Figure 5.
The same as Fig. 4, but now plotting the flux value assigned to the brightest component instead of the fraction of the total flux. The brightest components at high 250-μm fluxes are still brighter than the low 250-μm flux components. A Spearman Rank correlation test on the unbinned data gives a p-value of 1.08 × 10−13, indicating an exclusion of the null hypothesis of no correlation at >7σ.
