{
  "bibcode": "2005GCN..3070....1G",
  "body": "S. Golenetskii, R.Aptekar, E. Mazets, V. Pal'shin, D. Frederiks\non behalf of Konus-Wind and Helicon/Coronas-F teams, and\nT. Cline on behalf of the Konus-Wind team report:\n\nSGR-like burst 050304 was detected by Konus-Wind\nat 10:17:14.537 UT and Helicon-Coronas-F at 10:17:17.941 UT.\nWe have triangulated it to an annulus centered at\nRA(2000) = 321.683 deg, Decl(2000) = -15.478 deg,\nwhose radius is 47.167 � 0.092 deg (3 sigma).\nAs the center line of this annulus passes 0.033 degrees (1.1 sigma)\nfrom the position of SGR 1806-20\nand the Konus ecliptic latitude response indicates\nthat the source of the burst is near ecliptic plane,\nwe conclude that this burst originated from SGR 1806-20.\n\nThe burst had a duration of 0.13 sec,\nfluence 7.9x10-7 erg cm-2, and peak flux\n8.7x10-6 erg cm-2 s-1, both in 20-200 keV range.\nThe time-integrated spectrum of the burst can be fitted by the OTTB\nspectral model:\ndN/dE ~ E^{-1} exp(-E/kT),\nwith kT = 22 � 1 keV.\n\n\nSince the giant flare on 2004 December 27,\nKonus-Wind and/or Helicon-Coronas-F has detected\n10 SGR-like bursts in the trigger mode,\nprobably originated from SGR 1806-20.",
  "circularId": 3070,
  "createdOn": 1110037636000,
  "email": "fred@mail.ioffe.ru",
  "subject": "Ongoing activity of SGR 1806-20 after the giant flare",
  "submitter": "Dmitry Frederiks at Ioffe Institute  <fred@mail.ioffe.ru>"
}