Auto-correlation function of various flux-selected sample of infrared galaxies and comparison with our model (same color coding as in Fig. 7). The data come from Magliocchetti et al. (2011) at 100 μm and 160 μm and Cooray et al. (2010) and Maddox et al. (2010) at 250, 350, and 500 μm. We used the same flux cuts as Magliocchetti et al. (2011) and Cooray et al. (2010). Models A, B, and C are represented by a long green dash, a short blue dash, and a solid red line, respectively.