TITLE: GCN CIRCULAR NUMBER: 20296 SUBJECT: GRB 161219B: Swift detection of a burst with an optical afterglow DATE: 16/12/19 19:07:03 GMT FROM: David Palmer at LANL A. D'Ai (INAF-IASFPA), J. A. Kennea (PSU), H. A. Krimm (CRESST/NSF/USRA), N. P. M. Kuin (UCL-MSSL), F. E. Marshall (NASA/GSFC), K. L. Page (U Leicester), D. M. Palmer (LANL), B. Sbarufatti (INAF-OAB/PSU) and M. H. Siegel (PSU) report on behalf of the Swift Team: At 18:48:39 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 161219B (trigger=727541). Swift slewed immediately to the burst. The BAT on-board calculated location is RA, Dec 91.717, -26.790 which is RA(J2000) = 06h 06m 52s Dec(J2000) = -26d 47' 23" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a single triangle- shaped structure with a duration of about 10 sec. The peak count rate was ~3900 counts/sec (15-350 keV), at ~2 sec after the trigger. The XRT began observing the field at 18:50:27.5 UT, 108.2 seconds after the BAT trigger. Using promptly downlinked data we find an uncatalogued X-ray source with an enhanced position: RA, Dec 91.7140, -26.7915 which is equivalent to: RA(J2000) = 06h 06m 51.35s Dec(J2000) = -26d 47' 29.4" with an uncertainty of 2.2 arcseconds (radius, 90% containment). This location is 11 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 in excess of the Galactic value (3.06 x 10^20 cm^-2, Willingale et al. 2013), with an excess column of 4 (+2.38/-1.96) x 10^21 cm^-2 (90% confidence). UVOT took a finding chart exposure of 150 seconds with the White filter starting 111 seconds after the BAT trigger. There is a candidate afterglow in the rapidly available 2.7'x2.7' sub-image at RA(J2000) = 06:06:51.41 = 91.71421 DEC(J2000) = -26:47:29.2 = -26.79144 with a 90%-confidence error radius of about 0.5 arc sec. This position is 0.9 arc sec. from the center of the XRT error circle. The estimated magnitude is 16.10 with a 1-sigma error of about 0.03. No correction has been made for the expected extinction corresponding to E(B-V) of 0.03. Burst Advocate for this burst is A. D'Ai (antonino.dai AT ifc.inaf.it). 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.) [GCN OPS NOTE(20dec16): Per author's request, the "-29:47:29.2" in the 4th paragraph was changed to "-26:47:29.2".]