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Table 3
Internal errors on abundance determination due to uncertainties in stellar parameters for one of the coolest stars (HAT-P-12 for all elements but C and N; WASP-10 for C and N) and for one of the warmest stars (HAT-P-30) in our sample.
| HAT-P-12 | Teff = 4650 K | log g = 4.50 dex | ξ = 0.49 km s−1 | [Fe/H] = −0.25 dex |
|---|---|---|---|---|
| ∆Teff = −/+60 K | ∆ log g = −/+0.10 dex | ∆ξ = −/+0.15 kms−1 | ∆[Fe/H] = −/+0.08 dex | |
| [Fe I/H] | 0.00/0.00 | 0.01/-0.01 | 0.01/-0.02 | …/… |
| [Fe II/H] | 0.08/-0.07 | -0.03/0.09 | 0.01/-0.01 | …/… |
| [C I/H] | 0.09/-0.09 | 0.01/-0.01 | 0.01/-0.01 | −0.01/0.01 |
| [N I/H] | 0.05/-0.05 | 0.00/0.00 | 0.00/0.00 | 0.00/0.00 |
| [O I/H] | 0.08/-0.08 | 0.05/-0.05 | 0.00/0.00 | 0.00/0.00 |
| [Na I/H] | -0.03/0.05 | 0.03/0.00 | 0.01/-0.01 | −0.01/0.01 |
| [Mg I/H] | 0.01/0.00 | 0.01/0.00 | 0.00/0.00 | −0.02/0.02 |
| [Al I/H] | -0.02/0.04 | 0.02/0.00 | 0.01/-0.01 | −0.01/0.01 |
| [Si I/H] | 0.04/-0.04 | -0.01/0.00 | 0.00/0.00 | −0.02/0.02 |
| [S I/H] | 0.04/-0.06 | -0.02/0.00 | 0.00/0.00 | 0.00/0.00 |
| [Ca I/H] | -0.03/0.07 | 0.04/0.00 | 0.01/-0.01 | −0.02/0.02 |
| [Sc II/H] | 0.01/-0.06 | -0.03/0.03 | 0.00/0.00 | −0.03/0.03 |
| [Ti I/H] | -0.06/0.08 | 0.03/0.00 | 0.02/-0.03 | −0.02/0.02 |
| [Ti II/H] | -0.01/0.01 | -0.02/0.00 | 0.02/-0.03 | −0.04/0.03 |
| [V I/H] | -0.08/0.09 | 0.01/-0.01 | 0.02/-0.03 | −0.01/0.01 |
| [Cr I/H] | -0.04/0.05 | 0.01/0.00 | 0.02/-0.02 | −0.01/0.02 |
| [Cr II/H] | 0.03/-0.05 | -0.03/0.00 | 0.01/-0.01 | −0.03/0.02 |
| [Mn I/H] | -0.03/0.03 | 0.02/-0.02 | 0.02/-0.02 | −0.04/0.03 |
| [Co I/H] | -0.01/0.01 | -0.02/0.03 | 0.00/-0.01 | −0.03/0.03 |
| [Ni I/H] | 0.00/-0.01 | -0.01/0.00 | 0.00/-0.02 | −0.03/0.02 |
| [Cu I/H] | 0.00/0.00 | -0.01/0.03 | 0.01/-0.01 | −0.03/0.03 |
| [Zn I/H] | 0.03/-0.04 | 0.00/0.00 | 0.01/-0.02 | −0.03/0.03 |
| [Y I/H] | -0.03/0.00 | -0.02/0.00 | 0.03/-0.03 | −0.03/0.03 |
| [Zr II/H] | -0.04/0.00 | -0.04/0.00 | 0.02/-0.02 | −0.03/0.03 |
| [Ba II/H] | -0.02/0.02 | 0.00/0.00 | 0.03/-0.04 | −0.05/0.05 |
| [La II/H] | -0.02/0.02 | -0.04/0.05 | 0.00/0.00 | −0.03/0.03 |
| [Nd II/H] | -0.05/0.02 | -0.03/0.00 | 0.01/-0.01 | −0.03/0.03 |
| [Eu II/H] | 0.00/0.00 | -0.03/0.05 | 0.00/0.00 | −0.03/0.03 |
| HAT-P-30 | Teff = 6290 K | log g = 4. 30 dex | ξ = 1.05 km s−1 | [Fe/H] = 0.10dex |
|---|---|---|---|---|
| ∆Teff = −/+60 K | ∆ log g = −/+0.10 dex | ∆ξ = −/+0.15 km s−1 | ∆[Fe/H] = −/+0.08 dex | |
| [Fe I/H] | −0.04/0.04 | 0.01/−0.01 | 0.02/−0.03 | …/… |
| [Fe II/H] | 0.00/0.00 | −0.04/0.03 | 0.05/−0.02 | …/… |
| [C I/H] | 0.04/−0.04 | −0.03/0.03 | 0.02/−0.02 | 0.00/0.00 |
| [N I/H] | 0.04/−0.04 | −0.03/0.03 | 0.00/0.00 | −0.01/0.01 |
| [O I/H] | 0.04/−0.04 | .0.01/−0.01 | 0.02/−0.02 | 0.00/0.00 |
| [Na I/H] | −0.03/0.03 | 0.01/−0.01 | 0.01/−0.01 | 0.00/0.00 |
| [Mg I/H] | −0.03/0.02 | 0.00/0.00 | 0.01/−0.01 | 0.00/0.00 |
| [Al I/H] | −0.02/0.02 | 0.00/0.00 | 0.00/0.00 | 0.00/0.00 |
| [Si I/H] | −0.02/0.02 | 0.00/0.00 | 0.01/−0.01 | 0.00/0.00 |
| [S I/H] | 0.01/−0.01 | −0.03/0.03 | 0.00/0.00 | 0.00/0.00 |
| [Ca I/H] | −0.04/0.04 | 0.02/−0.02 | 0.03/−0.03 | 0.00/0.00 |
| [Sc II/H] | 0.00/0.01 | −0.04/0.04 | 0.01/−0.01 | −0.02/−0.05 |
| [Ti I/H] | −0.05/0.05 | 0.00/0.00 | 0.02/−0.02 | 0.00/0.00 |
| [Ti II/H] | 0.00/0.01 | −0.04/0.04 | 0.04/−0.04 | −0.01/0.01 |
| [V I/H] | −0.05/0.05 | 0.00/0.00 | 0.00/0.00 | 0.00/0.00 |
| [Cr I/H] | −0.04/0.04 | 0.00/0.00 | 0.02/−0.02 | 0.00/0.00 |
| [Cr II/H] | 0.01/−0.01 | −0.04/0.03 | 0.03/−0.03 | −0.01/0.01 |
| [Mn I/H] | −0.05/0.05 | 0.00/0.00 | 0.02/−0.02 | 0.00/0.00 |
| [Co I/H] | −0.05/0.05 | 0.00/0.00 | 0.00/0.00 | 0.00/0.00 |
| [Ni I/H] | −0.04/0.04 | 0.00/0.00 | 0.01/−0.02 | 0.00/0.00 |
| [Cu I/H] | −0.05/0.05 | 0.00/0.00 | 0.01/−0.01 | 0.00/0.00 |
| [Zn I/H] | −0.02/0.02 | 0.00/0.01 | 0.06/-0.06 | 0.00/0.00 |
| [Y I/H] | −0.01/0.01 | −0.04/0.04 | 0.07/−0.06 | −0.02/0.02 |
| [Zr II/H] | −0.01/0.01 | −0.04/0.04 | 0.04/−0.03 | −0.02/0.02 |
| [Ba II/H] | −0.03/0.03 | −0.02/0.02 | 0.08/−0.08 | −0.02/0.02 |
| [La II/H] | −0.02/0.02 | −0.04/0.04 | 0.00/0.00 | −0.02/0.02 |
| [Nd II/H] | −0.02/0.02 | −0.04/0.04 | 0.01/−0.01 | −0.02/0.02 |
| [Eu II/H] | −0.01/0.01 | −0.04/0.04 | 0.00/0.00 | −0.02/0.02 |
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