The present experimental results on neutrino flavour oscillations provide evidence for non-
zero neutrino masses, but give no hint on their absolute mass scale, which is the target of …

This is a review of models of inflation and of their predictions for the primordial non-
Gaussianity in the density perturbations which are thought to be at the origin of structures in …

We present cosmological parameter constraints based on the final nine-year Wilkinson
Microwave Anisotropy Probe (WMAP) data, in conjunction with a number of additional …

We present the final nine-year maps and basic results from the Wilkinson Microwave
Anisotropy Probe (WMAP) mission. The full nine-year analysis of the time-ordered data …

We present a data analysis methodology for a model-independent reconstruction of the
spectral shape of a stochastic gravitational wave background with LISA. We improve a …

ABSTRACT WMAP precision data enable accurate testing of cosmological models. We find
that the emerging standard model of cosmology, a flat Λ-dominated universe seeded by a …

A simple cosmological model with only six parameters (matter density, Ω mh 2, baryon
density, Ω bh 2, Hubble constant, H 0, amplitude of fluctuations, σ 8, optical depth, τ, and a …

We measure cosmological parameters using the three-dimensional power spectrum P (k)
from over 200 000 galaxies in the Sloan Digital Sky Survey (SDSS) in combination with …

The purpose of the MAP mission is to determine the geometry, content, and evolution of the
universe via a 13 &arcmin; full width half-maximum (FWHM) resolution full-sky map of the …

The WMAP mission has produced sky maps from seven years of observations at L2. We
present the angular power spectra derived from the seven-year maps and discuss the …