Fig. 5

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Total-to-peak flux ratio versus signal-to-noise ratio plot for all the sources in the catalogue. The upper panel shows the ratio derived using the Sp values derived by PyBDSF. The lower panel shows the same plot using instead of
is the corrected peak flux obtained by multiplying Sp by a radially dependent correction factor (see Sect. 4.4 for details). The upper black line separates resolved from unresolved sources according to the relation
. The lower black line shows the mirrored relation.
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