Two-point statistics without bins: A continuous-function generalization of the correlation function estimator for large-scale structure
arXiv:2011.01836 · doi:10.3847/1538-4357/abdc21
Abstract
The two-point correlation function (2pcf) is the key statistic in structure formation; it measures the clustering of galaxies or other density field tracers. Estimators of the 2pcf, including the standard Landy-Szalay (LS) estimator, evaluate the 2pcf in hard-edged separation bins, which is scientifically inappropriate and results in a poor trade-off between bias and variance. We present a new 2pcf estimator, the Continuous-Function Estimator, which generalizes LS to a continuous representation and obviates binning in separation or any other pair property. Our estimator, inspired by the mathematics of least-squares fitting, replaces binned pair counts with projections onto basis functions; it outputs the best linear combination of basis functions to describe the 2pcf. The choice of basis can take into account the expected form of the 2pcf, as well as its dependence on pair properties other than separation. We show that the Continuous-Function Estimator with a cubic-spline basis better represents the shape of the 2pcf compared to LS. We also estimate directly the baryon acoustic scale, using a small number of physically-motivated basis functions. Critically, this leads to a reduction in the number of mock catalogs required for covariance estimation, which is currently the limiting step in many 2pcf analyses. We discuss further applications of the Continuous-Function Estimator, including determination of the dependence of clustering on galaxy properties and searches for potential inhomogeneities or anisotropies in large-scale structure.
Accepted to ApJ
References in corpus (15)
- Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix
- Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
- A 2.5% measurement of the growth rate from small-scale redshift space clustering of SDSS-III CMASS galaxies
- Corrfunc --- A Suite of Blazing Fast Correlation Functions on the CPU
- Upper limits on the rates of binary neutron star and neutron-star--black-hole mergers from Advanced LIGO's first observing run
- Generating Log-normal Mock Catalog of Galaxies in Redshift Space
- Cosmological constraints from the redshift dependence of the Alcock-Paczynski effect: application to the SDSS-III BOSS DR12 galaxies
- Breaking Halo Occupation Degeneracies with Marked Statistics
- A Robust Estimator of the Small-Scale Galaxy Correlation Function
- Barry and the BAO Model Comparison
- A flexible method for estimating luminosity functions via Kernel Density Estimation
- Making maps of cosmological parameters
- Robust statistics toward detection of the 21 cm signal from the Epoch of Reionisation
- Modelling Stochastic Signatures in Classical Pulsators