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Table 3.
Stellar parameters of KIC 3526061 from this work together with those known from the literature.
| Parameter | Value | Reference | Parameter | Value | Reference | |
|---|---|---|---|---|---|---|
| mV (mag) | 10.37 ± 0.04 | Høg et al. (2000) | Δν (μHz) | 10.7 ± 0.3 | Hekker et al. (2011)(a) | |
| B − V (mag) | 0.96 ± 0.08 | Høg et al. (2000) | Δν (μHz) | 10.73 ± 0.05 | Mosser et al. (2014) | |
| Parallax (mas) | 2.5042 ± 0.0123 | Gaia Collaboration (2021a) | Δν (μHz) | 10.64 ± 0.23 | Pinsonneault et al. (2014) | |
| MV (mag) | 2.36 ± 0.04 | This work | Δν (μHz) | 10.670 ± 0.014 | Huber et al. (2017)(b) | |
| Distance (pc) | 399 ± 2 | This work | Δν (μHz) | 10.667 ± 0.004 | Pinsonneault et al. (2018) | |
| Distance (pc) |
 |
Rodrigues et al. (2014) | Δν (μHz) | 10.71 | Vrard et al. (2018) | |
| Distance (pc) | 645 ± 88 | Wang et al. (2016) | Δν (μHz) | 10.677 ± 0.016 | Yu et al. (2018) | |
| Distance (pc) |
 |
Huber et al. (2017)(b) | Δν (μHz) | 10.62 ± 0.05 | Gaulme et al. (2020) | |
| Distance (pc) | 392.44 ± 12.70 | Silva Aguirre et al. (2018) | νmax (μHz) | 129 ± 4 | Hekker et al. (2011)(a) | |
| Teff (K) |
 |
This work | νmax (μHz) | 127.52 ± 2.79 | Pinsonneault et al. (2014) | |
| Teff (K) | 4683 ± 77 | Pinsonneault et al. (2014) | νmax (μHz) | 128.607 ± 0.639 | Huber et al. (2017)(b) | |
| Teff (K) | 4747 ± 5 | Ness et al. (2016) | νmax (μHz) | 128.243 ± 0.012 | Pinsonneault et al. (2018) | |
| Teff (K) | 4747 ± 86 | Huber et al. (2017)(b) | νmax (μHz) | 130.0 | Vrard et al. (2018) | |
| Teff (K) | 4770 ± 73 | Pinsonneault et al. (2018) | νmax (μHz) | 128.74 ± 0.60 | Yu et al. (2018) | |
| Teff (K) | 4865 ± 100 | Yu et al. (2018) | νmax (μHz) | 129.82 ± 0.25 | Gaulme et al. (2020) | |
| [Fe/H] (dex) |
 |
This work | Age (Gyr) | 8.66 ± 1.06 | Ness et al. (2016) | |
| [Fe/H] (dex) | 0.23 ± 0.05 | Pinsonneault et al. (2014) | Age (Gyr) | 5.309 ± 0.001 | Pinsonneault et al. (2018) | |
| [Fe/H] (dex) | 0.13 ± 0.11 | Hawkins et al. (2016) | Age (Gyr) | 5.169 ± 1.270 | Silva Aguirre et al. (2018) | |
| [Fe/H] (dex) | 0.237 ± 0.004 | Ness et al. (2016) | M* (M⊙) | 1.48 ± 0.20 | Mosser et al. (2014) | |
| [Fe/H] (dex) | 0.157 ± 0.060 | Huber et al. (2017)(b) | M* (M⊙) |
 |
Pinsonneault et al. (2014) | |
| [Fe/H] (dex) | 0.224 ± 0.027 | Pinsonneault et al. (2018) | M* (M⊙) | 1.11 ± 1.02 | Ness et al. (2016) | |
| [Fe/H] (dex) | 0.23 ± 0.15 | Yu et al. (2018) | M* (M⊙) | 1.274 ± 0.046 | Pinsonneault et al. (2018) | |
| vturb (km s−1) |
 |
This work | M* (M⊙) | 1.291 ± 0.061 | Silva Aguirre et al. (2018) | |
| vturb (km s−1) | 1.037 ± 0.081 | Hawkins et al. (2016) | M* (M⊙) | 1.42 ± 0.041 | Vrard et al. (2018) | |
| vmacro (km s−1) |
 |
This work | M* (M⊙) | 1.38 ± 0.07 | Yu et al. (2018) | |
| v sini (km s−1) |
 |
This work | M* (M⊙) | 1.42 ± 0.09 | Gaulme et al. (2020) | |
| log g (dex) |
 |
This work | M* (M⊙) |
 |
Sayeed et al. (2021) | |
| log g (dex) | 3.001 ± 0.011 | Pinsonneault et al. (2014) | R* (R⊙) |
 |
Pinsonneault et al. (2014) | |
| log g (dex) | 2.94 ± 0.01 | Ness et al. (2016) | R* (R⊙) |
 |
Huber et al. (2017)(b) | |
| log g (dex) | 3.015 ± 0.004 | Huber et al. (2017)(b) | R* (R⊙) | 5.797 ± 0.016 | Pinsonneault et al. (2018) | |
| log g (dex) | 3.017 ± 0.006 | Pinsonneault et al. (2018) | R* (R⊙) | 5.834 ± 0.121 | Silva Aguirre et al. (2018) | |
| log g (dex) | 3.016 ± 0.005 | Silva Aguirre et al. (2018) | R* (R⊙) | 6.02 ± 0.11 | Yu et al. (2018) | |
| log g (dex) | 3.021 ± 0.007 | Yu et al. (2018) | R* (R⊙) | 6.09 ± 0.12 | Gaulme et al. (2020) | |
| log g (dex) | 3.02 ± 0.01 | Gaulme et al. (2020) | R* (R⊙) |
 |
Sayeed et al. (2021) | |
| log g (dex) | 3.012 ± 0.200 | Sayeed et al. (2021) | Status | RGB (c) | Mosser et al. (2014) | |
| L (L⊙) | 16.4 ± 1.4 | This work | Status | RGB (c) | Ness et al. (2016) | |
| L (L⊙) | 15.716 ± 1.325 | Silva Aguirre et al. (2018) | Status | RGB (c) | Elsworth et al. (2017) | |
| Status | non He-core burning | Huber et al. (2017)(b) | ||||
| Status | RGB (c) | Vrard et al. (2018) | ||||
| Status | RGB (c) | Yu et al. (2018) |
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