TITLE: GCN CIRCULAR NUMBER: 21146 SUBJECT: GRB 170511A CALET Gamma-Ray Burst Monitor detection DATE: 17/05/26 08:50:40 GMT FROM: Takanori Sakamoto at AGU K. Yamaoka (Nagoya U), A. Yoshida, T. Sakamoto, Y. Kawakubo, M. Moriyama, Y. Yamada, A. Tezuka, S. Matsukawa (AGU), 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 170511A (Takao et al., GCN Circ. 21137; Fermi-GBM trigger #516175156) was detected by the CALET Gamma-ray Burst Monitor (CGBM). The burst signal was only seen by the SGM instrument. Since the detection significance is less than 7 sigma in the CGBM data, no on-board trigger occurred for this event. The light curve of the SGM shows two separated peaks. The initial peak starts at T+25 sec, peaks at T+28 sec and ends at T+33 sec (T is the trigger time of Fermi-GBM). The second peak starts at T+35 sec, peaks at T+38 sec and ends at T+40 sec. The T90 duration measured by the SGM data is 12.5 +- 1.0 sec (40-1000 keV). The light curve is available at http://cgbm.calet.jp/cgbm_trigger/flight/1178517128/ The CALET data used in this analysis are provided by the Waseda CALET Operation Center located at the Waseda University.