Table 2
Stellar and seismic parameters of our sample of stars.
| ID | Teff | Seismic | Predicted | Spectroscopic | [Fe/H] | νmic | νmax | Δv |
|---|---|---|---|---|---|---|---|---|
| (K) | log ɡ | log ɡ | log ɡ | dex | (km/s) | (µHz) | (µHz) | |
| 401 | 4337 ± 10 | – | 1.13 ± 0.04 | 1.05 ± 0.07 | −1.11 ± 0.02 | 1.78 ± 0.05 | – | – |
| 402 | 4697 ± 52 | – | 1.34 ± 0.05 | 1.25 ± 0.10 | −1.66 ± 0.01 | 2.05 ± 0.08 | – | – |
| 403 | 4476 ± 43 | – | 1.17 ± 0.37 | 1 .91 ± 0.09 | −1.45 ± 0.03 | 0.95 ± 0.06 | – | – |
| 404 | 4923 ± 117 | – | 2.07 ± 0.05 | 1.96 ± 0.09 | −1.45 ± 0.01 | 1.58 ± 0.09 | – | – |
| 405 | 5297 ± 35 | 2.07 ± 0.01 | 2.31 ± 0.01 | 2.30 ± 0.12 | −1.26 ± 0.01 | 1.58 ± 0.11 | 3.64 ± 0.49 | 0.68 ± 0.12 |
| 406 | 5112±96 | 2.29 ± 0.01 | 2.37 ± 0.11 | 2.60 ± 0.10 | −0.58 ± 0.01 | 1.77 ± 0.08 | 23.47 ± 1.50 | 3.53 ± 0.29 |
| 407 | 5243 ± 100 | 2.94 ± 0.01 | 2.84 ± 0.11 | 3.07 ± 0.08 | −0.66 ± 0.01 | 1 .45 ± 0.09 | 104.65 ± 1.24 | 9.22 ± 0.61 |
| 408 | 5342 ± 60 | 3.12 ± 0.01 | 3.11 ± 0.02 | 3.06 ± 0.10 | −1.30 ± 0.01 | 1.28 ± 0.13 | 155.54 ± 3.30 | 10.43 ± 0.32 |
| 409 | 4854 ± 37 | 1.76 ± 0.01 | 1.82 ± 0.06 | 1.52 ± 0.11 | −1.17 ± 0.02 | 1.52 ± 0.10 | 7.08 ± 0.57 | 1.21 ± 0.50 |
| 410 | 5094 ± 36 | − | 2.42 ± 0.23 | 1.97 ± 0.11 | −1.28 ± 0.01 | 1.23 ± 0.11 | – | – |
| 411 | 4335 ± 74 | − | 0.76 ± 0.14 | 1.03 ± 0.09 | −1.55 ± 0.01 | 2.01 ± 0.05 | – | – |
| 412 | 4996 ± 99 | 2.76 ± 0.01 | 2.76 ± 0.02 | 2.72 ± 0.11 | −0.64 ± 0.01 | 1.36 ± 0.08 | 69.90 ± 1.68 | 7.52 ± 0.07 |
| 413 | 4850 ± 85 | 1.97 ± 0.01 | 2.00 ± 0.03 | 2.05 ± 0.09 | −1.09 ± 0.01 | 1.54 ± 0.08 | 11.50 ± 1.12 | 1.68 ± 0.19 |
| 414 | 4598 ± 71 | 1.87 ± 0.02 | 1.76 ± 0.16 | 2.07 ± 0.09 | −0.73 ± 0.01 | 1.58 ± 0.08 | 8.88 ± 0.16 | 1 . 45 ± 0.24 |
| 415 | 4342±16 | 1.79 ± 0.01 | 1.73 ± 0.14 | 2.01 ± 0.07 | −0.39 ± 0.01 | 1.65 ± 0.07 | 7.97 ± 1.36 | 1.27 ± 0.01 |
| 416 | 4600 ± 27 | – | 1.63 ± 0.21 | 2.06 ± 0.10 | −0.33 ± 0.01 | 1.79 ± 0.07 | – | – |
| 417 | 5314 ±84 | – | 3.56 ± 0.04 | 3.65 ± 0.08 | −0.63 ± 0.01 | 1.24 ± 0.10 | – | – |
| 418 | 5211±55 | 2.70 ± 0.01 | 2.74 ± 0.04 | 2.65 ± 0.09 | −1.29 ± 0.01 | 1.66 ± 0.10 | 59.81 ± 3.12 | 6.61 ± 0.06 |
| 419 | 4658 ± 36 | 1.50 ± 0.01 | 1.47 ± 0.03 | 1.53 ± 0.09 | −1.40 ± 0.02 | 1 .48 ± 0.06 | 3.92 ± 0.35 | 0.76 ± 0.02 |
| 420 | 5398 ± 47 | – | 2.55 ± 0.20 | 2.14 ± 0.09 | −1.02 ± 0.01 | 2.10 ± 0.10 | – | – |
| 421 | 4802 ± 32 | – | 1.50 ± 0.04 | 1.59 ± 0.08 | −1.18 ± 0.01 | 1.76 ± 0.06 | – | – |
| 422 | 4956 ± 84 | 2.52 ± 0.01 | 2.45 ± 0.14 | 2.76 ± 0.09 | −0.61 ± 0.03 | 1 .49 ± 0.07 | 40.91 ± 0.24 | 4.86 ± 0.16 |
| 423 | 4744 ± 99 | – | 1.76 ± 0.06 | 1.87 ± 0.14 | −1.13 ± 0.01 | 1.67 ± 0.06 | – | – |
| 424 | 5406 ± 58 | 2.89 ± 0.01 | 2.71 ± 0.05 | 2.61 ± 0.13 | −1.67 ± 0.04 | 1.71 ± 0.09 | 91.17 ± 0.19 | 8.31 ± 0.05 |
| 425 | 4865 ± 50 | 1.70 ± 0.01 | 1.69 ± 0.04 | 1.77 ± 0.17 | −2.32 ± 0.07 | 1.82 ± 0.09 | 6.14 ± 0.09 | 0.99 ± 0.01 |
| 426 | 4609 ± 75 | 1.65 ± 0.01 | 1.65 ± 0.05 | 1.55 ± 0.11 | −0.94 ± 0.01 | 1.67 ± 0.06 | 5.68 ± 0.06 | 1.13 ± 0.32 |
| 427 | 4285 ± 30 | – | 0.65 ± 0.07 | 0.78 ± 0.08 | −1.62 ± 0.02 | 2.13 ± 0.05 | – | – |
| 428 | 4156±78 | – | 1.08 ± 0.04 | 1.17 ± 0.14 | −0.82 ± 0.01 | 1.80 ± 0.06 | – | – |
| 429 | 4649 ± 53 | – | 1.25 ± 0.07 | 1 .40 ± 0.10 | −1.59 ± 0.05 | 1.00 ± 0.09 | – | – |
| 430 | 4336 ± 67 | 1.98 ± 0.02 | 0.99 ± 0.00 | 1.00 ± 0.09 | −1.30 ± 0.02 | 2.24 ± 0.07 | 22.77 ± 1.54 | 2.65 ± 0.37 |
Notes. Values of Teff, seismic log ɡ, predicted log ɡ, spectroscopic log ɡ, [Fe/H], microturbulence velocity (vmic), νmax and Δν adopted for our sample of stars. We note that the values for [Fe/H] and vmic presented in this table were obtained using the spectroscopic log ɡ, which allowed it to be available for the 30 stars presented in this work. We also note that while a substantial part of our study is focused on the stars for which νmax and Δν were available, in Sect. 4.5 we present the chemical distribution of the stars shown in this table, even if seismic information was not available for the object.
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