Angular power spectrum of CIB anisotropies at 217, 353, 545, and 857 GHz. Each panel corresponds to one frequency. For each frequency, the blue points correspond to the angular auto power-spectra, and the associated error bars include statistical and photometric calibration systematic contributions. The best-fit model per frequency (including shot noise) corresponds to the solid orange line. The dashed (dot-dashed) orange lines correspond to the 2 h (1 h) contributions. The green triple dot-dashed curve corresponds to the Poisson noise level, fixed to its expected value. To obtain these fits, three parameters per frequency were varied: log ₁₀M_min, α_sat and j_eff. The fits are obviously qualitatively very good.