{
  "bibcode": "2002GCN..1663....1H",
  "body": "K. Hurley and T. Cline, on behalf of the Ulysses, Konus, and HETE GRB\nteams,\n\nE. Mazets and S. Golenetskii, on behalf of the Konus-Wind GRB team,\n\nD. M. Smith, R. P. Lin, J. McTiernan, R. Schwartz, C. Wigger, W.\nHajdas, and A. Zehnder, on behalf of the RHESSI GRB team, and\n\nG. Ricker, J-L Atteia, N. Kawai, D. Lamb, S. Woosley, J. Doty, R.\nVanderspek, J. Villasenor, G. Crew, G. Monnelly, N. Butler, J.G.\nJernigan, A. Levine, F. Martel, E. Morgan, G. Prigozhin, J. Braga, R.\nManchanda, G. Pizzichini, Y. Shirasaki, C. Graziani, M. Matsuoka, T.\nTamagawa, K. Torii, T. Sakamoto, A. Yoshida, E. Fenimore, M. Galassi,\nT. Tavenner, T. Donaghy, M. Boer, J-F Olive, and J-P Dezalay, on behalf\nof the HETE GRB team, report:\n\nKonus and RHESSI also observed this event (GCN 1656).  The Konus\necliptic latitude response limits the IPN annulus (RA, Decl=178.652,\n+35.689 degrees, radius 73.524 +/- 0.111 degrees, 3 sigma) to the\nportion in the south ecliptic hemisphere, that is, the portion between\nRA, Decl = 92.5, +23.4 and 231.0, -18.5 degrees.  The 3-spacecraft\ntriangulation indicates that the most likely position along this\nportion of the annulus is very roughly located at RA, Decl= 115.6, -7.8\ndegrees.\n\nThis error box may be improved slightly, but as the event was\nnot observed by MO, a small error box cannot be derived for it.",
  "circularId": 1663,
  "createdOn": 1035912888000,
  "email": "khurley@sunspot.ssl.berkeley.edu",
  "subject": "IPN triangulation of GRB021025 (portion of annulus)",
  "submitter": "Kevin Hurley at UCBerkeley/SSL  <khurley@sunspot.ssl.berkeley.edu>",
  "eventId": "GRB 021025"
}