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Fig. 7.


Spectral indices derived for subsets of the RxAGN sample divided by redshift, z, and radio luminosity, log L1.4 [W Hz−1], described in Sect. 5.2. The color-scale in the left panel shows the spectral index of the PL model, while the color-scales in the middle and right panels show the spectral indices α1 and α2 of the broken power-law model. Bins are outlined by black dashed lines. The panels show the spectral indices radio SEDs shown in Fig. 6 for different subsets of RxAGN and correspond to numbered bins presented in Table 1 and Fig. 8.

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