AGN Population and Luminosity Function in the Sloan Digital Sky

Details AGN Population and Luminosity Function in the Sloan Digital Sky AGN Population and Luminosity Function in the Sloan Digital Sky

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..311..445h&link_type=abstract

AGN Physics with the Sloan Digital Sky Survey, Proceedings of a conference held in Princeton, NJ, USA, 27-31 July 2003, Edited b

Physics

Scientific paper

From the Sloan Digital Sky Survey (SDSS) spectroscopic data, we have compiled a large low-redshift active galactic nuclei (AGN) sample including 1,543 broad-line and 3,035 narrow-line AGN. We measure and compare the emission line luminosity functions of Seyfert 1s and Seyfert 2s and show that the relative number of the two types of AGN is a function of luminosity. We demonstrate that the AGN nuclear luminosity is independent of the host galaxy luminosity.

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