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We combine the Herschel Space Observatory PACS and SPIRE photometry witharchival WISE photometry to construct the spectral energy distributions (SED)for over 300 local ($z < 0.05$), ultra-hard X-ray (14 - 195 keV) selectedactive galactic nuclei (AGN) from the Swift Burst Alert Telescope (BAT) 58month catalogue. Using a simple analytical model that combines an exponentiallycut-off powerlaw with a single temperature modified blackbody, we decompose theSEDs into a host-galaxy and AGN component. We calculate dust masses, dusttemperatures, and star-formation rates (SFR) for our entire sample and comparethem to a stellar mass-matched sample of local non-AGN galaxies. We find AGNhost galaxies have systematically higher dust masses, dust temperatures, andSFRs due to the higher prevalence of late-type galaxies to host an AGN, inagreement with previous studies of the Swift/BAT AGN. We provide a scaling toconvert X-ray luminosities into 8 - 1000 $\mu$m AGN luminosities, as well asdetermine the best mid-to-far IR colors for identifying AGN dominated galaxiesin the IR regime. We find that for nearly 30 per cent of our sample, the 70$\mu$m emission contains a significant contribution from the AGN ($> 0.5$),especially at higher luminosities ($L_{14-195\,\rm{keV}} > 10^{42.5}$ ergss$^{-1}$). Finally, we measure the local SFR-AGN luminosity relationship,finding a slope of 0.18, large scatter (0.37 dex), and no evidence for anupturn at high AGN luminosity. We conclude with a discussion on theimplications of our results within the context of galaxy evolution with andwithout AGN feedback.

monthly notices of the royal astronomical society

Herschel far-infrared photometry of the Swift Burst Alert Telescope  active galactic nuclei sample of the local universe - III. Global  star-forming properties and the lack of a connection to nuclear activity