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Table A.1

Atomic data used in the HD models.

Ion Levels Linesa Ion Levels Linesa
H I 22 231 Si III 24 69
H II 1 0 Si IV 23 (23) 72 (69)
He I 35 271 Si V 11 (23) 11 (48)
He II 26 325 Si VI 0 (1) 0 (0)
He III 1 0 P III 1 (47) 0 (175)
C I 15 (10) 30 (10) P IV 12 16
C II 32 148 P V 11 22
C III 40 226 P VI 1 0
C IV 25 230 S I 30 (5) 76 (4)
C V 10 13 S II 32 (15) 80 (18)
C VI 1 (10) 10 (45) S III 23 38
C VII 0 (1) 0 (0) S IV 25 54
N I 10 13 S V 10 13
N II 38 (20) 201 (29) S VI 22 (10) 75 (21)
N III 30 94 S VII 0 (1) 0 (0)
N IV 38 154 Cl III 1 0
N V 20 114 Cl VI 24 (15) 34 (17)
N VI 14 48 Cl V 18 29
N VII 1 (10) 0 (7) Cl VI 23 46
N VIII 0 (1) 0 (0) Cl VII 1 0
O I 13 (10) 15 (9) Ar I 14 (10) 34 (17)
O II 37 150 Ar II 20 (10) 33 (9)
O III 33 121 Ar III 14 (10) 13 (8)
O IV 29 77 Ar IV 13 20
O V 36 (54) 153 (260) Ar V 10 11
O VI 16 101 Ar VI 9 11
O VII 1 (15) 0 (64) Ar VII 20 34
O VIII 0 (15) 0 (105) Ar VIII 1 0
O IX 0 (1) 0 (0) K I 20 (15) 48 (32)
Ne I 8 (10) 14 (26) K II 20 (15) 56 (30)
Ne II 18 (10) 40 (9) K III 20 (10) 40 (12)
Ne III 18 18 K IV 23 (10) 27 (9)
Ne IV 35 (20) 159 (26) K V 19 (10) 33 (16)
Ne V 20 23 K VI 1 0
Ne VI 20 35 Ca I 20 (15) 35 (24)
Ne VII 1 (10) 0 (11) Ca II 20 (15) 48 (31)
Ne VIII 0 (10) 0 (20) Ca III 14 18
Ne IX 0 (10) 0 (13) Ca IV 24 43
Ne X 0 (10) 0 (13) Ca V 15 12
Ne XI 0 (1) 0 (0) Ca VI 15 17
Mg I 1 0 Ca VII 20 28
Mg II 20 57 Ca VIII 1 0
Mg III 20 41 FebI 1 0
Mg IV 17 27 FebII 3 [15 077] 2 [3 688 311]
Al I 10 (1) 16 (0) FebIII 13 [15 233] 40 [2 888 649]
Al II 10 11 FebIV 18 [30 302] 77 [7 230 222]
Al III 10 18 FebV 22 [20 639] 107 [5 924 318]
Al IV 10 10 FebVI 29 [17 728] 194 [3 948 149]
Al V 10 9 FebVII 19 [16 752] 87 [4 002 080]
Al VI 1 0 FebVIII 1 0
Si I 20 (3) 45 (2)
Si II 20 35 Total 1524 (1486) 4976 (4783)

Notes. The numbers in parentheses refer to the model with the high X-ray illumination, which requires the inclusion of higher ionization stages. The numbers in parentheses refer to the model with the high X-ray illumination, which requires the inclusion of higher ionization stages. (a) Number of transitions with non-negligible oscillator strengths as considered in the radiative transfer calculations. (b) For Fe, the large numbers refer to superlevels and superline transitions that are used to cope with the enormous number of lines and transitions given as smaller numbers in brackets. The atom listed as Fe here is a generic element that also includes the iron group elements Sc, Ti, V, Cr, Mn, Co, and Ni (see Gräfener et al. 2002, for details).

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