[vsnet-grb-info 18585] GRB 161010A: CALET Gamma-Ray Burst Monitor detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Thu Oct 13 09:12:56 JST 2016
TITLE: GCN CIRCULAR
NUMBER: 20033
SUBJECT: GRB 161010A: CALET Gamma-Ray Burst Monitor detection
DATE: 16/10/13 00:11:55 GMT
FROM: Takanori Sakamoto at AGU <tsakamoto at phys.aoyama.ac.jp>
K. Yamaoka (Nagoya U), A. Yoshida, T. Sakamoto, Y. Kawakubo, M. Moriyama,
Y. Yamada (AGU), S. Nakahira (JAXA), I. Takahashi (IPMU), Y. Asaoka, S. Ozawa,
S. Torii (Waseda U), Y. Shimizu, 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 long-duration GRB 161010A (Mereghetti et al., GCN Circ. 20021; Svinkin et al.,
GCN Circ. 20027; McCauley et al., GCN Circ. 20025) triggered the CALET Gamma-ray
Burst Monitor (CGBM) at 13:36:31.69 on 10 October 2016.
The burst signal was seen by the SGM instrument.
The light curve of the SGM shows a single weak peak starting at T0, peaking at
T+3 sec and ending at T+8 sec. The T90 duration measured by the SGM data
is 4.9 +- 0.5 sec (40-1000 keV).
The light curve is available at
http://cgbm.calet.jp/cgbm_trigger/flight/1160141725/
The CALET data used in this analysis are provided by the Waseda
CALET Operation Center located at the Waseda University.
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