Table B.2
A comparison of estimated stellar parameters of WDMS binaries with SIMBAD.
| Index | Gaia ID | SED parameters | SIMBAD parameters | ||
|---|---|---|---|---|---|
| WD Teff (103K) |
MS Teff (103K) |
SIMBAD ID (103K) |
Spectral Types | ||
| 1 | 1006621281985546240 | 13.50±0.12 | 3.40±0.05 | GALEX J063330.3+612325 | D+M3 |
| 2 | 1089733400290040320 | 11.00±0.12 | 3.10±0.05 | GALEX J073534.3+650649 | DA+M4 |
| 3 | 1911816151065187456 | 14.75 ±0.12 | 3.30±0.05 | PM J23283+3319 | DA+dM |
| 4 | 245807579721338752 | 8.00±0.12 | 2.50±0.05 | EGGR 570 | DA+dM |
| 5 | 2560009007603950720 | 9.50±0.12 | 2.70±0.05 | PHL 3418 | D+dM6 |
| 6 | 2864507860881192320 | 12.00±0.12 | 2.70±0.05 | GALEX J233910.9+255205 | DA5+M7 |
| 7 | 3387904051723656320 | 16.75±0.12 | 3.30±0.05 | UCAC4 506-010126 | D+dM4 |
| 8 | 3612227169936143360a | 21.00±0.5 | 3.40±0.05 | V* QS Vir | DA3+dM |
| 9 | 3662988495054111232 | 8.00±0.12 | 3.20±0.05 | LP 618-14 | DA+dM |
| 10 | 3945572123083449984 | 6.25±0.12 | 2.80±0.05 | LBQS 1216+1628 | DA+M6 |
| 11 | 4028597414327329664 | 5.75±0.12 | 3.00±0.05 | G 148-36 | DAZ+M |
| 12 | 4333046892662353152 | 14.50±0.12 | 3.10±0.05 | GALEX J165737.2-125633 | DA3+M4 |
| 13 | 43789772861265792a | 6.75±0.12 | 4.70±0.05 | V* V471 Tau | K2V+DA |
| 14 | 4411741894799595776 | 9.25±0.12 | 2.90±0.05 | HS 1606+0153 | DA3+dM |
| 15 | 4437836226304032384 | 13.00±0.12 | 3.00±0.05 | PM J16171+0530 | DA+dM |
| 16 | 6182278665776280320 | 12.75±0.12 | 3.20±0.05 | EC 13198-2849 | DA5+dM |
| 17 | 6216887306090464000 | 12.50±0.12 | 3.00±0.05 | GALEX J143830.0-312719 | DA+? |
| 18 | 759601941671398272 | 5.500±0.12 | 3.00±0.05 | EGGR 388 | DC+M4.5Ve |
| 19 | 830644063706298496 | 24.00±0.5 | 2.70±0.05 | GD 123 | DA+M3 |
| 20 | 881086019353249280 | 11.75±0.12 | 3.10±0.05 | GALEX J075919.4+321948 | DA+M |
| 21 | 917083205411949056 | 11.50±0.12 | 3.30±0.05 | UCAC4 670-053833 | D+dM3 |
Notes. The table presents a comparison for WD and MS temperatures estimated in our study with the spectral classification of SIMBAD. This is truncated list of cross-matched sources, classified as DA+M spectral type binaries in SIMBAD. The comparison shows a well-match between temperatures estimated using SED analysis and SIMBAD classification. A full cross-matched catalog is available on on Zenodo.
(a) These are classified as spectroscopic binaries.
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