TITLE: GCN CIRCULAR NUMBER: 19126 SUBJECT: GRB 160303A: Swift detection of a burst, possibly short DATE: 16/03/03 11:14:26 GMT FROM: David Palmer at LANL A. P. Beardmore (U Leicester), D. N. Burrows (PSU), P.A. Evans (U Leicester), L. M. McCauley (PSU), K. L. Page (U Leicester) and D. M. Palmer (LANL) report on behalf of the Swift Team: At 10:54:42 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 160303A (trigger=677495). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 168.681, +22.742 which is RA(J2000) = 11h 14m 44s Dec(J2000) = +22d 44' 33" 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 0.5 s sec. There is some suggestion of additional peaks at T-1 and T+5. The peak count rate was ~6000 counts/sec (15-350 keV), at ~0.1 sec after the trigger. The XRT began observing the field at 10:56:26.1 UT, 104.1 seconds after the BAT trigger. Using promptly downlinked data we find a fading, uncatalogued X-ray source with an enhanced position: RA, Dec 168.7005, 22.7424 which is equivalent to: RA(J2000) = 11h 14m 48.11s Dec(J2000) = +22d 44' 32.5" with an uncertainty of 2.2 arcseconds (radius, 90% containment). This location is 64 arcseconds from the BAT onboard position, within the BAT error circle. This position may be improved as more data are received; the latest position is available at http://www.swift.ac.uk/sper. A power-law fit to a spectrum formed from promptly downlinked event data gives a column density consistent with the Galactic value of 1.07 x 10^20 cm^-2 (Willingale et al. 2013). UVOT took a finding chart exposure of 150 seconds with the White filter starting 108 seconds after the BAT trigger. No credible 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 19.6 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. 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.)