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Table 2.
Stellar parameters of the selected targets in Trumpler 10.
| TIC |
 |
log (L/L⊙)(1) | M (M⊙)(1) | R (R⊙)(1) |
 |
log g(1) | Teff (K)(1) |
 |
Spectral type(3) |
|---|---|---|---|---|---|---|---|---|---|
| 28943819 | 10.545 ± 0.007 | 1.11 ± 0.04 | 2.2 ± 0.3 | 1.60 ± 0.06 | 0.53 ± 0.14 | 4.37 ± 0.08 | 8646 ± 161 | 1.0 | – |
| 30307085 | 10.294 ± 0.006 | 1.28 ± 0.04 | 2.5 ± 0.3 | 1.47 ± 0.04 | 0.80 ± 0.17 | 4.51 ± 0.06 | 9931 ± 202 | 0.8 | A0 |
| 28944596 | 10.354 ± 0.006 | 1.12 ± 0.03 | 2.1 ± 0.3 | 1.72 ± 0.06 | 0.41 ± 0.10 | 4.28 ± 0.07 | 8383 ± 149 | 1.0 | A2 |
| 271061334 | 10.347 ± 0.006 | 1.12 ± 0.03 | 2.2 ± 0.3 | 1.58 ± 0.05 | 0.56 ± 0.13 | 4.38 ± 0.07 | 8773 ± 170 | 0.9 | – |
| 271062192 | 10.238 ± 0.006 | 1.16 ± 0.03 | 2.2 ± 0.3 | 1.68 ± 0.05 | 0.46 ± 0.11 | 4.33 ± 0.07 | 8689 ± 158 | 1.0 | A3 |
Notes. From left to right: TESS magnitude, luminosity, mass, radii, density, surface gravity, effective temperature, cluster member probability, and spectral type.
References. (1)Stassun (2019), (2)Cantat-Gaudin et al. (2018), (3)Skiff (2014).
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