[vsnet-grb-info 20022] GRB 171101A CALET Gamma-Ray Burst Monitor detection
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Thu Nov 9 09:32:02 JST 2017
TITLE: GCN CIRCULAR
NUMBER: 22110
SUBJECT: GRB 171101A CALET Gamma-Ray Burst Monitor detection
DATE: 17/11/09 00:31:16 GMT
FROM: Takanori Sakamoto at AGU <tsakamoto at phys.aoyama.ac.jp>
T. Sakamoto, A. Yoshida, Y. Kawakubo, M. Moriyama, Y. Yamada,
A. Tezuka, S. Matsukawa (AGU), K. Yamaoka (Nagoya U), S. Nakahira (RIKEN),
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), A. V. Penacchioni, P. S. Marrocchesi (U of Siena)
and the CALET collaboration:
The long-duration GRB 171101A (INTEGRAL SPI-ACS trigger #7954) triggered the
CALET Gamma-ray Burst Monitor (CGBM) at 10:49:47.91 on 1 November 2017.
The burst signal was seen by the all CGBM instruments.
The light curve of the SGM shows a single peak. The emission starts at T+3 sec,
peaks at T+4.5 sec and ends at T+15 sec. The T90 duration measured by the
SGM data is 6.0 +- 0.4 sec (40-1000 keV).
The light curve is available at
http://cgbm.calet.jp/cgbm_trigger/flight/1193568506/index.html
The CALET data used in this analysis are provided by the Waseda CALET Operation
Center located at the Waseda University.
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