Zodiacal emission: Planck Collaboration: 2014 A&A 571, A14: Planck 2013 results. (2013), Planck Collaboration XII (2013), Planck Collaboration. Production process . arXiv is committed to these values and only works with partners that adhere to them. However the most accurate model of the Universe requires consideration of a range of observations, with complementary probes providing consistency checks, lifting parameter degeneracies, and enabling the strongest constraints to be placed. The tension in the determination of some cosmological parameters on the basis of the two CMB datasets WMAP9 and Planck-2013 is highlighted. 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 - XIII. Cosmological parameters: Author(s): Ade, P.A.R. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. 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. In this model Planck data determine the cosmological parameters to high precision. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. We provide results from MCMC exploration chains, as well as best fits, and sets of parameter tables. The cosmological parameter results explore a variety of cosmological models with combinations of Planck and other data. 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. Further results were discussed at a science briefing on 21 March 2013, 14:00-15:45 CET. Constraints on cosmological parameters from Planck were re-ported inPlanck Collaboration XVI(2014)2. CMB power spectra, likelihoods, and robustness of parameters. 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. The high-quality data the mission has produced will continue to be scientifically explored in the years to come. Planck 2013 results. XVI. 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. CMB power spectra, likelihoods, and robustness of... Planck 2015 results - XI. arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. : Beyond the Cosmological Standard Model . Planck 2015 Results: Cosmological Parameter Tables January 19, 2015 Abstract These tables summarize the results of Planck 2015 parameter estimation exploration results. ; Genre: Zeitschriftenartikel; Im Druck veröffentlicht: 2014-11; Titel: Planck 2013 results - XVI. 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. 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. They include Planck data in combination with WMAP polarization, Planck lensing, and high-l CMB experiments, as well as additional non-CMB data as detailed in the main parameter papers. logical parameters unlike the Planck collaboration anal-ysis [5]. 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: 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. Title: Planck 2013 results. Discover the world's research 17+ million members 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. Planck was turned off on 23 October 2013. XV (2013), and Planck Collaboration XVII (2013). Definitions, conventions and reference are contained in Planck-2013-XVI. XVI. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) 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. 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 Get PDF (17 MB) Abstract. 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. XV. XIV. The Planck 2013 ; Rachen, J.P.; Zonca, A.; et al. We find a low value of the Hubble constant, H0=67.3+/-1.2 … We present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra. Autor: Planck Collaboration et al. XVI. Planck 2013 results. Other. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with … Publication year: 2014: Source: Request PDF | On Mar 1, 2013, P ~A ~R Ade and others published Planck 2013 results. Cosmological parameters | Find, read and cite all the research you need on ResearchGate those of the Planck Satellite [1,2] which supersede the landmark WMAP results [3,4]. By A Lewis, D Munshi and The Planck Collaboration et al. A reply of the briefing is available here. Cosmological parameters. Abstract. 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 … Cosmological parameters . Please note that these pages are largely directed to the astronomical and Planck communities. 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, März 2013 (69 S.) arxiv:1303.5076 Einzelnachweise [ Bearbeiten | Quelltext bearbeiten ] ↑ Austin Joyce et al. Cosmological parameters 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). Cosmological parameters: Planck Collaboration: 2014 A&A 571, A16: Planck 2013 results. XVII. 1. The Planck spectra at high multipoles are extremely well described by the standard spatially-flat six-parameter LCDM cosmology. CMB power spectra and likelihood: Planck Collaboration: 2014 A&A 571, A15: Planck 2013 results. 1. More information on Planck may be accessed via the links to the left and right (some of the links are restricted). Cosmological parameters Planck 2015 results - XIII. Planck 2015 results - XI. 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