CMB likelihood functions for beginners and experts
3 K COSMOLOGY 476 (1999) 249-265
Clustering in the VIRMOS survey: Expected cosmic errors
ASTR SOC P 200 (1999) 153-157
Abstract:
We predict the errors on counts-in-cells statistics measured in the future VIRMOS survey. Several effects are included, such as variation of clustering, biasing, and geometry. Most importantly for the survey strategy, sparse sampling appears to have no particular advantage in this case, especially for higher order statistics at high redshift. The predicted accuracy is a few percent for the variance, and about 10 percent for the skewness at z = 1 in a small dynamic range around 1 h(-1) Mpc.Cosmological evolution and hierarchical galaxy formation
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 309:4 (1999) 823-832
MAXIMA: an experiment to measure temperature anisotropy in the cosmic microwave background
3 K COSMOLOGY 476 (1999) 224-236
QSO clustering and the AAT 2dF QSO redshift survey
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES 357:1750 (1999) 185-198