  We present analysis of spectral energy distributions (SEDs) from mid-infrared
through X-ray of a sample of 420 hard X-ray selected, z-band and Spitzer/IRAC
detected active galactic nuclei (AGN) and AGN candidates from the GOODS
multiwavelength survey. We fit local empirical SED templates of both normal and
active galaxies to the rest-frame luminosities calculated from spectroscopic
(where available) and photometric redshifts. The majority of the optically
stellar-dominated (with early-type galaxy fits) sources are moderately luminous
(L_X,2-10 keV ~ 10^43 erg/s) hard X-ray sources with high X-ray hardness ratios
(HR > 0.2), high MIR luminosities and red MIR colors in excess of a typical
stellar dominated elliptical galaxy. These sources likely harbor heavily
obscured (though Compton-thin) AGN. The observed ratio of obscured to
unobscured AGN has an integrated mean of ~3.4:1 but declines with increasing
redshift. This effect has been explained by Treister et al. (2004) as an
observational bias triggered by the lack of spectroscopic redshifts at R > 24
which are predominantly higher redshift obscured sources.
