Table 2
Magnetic field measurements.
| Karmn | Name | Gl/GJ | SpT | Teff | log (g) | Ti I lines | FeH lines | P | ⟨B⟩ | ||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| number | K | dex | α(Ti) | υ sin i | ⟨B⟩ | α(Fe) | υ sin i | ⟨B⟩ | d | adopted | |||
| dex | km s−1 | kG | dex | km s−1 | kG | kG | |||||||
| J01033+623 | V388 Cas | 51 | M5.0 | 3200 | 5.1 | −6.98 ± 0.02 | 11.7 ± 0.2 | 5.0 | −4.42 ± 0.01 | 11.3 ± 0.1 | 4.7 | 1.06 | 4.8 ± 0.3 |
| J01352-072 | Barta 161 12 | M4.0 | 3400 | 4.9 | −6.99 ± 0.03 | 47.8 ± 0.7 | 5.8 | −4.73 ± 0.02 | 41.8 ± 0.5 | 4.6 | 0.7031 | 5.8 ± 1.0 | |
| J02088+494 | G 173-039 | 3136 | M3.5 | 3400 | 4.9 | −6.91 ± 0.02 | 22.9 ± 0.4 | 4.9 | −4.55 ± 0.01 | 21.3 ± 0.2 | 4.5 | 0.748 | 4.9 ± 1.0 |
| J03473-019 | G 080-021 | M3.0 | 3500 | 4.9 | −6.93 ± 0.01 | 5.7 ± 0.1 | 3.2 | −4.46 ± 0.01 | 6.4 ± 0.1 | 3.1 | 3.88 | 3.2 ± 0.1 | |
| J04472+206 | RX J0447.2+2038 | M5.0 | 3200 | 5.1 | −7.01 ± 0.03 | 46.5 ± 0.6 | 5.7 | −4.93 ± 0.03 | 37.5 ± 0.7 | 5.2 | 0.342 | 5.7 ± 1.0 | |
| J05365+113 | V2689 Ori | 208 | M0.0 | 3800 | 4.7 | −6.99 ± 0.01 | 0.4 ± 1.1 | 1.0 | −4.73 ± 0.01 | 2.9 ± 0.1 | 1.3 | 12.04 | 1.2 ± 0.3 |
| J06000+027 | G 099-049 | 3379 | M4.0 | 3400 | 4.9 | −6.82 ± 0.02 | 6.5 ± 0.2 | 2.0 | −4.28 ± 0.01 | 5.6 ± 0.1 | 3.0 | 1.81 | 2.5 ± 1.0 |
| J07446+035 | YZ CMi | 285 | M4.5 | 3300 | 5.0 | −6.93 ± 0.02 | 4.5 ± 0.1 | 4.7 | −4.41 ± 0.01 | 5.4 ± 0.1 | 4.4 | 2.78 | 4.6 ± 0.3 |
| J08298+267 | DX Cnc | 1111 | M6.5 | 2700 | 5.3 | −7.19 ± 0.03 | 12.4 ± 0.4 | 3.0 | −5.02 ± 0.01 | 10.4 ± 0.1 | 3.6 | 0.459 | 3.3 ± 0.6 |
| J09449-123 | G 161-071 | M5.0 | 3200 | 5.1 | −7.08 ± 0.03 | 30.1 ± 0.6 | 5.3 | −4.70 ± 0.01 | 27.3 ± 0.3 | 4.5 | 0.306 | 5.3 ± 1.0 | |
| J12156+526 | StKM 2-809 | M4.0 | 3400 | 4.9 | −6.90 ± 0.02 | 37.6 ± 0.4 | 4.5 | −4.83 ± 0.01 | 28.0 ± 0.3 | 4.2 | <0.4 | 4.5 ± 1.0 | |
| J12189+111 | GL Vir | 1156 | M5.0 | 3200 | 5.1 | −6.89 ± 0.02 | 15.4 ± 0.3 | 3.3 | −4.22 ± 0.01 | 15.3 ± 0.1 | 4.0 | 0.491 | 3.6 ± 0.7 |
| J14173+454 | RX J1417.3+4525 | M5.0 | 3200 | 5.1 | −7.05 ± 0.03 | 13.8 ± 0.4 | 5.1 | −4.56 ± 0.01 | 15.3 ± 0.1 | 5.3 | <0.7 | 5.2 ± 0.2 | |
| J15218+209 | OT Ser | 9520 | M1.5 | 3600 | 4.8 | −6.95 ± 0.02 | 3.9 ± 0.2 | 3.3 | −4.49 ± 0.01 | 5.0 ± 0.1 | 3.1 | 3.372 | 3.2 ± 0.2 |
| J15499+796 | LP 022-420 | M5.0 | 3200 | 5.1 | −6.86 ± 0.02 | 27.7 ± 0.5 | 3.4 | −4.73 ± 0.02 | 22.9 ± 0.5 | 4.2 | <0.3 | 3.4 ± 1.0 | |
| J16313+408 | G 180-060 | 3959 | M5.0 | 3200 | 5.1 | −6.92 ± 0.02 | 7.5 ± 0.2 | 4.1 | −4.31 ± 0.01 | 8.1 ± 0.1 | 4.0 | 0.51 | 4.1 ± 0.1 |
| J16555-083 | vB 8 | 644 C | M7.0 | 2600 | 5.3 | −7.21 ± 0.04 | 5.8 ± 0.5 | 2.6 | −5.07 ± 0.01 | 7.0 ± 0.1 | 3.0 | <1.0 | 2.8 ± 0.4 |
| J16570-043 | LP 686-027 | 1207 | M3.5 | 3400 | 4.9 | −6.93 ± 0.02 | 10.5 ± 0.2 | 3.1 | −4.31 ± 0.01 | 10.7 ± 0.1 | 3.5 | 1.21 | 3.3 ± 0.4 |
| J17338+169 | 1RXS J173353.5+165515 | M5.5 | 3000 | 5.2 | −7.15 ± 0.04 | 36.6 ± 1.0 | 6.9 | −5.18 ± 0.03 | 29.1 ± 0.6 | 4.5 | 0.27 | 6.9 ± 1.0 | |
| J18022+642 | LP 071-082 | M5.0 | 3200 | 5.1 | −6.90 ± 0.02 | 10.6 ± 0.2 | 3.8 | −4.37 ± 0.01 | 10.9 ± 0.1 | 4.7 | 0.28 | 4.3 ± 0.9 | |
| J18189+661 | LP 071-165 | 4053 | M4.5 | 3300 | 5.0 | −6.59 ± 0.04 | 15.6 ± 0.3 | 1.8 | −4.30 ± 0.02 | 14.4 ± 0.2 | 3.4 | <0.7 | 2.6 ± 1.6 |
| J18498-238 | V1216 Sgr | 729 | M3.5 | 3400 | 4.9 | −6.73 ± 0.03 | 5.4 ± 0.2 | 1.8 | −4.27 ± 0.01 | 4.1 ± 0.1 | 2.6 | 2.87 | 2.2 ± 0.8 |
| J19169+051S | V1298 Aql (vB 10) | 752 B | M8.0 | 2500 | 5.3 | −7.55 ± 0.10 | 5.1 ± 0.5 | 2.2 | −5.11 ± 0.01 | 5.4 ± 0.1 | 2.4 | 0.8 | 2.3 ± 0.2 |
| J19511+464 | G 208-042 | 1243 | M4.0 | 3400 | 4.9 | −6.87 ± 0.02 | 23.3 ± 0.3 | 3.2 | −4.53 ± 0.01 | 21.1 ± 0.2 | 3.3 | 0.594 | 3.2 ± 1.0 |
| J20093-012 | SCR J2009-0113 | M5.0 | 3200 | 5.1 | −6.95 ± 0.03 | 5.1 ± 0.2 | 3.1 | −4.31 ± 0.01 | 5.9 ± 0.1 | 3.4 | <1.8 | 3.2 ± 0.3 | |
| J22012+283 | V374 Peg | 4247 | M4.0 | 3400 | 4.9 | −6.84 ± 0.01 | 36.3 ± 0.3 | 4.4 | −4.53 ± 0.01 | 31.5 ± 0.3 | 4.4 | 0.45 | 4.4 ± 1.0 |
| J22468+443 | EV Lac | 873 | M3.5 | 3400 | 4.9 | −6.90 ± 0.02 | 4.5 ± 0.2 | 4.2 | −4.44 ± 0.01 | 5.1 ± 0.1 | 4.0 | 4.379 | 4.1 ± 0.2 |
| J22518+317 | GT Peg | 875.1 | M3.0 | 3500 | 4.9 | −6.90 ± 0.02 | 14.3 ± 0.2 | 3.1 | −4.49 ± 0.01 | 13.2 ± 0.1 | 3.7 | 1.64 | 3.4 ± 0.6 |
| J23548+385 | RX J2354.8+3831 | M4.0 | 3400 | 5.0 | −6.92 ± 0.02 | 4.3 ± 0.2 | 4.8 | −4.34 ± 0.01 | 4.7 ± 0.1 | 4.4 | 4.76 | 4.6 ± 0.4 | |
Notes. Forstars without measured rotational periods we esimate them from υ sin i values and stellar radii estimated from spectral types. The last column lists adopted values of the surface magnetic fields. For stars with υ sin i < 20 km s−1 they were taken as a mean between meaurements from Ti and FeH lines, respectively, and the error bars were assumed to be the corresponding difference between these measurements. For stars with υ sin i > 20 km s−1 we adopt measurements from the Ti lines and similar to Shulyak et al. (2017) assume conservative uncertainties of 1 kG. The rotational velocities derived from Ti lines should be preferred over those derived from FeH lines.
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