Add to ORKGWe have constrained the redshift-distortion parameter $beta equiv Omega^{0.6}/b$ and the real-space power spectrum of the IRAS PSCz survey using a spherical-harmonic redshift-distortion analysis combined with a data compression method which is designed to deal with correlated parameters. Our latest result, $beta=0.4 pm 0.1$, strongly rules out $beta=1$
We summarise results for the predicted density and peculiar velocity fields from the PSCz survey. We...
We investigate the impact of different observational effects affecting a precise and accurate measur...
The observed two-point correlation functions of galaxies in redshift space become anisotropic due to...
We apply the formalism of spherical harmonic decomposition to the galaxy density field of the IRAS P...
We apply a spherical harmonic analysis to the Point Source Redshift Survey (PSCz), to compute the re...
Introduction We examine the redshift space distortions in the density field of the IRAS PSCz redshi...
Redshift space distortions on large scales can be used to measure the linear growth rate parameter \...
We present the results of reconstruction analysis of the galaxy distribution in a spherical region o...
We present the results of reconstruction analysis of the galaxy distribution in a spherical region o...
We measure the redshift-space power spectrum P(k) for the recently completed IRAS Point Source Catal...
We re-examine the gravitational acceleration (dipole) induced on the Local Group of galaxies by the ...
We investigate the spatial clustering of galaxies in the PSCz galaxy redshift survey, as revealed by...
We present a direct comparison of the clustering properties of two redshift surveys covering a commo...
We use a set of large, high-resolution cosmological N-body simulations to examine the redshift-space...
We compute the bispectrum fur the IRAS PSCz catalog and find that the galaxy distribution displays t...
We summarise results for the predicted density and peculiar velocity fields from the PSCz survey. We...
We investigate the impact of different observational effects affecting a precise and accurate measur...
The observed two-point correlation functions of galaxies in redshift space become anisotropic due to...
We apply the formalism of spherical harmonic decomposition to the galaxy density field of the IRAS P...
We apply a spherical harmonic analysis to the Point Source Redshift Survey (PSCz), to compute the re...
Introduction We examine the redshift space distortions in the density field of the IRAS PSCz redshi...
Redshift space distortions on large scales can be used to measure the linear growth rate parameter \...
We present the results of reconstruction analysis of the galaxy distribution in a spherical region o...
We present the results of reconstruction analysis of the galaxy distribution in a spherical region o...
We measure the redshift-space power spectrum P(k) for the recently completed IRAS Point Source Catal...
We re-examine the gravitational acceleration (dipole) induced on the Local Group of galaxies by the ...
We investigate the spatial clustering of galaxies in the PSCz galaxy redshift survey, as revealed by...
We present a direct comparison of the clustering properties of two redshift surveys covering a commo...
We use a set of large, high-resolution cosmological N-body simulations to examine the redshift-space...
We compute the bispectrum fur the IRAS PSCz catalog and find that the galaxy distribution displays t...
We summarise results for the predicted density and peculiar velocity fields from the PSCz survey. We...
We investigate the impact of different observational effects affecting a precise and accurate measur...
The observed two-point correlation functions of galaxies in redshift space become anisotropic due to...