Euclid: Fast two-point correlation function covariance through linear construction
arXiv:2205.11852 · doi:10.1051/0004-6361/202244065
Abstract
We present a method for fast evaluation of the covariance matrix for a two-point galaxy correlation function (2PCF) measured with the Landy-Szalay estimator. The standard way of evaluating the covariance matrix consists in running the estimator on a large number of mock catalogs, and evaluating their sample covariance. With large random catalog sizes (data-to-random objects ratio M>>1) the computational cost of the standard method is dominated by that of counting the data-random and random-random pairs, while the uncertainty of the estimate is dominated by that of data-data pairs. We present a method called Linear Construction (LC), where the covariance is estimated for small random catalogs of size M = 1 and M = 2, and the covariance for arbitrary M is constructed as a linear combination of these. We validate the method with PINOCCHIO simulations in range r = 20-200 Mpc/h, and show that the covariance estimate is unbiased. With M = 50 and with 2 Mpc/h bins, the theoretical speed-up of the method is a factor of 14. We discuss the impact on the precision matrix and parameter estimation, and derive a formula for the covariance of covariance.
17 pages, 11 figures
References in corpus (29)
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: a large sample of mock galaxy catalogues
- The Clustering of Galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Including covariance matrix errors
- Parameter inference with estimated covariance matrices
- The Effect of Covariance Estimator Error on Cosmological Parameter Constraints
- Putting the Precision in Precision Cosmology: How accurate should your data covariance matrix be?
- The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s
- Estimating Cosmological Parameter Covariance
- The 3-point function in large scale structure: redshift distortions and galaxy bias
- Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum
- Improving fast generation of halo catalogs with higher-order Lagrangian perturbation theory
- Shrinkage Estimation of the Power Spectrum Covariance Matrix
- Improving the precision matrix for precision cosmology
- Precision matrix expansion - efficient use of numerical simulations in estimating errors on cosmological parameters
- Non-linear shrinkage estimation of large-scale structure covariance
- Estimating the galaxy two-point correlation function using a split random catalog
- A map-based method for eliminating systematic modes from galaxy clustering power spectra with application to BOSS
- Estimating sparse precision matrices
- Bayesian power-spectrum inference with foreground and target contamination treatment
- A blind method to recover the mask of a deep galaxy survey
- Improved two-point correlation function estimates using glass-like distributions as a reference sample
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey quasar sample: Testing observational systematics on the Baryon Acoustic Oscillation measurement