TITLE: GCN CIRCULAR NUMBER: 5936 SUBJECT: Swift triggers (#251863) on a possible burst DATE: 06/12/18 04:33:40 GMT FROM: Scott Barthelmy at NASA/GSFC S. Zane (UCL-MSSL), S. D. Barthelmy (GSFC), D. N. Burrows (PSU), M. M. Chester (PSU), N. Gehrels (NASA/GSFC), J. A. Kennea (PSU), F. E. Marshall (NASA/GSFC), K. M. McLean (LANL/UTD), S. R. Oates (UCL-MSSL), C. Pagani (PSU), D. M. Palmer (LANL) and M. Stamatikos (NASA/ORAU) report on behalf of the Swift Team: At 04:05:05 UT, the Swift Burst Alert Telescope (BAT) triggered and located trigger=251863. Swift slewed immediately to the location. The BAT on-board calculated location is RA, Dec 149.223, -35.146 which is RA(J2000) = 09h 56m 53s Dec(J2000) = -35d 08' 45" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows a possible very weak pulse lasting about 10 sec, overlying the much stronger periodic variation of Vela X-1 in the same field. The peak count rate was ~500 counts/sec (15-350 keV), at ~1 sec before the trigger. The XRT began taking data at 04:06:51 UT, 106 seconds after the BAT trigger. The XRT on-board centroid algorithm did not find a source in the image and no prompt position is available. No source is detected in 275s of quicklook photon counting mode data. UVOT took a finding chart exposure of 100 seconds with the White (160-650 nm) filter starting 110 seconds after the BAT trigger, and a finding chart exposure of nominal 400 seconds with the V filter starting 216 seconds after the BAT trigger. No afterglow candidate has been found in the initial data products. The 2.7'x2.7' sub-image covers 25% of the BAT error circle. The typical 3-sigma upper limit has been about 18.5 mag (in White). The 8'x8' region for the list of sources generated on-board covers 100% of the BAT error circle. The list of sources is typically complete to about 18 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.125