TITLE: GCN CIRCULAR NUMBER: 38278 SUBJECT: GRB 241115A: CALET Gamma-Ray Burst Monitor detection DATE: 24/11/20 02:32:57 GMT FROM: Yuta Kawakubo at Aoyama Gakuin University <kawakubo@phys.aoyama.ac.jp> N. Cannady (GSFC/UMBC), A. Yoshida, T. Sakamoto, S. Sugita, Y. Kawakubo (AGU), K. Yamaoka (Nagoya U), S. Nakahira (JAXA), Y. Asaoka (ICRR), S. Torii, Y. Akaike, K. Kobayashi (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 GRB 241115A (Fermi GBM Final Real-time Localization: Fermi GBM team, GCN Circ 38234; Swift detection of a burst: Williams et al., GCN Circ 38235; Fermi GBM Observation: de Barra et al., GCN Circ 38247) triggered the CALET Gamma-ray Burst Monitor (CGBM) at 13:18:24.988 UTC on 15 November 2024 (https://cgbm.calet.jp/cgbm_trigger/flight/1415711919/index.html). The burst signal was seen by all CGBM detectors. Because of a problem with the ground alert processing script, the GCN notice was not distributed automatically for this event. The burst light curve shows a single pulse that starts at T-0.6 sec, peaks at T+0.1 sec, and ends at T+1.6 sec. The T90 and T50 durations measured by the SGM data are 2.0 +/- 0.3 sec and 1.1 +/- 0.1 sec (40-1000 keV), respectively. The ground-processed light curve is available at https://cgbm.calet.jp/cgbm_trigger/ground/1415711919/ 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/38278. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...