TITLE: GCN CIRCULAR NUMBER: 26595 SUBJECT: GRB 191227A: Swift detection of a burst DATE: 19/12/27 01:52:07 GMT FROM: Amy Lien at GSFC A. Melandri (INAF-OAB), S. D. Barthelmy (GSFC), M. G. Bernardini (INAF-OAB), N. J. Klingler (PSU), S Laha (GSFC/UMBC/CRESST), A. Y. Lien (GSFC/UMBC) and M. J. Moss (GWU) report on behalf of the Neil Gehrels Swift Observatory Team: At 01:39:37 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 191227A (trigger=946344). Swift did not slew immediately due to an observing constraint. The BAT on-board calculated location is RA, Dec 319.170, -16.704 which is RA(J2000) = 21h 16m 41s Dec(J2000) = -16d 42' 15" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a multi-peaked structure with a duration of about 30 sec. The peak count rate was ~12000 counts/sec (15-350 keV), at ~3 sec after the trigger. Due to a Sun observing constraint, Swift cannot slew to the BAT position until 15:10 UT on 2020 March 23. There will thus be no XRT or UVOT data for this trigger before this time. Burst Advocate for this burst is A. Melandri (andrea.melandri AT brera.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/)