the PRIMAT code, and the DES team for sharing their likelihoods. No commercial reproduction, distribution, display or performance rights in this work are provided. The analysis of the cosmological parameters (Planck … Results of the parameter exploration runs should be reproducible using CosmoMC with the Planck likelihood code. IV. These results are only weakly dependent on the cosmological model and remain stable, with somewhat increased errors, in many commonly considered extensions. Cosmological parameters Tools RDF+XML BibTeX RIOXX2 XML RDF+N-Triples JSON RefWorks Dublin Core Simple Metadata Refer METS Dublin Core HTML Unit Citation HTML Citation ASCII Citation HTML Profile Citation OpenURL ContextObject EndNote OpenURL ContextObject in Span MODS MPEG-21 DIDL EP3 XML Reference Manager RDF+N3 OAI-PMH RIOXX Multiline CSV The CMB spectra continue to prefer higher lensing amplitudes than predicted in base ΛCDM at over 2σ, which pulls some parameters that affect the lensing amplitude away from the ΛCDM model; however, this is not supported by the lensing reconstruction or (in models that also change the background geometry) BAO data. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with … We provide results from MCMC exploration chains, as well as best fits, and sets of parameter tables. al., The term ‘cosmological parameters’ is forever increasing in its scope, and nowadays often includes the parameterization of some functions, as well as simple numbers describing properties of the Universe. Confidence intervals are derived from the MCMC samples, and assume the input likelihoods are exactly correct, so there is no quantification for systematic errors other than via the covariance, foreground and beam error models assumed in the likelihood codes. description of the Planck Collaboration and a list of its members, indicating Planck not only confirmed this picture but made it much more precise, pinning down the free parameters to unprecedented accuracy (figure 5). Where determined from BBN consistency, the. A compilation of all the papers using Planck data (by the Planck Collaboration and by o… Constraints on inflation • Planck 2018 results. Some results with additional data are produced by importance sampling. A&A, 641 (2020) A6; VI. In this model Planck data determine the cosmological parameters to high precision. This project has received funding From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H0 = (67.8 ± 0.9) km s-1Mpc-1, a matter density parameter Ωm = 0.308 ± 0.012, and a tilted scalar spectral index with ns = 0.968 ± 0.006, consistent with the 2013 analysis. Cosmological parameters - NASA/ADS We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) anisotropies, combining information from the temperature and polarization maps and the lensing reconstruction. A Note that alpha1 results are not used in the parameter paper, and are separate from the isocurvature results in the inflation paper. X. ISSN 0004-6361. This page contains cosmological parameters, likelihoods, power spectra, noise covariance matrices, polarization leakage corrections maps, beams, instrument models, mask files, planet intensities and dates on which positions on the sky were observed. First combined constraints on polarized synchrotron emission from Planck and WMAP. A combined analysis gives dark matter density Ω_ch² = 0.120 ± 0.001, baryon density Ω_bh² = 0.0224 ± 0.0001, scalar spectral index n_s = 0.965 ± 0.004, and optical depth τ = 0.054 ± 0.007 (in this abstract we quote 68% confidence regions on measured parameters and 95% on upper limits). Standard big-bang nucleosynthesis predictions for the helium and deuterium abundances for the base-ΛCDM cosmology are in excellent agreement with observations. 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