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.
Data sets Fe XXIV Fe XXIII Fe XXII Fe XXI Fe XX Fe XIX Fe XVIII

$\overline{R}_{Q_d}({\rm HFR4,AST3})$ $2.29\pm 2.75$ 1.02 $\pm$ 0.15 0.98 $\pm$ 0.11 0.81 $\pm$ 0.13 0.83 $\pm$ 0.07 1.01 $\pm$ 0.03 1.02

$\overline{R}_{B_r}({\rm HFR4,AST3})$ $0.93\pm 0.22$ 1.06 $\pm$ 0.13 1.07 $\pm$ 0.09 1.23 $\pm$ 0.16 1.26 $\pm$ 0.07 1.06 $\pm$ 0.02 1.06

**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.
Data sets	Fe XXIV	Fe XXIII	Fe XXII	Fe XXI	Fe XX	Fe XIX	Fe XVIII
$\overline{R}_{Q_d}({\rm HFR4,AST3})$	$2.29\pm 2.75$	1.02 $\pm$ 0.15	0.98 $\pm$ 0.11	0.81 $\pm$ 0.13	0.83 $\pm$ 0.07	1.01 $\pm$ 0.03	1.02
$\overline{R}_{B_r}({\rm HFR4,AST3})$	$0.93\pm 0.22$	1.06 $\pm$ 0.13	1.07 $\pm$ 0.09	1.23 $\pm$ 0.16	1.26 $\pm$ 0.07	1.06 $\pm$ 0.02	1.06

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