G. Ricker, D. Lamb, and S. Woosley on behalf of the HETE Science Team;
R. Vanderspek, G. Crew, J. Doty, G. Monnelly, J. Villasenor; N.
Butler, T. Cline, J.G. Jernigan, A. Levine, F. Martel, G. Pizzichini,
and G. Prigozhin, on behalf of the HETE Operations and HETE
N. Kawai, M. Matsuoka, Y. Shirasaki, T. Tamagawa, A. Yoshida, E.
Fenimore, M. Galassi, B. Preger, and C. Graziani, on behalf of the
HETE WXM Team;
J-L Atteia, M. Boer, J-F Olive, J-P Dezalay, and K. Hurley on behalf
of the HETE FREGATE Team;
The systematic error radius for the HETE localization of GRB010326 by
the WXM has been refined to 10 arcminutes. Further refinement is
Follow-up observations of this GRB event are encouraged.
Additional information on GRB010326, as well as for the HETE mission,
is available at:
Acronyms: HETE=High Energy Transient Explorer FREGATE=French Gamma
Ray Telescope WXM=Wide Field X-ray Monitor SXC=Soft X-ray Camera
This message may be cited.