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Table B.1

Ions and number of levels, superlevels, and transitions considered per ion used in our B supergiant models. The group letters indicate whether the ion is used in the early set (E), representing models hotter than 21 kK, or in the late set (L).

Ion group levels superlevels transitions
H I EL 30 30 435

He I EL 69 69 905
He II EL 30 30 435

C II EL 39 21 202
C III EL 243 99 5528
C IV EL 64 64 1446

N I L 104 44 855
N II EL 105 59 898
N III EL 287 57 6223
N IV EL 70 44 440
N V EL 49 41 519

O I L 199 58 4193
O II EL 340 137 8937
O III EL 104 36 761
O IV EL 64 30 359
O V EL 56 32 314
O VI E 65 65 1569

Ne II EL 48 14 328
Ne III EL 71 23 460
Ne IV EL 52 17 315
Ne V EL 166 37 1813

Mg II EL 45 18 362
Mg III EL 201 29 3052

Al II EL 58 38 270
Al III EL 65 21 1452

Si II EL 80 52 628
Si III EL 147 99 1639
Si IV EL 66 66 1090

P IV EL 90 30 656
P V EL 62 16 561

S III EL 44 24 193
S IV EL 142 51 1503
S V EL 101 40 831

Ca III EL 110 33 868
Ca IV E 378 43 8532
Ca V E 613 73 18272

Cr II L 1000 84 66400
Cr III EL 1000 68 73962
Cr IV EL 234 29 6354
Cr V E 223 30 4124
Cr VI E 215 30 4406

Mn II L 1000 58 49066
Mn III EL 1000 47 70218
Mn IV EL 464 39 19176
Mn V E 80 16 867
Mn VI E 181 23 2005

Fe II L 827 62 13182
Fe III EL 607 65 6670
Fe IV EL 1000 100 37899
Fe V EL 1000 139 37737
Fe VI E 1000 59 6670

Ni II L 1000 59 33555
Ni III EL 150 24 1345
Ni IV EL 200 36 2337
Ni V EL 183 46 1524

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