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Fig. 2

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Color-magnitude diagrams displaying the location of GJ7 (TOI-198), the young stellar sequence of Group 29 (Oh et al. 2017; Luhman 2018), the main sequence of M-type stars (Cifuentes et al. 2020), and several confirmed low-metallicity field stars with spectral types M1–M6 from the catalog of Leggett et al. (2000). The dispersion of the main sequence is shown by the gray-shaded area.

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