[vsnet-grb-info 18303] GRB 160726A: CALET Gamma-Ray Burst Monitor detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Aug 2 06:11:42 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 19751
SUBJECT: GRB 160726A: CALET Gamma-Ray Burst Monitor detection
DATE: 16/08/01 21:03:22 GMT
FROM: Takanori Sakamoto at AGU <tsakamoto at phys.aoyama.ac.jp>
Y. Shimizu (Kanagawa U), A. Yoshida, T. Sakamoto, Y. Kawakubo, M. Moriyama,
Y. Yamada (AGU), K. Yamaoka (Nagoya U), S. Nakahira (JAXA), I. Takahashi (IPMU),
Y. Asaoka, S. Ozawa, S. Torii (Waseda U), T. Tamura (Kanagawa U), W. Ishizaki (ICRR),
M. L. Cherry (LSU), S. Ricciarini (U of Florence), P. S. Marrocchesi (U of Siena)
and the CALET collaboration:
The short-duration GRB 160726A (Starling, et al., GCN circ. 19731;
Hamburg, et al., GCN circ. 19732; Frederiks, et al. GCN circ. 19733)
triggered the CALET Gamma-ray Burst Monitor (CGBM) at 01:34:08.25
on 26 July 2016. The burst signal was seen by all CGBM instruments.
The light curve of the SGM shows two peaks. The first weak episode
peaks at T-0.55 s. The second peak starts at T-0.1 s, peaks at T+0.1 s
and ends at T+0.3 s. The T90 duration measured by the SGM data is
0.83 +- 0.09 sec (40-1000 keV).
The light curve is available at
http://cgbm.calet.jp/cgbm_trigger/flight/1153531947/
The CALET data used in this analysis are provided by the Waseda
CALET Operation Center located at the Waseda University.
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