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GCN Circular 1787

IPN triangulation of GRB030102 (annulus)
2003-01-05T00:09:22Z (21 years ago)
Kevin Hurley at UCBerkeley/SSL <>
K. Hurley and T. Cline, on behalf of the Ulysses GRB team, 

A. von Kienlin, G. Lichti, and A. Rau, on behalf of the

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
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