Nature Astronomy, Published online: 07 December 2023; doi:10.1038/s41550-023-02148-w

A reanalysis of Kepler and Hubble data with Bayesian inference and a photodynamical model shows that the two exomoon candidates around Kepler-1625 b and Kepler-1708 b have a substantially lower probability to be actual detections than previous analyses suggest.

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