{
  "bibcode": "2005GCN..3649....1R",
  "body": "T.P. Roberts, K. Page, A. Beardmore (U. Leicester), J.L. Racusin,\nJ.A. Kennea (PSU), N. White (GSFC), D. Hinshaw (GSFC-SPSYS) report on\nbehalf of the Swift XRT team:\n\nWe have re-analysed the complete Swift dataset from the TOO\nobservation of the INTEGRAL-detected GRB050714a (see GCN circ. 3610),\nbeginning 13.7 hours after the burst.  The new refined coordinates of\nthe afterglow candidate are:\n\nRA(J2000) = 02 54 22.2\nDec(J2000) = +69 06 46\n\nWe estimate an uncertainty of 6.9 arcseconds on this position (90%\ncontainment).  However, we were unable establish from this data whether\nthe source was definitely fading due its low count rate.\n\nSwift began a second observation of this GRB at 00:05 UT on 19th July\n2005 (5.0 days since the burst event).  In 9.7 ks of data we do not\ndetect the candidate afterglow.  Hence we confirm that the behaviour\nof the X-ray source identified in our first circular is consistent\nwith it being the afterglow of GRB 050714a.",
  "circularId": 3649,
  "createdOn": 1121803174000,
  "email": "tro@star.le.ac.uk",
  "subject": "GRB 050714a: Refined XRT analysis and afterglow confirmation",
  "submitter": "Tim Roberts at Leicester U/BA  <tro@star.le.ac.uk>",
  "eventId": "GRB 050714A"
}