TITLE: GCN CIRCULAR NUMBER: 22902 SUBJECT: GRB 180705A: Swift detection of a burst DATE: 18/07/05 15:55:08 GMT FROM: Scott Barthelmy at NASA/GSFC M. Stamatikos (OSU/NASA/GSFC), S. D. Barthelmy (GSFC), A. A. Breeveld (UCL-MSSL), A. D'Ai (INAF-IASFPA), V. D'Elia (ASDC), A. Deich (PSU), S. W. K Emery (UCL-MSSL), J.D. Gropp (PSU), J. A. Kennea (PSU), N. P. M. Kuin (UCL-MSSL), F. E. Marshall (NASA/GSFC), D. M. Palmer (LANL), B. Sbarufatti (PSU) and M. H. Siegel (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 15:41:14 UT, the Swift Burst Alert Telescope (BAT) triggered and located GRB 180705A (trigger=846299). Swift did not slew due to an observing constraint. The BAT on-board calculated location is RA, Dec 212.594, -11.630, which is RA(J2000) = 14h 10m 23s Dec(J2000) = -11d 37' 48" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). As is typical for image triggers, the real-time light curve does not show anything significant. The image trigger significance is 7.8 sigma, therefore we have high confidence in this event. Due to an observing constraint, Swift will not slew until T0+54 minutes. There will be no XRT or UVOT data until this time. Burst Advocate for this burst is M. Stamatikos (Michael.Stamatikos-1 AT nasa.gov). 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.)