TITLE: GCN CIRCULAR NUMBER: 8344 SUBJECT: GRB 081008: Swift detection of a burst with optical afterglow DATE: 08/10/08 20:12:50 GMT FROM: Jamie A. Kennea at PSU/Swift-XRT J. L. Racusin (PSU), W. H. Baumgartner (GSFC/UMBC), P. J. Brown (PSU), D. N. Burrows (PSU), P. A. Evans (U Leicester), D. Grupe (PSU), S. T. Holland (CRESST/USRA/GSFC), E. A. Hoversten (PSU), J. A. Kennea (PSU), V. La Parola (INAF-IASFPA), F. E. Marshall (NASA/GSFC), P. T. O'Brien (U Leicester), J. P. Osborne (U Leicester), A. M. Parsons (GSFC), M. Stamatikos (NASA/ORAU), R. L. C. Starling (U Leicester), G. Tagliaferri (INAF-OAB), T. N. Ukwatta (GSFC/GWU) and L. Vetere (PSU) report on behalf of the Swift Team: At 19:58:09 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 081008 (trigger=331093). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 279.987, -57.464 which is RA(J2000) = 18h 39m 57s Dec(J2000) = -57d 27' 50" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a double-peaked structure with a duration of about 150 sec. The peak count rate was ~2500 counts/sec (15-350 keV), at ~0 sec after the trigger. The XRT began observing the field at 19:59:36.5 UT, 87.1 seconds after the BAT trigger. XRT found a bright, uncatalogued X-ray source located at RA, Dec 279.9587, -57.4312 which is equivalent to: RA(J2000) = 18h 39m 50.08s Dec(J2000) = -57d 25' 52.3" with an uncertainty of 5.3 arcseconds (radius, 90% containment). This location is 130 arcseconds from the BAT onboard position, within the BAT error circle. No event data are yet available to determine the column density using X-ray spectroscopy. UVOT took a finding chart exposure of 150 seconds with the White (160-650 nm) filter starting 96 seconds after the BAT trigger. There is a candidate afterglow in the rapidly available 2.7'x2.7' sub-image at RA(J2000) = 18:39:50.11 = 279.9588 DEC(J2000) = -57:25:52.3 = -57.4312 with a 1-sigma error radius of about 1.6 arc sec. This position is 0.3 arcseconds from the center of the XRT error circle. The estimated magnitude is 15.0 with a 1-sigma error of about 0.5 mag. No correction has been made for the expected extinction corresponding to E(B-V) of 0.10. Burst Advocate for this burst is J. L. Racusin (racusin AT astro.psu.edu). Please contact the BA by email if you require additional information regarding Swift followup of this burst. In extremely urgent cases, after trying the Burst Advocate, you can contact the Swift PI by phone (see Swift TOO web site for information: http://www.swift.psu.edu/too.html.)