Table D.1.
Stellar properties and jitter of the 239 targets in the CARMENES VIS jitter sample.a
| Karmn | Name | R | Prot | Ref | veq | v sin i | Ref | log Ro | ⟨B⟩ | NRV | σjitter | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [R⊙] | [d] | [km s−1] | [km s−1] | [G] | [m s−1] | |||||||
| J00051+457 | BD+44 4548 | 0.4888 ± 0.0044 | ≤ 2.0 | Rei18 | 51 | 2.42 ± 0.33 | ||||||
| J00158+135 | GJ 12 | 0.2688 ± 0.0083 | 17 | 2.01 ± 0.54 | ||||||||
| J00162+198E | LP 404-062 | 0.2796 ± 0.0051 | 105 ± 10 | DA19 | 0.135 ± 0.013 | ≤ 2.0 | Rei18 | 0.10 | 22 | 2.26 ± 0.43 | ||
| J00286−066 | GJ 1012 | 0.3490 ± 0.0059 | ≤ 2.0 | Rei18 | 50 | 2.01 ± 0.27 | ||||||
| J00389+306 | Wolf 1056 | 0.4143 ± 0.0041 | 50.2 ± 2.7 | DA19 | 0.418 ± 0.023 | ≤ 2.0 | Rei18 | −0.04 | 57 | 1.71 ± 0.21 | ||
| J00570+450 | G 172-030 | 0.3358 ± 0.0044 | ≤ 2.0 | Rei18 | 23 | 1.95 ± 0.45 | ||||||
| J01013+613 | GJ 47 | 0.3706 ± 0.0040 | 34.7 ± 1.4 | SM18 | 0.540 ± 0.022 | ≤ 2.0 | Rei18 | −0.18 | 10 | 1.95 ± 0.80 | ||
| J01019+541 | G 218-020 | 0.1560 ± 0.0014 | 0.280 ± 0.005 | DA19 | 28.18 ± 0.56 | 30.6 ± 3.1 | Rei18 | −2.76 | 20 | 34 ± 18 | ||
| J01025+716 | Ross 318 | 0.4636 ± 0.0070 | 50.5 ± 2.7 | Sha24 | 0.464 ± 0.026 | ≤ 2.0 | Rei18 | −0.09 | 114 | 1.99 ± 0.19 | ||
| J01033+623 | V388 Cas | 0.2433 ± 0.0078 | 1.020 ± 0.005 | Sha24 | 12.07 ± 0.39 | 10.5 ± 1.5 | Rei18 | −2.04 | 23 | 187 ± 24 | ||
| J01048−181 | GJ 1028 | 0.1529 ± 0.0040 | 143 ± 18 | New18 | 0.0540 ± 0.0068 | ≤ 2.0 | Rei18 | −0.01 | 109 | 3.60 ± 0.33 | ||
| J01078+128 | G 2-21 | 0.506 ± 0.015 | 47 | 4.56 ± 0.58 | ||||||||
| J01339−176 | LP 768-113 | 0.2767 ± 0.0056 | 7.750 ± 0.095 | Sha24 | 1.806 ± 0.043 | ≤ 2.0 | Rei18 | −1.02 | 26 | 9.6 ± 1.9 | ||
| J01352−072 | Barta 161 12 | 0.718 ± 0.016 | 0.70 ± 0.05 | Sha24 | 51.9 ± 3.9 | 59.8 ± 6.9 | Rei18 | −2.13 | 11 | 270 ± 80 | ||
| J01433+043 | GJ 70 | 0.3991 ± 0.0047 | 14.65 ± 0.30 | Sha24 | 1.378 ± 0.032 | ≤ 2.0 | Rei18 | −0.53 | 37 | 1.70 ± 0.25 | ||
| J01550+379 | LSR J0155+3758 | 0.2071 ± 0.0067 | 19 | 5.8 ± 2.8 | ||||||||
| J02015+637 | G 244-047 | 0.4215 ± 0.0056 | ≤ 2.0 | Rei18 | 49 | 2.41 ± 0.32 | ||||||
| J02022+103 | LP 469-067 | 0.1487 ± 0.0053 | 4.5 | Jen09 | 12 | (1.5 ± 2.4) i b | ||||||
| J02070+496 | G 173-037 | 0.3284 ± 0.0043 | 7.200 ± 0.083 | DA19 | 2.307 ± 0.040 | ≤ 2.0 | Rei18 | −0.95 | 53 | 3.67 ± 0.44 | ||
| J02088+494 | G 173-039 | 0.417 ± 0.031 | 0.750 ± 0.005 | Sha24 | 28.1 ± 2.1 | 24.1 ± 2.4 | Rei18 | −1.98 | 17 | 75 ± 14 | ||
| J02123+035 | BD+02 348 | 0.4658 ± 0.0038 | ≤ 2.0 | Rei18 | 64 | 1.30 ± 0.30 | ||||||
| J02336+249 | GJ 102 | 0.2272 ± 0.0033 | 3.00 ± 0.05 | Sha24 | 3.832 ± 0.085 | 3.0 ± 1.5 | Rei18 | −1.50 | 30 | 5.8 ± 1.0 | ||
| J02358+202 | BD+19 381 | 0.4836 ± 0.0052 | ≤ 2.0 | Rei18 | 43 | 1.55 ± 0.37 | ||||||
| J02362+068 | BX Cet | 0.2688 ± 0.0073 | ≤ 2.0 | Rei18 | 50 | 2.38 ± 0.31 | ||||||
| J02442+255 | VX Ari | 0.3491 ± 0.0043 | 38.7 ± 1.7 | DA19 | 0.456 ± 0.021 | ≤ 2.0 | Rei18 | −0.21 | 51 | 1.53 ± 0.24 | ||
| J02465+164 | LP 411-006 | 0.127 ± 0.013 | 6.20 ± 0.80 | Jen09 | 17 | 53.1 ± 8.7 | ||||||
| J02519+224 | RBS 365 | 0.611 ± 0.014 | 0.860 ± 0.005 | DA19 | 35.94 ± 0.87 | 27.2 ± 2.7 | Rei18 | −2.01 | 14 | 112 ± 11 | ||
| J02565+554W | Ross 364 | 0.6096 ± 0.0035 | 51.2 ± 2.8 | SM18 | 0.602 ± 0.033 | ≤ 2.0 | Rei18 | 0.09 | 0 | 10 | 1.59 ± 0.89 | |
| J03090+100 | GJ 1055 | 0.1780 ± 0.0060 | 4.70 ± 0.70 | Jen09 | 10 | 3.5 ± 2.2 | ||||||
| J03142+286 | LP 299-036 | 0.1295 ± 0.0045 | 12 | 176 ± 45 | ||||||||
| J03181+382 | HD 275122 | 0.5690 ± 0.0047 | 77.2 ± 5.8 | DA19 | 0.373 ± 0.028 | ≤ 2.0 | Rei22 | 0.22 | ≤180 | 0 | 56 | 1.52 ± 0.22 |
| J03213+799 | GJ 133 | 0.4048 ± 0.0033 | ≤ 2.0 | Rei22 | 320 ± 110 | 0 | 34 | 2.19 ± 0.33 | ||||
| J03217−066 | G 77-046 | 0.4510 ± 0.0044 | 21.00 ± 0.57 | Sha24 | 1.087 ± 0.031 | ≤ 2.0 | Rei22 | −0.40 | 930 ± 110 | 1.7 | 18 | 3.51 ± 0.83 |
| J03230+420 | GJ 1059 | 0.1673 ± 0.0056 | 16 | 7.9 ± 3.2 |
Notes. (a)Listed are: CARMENES star identifier, additional identifier, stellar radius, stellar rotation period, equatorial rotation velocity, projected equatorial rotation velocity, average magnetic field strength, magnetic field component distribution index, number of RV measurements, and RV jitter. The table contains the first 35 entries. A list with all 239 stars is available at the CDS. (b)The letter i stands for an imaginary jitter value, i.e. a negative jitter variance σjitter2. A negative jitter variance results from overestimated internal RV uncertainties. DA19: Díez Alonso et al. (2019), Rei18: Reiners et al. (2018), Jen09: Jenkins et al. (2009).
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