Linear redshift distortion in galaxy survey

Details Linear redshift distortion in galaxy survey Linear redshift distortion in galaxy survey

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002pabei..20..371x&link_type=abstract

Progress in Astronomy (ISSN 1000-8349), Vol. 20, No. 4, p. 371 - 378 (2002)

Astronomy and Astrophysics

Astronomy

Large Scale Structure, Galaxies, Peculiar Velocity, Redshift Distortion

Scientific paper

The maps of galaxy distribution in the Universe obtained from the redshift survey are distorted by the peculiar velocities of galaxies. This effect, which is called redshift distortion, provides a way to investigate the matter distribution on large scale by analysing the linear redshift distortion parameter β with dynamical and statistical methods. The theory of the linear redshift distortions, the basic methods of measuring β and some new measurements are reviewed.

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