Planck 2015 results. XXI. The integrated Sachs-Wolfe effect

Abstract

This paper presents a study of the ISW effect from the Planck 2015 temperature and polarization data release. The CMB is cross-correlated with different LSS tracers: the NVSS, SDSS and WISE catalogues, and the Planck 2015 lensing map. This cross-correlation yields a detection at $4\sigma$, where most of the signal-to-noise is due to the Planck lensing and NVSS. In fact, the ISW effect is detected only from the Planck data (through the ISW-lensing bispectrum) at $\approx 3\sigma$, which is similar to the detection level achieved by combining the cross-correlation signal coming from all the catalogues. The ISW signal allow us to detect ${\Omega }_{\Lambda }$ at more than $3\sigma$. This cross-correlation analysis is performed only with the Planck temperature data, since the polarization scales available in the 2015 release do not permit significant improvement of the CMB-LSS cross-correlation detectability. Nevertheless, polarization data is used to study the anomalously large ISW signal previously reported through the stacking of CMB features at the locations of known superstructures. We find that the current Planck polarization data do not exclude that this signal could be caused by the ISW effect. In addition, the stacking of the Planck lensing map on the locations of superstructures exhibits a positive cross-correlation with these large-scale structures. Finally, we have improved our previous reconstruction of the ISW temperature fluctuations by combining the information encoded in all the previously mentioned LSS tracers. In particular, we construct a map of the ISW secondary anisotropies and the corresponding uncertainties map, obtained from simulations. We also explore the reconstruction of the ISW anisotropies caused by the LSS traced by the 2MPZ survey by directly inverting the density field into the gravitational potential field.

34 pages, 24 figures, abstract abridged for arXiv. This paper is one of a set associated with the 2015 data release from Planck. Final version, accepted for publication in A&A

References in corpus (51)

• Planck 2015 results. XIII. Cosmological parameters
• Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters
• Planck 2015 results. XVII. Constraints on primordial non-Gaussianity
• Planck 2015 results. XXIV. Cosmology from Sunyaev-Zeldovich cluster counts
• Planck 2015 results. XVI. Isotropy and statistics of the CMB
• Planck 2015 results. XIV. Dark energy and modified gravity
• ZOBOV: a parameter-free void-finding algorithm
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectra
• Correlation of CMB with large-scale structure: I. ISW Tomography and Cosmological Implications
• Planck 2015 results. XXVII. The Second Planck Catalogue of Sunyaev-Zeldovich Sources
• An Imprint of Super-Structures on the Microwave Background due to the Integrated Sachs-Wolfe Effect
• Planck 2015 results. XV. Gravitational lensing
• Planck 2015 results. X. Diffuse component separation: Foreground maps
• Planck 2015 results. IX. Diffuse component separation: CMB maps
• Planck 2015 results. VIII. High Frequency Instrument data processing: Calibration and maps
• Detection of the ISW and SZ effects from the CMB-Galaxy correlation
• Planck 2015 results. XXI. The integrated Sachs-Wolfe effect
• Planck 2015 results. XXII. A map of the thermal Sunyaev-Zeldovich effect
• Planck 2015 results. XIX. Constraints on primordial magnetic fields
• A high redshift detection of the integrated Sachs-Wolfe effect
• Probing modifications of General Relativity using current cosmological observations
• Planck 2015 results. XXVI. The Second Planck Catalogue of Compact Sources
• Planck 2015 results. XXIII. The thermal Sunyaev-Zeldovich effect--cosmic infrared background correlation
• Constraining dark energy with cross-correlated CMB and Large Scale Structure data
• The significance of the integrated Sachs-Wolfe effect revisited
• Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds
• Planck 2015 results. XXVIII. The Planck Catalogue of Galactic Cold Clumps
• Planck 2015 results. IV. Low Frequency Instrument beams and window functions
• Planck 2015 results. III. LFI systematic uncertainties
• Error analysis in cross-correlation of sky maps: application to the ISW detection
• Planck 2015 results. V. LFI calibration
• Detection of the ISW effect and corresponding dark energy constraints
• Detection of the ISW effect and corresponding dark energy constraints made with directional spherical wavelets
• Cross-correlation of 2MASS and WMAP3: Implications for the Integrated Sachs-Wolfe effect
• Planck 2015 results. XVIII. Background geometry & topology
• Planck 2015 results. XII. Full Focal Plane simulations
• VOBOZ: An Almost-Parameter-Free Halo-Finding Algorithm
• Planck 2015 results. VII. HFI TOI and beam processing
• Impact of Secondary non-Gaussianities on the Search for Primordial Non-Gaussianity with CMB Maps
• Planck 2015 results. II. Low Frequency Instrument data processing
• The High Redshift Integrated Sachs-Wolfe Effect
• Planck 2015 results. VI. LFI mapmaking
• The Jubilee ISW Project II: observed and simulated imprints of voids and superclusters on the cosmic microwave background
• Mapping the Integrated Sachs-Wolfe Effect
• Cold imprint of supervoids in the Cosmic Microwave Background re-considered with Planck and BOSS DR10
• Optimal ISW detection and joint likelihood for cosmological parameter estimation
• A linear filter to reconstruct the ISW effect from CMB and LSS observations
• Constraints on Dark Energy Parameters from Correlations of CMB with LSS
• Dark Energy Detected with Supervoids and Superclusters
• On the recovery of ISW fluctuations using large-scale structure tracers and CMB temperature and polarization anisotropies
• Measuring dark energy with the integrated Sachs-Wolfe effect

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• Imitating intrinsic alignments: A bias to the CMB lensing-galaxy shape cross-correlation power spectrum induced by the large-scale structure bispectrum
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• Impact of SZ cluster residuals in CMB maps and CMB-LSS cross-correlations
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• Perturbation level interacting dark energy model and its consequence on late-time cosmological parameters
• Reconstructing FHDE with Scalar and Gauge Fields
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• Ray tracing the integrated Sachs-Wolfe effect through the light cones of the Dark Energy Universe Simulation -- Full Universe Runs
• Galaxy cluster mass density profile derived using the submillimetre galaxies magnification bias
• ISW in $\Lambda$CDM or something else?
• The CMB lensing imprint of cosmic voids detected in the WISE-Pan-STARRS luminous red galaxy catalog
• Accurate estimation of angular power spectra for maps with correlated masks
• Constraining deceleration, jerk and transition redshift using cosmic chronometers, Type Ia supernovae and ISW effect
• Full sky Integrated Sachs-Wolfe maps for the MICE Grand Challenge lightcone simulation
• Dynamics of cosmological perturbations in modified Brans-Dicke cosmology with matter-scalar field interaction
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