Forecasting Cosmological Constraints from Redshift Surveys

Abstract

Observations of redshift-space distortions in spectroscopic galaxy surveys offer an attractive method for observing the build-up of cosmological structure, which depends both on the expansion rate of the Universe and our theory of gravity. In this paper we present a formalism for forecasting the constraints on the growth of structure which would arise in an idealized survey. This Fisher matrix based formalism can be used to study the power and aid in the design of future surveys.

7 pages, 5 figures, minor revisions to match version accepted by MNRAS

References in corpus (12)

• Cosmological Constraints from the SDSS Luminous Red Galaxies
• A test of the nature of cosmic acceleration using galaxy redshift distortions
• Fingers of God
• Testing cosmological structure formation using redshift-space distortions
• Observational Tests of Modified Gravity
• The 2dF-SDSS LRG and QSO Survey: QSO clustering and the L-z degeneracy
• Testing LCDM with the Growth Function δ(a): Current Constraints
• Large-Scale Anisotropic Correlation Function of SDSS Luminous Red Galaxies
• The Vimos VLT Deep Survey: Stellar mass segregation and large-scale galaxy environment in the redshift range 0.2<z<1.4
• The Vimos VLT Deep Survey: Global properties of 20000 galaxies in the I_AB<=22.5 WIDE survey
• Simulations of Baryon Oscillations
• Velocity distributions in clusters of galaxies

Cited by in corpus (145)

• SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems
• Observational Probes of Cosmic Acceleration
• The linear power spectrum of observed source number counts
• The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
• Holographic Dark Energy
• 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
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• The VIMOS Public Extragalactic Redshift Survey (VIPERS). An unprecedented view of galaxies and large-scale structure at 0.5<z<1.2
• Late-time cosmology with 21cm intensity mapping experiments
• The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
• A Lower Growth Rate from Recent Redshift Space Distortion Measurements than Expected from Planck
• How to measure redshift-space distortions without sample variance
• Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure
• Towards an accurate model of the redshift space clustering of halos in the quasilinear regime
• Growth of Cosmic Structure: Probing Dark Energy Beyond Expansion
• Modelling redshift space distortions in hierarchical cosmologies
• Coupled dark matter-dark energy in light of near Universe observations
• Redshift space correlations and scale-dependent stochastic biasing of density peaks
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
• Velocities as a probe of dark sector interactions
• Are peculiar velocity surveys competitive as a cosmological probe?
• The significance of the integrated Sachs-Wolfe effect revisited
• An analytic model for redshift-space distortions
• The WiggleZ Dark Energy Survey: the selection function and z=0.6 galaxy power spectrum
• The extended Baryon Oscillation Spectroscopic Survey (eBOSS): a cosmological forecast
• Gravitational redshift and other redshift-space distortions of the imaginary part of the power spectrum
• Distribution function approach to redshift space distortions
• Findings of the Joint Dark Energy Mission Figure of Merit Science Working Group
• Why multi-tracer surveys beat cosmic variance
• Recovering 3D clustering information with angular correlations
• Designing a space-based galaxy redshift survey to probe dark energy
• Complementarity of Weak Lensing and Peculiar Velocity Measurements in Testing General Relativity
• Consistency test of general relativity from large scale structure of the Universe
• Covariance of cross-correlations: towards efficient measures for large-scale structure
• Probing primordial features with future galaxy surveys
• Cross-Correlation of spectroscopic and photometric galaxy surveys: cosmology from lensing and redshift distortions
• Systematic Effects on Determination of the Growth Factor from Redshift-space Distortions
• Erasing the Milky Way: new cleaning technique applied to GBT intensity mapping data
• Distribution function approach to redshift space distortions. Part IV: perturbation theory applied to dark matter
• Large Scale Structures in Kinetic Gravity Braiding Model That Can Be Unbraided
• Deconstructing the neutrino mass constraint from galaxy redshift surveys
• Where are the Luminous Red Galaxies (LRGs)? Using correlation measurements and lensing to relate LRGs to dark matter halos
• Tests of redshift-space distortions models in configuration space for the analysis of the BOSS final data release
• HI and cosmological constraints from intensity mapping, optical, and CMB surveys
• Difficulties Distinguishing Dark Energy from Modified Gravity via Redshift Distortions
• Distribution function approach to redshift space distortions, Part III: halos and galaxies
• Mapping the Real Space Distributions of Galaxies in SDSS DR7: II. Measuring the growth rate, clustering amplitude of matter and biases of galaxies at redshift $0.1$
• Forecasting the Cosmological Constraints with Anisotropic Baryon Acoustic Oscillations from Multipole Expansion
• The potential of X-ray cluster surveys to constrain primordial non-Gaussianity
• Cosmological Parameters Degeneracies and Non-Gaussian Halo Bias
• The velocity field of 2MRS Ks=11.75 galaxies: constraints on beta and bulk flow from the luminosity function
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys. II. Dark Matter Velocity Statistics
• Scale-Dependent Galaxy Bias from Massive Particles with Spin during Inflation
• Distribution function approach to redshift space distortions. Part V: perturbation theory applied to dark matter halos
• The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: a multi-tracer analysis in Fourier space for measuring the cosmic structure growth and expansion rate
• The kinetic SZ tomography with spectroscopic redshift surveys
• Cosmology without cosmic variance
• Combining weak lensing tomography and spectroscopic redshift surveys
• Improving the modelling of redshift-space distortions: I. A bivariate Gaussian description for the galaxy pairwise velocity distributions
• Cosmology with dropout selection: Straw-man surveys and CMB lensing
• Modeling CMB Lensing Cross Correlations with {\sc CLEFT}
• Peculiar Velocity Decomposition, Redshift Space Distortion and Velocity Reconstruction in Redshift Surveys - I. The Methodology
• Effects of cosmological model assumptions on galaxy redshift survey measurements
• Fourier analysis of multi-tracer cosmological surveys
• Constraint on the cosmological f(R) model from the multipole power spectrum of the SDSS luminous red galaxy sample and prospects for a future redshift survey
• Galaxy power spectrum in redshift space: combining perturbation theory with the halo model
• Constraints on growth index parameters from current and future observations
• Measuring Redshift-Space Distortions using Photometric Surveys
• Consistent Modified Gravity Analysis of Anisotropic Galaxy Clustering Using BOSS DR11
• Probing deviations from General Relativity with the Euclid spectroscopic survey
• Cosmology with anisotropic galaxy clustering from the combination of power spectrum and bispectrum
• A step towards testing general relativity using weak gravitational lensing and redshift surveys
• Cosmology with clustering anisotropies: disentangling dynamic and geometric distortions in galaxy redshift surveys
• Power spectrum multipoles on the curved sky: an application to the 6-degree Field Galaxy Survey
• Statistical and systematic errors in redshift-space distortion measurements from large surveys
• Optimal Weighting in Galaxy Surveys: Application to Redshift-Space Distortions
• The Redshift-Space Momentum Power Spectrum I: Optimal Estimation From Peculiar Velocity Surveys
• Using galaxy-galaxy weak lensing measurements to correct the Finger-of-God
• The full Fisher matrix for galaxy surveys
• A New Statistic for Analyzing Baryon Acoustic Oscillations
• Measuring the growth of structure with intensity mapping surveys
• Testing for dynamical dark energy models with redshift-space distortions
• Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
• How to Falsify the GR+LambdaCDM Model with Galaxy Redshift Surveys
• The BOSS-WiggleZ overlap region II: dependence of cosmic growth on galaxy type
• Relativistic corrections and non-Gaussianity in radio continuum surveys
• The Gigaparsec WiggleZ Simulations: Characterising scale dependant bias and associated systematics in growth of structure measurements
• J-PAS: forecasts on dark energy and modified gravity theories
• On the streaming model for redshift-space distortions
• Study on the mapping of dark matter clustering from real space to redshift space
• Measuring Coherent Motions in the Universe
• The Clustering of Galaxies in the Completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmic Flows and Cosmic Web from Luminous Red Galaxies
• Cosmological lensing ratios with DES Y1, SPT and Planck
• Synergies between radio, optical and microwave observations at high redshift
• Galaxy Peculiar Velocities From Large-Scale Supernova Surveys as a Dark Energy Probe
• Bayesian cosmic density field inference from redshift space dark matter maps
• Likelihood reconstruction method of real-space density and velocity power spectra from a redshift galaxy survey
• Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum
• Redshift-space distortions from the cross-correlation of photometric populations
• Measurement of Redshift Space Power Spectrum for BOSS galaxies and the Growth Rate at redshift 0.57
• Characterizing unknown systematics in large scale structure surveys
• Radiative Transfer Distortions of Lyman-$\alpha$ Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space
• Decomposition of Spectra from Redshift Distortion Maps
• Extracting the late-time kinetic Sunyaev-Zel'dovich effect
• A brief review on cosmological analysis of galaxy surveys with multiple tracers
• The Complementarity of Redshift-space Distortions and the Integrated Sachs-Wolfe Effect: A 3D Spherical Analysis
• The 6x2pt method: supernova velocities meet multiple tracers
• Large-scale Velocities and Primordial Non-Gaussianity
• Broadband Alcock-Paczynski test exploiting redshift distortions
• Future constraints on the Hu-Sawicki modified gravity scenario
• Cosmology before noon with multiple galaxy populations
• Bayesian redshift-space distortions correction from galaxy redshift surveys
• Measuring BAO and non-Gaussianity via QSO clustering
• Describing variations of the Fisher-matrix across parameter space
• A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
• Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
• Testing Standard Cosmology with Large Scale Structure
• Redshift space distortions in the presence of non-minimally coupled dark matter
• Fisher matrix for multiple tracers: model independent constraints on the redshift distortion parameter
• Forecasts for interacting dark energy with time-dependent momentum exchange
• Shot noise in multi-tracer constraints on $f_{\text{NL}}$ and relativistic projections: Power Spectrum
• Cosmological Fisher forecasts for next-generation spectroscopic surveys
• Coherent Combination of Baryon Acoustic Oscillation Statistics and Peculiar Velocity Measurements from Redshift Survey
• Cosmological constraints from multiple tracers in spectroscopic surveys
• Study on the mapping of halo clustering from real space to redshift space
• Simultaneous constraints on bias, normalization and growth index through power spectrum measurements
• The exact analytical solution of the linear structure growth rate in LCDM cosmology and its cosmological applications
• The Fisher gAlaxy suRvey cOde ($\text{FARO}$)
• Power Spectrum Precision for Redshift Space Distortions
• Multi-wavelength consensus of large-scale linear bias
• Reconstructing the Thermal Sunyaev-Zel'dovich Effect in 3D
• Fisher forecast for the BAO measurements from the CSST spectroscopic and photometric galaxy clustering
• Cosmic Growth Signatures of Modified Gravitational Strength
• Chasing Unbiased Spectra of the Universe
• Fisher matrix for multiple tracers: all you can learn from large-scale structure without assuming a model
• Constraining primordial non-Gaussianity by combining photometric galaxy and 21cm intensity mapping surveys
• Multi-tracing the primordial Universe with future surveys
• Principal Components for Model-Agnostic Modified Gravity with 3x2pt
• Detecting Relativistic Doppler by Multi-Tracing a Single Galaxy Population
• Direct Determination of Expansion History Using Redshift Distortions
• Constraining the halo-ISM connection through multi-transition carbon monoxide line-intensity mapping
• Observational signatures of dark energy produced in an ancestor vacuum: Forecast for galaxy surveys
• Reconstructing the velocity field beyond the local universe
• Testing Large-Scale Structure Measurements Against Fisher Matrix Predictions
• Constraining the growth rate on linear scales by combining SKAO and DESI surveys