TITLE: GCN GRB OBSERVATION REPORT NUMBER: 4361 SUBJECT: Swift-BAT discovery of hard x-ray transient SWIFT J1626.6-5156 DATE: 05/12/18 19:55:18 GMT FROM: Scott Barthelmy at NASA/GSFC H. Krimm (GSFC/USRA), S. Barthelmy (GSFC), M. Capalbi (ASDC), N. Gehrels (GSFC), C. Gronwall (PSU), D. Palmer (LANL) on behalf of the Swift team: At 19:06:48 UT, Swift-BAT triggered and located a hard x-ray transient which we name SWIFT J1626.6-5156 (trigger=173321). The spacecraft did not slew because of the Sun observing constraint (Sun distance 32 deg). The BAT on-board calculated location is RA,Dec 246.657d,-51.937d {16h 26m 38s,-51d 56' 13"} (J2000), with an uncertainty of 3 arcmin (radius, 90% containment, stat+sys). We note that (a) this is close to the galactic center (lon=333, lat=-2), (b) the image significance is a strong 8.2 sigma, and (c) BAT has detected emission from this location multiple times within the last 24 hours. We therefore conclude that this is a hard x-ray transient, and not a GRB. The full Malindi data set in ~5 hours will likely provide the final determination of the nature of this event.