Table 2.
Spectral lines with their wavelength ranges, their central wavelengths and continuum regions that have been used for the calculation of their EWs, during the spectral line fitting.
Line ID | Spectral line | Continuum blue | Continuum red | ||||
---|---|---|---|---|---|---|---|
λcentral | λstart | λend | λstart | λend | λstart | λend | |
(Å) | (Å) | (Å) | (Å) | (Å) | (Å) | (Å) | |
He I | 4009 | 4004 | 4016 | 3990 | 4002 | 4035 | 4060 |
He I+He II | 4026 | 4017 | 4034 | 3990 | 4002 | 4035 | 4060 |
Si IV | 4088 | 4084 | 4091 | 4055 | 4075 | 4150 | 4170 |
H[[INLINE67]] | 4100 | 4095 | 4110 | 4055 | 4075 | 4150 | 4170 |
Si IV | 4116 | 4113 | 4118 | 4055 | 4075 | 4150 | 4170 |
He I | 4121 | 4118 | 4125 | 4035 | 4060 | 4150 | 4170 |
Si II | 4130 | 4125 | 4135 | 4035 | 4060 | 4150 | 4190 |
He I | 4144 | 4140 | 4150 | 4035 | 4060 | 4150 | 4170 |
He II | 4200 | 4190 | 4207 | 4150 | 4190 | 4245 | 4260 |
Fe II | 4233 | 4229 | 4237 | 4205 | 4225 | 4238 | 4260 |
He I | 4387 | 4382 | 4392 | 4365 | 4380 | 4398 | 4415 |
O II | 4416 | 4412 | 4421 | 4398 | 4411 | 4440 | 4460 |
He I | 4471 | 4462 | 4477 | 4440 | 4460 | 4495 | 4535 |
Mg II | 4481 | 4477 | 4488 | 4440 | 4460 | 4490 | 4505 |
He II | 4541 | 4537 | 4547 | 4510 | 4535 | 4590 | 4620 |
Si III | 4553 | 4548 | 4558 | 4485 | 4507 | 4600 | 4620 |
O II+C III | 4645 | 4635 | 4655 | 4600 | 4625 | 4660 | 4685 |
He II | 4686 | 4679 | 4692 | 4660 | 4670 | 4730 | 4745 |
Notes. We used slightly different continuum bands for VFTS, LAMOST and GOSC surveys because the different spectral resolutions of each of them can cause the presence of undesirable spectral features within the predefined continuum regions, adding noise in the data. Here, we present the continuum regions that selected for LAMOST data since their population dominates among the other surveys. This is the final scheme of features that is used through this work, except for the H[[INLINE68]]/4100 Å spectral line, which is used only for the fit.
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