Type 1 AGN SEDs in COSMOS

Details Type 1 AGN SEDs in COSMOS Type 1 AGN SEDs in COSMOS

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009cfdd.confe.115h&link_type=abstract

Chandra's First Decade of Discovery, Proceedings of the conference held 22-25 September, 2009 in Boston, MA. Edited by Scott Wo

Mathematics

Logic

Agn Evolution

Scientific paper

A detailed study of the evolution of the Spectral Energy Distribution (SED) shapes near 1μ m of 324 Type 1 AGNs in the wide-field ``Cosmological Evolution Survey'' (COSMOS) as a function of luminosity, redshift and Eddington ratio is presented. We study the mean SEDs in redshift bins and bolometric luminosity bins and compare them with Elvis et al. 1994 Type 1 AGN mean SED (E94). We also study the position of our sources in the slope plot relative to the quasar-host galaxy mixing curve and dust reddening curve. We found that E94 is remarkably good in describing the SED shape near 1μ m even for high luminosity, redshift and Eddington ratio Type 1 AGNs. We also show examples of some outliers which might be AGNs in different evolution stages compared to normal AGNs.

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