activity
20032026
most citedPlanck 2013 results. XVI. Cosmological parameters

6.6k citations · 30.5k across the 130 of their papers we have counts for

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Showing 2008Show all

6 papers · 1 filter

astro-ph2008★ 43 cited

Cosmological parameters after WMAP5: forecasts for Planck and future galaxy surveys

L. P. L. Colombo, E. Pierpaoli, J. R. Pritchard

The Planck satellite is expected to improve the measurement of most cosmological parameters by several factors with respect to current WMAP results. The actual performance may depe…

astro-ph2008★ 13 cited

CMBPol Mission Concept Study: Reionization Science with the Cosmic Microwave Background

Matias Zaldarriaga, Loris Colombo, Eiichiro Komatsu +6

We summarize existing constraints on the epoch of reionization and discuss the observational probes that are sensitive to the process. We focus on the role large scale polarization…

astro-ph2008★ 303 cited

CMBPol Mission Concept Study: Probing Inflation with CMB Polarization

Daniel Baumann, Mark G. Jackson, Peter Adshead +56

We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measu…

astro-ph2008★ 21 cited

Higher neutrino mass allowed if Cold Dark Matter and Dark Energy are coupled

G. La Vacca, S. A. Bonometto, L. P. L. Colombo

Cosmological limits on neutrino masses are softened, by more than a factor 2, if Cold Dark Matter (CDM) and Dark Energy (DE) are coupled. In turn, a neutrino mass yielding up…

astro-ph2008★ 14 cited

Model independent approaches to reionization in the analysis of upcoming CMB data

Loris P. L. Colombo, Elena Pierpaoli

On large angular scales, CMB polarization depends mostly on the evolution of the ionization level of the IGM during reionization. In order to avoid biasing parameter estimates, an…

astro-ph2008★ 19 cited

Dark Matter - Dark Energy coupling biasing parameter estimates from CMB data

Giuseppe La Vacca, Loris P. L. Colombo, Luca Vergani +1

When CMB data are used to derive cosmological parameters, their very choice does matter: some parameter values can be biased if the parameter space does not cover the "true" model.…