Table 2.
Effective temperatures and surface gravities of the cool components of the target stars used in the limb-darkening model, along with their orbital elements.
| Object | Teff | log g | Ref. | P | e | f(m) | Ref. |
|---|---|---|---|---|---|---|---|
| [K] | [dex] | [days] | [M⊙] | ||||
| AG Peg | 3500 | 0.5 | 1 | 818.2±1.6 | 0.11±0.04 | 0.0135±0.0015 | 2 |
| FG Ser | 3400 | 0.5 | 1 | 633.5±2.4 | 0 | 0.0218±0.0025 | 3 |
| ER Del (a) | 3500 | 0.5 | 4 | 2081±2 | 0.281±0.003 | 0.0689±0.002 | 5 |
| V1261 Ori (a) | 3500 | 0.5 | 4 | 638.1±0.1 | 0.061±0.003 | 0.0454 | This work |
| RW Hya | 3700 | 0.5 | 6 | 370.4±0.8 | 0 | 0.026±0.004 | 7 |
| V399 Pav | 3300 | 0.0 | 6 | 560 | 0.05±0.04 | 0.022 | 8 |
Notes.
The giant in this system is an S star. (1) Gałan et al. (2023); (2) Fekel et al. (2000b); (3) Fekel et al. (2000a); (4) Boffin et al. (2014); (5) Jorissen et al. (2019); (6) Gałan et al. (2016); (7) Schild et al. (1996); (8) Brandi et al. (2006).
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