Fig. 10
Mean halo mass versus galaxy number density for our range of galaxy stellar mass and redshift ranges. The points show our results with different point types giving different redshift ranges. The long-dashed line shows the best fit determined by Coupon et al. (2012) for z < 1 galaxies in the CFHTLS. The short-dashed curves show the galform predictions with the same colour coding as given in Fig. 9.
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