All Tables

Table 1: Atomic data for the isotopic components of Ca II $\lambda~8498$ . The fractional isotope abundances $\epsilon$ correspond to solar-system matter.
Table 2: NLTE abundance corrections^* (dex) for the Ca I and Ca II lines depending on effective temperature, surface gravity, and metallicity as computed by ignoring hydrogenic collisions ( $S_{\rm H}$ = 0) in SE calculations.
Table 3: Uncertainties in the NLTE analysis of Ca I/II, where blanks denote NLTE theoretical equivalent widths below 5 mÅ.
Table 4: Atomic data for the Ca I and Ca II lines, solar $\log gf\varepsilon_{\rm Ca}^\odot$ values determined from NLTE analysis of the Ca line profiles in the Kitt Peak Solar Atlas (Kurucz et al. 1984) neglecting hydrogenic collisions ( $S_{\rm H}$ = 0), and abundance corrections $\Delta_{\rm X} = \log\varepsilon_{\rm X} - \log\varepsilon_{\rm S_H = 0}$ where X takes the meaning 0.1, 1, and LTE for $S_{\rm H}$ = 0.1, $S_{\rm H}$ = 1 and the LTE assumption, respectively.
Table 5: Stellar parameters and obtained NLTE elemental abundance ratios of the selected stars.