English

A Maximum Likelihood Approach to Estimating Correlation Functions

Cosmology and Nongalactic Astrophysics 2013-11-27 v2 Instrumentation and Methods for Astrophysics

Abstract

We define a Maximum Likelihood (ML for short) estimator for the correlation function, {\xi}, that uses the same pair counting observables (D, R, DD, DR, RR) as the standard Landy and Szalay (1993, LS for short) estimator. The ML estimator outperforms the LS estimator in that it results in smaller measurement errors at any fixed random point density. Put another way, the ML estimator can reach the same precision as the LS estimator with a significantly smaller random point catalog. Moreover, these gains are achieved without significantly increasing the computational requirements for estimating {\xi}. We quantify the relative improvement of the ML estimator over the LS estimator, and discuss the regimes under which these improvements are most significant. We present a short guide on how to implement the ML estimator, and emphasize that the code alterations required to switch from a LS to a ML estimator are minimal.

Keywords

Cite

@article{arxiv.1305.4613,
  title  = {A Maximum Likelihood Approach to Estimating Correlation Functions},
  author = {Eric Jones Baxter and Eduardo Rozo},
  journal= {arXiv preprint arXiv:1305.4613},
  year   = {2013}
}

Comments

16 pages, 8 figures

R2 v1 2026-06-22T00:19:21.524Z