TITLE: GCN CIRCULAR NUMBER: 35582 SUBJECT: GRB 240117A: CALET Gamma-Ray Burst Monitor detection DATE: 24/01/19 18:53:39 GMT FROM: Yuta Kawakubo at Louisiana State University <kawakubo1@lsu.edu> M. L. Cherry (LSU) A. Yoshida, T. Sakamoto, S. Sugita (AGU), Y. Kawakubo (LSU), K. Yamaoka (Nagoya U), S. Nakahira (JAXA), Y. Asaoka (ICRR), S. Torii, Y. Akaike, K. Kobayashi (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U), N. Cannady (GSFC/UMBC), S. Ricciarini (U of Florence), P. S. Marrocchesi (U of Siena), and the CALET collaboration: The long GRB 240117A (Glowbug gamma-ray detection: Cheung et al., GCN Circ 35569; AstroSat CZTI detection: Joshi et al., GCN Circ 35574) triggered the CALET Gamma-ray Burst Monitor (CGBM) at 19:52:31.44 UTC on 17 January 2024 (http://cgbm.calet.jp/cgbm_trigger/flight/1389556167/). The burst signal was seen by only the SGM detector. The burst light curve shows a single pulse that starts at T+2.4 sec, peaks at T+4.5 sec, and ends at T+8.8 sec. The T90 and T50 durations measured by the SGM data are 5.7 +/- 0.6 sec and 2.6 +/- 0.3 sec (40-1000 keV), respectively. The ground-processed light curve is available at http://cgbm.calet.jp/cgbm_trigger/ground/1389556167/index.html The CALET data used in this analysis are provided by the Waseda CALET Operation Center located at Waseda University. View this GCN Circular online at https://gcn.nasa.gov/circulars/35582. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...