Sample variance in weak lensing: how many simulations are required?
arXiv:1601.06792 · doi:10.1103/PhysRevD.93.063524
Abstract
Constraining cosmology using weak gravitational lensing consists of comparing a measured feature vector of dimension with its simulated counterpart. An accurate estimate of the feature covariance matrix is essential to obtain accurate parameter confidence intervals. When is measured from a set of simulations, an important question is how large this set should be. To answer this question, we construct different ensembles of realizations of the shear field, using a common randomization procedure that recycles the outputs from a smaller number of independent ray-tracing --body simulations. We study parameter confidence intervals as a function of () in the range and . Previous work has shown that Gaussian noise in the feature vectors (from which the covariance is estimated) lead, at quadratic order, to an degradation of the parameter confidence intervals. Using a variety of lensing features measured in our simulations, including shear-shear power spectra and peak counts, we show that cubic and quartic covariance fluctuations lead to additional error degradation that is not negligible when is only a factor of few larger than . We study the large limit, and find that a single, 240Mpc sized -particle --body simulation () can be repeatedly recycled to produce as many as shear maps whose power spectra and high-significance peak counts can be treated as statistically independent. As a result, a small number of simulations ( or ) is sufficient to forecast parameter confidence intervals at percent accuracy.
12 pages, 6 figures, 2 tables; PRD accepted
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