Free Access
Table 1
Stellar parameters of TOI-1062.
| Parameter | Value | Source |
|---|---|---|
| Identifying information | ||
| TOI | TOI-1062 | TESS |
| TIC ID | 299799658 | TESS |
| 2MASS ID | J02322848-7801256 | 2MASS |
| Gaia ID 4632865331094140928 | Gaia DR3 | |
| Astrometric parameters | ||
| RA (J2015.5, h:m:s) | 02:32:29 | Gaia DR3 |
| Dec (J2015.5, h:m:s) | −78:01:25 | Gaia DR3 |
| Parallax (mas) | 12.14 ± 0.01 | Gaia DR3 |
| Distance (pc) | 82.2± 0.2 | Gaia DR3 |
| Photometric parameters | ||
| B | 11.02 ± 0.07 | Tycho |
| V | 10.25 ± 0.01 | Tycho |
| T | 9.48 ± 0.01 | TESS |
| G | 10.00 ± 0.01 | Gaia |
| J | 8.78 ± 0.02 | 2MASS |
| H | 8.41 ± 0.03 | 2MASS |
| K | 8.30 ± 0.03 | 2MASS |
| W1 | 8.257 ± 0.02 | WISE |
| W2 | 8.322 ± 0.02 | WISE |
| W3 | 8.256 ± 0.02 | WISE |
| W4 | 8.35 ± 0.19 | WISE |
| AV | 0.13 ± 0.04 | Sect. 3 |
| Abundances | ||
| [Fe/H](dex) | 0.14 ± 0.04 | Sect. 3 |
| [O/H](dex) | −0.14 ± 0.16 | Sect. 3 |
| [C/H](dex) | 0.13 ± 0.02 | Sect. 3 |
| [Cu/H](dex) | 0.25 ± 0.04 | Sect. 3 |
| [Zn/H](dex) | 0.08 ± 0.04 | Sect. 3 |
| [Sr/H](dex) | 0.17 ± 0.08 | Setc. 3 |
| [Y/H](dex) | 0.04 ± 0.08 | Sect. 3 |
| [Zr/H](dex) | 0.20 ± 0.06 | Sect. 3 |
| [Ba/H](dex) | −0.02 ± 0.04 | Sect. 3 |
| [Ce/H](dex) | 0.16 ± 0.10 | Sect. 3 |
| [Nd/H](dex) | 0.10 ± 0.06 | Sect. 3 |
| [MgI/H](dex) | 0.16 ± 0.07 | Sect. 3 |
| [AlI/H](dex) | 0.25 ± 0.04 | Sect. 3 |
| [SiI/H](dex) | 0.20 ± 0.07 | Sect. 3 |
| [CaI/H](dex) | 0.10 ± 0.08 | Sect. 3 |
| [TiI/H](dex) | 0.23 ± 0.07 | Sect. 3 |
| [CrI/H](dex) | 0.17 ± 0.07 | Sect. 3 |
| [NiI/H](dex) | 0.17 ± 0.05 | Sect. 3 |
| Bulk parameters | ||
| Mass (M⊙) | 0.94 ± 0.02 | Sect. 3 |
| Radius (R⊙) | 0.84 ± 0.09 | Sect. 3 |
| Teff (K) | 5328 ± 56 | Sect. 3 |
| log g (cm s−2) | 4.55 ± 0.09 | Sect. 3 |
| Spectral type | G9V | Sect. 3 |
| ρ (g cm−3) | 2.22 ± 0.10 | Sect. 3 |
| v sin i (km s−1) | 2.13 ± 0.5 | Sect. 3 |
| Prot (d) | 21.8 ± 2.4 | Sect. 3 |
| Age (Gyrs) | 2.5 ± 0.3 | Sect. 3 |
References. 2MASS (Skrutskie et al. 2006); Tycho (Høg et al. 2000); WISE (Wright et al. 2010); and Gaia (Gaia Collaboration 2018).
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