{
  "bibcode": "2020GCN.28812....1C",
  "body": "D.F. Cowen (PSU), J. DeLaunay (PSU), D. B. Fox (PSU),\nA. Keivani (Columbia U.), J.P. Osborne (U. Leicester),\nF. Krauss (PSU), T. Gregoire (PSU), P.A. Evans (U. Leicester),\nJ.A. Kennea (PSU) and H. A. Ayala Solares (PSU) report:\n\nWe have analysed 2.7 ks of XRT data for Fermi J1725.51312 (Buson et al.\nGCN Circ. 28751). The data were taken in Photon Counting (PC) mode.\nXRT observations establish a refined position for the\nsource: R.A. 17:23:14.09, Dec. +14:20:59.1, with a 90% containment\nradius r_90 = 2.9\".\nThe best-fit power-law spectrum has a photon index alpha = 1.5 (+0.8, -0.4)\nand observed flux f_X = 6.5 (+3.1, -2.5) x 10-13 erg cm-2 s-1 (0.3-10 keV)\nThe observed flux is lower by a factor of 4 to 10 by comparison to its XMM\nslew observation on 2006-09-04 (XMMSL2 J172313.9+142100, OsID:9123400002)\n\nWe do not claim this source as a counterpart to IceCube 201021A from these\nobservations.",
  "circularId": 28812,
  "createdOn": 1604090641000,
  "email": "tmg5746@psu.edu",
  "subject": "IceCube 201021A: Swift follow-up of Fermi J1725.5+1312",
  "submitter": "Timothee Gregoire at Penn State  <tmg5746@psu.edu>",
  "eventId": "IceCube-201021A"
}