Table 4
Basic information and stellar kinematic properties of our targets.
| Name | α (deg) | δ (deg) | Parallax (mas) | Sp.T. | G (mag) | U (km/s) | V (km/s) | W (km/s) | TD/D | Group |
|---|---|---|---|---|---|---|---|---|---|---|
| TOI-179 | 44.26±0.01 | −56.19±0.01 | 25.88±0.01 | K1V | 8.74 | −12.06±0.05 | 22.31 ±0.72 | 0.26±0.96 | 0.02 | Field(a) |
| TOI-1136 | 192.18±0.01 | 64.86±0.01 | 11.82± 0.01 | G2V | 9.38 | −8.87±0.07 | 14.71±0.10 | 14.78±0.16 | 0.02 | Field(b) |
| TOI-1430 | 300.61±0.01 | 53.38±0.01 | 24.25±0.01 | K2V | 8.95 | −50.27±0.02 | −8.65±0.20 | −12.53±0.04 | 0.02 | Field(c) |
| TOI-1726 | 117.48±0.02 | 27.36±0.01 | 44.68±0.02 | G3V | 6.74 | 5.14±0.18 | 15.81±0.04 | −1.27±0.08 | 0.01 | Ursa Major(d) |
| TOI-2048 | 237.92±0.01 | 52.31 ± 0.01 | 8.59±0.01 | K2V | 11.32 | −10.87±0.02 | 4.04±0.13 | 4.20±0.15 | 0.01 | Group X(e) |
| TOI-2076 | 217.39±0.01 | 39.79±0.01 | 23.81±0.01 | K1V | 8.92 | −24.71±0.03 | −7.78±0.08 | 3.76±0.18 | 0.01 | Comoving pair with TOI-1807(f) |
| TOI-4515 | 21.19±0.02 | 21.51 ± 0.01 | 5.16±0.02 | G8V | 11.80 | −13.14±0.11 | 24.79±0.11 | −0.14±0.13 | 0.02 | Field(g) |
| TOI-5082 | 106.57±0.02 | 22.68±0.02 | 23.24±0.03 | G5V | 8.09 | −52.69±0.19 | −4.80±0.05 | −6.80±0.05 | 0.02 | ... |
| TOI-5398 | 161.88±0.01 | 36.33±0.01 | 7.62±0.01 | F9.5V | 9.99 | −4.55±0.09 | 18.25±0.01 | −1.83±0.18 | 0.01 | Field(h) |
| TOI-5543 | 66.14±0.02 | 23.27±0.01 | 7.99±0.02 | K2V | 11.23 | −20.28±0.19 | −10.31±0.06 | −4.45±0.08 | 0.01 | ... |
Notes. Columns list right ascensions, declinations, Gaia DR3 magnitudes, and parallaxes taken from Gaia Collaboration (2016, 2021), spectral types obtained from the Pecaut & Mamajek (2013) table (version 2022) and our Teff, UVW velocities, and thick-to-thin disk probability (TD/D) as derived in the present work. The last column lists the membership group from the literature. (a)Desidera et al. (2023), (b)Dai et al. (2023), (c)Nardiello et al. (2024), (d)Mann et al. (2020), (e)Newton et al. (2023), (f)Hedges et al. (2021), (g)Carleo et al. (2024), (h)Mantovan et al. (2024a).
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