Fig. 11
Mass-to-light ratio using the total halo mass and luminosity within r200, as a function of L200. The red squares (blue triangles) denote the early-type (late-type) results. The hatched area indicates the converted M200/L200 of the maxBCG clusters from Sheldon et al. (2009a). The M200/L200 for individual galaxies at low luminosities are naturally extended to the ratios for the maxBCG clusters.
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