Estimating cosmological parameter covariance

Abstract

We investigate the bias and error in estimates of the cosmological parameter covariance matrix due to sampling or modelling the data covariance matrix, for likelihood width and peak scatter estimators.We show that these estimators do not coincide unless the data covariance is exactly known. For sampled data covariances with Gaussian-distributed data and parameters, the parameter covariance matrix estimated from the width of the likelihood has aWishart distribution, from which we derive the mean and covariance. This mean is biased and we propose an unbiased estimator of the parameter covariance matrix. Comparing our analytic results to a numerical Wishart sampler of the data covariance matrix we find excellent agreement. An accurate ansatz for the mean parameter covariance for the peak scatter estimator is found, and we fit its covariance to our numerical analysis. The mean is again biased and we propose an unbiased estimator for the peak parameter covariance. For sampled data covariances, the width estimator is more accurate than the peak scatter estimator. We investigate modelling the data covariance, or equivalently data compression, and show that the peak scatter estimator is less sensitive to biases in the model data covariance matrix than the width estimator, but requires independent realizations of the data to reduce the statistical error. If the model bias on the peak estimator is sufficiently low, this is promising, otherwise the sampled width estimator is preferable © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.