Fig. 9
Upper panel: correlation length of our various subsamples of log (M⋆/M⊙) > 10.5 galaxies as a function of their sSFR measured at various wavelengths (purple for UV, orange for MIPS 24 μm, and red for PACS). For comparison, the data from Lin et al. (2012) are plotted with black squares. Lower panel: mean mass of halos, which host log (M⋆/M⊙) > 10.5 galaxies as a function of their sSFR.
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