TITLE: GCN CIRCULAR NUMBER: 11629 SUBJECT: GRB 110205A: Swift detection of a burst with an optical candidate DATE: 11/02/05 02:17:32 GMT FROM: David Palmer at LANL A. P. Beardmore (U Leicester), W. H. Baumgartner (GSFC/UMBC), D. N. Burrows (PSU), M. M. Chester (PSU), J. M. Gelbord (PSU), S. T. Holland (CRESST/USRA/GSFC), N. P. M. Kuin (UCL-MSSL), O. M. Littlejohns (U Leicester), C. B. Markwardt (NASA/GSFC), F. E. Marshall (NASA/GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL), T. Sakamoto (NASA/UMBC), C. J. Saxton (UCL-MSSL), M. H. Siegel (PSU), E. Sonbas (GSFC/USRA/Adiyaman Univ.), M. Stamatikos (OSU/NASA/GSFC), C. A. Swenson (PSU) and T. N. Ukwatta (MSU) report on behalf of the Swift Team: At 02:02:41 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 110205A (trigger=444643). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 164.589, +67.516 which is RA(J2000) = 10h 58m 21s Dec(J2000) = +67d 30' 58" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT lightcurve shows activity with multiple peaks until at least T+300 seconds, with a peak count rate of 4500 counts/s (15-150 keV) at T+210 s. The XRT began observing the field at 02:05:16.8 UT, 155.4 seconds after the BAT trigger. XRT found a bright, uncatalogued X-ray source located at RA, Dec 164.6321, +67.5230 which is equivalent to: RA(J2000) = 10h 58m 31.70s Dec(J2000) = +67d 31' 22.7" with an uncertainty of 6.2 arcseconds (radius, 90% containment). This location is 64 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 filter starting 164 seconds after the BAT trigger. There is a candidate afterglow in the rapidly available 2.7'x2.7' sub-image at RA(J2000) = 10:58:31.12 = 164.62965 DEC(J2000) = +67:31:31.2 = 67.52532 with a 90%-confidence error radius of about 0.63 arc sec. This position is 9.0 arc sec. from the center of the XRT error circle. The estimated magnitude is 18.71 with a 1-sigma error of about 0.15. No correction has been made for the expected extinction corresponding to E(B-V) of 0.01. Burst Advocate for this burst is A. P. Beardmore (apb AT star.le.ac.uk). 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.)