Fig. 1

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Gaia CMD based on DR2 data for the LG11 sample with Gaia distance and photometry. The pink line represents the main sequence by E. Mamajek (see footnote 1). A residual contamination by giant stars is present. Stars with MG > 5 mag and MKs > 4.6 (the magnitude above which the polynomial relations between photometry and stellar parameters of (Mann et al. 2015) are valid) are highlighted in green.

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