[vsnet-grb-info 18023] GRB 160525C: CALET Gamma-Ray Burst Monitor detection

GCN Circulars gcncirc at capella2.gsfc.nasa.gov
Sun May 29 08:40:30 JST 2016


TITLE:   GCN CIRCULAR
NUMBER:  19471
SUBJECT: GRB 160525C: CALET Gamma-Ray Burst Monitor detection
DATE:    16/05/28 23:39:39 GMT
FROM:    Takanori Sakamoto at AGU  <tsakamoto at phys.aoyama.ac.jp>

T. Sakamoto, A. Yoshida, 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), 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:

GRB 160525C (Konus-Wind trigger time on 10:54:28.0 UT) triggered the CALET Gamma-Ray 
Burst Monitor (CGBM) at 10:54:20.25 on 25 May 2016.  The burst signal was seen by all 
CGBM instruments.

The light curve of the SGM shows a double peak structure starting at T0+4 sec, peaking 
at T0+5 sec, and ending at T0+6.5 sec sec.  The T90 duration measured by the SGM data 
is 2.4 +- 0.3 sec (40-230 keV).  The light curve is available at

http://cgbm.calet.jp/cgbm_trigger/flight/1148208864/index.html

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



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