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Low‐Frequency Gravitational Waves from Massive Black Hole Binaries: Predictions for<i>LISA</i>and Pulsar Timing Arrays
The coalescence of massive black hole (BH) binaries due to galaxy mergers provides a primary source of low-frequency gravitational radiation detectable by pulsar timing measurements and by the proposed the Laser Interferometry Space Antenna (LISA) observatory. We compute the expected gravitational radiation signal from sources at all redshifts by combining …