The distribution of faint galaxies in a field of 15 square degrees near the South Galactic Pole

Details The distribution of faint galaxies in a field of 15 square degrees near the South Galactic Pole The distribution of faint galaxies in a field of 15 square degrees near the South Galactic Pole

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.193....1m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 193, Oct. 1980, p. 1-6.

Astronomy and Astrophysics

Astronomy

14

Galaxies, Spatial Distribution, Astronomical Maps, Data Reduction, Galactic Clusters, Tables (Data)

Scientific paper

Measurements made with the Cosmos machine on a deep photograph taken with the UK Schmidt Telescope have been used to examine the distribution of galaxies down to B of approximately 22.0 in a field of 15 sq deg near the South Galactic Pole. The mean multiplicity of galaxies is 3.6, in good agreement with analyses of the Lick and Jagellonian galaxy counts, indicating no strong evolutionary effect in the clustering of galaxies at least out to redshifts of 0.4-0.7.

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