TITLE: GCN CIRCULAR NUMBER: 28107 SUBJECT: GRB 200714E: Swift-XRT observations DATE: 20/07/15 13:24:55 GMT FROM: Phil Evans at U of Leicester V. D'Elia (ASDC), A. D'Ai (INAF-IASFPA), B. Sbarufatti (PSU), D.N. Burrows (PSU), J. D. Gropp (PSU), A.P. Beardmore (U. Leicester), J.P. Osborne (U. Leicester), A. Melandri (INAF-OAB) and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the Fermi-GBM and Swift/BAT (GUANO)-detected burst GRB 200714E (GCN Circs. 28098 and 28103), collecting 2.2 ks of Photon Counting (PC) mode data between T0+37.3 ks and T0+44.5 ks. One uncatalogued X-ray source has been detected, it is below the RASS limit and shows no definitive signs of fading. Therefore, at the present time we cannot confirm this as the afterglow. Details of this source are given below: Source 1: RA (J2000.0): 196.8225 = 13:07:17.41 Dec (J2000.0): -51.6390 = -51:38:20.4 Error: 3.1 arcsec (radius, 90% conf. [Enhanced position]) Count-rate: 0.0138 +/- 0.0033 ct s^-1 Distance: 96 arcsec from Swift/BAT position. Flux: (6.2 +/- 1.5)e-13 erg cm^-2 s^-1 (observed, 0.3-10 keV) The results of the XRT-team automatic analysis of the XRT observations, including a position-specific upper limit calculator, are available at https://www.swift.ac.uk/ToO_GRBs/00021017. Further observations are planned. This circular is an official product of the Swift-XRT team.