{
  "bibcode": "2016GCN.19551....1E",
  "body": "P.A. Evans, A.P. Beardmore, M.R. Goad and J.P. Osborne (U. Leicester) \nreport on behalf of the Swift-XRT team.\n\nUsing 2.1 ks of XRT Photon Counting mode data and 5 UVOT images for the \nrecent BAT trigger on SGR 1617-5103 (trigger 700791, GCN Circs. 19547, \n19548, 19550) we have produced an enhanced XRT position (using the \nXRT-UVOT alignment and matching UVOT field sources to the USNO-B1 \ncatalogue) of: RA, Dec= 244.40105, -51.04011, which is equivalent to:\n\nRA (J2000):  16h 17m 36.25s\nDec (J2000): -51d 02' 24.4\"\n\nwith an uncertainty of 1.4 arcsec (90% confidence). This position is \n5.2\" from the position reported in GCN Circ. 19548, and 0.6\" from the \nChandra position of the central source of RCW103 given in IAU Circ. 7350.\n\nNote that there was a typo in GCN Circ. 19548; the decimal position was \ncorrect but the minus sign was missing from the sexagesimal declination.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 19551,
  "createdOn": 1466688372000,
  "email": "pae9@leicester.ac.uk",
  "subject": "SGR 1617-5103 (BAT trigger 700791): Enhanced Swift-XRT position.",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>"
}