Fig. 11.
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Teff − log g diagram of the Gaia-ESO clusters. Only data analysed in this work with the SAPP are shown. In each panel, the black solid circles are a star with corresponding error bars in Teff and log g. There are three isochrones varying in age (blue youngest, orange median, green oldest) which have a metallicity close to the average [Fe/H] of the cluster.
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