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Table 1

Our catalogue of 121 LAMOST DA/M binaries.

Jname S/N MJD Plateid Spid Fiberid Err log(g)wd Err M wd Err d Err Sp Type
[K] [M] [pc]

J002237.90+334322.1 5.48 56 255 VB007N33V1 03 085 0 0 0 0 0 0 0 0 –1 0
J002952.22+434205.8 37.36 56 266 M31007N41B2 11 196 34926 1011 8.29 0.19 0.83 0.11 245 34 2 0
J004232.56+415403.0 8.75 55 886 M31_004437N404045_M2 15 202 15071 702 7.08 0.16 0.26 0.04 238 27 6 0
J004432.63+402635.2 11.25 55 886 M31_004437N404045_M2 04 127 0 0 0 0 0 0 0 0 3 0
J004545.96+415029.9 4.57 55 863 M31_011N40_B1 15 128 0 0 0 0 0 0 0 0 2 0
J005221.55+440335.4 15.87 56 207 M31011N44B1 08 149 22292 3046 8.23 0.48 0.77 0.29 225 74 2 0
J005601.44+400718.4 28.14 55 886 M31_004437N404045_M2 06 151 0 0 0 0 0 0 0 0 2 0
J005636.91+383332.6 16.69 55 914 M31_01h38_F1 03 098 0 0 0 0 0 0 0 0 4 0
J005853.40+064849.3 59.70 56 240 EG010249N073002F 03 027 11565 247 7.55 0.25 0.38 0.11 229 35 1 0
J011447.51+254229.6 16.66 56 267 EG011927N271550M01 02 241 35740 628 7.81 0.12 0.57 0.06 140 12 1 0

Notes. White dwarf stellar parameters (effective temperature, surface gravity and mass), spectral type of the companions and distances are given when available, however only those with a S/N higher than 12 (second column) are considered in the analysis of this paper. Spectral types of −1 imply that no values are available. Modified Julian date (MJD), plate (plateid), spectrograph (spid) and fiber (fiberid) identifiers for each of the LAMOST spectra are also provided. For completeness, we also include 181 systems that are not considered by us as DA/M binaries but that show blue and red components in their spectra. These are flagged as 1 in the last column. The complete table can be found at the CDS.

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