcs0001@uah.edu>",
  "eventId": "GRB 141022B"
}