Table 2.
Stellar parameters from the TIC (v8.1, Stassun et al. 2018) for our two selected targets observed by K2 and TESS.
| EPIC 202059229 | EPIC 245919787 | |
|---|---|---|
| TIC 372611670 | TIC 434101713 | |
| Parameter | Value | |
| K2 campaign | C00 | C12 |
| Kp [mag] (a) | 10.500 | 10.329 |
| TESS sector | 6 | 2 |
| T [mag] | 9.2238 ± 0.0075 | 8.8813 ± 0.0069 |
| R* [R⊙] | 0.5498 ± 0.0163 | 0.8043 ± 0.0937 |
| M* [M⊙] | 0.545 ± 0.020 | 0.590 ± 0.083 |
| Teff [K] | 3720 ± 157 | 3821 ± 123 |
| log g | 4.6942 ± 0.0096 | 4.3981 ± 0.1388 |
| Distance [pc] | 22.3819 ± 0.0263 | 27.3518 ± 0.04365 |
| uK2 | 0.3677 | 0.4515 |
| vK2 | 0.3552 | 0.3000 |
| uTESS | 0.2763 | 0.3667 |
| vTESS | 0.3605 | 0.2858 |
| Spectral type (b) | M1.0 | M1.0 |
Notes. The limb darkening coefficients, u and v, for the quadratic limb-darkening law are inferred from the tables by Sing (2010) and Claret (2017) (see Sect. 5).
From the K2 Ecliptic Plane Input Catalog (EPIC, Huber & Bryson 2017).
From Raetz et al. (2020b).
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