TITLE: GCN CIRCULAR NUMBER: 6074 SUBJECT: GRB 070208: Swift detection of a burst DATE: 07/02/08 09:34:19 GMT FROM: Scott Barthelmy at NASA/GSFC G. Sato (GSFC/ISAS), S. D. Barthelmy (GSFC), S. Campana (INAF-OAB), M. L. Conciatore (ASDC), P. A. Evans (U Leicester), N. Gehrels (NASA/GSFC), C. Gronwall (PSU), C. Guidorzi (Univ Bicocca&INAF-OAB), V. Mangano (INAF-IASFPA), P. T. O'Brien (U Leicester), J. P. Osborne (U Leicester), K. L. Page (U Leicester), D. M. Palmer (LANL), P. Romano (Univ. Bicocca & INAF-OAB), G. Stratta (ASDC), G. Tagliaferri (INAF-OAB), S. D. Vergani (DIAS-DCU) and H. Ziaeepour (UCL-MSSL) report on behalf of the Swift Team: At 09:10:34 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 070208 (trigger=259714). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 197.920, +61.959 which is RA(J2000) = 13h 11m 41s Dec(J2000) = +61d 57' 31" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve shows a single peak structure with a duration of about 2 sec. The peak count rate was ~1200 counts/sec (15-350 keV), at ~0 sec after the trigger. The XRT began taking data at 09:12:29 UT, 116 seconds after the BAT trigger. XRT could not centroid onboard, however in a 222 s ground-processed image, we found a previously uncatalogued X-ray source in the field of view at the following coordinates: RA(J2000) = 13h 11m 32.77s Dec(J2000)= +61d 57' 55.17" with an uncertainty of 5 arcseconds radius (90% containment). This position lies 63 arcseconds from the center of the BAT error circle. The approximate initial flux is 1.044e-11 erg/cm2/sec (0.2-10 keV). UVOT took a finding chart exposure of 100 seconds with the White (160-650 nm) filter starting 119 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 0.01.