{
  "bibcode": "2008GCN..8364....1K",
  "body": "J. A. Kennea and M. Stroh (PSU) report on behalf of the Swift/XRT Team\n\nWe have analyzed downlinked data from the XRT observations of GRB 081012\n(Stroh et al, GCN #8361). The XRT began observing the field at 14:00:09 \nUT, approximately 49 minutes after the BAT trigger. Data from the first \norbit of observations reveal an uncatalogued point source at RA, Dec = \n30.20029, -17.63715 which is the equivalent to:\n\nRA(J2000) = 02h 00m 48.0s\nDec(J2000) = -17d 38m 13.7s\n\nwith an estimated uncertainty of 8 arcseconds radius (90% confidence). \nThis position is 67 arcseconds from the BAT refined position (Sato et \nal, GCN #8363).",
  "circularId": 8364,
  "createdOn": 1223831188000,
  "email": "kennea@astro.psu.edu",
  "subject": "GRB 081012: Swift/XRT detection",
  "submitter": "Jamie A. Kennea at PSU/Swift-XRT  <kennea@astro.psu.edu>",
  "eventId": "GRB 081012"
}