Open Access
Table 3.
Spectroscopic estimates of pulsating hot subdwarfs reported here and in Paper I, for which we derived an acceptable spectroscopic fits.
| TIC | Teff | σ | log(g/cm s−2) | σ | log(n(He)/n(H)) | σ | Telescope | Reference |
|---|---|---|---|---|---|---|---|---|
| 968226 | 28 982 | 198 | 5.42 | 0.03 | –3.15 | 0.09 | NOT | |
| 4632676 | 33 589 | 210 | 5.57 | 0.04 | –1.64 | 0.05 | SDSS | Archive |
| 16993518 | 32 194 | 187 | 5.37 | 0.04 | –2.27 | 0.09 | NOT | |
| 19690565 | 31 033 | 225 | 5.75 | 0.05 | –3.12 | 0.15 | NOT | Baran et al. (2023) |
| 26291471 | 34 376 | 106 | 5.76 | 0.02 | –1.34 | 0.03 | VLT | Archive |
| 33318760 | 34 806 | 233 | 5.79 | 0.04 | –1.68 | 0.06 | NTT | Randall et al. (2009) |
| 47377536 | 35 149 | 251 | 5.78 | 0.04 | –1.84 | 0.06 | LAMOST | Archive |
| 55753808 | 34 889 | 263 | 5.80 | 0.05 | –1.80 | 0.06 | LAMOST | Archive |
| 56863037 | 31 940 | 220 | 5.77 | 0.03 | –2.55 | 0.06 | 2.3mKP | Randall et al. (2007) |
| 62381958 | 35 779 | 352 | 5.76 | 0.03 | –1.30 | 0.00 | NTT | Archive |
| 63168679 | 35 885 | 318 | 5.81 | 0.02 | –1.60 | 0.03 | LAMOST | Archive |
| 68495594 | 33 253 | 137 | 5.45 | 0.02 | –1.40 | 0.05 | NOT | |
| 69298924 | 28 063 | 163 | 5.39 | 0.02 | –2.97 | 0.06 | NOT | Baran et al. (2011) |
| 70549283 | 33 879 | 178 | 5.70 | 0.04 | –1.51 | 0.05 | LAMOST | Archive |
| 85145647 | 32 287 | 656 | 5.41 | 0.12 | –3.03 | 0.39 | INT | |
| 88484868 | 29 040 | 140 | 5.47 | 0.02 | –2.85 | 0.06 | INT | Archive |
| 88565376 | 28 400 | 200 | 5.35 | 0.03 | –2.7 | 0.03 | 3.5mCA | Dreizler et al. (2002) |
| 90960668 | 28 932 | 23 | 5.421 | 0.003 | –2.721 | 0.003 | NOT | Østensen et al. (2007) |
| 95752908 | 34 656 | 133 | 5.85 | 0.02 | –1.31 | 0.03 | NOT | Holdsworth et al. (2017) |
| 114196505 | 27 594 | 442 | 5.30 | 0.06 | –2.99 | 0.19 | NOT | |
| 136975077 | 31 800 | 600 | 5.76 | 0.05 | –2.23 | 0.1 | Keck | Heber et al. (2000) |
| 137502282 | 34 259 | 267 | 5.79 | 0.05 | –1.31 | 0.07 | INT | |
| 138618727 | 29 500 | 300 | 5.51 | 0.05 | –2.93 | 0.05 | Keck | Heber et al. (2000) |
| 139481265 | 31 720 | 529 | 5.81 | 0.05 | –2.23 | 0.08 | NOT | Baran et al. (2023) |
| 142200764 | 30 235 | 66 | 5.52 | 0.01 | –2.84 | 0.04 | VLT | Archive |
| 154818961 | 28 330 | 281 | 5.29 | 0.04 | –1.71 | 0.05 | NOT | |
| 156618553 | 28 065 | 43 | 5.51 | 0.01 | –2.45 | 0.02 | VLT | Vučković et al. (2014) |
| 157141133 | 31 076 | 207 | 5.60 | 0.04 | –2.97 | 0.16 | INT | |
| 159644241 | 32 035 | 117 | 5.66 | 0.02 | –2.13 | 0.04 | NOT | Baran et al. (2012) |
| 165312944 | 33 570 | 88 | 5.80 | 0.01 | –1.47 | 0.03 | NOT | Reed et al. (2009) |
| 175402069 | 31 300 | 250 | 5.60 | 0.05 | –2.93 | 0.05 | VLT | Vučković et al. (2007) |
| 178081355 | 33 186 | 176 | 5.67 | 0.03 | –1.77 | 0.03 | SDSS | Archive |
| 186484490 | 28 401 | 274 | 5.40 | 0.04 | –2.90 | 0.09 | LAMOST | Archive |
| 191442416 | 32 400 | 700 | 5.70 | 0.10 | –2.20 | 0.20 | 2.2mCA | Østensen et al. (2001a) |
| 199715319 | 28 144 | 310 | 5.32 | 0.04 | –3.15 | 0.10 | NOT | |
| 202354658 | 29 060 | 280 | 5.43 | 0.05 | –3.44 | 0.26 | NTT/4mKP | Németh et al. (2012) |
| 207440586 | 34 037 | 132 | 5.72 | 0.03 | –1.58 | 0.07 | NOT | |
| 219492314 | 34 575 | 299 | 5.75 | 0.06 | –1.34 | 0.08 | LAMOST | Archive |
| 222892604 | 30 363 | 188 | 5.47 | 0.03 | –3.08 | 0.13 | NOT | |
| 248776104 | 32 891 | 205 | 5.52 | 0.04 | –2.89 | 0.14 | NOT | |
| 266013993 | 32 460 | 290 | 5.77 | 0.07 | –2.33 | 0.11 | NOT | Reed et al. (2009) |
| 273255412 | 33 108 | 140 | 5.21 | 0.02 | –2.63 | 0.07 | LAMOST | Archive |
| 284692897 | 34 594 | 236 | 5.53 | 0.05 | –1.61 | 0.08 | NOT | |
| 310937915 | 34 465 | 131 | 5.74 | 0.02 | –1.67 | 0.05 | NOT | |
| 331656308 | 28 411 | 230 | 5.36 | 0.03 | –2.95 | 0.11 | NOT | |
| 355754830 | 30 750 | 250 | 5.70 | 0.08 | –2.59 | 0.29 | 4mKP | Vennes et al. (2011) |
| 357232133 | 33 470 | 430 | 5.76 | 0.12 | –1.93 | 0.17 | NTT/4mKP | Németh et al. (2012) |
| 364966239 | 33 587 | 241 | 5.70 | 0.05 | –1.50 | 0.07 | NOT | |
| 366656123 | 31 331 | 140 | 5.56 | 0.03 | –2.82 | 0.06 | SDSS | Baran et al. (2023) |
| 392092589 | 27 654 | 280 | 5.40 | 0.04 | –2.97 | 0.10 | NOT | |
| 396954061 | 33 214 | 199 | 5.83 | 0.04 | –1.57 | 0.04 | NOT | |
| 397595169 | 29 300 | 200 | 5.40 | 0.03 | –3.00 | 0.15 | 3.5mCA | Østensen et al. (2001b) |
| 424720852 | 28 311 | 149 | 5.40 | 0.03 | –2.79 | 0.07 | INT | Archive |
| 436579904 | 31 360 | 240 | 5.57 | 0.04 | –2.65 | 0.10 | NOT | Reed et al. (2020) |
| 437043466 | 28 557 | 82 | 5.40 | 0.01 | –3.07 | 0.02 | NOT | Baran et al. (2017) |
| 441725813 | 27 204 | 141 | 5.37 | 0.02 | –2.93 | 0.05 | NOT | |
| 455095580 | 30 817 | 380 | 5.70 | 0.07 | –2.60 | 0.16 | NOT | Baran et al. (2023) |
| 471013461 | 28 551 | 548 | 5.39 | 0.08 | –2.94 | 0.02 | SOAR | Archive |
| 471015194 | 33 150 | 592 | 5.71 | 0.12 | –2.93 | 0.44 | NOT | |
| 673345538 | 29 693 | 396 | 5.44 | 0.09 | –2.72 | 0.21 | LAMOST | Archive |
Notes. The archive spectra were (re-)fit using the same model and method as described in Sect. 2.
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