{
  "bibcode": "2013GCN.14695....1Z",
  "body": "B.-B. Zhang (PSU), Dirk Grupe (PSU). D. Malesani (DARK/NBI) and J. Kennea (PSU) \nreport  on behalf of the Swift-XRT team:\n\nWe have analyzed 6.8 ks of XRT data for the INTEGRAL-detected burst: \nGRB 130514B,  from 314.3 ks to 321.1 ks after the INTERGRAL trigger.\nThe data are entirely in Photon Counting (PC) mode. We confirm that \nthe X-ray source reported in Zhang et al. GCN 14651 has been faded with \ncurrent count rate of  around 3e-3 count/s.  The light curve can be modeled with  \na power-law decay with a decay index of alpha=0.98 (+0.27, -0.15). \nWe therefore conclude that the X-ray source reported in Zhang et al. GCN 14651 \nis the X-ray afterglow of GRB 130514B.\n\nThe results of the XRT-team automatic analysis are available at\n\nhttp://www.swift.ac.uk/xrt_curves/00020275/\n\n\nThis circular is an official product of the Swift-XRT team.\n\n[GCN OPS NOTE(25may13):  The \"144651\" hasn corrected to \"14651\".]",
  "circularId": 14695,
  "createdOn": 1369255164000,
  "email": "bbzhang@psu.edu",
  "subject": "GRB 130514B: Further Swift-XRT Observations",
  "submitter": "Binbin Zhang at PSU  <bbzhang@psu.edu>",
  "eventId": "GRB 130514B"
}