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For the first time, we present an extensive study of stars with individualnon-local thermodynamic equilibrium (NLTE) abundances for 17 chemical elementsfrom Li to Eu in a sample of stars uniformly distributed over the $-2.62 \le$[Fe/H] $\le +0.24$ metallicity range that is suitable for the Galactic chemicalevolution research. The star sample has been kinematically selected to tracethe Galactic thin and thick disks and halo. We find new and improve earlierresults as follows. (i) The element-to-iron ratios for Mg, Si, Ca, and Ti forma MP plateau at a similar height of 0.3~dex, and the knee occurs at common[Fe/H] $\simeq -0.8$. The knee at the same metallicity is observed for [O/Fe],and the MP plateau is formed at [O/Fe] = 0.61. (ii) The upward trend of [C/O]with decreasing metallicity exists at [Fe/H] $< -1.2$, supporting the earlierfinding of Akerman et al. (iii) An underabundance of Na relative to Mg in the[Fe/H] $< -1$ stars is nearly constant, with the mean [Na/Mg] $\simeq -0.5$.(iv) The K/Sc, Ca/Sc, and Ti/Sc ratios form well-defined trends, suggesting acommon site of the K-Ti production. (v) Sr follows the Fe abundance down to[Fe/H] $\simeq -2.5$, while Zr is enhanced in MP stars. (vi) The comparisons ofour results with some widely used Galactic evolution models are given. The useof the NLTE element abundances raises credit to the interpretation of the datain the context of the chemical evolution of the Galaxy.

Systematic non-LTE study of the $-2.6 \le$ [Fe/H] $\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu