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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 2 . 65 0.14 + 0.11 $ 2.65^{+0.11}_{-0.14} $ 382 . 39 16.00 + 13.54 $ 382.39^{+13.54}_{-16.00} $ 0 . 152 0.027 + 0.017 $ 0.152^{+0.017}_{-0.027} $ 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 6 . 69 0.07 + 0.07 $ 6.69^{+0.07}_{-0.07} $ 149 . 77 1.80 + 1.72 $ 149.77^{+1.72}_{-1.80} $ 0 . 063 0.023 + 0.026 $ 0.063^{+0.026}_{-0.023} $ 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 14 . 57 0.04 + 0.04 $ 14.57^{+0.04}_{-0.04} $ 68 . 51 0.11 + 0.12 $ 68.51^{+0.12}_{-0.11} $ 0 . 025 0.017 + 0.027 $ 0.025^{+0.027}_{-0.017} $ 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 23 . 24 0.03 + 0.02 $ 23.24^{+0.02}_{-0.03} $ 42 . 99 0.05 + 0.04 $ 42.99^{+0.04}_{-0.05} $ 0 . 010 0.007 + 0.008 $ 0.010^{+0.008}_{-0.007} $ 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 5 . 69 0.06 + 0.05 $ 5.69^{+0.05}_{-0.06} $ 175 . 73 1.58 + 1.53 $ 175.73^{+1.53}_{-1.58} $ 0 . 062 0.019 + 0.011 $ 0.062^{+0.011}_{-0.019} $ 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 8 . 48 0.06 + 0.05 $ 8.48^{+0.05}_{-0.06} $ 117 . 95 0.75 + 0.68 $ 117.95^{+0.68}_{-0.75} $ 0 . 181 0.108 + 0.108 $ 0.181^{+0.108}_{-0.108} $ 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 10 . 93 0.03 + 0.03 $ 10.93^{+0.03}_{-0.03} $ 91 . 48 0.23 + 0.22 $ 91.48^{+0.22}_{-0.23} $ 0 . 040 0.024 + 0.024 $ 0.040^{+0.024}_{-0.024} $ 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 10 . 54 0.05 + 0.04 $ 10.54^{+0.04}_{-0.05} $ 94 . 62 0.37 + 0.34 $ 94.62^{+0.34}_{-0.37} $ 0 . 927 0.566 + 0.566 $ 0.927^{+0.566}_{-0.566} $ 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 14 . 47 0.01 + 0.02 $ 14.47^{+0.02}_{-0.01} $ 69 . 09 0.12 + 0.14 $ 69.09^{+0.14}_{-0.12} $ 0 . 544 0.326 + 0.326 $ 0.544 ^{+0.326}_{-0.326} $ Rolland et al. (2018)

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