Open Access

Table B.1

A comparison of estimated stellar parameters of WDMS binaries with LAMOST catalog.

Index Gaia ID SED parameters LAMOST parameters
WD Teff (103K) MS Teff (103K) combined Teff (103K) classification
1 1006621281985546240 13.50±0.12 3.4±0.05 Double Star
2 1015888309580557056 11.25±0.12 3.8±0.05 3.66 MS (M1)
3 1607603170812636928a 16.75±0.12 3.6±0.05 3.73-3.79 MS (M1)
4 1911816151065187456 14.75 ±0.12 3.3±0.05 Double Star
5 245807579721338752 8.00±0.12 2.5±0.05 WD (DA)
6 2560009007603950720a 9.50±0.12 2.7±0.05 3.70-3.80 DC+M7
7 3387904051723656320 16.75±0.12 3.3±0.05 23.88 WD (DA)
8 3412836302516713600a 5.25±0.12 4.1 ±0.05 5.74-5.79 MS (G3)
9 3853617934132069760 6.75±0.12 2.7±0.05 3.52 MS (M8)
10 3869392249498967168α 9.50±0.12 3.2±0.05 4.49-4.89 MS (F9 - G5)
11 3992861740235753216a 11.50±0.12 2.7±0.05 16.09-19.87 DAZ+M
12 4437836226304032384 13.00±0.12 3.0±0.05 10.04 DA+M
13 704748371716051072 15.25±0.12 3.3±0.05 3.39 DAZ+M4
14 707217153276016000a 14.75 ±0.12 3.5±0.05 3.50-3.54 MS(M2)
15 830644063706298496 24.00±0.5 2.7±0.05 29.90 DAZ+M
16 881086019353249280 11.75±0.12 3.1±0.05 14.54 DAZ+M

Notes. The table presents a comparison for WD and MS temperatures estimated in our study with the combined temperature of WD and MS as mentioned in the LAMOST DR11 catalog. Spectral classification from LAMOST catalog are also listed. This is truncated list of cross-matched sources, where we noticed the presence of H-absorption line and/or excess UV emissions. A full cross-matched catalog is available on on Zenodo, along with the spectra.

(a)These sources have multi-epoch LAMOST observations.

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