Figure 8From: Cosmological N-body simulations: a challenge for scalable generative modelsStatistics of the samples produced by \(M_{2}\). The fake samples are generated by conditioning WGAN \(M_{2}\) on the real down-scaled 323 samples. The power spectrum density is shown in units of h Mpc−1, where \(\mbox{h} = \mbox{H}_{0}/100\) corresponds to the Hubble parameterBack to article page