Residual Smoothing: Using Mocks to Correct Model Covariance Matrices

Abstract

Abstract Covariance matrix estimation is a challenging problem in cosmology. Recent work has shown that model covariance matrices can be precise, and that at relatively large scales they can also be accurate. We introduce a data-driven method that can identify features from a mock covariance matrix that are missing from a corresponding model, then incorporate them into the model without significantly degrading the model's precision. We apply this method to a BOSS-like survey and extend a model covariance to be valid at scales relevant for measurements of Redshift Space Distortions (8-40 Mpc/h), where the galaxy field is significantly non-Gaussian.

References in corpus (2)

• Non-linear shrinkage estimation of large-scale structure covariance
• Galaxy 2-Point Covariance Matrix Estimation for Next Generation Surveys