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The document discusses the successful prediction of a fourth gamma-ray flare from the supermassive black hole binary candidate J1048+7143, which aligns with previous predictions based on the spin-orbit precession model. The study refines the mass ratio of the black hole binary and suggests that the occurrence of sub-flares is indicative of jet precession interacting with surrounding matter. This research contributes to the understanding of active galactic nuclei and multimessenger astronomy by analyzing gam

Author

calebloyd12

Language

EN