Large sky area redshift surveys of galaxies.

Details Large sky area redshift surveys of galaxies. Large sky area redshift surveys of galaxies.

Jun 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pabei..16..150c&link_type=abstract

Prog. Astron., Vol. 16, No. 2, p. 150 - 157

Mathematics

Logic

Redshift Surveys: Galaxies, Universe: Large-Scale Structure

Scientific paper

This paper briefly introduces the present and future large sky area redshift surveys of galaxies, which are the fundamental work for observational cosmology. Many key problems about large scale structure, such as the topological characters and the largest scale of the structure in the universe and many basic properties of density and velocity fields as well, depend on the sky coverage and deepness of complete samples of redshift surveys of galaxies. Particularly, the authors analyze and compare the sky coverage, magnitude limit, criteria of selected sample, sampling rate and so on of the newly finished redshift surveys: IRAS, CfA, SSRS, ORS, LCRS. The proposed 2dF and SDSS surveys have also been discussed.

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