All Tables

Table 1: MCDF results for energy levels of Fe XXII. The energies of levels are presented relative to the ground energy. The leading percentage compositions (>10%) of levels are provided in the last column.
Table 2: Suggested change of spectroscopic identifications of levels to ensure the completeness of spectroscopic dataset. The indices of levels for which spectroscopic identifications are changed are presented in the first column. The second column contains index of level with the same highest contribution of configuration state function (Table 1) as level from the first column before change. Indices of levels in the first two columns are taken from Table 1.
Table 3: Comparison of calculated energies $E^{{\rm GRASP}}$ and $E^{{\rm CITRO}}$ for Fe XXII levels with data compiled by NIST ( $E^{{\rm NIST}}$ ). Indices of levels in the first column and CSFs in the second column are taken from Table 1. Energies are in cm^-1. The lifetimes of levels are presented in the last two columns.
Table 4: Comparison of calculated wavelengths ( $\lambda ^{{\rm GRASP}}$ , $\lambda ^{{\rm CITRO}}$ ) and line strengths ( $S^{{\rm GRASP}}$ , $S^{{\rm CITRO}}$ ) for Fe XXII with values presented by NIST ( $\lambda ^{{\rm NIST}}$ , $S^{{\rm NIST}}$ ). Indices of levels in the first two columns are taken from Table 1.
Table 5: The five major spontaneous radiative transition probabilities A^r from each level of Fe XXII and the sum of all radiative probabilities $\sum A^{r}$ from the corresponding level. Electric dipole, quadrupole and octupole as well as magnetic dipole and quadrupole transitions are included. Arrow marks the final level to which radiative transition happens from the level.