TITLE: GCN CIRCULAR NUMBER: 27008 SUBJECT: Swift Trigger 954840 is not a GRB DATE: 20/02/07 03:42:44 GMT FROM: David Palmer at LANL J.D. Gropp (PSU), J. A. Kennea (PSU), N. J. Klingler (PSU), S. Laha (GSFC/UMBC/CRESST), A. Y. Lien (GSFC/UMBC), F. E. Marshall (NASA/GSFC), K. L. Page (U Leicester), B. Sbarufatti (PSU) and M. H. Siegel (PSU) report on behalf of the Neil Gehrels Swift Observatory Team: At 03:02:18 UT, the Swift Burst Alert Telescope (BAT) triggered on a rate increase and found a marginal significance peak in the image plane (trigger=954840). Swift slewed immediately to the location. The BAT on-board calculated location is RA, Dec 163.623, -49.581 which is RA(J2000) = 10h 54m 30s Dec(J2000) = -49d 34' 52" with an uncertainty of 3 arcmin (radius, 90% containment, including systematic uncertainty). The BAT light curve showed a steady rate increase due to Swift's approach and entry into the SAA. The XRT began observing the field at 03:03:44.9 UT, 86.8 seconds after the BAT trigger. No source was detected in 594 s of promptly downlinked data. UVOT took a finding chart exposure of 150 seconds with the White filter starting 1628 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 8% of the BAT 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 BAT 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 0.38. Because the BAT rate increase was due to the SAA, the image significance was marginal (6.5 sigma) and much below that implied by the rate increase, and XRT did not detect any afterglow, we believe that this trigger was a statistical fluctuation in the image plane and not an astrophysical event. The full downlinked dataset will be used to verify the nature of this trigger.