International audienceWith its wide frequency coverage Planck is a unique tool not only to test the standard cosmo- logical model (LCDM) but to explore beyond it, looking, for example, for the absolute scale of neutrino masses. Cosmological parameters are traditionally determined using a Bayesian approach based on Markov chains (MCMC) but a Frequentist approach based on profiles- Likelihood is also possible. The two methods are presented, with special focus on the latter, which gives results remarka- bly consistent with Bayesian approach for the LCDM model. The interesting case of neutrinos is discussed. Here the presence of a physical boundary on the masses induces differences in the two approaches nevertheless giving results in perfect ag...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
The cosmic microwave background (CMB), relic of the hot Big-Bang, carries the traces of both the ric...
Submitted to A&AWe explore the 2013 Planck likelihood function with a high-precision multi-dimension...
Massive neutrinos leave peculiar imprints in the different cosmological data sets allowing cosmology...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
The cosmic microwave background (CMB), relic of the hot Big-Bang, carries the traces of both the ric...
Submitted to A&AWe explore the 2013 Planck likelihood function with a high-precision multi-dimension...
Massive neutrinos leave peculiar imprints in the different cosmological data sets allowing cosmology...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
We explore the 2013 Planck likelihood function with a high-precision multi-dimensional minimizer (Mi...
The cosmic microwave background (CMB), relic of the hot Big-Bang, carries the traces of both the ric...