Table 2
Formulae to estimate the summed up flux in an 1 Å-window in the center of all three Ca ii IRT lines for inactive objects.
| Estimated total flux in 1 Å-bandpasses in all Ca ii IRT lines | ||||||
| Object | B − V | log g | [Fe/H] |
|
in 106 erg s-1 cm-2 | from normalized spectra in Å |
|
|
||||||
| HD 739 | 0.40 | 4.27 | –0.09 | –4.91 |
|
|
| HD 159332 | 0.45 | 3.85 | –0.23 | –4.99 |
|
|
| HD 216385 | 0.48 | 3.95 | –0.29 | –4.98 |
|
|
| HD 45067 | 0.53 | 4.01 | –0.09 | –4.90 |
|
|
| HD 187691 | 0.56 | 4.26 | +0.10 | –4.89 |
|
|
| HD 100180 | 0.57 | 4.25 | –0.06 | –4.76 |
|
|
| HD 124570 | 0.58 | 4.05 | +0.08 | –5.05 |
|
|
| HD 19373 | 0.59 | 4.21 | +0.08 | –4.84 |
|
|
| HD 168009 | 0.60 | 4.23 | –0.01 | –4.77 |
|
|
| HD 10307 | 0.62 | 4.32 | +0.03 | –4.84 |
|
|
| HD 157214 | 0.62 | 4.31 | –0.40 | –4.80 |
|
|
| HD 34411 | 0.62 | 4.22 | +0.08 | –4.85 |
|
|
| HD 95128 | 0.62 | 4.30 | +0.01 | –4.85 |
|
|
| HD 38858 | 0.64 | 4.48 | –0.22 | –4.79 |
|
|
| HD 146233 | 0.65 | 4.42 | +0.03 | –4.75 |
|
|
| HD 186427 | 0.65 | 4.32 | +0.07 | –4.80 |
|
|
| HD 12846 | 0.66 | 4.38 | –0.26 | –4.78 |
|
|
| HD 43587 | 0.67 | 4.29 | –0.04 | –4.80 |
|
|
| HD 115617 | 0.70 | 4.39 | –0.01 | –4.80 |
|
|
| HD 178428 | 0.70 | 4.25 | +0.14 | –4.88 |
|
|
| HD 3795 | 0.70 | 3.91 | –0.63 | –4.83 |
|
|
| HD 117176 | 0.71 | 3.97 | –0.06 | –4.90 |
|
|
| HD 10700 | 0.72 | 4.48 | –0.50 | –4.75 |
|
|
| HD 26965 | 0.85 | 4.51 | –0.27 | –4.89 |
|
|
| HD 75732 | 0.87 | 4.41 | +0.28 | –4.84 |
|
|
| HD 145675 | 0.90 | 4.45 | +0.41 | –4.80 |
|
|
Notes. vrot must be entered in units of km s-1. To obtain the best fit, it is recommended to compare the values from normalized spectra and to subtract an additional 20 mÅ, as described in the text. Values for B − V, log g and [Fe/H] are taken from Soubiran et al. (2010).
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