EZmocks: extending the Zel'dovich approximation to generate mock galaxy catalogues with accurate clustering statistics
arXiv:1409.1124 · doi:10.1093/mnras/stu2301
Abstract
We present a new methodology to generate mock halo or galaxy catalogues, which have accurate clustering properties, nearly indistinguishable from full -body solutions, in terms of the one-point, two-point, and three-point statistics. In particular, the agreement is remarkable, within up to Mpc and down to Mpc, for the power spectrum and two-point correlation function respectively, while the bispectrum agrees in general within for different scales and shapes. Our approach is based on the Zel'dovich approximation, however, effectively including with the simple prescriptions the missing physical ingredients, and stochastic scale-dependent, non-local and nonlinear biasing contributions. The computing time and memory required to produce one mock is similar to that using the log-normal model. With high accuracy and efficiency, the effective Zel'dovich approximation mocks (EZmocks) provide a reliable and practical method to produce massive mock galaxy catalogues for the analysis of large-scale structure measurements.
8 pages, 6 figures, matches the version accepted by MNRAS
References in corpus (7)
- The DESI Experiment, a whitepaper for Snowmass 2013
- Modelling Baryon Acoustic Oscillations with Perturbation Theory and Stochastic Halo Biasing
- The Bispectrum in the Effective Field Theory of Large Scale Structure
- J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey
- An accurate tool for the fast generation of dark matter halo catalogs
- Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias
- One-point remapping of Lagrangian perturbation theory in the mildly non-linear regime of cosmic structure formation
Cited by in corpus (140)
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: First measurement of Baryon Acoustic Oscillations between redshift 0.8 and 2.2
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the Quasar sample between redshift 0.8 and 2.2
- DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
- Large-scale dark matter simulations
- 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
- Redshift-weighted constraints on primordial non-Gaussianity from the clustering of the eBOSS DR14 quasars in Fourier space
- The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope
- The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: 1000 multi-tracer mock catalogues with redshift evolution and systematics for galaxies and quasars of the final data release
- Cosmological constraints from BOSS with analytic covariance matrices
- ICE-COLA: Towards fast and accurate synthetic galaxy catalogues optimizing a quasi -body method
- The mass-Peak Patch algorithm for fast generation of deep all-sky dark matter halo catalogues and its N-Body validation
- Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles
- Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
- nIFTy Cosmology: Galaxy/halo mock catalogue comparison project on clustering statistics
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
- DESI 2024 II: Sample Definitions, Characteristics, and Two-point Clustering Statistics
- Fast and accurate mock catalogue generation for low-mass galaxies
- Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum
- DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars
- Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
- Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space
- HALOGEN: A tool for fast generation of mock halo catalogues
- Galaxy redshift-space bispectrum: the Importance of Being Anisotropic
- Statistical properties of paired fixed fields
- A Lightcone Catalogue from the Millennium-XXL Simulation
- Inflation and Early Dark Energy with a Stage II Hydrogen Intensity Mapping Experiment
- The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological implications from multi-tracer BAO analysis with galaxies and voids
- 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
- CARPool: fast, accurate computation of large-scale structure statistics by pairing costly and cheap cosmological simulations
- A volumetric deep Convolutional Neural Network for simulation of mock dark matter halo catalogues
- Improving the precision matrix for precision cosmology
- 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
- Primordial non-Gaussianity from the Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey I: Catalogue Preparation and Systematic Mitigation
- Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
- Field Level Neural Network Emulator for Cosmological N-body Simulations
- Constraints on the growth of structure around cosmic voids in eBOSS DR14
- Dark Energy Survey Year 1 Results: galaxy mock catalogues for BAO
- ADDGALS: Simulated Sky Catalogs for Wide Field Galaxy Surveys
- Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
- The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: N-body Mock Challenge for Galaxy Clustering Measurements
- Measuring Baryon Acoustic Oscillations from the clustering of voids
- First Detection of the BAO Signal from Early DESI Data
- BAM: Bias Assignment Method to generate mock catalogs
- The Zeldovich approximation and wide-angle redshift-space distortions
- ICE-COLA: fast simulations for weak lensing observables
- Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys
- CoLoRe: fast cosmological realisations over large volumes with multiple tracers
- sCOLA: The N-body COLA Method Extended to the Spatial Domain
- Mitigation of DESI fiber assignment incompleteness effect on two-point clustering with small angular scale truncated estimators
- The weak, the strong and the ugly -- A comparative analysis of interacting stepped dark radiation
- NECOLA: Towards a Universal Field-level Cosmological Emulator
- Semi-analytical covariance matrices for two-point correlation function for DESI 2024 data
- BAO reconstruction: a swift numerical action method for massive spectroscopic surveys
- Optimal Reconstruction of Baryon Acoustic Oscillations for DESI 2024
- Testing General Relativity on cosmological scales at redshift z ~ 1.5 with quasar and CMB lensing
- Removing Imaging Systematics from Galaxy Clustering Measurements with Obiwan : Application to the SDSS-IV extended Baryon Oscillation Spectroscopic Survey Emission Line Galaxy Sample
- Simulating cosmologies beyond CDM with PINOCCHIO
- Analysis of Unified Galaxy Power Spectrum Multipole Measurements
- Analytical and EZmock covariance validation for the DESI 2024 results
- ATLAS Probe: Breakthrough Science of Galaxy Evolution, Cosmology, Milky Way, and the Solar System
- Enabling matter power spectrum emulation in beyond-CDM cosmologies with COLA
- The bias of dark matter tracers: assessing the accuracy of mapping techniques
- A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
- The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: GLAM-QPM mock galaxy catalogs for the Emission Line Galaxy Sample
- HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
- Cosmological parameter inference from galaxy clustering: The effect of the posterior distribution of the power spectrum
- One simulation to have them all: performance of the Bias Assignment Method against N-body simulations
- Does jackknife scale really matter for accurate large-scale structure covariances?
- Testing approximate predictions of displacements of cosmological dark matter halos
- Validation of semi-analytical, semi-empirical covariance matrices for two-point correlation function for Early DESI data
- Cosmological measurements from void-galaxy and galaxy-galaxy clustering in the Sloan Digital Sky Survey
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Anisotropic Baryon Acoustic Oscillations measurements in Fourier-space with optimal redshift weights
- Fast and realistic large-scale structure from machine-learning-augmented random field simulations
- The cosmic web connection to the dark matter halo distribution through gravity
- Towards alleviating the and tensions with Early Dark Energy - Dark Matter drag
- Accurate halo-galaxy mocks from automatic bias estimation and particle mesh gravity solvers
- Mitigating the noise of DESI mocks using analytic control variates
- Integrated trispectrum detection from BOSS DR12 NGC CMASS
- Baryon Acoustic Oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
- fkPT: Constraining scale-dependent modified gravity with the full-shape galaxy power spectrum
- Robustness of the covariance matrix for galaxy clustering measurements
- Reducing the Variance of Redshift Space Distortion Measurements from Mock Galaxy Catalogues with Different Lines of Sight
- Primordial feature constraints from BOSS+eBOSS
- Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
- Fast generation of weak lensing maps by the inverse-Gaussianization method
- Clustering in the Simulated H Galaxy Redshift Survey from Nancy Grace Roman Space Telescope
- Probing Gravitational Lensing of the CMB with SDSS-IV Quasars
- Efficient Construction of Mock Catalogs for Baryon Acoustic Oscillation Surveys
- Bayesian Control Variates for optimal covariance estimation with pairs of simulations and surrogates
- Tomographic redshift dipole: Testing the cosmological principle
- : A generative, fast, and differentiable halo model for wide-field galaxy surveys
- Rapid Simulations of Halo and Subhalo Clustering
- MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
- Model-Independent Measurement of the Matter-Radiation Equality Scale in DESI 2024
- The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
- The 2-point correlation function covariance with fewer mocks
- Choose to smooth: Gaussian streaming with the truncated Zel'dovich approximation
- Can acoustic and axion-like early dark energy still resolve the Hubble tension?
- Validating galaxy clustering models with Fixed & Paired and Matched-ICs simulations: application to Primordial Non-Gaussianities
- Non-linear Structure Formation for Dark Energy Models with a Steep Equation of State
- The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
- The Weak Lensing Peak Statistics in the Mocks by the inverse-Gaussianization Method
- Perturbation Theory Remixed: Improved Nonlinearity Modeling beyond Standard Perturbation Theory
- The importance of the cosmic web and halo substructure for power spectra
- Angular systematics-free cosmological analysis of galaxy clustering in configuration space
- Cosmic void exclusion models and their impact on the distance scale measurements from large scale structure
- Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: Possibility of estimateing the non-linear systematics using fast simulations
- Euclid preparation. Simulating thousands of Euclid spectroscopic skies
- The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data
- DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
- Faster cosmological analysis with power spectrum without simulations
- Covariance matrices for variance-suppressed simulations
- Bispectrum constraints on Primordial non-Gaussianities with the eBOSS DR16 quasars
- Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method
- The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
- Angular Correlation Function from sample covariance with BOSS and eBOSS LRG
- Exploring HOD-dependent systematics for the DESI 2024 Full-Shape galaxy clustering analysis
- Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1
- The Low Redshift survey at Calar Alto (LoRCA)
- Phenomenological power spectrum models for H emission line galaxies from the Nancy Grace Roman Space Telescope
- Baryon acoustic oscillations from a joint analysis of the large-scale clustering in Fourier and configuration space
- Approximate methods for the generation of dark matter halo catalogs in the age of precision cosmology
- Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
- Constraining primordial non-Gaussianity from the large scale structure two-point and three-point correlation functions
- Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
- Dark Energy Survey Year 3 Results: Galaxy mock catalogs for BAO analysis
- The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from cosmic voids
- Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data
- An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: Testing observational systematics on the Baryon Acoustic Oscillation measurement
- Parity-odd Four-Point Correlation Function from DESI Data Release 1 Luminous Red Galaxy Sample
- Growth rate measurements from a joint analysis of the large-scale galaxy clustering in Fourier and configuration space
- Model-agnostic interpretation of 10 billion years of cosmic evolution traced by BOSS and eBOSS data
- Improving cosmological covariance matrices with machine learning
- Measuring peculiar velocity and tomographic redshift dipole with DESI DR1 catalogs