Deep Extragalactic VIsible Legacy Survey (DEVILS): identification of AGN through SED fitting and the evolution of the bolometric AGN luminosity function

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....

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Bibliographic Details
Main Authors:	Thorne, JE, Robotham, ASG, Davies, LJM, Bellstedt, S, Brown, MJI, Croom, SM, Delvecchio, I, Groves, B, Jarvis, MJ, Shabala, SS, Seymour, N, Whittam, IH, Bravo, M, Cook, RHW, Driver, SP, Holwerda, B, Phillipps, S, Siudek, M
Format:	Journal article
Language:	English
Published:	Oxford University Press 2021

Deep Extragalactic VIsible Legacy Survey (DEVILS): identification of AGN through SED fitting and the evolution of the bolometric AGN luminosity function

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