Fig. 1.
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Angular size as a function of flux density (left panel) and redshift (right panel) for the 1560 sources considered in this paper. We separated our sources into 1146 FRI and 414 FRII morphologies with separated colors and draw dashed lines for 40″ and 400″. These lines determine the angular size cuts that we applied in this paper before doing completeness corrections (see Sect. 4.2).
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