Anisotropy of the Cosmic Microwave Background
The aim of the project is to determine the angular power spectrum of Cosmic Microwave Background (CMB) in angular scales from a few degrees to several arcminutes. The primordial matter density fluctuations that originated the present structure of the Universe left imprinted spatial variations in the CMB radiation. From high sensitivity maps of this radiation we aim to constrain the most relevant cosmological parameters: total energy/matter density, density of cold dark matter, density of baryonic matter, the Hubble constant, density of dark energy, neutrino density, reionization epoch, etc.
Internal code of the project: P/308605.
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