{
  "bibcode": "2013GCN.14584....1D",
  "body": "P. D'Avanzo, A. Melandri (INAF-OAB) report on behalf of  the Swift team:\n\nWe have analysed 1.3 ks of Swift-XRT data for the Fermi 130504C (Kocevski\nGCN Circ. 14574; Burgess et al. GCN Circ. 14583), from 65.6 ks to 70.1 ks\nafter the LAT trigger. The data are all in Photon Counting (PC) mode.\n\nWe detect an uncatalogued X-ray source inside the LAT error circle\n(Kocevski GCN Circ. 14574), at the following position: RA, Dec=91.63047,\n3.83388 which is equivalent to:\n\nRA (J2000): 06 06 31.3\nDec (J2000): +03 50 01.96\n\nwith an uncertainty of 4.8 arcsec (radius, 90% confidence).\nThe count rate at this position is (4.4 +/- 0.7) x 10^-2 cts/s. At the\npresent stage, it is not possible to determine whether the source is\nfading.",
  "circularId": 14584,
  "createdOn": 1367800398000,
  "email": "paolo.davanzo@brera.inaf.it",
  "subject": "GRB 130504C: Swift-XRT observations",
  "submitter": "Paolo D'Avanzo at INAF-OAB  <paolo.davanzo@brera.inaf.it>",
  "eventId": "GRB 130504C"
}