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Article Contents

ABSTRACT

1.INTRODUCTION

2.THE AGN SPECTRAL ENERGY DISTRIBUTION OBSERVED

2.1.General Characteristics

2.2.Origin of the various components

3.HOW WELL DOES THE PICTURE FIT?

3.1.The Optical/UV Big Blue Bump

3.2.IR continuum

3.3.Orientation, obscuration and AGN Class

3.4.The Effects of Luminosity

3.5.Ingredients which determine the Shape of the SED

4.OUR EXPANDING VIEW OF AGN

REFERENCES