HALO OCCUPATION DISTRIBUTION MODELING OF CLUSTERING OF LUMINOUS RED GALAXIES

We perform halo occupation distribution (HOD) modeling to interpret small-scale and intermediate-scale clustering of 35,000 luminous early-type galaxies and their cross-correlation with a reference imaging sample of normal L-* galaxies in the Sloan Digital Sky Survey. The modeling results show that most of these luminous red galaxies (LRGs) are central galaxies residing in massive halos of typical mass M similar to a few times 10(13)-10(14) h(-1) M-circle dot, while a few percent of them have to be satellites within halos in order to produce the strong auto-correlations exhibited on smaller scales. The mean luminosity L-c of central LRGs increases with the host halo mass, with a rough scaling relation of L-c alpha M-0.5. The halo mass required to host on average one satellite LRG above a luminosity threshold is found to be about 10 times higher than that required to host a central LRG above the same threshold. We find that in massive halos the distribution of L-* galaxies roughly follows that of the dark matter and their mean occupation number scales with halo mass as M-1.5. The HOD modeling results also allow for an intuitive understanding of the scale-dependent luminosity dependence of the cross-correlation between LRGs and L-* galaxies. Constraints on the LRG HOD provide tests for models of formation and evolution of massive galaxies, and they are also useful for cosmological parameter investigations. In one of the appendices, we provide LRG HOD parameters with dependence on cosmology inferred from modeling the two-point auto-correlation functions of LRGs.