{
  "bibcode": "2016GCN.20057....1D",
  "body": "P. D'Avanzo, A. Melandri (INAF-OAB), P. A. Evans (U. Leicester), \nreport on behalf of the Swift-XRT team: \n\nSwift-XRT has performed follow-up observations of the Fermi/LAT-detected \nburst GRB 161015A (Masanori Ohno et al., GCN 20054; Stanbro & Meegan, \nGCN Circ. 20056) in a series of observations tiled on the sky. The total \nexposure time is 5 ks, distributed over 4 tiles. The data were collected \nbetween T0+38.2 ks and T0+45.8 ks, and are entirely in Photon Counting \n(PC) mode. \n\nAn uncatalogued X-ray source is detected within the Fermi/LAT error circle. \nThe position of this source is RA, Dec=269.2518, +30.37356 which is \nequivalent to:\n\nRA (J2000): 17:57:00.43\nDec(J2000): +30:22:24.8\n\nwith an uncertainty of 2.7 arcsec (radius, 90% confidence). This\nposition is 12.2 arcmin from the Fermi/LAT position. The source has a \n0.3-10 keV count rate of about 0.03 ct/sec. We cannot determine fading \nat this time.\n\n[GCN OPS NOTE(17oct16): Per author's request, the GRB name in the first sentence\nwas corrected from 16A to 15A.]",
  "circularId": 20057,
  "createdOn": 1476630683000,
  "email": "paolo.davanzo@brera.inaf.it",
  "subject": "GRB 161015A: Swift-XRT observations",
  "submitter": "Paolo D'Avanzo at INAF-OAB  <paolo.davanzo@brera.inaf.it>",
  "eventId": "GRB 161015A"
}