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Fig. 3.


Histogram showing the CP distribution of candidate restarted radio sources (green), candidate remnant radio sources (orange), where CP is mostly an upper limit as the majority of the radio cores are not detected in the FIRST images, and comparison active radio galaxies (blue). The restarted sample shown here includes all candidates selected with the different criteria, not only CP + low-SB; see Sect. 4.3.

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