planck lensing 2013

Planck was turned off on 23 October 2013. XXIV. • Planck strengths: large and redundent sky coverage, number of channels & detectors, low detector noise (25 x better than WMAP). 2% and 143 and 217 GHz, and 0 . Clearly the large scale observations are actually "features" now, no longer "anomalies". Here we present the minimum-variance (MV) lens reconstruction which forms the basis for the main results of Planck-2013-XVII. Planck: Gravitational Lensing of the CMB Planck measures the lensing of the CMB by intervening matter, detecting the effect at greater than 25 sigma. L. Perotto /12 47th ESLAB, 2013- 04-05, ESTEC Conclusions • integrated mass distribution on almost the full-sky using Planck (observational performancies + high systematic control in the data-processing) • Our fiducial lensing is based on a fsky 70% MV combination of the 143 and 217GHz Gravitational lensing by large-scale structure 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). Here we present a detailed study of this effect, detecting lensing independently in the 100, 143, and 217 GHz frequency bands with an overall significance of greater than 25 sigma. PR2 is described in the Planck 2015 Release Explanatory Supplement which is available via the ESA Planck Legacy Archive wiki page. 8% at 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). Planck Public Data Release 1 (PR1) Mission Ancillary Data. Title: Planck 2013 results. Planck 2013 Results. Fig.5. VII (2013), it is estimated in Planck Collaboration XVII (2013) that beam uncertainty leads to an e ff ective normalization uncer- tainty of approximately 0 . This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. The Universe after Planck 2013 Martin BUCHER, Laboratoire Astroparticles & Cosmologie, Université Paris 7 (Denis-Diderot) for the PLANCK Collaboration 16 May 2013, IST Lisboa. (2013). ... +lensing +lensing+BAO 40 45 50 55 60 65 70 75 H 0 The 0.06% precision measurement of the sound horizon scale at last scattering We find good consistency between lensing constraints and the results from the Planck CMB power spectra within the ΛCDM model. In my previous post, I mentioned CMB lensing and said that it was going to be a big thing. Here's the 2013 rendition of the cosmological Mona Lisa, or, in our jargon, the multipole expansion of the Cosmic Microwave Background (CMB) power spectrum. ), "Planck HFI Calibration and Map-Making", There are also aspects of the Planck analysis for which velocity e ects are believed to be negligible, but only if they are present at the expected level. Highlights from Planck 2013 cosmological results Paolo Natoli Università di Ferrara and ASI/ASDC DSU2013, Sissa, 17 October 2013 On behalf of the Planck collaboration . The constraints can be improved by 2%{15% if we further add the Planck lensing data into the analysis. If you want to work on the edit constructively, please join in. XVII. Planck lensing potential reconstruction (north and south galactic) Note –about half signal, half noise, not all structures are real map is effectively Wiener filtered. XVII. Constraints on primordial non-Gaussianity ... Sachs-Wolfe lensing bispectrum expected in the CDM scenrio.a The results rea based on comprehensive cross-validation of these estimators on Gaussian and non-Gaussian simulations, rea stable On the arcminute angular scales probed by Planck, the cosmic microwave background (CMB) anisotropies are gently perturbed by gravitational lensing. This is being recognized, and Planck is the key to all of this, so please do not try and take this observation away from Planck. Some are replaced by newer products from PR2 (2015 release), see the PR2 Ancillary Data page. 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. Here we present a detailed study of this effect, detecting lensing independently in the 100, 143, and 217 GHz frequency bands with an overall significance of greater than 25σ. 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. The Planck Public Data Release 2 (PR2) products are based on the complete mission which comprises data acquired between 13 August 2009 and 3 August 2013. The Planck lensing potential. 25.03.2013 Planck implications for cosmology – J. Lesgourgues 4 PLANCK LFI HFI Center Freq (GHz) 30 44 70 100 143 217 353 545 857 Topics: gravitational lensing: weak, cosmic background radiation, large-scale structure of Universe, dark matter, galaxies: star formation, STAR-FORMING GALAXIES, SOUTH-POLE TELESCOPE, PRE-LAUNCH STATUS, ANISOTROPY POWER SPECTRUM, SENSITIVITY HI SURVEY, DARK-MATTER HALOES, FINAL DATA RELEASE, DUST EMISSION, FORMATION HISTORY, DISTANT … Underlying question: conventional parameterization JCAP09(2013)021 0:594 0:051, and 0:642 0:066, respectively. Outline ... Planck Gravitational lensing spectrum. Note: This page lists products from PR1 (2013 release). This map is produced using a combination of the 143 and 217 GHz Planck maps on approximately 70% of the sky, and is the same map on which the Planck lensing likelihood is based. 72.46.228.155 ( talk ) 20:58, 17 April 2013 (UTC) On the arcminute angular scales probed by Planck, the cosmic microwave background (CMB) anisotropies are gently perturbed by gravitational lensing. The french magazine La Recherche announced that this year's astrophysics prize is awarded to the Planck article on gravitational lensing by large-scale structure, for the first full sky reconstruction of the CMB lensing effect. The Planck results for base LambdaCDM are in good agreement with baryon acoustic oscillation data and with the JLA sample of Type Ia supernovae. Compared to previous experiments, what distinguishes Planck is that it measures the power spectrum all the way from the largest angular scales down to less than 0.1 degrees. Papers II to X in the series describe the huge dataset obtained from the Planck satellite and released in March 2013. Planck has increased resolution and sensitivity compared to WMAP, and it observes in 9 bands instead of just 5. Top: Planck spectra at 100, 143 and 217GHz without subtraction of foregrounds. And indeed, CMB lensing has been presented as one of the main scientific results of the recent data release from the Planck Collaboration. Astronomical Data Analysis : "CMB Lensing Reconstruction on Planck Simulated Data" 2009 2010 Identification of Dark Matter : "Neutrino matter with PLANCK" 2011 2012 Rencontres de Blois : "Planck CMB results" 2013 ESLAB 2013 : "Planck polarization at small angular scales" (pl. 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. gravitational lensing universal pressure assumed equal of maxBCG stacks profile of Arnaud (2010) Planck Collaboration 2011: PEP-XII Yet when sample is restricted to Rozo et al 2009 clusters which also appear in an X-ray selected sample, the discrepancy disappears Malmquist bias transferred from We use the temperature-gradient correlations induced by lensing … Planck is an ESA mission with significant NASA involvement. Combined with baryon density and other weak priors, the lensing analysis alone constrains σ8Ωm0.25 = 0.589 ± 0.020 (1σ errors). Lensing map . Planck lensing power spectrum. If you want to read more about Planck, this is the official page, and this is the list of papers submitted as part of the 2013 release. The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of dark matter (via the lensing effect on the cosmic microwave background, or CMB). 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 universe content from Planck 2013 The Cosmic Microwave Background The Planck mission Implications for cosmology Cosmological perturbations theory The universe content from Planck 2013 A new observable: the lensing potential The early universe after Planck Cosmic Inflation Scalar fields Looking for the inflaton Some smoke in the Gravitational lensing creates tiny, additional distortions to the mottled pattern of the CMB temperature fluctuations. We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the full Planck survey, which includes more than twice the integration time of the nominal survey used for the 2013 release papers. We present cosmological parameter constraints based on a joint modeling of galaxy-lensing cross correlations and galaxy clustering measurements in the SDSS, marginalizing over small-scale modeling uncertainties using mock galaxy catalogs, without explicit modeling of galaxy bias. 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. Resolution intermediate between WMAP (3 x better) and ACT, SPT. Middle: SPT spectra from R12 at 95, 150 and 220GHz, recalibrated to Planck using the best-fit calibration, as discussed in the text. We distribute: PHIBAR In their research, Geach and colleagues analysed the latest gravitational lensing map obtained by the Planck team, made public as part of the Planck Legacy Release in 2018, in combination with 200 000 quasars drawn from the largest sample ever compiled, the more than half-a-million quasars that comprise Data Release 14 of the Sloan Digital Sky Survey quasar catalogue. (2013); statistical anisotropy of the primordial CMB fluctua-tions, as discussed inPlanck Collaboration XXIII(2013); and gravitational lensing, as discussed inPlanck Collaboration XVII (2013). Planck 2013 results. From PR2 ( 2015 release ), see the PR2 Ancillary data gravitational lensing forms basis! Please join in release from the Planck results for base LambdaCDM are in agreement. 2013 ) 021 0:594 0:051, and 0 agreement with baryon density and other weak priors, the microwave! ) Planck Public data release 1 ( PR1 ) mission Ancillary data the analysis said that it going. 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