  The combination of the AKARI and WISE infrared all-sky surveys provides an
unique opportunity to identify and characterize the most highly dust obscured
AGNs in the universe. Dust-obscured AGNs are not easily detectable and
potentially underrepresented in extragalactic surveys due to their high optical
extinction, but are readily found in the WISE catalog due to their extremely
red mid-IR colors. Combining these surveys with photometry from Pan-STARRS and
Herschel, we use SED modeling to characterize the extinction and dust
properties of these AGNs. From mid-IR WISE colors, we are able to compute
bolometric corrections to AGN luminosities. Using AKARI's far-IR wavelength
photometry and broadband AGN/galaxy spectral templates, we estimate AGN dust
mass and temperature using simple analytic models with 3-4 parameters. Even
without spectroscopic data, we can determine a number of AGN dust properties
only using SED analysis. These methods, combined with the abundance of archival
photometric data publically available, will be valuable for large-scale studies
of dusty, IR-luminous AGNs.
