Table 1
Identification of the cool stars chosen for this study, their average magnetic field, <B>, and their RVs with respect to the heliocentric rest frame.
| Star | Instrument | <B> tesla | RV kms−1 |
|---|---|---|---|
| GJ 411 | SPIRou | <0.02(a) | −85.02 (2) |
| GJ 1002 | ESPaDOnS | 0.08(b) | −40.12(2) |
| GJ 49 | Narval | 0.08((2)(c) | −6.30 (2) |
| GJ 406 (CN Leo) | ESPaDOnS | 0.345(20)(d) | +19.28 (2) |
| GJ 388 (AD Leo) | SPIRou | 0.303(6)(d) | +12.29 (2) |
| GJ 873 (EV Lac) | SPIRou | 0.453(7) (d) | +0.35 (3) |
| GJ 412B (WX UMa) | ESPaDOnS | 0.73(3)(c) | +69.16(2) |
Notes. Uncertainties are indicated in parentheses, in units of last digit. <B> values are taken from publications by (a)Reiners et al. (2022), (b)Kochukhov (2021), (c)Shulyak et al. (2017), and from (d)Cristofari et al. (2023). RV values come from supplementary data associated with work by Lafarga et al. (2020).
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