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Fig. A.3.

image

The fraction of the trial cosmologies from the bulk ensemble, , with accuracies, averaged over a range of angular scales (0.5−72 arcmin for ξ+, 8.0−300 arcmin for ξ), better than the value, Ac, plotted on the horizontal axis. The grey curves correspond to ξ+ predictions, magenta to ξ. The solid curves result from training the emulator on the noise-free theoretical predictions from NICAEA, whereas the dashed result from training on cosmo-SLICS itself. The decrement in performance when training on cosmo-SLICS is expected due to the added noise in the training set and inaccuracies in the theoretical predictions.

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