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Abstract The late stages of galaxy mergers—when two supermassive black holes (SMBHs) reach kiloparsec-scale separations—represent a critical phase for understanding SMBH growth, galaxy co-evolution and the progenitors of low-frequency gravitational waves. However, confirmed close-separation (<3 kpc) dual active galactic nuclei (AGNs) remain rare, particularly in the merger-rich early Universe.
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