GCN Circular 5059
E. Troja (INAF-IASFPA), V. Mangano (INAF-IASFPA), J. Kennea (PSU), A. Moretti (INAF-OAB) on behalf of the Swift XRT team: A re-analysis of the XRT TDRSS data has led to a different position from the one issued with GCN 5055. The new estimated position for the candidate X-ray afterglow is: RA (2000) = 18 35 45.6 Dec (2000) = +52 37 54.2 with an uncertainty of 7 arcsec (90% confinement). We are still waiting for down-linked data for refined coordinates of the source. We apologize for the inconvenient.