The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 LRG sample: structure growth rate measurement from the anisotropic LRG correlation function in the redshift range 0.6 < z < 1.0

Abstract

We analyze the anisotropic clustering of the Sloan Digital Sky Survey-IV Extended Baryon Oscillation Spectroscopic Survey (eBOSS) Luminous Red Galaxy Data Release 14 (DR14) sample combined with Baryon Oscillation Spectroscopic Survey (BOSS) CMASS sample of galaxies in the redshift range 0.6$<z<$1.0, which consists of 80,118 galaxies from eBOSS and 46,439 galaxies from the BOSS-CMASS sample. The eBOSS-CMASS Luminous Red Galaxy sample has a sky coverage of 1,844 deg${}^2$, with an effective volume of 0.9 Gpc${}^3$. The analysis was made in configuration space using a Legendre multipole expansion. The Redshift Space Distortion signal is modeled as a combination of the Convolution Lagrangian Perturbation Model and the Gaussian Streaming Model. We constrain the logarithmic growth of structure times the amplitude of dark matter density fluctuations, $f(z_{\mathrm{eff}}){\sigma }_8(z_{\mathrm{eff}})=0.454\pm 0.139$, and the Alcock-Paczynski dilation scales which constraints the angular diameter distance $D_A(z_{eff})=1466.5\pm 136.6(r_s/r_s^{\mathrm{fid}})$ and $H(z_{\mathrm{eff}})=105.8\pm 16(r_s^{\mathrm{fid}}/r_s)\mathrm{km}{\mathrm{s}}^{-1}\mathrm{Mp}{\mathrm{c}}^{-1}$, where $r_s$ is the sound horizon at the end of the baryon drag epoch and $r_s^{\mathrm{fid}}$ is its value in the fiducial cosmology at an effective redshift $z_{\mathrm{eff}}=0.72$. These results are in full agreement with the current $\Lambda$-Cold Dark Matter ($\Lambda$-CDM) cosmological model inferred from Planck measurements. This study is the first eBOSS LRG full-shape analysis i.e. including Redshift-Space Distortions (RSD) simultaneously with the Alcock-Paczynski (AP) effect and the Baryon Acoustic Oscillation (BAO) scale.

arXiv commentAccepted on the 5th December 2019, 28 pages,27 figures

References in corpus (53)

• Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
• Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
• The cosmological simulation code GADGET-2
• Efficient Computation of CMB anisotropies in closed FRW models
• Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
• f(R) Theories Of Gravity
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The 2.5 m Telescope of the Sloan Digital Sky Survey
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
• The Sloan Digital Sky Survey Photometric Camera
• Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
• Beyond the Cosmological Standard Model
• The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
• Power Spectrum Analysis of Three-Dimensional Redshift Surveys
• 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
• Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
• redMaPPer I: Algorithm and SDSS DR8 Catalog
• Cosmic Growth History and Expansion History
• A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
• The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment
• Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
• Measuring cosmological parameters with galaxy surveys
• Planck 2015 results. XVI. Isotropy and statistics of the CMB
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: measurements of the growth of structure and expansion rate at z=0.57 from anisotropic clustering
• Measuring the cosmological constant with redshift surveys
• The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function
• Baryon acoustic oscillations from the complete SDSS-III Ly$\alpha$-quasar cross-correlation function at $z=2.4$
• Towards an accurate model of the redshift space clustering of halos in the quasilinear regime
• Convolution Lagrangian perturbation theory for biased tracers
• EZmocks: extending the Zel'dovich approximation to generate mock galaxy catalogues with accurate clustering statistics
• Mock galaxy catalogs using the quick particle mesh method
• The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations at redshift of 0.72 with the DR14 Luminous Red Galaxy Sample
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range $0.8<z<2.2$
• Challenges to the DGP Model from Horizon-Scale Growth and Geometry
• Cosmological Constraints from Galaxy Clustering and the Mass-to-Number Ratio of Galaxy Clusters
• A 2% Distance to z=0.35 by Reconstructing Baryon Acoustic Oscillations - II: Fitting Techniques
• Clustering of luminous red galaxies I: large scale redshift space distortions
• Constraints onOmega from the IRAS Redshift Surveys
• The SDSS-IV extended Baryonic Oscillation Spectroscopic Survey: Luminous Red Galaxy Target Selection
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• An analytic model for redshift-space distortions
• Constraints on gravity and dark energy from the pairwise kinematic Sunyaev-Zeldovich effect
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
• The clustering of luminous red galaxies at z $\sim$ 0.7 from eBOSS and BOSS data
• Difficulties Distinguishing Dark Energy from Modified Gravity via Redshift Distortions
• CUTE solutions for two-point correlation functions from large cosmological datasets
• Testing General Relativity with Growth rate measurement from Sloan Digital Sky Survey III Baryon Oscillations Spectroscopic Survey galaxies
• SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of Potential Systematics in Fitting of Baryon Acoustic Feature

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• 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
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• Is there evidence for a hotter Universe?
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• A new test of gravity -- I: Introduction to the method
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• Novel Cosmological Joint Constraints in Multidimensional Observables Space with Redshift-free Inferences
• The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids
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• Prospects for measuring the Doppler magnification dipole with LSST and DESI
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Perturbations In Some Dark Energy Models