TITLE: GCN CIRCULAR NUMBER: 35842 SUBJECT: GRB 240229A: CALET Gamma-Ray Burst Monitor detection DATE: 24/03/01 04:42:26 GMT FROM: Yuta Kawakubo at Louisiana State University <kawakubo1@lsu.edu> K. Yamaoka (Nagoya U), A. Yoshida, T. Sakamoto, S. Sugita (AGU), Y. Kawakubo (LSU), S. Nakahira (JAXA), Y. Asaoka (ICRR), S. Torii, Y. Akaike, K. Kobayashi (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U), N. Cannady (GSFC/UMBC), M. L. Cherry (LSU), S. Ricciarini (U of Florence), P. S. Marrocchesi (U of Siena), and the CALET collaboration: The long GRB 240229 (Fermi GBM Final Real-time Localization: Fermi GBM team, GCN Circ. 35833; BALROG localization: Biltzinger et al., GCN Circ 35834; INTEGRAL SPI ACS: Trigger Num. 10602) triggered the CALET Gamma-ray Burst Monitor (CGBM) at 14:07:07.40 UTC on 29 February 2024 (http://cgbm.calet.jp/cgbm_trigger/flight/1393250567/). The burst signal was seen by all CGBM detectors. The burst light curve shows a double-peaked structure that starts at T+2.9 sec, peaks at T+26.5 sec, and ends at T+36.8 sec. The T90 and T50 durations measured by the SGM data are 27.6 +/- 2.5 sec and 19.2 +/- 0.4 sec (40-1000 keV), respectively. The ground-processed light curve is available at http://cgbm.calet.jp/cgbm_trigger/ground/1393250567/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/35842. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...