{
  "bibcode": "2014GCN.16455....1D",
  "body": "M. De Pasquale (INAF-Palermo) reports on behalf of the Swift team:\n\nAnalyzing XRT data of the X-ray source at the position of the iPTF14cva transient\n(De Pasquale, GCN Circ. 16428) from 37.6 to 367.3 ks after the trigger, we found\nthat this source is fading with a decay slope of 1.32 (+0.18, -0.15). We therefore\nconfirm that this source is the X-ray afterglow of the GRB associated with this\ntransient.\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/00020387.\n\nThis circular is an official product of the Swift-XRT team.\nI.A.S.F.   INAF   Mailing System\nOutgoing mail is certified Virus Free.\nChecked by Kaspersky anti-virus system",
  "circularId": 16455,
  "createdOn": 1403707312000,
  "email": "mdp@ifc.inaf.it",
  "subject": "Further Swift/XRT observations of GRB140620A/iPTFcva",
  "submitter": "Massimiliano de Pasquale at IASF-Palermo  <mdp@ifc.inaf.it>",
  "eventId": "GRB 140620A"
}