# Differences

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cmb [2015/02/10 16:11] valeria |
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angular power spectrum. Given a cosmological model, the angular power spectrum can be computed and compared to observational data in order to constrain the set of cosmological parameters. | angular power spectrum. Given a cosmological model, the angular power spectrum can be computed and compared to observational data in order to constrain the set of cosmological parameters. | ||

- | Our group is involved in the ESA Planck collaboration and has contributed to [[http://arxiv.org/abs/1303.5076|2013 results]] and to the 2015 release, including [[http://arxiv.org/abs/1502.01589|cosmological parameter estimation]], | + | Our group is involved in the ESA Planck collaboration and has contributed to [[http://arxiv.org/abs/1303.5076|2013 results]] and to [[http://www.cosmos.esa.int/web/planck/publications|the 2015 release]], including [[http://arxiv.org/abs/1502.01590|a new paper, coordinated in Heidelberg, on dark energy and modified gravity]], as well as [[http://arxiv.org/abs/1502.01589|cosmological parameter estimation]], [[http://arxiv.org/abs/1502.00612|joint analysis Planck/BICEP2+Keck Array]]. |

- | [[http://arxiv.org/abs/1502.01590|a new paper, coordinated in Heidelberg, on dark energy and modified gravity]], as well as the [[http://arxiv.org/abs/1502.00612|joint analysis Planck/BICEP2+Keck Array]]. | + | |

The all-sky image realized by the Planck satellite is the most precise picture of the early Universe and the results confirm that the Universe is in agreement with Lambda-CDM model. | The all-sky image realized by the Planck satellite is the most precise picture of the early Universe and the results confirm that the Universe is in agreement with Lambda-CDM model. |