{
  "bibcode": "2019GCN.23647....1S",
  "body": "T. Sakamoto, V. Pal'shin (AGU), Y. Kawakubo (LSU),\nA. Yoshida, S. Sugita (AGU), A. Tezuka, S. Matsukawa, H. Onozawa,\nT. Ito, H. Morita, Y. Sone (AGU), K. Yamaoka (Nagoya U), S. Nakahira (RIKEN),\nI. Takahashi (IPMU), Y. Asaoka, S. Ozawa, S. Torii (Waseda U),\nY. Shimizu, T. Tamura (Kanagawa U), W. Ishizaki (ICRR), M. L. Cherry (LSU),\nS. Ricciarini (U of Florence), A. V. Penacchioni, P. S. Marrocchesi (U of Siena)\nand the CALET collaboration:\n\nSince the start of the operation of CALET Gamma-ray Burst Monitor (CGBM)\non October 2015, the CGBM team has been issuing the GCN circulars for\nalmost all the confirmed GRBs.  However, starting on January 2019, we will\nonly issue the GCN circulars for the particular types of GRBs such as\n1) well localized GRBs, 2) short GRBs and 3) peculiar GRBs\n(e.g., ultra-long GRBs, very bright GRBs, etc).  We will report the results\nfor gravitational wave and neutrino events in case the CGBM observes them\nat favorable location and timing.\n\nNote that the CALET-GBM Lightcurve Notices (https://gcn.gsfc.nasa.gov/calet.html)\ncontinue to be distributed to the community as before.",
  "circularId": 23647,
  "createdOn": 1547035651000,
  "email": "tsakamoto@phys.aoyama.ac.jp",
  "subject": "CALET Gamma-Ray Burst Monitor: Policy change in the GCN circulars",
  "submitter": "Takanori Sakamoto at AGU  <tsakamoto@phys.aoyama.ac.jp>"
}