Fig. 3.
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Spectral indices plotted as α1.5 − 5 vs. α0.144 − 1.5, α3 − 5 vs. α1.5 − 3, α5 − 10 vs. α3 − 5, and α5 − 10 vs. α1.5 − 5. Markers are colored according to the dominating mechanism responsible for the detected radio emission (Table 2). The dashed line indicates the 1 : 1 ratio of equal slopes, while the horizontal and vertical dotted lines correspond to α = −0.5. The region showing flat or inverted spectra, which may be associated with a core-dominated jet or a corona, is shaded gray. The region with a spectral index α = −0.8 ± 0.4 and a scatter of 0.2, possibly related to SF, is shaded turquoise. The region showing very steep spectral slopes with α5 − 10 < −2 in the right-hand panel, which may imply possible relic emission, is shaded blue.
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