{
  "bibcode": "2014GCN.15747....1M",
  "body": "A. Maselli (INAF-IASFPA), D. Malesani (DARK/NBI) and P. A. Evans (U. \nLeicester) report on behalf of the Swift team:\n\nOn 2014 January 15, Swift has returned to observe the field of the Fermi \nGRB 140110A (Bissaldi et al., GCN 15714; von Kienlin & Connaughton, GCN \n15716). Five uncatalogued X-ray sources were listed by Maselli et al. \n(GCN 15721) as a result of the analysis of seven tiled XRT observations \n(Evans, GCN 15715) carried out on January 10. According to Pal'shin et \nal. (GCN 15725), the position of just one of these sources (#7) is \nconsistent with the IPN annulus.\n\nDuring the XRT observation carried out on January 15, which started 455 \nks after the LAT trigger, the source #7 was detected at a mean count \nrate of 2.64 (+1.06, -0.84) x 10^-3 ct s^-1 which is consistent with the \none [2.61 (+1.25, -0.95) x 10^-3 ct s^-1] corresponding to five days \nearlier. Consequently, this source is unlikely to be the afterglow of \nGRB 140110A. Further details of the XRT analysis carried out on the \nfield of GRB 140110A are available at the following link: \nhttp://www.swift.ac.uk/xrt_products/TILED_GRB00023/.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 15747,
  "createdOn": 1389890172000,
  "email": "maselli@ifc.inaf.it",
  "subject": "GRB 140110A: Further Swift-XRT Observation",
  "submitter": "Alessandro Maselli at INAF/IASF Palermo  <maselli@ifc.inaf.it>",
  "eventId": "GRB 140110A"
}