Non-Gaussianity from Large-Scale Structure Surveys
Figure 5
Effect of the non-Gaussian halo bias on the power spectrum. In the left-top of (a) panel we show the halo-matter cross-power spectrum for masses above at . The left-bottom panel of (a) shows the ratio of the non-Gaussian to Gaussian bias. Figure reproduced from [33]. The values reported in the figure legend should be interpreted as . On the right panel we show the expected effect and error-bars for the large-scale power spectrum for a survey like LSST. Figure reproduced from [26].
