Review for "Supermassive Black Holes in the Distant
Universe", Ed. A. J. Barger, Kluwer Academic Publishers.
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astro-ph/0403618
Abstract. We review the continuum emission of Active Galactic Nuclei (AGN) over the entire electromagnetic spectrum. After a brief historical introduction, we describe the main spectral properties of unobscured AGN, discussing the selection biases which prevent us from having a complete view of the AGN population in the universe, and trying to build an updated spectral energy distribution of optically selected quasars. In the second part of the review, we describe the spectral properties of obscured AGN. Finally, we discuss the main observational methods in the different wavelength bands for disentangling AGN and stellar emission, and the ability of these methods to find new (mainly obscured) AGN, a significant fraction of which are probably still missing in current surveys.
Table of Contents
INTRODUCTION
SPECTRAL PROPERTIES OF QUASARS
Optical/UV
Radio/submillimeter
Infrared
X-rays
Bolometric Corrections
Luminosity and Redshift Effects
Intrinsic Dispersion
SEDs OF OBSCURED AGN
Radio/IR
Near-IR/UV
X-rays
Relation between Dust and Gas Absorption
FINDING OBSCURED AGN IN THE UNIVERSE
Indicators for (Local) AGN and Starbursts
Limitations
SUMMARY
REFERENCES