TITLE: GCN CIRCULAR NUMBER: 14900 SUBJECT: GRB 130615A: Enhanced Swift-XRT position DATE: 13/06/15 16:33:43 GMT FROM: Phil Evans at U of Leicester P.A. Evans, M.R. Goad, J.P. Osborne and A.P. Beardmore (U. Leicester) report on behalf of the Swift-XRT team. Using 1436 s of XRT Photon Counting mode data and 1 UVOT images for GRB 130615A, we find an astrometrically corrected X-ray position (using the XRT-UVOT alignment and matching UVOT field sources to the USNO-B1 catalogue): RA, Dec = 274.82896, -68.16092 which is equivalent to: RA (J2000): 18h 19m 18.95s Dec (J2000): -68d 09' 39.3" with an uncertainty of 2.3 arcsec (radius, 90% confidence). This position may be improved as more data are received. The latest position can be viewed at http://www.swift.ac.uk/xrt_positions. Position enhancement is described by Goad et al. (2007, A&A, 476, 1401) and Evans et al. (2009, MNRAS, 397, 1177). This circular was automatically generated, and is an official product of the Swift-XRT team.