Cosmological parameters. Cosmological parameters This study presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlationfunctions of the cosmic microwave background (CMB) temperature and polarization fluctuations that account for relevant uncertainties, both instrumental and astrophysical in nature. Results of the Planck mission released in 2015 show the cosmological curvature parameter, Ω K, to be 0.000±0.005, consistent with a flat universe. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. By A Lewis, D Munshi and et al. XIII. From the Planck temperature and lensing data, for this cosmology we find a Hubble constant, H0= (67.8 +/- 0.9) km/s/Mpc, a matter density parameter Omega_m = 0.308 +/- 0.012 and a scalar spectral index with n_s = 0.968 +/- … Planck 2015 results. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. It scanned the microwave and submillimetre sky continuously between 12 August 2009 and 23 October 2013, producing deep, high-resolution, all-sky maps in nine frequency bands from 30 to 857 GHz. Received 6 February 2015 / Accepted 4 June 2016 ABSTRACT This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. ; Rachen, J.P.; Zonca, A.; et al. Cosmological parameters . These data are consistent with the six-parameter inflationary LCDM cosmology. These data are consistent with the six-parameter inflationary LCDM cosmology. These data are consistent with the six-parameter inflationary LCDM cosmology. Planck; ... Cosmological parameter constraints as derived from the Wilkinson Microwave Anisotropy Probe data via Gibbs sampling and the Blackwell-Rao estimator. Papers XIII and XIV detail the cosmological parameters measured and the findings on dark energy, while several additional papers examine potential departures from a canonical cosmological model and constraints on inflationary models. Much more precise spacecraft measurements of the microwave background from WMAP in 2003–2010 and Planck in 2013–2015 have continued to support the model and pin down the parameter values, most of which are now constrained below 1 percent uncertainty. Cosmological parameters: Author(s): Ade, P.A.R. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission Papers by the Planck Collaboration, categorized into groups: Planck 2018 results /Planck 2015 results /Joint BICEP2 Keck Planck 2015 results /Planck 2013 results / Planck intermediate results (2012 -...) / Planck early results (2011) / Pre-launch results (2010) / Technical results (2003 - ...) / The Scientific Programme of Planck(2005) 2. ... Planck 2013 results. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with … A compilation of all the papers using Planck data (by the Planck Collaboration and by o… XIII. Planck 2015 results. In this model Planck data determine the cosmological parameters to high precision. For a full description see the parameters paper. Here, this paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. 1. Of these parameters, only … We present cosmological parameter results from the final full-mission Planck measurements of the cosmic microwave background (CMB) an-isotropies, combining information from the temperature and polarization maps and the lensing reconstruction. XIII. Dark energy and modified gravity ... Planck 2013 results. Math. Planck Collaboration, P. A. R. Ade, N. Aghanim, M. Arnaud, M. Ashdown, J. Aumont, C. Baccigalupi, A. J. Banday, R. B. Barreiro, J. G. Bartlett, and et al. 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. The Planck Collaboration. XVI. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. The Planck results for base LambdaCDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of Type Ia supernovae. We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. ; Genre: Journal Article; Published online: 2016-10; Title: Planck 2015 results - XIII. CMB power spectra, likelihoods, and robustness of parameters. XI. Publication year: 2016: Source: This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. XIV. XIII. The European Space Agency's Planck satellite, which was dedicated to studying the early Universe and its subsequent evolution, was launched on 14 May 2009. The first paper in the series, Planck 2015 Results I, provides an overview of these results. Planck 2015 Results: Cosmological Parameter Name Tags January 16, 2015 This table summarises cosmological parameters used in the Planck chains. The temperature and polarization power spectra are consistent with the standard spatially-flat 6-parameter ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations (denoted “base ΛCDM” in this paper). Universe with zero curvature Cosmological parameters. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. Planck 2015 results. This leaves seven parameters, which is the smallest set that can usefully be compared to the present cosmological data set. Planck was a space observatory operated by the European Space Agency (ESA) from 2009 to 2013, which mapped the anisotropies of the cosmic microwave background (CMB) at microwave and infra-red frequencies, with high sensitivity and small angular resolution.The mission substantially improved upon observations made by the NASA Wilkinson Microwave Anisotropy Probe (WMAP). Abstract. On this page you can find a list of Planck publications, ordered as follows. Abstract. 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 Planck base-ΛCDM results are in good agreement with BAO, SNe, and some galaxy lensing observations, but in slight tension with the Dark Energy Survey’s combined-probe results including galaxy clustering (which prefers lower fluctuation amplitudes or matter density parameters), and in significant, 3.6σ, tension with local measurements of the Hubble constant (which prefer a higher value). We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. Number of Authors: 261 2016 (English) In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. This model is referred to by various names, including ΛCDM, the concordance cosmology, and the standard cosmological model. We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. 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. 594, article id A13 Article in journal (Refereed) Published Abstract [en] This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. M. Chu (UC, Davis, Dept. Request PDF | Planck 2015 results. ), The cosmological parameters are set to Ω m = 0.301, Ω b = 0.0457, = 0.961, 0 = 70.2 km s −1 Mpc −1 and 8 = 0.829 (Ade et al. 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. XVI. XIII. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) Compared to the 2015 results, Cosmological parameters | severely abridged - Subm. Planck 2015 results: XIII. Planck 2015 Results: Cosmological Parameter Tables January 19, 2015 Abstract These tables summarize the results of Planck 2015 parameter estimation exploration results. XVII. Planck 2015 results. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. Author: Planck Collaboration et al. Title: Planck 2015 results. The Planck 2015 cosmogical results are discussed with an emphasis on the improvements compared to the last data release, and on the methodology used to extract the parameters, both for the likelihood building and for the statistical method. Cosmological parameters Planck Collaboration, et.al., 2014, A&&, 571A, 16P ADS / astro-ph. These data are consistent with the six-parameter inflationary LCDM cosmology. If the true value of the cosmological curvature parameter is larger than 10 −3 we will be able to distinguish between these three models even now. Finally, scientific results include cosmological parameters derived from CMB power spectra, gravitational lensing, and cluster counts, as well as constraints on inflation, non-Gaussianity, primordial magnetic fields, dark energy, and modified gravity, and new results on low-frequency Galactic foregrounds. We present new constraints on the rest-frame sound speed, c_{eff}^2, and the viscosity parameter, c_{vis}^2, of the Cosmic Neutrino Background from the recent measurements of the Cosmic Microwave Background anisotropies provided by the Planck satellite. Cosmological parameters Planck Collaboration, 2016, A&A.., 594A, 13P ADS / astro-ph. Download PDF (13 MB) Abstract. 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