All Tables

Table 3: Comparison of A-value data sets for Fe XVIII-Fe XXIV in terms of mean ratios.
Table 4: Radiative transition rates (s^-1) in SAF that show large discrepancies with AST3. Note: $a\pm\!b\equiv a\times 10^{\pm b}$ .
Table 5: Radiative transition rates (s^-1) in MCDF that show large discrepancies with AST3. Note: $a\pm\!b\equiv a\times 10^{\pm b}$ .
Table 6: Comparison of Auger rate data sets for Fe XVIII-Fe XXIV in terms of mean ratios.
Table 7: Comparison of satellite intensity $Q_{\rm d}$ factors and radiative branching ratios, $B_{\rm r}$ , for Fe XVIII-Fe XXIV in terms of mean ratios.
Table 1: Energies, total radiative and Auger widths and fluorescence yields for levels within the n=2 complex of N-electron ( $2\leq N\leq 9$ ) Fe ions. Note: $a\pm\!b\equiv a\times 10^{\pm b}$ .
Table 2: Wavelengths and radiative rates for N-electron Fe ions. Note: $a\pm\!b\equiv a\times 10^{\pm b}$ .
Table 8: Transition energies and partial Auger rates for N-electron Fe ions. Note: $a\pm\!b\equiv a\times 10^{\pm b}$ .