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Fig. 7
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Distribution of rotation stellar periods against the G − J colour for Pleiades (∼125 Myr; Rebull et al. 2016), M48 (∼450 Myr; Barnes et al. 2015), Praesepe (∼590 Myr; Douglas et al. 2017), Hyades (∼650 Myr; Douglas et al. 2019), and NGC6811 (∼1000 Myr; Curtis et al. 2019) clusters. TOI-1135 is represented as a gold star.
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