Glass-Like Random Catalogues for Two-Point Estimates on the Light Cone
arXiv:2304.02040 · doi:10.1093/mnras/stad2868
Abstract
We introduce grlic, a publicly available Python tool for generating glass-like point distributions with a radial density profile as it is observed in large-scale surveys of galaxy distributions on the past light cone. Utilising these glass-like catalogues, we assess the bias and variance of the Landy-Szalay (LS) estimator of the first three two-point correlation function (2PCF) multipoles in halo and particle catalogues created with the cosmological N-body code gevolution. Our results demonstrate that the LS estimator calculated with the glass catalogues is biased by less than with respect to the estimate derived from Poisson-sampled random catalogues, for all multipoles considered and on all but the smallest scales. Additionally, the estimates derived from glass-like catalogues exhibit significantly smaller standard deviation than estimates based on commonly used Poisson-sampled random catalogues of comparable size. The standard deviation of the estimate depends on a power of the number of objects in the random catalogue; we find a power law for glass-like random catalogues as opposed to using Poisson-sampled random catalogues. Given a required precision, this allows for a much reduced number of objects in the glass-like random catalogues used for the LS estimate of the 2PCF multipoles, significantly reducing the computational costs of each estimate.
arXiv comment16 pages, 14 figures
References in corpus (55)
- 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
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Baryon Acoustic Oscillations in the Sloan Digital Sky Survey Data Release 7 Galaxy Sample
- The 3D power spectrum of galaxies from the SDSS
- The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Cosmological Constraints from the SDSS Luminous Red Galaxies
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Cosmology and Fundamental Physics with the Euclid Satellite
- The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1
- Power Spectrum Analysis of Three-Dimensional Redshift Surveys
- A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey
- A test of the nature of cosmic acceleration using galaxy redshift distortions
- Redshift-Space Distortions, Pairwise Velocities and Nonlinearities
- The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
- The Sloan Digital Sky Survey Quasar Catalog: Fourteenth Data Release
- Fingers of God
- 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
- Interpreting large-scale redshift-space distortion measurements
- 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 VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z=0.8 in the first data release
- Evidence for a non-zero Lambda and a low matter density from a combined analysis of the 2dF Galaxy Redshift Survey and Cosmic Microwave Background Anisotropies
- A comparison of estimators for the two-point correlation function
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the configuration-space clustering wedges
- The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at from redshift-space distortions in the clustering of the PDR-2 final sample
- 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 APM Galaxy Survey III: An Analysis of Systematic Errors in the Angular Correlation Function and Cosmological Implications
- The Glass-like Universe: Real-space correlation properties of standard cosmological models
- gevolution: a cosmological N-body code based on General Relativity
- Asymmetric galaxy correlation functions
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
- A comparison of the evolution of the density field in perturbation theory and numerical simulations - II Counts in cells analysis
- Reconstruction in Fourier space
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: anisotropic clustering analysis in configuration-space
- Imprints of relativistic effects on the asymmetry of the halo cross-correlation function: from linear to non-linear scales
- The SDSS Galaxy Angular Two-Point Correlation Function
- Magnification and evolution biases in large-scale structure surveys
- Towards quantitative control on discreteness error in the non-linear regime of cosmological N body simulations
- Improving the modelling of redshift-space distortions: I. A bivariate Gaussian description for the galaxy pairwise velocity distributions
- Improving the modelling of redshift-space distortions - II. A pairwise velocity model covering large and small scales
- Weak-lensing observables in relativistic N-body simulations
- COFFE: a code for the full-sky relativistic galaxy correlation function
- An optimized correlation function estimator for galaxy surveys
- Estimating the galaxy two-point correlation function using a split random catalog
- Mapping the real space distributions of galaxies in SDSS DR7: I. Two Point Correlation Functions
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift space distortions between redshift 0.8 and 2.2
- An alternative to grids and glasses: Quaquaversal pre-initial conditions for N-body simulations
- Nonlinear Behavior of Baryon Acoustic Oscillations from the Zel'dovich Approximation Using a Non-Fourier Perturbation Approach
- The halo bias for number counts on the light cone from relativistic N-body simulations
- Fast analytical calculation of the random pair counts for realistic survey geometry
- Nonlinear Behavior of Baryon Acoustic Oscillations in Redshift Space from the Zel'dovich Approximation
- Improved two-point correlation function estimates using glass-like distributions as a reference sample