{
  "bibcode": "2003GCN..2451....1H",
  "body": "K. Hurley and T. Cline, on behalf of the Ulysses, Konus, and Mars\nOdyssey GRB teams,\n\nE. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team,\n\nI. Mitrofanov, S. Charyshnikov, V. Grinkov, A. Kozyrev, M. Litvak, and\nA. Sanin, on behalf of the HEND-Odyssey GRB team, and\n\nW. Boynton, C. Fellows, K. Harshman, C. Shinohara and R. Starr, on\nbehalf of the GRS/Odyssey GRB team, report:\n\nKonus-Wind and Mars Odyssey-HEND  observed this GRB at 26660 seconds on\n14 November 2003.  As observed by Konus, it had a duration of\napproximately 1.4 seconds, an 18-200 keV fluence of approximately\n3.6E+-05 erg/cm2, and a peak flux of approximately 6.3E-05 erg/cm2 s.\n\nWe have triangulated it to a preliminary annulus centered at RA, Decl\n(2000) =  344.192, -8.447 degrees, whose radius is 70.299 +/-  0.036\ndegrees (3 sigma).   As the center line of this annulus passes 0.009\ndegrees from the position of SGR1806-20, and 0.092 degrees from the\ncenter of the error circle of SGR1808-20, we conclude that the origin\nof this burst was most likely SGR1806-20.",
  "circularId": 2451,
  "createdOn": 1069178541000,
  "email": "khurley@sunspot.ssl.berkeley.edu",
  "subject": "IPN detection of activity from SGR1806-20",
  "submitter": "Kevin Hurley at UCBerkeley/SSL  <khurley@sunspot.ssl.berkeley.edu>"
}