GCN Circular 2234

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

D. M. Smith, R. P. Lin, J. McTiernan, R. Schwartz, C. Wiggger, W.
Hajdas, and A. Zehnder, on behalf of the RHESSI GRB team,

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, RHESSI, and INTEGRAL (SPI-ACS), and HETE-FREGATE observed this
GRB at 34342 seconds.  As observed by Ulysses, it had a duration of
approximately 10 seconds, a 25-100 keV fluence of approximately
7.2E-06 erg/cm2, and a peak flux of approximately  5.0E-07 erg/cm2 s
over 0.25 seconds.

We have triangulated it to a preliminary annulus centered  at RA,
Decl(2000)= 151.655,  35.124 degrees, whose radius is 80.349 +/-  0.080
degrees (3 sigma).

This annulus can be constrained and/or improved, but as the event was
not observed by Mars Odyssey, a small error box cannot be derived for
it.