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Fig. 6

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[Oi]-based diagnostic diagrams for the optical-radio sample. From top to bottom and from left to right, z increases. The number of radio emitters per bin is constant and equal to 2350 ± 5. The contours represent the number density of the radio emitters (20 galaxies per level). The bulk of the population is always placed in the SF region, though the number of AGNs slightly increases with z.

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