{
  "bibcode": "2013GCN.15339....1E",
  "body": "P.A. Evans (U. Leicester) and A. Amral-Rogers (U. Leicester) report on\nbehalf of the Swift-XRT team:\n\nUsing 1.7 ks of XRT Photon Counting mode data and 5 UVOT images for GRB\n131014A, we find an astrometrically corrected X-ray position (using the \nXRT-UVOT alignment and matching UVOT field sources to the USNO-B1 \ncatalogue): RA, Dec = 100.30220, -19.09781 which is equivalent to:\n   RA (J2000.0)\t= 06h 41m 12.53s\n   Dec (J2000.0) = -19d 05' 52.1\"\nwith an uncertainty of 2.3 arcsec (radius, 90% confidence).\n\nThis position is 5.9 arcsec from the initial XRT position reported by \nKennea & Rogers (GCN 15335) and 11.2 arcmin from the LAT position \n(Desiante et al. (GCN 15333), but 4.1 arcsec from the NOT optical \nposition of Schulze et al (GCN 15337).\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 15339,
  "createdOn": 1381843091000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 131014A: Enhanced XRT position",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 131014A"
}