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Fig. 3

image

Iso-correlation contours of the redshift-space two-point correlation function, corresponding to the values ξ(s,s)  = [0.05,0.1,0.2,0.4,1,3], for galaxies with log (MSTAR [h-1M] ) > 10, at z = 0.2 (black contours). The dot-dashed green and solid red contours show the best-fit model given by Eq. (16), with the real-space correlation function ξ(r) measured from the simulation, and estimated from the CAMB power spectrum, respectively. The blue dashed contours show the linear best-fit model given by Eq. (10) with the CAMB real-space correlation function.

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