GCN Circular 1814

K. Hurley and T. Cline, on behalf of the Ulysses and HETE GRB teams,

A. von Kienlin, G. Lichti, and A. Rau, on behalf of the
INTEGRAL SPI-ACS GRB team, and

G. Ricker, J-L Atteia, N. Kawai, D. Lamb, S. Woosley, J. Doty, R.
Vanderspek, J. Villasenor, G. Crew, G. Monnelly, N. Butler, J.G.
Jernigan, A. Levine, F. Martel, E. Morgan, G. Prigozhin, J. Braga, R.
Manchanda, G.  Pizzichini, Y. Shirasaki, C. Graziani, M. Matsuoka, T.
Tamagawa, K. Torii, T. Sakamoto, A. Yoshida, E. Fenimore, M. Galassi,
T. Tavenner, T.  Donaghy, M. Boer, J-F Olive, and J-P Dezalay, on
behalf of the HETE GRB team, report:

Ulysses, INTEGRAL (SPI-ACS) and HETE (Fregate) observed this burst at
23070 s.  As observed by Ulysses, it had a duration of approximately
100 seconds, a 25-100 keV fluence of approximately  1.2E-05 erg/cm2,
and a peak flux of approximately  1.0E-06 erg/cm2 s over 0.25 seconds.

We have triangulated it to a preliminary annulus centered at
RA, Dec (2000)= 0.310, -38.800 degrees, whose radius is 43.532 +/- 
0.031 degrees.  

This annulus may be improved and/or constrained.