{
  "bibcode": "2017GCN.21379....1G",
  "body": "B. Gendre (UVI, USA), L. Piro (IAPS/INAF, Italy), E. Troja (GSFC, USA), R. \nRicci (INAF/IRA-Bologna), M. Wieringa (ATNF,CSIRO), K. Bannister \n(ATNF,CSIRO) report:\n\nWe observed the field of GRB 170714A (D'Ai et al., GCN 21340) with \nXMM-Newton between 370,993 and 506,293 seconds post-trigger under our XMM \nprogram on ultralong GRBs (PI: Piro).\n\nThe X-ray afterglow is clearly visible during the whole observation, at \nthe position:\n\nRA: 2h17m24.02s\nDEC: +1d59'28.51\"\n\nwith an error of 1.3\" (statistic + systematic, 90% confidence),\nconsistent with the position of the optical counterpart (de Ugarte Postigo \net al. GCN 21346) and of XRT (Evans et al. GCN 21341).\n\nThe observed mean X-ray flux(0.3-10 keV) is 3.7e-14 erg/s/cm2\n\nWe thank the ESA and XMM SOC staff for performing this TOO trigger.",
  "circularId": 21379,
  "createdOn": 1501317191000,
  "email": "luigi.piro@iaps.inaf.it",
  "subject": "GRB170714A: XMM observation of the afterglow",
  "submitter": "Luigi Piro at INAF  <luigi.piro@iaps.inaf.it>",
  "eventId": "GRB 170714A"
}