Table A.1
Measured vanadium abundances for the sample (excerpt) a
| Karmn | SpT | v sin i b | Schw19 Stellar Parameters | Marfil+ Stellar Parameters | Kinematic | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (km/s) | Teff (K) | logg | [Fe/H] | [V/H] | δ[V/H] b | Teff (K) | logg | [Fe/H] | [V/H] | δ[V/H] c | Membership | ||
| J00051+457 | M1.0V | 2.0 | 3675 | 4.84 | -0.16 | -0.01 | 0.03 | 3759 | 4.72 | -0.02 | 0.02 | 0.04 | YD |
| J00183+440 | M1.0V | 2.0 | 3615 | 4.91 | -0.25 | -0.25 | 0.07 | 3613 | 4.86 | -0.47 | -0.31 | 0.06 | D |
| J00389+306 | M2.5V | 2.0 | 3537 | 4.89 | -0.05 | -0.04 | 0.06 | 3559 | 4.81 | -0.18 | -0.10 | 0.06 | D |
| J01013+613 | M2.0V | 2.0 | 3529 | 4.94 | -0.16 | -0.15 | 0.06 | 3562 | 4.81 | -0.24 | -0.20 | 0.06 | D |
| J01025+716 | M3.0V | 2.0 | 3488 | 4.91 | 0.02 | 0.06 | 0.07 | 3523 | 4.76 | -0.06 | 0.00 | 0.07 | D |
| J01026+623 | M1.5V | 2.0 | 3805 | 4.69 | 0.13 | 0.13 | 0.04 | 3806 | 4.71 | 0.02 | 0.12 | 0.04 | YD |
| J01433+043 | M2.0V | 2.0 | 3532 | 4.91 | -0.09 | -0.09 | 0.06 | 3550 | 4.82 | -0.20 | -0.14 | 0.06 | D |
| J01518+644 | M2.5V | 2.0 | 3555 | 4.90 | -0.08 | 0.06 | 0.03 | 3648 | 4.55 | -0.02 | -0.05 | 0.04 | YD |
| J02015+637 | M3.0V | 2.0 | 3489 | 4.93 | -0.05 | 0.09 | 0.05 | 3563 | 4.81 | -0.13 | 0.05 | 0.04 | D |
| J02123+035 | M1.5V | 2.0 | 3663 | 4.81 | -0.05 | -0.24 | 0.07 | 3595 | 4.87 | -0.49 | -0.35 | 0.04 | TD |
Notes. (a) : this table is available in its entirety in machine-readable form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/. (b) : the v sin i’s given here are the rotational broadening parameters used for each star in the spectral fits. It is set to 2.0 km/s when the measurement (from Reiners et al. 2018) only gives an upper limit of 2.0 km/s, i.e., the true v sin i ≤ 2 km/s. (c) : [V/H] error is given as the sample standard deviation of the fitted abundances over all line regions used for that particular star.
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