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Clustering in redshift space: Linear theory
Saleem Zaroubi
, Yehuda Hoffman
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Keyphrases
All-sky Survey
50%
Anisotropy
50%
Biasing Parameter
50%
Cold Dark Matter Model
50%
Covariance Matrix
50%
Explicit Dependence
50%
First-order
50%
Fourier Space
100%
Full Covariance Matrix
50%
Galaxies
50%
Galaxy Distribution
50%
Gravitational Instability
50%
Line-of-sight
50%
Linear Calculation
50%
Linear Theory
100%
Mode Coupling
50%
Peculiar Velocity
50%
Real Space
100%
Small-angle Approximation
50%
Physics
Anisotropy
50%
Cold Dark Matter
50%
Coupled Mode
50%
Covariance
100%
Dark Matter Model
50%
Galaxy Distribution
50%
Gravitational Instability
50%
Line of Sight
50%
Sky Surveys
50%