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arXiv · 0804.4252

Autocorrelation Function for Radio Galaxies

Wlodzimierz Godlowski
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Abstract

We discuss the autocorrelation function $/zeta (r)$ for the sample 1157 radio-identified galaxies . The sample of galaxies is based on the Las Campanas Redshift Survey (LCRS) and 1.4 Ghz NRA)-VLA Sky Survey (NVSS) catalog of the radio sources. For separation $2-15h^{-1}$ Mpc autocorrelation function $/zeta (r)$$γ(s)$ can be approximated by the power law with correlation length and slope $-γ(s)=-1.8$. There are no clearly differences for correlation length between AGN and SB galaxies while value $γ$ for both samples are different: $γ=2.4$ for AGN and $γ=1.7$ for SB.

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Wlodzimierz Godlowski. 2008-04-26. Autocorrelation Function for Radio Galaxies. https://arxiv.org/abs/0804.4252

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