Fig. 5
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Chaoticity map of Kepler-444 in the space of the period ratios P12 and P23. The dotted line follows the expected location of the zeroth-order three-body MMR n1 − 2n2 + n3 = 0. The star depicts the position of the Kepler-444 b-c-d triplet in that space. The colour scale is different from that in Fig. 4 in order to optimise the visibility of the different MMRs.
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