TITLE: GCN CIRCULAR NUMBER: 19967 SUBJECT: GRB 161001A: Swift detection of a burst DATE: 16/10/01 01:15:39 GMT FROM: David Palmer at LANL K. L. Page (U Leicester), A. Y. Lien (GSFC/UMBC), F. E. Marshall (NASA/GSFC), D. M. Palmer (LANL) and M. H. Siegel (PSU) report on behalf of the Swift Team: At 01:05:16 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 161001A (trigger=714404). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 71.913, -57.283 which is RA(J2000) = 04h 47m 39s Dec(J2000) = -57d 16' 57" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a complex structure with a duration of about 3 sec. The peak count rate was ~11000 counts/sec (15-350 keV), at ~1 sec after the trigger. The XRT began observing the field at 01:06:21.5 UT, 65.0 seconds after the BAT trigger. Using promptly downlinked data we find an uncatalogued X-ray source located at RA, Dec 71.91848, -57.26127 which is equivalent to: RA(J2000) = 04h 47m 40.44s Dec(J2000) = -57d 15' 40.6" with an uncertainty of 3.9 arcseconds (radius, 90% containment). This location is 78 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. We cannot determine whether the source is fading at the present time. No spectrum from the promptly downlinked event data is yet available to determine the column density. UVOT took a finding chart exposure of 150 seconds with the White filter starting 68 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 0.01. Burst Advocate for this burst is K. L. Page (klp5 AT leicester.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.)