Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory

Abstract

We present a formalism for jointly fitting pre- and post-reconstruction redshift-space clustering (RSD) and baryon acoustic oscillations (BAO) plus gravitational lensing (of the CMB) that works directly with the observed 2-point statistics. The formalism is based upon (effective) Lagrangian perturbation theory and a Lagrangian bias expansion, which models RSD, BAO and galaxy-lensing cross correlations within a consistent dynamical framework. As an example we present an analysis of clustering measured by the Baryon Oscillation Spectroscopic Survey in combination with CMB lensing measured by Planck. The post-reconstruction BAO strongly constrains the distance-redshift relation, the full-shape redshift-space clustering constrains the matter density and growth rate, and CMB lensing constrains the clustering amplitude. Using only the redshift space data we obtain ${\Omega }_{\mathrm{m}}=0.303\pm 0.008$, $H_0=69.21\pm 0.78$ and ${\sigma }_8=0.743\pm 0.043$. The addition of lensing information, even when restricted to the Northern Galactic Cap, improves constraints to ${\Omega }_m=0.300\pm 0.008$, $H_0=69.21\pm 0.77$ and ${\sigma }_8=0.707\pm 0.035$, in tension with CMB and cosmic shear constraints. The combination of ${\Omega }_m$ and $H_0$ are consistent with Planck, though their constraints derive mostly from redshift-space clustering. The low ${\sigma }_8$ value are driven by cross correlations with CMB lensing in the low redshift bin ($z\simeq 0.38$) and at large angular scales, which show a $20\%$ deficit compared to expectations from galaxy clustering alone. We conduct several systematics tests on the data and find none that could fully explain these tensions.

arXiv comment46 pages, 15 figures, updated to match version accepted by JCAP

References in corpus (117)

• Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
• Planck 2015 results. XIII. Cosmological parameters
• HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere
• Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
• Efficient Computation of CMB anisotropies in closed FRW models
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• Baryonic Features in the Matter Transfer Function
• SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
• Stable clustering, the halo model and nonlinear cosmological power spectra
• The Baryon Oscillation Spectroscopic Survey of SDSS-III
• Large-Scale Structure of the Universe and Cosmological Perturbation Theory
• Planck 2018 results. I. Overview and the cosmological legacy of Planck
• Observational Probes of Cosmic Acceleration
• The DESI Experiment Part I: Science,Targeting, and Survey Design
• Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
• Revising the Halofit Model for the Nonlinear Matter Power Spectrum
• Large-Scale Galaxy Bias
• Planck 2018 results. VIII. Gravitational lensing
• MASTER of the CMB Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex CMB Data Sets
• Cobaya: Code for Bayesian Analysis of hierarchical physical models
• CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
• Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• Nonlinear Evolution of Baryon Acoustic Oscillations
• The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• Dark Energy vs. Modified Gravity
• On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Data Calibration
• Cosmological Parameters from the BOSS Galaxy Power Spectrum
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• A unified pseudo-$C_{\ell }$ framework
• A discriminating probe of gravity at cosmological scales
• Dark Energy Survey Year 3 Results: Cosmology from Cosmic Shear and Robustness to Modeling Uncertainty
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
• SPT-3G: A Next-Generation Cosmic Microwave Background Polarization Experiment on the South Pole Telescope
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function
• Baryonic Signatures in Large-Scale Structure
• The Atacama Cosmology Telescope: The polarization-sensitive ACTPol instrument
• Convolution Lagrangian perturbation theory for biased tracers
• The clustering of intermediate redshift quasars as measured by the Baryon Oscillation Spectroscopic Survey
• Bias in the Effective Field Theory of Large Scale Structures
• Corrfunc --- A Suite of Blazing Fast Correlation Functions on the CPU
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
• Redshift evolution of clustering
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
• Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• A Lagrangian effective field theory
• Reconstructing Baryon Oscillations: A Lagrangian Theory Perspective
• A new, large-scale map of interstellar reddening derived from HI emission
• Redshift-Space Distortions in Lagrangian Perturbation Theory
• An algorithm for the direct reconstruction of the dark matter correlation function from weak lensing and galaxy clustering
• Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory
• Extragalactic Foreground Contamination in Temperature-based CMB Lens Reconstruction
• CMB Lensing Power Spectrum Biases from Galaxies and Clusters using High-angular Resolution Temperature Maps
• Constraining Anisotropic Baryon Oscillations
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• The Atacama Cosmology Telescope: A CMB lensing mass map over 2100 square degrees of sky and its cross-correlation with BOSS-CMASS galaxies
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a $5\%$ determination of ${\sigma }_8$
• The Gaussian streaming model and Lagrangian effective field theory
• Reconstruction within the Zeldovich approximation
• An optimal FFT-based anisotropic power spectrum estimator
• BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
• Cubic Halo Bias in Eulerian and Lagrangian Space
• The cosmology dependence of galaxy clustering and lensing from a hybrid $N$-body-perturbation theory model
• Precision analysis of the redshift-space galaxy bispectrum
• The growth of density perturbations in the last $\sim$10 billion years from tomographic large-scale structure data
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: theoretical systematics and Baryon Acoustic Oscillations in the galaxy correlation function
• Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
• Modeling the reconstructed BAO in Fourier space
• Simulations and symmetries
• Beyond LIMD bias: a measurement of the complete set of third-order halo bias parameters
• Third-Order Density Perturbation and One-Loop Power Spectrum in Dark-Energy-Dominated Universe
• Testing the theory of gravity with DESI: estimators, predictions and simulation requirements
• unWISE tomography of Planck CMB lensing
• Constraining Gravity at the Largest Scales through CMB Lensing and Galaxy Velocities
• Dark Energy Survey Year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space
• Constraints on the correlation between QSO luminosity and host halo mass from high-redshift quasar clustering
• Cross-correlating Planck CMB lensing with SDSS: Lensing-lensing and galaxy-lensing cross-correlations
• Cosmological constraints from the power spectrum of eBOSS emission line galaxies
• Tidal alignments as a contaminant of redshift space distortions
• Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ
• KiDS-1000: cosmic shear with enhanced redshift calibration
• Cosmological constraints from galaxy-lensing cross correlations using BOSS galaxies with SDSS and CMB lensing
• The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
• Dark Energy Survey Year 1 Results: Methodology and Projections for Joint Analysis of Galaxy Clustering, Galaxy Lensing, and CMB Lensing Two-point Functions
• Non-linear Fields in Generalized Cosmologies
• Hefty enhancement of cosmological constraints from the DES Y1 data using a Hybrid Effective Field Theory approach to galaxy bias
• Probing gravity with a joint analysis of galaxy and CMB lensing and SDSS spectroscopy
• Modeling CMB Lensing Cross Correlations with {\sc CLEFT}
• Biased Tracers in Redshift Space in the EFTofLSS with exact time dependence
• The matter power spectrum in redshift space using effective field theory
• Cosmological constraints from a joint analysis of cosmic microwave background and spectroscopic tracers of the large-scale structure
• ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
• Dark Energy Survey Year 3 results: cosmology from combined galaxy clustering and lensing -- validation on cosmological simulations
• Detection of anisotropic galaxy assembly bias in BOSS DR12
• The Reconstructed Power Spectrum in the Zeldovich Approximation
• Cross-Correlation of Planck CMB Lensing with DESI-Like LRGs
• Priors on red galaxy stochasticity from hybrid effective field theory
• Optimal Redshift Weighting For Baryon Acoustic Oscillations
• Perturbative description of bias tracers using consistency relations of LSS
• Magnification bias in galaxy surveys with complex sample selection functions
• Beware of Fake $\nu$s: The Effect of Massive Neutrinos on the Nonlinear Evolution of Cosmic Structure
• The effect of FIR emission from SDSS galaxies on the SFD Galactic extinction map
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Optimal multifrequency weighting for CMB lensing
• Towards Neutrino Mass from Cosmology without Optical Depth Information
• The galaxy power spectrum on the lightcone: deep, wide-angle redshift surveys and the turnover scale
• Neural Network Acceleration of Large-scale Structure Theory Calculations

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• A non-linear solution to the $S_8$ tension?
• Evidence for suppression of structure growth in the concordance cosmological model
• Cosmology with the EFTofLSS and BOSS: dark energy constraints and a note on priors
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• The Sigma-8 Tension is a Drag
• DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
• Going Beyond the Galaxy Power Spectrum: an Analysis of BOSS Data with Wavelet Scattering Transforms
• Unveiling dark fifth forces with linear cosmology
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• Growth of Cosmic Structure
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• The Atacama Cosmology Telescope DR6 and DESI: Structure formation over cosmic time with a measurement of the cross-correlation of CMB Lensing and Luminous Red Galaxies
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Cold New Early Dark Energy pulls the trigger on the $H_0$ and $S_8$ tensions: a simultaneous solution to both tensions without new ingredients
• Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
• Constraining primordial non-Gaussianity from DESI quasar targets and Planck CMB lensing
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Robust Evidence for Dynamical Dark Energy from DESI Galaxy-CMB Lensing Cross-Correlation and Geometric Probes
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
• Magnification Bias Estimators for Realistic Surveys: an Application to the BOSS Survey
• Constraining gravity with a new precision $E_G$ estimator using Planck + SDSS BOSS
• Perturbation theory of LSS in the $\Lambda$CDM Universe: exact time evolution and the two-loop power spectrum
• Cosmology before noon with multiple galaxy populations
• The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman-$\alpha$ Forest
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• Stellar Reddening Based Extinction Maps for Cosmological Applications
• CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering
• Combining cosmic shear data with correlated photo-$z$ uncertainties: constraints from DESY1 and HSC-DR1
• Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• AMICO galaxy clusters in KiDS-DR3: constraints on $\Lambda$CDM from extreme value statistics
• Cosmological perturbation theory for large scale structure in phase space
• Cosmological perturbation theory using generalized Einstein de Sitter cosmologies
• Parameterization of Stochasticity in Galaxy Clustering and Reconstruction of Tomographic Matter Clustering
• Mitigation of nonlinear galaxy bias with a theoretical-error likelihood
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order
• Probing gravity with non-linear clustering in redshift space
• The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes