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Fig. A.3.

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Gradient’s slope (Δα) of the AGN-FS (dark red triangles) and AGN-RPS (red circles) as a function of the [O III] λ5007 luminosity within an aperture of r ∼ 1 kpc (log L [O III]λ5007r <  1kpc) and of the host’s galaxy stellar mass (logM*/M). The legend shows the Kendall τ test’s coefficients (e.g., ktAGN) for the 10 galaxies part of the AGN-RPS and for the 52 galaxies part of the AGN-FS, revealing that the slopes do not correlate with the other galaxy’s properties in both the AGN-RPS and AGN-FS.

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