{
  "bibcode": "2010GCN.10530....1E",
  "body": "P.A. Evans and M.R. Goad (U. Leicester) report on behalf of the Swift-XRT team:\n\nUsing 5452 s of XRT Photon Counting mode data and 8 UVOT images, we find an\nastrometrically corrected X-ray position (using the XRT-UVOT alignment and\nmatching UVOT field sources to the USNO-B1 catalogue):\nRA, Dec = 278.43520, -8.51880 which is equivalent to:\n\nRA (J2000):  18 33 44.45\nDec (J2000): -08 31 07.7\n\nwith an uncertainty of 1.6 arcsec (radius, 90% confidence).\n\nThis position may be improved as more data are received.  The latest position\ncan be viewed at http://www.swift.ac.uk/xrt_positions; all XRT products for this\nevent are available at http://www.swift.ac.uk/xrt_products/00416485. Position\nenhancement is described by Goad et al. (2007, A&A, 476, 1401) and Evans et al.\n(2009, MNRAS, 397, 1177).\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 10530,
  "createdOn": 1269070958000,
  "email": "pae9@star.le.ac.uk",
  "subject": "Probable SGR 1833-0832: Enhanced Swift-XRT position",
  "submitter": "Phil Evans at U of Leicester  <pae9@star.le.ac.uk>"
}