{
  "bibcode": "2008GCN..8358....1K",
  "body": "J. A. Kennea and D. Grupe (PSU) report on behalf of the Swift/XRT Team\n\nWe have analyzed downlinked data from the XRT observations of GRB 081011 \n(Grupe et al, GCN #8355). The XRT began observing the field at 00:30:24.4 \nUT, 94 seconds after the BAT trigger. Data from the first orbit of \nobservations reveal an uncatalogued fading point source at RA, Dec = \n220.34435, +33.544771 which is the equivalent to:\n\nRA(J2000) = 14h 41m 22.6s\nDec(J2000) = +33d 32m 41.1s\n\nwith an estimated uncertainty of 8 arcseconds radius (90% confidence). \nThis position is 57 arcseconds from the BAT refined position (Sakamoto et \nal, GCN #8357).",
  "circularId": 8358,
  "createdOn": 1223735919000,
  "email": "kennea@astro.psu.edu",
  "subject": "GRB 081011: Swift/XRT detection",
  "submitter": "Jamie A. Kennea at PSU/Swift-XRT  <kennea@astro.psu.edu>",
  "eventId": "GRB 081011"
}