GCN Circular 29138
S. D. Barthelmy (GSFC), A. Y. Lien (GSFC/UMBC) and K. L. Page (U Leicester) report on behalf of the Neil Gehrels Swift Observatory Team: Using the full data set from recent downlinks, we report further ground data analysis for Swift trigger 1014012 (Page et al. GCN Circ. 29106). The BAT analysis uses data from T-239 to T+963 sec. The BAT image significance has now decreased to 5.2 sigma (15-350 keV). Also, the mask-weighted light curve does not show anything significant. There is no good evidence for an X-ray source in 4.7 ks data, to a 3 sigma upper limit of 2.3x10^-3 count s^-1 (corresponding to an observed flux of 1x10^-13 erg cm^-2 s^-1, assuming a typical power-law spectrum). We therefore conclude that this event is likely due to noise, and is not an astrophysical event.