{
  "bibcode": "2022GCN.32294....1D",
  "body": "S. Dichiara (PSU), P. A. Evans (U Leicester), D. M. Palmer (LANL) and\nT. M. Parsotan (GSFC/UMBC/CRESSTII) report on behalf of the Neil\nGehrels Swift Observatory Team:\n\nAt 14:26:58 UT on 29 June 2022, the Swift Burst Alert Telescope (BAT)\ntriggered and located MAXI J0655-013 (trigger=1113743).  Swift did\nnot slew to this source as Sun constraint currently prevents the \nUVOT and XRT from pointing at this location. \nThe BAT on-board calculated location is \nRA, Dec 103.786, -1.493 which is \n   RA(J2000) = 06h 55m 09s\n   Dec(J2000) = -01d 29' 33\"\nwith an uncertainty of 3 arcmin (radius, 90% containment, including \nsystematic uncertainty).  As is usual for an image trigger, there\nis no obvious variation in the immediately available BAT lightcurve. \n\nThis source has continued to be in outburst and is continuing to\nrise, with high variability, since its earliest detection and\nidentification as a Galactic transient.  (Serino et al. ATel#15442)\n\nBAT has detected this source in its on-board imaging ~250 times, with\nan average position of ra,dec = 103.798, -1.495 (uncertainty\nless than 1 arcminute). \n\nIts history in the Swift/BAT Hard X-ray Transient Monitor is\navailable at\nhttps://swift.gsfc.nasa.gov/results/transients/weak/MAXIJ0655-013/",
  "circularId": 32294,
  "createdOn": 1656516015000,
  "email": "palmer@lanl.gov",
  "subject": "Trigger 1113743: Swift detection of MAXI J0655-013",
  "submitter": "David Palmer at LANL  <palmer@lanl.gov>"
}