Clustering in Redshift Space: Linear Theory

Details Clustering in Redshift Space: Linear Theory Clustering in Redshift Space: Linear Theory

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apj...462...25z&link_type=abstract

Astrophysical Journal v.462, p.25

Astronomy and Astrophysics

Astronomy

41

Galaxies: Clusters: General, Galaxies: Distances And Redshifts, Cosmology: Large-Scale Structure Of Universe

Scientific paper

The clustering in redshift space is studied here to first order within the framework of gravitational instability. The distortion introduced by the peculiar velocities of galaxies results in anisotropy in the galaxy distribution and mode-mode coupling when analyzed in Fourier space. An exact linear calculation of the full covariance matrix in both real and Fourier space is presented here. The explicit dependence on {OMEGA}_0_ and the biasing parameter is calculated, and its potential use as a probe of these parameters is discussed. Kaiser's formalism, which is valid in the small-angle approximation, is extended here to the general case, including all-sky surveys. The covariance matrix in real space is calculated explicitly for the cold dark matter model, where the behavior along and perpendicular to the line of sight is shown.

Affiliated with

Also associated with

No associations

Rating

Clustering in Redshift Space: Linear Theory does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Clustering in Redshift Space: Linear Theory, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Clustering in Redshift Space: Linear Theory will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1356597