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The document discusses the detection of milliarcsecond astrometric oscillations in the quasar J0204+1514, suggesting it may be a supermassive black hole binary (SMBHB) and a potential source of gravitational waves (GW). The authors analyze VLBI astrometry data to provide evidence of these oscillations and propose a toy model to predict GW emissions from such systems. The findings highlight the importance of astrometric monitoring for identifying SMBHBs as multi-messenger targets in future astronomical studi

Author

Jean

Language

EN