Fig. B.1
Comparison of injected and recovered MHW2 flux densities for point sources at 100 GHz. The saturation of points is proportional to the S/N of the MHW2 detection. The outliers towards the upper left are associated with faint sources with injected flux densities <1 Jy located in areas with complicated backgrounds close to the Galactic plane. It is known that in these regions the MHW2 algorithm may give biased flux-density estimates.
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