{
  "bibcode": "2014GCN.16390....1E",
  "body": "P.A. Evans, K.L. Page and A. Amaral-Rogers (U. Leicester) report on\nbehalf of the Swift-XRT team:\n\nWe have analysed 4.8 ks of XRT data for the IPN-detected burst: GRB\n140611A, from 80.5 ks to 92.1 ks after the IPN trigger (Golenetskii et\nal., GCN Circ. 16384). The burst was also detected in ground analysis\nof BAT data (Cummings, GCN Circ. 16386). The data are entirely in\nPhoton Counting (PC) mode.  An X-ray source is detected within the IPN\nand BAT error regions. The refined XRT position is RA, Dec = 349.9173,\n-40.1044 which is equivalent to:\n\nRA (J2000): 23 19 40.15\nDec(J2000): -40 06 16.0\n\nwith an uncertainty of 5.5 arcsec (radius, 90% confidence). This\nposition is 64 arcsec from the BAT ground position and 106 arcsec from\nthe centre of the IPN error box. The source has a mean count rate of\n(1.9 +0.9,-0.7) x 10^-3 count s^-1 over this time interval. Within the\n4-arcmin radius BAT error circle, we would expect approximately 0.25\nserendipitous sources of at least this brightness. We cannot determine\nwhether the source is fading and no further observations are planned.\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/00020385.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 16390,
  "createdOn": 1402581567000,
  "email": "kpa@star.le.ac.uk",
  "subject": "GRB 140611A: Swift-XRT observations",
  "submitter": "Kim Page at U.of Leicester  <kpa@star.le.ac.uk>",
  "eventId": "GRB 140611A"
}