Williams, PeterBerger, Edo2017-03-032016Williams, P. K. G., and E. Berger. 2016. No Precise Localization for Frb 150418: Claimed Radio Transient Is Agn Variability. The Astrophysical Journal 821, no. 2: L22. doi:10.3847/2041-8205/821/2/l22.2041-8213http://nrs.harvard.edu/urn-3:HUL.InstRepos:30510187Keane et al. have recently claimed to have obtained the first precise localization for a Fast Radio Burst (FRB) thanks to the identification of a contemporaneous fading slow (∼week-timescale) radio transient. They use this localization to pinpoint the FRB to a galaxy at z ≈ 0.49 that exhibits no discernible star formation activity. We argue that the transient is not genuine and that the host candidate, WISE J071634.59−190039.2, is instead a radio variable: the available data did not exclude this possibility; a random radio variable consistent with the observations is not unlikely to have a redshift compatible with the FRB dispersion measure; and the proposed transient light curve is better explained as a scintillating steady source, perhaps also showing an active galactic nucleus (AGN) flare, than a synchrotron-emitting blastwave. The radio luminosity of the host candidate implies that it is an AGN and we present new late-time Very Large Array observations showing that the galaxy is indeed variable at a level consistent with the claimed transient. Therefore the claimed precise localization and redshift determination for FRB 150418 cannot be justified.en-USgalaxies: activeintergalactic mediumradio continuum: generalscatteringJournal Article2017-03-0310.3847/2041-8205/821/2/l22