Fig. 2.
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Boxplot representation of comparison between stellar parameters provided by Gaia DR3 and spectral type from LEMC. Top: The distribution between different Teff values provided by Gaia DR3 and the spectral type estimated in LEMC. The red dashed line represents the Teff versus spectral type calibration relation from Pecaut & Mamajek (2013). Bottom: The distribution between log g values of stars from Gaia DR3 and the spectral type estimated in LEMC.
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