The same as Fig. 5 but for IRAS 09149-6206. Since the contour is open to large values of Θg, we consider this source to consist of an over-resolved and an unresolved source and determine the model fit parameter fp (and its derived values Fg and Fp) for the limit Θg → ∞. This is equivalent to computing Fp from the weighted average of all correlated fluxes and Fg from Fg = Fν,tot − Fp. The flux level of Fp is indicated in the radial plot (bottom left) as a straight line.
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