Cosmological parameters Planck Collaboration: P. A. R. Ade105, N. Aghanim71, M. Arnaud87, M ... 0:002 < 0:11, consistent with the Planck 2013 results and consistent with the B-mode polarization constraints from a joint analysis of BICEP2, Keck Array, and Planck (BKP) data. arXiv is committed to these values and only works with partners that adhere to them. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. Constraints on cosmological parameters from Planck were re-ported inPlanck Collaboration XVI(2014)2. those of the Planck Satellite [1,2] which supersede the landmark WMAP results [3,4]. This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. By A Lewis, D Munshi and The Planck Collaboration et al. Discover the world's research 17+ million members XV (2013), and Planck Collaboration XVII (2013). Cosmological parameters | Find, read and cite all the research you need on ResearchGate Zodiacal emission: Planck Collaboration: 2014 A&A 571, A14: Planck 2013 results. The cosmological parameter results explore a variety of cosmological models with combinations of Planck and other data. This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. Cosmological parameters: Planck Collaboration: 2014 A&A 571, A16: Planck 2013 results. : Beyond the Cosmological Standard Model . Cosmological parameters We provide results from MCMC exploration chains, as well as best fits, and sets of parameter tables. Abstract. 1. Production process . Within the context of this cosmology, the Planck data determine the cosmological parameters to high precision: the angular size of the sound horizon at recombination, the physical densities of baryons and cold dark matter, and the scalar spectral index are estimated to be ? Planck 2015 Results: Cosmological Parameter Tables January 19, 2015 Abstract These tables summarize the results of Planck 2015 parameter estimation exploration results. Further results were discussed at a science briefing on 21 March 2013, 14:00-15:45 CET. We find that the Planck spectra at high multipoles (>_ 40) are extremely well described by the standard spatially flat six-parameter _CDM cosmology with a power-law spectrum of adiabatic scalar perturbations. They include Planck HFI data in combination with LFI polarization, Planck lensing, as well as additional non-CMB data as detailed in the main parameter papers. The new data from Planck and the cosmological results based on them have been presented at a media briefing organised by the European Space Agency at Headquarters in Paris, on 21 March 2013, 10:00-12:00 CET. CMB power spectra and likelihood: Planck Collaboration: 2014 A&A 571, A15: Planck 2013 results. This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. Planck 2013 results. (2013), Planck Collaboration XII (2013), Planck Collaboration. We find that the Planck spectra at high multipoles (ℓ ≳ 40) are extremely well described by the standard spatially-flat six-parameter ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations. Compared to the 2015 results, improved measurements of large-scale polarization … Definitions, conventions and reference are contained in Planck-2013-XVI. Publication year: 2014: Source: We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. The high-quality data the mission has produced will continue to be scientifically explored in the years to come. CMB power spectra, likelihoods, and robustness of... Planck 2015 results - XI. Because the presence of step oscillations also changes the broadband average power in the spectrum, joint variation is crucial for interpreting constraints on step parameters. Other. 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 logical parameters unlike the Planck collaboration anal-ysis [5]. ; Rachen, J.P.; Zonca, A.; et al. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. Abstract: (EDP Sciences) 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. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with … The Planck 2013 From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H 0 = (67.8 ± 0.9) km s-1 Mpc-1, a matter density parameter Ω m = 0.308 ± 0.012, and a tilted scalar spectral index with n s = 0.968 ± 0.006, consistent with the 2013 analysis. A reply of the briefing is available here. 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. From the Planck temperature data combined with Planck lensing, for this cosmology we find a Hubble constant, H_0 = (67.8 +- 0.9) km s^-1Mpc^-1, a matter density parameter Omega_m = 0.308 +- 0.012, and a tilted scalar spectral index with n_s = 0.968 +- 0.006, consistent with the 2013 analysis. Cosmological parameters . Get PDF (17 MB) Abstract. Cosmological parameters Planck 2015 results - XIII. Planck Collaboration I2014, and references therein) together with a public release of the first 15.5 months of temperature data (which we will refer to as the nominal mission data). 2005 2009 2013 2017 2020 0 500 1K 1.5K. 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