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, the Laser Interferometer Space Antenna (LISA) will begin to observe thousands of low-frequency gravitational-wave sources, including ultracompact stellar-remnant binaries in the Milky Way, and the mergers
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establishing the existence of binaries of stellar-mass black holes. In the mid-2030s, the Laser Interferometer Space Antenna (LISA) will begin to observe thousands of low-frequency gravitational-wave sources
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