TITLE: GCN GRB OBSERVATION REPORT NUMBER: 5502 SUBJECT: GRB 060904: Swift detection of a bright burst DATE: 06/09/04 01:21:19 GMT FROM: Scott Barthelmy at NASA/GSFC D. Grupe (PSU), S. D. Barthelmy (GSFC), D. N. Burrows (PSU), M. M. Chester (PSU), N. Gehrels (NASA/GSFC), S. T. Holland (GSFC/USRA), S. D. Hunsberger (PSU), J. A. Kennea (PSU), H. A. Krimm (GSFC/USRA), C. B. Markwardt (GSFC/UMD), F. E. Marshall (NASA/GSFC), D. M. Palmer (LANL), M. Stamatikos (NASA/ORAU) and M. C. Stroh (PSU) report on behalf of the Swift Team: At 01:03:21 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 060904 (trigger=227996). Swift slewed immediately to the burst. The BAT on-board calculated location is RA,Dec 237.743, +44.966 {15h 50m 58s, +44d 57' 57"} (J2000) with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows 3 little peaks starting out and then a large peak at T+55 sec and a total burst duration of about 85 sec. The peak count rate was ~9000 counts/sec (15-350 keV), at ~55 sec after the trigger. The XRT began observing the field at 01:04:27 UT, 66 seconds after the BAT trigger. XRT found a bright, fading, uncatalogued X-ray source located at RA(J2000) = 15h 50m 54.9s, Dec(J2000) = +44d 59' 07.8", with an estimated uncertainty of 5.4 arcseconds (90% confidence radius). This location is 79 arcseconds from the BAT on-board position, within the BAT error circle. The initial flux in the 0.1s image was 2.7e-08 erg/cm2/s (0.2-10 keV). UVOT took a finding chart exposure of 100 seconds with the White (160-650 nm) filter starting 75 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 typical 3-sigma upper limit has been about 18.5 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 0.02.