Table 5.
Available photometry for the spectroscopic binaries analysed in this work.
| Karmn | pEW(Hα) (Å) |
Survey | Nobs (Nused) (#) |
Δt (d) |
σ (mmag) |
Prot (d) |
Aλ (mmag) |
|---|---|---|---|---|---|---|---|
| EZ Psc | −4.16 ± 0.06 | MEarth | 1660 (1581) | 2841 | 7.5 | 4.8063 ± 0.0023 | 3.9 |
| GJ 1029 | −0.12 ± 0.02 | MEarth | 862 (833) | 2195 | 6.1 | 16.32 ± 0.24 | 4.3 |
| Ross 59 | −0.034 ± 0.001 | ASAS | 318 (296) | 2544 | 22.4 | ⋯ | ⋯ |
| NLTT 23956 | −7.63 ± 0.09 | SuperWASP | 14814 (12450) | 504 | 49.9 | 7.314 ± 0.040 | 13.3 |
| GJ 3612 | 0.070 ± 0.008 | NSVS | 163 (151) | 359 | 19.1 | 123 ± 15 | 10.8 |
| GJ 1182 | 0.10 ± 0.10 | MEarth | 1203 (1145) | 901 | 4.8 | 8.92 ± 0.24 | 1.7 |
| UU UMi | −0.11 ± 0.02 | MEarth | 1432 (1405) | 747 | 6.6 | 90 ± 26 | 2.6 |
| LP 395-8 | −3.03 ± 0.16 | SuperWASP | 986 (880) | 67 | 21.2 | 1.125 ± 0.011 | 15.1 |
| GJ 810A | −0.02 ± 0.07 | ASAS | 417 (394) | 3170 | 65.8 | ⋯ | ⋯ |
Notes. Number of observations after 2.5-σ clipping, standard deviation, best period and variability semi-amplitude are listed for each target. Only periods with FAP < 0.1% are given. The pseudo-equivalent width of the Hα line is taken from Jeffers et al. (2018), and is also reported as an activity indicator.
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