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Non-linear shrinkage estimation of large-scale structure covariance

Joachimi, B; (2017) Non-linear shrinkage estimation of large-scale structure covariance. Monthly Notices of the Royal Astronomical Society: Letters , 466 (1) L83-L87. 10.1093/mnrasl/slw240. Green open access

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Abstract

In many astrophysical settings, covariance matrices of large data sets have to be determined empirically from a finite number of mock realizations. The resulting noise degrades inference and precludes it completely if there are fewer realizations than data points. This work applies a recently proposed non-linear shrinkage estimator of covariance to a realistic example from large-scale structure cosmology. After optimizing its performance for the usage in likelihood expressions, the shrinkage estimator yields subdominant bias and variance comparable to that of the standard estimator with a factor of ∼50 less realizations. This is achieved without any prior information on the properties of the data or the structure of the covariance matrix, at a negligible computational cost.

Type: Article
Title: Non-linear shrinkage estimation of large-scale structure covariance
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnrasl/slw240
Publisher version: http://doi.org/10.1093/mnrasl/slw240
Language: English
Additional information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society: Letters ©: 2016 The Author. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Keywords: Methods: data analysis, methods: numerical, methods: statistical, large-scale structure of Universe
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/1530928
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