Table B.3
Pfund β line fluxes and FWHM values for the programme stars.
| Target | FWHM | Error | Line flux | Error |
| [km s-1] | [km s-1] | [erg cm-2 s-1 ] | [erg cm-2 s-1 ] | |
|
|
||||
| HD 100546 | 218 | 17 | 8.75 × 10-13 | 1.31 × 10-13 |
| HD 97048 | 149 | 10 | 5.71 × 10-13 | 9.99 × 10-14 |
| HD 179218 | 150 | 10 | 8.19 × 10-13 | 9.35 × 10-14 |
| HD 101412 | – | – | <8.7 × 10-14 | |
| HD 141569 | 420 | 60 | 1.19 × 10-13 | 3.32 × 10-14 |
| HD 190073 | 92 | 9 | 3.41 × 10-13 | 8.68 × 10-14 |
| HD 98922 | 140 | 12 | 1.07 × 10-12 | 2.67 × 10-13 |
| HD 95881⋆ | – | – | – | – |
| R CrA | 230 | 40 | 2.82 × 10-12 | 6.45 × 10-13 |
| HD 135344B | 142 | 10 | 8.06 × 10-14 | 4.03 × 10-15 |
| HD 150193⋆ | – | – | – | – |
| HD 104237 | 117 | 14 | 1.08 × 10-12 | 1.14 × 10-13 |
| HD 142666 | 325 | 30 | 5.82 × 10-14 | 1.77 × 10-13 |
Notes. Line fluxes are calculated using the continuum fluxes listed in Table B.1. We note that for HD 95881 and HD 150193 (marked with a “⋆”), the Pfund β line there are lines visible in the raw spectra and have a respective FWHM of ≈100 and 180 km s-1 and a maximum intensity of ≈20% and 15% above the continuum. Because of the presence of Pfund β emission in the spectrum of the telluric standard star we are unable to calculate the line fluxes, and therefore do not list these values in the table.
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