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Steps toward the Power Spectrum of Matter. I. The Mean Spectrum of Galaxies
We calculate the mean power spectrum of galaxies using published power spectra of galaxies and clusters of galaxies. On small scales we use the power spectrum derived from the 2-dimensional distribution of APM galaxies, on large scales we use power spectra derived from 3-dimensional data for galaxy and cluster samples. Spectra are reduced to real space and to the amplitude of the power spectrum of APM galaxies. Available data indicate the presence of two different populations in the nearbydoi:10.1086/307384 fatcat:nhhfagpnczexzovqxv76hrh7mq