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The Clustering of AGN Using Photometric Redshifts
Elias Koulouridis
Antonis Georgakakis
National Observatory of Athens
Previous Results
A. Coil et al. 2009 projected cross-correlation function (wp) in AEGIS of 132 X-ray AGNs with 4669 galaxies from DEEP2 survey.
Limitations
Deep2 is a unique catalogue of spectroscopic redshifts.
Small number of X-ray AGN in AEGIS/DEEP2.
Other studies are not possible, like the study of the Luminosity dependent evolution of the AGN clustering.
Probability Density Function (PDF) of Photometric Redshifts
Binned distribution with dz=0.04 from z=0 up to z=6
Our redshift bin is ±300 h -1Mpc = 5 bins in the PDF