GCN Circular 2297

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. Wigger, 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, INTEGRAL (SPI-ACS), RHESSI, and HETE have observed
two events whose arrival directions are consistent with that
of SGR1806-20:

DATE	UT	ANNULUS	 ANNULUS    ANNULUS    deltaR	DISTANCE  DURATION  PEAK FLUX  FLUENCE  SPACECRAFT  
        S.	RA(2000) DEC(2000)  RADIUS    (3 SIGMA)  DEG.	   S.       erg/cm2s   erg/cm2
030712 76693.0  335.440 -27.794     57.625     0.017    0.003     0.180     5E-6       4E-6	ULYSSES, RHESSI, INTEGRAL
030713 77470.8  335.566 -27.667	    57.749     0.017    0.0001    0.032     1E-6       1E-7     ULYSSES, HETE(2763)

The annulus half-width is deltaR; distance is the angular distance between the centerline
of the annulus and the position of SGR1806-20; duration is the duration as observed
by Ulysses; peak fluxes and fluences are as observed by Ulysses, and are over 0.03125 s, 
and 25-100 keV.