{
  "bibcode": "2000GCN...895....1H",
  "body": "K. Hurley, on behalf of the Ulysses GRB team, T. Cline, on behalf of\nthe Konus-Wind and NEAR GRB teams, F. Frontera, C. Guidorzi, and E.\nMontanari, on behalf of the BeppoSAX GRBM team, and E. Mazets and S.\nGolenetskii, on behalf of the KONUS-WIND GRB team, report:\n\nUlysses and NEAR have only recently emerged from an intense solar\nproton event lasting approximately two weeks.  Ulysses, NEAR, BeppoSAX\nGRBM, and KONUS-WIND observed this GRB at 28869 seconds.  Its spectrum\nand duration place it firmly in the \"short/hard\" class of gamma-ray\nbursts.  As observed by Ulysses, it had a duration of \n<0.5 seconds, a 25-100 keV fluence of approximately  3.7E-7 erg/cm2,\nand a peak flux of approximately  6.8E-7 erg/cm2 s over 0.5 seconds.\n\nWe have triangulated it to a preliminary, 3 sigma error box with approximate area  18 square arcminutes, whose coordinates are:\n\n ERROR BOX CENTER:   2 h 41 m  8.59 s     12 o 53 '  46.31 \" \n ERROR BOX CORNER 1:  2 h 41 m 10.35 s     12 o 51 '  56.95 \" \n ERROR BOX CORNER 2:  2 h 40 m 50.39 s     12 o 51 '  35.60 \" \n ERROR BOX CORNER 3:  2 h 41 m 26.79 s     12 o 55 '  57.13 \" \n ERROR BOX CORNER 4:  2 h 41 m  6.83 s     12 o 55 '  35.67 \" \n\nBecause solar protons were still being recorded by Ulysses,\nthis burst was detected at slightly under 5 sigma significance\n(statistical only), making it somewhat marginal.  However,\nfinal consistency checks are now being carried out, and the\nresults will be communicated as soon as they are available.",
  "circularId": 895,
  "createdOn": 976151989000,
  "email": "khurley@sunspot.ssl.berkeley.edu",
  "subject": "IPN triangulation of GRB001204 (short/hard)",
  "submitter": "Kevin Hurley at UCBerkeley/SSL  <khurley@sunspot.ssl.berkeley.edu>",
  "eventId": "GRB 001204"
}