Table A.4.
Visual and UVA spectral lines used for the abundance determination.
Element+ion. stage | Wavelength (Å) |
---|---|
C III | 3883.81 |
C III | * |
* | 3608.78 |
* | 3609.05 |
* | 3609.07 |
* | 3609.62 |
* | 3609.68 |
C III | 4056.06 |
C III | * |
* | 4067.94 |
* | 4068.91 |
* | 4070.26 |
C III | 4121.85 |
C III | 4186.90 |
C III | 4247.31 |
C III | 4325.56 |
C III | 4361.85 |
C III | 4382.90 |
C III | 4516.79 |
C III | * |
* | 4647.42 |
* | 4650.25 |
* | 4651.02 |
* | 4651.47 |
* | 4652.05 |
C III | 5695.92 |
C III | * |
* | 6149.28 |
* | 6154.16 |
* | 6155.12 |
* | 6156.69 |
* | 6160.01 |
C IV | 4658.30 |
C IV | * |
* | 5016.62 |
* | 5018.40 |
C IV | * |
* | 5801.33 |
* | 5811.97 |
N II | 3838.37 |
N II | 3842.19 |
N II | 3995.00 |
N II | 4176.16 |
N II | 4227.74 |
N II | 4447.03 |
N II | 4694.27 |
N II | 4779.72 |
N II | 4788.13 |
N II | 4803.29 |
N II | 4987.38 |
N II | 5002.80 |
N II | 5007.32 |
N II | 5010.62 |
N II | 5025.66 |
N II | 5045.10 |
N II | 5495.67 |
N II | 5666.63 |
N II | 5676.02 |
N II | 5679.56 |
N II | 5686.21 |
N II | 5710.77 |
N II | 5931.78 |
N III | 3004.03 |
N III | 3330.11 |
N III | 3342.09 |
N III | * |
* | 3353.98 |
* | 3354.32 |
N III | * |
* | 3360.98 |
* | 3365.80 |
N III | * |
* | 3365.80 |
* | 3367.30 |
* | 3374.07 |
N III | * |
* | 3754.62 |
* | 3757.65 |
* | 3762.60 |
N III | * |
* | 3771.05 |
* | 3771.36 |
N III | 3792.97 |
N III | 3938.52 |
N III | 3942.88 |
N III | * |
* | 3998.63 |
* | 4003.58 |
N III | 4097.33 |
N III | 4103.39 |
N III | 4195.70 |
N III | 4200.02 |
N III | 4215.77 |
N III | 4318.78 |
N III | * |
* | 4318.78 |
* | 4321.22 |
* | 4325.43 |
* | 4327.88 |
N III | * |
* | 4332.91 |
* | 4337.01 |
N III | * |
* | 4345.68 |
* | 4345.81 |
* | 4351.11 |
N III | * |
* | 4514.86 |
* | 4518.91 |
N III | 4523.56 |
N III | 4530.86 |
N III | 4534.58 |
N III | 4547.30 |
N III | * |
* | 4589.18 |
* | 4591.98 |
N III | 4634.14 |
N III+ He II&Hβ | * |
* | 4858.82 |
* | 4861.22 |
* | 4867.15 |
N III | 4873.10 |
N III | 4884.14 |
N III | * |
* | 5260.86 |
* | 5270.57 |
* | 5272.68 |
* | 5282.43 |
N III | * |
* | 5297.75 |
* | 5298.95 |
N III* | |
* | 5314.35 |
* | 5320.32 |
* | 5327.18 |
N III | * |
* | 5817.79 |
* | 5820.57 |
N III | 5847.94 |
N III | 5954.70 |
N IV | * |
* | 3478.71 |
* | 3482.99 |
* | 3484.96 |
N IV | 4057.76 |
N IV | 6380.77 |
O II | 3759.87 |
O II | 3857.16 |
O II | 4069.89 |
O II | 4072.15 |
O II | 4075.86 |
O II | * |
* | 4307.23 |
* | 4312.10 |
* | 4313.44 |
* | 4317.14 |
* | 4317.70 |
* | 4319.63 |
* | 4325.75 |
O II | 4349.42 |
O II | 4336.87 |
O II | 6152.56 |
O III | 3340.74 |
O III | 3459.48 |
O III | 3715.08 |
O III | 3757.21 |
O III | 3759.87 |
O III | 5592.37 |
O III | 6507.55 |
Ne II | 3323.73 |
Ne II | 3327.15 |
Ne II | 3388.41 |
Ne II | 3406.94 |
Ne II | * |
* | 3416.91 |
* | 3417.69 |
Ne II | 3542.84 |
Ne II | * |
* | 3565.82 |
* | 3568.50 |
* | 3571.23 |
* | 3574.61 |
Ne II | * |
* | 3643.93 |
* | 3644.86 |
Ne II | 3664.07 |
Ne II | 3694.21 |
Ne II | 3709.62 |
Ne II | 3713.08 |
Ne II | 3727.11 |
Ne II | 3766.26 |
Ne II | 3777.13 |
Ne II | 4150.69 |
Ne II | * |
* | 4217.17 |
* | 4219.37 |
* | 4219.74 |
Ne II | 4250.64 |
Ne II | * |
* | 4290.37 |
* | 4290.60 |
Ne II | 4379.55 |
Ne II | 4397.99 |
Ne II | * |
* | 4409.30 |
* | 4412.59 |
Ne II | * |
* | 4428.52 |
* | 4428.63 |
* | 4430.90 |
* | 4431.81 |
Mg II | 4242.45 |
Mg II | * |
* | 4481.13 |
* | 4481.33 |
Mg II | * |
* | 5916.43 |
* | 5918.16 |
Mg II | 5928.23 |
Mg II | * |
* | 6346.74 |
* | 6346.96 |
Al III | 3601.63 |
Al III | 4149.96 |
* | 4159.91 |
* | 4149.96 |
* | 4150.17 |
Al III | * |
* | 4479.83 |
* | 4479.97 |
Al III | 4512.57 |
Al III | 5722.73 |
Al III | 5696.60 |
Si III | 3486.91 |
Si III | 3791.41 |
Si III | 3806.54 |
Si III | 3924.47 |
Si III | 4552.65 |
Si III | 4567.87 |
Si III | 4574.78 |
Si III | 4716.66 |
Si III | 4813.39 |
Si III | 4819.72 |
Si III | 5739.73 |
Si IV | 3773.15 |
Si IV | 4088.86 |
Si IV | 4116.10 |
Si IV | 4212.41 |
Si IV | 4314.10 |
Si IV | 4631.24 |
Si IV | 4654.32 |
Si IV | 4950.11 |
P IV | 3347.74 |
P IV | 3364.47 |
P IV | 4249.66 |
P IV | 4728.37 |
P V | 5122.19 |
S III | 3632.02 |
S III | 3662.01 |
Notes. The profiles of some spectral lines were calculated together, either because they are closely blended lines or resolved multiple lines, for which no lines from other species intervene (e.g. Ne II, 3643.93/3644.86 Å, see Fig. 6). The wavelengths of such “combined” lines are marked by asterisks.
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