Spectral Energy Distributions (seds) of Quasars and Active Galactic Nuclei (agn)

Details Spectral Energy Distributions (seds) of Quasars and Active Galactic Nuclei (agn) Spectral Energy Distributions (seds) of Quasars and Active Galactic Nuclei (agn)

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mas..conf..262w&link_type=abstract

MULTIWAVELENGTH AGN SURVEYS. Proceedings of the Guillermo Haro Conference 2003. Held 8-12 December 2003 in Cozumel, Mexico. Edit

Astronomy and Astrophysics

Astronomy

Scientific paper

Active Galactic Nuclei (AGNa) are multiwavelength emitters. To study them, or even to determine their energy output, they must be observed with many telescopes. I will review what we have learned from broad-band observations of relatively bright, low-redshift AGN over the past ~ 15 years. AGN can be found at all wavelengths but each selection provides a different view of the intrinsic population, often with little overlap between samples. New, on-going surveys using today's new, sensitive observatories will provide an unprecendent view of the parent AGN population. They are already finding enough new and different AGN candidates to pose the observational question: "How do we know we have an AGN?".

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