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This paper investigates the detection of giant planets in the outer Solar System using thermal emissions from far-infrared all-sky surveys conducted by IRAS and AKARI over a 23.4-year interval. The study identifies 535 potential candidates, primarily below 1,000 AU and with masses near or below that of Neptune, but concludes that none are compelling due to confusion with Galactic cirrus. The research confirms previous findings regarding the upper mass limits of unknown planets and provides additional observ

Author

makogebe

Language

EN