{
  "bibcode": "2013GCN.15335....1K",
  "body": "J. A. Kennea (PSU) and Alex Amaral-Rogers (U Leicester) report on behalf \nof the Swift/XRT team\n\nOn October 14, 2013 at 17:24 UT, Swift began a series of target of \nopportunity observations to cover the region around GRB131014A \n(Fitzpatrick et al., GCN #15332, Evans, GCN #15334), approximately 12.3 \nhours after the burst was detected by Fermi. In Swift/XRT Photon Counting \nmode data we detect an uncatalogued point source at the following \nlocation: RA/Dec(J2000) = 100.30064, -19.09711, which is equivalent to:\n\nRA(J2000) = 06h 41m 12.2s\nDec(J2000) = -19d 05m 49.6s\n\nwith an estimated uncertainty of 4.4 arc-seconds radius (90% containment). \nThis position is 11.3' from the LAT position reported by Desiante et al. \n(GCN #15333). The source brightness is 0.07 +/- 0.01 XRT count/s. We \ncannot yet confirm whether this source is fading.",
  "circularId": 15335,
  "createdOn": 1381788616000,
  "email": "kennea@swift.psu.edu",
  "subject": "GRB 131014A: Swift detection of a possible X-ray afterglow",
  "submitter": "Jamie A. Kennea at PSU/Swift-XRT  <kennea@swift.psu.edu>",
  "eventId": "GRB 131014A"
}