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Table 5

Comparison between HFR and other Kβ/Kα UTA line ratios.

Z N Kβ/Kα
HFRa ASb MCDFc EXPd FITh

15 14 0.050 0.044 0.058 0.043(4)
17 16 0.084 0.080 0.086 0.077(4)
19 18 0.104 0.107 0.108 0.1103(24)
21 20 0.107 0.112 0.118 0.1187(21)
22 21 0.111 0.114 0.121 0.1231(17)f 0.1193(18)
23 22 0.113 0.114 0.124 0.1247(17)f 0.1201(16)
24 23 0.116 0.115 0.126 0.125e 0.1211(14)
0.1260(17)f
25 24 0.117 0.114 0.127 0.126e 0.1223(14)
0.1256(17)f
0.119(11)g
27 26 0.121 0.114 0.129 0.123e 0.1235(14)
0.1247(17)f
0.123(11)g
29 28 0.123 0.109 0.130 0.127e 0.1252(14)
0.1249(17)f
0.125(13)g
30 29 0.124 0.108 0.130 0.127(10)g 0.1275(12)

Notes.

(a)

HFR calculations. This work. Summed over all the fine-structure lines.

(b)

AUTOSTRUCTURE calculations. This work. Summed over all the fine-structure lines.

(c)

MCDF-EAL calculations. This work. Summed over all the fine-structure lines.

(d)

Experimental values are scaled down by a scaling factor of 0.9 for ions with 17  ≤  Z  ≤  30 in order to delete the radiative Auger and the solid-state Kβ5 emission contributions not considered in our free atom models (Török et al. 1996; Bé et al. 1998; Verma 2000).

(e)

Measurements by Hölzer et al. (1997).

(f)

Measurements by Bé et al. (1998). The number in parenthesis is the error affecting the last digits.

(g)

Measurements by Öz (2006). The number in parenthesis is the error affecting the last digits.

(h)

Empirical fit by Schönfeld & Janssen (1996). The number in parenthesis is the error affecting the last digits. Values are scaled down by a scaling factor of 0.9 for ions with 17 ≤ Z ≤ 30 in order to delete the radiative Auger and the solid-state Kβ5 emission contributions not considered in our free atom models (Török et al. 1996; Bé et al. 1998; Verma 2000).

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