{
  "bibcode": "2018GCN.22606....1M",
  "body": "C. Malacaria (NASA-MSFC/USRA) and A. von Kienlin (MPE)\nreport on behalf of the Fermi GBM Team:\n\n\"The Fermi Gamma-ray Burst Monitor (GBM) triggers\n\n544628550/180405571 at 13:42:25.886 UT on 5 April 2018\n544542853/180404579 at 13:54:08.080 UT on 4 April 2018\n544531428/180404447 at 10:43:43.753 UT on 4 April 2018\n\ntentatively classified as GRBs, are in fact not due to GRBs.\nThese triggers are caused by an occultation step due to\nMAXI J1820+070 (von Kienlin, GCN Circ. 22595).\n\nAdditional triggers are likely expected from this source in the next\ndays which, however, will not be reported in future circulars.\"",
  "circularId": 22606,
  "createdOn": 1522949203000,
  "email": "christian.malacaria@nasa.gov",
  "subject": "Fermi GBM triggers 544628550/180405571, 544542853/180404579, 544531428/180404447 are not GRBs",
  "submitter": "Christian Malacaria at U of Alabama/MSFC  <christian.malacaria@nasa.gov>"
}