AGN populations in the local Universe: Their alignment with the main sequence, stellar population characteristics, accretion efficiency, and the impact of AGN feedback

Open Access

Fig. 7.

Distribution of the different AGN populations in the H_δ–D_n4000 space. We also plot the results for the heavily obscured (N_H > 10²³ cm⁻²) AGN sample used in Georgantopoulos et al. (2023), at z ∼ 1 (LEGA-C, brown, dotted contours).

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