Large-scale clustering of galaxies in the CfA Redshift Survey

Details Large-scale clustering of galaxies in the CfA Redshift Survey Large-scale clustering of galaxies in the CfA Redshift Survey

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...391l...5v&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 391, no. 1, May 20, 1992, p. L5-L8. Research supported by Smithso

Mathematics

Logic

160

Galactic Clusters, Power Spectra, Red Shift, Star Distribution, Cosmology, Spatial Distribution

Scientific paper

The power spectrum of the galaxy distribution in the Center for Astrophysics Redshift Survey (de Lapparent et al., 1986; Geller and Huchra, 1989; and Huchra et al., 1992) is measured up to wavelengths of 200/h Mpc. Results are compared with several cosmological simulations with Gaussian initial conditions. It is shown that the power spectrum of the standard CDM model is inconsistent with the observed power spectrum at the 99 percent confidence level.

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