Full-shape cosmology analysis of SDSS-III BOSS galaxy power spectrum using emulator-based halo model: a determination of
arXiv:2110.06969 · doi:10.1103/PhysRevD.105.083517
Abstract
We present the results obtained from the full-shape cosmology analysis of the redshift-space power spectra for 4 galaxy samples of the SDSS-III BOSS DR12 galaxy catalog over . For the theoretical template, we use an emulator that was built from an ensemble set of -body simulations, which enables fast and accurate computation of the redshift-space power spectrum of halos. Combining with the halo occupation distribution to model the halo-galaxy connection, we can compute the redshift-space power spectrum of BOSS-like galaxies in the flat CDM cosmology. In our cosmology inference, we use the power spectrum monopole, quadrupole and hexadecapole and include 7 nuisance parameters to model uncertainties in the halo-galaxy connection for each galaxy sample, but do not use any information on the abundance of galaxies. We demonstrate a validation of our analysis pipeline using the mock catalogs of BOSS-like galaxies, generated using different recipes of the halo-galaxy connection and including the assembly bias effect. Assuming weak priors on cosmological parameters, except for and , we show that our model well reproduces the BOSS power spectra. Including the power spectrum information up to , we find , , and , for the mode and 68\% credible interval, after marginalization over nuisance parameters. We find little improvement in the cosmological parameters beyond a maximum wavelength due to the shot noise domination and marginalization of the halo-galaxy connection parameters. Our results are consistent with the Planck CMB results within statistical uncertainties.
arXiv comment27 pages, 18 figures, accepted by Phys. Rev. D. The main results are replaced with the analysis of the updated measurement of BOSS DR12 power spectrum provided by Beutler & McDonald (2021, arXiv:2106.06324)
References in corpus (75)
- The Structure of Cold Dark Matter Halos
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- The Baryon Oscillation Spectroscopic Survey of SDSS-III
- Halo Models of Large Scale Structure
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Rank-normalization, folding, and localization: An improved for assessing convergence of MCMC
- X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
- Analytic model for galaxy and dark matter clustering
- Halo occupation numbers and galaxy bias
- MultiDark simulations: the story of dark matter halo concentrations and density profiles
- Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
- Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix
- The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
- Large-Scale Galaxy Bias
- KiDS-1000 Cosmology: Multi-probe weak gravitational lensing and spectroscopic galaxy clustering constraints
- Extragalactic Science, Cosmology and Galactic Archaeology with the Subaru Prime Focus Spectrograph (PFS)
- How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
- Cosmological Non-Linearities as an Effective Fluid
- The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
- One percent determination of the primordial deuterium abundance
- Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data
- COLOSSUS: A python toolkit for cosmology, large-scale structure, and dark matter halos
- The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
- Cosmological Parameters from the BOSS Galaxy Power Spectrum
- Spatial correlation function and pairwise velocity dispersion of galaxies: CDM models versus the Las Campanas Survey
- Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
- The effects of He I 10830 on helium abundance determinations
- A discriminating probe of gravity at cosmological scales
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
- A universal model for halo concentrations
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
- The WiggleZ Dark Energy Survey: Final data release and cosmological results
- The clustering of massive galaxies at z~0.5 from the first semester of BOSS data
- Halo Assembly Bias in Hierarchical Structure Formation
- An accurate physical model for halo concentrations
- The Subaru FMOS galaxy redshift survey (FastSound). IV. New constraint on gravity theory from redshift space distortions at
- Halo Occupation Distribution Modeling of Clustering of Luminous Red Galaxies
- Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
- A 2.5% measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Modeling the clustering and halo occupation distribution of BOSS-CMASS galaxies in the Final Data Release
- Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
- Generation of Vorticity and Velocity Dispersion by Orbit Crossing
- The BAO+BBN take on the Hubble tension
- Large-Scale Anisotropic Correlation Function of SDSS Luminous Red Galaxies
- 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
- Cosmological Redshift Distortion of Correlation Functions as a Probe of the Density Parameter and the Cosmological Constant
- The Weak Lensing Signal and the Clustering of BOSS Galaxies II: Astrophysical and Cosmological Constraints
- Cosmological perturbation theory at three-loop order
- On Detecting Halo Assembly Bias with Galaxy Populations
- BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
- Constraining the LRG Halo Occupation Distribution using Counts-in-Cylinders
- Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
- The Effect of Fiber Collisions on the Galaxy Power Spectrum Multipole
- Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
- Baryon Acoustic Oscillations in 2D II: Redshift-space halo clustering in N-body simulations
- Extensions to models of the galaxy-halo connection
- Accurate emulator for the redshift-space power spectrum of dark matter halos and its application to galaxy power spectrum
- Response function of the large-scale structure of the universe to the small scale inhomogeneities
- Post-collapse perturbation theory in 1D cosmology -- beyond shell-crossing
- Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
- Cosmic propagators at two-loop order
- Model-independent versus model-dependent interpretation of the SDSS-III BOSS power spectrum: Bridging the divide
- Wide-Field InfraRed Survey Telescope (WFIRST) Mission and Synergies with LISA and LIGO-Virgo
- Validating a minimal galaxy bias method for cosmological parameter inference using HSC-SDSS mock catalogs
- Lagrangian cosmological perturbation theory at shell-crossing
- Cosmological information content in redshift-space power spectrum of SDSS-like galaxies in the quasi-nonlinear regime up to Mpc
- Impacts of satellite galaxies on the redshift-space distortions
- Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
Cited by in corpus (55)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements
- Consistent lensing and clustering in a low- Universe with BOSS, DES Year 3, HSC Year 1 and KiDS-1000
- Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
- Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
- Stringent constraints from small-scale galaxy clustering using a hybrid MCMC+emulator framework
- BAO+BBN revisited -- Growing the Hubble tension with a 0.7km/s/Mpc constraint
- Going Beyond the Galaxy Power Spectrum: an Analysis of BOSS Data with Wavelet Scattering Transforms
- The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies
- Determining the Hubble Constant without the Sound Horizon: A Constraint on from Galaxy Surveys, CMB Lensing and Supernovae
- Growth of Cosmic Structure
- Quijote-PNG: Simulations of primordial non-Gaussianity and the information content of the matter field power spectrum and bispectrum
- Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
- The Bacco Simulation Project: Bacco Hybrid Lagrangian Bias Expansion Model in Redshift Space
- Tightening geometric and dynamical constraints on dark energy and gravity: galaxy clustering, intrinsic alignment and kinetic Sunyaev-Zel'dovich effect
- Machine Learning for Observational Cosmology
- Precise Cosmological Constraints from BOSS Galaxy Clustering with a Simulation-Based Emulator of the Wavelet Scattering Transform
- Cosmographic view on the and tensions
- : Mock Challenge for a Forward Modeling Approach to Galaxy Clustering
- A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
- A comparison of template vs. direct model fitting for redshift-space distortions in BOSS
- Cosmological inference from emulator based halo model I: Validation tests with HSC and SDSS mock catalogs
- Constraints on anisotropic primordial non-Gaussianity from intrinsic alignments of SDSS-III BOSS galaxies
- Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
- New constraints on cosmological modified gravity theories from anisotropic three-point correlation functions of BOSS DR12 galaxies
- Analysis of Unified Galaxy Power Spectrum Multipole Measurements
- Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
- Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and -body simulations
- Combined full shape analysis of BOSS galaxies and eBOSS quasars using an iterative emulator
- RSD measurements from BOSS galaxy power spectrum using the halo perturbation theory model
- Accelerating cosmological inference with Gaussian processes and neural networks -- an application to LSST Y1 weak lensing and galaxy clustering
- Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
- A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
- Accurate field-level weak lensing inference for precision cosmology
- Analysis method for 3D power spectrum of projected tensor field with fast estimator and window convolution modelling: an application to intrinsic alignments
- Galaxy clustering from the bottom up: A Streaming Model emulator I
- Shedding Light on Low Surface Brightness Galaxies in Dark Energy Survey with Transformers
- The Uchuu-GLAM BOSS and eBOSS LRG lightcones: Exploring clustering and covariance errors
- Cosmology with Galaxy Cluster Properties using Machine Learning
- Tracking the validity of the quasi-static and sub-horizon approximations in modified gravity
- Isolating the linear signal when making redshift space distortion measurements
- Impact of intrinsic alignments on clustering constraints of the growth rate
- Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
- Predictive uncertainty on improved astrophysics recovery from multifield cosmology
- Unraveling emission line galaxy conformity at z~1 with DESI early data
- Neutrino mass and kinetic gravity braiding degeneracies
- Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
- Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
- Constraining cosmology with N-body simulations for future spectroscopic galaxy surveys at
- Emulating galaxy and peculiar velocity clustering on non-linear scales
- Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order
- An emulation-based model for the projected correlation function
- The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
- An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
- Euclid preparation. 3D reconstruction of the cosmic web with simulated Euclid Deep spectroscopic samples