{
  "bibcode": "2006GCN..5251....1P",
  "body": "K. L. Page, A. P. Beardmore (U. Leicester) and J. A. Kennea (PSU) report \non behalf of the Swift/XRT team:\n\nWe have analysed 37.8 ks of XRT data obtained for the field of GRB 060602A \n(Schady et al.; GCN 5196), starting 1.8 days after the trigger, when the \nburst was no longer Moon constrained.\n\nA faint source was found within the BAT error circle, at a position of\n\nRA(J2000)  =  09 58 16.80\nDec(J2000) = +00 18 14.8\n\nwith an estimated uncertainty of 4.2 arcsec (90% containment). This source \nis fading with an approximate slope of alpha = 1.10, so is very likely the \nX-ray afterglow.\n\nThis source is 2.3 arcsec from the possible counterpart identified by \nJensen et al. (GCN 5203).\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 5251,
  "createdOn": 1150147422000,
  "email": "kennea@astro.psu.edu",
  "subject": "GRB 060602A: Swift/XRT analysis",
  "submitter": "Jamie A. Kennea at PSU/Swift-XRT  <kennea@astro.psu.edu>",
  "eventId": "GRB 060602A"
}