Investigating the Candidate Displaced Active Galactic Nucleus in NGC 3115

The nearby galaxy NGC 3115 contains a known radio-emitting, low-luminosity active galactic nucleus (AGN), and was recently claimed to host a candidate AGN displaced 14.3 pc from the galaxy's optical photocenter. Our goal is to understand whether this represents a single offset AGN, an AGN in orbit around a central black hole, or something else. We present a new, sensitive (rms = 4.4 mu Jy beam(-1)) 10 GHz image, which finds evidence for only one AGN. We place a stringent limit on the radio luminosity of any secondary supermassive black hole of L-10 (GHz) < 5.8 x 10(33 )erg s(-1). An analysis of the relative positioning of the radio core, X-ray nucleus, and stellar bulge in this galaxy indicate that the radio source is centrally located, and not offset from the galactic bulge. This provides an argument against a single offset AGN in NGC 3115; however, it does not provide conclusive evidence against the purported offset AGN as an inspiralling secondary black hole.