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Fig. 8

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Orbital period and eccentricity of each confirmed Jupiter-like planet in the Encyclopaedia of Exoplanetary Systems (Schneider et al. 2011) as of 23 November 2023. Only planets with a mass of at least 0.1 MJ and a radius of at least 0.4 RJ are included. The black squares indicate the planets modelled in this work, and the purple stars mark three other potential candidates for the observation of ringing.

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