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Fig. 6.

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In clockwise direction, halo occupation distribution for stellar mass, r-band, blue, and red galaxy samples with n = 0.003 h3 Mpc−3 at z = 0. The solid, dotted, and dashed lines show the results for all galaxies, centrals, and satellites, respectively. The results for the 25% of galaxies with the highest and lowest concentration are in orange and green, respectively, while the complete sample is in blue. We note that the occupancy of halos depends on the concentration for all galaxy samples.

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