Open Access

Table B.1

Spectral lines included in the likelihood evaluation.

Element Lines (Å)
H Balmer series Hϵ to Hα
He i 4026, 4387, 4471, 4713, 4922, 5015, 5048, 5876, 6678, 7065, 7281 (not used) 3820, 3868, 3889, 3927, 3965, 4009, 4024, 4120, 4143, 4437
He ii 4200, 4541, 5411, 6683
C ii 3919, 3920, 4267, 6578, 6582
C iii 4056, 4069, 4163, 4187, 4517, 4664, 4666, 4674, 5273, 5826, 8500
C iv 5801, 5811
N ii 3995, 4004, 4035, 4041, 4447, 4607, 4803, 5001, 5005, 5011, 5026, 5045, 5676, 5680, 6480
N iii 3999, 4003, 4511, 4515, 4518, 4523, 4527, 4634
O i 6156-7-8, 7772-4-5
O ii 3792, 3913, 3955, 3963, 4277–78, 4284, 4305, 4318, 4321, 4368, 4416, 4418, 4592, 4597, 4603, 4611, 4663, 4678, 4700, 4707, 4945, 6721
O iii 4073, 4074, 4081, 4611, 5268, 5508, 7711
Mg ii 4481, 7877, 7896
Si ii 4128, 4130, 6347, 6371
Si iii 4553, 4568, 4575, 4716, 4813, 4820, 4829, 5740
Si iv 3762, 4116, 4212, 4631, 4654, 6668, 6701

Notes. These features constitute the set of diagnostics used by MAUI to constrain the stellar and wind parameters and chemical abundances.

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