51 citations · 51 across the 1 of their papers we have counts for
6 papers
The mass and anisotropy profiles of galaxy clusters from the projected phase space density: testing the method on simulated data
Radoslaw Wojtak, Ewa L. Lokas, Gary A. Mamon +1
We present a new method of constraining the mass and velocity anisotropy profiles of galaxy clusters from kinematic data. The method is based on a model of the phase space density…
A built-in scale in the initial spectrum of density perturbations: evidence from cluster and CMB data
F. Atrio-Barandela, J. Einasto, S. Gottlöber +2
We calculate temperature anisotropies of the cosmic microwave background (CMB) for several initial power spectra of density perturbations with a built-in scale suggested by recent…
The supercluster--void network III. The correlation function as a geometrical statistic
J. Einasto, M. Einasto, P. Frisch +5
We investigate properties of the correlation function of clusters of galaxies using geometrical models. On small scales the correlation function depends on the shape and the size o…
The supercluster--void network II. An oscillating cluster correlation function
J. Einasto, M. Einasto, P. Frisch +7
We use rich clusters of galaxies in the Northern and Southern Galactic hemispheres up to a redshift z=0.12 to determine the cluster correlation function. We show that superclusters…
The Las Campanas Redshift Survey Galaxy-Galaxy Autocorrelation Function
D. L. Tucker, A. Oemler, R. P. Kirshner +7
Presented are measurements of the observed redshift-space galaxy-galaxy autocorrelation function, xi(s), for the Las Campanas Redshift Survey (LCRS). For separations 2.0/h Mpc < s…
The accuracy of parameters determined with the core-sampling method: application to Voronoi tessellations
Andrei G. Doroshkevich, Stefan Gottloeber, Soeren Madsen
The large-scale matter distribution represents a complex network of structure elements such as voids, clusters, filaments, and sheets. This network is spanned by a point distributi…