Comparison of atmospheric parameters for targets with high resolution spectroscopic determinations. We plot out T_eff in the x axis and the difference (our minus literature) and the error from literature on the y-axis. In the right column we show the different sources in NGC 2682 and in the left column all other clusters. Ref: (1) Jacobson et al. (2011); (2) APOGEE DR16; (3) (Casamiquela et al. 2017) EW; (4) Casamiquela et al. (2017) SS; (5) Gao et al. (2018); (6) Luck (2015); (7) Spina et al. (2021).