TITLE: GCN CIRCULAR NUMBER: 17686 SUBJECT: Swift detection of SAX J1808.4-3658 DATE: 15/04/11 19:57:28 GMT FROM: David Palmer at LANL D. Malesani (DARK/NBI), D. M. Palmer (LANL) and T. N. Ukwatta (LANL) report on behalf of the Swift Team: At 19:36:25 UT, the Swift Burst Alert Telescope (BAT) triggered and located a burst from SAX J1808.4-3658 (trigger=637765). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 272.073, -36.974 which is RA(J2000) = 18h 08m 18s Dec(J2000) = -36d 58' 27" 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 20 sec. The peak count rate was ~2400 counts/sec (15-350 keV), at ~6 sec after the trigger. The XRT began observing the field at 19:37:11.2 UT, 46.1 seconds after the BAT trigger. XRT found a bright X-ray source located at RA, Dec 272.1135, -36.9774 which is equivalent to: RA(J2000) = +18h 08m 27.24s Dec(J2000) = -36d 58' 38.6" with an uncertainty of 4.8 arcseconds (radius, 90% containment). This location is 117 arcseconds from the BAT onboard position, within the BAT error circle. This position is 6.7 arcseconds from a known X-ray source: SAX J1808.4-3658. This source is in the Swift XRT 1SXPS catalogue with a mean 0.3-10 keV count-rate of 0.3550 +/- 0.0038 ct/sec; see http://www.swift.ac.uk/1SXPS/1SXPSJ180827.6-365843 for details of these previous observations. No event data are yet available to determine the column density using X-ray spectroscopy. The initial flux in the 2.5 s image was 6.62e-09 erg cm^-2 s^-1 (0.2-10 keV). UVOT took a finding chart exposure of 150 seconds with the White filter starting 54 seconds after the BAT trigger. The source is clearly visible in the UVOT image, but the crowded field prevents automatic estimation of its brightness at this time. This source is currently in outburst (Sanna et al., ATel 7364). Its BAT lightcurve is given at http://swift.gsfc.nasa.gov/results/transients/weak/SAXJ1808.4-3658/