Table E.1.
LSD Stokes I fitting results, veiling values, and longitudinal magnetic field detection and measurements.
| ID | BJD | Depth I | v sin i | vrad | FAP | B | rH | rK | Bℓ | |
|---|---|---|---|---|---|---|---|---|---|---|
| -2 400 000 | ×10−4 | (km s−1) | (km s−1) | detection | (G) | |||||
| V806 Tau* | 59900.12063 | 210 ± 1 | 27.4 ± 0.5 | 12.7 ± 0.3 | 7.1 × 10−6 | DD | 0.7 ± 0.1 | 2 ± 0.1 | 80 | 18 |
| 59901.12629 | 160 ± 1 | 25.7 ± 0.6 | 10.9 ± 0.4 | 5.5 × 10−6 | DD | 1.2 ± 0.1 | 3.3 ± 0.2 | 77 | 21 | |
| 59915.02084 | 140 ± 1 | 25.6 ± 0.8 | 12.7 ± 0.5 | 1.9 × 10−3 | ND | 1.6 ± 0.1 | – | 100 | 25 | |
| MHO 3* | 59900.09753 | 100 ± 1 | 56.1 ± 0.8 | 13.1 ± 0.6 | 1.2 × 10−1 | ND | 1 ± 0.1 | 2 ± 0.1 | -92 | 50 |
| 59914.97152 | 100 ± 1 | 53.9 ± 0.7 | 13.5 ± 0.4 | 1.9 × 10−1 | ND | 0.5 ± 0.1 | 1.8 ± 0.1 | -142 | 42 | |
| 59918.01608 | 60 ± 1 | 50.5 ± 1.2 | 12.9 ± 0.9 | 9.1 × 10−1 | ND | – | – | -85 | 67 | |
| 59945.96152 | 100 ± 1 | 55.4 ± 0.7 | 14.2 ± 0.4 | 7.9 × 10−6 | DD | 0.4 ± 0.1 | 1.3 ± 0.1 | -144 | 45 | |
| MHO 2* | 59918.04028 | 100 ± 1 | 30.4 ± 1.1 | 13.5 ± 0.7 | 7.7 × 10−1 | ND | 0.3 ± 0.1 | 0.6 ± 0.1 | -69 | 29 |
| 59946.87428 | 200 ± 1 | 30.5 ± 0.9 | 13.9 ± 0.5 | 2.5 × 10−10 | DD | 0.3 ± 0.1 | 0.6 ± 0.1 | -97 | 17 | |
| 59947.85486 | 160 ± 1 | 31.5 ± 1.0 | 12.7 ± 0.6 | 2.8 × 10−5 | MD | 0.5 ± 0.1 | 0.6 ± 0.1 | 26 | 19 | |
| IRAS 04292+2422 W | 59946.90951 | 900 ± 20 | 7.9 ± 0.2 | 28.1 ± 0.3 | 2.2 × 10−1 | ND | 0.1 ± 0.1 | 0.2 ± 0.1 | -2.4 | 2.8 |
| 59947.89613 | 1010 ± 20 | 7.8 ± 0.3 | 28.1 ± 0.3 | 9.6 × 10−1 | ND | 0.2 ± 0.1 | 0.2 ± 0.1 | -1.4 | 2.7 | |
| 59952.97509 | 900 ± 30 | 7.9 ± 0.2 | 28.1 ± 0.3 | 3.5 × 10−1 | ND | 0.2 ± 0.1 | 0.2 ± 0.1 | -3.1 | 3.1 | |
| IRAS 04113+2758 N* | 59948.93997 | 160 ± 10 | 17.9 ± 0.8 | 12.7 ± 0.4 | 1.2 × 10−1 | ND | 1.1 ± 0.1 | 2.4 ± 0.1 | 11 | 10 |
| 59953.85844 | 140 ± 10 | 17.2 ± 1.0 | 12.4 ± 0.5 | 1.6 × 10−2 | ND | 2 ± 0.1 | 3.1 ± 0.1 | -4 | 12 | |
| 59954.83884 | 140 ± 10 | 18.3 ± 1.2 | 12.4 ± 0.6 | 4.7 × 10−1 | ND | 1.6 ± 0.1 | 2.6 ± 0.1 | -7 | 12 | |
| IRAS 04369+2539* | 59903.13177 | 80 ± 1 | 40.6 ± 0.5 | 13.8 ± 0.3 | 6.4 × 10−1 | ND | 1.6 ± 0.1 | 4.7 ± 0.6 | 9 | 52 |
| 59905.05519 | 90 ± 1 | 40.7 ± 0.6 | 14.5 ± 0.4 | 8.1 × 10−1 | ND | 1.4 ± 0.1 | 5.2 ± 0.8 | -10 | 62 | |
| 59915.06549 | 90 ± 1 | 41.9 ± 0.7 | 12.7 ± 0.5 | 4.9 × 10−1 | ND | 1.5 ± 0.1 | 2.3 ± 0.2 | 42 | 44 | |
| HL Tau | 58384.11335 | 60 ± 1 | 52.5 ± 2.5 | 11.9 ± 2.5 | 9.1 × 10−1 | ND | 1.2 ± 0.1 | 4.5 ± 0.2 | 31 | 71 |
| 58385.09837 | 70 ± 1 | 51.9 ± 1.7 | 12.8 ± 1.2 | 1.5 × 10−1 | ND | 1.1 ± 0.1 | 6.4 ± 0.3 | -92 | 69 | |
| 58387.08102 | 70 ± 1 | 49.4 ± 1.6 | 13.4 ± 1.1 | 1.5 × 10−1 | ND | 1.4 ± 0.1 | 8.6 ± 0.4 | -125 | 79 | |
| 58499.80432 | 60 ± 1 | 57.7 ± 3.7 | 12.9 ± 2.9 | 4.4 × 10−1 | ND | 1.5 ± 0.1 | 8.8 ± 0.4 | -25 | 78 | |
| 58500.79189 | 60 ± 1 | 54.2 ± 2.0 | 13.7 ± 1.5 | 7.5 × 10−1 | ND | 1.5 ± 0.2 | 12 ± 0.6 | -58 | 69 | |
| 59111.08910 | 60 ± 1 | 51.1 ± 1.6 | 12.1 ± 1.2 | 1.2 × 10−1 | ND | 1.7 ± 0.1 | 6.9 ± 0.3 | -13 | 60 | |
| 59115.05352 | 60 ± 1 | 52.9 ± 2.1 | 14.8 ± 1.5 | 5.4 × 10−1 | ND | 1.8 ± 0.1 | 9.7 ± 0.5 | 54 | 58 | |
| IRAS 16191-1936* | 60388.10393 | 80 ± 1 | 59.5 ± 0.7 | −5.2 ± 0.4 | 5.3 × 10−1 | ND | 0.9 ± 0.1 | 2.9 ± 0.2 | 38 | 56 |
| 60433.02290 | 100 ± 1 | 53.9 ± 0.5 | −7.7 ± 0.9 | 4.8 × 10−13 | DD | 0.4 ± 0.1 | 1.7 ± 0.1 | 204 | 46 | |
| 60487.76569 | 80 ± 1 | 53.0 ± 0.3 | −9.1 ± 0.9 | 9.1 × 10−8 | DD | 0.6 ± 0.1 | 2.3 ± 0.1 | 151 | 44 | |
| L1689 SNO2* | 58618.10070 | 150 ± 1 | 24.1 ± 0.7 | −7.6 ± 0.4 | 1.4 × 10−1 | ND | 0.6 ± 0.1 | 2.1 ± 0.1 | 56 | 44 |
| 60509.89855 | 170 ± 1 | 23.3 ± 0.5 | −8.1 ± 0.3 | 4.1 × 10−13 | DD | 0.6 ± 0.1 | 1.9 ± 0.1 | -130 | 21 | |
| 60517.85402 | 160 ± 1 | 23.4 ± 0.5 | −7.0 ± 0.3 | < 10−15 | DD | 0.6 ± 0.1 | 2.2 ± 0.1 | -180 | 24 | |
| IRAS 03247+3001* | 59946.84774 | 90 ± 1 | 67.2 ± 1.2 | 12.0 ± 0.8 | 4.1 × 10−1 | ND | 0.7 ± 0.1 | 2.5 ± 0.1 | -260 | 133 |
| 59947.81412 | 100 ± 1 | 67.4 ± 1.9 | 11.8 ± 1.4 | 9.9 × 10−1 | ND | 1 ± 0.2 | 3.8 ± 0.2 | 22 | 123 | |
| 59948.84853 | 120 ± 1 | 68.2 ± 2.7 | −6.4 ± 1.4 | 9.0 × 10−1 | ND | 1.4 ± 0.3 | 3 ± 0.2 | 142 | 99 | |
| 59953.90247 | 100 ± 1 | 63.5 ± 1.3 | −0.8 ± 1.3 | 5.4 × 10−1 | ND | 0.7 ± 0.1 | 2.6 ± 0.2 | -12 | 72 | |
| 59954.88269 | 110 ± 1 | 66.9 ± 1.5 | −2.5 ± 1.3 | 7.4 × 10−1 | ND | 0.9 ± 0.1 | 3.1 ± 0.2 | 82 | 83 | |
| 59955.89845 | 90 ± 1 | 76.9 ± 4.1 | 17.3 ± 3.0 | 8.3 × 10−1 | ND | 0.9 ± 0.1 | 2.9 ± 0.2 | -42 | 83 | |
| V512 Per | 59090.03171 | 140 ± 10 | 23.8 ± 2.7 | 13.9 ± 1.1 | 9.6 × 10−1 | ND | 0.9 ± 0.1 | 0.8 ± 0.2 | 55 | 37 |
| 59948.87769 | 140 ± 10 | 22.4 ± 2.9 | 14.6 ± 1.8 | 9.6 × 10−1 | ND | 2.1 ± 0.1 | 2.8 ± 0.3 | 28 | 55 | |
| VV CrA SW | 60402.15170 | 90 ± 1 | 36.8 ± 2.2 | 4.6 ± 1.2 | 3.6 × 10−2 | ND | – | – | 141 | 56 |
| 60425.12513 | 90 ± 1 | 31.5 ± 1.3 | 2.3 ± 0.6 | 9.6 × 10−2 | ND | – | – | -107 | 74 | |
| 60484.02208 | 40 ± 1 | 43.6 ± 3.2 | 4.1 ± 1.5 | 3.1 × 10−1 | ND | – | – | 199 | 159 | |
| 60484.96903 | 40 ± 1 | 31.8 ± 1.7 | 7.2 ± 1.6 | 3.1 × 10−1 | ND | – | – | -18 | 157 | |
| VV CrA NE* | 60426.07900 | 80 ± 1 | 13.8 ± 2.5 | −0.4 ± 0.5 | 6.3 × 10−1 | ND | – | – | 17 | 72 |
| 60484.99885 | 110 ± 1 | 15.2 ± 1.4 | −3.1 ± 0.2 | 4.5 × 10−1 | ND | 4.6 ± 0.3 | 8.8 ± 0.4 | 87 | 49 | |
| 60485.98446 | 110 ± 1 | 16.6 ± 2.3 | −6.2 ± 0.6 | 7.2 × 10−1 | ND | 7.9 ± 0.4 | 11.6 ± 0.5 | 169 | 74 | |
| SVS 20 S* | 60430.99864 | 30 ± 1 | 61.6 ± 2.2 | −10.6 ± 1.3 | 7.5 × 10−1 | ND | 2 ± 0.2 | 10.9 ± 0.5 | 57 | 104 |
| 60487.99729 | 30 ± 1 | 59.7 ± 1.0 | −9.8 ± 0.8 | 1.2 × 10−2 | ND | 1.8 ± 0.1 | 18 ± 0.9 | 120 | 68 | |
| 60488.91144 | 30 ± 1 | 58.6 ± 1.1 | −10.9 ± 0.7 | 2.3 × 10−2 | ND | 2.2 ± 0.2 | 9.2 ± 0.6 | -49 | 61 | |
| 60489.91152 | 30 ± 1 | 59.5 ± 1.2 | −9.5 ± 0.8 | 7.5 × 10−1 | ND | 1.8 ± 0.2 | 15.2 ± 0.8 | 170 | 82 | |
Notes. From left to right the columns show the depth, the projected rotational velocity (v sin i), the radial velocity (vrad), computed with a physical stellar model (see Appendix A), the false alarm probability, the magnetic detection status (defined as DD for definite detection, MD for marginal detection, and ND for no detection), the veiling values in H and K band, the longitudinal magnetic field values, and their corresponding uncertainties. The stars indicated in bold are detected magnetic stars (at least one DD in the different observations). Sources with an * symbol are flat-spectrum targets.
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