An extension of the galaxy covariance function to small scales

Details An extension of the galaxy covariance function to small scales An extension of the galaxy covariance function to small scales

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...232l..79g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 232, Sept. 1, 1979, p. L79-L81.

Astronomy and Astrophysics

Astrophysics

40

Cosmology, Galactic Clusters, Galactic Evolution, Astronomical Models, Covariance

Scientific paper

The description of galaxy clustering by the galaxy covariance function, used by Totsuji and Kihara (1969) and by Peebles (1974), has provided deeper insight into the nature and origin of large-scale inhomogeneities in the universe. In the present paper, accurate measurements of the angular separation of pairs of galaxies are used to extend the measured range of the galaxy angular covariance function to scales nearly ten times smaller than those previously examined.

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