Key points are not available for this paper at this time.
We use an all-sky sample of radio galaxies at redshifts z ≲ 0. 1 to study clustering in the Universe on scales up to several hundred Mpc. The two-point correlation function for these galaxies is consistent with their high optical luminosity and location in moderately rich environments: | (r) (r/11\, h^-1\, Mpc) ^-1. 8, \, where\, h H₀/100\, km s^-1\, Mpc^-1. |
Peacock et al. (1991) studied this question.