The distribution of galaxies and clusters in the APM survey

Details The distribution of galaxies and clusters in the APM survey The distribution of galaxies and clusters in the APM survey

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992daec.conf..194m&link_type=abstract

In Distribution of Matter in the Universe, 2nd DAEC mtg, ed. G.A. Mamon and D. Gerbal (Meudon: Obs. de Paris) p. 194-201

Physics

Scientific paper

This paper describes the distribution of faint galaxies in 2 steradians covering the South Galactic cap. Clustering in the distribution is quantified using the angular autocorrelation function of galaxies, wgg(theta) . The differences between w_≫(theta) measured for galaxies in different magnitude ranges are consistent with the predictions from Limbers equation.

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