{
  "bibcode": "2014GCN.16041....1B",
  "body": "S. D. Barthelmy (GSFC), N. Gehrels (NASA/GSFC), J. A. Kennea (PSU) and\nD. M. Palmer (LANL) report on behalf of the Swift Team:\n\nAt 15:18:44 UT, the Swift Burst Alert Telescope (BAT) triggered and\nlocated a peak consistent with the flare star UV Cet (trigger=593744). \nSwift could not slew to the location due to the Sun constraint. \nThe BAT on-board calculated location is \nRA, Dec 24.764, -17.961, which is \n   RA(J2000)  =  01h 39m 03s\n   Dec(J2000) = -17d 57' 40\"\nwith an uncertainty of 3 arcmin (radius, 90% containment, including \nsystematic uncertainty).  The BAT light curve showed no obvious\nactivity, as is typical for a 64 second image trigger. \n\nBecause of the Sun constraint, Swift will not be able to observe\nthis source with the XRT and UVOT at this time. \n\nAlthough the image peak was of marginal significance (6.28 sigma)\nthe close proximity to the known source location (0.013 degrees) and its\nstatus as a flare star make it highly likely that this is\na real astrophysical event.",
  "circularId": 16041,
  "createdOn": 1396119269000,
  "email": "scott@milkyway.gsfc.nasa.gov",
  "subject": "Swift trigger 593744: detection of a flare from UV Cet",
  "submitter": "Scott Barthelmy at NASA/GSFC  <scott@milkyway.gsfc.nasa.gov>"
}