{
  "bibcode": "2018GCN.22744....1M",
  "body": "S. Matsukawa, A. Yoshida, T. Sakamoto, V. Pal'shin, Y. Kawakubo,\nA. Tezuka, H. Onozawa (AGU), K. Yamaoka (Nagoya U),\nS. Nakahira (RIKEN), I. Takahashi (IPMU), Y. Asaoka, S. Ozawa,\nS. Torii (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U),\nW. Ishizaki (ICRR), M. L. Cherry (LSU), S. Ricciarini (U of Florence),\nA. V. Penacchioni, P. S. Marrocchesi (U of Siena)\nand the CALET collaboration:\n\nThe long, bright GRB 180526A (INTEGRAL SPI-ACS trigger #8067,\nKonus-Wind trigger time on 11:03:36.006, AstroSat CZTI detection:\nSharma et al., GCN circ. 22742) triggered the CALET Gamma-ray\nBurst Monitor (CGBM) at 11:03:36.200 UTC on 26 May 2018.\nNo real-time CGBM GCN notice was distributed about this\ntrigger because the real-time communication from the ISS was off\n(loss of signal). The burst signal was seen by all CGBM detectors.\n\nThe burst light curve shows a multi-peaked structure which starts\nat T-2.2 sec, peaks at T+44.4 sec and ends at T+79.2 sec.\nThe T90 and the T50 durations measured by the SGM data are\n56.9 +- 2.8 sec and 16.3 +- 1.3 sec (40-1000 keV), respectively.\n\nThe ground processed light curve is available at\n\nhttp://cgbm.calet.jp/cgbm_trigger/ground/1211367794/\n\nThe CALET data used in this analysis are provided by the Waseda CALET\nOperation Center located at the Waseda University.",
  "circularId": 22744,
  "createdOn": 1527603373000,
  "email": "tsakamoto@phys.aoyama.ac.jp",
  "subject": "GRB 180526A: CALET Gamma-Ray Burst Monitor detection",
  "submitter": "Takanori Sakamoto at AGU  <tsakamoto@phys.aoyama.ac.jp>",
  "eventId": "GRB 180526A"
}