Fig. 8

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Angular power spectra of the dark matter haloes in the lightcone at redshifts z = 0.5 and 1.5. The top panels show the clustering for haloes of mass 1013h−1M⊙ > Mh > 1012h−1M⊙, whereas the bottom panels display the corresponding results for 1012h−1M⊙ > Mh > 1011 h−1M⊙. The lower panels show the ratios with respect to nonlinear theory, with dotted lines displaying the envelope for sample variance errors.
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