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Table 3

Measured longitudinal field Bl and null polarization Nl, with their error bars σ.

Star Date Comp. B l N l σ
HD G G G

36486 23.10.08 43 13 38
24.10.08 18 1 7
37468 17.10.08 prim –3 35 19
sec 16 –18 9
47839 10.12.06 prim –27 17 25
sec –260 –173 210
15.12.06 prim –6 14 13
sec 5 256 185
09.09.07 prim 3 –13 20
sec –243 –173 210
10.09.07 prim 8 7 15
sec –41 278 154
11.09.07 prim 14 –14 23
sec –141 –95 211
20.10.07 prim –9 4 13
sec –98 146 140
23.10.07 prim –1 23 12
sec –27 –154 142
02.02.12 prim –6 –4 10
sec 17 22 132
93250 17.02.13 –24 175 135
151804 26.05.11 –13 –34 33
152408 05.07.12 2 60 34
164794 19.06.05 –3 –18 52
20.06.05 –2 44 52
23.06.05 64 25 50
25.05.11 6 87 54
14.06.11 61 29 27
167971 30.06.13 prim 3 –16 40
sec 98 16 59
ter –19 –216 115
190918 25.07.10 8 93 70

Notes. When several components are visible in the spectra, the values were estimated for each component (primary, secondary, and possibly tertiary).

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