When applied to deep photometric catalogs, the two-point angular correlation function, ω (θ),
is a sensitive probe of the evolution of galaxy clustering properties. Here we present …

We have measured the angular correlation function w (&thetas;) for a sample of 871 Lyman-
break galaxies (LBGs) in five fields at redshift z∼ 3. Fitting the power law A w &thetas;-β to a …

We study the biasing relation between dark matter haloes or galaxies and the underlying
mass distribution, using cosmological N-body simulations in which galaxies are modelled …

We use the two-point correlation function to calculate the clustering properties of the recently
completed SSRS2 survey, which probes two well-separated regions of the sky, allowing one …

We investigate the potential and accuracy of clustering-based redshift estimation using the
method proposed by Ménard et al. This technique enables the inference of redshift …

Cross-correlations between the lensing of the cosmic microwave background (CMB) and
other tracers of large-scale structure provide a unique way to reconstruct the growth of dark …

We evaluate the impact of imaging systematics on the clustering of luminous red galaxies
(LRG), emission-line galaxies (ELG), and quasars (QSO) targeted for the upcoming Dark …

We present the results of the deepest optically identified X-ray survey yet made. The X-ray
survey was obtained with the ROSAT position-sensitive proportional counter (PSPC) and …

We use a combination of N-body simulations of the hierarchical clustering of dark matter and
semi-analytic modelling of the physics of galaxy formation to probe the relationship between …

We explore the accuracy of the clustering-based redshift estimation proposed by Ménard et
al. when applied to VIMOS Public Extragalactic Redshift Survey (VIPERS) and Canada …