TITLE: GCN CIRCULAR NUMBER: 9810 SUBJECT: GRB 090814B: Confirmation of the X-ray afterglow DATE: 09/08/15 08:16:49 GMT FROM: Phil Evans at U of Leicester P.A. Evans (U. Leicester) and W.H. Baumgartner (GSFC/UMBC) report on behalf of the Swift-XRT team: The Swift-XRT conducted a second observation of GRB 090814B (Beckmann et al. GCN. Circ. 9795), gathering 3.3 ks of data between T0+48 ks and T0+60 ks. The source reported by Evans & Baumgartner (GCN Circ. 9803) has faded to a level of 0.11 ± 0.03 count/sec, with a power-law decay index of alpha=0.7+/-0.3. This source is thus confirmed as the afterglow of GRB 090814B. The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00020107. This circular is an official product of the Swift-XRT team.