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43024 objects, which were primarily identified as quasars in SDSS DR5 andhave spectroscopic redshifts were used to study the luminosity dependence ofthe quasar clustering with the help of two different techniques. The obtainedresults reveal that brighter quasars are more clustered, but this dependence isweak, which is in agreement with the results by Porciani & Norberg, 2006 andtheoretical predictions by Lidz et al., 2006.

Luminosity Dependence of the Quasar Clustering from SDSS DR5