Table 1
Our catalogue of 121 LAMOST DA/M binaries.
Jname | S/N | MJD | Plateid | Spid | Fiberid |
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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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