Review Article

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

Figure 9

Fractional correction to the Gaussian halo bias in the and Gaussian models. In contrast to Figure 8, halos were identified with a FOF finder of linking length . Only the wavemodes to the left of the vertical line were used to fit . For this low biased sample, the scale-independent correction is and can thus be ignored. The best-fit value of and the corresponding 1 error is quoted for each model (Figure taken from [170]).
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