Table 3.
Results from the magnetic field inference including both the two- and multi-component models.
| Two-component model |
Multi-component model |
|||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Star | Night | ⟨B⟩I (kG) | B (kG) | fB | εFe | vmac (km s−1) | ⟨B⟩I (kG) | f1 | f2 | f3 | εFe | vmac (km s−1) |
| HD 1835 | 21-10-30 | 0.279(17) | 1.517(61) | 0.184(13) | −4.350(2) | 4.28(20) | 0.330(20) | 0.170(20) | 0.080(10) | – | −4.381(2) | 4.06(20) |
| HD 3651 | 21-10-30 | 0.092(06) | 1.547(70) | 0.059(05) | −4.413(1) | 1.47(8) | 0.121(07) | 0.059(08) | 0.031(03) | – | −4.419(2) | 1.15(12) |
| HD 9986 | 21-10-30 |
 |
 |
 |
−4.479(3) | 2.84(12) | 0.049(09) | 0.014(09) | 0.017(05) | – | −4.477(2) | 0.83(12) |
| HD 10476 | 21-10-30 | 0.065(10) | 0.870(86) | 0.075(15) | −4.569(2) | 1.85(12) | 0.060(09) | 0.060(09) | – | – | −4.573(2) | 1.90(10) |
| HD 20630 | 22-02-07 | 0.277(13) |
 |
0.141(08) | −4.460(3) | 3.95(13) | 0.382(20) | 0.103(18) | 0.087(11) | 0.035(07) | −4.463(3) | 3.35(18) |
| HD 22049 | 22-02-09 | 0.209(07) | 1.646(34) | 0.127(05) | −4.569(1) | 2.07(9) | 0.316(11) | 0.124(09) | 0.060(05) | 0.024(04) | −4.572(2) | 1.12(20) |
| HD 59967 | 21-10-30 | 0.250(15) | 1.712(59) | 0.146(10) | −4.536(2) | 3.72(15) | 0.306(18) | 0.102(18) | 0.102(08) | – | −4.542(2) | 3.40(18) |
| HD 59967 | 22-02-09 | 0.375(13) | 1.940(42) | 0.193(08) | −4.524(2) | 3.47(14) | 0.498(22) | 0.115(19) | 0.132(11) | 0.040(07) | −4.530(3) | 2.65(25) |
| HD 59967 | 22-03-23 | 0.316(14) | 1.949(57) | 0.162(09) | −4.534(3) | 3.50(15) | 0.431(24) | 0.108(20) | 0.109(11) | 0.035(06) | −4.540(3) | 2.76(25) |
| HD 59967 | 22-03-24 | 0.339(14) | 2.145(59) | 0.158(08) | −4.517(3) | 3.87(13) | 0.474(23) | 0.101(22) | 0.100(11) | 0.057(07) | −4.524(3) | 3.00(22) |
| HD 59967 | 22-03-30 | 0.336(14) |
 |
0.171(09) | −4.521(2) | 3.79(14) | 0.440(23) | 0.096(21) | 0.122(11) | 0.033(08) | −4.528(3) | 3.15(22) |
| HD 73256 | 21-10-08 | 0.279(11) | 1.611(51) | 0.174(09) | −4.290(3) | 3.79(11) | 0.359(15) | 0.153(15) | 0.103(07) | – | −4.300(2) | 3.33(15) |
| HD 73256 | 21-10-30 | 0.255(12) | 1.556(49) | 0.164(10) | −4.299(3) | 3.31(13) | 0.322(15) | 0.144(15) | 0.089(07) | – | −4.308(3) | 2.90(14) |
| HD 73256 | 22-02-07 | 0.264(09) | 1.513(31) | 0.174(07) | −4.310(2) | 2.81(10) | 0.336(12) | 0.162(11) | 0.087(05) | – | −4.318(2) | 2.29(14) |
| HD 73256 | 22-03-30 | 0.262(10) | 1.544(30) | 0.170(08) | −4.316(2) | 2.76(11) | 0.344(13) | 0.160(11) | 0.092(05) | – | −4.326(2) | 2.08(17) |
| HD 73350 | 22-02-09 | 0.157(12) | 1.585(77) | 0.099(10) | −4.432(2) | 3.66(11) | 0.210(15) | 0.090(14) | 0.060(06) | – | −4.438(2) | 3.39(13) |
| HD 73350 | 22-03-10 | 0.152(12) | 1.359(55) | 0.112(11) | −4.455(2) | 3.51(11) | 0.190(16) | 0.112(14) | 0.039(06) | – | −4.459(2) | 3.37(13) |
| HD 73350 | 22-03-30 | 0.137(14) | 1.412(73) | 0.097(11) | −4.452(2) | 3.68(11) | 0.176(16) | 0.094(15) | 0.041(06) | – | −4.457(2) | 3.53(14) |
| HD 75732 | 22-03-23 | 0.052(08) | 0.927(91) | 0.056(11) | −4.331(2) | 1.56(10) | 0.050(07) | 0.050(07) | – | – | −4.338(2) | 1.57(10) |
| HD 76151 | 22-02-07 | 0.111(10) | 1.160(66) | 0.096(11) | −4.451(2) | 2.76(9) | 0.135(12) | 0.101(12) | 0.017(05) | – | −4.456(2) | 2.65(10) |
| HD 76151 | 22-03-30 | 0.096(10) | 1.133(66) | 0.084(11) | −4.460(2) | 2.67(9) | 0.115(12) | 0.087(11) | 0.014(05) | – | −4.464(2) | 2.58(10) |
| HD 102195 | 22-03-11 | 0.226(08) |
 |
0.145(07) | −4.416(2) | 2.33(10) | 0.335(13) | 0.143(10) | 0.061(07) | 0.023(05) | −4.421(2) | 1.56(16) |
| HD 130322 | 22-03-23 | 0.081(10) |
 |
0.064(11) | −4.522(2) | 2.38(10) | 0.107(12) | 0.064(11) | 0.021(05) | – | −4.526(2) | 2.26(10) |
| HD 131156A | 22-03-23 | 0.299(13) | 1.692(46) | 0.177(10) | −4.582(2) | 2.87(17) | 0.361(13) | 0.126(18) | 0.118(06) | – | −4.590(2) | 2.28(25) |
| HD 179949 | 21-10-08 | 0.188(21) | 1.89(14) | 0.100(13) | −4.380(3) | 3.72(24) | 0.209(23) | 0.049(28) | 0.080(13) | – | −4.388(3) | 3.59(25) |
| HD 206860 | 21-10-28 | 0.270(29) | 1.88(24) | 0.144(29) | −4.527(4) | 3.95(14) | 0.302(35) | 0.102(60) | 0.099(27) | – | −4.535(4) | 4.58(35) |
Notes. From left to right: HD number, date at the start of the observing night (yy-mm-dd), the average field strength, field strength of the magnetic component of the synthetic model, the filling factor, the Fe abundance in log(NFe/Ntotal) units, and macroturbulent velocity. For multi-component models, the columns give the average field strength and filling factor values for the 1, 2, and 3 kG magnetic components. Filling factors marked with ‘–’ did not significantly improve the fit, according to the BIC given by Eq. (3). Uncertainties derived from asymmetric posterior distributions (see Appendix B) are indicated with ±; in other cases, the error in the last significant digits is provided in brackets.
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