To appear in the proceedings of IAU Colloquium #184 "AGN Surveys" held at the Byurakan Observatory, Armenia in June 2001.
astro-ph/0201118

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SPECTROSCOPIC DIAGNOSTICS FOR AGNs

Sylvain Veilleux


Department of Astronomy, University of Maryland, College Park, MD 20742


Abstract. A review of the spectroscopic tools needed to characterize AGNs is presented. This review focusses on ultraviolet, optical and infrared emission-line diagnostics specifically designed to help differentiate AGNs from starburst-dominated galaxies. The strengths and weaknesses of these methods are discussed in the context of on-going and future AGN surveys.


Table of Contents

INTRODUCTION

BASIC PRINCIPLES

ULTRAVIOLET EMISSION-LINE DIAGNOSTICS

OPTICAL EMISSION-LINE DIAGNOSTICS

NEAR-INFRARED EMISSION-LINE DIAGNOSTICS

MID-TO-FAR INFRARED EMISSION-LINE DIAGNOSTICS

COMPLICATIONS
Contribution from Shocks
Aperture Effects
Morphological Biases
Metallicity Effects

SUMMARY

REFERENCES

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