Measuring inhomogeneities in galaxy distributions on very large scales.

Details Measuring inhomogeneities in galaxy distributions on very large scales. Measuring inhomogeneities in galaxy distributions on very large scales.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sucg.conf...25s&link_type=abstract

Workshop on Studying the Universe with Clusters of Galaxies, p. 25 - 36

Mathematics

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Galaxy Distribution: Universe, Large-Scale Structure: Universe, Redshift Surveys: Universe

Scientific paper

Problems of measuring fluctuations of comoving galaxy number densities on scales ≫50 h-1Mpc (h = H0/(100 km sec-1Mpc-1) are discussed. The accuracy depends on the size of the survey volume, on the adopted magnitude corrections for K-effect and evolution, and on the decelaration parameter q0. The value of the cosmological constant is assumed to be zero. Preliminary results from subsamples of 0.9 million low resolution galaxy redshift obtained in the Münster Redshift Project are given.

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