{
  "bibcode": "2016GCN.19225....1Y",
  "body": "A. Yoshida, T. Sakamoto, I. Takahashi, Y. Kawakubo, K. Senuma, \nM. Moriyama, Y. Yamada (AGU), K. Yamaoka (Nagoya U), S. Nakahira (JAXA), \nY. Asaoka, S. Ozawa, S. Torii (Waseda U), Y. Shimizu, T. Tamura (Kanagawa U), \nW. Ishizaki (ICRR), M. L. Cherry (LSU), S. Ricciarini (U of Florence) \nP. S. Marrocchesi (U of Siena) and the CALET collaboration:\n\nThe CALET Gamma-ray Burst Monitor (CGBM) was operating at the trigger time \nof G211117 (GCN Circ. 18728).  No CGBM on-board trigger occurred at the time \nof the event.  Based on the updated LIGO sky map (GCN Circ. 18858), \nthe southern arc of the high probability area was in the field-of-view of CGBM.  \n\nBased on the analysis of the light curve data with 0.125 sec time resolution \nfrom -60 sec to 60 sec from the trigger time, we found no significant excess \naround the trigger time in either the HXM (7-1000 keV) or the SGM (0.1-20 MeV) \ndata.",
  "circularId": 19225,
  "createdOn": 1458910443000,
  "email": "tsakamoto@phys.aoyama.ac.jp",
  "eventId": "LIGO/Virgo G211117",
  "subject": "LIGO/Virgo G211117: CALET GBM Observations",
  "submitter": "Takanori Sakamoto at Aoyama Gakuin U  <tsakamoto@phys.aoyama.ac.jp>"
}