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Fig. 7.

image

Distributions of the active and non-active galaxies in each quenching stage through Hubble type (panels B-G). The blank bars outline the distribution of the non-active galaxies, while the grey-filled bars and the slashes correspond to the wAGN and sAGN distributions, respectively. Panel A: distribution of the full sample. N gives the number of the galaxies for each nuclear activity group (see Sect. 5.1).

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