{
  "bibcode": "2015GCN.18022....1M",
  "body": "A. Melandri, P. D'Avanzo, M.G. Bernardini (INAF-OAB), K.L. Page, P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team:\n\nSwift-XRT has conducted further observations of the field of the Swift/BAT-detected burst GRB 150710B (Cummings et al. GCN Circ. 18009). The observations now extend from T0+115 ks to T0+259 ks.\n\nThe source reported by Melandri et al. (GCN Circ. 18018) has significantly faded between two epochs, down to a level of (7 +/- 2)e-3 cts/s, and is therefore the GRB afterglow.\n\nThe results of the full analysis of the XRT observations are available at http://www.swift.ac.uk/ToO_GRBs/00020542.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 18022,
  "createdOn": 1436799898000,
  "email": "andrea.melandri@brera.inaf.it",
  "subject": "GRB 150710B: Swift-XRT afterglow detection",
  "submitter": "Andrea Melandri at INAF-OAB  <andrea.melandri@brera.inaf.it>",
  "eventId": "GRB 150710B"
}