Euclid preparation. LXXXIX. Accurate and precise data-driven angular power spectrum covariances
Euclid Collaboration: K. Naidoo (1, 2), J. Ruiz-Zapatero (1), N. Tessore (1), B. Joachimi (1), A. Loureiro (3, 4), N. Aghanim (5), B. Altieri (6), A. Amara (7), L. Amendola (8), S. Andreon (9), N. Auricchio (10), C. Baccigalupi (11, 12, 13, 14), D. Bagot (15), M. Baldi (16, 10

TL;DR
This paper introduces DICES, a novel method for generating accurate, non-singular covariance matrices for Euclid's large-scale structure data, crucial for unbiased cosmological inference.
Contribution
The authors develop DICES, a data-driven covariance estimation technique combining jackknife resampling, shrinkage, and bias correction, tailored for Euclid's survey data.
Findings
DICES achieves 33% lower relative error in covariance estimation.
The method produces non-singular, unbiased covariance matrices.
Validated on synthetic Euclid-like catalogues, DICES improves accuracy over traditional jackknife estimates.
Abstract
We develop techniques for generating accurate and precise internal covariances for measurements of clustering and weak-lensing angular power spectra. These methods have been designed to produce non-singular and unbiased covariances for Euclid's large anticipated data vector and will be critical for validation against observational systematic effects. We constructed jackknife segments that are equal in area to a high precision by adapting the binary space partition algorithm to work on arbitrarily shaped regions on the unit sphere. Jackknife estimates of the covariances are internally derived and require no assumptions about cosmology or galaxy population and bias. Our covariance estimation, called DICES (Debiased Internal Covariance Estimation with Shrinkage), first estimated a noisy covariance through conventional delete-1 jackknife resampling. This was followed by linear shrinkage of…
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