On the accuracy and precision of correlation functions and field-level
inference in cosmology
F. Leclercq, и A. Heavens. (2021)cite arxiv:2103.04158Comment: 6+8 pages, 4+5 figures. Matches MNRAS Letters published version. Appendices provide supplementary information, including calculations of Fisher matrices. Our code and data are publicly available at https://github.com/florent-leclercq/correlations_vs_field.
DOI: 10.1093/mnrasl/slab081
Аннотация
We present a comparative study of the accuracy and precision of correlation
function methods and full-field inference in cosmological data analysis. To do
so, we examine a Bayesian hierarchical model that predicts log-normal fields
and their two-point correlation function. Although a simplified analytic model,
the log-normal model produces fields that share many of the essential
characteristics of the present-day non-Gaussian cosmological density fields. We
use three different statistical techniques: (i) a standard likelihood-based
analysis of the two-point correlation function; (ii) a likelihood-free
(simulation-based) analysis of the two-point correlation function; (iii) a
field-level analysis, made possible by the more sophisticated data assimilation
technique. We find that (a) standard assumptions made to write down a
likelihood for correlation functions can cause significant biases, a problem
that is alleviated with simulation-based inference; and (b) analysing the
entire field offers considerable advantages over correlation functions, through
higher accuracy, higher precision, or both. The gains depend on the degree of
non-Gaussianity, but in all cases, including for weak non-Gaussianity, the
advantage of analysing the full field is substantial.
Описание
On the accuracy and precision of correlation functions and field-level inference in cosmology
cite arxiv:2103.04158Comment: 6+8 pages, 4+5 figures. Matches MNRAS Letters published version. Appendices provide supplementary information, including calculations of Fisher matrices. Our code and data are publicly available at https://github.com/florent-leclercq/correlations_vs_field
%0 Generic
%1 leclercq2021accuracy
%A Leclercq, Florent
%A Heavens, Alan
%D 2021
%K cosmology lss machine_learning phd
%R 10.1093/mnrasl/slab081
%T On the accuracy and precision of correlation functions and field-level
inference in cosmology
%U http://arxiv.org/abs/2103.04158
%X We present a comparative study of the accuracy and precision of correlation
function methods and full-field inference in cosmological data analysis. To do
so, we examine a Bayesian hierarchical model that predicts log-normal fields
and their two-point correlation function. Although a simplified analytic model,
the log-normal model produces fields that share many of the essential
characteristics of the present-day non-Gaussian cosmological density fields. We
use three different statistical techniques: (i) a standard likelihood-based
analysis of the two-point correlation function; (ii) a likelihood-free
(simulation-based) analysis of the two-point correlation function; (iii) a
field-level analysis, made possible by the more sophisticated data assimilation
technique. We find that (a) standard assumptions made to write down a
likelihood for correlation functions can cause significant biases, a problem
that is alleviated with simulation-based inference; and (b) analysing the
entire field offers considerable advantages over correlation functions, through
higher accuracy, higher precision, or both. The gains depend on the degree of
non-Gaussianity, but in all cases, including for weak non-Gaussianity, the
advantage of analysing the full field is substantial.
@misc{leclercq2021accuracy,
abstract = {We present a comparative study of the accuracy and precision of correlation
function methods and full-field inference in cosmological data analysis. To do
so, we examine a Bayesian hierarchical model that predicts log-normal fields
and their two-point correlation function. Although a simplified analytic model,
the log-normal model produces fields that share many of the essential
characteristics of the present-day non-Gaussian cosmological density fields. We
use three different statistical techniques: (i) a standard likelihood-based
analysis of the two-point correlation function; (ii) a likelihood-free
(simulation-based) analysis of the two-point correlation function; (iii) a
field-level analysis, made possible by the more sophisticated data assimilation
technique. We find that (a) standard assumptions made to write down a
likelihood for correlation functions can cause significant biases, a problem
that is alleviated with simulation-based inference; and (b) analysing the
entire field offers considerable advantages over correlation functions, through
higher accuracy, higher precision, or both. The gains depend on the degree of
non-Gaussianity, but in all cases, including for weak non-Gaussianity, the
advantage of analysing the full field is substantial.},
added-at = {2023-04-16T23:41:37.000+0200},
author = {Leclercq, Florent and Heavens, Alan},
biburl = {https://www.bibsonomy.org/bibtex/26d86e5cf92d01e5ac9015e33de34b45f/intfxdx},
description = {On the accuracy and precision of correlation functions and field-level inference in cosmology},
doi = {10.1093/mnrasl/slab081},
interhash = {ed0e4155a3b06cda93af89f2700cd96e},
intrahash = {6d86e5cf92d01e5ac9015e33de34b45f},
keywords = {cosmology lss machine_learning phd},
note = {cite arxiv:2103.04158Comment: 6+8 pages, 4+5 figures. Matches MNRAS Letters published version. Appendices provide supplementary information, including calculations of Fisher matrices. Our code and data are publicly available at https://github.com/florent-leclercq/correlations_vs_field},
timestamp = {2023-04-16T23:41:37.000+0200},
title = {On the accuracy and precision of correlation functions and field-level
inference in cosmology},
url = {http://arxiv.org/abs/2103.04158},
year = 2021
}