[vsnet-grb-info 17648] GRB 160223B: CALET Gamma-Ray Burst Monitor detection

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Fri Feb 26 12:06:28 JST 2016


TITLE:   GCN CIRCULAR
NUMBER:  19085
SUBJECT: GRB 160223B: CALET Gamma-Ray Burst Monitor detection
DATE:    16/02/26 03:05:55 GMT
FROM:    Takanori Sakamoto at AGU  <tsakamoto at phys.aoyama.ac.jp>

S. Ozawa (Wasoeda U), A. Yoshida, T. Sakamoto, I. Takahashi, Y. Kawakubo, 
K. Senuma, M. Moriyama, Y. Yamada (AGU), K. Yamaoka (Nagoya U), S. Nakahira (JAXA), 
Y. Asaoka, 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 GRB160223B (Gotz et al., GCN Circ. 19059; von Kienlin et al., GCN Circ. 19061) 
triggered the CALET Gamma-Ray Burst Monitor (CGBM) at 09:58:59.5 on 23 February 2016.  
The burst signal was detected by SGM instrument.  

The light curve of the SGM shows at least three peaks.  The emission starts at T0, 
peaks at T0+1 sec and ends at T0+25 sec.   The T90 duration measured by the SGM data 
is 11 +- 1 sec (40-1000 keV). 

The CGBM data used in this analysis are provided by the Waseda CALET Operation Center 
located at the Waseda University.



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