Table A.1.
Identification, common name, Gliese number, spectral type (SpT), stellar population (Pop.), rotational velocity, rotation period, normalised Hα luminosity, 
, absolute Hα variation, andthe three best-fit frequencies for Hα.
| No. | ID | Name | Gl/GJ | SpT | Ref. | Pop. | v sin i | Prot | Ref. | log (LH α ∕Lbol) |  |
abs. Hα variation | Hα best-fit freq. | 2nd | 3rd |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (km s−1) | (d) | (Å) | (Å) | (d−1) | (d−1) | (d−1) | |||||||||
| 1 | J00051+457 | GJ 2 | 2 | M1.0 V | PMSU | YD | … | 15.5 ± 0.7 | DA19 | … | –0.064 ± 0.008 | 0.048 ± 0.007 | 0.0556 ± 0.0002 | 0.1283 ± 0.0003 | 0.7301 ± 0.0003 |
| 2 | J00067–075 | GJ 1002 | 1002 | M5.5 V | PMSU | D | … | … | … | … | 0 | 0.13 ± 0.03 | 0.0459 ± 0.0003 | 0.9866 ± 0.0003 | 0.8991 ± 0.0003 |
| 3 | J00162+198E | LP 404–062 | 1006B | M4.0 V | AF15 | TD-D | … | 105 ± 44 | DA19 | … | 0.052 ± 0.011 | 0.14 ± 0.08 | 0.2681 ± 0.0007 | 0.5012 ± 0.0004 | 0.1764 ± 0.0014 |
| 4 | J00183+440 | GX And | 15A | M1.0 V | AF15 | D | … | … | … | … | –0.073 ± 0.007 | 0.031 ± 0.004 | 0.0070 ± 0.0002 | 0.2717 ± 0.0003 | 0.5607 ± 0.0004 |
| 5 | J00184+440 | GQ And | 15B | M3.5 V | PMSU | YD | … | … | … | … | –0.033 ± 0.012 | 0.048 ± 0.005 | 0.0024 ± 0.0002 | 0.3850 ± 0.0002 | 0.9727 ± 0.0003 |
| 6 | J00286–066 | GJ 1012 | 1012 | M4.0 V | PMSU | D | … | … | … | … | 0.122 ± 0.016 | 0.06 ± 0.03 | 0.2750 ± 0.0003 | 0.6070 ± 0.0004 | 0.2637 ± 0.0006 |
| 7 | J00389+306 | Wolf 1056 | 26 | M2.5 V | AF15 | D | … | 50.2 ± 1.3 | DA19 | … | 0.036 ± 0.007 | 0.044 ± 0.017 | 0.8385 ± 0.0007 | 0.2051 ± 0.0004 | 0.8922 ± 0.0008 |
| 8 | J00570+450 | G 172–030 | … | M3.0 V | Lep13 | YD | … | … | … | … | –0.081 ± 0.011 | 0.13 ± 0.05 | 0.0380 ± 0.0005 | 0.0272 ± 0.0007 | 0.1121 ± 0.0004 |
| 9 | J01013+613 | GJ 47 | 47 | M2.0 V | PMSU | D | … | … | … | … | –0.069 ± 0.008 | 0.15 ± 0.11 | 0.6223 ± 0.0001 | 0.9434 ± 0.0001 | 0.0538 ± 0.0001 |
| 10 | J01019+541 | G 218–020 | 3069 | M5.0 V | PMSU | D | 30.6 ± 3.1 | 0.278 ± 0.001 | DA19 | –3.764 ± 0.004 | –5.74 ± 0.06 | 3.5 ± 1.8 | 0.1302 ± 0.0003 | 0.8110 ± 0.0002 | 0.5330 ± 0.0002 |
Notes. The full table with all activity indicators is available at the CDS. Stellar populations are adopted from Cortés-Contreras (2016) and abbreviated as follows: YD: young disc, D: thin disc, TD-D: transition between thin and thick disc, TD: thick disc. v sin i are adopted from from Reiners et al. (2018).
References. PMSU: Palomar/Michigan State University survey (Reid et al. 1995); Lep13: Lépine et al. (2013); AF15: Alonso-Floriano et al. (2015); DA19: Díez Alonso et al. (2019).
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