These results are consistent with those from WMAP polarization measurements cleaned for dust emission using 353-GHz polarization maps from the High Frequency Instrument. Cosmological parameters . Cited 3469 times in Scopus. We find no evidence for any departure from base ΛCDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find Neff = 3.15 ± 0.23 for the effective number of relativistic degrees of freedom, consistent with the value Neff = 3.046 of the Standard Model of particle physics. The standard big bang nucleosynthesis predictions for the helium and deuterium abundances for the best-fit Planck base ΛCDM cosmology are in excellent agreement with observations. 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. Cosmological parameters: Author(s): Ade, P.A.R. 1. XIII. However, as in the 2013 analysis, the amplitude of the fluctuation spectrum is found to be higher than inferred from some analyses of rich cluster counts and weak gravitational lensing. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. Adding a tensor component as a single-parameter extension to base ΛCDM we find an upper limit on the tensor-to-scalar ratio of r0.002< 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. Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. The temperature and polarization power spectra are consistent with … We make a comparison for ten typical, popular dark energy models according to their capabilities of fitting the current observational data. Planck 2015 results. 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). Powered By Scopus® Data, http://dx.doi.org/10.1051/0004-6361/201525830. We find no evidence for any contribution from isocurvature perturbations or from cosmic defects. Number of Authors: 261 2016 (English) In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. The spatial curvature of our Universe is found to be very close to zero, with | ΩK | < 0.005. Received 2014 September 26; accepted 2015 January 14; published 2015 February 24 ABSTRACT We examine the consistency of the 9yr WMAP data and the ﬁrst-release Planck data. Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. The standard big bang nucleosynthesis predictions for the helium and deuterium abundances for the best-fit Planck base ΛCDM cosmology are in excellent agreement with observations. Lewis, A, Munshi, D and The Planck Collaboration, et al. The European Space Agency's Planck satellite gathered data for over 4 years, and a series of 28 papers releasing the results and evaluating constraints on cosmological models have been recently released. Cosmological parameters. Publication year: 2016: Source: @article{Aghanim2020Planck2R, title={Planck 2018 results. 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). Planck 2015 results. XIII. In neither case do we find no evidence for new physics. Updated November 2015, by O. Lahav (University College London) and A.R. © 2016 ESO. Parametrizing the Universe Rapid advances in observational cosmology have led to the establishment of a precision cosmological model, with many of the key cosmological parameters determined to one or two signiﬁcant ﬁgure accuracy. Combined with the Planck temperature and lensing data, these measurements give a reionization optical depth of τ = 0.066 ± 0.016, corresponding to a reionization redshift of . This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. The Planck Collaboration. 3 Constraints on the parameters of the base bold0mu mumu CDM cosmology from Planck, 4 Comparison of the Planck power spectrum with high-resolution experiments, 5 Comparison of the Planck base CDM model with other astrophysical data sets. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. February 2015; Astronomy ... (We quote 68% errors on measured parameters and 95% limits on other parameters.) For example, Larson et al. View in Scopus. The Planck 2015 cosmological parameters using both temperature and polarization data are in very good agreement with those from the 2013 release, but with significantly improved precision. These data are consistent with the six-parameter inflationary LCDM cosmology. The six free parameters can be well constrained by the TT spectrum alone, and then the TE and EE spectra can … On this page you can find a list of Planck publications, ordered as follows. (2016). By A Lewis, D Munshi and et al. Cosmological parameters. We speciﬁcally compare sky maps, power spectra, and the inferred Λ cold dark matter (ΛCDM) cosmological parameters. ; Rachen, J.P.; Zonca, A.; et al. We also constraints on annihilating dark matter and on possible deviations from the standard recombination history. The sum of neutrino masses is constrained to â'mν < 0.23 eV. The WMAP and Planck 2015 TT spectra now appear to be in agreement over their common multipole range (Figure 46 of Planck Collaboration XI 2015). We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. 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. The observational data we use in this work include the JLA sample of type Ia supernovae observation, the Planck 2015 distance priors of cosmic microwave background observation, the baryon acoustic oscillations measurements, and the direct measurement … 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. 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. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. A compilation of all the papers using Planck data (by the Planck Collaboration and by o… 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. 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. 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 polarization of the CMB, discovered in 2002 by DASI, is now a dramatic success: in the 2015 Planck data release, there are seven observed peaks in the temperature (TT) power spectrum, six peaks in the temperature-polarization (TE) cross spectrum, and five peaks in the polarization (EE) spectrum. In approximate percentage terms… 24.1. (2016) Planck 2015 results. ISSN 0004-6361 We present the first results of polarization measurements with the Low Frequency Instrument at large angular scales. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. 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. In neither case do we find no evidence for new physics. Request PDF | Planck 2015 results. Let us know how this access is important for you. Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with … Astronomy and Astrophysics, 594 (A13). Note that in this abstract we quote 68% confidence limits on measured parameters and 95% upper limits on other parameters. The main goal of the work is to constrain the free parameters of the model utilizing the latest observational data released by Planck-2015 [19, 25]. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. With four unified, simplified and workable assumptions, a number of useful cosmological formulae can be generated and the current Hubble parameter and current microwave back ground temperature can be fitted accurately. Many UC-authored scholarly publications are freely available on this site because of the UC's open access policies. We present results based on full-mission Planck observations of temperature and polarization anisotropies of the CMB. The addition of Planck polarization data leads to strong constraints on deviations from a purely adiabatic spectrum of fluctuations. Here, this paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. 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. We find no evidence for any contribution from isocurvature perturbations or from cosmic defects. Enter the password to open this PDF file: Open Access Publications from the University of California, Planck 2015 results: XIII. 1. Planck Collaboration, Ade, P. A. R., Aghanim, N., Arnaud, M., Ashdown, M., Aumont, J., et al. Apart from these tensions, the base ΛCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets. These results are consistent with those from WMAP polarization measurements cleaned for dust emission using 353-GHz polarization maps from the High Frequency Instrument. When the additional informa- Prediction of quantum perturbation is one of interesting features of inflationary scenario. We present the first results of polarization measurements with the Low Frequency Instrument at large angular scales. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission We show that these tensions cannot easily be resolved with simple modifications of the base ΛCDM cosmology. Adding a tensor component as a single-parameter extension to base ΛCDM we find an upper limit on the tensor-to-scalar ratio of r0.002< 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. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Download PDF (13 MB) Abstract. Cosmological parameters Planck Collaboration: P. A. R. Ade 105 , N. Aghanim 71 , M. Arnaud 87 , M. Ashdown 83;7 , J. Aumont 71 , C. Baccigalupi 103 , A. J. Banday 117;12 , R. B. Barreiro 78 , J. G. Bartlett 1;80 , N. Bartolo 38;79 , E. Battaner 120;121 , R. Battye 81 , K. Benabed 72;116 , A. Benoˆıt 69 , A. Benoit-L´evy 29 ;72 116 , 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 +/- 0.006. This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) Introduction Since its first discovery by Penzias and Wilson (1965), observations of the cosmic Compared to the 2015 results, improved measurements of large-scale polarization allow the reionization optical depth to be measured with … However, as in the 2013 analysis, the amplitude of the fluctuation spectrum is found to be higher than inferred from some analyses of rich cluster counts and weak gravitational lensing. Planck 2015 results - XIII. In general, the Planck mission’s complete results confirm the canonical cosmological model, known as Lambda Cold Dark Matter, or ΛCDM. XIII. Combining Planck data with other astrophysical data, including Type Ia supernovae, the equation of state of dark energy is constrained to w = −1.006 ± 0.045, consistent with the expected value for a cosmological constant. We also constraints on annihilating dark matter and on possible deviations from the standard recombination history. 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. Residual dipoles are between the cosmological parameters inferred. Combining Planck data with other astrophysical data, including Type Ia supernovae, the equation of state of dark energy is constrained to w =-1.006 ± 0.045, consistent with the expected value for a cosmological constant. XIII. VI. Liddle (University of Edinburgh). Let us know how this access is important for you. The spatial curvature of our Universe is found to be very close to zero, with | ΩK | < 0.005. The sum of neutrino masses is constrained to ∑ mν < 0.23 eV. XIII. Cosmological parameters, From wave to tsunami: the growth of third wave whiteness, Semimartingale properties of a generalized fractional Brownian motion and its mixtures with applications in finance, Linear-Quadratic Stochastic Differential Games on Random Directed Networks, Visual Sociology in a Discipline of Words: Racial Literacy, Visual Literacy and Qualitative Research Methods, GENDER-FLUID GEEK GIRLS: Negotiating Inequality Regimes in the Tech Industry, UC Santa Barbara Previously Published Works, https://doi.org/10.1051/0004-6361/201525830. Combined with the Planck temperature and lensing data, these measurements give a reionization optical depth of τ = 0.066 ± 0.016, corresponding to a reionization redshift of \hbox{$z-{\rm re}=8.8{+1.7}-{-1.4}$}. Cosmological parameters | severely abridged - Subm. Our results are in very good agreement with the 2013 analysis of the Planck nominal-mission temperature data, but with increased precision. Cosmological parameters. 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. Adding the BKP B-mode data to our analysis leads to a tighter constraint of r0.002 < 0.09 and disfavours inflationarymodels with a V(φ) ∝ φ2 potential. XIII. 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 results for base ΛCDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of Type Ia supernovae. (We quote 68% errors on measured parameters and 95% limits on other parameters.) Apart from these tensions, the base ΛCDM cosmology provides an excellent description of the Planck CMB observations and many other astrophysical data sets. Cosmological parameters. @article{Ade:2015xua, author = "Ade, P. A. R. and others", title = "{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. We show that these tensions cannot easily be resolved with simple modifications of the base ΛCDM cosmology. The addition of Planck polarization data leads to strong constraints on deviations from a purely adiabatic spectrum of fluctuations. Planck 2015 Results: Cosmological Parameter Tables January 19, 2015 Abstract These tables summarize the results of Planck 2015 parameter estimation exploration results. Planck 2015 results: XIII. We present the first results of polarization measurements with the Low Frequency Instrument at large angular scales. 1 We find no evidence for any departure from base ΛCDM in the neutrino sector of the theory; for example, combining Planck observations with other astrophysical data we find Neff = 3.15 ± 0.23 for the effective number of relativistic degrees of freedom, consistent with the value Neff = 3.046 of the Standard Model of particle physics. 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). Adding the BKP B-mode data to our analysis leads to a tighter constraint of r0.002 < 0.09 and disfavours inflationarymodels with a V(φ) φ2 potential. Title: 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. 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