Fig. C.1.
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MBH-M* relation of the galaxy sample at z ≈ 0. Especially for the mass range of 1010M⊙ ≤ M⊙ ≤ 1011M⊙, a clear transition order from quenched galaxies along the Magorrian relation to lower black hole masses for star-forming galaxies. Specifically, early-quenched galaxies (dark red) have the highest values, followed by late-quenched (dark blue), rejuvenated quenched (lilac), MS-evolved (cyan), and finally rejuvenated main-sequence (pink) galaxies as well as caught-type galaxies (blue) at the lower black hole mass end.
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