We show, with the help of large N-body simulations, that the real-space two-point correlation function and pairwise velocity dispersion of galaxies can both be measured reliably from the Las Campanas Redshift Survey. The real-space correlation function is well fitted by the power law #xi#(r)=(r_0/r)"#gamma# with r_0=(5.06#+-#0.12) h"-"1 Mpc and #gamma#=1.862#+-#0.034, and the pairwise velocity dispersion at 1 h"-"1 Mpc is (570#+-#80) km s"-"1. A detailed comparison between these observational results and the predictions of current CDM cosmogonies is carried out. We construct 60 mock samples for each theoretical model from a large set of high resolution N-body simulations, which allows us to include various...
We present analyses of the two-point correlation function derived from an all-sky redshift survey of...
It has long been regarded as difficult if not impossible for a cosmological model to account simulta...
We present a new statistic---the redshift dispersion--- which may prove useful for comparing next ge...
We report on the measurement of the two-point correlation function and the pairwise peculiar velocit...
The standard method of measuring the galaxy pairwise velocity dispersion on small scales is heavily ...
We use high-resolution N-body simulations to develop a new, flexible, empirical ap-proach for measur...
We present a novel measurement of the pairwise peculiar velocity distribution function of galaxies o...
We present the first determination of the pairwise velocity dispersion (PVD) for galaxies in differe...
We investigate the feasibility of determining the pairwise velocity dispersion (PVD) for Lyman break...
We present a detailed analysis of the two-point correlation function, ξ (σ, π), from the 2dFGalaxy R...
We have investigated the statistical clustering properties of galaxies by calculating the two-point ...
SIGLEAvailable from TIB Hannover / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische Infor...
(Abridged) We make predictions for the pairwise velocity dispersion (PVD) of galaxies with models th...
We present the first determination of the pairwise velocity dispersion (PVD) for galaxies in differe...
The pair-weighted relative velocity dispersion of galaxies provides a measure of the thermal energy ...
We present analyses of the two-point correlation function derived from an all-sky redshift survey of...
It has long been regarded as difficult if not impossible for a cosmological model to account simulta...
We present a new statistic---the redshift dispersion--- which may prove useful for comparing next ge...
We report on the measurement of the two-point correlation function and the pairwise peculiar velocit...
The standard method of measuring the galaxy pairwise velocity dispersion on small scales is heavily ...
We use high-resolution N-body simulations to develop a new, flexible, empirical ap-proach for measur...
We present a novel measurement of the pairwise peculiar velocity distribution function of galaxies o...
We present the first determination of the pairwise velocity dispersion (PVD) for galaxies in differe...
We investigate the feasibility of determining the pairwise velocity dispersion (PVD) for Lyman break...
We present a detailed analysis of the two-point correlation function, ξ (σ, π), from the 2dFGalaxy R...
We have investigated the statistical clustering properties of galaxies by calculating the two-point ...
SIGLEAvailable from TIB Hannover / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische Infor...
(Abridged) We make predictions for the pairwise velocity dispersion (PVD) of galaxies with models th...
We present the first determination of the pairwise velocity dispersion (PVD) for galaxies in differe...
The pair-weighted relative velocity dispersion of galaxies provides a measure of the thermal energy ...
We present analyses of the two-point correlation function derived from an all-sky redshift survey of...
It has long been regarded as difficult if not impossible for a cosmological model to account simulta...
We present a new statistic---the redshift dispersion--- which may prove useful for comparing next ge...