You still seem to be missing my point. The actual merger of 2 SMBHs is not likely to be a long-term event. A quasar is probably NOT the actual merging event, but maybe the prelude to one, where 2 SMBHs are in close orbits BEFORE merging. That would fit the observation that there are a lot more quasars than ORCs in our field of view.
But, on the other hand, I am not clear on how far away we are currently able to detect ORCs. Maybe their population density is closer to the density of quasars.
It would not surprise me if all galaxy mergers went through phases that include their central SMBHs creating a quasar, and then merging and emitting an ORC shock wave, and then a quiescent period where the material near the now-merged SMBH is depleted by the shock from the merger.
Which brings me back to my wondering what all that energy emission in the center of a galaxy would do to the environments of planets orbiting stars in their galaxies. Could life survive? If so, then maybe there is some life form that is extremely old out there somewhere. IF not, then that would say something about the prospects for life forms older than the last merger time for any particular galaxy.