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Fig. 1.

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Apparent K-band magnitude distributions for the halos in our simulation and for SDSS galaxies. The orange line refers to the Legacy MGS galaxies with apparent K-band magnitude from the NYU-VAGC sample. The light blue line refers to the mK distribution for all halos in our simulation (with mK computed with Eq. (1)). The green line shows the distribution for our magnitude-selected simulated galaxy sample. The vertical black dashed line shows our magnitude threshold of mK = 14.

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