Review Article

Primordial Non-Gaussianity in the Large-Scale Structure of the Universe

Figure 7

Non-Gaussian bias correction (filled symbols) for halos of mass extracted at from simulations of the local model. The solid curve represents the theoretical model (42). The dashed, dotted-dashed-dotted, and dotted curves show the scale-dependent bias , the scale-independent offset and the contribution from the matter power spectrum that arise at first order in (see Figure 2). The error bars indicate the scatter among 8 realizations of simulations with box size .
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