Cosmic evolution of BH-455 (upper left panel), BH-936 (upper right), BH-549 (lower left panel), and BH-132 (lower right panel). Same as Fig. 4 but for BH-455 and BH-936 display typical Ψ_star, BH evolution. BH-549 is displaying a long phase where its spin is anti-aligned with the stellar angular momentum. In this example, the gas accretion disk is in counter-rotation with respect to the stellar component. As far as BH-132 is concerned, it is off-centered from the galaxy center. In this latter case, the efficiency of gas accretion and Eddington ratio are generally low and BH spin is mis-aligned with J_star.