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Table 2: Suggested change of spectroscopic identifications of levels to ensure the completeness of spectroscopic dataset. The indexes 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. Identification of level with index 492 was changed due to use for identification its LS-configuration state function for level with index 482. Indexes of levels in the first two columns are taken from Table 1.
Table 3: Comparison of some calculated energies of Fe XIX levels with data presented by NIST ( $E^{\rm NIST}$ ). $E^{\rm McLaughlin}$ - values obtained by McLaughlin et al. (2001), $E^{\rm Butler}$ - energies calculated by Butler & Zeippen (2001), $E^{\rm GRASP}$ - our values. Indexes of levels in the first column are taken from Table 1. Energies are in cm^-1.
Table 4: Comparison of some calculated (GRASP) Fe XIX wavelengths $\lambda$ , radiative transition probabilities A^r_ki, oscillator f_ik and line S strengths with values presented by NIST. Indexes of levels in the first two columns are taken from Table 1.
Table 1: Calculated energy levels of Fe XIX with spectroscopic identification (in cm^-1) relative to the ground energy. The leading percentage compositions of levels which contributions exceed 10% are presented in the last column.
Table 5: Calculated energy levels of Fe XIX (in cm^-1) relative to the ground energy with spectroscopic notations. The five major spontaneous radiative transition probabilities A^r (in s^-1) from each level are given. Arrow marks the final level to which radiative transition happens from the level. The sum of all radiative probabilities from the corresponding level is given in the last column.