{
  "bibcode": "2002GCN..1643....1H",
  "body": "K. Hurley, on behalf of the Ulysses GRB team,\n\nE. Mazets, S. Golenetskii, and D. Frederiks, on behalf of the\nKonus-Wind GRB team, and\n\nT. Cline, on behalf of the Ulysses and Konus GRB teams, report:\n\nUlysses and Konus observed this burst at 84276 s.  As observed by\nUlysses, it had a duration of ~150 ms, a 25-100 keV fluence of ~7E-7\nerg/cm2, and a peak flux over 32 ms of 3E-6 erg/cm2 s.  The burst\ntriggered Ulysses, but was observed in waiting mode (~ 3 s resolution)\nby Konus, which had triggered on a solar flare.  We have triangulated\nit to an annulus centered at RA, Decl= 356.131, -36.621 degrees, whose\nradius is 79.502 +/- 0.056 degrees.  As the center line of this annulus\npasses within 0.049 degrees of SGR1900+14, we conclude that this event\noriginated from that source.\n\nOnly small improvements to this localization are expected.\n\nA subsequent short burst was detected by Ulysses on October 11\nat 35680 s (Ulysses time).  This burst has not yet been confirmed\nby any other spacecraft, but if it originated from SGR1900+14,\nits Earth-crossing time would have been around 35420 s.\n\nAs of October 16, no other short events have been detected\nby Ulysses.",
  "circularId": 1643,
  "createdOn": 1034887561000,
  "email": "khurley@sunspot.ssl.berkeley.edu",
  "subject": "SGR1900+14: burst on October 10 2002",
  "submitter": "Kevin Hurley at UCBerkeley/SSL  <khurley@sunspot.ssl.berkeley.edu>"
}