K. Hurley and T. Cline, on behalf of the Ulysses GRB team,
A. von Kienlin, G. Lichti, and A. Rau, on behalf of the
INTEGRAL SPI-ACS GRB team, and
D. M. Smith, R. P. Lin, J. McTiernan, R. Schwartz, C. Wigger, W. Hajdas,
and A. Zehnder, on behalf of the RHESSI GRB team, report:
Ulysses and RHESSI also observed this burst (GCN 1786). As observed by
Ulysses, it had a duration of approximately 5 seconds, a 25-100 keV
fluence of approximately 5.1E-06 erg/cm2, and a peak flux of
approximately 6.9E-07 erg/cm2 s over 0.50 seconds.
We have triangulated it to a preliminary annulus centered at RA,
Decl(2000) = 2.023, -37.567 degrees, whose radius is 14.958 +/-
0.144 degrees (3 sigma ).
This annulus may be constrained and/or improved. but as the event was
not observed by Mars Odyssey, a small error box cannot be derived for