The chemical evolution of the Milky Way thin disk using solar twins

Open Access

Fig. 3

Comparison of age and metallicity derived by different methods. Left: comparison of age derived in this work and in Casali et al. (2020). Middle: comparison of age derived in this work and in Nissen et al. (2020) (blue circles), its mean difference $(\bar{d i f_{age}})$ $\left( {\overline {di{f_{{\rm{age }}}}} } \right)$ , and standard deviation (SD); comparison of age derived in Casali et al. (2020) and in Nissen et al. (2020) (gray circles). Right: comparison of metallicity derived in this work and in Nissen et al. (2020).

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