GCN Circular 10554
Subject
IPN triangulation of GRB100324B
Date
2010-03-31T00:01:13Z (15 years ago)
From
Kevin Hurley at UCBerkeley/SSL <khurley@ssl.berkeley.edu>
K. Hurley, on behalf of the IPN team,
I. G. Mitrofanov, D. Golovin, M. L. Litvak, and A. B. Sanin,
on behalf of the HEND-Odyssey GRB team,
W. Boynton, C. Fellows, K. Harshman, H. Enos, and R. Starr, on
behalf of the GRS-Odyssey GRB team,
S. Golenetskii, R. Aptekar, E. Mazets, V. Pal'shin, D. Frederiks, and
T. Cline, on behalf of the Konus-Wind team,
K. Yamaoka, M. Ohno, Y. Hanabata, Y. Fukazawa, T. Takahashi, M. Tashiro,
Y. Terada, T. Murakami, and K. Makishima, on behalf of the Suzaku WAM team,
V. Connaughton, M. Briggs, and C. Meegan, on behalf of the Fermi GBM team,
and
J. Goldsten, on behalf of the MESSENGER NS GRB team, report:
This bright, long GRB was detected by Fermi (GBM), Suzaku (WAM),
Konus-Wind, Mars Odyssey (HEND), and MESSENGER (GRNS) AT 04:07:36 UT on
March 24, 2010. We have triangulated it to a preliminary, 38 square
arcminute (3 sigma) error box whose coordinates are:
RA(2000) Dec(2000)
Center 39.672 -19.287
Corners 39.713 -19.311
39.717 -19.449
39.628 -19.123
39.632 -19.262
This error box may be improved. Details of this burst will be presented
in forthcoming GCN Circulars.