Angular Correlation Function of Quasars from SDSS DR3

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dc.creatorIvashchenko, G. Yu.
dc.creatorZhdanov, V. I.
dc.date2006-06-04
dc.date2006-09-15
dc.date.accessioned2026-07-07T07:12:07Z
dc.date.available2026-07-07T07:12:07Z
dc.descriptionWe estimate the two-point angular correlation function (CF) of quasars from SDSS DR3 using a special method of comparison random catalog generation. The best-fit value for the CF power-law index is found to be $α=0.78\pm0.18$ on the $2<θ<250$ $arcmin$ interval. This is lower (though in marginal agreement) than earlier result of \markcite{{\it Myers et al.} (2005)} based on SDSS DR1 catalogue of photometrically-classified quasars.
dc.description4 pages, 1 figure. Accepted for publication in WDS'06 Proceedings of Contributed Papers
dc.identifierhttps://arxiv.org/abs/astro-ph/0606074
dc.identifierhttp://arxiv.org/abs/astro-ph/0606074
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/111972
dc.subjectAstrophysics
dc.titleAngular Correlation Function of Quasars from SDSS DR3
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