{
  "bibcode": "2005GCN..4362....1B",
  "body": "S. Barthelmy (GSFC), L. Barbier (GSFC), J. Cummings (GSFC/NRC),\nE. Fenimore (LANL), N. Gehrels (GSFC), D. Hinshaw (GSFC-SPSYS),\nD. Hullinger (GSFC/UMD), J. Kennea (PSU), H. Krimm (GSFC/USRA),\nC. Markwardt (GSFC/UMD), K. McLean (LANL), D. Palmer (LANL),\nA. Parsons (GSFC), T. Sakamoto (GSFC/NRC), G. Sato (ISAS), J. Tueller (GSFC)\non behalf of the Swift-BAT team:\n\nUsing the data from T-60 to T+120 sec from telemetry downlinks, we report\nfurther analysis of Swift-BAT hard x-ray source J1626.6-5156 (trigger 173321)\n(Krimm, et al., GCN 4361).  The ground-analysis position is\nRA,Dec 246.632,-51.945 {16h 26m 31.8s,-51d 56' 41.6\"} (J2000)\nwith an uncertainty of 2.5 arcmin (radius, 90%, stat+sys).\n\nThe partial coding fraction is 30%.  This source has been detected by BAT\n22 times in the last 24 hours.  It is higly variable ranging from 100 mCrab\nto 1500 mCrab.\n\nFitting a simple power law over the full interval from T0 to T+64 sec,\nthe photon index is 3.3 +/- 0.6 (15-150 keV band at the 90% confidence level).\n\nThis location will come out of the Swift Sun observing contraint\non 09 Jan 2005.",
  "circularId": 4362,
  "createdOn": 1135005363000,
  "email": "Scott@lheamail.gsfc.nasa.gov",
  "subject": "Refined analysis of the SWIFT J1626.6-5156",
  "submitter": "Scott Barthelmy at NASA/GSFC  <Scott@lheamail.gsfc.nasa.gov>"
}