TITLE: GCN CIRCULAR NUMBER: 30854 SUBJECT: GRB 210919A: Swift-XRT refined Analysis DATE: 21/09/19 15:57:30 GMT FROM: Phil Evans at U of Leicester <pae9@leicester.ac.uk> M. Perri (SSDC & INAF-OAR), V. D'Elia (SSDC & INAF-OAR), A. D'Ai (INAF-IASFPA), J. D. Gropp (PSU), J.A. Kennea (PSU), P.A. Evans (U. Leicester), J.P. Osborne (U. Leicester), K.L. Page (U. Leicester) and A. Tohuvavohu report on behalf of the Swift-XRT team: We have analysed 1.5 ks of XRT data for GRB 210919A (Tohuvavohu et al. GCN Circ. 30846), from 105 s to 1.6 ks after the BAT trigger. The data are entirely in Photon Counting (PC) mode. The enhanced XRT position for this burst was given by Goad et al. (GCN Circ. 30850). We cannot determine at the present time whether the source is fading. The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/01073893. This circular is an official product of the Swift-XRT team.