Autocorrelation Function for Radio Galaxies
| dc.creator | Godlowski, Wlodzimierz | |
| dc.date | 2008-04-26 | |
| dc.date.accessioned | 2026-07-07T09:35:32Z | |
| dc.date.available | 2026-07-07T09:35:32Z | |
| dc.description | 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. | |
| dc.description | 7pages, 5 figures accepted in : "Problems of Practical Cosmology" PPC08, St. Petersburg 2008 | |
| dc.identifier | https://arxiv.org/abs/0804.4252 | |
| dc.identifier | http://arxiv.org/abs/0804.4252 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/159860 | |
| dc.subject | Astrophysics | |
| dc.title | Autocorrelation Function for Radio Galaxies | |
| dc.type | text |