TITLE: GCN GRB OBSERVATION REPORT NUMBER: 5409 SUBJECT: GRB 060807: Swift detection of a burst DATE: 06/08/07 15:04:49 GMT FROM: Scott Barthelmy at NASA/GSFC M. De Pasquale (UCL-MSSL), S. D. Barthelmy (GSFC), S. Campana (INAF-OAB), J. R. Cummings (NASA/UMD), O. Godet (U Leicester), C. Guidorzi (Univ Bicocca&INAF-OAB), J. E. Hill (GSFC/USRA), S. T. Holland (GSFC/USRA), J. A. Kennea (PSU), H. A. Krimm (GSFC/USRA), F. E. Marshall (NASA/GSFC), K. M. McLean (LANL/UTD), K. L. Page (U Leicester), D. M. Palmer (LANL), S. B. Pandey (UCL-MSSL), A. M. Parsons (GSFC), T. Sakamoto (NASA/ORAU) and D. E. Vanden Berk (PSU) report on behalf of the Swift Team: At 14:41:35 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 060807 (trigger=223217). Swift slewed immediately to the burst. The BAT on-board calculated location is RA,Dec 252.527, +31.590 {16h 50m 07s, +31d 35' 25"} (J2000) with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows 1, possibly 2, peaks with a duration of about 15 sec. The peak count rate was ~1000 counts/sec (15-350 keV), at ~1 sec after the trigger. The XRT began taking data at 14:43:21 UT, 106 seconds after the BAT trigger. The XRT on-board centroid algorithm did not find a source in the image, however analysis of downlinked data finds an uncatalogued, variable point source at the following location: RA(J2000): 16h 50m 02.77s, Dec(J2000) 31d 35m 31.1s with an estimated uncertainty of 4.2 arcseconds radius (90% containment). UVOT took a finding chart exposure of 100 seconds with the White (160-650 nm) filter starting 110 seconds after the BAT trigger. No afterglow candidate has been found in the initial data products. The 2.7'x2.7' sub-image covers 100% of the XRT error circle. The 3-sigma upper limit is about 19.7 mag. The 8'x8' region for the list of sources generated on-board covers 100% of the XRT 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 0.03. The Malindi telemetry downlink gap has just started, so we will not get the full data set until ~22:30 UT. [GCN OPS NOTE(07aug06): Per author's request, the affilation of S.B.Pandey was changed.]