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Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
F. Finelli, M. Rianna, N. Mandolesi
We present the constraints on inflationary parameters in a flat CDM universe obtained by WMAP three year data release, plus smaller scale CMB and two LSS data sets, 2dF and SDSS…
Radiative effects by high-z UV radiation background: Implications for the future CMB polarization measurements
L. A. Popa, C. Burigana, N. Mandolesi
We investigate the role of the radiative effects for the temporal evolution of the reionization fraction by using cosmological Smooth Particle Hydrodynamics (SPH) simulations. We f…
The Planck Low Frequency Instrument
N. Mandolesi, C. Burigana, R. C. Butler +14
Planck is the third generation of mm-wave instruments designed for space observations of the cosmic microwave background (CMB) anisotropies within the new Cosmic Vision 2020 ESA Sc…
Galactic foreground contribution to the BEAST CMB Anisotropy Maps
Jorge Mejía, Marco Bersanelli, Carlo Burigana +17
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 estimate t…
The CMB Power Spectrum from the Background Emission Anisotropy Scanning Telescope (BEAST) Experiment
Ian J. O'Dwyer, Marco Bersanelli, Jeffrey Childers +19
The Background Emission Anisotropy Scanning Telescope (BEAST) is a 2.2m off-axis telescope with an 8 element mixed Q (38-45GHz) and Ka (26-36GHz) band focal plane, designed for bal…
Signature of HDM clustering at Planck angular scales
L. A. Popa, C. Burigana, N. Mandolesi
We present the CMB anisotropy induced by the non-linear perturbations in the massive neutrino density associated to the non-linear gravitational clustering. We show that the non-li…