Table A.2.
Sample of the nine DBV stars considered in this work. Each column contains information similar to that presented in Table A.1. In this case, column (m) gives the interstellar extinction measured in the V band, computed from the reddening E(B − V) for each star. The spectroscopic effective temperature and surface gravity are those tabulated by Córsico et al. (2019a) that have been corrected by 3D effects following Cukanovaite et al. (2018), unless another reference is indicated.
Name | RA | DEC | V | G | GBP | GRP | S. Type | Teff | log g | π | dBJ | AV | Reference |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(deg) | (deg) | (mag) | (mag) | (mag) | (mag) | (K) | (cgs) | (mas) | (pc) | (mag) | |||
(a) | (b) | (c) | (d) | (e) | (f) | (g) | (h) | (i) | (j) | (k) | (l) | (m) | (n) |
KIC 8626021 | 292.269496 | 44.785841 | 18.545 ± 0.033 | 18.500 | 18.409 | 18.692 | DB | 28 480 ± 750 | 7.89 ± 0.07 |
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Córsico et al. (2019a) |
KUV 05134+2605 | 79.115780 | 26.143762 | 16.795 ± 0.019 | 16.749 | 16.657 | 16.923 | DBA | 24 680 ± 1300 | 8.21 ± 0.06 |
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Córsico et al. (2019a) |
TIC 257459955 | 30.236306 | −15.769369 | 14.707 ± 0.016 | 14.657 | 14.554 | 14.846 | DB | 25 500 ± 1369 | 7.88 ± 0.03 |
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Córsico et al. (2019a) |
GD 358 | 251.826636 | 32.475796 | 13.630 ± 0.020 | 13.580 | 13.476 | 13.770 | DB2.3 | 24 940 ± 1018 | 7.75 ± 0.05 |
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Córsico et al. (2019a) |
PG 1351+489 | 208.292000 | 48.672500 | 16.728 ± 0.024 | 16.678 | 16.586 | 16.877 | DB | 26 010 ± 1536 | 7.91 ± 0.07 |
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Córsico et al. (2019a) |
EC 20058−5234 | 302.416147 | −52.421304 | 15.806 ± 0.016 | 15.756 | 15.647 | 15.938 | DB | 25 500 ± 500 | 8.01 ± 0.05 |
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Córsico et al. (2019a) |
EC 04207−4748 | 65.547319 | −47.695004 | 15.280 ± 0.022 | 15.229 | 15.128 | 15.423 | DB | 25 970 ± 545 | 7.79 ± 0.06 |
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Córsico et al. (2019a) |
WD J152738.37−450207.3 | 231.909792 | −45.035391 | 15.527 ± 0.018 | 15.482 | 15.375 | 15.634 | DB | 25 228 ± 630 | 8.12 ± 0.01 |
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Córsico et al. (2022a) |
L 7−44 | 263.228940 | −87.167376 | 14.785 ± 0.011 | 14.737 | 14.639 | 14.918 | DB | 23 980 ± 1686 | 8.05 ± 0.03 |
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Rolland et al. (2018) |
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