The evolution of the correlation function of early type galaxies.

Details The evolution of the correlation function of early type galaxies. The evolution of the correlation function of early type galaxies.

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apl%26c..36..327i&link_type=abstract

Astrophysical Letters and Communications, Vol. 36, Nos. 1 - 6, p. 327 - 332

Astronomy and Astrophysics

Astrophysics

1

Galaxy Clustering: Correlation Analysis, Galaxy Clustering: Cosmology

Scientific paper

The authors report the results of a study of the evolution of the galaxy correlation function using a sample of distant early type galaxies (z ≡ 0.4), selected by color criteria from Schmidt plates. The goal of this work is to distinguish between different theories for the growth of large-scale structure with cosmic time. The authors compare their measurement of the correlation function ξ(r) at z ≡ 0.4 with the value found locally, estimated from an analysis of the Perseus-Pisces and the CfA redshift surveys.

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