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We present far-infrared (FIR) and submillimeter photometry from the HerschelSpace Observatory's Spectral and Photometric Imaging Receiver (SPIRE) for 313nearby z<0.05 active galactic nuclei (AGN). We selected AGN from the 58 monthSwift Burst Alert Telescope (BAT) catalog, the result of an all-sky survey inthe 14-195 keV energy band, allowing for a reduction in AGN selection effectsdue to obscuration and host galaxy contamination. We find 46% (143/313) of oursample is detected at all three wavebands and combined with our PACSobservations represents the most complete FIR spectral energy distributions oflocal, moderate luminosity AGN. We find no correlation between the 250, 350,and 500 micron luminosities with 14-195 keV luminosity, indicating the bulk ofthe FIR emission is not related to the AGN. However, Seyfert 1s do show a veryweak correlation with X-ray luminosity compared to Seyfert 2s and we discusspossible explanations. We compare the SPIRE colors (F250/F350 and F350/F500) toa sample of normal star-forming galaxies, finding the two samples arestatistically similar, especially after matching in stellar mass. But acolor-color plot reveals a fraction of the Herschel-BAT AGN are displaced fromthe normal star-forming galaxies due to excess 500 micron emission E500). Ouranalysis shows E500 is strongly correlated with the 14-195 keV luminosity and3.4/4.6 micron flux ratio, evidence the excess is related to the AGN. Wespeculate these sources are experiencing millimeter excess emission originatingin the corona of the accretion disk.

Herschel Far-Infrared Photometry of the Swift Burst Alert Telescope Active Galactic Nuclei Sample of the Local Universe. II. SPIRE Observations