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The coalescence of massive black hole binaries (with masses $10^4 - 10^7 M_{\odot}$) leads to gravitational wave emission that is detectable out to high redshifts ($z \sim 20$) with the forthcoming LISA observatory.
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S. M. Koushiappas and A. R. Zentner, Testing Models of Supermassive Black Hole Seed Formation through Gravity Waves , ApJ 639
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R. N. Lang and S. A. Hughes, Measuring coalescing massive binary black holes with gravitational waves: The impact of spin-induced precession , Phys.Rev.D 74
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A. Loeb, Electromagnetic Counterparts to Black Hole Mergers Detected by LIGO , ApJ 819
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D. J. Mortlock, S. M. Feeney, H. V. Peiris, A. R. Williamson and S. M. Nissanke, Unbiased hubble constant estimation from binary neutron star mergers , Phys. Rev. D 100
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