Table 12.
Atmospheric parameters of the ZZ Ceti stars observed by TESS during the survey measurements of the southern ecliptic hemisphere (Sectors 1–13).
| Object | Teff | log g |
|---|---|---|
| [K] | [dex] | |
| Ross 548 | 12 357 | 7.946 |
| EC 23487−2424 | 11 409 | 7.969 |
| BPM 31594 | 11 786 | 8.020 |
| BPM 30551 | 11 392 | 8.049 |
| MCT 0145−2211 | 11 661 | 8.064 |
| L 19−2 | 12 794 | 8.076 |
| HE 0532−5605 | 11 751 | 8.381 |
| HS 0507+0434B | 12 027 | 8.094 |
| MCT 2148−2911 | 12 220 | 7.968 |
| EC 00497−4723 | 11 321 | 7.994 |
| EC 11266−2217 | 12 074 | 7.985 |
| MCT 0016−2553 | 10 972 | 7.962 |
| HS 1013+0321 | 12 639 | 8.033 |
| HE 0031−5525 | 12 293 | 7.891 |
| WD J0925+0509 | 11 215 | 8.166 |
| WD 0108−001 | 10 545 | 7.979 |
| HS 0235+0655 | 10 914 | 7.967 |
| KUV 03442+0719 | 10 870 | 7.78 |
Notes. The Teff and log g values are from Fuchs (2017), except for KUV 03442+0719, where we used the values listed in Bognár & Sódor (2016). The external uncertainties for the observations presented by Fuchs (2017) are 52 K in Teff and 0.013 dex in log g, respectively, while 173 K and 0.06 dex for KUV 03442+0719, as given by Gianninas et al. (2011).
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