Fig. 5
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Kiel diagrams of main-sequence member stars in NGC 2516 (archival spectra from the Gaia-ESO survey). In red the parsec isochrone corresponding to the age and metallicity of NGC 2516, [Fe/H] = −0.04 ± 0.04 from Randich et al. (2022). Left panel: Stellar parameters derived from pure spectroscopic analysis. Right panel: Stellar parameters from the spectro-photometric method.
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