Table 1
Properties of the sample stars.
| Karmn | Name | No. | No. | Sp. | Ref. | Popc | v sin id | Pest | Plit | Refe |
|---|---|---|---|---|---|---|---|---|---|---|
| spec.a | shortb | type | (SpT) | (km s−1) | (d) | (d) | (Plit) | |||
| J00183+440 | GX And | 190 | 112 | M1.0 | AF15a | D | <2.0 | ... | ... | ... |
| J01026+623 | BD+61 195 | 68 | 2 | M1.5 | AF15a | YD | <2.0 | ... | 19.9 ± 0.4, 18.4 ± 0.7 | DA18, SM17 |
| J04290+219 | BD+21 652 | 161 | 23 | M0.5 | Gra06 | D | 3.9 ± 1.4 | 8.3 | 25.4 ± 0.3 | DA18 |
| J04376+528 | BD+52 857 | 78 | 11 | M0.0 | Gra03 | D | 3.4 ± 0.6 | 8.5 | ... | ... |
| J05314−036 | HD 36395 | 87 | 7 | M1.5 | AF15a | D | <2.0 | ... | 33.8 ± 0.6, 33.61 | DA18, KS07 |
| J05365+113 | V2689 Ori | 50 | 12 | M0.0 | Lep13 | YD | 3.8 ± 0.4 | 7.5 | 12.3 ± 0.1, 12.02 | DA18, Kir12 |
| J09144+526 | HD 79211 | 115 | 9 | M0.0 | AF15a | YD | 2.3 ± 0.4 | 12.7 | ... | ... |
| J09561+627 | BD+63 869 | 57 | 7 | M0.0 | PMSU | YD | <2.0 | ... | ... | ... |
| J10122−037 | AN Sex | 61 | 6 | M1.5 | PMSU | YD | <2.0 | ... | 21.6 ± 0.2,21.56 | DA18,Kir12 |
| J11033+359 | Lalande 21185 | 147 | 21 | M1.5 | AF15a | TD | <2.0 | ... | 48.0 | No84 |
| J11054+435 | BD+44 2051A | 100 | 7 | M1.0 | AF15a | TD-D | <2.0 | ... | ... | ... |
| J13299+102 | BD+11 2576 | 64 | 7 | M0.5 | PMSU | D | <2.0 | ... | 28.0 ± 2.9 | SM15 |
| J13457+148 | HD 119850 | 223 | 58 | M1.5 | PMSU | D | <2.0 | ... | 52.3 ± 1.7 | SM15 |
| J16167+672S | HD 147379 | 124 | 4 | M0.0 | AF15a | YD | 2.7 ± 0.2 | 11.6 | ... | ... |
| J20533+621 | HD 199305 | 133 | 2 | M1.0 | Lep13 | D | <2.0 | ... | ... | ... |
| J22565+165 | HD 216899 | 203 | 14 | M1.5 | PMSU | TD | <2.0 | ... | 39.5 ± 0.2, 37.5 ± 0.1 | DA18, SM15 |
Notes. (a) Total number of spectra used in the analysis. (b) Number of spectra obtained at short sub-day cadence. (c) All kinematic population designations are measured by Cortés-Contreras (2016): abbreviations: YD: young disc, D: disc, TD: thick disc, TD-D: thin-to-thick transition disc; there are no halo stars in our sample. (d) All rotational velocities are measured by Reiners et al. (2018) and are included in the catalogue of Jeffers et al. (2018). (e) No84 and SM15 determined spectroscopically, all other periods determined photometrically.
References. AF15a: Alonso-Floriano et al. (2015); DA18: Díez Alonso et al. (2019); Gra03: Gray et al. (2003); Gra06: Gray et al. (2006); Kir12: Kirkpatrick et al. (2012); KS07: Kiraga & Stepien (2007); Lep13: Lépine et al. (2013); No84: Noyes et al. (1984); PMSU: Reid et al. (1995); SM15: Suárez Mascareño et al. (2015); SM17: Suárez Mascareño et al. (2018).
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