Deep Extragalactic VIsible Legacy Survey (DEVILS): Identification of AGN through SED Fitting and the Evolution of the Bolometric AGN Luminosity Function
Jessica E. Thorne,
Aaron S. G. Robotham,
Luke J. M. Davies
et al.
Abstract:Active galactic nuclei (AGN) are typically identified through radio, mid-infrared, or X-ray emission or through the presence of broad and/or narrow emission lines. AGN can also leave an imprint on a galaxy's spectral energy distribution (SED) through the re-processing of photons by the dusty torus. Using the SED fitting code P S with an incorporated AGN component, we fit the far ultraviolet to far-infrared SEDs of ∼494,000 galaxies in the D10-COSMOS field and ∼230,000 galaxies from the GAMA survey. By combinin… Show more
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