{
  "bibcode": "2008GCN..8319....1P",
  "body": "K.L. Page, A.P. Beardmore (U. Leicester) and H.A. Krimm (CRESST/GSFC/USRA) \nreport on behalf of the Swift-XRT team:\n\nSwift began observing the field of the INTEGRAL GRB 081003A (Mereghetti et \nal., GCN Circ. 8314) 7.6 ks after the trigger. In 1.8 ks of Photon \nCounting mode data, we detect a single source within the INTEGRAL error \ncircle at a position of RA, Dec = 262.39082, 16.57103, which is equivalent \nto\n\nRA(J2000):   17 29 33.80\nDec(J2000): +16 34 15.70\n\nwith an uncertainty of 3.9 arcsec (radius, 90% containment). The source \nhas a count rate of ~0.026 during this observation.\n\nThe spectrum of the source can be fitted by an absorbed power-law, with \nGamma = 3.6 +1.6/-1.2 and NH = (7 +6/-4)x10^21 cm^-2, compared to the \nGalctic value of 6.67x10^20 cm^-2. It is not possible to determine whether \nthis source is fading given the current statistics.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 8319,
  "createdOn": 1223076693000,
  "email": "kpa@star.le.ac.uk",
  "subject": "GRB 081003A: Swift-XRT Team position and analysis",
  "submitter": "Kim Page at U.of Leicester  <kpa@star.le.ac.uk>",
  "eventId": "GRB 081003A"
}