In this introductory talk we will establish connections between the statistical analysis of galaxy clustering in cosmology and recent work in mainstream spatial statistics. The lecture will review the methods of spatial statistics used by both sets of scholars, having in mind the cross-fertilizing purpose of the meeting series. Special topics will be: description of the galaxy samples, selection effects and biases, correlation functions, nearest neighbor distances, void probability functions, Fourier analysis, and structure statistics
We propose a method to analyze the clustering property of samples of discrete sources. With that met...
We present measurements of the higher-order clustering of red and blue galaxies as a function of sca...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...
A brief introduction is given to some aspects of the statistical description of the luminous matter ...
We follow the evolution of the galaxy population in a ΛCDM cosmology by means of high-resolution N-b...
The purpose of this thesis is to study the role of the spatial and angular correlation functions for...
We describe a method for estimating the power spectrum of density fluctuations from galaxy redshift ...
Context. The clustering of galaxy clusters is sensitive not only to the parameters charact...
This paper investigates whether nonlinear gravitational instability can account for the clustering o...
These lectures cover various aspects of the statistical description of cosmological density fields. ...
We present the three-dimensional power spectrum of galaxy clustering using measurements of the angul...
Context. The clustering properties of galaxies belonging to different luminosity ranges or having di...
These lecture notes concentrate on a few specific topics concerning the distribution of galaxies on ...
This paper reviews the measurements of galaxy correlations at high redshifts, and discusses how thes...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...
We propose a method to analyze the clustering property of samples of discrete sources. With that met...
We present measurements of the higher-order clustering of red and blue galaxies as a function of sca...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...
A brief introduction is given to some aspects of the statistical description of the luminous matter ...
We follow the evolution of the galaxy population in a ΛCDM cosmology by means of high-resolution N-b...
The purpose of this thesis is to study the role of the spatial and angular correlation functions for...
We describe a method for estimating the power spectrum of density fluctuations from galaxy redshift ...
Context. The clustering of galaxy clusters is sensitive not only to the parameters charact...
This paper investigates whether nonlinear gravitational instability can account for the clustering o...
These lectures cover various aspects of the statistical description of cosmological density fields. ...
We present the three-dimensional power spectrum of galaxy clustering using measurements of the angul...
Context. The clustering properties of galaxies belonging to different luminosity ranges or having di...
These lecture notes concentrate on a few specific topics concerning the distribution of galaxies on ...
This paper reviews the measurements of galaxy correlations at high redshifts, and discusses how thes...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...
We propose a method to analyze the clustering property of samples of discrete sources. With that met...
We present measurements of the higher-order clustering of red and blue galaxies as a function of sca...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...