TITLE: GCN CIRCULAR NUMBER: 16455 SUBJECT: Further Swift/XRT observations of GRB140620A/iPTFcva DATE: 14/06/25 14:41:52 GMT FROM: Massimiliano de Pasquale at IASF-Palermo M. De Pasquale (INAF-Palermo) reports on behalf of the Swift team: Analyzing XRT data of the X-ray source at the position of the iPTF14cva transient (De Pasquale, GCN Circ. 16428) from 37.6 to 367.3 ks after the trigger, we found that this source is fading with a decay slope of 1.32 (+0.18, -0.15). We therefore confirm that this source is the X-ray afterglow of the GRB associated with this transient. The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00020387. This circular is an official product of the Swift-XRT team. I.A.S.F. INAF Mailing System Outgoing mail is certified Virus Free. Checked by Kaspersky anti-virus system