Table 5.
Mean magnetic field characteristics derived in this study in comparison with the global magnetic field strength inferred with ZDI.
| Star | B (kG) | f | ⟨B⟩ (kG) | ⟨BV⟩ (G) | ZDI reference |
|---|---|---|---|---|---|
| HD 1835 |  |
 |
 |
19 | Rosén et al. (2016) |
| HD 20630 |  |
 |
 |
 |
Rosén et al. (2016) |
| HD 29615 |  |
 |
 |
89 | Hackman et al. (2016) |
| HD 39587 |  |
 |
 |
 |
Rosén et al. (2016) |
| HD 56124 |  |
 |
 |
2.2 | See et al. (2019) |
| HD 72905 |  |
 |
 |
 |
Rosén et al. (2016) |
| HD 73350 (a) |  |
 |
 |
11 | Petit et al. (2008) |
| HD 76151 (a) |  |
 |
 |
3.0 | Petit et al. (2008) |
| HD 82558 |  |
 |
 |
 |
Lehtinen et al. (2020) |
| HD 129333 |  |
 |
 |
 |
Waite et al. (2017) |
| HD 131156A (a) |  |
 |
 |
 |
Morgenthaler et al. (2012) |
| HD 166435 |  |
 |
 |
20 | See et al. (2019) |
| HD 175726 |  |
 |
 |
10 | See et al. (2019) |
| HD 190771 (a) |  |
 |
 |
14 | Petit et al. (2008) |
| HD 206860 |  |
 |
 |
 |
Rosén et al. (2016) |
Notes. The fifth column lists the mean ZDI field strength, ⟨BV⟩, taken from the references listed in the last column. For stars with multiple ZDI maps, column five gives the median field strength and the error bars corresponding to extreme values.
⟨BV⟩ is given according to the compilation by See et al. (2019).
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