{
  "bibcode": "2006GCN..4468....1T",
  "body": "K. Torii (Osaka U.) reports:\n\n We investigated our early Ic band frames for the IR afterglow\ncandidate (Bloom, GCN 4465; Bloom and Li, GCN 4467).\n\n In our stacked frame, we identify a low significance enhancement at\nthe position (J2000)\n\n04:50:57.9 +28:25:56\n\nwith 2\" uncertainty. There is no corresponding object in DSS2 red.\nThe Ic band magnitude in our frame corresponds to ~16.3 mag.  As of\nthis writing, we are not confident if this is an astrophysical source\nor a noise, due to its low SN.\n\n We note that this position is about 7\" north of that given in GCN\n4467.  We also note that the position given in GCN 4467 is very close\nto, but formally outside of, the BAT 3' error radius.\n\n===",
  "circularId": 4468,
  "createdOn": 1136889364000,
  "email": "torii@ess.sci.osaka-u.ac.jp",
  "subject": "GRB 060110: Optical observation",
  "submitter": "Ken ichi Torii at RIKEN  <torii@ess.sci.osaka-u.ac.jp>",
  "eventId": "GRB 060110"
}