The APM cluster-galaxy cross-correlation function : Constraints on Omega and galaxy bias
(abridged) We estimate the cluster-galaxy cross-correlation function (Xi_cg), from the APM galaxy and galaxy cluster surveys, both in real space from the inversion of projected statistics and in redshift space using the galaxy and cluster redshift samples. The amplitude of Xi_cg is found to be almos...
Main Authors: | , , |
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Format: | Journal article |
Language: | English |
Published: |
1998
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