Ruprecht Karls Universität Heidelberg

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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.

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