We perform a detailed comparison of the IRAS PSCz and 1.2-Jy spherical harmonic coefficients of the density and velocity fields in redshift space. The monopole terms predicted from the two surveys show some differences. The mismatch between the velocity monopoles arises from faint sources and disappears when extracting a PSCz subsample of galaxies with fluxes larger than 1.2 Jy. The analysis of PSCz dipole moments confirms the same inconsistencies found by Davis, Nusser and Willick (1996) between the IRAS 1.2-Jy gravity field and MARK III peculiar velocities. We conclude that shot-noise, which is greatly reduced in our PSCz gravity field, cannot be responsible for the observed mismatch
Introduction We examine the redshift space distortions in the density field of the IRAS PSCz redshi...
We compare the peculiar velocities derived from the I-band Tully–Fisher (TF) relation for 989 field ...
We present a self-consistent non-parametric model of the local cosmic velocity field derived from th...
We perform a detailed comparison of the IRAS PSCz and 1.2-Jy spherical harmonic coefficients of the ...
We present a comparison between the peculiar velocity field measured from the ENEAR all-sky Dn−σ cat...
We present a comparison between the peculiar velocity field measured from the ENEAR all-sky D-n-sigm...
We summarise results for the predicted density and peculiar velocity fields from the PSCz survey. We...
We apply the formalism of spherical harmonic decomposition to the galaxy density field of the IRAS P...
We constructed a Bayesian hyper-parameter statistical method to quantify the difference between pred...
We re-examine the gravitational acceleration (dipole) induced on the Local Group of galaxies by the ...
We present a self consistent nonparametric model of the local cosmic velocity field based on the den...
We have constrained the redshift-distortion parameter $beta equiv Omega^{0.6}/b$ and the real-space ...
We compare the peculiar velocities derived from the I-band Tully-Fisher (TF) relation for 989 field ...
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...
We compare the peculiar velocities derived from the I-band Tully–Fisher (TF) relation for 989 field ...
We present a self-consistent non-parametric model of the local cosmic velocity field derived from th...
We perform a detailed comparison of the IRAS PSCz and 1.2-Jy spherical harmonic coefficients of the ...
We present a comparison between the peculiar velocity field measured from the ENEAR all-sky Dn−σ cat...
We present a comparison between the peculiar velocity field measured from the ENEAR all-sky D-n-sigm...
We summarise results for the predicted density and peculiar velocity fields from the PSCz survey. We...
We apply the formalism of spherical harmonic decomposition to the galaxy density field of the IRAS P...
We constructed a Bayesian hyper-parameter statistical method to quantify the difference between pred...
We re-examine the gravitational acceleration (dipole) induced on the Local Group of galaxies by the ...
We present a self consistent nonparametric model of the local cosmic velocity field based on the den...
We have constrained the redshift-distortion parameter $beta equiv Omega^{0.6}/b$ and the real-space ...
We compare the peculiar velocities derived from the I-band Tully-Fisher (TF) relation for 989 field ...
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...
We compare the peculiar velocities derived from the I-band Tully–Fisher (TF) relation for 989 field ...
We present a self-consistent non-parametric model of the local cosmic velocity field derived from th...