Table A.1
Magnesium and silicon abundances and main parameters of investigated starsa (sorted by SpT).
| Karmn | Name | SpT | S/N | v sin i | Teff | log ɡ | [Fe/H] | [Mg/H] | [Si/H] | Pop. | Nplanets |
|---|---|---|---|---|---|---|---|---|---|---|---|
| [km s−1] | [K] | [dex] | [dex] | [dex] | [dex] | ||||||
| J04167−120 | LP 714-47 | K7.0 V | 258 | ≤ 2.0 | 3961 ± 13 | 5.01 ± 0.09 | 0.15 ± 0.04 | −0.02 ± 0.14 | 0.22 ± 0.03 | D | 1 |
| J11110+304E | HD 97101A | K7.0 V | 422 | ≤ 2.0 | 4211 ± 13 | 4.98 ± 0.07 | 0.04 ± 0.03 | 0.03 ± 0.06 | 0.08 ± 0.02 | D | 2 |
| J18198−019 | HD 168442 | K7.0 V | 1447 | ≤ 3.0 | 4155 ± 14 | 5.01 ± 0.06 | −0.14 ± 0.04 | −0.18 ± 0.04 | −0.14 ± 0.02 | YD | 0 |
| … | … | … | … | … | … | … | … | … | … | … | … |
Notes. aKarmn identifier, spectral types (SpT), signal-to-noise ratio (S/N), projected rotational velocities (v sin i), effective temperatures (Teff), surface gravities (log ɡ), metallicity ([Fe/H]), magnesium and silicon abundances ([Mg/H], [Si/H]), galactic population kinematic membership, and planet occurrence (Nplanets) for the stars analysed in this work. The full version of this table is available at the CDS.
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