GCN Circular 20556
Subject
GRB 170124A: CALET Gamma-Ray Burst Monitor detection
Date
2017-01-28T04:30:56Z (8 years ago)
From
Takanori Sakamoto at AGU <tsakamoto@phys.aoyama.ac.jp>
W. Ishizaki (ICRR), 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), Y. Shimizu, T. Tamura (Kanagawa U),
M. L. Cherry (LSU), S. Ricciarini (U of Florence), P. S. Marrocchesi (U of Siena)
and the CALET collaboration:
The long-duration GRB 170124A (Fermi-GBM trigger #506984291; Konus-Wind trigger
time on 20:58:06.428 UT) triggered the CALET Gamma-ray Burst Monitor (CGBM) at
20:58:04.58 on 24 January 2017. The burst signal was seen by all CGBM instruments.
The light curve of the SGM shows two peaks. The first peak starts at T0,
peaks at T+8 sec and ends at T+15 sec. The second peak starts at T+15 sec,
peaks at T+23 sec and ends at T+30 sec. The T90 duration measured by
the SGM data is 20.9 +- 1.3 sec (40-1000 keV).
The light curve is available at
http://cgbm.calet.jp/cgbm_trigger/flight//1169326441/index.html
The CALET data used in this analysis are provided by the Waseda
CALET Operation Center located at the Waseda University.