Key points are not available for this paper at this time.
We use the Center for Astrophysics Redshift Survey, now complete to mB_ 400 h^-1^ Mpc) N-body simulations of cosmological models shows that the power spectrum of the standard CDM model (OMEGAh = 0. 5 and σ₈_ = 1; see below for definitions) is inconsistent with the observed power spectrum at the 99% confidence level. The power spectrum of an open CDM model (OMEGAh = 0. 2 and σ₈_ = 1) best approximates the observed power spectrum for wavelengths < 125 h^-1^ Mpc.
Vogeley et al. (Fri,) studied this question.