Table 3.
Summary statistics of the detailed analysis of chosen representative stars and the normalisation of synthetic spectra.
| Star | HD 155806 | HD 90882 | HD 27411 | HD 37495 | HD 59967 | HD 25069 |
|---|---|---|---|---|---|---|
| Spectral type | O7.5 V | B9.5 V | A3m | F4 V | G4 V | K0 III |
| SUPPNet (synth) |
 |
 |
 |
 |
 |
 |
| SUPPNet (active) |
 |
 |
 |
 |
 |
 |
| SUPPNet (synth) |
 |
 |
 |
 |
 |
 |
| SUPPNet (active) |
 |
 |
 |
 |
 |
 |
| NP–TR |
 |
 |
 |
 |
 |
 |
| EN–TR |
 |
 |
 |
 |
 |
 |
Notes. Each value is reported in the following format: the main number is the median of residuals with 15.87 percentile in the upper index and 84.13 percentile in the lower index. The first two rows summarise the quality of normalisation of related synthetic spectra distorted with pseudo-continuum fits obtained from manual normalisation (see Sect. 4.1 for details). Here, contrary to the results on observed spectra, the correct normalisation is known, and the best values are in bold. The four bottom rows contain the statistics of SUPPNet and manual normalisation residuals. Manual normalisation of TR was used as the reference. All those residuals and statistics were calculated in the wavelength range from 3900 Å to 7000 Å (see the Sect. 4.3 for details).
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