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. 8.

Specific black hole accretion rate, λ_sBHAR, for the different AGN populations. The top panel shows the distribution of λ_sBHAR for the different AGN classes. The bottom panel shows the distribution of our sources in the H_δ–D_n4000 space, which are color coded based on their λ_sBHAR values.

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