Fig. 12
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MSR upper limit around TOI-2257 b as a function of the planetary mass. The blue line represents the solution when considering TOI-2257 b as a giant planet, while the yellow line is considering it as a rocky planet. Each data point is the MSR computed by simulating 1000 exomoons orbiting around TOI-2257 b, for a total of 64 000 scenarios tested.
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