We measured the two dimensional galaxy--galaxy correlation function from the Muenster Red Sky Survey (Ungruhe 1999). This survey has a slightly larger surface as the APM survey and complete up to r_F<18.3 mag (z_{med} \sim 0.14). The large dynamical range of the survey made it possible to examine sub-catalogues with different limiting magnitudes. The positive part of our measured angular correlation functions (after the colour correction) agree excellently with those measured by Maddox, Efstathiou and Shutherland 1996 from the APM galaxy catalogue (Maddox et al. 1990). From the measured angular correlation functions the three dimensional two-point correlation function \xi(r) was calculated. We have chosen the evolution parameter \epsilon so...
We have investigated the statistical clustering properties of galaxies by calculating the two-point ...
We have calculated the two-point correlation functions in redshift space, ξ(σ, π), for galaxies of d...
Several papers have recently highlighted the possibility of measuring redshift-space distortions fro...
We present measurements of the angular two-point galaxy correlation function, w(theta), from the APM...
For faint photometric surveys our ability to quantify the clustering of galaxies has depended on int...
Significant uncertainties exist in the measured amplitude of the angular two-point correlation funct...
We present the three-dimensional power spectrum of galaxy clustering using measurements of the angul...
We calculate the angular correlation function of galaxies in the Two Micron All Sky Survey. We minim...
We present a detailed analysis of the two-point correlation function, ξ(σ, π), from the 2dF Galaxy R...
We have investigated the statistical clustering properties of galaxies by calculating the 2-point ga...
A photometric survey of faint galaxies in three high Galactic latitude fields (each $\sim49~\rm{arcm...
We present a systematic comparison of some usual estimators of the 2--point correlation function, so...
We present a detailed analysis of the two-point correlation function, ξ (σ, π), from the 2dFGalaxy R...
The three-point correlation function (3PCF) can now be measured in large galaxy redshift surveys, bu...
We present new results for the three-point correlation function, ζ, measured as a function of scale,...
We have investigated the statistical clustering properties of galaxies by calculating the two-point ...
We have calculated the two-point correlation functions in redshift space, ξ(σ, π), for galaxies of d...
Several papers have recently highlighted the possibility of measuring redshift-space distortions fro...
We present measurements of the angular two-point galaxy correlation function, w(theta), from the APM...
For faint photometric surveys our ability to quantify the clustering of galaxies has depended on int...
Significant uncertainties exist in the measured amplitude of the angular two-point correlation funct...
We present the three-dimensional power spectrum of galaxy clustering using measurements of the angul...
We calculate the angular correlation function of galaxies in the Two Micron All Sky Survey. We minim...
We present a detailed analysis of the two-point correlation function, ξ(σ, π), from the 2dF Galaxy R...
We have investigated the statistical clustering properties of galaxies by calculating the 2-point ga...
A photometric survey of faint galaxies in three high Galactic latitude fields (each $\sim49~\rm{arcm...
We present a systematic comparison of some usual estimators of the 2--point correlation function, so...
We present a detailed analysis of the two-point correlation function, ξ (σ, π), from the 2dFGalaxy R...
The three-point correlation function (3PCF) can now be measured in large galaxy redshift surveys, bu...
We present new results for the three-point correlation function, ζ, measured as a function of scale,...
We have investigated the statistical clustering properties of galaxies by calculating the two-point ...
We have calculated the two-point correlation functions in redshift space, ξ(σ, π), for galaxies of d...
Several papers have recently highlighted the possibility of measuring redshift-space distortions fro...