  Recent progress with pulsar timing array experiments, especially from the
NANOGrav collaboration indicate that we are on the cusp of detecting
significant signals from the inspiral of super-massive black hole binaries
(SMBHB). While recent analysis has focused on nearby galaxies as possible
sources of the loudest signals, we show that mergers in identified clusters at
z~1 can have larger strain amplitudes. We make an estimate comparing the nearby
2MASS redshift survey galaxy sample with the more distant MaDCoWS cluster
sample, showing that the latter might be expected to contribute more, and
louder, gravitational wave events. Thus the first individual source detections
may well be from ultra-massive BH in clusters at z~1, rather than nearby
galaxies.
