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 …

The Atacama Cosmology Telescope is a 6 m telescope designed to map the cosmic
microwave background simultaneously at 145, 215, and 280 GHz with arcminute resolution …

We discuss the derivation of the analytic properties of the cross-power spectrum estimator
from multi-detector CMB anisotropy maps. The method is computationally convenient and it …

We present the first sky maps from the BEAST (Background Emission Anisotropy Scanning
Telescope) experiment. BEAST consists of a 2.2 m off-axis Gregorian telescope fed by a …

Context. Determining the spectral and spatial characteristics of the radio continuum of our
Galaxy is an experimentally challenging endeavour for improving our understanding of the …

Context. Multi-frequency observations are needed to separate the cosmic microwave
background (CMB) from foreground emission and accurately extract cosmological …

Abstract The Background Emission Anisotropy Scanning Telescope (BEAST) is a millimeter
wavelength experiment designed to generate maps of fluctuations in the cosmic microwave …

We report limits on the Galactic foreground emission contribution to the Background
Emission Anisotropy Scanning Telescope (BEAST) Ka-and Q-band CMB anisotropy maps …

We present the angular power spectrum of the cosmic microwave background (CMB)
component extracted with fastica from the Background Emission Anisotropy Scanning …

The COsmic Foreground Explorer (COFE) is a balloon-borne microwave polarimeter
designed to measure the low-frequency and low-ℓ characteristics of dominant diffuse …