{
  "bibcode": "2019GCN.23714....1M",
  "body": "P. Minaev (IKI), A. Pozanenko (IKI) report:\n\nWe analyzed the publicly available SPI-ACS data (>~ 80 keV) of INTEGRAL \nobservatory covering trigger time (UT) 20:57:02 of the GRB 190114C \n(Gropp et al. 2019, GCN 23688; Hamburg et al. 2019, GCN 23707).\n\nWe found statistically significant extended emission up to ~ 5000 sec \nafter the trigger. The extended emission can be approximated by power \nlaw model with the index of 0.99 +/- 0.05.\n\nWe do not detect any significant emission from possible precursor on \ntime scales 0.05 ��� 10 sec within (-500, 0) sec time interval before the \ntrigger.\n\nThe SPI-ACS/INTEGRAL light curve can be found at:\nhttp://grb.rssi.ru/GRB190114C/GRB190114C_SPI-ACS_LC.png",
  "circularId": 23714,
  "createdOn": 1547557937000,
  "email": "apozanen@iki.rssi.ru",
  "subject": "GRB 190114C: SPI-ACS/INTEGRAL extended emission detection",
  "submitter": "Alexei Pozanenko at IKI, Moscow  <apozanen@iki.rssi.ru>",
  "eventId": "GRB 190114C"
}