TITLE: GCN CIRCULAR NUMBER: 16016 SUBJECT: GRB 140320A: Confirmation of a fading X-ray afterglow DATE: 14/03/21 10:08:11 GMT FROM: Kim Page at U.of Leicester K.L. Page, C. Pagani, P.A. Evans (U. Leicester) & J.K. Cannizzo (NASA/UMBC) report on behalf of the Swift-XRT team: We have now analysed 9.8 ks of Swift-XRT data for GRB 140320A, between 93 s and 33.5 ks after the trigger. The X-ray source given by Page, Pagani & Cannizzo in GCN Circ. 16010 has now faded, with a 3-sigma upper limit on the count rate centred at 27 ks after the trigger of 1.2 x 10^-3 count s^-1. We therefore confirm this source as the X-ray afterglow of GRB 140320A. This circular is an official product of the Swift-XRT team.