{
  "bibcode": "2008GCN..8156....1B",
  "body": "S. D. Barthelmy (GSFC), W. Baumgartner (GSFC/UMBC), A. P. Beardmore (U Leicester),\nJ. Cummings (GSFC/UMBC), P. A. Evans (U Leicester), N. Gehrels (GSFC),\nJ. Kennea (PSU), C. B. Markwardt (GSFC/UMD), P. T. O'Brien (U Leicester)\n(on behalf of the Swift team):\n\nUsing the BAT data set from T-119 to T+183 sec from the recent\ntelemetry downlink for trigger 322590 at 08:15:09 UT (GCN 8153),\nwe conclude the likelihood that this trigger is a real GRB is very low.\nThe automated ground processing of the BAT data yields a very weak peak\nin the image domain (5.9 sigma).\n\nAnd 5 ksec of XRT data (the first 4 orbits) does not show any source.\n\nThe UVOT candidate mentioned in Circ 5183 is not an afterglow\nand is consistant with the known source 2MASS J21334565+4201499.",
  "circularId": 8156,
  "createdOn": 1219948757000,
  "email": "scott@lheamail.gsfc.nasa.gov",
  "subject": "Swift-BAT trigger 322590 is not a GRB",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@lheamail.gsfc.nasa.gov>"
}