Table 3
Stellar parameters derived from SED fitting and empirical relations.
| Star |  |
Teff | [Fe/H] | log g* | AV | Fbol | R⋆ |
|---|---|---|---|---|---|---|---|
| [K] | dex | [cgs] | mag | 10−10 [erg s−1 cm−2] | R⊙ | ||
| TOI-148 | 1.4 | 5975 ± 150 | –0.50 ± 0.25 | 4.25 ± 0.1 | 0.03 ± 0.03 | 3.405 ± 0.079 | 1.192 ± 0.068 |
| TOI-587 | 0.9 | 9800 ± 200 | –0.10 ± 0.15 | 4.15 ± 0.15 | 0.02 ± 0.02 | 252.9 ± 5.9 | 2.031 ± 0.092 |
| TOI-681 | 1.0 | 7390 ± 150 | –0.25 ± 0.25 | 4.20 ± 0.15 | 0.22 ± 0.02 | 12.41 ± 0.14 | 1.586 ± 0.067 |
| TOI-746 | 1.6 | 5700 ± 150 | –0.25 ± 0.25 | 4.40 ± 0.10 | 0.18 ± 0.02 | 5.126 ± 0.059 | 0.957 ± 0.051 |
| TOI-1213 | 1.2 | 5675 ± 175 | 0.00 ± 0.25 | 4.45 ± 0.10 | 0.34 ± 0.03 | 10.47 ± 0.12 | 0.951 ± 0.059 |
| Star |  |
 |
Prot∕sin i |  |
 |
 |
|
| M⊙ | M⊙ | [d] | [Gyr] | dex | [Gyr] | ||
| TOI-148 | 0.94 ± 0.26 | 1.03 ± 0.06 | 5.97 ± 0.47 | 0.55 ± 0.07 | – | – | |
| TOI-587 | 2.12 ± 0.29 | 2.32 ± 0.14 | 3.02 ± 0.18 | – | – | – | |
| TOI-681 | 1.45 ± 0.25 | 1.51 ± 0.09 | 2.61 ± 0.13 | – | – | – | |
| TOI-746 | 0.84 ± 0.12 | 0.98 ± 0.06 | 7.9 ± 1.6 | 0.52 ± 0.06 | − 4.50 ± 0.05 | 0.60 ± 0.23 | |
| TOI-1213 | 0.93 ± 0.15 | 1.01 ± 0.06 | 12.0 ± 3.6 | 1.1 ± 0.2 | – | – | |
Notes. We refer thereader to the final adopted parameters for each star presented in Tables A.2–A.6. (a) Stellar mass inferred from R⋆ and spectroscopic log g*. (b) Stellar mass estimated via empirical relations of Torres et al. (2010). (c)System age estimated from inferred rotation period via empirical relations of Mamajek & Hillenbrand (2008). (d) System age estimated from inferred 
via empirical relations of Mamajek & Hillenbrand (2008). The ages derived from stellar rotation and activity are likely underestimated due to the stellar rotations likely being affected by the companions as discussed in Sect. 4.1.
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