Journal of Physical Studies 12(3), Article 3902 [7 pages] (2008)
DOI: https://doi.org/10.30970/jps.12.3902

LUMINOSITY DEPENDENCE OF THE QUASAR CLUSTERING FROM SDSS DR5

G. Ivashchenko

Kyiv National Taras Shevchenko University,
2, Glushkova ave.,Kyiv, 03127, Ukraine
email: hanna@univ.kiev.ua

43024 objects which were primarily identified as quasars in SDSS DR5 and have spectroscopic redshifts were used to study the luminosity dependence of the quasar clustering with the help of two different techniques. The obtained results reveal that brighter quasars are more clustered, but this dependence is weak, which is in agreement with the results by Porciani \& Norberg [C. Porciani, P. Norberg, Mon. Notic. Roy. Astron. Soc. \textbf{371}, 1824 (2006)] and theoretical predictions made by Lidz {\em et al.} [A. Lidz, {\em et al.}, Astrophys J. \textbf{641}, 41 (2006)].

PACS number(s): 98.65.Aj, 98.54.-h, 98.62.Ve

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