[vsnet-grb-info 10050] GRB 101225A: MAXI/GSC observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Wed Dec 29 14:38:30 JST 2010
TITLE: GCN CIRCULAR
NUMBER: 11505
SUBJECT: GRB 101225A: MAXI/GSC observations
DATE: 10/12/29 05:38:26 GMT
FROM: Nobuyuki Kawai at Tokyo Tech <nkawai at hp.phys.titech.ac.jp>
M. Serino, T. Mihara, Y.E. Nakagawa, M. Sugizaki,
T. Yamamoto, T. Sootome, M. Matsuoka (RIKEN),
N. Kawai, M. Morii, K. Sugimori, R. Usui (Tokyo Tech),
K. Kawasaki, S. Ueno, H. Tomida, M. Kohama, M. Ishikawa (JAXA),
A. Yoshida, K. Yamaoka, S. Nakahira (AGU),
H. Tsunemi, M. Kimura (Osaka U.), H. Negoro, M. Nakajima
H. Ozawa, F. Suwa (Nihon U.), Y. Ueda, N. Isobe,
S. Eguchi, K. Hiroi (Kyoto U.), A. Daikyuji (Miyazaki U.),
K. Yamazaki, A. Uzawa, T. Matsumura (Chuo U.),
report on behalf of the MAXI team:
MAXI/GSC observed the field of the Swift trigger 441015 = GRB 101225A
(Racusin et al, GCN 11493) before and after the trigger time.
The transit times (UT) and the observed fluxes in 2-10 keV energy band are
15:51 (T-9988s) -19 +- 11 mCrab
17:23 (T-4483s) 20 +- 13 mCrab
18:54 (T+1002s) 20 +- 15 mCrab
20:05 (T+5218s) 11 +- 9 mCrab
23:08 (T+16209s) 2 +- 7 mCrab
All the quoted uncertainties are 1-sigma statistical errors.
Note that the third transit occurred within the 1088-second Swift image trigger interval. While it is not statistically significant, there appears be a weak X-ray enhancement at the location of the Swift trigger position during or near the BAT detection times (Cummings and Sakamoto, GCN 11504).
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